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Ratneswaren T, Chan N, Aeron-Thomas J, Sait S, Adesalu O, Alhawamdeh M, Benger M, Garnham J, Dixon L, Tona F, McNamara C, Taylor E, Lobotesis K, Lim E, Goldberg O, Asmar N, Evbuomwan O, Banerjee S, Holm-Mercer L, Senor J, Tsitsiou Y, Tantrige P, Taha A, Ballal K, Mattar A, Daadipour A, Elfergani K, Barker R, Chakravartty R, Murchison AG, Kemp BJ, Simister R, Davagnanam I, Wong OY, Werring D, Banaras A, Anjari M, Rodrigues JCL, Thompson CAS, Haines IR, Burnett TA, Zaher REY, Reay VL, Banerjee M, Sew Hee CSL, Oo AP, Lo A, Rogers P, Hughes T, Marin A, Mukherjee S, Jaber H, Sanders E, Owen S, Bhandari M, Sundayi S, Bhagat A, Elsakka M, Hashmi OH, Lymbouris M, Gurung-Koney Y, Arshad M, Hasan I, Singh N, Patel V, Rahiminejad M, Booth TC. COVID-19 Stroke Apical Lung Examination Study 2: a national prospective CTA biomarker study of the lung apices, in patients presenting with suspected acute stroke (COVID SALES 2). Neuroimage Clin 2024; 42:103590. [PMID: 38513535 DOI: 10.1016/j.nicl.2024.103590] [Citation(s) in RCA: 0] [Impact Index Per Article: 0] [Reference Citation Analysis] [What about the content of this article? (0)] [Affiliation(s)] [Abstract] [Key Words] [Track Full Text] [Journal Information] [Subscribe] [Scholar Register] [Received: 01/26/2024] [Revised: 03/10/2024] [Accepted: 03/13/2024] [Indexed: 03/23/2024]
Abstract
BACKGROUND Apical ground-glass opacification (GGO) identified on CT angiography (CTA) performed for suspected acute stroke was developed in 2020 as a coronavirus-disease-2019 (COVID-19) diagnostic and prognostic biomarker in a retrospective study during the first wave of COVID-19. OBJECTIVE To prospectively validate whether GGO on CTA performed for suspected acute stroke is a reliable COVID-19 diagnostic and prognostic biomarker and whether it is reliable for COVID-19 vaccinated patients. METHODS In this prospective, pragmatic, national, multi-center validation study performed at 13 sites, we captured study data consecutively in patients undergoing CTA for suspected acute stroke from January-March 2021. Demographic and clinical features associated with stroke and COVID-19 were incorporated. The primary outcome was the likelihood of reverse-transcriptase-polymerase-chain-reaction swab-test-confirmed COVID-19 using the GGO biomarker. Secondary outcomes investigated were functional status at discharge and survival analyses at 30 and 90 days. Univariate and multivariable statistical analyses were employed. RESULTS CTAs from 1,111 patients were analyzed, with apical GGO identified in 8.5 % during a period of high COVID-19 prevalence. GGO showed good inter-rater reliability (Fleiss κ = 0.77); and high COVID-19 specificity (93.7 %, 91.8-95.2) and negative predictive value (NPV; 97.8 %, 96.5-98.6). In subgroup analysis of vaccinated patients, GGO remained a good diagnostic biomarker (specificity 93.1 %, 89.8-95.5; NPV 99.7 %, 98.3-100.0). Patients with COVID-19 were more likely to have higher stroke score (NIHSS (mean +/- SD) 6.9 +/- 6.9, COVID-19 negative, 9.7 +/- 9.0, COVID-19 positive; p = 0.01), carotid occlusions (6.2 % negative, 14.9 % positive; p = 0.02), and larger infarcts on presentation CT (ASPECTS 9.4 +/- 1.5, COVID-19 negative, 8.6 +/- 2.4, COVID-19 positive; p = 0.00). After multivariable logistic regression, GGO (odds ratio 15.7, 6.2-40.1), myalgia (8.9, 2.1-38.2) and higher core body temperature (1.9, 1.1-3.2) were independent COVID-19 predictors. GGO was associated with worse functional outcome on discharge and worse survival after univariate analysis. However, after adjustment for factors including stroke severity, GGO was not independently predictive of functional outcome or mortality. CONCLUSION Apical GGO on CTA performed for patients with suspected acute stroke is a reliable diagnostic biomarker for COVID-19, which in combination with clinical features may be useful in COVID-19 triage.
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Affiliation(s)
- T Ratneswaren
- Charing Cross Hospital, London, UK; Addenbrooke's Hospital, Cambridge, UK
| | - N Chan
- Royal London Hospital, London, UK
| | | | - S Sait
- King's College Hospital, London, UK
| | | | | | - M Benger
- King's College Hospital, London, UK
| | | | - L Dixon
- Charing Cross Hospital, London, UK
| | - F Tona
- Charing Cross Hospital, London, UK
| | | | - E Taylor
- Charing Cross Hospital, London, UK
| | | | - E Lim
- Charing Cross Hospital, London, UK
| | | | - N Asmar
- Charing Cross Hospital, London, UK
| | | | | | | | - J Senor
- Charing Cross Hospital, London, UK
| | | | - P Tantrige
- Princess Royal University Hospital, Orpington, UK
| | - A Taha
- Princess Royal University Hospital, Orpington, UK
| | - K Ballal
- Princess Royal University Hospital, Orpington, UK
| | - A Mattar
- Princess Royal University Hospital, Orpington, UK
| | - A Daadipour
- Princess Royal University Hospital, Orpington, UK
| | - K Elfergani
- Princess Royal University Hospital, Orpington, UK
| | - R Barker
- Frimley Park Hospital, Surrey, UK
| | | | | | - B J Kemp
- John Radcliffe Hospital, Oxford, UK
| | | | | | - O Y Wong
- University College Hospital, London, UK
| | - D Werring
- Comprehensive Stroke Service, National Hospital for Neurology and Neurosurgery, University College Hospitals NHS Foundation Trust, London, UK; Stroke Research Centre, UCL Queen Square Institute of Neurology, London, UK
| | - A Banaras
- University College Hospital, London, UK
| | - M Anjari
- Lysholm Department of Neuroradiology, National Hospital for Neurology and Neurosurgery, University College London Hospitals NHS Foundation Trust, UK
| | | | | | | | | | - R E Y Zaher
- Southampton General Hospital, Southampton, UK
| | - V L Reay
- Southampton General Hospital, Southampton, UK
| | - M Banerjee
- Southampton General Hospital, Southampton, UK
| | | | - A P Oo
- Southampton General Hospital, Southampton, UK
| | - A Lo
- Addenbrooke's Hospital, Cambridge, UK
| | - P Rogers
- Addenbrooke's Hospital, Cambridge, UK
| | - T Hughes
- Cardiff and Vale University Health Board, Cardiff, UK
| | - A Marin
- Cardiff and Vale University Health Board, Cardiff, UK
| | - S Mukherjee
- Cardiff and Vale University Health Board, Cardiff, UK
| | - H Jaber
- Cardiff and Vale University Health Board, Cardiff, UK
| | - E Sanders
- Cardiff and Vale University Health Board, Cardiff, UK
| | - S Owen
- Cardiff and Vale University Health Board, Cardiff, UK
| | | | - S Sundayi
- Watford General Hospital, Watford, UK
| | - A Bhagat
- Watford General Hospital, Watford, UK
| | - M Elsakka
- Watford General Hospital, Watford, UK
| | - O H Hashmi
- Norfolk and Norwich University Hospital, Norwich, UK
| | - M Lymbouris
- Norfolk and Norwich University Hospital, Norwich, UK
| | | | - M Arshad
- Norfolk and Norwich University Hospital, Norwich, UK
| | - I Hasan
- Norfolk and Norwich University Hospital, Norwich, UK
| | - N Singh
- Norfolk and Norwich University Hospital, Norwich, UK
| | - V Patel
- St Thomas' Hospital, London, UK
| | | | - T C Booth
- King's College Hospital, London, UK; School of Biomedical Engineering & Imaging Sciences, King's College London, London, UK.
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Saini S, Sharma A, Kaur N, Singh N. Solvent directed morphogenesis of a peptidic-benzimidazolium dipodal receptor: ratiometric detection and catalytic degradation of ochratoxin A. Anal Methods 2024; 16:1111-1122. [PMID: 38293839 DOI: 10.1039/d3ay02045b] [Citation(s) in RCA: 0] [Impact Index Per Article: 0] [Reference Citation Analysis] [What about the content of this article? (0)] [Affiliation(s)] [Abstract] [MESH Headings] [Track Full Text] [Subscribe] [Scholar Register] [Indexed: 02/01/2024]
Abstract
Ochratoxin A (OTA) is the most abundant and harmful toxin found in agriculture and processed food. The environment and human health are both harmed by this mycotoxin. As a result, in various scenarios, selective detection and biodegradation of ochratoxin A are essential. The current study reveals the morphogenesis of a peptidic-benzimidazolium dipodal receptor (SS4) and its application as a catalytic and sensing unit for the detection and degradation of OTA in an aqueous medium. Initially, a facile and scalable method was executed to synthesize SS4, and solvent-directed morphogenesis were examined under SEM analysis. Consequently, molecular recognition properties of self-assembled architectures were explored using UV-visible absorption, fluorescence spectroscopy, and atomic force microscopy (AFM). The designed probe showed a ratiometric response for OTA and served as a catalytic unit for the degradation of OTA at a short interval of 25 min. The biodegradation pathway for OTA was accomplished using LC-MS analysis. Furthermore, the reliability of the developed method was checked by determining the spiked concentrations of the OTA in cereals and wine samples. The results obtained are in good agreement with the % recovery and RSD values. The present work provides a robust, selective, and sensitive method of detection and degradation for OTA.
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Affiliation(s)
- Sanjeev Saini
- Department of Chemistry, Indian Institute of Technology Ropar, Punjab 140001, India.
- Department of Chemistry, School of Physical Sciences, DIT University, Dehradun 248009, India
| | - Arun Sharma
- Department of Chemistry, Indian Institute of Technology Ropar, Punjab 140001, India.
| | - Navneet Kaur
- Department of Chemistry, Panjab University, Chandigarh 160014, India
| | - Narinder Singh
- Department of Chemistry, Indian Institute of Technology Ropar, Punjab 140001, India.
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deBoer RJ, Febbraro M, Bardayan DW, Boomershine C, Brandenburg K, Brune C, Coil S, Couder M, Derkin J, Dede S, Fang R, Fritsch A, Gula A, Gyürky G, Hackett B, Hamad G, Jones-Alberty Y, Kelmar R, Manukyan K, Matney M, McDonaugh J, Meisel Z, Moylan S, Nattress J, Odell D, O'Malley P, Paris MW, Robertson D, Shahina, Singh N, Smith K, Smith MS, Stech E, Tan W, Wiescher M. Measurement of the ^{13}C(α, n_{0})^{16}O Differential Cross Section from 0.8 to 6.5 MeV. Phys Rev Lett 2024; 132:062702. [PMID: 38394565 DOI: 10.1103/physrevlett.132.062702] [Citation(s) in RCA: 0] [Impact Index Per Article: 0] [Reference Citation Analysis] [What about the content of this article? (0)] [Affiliation(s)] [Abstract] [Track Full Text] [Subscribe] [Scholar Register] [Received: 03/18/2023] [Revised: 09/05/2023] [Accepted: 01/17/2024] [Indexed: 02/25/2024]
Abstract
The cross section of the ^{13}C(α,n)^{16}O reaction is needed for nuclear astrophysics and applications to a precision of 10% or better, yet inconsistencies among 50 years of experimental studies currently lead to an uncertainty of ≈15%. Using a state-of-the-art neutron detection array, we have performed a high resolution differential cross section study covering a broad energy range. These measurements result in a dramatic improvement in the extrapolation of the cross section to stellar energies potentially reducing the uncertainty to ≈5% and resolving long standing discrepancies in higher energy data.
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Affiliation(s)
- R J deBoer
- Department of Physics and Astronomy, University of Notre Dame, Notre Dame, Indiana 46556, USA
| | - M Febbraro
- Oak Ridge National Laboratory, Oak Ridge, Tennessee 37831, USA
| | - D W Bardayan
- Department of Physics and Astronomy, University of Notre Dame, Notre Dame, Indiana 46556, USA
| | - C Boomershine
- Department of Physics and Astronomy, University of Notre Dame, Notre Dame, Indiana 46556, USA
| | - K Brandenburg
- Department of Physics and Astronomy, Ohio University, Athens, Ohio 45701, USA
| | - C Brune
- Department of Physics and Astronomy, Ohio University, Athens, Ohio 45701, USA
| | - S Coil
- Department of Physics and Astronomy, University of Notre Dame, Notre Dame, Indiana 46556, USA
| | - M Couder
- Department of Physics and Astronomy, University of Notre Dame, Notre Dame, Indiana 46556, USA
| | - J Derkin
- Department of Physics and Astronomy, Ohio University, Athens, Ohio 45701, USA
| | - S Dede
- Department of Physics and Astronomy, University of Notre Dame, Notre Dame, Indiana 46556, USA
| | - R Fang
- Department of Physics and Astronomy, University of Notre Dame, Notre Dame, Indiana 46556, USA
| | - A Fritsch
- Department of Physics, Gonzaga University, Spokane, Washington 99258, USA
| | - A Gula
- Department of Physics and Astronomy, University of Notre Dame, Notre Dame, Indiana 46556, USA
| | - Gy Gyürky
- Institute for Nuclear Research (Atomki), P.O.B 51, H-4001 Debrecen, Hungary
| | - B Hackett
- Department of Physics and Astronomy, University of Tennessee, Knoxville, Tennessee 37996, USA
| | - G Hamad
- Department of Physics and Astronomy, Ohio University, Athens, Ohio 45701, USA
| | - Y Jones-Alberty
- Department of Physics and Astronomy, Ohio University, Athens, Ohio 45701, USA
| | - R Kelmar
- Department of Physics and Astronomy, University of Notre Dame, Notre Dame, Indiana 46556, USA
| | - K Manukyan
- Department of Physics and Astronomy, University of Notre Dame, Notre Dame, Indiana 46556, USA
| | - M Matney
- Department of Physics and Astronomy, University of Notre Dame, Notre Dame, Indiana 46556, USA
| | - J McDonaugh
- Department of Physics and Astronomy, University of Notre Dame, Notre Dame, Indiana 46556, USA
| | - Z Meisel
- Department of Physics and Astronomy, Ohio University, Athens, Ohio 45701, USA
| | - S Moylan
- Department of Physics and Astronomy, University of Notre Dame, Notre Dame, Indiana 46556, USA
| | - J Nattress
- Oak Ridge National Laboratory, Oak Ridge, Tennessee 37831, USA
| | - D Odell
- Department of Physics and Astronomy, Ohio University, Athens, Ohio 45701, USA
| | - P O'Malley
- Department of Physics and Astronomy, University of Notre Dame, Notre Dame, Indiana 46556, USA
| | - M W Paris
- Theoretical Division, Los Alamos National Laboratory, Los Alamos, New Mexico 87545, USA
| | - D Robertson
- Department of Physics and Astronomy, University of Notre Dame, Notre Dame, Indiana 46556, USA
| | - Shahina
- Department of Physics and Astronomy, University of Notre Dame, Notre Dame, Indiana 46556, USA
| | - N Singh
- Department of Physics and Astronomy, Ohio University, Athens, Ohio 45701, USA
| | - K Smith
- Los Alamos National Laboratory, Los Alamos, New Mexico 87545, USA
| | - M S Smith
- Oak Ridge National Laboratory, Oak Ridge, Tennessee 37831, USA
| | - E Stech
- Department of Physics and Astronomy, University of Notre Dame, Notre Dame, Indiana 46556, USA
| | - W Tan
- Department of Physics and Astronomy, University of Notre Dame, Notre Dame, Indiana 46556, USA
| | - M Wiescher
- Department of Physics and Astronomy, University of Notre Dame, Notre Dame, Indiana 46556, USA
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Sharma A, Singh G, Kaur N, Singh N. Core-Labeled Reverse Micelle-Based Supramolecular Solvents for Assisted Quick and Sensitive Determination of Amitriptyline in Wastewater. Langmuir 2024. [PMID: 38319126 DOI: 10.1021/acs.langmuir.3c03691] [Citation(s) in RCA: 0] [Impact Index Per Article: 0] [Reference Citation Analysis] [What about the content of this article? (0)] [Affiliation(s)] [Abstract] [Track Full Text] [Subscribe] [Scholar Register] [Indexed: 02/07/2024]
Abstract
In recent years, the issue of pharmaceutical contaminants in water bodies has emerged as a significant environmental concern owing to the potential negative impacts on both aquatic ecosystems and human health. Consequently, the development of efficient and eco-friendly methods for their determination and removal is of paramount importance. In this context, the development of a surfactant ensemble sensor has been explored for hard-to-sense amphiphilic drug, i.e., amitriptyline. Herein, a pyrene-based amphiphile chemoreceptor was synthesized and characterized through various spectroscopic techniques such as 1H, 13C NMR, single-crystal XRD, FTIR, and ES-mass spectrometry. Then, dodecanoic acid (DA) and a pyrene-based receptor in a THF/water solvent system were used to generate reverse micelle-based self-aggregates of SUPRAS (SUPRAmolecular Solvent). The structural aspects, such as morphology and size, along with the stability of the SUPRAS aggregates were unfolded through spectroscopic and microscopic insights. The present investigation describes a synergistic approach that combines the unique properties of premicellar concentration of supramolecular solvent with the promising potential of pyrene-based receptor for enhanced amitriptyline extraction with simultaneous determination from water (LOD = 12 nM). To evaluate the effectiveness of the developed aggregates in real-world scenarios, experiments were conducted to determine the sensing efficiency among various pharmaceutical pollutants commonly found in water sources. The results reveal that the synergistic nanoensemble exhibits remarkable sensing ability, toward the amitriptyline (AMT) drug outperforming conventional methods.
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Affiliation(s)
- Arun Sharma
- Department of Chemistry, Indian Institute of Technology Ropar, Rupnagar, Punjab 140001, India
| | - Gagandeep Singh
- Department of Biomedical Engineering, Indian Institute of Technology Ropar, Rupnagar, Punjab 140001, India
| | - Navneet Kaur
- Department of Chemistry, Panjab University, Chandigarh 160014, India
| | - Narinder Singh
- Department of Chemistry, Indian Institute of Technology Ropar, Rupnagar, Punjab 140001, India
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Mala R, Malhotra S, Singh N, Gupta S, Upadhyay DA, Kapil A, Sood S. Deciphering Intermediate Nugent scores: Utility of Real-time PCR for Bacterial Vaginosis diagnosis. Diagn Microbiol Infect Dis 2024; 108:116152. [PMID: 38061216 DOI: 10.1016/j.diagmicrobio.2023.116152] [Citation(s) in RCA: 0] [Impact Index Per Article: 0] [Reference Citation Analysis] [What about the content of this article? (0)] [Affiliation(s)] [Abstract] [Key Words] [MESH Headings] [Track Full Text] [Journal Information] [Subscribe] [Scholar Register] [Received: 04/23/2023] [Revised: 11/16/2023] [Accepted: 11/26/2023] [Indexed: 01/22/2024]
Abstract
PURPOSE To optimize real-time PCR assays for diagnosis of Bacterial Vaginosis (BV) and determine cut-off loads by ROC analysis for Gardnerella vaginalis, Atopobium vaginae and Lactobacillus spp. as compared to Nugent scoring (Gold standard) in clinical samples. RESULTS Out of 125 women, 34 were positive, 26 intermediate and 65 negative for BV by Nugent scoring. All three real-time PCR assays were found to be highly sensitive & specific and AUC suggested excellent diagnostic accuracy. An optimal cut-off was >9.45 × 103 copies/ ml, >3.34 × 103 copies/ ml & ≤ 18.63 × 103 copies/ ml for G. vaginalis, A. vaginae and Lactobacillus spp. respectively, in BV positives. Gram staining and qPCR were discordant only in patients with intermediate scores (n = 26) where qPCR identified 15 (57.69%) as positive and 11 (42.3%) as negative. CONCLUSION PCR-based molecular BV diagnosis is more accurate and can be used for deciphering intermediate Nugent scores.
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Affiliation(s)
- R Mala
- Department of Microbiology, AIIMS, New Delhi, India
| | - S Malhotra
- Department of Microbiology, AIIMS, New Delhi, India
| | - N Singh
- Department of Obstetrics & Gynaecology, AIIMS, New Delhi, India
| | - S Gupta
- Department of Dermatology & Venereology, AIIMS, New Delhi, India
| | - D A Upadhyay
- Department of Biostatistics, AIIMS, New Delhi, India
| | - A Kapil
- Department of Microbiology, AIIMS, New Delhi, India
| | - S Sood
- Department of Microbiology, AIIMS, New Delhi, India.
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Thomas HA, Singh N, Thomas AM, Masih S, Cherian JM, Varghese KG. Effect of protective coating agents on microleakage and flexural strength of glass ionomer cement and zirconomer. an in vitro study. Eur Arch Paediatr Dent 2024; 25:57-63. [PMID: 37991624 DOI: 10.1007/s40368-023-00853-8] [Citation(s) in RCA: 0] [Impact Index Per Article: 0] [Reference Citation Analysis] [What about the content of this article? (0)] [Affiliation(s)] [Abstract] [Key Words] [MESH Headings] [Track Full Text] [Journal Information] [Subscribe] [Scholar Register] [Received: 07/18/2023] [Accepted: 10/25/2023] [Indexed: 11/23/2023]
Abstract
PURPOSE The objective of this study was to assess the microleakage and flexural strength of glass ionomer cement (GIC) and modified GIC (Zirconomer) when coated with protective coating agents such as COAT-IT and G-COAT plus. METHODS Sixty tooth specimens were grouped into two groups based on the type of restorations (GIC (n = 30) and Zirconomer (n = 30)). The samples were further divided into three subgroups (n = 10) based on the protective coating agent (Petroleum jelly, G-COAT Plus, or COAT IT) applied. This study evaluated the microleakage at the occlusal and cervical margins of class V restoration after being subjected to dye penetration and sectioning. Each specimen was viewed under a 40 × microscope and was given scores based on the depth of dye penetration. They were statistically analyzed using the Kruskal-Wallis test and compared within the groups using the Mann- Whitney Test. In addition, flexural strength was assessed using standardized cuboid (25 × 2 × 2 mm) specimens of restorative materials with and without protective coating agents. The mean flexural strength data of all the subgroups were statistically evaluated using a one-way analysis of variance (ANOVA) and compared within the subgroups using the student t test. RESULTS A statistically significant difference was found when occlusal margin microleakage scores were evaluated with G-COAT Plus demonstrating the lowest occlusal margin microleakage when applied over GIC restoration. The increasing order of occlusal margin microleakage scores is as follows: GIC with G-COAT Plus, Zirconomer with COAT-IT, GIC with COAT-IT, GIC, Zirconomer with G-COAT Plus, and Zirconomer. However, the cervical margin microleakage scores revealed no significant difference. While flexural strength was found to be highest for the GIC group coated with G-COAT Plus, it was observed that there was a significant improvement in the flexural strength of both GIC and Zirconomer when coated with either of the protective coating agents. CONCLUSION Within the limitations of this in vitro study, it was observed that the application of protective coating agents can significantly reduce the potential microleakage and improve the flexural strength of the restorative material especially when zirconia-reinforced GIC is the restorative material.
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Affiliation(s)
- H A Thomas
- Department of Pedodontics and Preventive Dentistry, Christian Dental College, Ludhiana, Punjab, India.
| | - N Singh
- Department of Pedodontics and Preventive Dentistry, Christian Dental College, Ludhiana, Punjab, India
| | - A M Thomas
- Department of Pedodontics and Preventive Dentistry, Christian Dental College, Ludhiana, Punjab, India
| | - S Masih
- Department of Pedodontics and Preventive Dentistry, Christian Dental College, Ludhiana, Punjab, India
| | - J M Cherian
- Department of Pedodontics and Preventive Dentistry, Christian Dental College, Ludhiana, Punjab, India
| | - K G Varghese
- Department of Prosthodontics and Crown and Bridge, Christian Dental College, Ludhiana, Punjab, India
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Park S, Bong SY, Sharma S, Singh N, Park YI, Park J, Ok Jang D. Simple turn-on fluorescent chemosensor for ultrafast and highly selective trace-level detection of Cu 2+ ions in aqueous solutions. Spectrochim Acta A Mol Biomol Spectrosc 2024; 305:123555. [PMID: 37871525 DOI: 10.1016/j.saa.2023.123555] [Citation(s) in RCA: 0] [Impact Index Per Article: 0] [Reference Citation Analysis] [What about the content of this article? (0)] [Affiliation(s)] [Abstract] [Key Words] [Track Full Text] [Subscribe] [Scholar Register] [Received: 07/27/2023] [Revised: 10/14/2023] [Accepted: 10/16/2023] [Indexed: 10/25/2023]
Abstract
A benzimidazole-based probe, BIPMA (2-(1H-benzo[d]imidazol-2-yl)-N-(pyridin-2-ylmethyl)aniline), was designed and synthesized to detect Cu2+ ions. BIPMA exhibited a fluorescent "turn-on" mechanism when bound to Cu2+ ions in an acetonitrile/water mixture (5:5, v/v, HEPES 10 mM, pH 7.4) owing to the synergistic effect of the chelation-enhanced fluorescence and internal charge-transfer mechanisms. Moreover, the BIPMA probe effectively detected nanomolar-range concentrations (0-400 nM) of Cu2+ ions in an aqueous system with a detection limit of 4.80 nM; this value is significantly lower than that set by the U.S. Environmental Protection Agency (≈20 μM). Additionally, BIPMA showed an ultrafast response to Cu2+ ions, with a maximum intensity achieved 25 s after adding Cu2+. Furthermore, BIPMA detected Cu2+ ions in solutions with a pH range of 5-11, without being influenced by pH, underscoring its applicability under various physiological conditions. Density functional theory studies revealed that internal charge transfer was responsible for emission. Finally, BIPMA effectively detected Cu2+ ions in real water samples and living cells.
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Affiliation(s)
- Seonmin Park
- Department of Chemistry, Yonsei University, Wonju 26493, Republic of Korea
| | - So Yeon Bong
- Department of Chemistry, Yonsei University, Wonju 26493, Republic of Korea
| | - Shilpa Sharma
- Department of Chemistry, Indian Institute of Technology Ropar, Rupnagar, Punjab 140001, India
| | - Narinder Singh
- Department of Chemistry, Indian Institute of Technology Ropar, Rupnagar, Punjab 140001, India.
| | - Yea-In Park
- Division of Biological Science and Technology, Yonsei University, Wonju 26493, Republic of Korea
| | - Junsoo Park
- Division of Biological Science and Technology, Yonsei University, Wonju 26493, Republic of Korea
| | - Doo Ok Jang
- Department of Chemistry, Yonsei University, Wonju 26493, Republic of Korea.
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Smith AL, Smit AK, Laginha BI, Singh N, Gallo B, Martin L, Cust AE. Implementing systematic melanoma risk assessment and risk-tailored surveillance in a skin cancer focussed dermatology clinic: A qualitative study of feasibility and acceptability to patients and clinic staff. Cancer Med 2024; 13:e6976. [PMID: 38379327 PMCID: PMC10839129 DOI: 10.1002/cam4.6976] [Citation(s) in RCA: 0] [Impact Index Per Article: 0] [Reference Citation Analysis] [What about the content of this article? (0)] [Affiliation(s)] [Abstract] [Key Words] [MESH Headings] [Grants] [Track Full Text] [Journal Information] [Subscribe] [Scholar Register] [Received: 10/11/2023] [Revised: 01/10/2024] [Accepted: 01/18/2024] [Indexed: 02/22/2024] Open
Abstract
BACKGROUND International bodies recommend that melanoma risk assessment should be integrated into skin cancer care provision, but evidence to support implementation is lacking. AIM To explore the acceptability and feasibility of implementing personalised melanoma risk assessment and tailored patient education and skin surveillance within routine clinical care. METHODS This prospective qualitative implementation study was informed by the Theoretical Framework of Acceptability (TFA). Personalised, systematic melanoma risk assessment was implemented in the dermatology clinic at the Melanoma Institute Australia, Sydney, Australia February-May 2021. Pre- and post-implementation observations and semi-structured interviews with patients and staff were conducted (September 2020-March 2021). Observational notes and interview transcript data were analysed thematically using the TFA as a classifying framework. RESULTS A total of 37 h of observations were made, and 29 patients and 12 clinic staff were interviewed. We found that the delivery of personalised melanoma risk estimates did not impact on patient flow through the clinic. Dermatologists reported that the personalised risk information enhanced their confidence in assessing patient risk and recommending tailored surveillance schedules. Most patients reported that the risk assessment and tailored information were a beneficial addition to their care. Among patients whose risk deviated from their expectations, some reported feeling worried, confused or mistrust in the risk information, including those at lower risk who were recommended to decrease surveillance frequency. CONCLUSIONS It is feasible and acceptable to patients and clinic staff to calculate and deliver personalised melanoma risk information and tailored surveillance as part of routine clinical care within dermatology clinics.
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Affiliation(s)
- A. L. Smith
- The Daffodil CentreThe University of Sydney, a joint venture with Cancer Council NSWSydneyNew South WalesAustralia
| | - A. K. Smit
- The Daffodil CentreThe University of Sydney, a joint venture with Cancer Council NSWSydneyNew South WalesAustralia
- Melanoma Institute Australia, The University of SydneySydneyNew South WalesAustralia
- Faculty of Medicine and Health, Sydney School of Public HealthThe University of SydneySydneyNew South WalesAustralia
| | - B. I. Laginha
- Australian Institute of Health Innovation, Macquarie UniversitySydneyNew South WalesAustralia
| | - N. Singh
- The Daffodil CentreThe University of Sydney, a joint venture with Cancer Council NSWSydneyNew South WalesAustralia
- Australian Institute of Health Innovation, Macquarie UniversitySydneyNew South WalesAustralia
| | - B. Gallo
- Melanoma Institute Australia, The University of SydneySydneyNew South WalesAustralia
| | - L. Martin
- Melanoma Institute Australia, The University of SydneySydneyNew South WalesAustralia
- Faculty of Medicine and HealthUniversity of New South WalesSydneyNew South WalesAustralia
| | - A. E. Cust
- The Daffodil CentreThe University of Sydney, a joint venture with Cancer Council NSWSydneyNew South WalesAustralia
- Melanoma Institute Australia, The University of SydneySydneyNew South WalesAustralia
- Faculty of Medicine and Health, Sydney School of Public HealthThe University of SydneySydneyNew South WalesAustralia
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9
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Khatri H, Salati H, Wong E, Bradshaw K, Inthavong K, Sacks R, Singh N. Modelling the effects of post-FESS middle turbinate synechiae on sinonasal physiology: A computational fluid dynamics study. Auris Nasus Larynx 2023; 50:911-920. [PMID: 37137797 DOI: 10.1016/j.anl.2023.04.003] [Citation(s) in RCA: 2] [Impact Index Per Article: 2.0] [Reference Citation Analysis] [What about the content of this article? (0)] [Affiliation(s)] [Abstract] [Key Words] [MESH Headings] [Track Full Text] [Journal Information] [Subscribe] [Scholar Register] [Received: 11/20/2022] [Revised: 03/23/2023] [Accepted: 04/11/2023] [Indexed: 05/05/2023]
Abstract
OBJECTIVE(S) Chronic rhinosinusitis (CRS) is common and often requires surgical intervention. Surgical failure may lead to persistent symptoms and recalcitrant disease, often secondary to synechiae between the middle turbinate (MT) and lateral nasal wall. Synechiae prevention techniques have been extensively investigated, however evidence for the effect of synechiae on sinonasal physiology is lacking. We aimed to model the effects of MT synechiae on a post-functional endoscopic sinus surgery (FESS) sinonasal cavity using computational fluid dynamics (CFD). METHODS DICOM data from a CT-sinus of a healthy 25-year-old female was segmented to create a three-dimensional model. Virtual surgery was performed to simulate a "full-house" FESS procedure. Multiple models were created, each with a single unilateral virtual MT synechia of varying extent. CFD analysis was performed on each model and compared with a post-FESS control model without synechiae. Airflow velocity, humidity and mucosal surface and air temperature values were calculated. RESULTS All synechiae models demonstrated aberrant downstream sinonasal airflow. There was reduced ventilation of the ipsilateral frontal, ethmoid and sphenoid sinuses, with a concentrated central "jet" in the middle meatus region. Effects were proportionate to the size of synechiae. The impact on bulk inspired airflow was negligible. CONCLUSION Post-FESS synechiae between the MT and lateral nasal wall significantly disrupt local downstream sinus ventilation and nasal airflow. These findings may explain the persistent symptoms seen in post-FESS CRS patients with MT synechiae, reinforcing the importance of prevention and adhesiolysis. Larger cohort studies with multiple models of actual post-FESS patients with synechiae are required to validate these findings.
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Affiliation(s)
- Hershil Khatri
- Department of Otolaryngology, University of Sydney, Sydney, NSW, Australia
| | - Hana Salati
- School of Engineering, Royal Melbourne Institute of Technology, Melbourne, Vic, Australia
| | - Eugene Wong
- Department of Otolaryngology, University of Sydney, Sydney, NSW, Australia
| | - Kimberley Bradshaw
- Department of Otolaryngology, University of Sydney, Sydney, NSW, Australia
| | - Kiao Inthavong
- School of Engineering, Royal Melbourne Institute of Technology, Melbourne, Vic, Australia.
| | - Raymond Sacks
- Department of Otolaryngology, University of Sydney, Sydney, NSW, Australia
| | - Narinder Singh
- Department of Otolaryngology, University of Sydney, Sydney, NSW, Australia
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10
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Taylor A, Habib AR, Kumar A, Wong E, Hasan Z, Singh N. An artificial intelligence algorithm for the classification of sphenoid sinus pneumatisation on sinus computed tomography scans. Clin Otolaryngol 2023; 48:888-894. [PMID: 37488094 DOI: 10.1111/coa.14088] [Citation(s) in RCA: 0] [Impact Index Per Article: 0] [Reference Citation Analysis] [What about the content of this article? (0)] [Affiliation(s)] [Abstract] [Key Words] [Track Full Text] [Journal Information] [Subscribe] [Scholar Register] [Received: 07/15/2022] [Revised: 02/17/2023] [Accepted: 06/18/2023] [Indexed: 07/26/2023]
Abstract
BACKGROUND Classifying sphenoid pneumatisation is an important but often overlooked task in reporting sinus CT scans. Artificial intelligence (AI) and one of its key methods, convolutional neural networks (CNNs), can create algorithms that can learn from data without being programmed with explicit rules and have shown utility in radiological image classification. OBJECTIVE To determine if a trained CNN can accurately classify sphenoid sinus pneumatisation on CT sinus imaging. METHODS Sagittal slices through the natural ostium of the sphenoid sinus were extracted from retrospectively collected bone-window CT scans of the paranasal sinuses for consecutive patients over 6 years. Two blinded Otolaryngology residents reviewed each image and classified the sphenoid sinus pneumatisation as either conchal, presellar or sellar. An AI algorithm was developed using the Microsoft Azure Custom Vision deep learning platform to classify the pattern of pneumatisation. RESULTS Seven hundred eighty images from 400 patients were used to train the algorithm, which was then tested on a further 118 images from 62 patients. The algorithm achieved an accuracy of 93.2% (95% confidence interval [CI] 87.1-97.0), 87.3% (95% CI 79.9-92.7) and 85.6% (95% CI 78.0-91.4) in correctly identifying conchal, presellar and sellar sphenoid pneumatisation, respectively. The overall weighted accuracy of the CNN was 85.9%. CONCLUSION The CNN described demonstrated a moderately accurate classification of sphenoid pneumatisation subtypes on CT scans. The use of CNN-based assistive tools may enable surgeons to achieve safer operative planning through routine automated reporting allowing greater resources to be directed towards the identification of pathology.
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Affiliation(s)
- Alon Taylor
- Department of Otolaryngology - Head and Neck Surgery, Westmead Hospital, Westmead, New South Wales, Australia
| | - Al-Rahim Habib
- Department of Otolaryngology - Head and Neck Surgery, Westmead Hospital, Westmead, New South Wales, Australia
- Faculty of Medicine and Health, University of Sydney, Sydney, New South Wales, Australia
| | - Ashnil Kumar
- School of Biomedical Engineering, Faculty of Engineering, University of Sydney, Sydney, New South Wales, Australia
- ARC Training Centre for Innovative BioEngineering, Sydney, New South Wales, Australia
| | - Eugene Wong
- Department of Otolaryngology - Head and Neck Surgery, Westmead Hospital, Westmead, New South Wales, Australia
- Westmead Clinical School, Faculty of Medicine and Health, University of Sydney, Sydney, New South Wales, Australia
| | - Zubair Hasan
- Department of Otolaryngology - Head and Neck Surgery, Westmead Hospital, Westmead, New South Wales, Australia
| | - Narinder Singh
- Department of Otolaryngology - Head and Neck Surgery, Westmead Hospital, Westmead, New South Wales, Australia
- Westmead Clinical School, Faculty of Medicine and Health, University of Sydney, Sydney, New South Wales, Australia
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11
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Ranbir, Singh G, Singh H, Kaur N, Singh N. Portable Sensor Array for On-Site Detection and Discrimination of Pesticides and Herbicides Using Multivariate Analysis. Anal Chem 2023; 95:14533-14540. [PMID: 37726218 DOI: 10.1021/acs.analchem.3c01331] [Citation(s) in RCA: 1] [Impact Index Per Article: 1.0] [Reference Citation Analysis] [What about the content of this article? (0)] [Affiliation(s)] [Abstract] [MESH Headings] [Track Full Text] [Journal Information] [Subscribe] [Scholar Register] [Indexed: 09/21/2023]
Abstract
Modern agricultural practice relies heavily on pesticides and herbicides to increase crop productivity, and consequently, their residues have a negative impact on the environment and public health. Thus, keeping these issues in account, herein we developed an azodye-based chromogenic sensor array for the detection and discrimination of pesticides and herbicides in food and soil samples, utilizing machine learning approaches such as hierarchical clustering analysis, principal component analysis, linear discriminant analysis (LDA), and partial least square regression (PLSR). The azodye-based sensor array was developed in combination with various metal ions owing to their different photophysical properties, which led to distinct patterns toward various pesticides and herbicides. The obtained distinct patterns were recognized and processed through automated multivariate analysis, which enables the selective and sensitive identification and discrimination of various target analytes. Further, the qualitative and quantitative determination of target analytes were performed using LDA and PLSR; the results obtained show a linear correlation with varied concentrations of target analytes with R2 values from 0.89 to 0.96, the limit of detection from 5.3 to 11.8 ppm with a linear working range from 1 to 30 μM toward analytes under investigation. Further, the developed sensor array was successfully utilized for the discrimination of a binary mixture of pesticide (chlorpyrifos) and herbicide (glyphosate).
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Affiliation(s)
- Ranbir
- Department of Chemistry, Indian Institute of Technology Ropar, Rupnagar, Punjab 140001, India
| | - Gagandeep Singh
- Department of Biomedical Engineering, Indian Institute of Technology Ropar, Rupnagar, Punjab 140001, India
| | - Harupjit Singh
- Department of Biomedical Engineering, Indian Institute of Technology Ropar, Rupnagar, Punjab 140001, India
| | - Navneet Kaur
- Department of Chemistry, Panjab University, Chandigarh, Punjab160014, India
| | - Narinder Singh
- Department of Chemistry, Indian Institute of Technology Ropar, Rupnagar, Punjab 140001, India
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12
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Hasan Z, Key S, Lee M, Chen F, Aweidah L, Esmaili A, Sacks R, Singh N. A Deep Learning Algorithm to Identify Anatomical Landmarks on Computed Tomography of the Temporal Bone. J Int Adv Otol 2023; 19:360-367. [PMID: 37789621 PMCID: PMC10645193 DOI: 10.5152/iao.2023.231073] [Citation(s) in RCA: 0] [Impact Index Per Article: 0] [Reference Citation Analysis] [What about the content of this article? (0)] [Affiliation(s)] [Abstract] [Key Words] [MESH Headings] [Track Full Text] [Journal Information] [Subscribe] [Scholar Register] [Received: 01/22/2023] [Accepted: 05/18/2023] [Indexed: 10/05/2023] Open
Abstract
BACKGROUND Petrous temporal bone cone-beam computed tomography scans help aid diagnosis and accurate identification of key operative landmarks in temporal bone and mastoid surgery. Our primary objective was to determine the accuracy of using a deep learning convolutional neural network algorithm to augment identification of structures on petrous temporal bone cone-beam computed tomography. Our secondary objective was to compare the accuracy of convolutional neural network structure identification when trained by a senior versus junior clinician. METHODS A total of 129 petrous temporal bone cone-beam computed tomography scans were obtained from an Australian public tertiary hospital. Key intraoperative landmarks were labeled in 68 scans using bounding boxes on axial and coronal slices at the level of the malleoincudal joint by an otolaryngology registrar and board-certified otolaryngologist. Automated structure identification was performed on axial and coronal slices of the remaining 61 scans using a convolutional neural network (Microsoft Custom Vision) trained using the labeled dataset. Convolutional neural network structure identification accuracy was manually verified by an otolaryngologist, and accuracy when trained by the registrar and otolaryngologist labeled datasets respectively was compared. RESULTS The convolutional neural network was able to perform automated structure identification in petrous temporal bone cone-beam computed tomography scans with a high degree of accuracy in both axial (0.958) and coronal (0.924) slices (P < .001). Convolutional neural network accuracy was proportionate to the seniority of the training clinician in structures with features more difficult to distinguish on single slices such as the cochlea, vestibule, and carotid canal. CONCLUSION Convolutional neural networks can perform automated structure identification in petrous temporal bone cone-beam computed tomography scans with a high degree of accuracy, with the performance being proportionate to the seniority of the training clinician. Training of the convolutional neural network by the most senior clinician is desirable to maximize the accuracy of the results.
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Affiliation(s)
- Zubair Hasan
- University of Sydney, Faculty of Medicine and Health, New South Wales, Australia
- Department of Otolaryngology - Head and Neck Surgery, Westmead Hospital, New South Wales, Australia
| | - Seraphina Key
- Monash University, Faculty of Medicine, Nursing and Health Sciences, Victoria, Australia
| | - Michael Lee
- University of Sydney, Faculty of Medicine and Health, New South Wales, Australia
| | - Fiona Chen
- Department of Otolaryngology, Royal Children’s Hospital Melbourne, Melbourne, Australia
| | - Layal Aweidah
- Department of Otolaryngology - Head and Neck Surgery, Westmead Hospital, New South Wales, Australia
| | - Aaron Esmaili
- Department of Otolaryngology, Sir Charles Gairdner Hospital, Nedlands, Australia
| | - Raymond Sacks
- University of Sydney, Faculty of Medicine and Health, New South Wales, Australia
- Department of Otolaryngology - Head and Neck Surgery, Concord Hospital, New South Wales, Australia
| | - Narinder Singh
- University of Sydney, Faculty of Medicine and Health, New South Wales, Australia
- Department of Otolaryngology - Head and Neck Surgery, Westmead Hospital, New South Wales, Australia
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13
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Singh H, Brar P, Honparkhe M, Singh N, Jan MH, Maharana BR, Dadarwal D. Local and systemic inflammatory response to the intrauterine infusion of enzymes during estrus in water buffaloes with subclinical endometritis. Res Vet Sci 2023; 162:104951. [PMID: 37442014 DOI: 10.1016/j.rvsc.2023.104951] [Citation(s) in RCA: 0] [Impact Index Per Article: 0] [Reference Citation Analysis] [What about the content of this article? (0)] [Affiliation(s)] [Abstract] [Key Words] [MESH Headings] [Track Full Text] [Journal Information] [Subscribe] [Scholar Register] [Received: 04/06/2023] [Revised: 06/07/2023] [Accepted: 07/02/2023] [Indexed: 07/15/2023]
Abstract
Our objective was to determine the effects of intrauterine infusion of proteolytic enzymes in buffaloes with subclinical endometritis (SCE) at estrus on the resolution of endometrial inflammation and reproductive performance. Buffaloes at spontaneous estrus (E1) were screened for SCE by endometrial cytology to identify SCE (≥5% PMN, n = 22) and non-SCE (<5% PMNs, n = 14) animals. All buffaloes underwent uterine ultrasonographic examination, low volume uterine lavage (cytokines and acute phase proteins) and blood sampling (cytokines and acute-phase proteins) at E1. On the same day (E1), SCE buffaloes were randomly selected either for intrauterine infusion of proteolytic enzymes (ENY, n = 11) or saline (PC, n = 11). Buffaloes without SCE were kept as untreated control (NC; n = 14). All buffaloes were re-examined and re-sampled during subsequent estrus (E2), inseminated during the following estrus (E3), and assessed for fertility related outcomes. Proteolytic infusion resulted a reduction in uterine PMN (P < 0.01) in SCE buffaloes. The concentrations of interleukin (IL)-1β and tumor necrosis factor (TNF)-α in uterus, and TNF-α and IL-10 in serum were higher (P < 0.01) at E1 in buffaloes with SCE (PC and ENY) compared to NC. After treatment, uterine IL-1β and TNF-α (P = 0.02), and serum TNF-α and IL-10 were lower within the animals of ENY group (P < 0.01). Before treatment, buffaloes with SCE had higher concentrations (P < 0.01) of serum and uterine amyloid-A and haptoglobin, which decreased (P < 0.01) after treatment in the ENY group. None of the fertility outcomes differ between the treatment groups. In conclusion, intrauterine infusion of proteolytic enzymes reduced endometrial inflammation; however, did not improve reproductive outcomes.
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Affiliation(s)
- Harpreet Singh
- Regional Centre, Lala Lajpat Rai University of Veterinary and Animal Sciences, Karnal, Haryana, India
| | - Parkash Brar
- Veterinary Gynecology and Obstetrics, Guru Angad Dev Veterinary and Animal Sciences University, Ludhiana, Punjab, India
| | - Mrigank Honparkhe
- Veterinary Gynecology and Obstetrics, Guru Angad Dev Veterinary and Animal Sciences University, Ludhiana, Punjab, India
| | - Narinder Singh
- Directorate of Livestock Farms, Guru Angad Dev Veterinary and Animal Sciences University, Ludhiana, India
| | - Mustafa Hassan Jan
- ICAR-Central Institute for Research on Buffaloes, Sub Campus Bir Dosanjh, Nabha, Punjab, India
| | - Biswa Ranjan Maharana
- Regional Centre, Lala Lajpat Rai University of Veterinary and Animal Sciences, Karnal, Haryana, India
| | - Dinesh Dadarwal
- Large Animal Clinical Sciences, Western College of Veterinary Medicine, 52 Campus Drive, University of Saskatchewan, Saskatoon, SK, Canada.
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14
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Pezato R, Stamm AC, Douglas R, Han JK, Chen PG, Neto CDP, Tepedino MS, Singh N, Balsalobre L, Ryu CH, Gregório L, Almatrafi S, Felippu AWD, Iturriaga E, Toledo RN, Cascio F, Dassi C, Alkholaiwi F, Bezerra TFP, Javer A, Dutra DL, Psaltis AJ, Migueis DP, Almutari N, Avelino MAG, Gunaratne DA, Felippu A, Pinna FDR, Nakanishi M, Perez-Novo CA, Singhera GK, Choby G, Wang EW, Patel ZM, Thamboo A. Nasal disease with polyps: Need for clarity. Int Forum Allergy Rhinol 2023; 13:1829-1831. [PMID: 36869634 DOI: 10.1002/alr.23150] [Citation(s) in RCA: 0] [Impact Index Per Article: 0] [Reference Citation Analysis] [What about the content of this article? (0)] [Affiliation(s)] [MESH Headings] [Track Full Text] [Journal Information] [Subscribe] [Scholar Register] [Received: 01/10/2023] [Revised: 02/24/2023] [Accepted: 02/28/2023] [Indexed: 03/05/2023]
Affiliation(s)
- Rogerio Pezato
- Division of Rhinology, University of British Columbia, Vancouver, Canada
| | - Aldo Cassol Stamm
- Ear, Nose, and Throat (ENT) and Skull Base Surgery, Hospital Edmundo Vasconcellos, São Paulo, Brazil
| | - Richard Douglas
- Department of Surgery, University of Auckland, Auckland, New Zealand
| | - Joseph K Han
- Division of Endoscopy and Endoscopic Sinus and Skull Base Surgery, Eastern Virginia Medical School, Norflok, United States
| | - Philip G Chen
- Department of Otolaryngology-Head and Neck Surgery, University of Texas Health Science Center, San Antonio, United States
| | | | - Miguel Soares Tepedino
- Rhinology and Skull Base Division, Universidade do Estado do Rio de Janeiro, Rio de Janeiro, Brazil
| | - Narinder Singh
- Department of Otolaryngology-Head and Neck Surgery, Sydney Medical School, University of Sidney, Sydney, Australia
| | - Leonardo Balsalobre
- Ear, Nose, and Throat (ENT) and Skull Base Surgery, Hospital Edmundo Vasconcellos, São Paulo, Brazil
| | - Chang Hwan Ryu
- Department of Otolaryngology-Head and Neck Surgery, National Cancer Center, Goyang-si, South Korea
| | - Luciano Gregório
- Department of Otorhinolaryngology-Head and Neck Surgery, Federal University of São Paulo, São Paulo, Brazil
| | - Sharif Almatrafi
- Department of Otolaryngology-Head and Neck Surgery, College of Medicine, Prince Sattam Bin Abdulaziz University, Alkharj, Saudi Arabia
| | | | - Enrique Iturriaga
- Department of ENT and HSN/Skull Base Program, Centro Médico Caracas, Caracas, Venezuela
| | - Ronaldo Nunes Toledo
- Department of Otorhinolaryngology-Head and Neck Surgery, ACCamargo Cancer Center, São Paulo, Brazil
| | - Filippo Cascio
- Department of Otorhinolaryngology, Parpado Hospital, Messina, Italy
| | - Camilla Dassi
- Department of Otorhinolaryngology-Head and Neck Surgery, Federal University of São Paulo, São Paulo, Brazil
| | - Feras Alkholaiwi
- Department of Otolaryngology-Head and Neck Surgery, College of Medicine, Imam Mohammad Ibn Saud Islamic University, Riyadh, Saudi Arabia
| | | | - Amin Javer
- Division of Rhinology, University of British Columbia, Vancouver, Canada
| | - Daniel Lorena Dutra
- Department of Otolaryngology-Head and Neck Surgery, Adelaide University, Adelaide, Australia
| | - Alkis James Psaltis
- Department of Otolaryngology-Head and Neck Surgery, Adelaide University, Adelaide, Australia
| | | | - Nasser Almutari
- Department of Otolaryngology-Head and Neck Surgery, Alfaisal University, Riyadh, Saudi Arabia
| | | | | | - Alexandre Felippu
- Department of Otorhinolaryngology, Instituto Fellipo de Otorrinolaringologia, São Paulo, Brazil
| | - Fábio de Rezende Pinna
- Department of Ophthalmology and Otorhinolaryngology, Universidade de São Paulo, São Paulo, Brazil
| | - Márcio Nakanishi
- Medical Sciences Faculty of Medicine, Universidade de Brasília, Brasília, Brazil
| | | | - Gurpreet K Singhera
- Department of Medicine, Division of Respirology, Faculty of Medicine, University of British Columbia, Vancouver, Canada
| | - Garret Choby
- Department of Otolaryngology-Head and Neck Surgery, Mayo Clinic, Rochester, United States
| | - Eric W Wang
- Department of Otolaryngology, Ophthalmology and Neurological Surgery, University of Pittsburgh, Pittsburg, USA
| | - Zara M Patel
- Division of Rhinology, Department of Otolaryngology-Head and Neck Surgery, Stanford School of Medicine, Palo Alto, USA
| | - Andrew Thamboo
- Division of Rhinology, University of British Columbia, Vancouver, Canada
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15
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Singh A, Singh G, Kaur N, Singh N. Fabrication of FRET based nano sensor from biomass-derived fluorescent carbon quantum dots and naphthalimide for ratiometric detection of nitric oxide: To examine nitrite levels in meat samples. Anal Chim Acta 2023; 1270:341444. [PMID: 37311616 DOI: 10.1016/j.aca.2023.341444] [Citation(s) in RCA: 1] [Impact Index Per Article: 1.0] [Reference Citation Analysis] [What about the content of this article? (0)] [Affiliation(s)] [Abstract] [Key Words] [Track Full Text] [Journal Information] [Subscribe] [Scholar Register] [Received: 04/13/2023] [Revised: 05/22/2023] [Accepted: 05/26/2023] [Indexed: 06/15/2023]
Abstract
Nitric oxide (NO) is a ubiquitous, gaseous, free radical signaling molecule which plays a key role in physiological and pathological processes. Literature reports revealed that the conventional methods such as colorimetry, electron paramagnetic resonance (EPR), electrochemical etc. to detect NO are costly, time consuming and lack resolution, particularly in aqueous or biological system. Thus, in this context, herein we have developed covalently linked biomass derived carbon quantum dots (CQDs) and naphthalimide based nano sensor system for FRET based ratiometric detection of nitric oxide (NO) in pure aqueous media. The CQDs derived from orange peels were characterized using UV-visible absorption, fluorescence spectroscopy, PXRD, TEM, FT-IR and zeta potential studies. Further, the obtained CQDs were functionalized with amine functionality, and subsequently linked with naphthalimide derivative (5) using terephthaldehyde through covalent bond formation. The conjugation of naphthalimide (5) and functionalized CQDs was studied using DLS, zeta potential, FT-IR and time resolved fluorescence spectroscopy. The excitation of developed nano sensor system at λex 360 nm results in fluorescence emission at λem 530 nm which establishes the FRET pair between the CQDs and naphthalimide unit. However, in the presence of NO, the observed FRET pair abolishes due to the cleavage of NO susceptible imine bond. The developed sensor demonstrates high selectivity towards NO with limit of detection (LOD) and limit of quantification (LOQ) of 15 nM and 50 nM respectively. Further, the developed sensor system was also utilized for indirect detection of nitrite (NO2-) in food samples for food safety and monitoring.
