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Kim JY, Lee CH, Sung MW, Min YG, Chung PS. Experimental study of the pathological changes of rabbit tonsils exposed to anthracite coal briquette gas. Adv Otorhinolaryngol 2015; 47:161-7. [PMID: 1456126 DOI: 10.1159/000421736] [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] [Indexed: 12/27/2022]
Affiliation(s)
- J Y Kim
- Department of Otolaryngology, Seoul National University, College of Medicine, Korea
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Goh SY, Ang SB, Bee YM, Chen YT, Gardner DS, Ho ET, Adaikan K, Lee YC, Lee CH, Lim FS, Lim HB, Lim SC, Seow J, Soh AW, Sum CF, Tai ES, Thai AC, Wong TY, Yap F. Ministry of Health Clinical Practice Guidelines: Diabetes Mellitus. Singapore Med J 2015; 55:334-47. [PMID: 25017409 DOI: 10.11622/smedj.2014079] [Citation(s) in RCA: 33] [Impact Index Per Article: 3.7] [Reference Citation Analysis] [What about the content of this article? (0)] [Affiliation(s)] [Abstract] [Track Full Text] [Journal Information] [Subscribe] [Scholar Register] [Indexed: 12/22/2022]
Abstract
The Ministry of Health (MOH) have updated the clinical practice guidelines on Diabetes Mellitus to provide doctors and patients in Singapore with evidence-based treatment for diabetes mellitus. This article reproduces the introduction and executive summary (with recommendations from the guidelines) from the MOH clinical practice guidelines on Diabetes Mellitus, for the information of SMJ readers. Chapters and page numbers mentioned in the reproduced extract refer to the full text of the guidelines, which are available from the Ministry of Health website: http://www.moh.gov.sg/content/moh_web/healthprofessionalsportal/doctors/guidelines/cpg_medical.html. The recommendations should be used with reference to the full text of the guidelines. Following this article are multiple choice questions based on the full text of the guidelines.
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Affiliation(s)
- S Y Goh
- Department of Endocrinology, Singapore General Hospital, Outram Road, Singapore 169608.
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Lee CH, Hui EYL, Woo YC, Yeung CY, Chow WS, Yuen MMA, Fong CHY, Xu A, Lam KSL. Circulating fibroblast growth factor 21 levels predict progressive kidney disease in subjects with type 2 diabetes and normoalbuminuria. J Clin Endocrinol Metab 2015; 100:1368-75. [PMID: 25625802 DOI: 10.1210/jc.2014-3465] [Citation(s) in RCA: 68] [Impact Index Per Article: 7.6] [Reference Citation Analysis] [What about the content of this article? (0)] [Affiliation(s)] [Abstract] [MESH Headings] [Track Full Text] [Journal Information] [Submit a Manuscript] [Subscribe] [Scholar Register] [Indexed: 02/13/2023]
Abstract
BACKGROUND Elevated fibroblast growth factor 21 (FGF21) levels have been suggested, from cross-sectional studies, as an indicator of subclinical diabetic nephropathy. We investigated whether serum FGF21 was predictive of the development of diabetic nephropathy. METHOD Baseline serum FGF21 levels were measured in 1136 Chinese type 2 diabetic subjects recruited from the Hong Kong West Diabetes Registry. The role of serum FGF21 in predicting decline in estimated glomerular filtration rate (eGFR) over a median follow-up of 4 years was analyzed using Cox regression analysis. RESULTS At baseline, serum FGF21 levels increased progressively with eGFR category (P for trend <.001). Among 1071 subjects with baseline eGFR ≥ 30 mL/min/1.73 m(2), serum FGF21 levels were significantly higher in those with eGFR decline during follow-up (n = 171) than those without decline (n = 900) (P < .001). In multivariable Cox regression analysis, baseline serum FGF21 was independently associated with eGFR decline (hazard ratio, 1.21; 95% confidence interval [CI], 1.01-1.43; P = .036), even after adjustment for baseline eGFR. In a subgroup of 559 subjects with baseline eGFR ≥ 60 mL/min/1.73 m(2) and normoalbuminuria, serum FGF21 level remained an independent predictor of eGFR decline (hazard ratio, 1.36; 95% CI, 1.06-1.76; P = .016). Integrated discrimination improvement (IDI) suggested that the inclusion of baseline serum FGF21 significantly improved the prediction of eGFR decline (IDI, 1%; 95% CI, 0.1-3.0; P = .013) in this subgroup, but not in the initial cohort involving all subjects. CONCLUSIONS Elevated serum FGF21 levels may be a useful biomarker for predicting kidney disease progression, especially in the early stages of diabetic nephropathy.
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Affiliation(s)
- C H Lee
- Department of Medicine (C.H.L., E.Y.L.H., Y.C.W., C.Y.Y., W.S.C., M.M.A.Y., C.H.Y.F. A.X., K.S.L.L.), Queen Mary Hospital, Hong Kong SAR; Research Centre of Heart, Brain, Hormone and Healthy Aging (E.Y.L.H., A.X., K.S.L.L.), The University of Hong Kong, Pokfulam, Hong Kong SAR; and State Key Laboratory of Pharmaceutical Biotechnology (A.X., K.S.L.L.), The University of Hong Kong, Pokfulam, Hong Kong SAR
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104
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Han SY, Ryu KJ, Ahn KH, Cho SB, Lee CH, Hong SC. Conservative treatment of uterine fistula with abdominal abscess after caesarean section. J OBSTET GYNAECOL 2014; 35:650-1. [PMID: 25496617 DOI: 10.3109/01443615.2014.987115] [Citation(s) in RCA: 2] [Impact Index Per Article: 0.2] [Reference Citation Analysis] [What about the content of this article? (0)] [Affiliation(s)] [Track Full Text] [Journal Information] [Subscribe] [Scholar Register] [Indexed: 11/13/2022]
Affiliation(s)
- S Y Han
- a Department of Obstetrics and Gynecology , College of Medicine, Korea University , Seoul , Republic of Korea
| | - K J Ryu
- a Department of Obstetrics and Gynecology , College of Medicine, Korea University , Seoul , Republic of Korea
| | - K H Ahn
- a Department of Obstetrics and Gynecology , College of Medicine, Korea University , Seoul , Republic of Korea
| | - S B Cho
- b Department of Radiology , College of Medicine, Korea University , Seoul , Republic of Korea
| | - C H Lee
- c Department of Science , University of Manitoba , Winnipeg , MB , Canada
| | - S C Hong
- a Department of Obstetrics and Gynecology , College of Medicine, Korea University , Seoul , Republic of Korea
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105
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Chohan M, Mackedenski S, Li WM, Lee CH. Human apurinic/apyrimidinic endonuclease 1 (APE1) has 3' RNA phosphatase and 3' exoribonuclease activities. J Mol Biol 2014; 427:298-311. [PMID: 25498387 DOI: 10.1016/j.jmb.2014.12.001] [Citation(s) in RCA: 19] [Impact Index Per Article: 1.9] [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: 09/01/2014] [Revised: 12/02/2014] [Accepted: 12/02/2014] [Indexed: 10/24/2022]
Abstract
Apurinic/apyrimidinic endonuclease 1 (APE1) is the predominant mammalian enzyme in DNA base excision repair pathway that cleaves the DNA backbone immediately 5' to abasic sites. In addition to its abasic endonuclease activity, APE1 has 3' phosphatase and 3'-5' exonuclease activities against DNA. We recently identified APE1 as an endoribonuclease that preferentially cleaves at UA, UG, and CA sites in single-stranded regions of RNAs and can regulate c-myc mRNA level and half-life in cells. APE1 can also endonucleolytically cleave abasic single-stranded RNA. Here, we show for the first time that the human APE1 has 3' RNA phosphatase and 3' exoribonuclease activities. Using three distinct RNA substrates, we show that APE1, but not RNase A, can remove the phosphoryl group from the 3' end of RNA decay products. Studies using various site-directed APE1 mutant proteins (H309N, H309S, D283N, N68A, D210N, Y171F, D308A, F266A, and D70A) suggest that the 3' RNA phosphatase activity shares the same active center as its other known nuclease activities. A number of APE1 variants previously identified in the human population, including the most common D148E variant, have greater than 80% reduction in the 3' RNA phosphatase activity. APE1 can remove a ribonucleotide from the 3' overhang of RNA decay product, but its 3'-5' exoribonuclease activity against unstructured poly(A), poly(C), and poly(U) RNAs is relatively weak. This study further underscores the significance of understanding the role of APE1 in RNA metabolism in vivo.