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Affiliation(s)
- Amanpreet Singh
- Department of Chemistry, Indian Institute of Technology Ropar, Punjab, 140001, India
| | - Gagandeep Singh
- Department of Biomedical Engineering, Indian Institute of Technology Ropar, Punjab, 140001, India
| | - Navneet Kaur
- Department of Chemistry, Panjab University, Chandigarh, 160014, India.
| | - Narinder Singh
- Department of Chemistry, Indian Institute of Technology Ropar, Punjab, 140001, India.
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16
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Acernese F, Agathos M, Ain A, Albanesi S, Alléné C, Allocca A, Amato A, Amra C, Andia M, Andrade T, Andres N, Andrés-Carcasona M, Andrić T, Ansoldi S, Antier S, Apostolatos T, Appavuravther EZ, Arène M, Arnaud N, Assiduo M, Melo SADS, Astone P, Aubin F, Babak S, Badaracco F, Bagnasco S, Baird J, Baka T, Ballardin G, Baltus G, Banerjee B, Barneo P, Barone F, Barsuglia M, Barta D, Basti A, Bawaj M, Bazzan M, Beirnaert F, Bejger M, Benedetto V, Berbel M, Bernuzzi S, Bersanetti D, Bertolini A, Bhardwaj U, Bianchi A, Bilicki M, Bini S, Bischi M, Bitossi M, Bizouard MA, Bobba F, Boër M, Bogaert G, Boileau G, Boldrini M, Bonavena LD, Bondarescu R, Bondu F, Bonnand R, Boschi V, Boudart V, Bouffanais Y, Bozzi A, Bradaschia C, Braglia M, Branchesi M, Breschi M, Briant T, Brillet A, Brooks J, Bruno G, Bucci F, Bulashenko O, Bulik T, Bulten HJ, Buscicchio R, Buskulic D, Buy C, Cabras G, Cabrita R, Cagnoli G, Calloni E, Canepa M, Santoro GC, Cannavacciuolo M, Capocasa E, Carapella G, Carbognani F, Carpinelli M, Carullo G, Diaz JC, Casentini C, Caudill S, Cavalieri R, Cella G, Cerdá-Durán P, Cesarini E, Chaibi W, Chanial P, Chassande-Mottin E, Chaty S, Chessa P, Chiadini F, Chiarini G, Chierici R, Chincarini A, Chiofalo ML, Chiummo A, Christensen N, Chua S, Ciani G, Ciecielag P, Cieślar M, Cifaldi M, Ciolfi R, Clesse S, Cleva F, Coccia E, Codazzo E, Cohadon PF, Colombo A, Colpi M, Conti L, Cordero-Carrión I, Corezzi S, Cortese S, Coulon JP, Coupechoux JF, Croquette M, Cudell JR, Cuoco E, Curyło M, Dabadie P, Canton TD, Dall'Osso S, Dálya G, D'Angelo B, Dangoisse G, Danilishin S, D'Antonio S, Dattilo V, Davier M, Degallaix J, De Laurentis M, Deléglise S, De Lillo F, Dell'Aquila D, Del Pozzo W, De Matteis F, Depasse A, De Pietri R, De Rosa R, De Rossi C, De Simone R, Di Fiore L, Di Giorgio C, Di Giovanni F, Di Giovanni M, Di Girolamo T, Diksha D, Di Lieto A, Di Michele A, Ding J, Di Pace S, Di Palma I, Di Renzo F, D'Onofrio L, Dooney T, Dorosh O, Drago M, Ducoin JG, Dupletsa U, Durante O, D'Urso D, Duverne PA, Eisenmann M, Errico L, Estevez D, Fabrizi F, Faedi F, Fafone V, Favaro G, Fays M, Fenyvesi E, Ferrante I, Fidecaro F, Figura P, Fiori A, Fiori I, Fittipaldi R, Fiumara V, Flaminio R, Font JA, Frasca S, Frasconi F, Freise A, Freitas O, Fronzé GG, Gadre B, Gamba R, Garaventa B, Garcia-Bellido J, Gargiulo J, Garufi F, Gasbarra C, Gemme G, Gennai A, Ghosh A, Giacoppo L, Giri P, Gissi F, Gkaitatzis S, Glotin F, Goncharov B, Gosselin M, Gouaty R, Grado A, Granata M, Granata V, Greco G, Grignani G, Grimaldi A, Guerra D, Guetta D, Guidi GM, Gulminelli F, Guo Y, Gupta P, Gutierrez N, Haegel L, Halim O, Hannuksela O, Harder T, Haris K, Harmark T, Harms J, Haskell B, Heidmann A, Heitmann H, Hello P, Hemming G, Hennes E, Hennig JS, Hennig M, Hild S, Hofman D, Holland NA, Hui V, Iandolo GA, Idzkowski B, Iess A, Iorio G, Iosif P, Jacqmin T, Jacquet PE, Janquart J, Janssens K, Jaraba S, Jaranowski P, Jasal P, Juste V, Kalaghatgi C, Karathanasis C, Katsanevas S, Kéfélian F, Koekoek G, Koley S, Kolstein M, Kranzhoff SL, Królak A, Kuijer P, Kuroyanagi S, Lagabbe P, Laghi D, Lalleman M, Lamberts A, La Rana A, La Rosa I, Lartaux-Vollard A, Lazzaro C, Leaci P, Lemaître A, Lenti M, Leonova E, Lequime M, Leroy N, Letendre N, Lethuillier M, Leyde K, Linde F, London L, Longo A, Portilla ML, Lorenzini M, Loriette V, Losurdo G, Lumaca D, Macquet A, Magazzù C, Maggiore R, Magnozzi M, Majorana E, Man N, Mangano V, Mantovani M, Mapelli M, Marchesoni F, Pina DM, Marion F, Marquina A, Marsat S, Martelli F, Martinez M, Martinez V, Masserot A, Mastrodicasa M, Mastrogiovanni S, Meijer Q, Menendez-Vazquez A, Mereni L, Merzougui M, Miani A, Michel C, Miller A, Miller B, Milotti E, Minenkov Y, Mir LM, Miravet-Tenés M, Mitchell AL, Mondal C, Montani M, Morawski F, Morras G, Moscatello A, Mours B, Mow-Lowry CM, Msihid E, Muciaccia F, Mukherjee S, Nagar A, Napolano V, Nardecchia I, Narola H, Naticchioni L, Neilson J, Nesseris S, Nguyen C, Nieradka G, Nissanke S, 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Vardaro M, Vasúth M, Vedovato G, Verdier P, Verkindt D, Verma P, Vetrano F, Viceré A, Vinet JY, Viret S, Virtuoso A, Vocca H, Walet RC, Was M, Yadav N, Zadrożny A, Zelenova T, Zendri JP, Zhao Y, Zerrad M, Vahlbruch H, Mehmet M, Lück H, Danzmann K. Frequency-Dependent Squeezed Vacuum Source for the Advanced Virgo Gravitational-Wave Detector. Phys Rev Lett 2023; 131:041403. [PMID: 37566847 DOI: 10.1103/physrevlett.131.041403] [Citation(s) in RCA: 0] [Impact Index Per Article: 0] [Reference Citation Analysis] [What about the content of this article? (0)] [Affiliation(s)] [Abstract] [Track Full Text] [Subscribe] [Scholar Register] [Received: 02/12/2023] [Revised: 04/24/2023] [Accepted: 05/09/2023] [Indexed: 08/13/2023]
Abstract
In this Letter, we present the design and performance of the frequency-dependent squeezed vacuum source that will be used for the broadband quantum noise reduction of the Advanced Virgo Plus gravitational-wave detector in the upcoming observation run. The frequency-dependent squeezed field is generated by a phase rotation of a frequency-independent squeezed state through a 285 m long, high-finesse, near-detuned optical resonator. With about 8.5 dB of generated squeezing, up to 5.6 dB of quantum noise suppression has been measured at high frequency while close to the filter cavity resonance frequency, the intracavity losses limit this value to about 2 dB. Frequency-dependent squeezing is produced with a rotation frequency stability of about 6 Hz rms, which is maintained over the long term. The achieved results fulfill the frequency dependent squeezed vacuum source requirements for Advanced Virgo Plus. With the current squeezing source, considering also the estimated squeezing degradation induced by the interferometer, we expect a reduction of the quantum shot noise and radiation pressure noise of up to 4.5 dB and 2 dB, respectively.
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Affiliation(s)
- F Acernese
- Dipartimento di Farmacia, Università di Salerno, I-84084 Fisciano, Salerno, Italy
- INFN, Sezione di Napoli, I-80126 Napoli, Italy
| | - M Agathos
- Theoretisch-Physikalisches Institut, Friedrich-Schiller-Universität Jena, D-07743 Jena, Germany
| | - A Ain
- INFN, Sezione di Pisa, I-56127 Pisa, Italy
| | - S Albanesi
- Dipartimento di Fisica, Università degli Studi di Torino, I-10125 Torino, Italy
- INFN Sezione di Torino, I-10125 Torino, Italy
| | - C Alléné
- Université Savoie Mont Blanc, CNRS, Laboratoire d'Annecy de Physique des Particules - IN2P3, F-74000 Annecy, France
| | - A Allocca
- INFN, Sezione di Napoli, I-80126 Napoli, Italy
- Università di Napoli "Federico II", I-80126 Napoli, Italy
| | - A Amato
- Maastricht University, 6200 MD Maastricht, Netherlands
- Nikhef, 1098 XG Amsterdam, Netherlands
| | - C Amra
- Institut Fresnel, Faculté des Sciences St Jérôme Avenue Escadrille Normandie-Niemen, F-13013 Marseille, France
| | - M Andia
- Université Paris-Saclay, CNRS/IN2P3, IJCLab, 91405 Orsay, France
| | - T Andrade
- Institut de Ciències del Cosmos (ICCUB), Universitat de Barcelona (UB), carrer Martí i Franquès, 1, 08028 Barcelona, Spain
| | - N Andres
- Université Savoie Mont Blanc, CNRS, Laboratoire d'Annecy de Physique des Particules - IN2P3, F-74000 Annecy, France
| | - M Andrés-Carcasona
- Institut de Física d'Altes Energies (IFAE), Barcelona Institute of Science and Technology, and ICREA, E-08193 Barcelona, Spain
| | - T Andrić
- Gran Sasso Science Institute (GSSI), I-67100 L'Aquila, Italy
| | - S Ansoldi
- Dipartimento di Scienze Matematiche, Informatiche e Fisiche, Università di Udine, I-33100 Udine, Italy
- INFN, Sezione di Trieste, I-34127 Trieste, Italy
| | - S Antier
- Université Côte d'Azur, Observatoire Côte d'Azur, CNRS, Artemis, F-06304 Nice, France
| | - T Apostolatos
- Department of Physics, National and Kapodistrian University of Athens, 15771 Ilissia, Greece
| | - E Z Appavuravther
- INFN, Sezione di Perugia, I-06123 Perugia, Italy
- Università di Camerino, I-62032 Camerino, Italy
| | - M Arène
- Université Paris Cité, CNRS, Astroparticule et Cosmologie, F-75013 Paris, France
| | - N Arnaud
- Université Paris-Saclay, CNRS/IN2P3, IJCLab, 91405 Orsay, France
- European Gravitational Observatory (EGO), I-56021 Cascina, Pisa, Italy
| | - M Assiduo
- Università degli Studi di Urbino "Carlo Bo", I-61029 Urbino, Italy
- INFN, Sezione di Firenze, I-50019 Sesto Fiorentino, Firenze, Italy
| | | | - P Astone
- INFN, Sezione di Roma, I-00185 Roma, Italy
| | - F Aubin
- INFN, Sezione di Firenze, I-50019 Sesto Fiorentino, Firenze, Italy
| | - S Babak
- Université Paris Cité, CNRS, Astroparticule et Cosmologie, F-75013 Paris, France
| | - F Badaracco
- Université catholique de Louvain, B-1348 Louvain-la-Neuve, Belgium
| | - S Bagnasco
- INFN Sezione di Torino, I-10125 Torino, Italy
| | - J Baird
- Université Paris Cité, CNRS, Astroparticule et Cosmologie, F-75013 Paris, France
| | - T Baka
- Institute for Gravitational and Subatomic Physics (GRASP), Utrecht University, 3584 CC Utrecht, Netherlands
| | - G Ballardin
- European Gravitational Observatory (EGO), I-56021 Cascina, Pisa, Italy
| | - G Baltus
- Université de Liège, B-4000 Liège, Belgium
| | - B Banerjee
- Gran Sasso Science Institute (GSSI), I-67100 L'Aquila, Italy
| | - P Barneo
- Institut de Ciències del Cosmos (ICCUB), Universitat de Barcelona (UB), carrer Martí i Franquès, 1, 08028 Barcelona, Spain
- Departament de Física Quàntica i Astrofísica (FQA), Universitat de Barcelona (UB), carrer Martí i Franqués, 1, 08028 Barcelona, Spain
| | - F Barone
- INFN, Sezione di Napoli, I-80126 Napoli, Italy
- Dipartimento di Medicina, Chirurgia e Odontoiatria "Scuola Medica Salernitana", Università di Salerno, I-84081 Baronissi, Salerno, Italy
| | - M Barsuglia
- Université Paris Cité, CNRS, Astroparticule et Cosmologie, F-75013 Paris, France
| | - D Barta
- Wigner RCP, RMKI, H-1121 Budapest, Hungary
| | - A Basti
- INFN, Sezione di Pisa, I-56127 Pisa, Italy
- Università di Pisa, I-56127 Pisa, Italy
| | - M Bawaj
- INFN, Sezione di Perugia, I-06123 Perugia, Italy
- Università di Perugia, I-06123 Perugia, Italy
| | - M Bazzan
- Università di Padova, Dipartimento di Fisica e Astronomia, I-35131 Padova, Italy
- INFN, Sezione di Padova, I-35131 Padova, Italy
| | | | - M Bejger
- Nicolaus Copernicus Astronomical Center, Polish Academy of Sciences, 00-716, Warsaw, Poland
| | - V Benedetto
- Dipartimento di Ingegneria, Università del Sannio, I-82100 Benevento, Italy
| | - M Berbel
- Departamento de Matemáticas, Universitat Autònoma de Barcelona, 08193 Bellaterra (Barcelona), Spain
| | - S Bernuzzi
- Theoretisch-Physikalisches Institut, Friedrich-Schiller-Universität Jena, D-07743 Jena, Germany
| | | | | | - U Bhardwaj
- Nikhef, 1098 XG Amsterdam, Netherlands
- GRAPPA, Anton Pannekoek Institute for Astronomy and Institute for High-Energy Physics, University of Amsterdam, 1098 XH Amsterdam, Netherlands
| | - A Bianchi
- Nikhef, 1098 XG Amsterdam, Netherlands
- Department of Physics and Astronomy, Vrije Universiteit Amsterdam, 1081 HV Amsterdam, Netherlands
| | - M Bilicki
- Center for Theoretical Physics, Polish Academy of Sciences, 02-668 Warsaw, Poland
| | - S Bini
- Università di Trento, Dipartimento di Fisica, I-38123 Povo, Trento, Italy
- INFN, Trento Institute for Fundamental Physics and Applications, I-38123 Povo, Trento, Italy
| | - M Bischi
- Università degli Studi di Urbino "Carlo Bo", I-61029 Urbino, Italy
- INFN, Sezione di Firenze, I-50019 Sesto Fiorentino, Firenze, Italy
| | - M Bitossi
- INFN, Sezione di Pisa, I-56127 Pisa, Italy
- European Gravitational Observatory (EGO), I-56021 Cascina, Pisa, Italy
| | - M-A Bizouard
- Université Côte d'Azur, Observatoire Côte d'Azur, CNRS, Artemis, F-06304 Nice, France
| | - F Bobba
- Dipartimento di Fisica "E.R. Caianiello", Università di Salerno, I-84084 Fisciano, Salerno, Italy
- INFN, Sezione di Napoli, Gruppo Collegato di Salerno, I-80126 Napoli, Italy
| | - M Boër
- Université Côte d'Azur, Observatoire Côte d'Azur, CNRS, Artemis, F-06304 Nice, France
| | - G Bogaert
- Université Côte d'Azur, Observatoire Côte d'Azur, CNRS, Artemis, F-06304 Nice, France
| | - G Boileau
- Université Côte d'Azur, Observatoire Côte d'Azur, CNRS, Artemis, F-06304 Nice, France
- Universiteit Antwerpen, 2000 Antwerpen, Belgium
| | - M Boldrini
- INFN, Sezione di Roma, I-00185 Roma, Italy
- Università di Roma "La Sapienza", I-00185 Roma, Italy
| | - L D Bonavena
- Università di Padova, Dipartimento di Fisica e Astronomia, I-35131 Padova, Italy
| | - R Bondarescu
- Institut de Ciències del Cosmos (ICCUB), Universitat de Barcelona (UB), carrer Martí i Franquès, 1, 08028 Barcelona, Spain
| | - F Bondu
- Univ Rennes, CNRS, Institut FOTON - UMR 6082, F-35000 Rennes, France
| | - R Bonnand
- Université Savoie Mont Blanc, CNRS, Laboratoire d'Annecy de Physique des Particules - IN2P3, F-74000 Annecy, France
| | - V Boschi
- INFN, Sezione di Pisa, I-56127 Pisa, Italy
| | - V Boudart
- Université de Liège, B-4000 Liège, Belgium
| | - Y Bouffanais
- Università di Padova, Dipartimento di Fisica e Astronomia, I-35131 Padova, Italy
- INFN, Sezione di Padova, I-35131 Padova, Italy
| | - A Bozzi
- European Gravitational Observatory (EGO), I-56021 Cascina, Pisa, Italy
| | | | - M Braglia
- Instituto de Fisica Teorica UAM-CSIC, Universidad Autonoma de Madrid, 28049 Madrid, Spain
| | - M Branchesi
- Gran Sasso Science Institute (GSSI), I-67100 L'Aquila, Italy
- INFN, Laboratori Nazionali del Gran Sasso, I-67100 Assergi, Italy
| | - M Breschi
- Theoretisch-Physikalisches Institut, Friedrich-Schiller-Universität Jena, D-07743 Jena, Germany
| | - T Briant
- Laboratoire Kastler Brossel, Sorbonne Université, CNRS, ENS-Université PSL, Collège de France, F-75005 Paris, France
| | - A Brillet
- Université Côte d'Azur, Observatoire Côte d'Azur, CNRS, Artemis, F-06304 Nice, France
| | - J Brooks
- European Gravitational Observatory (EGO), I-56021 Cascina, Pisa, Italy
| | - G Bruno
- Université catholique de Louvain, B-1348 Louvain-la-Neuve, Belgium
| | - F Bucci
- INFN, Sezione di Firenze, I-50019 Sesto Fiorentino, Firenze, Italy
| | - O Bulashenko
- Institut de Ciències del Cosmos (ICCUB), Universitat de Barcelona (UB), carrer Martí i Franquès, 1, 08028 Barcelona, Spain
- Departament de Física Quàntica i Astrofísica (FQA), Universitat de Barcelona (UB), carrer Martí i Franqués, 1, 08028 Barcelona, Spain
| | - T Bulik
- Astronomical Observatory Warsaw University, 00-478 Warsaw, Poland
| | | | - R Buscicchio
- Università degli Studi di Milano-Bicocca, I-20126 Milano, Italy
- INFN, Sezione di Milano-Bicocca, I-20126 Milano, Italy
| | - D Buskulic
- Université Savoie Mont Blanc, CNRS, Laboratoire d'Annecy de Physique des Particules - IN2P3, F-74000 Annecy, France
| | - C Buy
- L2IT, Laboratoire des 2 Infinis - Toulouse, Université de Toulouse, CNRS/IN2P3, UPS, F-31062 Toulouse Cedex 9, France
| | - G Cabras
- Dipartimento di Scienze Matematiche, Informatiche e Fisiche, Università di Udine, I-33100 Udine, Italy
- INFN, Sezione di Trieste, I-34127 Trieste, Italy
| | - R Cabrita
- Université catholique de Louvain, B-1348 Louvain-la-Neuve, Belgium
| | - G Cagnoli
- Université de Lyon, Université Claude Bernard Lyon 1, CNRS, Institut Lumière Matière, F-69622 Villeurbanne, France
| | - E Calloni
- INFN, Sezione di Napoli, I-80126 Napoli, Italy
- Università di Napoli "Federico II", I-80126 Napoli, Italy
| | - M Canepa
- INFN, Sezione di Genova, I-16146 Genova, Italy
- Dipartimento di Fisica, Università degli Studi di Genova, I-16146 Genova, Italy
| | - G Caneva Santoro
- Institut de Física d'Altes Energies (IFAE), Barcelona Institute of Science and Technology, and ICREA, E-08193 Barcelona, Spain
| | - M Cannavacciuolo
- Dipartimento di Fisica "E.R. Caianiello", Università di Salerno, I-84084 Fisciano, Salerno, Italy
| | - E Capocasa
- Université Paris Cité, CNRS, Astroparticule et Cosmologie, F-75013 Paris, France
| | - G Carapella
- Dipartimento di Fisica "E.R. Caianiello", Università di Salerno, I-84084 Fisciano, Salerno, Italy
- INFN, Sezione di Napoli, Gruppo Collegato di Salerno, I-80126 Napoli, Italy
| | - F Carbognani
- European Gravitational Observatory (EGO), I-56021 Cascina, Pisa, Italy
| | - M Carpinelli
- European Gravitational Observatory (EGO), I-56021 Cascina, Pisa, Italy
- Università degli Studi di Milano-Bicocca, I-20126 Milano, Italy
- INFN, Laboratori Nazionali del Sud, I-95125 Catania, Italy
| | - G Carullo
- INFN, Sezione di Pisa, I-56127 Pisa, Italy
- Università di Pisa, I-56127 Pisa, Italy
| | - J Casanueva Diaz
- European Gravitational Observatory (EGO), I-56021 Cascina, Pisa, Italy
| | - C Casentini
- Università di Roma Tor Vergata, I-00133 Roma, Italy
- INFN, Sezione di Roma Tor Vergata, I-00133 Roma, Italy
| | - S Caudill
- Nikhef, 1098 XG Amsterdam, Netherlands
- Institute for Gravitational and Subatomic Physics (GRASP), Utrecht University, 3584 CC Utrecht, Netherlands
| | - R Cavalieri
- European Gravitational Observatory (EGO), I-56021 Cascina, Pisa, Italy
| | - G Cella
- INFN, Sezione di Pisa, I-56127 Pisa, Italy
| | - P Cerdá-Durán
- Departamento de Astronomía y Astrofísica, Universitat de València, E-46100 Burjassot, València, Spain
| | - E Cesarini
- INFN, Sezione di Roma Tor Vergata, I-00133 Roma, Italy
| | - W Chaibi
- Université Côte d'Azur, Observatoire Côte d'Azur, CNRS, Artemis, F-06304 Nice, France
| | - P Chanial
- Université Paris Cité, CNRS, Astroparticule et Cosmologie, F-75013 Paris, France
- European Gravitational Observatory (EGO), I-56021 Cascina, Pisa, Italy
| | - E Chassande-Mottin
- Université Paris Cité, CNRS, Astroparticule et Cosmologie, F-75013 Paris, France
| | - S Chaty
- Université Paris Cité, CNRS, Astroparticule et Cosmologie, F-75013 Paris, France
| | - P Chessa
- INFN, Sezione di Pisa, I-56127 Pisa, Italy
- Università di Pisa, I-56127 Pisa, Italy
| | - F Chiadini
- INFN, Sezione di Napoli, Gruppo Collegato di Salerno, I-80126 Napoli, Italy
- Dipartimento di Ingegneria Industriale (DIIN), Università di Salerno, I-84084 Fisciano, Salerno, Italy
| | - G Chiarini
- INFN, Sezione di Padova, I-35131 Padova, Italy
| | - R Chierici
- Université Lyon, Université Claude Bernard Lyon 1, CNRS, IP2I Lyon / IN2P3, UMR 5822, F-69622 Villeurbanne, France
| | | | - M L Chiofalo
- INFN, Sezione di Pisa, I-56127 Pisa, Italy
- Università di Pisa, I-56127 Pisa, Italy
| | - A Chiummo
- European Gravitational Observatory (EGO), I-56021 Cascina, Pisa, Italy
| | - N Christensen
- Université Côte d'Azur, Observatoire Côte d'Azur, CNRS, Artemis, F-06304 Nice, France
| | - S Chua
- Laboratoire Kastler Brossel, Sorbonne Université, CNRS, ENS-Université PSL, Collège de France, F-75005 Paris, France
| | - G Ciani
- Università di Padova, Dipartimento di Fisica e Astronomia, I-35131 Padova, Italy
- INFN, Sezione di Padova, I-35131 Padova, Italy
| | - P Ciecielag
- Nicolaus Copernicus Astronomical Center, Polish Academy of Sciences, 00-716, Warsaw, Poland
| | - M Cieślar
- Nicolaus Copernicus Astronomical Center, Polish Academy of Sciences, 00-716, Warsaw, Poland
| | - M Cifaldi
- Università di Roma Tor Vergata, I-00133 Roma, Italy
- INFN, Sezione di Roma Tor Vergata, I-00133 Roma, Italy
| | - R Ciolfi
- INFN, Sezione di Padova, I-35131 Padova, Italy
- INAF, Osservatorio Astronomico di Padova, I-35122 Padova, Italy
| | - S Clesse
- Université libre de Bruxelles, 1050 Bruxelles, Belgium
| | - F Cleva
- Université Côte d'Azur, Observatoire Côte d'Azur, CNRS, Artemis, F-06304 Nice, France
| | - E Coccia
- Gran Sasso Science Institute (GSSI), I-67100 L'Aquila, Italy
- INFN, Laboratori Nazionali del Gran Sasso, I-67100 Assergi, Italy
| | - E Codazzo
- Gran Sasso Science Institute (GSSI), I-67100 L'Aquila, Italy
| | - P-F Cohadon
- Laboratoire Kastler Brossel, Sorbonne Université, CNRS, ENS-Université PSL, Collège de France, F-75005 Paris, France
| | - A Colombo
- Università degli Studi di Milano-Bicocca, I-20126 Milano, Italy
- INFN, Sezione di Milano-Bicocca, I-20126 Milano, Italy
| | - M Colpi
- Università degli Studi di Milano-Bicocca, I-20126 Milano, Italy
- INFN, Sezione di Milano-Bicocca, I-20126 Milano, Italy
| | - L Conti
- INFN, Sezione di Padova, I-35131 Padova, Italy
| | - I Cordero-Carrión
- Departamento de Matemáticas, Universitat de València, E-46100 Burjassot, València, Spain
| | - S Corezzi
- INFN, Sezione di Perugia, I-06123 Perugia, Italy
- Università di Perugia, I-06123 Perugia, Italy
| | - S Cortese
- European Gravitational Observatory (EGO), I-56021 Cascina, Pisa, Italy
| | - J-P Coulon
- Université Côte d'Azur, Observatoire Côte d'Azur, CNRS, Artemis, F-06304 Nice, France
| | - J-F Coupechoux
- Université Lyon, Université Claude Bernard Lyon 1, CNRS, IP2I Lyon / IN2P3, UMR 5822, F-69622 Villeurbanne, France
| | - M Croquette
- Laboratoire Kastler Brossel, Sorbonne Université, CNRS, ENS-Université PSL, Collège de France, F-75005 Paris, France
| | - J R Cudell
- Université de Liège, B-4000 Liège, Belgium
| | - E Cuoco
- INFN, Sezione di Pisa, I-56127 Pisa, Italy
- European Gravitational Observatory (EGO), I-56021 Cascina, Pisa, Italy
- Scuola Normale Superiore, I-56126 Pisa, Italy
| | - M Curyło
- Astronomical Observatory Warsaw University, 00-478 Warsaw, Poland
| | - P Dabadie
- Université de Lyon, Université Claude Bernard Lyon 1, CNRS, Institut Lumière Matière, F-69622 Villeurbanne, France
| | - T Dal Canton
- Université Paris-Saclay, CNRS/IN2P3, IJCLab, 91405 Orsay, France
| | | | - G Dálya
- Universiteit Gent, B-9000 Gent, Belgium
| | - B D'Angelo
- INFN, Sezione di Genova, I-16146 Genova, Italy
- Dipartimento di Fisica, Università degli Studi di Genova, I-16146 Genova, Italy
| | - G Dangoisse
- Laboratoire Kastler Brossel, Sorbonne Université, CNRS, ENS-Université PSL, Collège de France, F-75005 Paris, France
| | - S Danilishin
- Maastricht University, 6200 MD Maastricht, Netherlands
- Nikhef, 1098 XG Amsterdam, Netherlands
| | - S D'Antonio
- INFN, Sezione di Roma Tor Vergata, I-00133 Roma, Italy
| | - V Dattilo
- European Gravitational Observatory (EGO), I-56021 Cascina, Pisa, Italy
| | - M Davier
- Université Paris-Saclay, CNRS/IN2P3, IJCLab, 91405 Orsay, France
| | - J Degallaix
- Université Lyon, Université Claude Bernard Lyon 1, CNRS, Laboratoire des Matériaux Avancés (LMA), IP2I Lyon / IN2P3, UMR 5822, F-69622 Villeurbanne, France
| | - M De Laurentis
- INFN, Sezione di Napoli, I-80126 Napoli, Italy
- Università di Napoli "Federico II", I-80126 Napoli, Italy
| | - S Deléglise
- Laboratoire Kastler Brossel, Sorbonne Université, CNRS, ENS-Université PSL, Collège de France, F-75005 Paris, France
| | - F De Lillo
- Université catholique de Louvain, B-1348 Louvain-la-Neuve, Belgium
| | - D Dell'Aquila
- INFN, Laboratori Nazionali del Sud, I-95125 Catania, Italy
- Università degli Studi di Sassari, I-07100 Sassari, Italy
| | - W Del Pozzo
- INFN, Sezione di Pisa, I-56127 Pisa, Italy
- Università di Pisa, I-56127 Pisa, Italy
| | - F De Matteis
- Università di Roma Tor Vergata, I-00133 Roma, Italy
- INFN, Sezione di Roma Tor Vergata, I-00133 Roma, Italy
| | - A Depasse
- Université catholique de Louvain, B-1348 Louvain-la-Neuve, Belgium
| | - R De Pietri
- Dipartimento di Scienze Matematiche, Fisiche e Informatiche, Università di Parma, I-43124 Parma, Italy
- INFN, Sezione di Milano Bicocca, Gruppo Collegato di Parma, I-43124 Parma, Italy
| | - R De Rosa
- INFN, Sezione di Napoli, I-80126 Napoli, Italy
- Università di Napoli "Federico II", I-80126 Napoli, Italy
| | - C De Rossi
- European Gravitational Observatory (EGO), I-56021 Cascina, Pisa, Italy
| | - R De Simone
- Dipartimento di Ingegneria Industriale (DIIN), Università di Salerno, I-84084 Fisciano, Salerno, Italy
| | - L Di Fiore
- INFN, Sezione di Napoli, I-80126 Napoli, Italy
| | - C Di Giorgio
- Dipartimento di Fisica "E.R. Caianiello", Università di Salerno, I-84084 Fisciano, Salerno, Italy
- INFN, Sezione di Napoli, Gruppo Collegato di Salerno, I-80126 Napoli, Italy
| | - F Di Giovanni
- Departamento de Astronomía y Astrofísica, Universitat de València, E-46100 Burjassot, València, Spain
| | - M Di Giovanni
- Gran Sasso Science Institute (GSSI), I-67100 L'Aquila, Italy
| | - T Di Girolamo
- INFN, Sezione di Napoli, I-80126 Napoli, Italy
- Università di Napoli "Federico II", I-80126 Napoli, Italy
| | - D Diksha
- Maastricht University, 6200 MD Maastricht, Netherlands
- Nikhef, 1098 XG Amsterdam, Netherlands
| | - A Di Lieto
- INFN, Sezione di Pisa, I-56127 Pisa, Italy
- Università di Pisa, I-56127 Pisa, Italy
| | | | - J Ding
- Université Paris Cité, CNRS, Astroparticule et Cosmologie, F-75013 Paris, France
- Corps des Mines, Mines Paris, Université PSL, Paris F-75272, France
| | - S Di Pace
- INFN, Sezione di Roma, I-00185 Roma, Italy
- Università di Roma "La Sapienza", I-00185 Roma, Italy
| | - I Di Palma
- INFN, Sezione di Roma, I-00185 Roma, Italy
- Università di Roma "La Sapienza", I-00185 Roma, Italy
| | - F Di Renzo
- INFN, Sezione di Pisa, I-56127 Pisa, Italy
- European Gravitational Observatory (EGO), I-56021 Cascina, Pisa, Italy
| | - L D'Onofrio
- INFN, Sezione di Napoli, I-80126 Napoli, Italy
- Università di Napoli "Federico II", I-80126 Napoli, Italy
| | - T Dooney
- Institute for Gravitational and Subatomic Physics (GRASP), Utrecht University, 3584 CC Utrecht, Netherlands
| | - O Dorosh
- National Center for Nuclear Research, 05-400 Świerk-Otwock, Poland
| | - M Drago
- INFN, Sezione di Roma, I-00185 Roma, Italy
- Università di Roma "La Sapienza", I-00185 Roma, Italy
| | - J-G Ducoin
- Université Paris Cité, CNRS, Astroparticule et Cosmologie, F-75013 Paris, France
- Institut d'Astrophysique de Paris, Sorbonne Université, CNRS, UMR 7095, 75014 Paris, France
| | - U Dupletsa
- Gran Sasso Science Institute (GSSI), I-67100 L'Aquila, Italy
| | - O Durante
- Dipartimento di Fisica "E.R. Caianiello", Università di Salerno, I-84084 Fisciano, Salerno, Italy
- INFN, Sezione di Napoli, Gruppo Collegato di Salerno, I-80126 Napoli, Italy
| | - D D'Urso
- INFN, Laboratori Nazionali del Sud, I-95125 Catania, Italy
- Università degli Studi di Sassari, I-07100 Sassari, Italy
| | - P-A Duverne
- Université Paris-Saclay, CNRS/IN2P3, IJCLab, 91405 Orsay, France
| | - M Eisenmann
- Laboratoire dâAnnecy-le-Vieux de Physique des Particules (LAPP), UniversitÂ'e Savoie Mont Blanc, CNRS/IN2P3, F-74941 Annecy-le-Vieux, France
- National Astronomical Observatory of Japan, 2-21-1 Osawa, Mitaka, Tokyo 181-8588, Japan
| | - L Errico
- INFN, Sezione di Napoli, I-80126 Napoli, Italy
- Università di Napoli "Federico II", I-80126 Napoli, Italy
| | - D Estevez
- Université de Strasbourg, CNRS, IPHC UMR 7178, F-67000 Strasbourg, France
| | - F Fabrizi
- Università degli Studi di Urbino "Carlo Bo", I-61029 Urbino, Italy
- INFN, Sezione di Firenze, I-50019 Sesto Fiorentino, Firenze, Italy
| | - F Faedi
- INFN, Sezione di Firenze, I-50019 Sesto Fiorentino, Firenze, Italy
| | - V Fafone
- Gran Sasso Science Institute (GSSI), I-67100 L'Aquila, Italy
- Università di Roma Tor Vergata, I-00133 Roma, Italy
- INFN, Sezione di Roma Tor Vergata, I-00133 Roma, Italy
| | - G Favaro
- Università di Padova, Dipartimento di Fisica e Astronomia, I-35131 Padova, Italy
| | - M Fays
- Université de Liège, B-4000 Liège, Belgium
| | - E Fenyvesi
- Wigner RCP, RMKI, H-1121 Budapest, Hungary
- Institute for Nuclear Research, H-4026 Debrecen, Hungary
| | - I Ferrante
- INFN, Sezione di Pisa, I-56127 Pisa, Italy
- Università di Pisa, I-56127 Pisa, Italy
| | - F Fidecaro
- INFN, Sezione di Pisa, I-56127 Pisa, Italy
- Università di Pisa, I-56127 Pisa, Italy
| | - P Figura
- Astronomical Observatory Warsaw University, 00-478 Warsaw, Poland
| | - A Fiori
- INFN, Sezione di Pisa, I-56127 Pisa, Italy
- Università di Pisa, I-56127 Pisa, Italy
| | - I Fiori
- European Gravitational Observatory (EGO), I-56021 Cascina, Pisa, Italy
| | - R Fittipaldi
- INFN, Sezione di Napoli, Gruppo Collegato di Salerno, I-80126 Napoli, Italy
- CNR-SPIN, I-84084 Fisciano, Salerno, Italy
| | - V Fiumara
- INFN, Sezione di Napoli, Gruppo Collegato di Salerno, I-80126 Napoli, Italy
- Scuola di Ingegneria, Università della Basilicata, I-85100 Potenza, Italy
| | - R Flaminio
- Université Savoie Mont Blanc, CNRS, Laboratoire d'Annecy de Physique des Particules - IN2P3, F-74000 Annecy, France
| | - J A Font
- Departamento de Astronomía y Astrofísica, Universitat de València, E-46100 Burjassot, València, Spain
- Observatori Astronòmic, Universitat de València, E-46980 Paterna, València, Spain
| | - S Frasca
- INFN, Sezione di Roma, I-00185 Roma, Italy
- Università di Roma "La Sapienza", I-00185 Roma, Italy
| | - F Frasconi
- INFN, Sezione di Pisa, I-56127 Pisa, Italy
| | - A Freise
- Nikhef, 1098 XG Amsterdam, Netherlands
- Department of Physics and Astronomy, Vrije Universiteit Amsterdam, 1081 HV Amsterdam, Netherlands
| | - O Freitas
- Centro de Física das Universidades do Minho e do Porto, Universidade do Minho, PT-4710-057 Braga, Portugal
| | - G G Fronzé
- INFN Sezione di Torino, I-10125 Torino, Italy
| | - B Gadre
- Institute for Gravitational and Subatomic Physics (GRASP), Utrecht University, 3584 CC Utrecht, Netherlands
| | - R Gamba
- Theoretisch-Physikalisches Institut, Friedrich-Schiller-Universität Jena, D-07743 Jena, Germany
| | - B Garaventa
- INFN, Sezione di Genova, I-16146 Genova, Italy
- Dipartimento di Fisica, Università degli Studi di Genova, I-16146 Genova, Italy
| | - J Garcia-Bellido
- Instituto de Fisica Teorica UAM-CSIC, Universidad Autonoma de Madrid, 28049 Madrid, Spain
| | - J Gargiulo
- European Gravitational Observatory (EGO), I-56021 Cascina, Pisa, Italy
| | - F Garufi
- INFN, Sezione di Napoli, I-80126 Napoli, Italy
- Università di Napoli "Federico II", I-80126 Napoli, Italy
| | - C Gasbarra
- Università di Roma Tor Vergata, I-00133 Roma, Italy
- INFN, Sezione di Roma Tor Vergata, I-00133 Roma, Italy
| | - G Gemme
- INFN, Sezione di Genova, I-16146 Genova, Italy
| | - A Gennai
- INFN, Sezione di Pisa, I-56127 Pisa, Italy
| | | | - L Giacoppo
- INFN, Sezione di Roma, I-00185 Roma, Italy
- Università di Roma "La Sapienza", I-00185 Roma, Italy
| | - P Giri
- INFN, Sezione di Pisa, I-56127 Pisa, Italy
- Università di Pisa, I-56127 Pisa, Italy
| | - F Gissi
- Dipartimento di Ingegneria, Università del Sannio, I-82100 Benevento, Italy
| | - S Gkaitatzis
- European Gravitational Observatory (EGO), I-56021 Cascina, Pisa, Italy
| | - F Glotin
- Université Paris-Saclay, CNRS/IN2P3, IJCLab, 91405 Orsay, France
| | - B Goncharov
- Gran Sasso Science Institute (GSSI), I-67100 L'Aquila, Italy
| | - M Gosselin
- European Gravitational Observatory (EGO), I-56021 Cascina, Pisa, Italy
| | - R Gouaty
- Université Savoie Mont Blanc, CNRS, Laboratoire d'Annecy de Physique des Particules - IN2P3, F-74000 Annecy, France
| | - A Grado
- INFN, Sezione di Napoli, I-80126 Napoli, Italy
- INAF, Osservatorio Astronomico di Capodimonte, I-80131 Napoli, Italy
| | - M Granata
- Université Lyon, Université Claude Bernard Lyon 1, CNRS, Laboratoire des Matériaux Avancés (LMA), IP2I Lyon / IN2P3, UMR 5822, F-69622 Villeurbanne, France
| | - V Granata
- Dipartimento di Fisica "E.R. Caianiello", Università di Salerno, I-84084 Fisciano, Salerno, Italy
| | - G Greco
- INFN, Sezione di Perugia, I-06123 Perugia, Italy
| | - G Grignani
- INFN, Sezione di Perugia, I-06123 Perugia, Italy
- Università di Perugia, I-06123 Perugia, Italy
| | - A Grimaldi
- Università di Trento, Dipartimento di Fisica, I-38123 Povo, Trento, Italy
- INFN, Trento Institute for Fundamental Physics and Applications, I-38123 Povo, Trento, Italy
| | - D Guerra
- Departamento de Astronomía y Astrofísica, Universitat de València, E-46100 Burjassot, València, Spain
| | - D Guetta
- INFN, Sezione di Roma, I-00185 Roma, Italy
| | - G M Guidi
- Università degli Studi di Urbino "Carlo Bo", I-61029 Urbino, Italy
- INFN, Sezione di Firenze, I-50019 Sesto Fiorentino, Firenze, Italy
| | - F Gulminelli
- Université de Normandie, ENSICAEN, UNICAEN, CNRS/IN2P3, LPC Caen, F-14000 Caen, France
- Laboratoire de Physique Corpusculaire Caen, 6 boulevard du maréchal Juin, F-14050 Caen, France
| | - Y Guo
- Nikhef, 1098 XG Amsterdam, Netherlands
| | - P Gupta
- Nikhef, 1098 XG Amsterdam, Netherlands
- Institute for Gravitational and Subatomic Physics (GRASP), Utrecht University, 3584 CC Utrecht, Netherlands
| | - N Gutierrez
- Université Lyon, Université Claude Bernard Lyon 1, CNRS, Laboratoire des Matériaux Avancés (LMA), IP2I Lyon / IN2P3, UMR 5822, F-69622 Villeurbanne, France
| | - L Haegel
- Université Paris Cité, CNRS, Astroparticule et Cosmologie, F-75013 Paris, France
| | - O Halim
- INFN, Sezione di Trieste, I-34127 Trieste, Italy
| | - O Hannuksela
- Nikhef, 1098 XG Amsterdam, Netherlands
- Institute for Gravitational and Subatomic Physics (GRASP), Utrecht University, 3584 CC Utrecht, Netherlands
| | - T Harder
- Université Côte d'Azur, Observatoire Côte d'Azur, CNRS, Artemis, F-06304 Nice, France
| | - K Haris
- Nikhef, 1098 XG Amsterdam, Netherlands
- Institute for Gravitational and Subatomic Physics (GRASP), Utrecht University, 3584 CC Utrecht, Netherlands
| | - T Harmark
- Niels Bohr Institute, Copenhagen University, 2100 København, Denmark
| | - J Harms
- Gran Sasso Science Institute (GSSI), I-67100 L'Aquila, Italy
- INFN, Laboratori Nazionali del Gran Sasso, I-67100 Assergi, Italy
| | - B Haskell
- Nicolaus Copernicus Astronomical Center, Polish Academy of Sciences, 00-716, Warsaw, Poland
| | - A Heidmann
- Laboratoire Kastler Brossel, Sorbonne Université, CNRS, ENS-Université PSL, Collège de France, F-75005 Paris, France
| | - H Heitmann
- Université Côte d'Azur, Observatoire Côte d'Azur, CNRS, Artemis, F-06304 Nice, France
| | - P Hello
- Université Paris-Saclay, CNRS/IN2P3, IJCLab, 91405 Orsay, France
| | - G Hemming
- European Gravitational Observatory (EGO), I-56021 Cascina, Pisa, Italy
| | - E Hennes
- Nikhef, 1098 XG Amsterdam, Netherlands
| | - J-S Hennig
- Maastricht University, 6200 MD Maastricht, Netherlands
- Nikhef, 1098 XG Amsterdam, Netherlands
| | - M Hennig
- Maastricht University, 6200 MD Maastricht, Netherlands
- Nikhef, 1098 XG Amsterdam, Netherlands
| | - S Hild
- Maastricht University, 6200 MD Maastricht, Netherlands
- Nikhef, 1098 XG Amsterdam, Netherlands
| | - D Hofman
- Université Lyon, Université Claude Bernard Lyon 1, CNRS, Laboratoire des Matériaux Avancés (LMA), IP2I Lyon / IN2P3, UMR 5822, F-69622 Villeurbanne, France
| | - N A Holland
- Nikhef, 1098 XG Amsterdam, Netherlands
- Department of Physics and Astronomy, Vrije Universiteit Amsterdam, 1081 HV Amsterdam, Netherlands
| | - V Hui
- Université Savoie Mont Blanc, CNRS, Laboratoire d'Annecy de Physique des Particules - IN2P3, F-74000 Annecy, France
| | - G A Iandolo
- Maastricht University, 6200 MD Maastricht, Netherlands
| | - B Idzkowski
- Astronomical Observatory Warsaw University, 00-478 Warsaw, Poland
| | - A Iess
- INFN, Sezione di Pisa, I-56127 Pisa, Italy
- Scuola Normale Superiore, I-56126 Pisa, Italy
| | - G Iorio
- Università di Padova, Dipartimento di Fisica e Astronomia, I-35131 Padova, Italy
| | - P Iosif
- Department of Physics, Aristotle University of Thessaloniki, 54124 Thessaloniki, Greece
| | - T Jacqmin
- Laboratoire Kastler Brossel, Sorbonne Université, CNRS, ENS-Université PSL, Collège de France, F-75005 Paris, France
| | - P-E Jacquet
- Laboratoire Kastler Brossel, Sorbonne Université, CNRS, ENS-Université PSL, Collège de France, F-75005 Paris, France
| | - J Janquart
- Nikhef, 1098 XG Amsterdam, Netherlands
- Institute for Gravitational and Subatomic Physics (GRASP), Utrecht University, 3584 CC Utrecht, Netherlands
| | - K Janssens
- Université Côte d'Azur, Observatoire Côte d'Azur, CNRS, Artemis, F-06304 Nice, France
- Universiteit Antwerpen, 2000 Antwerpen, Belgium
| | - S Jaraba
- Instituto de Fisica Teorica UAM-CSIC, Universidad Autonoma de Madrid, 28049 Madrid, Spain
| | - P Jaranowski
- University of Białystok, 15-424 Białystok, Poland
| | - P Jasal
- Institut de Ciències del Cosmos (ICCUB), Universitat de Barcelona (UB), carrer Martí i Franquès, 1, 08028 Barcelona, Spain
| | - V Juste
- Université de Strasbourg, CNRS, IPHC UMR 7178, F-67000 Strasbourg, France
| | - C Kalaghatgi
- Nikhef, 1098 XG Amsterdam, Netherlands
- Institute for Gravitational and Subatomic Physics (GRASP), Utrecht University, 3584 CC Utrecht, Netherlands
- Institute for High-Energy Physics, University of Amsterdam, 1098 XH Amsterdam, Netherlands
| | - C Karathanasis
- Institut de Física d'Altes Energies (IFAE), Barcelona Institute of Science and Technology, and ICREA, E-08193 Barcelona, Spain
| | - S Katsanevas
- European Gravitational Observatory (EGO), I-56021 Cascina, Pisa, Italy
| | - F Kéfélian
- Université Côte d'Azur, Observatoire Côte d'Azur, CNRS, Artemis, F-06304 Nice, France
| | - G Koekoek
- Maastricht University, 6200 MD Maastricht, Netherlands
- Nikhef, 1098 XG Amsterdam, Netherlands
| | - S Koley
- Gran Sasso Science Institute (GSSI), I-67100 L'Aquila, Italy
| | - M Kolstein
- Institut de Física d'Altes Energies (IFAE), Barcelona Institute of Science and Technology, and ICREA, E-08193 Barcelona, Spain
| | - S L Kranzhoff
- Maastricht University, 6200 MD Maastricht, Netherlands
- Nikhef, 1098 XG Amsterdam, Netherlands
| | - A Królak
- National Center for Nuclear Research, 05-400 Świerk-Otwock, Poland
- Institute of Mathematics, Polish Academy of Sciences, 00656 Warsaw, Poland
| | - P Kuijer
- Nikhef, 1098 XG Amsterdam, Netherlands
| | - S Kuroyanagi
- Instituto de Fisica Teorica UAM-CSIC, Universidad Autonoma de Madrid, 28049 Madrid, Spain
| | - P Lagabbe
- Université Savoie Mont Blanc, CNRS, Laboratoire d'Annecy de Physique des Particules - IN2P3, F-74000 Annecy, France
| | - D Laghi
- L2IT, Laboratoire des 2 Infinis - Toulouse, Université de Toulouse, CNRS/IN2P3, UPS, F-31062 Toulouse Cedex 9, France
| | - M Lalleman
- Universiteit Antwerpen, 2000 Antwerpen, Belgium
| | - A Lamberts
- Université Côte d'Azur, Observatoire Côte d'Azur, CNRS, Artemis, F-06304 Nice, France
- Université Côte d'Azur, Observatoire Côte d'Azur, CNRS, Lagrange, F-06304 Nice, France
| | - A La Rana
- INFN, Sezione di Roma, I-00185 Roma, Italy
| | - I La Rosa
- Université Savoie Mont Blanc, CNRS, Laboratoire d'Annecy de Physique des Particules - IN2P3, F-74000 Annecy, France
| | | | - C Lazzaro
- Università di Padova, Dipartimento di Fisica e Astronomia, I-35131 Padova, Italy
- INFN, Sezione di Padova, I-35131 Padova, Italy
| | - P Leaci
- INFN, Sezione di Roma, I-00185 Roma, Italy
- Università di Roma "La Sapienza", I-00185 Roma, Italy
| | - A Lemaître
- NAVIER, École des Ponts, Univ Gustave Eiffel, CNRS, Marne-la-Vallée, France
| | - M Lenti
- INFN, Sezione di Firenze, I-50019 Sesto Fiorentino, Firenze, Italy
- Università di Firenze, Sesto Fiorentino I-50019, Italy
| | - E Leonova
- GRAPPA, Anton Pannekoek Institute for Astronomy and Institute for High-Energy Physics, University of Amsterdam, 1098 XH Amsterdam, Netherlands
| | - M Lequime
- Institut Fresnel, Faculté des Sciences St Jérôme Avenue Escadrille Normandie-Niemen, F-13013 Marseille, France
| | - N Leroy
- Université Paris-Saclay, CNRS/IN2P3, IJCLab, 91405 Orsay, France
| | - N Letendre
- Université Savoie Mont Blanc, CNRS, Laboratoire d'Annecy de Physique des Particules - IN2P3, F-74000 Annecy, France
| | - M Lethuillier
- Université Lyon, Université Claude Bernard Lyon 1, CNRS, IP2I Lyon / IN2P3, UMR 5822, F-69622 Villeurbanne, France
| | - K Leyde
- Université Paris Cité, CNRS, Astroparticule et Cosmologie, F-75013 Paris, France
| | - F Linde
- Nikhef, 1098 XG Amsterdam, Netherlands
- Institute for High-Energy Physics, University of Amsterdam, 1098 XH Amsterdam, Netherlands
| | - L London
- GRAPPA, Anton Pannekoek Institute for Astronomy and Institute for High-Energy Physics, University of Amsterdam, 1098 XH Amsterdam, Netherlands
| | - A Longo
- INFN, Sezione di Roma Tre, I-00146 Roma, Italy
| | - M Lopez Portilla
- Institute for Gravitational and Subatomic Physics (GRASP), Utrecht University, 3584 CC Utrecht, Netherlands
| | - M Lorenzini
- Università di Roma Tor Vergata, I-00133 Roma, Italy
- INFN, Sezione di Roma Tor Vergata, I-00133 Roma, Italy
| | | | - G Losurdo
- INFN, Sezione di Pisa, I-56127 Pisa, Italy
| | - D Lumaca
- Università di Roma Tor Vergata, I-00133 Roma, Italy
- INFN, Sezione di Roma Tor Vergata, I-00133 Roma, Italy
| | - A Macquet
- Institut de Física d'Altes Energies (IFAE), Barcelona Institute of Science and Technology, and ICREA, E-08193 Barcelona, Spain
| | - C Magazzù
- INFN, Sezione di Pisa, I-56127 Pisa, Italy
| | - R Maggiore
- Nikhef, 1098 XG Amsterdam, Netherlands
- Department of Physics and Astronomy, Vrije Universiteit Amsterdam, 1081 HV Amsterdam, Netherlands
| | - M Magnozzi
- INFN, Sezione di Genova, I-16146 Genova, Italy
- Dipartimento di Fisica, Università degli Studi di Genova, I-16146 Genova, Italy
| | - E Majorana
- INFN, Sezione di Roma, I-00185 Roma, Italy
- Università di Roma "La Sapienza", I-00185 Roma, Italy
| | - N Man
- Université Côte d'Azur, Observatoire Côte d'Azur, CNRS, Artemis, F-06304 Nice, France
| | - V Mangano
- INFN, Sezione di Roma, I-00185 Roma, Italy
- Università di Roma "La Sapienza", I-00185 Roma, Italy
| | - M Mantovani
- European Gravitational Observatory (EGO), I-56021 Cascina, Pisa, Italy
| | - M Mapelli
- Università di Padova, Dipartimento di Fisica e Astronomia, I-35131 Padova, Italy
- INFN, Sezione di Padova, I-35131 Padova, Italy
| | - F Marchesoni
- INFN, Sezione di Perugia, I-06123 Perugia, Italy
- Università di Camerino, I-62032 Camerino, Italy
- School of Physics Science and Engineering, Tongji University, Shanghai 200092, China
| | - D Marín Pina
- Institut de Ciències del Cosmos (ICCUB), Universitat de Barcelona (UB), carrer Martí i Franquès, 1, 08028 Barcelona, Spain
- Departament de Física Quàntica i Astrofísica (FQA), Universitat de Barcelona (UB), carrer Martí i Franqués, 1, 08028 Barcelona, Spain
- Institut d'Estudis Espacials de Catalunya, carrer Gran Capità, 2-4, 08034 Barcelona, Spain
| | - F Marion
- Université Savoie Mont Blanc, CNRS, Laboratoire d'Annecy de Physique des Particules - IN2P3, F-74000 Annecy, France
| | - A Marquina
- Departamento de Matemáticas, Universitat de València, E-46100 Burjassot, València, Spain
| | - S Marsat
- L2IT, Laboratoire des 2 Infinis - Toulouse, Université de Toulouse, CNRS/IN2P3, UPS, F-31062 Toulouse Cedex 9, France
| | - F Martelli
- Università degli Studi di Urbino "Carlo Bo", I-61029 Urbino, Italy
- INFN, Sezione di Firenze, I-50019 Sesto Fiorentino, Firenze, Italy
| | - M Martinez
- Institut de Física d'Altes Energies (IFAE), Barcelona Institute of Science and Technology, and ICREA, E-08193 Barcelona, Spain
| | - V Martinez
- Université de Lyon, Université Claude Bernard Lyon 1, CNRS, Institut Lumière Matière, F-69622 Villeurbanne, France
| | - A Masserot
- Université Savoie Mont Blanc, CNRS, Laboratoire d'Annecy de Physique des Particules - IN2P3, F-74000 Annecy, France
| | | | - S Mastrogiovanni
- Université Côte d'Azur, Observatoire Côte d'Azur, CNRS, Artemis, F-06304 Nice, France
| | - Q Meijer
- Institute for Gravitational and Subatomic Physics (GRASP), Utrecht University, 3584 CC Utrecht, Netherlands
| | - A Menendez-Vazquez
- Institut de Física d'Altes Energies (IFAE), Barcelona Institute of Science and Technology, and ICREA, E-08193 Barcelona, Spain
| | - L Mereni
- Université Lyon, Université Claude Bernard Lyon 1, CNRS, Laboratoire des Matériaux Avancés (LMA), IP2I Lyon / IN2P3, UMR 5822, F-69622 Villeurbanne, France
| | - M Merzougui
- Université Côte d'Azur, Observatoire Côte d'Azur, CNRS, Artemis, F-06304 Nice, France
| | - A Miani
- Università di Trento, Dipartimento di Fisica, I-38123 Povo, Trento, Italy
- INFN, Trento Institute for Fundamental Physics and Applications, I-38123 Povo, Trento, Italy
| | - C Michel
- Université Lyon, Université Claude Bernard Lyon 1, CNRS, Laboratoire des Matériaux Avancés (LMA), IP2I Lyon / IN2P3, UMR 5822, F-69622 Villeurbanne, France
| | - A Miller
- Université catholique de Louvain, B-1348 Louvain-la-Neuve, Belgium
| | - B Miller
- Nikhef, 1098 XG Amsterdam, Netherlands
- GRAPPA, Anton Pannekoek Institute for Astronomy and Institute for High-Energy Physics, University of Amsterdam, 1098 XH Amsterdam, Netherlands
| | - E Milotti
- INFN, Sezione di Trieste, I-34127 Trieste, Italy
- Dipartimento di Fisica, Università di Trieste, I-34127 Trieste, Italy
| | - Y Minenkov
- INFN, Sezione di Roma Tor Vergata, I-00133 Roma, Italy
| | - Ll M Mir
- Institut de Física d'Altes Energies (IFAE), Barcelona Institute of Science and Technology, and ICREA, E-08193 Barcelona, Spain
| | - M Miravet-Tenés
- Departamento de Astronomía y Astrofísica, Universitat de València, E-46100 Burjassot, València, Spain
| | - A L Mitchell
- Nikhef, 1098 XG Amsterdam, Netherlands
- Department of Physics and Astronomy, Vrije Universiteit Amsterdam, 1081 HV Amsterdam, Netherlands
| | - C Mondal
- Université de Normandie, ENSICAEN, UNICAEN, CNRS/IN2P3, LPC Caen, F-14000 Caen, France
| | - M Montani
- Università degli Studi di Urbino "Carlo Bo", I-61029 Urbino, Italy
- INFN, Sezione di Firenze, I-50019 Sesto Fiorentino, Firenze, Italy
| | - F Morawski
- Nicolaus Copernicus Astronomical Center, Polish Academy of Sciences, 00-716, Warsaw, Poland
| | - G Morras
- Instituto de Fisica Teorica UAM-CSIC, Universidad Autonoma de Madrid, 28049 Madrid, Spain
| | - A Moscatello
- Università di Padova, Dipartimento di Fisica e Astronomia, I-35131 Padova, Italy
| | - B Mours
- Université de Strasbourg, CNRS, IPHC UMR 7178, F-67000 Strasbourg, France
| | - C M Mow-Lowry
- Nikhef, 1098 XG Amsterdam, Netherlands
- Department of Physics and Astronomy, Vrije Universiteit Amsterdam, 1081 HV Amsterdam, Netherlands
| | - E Msihid
- Université Paris Cité, CNRS, Astroparticule et Cosmologie, F-75013 Paris, France
| | - F Muciaccia
- INFN, Sezione di Roma, I-00185 Roma, Italy
- Università di Roma "La Sapienza", I-00185 Roma, Italy
| | - Suvodip Mukherjee
- GRAPPA, Anton Pannekoek Institute for Astronomy and Institute for High-Energy Physics, University of Amsterdam, 1098 XH Amsterdam, Netherlands
| | - A Nagar
- INFN Sezione di Torino, I-10125 Torino, Italy
- Institut des Hautes Etudes Scientifiques, F-91440 Bures-sur-Yvette, France
| | - V Napolano
- European Gravitational Observatory (EGO), I-56021 Cascina, Pisa, Italy
| | - I Nardecchia
- Università di Roma Tor Vergata, I-00133 Roma, Italy
- INFN, Sezione di Roma Tor Vergata, I-00133 Roma, Italy
| | - H Narola
- Institute for Gravitational and Subatomic Physics (GRASP), Utrecht University, 3584 CC Utrecht, Netherlands
| | | | - J Neilson
- Dipartimento di Ingegneria, Università del Sannio, I-82100 Benevento, Italy
- INFN, Sezione di Napoli, Gruppo Collegato di Salerno, I-80126 Napoli, Italy
| | - S Nesseris
- Instituto de Fisica Teorica UAM-CSIC, Universidad Autonoma de Madrid, 28049 Madrid, Spain
| | - C Nguyen
- Université Paris Cité, CNRS, Astroparticule et Cosmologie, F-75013 Paris, France
| | - G Nieradka
- Nicolaus Copernicus Astronomical Center, Polish Academy of Sciences, 00-716, Warsaw, Poland
| | - S Nissanke
- Nikhef, 1098 XG Amsterdam, Netherlands
- GRAPPA, Anton Pannekoek Institute for Astronomy and Institute for High-Energy Physics, University of Amsterdam, 1098 XH Amsterdam, Netherlands
| | - E Nitoglia
- Université Lyon, Université Claude Bernard Lyon 1, CNRS, IP2I Lyon / IN2P3, UMR 5822, F-69622 Villeurbanne, France
| | - F Nocera
- European Gravitational Observatory (EGO), I-56021 Cascina, Pisa, Italy
| | - J Novak
- Centre national de la recherche scientifique, 75016 Paris, France
- Laboratoire Univers et Théories, Observatoire de Paris, 92190 Meudon, France
- Observatoire de Paris, 75014 Paris, France
- Université PSL, 75006 Paris, France
| | - J F Nu No Siles
- Instituto de Fisica Teorica UAM-CSIC, Universidad Autonoma de Madrid, 28049 Madrid, Spain
| | - M Oertel
- Centre national de la recherche scientifique, 75016 Paris, France
- Laboratoire Univers et Théories, Observatoire de Paris, 92190 Meudon, France
- Observatoire de Paris, 75014 Paris, France
- Université PSL, 75006 Paris, France
- Université de Paris Cité, 75006 Paris, France
| | - G Oganesyan
- Gran Sasso Science Institute (GSSI), I-67100 L'Aquila, Italy
- INFN, Laboratori Nazionali del Gran Sasso, I-67100 Assergi, Italy
| | - R Oliveri
- Centre national de la recherche scientifique, 75016 Paris, France
- Laboratoire Univers et Théories, Observatoire de Paris, 92190 Meudon, France
- Observatoire de Paris, 75014 Paris, France
| | - M Orselli
- INFN, Sezione di Perugia, I-06123 Perugia, Italy
- Università di Perugia, I-06123 Perugia, Italy
| | - C Palomba
- INFN, Sezione di Roma, I-00185 Roma, Italy
| | - P T H Pang
- Nikhef, 1098 XG Amsterdam, Netherlands
- Institute for Gravitational and Subatomic Physics (GRASP), Utrecht University, 3584 CC Utrecht, Netherlands
| | - F Pannarale
- INFN, Sezione di Roma, I-00185 Roma, Italy
- Università di Roma "La Sapienza", I-00185 Roma, Italy
| | - F Paoletti
- INFN, Sezione di Pisa, I-56127 Pisa, Italy
| | - A Paoli
- European Gravitational Observatory (EGO), I-56021 Cascina, Pisa, Italy
| | - A Paolone
- INFN, Sezione di Roma, I-00185 Roma, Italy
- Consiglio Nazionale delle Ricerche - Istituto dei Sistemi Complessi, I-00185 Roma, Italy
| | - G Pappas
- Department of Physics, Aristotle University of Thessaloniki, 54124 Thessaloniki, Greece
| | - A Parisi
- INFN, Sezione di Pisa, I-56127 Pisa, Italy
- Scuola Normale Superiore, I-56126 Pisa, Italy
| | | | - A Pasqualetti
- European Gravitational Observatory (EGO), I-56021 Cascina, Pisa, Italy
| | - R Passaquieti
- INFN, Sezione di Pisa, I-56127 Pisa, Italy
- Università di Pisa, I-56127 Pisa, Italy
| | | | - B Patricelli
- INFN, Sezione di Pisa, I-56127 Pisa, Italy
- Università di Pisa, I-56127 Pisa, Italy
| | - R Pedurand
- INFN, Sezione di Napoli, Gruppo Collegato di Salerno, I-80126 Napoli, Italy
| | - R Pegna
- INFN, Sezione di Pisa, I-56127 Pisa, Italy
- Università di Pisa, I-56127 Pisa, Italy
| | - M Pegoraro
- INFN, Sezione di Padova, I-35131 Padova, Italy
| | - A Perego
- Università di Trento, Dipartimento di Fisica, I-38123 Povo, Trento, Italy
- INFN, Trento Institute for Fundamental Physics and Applications, I-38123 Povo, Trento, Italy
| | - A Pereira
- Université de Lyon, Université Claude Bernard Lyon 1, CNRS, Institut Lumière Matière, F-69622 Villeurbanne, France
| | - C Périgois
- INAF, Osservatorio Astronomico di Padova, I-35122 Padova, Italy
| | - A Perreca
- Università di Trento, Dipartimento di Fisica, I-38123 Povo, Trento, Italy
- INFN, Trento Institute for Fundamental Physics and Applications, I-38123 Povo, Trento, Italy
| | - S Perriès
- Université Lyon, Université Claude Bernard Lyon 1, CNRS, IP2I Lyon / IN2P3, UMR 5822, F-69622 Villeurbanne, France
| | - J W Perry
- Nikhef, 1098 XG Amsterdam, Netherlands
- Department of Physics and Astronomy, Vrije Universiteit Amsterdam, 1081 HV Amsterdam, Netherlands
| | - D Pesios
- Department of Physics, Aristotle University of Thessaloniki, 54124 Thessaloniki, Greece
| | - C Petrillo
- Università di Perugia, I-06123 Perugia, Italy
| | - K S Phukon
- Nikhef, 1098 XG Amsterdam, Netherlands
- Institute for High-Energy Physics, University of Amsterdam, 1098 XH Amsterdam, Netherlands
| | - O J Piccinni
- Institut de Física d'Altes Energies (IFAE), Barcelona Institute of Science and Technology, and ICREA, E-08193 Barcelona, Spain
| | - M Pichot
- Université Côte d'Azur, Observatoire Côte d'Azur, CNRS, Artemis, F-06304 Nice, France
| | - M Piendibene
- INFN, Sezione di Pisa, I-56127 Pisa, Italy
- Università di Pisa, I-56127 Pisa, Italy
| | - F Piergiovanni
- Università degli Studi di Urbino "Carlo Bo", I-61029 Urbino, Italy
- INFN, Sezione di Firenze, I-50019 Sesto Fiorentino, Firenze, Italy
| | - L Pierini
- INFN, Sezione di Roma, I-00185 Roma, Italy
- Università di Roma "La Sapienza", I-00185 Roma, Italy
| | - G Pierra
- Université Lyon, Université Claude Bernard Lyon 1, CNRS, IP2I Lyon / IN2P3, UMR 5822, F-69622 Villeurbanne, France
| | - V Pierro
- Dipartimento di Ingegneria, Università del Sannio, I-82100 Benevento, Italy
- INFN, Sezione di Napoli, Gruppo Collegato di Salerno, I-80126 Napoli, Italy
| | - G Pillant
- European Gravitational Observatory (EGO), I-56021 Cascina, Pisa, Italy
| | - M Pillas
- Université Paris-Saclay, CNRS/IN2P3, IJCLab, 91405 Orsay, France
| | - F Pilo
- INFN, Sezione di Pisa, I-56127 Pisa, Italy
| | - L Pinard
- Université Lyon, Université Claude Bernard Lyon 1, CNRS, Laboratoire des Matériaux Avancés (LMA), IP2I Lyon / IN2P3, UMR 5822, F-69622 Villeurbanne, France
| | - I M Pinto
- Università di Napoli "Federico II", I-80126 Napoli, Italy
- Dipartimento di Ingegneria, Università del Sannio, I-82100 Benevento, Italy
- INFN, Sezione di Napoli, Gruppo Collegato di Salerno, I-80126 Napoli, Italy
- Museo Storico della Fisica e Centro Studi e Ricerche "Enrico Fermi", I-00184 Roma, Italy
| | - M Pinto
- European Gravitational Observatory (EGO), I-56021 Cascina, Pisa, Italy
| | - M Pinto
- European Gravitational Observatory (EGO), I-56021 Cascina, Pisa, Italy
| | - K Piotrzkowski
- Université catholique de Louvain, B-1348 Louvain-la-Neuve, Belgium
| | - A Placidi
- INFN, Sezione di Perugia, I-06123 Perugia, Italy
- Università di Perugia, I-06123 Perugia, Italy
| | - E Placidi
- INFN, Sezione di Roma, I-00185 Roma, Italy
- Università di Roma "La Sapienza", I-00185 Roma, Italy
| | - W Plastino
- INFN, Sezione di Roma Tre, I-00146 Roma, Italy
- Dipartimento di Matematica e Fisica, Università degli Studi Roma Tre, I-00146 Roma, Italy
| | - R Poggiani
- INFN, Sezione di Pisa, I-56127 Pisa, Italy
- Università di Pisa, I-56127 Pisa, Italy
| | - E Polini
- Université Savoie Mont Blanc, CNRS, Laboratoire d'Annecy de Physique des Particules - IN2P3, F-74000 Annecy, France
| | | | - J Portell
- Institut de Ciències del Cosmos (ICCUB), Universitat de Barcelona (UB), carrer Martí i Franquès, 1, 08028 Barcelona, Spain
- Departament de Física Quàntica i Astrofísica (FQA), Universitat de Barcelona (UB), carrer Martí i Franqués, 1, 08028 Barcelona, Spain
- Institut d'Estudis Espacials de Catalunya, carrer Gran Capità, 2-4, 08034 Barcelona, Spain
| | - E K Porter
- Université Paris Cité, CNRS, Astroparticule et Cosmologie, F-75013 Paris, France
| | - R Poulton
- European Gravitational Observatory (EGO), I-56021 Cascina, Pisa, Italy
| | - M Pracchia
- Université Savoie Mont Blanc, CNRS, Laboratoire d'Annecy de Physique des Particules - IN2P3, F-74000 Annecy, France
| | - T Pradier
- Université de Strasbourg, CNRS, IPHC UMR 7178, F-67000 Strasbourg, France
| | - M Principe
- Dipartimento di Ingegneria, Università del Sannio, I-82100 Benevento, Italy
- INFN, Sezione di Napoli, Gruppo Collegato di Salerno, I-80126 Napoli, Italy
- Museo Storico della Fisica e Centro Studi e Ricerche "Enrico Fermi", I-00184 Roma, Italy
| | - G A Prodi
- INFN, Trento Institute for Fundamental Physics and Applications, I-38123 Povo, Trento, Italy
- Università di Trento, Dipartimento di Matematica, I-38123 Povo, Trento, Italy
| | - P Prosposito
- Università di Roma Tor Vergata, I-00133 Roma, Italy
- INFN, Sezione di Roma Tor Vergata, I-00133 Roma, Italy
| | - A Puecher
- Nikhef, 1098 XG Amsterdam, Netherlands
- Institute for Gravitational and Subatomic Physics (GRASP), Utrecht University, 3584 CC Utrecht, Netherlands
| | - M Punturo
- INFN, Sezione di Perugia, I-06123 Perugia, Italy
| | - F Puosi
- INFN, Sezione di Pisa, I-56127 Pisa, Italy
- Università di Pisa, I-56127 Pisa, Italy
| | - P Puppo
- INFN, Sezione di Roma, I-00185 Roma, Italy
| | - G Raaijmakers
- Nikhef, 1098 XG Amsterdam, Netherlands
- GRAPPA, Anton Pannekoek Institute for Astronomy and Institute for High-Energy Physics, University of Amsterdam, 1098 XH Amsterdam, Netherlands
| | - N Radulesco
- Université Côte d'Azur, Observatoire Côte d'Azur, CNRS, Artemis, F-06304 Nice, France
| | - P Rapagnani
- INFN, Sezione di Roma, I-00185 Roma, Italy
- Università di Roma "La Sapienza", I-00185 Roma, Italy
| | - M Razzano
- INFN, Sezione di Pisa, I-56127 Pisa, Italy
- Università di Pisa, I-56127 Pisa, Italy
| | - T Regimbau
- Université Savoie Mont Blanc, CNRS, Laboratoire d'Annecy de Physique des Particules - IN2P3, F-74000 Annecy, France
| | - L Rei
- INFN, Sezione di Genova, I-16146 Genova, Italy
| | - P Rettegno
- Dipartimento di Fisica, Università degli Studi di Torino, I-10125 Torino, Italy
- INFN Sezione di Torino, I-10125 Torino, Italy
| | - B Revenu
- Université Paris Cité, CNRS, Astroparticule et Cosmologie, F-75013 Paris, France
- Subatech, CNRS/IN2P3 - Institut Mines-Telecom Atlantique - Université de Nantes, 4 rue Alfred Kastler BP 20722 44307 Nantes C'EDEX 03, France
| | - A Reza
- Nikhef, 1098 XG Amsterdam, Netherlands
| | - A S Rezaei
- INFN, Sezione di Roma, I-00185 Roma, Italy
- Università di Roma "La Sapienza", I-00185 Roma, Italy
| | - F Ricci
- INFN, Sezione di Roma, I-00185 Roma, Italy
- Università di Roma "La Sapienza", I-00185 Roma, Italy
| | - S Rinaldi
- INFN, Sezione di Pisa, I-56127 Pisa, Italy
- Università di Pisa, I-56127 Pisa, Italy
| | - F Robinet
- Université Paris-Saclay, CNRS/IN2P3, IJCLab, 91405 Orsay, France
| | - A Rocchi
- INFN, Sezione di Roma Tor Vergata, I-00133 Roma, Italy
| | - L Rolland
- Université Savoie Mont Blanc, CNRS, Laboratoire d'Annecy de Physique des Particules - IN2P3, F-74000 Annecy, France
| | - M Romanelli
- Univ Rennes, CNRS, Institut FOTON - UMR 6082, F-35000 Rennes, France
| | - R Romano
- Dipartimento di Farmacia, Università di Salerno, I-84084 Fisciano, Salerno, Italy
- INFN, Sezione di Napoli, I-80126 Napoli, Italy
| | - A Romero
- Institut de Física d'Altes Energies (IFAE), Barcelona Institute of Science and Technology, and ICREA, E-08193 Barcelona, Spain
| | - S Ronchini
- Gran Sasso Science Institute (GSSI), I-67100 L'Aquila, Italy
- INFN, Laboratori Nazionali del Gran Sasso, I-67100 Assergi, Italy
| | - L Rosa
- INFN, Sezione di Napoli, I-80126 Napoli, Italy
- Università di Napoli "Federico II", I-80126 Napoli, Italy
| | - D Rosińska
- Astronomical Observatory Warsaw University, 00-478 Warsaw, Poland
| | - S Roy
- Institute for Gravitational and Subatomic Physics (GRASP), Utrecht University, 3584 CC Utrecht, Netherlands
| | - D Rozza
- INFN, Laboratori Nazionali del Sud, I-95125 Catania, Italy
- Università degli Studi di Sassari, I-07100 Sassari, Italy
| | - P Ruggi
- European Gravitational Observatory (EGO), I-56021 Cascina, Pisa, Italy
| | - E Ruiz Morales
- Instituto de Fisica Teorica UAM-CSIC, Universidad Autonoma de Madrid, 28049 Madrid, Spain
| | - P Saffarieh
- Nikhef, 1098 XG Amsterdam, Netherlands
- Department of Physics and Astronomy, Vrije Universiteit Amsterdam, 1081 HV Amsterdam, Netherlands
| | - O S Salafia
- Università degli Studi di Milano-Bicocca, I-20126 Milano, Italy
- INFN, Sezione di Milano-Bicocca, I-20126 Milano, Italy
- INAF, Osservatorio Astronomico di Brera sede di Merate, I-23807 Merate, Lecco, Italy
| | - L Salconi
- European Gravitational Observatory (EGO), I-56021 Cascina, Pisa, Italy
| | - F Salemi
- Università di Trento, Dipartimento di Fisica, I-38123 Povo, Trento, Italy
- INFN, Trento Institute for Fundamental Physics and Applications, I-38123 Povo, Trento, Italy
| | - M Sallé
- Nikhef, 1098 XG Amsterdam, Netherlands
| | - A Samajdar
- INFN, Sezione di Milano-Bicocca, I-20126 Milano, Italy
| | - N Sanchis-Gual
- Departamento de Astronomía y Astrofísica, Universitat de València, E-46100 Burjassot, València, Spain
- Departamento de Matemática da Universidade de Aveiro and Centre for Research and Development in Mathematics and Applications, 3810-183 Aveiro, Portugal
| | - A Sanuy
- Institut de Ciències del Cosmos (ICCUB), Universitat de Barcelona (UB), carrer Martí i Franquès, 1, 08028 Barcelona, Spain
| | - A Sasli
- Department of Physics, Aristotle University of Thessaloniki, 54124 Thessaloniki, Greece
| | - P Sassi
- INFN, Sezione di Perugia, I-06123 Perugia, Italy
- Università di Perugia, I-06123 Perugia, Italy
| | - B Sassolas
- Université Lyon, Université Claude Bernard Lyon 1, CNRS, Laboratoire des Matériaux Avancés (LMA), IP2I Lyon / IN2P3, UMR 5822, F-69622 Villeurbanne, France
| | - S Sayah
- Université Lyon, Université Claude Bernard Lyon 1, CNRS, Laboratoire des Matériaux Avancés (LMA), IP2I Lyon / IN2P3, UMR 5822, F-69622 Villeurbanne, France
| | - S Schmidt
- Institute for Gravitational and Subatomic Physics (GRASP), Utrecht University, 3584 CC Utrecht, Netherlands
| | - M Seglar-Arroyo
- Université Savoie Mont Blanc, CNRS, Laboratoire d'Annecy de Physique des Particules - IN2P3, F-74000 Annecy, France
| | - D Sentenac
- European Gravitational Observatory (EGO), I-56021 Cascina, Pisa, Italy
| | - V Sequino
- INFN, Sezione di Napoli, I-80126 Napoli, Italy
- Università di Napoli "Federico II", I-80126 Napoli, Italy
| | - G Servignat
- Laboratoire Univers et Théories, Observatoire de Paris, 92190 Meudon, France
| | - Y Setyawati
- Institute for Gravitational and Subatomic Physics (GRASP), Utrecht University, 3584 CC Utrecht, Netherlands
| | - N S Shcheblanov
- NAVIER, École des Ponts, Univ Gustave Eiffel, CNRS, Marne-la-Vallée, France
- Laboratoire MSME, Cité Descartes, 5 Boulevard Descartes, Champs-sur-Marne, 77454 Marne-la-Vallée Cedex 2, France
| | - M Sieniawska
- Université catholique de Louvain, B-1348 Louvain-la-Neuve, Belgium
| | - L Silenzi
- INFN, Sezione di Perugia, I-06123 Perugia, Italy
- Università di Camerino, I-62032 Camerino, Italy
| | - N Singh
- Astronomical Observatory Warsaw University, 00-478 Warsaw, Poland
| | - A Singha
- Maastricht University, 6200 MD Maastricht, Netherlands
- Nikhef, 1098 XG Amsterdam, Netherlands
| | - V Sipala
- INFN, Laboratori Nazionali del Sud, I-95125 Catania, Italy
- Università degli Studi di Sassari, I-07100 Sassari, Italy
| | - J Soldateschi
- INFN, Sezione di Firenze, I-50019 Sesto Fiorentino, Firenze, Italy
- Università di Firenze, Sesto Fiorentino I-50019, Italy
- INAF, Osservatorio Astrofisico di Arcetri, I-50125 Firenze, Italy
| | - V Sordini
- Université Lyon, Université Claude Bernard Lyon 1, CNRS, IP2I Lyon / IN2P3, UMR 5822, F-69622 Villeurbanne, France
| | | | - N Sorrentino
- INFN, Sezione di Pisa, I-56127 Pisa, Italy
- Università di Pisa, I-56127 Pisa, Italy
| | - R Soulard
- Université Côte d'Azur, Observatoire Côte d'Azur, CNRS, Artemis, F-06304 Nice, France
| | - V Spagnuolo
- Maastricht University, 6200 MD Maastricht, Netherlands
- Nikhef, 1098 XG Amsterdam, Netherlands
| | - M Spera
- Università di Padova, Dipartimento di Fisica e Astronomia, I-35131 Padova, Italy
- INFN, Sezione di Padova, I-35131 Padova, Italy
| | - P Spinicelli
- European Gravitational Observatory (EGO), I-56021 Cascina, Pisa, Italy
| | - C Stachie
- Université Côte d'Azur, Observatoire Côte d'Azur, CNRS, Artemis, F-06304 Nice, France
| | - D A Steer
- Université Paris Cité, CNRS, Astroparticule et Cosmologie, F-75013 Paris, France
| | - J Steinlechner
- Maastricht University, 6200 MD Maastricht, Netherlands
- Nikhef, 1098 XG Amsterdam, Netherlands
| | - S Steinlechner
- Maastricht University, 6200 MD Maastricht, Netherlands
- Nikhef, 1098 XG Amsterdam, Netherlands
| | - N Stergioulas
- Department of Physics, Aristotle University of Thessaloniki, 54124 Thessaloniki, Greece
| | - G Stratta
- INFN, Sezione di Roma, I-00185 Roma, Italy
- Institut für Theoretische Physik, Johann Wolfgang Goethe-Universität, Max-von-Laue-Straße 1, 60438 Frankfurt am Main, Germany
- Istituto di Astrofisica e Planetologia Spaziali di Roma, 00133 Roma, Italy
- INAF, Osservatorio di Astrofisica e Scienza dello Spazio, I-40129 Bologna, Italy
| | - M Suchenek
- Nicolaus Copernicus Astronomical Center, Polish Academy of Sciences, 00-716, Warsaw, Poland
| | - A Sur
- Nicolaus Copernicus Astronomical Center, Polish Academy of Sciences, 00-716, Warsaw, Poland
| | - J Suresh
- Université catholique de Louvain, B-1348 Louvain-la-Neuve, Belgium
| | | | - A Syx
- Université de Strasbourg, CNRS, IPHC UMR 7178, F-67000 Strasbourg, France
| | - P Szewczyk
- Astronomical Observatory Warsaw University, 00-478 Warsaw, Poland
| | - M Tacca
- Nikhef, 1098 XG Amsterdam, Netherlands
| | - N Tamanini
- L2IT, Laboratoire des 2 Infinis - Toulouse, Université de Toulouse, CNRS/IN2P3, UPS, F-31062 Toulouse Cedex 9, France
| | - A J Tanasijczuk
- Université catholique de Louvain, B-1348 Louvain-la-Neuve, Belgium
| | | | - C Taranto
- Università di Roma Tor Vergata, I-00133 Roma, Italy
| | - M Tonelli
- INFN, Sezione di Pisa, I-56127 Pisa, Italy
- Università di Pisa, I-56127 Pisa, Italy
| | - A Torres-Forné
- Departamento de Astronomía y Astrofísica, Universitat de València, E-46100 Burjassot, València, Spain
| | - I Tosta E Melo
- INFN, Laboratori Nazionali del Sud, I-95125 Catania, Italy
| | - E Tournefier
- Université Savoie Mont Blanc, CNRS, Laboratoire d'Annecy de Physique des Particules - IN2P3, F-74000 Annecy, France
| | - A Trapananti
- INFN, Sezione di Perugia, I-06123 Perugia, Italy
- Università di Camerino, I-62032 Camerino, Italy
| | - F Travasso
- INFN, Sezione di Perugia, I-06123 Perugia, Italy
- Università di Camerino, I-62032 Camerino, Italy
| | - J Trenado
- Institut de Ciències del Cosmos (ICCUB), Universitat de Barcelona (UB), carrer Martí i Franquès, 1, 08028 Barcelona, Spain
| | - M C Tringali
- European Gravitational Observatory (EGO), I-56021 Cascina, Pisa, Italy
| | - L Troiano
- INFN, Sezione di Napoli, Gruppo Collegato di Salerno, I-80126 Napoli, Italy
- Dipartimento di Scienze Aziendali - Management and Innovation Systems (DISA-MIS), Università di Salerno, I-84084 Fisciano, Salerno, Italy
| | - A Trovato
- INFN, Sezione di Trieste, I-34127 Trieste, Italy
- Dipartimento di Fisica, Università di Trieste, I-34127 Trieste, Italy
| | - L Trozzo
- INFN, Sezione di Napoli, I-80126 Napoli, Italy
| | - K W Tsang
- Nikhef, 1098 XG Amsterdam, Netherlands
- Institute for Gravitational and Subatomic Physics (GRASP), Utrecht University, 3584 CC Utrecht, Netherlands
- Van Swinderen Institute for Particle Physics and Gravity, University of Groningen, 9747 AG Groningen, Netherlands
| | - K Turbang
- Universiteit Antwerpen, 2000 Antwerpen, Belgium
- Vrije Universiteit Brussel, 1050 Brussel, Belgium
| | - M Turconi
- Université Côte d'Azur, Observatoire Côte d'Azur, CNRS, Artemis, F-06304 Nice, France
| | - C Turski
- Universiteit Gent, B-9000 Gent, Belgium
| | - H Ubach
- Institut de Ciències del Cosmos (ICCUB), Universitat de Barcelona (UB), carrer Martí i Franquès, 1, 08028 Barcelona, Spain
- Departament de Física Quàntica i Astrofísica (FQA), Universitat de Barcelona (UB), carrer Martí i Franqués, 1, 08028 Barcelona, Spain
| | - A Utina
- Maastricht University, 6200 MD Maastricht, Netherlands
- Nikhef, 1098 XG Amsterdam, Netherlands
| | - M Valentini
- Università di Trento, Dipartimento di Fisica, I-38123 Povo, Trento, Italy
- INFN, Trento Institute for Fundamental Physics and Applications, I-38123 Povo, Trento, Italy
| | - S Vallero
- INFN Sezione di Torino, I-10125 Torino, Italy
| | | | | | - M van Dael
- Nikhef, 1098 XG Amsterdam, Netherlands
- Eindhoven University of Technology, 5600 MB Eindhoven, Netherlands
| | - J F J van den Brand
- Maastricht University, 6200 MD Maastricht, Netherlands
- Nikhef, 1098 XG Amsterdam, Netherlands
- Department of Physics and Astronomy, Vrije Universiteit Amsterdam, 1081 HV Amsterdam, Netherlands
| | - C Van Den Broeck
- Nikhef, 1098 XG Amsterdam, Netherlands
- Institute for Gravitational and Subatomic Physics (GRASP), Utrecht University, 3584 CC Utrecht, Netherlands
| | - M van der Sluys
- Nikhef, 1098 XG Amsterdam, Netherlands
- Institute for Gravitational and Subatomic Physics (GRASP), Utrecht University, 3584 CC Utrecht, Netherlands
| | - A Van de Walle
- Université Paris-Saclay, CNRS/IN2P3, IJCLab, 91405 Orsay, France
| | - J van Dongen
- Nikhef, 1098 XG Amsterdam, Netherlands
- Department of Physics and Astronomy, Vrije Universiteit Amsterdam, 1081 HV Amsterdam, Netherlands
| | | | | | - Z van Ranst
- Maastricht University, 6200 MD Maastricht, Netherlands
| | | | - M Vardaro
- Nikhef, 1098 XG Amsterdam, Netherlands
- Institute for High-Energy Physics, University of Amsterdam, 1098 XH Amsterdam, Netherlands
| | - M Vasúth
- Wigner RCP, RMKI, H-1121 Budapest, Hungary
| | - G Vedovato
- INFN, Sezione di Padova, I-35131 Padova, Italy
| | - P Verdier
- Université Lyon, Université Claude Bernard Lyon 1, CNRS, IP2I Lyon / IN2P3, UMR 5822, F-69622 Villeurbanne, France
| | - D Verkindt
- Université Savoie Mont Blanc, CNRS, Laboratoire d'Annecy de Physique des Particules - IN2P3, F-74000 Annecy, France
| | - P Verma
- National Center for Nuclear Research, 05-400 Świerk-Otwock, Poland
| | - F Vetrano
- Università degli Studi di Urbino "Carlo Bo", I-61029 Urbino, Italy
| | - A Viceré
- Università degli Studi di Urbino "Carlo Bo", I-61029 Urbino, Italy
- INFN, Sezione di Firenze, I-50019 Sesto Fiorentino, Firenze, Italy
| | - J-Y Vinet
- Université Côte d'Azur, Observatoire Côte d'Azur, CNRS, Artemis, F-06304 Nice, France
| | - S Viret
- Université Lyon, Université Claude Bernard Lyon 1, CNRS, IP2I Lyon / IN2P3, UMR 5822, F-69622 Villeurbanne, France
| | - A Virtuoso
- INFN, Sezione di Trieste, I-34127 Trieste, Italy
- Dipartimento di Fisica, Università di Trieste, I-34127 Trieste, Italy
| | - H Vocca
- INFN, Sezione di Perugia, I-06123 Perugia, Italy
- Università di Perugia, I-06123 Perugia, Italy
| | - R C Walet
- Nikhef, 1098 XG Amsterdam, Netherlands
| | - M Was
- Université Savoie Mont Blanc, CNRS, Laboratoire d'Annecy de Physique des Particules - IN2P3, F-74000 Annecy, France
| | - N Yadav
- Nicolaus Copernicus Astronomical Center, Polish Academy of Sciences, 00-716, Warsaw, Poland
| | - A Zadrożny
- National Center for Nuclear Research, 05-400 Świerk-Otwock, Poland
| | - T Zelenova
- European Gravitational Observatory (EGO), I-56021 Cascina, Pisa, Italy
| | - J-P Zendri
- INFN, Sezione di Padova, I-35131 Padova, Italy
| | - Y Zhao
- Université Paris Cité, CNRS, Astroparticule et Cosmologie, F-75013 Paris, France
- National Astronomical Observatory of Japan, 2-21-1 Osawa, Mitaka, Tokyo 181-8588, Japan
- Institute for Cosmic Ray Research (ICRR), KAGRA Observatory, The University of Tokyo, Kamioka-cho, Hida City, Gifu 506-1205, Japan
| | - M Zerrad
- Institut Fresnel, Faculté des Sciences St Jérôme Avenue Escadrille Normandie-Niemen, F-13013 Marseille, France
| | - H Vahlbruch
- Institut für Gravitationsphysik, Leibniz Universität Hannover and Max-Planck-Institut für Gravitationsphysik (Albert-Einstein-Institut), Callinstraße 38, 30167 Hannover, Germany
| | - M Mehmet
- Institut für Gravitationsphysik, Leibniz Universität Hannover and Max-Planck-Institut für Gravitationsphysik (Albert-Einstein-Institut), Callinstraße 38, 30167 Hannover, Germany
| | - H Lück
- Institut für Gravitationsphysik, Leibniz Universität Hannover and Max-Planck-Institut für Gravitationsphysik (Albert-Einstein-Institut), Callinstraße 38, 30167 Hannover, Germany
| | - K Danzmann
- Institut für Gravitationsphysik, Leibniz Universität Hannover and Max-Planck-Institut für Gravitationsphysik (Albert-Einstein-Institut), Callinstraße 38, 30167 Hannover, Germany
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Chauhan R, Singh N, Reddy A, Singh A. The role of dexmedetomidine in post cranioplasty refractory status epilepticus. Anaesth Rep 2023; 11:e12246. [PMID: 37736063 PMCID: PMC10511152 DOI: 10.1002/anr3.12246] [Citation(s) in RCA: 0] [Impact Index Per Article: 0] [Reference Citation Analysis] [What about the content of this article? (0)] [Affiliation(s)] [Abstract] [Key Words] [Track Full Text] [Journal Information] [Subscribe] [Scholar Register] [Accepted: 09/05/2023] [Indexed: 09/23/2023] Open
Abstract
Cranioplasty, specifically a repair of the skull defect resulting from a previous decompressive craniectomy, is a relatively simple procedure associated with a minimal rate of complications. Even though seizures are seen in up to 30% of the patients postoperatively, status epilepticus is not commonly described. Cerebral oedema, ischaemia and neuro-inflammation have been reported as putative causes of seizures in this population. Here, we report a case of refractory status epilepticus unresponsive to standard anti-epileptic and anaesthetic agents. The use of dexmedetomidine helped terminate the episode and led to a favourable outcome. Most of the standard anti-epileptic and anaesthetic agents act through potentiation of GABAergic transmission or sodium channel blockade and postsynaptic adrenoceptor activation by dexmedetomidine may help potentiate their effect. Further studies are needed to investigate its anticonvulsant effect on post-traumatic brain injury and elaborate on optimal dosage.
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Affiliation(s)
- R. Chauhan
- Department of Anaesthesia and Intensive CarePostgraduate Institute of Medical Education and ResearchChandigarhIndia
| | - N. Singh
- Department of AnaesthesiologySanjay Gandhi Postgraduate Institute of Medical Sciences and ResearchLucknowIndia
| | - A. Reddy
- Department of Anaesthesia and Intensive CarePostgraduate Institute of Medical Education and ResearchChandigarhIndia
| | - A. Singh
- Department of NeurosurgeryPostgraduate Institute of Medical Education and ResearchChandigarhIndia
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Yadav IS, Singh N, Wu S, Raupp J, Wilson DL, Rawat N, Gill BS, Poland J, Tiwari VK. Exploring genetic diversity of wild and related tetraploid wheat species Triticum turgidum and Triticum timopheevii. J Adv Res 2023; 48:47-60. [PMID: 36084813 PMCID: PMC10248793 DOI: 10.1016/j.jare.2022.08.020] [Citation(s) in RCA: 2] [Impact Index Per Article: 2.0] [Reference Citation Analysis] [What about the content of this article? (0)] [Affiliation(s)] [Abstract] [Key Words] [MESH Headings] [Track Full Text] [Journal Information] [Subscribe] [Scholar Register] [Received: 06/20/2022] [Revised: 08/25/2022] [Accepted: 08/31/2022] [Indexed: 11/27/2022] Open
Abstract
INTRODUCTION The domestication bottleneck has reduced genetic diversity inwheat, necessitating the use of wild relatives in breeding programs. Wild tetraploid wheat are widely used in the breeding programs but with morphological characters, it is difficult to distinguish these, resulting in misclassification/mislabeling or duplication of accessions in the Gene bank. OBJECTIVES The study aims to exploreGenotyping by sequencing (GBS) to characterize wild and domesticated tetraploid wheat accessions to generate a core set of accessions to be used in the breeding program. METHODS TASSEL-GBS pipeline was used for SNP discovery, fastStructure was used to determine the population structure and PowerCore was used to generate a core sets. Nucleotide diversity matrices of Nie's and F-statistics (FST) index were used to determine the center of genetic diversity. RESULTS We found 65 % and 47 % duplicated accessions in Triticum timopheevii and T. turgidum respectively. Genome-wide nucleotide diversity and FST scan uncovered a lower intra and higher inter-species differentiation. Distinct FST regions were identified in genomic regions belonging to domestication genes: non-brittle rachis (Btr1) and vernalization (VRN-1).Our results suggest that Israel, Jordan, Syria, and Lebanonas the hub of genetic diversity of wild emmer;Turkey, and Georgia for T. durum; and Iraq, Azerbaijan, and Armenia for theT. timopheevii. Identified core set accessions preserved more than 93 % of the available genetic diversity. Genome wide association study (GWAS) indicated the potential chromosomal segment for resistance to leaf rust in T. timopheevii. CONCLUSION The present study explored the potential of GBS technology in data reduction while maintaining the significant genetic diversity of the species. Wild germplasm showed more differentiation than domesticated accessions, indicating the availability of sufficient diversity for crop improvement. With reduced complexity, the core set preserves the genetic diversity of the gene bank collections and will aid in a more robust characterization of wild germplasm.
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Affiliation(s)
- Inderjit S. Yadav
- Department of Plant Sciences and Landscape Architecture, University of Maryland, College Park, MD 20742, USA
| | | | - Shuangye Wu
- Department of Plant Pathology and Wheat Genetics Resource Center, Kansas State University, 1712 Claflin Road, Manhattan, KS 66506, USA
| | - Jon Raupp
- Department of Plant Pathology and Wheat Genetics Resource Center, Kansas State University, 1712 Claflin Road, Manhattan, KS 66506, USA
| | - Duane L. Wilson
- Department of Plant Pathology and Wheat Genetics Resource Center, Kansas State University, 1712 Claflin Road, Manhattan, KS 66506, USA
| | - Nidhi Rawat
- Department of Plant Sciences and Landscape Architecture, University of Maryland, College Park, MD 20742, USA
| | - Bikram S. Gill
- Department of Plant Pathology and Wheat Genetics Resource Center, Kansas State University, 1712 Claflin Road, Manhattan, KS 66506, USA
| | - Jesse Poland
- Biological and Environmental Science and Engineering Division, King Abdullah University of Science and Technology, 4700 KAUST, Thuwal 23955-6900, Saudi Arabia
| | - Vijay K. Tiwari
- Department of Plant Sciences and Landscape Architecture, University of Maryland, College Park, MD 20742, USA
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Hasan Z, Lee M, Chen F, Key S, Habib AR, Aweidah L, Sacks R, Singh N. A Computer Vision Algorithm to Classify Pneumatization of the Mastoid Process on Temporal Bone Computed Tomography Scans. J Int Adv Otol 2023; 19:217-222. [PMID: 37272639 DOI: 10.5152/iao.2023.22958] [Citation(s) in RCA: 0] [Impact Index Per Article: 0] [Reference Citation Analysis] [What about the content of this article? (0)] [Affiliation(s)] [Abstract] [Track Full Text] [Journal Information] [Subscribe] [Scholar Register] [Indexed: 06/06/2023] Open
Abstract
BACKGROUND Pneumatization of the mastoid process is variable and of significance to the operative surgeon. Surgical approaches to the temporal bone require an understanding of pneumatization and its implications for surgical access. This study aims to determine the feasibility of using deep learning convolutional neural network algorithms to classify pneumatization of the mastoid process. METHODS De-identified petrous temporal bone images were acquired from a tertiary hospital radiology picture archiving and communication system. A binary classification mode in the pretrained convolutional neural network was used to investigate the utility of convolutional neural networks in temporal bone imaging. False positive and negative images were reanalyzed by the investigators and qualitatively assessed to consider reasons for inaccuracy. RESULTS The overall accuracy of the model was 0.954. At a probability threshold of 65%, the sensitivity of the model was 0.860 (95% CI 0.783-0.934) and the specificity was 0.989 (95% CI 0.960-0.999). The positive predictive value was 0.973 (95% CI 0.904-0.993) and the negative predictive value was 0.935 (95% CI 0.901-0.965). The false positive rate was 0.006. The F1 number was 0.926 demonstrating a high accuracy for the model. CONCLUSION The temporal bone is a complex anatomical region of interest to otolaryngologists. Surgical planning requires high-resolution computed tomography scans, the interpretation of which can be augmented with machine learning. This initial study demonstrates the feasibility of utilizing machine learning algorithms to discriminate anatomical variation with a high degree of accuracy. It is hoped this will lead to further investigation regarding more complex anatomical structures in the temporal bone.