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Affiliation(s)
- Manbir Chohan
- Chemistry Program, University of Northern British Columbia, 3333 University Way, Prince George, British Columbia, V2N 4Z9, Canada
| | - Sebastian Mackedenski
- Chemistry Program, University of Northern British Columbia, 3333 University Way, Prince George, British Columbia, V2N 4Z9, Canada
| | - Wai-Ming Li
- Chemistry Program, University of Northern British Columbia, 3333 University Way, Prince George, British Columbia, V2N 4Z9, Canada
| | - Chow H Lee
- Chemistry Program, University of Northern British Columbia, 3333 University Way, Prince George, British Columbia, V2N 4Z9, Canada.
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Yoshida T, Ideta S, Shimojima T, Malaeb W, Shinada K, Suzuki H, Nishi I, Fujimori A, Ishizaka K, Shin S, Nakashima Y, Anzai H, Arita M, Ino A, Namatame H, Taniguchi M, Kumigashira H, Ono K, Kasahara S, Shibauchi T, Terashima T, Matsuda Y, Nakajima M, Uchida S, Tomioka Y, Ito T, Kihou K, Lee CH, Iyo A, Eisaki H, Ikeda H, Arita R, Saito T, Onari S, Kontani H. Anisotropy of the superconducting gap in the iron-based superconductor BaFe2(As(1-x)P(x))2. Sci Rep 2014; 4:7292. [PMID: 25465027 PMCID: PMC4252890 DOI: 10.1038/srep07292] [Citation(s) in RCA: 22] [Impact Index Per Article: 2.2] [Reference Citation Analysis] [What about the content of this article? (0)] [Affiliation(s)] [Abstract] [Track Full Text] [Download PDF] [Figures] [Journal Information] [Subscribe] [Scholar Register] [Received: 04/24/2014] [Accepted: 11/14/2014] [Indexed: 11/22/2022] Open
Abstract
We report peculiar momentum-dependent anisotropy in the superconducting gap observed by angle-resolved photoemission spectroscopy in BaFe2(As1-xPx)2 (x = 0.30, Tc = 30 K). Strongly anisotropic gap has been found only in the electron Fermi surface while the gap on the entire hole Fermi surfaces are nearly isotropic. These results are inconsistent with horizontal nodes but are consistent with modified s± gap with nodal loops. We have shown that the complicated gap modulation can be theoretically reproduced by considering both spin and orbital fluctuations.
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Affiliation(s)
- T Yoshida
- 1] Department of Physics, University of Tokyo, Bunkyo-ku, Tokyo 113-0033, Japan [2] JST, Transformative Research-Project on Iron Pnictides (TRIP), Chiyoda, Tokyo 102-0075, Japan
| | - S Ideta
- Department of Physics, University of Tokyo, Bunkyo-ku, Tokyo 113-0033, Japan
| | - T Shimojima
- Department of Applied Physics, University of Tokyo, Tokyo 113-8656, Japan
| | - W Malaeb
- Institute of Solid State Physics, University of Tokyo, Kashiwa 277-8581, Japan
| | - K Shinada
- Department of Applied Physics, University of Tokyo, Tokyo 113-8656, Japan
| | - H Suzuki
- Department of Physics, University of Tokyo, Bunkyo-ku, Tokyo 113-0033, Japan
| | - I Nishi
- Department of Physics, University of Tokyo, Bunkyo-ku, Tokyo 113-0033, Japan
| | - A Fujimori
- 1] Department of Physics, University of Tokyo, Bunkyo-ku, Tokyo 113-0033, Japan [2] JST, Transformative Research-Project on Iron Pnictides (TRIP), Chiyoda, Tokyo 102-0075, Japan
| | - K Ishizaka
- Department of Applied Physics, University of Tokyo, Tokyo 113-8656, Japan
| | - S Shin
- Institute of Solid State Physics, University of Tokyo, Kashiwa 277-8581, Japan
| | - Y Nakashima
- Graduate School of Science, Hiroshima University, Higashi-Hiroshima 739-8526, Japan
| | - H Anzai
- Hiroshima Synchrotron Radiation Center, Hiroshima University, Higashi-Hiroshima 739-0046, Japan
| | - M Arita
- Hiroshima Synchrotron Radiation Center, Hiroshima University, Higashi-Hiroshima 739-0046, Japan
| | - A Ino
- Graduate School of Science, Hiroshima University, Higashi-Hiroshima 739-8526, Japan
| | - H Namatame
- Hiroshima Synchrotron Radiation Center, Hiroshima University, Higashi-Hiroshima 739-0046, Japan
| | - M Taniguchi
- 1] Graduate School of Science, Hiroshima University, Higashi-Hiroshima 739-8526, Japan [2] Hiroshima Synchrotron Radiation Center, Hiroshima University, Higashi-Hiroshima 739-0046, Japan
| | - H Kumigashira
- KEK, Photon Factory, Tsukuba, Ibaraki 305-0801, Japan
| | - K Ono
- KEK, Photon Factory, Tsukuba, Ibaraki 305-0801, Japan
| | - S Kasahara
- 1] Research Center for Low Temperature and Materials Sciences, Kyoto University, Kyoto 606-8502, Japan [2] Department of Physics, Kyoto University, Kyoto 606-8502, Japan
| | - T Shibauchi
- Department of Physics, Kyoto University, Kyoto 606-8502, Japan
| | - T Terashima
- Research Center for Low Temperature and Materials Sciences, Kyoto University, Kyoto 606-8502, Japan
| | - Y Matsuda
- Department of Physics, Kyoto University, Kyoto 606-8502, Japan
| | - M Nakajima
- Department of Physics, University of Tokyo, Bunkyo-ku, Tokyo 113-0033, Japan
| | - S Uchida
- 1] Department of Physics, University of Tokyo, Bunkyo-ku, Tokyo 113-0033, Japan [2] JST, Transformative Research-Project on Iron Pnictides (TRIP), Chiyoda, Tokyo 102-0075, Japan
| | - Y Tomioka
- 1] JST, Transformative Research-Project on Iron Pnictides (TRIP), Chiyoda, Tokyo 102-0075, Japan [2] National Institute of Advanced Industrial Science and Technology (AIST), Tsukuba 305-8568, Japan
| | - T Ito
- 1] JST, Transformative Research-Project on Iron Pnictides (TRIP), Chiyoda, Tokyo 102-0075, Japan [2] National Institute of Advanced Industrial Science and Technology (AIST), Tsukuba 305-8568, Japan
| | - K Kihou
- 1] JST, Transformative Research-Project on Iron Pnictides (TRIP), Chiyoda, Tokyo 102-0075, Japan [2] National Institute of Advanced Industrial Science and Technology (AIST), Tsukuba 305-8568, Japan
| | - C H Lee
- 1] JST, Transformative Research-Project on Iron Pnictides (TRIP), Chiyoda, Tokyo 102-0075, Japan [2] National Institute of Advanced Industrial Science and Technology (AIST), Tsukuba 305-8568, Japan
| | - A Iyo
- 1] JST, Transformative Research-Project on Iron Pnictides (TRIP), Chiyoda, Tokyo 102-0075, Japan [2] National Institute of Advanced Industrial Science and Technology (AIST), Tsukuba 305-8568, Japan
| | - H Eisaki
- 1] JST, Transformative Research-Project on Iron Pnictides (TRIP), Chiyoda, Tokyo 102-0075, Japan [2] National Institute of Advanced Industrial Science and Technology (AIST), Tsukuba 305-8568, Japan
| | - H Ikeda
- 1] JST, Transformative Research-Project on Iron Pnictides (TRIP), Chiyoda, Tokyo 102-0075, Japan [2] Department of Physics, Kyoto University, Kyoto 606-8502, Japan
| | - R Arita
- 1] JST, Transformative Research-Project on Iron Pnictides (TRIP), Chiyoda, Tokyo 102-0075, Japan [2] Department of Applied Physics, University of Tokyo, Tokyo 113-8656, Japan
| | - T Saito
- 1] JST, Transformative Research-Project on Iron Pnictides (TRIP), Chiyoda, Tokyo 102-0075, Japan [2] Department of Physics, Nagoya University, Furo-cho, Nagoya 464-8602, Japan
| | - S Onari
- 1] JST, Transformative Research-Project on Iron Pnictides (TRIP), Chiyoda, Tokyo 102-0075, Japan [2] Department of Applied Physics, Nagoya University, Furo-cho, Nagoya 464-8602, Japan
| | - H Kontani
- 1] JST, Transformative Research-Project on Iron Pnictides (TRIP), Chiyoda, Tokyo 102-0075, Japan [2] Department of Physics, Nagoya University, Furo-cho, Nagoya 464-8602, Japan
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107
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Barnes M, van Rensburg G, Li WM, Mehmood K, Mackedenski S, Chan CM, King DT, Miller AL, Lee CH. Molecular insights into the coding region determinant-binding protein-RNA interaction through site-directed mutagenesis in the heterogeneous nuclear ribonucleoprotein-K-homology domains. J Biol Chem 2014; 290:625-39. [PMID: 25389298 DOI: 10.1074/jbc.m114.614735] [Citation(s) in RCA: 19] [Impact Index Per Article: 1.9] [Reference Citation Analysis] [What about the content of this article? (0)] [Affiliation(s)] [Abstract] [Key Words] [Track Full Text] [Journal Information] [Subscribe] [Scholar Register] [Indexed: 11/06/2022] Open
Abstract
The ability of its four heterogeneous nuclear RNP-K-homology (KH) domains to physically associate with oncogenic mRNAs is a major criterion for the function of the coding region determinant-binding protein (CRD-BP). However, the particular RNA-binding role of each of the KH domains remains largely unresolved. Here, we mutated the first glycine to an aspartate in the universally conserved GXXG motif of the KH domain as an approach to investigate their role. Our results show that mutation of a single GXXG motif generally had no effect on binding, but the mutation in any two KH domains, with the exception of the combination of KH3 and KH4 domains, completely abrogated RNA binding in vitro and significantly retarded granule formation in zebrafish embryos, suggesting that any combination of at least two KH domains cooperate in tandem to bind RNA efficiently. Interestingly, we found that any single point mutation in one of the four KH domains significantly impacted CRD-BP binding to mRNAs in HeLa cells, suggesting that the dynamics of the CRD-BP-mRNA interaction vary over time in vivo. Furthermore, our results suggest that different mRNAs bind preferentially to distinct CRD-BP KH domains. The novel insights revealed in this study have important implications on the understanding of the oncogenic mechanism of CRD-BP as well as in the future design of inhibitors against CRD-BP function.