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Affiliation(s)
- Zubair Hasan
- University of Sydney, Faculty of Medicine and Health, New South Wales, Australia;Department of Otolaryngology - Head and Neck Surgery, Westmead Hospital, New South
| | - Michael Lee
- Department of Otolaryngology - Head and Neck Surgery, Westmead Hospital, New South Wales, Australia
| | - Fiona Chen
- Department of Otolaryngology Royal Children's Hospital Melbourne, Victoria, Australia
| | - Seraphina Key
- Monash University, Faculty of Medicine, Nursing and Health Sciences, Victoria, Australia
| | - Al-Rahim Habib
- University of Sydney, Faculty of Medicine and Health, New South Wales, Australia;Department of Otolaryngology - Head and Neck Surgery, Westmead Hospital, New South
| | - Layal Aweidah
- University of Notre Dame, Faculty of Medicine, New South Wales, Australia
| | - Raymond Sacks
- University of Sydney, Faculty of Medicine and Health, New South Wales, Australia; Department of Otolaryngology - Head and Neck Surgery, Concord Hospital, New South Wales, Australia
| | - Narinder Singh
- University of Sydney, Faculty of Medicine and Health, New South Wales, Australia;Department of Otolaryngology - Head and Neck Surgery, Westmead Hospital, New South Wales, Australia
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Zhu K, Bala F, Zhang J, Benali F, Cimflova P, Kim BJ, McDonough R, Singh N, Hill MD, Goyal M, Demchuk A, Menon BK, Qiu W. Automated Segmentation of Intracranial Thrombus on NCCT and CTA in Patients with Acute Ischemic Stroke Using a Coarse-to-Fine Deep Learning Model. AJNR Am J Neuroradiol 2023; 44:641-648. [PMID: 37202113 PMCID: PMC10249699 DOI: 10.3174/ajnr.a7878] [Citation(s) in RCA: 0] [Impact Index Per Article: 0] [Reference Citation Analysis] [What about the content of this article? (0)] [Affiliation(s)] [Abstract] [MESH Headings] [Track Full Text] [Journal Information] [Subscribe] [Scholar Register] [Received: 10/18/2022] [Accepted: 04/20/2023] [Indexed: 05/20/2023]
Abstract
BACKGROUND AND PURPOSE Identifying the presence and extent of intracranial thrombi is crucial in selecting patients with acute ischemic stroke for treatment. This article aims to develop an automated approach to quantify thrombus on NCCT and CTA in patients with stroke. MATERIALS AND METHODS A total of 499 patients with large-vessel occlusion from the Safety and Efficacy of Nerinetide in Subjects Undergoing Endovascular Thrombectomy for Stroke (ESCAPE-NA1) trial were included. All patients had thin-section NCCT and CTA images. Thrombi contoured manually were used as reference standard. A deep learning approach was developed to segment thrombi automatically. Of 499 patients, 263 and 66 patients were randomly selected to train and validate the deep learning model, respectively; the remaining 170 patients were independently used for testing. The deep learning model was quantitatively compared with the reference standard using the Dice coefficient and volumetric error. The proposed deep learning model was externally tested on 83 patients with and without large-vessel occlusion from another independent trial. RESULTS The developed deep learning approach obtained a Dice coefficient of 70.7% (interquartile range, 58.0%-77.8%) in the internal cohort. The predicted thrombi length and volume were correlated with those of expert-contoured thrombi (r = 0.88 and 0.87, respectively; P < .001). When the derived deep learning model was applied to the external data set, the model obtained similar results in patients with large-vessel occlusion regarding the Dice coefficient (66.8%; interquartile range, 58.5%-74.6%), thrombus length (r = 0.73), and volume (r = 0.80). The model also obtained a sensitivity of 94.12% (32/34) and a specificity of 97.96% (48/49) in classifying large-vessel occlusion versus non-large-vessel occlusion. CONCLUSIONS The proposed deep learning method can reliably detect and measure thrombi on NCCT and CTA in patients with acute ischemic stroke.
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Affiliation(s)
- K Zhu
- From the Department of Clinical Neurosciences and Hotchkiss Brain Institute (K.Z., F. Bala, J.Z., F. Benali, P.C., R.M., N.S., M.D.H., M.G., A.D., B.K.M.)
- College of Electronic Engineering (K.Z.), Xi'an Shiyou University, Xi'an, Shaanxi, China
| | - F Bala
- From the Department of Clinical Neurosciences and Hotchkiss Brain Institute (K.Z., F. Bala, J.Z., F. Benali, P.C., R.M., N.S., M.D.H., M.G., A.D., B.K.M.)
| | - J Zhang
- From the Department of Clinical Neurosciences and Hotchkiss Brain Institute (K.Z., F. Bala, J.Z., F. Benali, P.C., R.M., N.S., M.D.H., M.G., A.D., B.K.M.)
| | - F Benali
- From the Department of Clinical Neurosciences and Hotchkiss Brain Institute (K.Z., F. Bala, J.Z., F. Benali, P.C., R.M., N.S., M.D.H., M.G., A.D., B.K.M.)
| | - P Cimflova
- From the Department of Clinical Neurosciences and Hotchkiss Brain Institute (K.Z., F. Bala, J.Z., F. Benali, P.C., R.M., N.S., M.D.H., M.G., A.D., B.K.M.)
- Department of Medicine, and Department of Radiology (P.C., M.D.H., A.D.), Cumming School of Medicine, University of Calgary, Calgary, Alberta, Canada
- St. Anne's University Hospital Brno and Faculty of Medicine (P.C.), Masaryk University, Brno, Czech Republic
| | - B J Kim
- Department of Neurology and Cerebrovascular Center (B.J.K.), Seoul National University Bundang Hospital, Seongnam-si, Gyeonggi-do, Korea
| | - R McDonough
- From the Department of Clinical Neurosciences and Hotchkiss Brain Institute (K.Z., F. Bala, J.Z., F. Benali, P.C., R.M., N.S., M.D.H., M.G., A.D., B.K.M.)
- Department of Diagnostic and Interventional Neuroradiology (R.M.), University Hospital Hamburg, Hamburg, Germany
| | - N Singh
- From the Department of Clinical Neurosciences and Hotchkiss Brain Institute (K.Z., F. Bala, J.Z., F. Benali, P.C., R.M., N.S., M.D.H., M.G., A.D., B.K.M.)
| | - M D Hill
- From the Department of Clinical Neurosciences and Hotchkiss Brain Institute (K.Z., F. Bala, J.Z., F. Benali, P.C., R.M., N.S., M.D.H., M.G., A.D., B.K.M.)
- Department of Community Health Sciences (M.D.H.)
- Department of Medicine, and Department of Radiology (P.C., M.D.H., A.D.), Cumming School of Medicine, University of Calgary, Calgary, Alberta, Canada
| | - M Goyal
- From the Department of Clinical Neurosciences and Hotchkiss Brain Institute (K.Z., F. Bala, J.Z., F. Benali, P.C., R.M., N.S., M.D.H., M.G., A.D., B.K.M.)
| | - A Demchuk
- From the Department of Clinical Neurosciences and Hotchkiss Brain Institute (K.Z., F. Bala, J.Z., F. Benali, P.C., R.M., N.S., M.D.H., M.G., A.D., B.K.M.)
- Department of Medicine, and Department of Radiology (P.C., M.D.H., A.D.), Cumming School of Medicine, University of Calgary, Calgary, Alberta, Canada
| | - B K Menon
- From the Department of Clinical Neurosciences and Hotchkiss Brain Institute (K.Z., F. Bala, J.Z., F. Benali, P.C., R.M., N.S., M.D.H., M.G., A.D., B.K.M.)
| | - W Qiu
- School of Life Science and Technology (W.Q.), Huazhong University of Science and Technology, Wuhan, Hubei, China
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Zobair THA, Singh N, Alameen MAS, Said-Hartley Q, Lephoi M, Raine RI. Abnormal chest radiograph in an asymptomatic young man - what is the differential diagnosis? Afr J Thorac Crit Care Med 2023; 29:29. [PMID: 37818208 PMCID: PMC10561714] [Citation(s) in RCA: 0] [Impact Index Per Article: 0] [Reference Citation Analysis] [What about the content of this article? (0)] [Affiliation(s)] [Download PDF] [Figures] [Journal Information] [Subscribe] [Scholar Register] [Indexed: 10/12/2023] Open
Affiliation(s)
- T H A Zobair
- Division of Pulmonology, Department of Medicine, Faculty of Health Sciences, University of Cape Town and Groote Schuur Hospital, Cape Town, South Africa
| | - N Singh
- Division of Pulmonology, Department of Medicine, Faculty of Health Sciences, University of Cape Town and Groote Schuur Hospital, Cape Town, South Africa
| | | | - Q Said-Hartley
- Division of Radiology, Faculty of Health Sciences, University of Cape Town and Groote Schuur Hospital, Cape Town, South Africa
| | - M Lephoi
- Chris Barnard Division of Cardiothoracic Surgery, Faculty of Health Sciences, University of Cape Town and Groote Schuur Hospital, Cape Town, South Africa
| | - R I Raine
- Division of Pulmonology, Department of Medicine, Faculty of Health Sciences, University of Cape Town and Groote Schuur Hospital, Cape Town, South Africa
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22
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Singh A, Singh G, Kaur N, Singh N. Quantitative and qualitative analysis of ochratoxin-A using fluorescent CQDs@DNA-based nanoarchitecture assembly to monitor food safety and quality. Anal Methods 2023; 15:1826-1835. [PMID: 36971227 DOI: 10.1039/d3ay00209h] [Citation(s) in RCA: 1] [Impact Index Per Article: 1.0] [Reference Citation Analysis] [What about the content of this article? (0)] [Affiliation(s)] [Abstract] [MESH Headings] [Track Full Text] [Subscribe] [Scholar Register] [Indexed: 06/18/2023]
Abstract
Ochratoxin A (OTA), a mycotoxin formed by various fungi, such as Aspergillus and Penicillium species, is dangerous to human health. Thus, to circumvent the risk of OTA ingestion, the recognition and quantification of OTA levels are of great significance. A perusal of the literature has revealed that the integration of DNA/Carbon Quantum Dot (CQD)-based hybrid systems may exhibit the unique electronic and optical properties of nanomaterials/nanoarchitecture and consequent recognition properties. Herein, we developed the CQDs@DNA-based hybrid nanoarchitecture system for the selective detection of OTA, which exhibits modulation in the emission spectrum after interaction with OTA, with a significant binding constant (Ka = 3.5 × 105 M-1), a limit of detection of 14 nM, limit of quantification of 47 nM and working range of 1-10 μM. The mechanism for sensing the OTA has been corroborated using fluorescence, UV-visible absorption spectroscopy, and FTIR techniques, demonstrating the binding mode of CQD@DNA hybrid nano-architecture assembly with OTA. Further, we demonstrated the sensing ability of developed CQDs@DNA-based nanoarchitecture assembly towards the quantification of OTA in real food monitoring analysis for real-time applications, which makes this developed nanoarchitecture assembly the potential candidate to conveniently monitor food safety and quality for human health.
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Affiliation(s)
- Amanpreet Singh
- Department of Chemistry, Indian Institute of Technology Ropar, Rupnagar, 140001, Punjab, India.
| | - Gagandeep Singh
- Department of Biomedical Engineering, Indian Institute of Technology Ropar, Rupnagar, 140001, Punjab, India
| | - Navneet Kaur
- Department of Chemistry, Panjab University, Chandigarh, 160014, Punjab, India.
| | - Narinder Singh
- Department of Chemistry, Indian Institute of Technology Ropar, Rupnagar, 140001, Punjab, India.
- Department of Biomedical Engineering, Indian Institute of Technology Ropar, Rupnagar, 140001, Punjab, India
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23
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Hasan Z, Key S, Habib AR, Wong E, Aweidah L, Kumar A, Sacks R, Singh N. Convolutional Neural Networks in ENT Radiology: Systematic Review of the Literature. Ann Otol Rhinol Laryngol 2023; 132:417-430. [PMID: 35651308 DOI: 10.1177/00034894221095899] [Citation(s) in RCA: 1] [Impact Index Per Article: 1.0] [Reference Citation Analysis] [What about the content of this article? (0)] [Affiliation(s)] [Abstract] [Key Words] [MESH Headings] [Track Full Text] [Journal Information] [Subscribe] [Scholar Register] [Indexed: 11/16/2022]
Abstract
INTRODUCTION Convolutional neural networks (CNNs) represent a state-of-the-art methodological technique in AI and deep learning, and were specifically created for image classification and computer vision tasks. CNNs have been applied in radiology in a number of different disciplines, mostly outside otolaryngology, potentially due to a lack of familiarity with this technology within the otolaryngology community. CNNs have the potential to revolutionize clinical practice by reducing the time required to perform manual tasks. This literature search aims to present a comprehensive systematic review of the published literature with regard to CNNs and their utility to date in ENT radiology. METHODS Data were extracted from a variety of databases including PubMED, Proquest, MEDLINE Open Knowledge Maps, and Gale OneFile Computer Science. Medical subject headings (MeSH) terms and keywords were used to extract related literature from each databases inception to October 2020. Inclusion criteria were studies where CNNs were used as the main intervention and CNNs focusing on radiology relevant to ENT. Titles and abstracts were reviewed followed by the contents. Once the final list of articles was obtained, their reference lists were also searched to identify further articles. RESULTS Thirty articles were identified for inclusion in this study. Studies utilizing CNNs in most ENT subspecialties were identified. Studies utilized CNNs for a number of tasks including identification of structures, presence of pathology, and segmentation of tumors for radiotherapy planning. All studies reported a high degree of accuracy of CNNs in performing the chosen task. CONCLUSION This study provides a better understanding of CNN methodology used in ENT radiology demonstrating a myriad of potential uses for this exciting technology including nodule and tumor identification, identification of anatomical variation, and segmentation of tumors. It is anticipated that this field will continue to evolve and these technologies and methodologies will become more entrenched in our everyday practice.
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Affiliation(s)
- Zubair Hasan
- Faculty of Medicine and Health, University of Sydney, Camperdown, NSW, Australia
- Department of Otolaryngology - Head and Neck Surgery, Westmead Hospital, Westmead, NSW, Australia
| | - Seraphina Key
- Faculty of Medicine, Nursing and Health Sciences, Monash University, Clayton, VIC, Australia
| | - Al-Rahim Habib
- Faculty of Medicine and Health, University of Sydney, Camperdown, NSW, Australia
- Department of Otolaryngology - Head and Neck Surgery, Westmead Hospital, Westmead, NSW, Australia
- Department of Otolaryngology - Head and Neck Surgery, Princess Alexandra Hospital, Woolloongabba, QLD, Australia
| | - Eugene Wong
- Department of Otolaryngology - Head and Neck Surgery, Westmead Hospital, Westmead, NSW, Australia
| | - Layal Aweidah
- Faculty of Medicine, University of Notre Dame, Darlinghurst, NSW, Australia
| | - Ashnil Kumar
- School of Biomedical Engineering, Faculty of Engineering, University of Sydney, Darlington, NSW, Australia
| | - Raymond Sacks
- Faculty of Medicine and Health, University of Sydney, Camperdown, NSW, Australia
- Department of Otolaryngology - Head and Neck Surgery, Concord Hospital, Concord, NSW, Australia
| | - Narinder Singh
- Faculty of Medicine and Health, University of Sydney, Camperdown, NSW, Australia
- Department of Otolaryngology - Head and Neck Surgery, Westmead Hospital, Westmead, NSW, Australia
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Habib AR, Xu Y, Bock K, Mohanty S, Sederholm T, Weeks WB, Dodhia R, Ferres JL, Perry C, Sacks R, Singh N. Evaluating the generalizability of deep learning image classification algorithms to detect middle ear disease using otoscopy. Sci Rep 2023; 13:5368. [PMID: 37005441 PMCID: PMC10067817 DOI: 10.1038/s41598-023-31921-0] [Citation(s) in RCA: 0] [Impact Index Per Article: 0] [Reference Citation Analysis] [What about the content of this article? (0)] [Affiliation(s)] [Abstract] [Journal Information] [Subscribe] [Scholar Register] [Received: 08/30/2022] [Accepted: 03/20/2023] [Indexed: 04/04/2023] Open
Abstract
To evaluate the generalizability of artificial intelligence (AI) algorithms that use deep learning methods to identify middle ear disease from otoscopic images, between internal to external performance. 1842 otoscopic images were collected from three independent sources: (a) Van, Turkey, (b) Santiago, Chile, and (c) Ohio, USA. Diagnostic categories consisted of (i) normal or (ii) abnormal. Deep learning methods were used to develop models to evaluate internal and external performance, using area under the curve (AUC) estimates. A pooled assessment was performed by combining all cohorts together with fivefold cross validation. AI-otoscopy algorithms achieved high internal performance (mean AUC: 0.95, 95%CI: 0.80-1.00). However, performance was reduced when tested on external otoscopic images not used for training (mean AUC: 0.76, 95%CI: 0.61-0.91). Overall, external performance was significantly lower than internal performance (mean difference in AUC: -0.19, p ≤ 0.04). Combining cohorts achieved a substantial pooled performance (AUC: 0.96, standard error: 0.01). Internally applied algorithms for otoscopy performed well to identify middle ear disease from otoscopy images. However, external performance was reduced when applied to new test cohorts. Further efforts are required to explore data augmentation and pre-processing techniques that might improve external performance and develop a robust, generalizable algorithm for real-world clinical applications.
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Affiliation(s)
- Al-Rahim Habib
- Faculty of Medicine and Health, University of Sydney, Sydney, NSW, Australia.
- Department of Otolaryngology, Head and Neck Surgery, Westmead Hospital, Sydney, NSW, Australia.
| | - Yixi Xu
- AI for Good Lab, Microsoft, Redmond, WA, USA
| | - Kris Bock
- Azure FastTrack Engineering, Brisbane, QLD, Australia
| | | | | | | | | | | | - Chris Perry
- University of Queensland Medical School, Brisbane, QLD, Australia
| | - Raymond Sacks
- Faculty of Medicine and Health, University of Sydney, Sydney, NSW, Australia
| | - Narinder Singh
- Faculty of Medicine and Health, University of Sydney, Sydney, NSW, Australia
- Department of Otolaryngology, Head and Neck Surgery, Westmead Hospital, Sydney, NSW, Australia
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Kaur M, Gaba J, Singh K, Bhatia Y, Singh A, Singh N. Recent Advances in Recognition Receptors for Electrochemical Biosensing of Mycotoxins-A Review. Biosensors (Basel) 2023; 13:391. [PMID: 36979603 PMCID: PMC10046307 DOI: 10.3390/bios13030391] [Citation(s) in RCA: 0] [Impact Index Per Article: 0] [Reference Citation Analysis] [What about the content of this article? (0)] [Affiliation(s)] [Abstract] [Key Words] [MESH Headings] [Track Full Text] [Figures] [Subscribe] [Scholar Register] [Received: 01/23/2023] [Revised: 03/06/2023] [Accepted: 03/08/2023] [Indexed: 06/18/2023]
Abstract
Mycotoxins are naturally occurring toxic secondary metabolites produced by fungi in cereals and foodstuffs during the stages of cultivation and storage. Electrochemical biosensing has emerged as a rapid, efficient, and economical approach for the detection and quantification of mycotoxins in different sample media. An electrochemical biosensor consists of two main units, a recognition receptor and a signal transducer. Natural or artificial antibodies, aptamers, molecularly imprinted polymers (MIP), peptides, and DNAzymes have been extensively employed as selective recognition receptors for the electrochemical biosensing of mycotoxins. This article affords a detailed discussion of the recent advances and future prospects of various types of recognition receptors exploited in the electrochemical biosensing of mycotoxins.
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Affiliation(s)
- Manpreet Kaur
- Department of Chemistry, Punjab Agricultural University, Ludhiana 141004, India
| | - Jyoti Gaba
- Department of Chemistry, Punjab Agricultural University, Ludhiana 141004, India
| | - Komal Singh
- Department of Chemistry, Punjab Agricultural University, Ludhiana 141004, India
| | - Yashika Bhatia
- Department of Chemistry, Punjab Agricultural University, Ludhiana 141004, India
| | - Anoop Singh
- Department of Chemistry, Indian Institute of Technology, Ropar 140001, India
| | - Narinder Singh
- Department of Chemistry, Indian Institute of Technology, Ropar 140001, India
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Habib AR, Perry C, Crossland G, Patel H, Kong K, Whitfield B, North H, Walton J, Da Cruz M, Suruliraj A, Smith M, Harris R, Hasan Z, Gunaratne DA, Sacks R, Singh N. Inter-rater agreement between 13 otolaryngologists to diagnose otitis media in Aboriginal and Torres Strait Islander children using a telehealth approach. Int J Pediatr Otorhinolaryngol 2023; 168:111494. [PMID: 37003013 DOI: 10.1016/j.ijporl.2023.111494] [Citation(s) in RCA: 2] [Impact Index Per Article: 2.0] [Reference Citation Analysis] [What about the content of this article? (0)] [Affiliation(s)] [Abstract] [Key Words] [Track Full Text] [Journal Information] [Submit a Manuscript] [Subscribe] [Scholar Register] [Received: 08/21/2022] [Revised: 01/07/2023] [Accepted: 02/19/2023] [Indexed: 04/03/2023]
Abstract
INTRODUCTION Telehealth programs are important to deliver otolaryngology services for Aboriginal and Torres Strait Islander children living in rural and remote areas, where distance and access to specialists is a critical factor. OBJECTIVE To evaluate the inter-rater agreement and value of increasing levels of clinical data (otoscopy with or without audiometry and in-field nurse impressions) to diagnose otitis media using a telehealth approach. DESIGN Blinded, inter-rater reliability study. SETTING Ear health and hearing assessments collected from a statewide telehealth program for Indigenous children living in rural and remote areas of Queensland, Australia. PARTICIPANTS Thirteen board-certified otolaryngologists independently reviewed 80 telehealth assessments from 65 Indigenous children (mean age 5.7 ± 3.1 years, 33.8% female). INTERVENTIONS Raters were provided increasing tiers of clinical data to assess concordance to the reference standard diagnosis: Tier A) otoscopic images alone, Tier B) otoscopic images plus tympanometry and category of hearing loss, and Tier C) as B plus static compliance, canal volume, pure-tone audiometry, and nurse impressions (otoscopic findings and presumed diagnosis). For each tier, raters were asked to determine which of the four diagnostic categories applied: normal aerated ear, acute otitis media (AOM), otitis media with effusion (OME), and chronic otitis media (COM). MAIN OUTCOME MEASURES Proportion of agreement to the reference standard, prevalence-and-bias adjusted κ coefficients, mean difference in accuracy estimates between each tier of clinical data. RESULTS Accuracy between raters and the reference standard increased with increased provision of clinical data (Tier A: 65% (95%CI: 63-68%), κ = 0.53 (95%CI: 0.48-0.57); Tier B: 77% (95%CI: 74-79%), 0.68 (95%CI: 0.65-0.72); C: 85% (95%CI: 82-87%), 0.79 (95%CI: 0.76-0.82)). Classification accuracy significantly improved between Tier A to B (mean difference:12%, p < 0.001) and between Tier B to C (mean difference: 8%, p < 0.001). The largest improvement in classification accuracy was observed between Tier A and C (mean difference: 20%, p < 0.001). Inter-rater agreement similarly improved with increasing provision of clinical data. CONCLUSIONS There is substantial agreement between otolaryngologists to diagnose ear disease using electronically stored clinical data collected from telehealth assessments. The addition of audiometry, tympanometry and nurse impressions significantly improved expert accuracy and inter-rater agreement, compared to reviewing otoscopic images alone.
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Affiliation(s)
- Al-Rahim Habib
- Sydney Medical School, Faculty of Medicine and Health, University of Sydney, Camperdown, New South Wales, 2006, Australia; Department of Otolaryngology - Head and Neck Surgery, Westmead Hospital, Westmead, New South Wales, 2145, Australia.
| | - Chris Perry
- University of Queensland Medical School, St Lucia, Queensland, 4072, Australia
| | - Graeme Crossland
- Royal Darwin Hospital, Top End Health Service, Department of Health, Tiwi, Northern Territory, 0810, Australia
| | - Hemi Patel
- Royal Darwin Hospital, Top End Health Service, Department of Health, Tiwi, Northern Territory, 0810, Australia
| | - Kelvin Kong
- School of Medicine and Public Health, University of Newcastle, Callaghan, New South Wales, 2308, Australia
| | - Bernard Whitfield
- Griffith Medical School, Griffith University, Southport, Queensland, 4215, Australia
| | - Hannah North
- Department of Otolaryngology - Head and Neck Surgery, Westmead Hospital, Westmead, New South Wales, 2145, Australia
| | - Joanna Walton
- Department of Otolaryngology - Head and Neck Surgery, The Children's Hospital at Westmead, Westmead, New South Wales, 2145, Australia
| | - Melville Da Cruz
- Sydney Medical School, Faculty of Medicine and Health, University of Sydney, Camperdown, New South Wales, 2006, Australia; Department of Otolaryngology - Head and Neck Surgery, Westmead Hospital, Westmead, New South Wales, 2145, Australia
| | - Anand Suruliraj
- Department of Otolaryngology - Head and Neck Surgery, Westmead Hospital, Westmead, New South Wales, 2145, Australia
| | - Murray Smith
- Department of Otolaryngology - Head and Neck Surgery, Westmead Hospital, Westmead, New South Wales, 2145, Australia
| | - Rhydian Harris
- Department of Otolaryngology - Head and Neck Surgery, Westmead Hospital, Westmead, New South Wales, 2145, Australia
| | - Zubair Hasan
- Department of Otolaryngology - Head and Neck Surgery, Westmead Hospital, Westmead, New South Wales, 2145, Australia
| | - Dakshika A Gunaratne
- Department of Otolaryngology - Head and Neck Surgery, Westmead Hospital, Westmead, New South Wales, 2145, Australia
| | - Raymond Sacks
- Sydney Medical School, Faculty of Medicine and Health, University of Sydney, Camperdown, New South Wales, 2006, Australia
| | - Narinder Singh
- Sydney Medical School, Faculty of Medicine and Health, University of Sydney, Camperdown, New South Wales, 2006, Australia; Department of Otolaryngology - Head and Neck Surgery, Westmead Hospital, Westmead, New South Wales, 2145, Australia
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Kaur R, Bhardwaj G, Singh N, Kaur N. Studies on Structural Changes of modified MWCNTs: Material for Electrochemical Monitoring of Antiviral Drug in Human Serum Samples. Chemistry 2023; 29:e202300017. [PMID: 36880483 DOI: 10.1002/chem.202300017] [Citation(s) in RCA: 0] [Impact Index Per Article: 0] [Reference Citation Analysis] [What about the content of this article? (0)] [Affiliation(s)] [Abstract] [Key Words] [Track Full Text] [Journal Information] [Subscribe] [Scholar Register] [Received: 01/03/2023] [Revised: 03/06/2023] [Accepted: 03/07/2023] [Indexed: 03/08/2023]
Abstract
<p style="margin:0cm;text-align:justify;line-height:200%"><span style="color:black">The development of a universal approach for precisely tuning the electrochemical characteristics of conducting carbon nanotubes for tracking harmful agents in the human body with high selectivity and sensitivity remains a challenge. Herein, we describe a simplistic, versatile, and general approach to the construction of functionalized electrochemical material. The design of electrochemical material consists of (i) modification of multiwalled carbon nanotubes (MWCNT) with dipodal naphthyl-based dipodal urea (KR-1) through non-covalent functionalization (KR-1@MWCNT) which enhances the dispersibility of MWCNT and hence conductivity, (ii) complexation of KR-1@MWCNT with Hg2+ accelerate the electron transfer in the material which amplify the detection response of functionalized material (<italic>i.e.,</italic> <bold>Hg/KR-1@MWCNT</bold>) towards various thymidine analogues. Further, the application of functionalized electrochemical material (<bold>Hg/KR-1@MWCNT)</bold> achieves real-time electrochemical monitoring of harmful antiviral drug 5-iodo-2'-iododeoxyuridine (IUdR) levels in human serum albumin for the first time.<o:p></o:p></span></p>.
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Affiliation(s)
| | | | | | - Navneet Kaur
- Panjab University, Centre for Nanoscience & Nanotechnology, Panjab University Chandigarh, 160014, Chandigarh, INDIA
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Kaur R, Bhardwaj G, Saini S, Kaur N, Singh N. A high-performance Calix@ZnO based bifunctional nanomaterial for selective detection and degradation of toxic azinphos methyl in environmental samples. Chemosphere 2023; 316:137693. [PMID: 36638927 DOI: 10.1016/j.chemosphere.2022.137693] [Citation(s) in RCA: 1] [Impact Index Per Article: 1.0] [Reference Citation Analysis] [What about the content of this article? (0)] [Affiliation(s)] [Abstract] [Key Words] [MESH Headings] [Track Full Text] [Subscribe] [Scholar Register] [Received: 11/21/2022] [Revised: 12/27/2022] [Accepted: 12/28/2022] [Indexed: 06/17/2023]
Abstract
One of the key tenets of sustainable agriculture and food safety is the removal of toxic pesticides from the environment. However, developing reliable, affordable, and efficient methods for detecting and degrading pesticides into non-toxic degradable products remains an immediate matter of concern. Herein, we attempt to develop a strategy for the detection as well as degradation of highly toxic phosphorodithioate pesticide, Azinphos methyl (AZM), using hybrid zinc oxide nanoparticles (ZnO NPs). Considering the non-selectivity of bare ZnO and receptor R1, we have fabricated the heterocalixarene-based Calix (R1) over zinc oxide (ZnO) surface in situ via the sol-gel process. The synthesized heterocaliaxrene-modified ZnO (R1@ZnO) NPs show an excellent affinity for the selective and sensitive detection of AZM with a tremendously low limit of detection (68 mg L-1) and no interference from other pesticides. Degradation of AZM was fully supported by fluorescence spectroscopy, scanning electron microscopy (SEM), 1H NMR titrations, FTIR spectroscopy, cyclic voltammetry, and mass spectroscopy, which unequivocally confirmed the formation of non-toxic products. According to our findings, R1@ZnO NPs are sustainable nanomaterials that can be employed for environmental remediation since they operate in an aqueous medium.
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Affiliation(s)
- Randeep Kaur
- Department of Chemistry & Centre for Advanced Studies in Chemistry, Panjab University, Chandigarh, 160014, India
| | - Geetika Bhardwaj
- Department of Chemistry & Centre for Advanced Studies in Chemistry, Panjab University, Chandigarh, 160014, India
| | - Sanjeev Saini
- Department of Chemistry, Indian Institute of Technology Ropar (IIT Ropar), Rupnagar, Punjab, 140001, India
| | - Navneet Kaur
- Department of Chemistry & Centre for Advanced Studies in Chemistry, Panjab University, Chandigarh, 160014, India.
| | - Narinder Singh
- Department of Chemistry, Indian Institute of Technology Ropar (IIT Ropar), Rupnagar, Punjab, 140001, India.
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Damaraju V, Singh N, Garg M, Kathirvel S, Basher RK, Grover S, Kalra N, Prasad KT. Effect of prior pulmonary TB on low-dose computed tomography during lung cancer screening. Int J Tuberc Lung Dis 2023; 27:223-225. [PMID: 36855039 DOI: 10.5588/ijtld.22.0560] [Citation(s) in RCA: 0] [Impact Index Per Article: 0] [Reference Citation Analysis] [What about the content of this article? (0)] [Affiliation(s)] [Track Full Text] [Journal Information] [Subscribe] [Scholar Register] [Indexed: 03/02/2023] Open
Affiliation(s)
- V Damaraju
- Department of Pulmonary Medicine, Postgraduate Institute of Medical Education and Research (PGIMER), Chandigarh, India
| | - N Singh
- Department of Pulmonary Medicine, Postgraduate Institute of Medical Education and Research (PGIMER), Chandigarh, India
| | - M Garg
- Department of Radiodiagnosis, Postgraduate Institute of Medical Education and Research (PGIMER), Chandigarh, India
| | - S Kathirvel
- Department of Community Medicine and School of Public Health, Postgraduate Institute of Medical Education and Research (PGIMER), Chandigarh, India
| | - R K Basher
- Department of Nuclear Medicine, Postgraduate Institute of Medical Education and Research (PGIMER), Chandigarh, India
| | - S Grover
- Department of Psychiatry, Postgraduate Institute of Medical Education and Research (PGIMER), Chandigarh, India
| | - N Kalra
- Department of Radiodiagnosis, Postgraduate Institute of Medical Education and Research (PGIMER), Chandigarh, India
| | - K T Prasad
- Department of Pulmonary Medicine, Postgraduate Institute of Medical Education and Research (PGIMER), Chandigarh, India
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Mourya H, Garud N, Joshi R, Akram W, Singh N. Formulation and Optimization of Propranolol Bilayer Tablets: A Potential Approach for Effective Management of Hypertension. Indian J Pharm Sci 2023. [DOI: 10.36468/pharmaceutical-sciences.1081] [Citation(s) in RCA: 0] [Impact Index Per Article: 0] [Reference Citation Analysis] [What about the content of this article? (0)] [Track Full Text] [Journal Information] [Subscribe] [Scholar Register] [Indexed: 03/02/2023] Open
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. M, Singh A, Saumaya KU, Joshi M, Kaur N, Garg N, Singh N. Anticancer SAR Establishment and α/β-Tubulin Isoforms Specific Targeting: A Detailed Insight of Anticancer potential of 4H-Chromene derivatives. NEW J CHEM 2023. [DOI: 10.1039/d2nj04822a] [Citation(s) in RCA: 0] [Impact Index Per Article: 0] [Reference Citation Analysis] [What about the content of this article? (0)] [Abstract] [Track Full Text] [Journal Information] [Subscribe] [Scholar Register] [Indexed: 04/05/2023]
Abstract
4H-Chromene derivatives are promising anticancer compounds known to bind within the colchicine binding site of tubulin protein. Among these 2-amino-4-phenyl-4H-benzo[h]chromene-3-carbonitrile based 4H-Chromenes scaffold is known to produce a significant impact...
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Pahwa B, Singh N, Singh G, Chavda V, Montemurro N, Chaurasia B. Surgical Approaches to Cavernous Sinus: A Narrative Review of the Literature with Anatomical Drawings. J Neurol Surg A Cent Eur Neurosurg 2022. [PMID: 36584879 DOI: 10.1055/a-2005-0482] [Citation(s) in RCA: 0] [Impact Index Per Article: 0] [Reference Citation Analysis] [What about the content of this article? (0)] [Affiliation(s)] [Abstract] [Track Full Text] [Journal Information] [Subscribe] [Scholar Register] [Indexed: 01/01/2023]
Abstract
IIntroduction. The cavernous sinus (CS) is a paired venous sinus in the human brain that is classified as a true dural venous sinus rather than a venous plexus. The entire CS is separated by septa into two small cavities called caves. The CS has a very close resemblance to various key structures present in the head. The CS is a blood compartment that contains ligaments, endothelium, and trabeculae. It is clinically significant because of its position and relationship with several cranial nerves. Clinical implications. For effective management and treatment of CS syndrome, CS thrombosis, carotid-cavernous fistula, and other CS-related problems, CS surgery became necessary. As a result of the lack of sophisticated surgical techniques in the past, CS surgery was exceedingly challenging, complicated, and deadly. The surgery of CSs can benefit from a variety of surgical procedures, including extradural and intradural, endoscopic endonasal, rhomboid, and temporopolar trans cavernous approaches. In this review, numerous surgical procedures for CS are discussed along with their intended uses. Conclusions. A greater understanding of the CS was made possible by the quick modifications and improvements in surgical methods, which aided in neurosurgery procedures.
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Affiliation(s)
| | - Narinder Singh
- -, Indian Institute of Management Amritsar, Amritsar, India
| | | | - Vishal Chavda
- Pathology, Stanford University School of Medicine, Stanford, United States
| | | | - Bipin Chaurasia
- Department of Neurosurgery, Tribhuvan University Institute of Medicine Nursing Campus Birgunj, Birgunj, Nepal
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Ranbir, Kumar M, Singh G, Singh J, Kaur N, Singh N. Machine Learning-Based Analytical Systems: Food Forensics. ACS Omega 2022; 7:47518-47535. [PMID: 36591133 PMCID: PMC9798398 DOI: 10.1021/acsomega.2c05632] [Citation(s) in RCA: 2] [Impact Index Per Article: 1.0] [Reference Citation Analysis] [What about the content of this article? (0)] [Affiliation(s)] [Abstract] [Grants] [Track Full Text] [Subscribe] [Scholar Register] [Received: 08/31/2022] [Accepted: 11/29/2022] [Indexed: 02/06/2024]
Abstract
Despite a large amount of money being spent on both food analyses and control measures, various food-borne illnesses associated with pathogens, toxins, pesticides, adulterants, colorants, and other contaminants pose a serious threat to human health, and thus food safety draws considerable attention in the modern pace of the world. The presence of various biogenic amines in processed food have been frequently considered as the primary quality parameter in order to check food freshness and spoilage of protein-rich food. Various conventional detection methods for detecting hazardous analytes including microscopy, nucleic acid, and immunoassay-based techniques have been employed; however, recently, array-based sensing strategies are becoming popular for the development of a highly accurate and precise analytical method. Array-based sensing is majorly facilitated by the advancements in multivariate analytical techniques as well as machine learning-based approaches. These techniques allow one to solve the typical problem associated with the interpretation of the complex response patterns generated in array-based strategies. Consequently, the machine learning-based neural networks enable the fast, robust, and accurate detection of analytes using sensor arrays. Thus, for commercial applications, most of the focus has shifted toward the development of analytical methods based on electrical and chemical sensor arrays. Therefore, herein, we briefly highlight and review the recently reported array-based sensor systems supported by machine learning and multivariate analytics to monitor food safety and quality in the field of food forensics.
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Affiliation(s)
- Ranbir
- Department
of Chemistry, Indian Institute of Technology
Ropar, Rupnagar 140001, Punjab, India
| | - Manish Kumar
- Department
of Chemistry, Indian Institute of Technology
Ropar, Rupnagar 140001, Punjab, India
| | - Gagandeep Singh
- Department
of Biomedical Engineering, Indian Institute
of Technology Ropar, Rupnagar 140001, Punjab, India
| | - Jasvir Singh
- Department
of Chemistry, Himachal Pradesh University, Shimla 171005, India
| | - Navneet Kaur
- Department
of Chemistry, Panjab University, Chandigarh 160014, India
| | - Narinder Singh
- Department
of Chemistry, Indian Institute of Technology
Ropar, Rupnagar 140001, Punjab, India
- Department
of Biomedical Engineering, Indian Institute
of Technology Ropar, Rupnagar 140001, Punjab, India
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Singh N, Miller R, Arbe-Barnes S, Kvalheim Eriksen H, Inderberg E, Iverson B, Eriksen J. 184P A phase I study of the cancer-specific vaccine FMPV-1 in healthy male subjects to assess safety and immune response. Immuno-Oncology and Technology 2022. [DOI: 10.1016/j.iotech.2022.100296] [Citation(s) in RCA: 0] [Impact Index Per Article: 0] [Reference Citation Analysis] [What about the content of this article? (0)] [Track Full Text] [Subscribe] [Scholar Register] [Indexed: 12/13/2022]
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Singh N, Houssein EH, Mirjalili S, Cao Y, Selvachandran G. An efficient improved African vultures optimization algorithm with dimension learning hunting for traveling salesman and large‐scale optimization applications. INT J INTELL SYST 2022. [DOI: 10.1002/int.23091] [Citation(s) in RCA: 0] [Impact Index Per Article: 0] [Reference Citation Analysis] [What about the content of this article? (0)] [Affiliation(s)] [Track Full Text] [Journal Information] [Subscribe] [Scholar Register] [Indexed: 12/03/2022]
Affiliation(s)
- Narinder Singh
- Department of Mathematics Punjabi University Patiala Punjab India
| | | | - Seyedali Mirjalili
- Institute for Integrated and Intelligent Systems Griffith University Nathan Queensland Australia
| | - Yankai Cao
- Faculty of Applied Science, UBC Chemical and Biological Engineering The University of British Columbia Vancouver British Columbia Canada
| | - Ganeshsree Selvachandran
- Department of Actuarial Science and Applied Statistics, Faculty of Business and Management UCSI University, Jalan Menara Gading Cheras Kuala Lumpur Malaysia
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Senanayake P, Warfield-McAlpine P, Salati H, Bradshaw K, Wong E, Inthavong K, Singh N. The Impact of Adhesions on Nasal Airflow: A Quantitative Analysis Using Computational Fluid Dynamics. Am J Rhinol Allergy 2022; 37:273-283. [PMID: 36373577 DOI: 10.1177/19458924221137982] [Citation(s) in RCA: 0] [Impact Index Per Article: 0] [Reference Citation Analysis] [What about the content of this article? (0)] [Affiliation(s)] [Abstract] [Track Full Text] [Journal Information] [Subscribe] [Scholar Register] [Indexed: 11/16/2022]
Abstract
Background Nasal adhesions (NAs) are a known complication of nasal airway surgery. Even minor NAs can lead to significant postoperative nasal airway obstruction (NAO). Division of such NAs often provides much greater relief than anticipated. Objective We examine the impact of NAs at various anatomical sites on nasal airflow and mucosal cooling using computational fluid dynamics (CFD) and multiple test subjects. Methods CT scans of healthy adult subjects were used to construct three-dimensional nasal airway computational models. A single virtual 2.5 mm diameter NA was placed at one of five sites commonly seen following NAO surgery within each nasal cavity bilaterally, resulting in 10 NA models and 1 NA-free control for each subject. CFD analysis was performed on each NA model and compared with the subject's NA-free control model. Results 4 subjects were recruited to create 44 computational models. The NAs caused the airflow streamlines to separate, leading to a statistically significant increase in mucosal temperature immediately downstream to the NAs (wake region). Changes in the mucosal temperature in the wake region of the NAs were most prominent in anteriorly located NAs with a mean increase of 1.62 °C for the anterior inferior turbinate NAs ( P < .001) and 0.63 °C for the internal valve NAs ( P < .001). Conclusion NAs result in marked disruption to airflow patterns and reduced mucosal cooling on critical surfaces, particularly in the wake region. Reduced wake region mucosal cooling may be a contributing factor to the exaggerated perception of nasal obstruction experienced by patients with NAs.
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Affiliation(s)
- Praween Senanayake
- Department of Otolaryngology, Head and Neck Surgery, Westmead Hospital, Sydney, NSW, Australia
| | | | - Hana Salati
- School of Engineering, RMIT University, Melbourne, Australia
| | - Kimberley Bradshaw
- Department of Otolaryngology, Head and Neck Surgery, Westmead Hospital, Sydney, NSW, Australia
| | - Eugene Wong
- Department of Otolaryngology, Head and Neck Surgery, Westmead Hospital, Sydney, NSW, Australia
| | - Kiao Inthavong
- School of Engineering, RMIT University, Melbourne, Australia
| | - Narinder Singh
- Department of Otolaryngology, Head and Neck Surgery, Westmead Hospital, Sydney, NSW, Australia
- Sydney Medical School, University of Sydney, Camperdown, NSW, Australia
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Kaur H, Verma M, Kaur S, Rana B, Singh N, Jena KC. Elucidating the Molecular Structure of Hydrophobically Modified Polyethylenimine Nanoparticles and Its Potential Implications for DNA Binding. Langmuir 2022; 38:13456-13468. [PMID: 36279506 DOI: 10.1021/acs.langmuir.2c01912] [Citation(s) in RCA: 3] [Impact Index Per Article: 1.5] [Reference Citation Analysis] [What about the content of this article? (0)] [Abstract] [MESH Headings] [Track Full Text] [Subscribe] [Scholar Register] [Indexed: 06/16/2023]
Abstract
The structural properties of the polyethylenimine (PEI) polymer are generally tuned and selectively modified to reinforce its potential in a broad spectrum of applied domains of medicine, healthcare, material design, sensing, and electronic optimization. The selective modification of the polymer brings about changes in its interfacial characteristics and behavior. The current work involves the synthesis of naphthalimide conjugated polyethylenimine organic nanoparticles (NPEI-ONPs). The interfacial molecular structure of NPEI-ONPs is explored in an aqueous medium at pH 7.4 using surface tensiometry and sum-frequency generation vibrational spectroscopy (SFG-VS). The hydrophobic functionalization rendered a concentration-dependent surface coverage of NPEI-ONPs, where the SFG-VS analysis exhibited the molecular rearrangement of its hydrophobic groups at the interface. The interaction of NPEI-ONPs with double-stranded DNA (dsDNA) is carried out to observe the relevance of the synthesized nanocomposites in the biomedical domain. The bulk-specific studies (i.e., thermal denaturation, viscometry, zeta (ζ) potential, and ATR-FTIR) reveal the condensation of dsDNA in the presence of NPEI-ONPs, making its structure more compact. The interface-sensitive SFG-VS showcased the impact of the dsDNA and NPEI-ONP interaction on the interfacial molecular behavior of NPEI-ONPs at the air-aqueous interface. Our results exhibit the potential of such hydrophobically functionalized ONPs as promising candidates for developing biomedical sealants, substrate coatings, and other biomedical domains.
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Das P, Arora S, Sharma P, Nath SK, Sivasami K, Singh GK, Bahuguna A, Sapra D, Singh N, Sharma AK, Verma P, Bellad P, Gupta A, G B P, Ranjan Das DS. Gastrointestinal: IgA vasculitis as a rare cause of acute pancreatitis. J Gastroenterol Hepatol 2022; 37:2027. [PMID: 35315539 DOI: 10.1111/jgh.15814] [Citation(s) in RCA: 1] [Impact Index Per Article: 0.5] [Reference Citation Analysis] [What about the content of this article? (0)] [Affiliation(s)] [Track Full Text] [Journal Information] [Submit a Manuscript] [Subscribe] [Scholar Register] [Received: 11/17/2021] [Revised: 01/11/2022] [Accepted: 02/08/2022] [Indexed: 12/09/2022]
Affiliation(s)
- P Das
- Department of Dermatology, Base Hospital Delhi Cantt and Army College of Medical Sciences, New Delhi, India
| | - S Arora
- Department of Dermatology, Base Hospital Delhi Cantt and Army College of Medical Sciences, New Delhi, India
| | - P Sharma
- Department of Lab Sciences and Molecular Medicine, Army Hospital Research and Referral, New Delhi, India
| | - S K Nath
- Department of Radiodiagnosis, Military Hospital Meerut, Uttar Pradesh, India
| | - K Sivasami
- Department of Rheumatology, Army Hospital Research and Referral, New Delhi, India
| | - G K Singh
- Department of Dermatology, Base Hospital Delhi Cantt and Army College of Medical Sciences, New Delhi, India
| | - A Bahuguna
- Department of Dermatology, Base Hospital Delhi Cantt and Army College of Medical Sciences, New Delhi, India
| | - D Sapra
- Department of Dermatology, Base Hospital Delhi Cantt and Army College of Medical Sciences, New Delhi, India
| | - N Singh
- Department of Dermatology, Base Hospital Delhi Cantt and Army College of Medical Sciences, New Delhi, India
| | - A K Sharma
- Office of Director General Medical Services, New Delhi, India
| | - P Verma
- Department of Dermatology, Base Hospital Delhi Cantt and Army College of Medical Sciences, New Delhi, India
| | - P Bellad
- Department of Dermatology, Base Hospital Delhi Cantt and Army College of Medical Sciences, New Delhi, India
| | - A Gupta
- Department of Dermatology, Base Hospital Delhi Cantt and Army College of Medical Sciences, New Delhi, India
| | - P G B
- Department of Dermatology, Base Hospital Delhi Cantt and Army College of Medical Sciences, New Delhi, India
| | - D S Ranjan Das
- Department of Radiodiagnosis and Imaging, Military Hospital Jabalpur, Madhya Pradesh, India
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Choma MA, Floriani JR, Gabriel PG, Urbisci L, Hu D, Troy TP, Hata T, Singh N, Blekic A. Initial Experience With AI-based Video Monitoring for Delirium-Associated Factors and Room Environment. J Acad Consult Liaison Psychiatry 2022. [DOI: 10.1016/j.jaclp.2022.10.247] [Citation(s) in RCA: 0] [Impact Index Per Article: 0] [Reference Citation Analysis] [What about the content of this article? (0)] [Track Full Text] [Journal Information] [Submit a Manuscript] [Subscribe] [Scholar Register] [Indexed: 11/11/2022]
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40
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Bhardwaj G, Kaur R, Kaur N, Singh N. Gold nanoparticles capped DHPMs for meliorate detection of antiretroviral drug: Azidothymidine. Talanta 2022; 249:123591. [DOI: 10.1016/j.talanta.2022.123591] [Citation(s) in RCA: 1] [Impact Index Per Article: 0.5] [Reference Citation Analysis] [What about the content of this article? (0)] [Track Full Text] [Journal Information] [Subscribe] [Scholar Register] [Received: 07/29/2021] [Revised: 12/10/2021] [Accepted: 05/25/2022] [Indexed: 11/17/2022]
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Evenden R, Singh N, Sornalingam S, Harrington S, Paudyal P. Language barriers for primary care access in Europe: a systematic review. Eur J Public Health 2022; 32:ckac129.724. [PMCID: PMC9594485 DOI: 10.1093/eurpub/ckac129.724] [Citation(s) in RCA: 1] [Impact Index Per Article: 0.5] [Reference Citation Analysis] [What about the content of this article? (0)] [Affiliation(s)] [Abstract] [Track Full Text] [Journal Information] [Subscribe] [Scholar Register] [Indexed: 04/13/2024] Open
Abstract
Background A recent increase in migration both inside Europe and from non-European countries has expanded the language profile of many European countries. As a result, there has been a significant increase in barriers to healthcare access experienced by linguistic minority migrants. This systematic review aims to explore language barriers in primary care, focusing on the experiences of linguistic minority migrants living in Europe. Methods PubMed, Embase, Scopus and Global Health were searched to identify studies published in English until May 2021. Qualitative and mixed methods studies on either linguistic minority migrants or healthcare workers working with linguistic minority migrants, exploring the impacts of language barriers in a primary care setting published were eligible. The studies were analysed using a Braun and Clarke's thematic analysis approach. Quality of the studies were assessed using the Mixed Methods Appraisal Tool. Results 16 studies from 14 different European countries were eligible. Participants in the studies included four groups: linguistic minority migrants (n = 11), healthcare workers (n = 10), interpreters (n = 1) and administrative staff (n = 1). Barriers identified included a lack of interpreters, limited cultural competence of practitioners, a lack of practitioner training and knowledge, a lack of accessible information for migrants, difficulties expressing emotions and building patient-practitioner relationships, and risks to women's bodily autonomy resulting from language barriers. Conclusions Linguistic minority migrants living in Europe face a number of barriers when accessing primary care. These barriers can risk patient safety, reduce the likelihood of seeking healthcare services, and impact patient experiences of healthcare services. There is a need for improved interpreter services, practitioner training, and information accessibility for both migrants and healthcare staff. Key messages • Linguistic minority migrants experience significant barriers to primary healthcare access across Europe. • There is a need for improved interpreter services, practitioner training, and information accessibility for both migrants and healthcare staff.
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Affiliation(s)
- R Evenden
- Primary Care and Public Health, Brighton and Sussex Medical School, Brighton, UK
| | - N Singh
- Primary Care and Public Health, Brighton and Sussex Medical School, Brighton, UK
| | - S Sornalingam
- Primary Care and Public Health, Brighton and Sussex Medical School, Brighton, UK
| | - S Harrington
- Primary Care and Public Health, Brighton and Sussex Medical School, Brighton, UK
| | - P Paudyal
- Primary Care and Public Health, Brighton and Sussex Medical School, Brighton, UK
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Vara Almirall B, Inthavong K, Bradshaw K, Singh N, Johnson A, Storey P, Salati H. Flow Patterns and Particle Residence Times in the Oral Cavity during Inhaled Drug Delivery. Pharmaceuticals (Basel) 2022; 15:ph15101259. [PMID: 36297371 PMCID: PMC9612176 DOI: 10.3390/ph15101259] [Citation(s) in RCA: 1] [Impact Index Per Article: 0.5] [Reference Citation Analysis] [What about the content of this article? (0)] [Affiliation(s)] [Abstract] [Key Words] [Grants] [Track Full Text] [Download PDF] [Figures] [Journal Information] [Subscribe] [Scholar Register] [Received: 09/12/2022] [Revised: 10/05/2022] [Accepted: 10/08/2022] [Indexed: 12/05/2022] Open
Abstract
Pulmonary drug delivery aims to deliver particles deep into the lungs, bypassing the mouth−throat airway geometry. However, micron particles under high flow rates are susceptible to inertial impaction on anatomical sites that serve as a defense system to filter and prevent foreign particles from entering the lungs. The aim of this study was to understand particle aerodynamics and its possible deposition in the mouth−throat airway that inhibits pulmonary drug delivery. In this study, we present an analysis of the aerodynamics of inhaled particles inside a patient-specific mouth−throat model generated from MRI scans. Computational Fluid Dynamics with a Discrete Phase Model for tracking particles was used to characterize the airflow patterns for a constant inhalation flow rate of 30 L/min. Monodisperse particles with diameters of 7 μm to 26 μm were introduced to the domain within a 3 cm-diameter sphere in front of the oral cavity. The main outcomes of this study showed that the time taken for particle deposition to occur was 0.5 s; a narrow stream of particles (medially and superiorly) were transported by the flow field; larger particles > 20 μm deposited onto the oropharnyx, while smaller particles < 12 μm were more disperse throughout the oral cavity and navigated the curved geometry and laryngeal jet to escape through the tracheal outlet. It was concluded that at a flow rate of 30 L/min the particle diameters depositing on the larynx and trachea in this specific patient model are likely to be in the range of 7 μm to 16 μm. Particles larger than 16 μm primarily deposited on the oropharynx.
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Affiliation(s)
- Brenda Vara Almirall
- Mechanical & Automotive Engineering, School of Engineering, Royal Melbourne Institute of Technology University, Bundoora, VIC 3083, Australia
| | - Kiao Inthavong
- Mechanical & Automotive Engineering, School of Engineering, Royal Melbourne Institute of Technology University, Bundoora, VIC 3083, Australia
- Correspondence:
| | - Kimberley Bradshaw
- Department of Otolaryngology, Head and Neck Surgery, Westmead Hospital, Westmead, NSW 2145, Australia
| | - Narinder Singh
- Department of Otolaryngology, Head and Neck Surgery, Westmead Hospital, Westmead, NSW 2145, Australia
- Sydney Medical School, Faculty of Medicine & Health, The University of Sydney, Sydney, NSW 2006, Australia
| | - Aaron Johnson
- Department of Otolaryngology-Head and Neck Surgery & Department of Rehabilitation Medicine, Grossman School of Medicine, New York University, New York, NY 10017, USA
| | - Pippa Storey
- Department of Radiology, Grossman School of Medicine, New York University, New York, NY 10016, USA
| | - Hana Salati
- Mechanical & Automotive Engineering, School of Engineering, Royal Melbourne Institute of Technology University, Bundoora, VIC 3083, Australia
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Singh A, Singh N, Kaur N. Ionic Liquid Functionalized Fe
3
O
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Core‐Shell Nanoparticles: A Magnetically Separable Bronsted Acid Catalyst for The Synthesis of Poly‐thioamides. Appl Organomet Chem 2022. [DOI: 10.1002/aoc.6909] [Citation(s) in RCA: 0] [Impact Index Per Article: 0] [Reference Citation Analysis] [What about the content of this article? (0)] [Affiliation(s)] [Track Full Text] [Journal Information] [Subscribe] [Scholar Register] [Indexed: 11/07/2022]
Affiliation(s)
- Anoop Singh
- Department of Chemistry Indian Institute of Technology Ropar Punjab India
| | - Narinder Singh
- Department of Chemistry Indian Institute of Technology Ropar Punjab India
| | - Navneet Kaur
- Department of Chemistry Panjab University Chandigarh India
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Kaur A, Singh N, Singh K, Sidhu SK, Kaur H, Jain P, Kaur M, Jairath M. SARS-CoV-2 IgG Antibody Seroprevalence in Children from the Amritsar District of Punjab. Korean J Clin Lab Sci 2022. [DOI: 10.15324/kjcls.2022.54.3.173] [Citation(s) in RCA: 0] [Impact Index Per Article: 0] [Reference Citation Analysis] [What about the content of this article? (0)] [Affiliation(s)] [Track Full Text] [Journal Information] [Subscribe] [Scholar Register] [Indexed: 11/05/2022] Open
Affiliation(s)
- Amandeep Kaur
- The Viral Research and Diagnostic Laboratory, Government Medical College, Amritsar, India
| | - Narinder Singh
- Department of Pediatrics, Government Medical College, Amritsar, India
| | - Kanwardeep Singh
- Department of Microbiology, Government Medical College, Amritsar, India
| | | | - Harleen Kaur
- The Viral Research and Diagnostic Laboratory, Government Medical College, Amritsar, India
| | - Poonam Jain
- The Viral Research and Diagnostic Laboratory, Government Medical College, Amritsar, India
| | - Manmeet Kaur
- Department of Pediatrics, Government Medical College, Amritsar, India
| | - Mohan Jairath
- The Viral Research and Diagnostic Laboratory, Government Medical College, Amritsar, India
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Salati H, Singh N, Khamooshi M, Vahaji S, Fletcher DF, Inthavong K. Nasal Irrigation Delivery in Three Post-FESS Models From a Squeeze-bottle Using CFD. Pharm Res 2022; 39:2569-2584. [PMID: 36056272 PMCID: PMC9556402 DOI: 10.1007/s11095-022-03375-y] [Citation(s) in RCA: 1] [Impact Index Per Article: 0.5] [Reference Citation Analysis] [What about the content of this article? (0)] [Affiliation(s)] [Abstract] [Key Words] [Track Full Text] [Download PDF] [Figures] [Journal Information] [Subscribe] [Scholar Register] [Received: 05/30/2022] [Accepted: 08/17/2022] [Indexed: 11/30/2022]
Abstract
Purpose Nasal saline irrigation is highly recommended in patients following functional endoscopic sinus surgery (FESS) to aid the postoperative recovery. Post-FESS patients have significantly altered anatomy leading to markedly different flow dynamics from those found in pre-op or non-diseased airways, resulting in unknown flow dynamics. Methods This work investigated how the liquid stream disperses through altered nasal cavities following surgery using Computational Fluid Dynamics (CFD). A realistic squeeze profile was determined from physical experiments with a 27-year-old male using a squeeze bottle with load sensors. The administration technique involved a head tilt of 45-degrees forward to represent a head position over a sink. After the irrigation event that lasted 4.5 s, the simulation continued for an additional 1.5 s, with the head orientation returning to an upright position. Results The results demonstrated that a large maxillary sinus ostium on the right side allows saline penetration into this sinus. The increased volume of saline entering the maxillary sinus limits the saline volume available to the rest of the sinonasal cavity and reduces the surface coverage of the other paranasal sinuses. The average wall shear stress was higher on the right side than on the other side for two patients. The results also revealed that head position alters the sinuses’ saline residual, especially the frontal sinuses. Conclusion While greater access to sinuses is achieved through FESS surgery, patients without a nasal septum limits posterior sinus penetration due to the liquid crossing over to the contralateral cavity and exiting the nasal cavity early.
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Affiliation(s)
- Hana Salati
- Mechanical & Automotive Engineering, School of Engineering, RMIT University, 3083, Bundoora, Victoria, Australia
| | - Narinder Singh
- Department of Otolaryngology, Head and Neck Surgery, Westmead Hospital, 2145, Westmead, New South Wales, Australia
| | - Mehrdad Khamooshi
- Cardio-Respiratory Engineering and Technology Laboratory (CREATElab), Department of Mechanical and Aerospace Engineering, Monash University, 3004, Melbourne, Victoria, Australia
| | - Sara Vahaji
- Mechanical & Automotive Engineering, School of Engineering, RMIT University, 3083, Bundoora, Victoria, Australia
| | - David F Fletcher
- School of Chemical and Biomolecular Engineering, The University of Sydney, 2145, New South Wales, Australia
| | - Kiao Inthavong
- Mechanical & Automotive Engineering, School of Engineering, RMIT University, 3083, Bundoora, Victoria, Australia.
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Abbott R, Abe H, Acernese F, Ackley K, Adhikari N, Adhikari R, Adkins V, Adya V, Affeldt C, Agarwal D, Agathos M, Agatsuma K, Aggarwal N, Aguiar O, Aiello L, Ain A, Ajith P, Akutsu T, Albanesi S, Alfaidi R, Allocca A, Altin P, Amato A, Anand C, Anand S, Ananyeva A, Anderson S, Anderson W, Ando M, Andrade T, Andres N, Andrés-Carcasona M, Andrić T, Angelova S, Ansoldi S, Antelis J, Antier S, Apostolatos T, Appavuravther E, Appert S, Apple S, Arai K, Araya A, Araya M, Areeda J, Arène M, Aritomi N, Arnaud N, Arogeti M, Aronson S, Arun K, Asada H, Asali Y, Ashton G, Aso Y, Assiduo M, Melo SADS, Aston S, Astone P, Aubin F, AultONeal K, Austin C, Babak S, Badaracco F, Bader M, Badger C, Bae S, Bae Y, Baer A, Bagnasco S, Bai Y, Baird J, Bajpai R, Baka T, Ball M, Ballardin G, Ballmer S, Balsamo A, Baltus G, Banagiri S, Banerjee B, Bankar D, Barayoga J, Barbieri C, Barish B, Barker D, Barneo P, Barone F, Barr B, Barsotti L, Barsuglia M, Barta D, Bartlett J, Barton M, Bartos I, Basak S, Bassiri R, Basti A, Bawaj M, Bayley J, Mills J, Milotti E, Minenkov Y, Mio N, Mir L, Miravet-Tenés M, Mishkin A, Mishra C, Mishra T, Mistry T, Bazzan M, Mitra S, Mitrofanov V, Mitselmakher G, Mittleman R, Miyakawa O, Miyo K, Miyoki S, Mo G, Modafferi L, Moguel E, Becher B, Mogushi K, Mohapatra S, Mohite S, Molina I, Molina-Ruiz M, Mondin M, Montani M, Moore C, Moragues J, Moraru D, Bécsy B, Morawski F, More A, Moreno C, Moreno G, Mori Y, Morisaki S, Morisue N, Moriwaki Y, Mours B, Mow-Lowry C, Bedakihale V, Mozzon S, Muciaccia F, Mukherjee A, Mukherjee D, Mukherjee S, Mukherjee S, Mukherjee S, Mukund N, Mullavey A, Munch J, Beirnaert F, Muñiz E, Murray P, Musenich R, Muusse S, Nadji S, Nagano K, Nagar A, Nakamura K, Nakano H, Nakano M, Bejger M, Nakayama Y, Napolano V, Nardecchia I, Narikawa T, Narola H, Naticchioni L, Nayak B, Nayak R, Neil B, Neilson J, Belahcene I, Nelson A, Nelson T, Nery M, Neubauer P, Neunzert A, Ng K, Ng S, Nguyen C, Nguyen P, Nguyen T, Benedetto V, Quynh LN, Ni J, Ni WT, Nichols S, Nishimoto T, Nishizawa A, Nissanke S, Nitoglia E, Nocera F, Norman M, Beniwal D, North C, Nozaki S, Nurbek G, Nuttall L, Obayashi Y, Oberling J, O’Brien B, O’Dell J, Oelker E, Ogaki W, Benjamin M, Oganesyan G, Oh J, Oh K, Oh S, Ohashi M, Ohashi T, Ohkawa M, Ohme F, Ohta H, Okada M, Bennett T, Okutani Y, Olivetto C, Oohara K, Oram R, O’Reilly B, Ormiston R, Ormsby N, O’Shaughnessy R, O’Shea E, Oshino S, Bentley J, Ossokine S, Osthelder C, Otabe S, Ottaway D, Overmier H, Pace A, Pagano G, Pagano R, Page M, Pagliaroli G, BenYaala M, Pai A, Pai S, Pal S, Palamos J, Palashov O, Palomba C, Pan H, Pan KC, Panda P, Pang P, Bera S, Pankow C, Pannarale F, Pant B, Panther F, Paoletti F, Paoli A, Paolone A, Pappas G, Parisi A, Park H, Berbel M, Park J, Parker W, Pascucci D, Pasqualetti A, Passaquieti R, Passuello D, Patel M, Pathak M, Patricelli B, Patron A, Bergamin F, Paul S, Payne E, Pedraza M, Pedurand R, Pegoraro M, Pele A, Arellano FP, Penano S, Penn S, Perego A, Berger B, Pereira A, Pereira T, Perez C, Périgois C, Perkins C, Perreca A, Perriès S, Pesios D, Petermann J, Petterson D, Bernuzzi S, Pfeiffer H, Pham H, Pham K, Phukon K, Phurailatpam H, Piccinni O, Pichot M, Piendibene M, Piergiovanni F, Pierini L, Bersanetti D, Pierro V, Pillant G, Pillas M, Pilo F, Pinard L, Pineda-Bosque C, Pinto I, Pinto M, Piotrzkowski B, Piotrzkowski K, Bertolini A, Pirello M, Pitkin M, Placidi A, Placidi E, Planas M, Plastino W, Pluchar C, Poggiani R, Polini E, Pong D, Betzwieser J, Ponrathnam S, Porter E, Poulton R, Poverman A, Powell J, Pracchia M, Pradier T, Prajapati A, Prasai K, Prasanna R, Beveridge D, Pratten G, Principe M, Prodi G, Prokhorov L, Prosposito P, Prudenzi L, Puecher A, Punturo M, Puosi F, Puppo P, Bhandare R, Pürrer M, Qi H, Quartey N, Quetschke V, Quinonez P, Quitzow-James R, Raab F, Raaijmakers G, Radkins H, Radulesco N, Bhandari A, Raffai P, Rail S, Raja S, Rajan C, Ramirez K, Ramirez T, Ramos-Buades A, Rana J, Rapagnani P, Ray A, Bhardwaj U, Raymond V, Raza N, Razzano M, Read J, Rees L, Regimbau T, Rei L, Reid S, Reid S, Reitze D, Bhatt R, Relton P, Renzini A, Rettegno P, Revenu B, Reza A, Rezac M, Ricci F, Richards D, Richardson J, Richardson L, Bhattacharjee D, Riemenschneider G, Riles K, Rinaldi S, Rink K, Robertson N, Robie R, Robinet F, Rocchi A, Rodriguez S, Rolland L, Bhaumik S, Rollins J, Romanelli M, Romano R, Romel C, Romero A, Romero-Shaw I, Romie J, Ronchini S, Rosa L, Rose C, Bianchi A, Rosińska D, Ross M, Rowan S, Rowlinson S, Roy S, Roy S, Rozza D, Ruggi P, Ruiz-Rocha K, Ryan K, Bilenko I, Sachdev S, Sadecki T, Sadiq J, Saha S, Saito Y, Sakai K, Sakellariadou M, Sakon S, Salafia O, Salces-Carcoba F, Billingsley G, Salconi L, Saleem M, Salemi F, Samajdar A, Sanchez E, Sanchez J, Sanchez L, Sanchis-Gual N, Sanders J, Sanuy A, Bini S, Saravanan T, Sarin N, Sassolas B, Satari H, Sauter O, Savage R, Savant V, Sawada T, Sawant H, Sayah S, Birney R, Schaetzl D, Scheel M, Scheuer J, Schiworski M, Schmidt P, Schmidt S, Schnabel R, Schneewind M, Schofield R, Schönbeck A, Birnholtz O, Schulte B, Schutz B, Schwartz E, Scott J, Scott S, Seglar-Arroyo M, Sekiguchi Y, Sellers D, Sengupta A, Sentenac D, Biscans S, Seo E, Sequino V, Sergeev A, Setyawati Y, Shaffer T, Shahriar M, Shaikh M, Shams B, Shao L, Sharma A, Bischi M, Sharma P, Shawhan P, Shcheblanov N, Sheela A, Shikano Y, Shikauchi M, Shimizu H, Shimode K, Shinkai H, Shishido T, Biscoveanu S, Shoda A, Shoemaker D, Shoemaker D, ShyamSundar S, Sieniawska M, Sigg D, Silenzi L, Singer L, Singh D, Singh M, Bisht A, Singh N, Singha A, Sintes A, Sipala V, Skliris V, Slagmolen B, Slaven-Blair T, Smetana J, Smith J, Smith L, Biswas B, Smith R, Soldateschi J, Somala S, Somiya K, Song I, Soni K, Soni S, Sordini V, Sorrentino F, Sorrentino N, Bitossi M, Soulard R, Souradeep T, Sowell E, Spagnuolo V, Spencer A, Spera M, Spinicelli P, Srivastava A, Srivastava V, Staats K, Bizouard MA, Stachie C, Stachurski F, Steer D, Steinlechner J, Steinlechner S, 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Search for continuous gravitational wave emission from the Milky Way center in O3 LIGO-Virgo data. Int J Clin Exp Med 2022. [DOI: 10.1103/physrevd.106.042003] [Citation(s) in RCA: 3] [Impact Index Per Article: 1.5] [Reference Citation Analysis] [What about the content of this article? (0)] [Track Full Text] [Journal Information] [Subscribe] [Scholar Register] [Indexed: 11/07/2022]
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RL, Warner J, Was M, Washington NY, Watchi J, Weaver B, Webster SA, Weinert M, Weinstein AJ, Weiss R, Weller CM, Wellmann F, Wen L, Weßels P, Wette K, Whelan JT, White DD, Whiting BF, Whittle C, Wilken D, Williams D, Williams MJ, Williamson AR, Willis JL, Willke B, Wilson DJ, Winkler W, Wipf CC, Wlodarczyk T, Woan G, Woehler J, Wofford JK, Wong ICF, Wu DS, Wysocki DM, Xiao L, Yamamoto H, Yang FW, Yang L, Yang Y, Yang Z, Yap MJ, Yeeles DW, Yelikar AB, Ying M, Yoo J, Yu H, Yu H, Zadrożny A, Zanolin M, Zelenova T, Zendri JP, Zevin M, Zhang J, Zhang L, Zhang T, Zhang Y, Zhao C, Zhao G, Zhao Y, Zhou R, Zhou Z, Zhu XJ, Zimmerman AB, Zucker ME, Zweizig J, Jeong D, Shandera S. Search for Subsolar-Mass Binaries in the First Half of Advanced LIGO's and Advanced Virgo's Third Observing Run. Phys Rev Lett 2022; 129:061104. [PMID: 36018635 DOI: 10.1103/physrevlett.129.061104] [Citation(s) in RCA: 0] [Impact Index Per Article: 0] [Reference Citation Analysis] [What about the content of this article? (0)] [Affiliation(s)] [Abstract] [Grants] [Track Full Text] [Subscribe] [Scholar Register] [Received: 10/01/2021] [Revised: 03/18/2022] [Accepted: 06/07/2022] [Indexed: 06/15/2023]
Abstract
We report on a search for compact binary coalescences where at least one binary component has a mass between 0.2 M_{⊙} and 1.0 M_{⊙} in Advanced LIGO and Advanced Virgo data collected between 1 April 2019 1500 UTC and 1 October 2019 1500 UTC. We extend our previous analyses in two main ways: we include data from the Virgo detector and we allow for more unequal mass systems, with mass ratio q≥0.1. We do not report any gravitational-wave candidates. The most significant trigger has a false alarm rate of 0.14 yr^{-1}. This implies an upper limit on the merger rate of subsolar binaries in the range [220-24200] Gpc^{-3} yr^{-1}, depending on the chirp mass of the binary. We use this upper limit to derive astrophysical constraints on two phenomenological models that could produce subsolar-mass compact objects. One is an isotropic distribution of equal-mass primordial black holes. Using this model, we find that the fraction of dark matter in primordial black holes in the mass range 0.2 M_{⊙}<m_{PBH}<1.0 M_{⊙} is f_{PBH}≡Ω_{PBH}/Ω_{DM}≲6%. This improves existing constraints on primordial black hole abundance by a factor of ∼3. The other is a dissipative dark matter model, in which fermionic dark matter can collapse and form black holes. The upper limit on the fraction of dark matter black holes depends on the minimum mass of the black holes that can be formed: the most constraining result is obtained at M_{min}=1 M_{⊙}, where f_{DBH}≡Ω_{DBH}/Ω_{DM}≲0.003%. These are the first constraints placed on dissipative dark models by subsolar-mass analyses.
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Affiliation(s)
- R Abbott
- LIGO Laboratory, California Institute of Technology, Pasadena, California 91125, USA
| | - T D Abbott
- Louisiana State University, Baton Rouge, Louisiana 70803, USA
| | - F Acernese
- Dipartimento di Farmacia, Università di Salerno, I-84084 Fisciano, Salerno, Italy
- INFN, Sezione di Napoli, Complesso Universitario di Monte S. Angelo, I-80126 Napoli, Italy
| | - K Ackley
- OzGrav, School of Physics & Astronomy, Monash University, Clayton 3800, Victoria, Australia
| | - C Adams
- LIGO Livingston Observatory, Livingston, Louisiana 70754, USA
| | - N Adhikari
- University of Wisconsin-Milwaukee, Milwaukee, Wisconsin 53201, USA
| | - R X Adhikari
- LIGO Laboratory, California Institute of Technology, Pasadena, California 91125, USA
| | - V B Adya
- OzGrav, Australian National University, Canberra, Australian Capital Territory 0200, Australia
| | - C Affeldt
- Max Planck Institute for Gravitational Physics (Albert Einstein Institute), D-30167 Hannover, Germany
- Leibniz Universität Hannover, D-30167 Hannover, Germany
| | - D Agarwal
- Inter-University Centre for Astronomy and Astrophysics, Pune 411007, India
| | - M Agathos
- University of Cambridge, Cambridge CB2 1TN, United Kingdom
- Theoretisch-Physikalisches Institut, Friedrich-Schiller-Universität Jena, D-07743 Jena, Germany
| | - K Agatsuma
- University of Birmingham, Birmingham B15 2TT, United Kingdom
| | - N Aggarwal
- Center for Interdisciplinary Exploration & Research in Astrophysics (CIERA), Northwestern University, Evanston, Illinois 60208, USA
| | - O D Aguiar
- Instituto Nacional de Pesquisas Espaciais, 12227-010 São José dos Campos, São Paulo, Brazil
| | - L Aiello
- Gravity Exploration Institute, Cardiff University, Cardiff CF24 3AA, United Kingdom
| | - A Ain
- INFN, Sezione di Pisa, I-56127 Pisa, Italy
| | - P Ajith
- International Centre for Theoretical Sciences, Tata Institute of Fundamental Research, Bengaluru 560089, India
| | - S Albanesi
- INFN Sezione di Torino, I-10125 Torino, Italy
| | - A Allocca
- INFN, Sezione di Napoli, Complesso Universitario di Monte S. Angelo, I-80126 Napoli, Italy
- Università di Napoli "Federico II", Complesso Universitario di Monte S. Angelo, I-80126 Napoli, Italy
| | - P A Altin
- OzGrav, Australian National University, Canberra, Australian Capital Territory 0200, Australia
| | - A Amato
- Université de Lyon, Université Claude Bernard Lyon 1, CNRS, Institut Lumière Matière, F-69622 Villeurbanne, France
| | - C Anand
- OzGrav, School of Physics & Astronomy, Monash University, Clayton 3800, Victoria, Australia
| | - S Anand
- LIGO Laboratory, California Institute of Technology, Pasadena, California 91125, USA
| | - A Ananyeva
- LIGO Laboratory, California Institute of Technology, Pasadena, California 91125, USA
| | - S B Anderson
- LIGO Laboratory, California Institute of Technology, Pasadena, California 91125, USA
| | - W G Anderson
- University of Wisconsin-Milwaukee, Milwaukee, Wisconsin 53201, USA
| | - T Andrade
- Institut de Ciències del Cosmos (ICCUB), Universitat de Barcelona, C/ Martí i Franquès 1, Barcelona, 08028, Spain
| | - N Andres
- Laboratoire d'Annecy de Physique des Particules (LAPP), Université Grenoble Alpes, Université Savoie Mont Blanc, CNRS/IN2P3, F-74941 Annecy, France
| | - T Andrić
- Gran Sasso Science Institute (GSSI), I-67100 L'Aquila, Italy
| | - S V Angelova
- SUPA, University of Strathclyde, Glasgow G1 1XQ, United Kingdom
| | - S Ansoldi
- Dipartimento di Scienze Matematiche, Informatiche e Fisiche, Università di Udine, I-33100 Udine, Italy
- INFN, Sezione di Trieste, I-34127 Trieste, Italy
| | - J M Antelis
- Embry-Riddle Aeronautical University, Prescott, Arizona 86301, USA
| | - S Antier
- Université de Paris, CNRS, Astroparticule et Cosmologie, F-75006 Paris, France
| | - S Appert
- LIGO Laboratory, California Institute of Technology, Pasadena, California 91125, USA
| | - K Arai
- LIGO Laboratory, California Institute of Technology, Pasadena, California 91125, USA
| | - M C Araya
- LIGO Laboratory, California Institute of Technology, Pasadena, California 91125, USA
| | - J S Areeda
- California State University Fullerton, Fullerton, California 92831, USA
| | - M Arène
- Université de Paris, CNRS, Astroparticule et Cosmologie, F-75006 Paris, France
| | - N Arnaud
- Université Paris-Saclay, CNRS/IN2P3, IJCLab, 91405 Orsay, France
- European Gravitational Observatory (EGO), I-56021 Cascina, Pisa, Italy
| | - S M Aronson
- Louisiana State University, Baton Rouge, Louisiana 70803, USA
| | - K G Arun
- Chennai Mathematical Institute, Chennai 603103, India
| | - Y Asali
- Columbia University, New York, New York 10027, USA
| | - G Ashton
- OzGrav, School of Physics & Astronomy, Monash University, Clayton 3800, Victoria, Australia
| | - M Assiduo
- Università degli Studi di Urbino "Carlo Bo", I-61029 Urbino, Italy
- INFN, Sezione di Firenze, I-50019 Sesto Fiorentino, Firenze, Italy
| | - S M Aston
- LIGO Livingston Observatory, Livingston, Louisiana 70754, USA
| | - P Astone
- INFN, Sezione di Roma, I-00185 Roma, Italy
| | - F Aubin
- Laboratoire d'Annecy de Physique des Particules (LAPP), Université Grenoble Alpes, Université Savoie Mont Blanc, CNRS/IN2P3, F-74941 Annecy, France
| | - C Austin
- Louisiana State University, Baton Rouge, Louisiana 70803, USA
| | - S Babak
- Université de Paris, CNRS, Astroparticule et Cosmologie, F-75006 Paris, France
| | - F Badaracco
- Université catholique de Louvain, B-1348 Louvain-la-Neuve, Belgium
| | - M K M Bader
- Nikhef, Science Park 105, 1098 XG Amsterdam, Netherlands
| | - C Badger
- King's College London, University of London, London WC2R 2LS, United Kingdom
| | - S Bae
- Korea Institute of Science and Technology Information, Daejeon 34141, Republic of Korea
| | - A M Baer
- Christopher Newport University, Newport News, Virginia 23606, USA
| | - S Bagnasco
- INFN Sezione di Torino, I-10125 Torino, Italy
| | - Y Bai
- LIGO Laboratory, California Institute of Technology, Pasadena, California 91125, USA
| | - J Baird
- Université de Paris, CNRS, Astroparticule et Cosmologie, F-75006 Paris, France
| | - M Ball
- University of Oregon, Eugene, Oregon 97403, USA
| | - G Ballardin
- European Gravitational Observatory (EGO), I-56021 Cascina, Pisa, Italy
| | - S W Ballmer
- Syracuse University, Syracuse, New York 13244, USA
| | - A Balsamo
- Christopher Newport University, Newport News, Virginia 23606, USA
| | - G Baltus
- Université de Liège, B-4000 Liège, Belgium
| | - S Banagiri
- University of Minnesota, Minneapolis, Minnesota 55455, USA
| | - D Bankar
- Inter-University Centre for Astronomy and Astrophysics, Pune 411007, India
| | - J C Barayoga
- LIGO Laboratory, California Institute of Technology, Pasadena, California 91125, USA
| | - C Barbieri
- Università degli Studi di Milano-Bicocca, I-20126 Milano, Italy
- INFN, Sezione di Milano-Bicocca, I-20126 Milano, Italy
- INAF, Osservatorio Astronomico di Brera sede di Merate, I-23807 Merate, Lecco, Italy
| | - B C Barish
- LIGO Laboratory, California Institute of Technology, Pasadena, California 91125, USA
| | - D Barker
- LIGO Hanford Observatory, Richland, Washington 99352, USA
| | - P Barneo
- Institut de Ciències del Cosmos (ICCUB), Universitat de Barcelona, C/ Martí i Franquès 1, Barcelona, 08028, Spain
| | - F Barone
- INFN, Sezione di Napoli, Complesso Universitario di Monte S. Angelo, I-80126 Napoli, Italy
- Dipartimento di Medicina, Chirurgia e Odontoiatria "Scuola Medica Salernitana," Università di Salerno, I-84081 Baronissi, Salerno, Italy
| | - B Barr
- SUPA, University of Glasgow, Glasgow G12 8QQ, United Kingdom
| | - L Barsotti
- LIGO Laboratory, Massachusetts Institute of Technology, Cambridge, Massachusetts 02139, USA
| | - M Barsuglia
- Université de Paris, CNRS, Astroparticule et Cosmologie, F-75006 Paris, France
| | - D Barta
- Wigner RCP, RMKI, H-1121 Budapest, Konkoly Thege Miklós út 29-33, Hungary
| | - J Bartlett
- LIGO Hanford Observatory, Richland, Washington 99352, USA
| | - M A Barton
- SUPA, University of Glasgow, Glasgow G12 8QQ, United Kingdom
| | - I Bartos
- University of Florida, Gainesville, Florida 32611, USA
| | - R Bassiri
- Stanford University, Stanford, California 94305, USA
| | - A Basti
- INFN, Sezione di Pisa, I-56127 Pisa, Italy
- Università di Pisa, I-56127 Pisa, Italy
| | - M Bawaj
- INFN, Sezione di Perugia, I-06123 Perugia, Italy
- Università di Perugia, I-06123 Perugia, Italy
| | - J C Bayley
- SUPA, University of Glasgow, Glasgow G12 8QQ, United Kingdom
| | - A C Baylor
- University of Wisconsin-Milwaukee, Milwaukee, Wisconsin 53201, USA
| | - M Bazzan
- Università di Padova, Dipartimento di Fisica e Astronomia, I-35131 Padova, Italy
- INFN, Sezione di Padova, I-35131 Padova, Italy
| | - B Bécsy
- Montana State University, Bozeman, Montana 59717, USA
| | - V M Bedakihale
- Institute for Plasma Research, Bhat, Gandhinagar 382428, India
| | - M Bejger
- Nicolaus Copernicus Astronomical Center, Polish Academy of Sciences, 00-716, Warsaw, Poland
| | - I Belahcene
- Université Paris-Saclay, CNRS/IN2P3, IJCLab, 91405 Orsay, France
| | - V Benedetto
- Dipartimento di Ingegneria, Università del Sannio, I-82100 Benevento, Italy
| | - D Beniwal
- OzGrav, University of Adelaide, Adelaide, South Australia 5005, Australia
| | - T F Bennett
- California State University, Los Angeles, 5151 State University Dr, Los Angeles, California 90032, USA
| | - J D Bentley
- University of Birmingham, Birmingham B15 2TT, United Kingdom
| | - M BenYaala
- SUPA, University of Strathclyde, Glasgow G1 1XQ, United Kingdom
| | - F Bergamin
- Max Planck Institute for Gravitational Physics (Albert Einstein Institute), D-30167 Hannover, Germany
- Leibniz Universität Hannover, D-30167 Hannover, Germany
| | - B K Berger
- Stanford University, Stanford, California 94305, USA
| | - S Bernuzzi
- Theoretisch-Physikalisches Institut, Friedrich-Schiller-Universität Jena, D-07743 Jena, Germany
| | - C P L Berry
- Center for Interdisciplinary Exploration & Research in Astrophysics (CIERA), Northwestern University, Evanston, Illinois 60208, USA
- SUPA, University of Glasgow, Glasgow G12 8QQ, United Kingdom
| | | | - A Bertolini
- Nikhef, Science Park 105, 1098 XG Amsterdam, Netherlands
| | - J Betzwieser
- LIGO Livingston Observatory, Livingston, Louisiana 70754, USA
| | - D Beveridge
- OzGrav, University of Western Australia, Crawley, Western Australia 6009, Australia
| | - R Bhandare
- RRCAT, Indore, Madhya Pradesh 452013, India
| | - U Bhardwaj
- Nikhef, Science Park 105, 1098 XG Amsterdam, Netherlands
- GRAPPA, Anton Pannekoek Institute for Astronomy and Institute for High-Energy Physics, University of Amsterdam, Science Park 904, 1098 XH Amsterdam, Netherlands
| | - D Bhattacharjee
- Missouri University of Science and Technology, Rolla, Missouri 65409, USA
| | - S Bhaumik
- University of Florida, Gainesville, Florida 32611, USA
| | - I A Bilenko
- Faculty of Physics, Lomonosov Moscow State University, Moscow 119991, Russia
| | - G Billingsley
- LIGO Laboratory, California Institute of Technology, Pasadena, California 91125, USA
| | - S Bini
- Università di Trento, Dipartimento di Fisica, I-38123 Povo, Trento, Italy
- INFN, Trento Institute for Fundamental Physics and Applications, I-38123 Povo, Trento, Italy
| | - R Birney
- SUPA, University of the West of Scotland, Paisley PA1 2BE, United Kingdom
| | - O Birnholtz
- Bar-Ilan University, Ramat Gan, 5290002, Israel
| | - S Biscans
- LIGO Laboratory, California Institute of Technology, Pasadena, California 91125, USA
- LIGO Laboratory, Massachusetts Institute of Technology, Cambridge, Massachusetts 02139, USA
| | - M Bischi
- Università degli Studi di Urbino "Carlo Bo", I-61029 Urbino, Italy
- INFN, Sezione di Firenze, I-50019 Sesto Fiorentino, Firenze, Italy
| | - S Biscoveanu
- LIGO Laboratory, Massachusetts Institute of Technology, Cambridge, Massachusetts 02139, USA
| | - A Bisht
- Max Planck Institute for Gravitational Physics (Albert Einstein Institute), D-30167 Hannover, Germany
- Leibniz Universität Hannover, D-30167 Hannover, Germany
| | - B Biswas
- Inter-University Centre for Astronomy and Astrophysics, Pune 411007, India
| | - M Bitossi
- INFN, Sezione di Pisa, I-56127 Pisa, Italy
- European Gravitational Observatory (EGO), I-56021 Cascina, Pisa, Italy
| | - M-A Bizouard
- Artemis, Université Côte d'Azur, Observatoire de la Côte d'Azur, CNRS, F-06304 Nice, France
| | - J K Blackburn
- LIGO Laboratory, California Institute of Technology, Pasadena, California 91125, USA
| | - C D Blair
- LIGO Livingston Observatory, Livingston, Louisiana 70754, USA
- OzGrav, University of Western Australia, Crawley, Western Australia 6009, Australia
| | - D G Blair
- OzGrav, University of Western Australia, Crawley, Western Australia 6009, Australia
| | - R M Blair
- LIGO Hanford Observatory, Richland, Washington 99352, USA
| | - F Bobba
- Dipartimento di Fisica "E.R. Caianiello," Università di Salerno, I-84084 Fisciano, Salerno, Italy
- INFN, Sezione di Napoli, Gruppo Collegato di Salerno, Complesso Universitario di Monte S. Angelo, I-80126 Napoli, Italy
| | - N Bode
- Max Planck Institute for Gravitational Physics (Albert Einstein Institute), D-30167 Hannover, Germany
- Leibniz Universität Hannover, D-30167 Hannover, Germany
| | - M Boer
- Artemis, Université Côte d'Azur, Observatoire de la Côte d'Azur, CNRS, F-06304 Nice, France
| | - G Bogaert
- Artemis, Université Côte d'Azur, Observatoire de la Côte d'Azur, CNRS, F-06304 Nice, France
| | - M Boldrini
- INFN, Sezione di Roma, I-00185 Roma, Italy
- Università di Roma "La Sapienza," I-00185 Roma, Italy
| | - L D Bonavena
- Università di Padova, Dipartimento di Fisica e Astronomia, I-35131 Padova, Italy
| | - F Bondu
- Université Rennes, CNRS, Institut FOTON-UMR6082, F-3500 Rennes, France
| | - E Bonilla
- Stanford University, Stanford, California 94305, USA
| | - R Bonnand
- Laboratoire d'Annecy de Physique des Particules (LAPP), Université Grenoble Alpes, Université Savoie Mont Blanc, CNRS/IN2P3, F-74941 Annecy, France
| | - P Booker
- Max Planck Institute for Gravitational Physics (Albert Einstein Institute), D-30167 Hannover, Germany
- Leibniz Universität Hannover, D-30167 Hannover, Germany
| | - B A Boom
- Nikhef, Science Park 105, 1098 XG Amsterdam, Netherlands
| | - R Bork
- LIGO Laboratory, California Institute of Technology, Pasadena, California 91125, USA
| | - V Boschi
- INFN, Sezione di Pisa, I-56127 Pisa, Italy
| | - N Bose
- Indian Institute of Technology Bombay, Powai, Mumbai 400 076, India
| | - S Bose
- Inter-University Centre for Astronomy and Astrophysics, Pune 411007, India
| | - V Bossilkov
- OzGrav, University of Western Australia, Crawley, Western Australia 6009, Australia
| | - V Boudart
- Université de Liège, B-4000 Liège, Belgium
| | - Y Bouffanais
- Università di Padova, Dipartimento di Fisica e Astronomia, I-35131 Padova, Italy
- INFN, Sezione di Padova, I-35131 Padova, Italy
| | - A Bozzi
- European Gravitational Observatory (EGO), I-56021 Cascina, Pisa, Italy
| | | | - P R Brady
- University of Wisconsin-Milwaukee, Milwaukee, Wisconsin 53201, USA
| | - A Bramley
- LIGO Livingston Observatory, Livingston, Louisiana 70754, USA
| | - A Branch
- LIGO Livingston Observatory, Livingston, Louisiana 70754, USA
| | - M Branchesi
- Gran Sasso Science Institute (GSSI), I-67100 L'Aquila, Italy
- INFN, Laboratori Nazionali del Gran Sasso, I-67100 Assergi, Italy
| | - J E Brau
- University of Oregon, Eugene, Oregon 97403, USA
| | - M Breschi
- Theoretisch-Physikalisches Institut, Friedrich-Schiller-Universität Jena, D-07743 Jena, Germany
| | - T Briant
- Laboratoire Kastler Brossel, Sorbonne Université, CNRS, ENS-Université PSL, Collège de France, F-75005 Paris, France
| | - J H Briggs
- SUPA, University of Glasgow, Glasgow G12 8QQ, United Kingdom
| | - A Brillet
- Artemis, Université Côte d'Azur, Observatoire de la Côte d'Azur, CNRS, F-06304 Nice, France
| | - M Brinkmann
- Max Planck Institute for Gravitational Physics (Albert Einstein Institute), D-30167 Hannover, Germany
- Leibniz Universität Hannover, D-30167 Hannover, Germany
| | - P Brockill
- University of Wisconsin-Milwaukee, Milwaukee, Wisconsin 53201, USA
| | - A F Brooks
- LIGO Laboratory, California Institute of Technology, Pasadena, California 91125, USA
| | - J Brooks
- European Gravitational Observatory (EGO), I-56021 Cascina, Pisa, Italy
| | - D D Brown
- OzGrav, University of Adelaide, Adelaide, South Australia 5005, Australia
| | - S Brunett
- LIGO Laboratory, California Institute of Technology, Pasadena, California 91125, USA
| | - G Bruno
- Université catholique de Louvain, B-1348 Louvain-la-Neuve, Belgium
| | - R Bruntz
- Christopher Newport University, Newport News, Virginia 23606, USA
| | - J Bryant
- University of Birmingham, Birmingham B15 2TT, United Kingdom
| | - T Bulik
- Astronomical Observatory Warsaw University, 00-478 Warsaw, Poland
| | - H J Bulten
- Nikhef, Science Park 105, 1098 XG Amsterdam, Netherlands
| | - A Buonanno
- University of Maryland, College Park, Maryland 20742, USA
- Max Planck Institute for Gravitational Physics (Albert Einstein Institute), D-14476 Potsdam, Germany
| | - R Buscicchio
- University of Birmingham, Birmingham B15 2TT, United Kingdom
| | - D Buskulic
- Laboratoire d'Annecy de Physique des Particules (LAPP), Université Grenoble Alpes, Université Savoie Mont Blanc, CNRS/IN2P3, F-74941 Annecy, France
| | - C Buy
- L2IT, Laboratoire des 2 Infinis-Toulouse, Université de Toulouse, CNRS/IN2P3, UPS, F-31062 Toulouse Cedex 9, France
| | - R L Byer
- Stanford University, Stanford, California 94305, USA
| | - L Cadonati
- School of Physics, Georgia Institute of Technology, Atlanta, Georgia 30332, USA
| | - G Cagnoli
- Université de Lyon, Université Claude Bernard Lyon 1, CNRS, Institut Lumière Matière, F-69622 Villeurbanne, France
| | - C Cahillane
- LIGO Hanford Observatory, Richland, Washington 99352, USA
| | - J Calderón Bustillo
- IGFAE, Campus Sur, Universidade de Santiago de Compostela, 15782 Spain
- The Chinese University of Hong Kong, Shatin, NT, Hong Kong
| | - J D Callaghan
- SUPA, University of Glasgow, Glasgow G12 8QQ, United Kingdom
| | - T A Callister
- Stony Brook University, Stony Brook, New York 11794, USA
- Center for Computational Astrophysics, Flatiron Institute, New York, New York 10010, USA
| | - E Calloni
- INFN, Sezione di Napoli, Complesso Universitario di Monte S. Angelo, I-80126 Napoli, Italy
- Università di Napoli "Federico II", Complesso Universitario di Monte S. Angelo, I-80126 Napoli, Italy
| | - J Cameron
- OzGrav, University of Western Australia, Crawley, Western Australia 6009, Australia
| | - J B Camp
- NASA Goddard Space Flight Center, Greenbelt, Maryland 20771, USA
| | - M Canepa
- INFN, Sezione di Genova, I-16146 Genova, Italy
- Dipartimento di Fisica, Università degli Studi di Genova, I-16146 Genova, Italy
| | - S Canevarolo
- Institute for Gravitational and Subatomic Physics (GRASP), Utrecht University, Princetonplein 1, 3584 CC Utrecht, Netherlands
| | - M Cannavacciuolo
- Dipartimento di Fisica "E.R. Caianiello," Università di Salerno, I-84084 Fisciano, Salerno, Italy
| | - K C Cannon
- RESCEU, University of Tokyo, Tokyo, 113-0033, Japan
| | - H Cao
- OzGrav, University of Adelaide, Adelaide, South Australia 5005, Australia
| | - E Capote
- Syracuse University, Syracuse, New York 13244, USA
| | - G Carapella
- Dipartimento di Fisica "E.R. Caianiello," Università di Salerno, I-84084 Fisciano, Salerno, Italy
- INFN, Sezione di Napoli, Gruppo Collegato di Salerno, Complesso Universitario di Monte S. Angelo, I-80126 Napoli, Italy
| | - F Carbognani
- European Gravitational Observatory (EGO), I-56021 Cascina, Pisa, Italy
| | - J B Carlin
- OzGrav, University of Melbourne, Parkville, Victoria 3010, Australia
| | - M F Carney
- Center for Interdisciplinary Exploration & Research in Astrophysics (CIERA), Northwestern University, Evanston, Illinois 60208, USA
| | - M Carpinelli
- European Gravitational Observatory (EGO), I-56021 Cascina, Pisa, Italy
- Università degli Studi di Sassari, I-07100 Sassari, Italy
- INFN, Laboratori Nazionali del Sud, I-95125 Catania, Italy
| | - G Carrillo
- University of Oregon, Eugene, Oregon 97403, USA
| | - G Carullo
- INFN, Sezione di Pisa, I-56127 Pisa, Italy
- Università di Pisa, I-56127 Pisa, Italy
| | - T L Carver
- Gravity Exploration Institute, Cardiff University, Cardiff CF24 3AA, United Kingdom
| | - J Casanueva Diaz
- European Gravitational Observatory (EGO), I-56021 Cascina, Pisa, Italy
| | - C Casentini
- Università di Roma Tor Vergata, I-00133 Roma, Italy
- INFN, Sezione di Roma Tor Vergata, I-00133 Roma, Italy
| | - G Castaldi
- University of Sannio at Benevento, I-82100 Benevento, Italy and INFN, Sezione di Napoli, I-80100 Napoli, Italy
| | - S Caudill
- Nikhef, Science Park 105, 1098 XG Amsterdam, Netherlands
- Institute for Gravitational and Subatomic Physics (GRASP), Utrecht University, Princetonplein 1, 3584 CC Utrecht, Netherlands
| | - M Cavaglià
- Missouri University of Science and Technology, Rolla, Missouri 65409, USA
| | - F Cavalier
- Université Paris-Saclay, CNRS/IN2P3, IJCLab, 91405 Orsay, France
| | - R Cavalieri
- European Gravitational Observatory (EGO), I-56021 Cascina, Pisa, Italy
| | - M Ceasar
- Villanova University, 800 Lancaster Avenue, Villanova, Pennsylvania 19085, USA
| | - G Cella
- INFN, Sezione di Pisa, I-56127 Pisa, Italy
| | - P Cerdá-Durán
- Departamento de Astronomía y Astrofísica, Universitat de València, E-46100 Burjassot, València, Spain
| | - E Cesarini
- INFN, Sezione di Roma Tor Vergata, I-00133 Roma, Italy
| | - W Chaibi
- Artemis, Université Côte d'Azur, Observatoire de la Côte d'Azur, CNRS, F-06304 Nice, France
| | - K Chakravarti
- Inter-University Centre for Astronomy and Astrophysics, Pune 411007, India
| | | | - E Champion
- Rochester Institute of Technology, Rochester, New York 14623, USA
| | - C-H Chan
- National Tsing Hua University, Hsinchu City, 30013 Taiwan, Republic of China
| | - C Chan
- RESCEU, University of Tokyo, Tokyo, 113-0033, Japan
| | - C L Chan
- The Chinese University of Hong Kong, Shatin, NT, Hong Kong
| | - K Chan
- The Chinese University of Hong Kong, Shatin, NT, Hong Kong
| | - K Chandra
- Indian Institute of Technology Bombay, Powai, Mumbai 400 076, India
| | - P Chanial
- European Gravitational Observatory (EGO), I-56021 Cascina, Pisa, Italy
| | - S Chao
- National Tsing Hua University, Hsinchu City, 30013 Taiwan, Republic of China
| | - P Charlton
- OzGrav, Charles Sturt University, Wagga Wagga, New South Wales 2678, Australia
| | - E A Chase
- Center for Interdisciplinary Exploration & Research in Astrophysics (CIERA), Northwestern University, Evanston, Illinois 60208, USA
| | - E Chassande-Mottin
- Université de Paris, CNRS, Astroparticule et Cosmologie, F-75006 Paris, France
| | - C Chatterjee
- OzGrav, University of Western Australia, Crawley, Western Australia 6009, Australia
| | | | - Deep Chatterjee
- University of Wisconsin-Milwaukee, Milwaukee, Wisconsin 53201, USA
| | | | - S Chaty
- Université de Paris, CNRS, Astroparticule et Cosmologie, F-75006 Paris, France
| | - K Chatziioannou
- LIGO Laboratory, California Institute of Technology, Pasadena, California 91125, USA
| | - H Y Chen
- LIGO Laboratory, Massachusetts Institute of Technology, Cambridge, Massachusetts 02139, USA
| | - J Chen
- National Tsing Hua University, Hsinchu City, 30013 Taiwan, Republic of China
| | - X Chen
- OzGrav, University of Western Australia, Crawley, Western Australia 6009, Australia
| | - Y Chen
- CaRT, California Institute of Technology, Pasadena, California 91125, USA
| | - Z Chen
- Gravity Exploration Institute, Cardiff University, Cardiff CF24 3AA, United Kingdom
| | - H Cheng
- University of Florida, Gainesville, Florida 32611, USA
| | - C K Cheong
- The Chinese University of Hong Kong, Shatin, NT, Hong Kong
| | - H Y Cheung
- The Chinese University of Hong Kong, Shatin, NT, Hong Kong