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Affiliation(s)
- Mark Barnes
- From the Chemistry Program, University of Northern British Columbia, Prince George, British Columbia V2N 4Z9, Canada
| | - Gerrit van Rensburg
- From the Chemistry Program, University of Northern British Columbia, Prince George, British Columbia V2N 4Z9, Canada
| | - Wai-Ming Li
- From the Chemistry Program, University of Northern British Columbia, Prince George, British Columbia V2N 4Z9, Canada
| | - Kashif Mehmood
- From the Chemistry Program, University of Northern British Columbia, Prince George, British Columbia V2N 4Z9, Canada
| | - Sebastian Mackedenski
- From the Chemistry Program, University of Northern British Columbia, Prince George, British Columbia V2N 4Z9, Canada
| | - Ching-Man Chan
- the Division of Life Science and The Key State Laboratory for Molecular Neuroscience, Hong Kong University of Science and Technology, Clear Water Bay, Kowloon, Hong Kong, and
| | - Dustin T King
- From the Chemistry Program, University of Northern British Columbia, Prince George, British Columbia V2N 4Z9, Canada
| | - Andrew L Miller
- the Division of Life Science and The Key State Laboratory for Molecular Neuroscience, Hong Kong University of Science and Technology, Clear Water Bay, Kowloon, Hong Kong, and the Marine Biological Laboratory, Woods Hole, Massachusetts 02543
| | - Chow H Lee
- From the Chemistry Program, University of Northern British Columbia, Prince George, British Columbia V2N 4Z9, Canada,
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108
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Han SY, Ahn KH, Lee CH, Hong SC, Oh MJ, Kim HJ. Concomitant therapy with hysterectomy and arterial embolisation for postpartum uterine haemorrhage. J OBSTET GYNAECOL 2014; 35:424-5. [PMID: 25207796 DOI: 10.3109/01443615.2014.954100] [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: 11/13/2022]
Affiliation(s)
- S Y Han
- Department of Obstetrics and Gynaecology, Korea University Medical Center, College of Medicine, Korea University , Seoul , South Korea
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Nakajima M, Ishida S, Tanaka T, Kihou K, Tomioka Y, Saito T, Lee CH, Fukazawa H, Kohori Y, Kakeshita T, Iyo A, Ito T, Eisaki H, Uchida S. Normal-state charge dynamics in doped BaFe₂As₂: roles of doping and necessary ingredients for superconductivity. Sci Rep 2014; 4:5873. [PMID: 25077444 PMCID: PMC5376192 DOI: 10.1038/srep05873] [Citation(s) in RCA: 39] [Impact Index Per Article: 3.9] [Reference Citation Analysis] [What about the content of this article? (0)] [Affiliation(s)] [Abstract] [Track Full Text] [Download PDF] [Figures] [Journal Information] [Subscribe] [Scholar Register] [Received: 01/28/2014] [Accepted: 07/11/2014] [Indexed: 11/30/2022] Open
Abstract
In high-transition-temperature superconducting cuprates and iron arsenides, chemical doping plays an important role in inducing superconductivity. Whereas in the cuprate case, the dominant role of doping is to inject charge carriers, the role for the iron arsenides is complex owing to carrier multiplicity and the diversity of doping. Here, we present a comparative study of the in-plane resistivity and the optical spectrum of doped BaFe2As2, which allows for separation of coherent (itinerant) and incoherent (highly dissipative) charge dynamics. The coherence of the system is controlled by doping, and the doping evolution of the charge dynamics exhibits a distinct difference between electron and hole doping. It is found in common with any type of doping that superconductivity with high transition temperature emerges when the normal-state charge dynamics maintains incoherence and when the resistivity associated with the coherent channel exhibits dominant temperature-linear dependence.
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Affiliation(s)
- M Nakajima
- 1] Department of Physics, University of Tokyo, Tokyo 113-0033, Japan [2] National Institute of Advanced Industrial Science and Technology, Tsukuba 305-8568, Japan [3] JST, Transformative Research-Project on Iron Pnictides (TRIP), Tokyo 102-0075, Japan [4]
| | - S Ishida
- 1] Department of Physics, University of Tokyo, Tokyo 113-0033, Japan [2] National Institute of Advanced Industrial Science and Technology, Tsukuba 305-8568, Japan [3] JST, Transformative Research-Project on Iron Pnictides (TRIP), Tokyo 102-0075, Japan
| | - T Tanaka
- 1] Department of Physics, University of Tokyo, Tokyo 113-0033, Japan [2] JST, Transformative Research-Project on Iron Pnictides (TRIP), Tokyo 102-0075, Japan
| | - K Kihou
- 1] National Institute of Advanced Industrial Science and Technology, Tsukuba 305-8568, Japan [2] JST, Transformative Research-Project on Iron Pnictides (TRIP), Tokyo 102-0075, Japan
| | - Y Tomioka
- 1] National Institute of Advanced Industrial Science and Technology, Tsukuba 305-8568, Japan [2] JST, Transformative Research-Project on Iron Pnictides (TRIP), Tokyo 102-0075, Japan
| | - T Saito
- Department of Physics, Chiba University, Chiba 263-8522, Japan
| | - C H Lee
- 1] National Institute of Advanced Industrial Science and Technology, Tsukuba 305-8568, Japan [2] JST, Transformative Research-Project on Iron Pnictides (TRIP), Tokyo 102-0075, Japan
| | - H Fukazawa
- 1] JST, Transformative Research-Project on Iron Pnictides (TRIP), Tokyo 102-0075, Japan [2] Department of Physics, Chiba University, Chiba 263-8522, Japan
| | - Y Kohori
- 1] JST, Transformative Research-Project on Iron Pnictides (TRIP), Tokyo 102-0075, Japan [2] Department of Physics, Chiba University, Chiba 263-8522, Japan
| | - T Kakeshita
- 1] Department of Physics, University of Tokyo, Tokyo 113-0033, Japan [2] JST, Transformative Research-Project on Iron Pnictides (TRIP), Tokyo 102-0075, Japan
| | - A Iyo
- 1] National Institute of Advanced Industrial Science and Technology, Tsukuba 305-8568, Japan [2] JST, Transformative Research-Project on Iron Pnictides (TRIP), Tokyo 102-0075, Japan
| | - T Ito
- 1] National Institute of Advanced Industrial Science and Technology, Tsukuba 305-8568, Japan [2] JST, Transformative Research-Project on Iron Pnictides (TRIP), Tokyo 102-0075, Japan
| | - H Eisaki
- 1] National Institute of Advanced Industrial Science and Technology, Tsukuba 305-8568, Japan [2] JST, Transformative Research-Project on Iron Pnictides (TRIP), Tokyo 102-0075, Japan
| | - S Uchida
- 1] Department of Physics, University of Tokyo, Tokyo 113-0033, Japan [2] JST, Transformative Research-Project on Iron Pnictides (TRIP), Tokyo 102-0075, Japan
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Seo JK, Park TS, Kwon IH, Piao MY, Lee CH, Ha JK. Characterization of Cellulolytic and Xylanolytic Enzymes of Bacillus licheniformis JK7 Isolated from the Rumen of a Native Korean Goat. Asian-Australas J Anim Sci 2014; 26:50-8. [PMID: 25049705 PMCID: PMC4093055 DOI: 10.5713/ajas.2012.12506] [Citation(s) in RCA: 51] [Impact Index Per Article: 5.1] [Reference Citation Analysis] [What about the content of this article? (0)] [Affiliation(s)] [Abstract] [Key Words] [Track Full Text] [Download PDF] [Figures] [Subscribe] [Scholar Register] [Received: 09/17/2012] [Revised: 11/02/2012] [Accepted: 10/26/2012] [Indexed: 12/01/2022]
Abstract
A facultative bacterium producing cellulolytic and hemicellulolytic enzymes was isolated from the rumen of a native Korean goat. The bacterium was identified as a Bacillus licheniformis on the basis of biochemical and morphological characteristics and 16S rDNA sequences, and has been designated Bacillus licheniformis JK7. Endoglucanase activities were higher than those of β-glucosidase and xylanase at all temperatures. Xylanase had the lowest activity among the three enzymes examined. The optimum temperature for the enzymes of Bacillus licheniformis JK7 was 70°C for endoglucanase (0.75 U/ml) and 50°C for β-glucosidase and xylanase (0.63 U/ml, 0.44 U/ml, respectively). All three enzymes were stable at a temperature range of 20 to 50°C. At 50°C, endoglucanse, β-glucosidase, and xylanase had 90.29, 94.80, and 88.69% residual activity, respectively. The optimal pH for the three enzymes was 5.0, at which their activity was 1.46, 1.10, and 1.08 U/ml, respectively. The activity of all three enzymes was stable in the pH range of 3.0 to 6.0. Endoglucanase activity was increased 113% by K+, while K+, Zn+, and tween 20 enhanced β-glucosidase activity. Xylanase showed considerable activity even in presence of selected chemical additives, with the exception of Mn2+ and Cu2+. The broad range of optimum temperatures (20 to 40°C) and the stability under acidic pH (4 to 6) suggest that the cellulolytic enzymes of Bacillus licheniformis JK7 may be good candidates for use in the biofuel industry.
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Affiliation(s)
- J K Seo
- Department of Agriculture Biotechnology, Research Institute for Agriculture and Life Sciences, College of Agriculture and Life Science, Seoul National University, Seoul 151-742, Korea
| | - T S Park
- Department of Agriculture Biotechnology, Research Institute for Agriculture and Life Sciences, College of Agriculture and Life Science, Seoul National University, Seoul 151-742, Korea
| | - I H Kwon
- Department of Agriculture Biotechnology, Research Institute for Agriculture and Life Sciences, College of Agriculture and Life Science, Seoul National University, Seoul 151-742, Korea
| | - M Y Piao
- Department of Agriculture Biotechnology, Research Institute for Agriculture and Life Sciences, College of Agriculture and Life Science, Seoul National University, Seoul 151-742, Korea
| | - C H Lee
- Department of Agriculture Biotechnology, Research Institute for Agriculture and Life Sciences, College of Agriculture and Life Science, Seoul National University, Seoul 151-742, Korea
| | - Jong K Ha
- Department of Agriculture Biotechnology, Research Institute for Agriculture and Life Sciences, College of Agriculture and Life Science, Seoul National University, Seoul 151-742, Korea
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Aasi J, Abbott BP, Abbott R, Abbott T, Abernathy MR, Acernese F, Ackley K, Adams C, Adams T, Addesso P, Adhikari RX, Affeldt C, Agathos M, Aggarwal N, Aguiar OD, Ajith P, Alemic A, Allen B, Allocca A, Amariutei D, Andersen M, Anderson RA, Anderson SB, Anderson WG, Arai K, Araya MC, Arceneaux C, Areeda JS, Ast S, Aston SM, Astone P, Aufmuth P, Augustus H, Aulbert C, Aylott BE, Babak S, Baker PT, Ballardin G, Ballmer SW, Barayoga JC, Barbet M, Barish BC, Barker D, Barone F, Barr B, Barsotti L, Barsuglia M, Barton MA, Bartos I, Bassiri R, Basti A, Batch JC, Bauchrowitz J, Bauer TS, Baune C, Bavigadda V, Behnke B, Bejger M, Beker MG, Belczynski C, Bell AS, Bell C, Bergmann G, Bersanetti D, Bertolini A, Betzwieser J, Bilenko IA, Billingsley G, Birch J, Biscans S, Bitossi M, Biwer C, Bizouard MA, Black E, Blackburn JK, Blackburn L, Blair D, Bloemen S, Bock O, Bodiya TP, Boer M, Bogaert G, Bogan C, Bond C, Bondu F, Bonelli L, Bonnand R, Bork R, Born M, Boschi V, Bose S, Bosi L, Bradaschia C, Brady PR, Braginsky VB, Branchesi M, Brau JE, Briant T, Bridges DO, Brillet A, Brinkmann M, Brisson V, Brooks AF, Brown DA, Brown DD, Brückner F, Buchman S, Buikema A, Bulik T, Bulten HJ, Buonanno A, Burman R, Buskulic D, Buy C, Cadonati L, Cagnoli G, Calderón Bustillo J, Calloni E, Camp JB, Campsie P, Cannon KC, Canuel B, Cao J, Capano CD, Carbognani F, Carbone L, Caride S, Castaldi G, Caudill S, Cavaglià M, Cavalier F, Cavalieri R, Celerier C, Cella G, Cepeda C, Cesarini E, Chakraborty R, Chalermsongsak T, Chamberlin SJ, Chao S, Charlton P, Chassande-Mottin E, Chen X, Chen Y, Chincarini A, Chiummo A, Cho HS, Cho M, Chow JH, Christensen N, Chu Q, Chua SSY, Chung S, Ciani G, Clara F, Clark DE, Clark JA, Clayton JH, Cleva F, Coccia E, Cohadon PF, Colla A, Collette C, Colombini M, Cominsky L, Constancio M, Conte A, Cook D, Corbitt TR, Cornish N, Corsi A, Costa CA, Coughlin MW, Coulon JP, Countryman S, Couvares P, Coward DM, Cowart MJ, Coyne DC, Coyne R, Craig K, Creighton JDE, Croce RP, Crowder SG, Cumming A, Cunningham L, Cuoco E, Cutler C, Dahl K, Dal Canton T, Damjanic M, Danilishin SL, D'Antonio S, Danzmann K, Dattilo V, Daveloza H, Davier M, Davies GS, Daw EJ, Day R, Dayanga T, DeBra D, Debreczeni G, Degallaix J, Deléglise S, Del Pozzo W, Denker T, Dent T, Dereli H, Dergachev V, De Rosa R, DeRosa RT, DeSalvo R, Dhurandhar S, Díaz M, Dickson J, Di Fiore L, Di Lieto A, Di Palma I, Di Virgilio A, Dolique V, Dominguez E, Donovan F, Dooley KL, Doravari S, Douglas R, Downes TP, Drago M, Drever RWP, Driggers JC, Du Z, Ducrot M, Dwyer S, Eberle T, Edo T, Edwards M, Effler A, Eggenstein HB, Ehrens P, Eichholz J, Eikenberry SS, Endrőczi G, Essick R, Etzel T, Evans M, Evans T, Factourovich M, Fafone V, Fairhurst S, Fan X, Fang Q, Farinon S, Farr B, Farr WM, Favata M, Fazi D, Fehrmann H, Fejer MM, Feldbaum D, Feroz F, Ferrante I, Ferreira EC, Ferrini F, Fidecaro F, Finn LS, Fiori I, Fisher RP, Flaminio R, Fournier JD, Franco S, Frasca S, Frasconi F, Frede M, Frei Z, Freise A, Frey R, Fricke TT, Fritschel P, Frolov VV, Fulda P, Fyffe M, Gair JR, Gammaitoni L, Gaonkar S, Garufi F, Gehrels N, Gemme G, Gendre B, Genin E, Gennai A, Ghosh S, Giaime JA, Giardina KD, Giazotto A, Gleason J, Goetz E, Goetz R, Gondan L, González G, Gordon N, Gorodetsky ML, Gossan S, Goßler S, Gouaty R, Gräf C, Graff PB, Granata M, Grant A, Gras S, Gray C, Greenhalgh RJS, Gretarsson AM, Groot P, Grote H, Grover K, Grunewald S, Guidi GM, Guido CJ, Gushwa K, Gustafson EK, Gustafson R, Ha J, Hall ED, Hamilton W, Hammer D, Hammond G, Hanke M, Hanks J, Hanna C, Hannam MD, Hanson J, Harms J, Harry GM, Harry IW, Harstad ED, Hart M, Hartman MT, Haster CJ, Haughian K, Heidmann A, Heintze M, Heitmann H, Hello P, Hemming G, Hendry M, Heng IS, Heptonstall AW, Heurs M, Hewitson M, Hild S, Hoak D, Hodge KA, Hofman D, Holt K, Hopkins P, Horrom T, Hoske D, Hosken DJ, Hough J, Howell EJ, Hu Y, Huerta E, Hughey B, Husa S, Huttner SH, Huynh M, Huynh-Dinh T, Idrisy A, Ingram DR, Inta R, Islas G, Isogai T, Ivanov A, Iyer BR, Izumi K, Jacobson M, Jang H, Jaranowski P, Ji Y, Jiménez-Forteza F, Johnson WW, Jones DI, Jones R, Jonker RJG, Ju L, Haris K, Kalmus P, Kalogera V, Kandhasamy S, Kang G, Kanner JB, Karlen J, Kasprzack M, Katsavounidis E, Katzman W, Kaufer H, Kaufer S, Kaur T, Kawabe K, Kawazoe F, Kéfélian F, Keiser GM, Keitel D, Kelley DB, Kells W, Keppel DG, Khalaidovski A, Khalili FY, Khazanov EA, Kim C, Kim K, Kim NG, Kim N, Kim S, Kim YM, King EJ, King PJ, Kinzel DL, Kissel JS, Klimenko S, Kline J, Koehlenbeck S, Kokeyama K, Kondrashov V, Koranda S, Korth WZ, Kowalska I, Kozak DB, Kringel V, Krishnan B, Królak A, Kuehn G, Kumar A, Kumar DN, Kumar P, Kumar R, Kuo L, Kutynia A, Lam PK, Landry M, Lantz B, Larson S, Lasky PD, Lazzarini A, Lazzaro C, Leaci P, Leavey S, Lebigot EO, Lee CH, Lee HK, Lee HM, Lee J, Lee PJ, Leonardi M, Leong JR, Leonor I, Le Roux A, Leroy N, Letendre N, Levin Y, Levine B, Lewis J, Li TGF, Libbrecht K, Libson A, Lin AC, Littenberg TB, Lockerbie NA, 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Search for gravitational waves associated with γ-ray bursts detected by the interplanetary network. Phys Rev Lett 2014; 113:011102. [PMID: 25032916 DOI: 10.1103/physrevlett.113.011102] [Citation(s) in RCA: 10] [Impact Index Per Article: 1.0] [Reference Citation Analysis] [What about the content of this article? (0)] [Affiliation(s)] [Abstract] [Track Full Text] [Subscribe] [Scholar Register] [Received: 04/07/2014] [Indexed: 05/21/2023]
Abstract