| | - H Y Chia
- University of Florida, Gainesville, Florida 32611, USA
| | - F Chiadini
- INFN, Sezione di Napoli, Gruppo Collegato di Salerno, Complesso Universitario di Monte S. Angelo, I-80126 Napoli, Italy
- Dipartimento di Ingegneria Industriale (DIIN), Università di Salerno, I-84084 Fisciano, Salerno, Italy
| | - G Chiarini
- INFN, Sezione di Padova, I-35131 Padova, Italy
| | - R Chierici
- Université Lyon, Université Claude Bernard Lyon 1, CNRS, IP2I Lyon / IN2P3, UMR 5822, F-69622 Villeurbanne, France
| | | | - M L Chiofalo
- INFN, Sezione di Pisa, I-56127 Pisa, Italy
- Università di Pisa, I-56127 Pisa, Italy
| | - A Chiummo
- European Gravitational Observatory (EGO), I-56021 Cascina, Pisa, Italy
| | - G Cho
- Seoul National University, Seoul 08826, Republic of Korea
| | - H S Cho
- Pusan National University, Busan 46241, Republic of Korea
| | - R K Choudhary
- OzGrav, University of Western Australia, Crawley, Western Australia 6009, Australia
| | - S Choudhary
- Inter-University Centre for Astronomy and Astrophysics, Pune 411007, India
| | - N Christensen
- Artemis, Université Côte d'Azur, Observatoire de la Côte d'Azur, CNRS, F-06304 Nice, France
| | - Q Chu
- OzGrav, University of Western Australia, Crawley, Western Australia 6009, Australia
| | - S Chua
- OzGrav, Australian National University, Canberra, Australian Capital Territory 0200, Australia
| | - K W Chung
- King's College London, University of London, London WC2R 2LS, United Kingdom
| | - G Ciani
- Università di Padova, Dipartimento di Fisica e Astronomia, I-35131 Padova, Italy
- INFN, Sezione di Padova, I-35131 Padova, Italy
| | - P Ciecielag
- Nicolaus Copernicus Astronomical Center, Polish Academy of Sciences, 00-716, Warsaw, Poland
| | - M Cieślar
- Nicolaus Copernicus Astronomical Center, Polish Academy of Sciences, 00-716, Warsaw, Poland
| | - M Cifaldi
- Università di Roma Tor Vergata, I-00133 Roma, Italy
- INFN, Sezione di Roma Tor Vergata, I-00133 Roma, Italy
| | - A A Ciobanu
- OzGrav, University of Adelaide, Adelaide, South Australia 5005, Australia
| | - R Ciolfi
- INFN, Sezione di Padova, I-35131 Padova, Italy
- INAF, Osservatorio Astronomico di Padova, I-35122 Padova, Italy
| | - F Cipriano
- Artemis, Université Côte d'Azur, Observatoire de la Côte d'Azur, CNRS, F-06304 Nice, France
| | - A Cirone
- INFN, Sezione di Genova, I-16146 Genova, Italy
- Dipartimento di Fisica, Università degli Studi di Genova, I-16146 Genova, Italy
| | - F Clara
- LIGO Hanford Observatory, Richland, Washington 99352, USA
| | - E N Clark
- University of Arizona, Tucson, Arizona 85721, USA
| | - J A Clark
- LIGO Laboratory, California Institute of Technology, Pasadena, California 91125, USA
- School of Physics, Georgia Institute of Technology, Atlanta, Georgia 30332, USA
| | - L Clarke
- Rutherford Appleton Laboratory, Didcot OX11 0DE, United Kingdom
| | - P Clearwater
- OzGrav, Swinburne University of Technology, Hawthorn VIC 3122, Australia
| | - S Clesse
- Université libre de Bruxelles, Avenue Franklin Roosevelt 50-1050 Bruxelles, Belgium
| | - F Cleva
- Artemis, Université Côte d'Azur, Observatoire de la Côte d'Azur, CNRS, F-06304 Nice, France
| | - E Coccia
- Gran Sasso Science Institute (GSSI), I-67100 L'Aquila, Italy
- INFN, Laboratori Nazionali del Gran Sasso, I-67100 Assergi, Italy
| | - E Codazzo
- Gran Sasso Science Institute (GSSI), I-67100 L'Aquila, Italy
| | - P-F Cohadon
- Laboratoire Kastler Brossel, Sorbonne Université, CNRS, ENS-Université PSL, Collège de France, F-75005 Paris, France
| | - D E Cohen
- Université Paris-Saclay, CNRS/IN2P3, IJCLab, 91405 Orsay, France
| | - L Cohen
- Louisiana State University, Baton Rouge, Louisiana 70803, USA
| | - M Colleoni
- Universitat de les Illes Balears, IAC3-IEEC, E-07122 Palma de Mallorca, Spain
| | - C G Collette
- Université Libre de Bruxelles, Brussels 1050, Belgium
| | - A Colombo
- Università degli Studi di Milano-Bicocca, I-20126 Milano, Italy
| | - M Colpi
- Università degli Studi di Milano-Bicocca, I-20126 Milano, Italy
- INFN, Sezione di Milano-Bicocca, I-20126 Milano, Italy
| | - C M Compton
- LIGO Hanford Observatory, Richland, Washington 99352, USA
| | - M Constancio
- Instituto Nacional de Pesquisas Espaciais, 12227-010 São José dos Campos, São Paulo, Brazil
| | - L Conti
- INFN, Sezione di Padova, I-35131 Padova, Italy
| | - S J Cooper
- University of Birmingham, Birmingham B15 2TT, United Kingdom
| | - P Corban
- LIGO Livingston Observatory, Livingston, Louisiana 70754, USA
| | - T R Corbitt
- Louisiana State University, Baton Rouge, Louisiana 70803, USA
| | - I Cordero-Carrión
- Departamento de Matemáticas, Universitat de València, E-46100 Burjassot, València, Spain
| | - S Corezzi
- INFN, Sezione di Perugia, I-06123 Perugia, Italy
- Università di Perugia, I-06123 Perugia, Italy
| | - K R Corley
- Columbia University, New York, New York 10027, USA
| | - N Cornish
- Montana State University, Bozeman, Montana 59717, USA
| | - D Corre
- Université Paris-Saclay, CNRS/IN2P3, IJCLab, 91405 Orsay, France
| | - A Corsi
- Texas Tech University, Lubbock, Texas 79409, USA
| | - S Cortese
- European Gravitational Observatory (EGO), I-56021 Cascina, Pisa, Italy
| | - C A Costa
- Instituto Nacional de Pesquisas Espaciais, 12227-010 São José dos Campos, São Paulo, Brazil
| | - R Cotesta
- Max Planck Institute for Gravitational Physics (Albert Einstein Institute), D-14476 Potsdam, Germany
| | - M W Coughlin
- University of Minnesota, Minneapolis, Minnesota 55455, USA
| | - J-P Coulon
- Artemis, Université Côte d'Azur, Observatoire de la Côte d'Azur, CNRS, F-06304 Nice, France
| | | | - B Cousins
- The Pennsylvania State University, University Park, Pennsylvania 16802, USA
| | - P Couvares
- LIGO Laboratory, California Institute of Technology, Pasadena, California 91125, USA
| | - D M Coward
- OzGrav, University of Western Australia, Crawley, Western Australia 6009, Australia
| | - M J Cowart
- LIGO Livingston Observatory, Livingston, Louisiana 70754, USA
| | - D C Coyne
- LIGO Laboratory, California Institute of Technology, Pasadena, California 91125, USA
| | - R Coyne
- University of Rhode Island, Kingston, Rhode Island 02881, USA
| | - J D E Creighton
- University of Wisconsin-Milwaukee, Milwaukee, Wisconsin 53201, USA
| | - T D Creighton
- The University of Texas Rio Grande Valley, Brownsville, Texas 78520, USA
| | - A W Criswell
- University of Minnesota, Minneapolis, Minnesota 55455, USA
| | - M Croquette
- Laboratoire Kastler Brossel, Sorbonne Université, CNRS, ENS-Université PSL, Collège de France, F-75005 Paris, France
| | - S G Crowder
- Bellevue College, Bellevue, Washington 98007, USA
| | - J R Cudell
- Université de Liège, B-4000 Liège, Belgium
| | - T J Cullen
- Louisiana State University, Baton Rouge, Louisiana 70803, USA
| | - A Cumming
- SUPA, University of Glasgow, Glasgow G12 8QQ, United Kingdom
| | - R Cummings
- SUPA, University of Glasgow, Glasgow G12 8QQ, United Kingdom
| | - L Cunningham
- SUPA, University of Glasgow, Glasgow G12 8QQ, United Kingdom
| | - E Cuoco
- INFN, Sezione di Pisa, I-56127 Pisa, Italy
- European Gravitational Observatory (EGO), I-56021 Cascina, Pisa, Italy
- Scuola Normale Superiore, Piazza dei Cavalieri, 7-56126 Pisa, Italy
| | - M Curyło
- Astronomical Observatory Warsaw University, 00-478 Warsaw, Poland
| | - P Dabadie
- Université de Lyon, Université Claude Bernard Lyon 1, CNRS, Institut Lumière Matière, F-69622 Villeurbanne, France
| | - T Dal Canton
- Université Paris-Saclay, CNRS/IN2P3, IJCLab, 91405 Orsay, France
| | - S Dall'Osso
- Gran Sasso Science Institute (GSSI), I-67100 L'Aquila, Italy
| | - G Dálya
- MTA-ELTE Astrophysics Research Group, Institute of Physics, Eötvös University, Budapest 1117, Hungary
| | - A Dana
- Stanford University, Stanford, California 94305, USA
| | - L M DaneshgaranBajastani
- California State University, Los Angeles, 5151 State University Dr, Los Angeles, California 90032, USA
| | - B D'Angelo
- INFN, Sezione di Genova, I-16146 Genova, Italy
- Dipartimento di Fisica, Università degli Studi di Genova, I-16146 Genova, Italy
| | - S Danilishin
- Nikhef, Science Park 105, 1098 XG Amsterdam, Netherlands
- Maastricht University, P.O. Box 616, 6200 MD Maastricht, Netherlands
| | - S D'Antonio
- INFN, Sezione di Roma Tor Vergata, I-00133 Roma, Italy
| | - K Danzmann
- Max Planck Institute for Gravitational Physics (Albert Einstein Institute), D-30167 Hannover, Germany
- Leibniz Universität Hannover, D-30167 Hannover, Germany
| | | | - A Dasgupta
- Institute for Plasma Research, Bhat, Gandhinagar 382428, India
| | - L E H Datrier
- SUPA, University of Glasgow, Glasgow G12 8QQ, United Kingdom
| | - S Datta
- Inter-University Centre for Astronomy and Astrophysics, Pune 411007, India
| | - V Dattilo
- European Gravitational Observatory (EGO), I-56021 Cascina, Pisa, Italy
| | - I Dave
- RRCAT, Indore, Madhya Pradesh 452013, India
| | - M Davier
- Université Paris-Saclay, CNRS/IN2P3, IJCLab, 91405 Orsay, France
| | - G S Davies
- University of Portsmouth, Portsmouth, PO1 3FX, United Kingdom
| | - D Davis
- LIGO Laboratory, California Institute of Technology, Pasadena, California 91125, USA
| | - M C Davis
- Villanova University, 800 Lancaster Avenue, Villanova, Pennsylvania 19085, USA
| | - E J Daw
- The University of Sheffield, Sheffield S10 2TN, United Kingdom
| | - R Dean
- Villanova University, 800 Lancaster Avenue, Villanova, Pennsylvania 19085, USA
| | - D DeBra
- Stanford University, Stanford, California 94305, USA
| | - M Deenadayalan
- Inter-University Centre for Astronomy and Astrophysics, Pune 411007, India
| | - J Degallaix
- Université Lyon, Université Claude Bernard Lyon 1, CNRS, Laboratoire des Matériaux Avancés (LMA), IP2I Lyon / IN2P3, UMR 5822, F-69622 Villeurbanne, France
| | - M De Laurentis
- INFN, Sezione di Napoli, Complesso Universitario di Monte S. Angelo, I-80126 Napoli, Italy
- Università di Napoli "Federico II", Complesso Universitario di Monte S. Angelo, I-80126 Napoli, Italy
| | - S Deléglise
- Laboratoire Kastler Brossel, Sorbonne Université, CNRS, ENS-Université PSL, Collège de France, F-75005 Paris, France
| | - V Del Favero
- Rochester Institute of Technology, Rochester, New York 14623, USA
| | - F De Lillo
- Université catholique de Louvain, B-1348 Louvain-la-Neuve, Belgium
| | - N De Lillo
- SUPA, University of Glasgow, Glasgow G12 8QQ, United Kingdom
| | - W Del Pozzo
- INFN, Sezione di Pisa, I-56127 Pisa, Italy
- Università di Pisa, I-56127 Pisa, Italy
| | - L M DeMarchi
- Center for Interdisciplinary Exploration & Research in Astrophysics (CIERA), Northwestern University, Evanston, Illinois 60208, USA
| | - F De Matteis
- Università di Roma Tor Vergata, I-00133 Roma, Italy
- INFN, Sezione di Roma Tor Vergata, I-00133 Roma, Italy
| | - V D'Emilio
- Gravity Exploration Institute, Cardiff University, Cardiff CF24 3AA, United Kingdom
| | - N Demos
- LIGO Laboratory, Massachusetts Institute of Technology, Cambridge, Massachusetts 02139, USA
| | - T Dent
- IGFAE, Campus Sur, Universidade de Santiago de Compostela, 15782 Spain
| | - A Depasse
- Université catholique de Louvain, B-1348 Louvain-la-Neuve, Belgium
| | - R De Pietri
- Dipartimento di Scienze Matematiche, Fisiche e Informatiche, Università di Parma, I-43124 Parma, Italy
- INFN, Sezione di Milano Bicocca, Gruppo Collegato di Parma, I-43124 Parma, Italy
| | - R De Rosa
- INFN, Sezione di Napoli, Complesso Universitario di Monte S. Angelo, I-80126 Napoli, Italy
- Università di Napoli "Federico II", Complesso Universitario di Monte S. Angelo, I-80126 Napoli, Italy
| | - C De Rossi
- European Gravitational Observatory (EGO), I-56021 Cascina, Pisa, Italy
| | - R DeSalvo
- University of Sannio at Benevento, I-82100 Benevento, Italy and INFN, Sezione di Napoli, I-80100 Napoli, Italy
| | - R De Simone
- Dipartimento di Ingegneria Industriale (DIIN), Università di Salerno, I-84084 Fisciano, Salerno, Italy
| | - S Dhurandhar
- Inter-University Centre for Astronomy and Astrophysics, Pune 411007, India
| | - M C Díaz
- The University of Texas Rio Grande Valley, Brownsville, Texas 78520, USA
| | - M Diaz-Ortiz
- University of Florida, Gainesville, Florida 32611, USA
| | - N A Didio
- Syracuse University, Syracuse, New York 13244, USA
| | - T Dietrich
- Nikhef, Science Park 105, 1098 XG Amsterdam, Netherlands
- Max Planck Institute for Gravitational Physics (Albert Einstein Institute), D-14476 Potsdam, Germany
| | - L Di Fiore
- INFN, Sezione di Napoli, Complesso Universitario di Monte S. Angelo, I-80126 Napoli, Italy
| | - C Di Fronzo
- University of Birmingham, Birmingham B15 2TT, United Kingdom
| | - C Di Giorgio
- Dipartimento di Fisica "E.R. Caianiello," Università di Salerno, I-84084 Fisciano, Salerno, Italy
- INFN, Sezione di Napoli, Gruppo Collegato di Salerno, Complesso Universitario di Monte S. Angelo, I-80126 Napoli, Italy
| | - F Di Giovanni
- Departamento de Astronomía y Astrofísica, Universitat de València, E-46100 Burjassot, València, Spain
| | - M Di Giovanni
- Gran Sasso Science Institute (GSSI), I-67100 L'Aquila, Italy
| | - T Di Girolamo
- INFN, Sezione di Napoli, Complesso Universitario di Monte S. Angelo, I-80126 Napoli, Italy
- Università di Napoli "Federico II", Complesso Universitario di Monte S. Angelo, I-80126 Napoli, Italy
| | - A Di Lieto
- INFN, Sezione di Pisa, I-56127 Pisa, Italy
- Università di Pisa, I-56127 Pisa, Italy
| | - B Ding
- Université Libre de Bruxelles, Brussels 1050, Belgium
| | - S Di Pace
- INFN, Sezione di Roma, I-00185 Roma, Italy
- Università di Roma "La Sapienza," I-00185 Roma, Italy
| | - I Di Palma
- INFN, Sezione di Roma, I-00185 Roma, Italy
- Università di Roma "La Sapienza," I-00185 Roma, Italy
| | - F Di Renzo
- INFN, Sezione di Pisa, I-56127 Pisa, Italy
- Università di Pisa, I-56127 Pisa, Italy
| | - A K Divakarla
- University of Florida, Gainesville, Florida 32611, USA
| | - A Dmitriev
- University of Birmingham, Birmingham B15 2TT, United Kingdom
| | - Z Doctor
- University of Oregon, Eugene, Oregon 97403, USA
| | - L D'Onofrio
- INFN, Sezione di Napoli, Complesso Universitario di Monte S. Angelo, I-80126 Napoli, Italy
- Università di Napoli "Federico II", Complesso Universitario di Monte S. Angelo, I-80126 Napoli, Italy
| | - F Donovan
- LIGO Laboratory, Massachusetts Institute of Technology, Cambridge, Massachusetts 02139, USA
| | - K L Dooley
- Gravity Exploration Institute, Cardiff University, Cardiff CF24 3AA, United Kingdom
| | - S Doravari
- Inter-University Centre for Astronomy and Astrophysics, Pune 411007, India
| | - I Dorrington
- Gravity Exploration Institute, Cardiff University, Cardiff CF24 3AA, United Kingdom
| | - M Drago
- INFN, Sezione di Roma, I-00185 Roma, Italy
- Università di Roma "La Sapienza," I-00185 Roma, Italy
| | - J C Driggers
- LIGO Hanford Observatory, Richland, Washington 99352, USA
| | - Y Drori
- LIGO Laboratory, California Institute of Technology, Pasadena, California 91125, USA
| | - J-G Ducoin
- Université Paris-Saclay, CNRS/IN2P3, IJCLab, 91405 Orsay, France
| | - P Dupej
- SUPA, University of Glasgow, Glasgow G12 8QQ, United Kingdom
| | - O Durante
- Dipartimento di Fisica "E.R. Caianiello," Università di Salerno, I-84084 Fisciano, Salerno, Italy
- INFN, Sezione di Napoli, Gruppo Collegato di Salerno, Complesso Universitario di Monte S. Angelo, I-80126 Napoli, Italy
| | - D D'Urso
- Università degli Studi di Sassari, I-07100 Sassari, Italy
- INFN, Laboratori Nazionali del Sud, I-95125 Catania, Italy
| | - P-A Duverne
- Université Paris-Saclay, CNRS/IN2P3, IJCLab, 91405 Orsay, France
| | - S E Dwyer
- LIGO Hanford Observatory, Richland, Washington 99352, USA
| | - C Eassa
- LIGO Hanford Observatory, Richland, Washington 99352, USA
| | - P J Easter
- OzGrav, School of Physics & Astronomy, Monash University, Clayton 3800, Victoria, Australia
| | - M Ebersold
- Physik-Institut, University of Zurich, Winterthurerstrasse 190, 8057 Zurich, Switzerland
| | - T Eckhardt
- Universität Hamburg, D-22761 Hamburg, Germany
| | - G Eddolls
- SUPA, University of Glasgow, Glasgow G12 8QQ, United Kingdom
| | - B Edelman
- University of Oregon, Eugene, Oregon 97403, USA
| | - T B Edo
- LIGO Laboratory, California Institute of Technology, Pasadena, California 91125, USA
| | - O Edy
- University of Portsmouth, Portsmouth, PO1 3FX, United Kingdom
| | - A Effler
- LIGO Livingston Observatory, Livingston, Louisiana 70754, USA
| | - J Eichholz
- OzGrav, Australian National University, Canberra, Australian Capital Territory 0200, Australia
| | | | - M Eisenmann
- Laboratoire d'Annecy de Physique des Particules (LAPP), Université Grenoble Alpes, Université Savoie Mont Blanc, CNRS/IN2P3, F-74941 Annecy, France
| | - R A Eisenstein
- LIGO Laboratory, Massachusetts Institute of Technology, Cambridge, Massachusetts 02139, USA
| | - A Ejlli
- Gravity Exploration Institute, Cardiff University, Cardiff CF24 3AA, United Kingdom
| | - E Engelby
- California State University Fullerton, Fullerton, California 92831, USA
| | - L Errico
- INFN, Sezione di Napoli, Complesso Universitario di Monte S. Angelo, I-80126 Napoli, Italy
- Università di Napoli "Federico II", Complesso Universitario di Monte S. Angelo, I-80126 Napoli, Italy
| | - R C Essick
- University of Chicago, Chicago, Illinois 60637, USA
| | - H Estellés
- Universitat de les Illes Balears, IAC3-IEEC, E-07122 Palma de Mallorca, Spain
| | - D Estevez
- Université de Strasbourg, CNRS, IPHC UMR 7178, F-67000 Strasbourg, France
| | - Z Etienne
- West Virginia University, Morgantown, West Virginia 26506, USA
| | - T Etzel
- LIGO Laboratory, California Institute of Technology, Pasadena, California 91125, USA
| | - M Evans
- LIGO Laboratory, Massachusetts Institute of Technology, Cambridge, Massachusetts 02139, USA
| | - T M Evans
- LIGO Livingston Observatory, Livingston, Louisiana 70754, USA
| | - B E Ewing
- The Pennsylvania State University, University Park, Pennsylvania 16802, USA
| | - V Fafone
- Gran Sasso Science Institute (GSSI), I-67100 L'Aquila, Italy
- Università di Roma Tor Vergata, I-00133 Roma, Italy
- INFN, Sezione di Roma Tor Vergata, I-00133 Roma, Italy
| | - H Fair
- Syracuse University, Syracuse, New York 13244, USA
| | - S Fairhurst
- Gravity Exploration Institute, Cardiff University, Cardiff CF24 3AA, United Kingdom
| | - A M Farah
- University of Chicago, Chicago, Illinois 60637, USA
| | - S Farinon
- INFN, Sezione di Genova, I-16146 Genova, Italy
| | - B Farr
- University of Oregon, Eugene, Oregon 97403, USA
| | - W M Farr
- Stony Brook University, Stony Brook, New York 11794, USA
- Center for Computational Astrophysics, Flatiron Institute, New York, New York 10010, USA
| | - N W Farrow
- OzGrav, School of Physics & Astronomy, Monash University, Clayton 3800, Victoria, Australia
| | - E J Fauchon-Jones
- Gravity Exploration Institute, Cardiff University, Cardiff CF24 3AA, United Kingdom
| | - G Favaro
- Università di Padova, Dipartimento di Fisica e Astronomia, I-35131 Padova, Italy
| | - M Favata
- Montclair State University, Montclair, New Jersey 07043, USA
| | - M Fays
- Université de Liège, B-4000 Liège, Belgium
| | - M Fazio
- Colorado State University, Fort Collins, Colorado 80523, USA
| | - J Feicht
- LIGO Laboratory, California Institute of Technology, Pasadena, California 91125, USA
| | - M M Fejer
- Stanford University, Stanford, California 94305, USA
| | - B Fekecs
- University of Szeged, Dóm tér 9, Szeged 6720, Hungary
| | - E Fenyvesi
- Wigner RCP, RMKI, H-1121 Budapest, Konkoly Thege Miklós út 29-33, Hungary
- Institute for Nuclear Research, Hungarian Academy of Sciences, Bem t'er 18/c, H-4026 Debrecen, Hungary
| | - D L Ferguson
- Department of Physics, University of Texas, Austin, Texas 78712, USA
| | - A Fernandez-Galiana
- LIGO Laboratory, Massachusetts Institute of Technology, Cambridge, Massachusetts 02139, USA
| | - I Ferrante
- INFN, Sezione di Pisa, I-56127 Pisa, Italy
- Università di Pisa, I-56127 Pisa, Italy
| | - T A Ferreira
- Instituto Nacional de Pesquisas Espaciais, 12227-010 São José dos Campos, São Paulo, Brazil
| | - F Fidecaro
- INFN, Sezione di Pisa, I-56127 Pisa, Italy
- Università di Pisa, I-56127 Pisa, Italy
| | - P Figura
- Astronomical Observatory Warsaw University, 00-478 Warsaw, Poland
| | - I Fiori
- European Gravitational Observatory (EGO), I-56021 Cascina, Pisa, Italy
| | - M Fishbach
- Center for Interdisciplinary Exploration & Research in Astrophysics (CIERA), Northwestern University, Evanston, Illinois 60208, USA
| | - R P Fisher
- Christopher Newport University, Newport News, Virginia 23606, USA
| | - R Fittipaldi
- INFN, Sezione di Napoli, Gruppo Collegato di Salerno, Complesso Universitario di Monte S. Angelo, I-80126 Napoli, Italy
- CNR-SPIN, c/o Università di Salerno, I-84084 Fisciano, Salerno, Italy
| | - V Fiumara
- INFN, Sezione di Napoli, Gruppo Collegato di Salerno, Complesso Universitario di Monte S. Angelo, I-80126 Napoli, Italy
- Scuola di Ingegneria, Università della Basilicata, I-85100 Potenza, Italy
| | - R Flaminio
- Laboratoire d'Annecy de Physique des Particules (LAPP), Université Grenoble Alpes, Université Savoie Mont Blanc, CNRS/IN2P3, F-74941 Annecy, France
- Gravitational Wave Science Project, National Astronomical Observatory of Japan (NAOJ), Mitaka City, Tokyo 181-8588, Japan
| | - E Floden
- University of Minnesota, Minneapolis, Minnesota 55455, USA
| | - H Fong
- RESCEU, University of Tokyo, Tokyo, 113-0033, Japan
| | - J A Font
- Departamento de Astronomía y Astrofísica, Universitat de València, E-46100 Burjassot, València, Spain
- Observatori Astronòmic, Universitat de València, E-46980 Paterna, València, Spain
| | - B Fornal
- The University of Utah, Salt Lake City, Utah 84112, USA
| | - P W F Forsyth
- OzGrav, Australian National University, Canberra, Australian Capital Territory 0200, Australia
| | - A Franke
- Universität Hamburg, D-22761 Hamburg, Germany
| | - S Frasca
- INFN, Sezione di Roma, I-00185 Roma, Italy
- Università di Roma "La Sapienza," I-00185 Roma, Italy
| | - F Frasconi
- INFN, Sezione di Pisa, I-56127 Pisa, Italy
| | | | - J P Freed
- Embry-Riddle Aeronautical University, Prescott, Arizona 86301, USA
| | - Z Frei
- MTA-ELTE Astrophysics Research Group, Institute of Physics, Eötvös University, Budapest 1117, Hungary
| | - A Freise
- Vrije Universiteit Amsterdam, 1081 HV, Amsterdam, Netherlands
| | - R Frey
- University of Oregon, Eugene, Oregon 97403, USA
| | - P Fritschel
- LIGO Laboratory, Massachusetts Institute of Technology, Cambridge, Massachusetts 02139, USA
| | - V V Frolov
- LIGO Livingston Observatory, Livingston, Louisiana 70754, USA
| | - G G Fronzé
- INFN Sezione di Torino, I-10125 Torino, Italy
| | - P Fulda
- University of Florida, Gainesville, Florida 32611, USA
| | - M Fyffe
- LIGO Livingston Observatory, Livingston, Louisiana 70754, USA
| | - H A Gabbard
- SUPA, University of Glasgow, Glasgow G12 8QQ, United Kingdom
| | - B U Gadre
- Max Planck Institute for Gravitational Physics (Albert Einstein Institute), D-14476 Potsdam, Germany
| | - J R Gair
- Max Planck Institute for Gravitational Physics (Albert Einstein Institute), D-14476 Potsdam, Germany
| | - J Gais
- The Chinese University of Hong Kong, Shatin, NT, Hong Kong
| | - S Galaudage
- OzGrav, School of Physics & Astronomy, Monash University, Clayton 3800, Victoria, Australia
| | - R Gamba
- Theoretisch-Physikalisches Institut, Friedrich-Schiller-Universität Jena, D-07743 Jena, Germany
| | - D Ganapathy
- LIGO Laboratory, Massachusetts Institute of Technology, Cambridge, Massachusetts 02139, USA
| | - A Ganguly
- International Centre for Theoretical Sciences, Tata Institute of Fundamental Research, Bengaluru 560089, India
| | - S G Gaonkar
- Inter-University Centre for Astronomy and Astrophysics, Pune 411007, India
| | - B Garaventa
- INFN, Sezione di Genova, I-16146 Genova, Italy
- Dipartimento di Fisica, Università degli Studi di Genova, I-16146 Genova, Italy
| | - C García-Núñez
- SUPA, University of the West of Scotland, Paisley PA1 2BE, United Kingdom
| | - C García-Quirós
- Universitat de les Illes Balears, IAC3-IEEC, E-07122 Palma de Mallorca, Spain
| | - F Garufi
- INFN, Sezione di Napoli, Complesso Universitario di Monte S. Angelo, I-80126 Napoli, Italy
- Università di Napoli "Federico II", Complesso Universitario di Monte S. Angelo, I-80126 Napoli, Italy
| | - B Gateley
- LIGO Hanford Observatory, Richland, Washington 99352, USA
| | - S Gaudio
- Embry-Riddle Aeronautical University, Prescott, Arizona 86301, USA
| | - V Gayathri
- University of Florida, Gainesville, Florida 32611, USA
| | - G Gemme
- INFN, Sezione di Genova, I-16146 Genova, Italy
| | - A Gennai
- INFN, Sezione di Pisa, I-56127 Pisa, Italy
| | - J George
- RRCAT, Indore, Madhya Pradesh 452013, India
| | | | - L Gergely
- University of Szeged, Dóm tér 9, Szeged 6720, Hungary
| | - P Gewecke
- Universität Hamburg, D-22761 Hamburg, Germany
| | - S Ghonge
- School of Physics, Georgia Institute of Technology, Atlanta, Georgia 30332, USA
| | - Abhirup Ghosh
- Max Planck Institute for Gravitational Physics (Albert Einstein Institute), D-14476 Potsdam, Germany
| | | | - Shaon Ghosh
- University of Wisconsin-Milwaukee, Milwaukee, Wisconsin 53201, USA
- Montclair State University, Montclair, New Jersey 07043, USA
| | - Shrobana Ghosh
- Gravity Exploration Institute, Cardiff University, Cardiff CF24 3AA, United Kingdom
| | - B Giacomazzo
- Università degli Studi di Milano-Bicocca, I-20126 Milano, Italy
- INFN, Sezione di Milano-Bicocca, I-20126 Milano, Italy
- INAF, Osservatorio Astronomico di Brera sede di Merate, I-23807 Merate, Lecco, Italy
| | - L Giacoppo
- INFN, Sezione di Roma, I-00185 Roma, Italy
- Università di Roma "La Sapienza," I-00185 Roma, Italy
| | - J A Giaime
- Louisiana State University, Baton Rouge, Louisiana 70803, USA
- LIGO Livingston Observatory, Livingston, Louisiana 70754, USA
| | - K D Giardina
- LIGO Livingston Observatory, Livingston, Louisiana 70754, USA
| | - D R Gibson
- SUPA, University of the West of Scotland, Paisley PA1 2BE, United Kingdom
| | - C Gier
- SUPA, University of Strathclyde, Glasgow G1 1XQ, United Kingdom
| | - M Giesler
- Cornell University, Ithaca, New York 14850, USA
| | - P Giri
- INFN, Sezione di Pisa, I-56127 Pisa, Italy
- Università di Pisa, I-56127 Pisa, Italy
| | - F Gissi
- Dipartimento di Ingegneria, Università del Sannio, I-82100 Benevento, Italy
| | - J Glanzer
- Louisiana State University, Baton Rouge, Louisiana 70803, USA
| | - A E Gleckl
- California State University Fullerton, Fullerton, California 92831, USA
| | - P Godwin
- The Pennsylvania State University, University Park, Pennsylvania 16802, USA
| | - E Goetz
- University of British Columbia, Vancouver, British Columbia V6T 1Z4, Canada
| | - R Goetz
- University of Florida, Gainesville, Florida 32611, USA
| | - N Gohlke
- Max Planck Institute for Gravitational Physics (Albert Einstein Institute), D-30167 Hannover, Germany
- Leibniz Universität Hannover, D-30167 Hannover, Germany
| | - B Goncharov
- OzGrav, School of Physics & Astronomy, Monash University, Clayton 3800, Victoria, Australia
- Gran Sasso Science Institute (GSSI), I-67100 L'Aquila, Italy
| | - G González
- Louisiana State University, Baton Rouge, Louisiana 70803, USA
| | - A Gopakumar
- Tata Institute of Fundamental Research, Mumbai 400005, India
| | - M Gosselin
- European Gravitational Observatory (EGO), I-56021 Cascina, Pisa, Italy
| | - R Gouaty
- Laboratoire d'Annecy de Physique des Particules (LAPP), Université Grenoble Alpes, Université Savoie Mont Blanc, CNRS/IN2P3, F-74941 Annecy, France
| | - D W Gould
- OzGrav, Australian National University, Canberra, Australian Capital Territory 0200, Australia
| | - B Grace
- OzGrav, Australian National University, Canberra, Australian Capital Territory 0200, Australia
| | - A Grado
- INFN, Sezione di Napoli, Complesso Universitario di Monte S. Angelo, I-80126 Napoli, Italy
- INAF, Osservatorio Astronomico di Capodimonte, I-80131 Napoli, Italy
| | - M Granata
- Université Lyon, Université Claude Bernard Lyon 1, CNRS, Laboratoire des Matériaux Avancés (LMA), IP2I Lyon / IN2P3, UMR 5822, F-69622 Villeurbanne, France
| | - V Granata
- Dipartimento di Fisica "E.R. Caianiello," Università di Salerno, I-84084 Fisciano, Salerno, Italy
| | - A Grant
- SUPA, University of Glasgow, Glasgow G12 8QQ, United Kingdom
| | - S Gras
- LIGO Laboratory, Massachusetts Institute of Technology, Cambridge, Massachusetts 02139, USA
| | - P Grassia
- LIGO Laboratory, California Institute of Technology, Pasadena, California 91125, USA
| | - C Gray
- LIGO Hanford Observatory, Richland, Washington 99352, USA
| | - R Gray
- SUPA, University of Glasgow, Glasgow G12 8QQ, United Kingdom
| | - G Greco
- INFN, Sezione di Perugia, I-06123 Perugia, Italy
| | - A C Green
- University of Florida, Gainesville, Florida 32611, USA
| | - R Green
- Gravity Exploration Institute, Cardiff University, Cardiff CF24 3AA, United Kingdom
| | - A M Gretarsson
- Embry-Riddle Aeronautical University, Prescott, Arizona 86301, USA
| | - E M Gretarsson
- Embry-Riddle Aeronautical University, Prescott, Arizona 86301, USA
| | - D Griffith
- LIGO Laboratory, California Institute of Technology, Pasadena, California 91125, USA
| | - W Griffiths
- Gravity Exploration Institute, Cardiff University, Cardiff CF24 3AA, United Kingdom
| | - H L Griggs
- School of Physics, Georgia Institute of Technology, Atlanta, Georgia 30332, USA
| | - G Grignani
- INFN, Sezione di Perugia, I-06123 Perugia, Italy
- Università di Perugia, I-06123 Perugia, Italy
| | - A Grimaldi
- Università di Trento, Dipartimento di Fisica, I-38123 Povo, Trento, Italy
- INFN, Trento Institute for Fundamental Physics and Applications, I-38123 Povo, Trento, Italy
| | - S J Grimm
- Gran Sasso Science Institute (GSSI), I-67100 L'Aquila, Italy
- INFN, Laboratori Nazionali del Gran Sasso, I-67100 Assergi, Italy
| | - H Grote
- Gravity Exploration Institute, Cardiff University, Cardiff CF24 3AA, United Kingdom
| | - S Grunewald
- Max Planck Institute for Gravitational Physics (Albert Einstein Institute), D-14476 Potsdam, Germany
| | - P Gruning
- Université Paris-Saclay, CNRS/IN2P3, IJCLab, 91405 Orsay, France
| | - D Guerra
- Departamento de Astronomía y Astrofísica, Universitat de València, E-46100 Burjassot, València, Spain
| | - G M Guidi
- Università degli Studi di Urbino "Carlo Bo", I-61029 Urbino, Italy
- INFN, Sezione di Firenze, I-50019 Sesto Fiorentino, Firenze, Italy
| | - A R Guimaraes
- Louisiana State University, Baton Rouge, Louisiana 70803, USA
| | - G Guixé
- Institut de Ciències del Cosmos (ICCUB), Universitat de Barcelona, C/ Martí i Franquès 1, Barcelona, 08028, Spain
| | - H K Gulati
- Institute for Plasma Research, Bhat, Gandhinagar 382428, India
| | - H-K Guo
- The University of Utah, Salt Lake City, Utah 84112, USA
| | - Y Guo
- Nikhef, Science Park 105, 1098 XG Amsterdam, Netherlands
| | - Anchal Gupta
- LIGO Laboratory, California Institute of Technology, Pasadena, California 91125, USA
| | - Anuradha Gupta
- The University of Mississippi, University, Mississippi 38677, USA
| | - P Gupta
- Nikhef, Science Park 105, 1098 XG Amsterdam, Netherlands
- Institute for Gravitational and Subatomic Physics (GRASP), Utrecht University, Princetonplein 1, 3584 CC Utrecht, Netherlands
| | - E K Gustafson
- LIGO Laboratory, California Institute of Technology, Pasadena, California 91125, USA
| | - R Gustafson
- University of Michigan, Ann Arbor, Michigan 48109, USA
| | - F Guzman
- Texas A&M University, College Station, Texas 77843, USA
| | - L Haegel
- Université de Paris, CNRS, Astroparticule et Cosmologie, F-75006 Paris, France
| | - O Halim
- INFN, Sezione di Trieste, I-34127 Trieste, Italy
- Dipartimento di Fisica, Università di Trieste, I-34127 Trieste, Italy
| | - E D Hall
- LIGO Laboratory, Massachusetts Institute of Technology, Cambridge, Massachusetts 02139, USA
| | - E Z Hamilton
- Physik-Institut, University of Zurich, Winterthurerstrasse 190, 8057 Zurich, Switzerland
| | - G Hammond
- SUPA, University of Glasgow, Glasgow G12 8QQ, United Kingdom
| | - M Haney
- Physik-Institut, University of Zurich, Winterthurerstrasse 190, 8057 Zurich, Switzerland
| | - J Hanks
- LIGO Hanford Observatory, Richland, Washington 99352, USA
| | - C Hanna
- The Pennsylvania State University, University Park, Pennsylvania 16802, USA
| | - M D Hannam
- Gravity Exploration Institute, Cardiff University, Cardiff CF24 3AA, United Kingdom
| | - O Hannuksela
- Nikhef, Science Park 105, 1098 XG Amsterdam, Netherlands
- Institute for Gravitational and Subatomic Physics (GRASP), Utrecht University, Princetonplein 1, 3584 CC Utrecht, Netherlands
| | - H Hansen
- LIGO Hanford Observatory, Richland, Washington 99352, USA
| | - T J Hansen
- Embry-Riddle Aeronautical University, Prescott, Arizona 86301, USA
| | - J Hanson
- LIGO Livingston Observatory, Livingston, Louisiana 70754, USA
| | - T Harder
- Artemis, Université Côte d'Azur, Observatoire de la Côte d'Azur, CNRS, F-06304 Nice, France
| | - T Hardwick
- Louisiana State University, Baton Rouge, Louisiana 70803, USA
| | - K Haris
- Nikhef, Science Park 105, 1098 XG Amsterdam, Netherlands
- Institute for Gravitational and Subatomic Physics (GRASP), Utrecht University, Princetonplein 1, 3584 CC Utrecht, Netherlands
| | - J Harms
- Gran Sasso Science Institute (GSSI), I-67100 L'Aquila, Italy
- INFN, Laboratori Nazionali del Gran Sasso, I-67100 Assergi, Italy
| | - G M Harry
- American University, Washington, D.C. 20016, USA
| | - I W Harry
- University of Portsmouth, Portsmouth, PO1 3FX, United Kingdom
| | - D Hartwig
- Universität Hamburg, D-22761 Hamburg, Germany
| | - B Haskell
- Nicolaus Copernicus Astronomical Center, Polish Academy of Sciences, 00-716, Warsaw, Poland
| | - R K Hasskew
- LIGO Livingston Observatory, Livingston, Louisiana 70754, USA
| | - C-J Haster
- LIGO Laboratory, Massachusetts Institute of Technology, Cambridge, Massachusetts 02139, USA
| | - K Haughian
- SUPA, University of Glasgow, Glasgow G12 8QQ, United Kingdom
| | - F J Hayes
- SUPA, University of Glasgow, Glasgow G12 8QQ, United Kingdom
| | - J Healy
- Rochester Institute of Technology, Rochester, New York 14623, USA
| | - A Heidmann
- Laboratoire Kastler Brossel, Sorbonne Université, CNRS, ENS-Université PSL, Collège de France, F-75005 Paris, France
| | - A Heidt
- Max Planck Institute for Gravitational Physics (Albert Einstein Institute), D-30167 Hannover, Germany
- Leibniz Universität Hannover, D-30167 Hannover, Germany
| | - M C Heintze
- LIGO Livingston Observatory, Livingston, Louisiana 70754, USA
| | - J Heinze
- Max Planck Institute for Gravitational Physics (Albert Einstein Institute), D-30167 Hannover, Germany
- Leibniz Universität Hannover, D-30167 Hannover, Germany
| | - J Heinzel
- Carleton College, Northfield, Minnesota 55057, USA
| | - H Heitmann
- Artemis, Université Côte d'Azur, Observatoire de la Côte d'Azur, CNRS, F-06304 Nice, France
| | - F Hellman
- University of California, Berkeley, California 94720, USA
| | - P Hello
- Université Paris-Saclay, CNRS/IN2P3, IJCLab, 91405 Orsay, France
| | | | - G Hemming
- European Gravitational Observatory (EGO), I-56021 Cascina, Pisa, Italy
| | - M Hendry
- SUPA, University of Glasgow, Glasgow G12 8QQ, United Kingdom
| | - I S Heng
- SUPA, University of Glasgow, Glasgow G12 8QQ, United Kingdom
| | - E Hennes
- Nikhef, Science Park 105, 1098 XG Amsterdam, Netherlands
| | - J Hennig
- Maastricht University, 6200 MD, Maastricht, Netherlands
| | - M H Hennig
- Maastricht University, 6200 MD, Maastricht, Netherlands
| | - A G Hernandez
- California State University, Los Angeles, 5151 State University Dr, Los Angeles, California 90032, USA
| | - F Hernandez Vivanco
- OzGrav, School of Physics & Astronomy, Monash University, Clayton 3800, Victoria, Australia
| | - M Heurs
- Max Planck Institute for Gravitational Physics (Albert Einstein Institute), D-30167 Hannover, Germany
- Leibniz Universität Hannover, D-30167 Hannover, Germany
| | - S Hild
- Nikhef, Science Park 105, 1098 XG Amsterdam, Netherlands
- Maastricht University, P.O. Box 616, 6200 MD Maastricht, Netherlands
| | - P Hill
- SUPA, University of Strathclyde, Glasgow G1 1XQ, United Kingdom
| | - A S Hines
- Texas A&M University, College Station, Texas 77843, USA
| | - S Hochheim
- Max Planck Institute for Gravitational Physics (Albert Einstein Institute), D-30167 Hannover, Germany
- Leibniz Universität Hannover, D-30167 Hannover, Germany
| | - D Hofman
- Université Lyon, Université Claude Bernard Lyon 1, CNRS, Laboratoire des Matériaux Avancés (LMA), IP2I Lyon / IN2P3, UMR 5822, F-69622 Villeurbanne, France
| | - J N Hohmann
- Universität Hamburg, D-22761 Hamburg, Germany
| | - D G Holcomb
- Villanova University, 800 Lancaster Avenue, Villanova, Pennsylvania 19085, USA
| | - N A Holland
- OzGrav, Australian National University, Canberra, Australian Capital Territory 0200, Australia
| | - I J Hollows
- The University of Sheffield, Sheffield S10 2TN, United Kingdom
| | - Z J Holmes
- OzGrav, University of Adelaide, Adelaide, South Australia 5005, Australia
| | - K Holt
- LIGO Livingston Observatory, Livingston, Louisiana 70754, USA
| | - D E Holz
- University of Chicago, Chicago, Illinois 60637, USA
| | - P Hopkins
- Gravity Exploration Institute, Cardiff University, Cardiff CF24 3AA, United Kingdom
| | - J Hough
- SUPA, University of Glasgow, Glasgow G12 8QQ, United Kingdom
| | - S Hourihane
- CaRT, California Institute of Technology, Pasadena, California 91125, USA
| | - E J Howell
- OzGrav, University of Western Australia, Crawley, Western Australia 6009, Australia
| | - C G Hoy
- Gravity Exploration Institute, Cardiff University, Cardiff CF24 3AA, United Kingdom
| | - D Hoyland
- University of Birmingham, Birmingham B15 2TT, United Kingdom
| | - A Hreibi
- Max Planck Institute for Gravitational Physics (Albert Einstein Institute), D-30167 Hannover, Germany
- Leibniz Universität Hannover, D-30167 Hannover, Germany
| | - Y Hsu
- National Tsing Hua University, Hsinchu City, 30013 Taiwan, Republic of China
| | - Y Huang
- LIGO Laboratory, Massachusetts Institute of Technology, Cambridge, Massachusetts 02139, USA
| | - M T Hübner
- OzGrav, School of Physics & Astronomy, Monash University, Clayton 3800, Victoria, Australia
| | - A D Huddart
- Rutherford Appleton Laboratory, Didcot OX11 0DE, United Kingdom
| | - B Hughey
- Embry-Riddle Aeronautical University, Prescott, Arizona 86301, USA
| | - V Hui
- Laboratoire d'Annecy de Physique des Particules (LAPP), Université Grenoble Alpes, Université Savoie Mont Blanc, CNRS/IN2P3, F-74941 Annecy, France
| | - S Husa
- Universitat de les Illes Balears, IAC3-IEEC, E-07122 Palma de Mallorca, Spain
| | - S H Huttner
- SUPA, University of Glasgow, Glasgow G12 8QQ, United Kingdom
| | - R Huxford
- The Pennsylvania State University, University Park, Pennsylvania 16802, USA
| | - T Huynh-Dinh
- LIGO Livingston Observatory, Livingston, Louisiana 70754, USA
| | - B Idzkowski
- Astronomical Observatory Warsaw University, 00-478 Warsaw, Poland
| | - A Iess
- Università di Roma Tor Vergata, I-00133 Roma, Italy
- INFN, Sezione di Roma Tor Vergata, I-00133 Roma, Italy
| | - C Ingram
- OzGrav, University of Adelaide, Adelaide, South Australia 5005, Australia
| | - M Isi
- LIGO Laboratory, Massachusetts Institute of Technology, Cambridge, Massachusetts 02139, USA
| | - K Isleif
- Universität Hamburg, D-22761 Hamburg, Germany
| | - B R Iyer
- International Centre for Theoretical Sciences, Tata Institute of Fundamental Research, Bengaluru 560089, India
| | - V JaberianHamedan
- OzGrav, University of Western Australia, Crawley, Western Australia 6009, Australia
| | - T Jacqmin
- Laboratoire Kastler Brossel, Sorbonne Université, CNRS, ENS-Université PSL, Collège de France, F-75005 Paris, France
| | - S J Jadhav
- Directorate of Construction, Services & Estate Management, Mumbai 400094, India
| | - S P Jadhav
- Inter-University Centre for Astronomy and Astrophysics, Pune 411007, India
| | - A L James
- Gravity Exploration Institute, Cardiff University, Cardiff CF24 3AA, United Kingdom
| | - A Z Jan
- Rochester Institute of Technology, Rochester, New York 14623, USA
| | - K Jani
- Vanderbilt University, Nashville, Tennessee 37235, USA
| | - J Janquart
- Nikhef, Science Park 105, 1098 XG Amsterdam, Netherlands
- Institute for Gravitational and Subatomic Physics (GRASP), Utrecht University, Princetonplein 1, 3584 CC Utrecht, Netherlands
| | - K Janssens
- Artemis, Université Côte d'Azur, Observatoire de la Côte d'Azur, CNRS, F-06304 Nice, France
- Universiteit Antwerpen, Prinsstraat 13, 2000 Antwerpen, Belgium
| | - N N Janthalur
- Directorate of Construction, Services & Estate Management, Mumbai 400094, India
| | - P Jaranowski
- University of Białystok, 15-424 Białystok, Poland
| | - D Jariwala
- University of Florida, Gainesville, Florida 32611, USA
| | - R Jaume
- Universitat de les Illes Balears, IAC3-IEEC, E-07122 Palma de Mallorca, Spain
| | - A C Jenkins
- King's College London, University of London, London WC2R 2LS, United Kingdom
| | - K Jenner
- OzGrav, University of Adelaide, Adelaide, South Australia 5005, Australia
| | - M Jeunon
- University of Minnesota, Minneapolis, Minnesota 55455, USA
| | - W Jia
- LIGO Laboratory, Massachusetts Institute of Technology, Cambridge, Massachusetts 02139, USA
| | - G R Johns
- Christopher Newport University, Newport News, Virginia 23606, USA
| | - A W Jones
- OzGrav, University of Western Australia, Crawley, Western Australia 6009, Australia
| | - D I Jones
- University of Southampton, Southampton SO17 1BJ, United Kingdom
| | - J D Jones
- LIGO Hanford Observatory, Richland, Washington 99352, USA
| | - P Jones
- University of Birmingham, Birmingham B15 2TT, United Kingdom
| | - R Jones
- SUPA, University of Glasgow, Glasgow G12 8QQ, United Kingdom
| | - R J G Jonker
- Nikhef, Science Park 105, 1098 XG Amsterdam, Netherlands
| | - L Ju
- OzGrav, University of Western Australia, Crawley, Western Australia 6009, Australia
| | - J Junker
- Max Planck Institute for Gravitational Physics (Albert Einstein Institute), D-30167 Hannover, Germany
- Leibniz Universität Hannover, D-30167 Hannover, Germany
| | - V Juste
- Université de Strasbourg, CNRS, IPHC UMR 7178, F-67000 Strasbourg, France
| | - C V Kalaghatgi
- Gravity Exploration Institute, Cardiff University, Cardiff CF24 3AA, United Kingdom
- Institute for Gravitational and Subatomic Physics (GRASP), Utrecht University, Princetonplein 1, 3584 CC Utrecht, Netherlands
| | - V Kalogera
- Center for Interdisciplinary Exploration & Research in Astrophysics (CIERA), Northwestern University, Evanston, Illinois 60208, USA
| | - B Kamai
- LIGO Laboratory, California Institute of Technology, Pasadena, California 91125, USA
| | - S Kandhasamy