We present the results of a search for gravitational waves associated with 223 γ-ray bursts (GRBs) detected by the InterPlanetary Network (IPN) in 2005-2010 during LIGO's fifth and sixth science runs and Virgo's first, second, and third science runs. The IPN satellites provide accurate times of the bursts and sky localizations that vary significantly from degree scale to hundreds of square degrees. We search for both a well-modeled binary coalescence signal, the favored progenitor model for short GRBs, and for generic, unmodeled gravitational wave bursts. Both searches use the event time and sky localization to improve the gravitational wave search sensitivity as compared to corresponding all-time, all-sky searches. We find no evidence of a gravitational wave signal associated with any of the IPN GRBs in the sample, nor do we find evidence for a population of weak gravitational wave signals associated with the GRBs. For all IPN-detected GRBs, for which a sufficient duration of quality gravitational wave data are available, we place lower bounds on the distance to the source in accordance with an optimistic assumption of gravitational wave emission energy of 10(-2)M⊙c(2) at 150 Hz, and find a median of 13 Mpc. For the 27 short-hard GRBs we place 90% confidence exclusion distances to two source models: a binary neutron star coalescence, with a median distance of 12 Mpc, or the coalescence of a neutron star and black hole, with a median distance of 22 Mpc. Finally, we combine this search with previously published results to provide a population statement for GRB searches in first-generation LIGO and Virgo gravitational wave detectors and a resulting examination of prospects for the advanced gravitational wave detectors.
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Affiliation(s)
- J Aasi
- LIGO, California Institute of Technology, Pasadena, California 91125, USA
| | - B P Abbott
- LIGO, California Institute of Technology, Pasadena, California 91125, USA
| | - R Abbott
- LIGO, California Institute of Technology, Pasadena, California 91125, USA
| | - T Abbott
- Louisiana State University, Baton Rouge, Louisiana 70803, USA
| | - M R Abernathy
- LIGO, California Institute of Technology, Pasadena, California 91125, USA
| | - F Acernese
- Università di Salerno, Fisciano, I-84084 Salerno, Italy and INFN, Sezione di Napoli, Complesso Universitario di Monte S. Angelo, I-80126 Napoli, Italy
| | - K Ackley
- University of Florida, Gainesville, Florida 32611, USA
| | - C Adams
- LIGO Livingston Observatory, Livingston, Louisiana 70754, USA
| | - T Adams
- Cardiff University, Cardiff CF24 3AA, United Kingdom
| | - P Addesso
- University of Sannio at Benevento, I-82100 Benevento, Italy and INFN, Sezione di Napoli, I-80100 Napoli, Italy
| | - R X Adhikari
- LIGO, California Institute of Technology, Pasadena, California 91125, USA
| | - C Affeldt
- Albert-Einstein-Institut, Max-Planck-Institut für Gravitationsphysik, D-30167 Hannover, Germany
| | - M Agathos
- Nikhef, Science Park, 1098 XG Amsterdam, The Netherlands
| | - N Aggarwal
- LIGO, Massachusetts Institute of Technology, Cambridge, Massachusetts 02139, USA
| | - O D Aguiar
- Instituto Nacional de Pesquisas Espaciais, 12227-010 - São José dos Campos, São Paulo, Brazil
| | - P Ajith
- International Centre for Theoretical Sciences, Tata Institute of Fundamental Research, Bangalore 560012, India
| | - A Alemic
- Syracuse University, Syracuse, New York 13244, USA
| | - B Allen
- Albert-Einstein-Institut, Max-Planck-Institut für Gravitationsphysik, D-30167 Hannover, Germany and University of Wisconsin-Milwaukee, Milwaukee, Wisconsin 53201, USA and Leibniz Universität Hannover, D-30167 Hannover, Germany
| | - A Allocca
- Università di Siena, I-53100 Siena, Italy and INFN, Sezione di Pisa, I-56127 Pisa, Italy
| | - D Amariutei
- University of Florida, Gainesville, Florida 32611, USA
| | - M Andersen
- Stanford University, Stanford, California 94305, USA
| | - R A Anderson
- LIGO, California Institute of Technology, Pasadena, California 91125, USA
| | - S B Anderson
- LIGO, California Institute of Technology, Pasadena, California 91125, USA
| | - W G Anderson
- University of Wisconsin-Milwaukee, Milwaukee, Wisconsin 53201, USA
| | - K Arai
- LIGO, California Institute of Technology, Pasadena, California 91125, USA
| | - M C Araya
- LIGO, California Institute of Technology, Pasadena, California 91125, USA
| | - C Arceneaux
- The University of Mississippi, University, Mississippi 38677, USA
| | - J S Areeda
- California State University Fullerton, Fullerton, California 92831, USA
| | - S Ast
- Leibniz Universität Hannover, D-30167 Hannover, Germany
| | - S M Aston
- LIGO Livingston Observatory, Livingston, Louisiana 70754, USA
| | - P Astone
- INFN, Sezione di Roma, I-00185 Roma, Italy
| | - P Aufmuth
- Leibniz Universität Hannover, D-30167 Hannover, Germany
| | - H Augustus
- University of Birmingham, Birmingham B15 2TT, United Kingdom
| | - C Aulbert
- Albert-Einstein-Institut, Max-Planck-Institut für Gravitationsphysik, D-30167 Hannover, Germany
| | - B E Aylott
- University of Birmingham, Birmingham B15 2TT, United Kingdom
| | - S Babak
- Albert-Einstein-Institut, Max-Planck-Institut für Gravitationsphysik, D-14476 Golm, Germany
| | - P T Baker
- Montana State University, Bozeman, Montana 59717, USA
| | - G Ballardin
- European Gravitational Observatory (EGO), I-56021 Cascina, Pisa, Italy
| | - S W Ballmer
- Syracuse University, Syracuse, New York 13244, USA
| | - J C Barayoga
- LIGO, California Institute of Technology, Pasadena, California 91125, USA
| | - M Barbet
- University of Florida, Gainesville, Florida 32611, USA
| | - B C Barish
- LIGO, California Institute of Technology, Pasadena, California 91125, USA
| | - D Barker
- LIGO Hanford Observatory, Richland, Washington 99352, USA
| | - F Barone
- Università di Salerno, Fisciano, I-84084 Salerno, Italy and INFN, Sezione di Napoli, Complesso Universitario di Monte S. Angelo, I-80126 Napoli, Italy
| | - B Barr
- SUPA, University of Glasgow, Glasgow G12 8QQ, United Kingdom
| | - L Barsotti
- LIGO, Massachusetts Institute of Technology, Cambridge, Massachusetts 02139, USA
| | - M Barsuglia
- APC, AstroParticule et Cosmologie, Université Paris Diderot, CNRS/IN2P3, CEA/Irfu, Observatoire de Paris, Sorbonne Paris Cité, 10, rue Alice Domon et Léonie Duquet, F-75205 Paris Cedex 13, France
| | - M A Barton
- LIGO Hanford Observatory, Richland, Washington 99352, USA
| | - I Bartos
- Columbia University, New York, New York 10027, USA
| | - R Bassiri
- Stanford University, Stanford, California 94305, USA
| | - A Basti
- INFN, Sezione di Pisa, I-56127 Pisa, Italy and Università di Pisa, I-56127 Pisa, Italy
| | - J C Batch
- LIGO Hanford Observatory, Richland, Washington 99352, USA
| | - J Bauchrowitz
- Albert-Einstein-Institut, Max-Planck-Institut für Gravitationsphysik, D-30167 Hannover, Germany
| | - Th S Bauer
- Nikhef, Science Park, 1098 XG Amsterdam, The Netherlands
| | - C Baune
- Albert-Einstein-Institut, Max-Planck-Institut für Gravitationsphysik, D-30167 Hannover, Germany
| | - V Bavigadda
- European Gravitational Observatory (EGO), I-56021 Cascina, Pisa, Italy
| | - B Behnke
- Albert-Einstein-Institut, Max-Planck-Institut für Gravitationsphysik, D-14476 Golm, Germany
| | | | - M G Beker
- Nikhef, Science Park, 1098 XG Amsterdam, The Netherlands
| | - C Belczynski
- Astronomical Observatory Warsaw University, 00-478 Warsaw, Poland
| | - A S Bell
- SUPA, University of Glasgow, Glasgow G12 8QQ, United Kingdom
| | - C Bell
- SUPA, University of Glasgow, Glasgow G12 8QQ, United Kingdom
| | - G Bergmann
- Albert-Einstein-Institut, Max-Planck-Institut für Gravitationsphysik, D-30167 Hannover, Germany
| | - D Bersanetti
- Università degli Studi di Genova, I-16146 Genova, Italy and INFN, Sezione di Genova, I-16146 Genova, Italy
| | - A Bertolini
- Nikhef, Science Park, 1098 XG Amsterdam, The Netherlands
| | - J Betzwieser
- LIGO Livingston Observatory, Livingston, Louisiana 70754, USA
| | - I A Bilenko
- Faculty of Physics, Lomonosov Moscow State University, Moscow 119991, Russia
| | - G Billingsley
- LIGO, California Institute of Technology, Pasadena, California 91125, USA
| | - J Birch
- LIGO Livingston Observatory, Livingston, Louisiana 70754, USA
| | - S Biscans
- LIGO, Massachusetts Institute of Technology, Cambridge, Massachusetts 02139, USA
| | - M Bitossi
- INFN, Sezione di Pisa, I-56127 Pisa, Italy
| | - C Biwer
- Syracuse University, Syracuse, New York 13244, USA
| | - M A Bizouard
- LAL, Université Paris-Sud, IN2P3/CNRS, F-91898 Orsay, France
| | - E Black
- LIGO, California Institute of Technology, Pasadena, California 91125, USA
| | - J K Blackburn
- LIGO, California Institute of Technology, Pasadena, California 91125, USA
| | - L Blackburn
- NASA/Goddard Space Flight Center, Greenbelt, Maryland 20771, USA
| | - D Blair
- University of Western Australia, Crawley, Western Australia 6009, Australia
| | - S Bloemen
- Nikhef, Science Park, 1098 XG Amsterdam, The Netherlands and Department of Astrophysics/IMAPP, Radboud University Nijmegen, P.O. Box 9010, 6500 GL Nijmegen, The Netherlands
| | - O Bock
- Albert-Einstein-Institut, Max-Planck-Institut für Gravitationsphysik, D-30167 Hannover, Germany
| | - T P Bodiya
- LIGO, Massachusetts Institute of Technology, Cambridge, Massachusetts 02139, USA
| | - M Boer
- Université Nice-Sophia-Antipolis, CNRS, Observatoire de la Côte d'Azur, F-06304 Nice, France
| | - G Bogaert
- Université Nice-Sophia-Antipolis, CNRS, Observatoire de la Côte d'Azur, F-06304 Nice, France
| | - C Bogan
- Albert-Einstein-Institut, Max-Planck-Institut für Gravitationsphysik, D-30167 Hannover, Germany
| | - C Bond
- University of Birmingham, Birmingham B15 2TT, United Kingdom
| | - F Bondu
- Institut de Physique de Rennes, CNRS, Université de Rennes 1, F-35042 Rennes, France
| | - L Bonelli
- INFN, Sezione di Pisa, I-56127 Pisa, Italy and Università di Pisa, I-56127 Pisa, Italy
| | - R Bonnand
- Laboratoire d'Annecy-le-Vieux de Physique des Particules (LAPP), Université de Savoie, CNRS/IN2P3, F-74941 Annecy-le-Vieux, France
| | - R Bork
- LIGO, California Institute of Technology, Pasadena, California 91125, USA
| | - M Born
- Albert-Einstein-Institut, Max-Planck-Institut für Gravitationsphysik, D-30167 Hannover, Germany
| | - V Boschi
- INFN, Sezione di Pisa, I-56127 Pisa, Italy
| | - Sukanta Bose
- Washington State University, Pullman, Washington 99164, USA and Inter-University Centre for Astronomy and Astrophysics, Pune - 411007, India
| | - L Bosi
- INFN, Sezione di Perugia, I-06123 Perugia, Italy
| | | | - P R Brady
- University of Wisconsin-Milwaukee, Milwaukee, Wisconsin 53201, USA and Yukawa Institute for Theoretical Physics, Kyoto University, Kyoto 606-8502, Japan
| | - V B Braginsky
- Faculty of Physics, Lomonosov Moscow State University, Moscow 119991, Russia
| | - M Branchesi
- Università degli Studi di Urbino 'Carlo Bo', I-61029 Urbino, Italy and INFN, Sezione di Firenze, I-50019 Sesto Fiorentino, Firenze, Italy
| | - J E Brau
- University of Oregon, Eugene, Oregon 97403, USA
| | - T Briant
- Laboratoire Kastler Brossel, ENS, CNRS, UPMC, Université Pierre et Marie Curie, F-75005 Paris, France
| | - D O Bridges
- LIGO Livingston Observatory, Livingston, Louisiana 70754, USA
| | - A Brillet
- Université Nice-Sophia-Antipolis, CNRS, Observatoire de la Côte d'Azur, F-06304 Nice, France
| | - M Brinkmann
- Albert-Einstein-Institut, Max-Planck-Institut für Gravitationsphysik, D-30167 Hannover, Germany
| | - V Brisson
- LAL, Université Paris-Sud, IN2P3/CNRS, F-91898 Orsay, France
| | - A F Brooks
- LIGO, California Institute of Technology, Pasadena, California 91125, USA
| | - D A Brown
- Syracuse University, Syracuse, New York 13244, USA
| | - D D Brown
- University of Birmingham, Birmingham B15 2TT, United Kingdom
| | - F Brückner
- University of Birmingham, Birmingham B15 2TT, United Kingdom
| | - S Buchman
- Stanford University, Stanford, California 94305, USA
| | - A Buikema
- LIGO, Massachusetts Institute of Technology, Cambridge, Massachusetts 02139, USA
| | - T Bulik
- Astronomical Observatory Warsaw University, 00-478 Warsaw, Poland
| | - H J Bulten
- Nikhef, Science Park, 1098 XG Amsterdam, The Netherlands and VU University Amsterdam, 1081 HV Amsterdam, The Netherlands
| | - A Buonanno
- University of Maryland, College Park, Maryland 20742, USA
| | - R Burman
- University of Western Australia, Crawley, Western Australia 6009, Australia
| | - D Buskulic
- Laboratoire d'Annecy-le-Vieux de Physique des Particules (LAPP), Université de Savoie, CNRS/IN2P3, F-74941 Annecy-le-Vieux, France
| | - C Buy
- APC, AstroParticule et Cosmologie, Université Paris Diderot, CNRS/IN2P3, CEA/Irfu, Observatoire de Paris, Sorbonne Paris Cité, 10, rue Alice Domon et Léonie Duquet, F-75205 Paris Cedex 13, France
| | - L Cadonati
- Cardiff University, Cardiff CF24 3AA, United Kingdom and University of Massachusetts Amherst, Amherst, Massachusetts 01003, USA
| | - G Cagnoli
- Laboratoire des Matériaux Avancés (LMA), IN2P3/CNRS, Université de Lyon, F-69622 Villeurbanne, Lyon, France
| | | | - E Calloni
- INFN, Sezione di Napoli, Complesso Universitario di Monte S. Angelo, I-80126 Napoli, Italy and Università di Napoli 'Federico II', Complesso Universitario di Monte S. Angelo, I-80126 Napoli, Italy
| | - J B Camp
- NASA/Goddard Space Flight Center, Greenbelt, Maryland 20771, USA
| | - P Campsie
- SUPA, University of Glasgow, Glasgow G12 8QQ, United Kingdom
| | - K C Cannon
- Canadian Institute for Theoretical Astrophysics, University of Toronto, Toronto, Ontario, M5S 3H8, Canada
| | - B Canuel