- Inter-University Centre for Astronomy and Astrophysics, Pune 411007, India
| | - G Kang
- Chung-Ang University, Seoul 06974, Republic of Korea
| | - J B Kanner
- LIGO Laboratory, California Institute of Technology, Pasadena, California 91125, USA
| | - Y Kao
- National Tsing Hua University, Hsinchu City, 30013 Taiwan, Republic of China
| | - S J Kapadia
- International Centre for Theoretical Sciences, Tata Institute of Fundamental Research, Bengaluru 560089, India
| | - D P Kapasi
- OzGrav, Australian National University, Canberra, Australian Capital Territory 0200, Australia
| | - S Karat
- LIGO Laboratory, California Institute of Technology, Pasadena, California 91125, USA
| | - C Karathanasis
- Institut de Física d'Altes Energies (IFAE), Barcelona Institute of Science and Technology, and ICREA, E-08193 Barcelona, Spain
| | - S Karki
- Missouri University of Science and Technology, Rolla, Missouri 65409, USA
| | - R Kashyap
- The Pennsylvania State University, University Park, Pennsylvania 16802, USA
| | - M Kasprzack
- LIGO Laboratory, California Institute of Technology, Pasadena, California 91125, USA
| | - W Kastaun
- Max Planck Institute for Gravitational Physics (Albert Einstein Institute), D-30167 Hannover, Germany
- Leibniz Universität Hannover, D-30167 Hannover, Germany
| | - S Katsanevas
- European Gravitational Observatory (EGO), I-56021 Cascina, Pisa, Italy
| | - E Katsavounidis
- LIGO Laboratory, Massachusetts Institute of Technology, Cambridge, Massachusetts 02139, USA
| | - W Katzman
- LIGO Livingston Observatory, Livingston, Louisiana 70754, USA
| | - T Kaur
- OzGrav, University of Western Australia, Crawley, Western Australia 6009, Australia
| | - K Kawabe
- LIGO Hanford Observatory, Richland, Washington 99352, USA
| | - F Kéfélian
- Artemis, Université Côte d'Azur, Observatoire de la Côte d'Azur, CNRS, F-06304 Nice, France
| | - D Keitel
- Universitat de les Illes Balears, IAC3-IEEC, E-07122 Palma de Mallorca, Spain
| | - J S Key
- University of Washington Bothell, Bothell, Washington 98011, USA
| | - S Khadka
- Stanford University, Stanford, California 94305, USA
| | - F Y Khalili
- Faculty of Physics, Lomonosov Moscow State University, Moscow 119991, Russia
| | - S Khan
- Gravity Exploration Institute, Cardiff University, Cardiff CF24 3AA, United Kingdom
| | - E A Khazanov
- Institute of Applied Physics, Nizhny Novgorod, 603950, Russia
| | - N Khetan
- Gran Sasso Science Institute (GSSI), I-67100 L'Aquila, Italy
- INFN, Laboratori Nazionali del Gran Sasso, I-67100 Assergi, Italy
| | | | - N Kijbunchoo
- OzGrav, Australian National University, Canberra, Australian Capital Territory 0200, Australia
| | - C Kim
- Ewha Womans University, Seoul 03760, Republic of Korea
| | - J C Kim
- Inje University Gimhae, South Gyeongsang 50834, Republic of Korea
| | - K Kim
- Korea Astronomy and Space Science Institute, Daejeon 34055, Republic of Korea
| | - W S Kim
- National Institute for Mathematical Sciences, Daejeon 34047, Republic of Korea
| | - Y-M Kim
- Ulsan National Institute of Science and Technology, Ulsan 44919, Republic of Korea
| | - C Kimball
- Center for Interdisciplinary Exploration & Research in Astrophysics (CIERA), Northwestern University, Evanston, Illinois 60208, USA
| | - M Kinley-Hanlon
- SUPA, University of Glasgow, Glasgow G12 8QQ, United Kingdom
| | - R Kirchhoff
- Max Planck Institute for Gravitational Physics (Albert Einstein Institute), D-30167 Hannover, Germany
- Leibniz Universität Hannover, D-30167 Hannover, Germany
| | - J S Kissel
- LIGO Hanford Observatory, Richland, Washington 99352, USA
| | - L Kleybolte
- Universität Hamburg, D-22761 Hamburg, Germany
| | - S Klimenko
- University of Florida, Gainesville, Florida 32611, USA
| | - A M Knee
- University of British Columbia, Vancouver, British Columbia V6T 1Z4, Canada
| | - T D Knowles
- West Virginia University, Morgantown, West Virginia 26506, USA
| | - E Knyazev
- LIGO Laboratory, Massachusetts Institute of Technology, Cambridge, Massachusetts 02139, USA
| | - P Koch
- Max Planck Institute for Gravitational Physics (Albert Einstein Institute), D-30167 Hannover, Germany
- Leibniz Universität Hannover, D-30167 Hannover, Germany
| | - G Koekoek
- Nikhef, Science Park 105, 1098 XG Amsterdam, Netherlands
- Maastricht University, P.O. Box 616, 6200 MD Maastricht, Netherlands
| | - S Koley
- Gran Sasso Science Institute (GSSI), I-67100 L'Aquila, Italy
| | - P Kolitsidou
- Gravity Exploration Institute, Cardiff University, Cardiff CF24 3AA, United Kingdom
| | - M Kolstein
- Institut de Física d'Altes Energies (IFAE), Barcelona Institute of Science and Technology, and ICREA, E-08193 Barcelona, Spain
| | - K Komori
- LIGO Laboratory, Massachusetts Institute of Technology, Cambridge, Massachusetts 02139, USA
| | - V Kondrashov
- LIGO Laboratory, California Institute of Technology, Pasadena, California 91125, USA
| | - A Kontos
- Bard College, 30 Campus Road, Annandale-On-Hudson, New York 12504, USA
| | - N Koper
- Max Planck Institute for Gravitational Physics (Albert Einstein Institute), D-30167 Hannover, Germany
- Leibniz Universität Hannover, D-30167 Hannover, Germany
| | - M Korobko
- Universität Hamburg, D-22761 Hamburg, Germany
| | - M Kovalam
- OzGrav, University of Western Australia, Crawley, Western Australia 6009, Australia
| | - D B Kozak
- LIGO Laboratory, California Institute of Technology, Pasadena, California 91125, USA
| | - V Kringel
- Max Planck Institute for Gravitational Physics (Albert Einstein Institute), D-30167 Hannover, Germany
- Leibniz Universität Hannover, D-30167 Hannover, Germany
| | - N V Krishnendu
- Max Planck Institute for Gravitational Physics (Albert Einstein Institute), D-30167 Hannover, Germany
- Leibniz Universität Hannover, D-30167 Hannover, Germany
| | - A Królak
- Institute of Mathematics, Polish Academy of Sciences, 00656 Warsaw, Poland
- National Center for Nuclear Research, 05-400 Świerk-Otwock, Poland
| | - G Kuehn
- Max Planck Institute for Gravitational Physics (Albert Einstein Institute), D-30167 Hannover, Germany
- Leibniz Universität Hannover, D-30167 Hannover, Germany
| | - F Kuei
- National Tsing Hua University, Hsinchu City, 30013 Taiwan, Republic of China
| | - P Kuijer
- Nikhef, Science Park 105, 1098 XG Amsterdam, Netherlands
| | - A Kumar
- Directorate of Construction, Services & Estate Management, Mumbai 400094, India
| | - P Kumar
- Cornell University, Ithaca, New York 14850, USA
| | - Rahul Kumar
- LIGO Hanford Observatory, Richland, Washington 99352, USA
| | - Rakesh Kumar
- Institute for Plasma Research, Bhat, Gandhinagar 382428, India
| | - K Kuns
- LIGO Laboratory, Massachusetts Institute of Technology, Cambridge, Massachusetts 02139, USA
| | - S Kuwahara
- RESCEU, University of Tokyo, Tokyo, 113-0033, Japan
| | - P Lagabbe
- Laboratoire d'Annecy de Physique des Particules (LAPP), Université Grenoble Alpes, Université Savoie Mont Blanc, CNRS/IN2P3, F-74941 Annecy, France
| | - D Laghi
- INFN, Sezione di Pisa, I-56127 Pisa, Italy
- Università di Pisa, I-56127 Pisa, Italy
| | - E Lalande
- Université de Montréal/Polytechnique, Montreal, Quebec H3T 1J4, Canada
| | - T L Lam
- The Chinese University of Hong Kong, Shatin, NT, Hong Kong
| | - A Lamberts
- Artemis, Université Côte d'Azur, Observatoire de la Côte d'Azur, CNRS, F-06304 Nice, France
- Laboratoire Lagrange, Université Côte d'Azur, Observatoire Côte d'Azur, CNRS, F-06304 Nice, France
| | - M Landry
- LIGO Hanford Observatory, Richland, Washington 99352, USA
| | - B B Lane
- LIGO Laboratory, Massachusetts Institute of Technology, Cambridge, Massachusetts 02139, USA
| | - R N Lang
- LIGO Laboratory, Massachusetts Institute of Technology, Cambridge, Massachusetts 02139, USA
| | - J Lange
- Department of Physics, University of Texas, Austin, Texas 78712, USA
| | - B Lantz
- Stanford University, Stanford, California 94305, USA
| | - I La Rosa
- Laboratoire d'Annecy de Physique des Particules (LAPP), Université Grenoble Alpes, Université Savoie Mont Blanc, CNRS/IN2P3, F-74941 Annecy, France
| | | | - P D Lasky
- OzGrav, School of Physics & Astronomy, Monash University, Clayton 3800, Victoria, Australia
| | - M Laxen
- LIGO Livingston Observatory, Livingston, Louisiana 70754, USA
| | - A Lazzarini
- LIGO Laboratory, California Institute of Technology, Pasadena, California 91125, USA
| | - C Lazzaro
- Università di Padova, Dipartimento di Fisica e Astronomia, I-35131 Padova, Italy
- INFN, Sezione di Padova, I-35131 Padova, Italy
| | - P Leaci
- INFN, Sezione di Roma, I-00185 Roma, Italy
- Università di Roma "La Sapienza," I-00185 Roma, Italy
| | - S Leavey
- Max Planck Institute for Gravitational Physics (Albert Einstein Institute), D-30167 Hannover, Germany
- Leibniz Universität Hannover, D-30167 Hannover, Germany
| | - Y K Lecoeuche
- University of British Columbia, Vancouver, British Columbia V6T 1Z4, Canada
| | - H M Lee
- Seoul National University, Seoul 08826, Republic of Korea
| | - H W Lee
- Inje University Gimhae, South Gyeongsang 50834, Republic of Korea
| | - J Lee
- Seoul National University, Seoul 08826, Republic of Korea
| | - K Lee
- Sungkyunkwan University, Seoul 03063, Republic of Korea
| | - J Lehmann
- Max Planck Institute for Gravitational Physics (Albert Einstein Institute), D-30167 Hannover, Germany
- Leibniz Universität Hannover, D-30167 Hannover, Germany
| | - A Lemaître
- NAVIER, École des Ponts, Université Gustave Eiffel, CNRS, Marne-la-Vallée, France
| | - N Leroy
- Université Paris-Saclay, CNRS/IN2P3, IJCLab, 91405 Orsay, France
| | - N Letendre
- Laboratoire d'Annecy de Physique des Particules (LAPP), Université Grenoble Alpes, Université Savoie Mont Blanc, CNRS/IN2P3, F-74941 Annecy, France
| | - C Levesque
- Université de Montréal/Polytechnique, Montreal, Quebec H3T 1J4, Canada
| | - Y Levin
- OzGrav, School of Physics & Astronomy, Monash University, Clayton 3800, Victoria, Australia
| | - J N Leviton
- University of Michigan, Ann Arbor, Michigan 48109, USA
| | - K Leyde
- Université de Paris, CNRS, Astroparticule et Cosmologie, F-75006 Paris, France
| | - A K Y Li
- LIGO Laboratory, California Institute of Technology, Pasadena, California 91125, USA
| | - B Li
- National Tsing Hua University, Hsinchu City, 30013 Taiwan, Republic of China
| | - J Li
- Center for Interdisciplinary Exploration & Research in Astrophysics (CIERA), Northwestern University, Evanston, Illinois 60208, USA
| | - T G F Li
- The Chinese University of Hong Kong, Shatin, NT, Hong Kong
| | - X Li
- CaRT, California Institute of Technology, Pasadena, California 91125, USA
| | - F Linde
- Nikhef, Science Park 105, 1098 XG Amsterdam, Netherlands
- Institute for High-Energy Physics, University of Amsterdam, Science Park 904, 1098 XH Amsterdam, Netherlands
| | - S D Linker
- California State University, Los Angeles, 5151 State University Dr, Los Angeles, California 90032, USA
| | - J N Linley
- SUPA, University of Glasgow, Glasgow G12 8QQ, United Kingdom
| | - T B Littenberg
- NASA Marshall Space Flight Center, Huntsville, Alabama 35811, USA
| | - J Liu
- Max Planck Institute for Gravitational Physics (Albert Einstein Institute), D-30167 Hannover, Germany
- Leibniz Universität Hannover, D-30167 Hannover, Germany
| | - K Liu
- National Tsing Hua University, Hsinchu City, 30013 Taiwan, Republic of China
| | - X Liu
- University of Wisconsin-Milwaukee, Milwaukee, Wisconsin 53201, USA
| | - F Llamas
- The University of Texas Rio Grande Valley, Brownsville, Texas 78520, USA
| | - M Llorens-Monteagudo
- Departamento de Astronomía y Astrofísica, Universitat de València, E-46100 Burjassot, València, Spain
| | - R K L Lo
- LIGO Laboratory, California Institute of Technology, Pasadena, California 91125, USA
| | - A Lockwood
- University of Washington, Seattle, Washington 98195, USA
| | - L T London
- LIGO Laboratory, Massachusetts Institute of Technology, Cambridge, Massachusetts 02139, USA
| | - A Longo
- Dipartimento di Matematica e Fisica, Università degli Studi Roma Tre, I-00146 Roma, Italy
- INFN, Sezione di Roma Tre, I-00146 Roma, Italy
| | - D Lopez
- Physik-Institut, University of Zurich, Winterthurerstrasse 190, 8057 Zurich, Switzerland
| | - M Lopez Portilla
- Institute for Gravitational and Subatomic Physics (GRASP), Utrecht University, Princetonplein 1, 3584 CC Utrecht, Netherlands
| | - M Lorenzini
- Università di Roma Tor Vergata, I-00133 Roma, Italy
- INFN, Sezione di Roma Tor Vergata, I-00133 Roma, Italy
| | | | - M Lormand
- LIGO Livingston Observatory, Livingston, Louisiana 70754, USA
| | - G Losurdo
- INFN, Sezione di Pisa, I-56127 Pisa, Italy
| | - T P Lott
- School of Physics, Georgia Institute of Technology, Atlanta, Georgia 30332, USA
| | - J D Lough
- Max Planck Institute for Gravitational Physics (Albert Einstein Institute), D-30167 Hannover, Germany
- Leibniz Universität Hannover, D-30167 Hannover, Germany
| | - C O Lousto
- Rochester Institute of Technology, Rochester, New York 14623, USA
| | - G Lovelace
- California State University Fullerton, Fullerton, California 92831, USA
| | | | - H Lück
- Max Planck Institute for Gravitational Physics (Albert Einstein Institute), D-30167 Hannover, Germany
- Leibniz Universität Hannover, D-30167 Hannover, Germany
| | - D Lumaca
- Università di Roma Tor Vergata, I-00133 Roma, Italy
- INFN, Sezione di Roma Tor Vergata, I-00133 Roma, Italy
| | - A P Lundgren
- University of Portsmouth, Portsmouth, PO1 3FX, United Kingdom
| | - J E Lynam
- Christopher Newport University, Newport News, Virginia 23606, USA
| | - R Macas
- University of Portsmouth, Portsmouth, PO1 3FX, United Kingdom
| | - M MacInnis
- LIGO Laboratory, Massachusetts Institute of Technology, Cambridge, Massachusetts 02139, USA
| | - D M Macleod
- Gravity Exploration Institute, Cardiff University, Cardiff CF24 3AA, United Kingdom
| | - I A O MacMillan
- LIGO Laboratory, California Institute of Technology, Pasadena, California 91125, USA
| | - A Macquet
- Artemis, Université Côte d'Azur, Observatoire de la Côte d'Azur, CNRS, F-06304 Nice, France
| | | | - C Magazzù
- INFN, Sezione di Pisa, I-56127 Pisa, Italy
| | - R M Magee
- LIGO Laboratory, California Institute of Technology, Pasadena, California 91125, USA
| | - R Maggiore
- University of Birmingham, Birmingham B15 2TT, United Kingdom
| | - M Magnozzi
- INFN, Sezione di Genova, I-16146 Genova, Italy
- Dipartimento di Fisica, Università degli Studi di Genova, I-16146 Genova, Italy
| | - S Mahesh
- West Virginia University, Morgantown, West Virginia 26506, USA
| | - E Majorana
- INFN, Sezione di Roma, I-00185 Roma, Italy
- Università di Roma "La Sapienza," I-00185 Roma, Italy
| | - C Makarem
- LIGO Laboratory, California Institute of Technology, Pasadena, California 91125, USA
| | | | - S Maliakal
- LIGO Laboratory, California Institute of Technology, Pasadena, California 91125, USA
| | - A Malik
- RRCAT, Indore, Madhya Pradesh 452013, India
| | - N Man
- Artemis, Université Côte d'Azur, Observatoire de la Côte d'Azur, CNRS, F-06304 Nice, France
| | - V Mandic
- University of Minnesota, Minneapolis, Minnesota 55455, USA
| | - V Mangano
- INFN, Sezione di Roma, I-00185 Roma, Italy
- Università di Roma "La Sapienza," I-00185 Roma, Italy
| | - J L Mango
- Concordia University Wisconsin, Mequon, Wisconsin 53097, USA
| | - G L Mansell
- LIGO Hanford Observatory, Richland, Washington 99352, USA
- LIGO Laboratory, Massachusetts Institute of Technology, Cambridge, Massachusetts 02139, USA
| | - M Manske
- University of Wisconsin-Milwaukee, Milwaukee, Wisconsin 53201, USA
| | - M Mantovani
- European Gravitational Observatory (EGO), I-56021 Cascina, Pisa, Italy
| | - M Mapelli
- Università di Padova, Dipartimento di Fisica e Astronomia, I-35131 Padova, Italy
- INFN, Sezione di Padova, I-35131 Padova, Italy
| | - F Marchesoni
- INFN, Sezione di Perugia, I-06123 Perugia, Italy
- Università di Camerino, Dipartimento di Fisica, I-62032 Camerino, Italy
- School of Physics Science and Engineering, Tongji University, Shanghai 200092, China
| | - F Marion
- Laboratoire d'Annecy de Physique des Particules (LAPP), Université Grenoble Alpes, Université Savoie Mont Blanc, CNRS/IN2P3, F-74941 Annecy, France
| | - Z Mark
- CaRT, California Institute of Technology, Pasadena, California 91125, USA
| | - S Márka
- Columbia University, New York, New York 10027, USA
| | - Z Márka
- Columbia University, New York, New York 10027, USA
| | - C Markakis
- University of Cambridge, Cambridge CB2 1TN, United Kingdom
| | - A S Markosyan
- Stanford University, Stanford, California 94305, USA
| | - A Markowitz
- LIGO Laboratory, California Institute of Technology, Pasadena, California 91125, USA
| | - E Maros
- LIGO Laboratory, California Institute of Technology, Pasadena, California 91125, USA
| | - A Marquina
- Departamento de Matemáticas, Universitat de València, E-46100 Burjassot, València, Spain
| | - S Marsat
- Université de Paris, CNRS, Astroparticule et Cosmologie, F-75006 Paris, France
| | - F Martelli
- Università degli Studi di Urbino "Carlo Bo", I-61029 Urbino, Italy
- INFN, Sezione di Firenze, I-50019 Sesto Fiorentino, Firenze, Italy
| | - I W Martin
- SUPA, University of Glasgow, Glasgow G12 8QQ, United Kingdom
| | - R M Martin
- Montclair State University, Montclair, New Jersey 07043, USA
| | - M Martinez
- Institut de Física d'Altes Energies (IFAE), Barcelona Institute of Science and Technology, and ICREA, E-08193 Barcelona, Spain
| | - V A Martinez
- University of Florida, Gainesville, Florida 32611, USA
| | - V Martinez
- Université de Lyon, Université Claude Bernard Lyon 1, CNRS, Institut Lumière Matière, F-69622 Villeurbanne, France
| | - K Martinovic
- King's College London, University of London, London WC2R 2LS, United Kingdom
| | - D V Martynov
- University of Birmingham, Birmingham B15 2TT, United Kingdom
| | - E J Marx
- LIGO Laboratory, Massachusetts Institute of Technology, Cambridge, Massachusetts 02139, USA
| | | | - K Mason
- LIGO Laboratory, Massachusetts Institute of Technology, Cambridge, Massachusetts 02139, USA
| | - E Massera
- The University of Sheffield, Sheffield S10 2TN, United Kingdom
| | - A Masserot
- Laboratoire d'Annecy de Physique des Particules (LAPP), Université Grenoble Alpes, Université Savoie Mont Blanc, CNRS/IN2P3, F-74941 Annecy, France
| | - T J Massinger
- LIGO Laboratory, Massachusetts Institute of Technology, Cambridge, Massachusetts 02139, USA
| | - M Masso-Reid
- SUPA, University of Glasgow, Glasgow G12 8QQ, United Kingdom
| | - S Mastrogiovanni
- Université de Paris, CNRS, Astroparticule et Cosmologie, F-75006 Paris, France
| | - A Matas
- Max Planck Institute for Gravitational Physics (Albert Einstein Institute), D-14476 Potsdam, Germany
| | - M Mateu-Lucena
- Universitat de les Illes Balears, IAC3-IEEC, E-07122 Palma de Mallorca, Spain
| | - F Matichard
- LIGO Laboratory, California Institute of Technology, Pasadena, California 91125, USA
- LIGO Laboratory, Massachusetts Institute of Technology, Cambridge, Massachusetts 02139, USA
| | - M Matiushechkina
- Max Planck Institute for Gravitational Physics (Albert Einstein Institute), D-30167 Hannover, Germany
- Leibniz Universität Hannover, D-30167 Hannover, Germany
| | - N Mavalvala
- LIGO Laboratory, Massachusetts Institute of Technology, Cambridge, Massachusetts 02139, USA
| | - J J McCann
- OzGrav, University of Western Australia, Crawley, Western Australia 6009, Australia
| | - R McCarthy
- LIGO Hanford Observatory, Richland, Washington 99352, USA
| | - D E McClelland
- OzGrav, Australian National University, Canberra, Australian Capital Territory 0200, Australia
| | - P K McClincy
- The Pennsylvania State University, University Park, Pennsylvania 16802, USA
| | - S McCormick
- LIGO Livingston Observatory, Livingston, Louisiana 70754, USA
| | - L McCuller
- LIGO Laboratory, Massachusetts Institute of Technology, Cambridge, Massachusetts 02139, USA
| | - G I McGhee
- SUPA, University of Glasgow, Glasgow G12 8QQ, United Kingdom
| | - S C McGuire
- Southern University and A&M College, Baton Rouge, Louisiana 70813, USA
| | - C McIsaac
- University of Portsmouth, Portsmouth, PO1 3FX, United Kingdom
| | - J McIver
- University of British Columbia, Vancouver, British Columbia V6T 1Z4, Canada
| | - T McRae
- OzGrav, Australian National University, Canberra, Australian Capital Territory 0200, Australia
| | - S T McWilliams
- West Virginia University, Morgantown, West Virginia 26506, USA
| | - D Meacher
- University of Wisconsin-Milwaukee, Milwaukee, Wisconsin 53201, USA
| | - M Mehmet
- Max Planck Institute for Gravitational Physics (Albert Einstein Institute), D-30167 Hannover, Germany
- Leibniz Universität Hannover, D-30167 Hannover, Germany
| | - A K Mehta
- Max Planck Institute for Gravitational Physics (Albert Einstein Institute), D-14476 Potsdam, Germany
| | - Q Meijer
- Institute for Gravitational and Subatomic Physics (GRASP), Utrecht University, Princetonplein 1, 3584 CC Utrecht, Netherlands
| | - A Melatos
- OzGrav, University of Melbourne, Parkville, Victoria 3010, Australia
| | - D A Melchor
- California State University Fullerton, Fullerton, California 92831, USA
| | - G Mendell
- LIGO Hanford Observatory, Richland, Washington 99352, USA
| | - A Menendez-Vazquez
- Institut de Física d'Altes Energies (IFAE), Barcelona Institute of Science and Technology, and ICREA, E-08193 Barcelona, Spain
| | - C S Menoni
- Colorado State University, Fort Collins, Colorado 80523, USA
| | - R A Mercer
- University of Wisconsin-Milwaukee, Milwaukee, Wisconsin 53201, USA
| | - L Mereni
- Université Lyon, Université Claude Bernard Lyon 1, CNRS, Laboratoire des Matériaux Avancés (LMA), IP2I Lyon / IN2P3, UMR 5822, F-69622 Villeurbanne, France
| | - K Merfeld
- University of Oregon, Eugene, Oregon 97403, USA
| | - E L Merilh
- LIGO Livingston Observatory, Livingston, Louisiana 70754, USA
| | - J D Merritt
- University of Oregon, Eugene, Oregon 97403, USA
| | - M Merzougui
- Artemis, Université Côte d'Azur, Observatoire de la Côte d'Azur, CNRS, F-06304 Nice, France
| | - S Meshkov
- LIGO Laboratory, California Institute of Technology, Pasadena, California 91125, USA
| | - C Messenger
- SUPA, University of Glasgow, Glasgow G12 8QQ, United Kingdom
| | - C Messick
- Department of Physics, University of Texas, Austin, Texas 78712, USA
| | - P M Meyers
- OzGrav, University of Melbourne, Parkville, Victoria 3010, Australia
| | - F Meylahn
- Max Planck Institute for Gravitational Physics (Albert Einstein Institute), D-30167 Hannover, Germany
- Leibniz Universität Hannover, D-30167 Hannover, Germany
| | - A Mhaske
- Inter-University Centre for Astronomy and Astrophysics, Pune 411007, India
| | - A Miani
- Università di Trento, Dipartimento di Fisica, I-38123 Povo, Trento, Italy
- INFN, Trento Institute for Fundamental Physics and Applications, I-38123 Povo, Trento, Italy
| | - H Miao
- University of Birmingham, Birmingham B15 2TT, United Kingdom
| | | | - C Michel
- Université Lyon, Université Claude Bernard Lyon 1, CNRS, Laboratoire des Matériaux Avancés (LMA), IP2I Lyon / IN2P3, UMR 5822, F-69622 Villeurbanne, France
| | - H Middleton
- OzGrav, University of Melbourne, Parkville, Victoria 3010, Australia
| | - L Milano
- Università di Napoli "Federico II", Complesso Universitario di Monte S. Angelo, I-80126 Napoli, Italy
| | - A Miller
- California State University, Los Angeles, 5151 State University Dr, Los Angeles, California 90032, USA
| | - A L Miller
- Université catholique de Louvain, B-1348 Louvain-la-Neuve, Belgium
| | - B Miller
- Nikhef, Science Park 105, 1098 XG Amsterdam, Netherlands
- GRAPPA, Anton Pannekoek Institute for Astronomy and Institute for High-Energy Physics, University of Amsterdam, Science Park 904, 1098 XH Amsterdam, Netherlands
| | - M Millhouse
- OzGrav, University of Melbourne, Parkville, Victoria 3010, Australia
| | - J C Mills
- Gravity Exploration Institute, Cardiff University, Cardiff CF24 3AA, United Kingdom
| | - E Milotti
- INFN, Sezione di Trieste, I-34127 Trieste, Italy
- Dipartimento di Fisica, Università di Trieste, I-34127 Trieste, Italy
| | - O Minazzoli
- Artemis, Université Côte d'Azur, Observatoire de la Côte d'Azur, CNRS, F-06304 Nice, France
- Centre Scientifique de Monaco, 8 quai Antoine Ier, MC-98000, Monaco
| | - Y Minenkov
- INFN, Sezione di Roma Tor Vergata, I-00133 Roma, Italy
| | - Ll M Mir
- Institut de Física d'Altes Energies (IFAE), Barcelona Institute of Science and Technology, and ICREA, E-08193 Barcelona, Spain
| | - M Miravet-Tenés
- Departamento de Astronomía y Astrofísica, Universitat de València, E-46100 Burjassot, València, Spain
| | - C Mishra
- Indian Institute of Technology Madras, Chennai 600036, India
| | - T Mishra
- University of Florida, Gainesville, Florida 32611, USA
| | - T Mistry
- The University of Sheffield, Sheffield S10 2TN, United Kingdom
| | - S Mitra
- Inter-University Centre for Astronomy and Astrophysics, Pune 411007, India
| | - V P Mitrofanov
- Faculty of Physics, Lomonosov Moscow State University, Moscow 119991, Russia
| | | | - R Mittleman
- LIGO Laboratory, Massachusetts Institute of Technology, Cambridge, Massachusetts 02139, USA
| | - Geoffrey Mo
- LIGO Laboratory, Massachusetts Institute of Technology, Cambridge, Massachusetts 02139, USA
| | - E Moguel
- Kenyon College, Gambier, Ohio 43022, USA
| | - K Mogushi
- Missouri University of Science and Technology, Rolla, Missouri 65409, USA
| | - S R P Mohapatra
- LIGO Laboratory, Massachusetts Institute of Technology, Cambridge, Massachusetts 02139, USA
| | - S R Mohite
- University of Wisconsin-Milwaukee, Milwaukee, Wisconsin 53201, USA
| | - I Molina
- California State University Fullerton, Fullerton, California 92831, USA
| | - M Molina-Ruiz
- University of California, Berkeley, California 94720, USA
| | - M Mondin
- California State University, Los Angeles, 5151 State University Dr, Los Angeles, California 90032, USA
| | - M Montani
- Università degli Studi di Urbino "Carlo Bo", I-61029 Urbino, Italy
- INFN, Sezione di Firenze, I-50019 Sesto Fiorentino, Firenze, Italy
| | - C J Moore
- University of Birmingham, Birmingham B15 2TT, United Kingdom
| | - D Moraru
- LIGO Hanford Observatory, Richland, Washington 99352, USA
| | - F Morawski
- Nicolaus Copernicus Astronomical Center, Polish Academy of Sciences, 00-716, Warsaw, Poland
| | - A More
- Inter-University Centre for Astronomy and Astrophysics, Pune 411007, India
| | - C Moreno
- Embry-Riddle Aeronautical University, Prescott, Arizona 86301, USA
| | - G Moreno
- LIGO Hanford Observatory, Richland, Washington 99352, USA
| | - S Morisaki
- University of Wisconsin-Milwaukee, Milwaukee, Wisconsin 53201, USA
| | - B Mours
- Université de Strasbourg, CNRS, IPHC UMR 7178, F-67000 Strasbourg, France
| | - C M Mow-Lowry
- University of Birmingham, Birmingham B15 2TT, United Kingdom
- Vrije Universiteit Amsterdam, 1081 HV, Amsterdam, Netherlands
| | - S Mozzon
- University of Portsmouth, Portsmouth, PO1 3FX, United Kingdom
| | - F Muciaccia
- INFN, Sezione di Roma, I-00185 Roma, Italy
- Università di Roma "La Sapienza," I-00185 Roma, Italy
| | - Arunava Mukherjee
- Saha Institute of Nuclear Physics, Bidhannagar, West Bengal 700064, India
| | - D Mukherjee
- The Pennsylvania State University, University Park, Pennsylvania 16802, USA
| | - Soma Mukherjee
- The University of Texas Rio Grande Valley, Brownsville, Texas 78520, USA
| | | | - Suvodip Mukherjee
- GRAPPA, Anton Pannekoek Institute for Astronomy and Institute for High-Energy Physics, University of Amsterdam, Science Park 904, 1098 XH Amsterdam, Netherlands
| | - N Mukund
- Max Planck Institute for Gravitational Physics (Albert Einstein Institute), D-30167 Hannover, Germany
- Leibniz Universität Hannover, D-30167 Hannover, Germany
| | - A Mullavey
- LIGO Livingston Observatory, Livingston, Louisiana 70754, USA
| | - J Munch
- OzGrav, University of Adelaide, Adelaide, South Australia 5005, Australia
| | - E A Muñiz
- Syracuse University, Syracuse, New York 13244, USA
| | - P G Murray
- SUPA, University of Glasgow, Glasgow G12 8QQ, United Kingdom
| | - R Musenich
- INFN, Sezione di Genova, I-16146 Genova, Italy
- Dipartimento di Fisica, Università degli Studi di Genova, I-16146 Genova, Italy
| | - S Muusse
- OzGrav, University of Adelaide, Adelaide, South Australia 5005, Australia
| | - S L Nadji
- Max Planck Institute for Gravitational Physics (Albert Einstein Institute), D-30167 Hannover, Germany
- Leibniz Universität Hannover, D-30167 Hannover, Germany
| | - A Nagar
- INFN Sezione di Torino, I-10125 Torino, Italy
- Institut des Hautes Etudes Scientifiques, F-91440 Bures-sur-Yvette, France
| | - V Napolano
- European Gravitational Observatory (EGO), I-56021 Cascina, Pisa, Italy
| | - I Nardecchia
- Università di Roma Tor Vergata, I-00133 Roma, Italy
- INFN, Sezione di Roma Tor Vergata, I-00133 Roma, Italy
| | | | - B Nayak
- California State University, Los Angeles, 5151 State University Dr, Los Angeles, California 90032, USA
| | - R K Nayak
- Indian Institute of Science Education and Research, Kolkata, Mohanpur, West Bengal 741252, India
| | - B F Neil
- OzGrav, University of Western Australia, Crawley, Western Australia 6009, Australia
| | - J Neilson
- Dipartimento di Ingegneria, Università del Sannio, I-82100 Benevento, Italy
- INFN, Sezione di Napoli, Gruppo Collegato di Salerno, Complesso Universitario di Monte S. Angelo, I-80126 Napoli, Italy
| | - G Nelemans
- Department of Astrophysics/IMAPP, Radboud University Nijmegen, P.O. Box 9010, 6500 GL Nijmegen, Netherlands
| | - T J N Nelson
- LIGO Livingston Observatory, Livingston, Louisiana 70754, USA
| | - M Nery
- Max Planck Institute for Gravitational Physics (Albert Einstein Institute), D-30167 Hannover, Germany
- Leibniz Universität Hannover, D-30167 Hannover, Germany
| | - P Neubauer
- Kenyon College, Gambier, Ohio 43022, USA
| | - A Neunzert
- University of Washington Bothell, Bothell, Washington 98011, USA
| | - K Y Ng
- LIGO Laboratory, Massachusetts Institute of Technology, Cambridge, Massachusetts 02139, USA
| | - S W S Ng
- OzGrav, University of Adelaide, Adelaide, South Australia 5005, Australia
| | - C Nguyen
- Université de Paris, CNRS, Astroparticule et Cosmologie, F-75006 Paris, France
| | - P Nguyen
- University of Oregon, Eugene, Oregon 97403, USA
| | - T Nguyen
- LIGO Laboratory, Massachusetts Institute of Technology, Cambridge, Massachusetts 02139, USA
| | - S A Nichols
- Louisiana State University, Baton Rouge, Louisiana 70803, USA
| | - S Nissanke
- Nikhef, Science Park 105, 1098 XG Amsterdam, Netherlands
- GRAPPA, Anton Pannekoek Institute for Astronomy and Institute for High-Energy Physics, University of Amsterdam, Science Park 904, 1098 XH Amsterdam, Netherlands
| | - E Nitoglia
- Université Lyon, Université Claude Bernard Lyon 1, CNRS, IP2I Lyon / IN2P3, UMR 5822, F-69622 Villeurbanne, France
| | - F Nocera
- European Gravitational Observatory (EGO), I-56021 Cascina, Pisa, Italy
| | - M Norman
- Gravity Exploration Institute, Cardiff University, Cardiff CF24 3AA, United Kingdom
| | - C North
- Gravity Exploration Institute, Cardiff University, Cardiff CF24 3AA, United Kingdom
| | - L K Nuttall
- University of Portsmouth, Portsmouth, PO1 3FX, United Kingdom
| | - J Oberling
- LIGO Hanford Observatory, Richland, Washington 99352, USA
| | - B D O'Brien
- University of Florida, Gainesville, Florida 32611, USA
| | - J O'Dell
- Rutherford Appleton Laboratory, Didcot OX11 0DE, United Kingdom
| | - E Oelker
- SUPA, University of Glasgow, Glasgow G12 8QQ, United Kingdom
| | - G Oganesyan
- Gran Sasso Science Institute (GSSI), I-67100 L'Aquila, Italy
- INFN, Laboratori Nazionali del Gran Sasso, I-67100 Assergi, Italy
| | - J J Oh
- National Institute for Mathematical Sciences, Daejeon 34047, Republic of Korea
| | - S H Oh
- National Institute for Mathematical Sciences, Daejeon 34047, Republic of Korea
| | - F Ohme
- Max Planck Institute for Gravitational Physics (Albert Einstein Institute), D-30167 Hannover, Germany
- Leibniz Universität Hannover, D-30167 Hannover, Germany
| | - H Ohta
- RESCEU, University of Tokyo, Tokyo, 113-0033, Japan
| | - M A Okada
- Instituto Nacional de Pesquisas Espaciais, 12227-010 São José dos Campos, São Paulo, Brazil
| | - C Olivetto
- European Gravitational Observatory (EGO), I-56021 Cascina, Pisa, Italy
| | - R Oram
- LIGO Livingston Observatory, Livingston, Louisiana 70754, USA
| | - B O'Reilly
- LIGO Livingston Observatory, Livingston, Louisiana 70754, USA
| | - R G Ormiston
- University of Minnesota, Minneapolis, Minnesota 55455, USA
| | - N D Ormsby
- Christopher Newport University, Newport News, Virginia 23606, USA
| | - L F Ortega
- University of Florida, Gainesville, Florida 32611, USA
| | - R O'Shaughnessy
- Rochester Institute of Technology, Rochester, New York 14623, USA
| | - E O'Shea
- Cornell University, Ithaca, New York 14850, USA
| | - S Ossokine
- Max Planck Institute for Gravitational Physics (Albert Einstein Institute), D-14476 Potsdam, Germany
| | - C Osthelder
- LIGO Laboratory, California Institute of Technology, Pasadena, California 91125, USA
| | - D J Ottaway
- OzGrav, University of Adelaide, Adelaide, South Australia 5005, Australia
| | - H Overmier
- LIGO Livingston Observatory, Livingston, Louisiana 70754, USA
| | - A E Pace
- The Pennsylvania State University, University Park, Pennsylvania 16802, USA
| | - G Pagano
- INFN, Sezione di Pisa, I-56127 Pisa, Italy
- Università di Pisa, I-56127 Pisa, Italy
| | - M A Page
- OzGrav, University of Western Australia, Crawley, Western Australia 6009, Australia
| | - G Pagliaroli
- Gran Sasso Science Institute (GSSI), I-67100 L'Aquila, Italy
- INFN, Laboratori Nazionali del Gran Sasso, I-67100 Assergi, Italy
| | - A Pai
- Indian Institute of Technology Bombay, Powai, Mumbai 400 076, India
| | - S A Pai
- RRCAT, Indore, Madhya Pradesh 452013, India
| | - J R Palamos
- University of Oregon, Eugene, Oregon 97403, USA
| | - O Palashov
- Institute of Applied Physics, Nizhny Novgorod, 603950, Russia
| | - C Palomba
- INFN, Sezione di Roma, I-00185 Roma, Italy
| | - H Pan
- National Tsing Hua University, Hsinchu City, 30013 Taiwan, Republic of China
| | - P K Panda
- Directorate of Construction, Services & Estate Management, Mumbai 400094, India
| | - P T H Pang
- Nikhef, Science Park 105, 1098 XG Amsterdam, Netherlands
- Institute for Gravitational and Subatomic Physics (GRASP), Utrecht University, Princetonplein 1, 3584 CC Utrecht, Netherlands
| | - C Pankow
- Center for Interdisciplinary Exploration & Research in Astrophysics (CIERA), Northwestern University, Evanston, Illinois 60208, USA
| | - F Pannarale
- INFN, Sezione di Roma, I-00185 Roma, Italy
- Università di Roma "La Sapienza," I-00185 Roma, Italy
| | - B C Pant
- RRCAT, Indore, Madhya Pradesh 452013, India
| | - F H Panther
- OzGrav, University of Western Australia, Crawley, Western Australia 6009, Australia
| | - F Paoletti
- INFN, Sezione di Pisa, I-56127 Pisa, Italy
| | - A Paoli
- European Gravitational Observatory (EGO), I-56021 Cascina, Pisa, Italy
| | - A Paolone
- INFN, Sezione di Roma, I-00185 Roma, Italy
- Consiglio Nazionale delle Ricerche-Istituto dei Sistemi Complessi, Piazzale Aldo Moro 5, I-00185 Roma, Italy
| | - H Park
- University of Wisconsin-Milwaukee, Milwaukee, Wisconsin 53201, USA
| | - W Parker
- LIGO Livingston Observatory, Livingston, Louisiana 70754, USA
- Southern University and A&M College, Baton Rouge, Louisiana 70813, USA
| | - D Pascucci
- Nikhef, Science Park 105, 1098 XG Amsterdam, Netherlands
| | - A Pasqualetti
- European Gravitational Observatory (EGO), I-56021 Cascina, Pisa, Italy
| | - R Passaquieti
- INFN, Sezione di Pisa, I-56127 Pisa, Italy
- Università di Pisa, I-56127 Pisa, Italy
| | | | - M Patel
- Christopher Newport University, Newport News, Virginia 23606, USA
| | - M Pathak
- OzGrav, University of Adelaide, Adelaide, South Australia 5005, Australia
| | - B Patricelli
- INFN, Sezione di Pisa, I-56127 Pisa, Italy
- European Gravitational Observatory (EGO), I-56021 Cascina, Pisa, Italy
| | - A S Patron
- Louisiana State University, Baton Rouge, Louisiana 70803, USA
| | - S Paul
- University of Oregon, Eugene, Oregon 97403, USA
| | - E Payne
- OzGrav, School of Physics & Astronomy, Monash University, Clayton 3800, Victoria, Australia
| | - M Pedraza
- LIGO Laboratory, California Institute of Technology, Pasadena, California 91125, USA
| | - M Pegoraro
- INFN, Sezione di Padova, I-35131 Padova, Italy
| | - A Pele
- LIGO Livingston Observatory, Livingston, Louisiana 70754, USA
| | - S Penn
- Hobart and William Smith Colleges, Geneva, New York 14456, USA
| | - A Perego
- Università di Trento, Dipartimento di Fisica, I-38123 Povo, Trento, Italy
- INFN, Trento Institute for Fundamental Physics and Applications, I-38123 Povo, Trento, Italy
| | - A Pereira
- Université de Lyon, Université Claude Bernard Lyon 1, CNRS, Institut Lumière Matière, F-69622 Villeurbanne, France
| | - T Pereira
- International Institute of Physics, Universidade Federal do Rio Grande do Norte, Natal RN 59078-970, Brazil
| | - C J Perez
- LIGO Hanford Observatory, Richland, Washington 99352, USA
| | - C Périgois
- Laboratoire d'Annecy de Physique des Particules (LAPP), Université Grenoble Alpes, Université Savoie Mont Blanc, CNRS/IN2P3, F-74941 Annecy, France
| | - C C Perkins
- University of Florida, Gainesville, Florida 32611, USA
| | - A Perreca
- Università di Trento, Dipartimento di Fisica, I-38123 Povo, Trento, Italy
- INFN, Trento Institute for Fundamental Physics and Applications, I-38123 Povo, Trento, Italy
| | - S Perriès
- Université Lyon, Université Claude Bernard Lyon 1, CNRS, IP2I Lyon / IN2P3, UMR 5822, F-69622 Villeurbanne, France
| | - J Petermann
- Universität Hamburg, D-22761 Hamburg, Germany
| | - D Petterson
- LIGO Laboratory, California Institute of Technology, Pasadena, California 91125, USA
| | - H P Pfeiffer
- Max Planck Institute for Gravitational Physics (Albert Einstein Institute), D-14476 Potsdam, Germany
| | - K A Pham
- University of Minnesota, Minneapolis, Minnesota 55455, USA
| | - K S Phukon
- Nikhef, Science Park 105, 1098 XG Amsterdam, Netherlands
- Institute for High-Energy Physics, University of Amsterdam, Science Park 904, 1098 XH Amsterdam, Netherlands
| | | | - M Pichot
- Artemis, Université Côte d'Azur, Observatoire de la Côte d'Azur, CNRS, F-06304 Nice, France
| | - M Piendibene
- INFN, Sezione di Pisa, I-56127 Pisa, Italy
- Università di Pisa, I-56127 Pisa, Italy
| | - F Piergiovanni
- Università degli Studi di Urbino "Carlo Bo", I-61029 Urbino, Italy
- INFN, Sezione di Firenze, I-50019 Sesto Fiorentino, Firenze, Italy
| | - L Pierini
- INFN, Sezione di Roma, I-00185 Roma, Italy
- Università di Roma "La Sapienza," I-00185 Roma, Italy
| | - V Pierro
- Dipartimento di Ingegneria, Università del Sannio, I-82100 Benevento, Italy
- INFN, Sezione di Napoli, Gruppo Collegato di Salerno, Complesso Universitario di Monte S. Angelo, I-80126 Napoli, Italy
| | - G Pillant
- European Gravitational Observatory (EGO), I-56021 Cascina, Pisa, Italy
| | - M Pillas
- Université Paris-Saclay, CNRS/IN2P3, IJCLab, 91405 Orsay, France
| | - F Pilo
- INFN, Sezione di Pisa, I-56127 Pisa, Italy
| | - L Pinard
- Université Lyon, Université Claude Bernard Lyon 1, CNRS, Laboratoire des Matériaux Avancés (LMA), IP2I Lyon / IN2P3, UMR 5822, F-69622 Villeurbanne, France
| | - I M Pinto
- Dipartimento di Ingegneria, Università del Sannio, I-82100 Benevento, Italy
- INFN, Sezione di Napoli, Gruppo Collegato di Salerno, Complesso Universitario di Monte S. Angelo, I-80126 Napoli, Italy
- Museo Storico della Fisica e Centro Studi e Ricerche "Enrico Fermi," I-00184 Roma, Italy
| | - M Pinto
- European Gravitational Observatory (EGO), I-56021 Cascina, Pisa, Italy
| | - K Piotrzkowski
- Université catholique de Louvain, B-1348 Louvain-la-Neuve, Belgium
| | - M Pirello
- LIGO Hanford Observatory, Richland, Washington 99352, USA
| | - M D Pitkin
- Lancaster University, Lancaster LA1 4YW, United Kingdom
| | - E Placidi
- INFN, Sezione di Roma, I-00185 Roma, Italy
- Università di Roma "La Sapienza," I-00185 Roma, Italy
| | - L Planas
- Universitat de les Illes Balears, IAC3-IEEC, E-07122 Palma de Mallorca, Spain
| | - W Plastino
- Dipartimento di Matematica e Fisica, Università degli Studi Roma Tre, I-00146 Roma, Italy
- INFN, Sezione di Roma Tre, I-00146 Roma, Italy
| | - C Pluchar
- University of Arizona, Tucson, Arizona 85721, USA
| | - R Poggiani
- INFN, Sezione di Pisa, I-56127 Pisa, Italy
- Università di Pisa, I-56127 Pisa, Italy
| | - E Polini
- Laboratoire d'Annecy de Physique des Particules (LAPP), Université Grenoble Alpes, Université Savoie Mont Blanc, CNRS/IN2P3, F-74941 Annecy, France
| | - D Y T Pong
- The Chinese University of Hong Kong, Shatin, NT, Hong Kong
| | - S Ponrathnam
- Inter-University Centre for Astronomy and Astrophysics, Pune 411007, India
| | - P Popolizio
- European Gravitational Observatory (EGO), I-56021 Cascina, Pisa, Italy
| | - E K Porter
- Université de Paris, CNRS, Astroparticule et Cosmologie, F-75006 Paris, France
| | - R Poulton
- European Gravitational Observatory (EGO), I-56021 Cascina, Pisa, Italy
| | - J Powell
- OzGrav, Swinburne University of Technology, Hawthorn VIC 3122, Australia
| | - M Pracchia
- Laboratoire d'Annecy de Physique des Particules (LAPP), Université Grenoble Alpes, Université Savoie Mont Blanc, CNRS/IN2P3, F-74941 Annecy, France
| | - T Pradier
- Université de Strasbourg, CNRS, IPHC UMR 7178, F-67000 Strasbourg, France
| | - A K Prajapati
- Institute for Plasma Research, Bhat, Gandhinagar 382428, India
| | - K Prasai
- Stanford University, Stanford, California 94305, USA
| | - R Prasanna
- Directorate of Construction, Services & Estate Management, Mumbai 400094, India
| | - G Pratten
- University of Birmingham, Birmingham B15 2TT, United Kingdom
| | - M Principe
- Dipartimento di Ingegneria, Università del Sannio, I-82100 Benevento, Italy
- INFN, Sezione di Napoli, Gruppo Collegato di Salerno, Complesso Universitario di Monte S. Angelo, I-80126 Napoli, Italy
- Museo Storico della Fisica e Centro Studi e Ricerche "Enrico Fermi," I-00184 Roma, Italy
| | - G A Prodi
- INFN, Trento Institute for Fundamental Physics and Applications, I-38123 Povo, Trento, Italy
- Università di Trento, Dipartimento di Matematica, I-38123 Povo, Trento, Italy
| | - L Prokhorov
- University of Birmingham, Birmingham B15 2TT, United Kingdom
| | - P Prosposito
- Università di Roma Tor Vergata, I-00133 Roma, Italy
- INFN, Sezione di Roma Tor Vergata, I-00133 Roma, Italy
| | - L Prudenzi
- Max Planck Institute for Gravitational Physics (Albert Einstein Institute), D-14476 Potsdam, Germany
| | - A Puecher
- Nikhef, Science Park 105, 1098 XG Amsterdam, Netherlands
- Institute for Gravitational and Subatomic Physics (GRASP), Utrecht University, Princetonplein 1, 3584 CC Utrecht, Netherlands