- European Gravitational Observatory (EGO), I-56021 Cascina, Pisa, Italy
| | - J Cao
- Tsinghua University, Beijing 100084, China
| | - C D Capano
- University of Maryland, College Park, Maryland 20742, USA
| | - F Carbognani
- European Gravitational Observatory (EGO), I-56021 Cascina, Pisa, Italy
| | - L Carbone
- University of Birmingham, Birmingham B15 2TT, United Kingdom
| | - S Caride
- University of Michigan, Ann Arbor, Michigan 48109, USA
| | - G Castaldi
- University of Sannio at Benevento, I-82100 Benevento, Italy and INFN, Sezione di Napoli, I-80100 Napoli, Italy
| | - S Caudill
- University of Wisconsin-Milwaukee, Milwaukee, Wisconsin 53201, USA
| | - M Cavaglià
- The University of Mississippi, University, Mississippi 38677, USA
| | - F Cavalier
- LAL, Université Paris-Sud, IN2P3/CNRS, F-91898 Orsay, France
| | - R Cavalieri
- European Gravitational Observatory (EGO), I-56021 Cascina, Pisa, Italy
| | - C Celerier
- Stanford University, Stanford, California 94305, USA
| | - G Cella
- INFN, Sezione di Pisa, I-56127 Pisa, Italy
| | - C Cepeda
- LIGO, California Institute of Technology, Pasadena, California 91125, USA
| | - E Cesarini
- INFN, Sezione di Roma Tor Vergata, I-00133 Roma, Italy
| | - R Chakraborty
- LIGO, California Institute of Technology, Pasadena, California 91125, USA
| | - T Chalermsongsak
- LIGO, California Institute of Technology, Pasadena, California 91125, USA
| | - S J Chamberlin
- University of Wisconsin-Milwaukee, Milwaukee, Wisconsin 53201, USA
| | - S Chao
- National Tsing Hua University, Hsinchu 300, Taiwan
| | - P Charlton
- Charles Sturt University, Wagga Wagga, New South Wales 2678, Australia
| | - E Chassande-Mottin
- APC, AstroParticule et Cosmologie, Université Paris Diderot, CNRS/IN2P3, CEA/Irfu, Observatoire de Paris, Sorbonne Paris Cité, 10, rue Alice Domon et Léonie Duquet, F-75205 Paris Cedex 13, France
| | - X Chen
- University of Western Australia, Crawley, Western Australia 6009, Australia
| | - Y Chen
- Caltech-CaRT, Pasadena, California 91125, USA
| | | | - A Chiummo
- European Gravitational Observatory (EGO), I-56021 Cascina, Pisa, Italy
| | - H S Cho
- Pusan National University, Busan 609-735, Korea
| | - M Cho
- University of Maryland, College Park, Maryland 20742, USA
| | - J H Chow
- Australian National University, Canberra, ACT 0200, Australia
| | | | - Q Chu
- University of Western Australia, Crawley, Western Australia 6009, Australia
| | - S S Y Chua
- Australian National University, Canberra, ACT 0200, Australia
| | - S Chung
- University of Western Australia, Crawley, Western Australia 6009, Australia
| | - G Ciani
- University of Florida, Gainesville, Florida 32611, USA
| | - F Clara
- LIGO Hanford Observatory, Richland, Washington 99352, USA
| | - D E Clark
- Stanford University, Stanford, California 94305, USA
| | - J A Clark
- University of Massachusetts Amherst, Amherst, Massachusetts 01003, USA
| | - J H Clayton
- University of Wisconsin-Milwaukee, Milwaukee, Wisconsin 53201, USA
| | - F Cleva
- Université Nice-Sophia-Antipolis, CNRS, Observatoire de la Côte d'Azur, F-06304 Nice, France
| | - E Coccia
- Università di Roma Tor Vergata, I-00133 Roma, Italy and INFN, Gran Sasso Science Institute, I-67100 L'Aquila, Italy
| | - P-F Cohadon
- Laboratoire Kastler Brossel, ENS, CNRS, UPMC, Université Pierre et Marie Curie, F-75005 Paris, France
| | - A Colla
- INFN, Sezione di Roma, I-00185 Roma, Italy and Università di Roma 'La Sapienza', I-00185 Roma, Italy
| | - C Collette
- University of Brussels, Brussels 1050, Belgium
| | - M Colombini
- INFN, Sezione di Perugia, I-06123 Perugia, Italy
| | - L Cominsky
- Sonoma State University, Rohnert Park, California 94928, USA
| | - M Constancio
- Instituto Nacional de Pesquisas Espaciais, 12227-010 - São José dos Campos, São Paulo, Brazil
| | - A Conte
- INFN, Sezione di Roma, I-00185 Roma, Italy and Università di Roma 'La Sapienza', I-00185 Roma, Italy
| | - D Cook
- LIGO Hanford Observatory, Richland, Washington 99352, USA
| | - T R Corbitt
- Louisiana State University, Baton Rouge, Louisiana 70803, USA
| | - N Cornish
- Montana State University, Bozeman, Montana 59717, USA
| | - A Corsi
- The George Washington University, Washington, DC 20052, USA
| | - C A Costa
- Instituto Nacional de Pesquisas Espaciais, 12227-010 - São José dos Campos, São Paulo, Brazil
| | - M W Coughlin
- University of Cambridge, Cambridge CB2 1TN, United Kingdom
| | - J-P Coulon
- Université Nice-Sophia-Antipolis, CNRS, Observatoire de la Côte d'Azur, F-06304 Nice, France
| | - S Countryman
- Columbia University, New York, New York 10027, USA
| | - P Couvares
- Syracuse University, Syracuse, New York 13244, USA
| | - D M Coward
- University of Western Australia, Crawley, Western Australia 6009, Australia
| | - M J Cowart
- LIGO Livingston Observatory, Livingston, Louisiana 70754, USA
| | - D C Coyne
- LIGO, California Institute of Technology, Pasadena, California 91125, USA
| | - R Coyne
- The George Washington University, Washington, DC 20052, USA
| | - K Craig
- SUPA, University of Glasgow, Glasgow G12 8QQ, United Kingdom
| | - J D E Creighton
- University of Wisconsin-Milwaukee, Milwaukee, Wisconsin 53201, USA
| | - R P Croce
- University of Sannio at Benevento, I-82100 Benevento, Italy and INFN, Sezione di Napoli, I-80100 Napoli, Italy
| | - S G Crowder
- University of Minnesota, Minneapolis, Minnesota 55455, USA
| | - A Cumming
- SUPA, University of Glasgow, Glasgow G12 8QQ, United Kingdom
| | - L Cunningham
- SUPA, University of Glasgow, Glasgow G12 8QQ, United Kingdom
| | - E Cuoco
- European Gravitational Observatory (EGO), I-56021 Cascina, Pisa, Italy
| | - C Cutler
- Caltech-CaRT, Pasadena, California 91125, USA
| | - K Dahl
- Albert-Einstein-Institut, Max-Planck-Institut für Gravitationsphysik, D-30167 Hannover, Germany
| | - T Dal Canton
- Albert-Einstein-Institut, Max-Planck-Institut für Gravitationsphysik, D-30167 Hannover, Germany
| | - M Damjanic
- Albert-Einstein-Institut, Max-Planck-Institut für Gravitationsphysik, D-30167 Hannover, Germany
| | - S L Danilishin
- University of Western Australia, Crawley, Western Australia 6009, Australia
| | - S D'Antonio
- INFN, Sezione di Roma Tor Vergata, I-00133 Roma, Italy
| | - K Danzmann
- Albert-Einstein-Institut, Max-Planck-Institut für Gravitationsphysik, D-30167 Hannover, Germany and Leibniz Universität Hannover, D-30167 Hannover, Germany
| | - V Dattilo
- European Gravitational Observatory (EGO), I-56021 Cascina, Pisa, Italy
| | - H Daveloza
- The University of Texas at Brownsville, Brownsville, Texas 78520, USA
| | - M Davier
- LAL, Université Paris-Sud, IN2P3/CNRS, F-91898 Orsay, France
| | - G S Davies
- SUPA, University of Glasgow, Glasgow G12 8QQ, United Kingdom
| | - E J Daw
- The University of Sheffield, Sheffield S10 2TN, United Kingdom
| | - R Day
- European Gravitational Observatory (EGO), I-56021 Cascina, Pisa, Italy