| | - M Punturo
- INFN, Sezione di Perugia, I-06123 Perugia, Italy
| | - F Puosi
- INFN, Sezione di Pisa, I-56127 Pisa, Italy
- Università di Pisa, I-56127 Pisa, Italy
| | - P Puppo
- INFN, Sezione di Roma, I-00185 Roma, Italy
| | - M Pürrer
- Max Planck Institute for Gravitational Physics (Albert Einstein Institute), D-14476 Potsdam, Germany
| | - H Qi
- Gravity Exploration Institute, Cardiff University, Cardiff CF24 3AA, United Kingdom
| | - V Quetschke
- The University of Texas Rio Grande Valley, Brownsville, Texas 78520, USA
| | - R Quitzow-James
- Missouri University of Science and Technology, Rolla, Missouri 65409, USA
| | - F J Raab
- LIGO Hanford Observatory, Richland, Washington 99352, USA
| | - G Raaijmakers
- Nikhef, Science Park 105, 1098 XG Amsterdam, Netherlands
- GRAPPA, Anton Pannekoek Institute for Astronomy and Institute for High-Energy Physics, University of Amsterdam, Science Park 904, 1098 XH Amsterdam, Netherlands
| | - H Radkins
- LIGO Hanford Observatory, Richland, Washington 99352, USA
| | - N Radulesco
- Artemis, Université Côte d'Azur, Observatoire de la Côte d'Azur, CNRS, F-06304 Nice, France
| | - P Raffai
- MTA-ELTE Astrophysics Research Group, Institute of Physics, Eötvös University, Budapest 1117, Hungary
| | - S X Rail
- Université de Montréal/Polytechnique, Montreal, Quebec H3T 1J4, Canada
| | - S Raja
- RRCAT, Indore, Madhya Pradesh 452013, India
| | - C Rajan
- RRCAT, Indore, Madhya Pradesh 452013, India
| | - K E Ramirez
- LIGO Livingston Observatory, Livingston, Louisiana 70754, USA
| | - T D Ramirez
- California State University Fullerton, Fullerton, California 92831, USA
| | - A Ramos-Buades
- Max Planck Institute for Gravitational Physics (Albert Einstein Institute), D-14476 Potsdam, Germany
| | - J Rana
- The Pennsylvania State University, University Park, Pennsylvania 16802, USA
| | - P Rapagnani
- INFN, Sezione di Roma, I-00185 Roma, Italy
- Università di Roma "La Sapienza," I-00185 Roma, Italy
| | - U D Rapol
- Indian Institute of Science Education and Research, Pune, Maharashtra 411008, India
| | - A Ray
- University of Wisconsin-Milwaukee, Milwaukee, Wisconsin 53201, USA
| | - V Raymond
- Gravity Exploration Institute, Cardiff University, Cardiff CF24 3AA, United Kingdom
| | - N Raza
- University of British Columbia, Vancouver, British Columbia V6T 1Z4, Canada
| | - M Razzano
- INFN, Sezione di Pisa, I-56127 Pisa, Italy
- Università di Pisa, I-56127 Pisa, Italy
| | - J Read
- California State University Fullerton, Fullerton, California 92831, USA
| | - L A Rees
- American University, Washington, D.C. 20016, USA
| | - T Regimbau
- Laboratoire d'Annecy de Physique des Particules (LAPP), Université Grenoble Alpes, Université Savoie Mont Blanc, CNRS/IN2P3, F-74941 Annecy, France
| | - L Rei
- INFN, Sezione di Genova, I-16146 Genova, Italy
| | - S Reid
- SUPA, University of Strathclyde, Glasgow G1 1XQ, United Kingdom
| | - S W Reid
- Christopher Newport University, Newport News, Virginia 23606, USA
| | - D H Reitze
- LIGO Laboratory, California Institute of Technology, Pasadena, California 91125, USA
- University of Florida, Gainesville, Florida 32611, USA
| | - P Relton
- Gravity Exploration Institute, Cardiff University, Cardiff CF24 3AA, United Kingdom
| | - A Renzini
- LIGO Laboratory, California Institute of Technology, Pasadena, California 91125, USA
| | - P Rettegno
- INFN Sezione di Torino, I-10125 Torino, Italy
- Dipartimento di Fisica, Università degli Studi di Torino, I-10125 Torino, Italy
| | - M Rezac
- California State University Fullerton, Fullerton, California 92831, USA
| | - F Ricci
- INFN, Sezione di Roma, I-00185 Roma, Italy
- Università di Roma "La Sapienza," I-00185 Roma, Italy
| | - D Richards
- Rutherford Appleton Laboratory, Didcot OX11 0DE, United Kingdom
| | - J W Richardson
- LIGO Laboratory, California Institute of Technology, Pasadena, California 91125, USA
| | - L Richardson
- Texas A&M University, College Station, Texas 77843, USA
| | - G Riemenschneider
- INFN Sezione di Torino, I-10125 Torino, Italy
- Dipartimento di Fisica, Università degli Studi di Torino, I-10125 Torino, Italy
| | - K Riles
- University of Michigan, Ann Arbor, Michigan 48109, USA
| | - S Rinaldi
- INFN, Sezione di Pisa, I-56127 Pisa, Italy
- Università di Pisa, I-56127 Pisa, Italy
| | - K Rink
- University of British Columbia, Vancouver, British Columbia V6T 1Z4, Canada
| | - M Rizzo
- Center for Interdisciplinary Exploration & Research in Astrophysics (CIERA), Northwestern University, Evanston, Illinois 60208, USA
| | - N A Robertson
- LIGO Laboratory, California Institute of Technology, Pasadena, California 91125, USA
- SUPA, University of Glasgow, Glasgow G12 8QQ, United Kingdom
| | - R Robie
- LIGO Laboratory, California Institute of Technology, Pasadena, California 91125, USA
| | - F Robinet
- Université Paris-Saclay, CNRS/IN2P3, IJCLab, 91405 Orsay, France
| | - A Rocchi
- INFN, Sezione di Roma Tor Vergata, I-00133 Roma, Italy
| | - S Rodriguez
- California State University Fullerton, Fullerton, California 92831, USA
| | - L Rolland
- Laboratoire d'Annecy de Physique des Particules (LAPP), Université Grenoble Alpes, Université Savoie Mont Blanc, CNRS/IN2P3, F-74941 Annecy, France
| | - J G Rollins
- LIGO Laboratory, California Institute of Technology, Pasadena, California 91125, USA
| | - M Romanelli
- Université Rennes, CNRS, Institut FOTON-UMR6082, F-3500 Rennes, France
| | - R Romano
- Dipartimento di Farmacia, Università di Salerno, I-84084 Fisciano, Salerno, Italy
- INFN, Sezione di Napoli, Complesso Universitario di Monte S. Angelo, I-80126 Napoli, Italy
| | - C L Romel
- LIGO Hanford Observatory, Richland, Washington 99352, USA
| | - A Romero-Rodríguez
- Institut de Física d'Altes Energies (IFAE), Barcelona Institute of Science and Technology, and ICREA, E-08193 Barcelona, Spain
| | - I M Romero-Shaw
- OzGrav, School of Physics & Astronomy, Monash University, Clayton 3800, Victoria, Australia
| | - J H Romie
- LIGO Livingston Observatory, Livingston, Louisiana 70754, USA
| | - S Ronchini
- Gran Sasso Science Institute (GSSI), I-67100 L'Aquila, Italy
- INFN, Laboratori Nazionali del Gran Sasso, I-67100 Assergi, Italy
| | - L Rosa
- INFN, Sezione di Napoli, Complesso Universitario di Monte S. Angelo, I-80126 Napoli, Italy
- Università di Napoli "Federico II", Complesso Universitario di Monte S. Angelo, I-80126 Napoli, Italy
| | - C A Rose
- University of Wisconsin-Milwaukee, Milwaukee, Wisconsin 53201, USA
| | - D Rosińska
- Astronomical Observatory Warsaw University, 00-478 Warsaw, Poland
| | - M P Ross
- University of Washington, Seattle, Washington 98195, USA
| | - S Rowan
- SUPA, University of Glasgow, Glasgow G12 8QQ, United Kingdom
| | - S J Rowlinson
- University of Birmingham, Birmingham B15 2TT, United Kingdom
| | - S Roy
- Institute for Gravitational and Subatomic Physics (GRASP), Utrecht University, Princetonplein 1, 3584 CC Utrecht, Netherlands
| | - Santosh Roy
- Inter-University Centre for Astronomy and Astrophysics, Pune 411007, India
| | - Soumen Roy
- Indian Institute of Technology, Palaj, Gandhinagar, Gujarat 382355, India
| | - D Rozza
- Università degli Studi di Sassari, I-07100 Sassari, Italy
- INFN, Laboratori Nazionali del Sud, I-95125 Catania, Italy
| | - P Ruggi
- European Gravitational Observatory (EGO), I-56021 Cascina, Pisa, Italy
| | - K Ryan
- LIGO Hanford Observatory, Richland, Washington 99352, USA
| | - S Sachdev
- The Pennsylvania State University, University Park, Pennsylvania 16802, USA
| | - T Sadecki
- LIGO Hanford Observatory, Richland, Washington 99352, USA
| | - J Sadiq
- IGFAE, Campus Sur, Universidade de Santiago de Compostela, 15782 Spain
| | - M Sakellariadou
- King's College London, University of London, London WC2R 2LS, United Kingdom
| | - O S Salafia
- Università degli Studi di Milano-Bicocca, I-20126 Milano, Italy
- INFN, Sezione di Milano-Bicocca, I-20126 Milano, Italy
- INAF, Osservatorio Astronomico di Brera sede di Merate, I-23807 Merate, Lecco, Italy
| | - L Salconi
- European Gravitational Observatory (EGO), I-56021 Cascina, Pisa, Italy
| | - M Saleem
- University of Minnesota, Minneapolis, Minnesota 55455, USA
| | - F Salemi
- Università di Trento, Dipartimento di Fisica, I-38123 Povo, Trento, Italy
- INFN, Trento Institute for Fundamental Physics and Applications, I-38123 Povo, Trento, Italy
| | - A Samajdar
- Nikhef, Science Park 105, 1098 XG Amsterdam, Netherlands
- Institute for Gravitational and Subatomic Physics (GRASP), Utrecht University, Princetonplein 1, 3584 CC Utrecht, Netherlands
| | - E J Sanchez
- LIGO Laboratory, California Institute of Technology, Pasadena, California 91125, USA
| | - J H Sanchez
- California State University Fullerton, Fullerton, California 92831, USA
| | - L E Sanchez
- LIGO Laboratory, California Institute of Technology, Pasadena, California 91125, USA
| | - N Sanchis-Gual
- Departamento de Matemática da Universidade de Aveiro and Centre for Research and Development in Mathematics and Applications, Campus de Santiago, 3810-183 Aveiro, Portugal
| | - J R Sanders
- Marquette University, 11420 W. Clybourn Street, Milwaukee, Wisconsin 53233, USA
| | - A Sanuy
- Institut de Ciències del Cosmos (ICCUB), Universitat de Barcelona, C/ Martí i Franquès 1, Barcelona, 08028, Spain
| | - T R Saravanan
- Inter-University Centre for Astronomy and Astrophysics, Pune 411007, India
| | - N Sarin
- OzGrav, School of Physics & Astronomy, Monash University, Clayton 3800, Victoria, Australia
| | - B Sassolas
- Université Lyon, Université Claude Bernard Lyon 1, CNRS, Laboratoire des Matériaux Avancés (LMA), IP2I Lyon / IN2P3, UMR 5822, F-69622 Villeurbanne, France
| | - H Satari
- OzGrav, University of Western Australia, Crawley, Western Australia 6009, Australia
| | - B S Sathyaprakash
- Gravity Exploration Institute, Cardiff University, Cardiff CF24 3AA, United Kingdom
- The Pennsylvania State University, University Park, Pennsylvania 16802, USA
| | - O Sauter
- University of Florida, Gainesville, Florida 32611, USA
| | - R L Savage
- LIGO Hanford Observatory, Richland, Washington 99352, USA
| | - D Sawant
- Indian Institute of Technology Bombay, Powai, Mumbai 400 076, India
| | - H L Sawant
- Inter-University Centre for Astronomy and Astrophysics, Pune 411007, India
| | - S Sayah
- Université Lyon, Université Claude Bernard Lyon 1, CNRS, Laboratoire des Matériaux Avancés (LMA), IP2I Lyon / IN2P3, UMR 5822, F-69622 Villeurbanne, France
| | - D Schaetzl
- LIGO Laboratory, California Institute of Technology, Pasadena, California 91125, USA
| | - M Scheel
- CaRT, California Institute of Technology, Pasadena, California 91125, USA
| | - J Scheuer
- Center for Interdisciplinary Exploration & Research in Astrophysics (CIERA), Northwestern University, Evanston, Illinois 60208, USA
| | - M Schiworski
- OzGrav, University of Adelaide, Adelaide, South Australia 5005, Australia
| | - P Schmidt
- University of Birmingham, Birmingham B15 2TT, United Kingdom
| | - S Schmidt
- Institute for Gravitational and Subatomic Physics (GRASP), Utrecht University, Princetonplein 1, 3584 CC Utrecht, Netherlands
| | - R Schnabel
- Universität Hamburg, D-22761 Hamburg, Germany
| | - M Schneewind
- Max Planck Institute for Gravitational Physics (Albert Einstein Institute), D-30167 Hannover, Germany
- Leibniz Universität Hannover, D-30167 Hannover, Germany
| | | | - A Schönbeck
- Universität Hamburg, D-22761 Hamburg, Germany
| | - B W Schulte
- Max Planck Institute for Gravitational Physics (Albert Einstein Institute), D-30167 Hannover, Germany
- Leibniz Universität Hannover, D-30167 Hannover, Germany
| | - B F Schutz
- Max Planck Institute for Gravitational Physics (Albert Einstein Institute), D-30167 Hannover, Germany
- Leibniz Universität Hannover, D-30167 Hannover, Germany
- Gravity Exploration Institute, Cardiff University, Cardiff CF24 3AA, United Kingdom
| | - E Schwartz
- Gravity Exploration Institute, Cardiff University, Cardiff CF24 3AA, United Kingdom
| | - J Scott
- SUPA, University of Glasgow, Glasgow G12 8QQ, United Kingdom
| | - S M Scott
- OzGrav, Australian National University, Canberra, Australian Capital Territory 0200, Australia
| | - M Seglar-Arroyo
- Laboratoire d'Annecy de Physique des Particules (LAPP), Université Grenoble Alpes, Université Savoie Mont Blanc, CNRS/IN2P3, F-74941 Annecy, France
| | - D Sellers
- LIGO Livingston Observatory, Livingston, Louisiana 70754, USA
| | - A S Sengupta
- Indian Institute of Technology, Palaj, Gandhinagar, Gujarat 382355, India
| | - D Sentenac
- European Gravitational Observatory (EGO), I-56021 Cascina, Pisa, Italy
| | - E G Seo
- The Chinese University of Hong Kong, Shatin, NT, Hong Kong
| | - V Sequino
- INFN, Sezione di Napoli, Complesso Universitario di Monte S. Angelo, I-80126 Napoli, Italy
- Università di Napoli "Federico II", Complesso Universitario di Monte S. Angelo, I-80126 Napoli, Italy
| | - A Sergeev
- Institute of Applied Physics, Nizhny Novgorod, 603950, Russia
| | - Y Setyawati
- Institute for Gravitational and Subatomic Physics (GRASP), Utrecht University, Princetonplein 1, 3584 CC Utrecht, Netherlands
| | - T Shaffer
- LIGO Hanford Observatory, Richland, Washington 99352, USA
| | - M S Shahriar
- Center for Interdisciplinary Exploration & Research in Astrophysics (CIERA), Northwestern University, Evanston, Illinois 60208, USA
| | - B Shams
- The University of Utah, Salt Lake City, Utah 84112, USA
| | - A Sharma
- Gran Sasso Science Institute (GSSI), I-67100 L'Aquila, Italy
- INFN, Laboratori Nazionali del Gran Sasso, I-67100 Assergi, Italy
| | - P Sharma
- RRCAT, Indore, Madhya Pradesh 452013, India
| | - P Shawhan
- University of Maryland, College Park, Maryland 20742, USA
| | - N S Shcheblanov
- NAVIER, École des Ponts, Université Gustave Eiffel, CNRS, Marne-la-Vallée, France
| | - M Shikauchi
- RESCEU, University of Tokyo, Tokyo, 113-0033, Japan
| | - D H Shoemaker
- LIGO Laboratory, Massachusetts Institute of Technology, Cambridge, Massachusetts 02139, USA
| | - D M Shoemaker
- Department of Physics, University of Texas, Austin, Texas 78712, USA
| | | | - M Sieniawska
- Astronomical Observatory Warsaw University, 00-478 Warsaw, Poland
| | - D Sigg
- LIGO Hanford Observatory, Richland, Washington 99352, USA
| | - L P Singer
- NASA Goddard Space Flight Center, Greenbelt, Maryland 20771, USA
| | - D Singh
- The Pennsylvania State University, University Park, Pennsylvania 16802, USA
| | - N Singh
- Astronomical Observatory Warsaw University, 00-478 Warsaw, Poland
| | - A Singha
- Nikhef, Science Park 105, 1098 XG Amsterdam, Netherlands
- Maastricht University, P.O. Box 616, 6200 MD Maastricht, Netherlands
| | - A M Sintes
- Universitat de les Illes Balears, IAC3-IEEC, E-07122 Palma de Mallorca, Spain
| | - V Sipala
- Università degli Studi di Sassari, I-07100 Sassari, Italy
- INFN, Laboratori Nazionali del Sud, I-95125 Catania, Italy
| | - V Skliris
- Gravity Exploration Institute, Cardiff University, Cardiff CF24 3AA, United Kingdom
| | - B J J Slagmolen
- OzGrav, Australian National University, Canberra, Australian Capital Territory 0200, Australia
| | - T J Slaven-Blair
- OzGrav, University of Western Australia, Crawley, Western Australia 6009, Australia
| | - J Smetana
- University of Birmingham, Birmingham B15 2TT, United Kingdom
| | - J R Smith
- California State University Fullerton, Fullerton, California 92831, USA
| | - R J E Smith
- OzGrav, School of Physics & Astronomy, Monash University, Clayton 3800, Victoria, Australia
| | - J Soldateschi
- INFN, Sezione di Firenze, I-50019 Sesto Fiorentino, Firenze, Italy
- Università di Firenze, Sesto Fiorentino I-50019, Italy
- INAF, Osservatorio Astrofisico di Arcetri, Largo E. Fermi 5, I-50125 Firenze, Italy
| | - S N Somala
- Indian Institute of Technology Hyderabad, Sangareddy, Khandi, Telangana 502285, India
| | - E J Son
- National Institute for Mathematical Sciences, Daejeon 34047, Republic of Korea
| | - K Soni
- Inter-University Centre for Astronomy and Astrophysics, Pune 411007, India
| | - S Soni
- Louisiana State University, Baton Rouge, Louisiana 70803, USA
| | - V Sordini
- Université Lyon, Université Claude Bernard Lyon 1, CNRS, IP2I Lyon / IN2P3, UMR 5822, F-69622 Villeurbanne, France
| | | | - N Sorrentino
- INFN, Sezione di Pisa, I-56127 Pisa, Italy
- Università di Pisa, I-56127 Pisa, Italy
| | - R Soulard
- Artemis, Université Côte d'Azur, Observatoire de la Côte d'Azur, CNRS, F-06304 Nice, France
| | - T Souradeep
- Inter-University Centre for Astronomy and Astrophysics, Pune 411007, India
- Indian Institute of Science Education and Research, Pune, Maharashtra 411008, India
| | - E Sowell
- Texas Tech University, Lubbock, Texas 79409, USA
| | - V Spagnuolo
- Nikhef, Science Park 105, 1098 XG Amsterdam, Netherlands
- Maastricht University, P.O. Box 616, 6200 MD Maastricht, Netherlands
| | - A P Spencer
- SUPA, University of Glasgow, Glasgow G12 8QQ, United Kingdom
| | - M Spera
- Università di Padova, Dipartimento di Fisica e Astronomia, I-35131 Padova, Italy
- INFN, Sezione di Padova, I-35131 Padova, Italy
| | - R Srinivasan
- Artemis, Université Côte d'Azur, Observatoire de la Côte d'Azur, CNRS, F-06304 Nice, France
| | - A K Srivastava
- Institute for Plasma Research, Bhat, Gandhinagar 382428, India
| | - V Srivastava
- Syracuse University, Syracuse, New York 13244, USA
| | - K Staats
- Center for Interdisciplinary Exploration & Research in Astrophysics (CIERA), Northwestern University, Evanston, Illinois 60208, USA
| | - C Stachie
- Artemis, Université Côte d'Azur, Observatoire de la Côte d'Azur, CNRS, F-06304 Nice, France
| | - D A Steer
- Université de Paris, CNRS, Astroparticule et Cosmologie, F-75006 Paris, France
| | - J Steinlechner
- Nikhef, Science Park 105, 1098 XG Amsterdam, Netherlands
- Maastricht University, P.O. Box 616, 6200 MD Maastricht, Netherlands
| | - S Steinlechner
- Nikhef, Science Park 105, 1098 XG Amsterdam, Netherlands
- Maastricht University, P.O. Box 616, 6200 MD Maastricht, Netherlands
| | - S Stevenson
- OzGrav, Swinburne University of Technology, Hawthorn VIC 3122, Australia
| | - D J Stops
- University of Birmingham, Birmingham B15 2TT, United Kingdom
| | - M Stover
- Kenyon College, Gambier, Ohio 43022, USA
| | - K A Strain
- SUPA, University of Glasgow, Glasgow G12 8QQ, United Kingdom
| | - L C Strang
- OzGrav, University of Melbourne, Parkville, Victoria 3010, Australia
| | - G Stratta
- INFN, Sezione di Firenze, I-50019 Sesto Fiorentino, Firenze, Italy
- INAF, Osservatorio di Astrofisica e Scienza dello Spazio, I-40129 Bologna, Italy
| | - A Strunk
- LIGO Hanford Observatory, Richland, Washington 99352, USA
| | - R Sturani
- International Institute of Physics, Universidade Federal do Rio Grande do Norte, Natal RN 59078-970, Brazil
| | - A L Stuver
- Villanova University, 800 Lancaster Avenue, Villanova, Pennsylvania 19085, USA
| | - S Sudhagar
- Inter-University Centre for Astronomy and Astrophysics, Pune 411007, India
| | - V Sudhir
- LIGO Laboratory, Massachusetts Institute of Technology, Cambridge, Massachusetts 02139, USA
| | - H G Suh
- University of Wisconsin-Milwaukee, Milwaukee, Wisconsin 53201, USA
| | | | - H Sun
- OzGrav, University of Western Australia, Crawley, Western Australia 6009, Australia
| | - L Sun
- OzGrav, Australian National University, Canberra, Australian Capital Territory 0200, Australia
| | - S Sunil
- Institute for Plasma Research, Bhat, Gandhinagar 382428, India
| | - A Sur
- Nicolaus Copernicus Astronomical Center, Polish Academy of Sciences, 00-716, Warsaw, Poland
| | - J Suresh
- RESCEU, University of Tokyo, Tokyo, 113-0033, Japan
| | - P J Sutton
- Gravity Exploration Institute, Cardiff University, Cardiff CF24 3AA, United Kingdom
| | - B L Swinkels
- Nikhef, Science Park 105, 1098 XG Amsterdam, Netherlands
| | | | - P Szewczyk
- Astronomical Observatory Warsaw University, 00-478 Warsaw, Poland
| | - M Tacca
- Nikhef, Science Park 105, 1098 XG Amsterdam, Netherlands
| | - S C Tait
- SUPA, University of Glasgow, Glasgow G12 8QQ, United Kingdom
| | - C J Talbot
- SUPA, University of Strathclyde, Glasgow G1 1XQ, United Kingdom
| | - C Talbot
- LIGO Laboratory, California Institute of Technology, Pasadena, California 91125, USA
| | - A J Tanasijczuk
- Université catholique de Louvain, B-1348 Louvain-la-Neuve, Belgium
| | - D B Tanner
- University of Florida, Gainesville, Florida 32611, USA
| | - D Tao
- LIGO Laboratory, California Institute of Technology, Pasadena, California 91125, USA
| | - L Tao
- University of Florida, Gainesville, Florida 32611, USA
| | | | - C Taranto
- Università di Roma Tor Vergata, I-00133 Roma, Italy
| | - J D Tasson
- Carleton College, Northfield, Minnesota 55057, USA
| | - R Tenorio
- Universitat de les Illes Balears, IAC3-IEEC, E-07122 Palma de Mallorca, Spain
| | - J E Terhune
- Villanova University, 800 Lancaster Avenue, Villanova, Pennsylvania 19085, USA
| | - L Terkowski
- Universität Hamburg, D-22761 Hamburg, Germany
| | | | - M Thomas
- LIGO Livingston Observatory, Livingston, Louisiana 70754, USA
| | - P Thomas
- LIGO Hanford Observatory, Richland, Washington 99352, USA
| | - J E Thompson
- Gravity Exploration Institute, Cardiff University, Cardiff CF24 3AA, United Kingdom
| | | | - K A Thorne
- LIGO Livingston Observatory, Livingston, Louisiana 70754, USA
| | - E Thrane
- OzGrav, School of Physics & Astronomy, Monash University, Clayton 3800, Victoria, Australia
| | - Shubhanshu Tiwari
- Physik-Institut, University of Zurich, Winterthurerstrasse 190, 8057 Zurich, Switzerland
| | - Srishti Tiwari
- Inter-University Centre for Astronomy and Astrophysics, Pune 411007, India
| | - V Tiwari
- Gravity Exploration Institute, Cardiff University, Cardiff CF24 3AA, United Kingdom
| | - A M Toivonen
- University of Minnesota, Minneapolis, Minnesota 55455, USA
| | - K Toland
- SUPA, University of Glasgow, Glasgow G12 8QQ, United Kingdom
| | - A E Tolley
- University of Portsmouth, Portsmouth, PO1 3FX, United Kingdom
| | - M Tonelli
- INFN, Sezione di Pisa, I-56127 Pisa, Italy
- Università di Pisa, I-56127 Pisa, Italy
| | - A Torres-Forné
- Departamento de Astronomía y Astrofísica, Universitat de València, E-46100 Burjassot, València, Spain
| | - C I Torrie
- LIGO Laboratory, California Institute of Technology, Pasadena, California 91125, USA
| | - I Tosta E Melo
- Università degli Studi di Sassari, I-07100 Sassari, Italy
- INFN, Laboratori Nazionali del Sud, I-95125 Catania, Italy
| | - D Töyrä
- OzGrav, Australian National University, Canberra, Australian Capital Territory 0200, Australia
| | - A Trapananti
- INFN, Sezione di Perugia, I-06123 Perugia, Italy
- Università di Camerino, Dipartimento di Fisica, I-62032 Camerino, Italy
| | - F Travasso
- INFN, Sezione di Perugia, I-06123 Perugia, Italy
- Università di Camerino, Dipartimento di Fisica, I-62032 Camerino, Italy
| | - G Traylor
- LIGO Livingston Observatory, Livingston, Louisiana 70754, USA
| | - M Trevor
- University of Maryland, College Park, Maryland 20742, USA
| | - M C Tringali
- European Gravitational Observatory (EGO), I-56021 Cascina, Pisa, Italy
| | - A Tripathee
- University of Michigan, Ann Arbor, Michigan 48109, USA
| | - L Troiano
- INFN, Sezione di Napoli, Gruppo Collegato di Salerno, Complesso Universitario di Monte S. Angelo, I-80126 Napoli, Italy
- Dipartimento di Scienze Aziendali-Management and Innovation Systems (DISA-MIS), Università di Salerno, I-84084 Fisciano, Salerno, Italy
| | - A Trovato
- Université de Paris, CNRS, Astroparticule et Cosmologie, F-75006 Paris, France
| | - L Trozzo
- INFN, Sezione di Napoli, Complesso Universitario di Monte S. Angelo, I-80126 Napoli, Italy
| | - R J Trudeau
- LIGO Laboratory, California Institute of Technology, Pasadena, California 91125, USA
| | - D S Tsai
- National Tsing Hua University, Hsinchu City, 30013 Taiwan, Republic of China
| | - D Tsai
- National Tsing Hua University, Hsinchu City, 30013 Taiwan, Republic of China
| | - K W Tsang
- Nikhef, Science Park 105, 1098 XG Amsterdam, Netherlands
- Institute for Gravitational and Subatomic Physics (GRASP), Utrecht University, Princetonplein 1, 3584 CC Utrecht, Netherlands
- Van Swinderen Institute for Particle Physics and Gravity, University of Groningen, Nijenborgh 4, 9747 AG Groningen, Netherlands
| | - M Tse
- LIGO Laboratory, Massachusetts Institute of Technology, Cambridge, Massachusetts 02139, USA
| | - R Tso
- CaRT, California Institute of Technology, Pasadena, California 91125, USA
| | - L Tsukada
- RESCEU, University of Tokyo, Tokyo, 113-0033, Japan
| | - D Tsuna
- RESCEU, University of Tokyo, Tokyo, 113-0033, Japan
| | - T Tsutsui
- RESCEU, University of Tokyo, Tokyo, 113-0033, Japan
| | - K Turbang
- Universiteit Antwerpen, Prinsstraat 13, 2000 Antwerpen, Belgium
- Vrije Universiteit Brussel, Boulevard de la Plaine 2, 1050 Ixelles, Belgium
| | - M Turconi
- Artemis, Université Côte d'Azur, Observatoire de la Côte d'Azur, CNRS, F-06304 Nice, France
| | - A S Ubhi
- University of Birmingham, Birmingham B15 2TT, United Kingdom
| | - R P Udall
- LIGO Laboratory, California Institute of Technology, Pasadena, California 91125, USA
| | - K Ueno
- RESCEU, University of Tokyo, Tokyo, 113-0033, Japan
| | | | - A L Urban
- Louisiana State University, Baton Rouge, Louisiana 70803, USA
| | - A Utina
- Nikhef, Science Park 105, 1098 XG Amsterdam, Netherlands
- Maastricht University, P.O. Box 616, 6200 MD Maastricht, Netherlands
| | - H Vahlbruch
- Max Planck Institute for Gravitational Physics (Albert Einstein Institute), D-30167 Hannover, Germany
- Leibniz Universität Hannover, D-30167 Hannover, Germany
| | - G Vajente
- LIGO Laboratory, California Institute of Technology, Pasadena, California 91125, USA
| | - A Vajpeyi
- OzGrav, School of Physics & Astronomy, Monash University, Clayton 3800, Victoria, Australia
| | - G Valdes
- Texas A&M University, College Station, Texas 77843, USA
| | - M Valentini
- Università di Trento, Dipartimento di Fisica, I-38123 Povo, Trento, Italy
- INFN, Trento Institute for Fundamental Physics and Applications, I-38123 Povo, Trento, Italy
| | - V Valsan
- University of Wisconsin-Milwaukee, Milwaukee, Wisconsin 53201, USA
| | - N van Bakel
- Nikhef, Science Park 105, 1098 XG Amsterdam, Netherlands
| | - M van Beuzekom
- Nikhef, Science Park 105, 1098 XG Amsterdam, Netherlands
| | - J F J van den Brand
- Nikhef, Science Park 105, 1098 XG Amsterdam, Netherlands
- Maastricht University, P.O. Box 616, 6200 MD Maastricht, Netherlands
- Vrije Universiteit Amsterdam, 1081 HV Amsterdam, Netherlands
| | - C Van Den Broeck
- Nikhef, Science Park 105, 1098 XG Amsterdam, Netherlands
- Institute for Gravitational and Subatomic Physics (GRASP), Utrecht University, Princetonplein 1, 3584 CC Utrecht, Netherlands
| | | | | | | | - J Vanosky
- LIGO Laboratory, California Institute of Technology, Pasadena, California 91125, USA
| | - N van Remortel
- Universiteit Antwerpen, Prinsstraat 13, 2000 Antwerpen, Belgium
| | - M Vardaro
- Nikhef, Science Park 105, 1098 XG Amsterdam, Netherlands
- Institute for High-Energy Physics, University of Amsterdam, Science Park 904, 1098 XH Amsterdam, Netherlands
| | - A F Vargas
- OzGrav, University of Melbourne, Parkville, Victoria 3010, Australia
| | - V Varma
- Cornell University, Ithaca, New York 14850, USA
| | - M Vasúth
- Wigner RCP, RMKI, H-1121 Budapest, Konkoly Thege Miklós út 29-33, Hungary
| | - A Vecchio
- University of Birmingham, Birmingham B15 2TT, United Kingdom
| | - G Vedovato
- INFN, Sezione di Padova, I-35131 Padova, Italy
| | - J Veitch
- SUPA, University of Glasgow, Glasgow G12 8QQ, United Kingdom
| | - P J Veitch
- OzGrav, University of Adelaide, Adelaide, South Australia 5005, Australia
| | - J Venneberg
- Max Planck Institute for Gravitational Physics (Albert Einstein Institute), D-30167 Hannover, Germany
- Leibniz Universität Hannover, D-30167 Hannover, Germany
| | - G Venugopalan
- LIGO Laboratory, California Institute of Technology, Pasadena, California 91125, USA
| | - D Verkindt
- Laboratoire d'Annecy de Physique des Particules (LAPP), Université Grenoble Alpes, Université Savoie Mont Blanc, CNRS/IN2P3, F-74941 Annecy, France
| | - P Verma
- National Center for Nuclear Research, 05-400 Świerk-Otwock, Poland
| | - Y Verma
- RRCAT, Indore, Madhya Pradesh 452013, India
| | - D Veske
- Columbia University, New York, New York 10027, USA
| | - F Vetrano
- Università degli Studi di Urbino "Carlo Bo", I-61029 Urbino, Italy
| | - A Viceré
- Università degli Studi di Urbino "Carlo Bo", I-61029 Urbino, Italy
- INFN, Sezione di Firenze, I-50019 Sesto Fiorentino, Firenze, Italy
| | - S Vidyant
- Syracuse University, Syracuse, New York 13244, USA
| | - A D Viets
- Concordia University Wisconsin, Mequon, Wisconsin 53097, USA
| | - A Vijaykumar
- International Centre for Theoretical Sciences, Tata Institute of Fundamental Research, Bengaluru 560089, India
| | - V Villa-Ortega
- IGFAE, Campus Sur, Universidade de Santiago de Compostela, 15782 Spain
| | - J-Y Vinet
- Artemis, Université Côte d'Azur, Observatoire de la Côte d'Azur, CNRS, F-06304 Nice, France
| | - A Virtuoso
- INFN, Sezione di Trieste, I-34127 Trieste, Italy
- Dipartimento di Fisica, Università di Trieste, I-34127 Trieste, Italy
| | - S Vitale
- LIGO Laboratory, Massachusetts Institute of Technology, Cambridge, Massachusetts 02139, USA
| | - T Vo
- Syracuse University, Syracuse, New York 13244, USA
| | - H Vocca
- INFN, Sezione di Perugia, I-06123 Perugia, Italy
- Università di Perugia, I-06123 Perugia, Italy
| | - E R G von Reis
- LIGO Hanford Observatory, Richland, Washington 99352, USA
| | - J S A von Wrangel
- Max Planck Institute for Gravitational Physics (Albert Einstein Institute), D-30167 Hannover, Germany
- Leibniz Universität Hannover, D-30167 Hannover, Germany
| | - C Vorvick
- LIGO Hanford Observatory, Richland, Washington 99352, USA
| | - S P Vyatchanin
- Faculty of Physics, Lomonosov Moscow State University, Moscow 119991, Russia
| | - L E Wade
- Kenyon College, Gambier, Ohio 43022, USA
| | - M Wade
- Kenyon College, Gambier, Ohio 43022, USA
| | - K J Wagner
- Rochester Institute of Technology, Rochester, New York 14623, USA
| | - R C Walet
- Nikhef, Science Park 105, 1098 XG Amsterdam, Netherlands
| | - M Walker
- Christopher Newport University, Newport News, Virginia 23606, USA
| | - G S Wallace
- SUPA, University of Strathclyde, Glasgow G1 1XQ, United Kingdom
| | - L Wallace
- LIGO Laboratory, California Institute of Technology, Pasadena, California 91125, USA
| | - S Walsh
- University of Wisconsin-Milwaukee, Milwaukee, Wisconsin 53201, USA
| | - J Z Wang
- University of Michigan, Ann Arbor, Michigan 48109, USA
| | - W H Wang
- The University of Texas Rio Grande Valley, Brownsville, Texas 78520, USA
| | - R L Ward
- OzGrav, Australian National University, Canberra, Australian Capital Territory 0200, Australia
| | - J Warner
- LIGO Hanford Observatory, Richland, Washington 99352, USA
| | - M Was
- Laboratoire d'Annecy de Physique des Particules (LAPP), Université Grenoble Alpes, Université Savoie Mont Blanc, CNRS/IN2P3, F-74941 Annecy, France
| | - N Y Washington
- LIGO Laboratory, California Institute of Technology, Pasadena, California 91125, USA
| | - J Watchi
- Université Libre de Bruxelles, Brussels 1050, Belgium
| | - B Weaver
- LIGO Hanford Observatory, Richland, Washington 99352, USA
| | - S A Webster
- SUPA, University of Glasgow, Glasgow G12 8QQ, United Kingdom
| | - M Weinert
- Max Planck Institute for Gravitational Physics (Albert Einstein Institute), D-30167 Hannover, Germany
- Leibniz Universität Hannover, D-30167 Hannover, Germany
| | - A J Weinstein
- LIGO Laboratory, California Institute of Technology, Pasadena, California 91125, USA
| | - R Weiss
- LIGO Laboratory, Massachusetts Institute of Technology, Cambridge, Massachusetts 02139, USA
| | - C M Weller
- University of Washington, Seattle, Washington 98195, USA
| | - F Wellmann
- Max Planck Institute for Gravitational Physics (Albert Einstein Institute), D-30167 Hannover, Germany
- Leibniz Universität Hannover, D-30167 Hannover, Germany
| | - L Wen
- OzGrav, University of Western Australia, Crawley, Western Australia 6009, Australia
| | - P Weßels
- Max Planck Institute for Gravitational Physics (Albert Einstein Institute), D-30167 Hannover, Germany
- Leibniz Universität Hannover, D-30167 Hannover, Germany
| | - K Wette
- OzGrav, Australian National University, Canberra, Australian Capital Territory 0200, Australia
| | - J T Whelan
- Rochester Institute of Technology, Rochester, New York 14623, USA
| | - D D White
- California State University Fullerton, Fullerton, California 92831, USA
| | - B F Whiting
- University of Florida, Gainesville, Florida 32611, USA
| | - C Whittle
- LIGO Laboratory, Massachusetts Institute of Technology, Cambridge, Massachusetts 02139, USA
| | - D Wilken
- Max Planck Institute for Gravitational Physics (Albert Einstein Institute), D-30167 Hannover, Germany
- Leibniz Universität Hannover, D-30167 Hannover, Germany
| | - D Williams
- SUPA, University of Glasgow, Glasgow G12 8QQ, United Kingdom
| | - M J Williams
- SUPA, University of Glasgow, Glasgow G12 8QQ, United Kingdom
| | - A R Williamson
- University of Portsmouth, Portsmouth, PO1 3FX, United Kingdom
| | - J L Willis
- LIGO Laboratory, California Institute of Technology, Pasadena, California 91125, USA
| | - B Willke
- Max Planck Institute for Gravitational Physics (Albert Einstein Institute), D-30167 Hannover, Germany
- Leibniz Universität Hannover, D-30167 Hannover, Germany
| | - D J Wilson
- University of Arizona, Tucson, Arizona 85721, USA
| | - W Winkler
- Max Planck Institute for Gravitational Physics (Albert Einstein Institute), D-30167 Hannover, Germany
- Leibniz Universität Hannover, D-30167 Hannover, Germany
| | - C C Wipf
- LIGO Laboratory, California Institute of Technology, Pasadena, California 91125, USA
| | - T Wlodarczyk
- Max Planck Institute for Gravitational Physics (Albert Einstein Institute), D-14476 Potsdam, Germany
| | - G Woan
- SUPA, University of Glasgow, Glasgow G12 8QQ, United Kingdom
| | - J Woehler
- Max Planck Institute for Gravitational Physics (Albert Einstein Institute), D-30167 Hannover, Germany
- Leibniz Universität Hannover, D-30167 Hannover, Germany
| | - J K Wofford
- Rochester Institute of Technology, Rochester, New York 14623, USA
| | - I C F Wong
- The Chinese University of Hong Kong, Shatin, NT, Hong Kong
| | - D S Wu
- Max Planck Institute for Gravitational Physics (Albert Einstein Institute), D-30167 Hannover, Germany
- Leibniz Universität Hannover, D-30167 Hannover, Germany
| | - D M Wysocki
- University of Wisconsin-Milwaukee, Milwaukee, Wisconsin 53201, USA
| | - L Xiao
- LIGO Laboratory, California Institute of Technology, Pasadena, California 91125, USA
| | - H Yamamoto
- LIGO Laboratory, California Institute of Technology, Pasadena, California 91125, USA
| | - F W Yang
- The University of Utah, Salt Lake City, Utah 84112, USA
| | - L Yang
- Colorado State University, Fort Collins, Colorado 80523, USA
| | - Yang Yang
- University of Florida, Gainesville, Florida 32611, USA
| | - Z Yang
- University of Minnesota, Minneapolis, Minnesota 55455, USA
| | - M J Yap
- OzGrav, Australian National University, Canberra, Australian Capital Territory 0200, Australia
| | - D W Yeeles
- Gravity Exploration Institute, Cardiff University, Cardiff CF24 3AA, United Kingdom
| | - A B Yelikar
- Rochester Institute of Technology, Rochester, New York 14623, USA
| | - M Ying
- National Tsing Hua University, Hsinchu City, 30013 Taiwan, Republic of China
| | - J Yoo
- Cornell University, Ithaca, New York 14850, USA
| | - Hang Yu
- CaRT, California Institute of Technology, Pasadena, California 91125, USA
| | - Haocun Yu
- LIGO Laboratory, Massachusetts Institute of Technology, Cambridge, Massachusetts 02139, USA
| | - A Zadrożny
- National Center for Nuclear Research, 05-400 Świerk-Otwock, Poland
| | - M Zanolin
- Embry-Riddle Aeronautical University, Prescott, Arizona 86301, USA
| | - T Zelenova
- European Gravitational Observatory (EGO), I-56021 Cascina, Pisa, Italy
| | - J-P Zendri
- INFN, Sezione di Padova, I-35131 Padova, Italy
| | - M Zevin
- University of Chicago, Chicago, Illinois 60637, USA
| | - J Zhang
- OzGrav, University of Western Australia, Crawley, Western Australia 6009, Australia
| | - L Zhang
- LIGO Laboratory, California Institute of Technology, Pasadena, California 91125, USA
| | - T Zhang
- University of Birmingham, Birmingham B15 2TT, United Kingdom
| | - Y Zhang
- Texas A&M University, College Station, Texas 77843, USA
| | - C Zhao
- OzGrav, University of Western Australia, Crawley, Western Australia 6009, Australia
| | - G Zhao
- Université Libre de Bruxelles, Brussels 1050, Belgium
| | - Yue Zhao
- The University of Utah, Salt Lake City, Utah 84112, USA
| | - R Zhou
- University of California, Berkeley, California 94720, USA
| | - Z Zhou
- Center for Interdisciplinary Exploration & Research in Astrophysics (CIERA), Northwestern University, Evanston, Illinois 60208, USA
| | - X J Zhu
- OzGrav, School of Physics & Astronomy, Monash University, Clayton 3800, Victoria, Australia
| | - A B Zimmerman
- Department of Physics, University of Texas, Austin, Texas 78712, USA
| | - M E Zucker
- LIGO Laboratory, California Institute of Technology, Pasadena, California 91125, USA
- LIGO Laboratory, Massachusetts Institute of Technology, Cambridge, Massachusetts 02139, USA
| | - J Zweizig
- LIGO Laboratory, California Institute of Technology, Pasadena, California 91125, USA
| | - Donghui Jeong
- The Pennsylvania State University, University Park, Pennsylvania 16802, USA
| | - Sarah Shandera
- The Pennsylvania State University, University Park, Pennsylvania 16802, USA
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Singh A, Singh N, Kaur N, Jang DO. Gold nanoparticles supported on ionic‐liquid‐functionalized cellulose (Au@CIL): a heterogeneous catalyst for the selective reduction of aromatic nitro compounds. Appl Organomet Chem 2022. [DOI: 10.1002/aoc.6855] [Citation(s) in RCA: 0] [Impact Index Per Article: 0] [Reference Citation Analysis] [What about the content of this article? (0)] [Affiliation(s)] [Track Full Text] [Journal Information] [Subscribe] [Scholar Register] [Indexed: 11/05/2022]
Affiliation(s)
- Anoop Singh
- Department of Chemistry Indian Institute of Technology Ropar Punjab India
| | - Narinder Singh
- Department of Chemistry Indian Institute of Technology Ropar Punjab India
| | - Navneet Kaur
- Department of Chemistry Panjab University Chandigarh India
| | - Doo Ok Jang
- Department of Chemistry Yonsei University Wonju Korea
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Singh A, Singh G, Sharma S, Kaur N, Singh N. Metal‐Free, Biomass‐Derived Nano‐Architectured Carbon Quantum Dots as an Efficient Acid‐Base Bifunctional Catalyst for Facile Synthesis of Benzo[g]chromene and Pyrimidine Analogs. ChemistrySelect 2022. [DOI: 10.1002/slct.202200942] [Citation(s) in RCA: 0] [Impact Index Per Article: 0] [Reference Citation Analysis] [What about the content of this article? (0)] [Affiliation(s)] [Track Full Text] [Journal Information] [Subscribe] [Scholar Register] [Indexed: 11/10/2022]
Affiliation(s)
- Amanpreet Singh
- Department of Chemistry Indian Institute of Technology Ropar Punjab 140001 India
| | - Gagandeep Singh
- Department of Biomedical Engineering Indian Institute of Technology Ropar Punjab 140001 India
| | - Shilpa Sharma
- Department of Chemistry Indian Institute of Technology Ropar Punjab 140001 India
| | - Navneet Kaur
- Department of Chemistry Panjab University Chandigarh 160014 India
| | - Narinder Singh
- Department of Chemistry Indian Institute of Technology Ropar Punjab 140001 India
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Tjahjono R, Salati H, Inthavong K, Singh N. Correlation of Nasal Mucosal Temperature and Nasal Patency—A Computational Fluid Dynamics Study. Laryngoscope 2022; 133:1328-1335. [PMID: 37158263 DOI: 10.1002/lary.30327] [Citation(s) in RCA: 0] [Impact Index Per Article: 0] [Reference Citation Analysis] [What about the content of this article? (0)] [Affiliation(s)] [Abstract] [Track Full Text] [Journal Information] [Subscribe] [Scholar Register] [Received: 05/24/2021] [Revised: 07/06/2022] [Accepted: 07/19/2022] [Indexed: 11/07/2022]
Abstract
OBJECTIVES Recent evidence suggests that detection of nasal mucosal temperature, rather than direct airflow detection, is the primary determinant of subjective nasal patency. This study examines the role of nasal mucosal temperature in the perception of nasal patency using in vivo and computational fluid dynamics (CFD) measurements. METHODS Healthy adult participants completed Nasal Obstruction Symptom Evaluation (NOSE) and Visual Analogue Scale (VAS) questionnaires. A temperature probe measured nasal mucosal temperature at the vestibule, inferior turbinate, middle turbinate, and nasopharynx bilaterally. Participants underwent a CT scan, used to create a 3D nasal anatomy model to perform CFD analysis of nasal mucosal and inspired air temperature and heat flux along with mucosal surface area where heat flux >50 W/m2 (SAHF50). RESULTS Eleven participants with a median age of 27 (IQR 24; 48) were recruited. Probe-measured temperature values correlated strongly with CFD-derived values (r = 0.87, p < 0.05). Correlations were seen anteriorly in the vestibule and inferior turbinate regions between nasal mucosal temperature and unilateral VAS (r = 0.42-0.46; p < 0.05), between SAHF50 and unilateral VAS (r = -0.31 to -0.36; p < 0.05) and between nasal mucosal temperature and SAHF50 (r = -0.37 to -0.41; p < 0.05). Subjects with high patency (VAS ≤10) had increased heat flux anteriorly compared with lower patency subjects (VAS >10; p < 0.05). CONCLUSION Lower nasal mucosal temperature and higher heat flux within the anterior nasal cavity correlates with a perception of improved unilateral nasal patency in healthy individuals. LEVEL OF EVIDENCE 4 Laryngoscope, 133:1328-1335, 2023.
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Affiliation(s)
- Richard Tjahjono
- Department of Otolaryngology Head and Neck Surgery Westmead Hospital Sydney New South Wales Australia
- Sydney Medical School, University of Sydney Sydney New South Wales Australia
| | - Hana Salati
- Faculty of Engineering RMIT University Melbourne Victoria Australia
| | - Kiao Inthavong
- Faculty of Engineering RMIT University Melbourne Victoria Australia
| | - Narinder Singh
- Department of Otolaryngology Head and Neck Surgery Westmead Hospital Sydney New South Wales Australia
- Sydney Medical School, University of Sydney Sydney New South Wales Australia
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