| | - T Dayanga
- Washington State University, Pullman, Washington 99164, USA
| | - D DeBra
- Stanford University, Stanford, California 94305, USA
| | - G Debreczeni
- Wigner RCP, RMKI, H-1121 Budapest, Konkoly Thege Miklós út 29-33, Hungary
| | - J Degallaix
- Laboratoire des Matériaux Avancés (LMA), IN2P3/CNRS, Université de Lyon, F-69622 Villeurbanne, Lyon, France
| | - S Deléglise
- Laboratoire Kastler Brossel, ENS, CNRS, UPMC, Université Pierre et Marie Curie, F-75005 Paris, France
| | - W Del Pozzo
- Nikhef, Science Park, 1098 XG Amsterdam, The Netherlands and University of Birmingham, Birmingham B15 2TT, United Kingdom
| | - T Denker
- Albert-Einstein-Institut, Max-Planck-Institut für Gravitationsphysik, D-30167 Hannover, Germany
| | - T Dent
- Albert-Einstein-Institut, Max-Planck-Institut für Gravitationsphysik, D-30167 Hannover, Germany
| | - H Dereli
- Université Nice-Sophia-Antipolis, CNRS, Observatoire de la Côte d'Azur, F-06304 Nice, France
| | - V Dergachev
- LIGO, California Institute of Technology, Pasadena, California 91125, USA
| | - R De Rosa
- INFN, Sezione di Napoli, Complesso Universitario di Monte S. Angelo, I-80126 Napoli, Italy and Università di Napoli 'Federico II', Complesso Universitario di Monte S. Angelo, I-80126 Napoli, Italy
| | - R T DeRosa
- Louisiana State University, Baton Rouge, Louisiana 70803, USA
| | - R DeSalvo
- University of Sannio at Benevento, I-82100 Benevento, Italy and INFN, Sezione di Napoli, I-80100 Napoli, Italy
| | - S Dhurandhar
- Inter-University Centre for Astronomy and Astrophysics, Pune - 411007, India
| | - M Díaz
- The University of Texas at Brownsville, Brownsville, Texas 78520, USA
| | - J Dickson
- Australian National University, Canberra, ACT 0200, Australia
| | - L Di Fiore
- INFN, Sezione di Napoli, Complesso Universitario di Monte S. Angelo, I-80126 Napoli, Italy
| | - A Di Lieto
- INFN, Sezione di Pisa, I-56127 Pisa, Italy and Università di Pisa, I-56127 Pisa, Italy
| | - I Di Palma
- Albert-Einstein-Institut, Max-Planck-Institut für Gravitationsphysik, D-30167 Hannover, Germany
| | | | - V Dolique
- Laboratoire des Matériaux Avancés (LMA), IN2P3/CNRS, Université de Lyon, F-69622 Villeurbanne, Lyon, France
| | - E Dominguez
- Argentinian Gravitational Wave Group, Cordoba Cordoba 5000, Argentina
| | - F Donovan
- LIGO, Massachusetts Institute of Technology, Cambridge, Massachusetts 02139, USA
| | - K L Dooley
- Albert-Einstein-Institut, Max-Planck-Institut für Gravitationsphysik, D-30167 Hannover, Germany
| | - S Doravari
- LIGO Livingston Observatory, Livingston, Louisiana 70754, USA
| | - R Douglas
- SUPA, University of Glasgow, Glasgow G12 8QQ, United Kingdom
| | - T P Downes
- University of Wisconsin-Milwaukee, Milwaukee, Wisconsin 53201, USA
| | - M Drago
- Università di Trento, I-38050 Povo, Trento, Italy and INFN, Gruppo Collegato di Trento, I-38050 Povo, Trento, Italy
| | - R W P Drever
- LIGO, California Institute of Technology, Pasadena, California 91125, USA
| | - J C Driggers
- LIGO, California Institute of Technology, Pasadena, California 91125, USA
| | - Z Du
- Tsinghua University, Beijing 100084, China
| | - M Ducrot
- Laboratoire d'Annecy-le-Vieux de Physique des Particules (LAPP), Université de Savoie, CNRS/IN2P3, F-74941 Annecy-le-Vieux, France
| | - S Dwyer
- LIGO Hanford Observatory, Richland, Washington 99352, USA
| | - T Eberle
- Albert-Einstein-Institut, Max-Planck-Institut für Gravitationsphysik, D-30167 Hannover, Germany
| | - T Edo
- The University of Sheffield, Sheffield S10 2TN, United Kingdom
| | - M Edwards
- Cardiff University, Cardiff CF24 3AA, United Kingdom
| | - A Effler
- Louisiana State University, Baton Rouge, Louisiana 70803, USA
| | - H-B Eggenstein
- Albert-Einstein-Institut, Max-Planck-Institut für Gravitationsphysik, D-30167 Hannover, Germany
| | - P Ehrens
- LIGO, California Institute of Technology, Pasadena, California 91125, USA
| | - J Eichholz
- University of Florida, Gainesville, Florida 32611, USA
| | | | - G Endrőczi
- Wigner RCP, RMKI, H-1121 Budapest, Konkoly Thege Miklós út 29-33, Hungary
| | - R Essick
- LIGO, Massachusetts Institute of Technology, Cambridge, Massachusetts 02139, USA
| | - T Etzel
- LIGO, California Institute of Technology, Pasadena, California 91125, USA
| | - M Evans
- LIGO, Massachusetts Institute of Technology, Cambridge, Massachusetts 02139, USA
| | - T Evans
- LIGO Livingston Observatory, Livingston, Louisiana 70754, USA
| | | | - V Fafone
- INFN, Sezione di Roma Tor Vergata, I-00133 Roma, Italy and Università di Roma Tor Vergata, I-00133 Roma, Italy
| | - S Fairhurst
- Cardiff University, Cardiff CF24 3AA, United Kingdom
| | - X Fan
- SUPA, University of Glasgow, Glasgow G12 8QQ, United Kingdom
| | - Q Fang
- University of Western Australia, Crawley, Western Australia 6009, Australia
| | - S Farinon
- INFN, Sezione di Genova, I-16146 Genova, Italy
| | - B Farr
- Northwestern University, Evanston, Illinois 60208, USA
| | - W M Farr
- University of Birmingham, Birmingham B15 2TT, United Kingdom
| | - M Favata
- Montclair State University, Montclair, New Jersey 07043, USA
| | - D Fazi
- Northwestern University, Evanston, Illinois 60208, USA
| | - H Fehrmann
- Albert-Einstein-Institut, Max-Planck-Institut für Gravitationsphysik, D-30167 Hannover, Germany
| | - M M Fejer
- Stanford University, Stanford, California 94305, USA
| | - D Feldbaum
- University of Florida, Gainesville, Florida 32611, USA and LIGO Livingston Observatory, Livingston, Louisiana 70754, USA
| | - F Feroz
- University of Cambridge, Cambridge CB2 1TN, United Kingdom
| | - I Ferrante
- INFN, Sezione di Pisa, I-56127 Pisa, Italy and Università di Pisa, I-56127 Pisa, Italy
| | - E C Ferreira
- Instituto Nacional de Pesquisas Espaciais, 12227-010 - São José dos Campos, São Paulo, Brazil
| | - F Ferrini
- European Gravitational Observatory (EGO), I-56021 Cascina, Pisa, Italy
| | - F Fidecaro
- INFN, Sezione di Pisa, I-56127 Pisa, Italy and Università di Pisa, I-56127 Pisa, Italy
| | - L S Finn
- The Pennsylvania State University, University Park, Pennsylvania 16802, USA
| | - I Fiori
- European Gravitational Observatory (EGO), I-56021 Cascina, Pisa, Italy
| | - R P Fisher
- Syracuse University, Syracuse, New York 13244, USA
| | - R Flaminio
- Laboratoire des Matériaux Avancés (LMA), IN2P3/CNRS, Université de Lyon, F-69622 Villeurbanne, Lyon, France
| | - J-D Fournier
- Université Nice-Sophia-Antipolis, CNRS, Observatoire de la Côte d'Azur, F-06304 Nice, France
| | - S Franco
- LAL, Université Paris-Sud, IN2P3/CNRS, F-91898 Orsay, France
| | - S Frasca
- INFN, Sezione di Roma, I-00185 Roma, Italy and Università di Roma 'La Sapienza', I-00185 Roma, Italy
| | - F Frasconi
- INFN, Sezione di Pisa, I-56127 Pisa, Italy
| | - M Frede
- Albert-Einstein-Institut, Max-Planck-Institut für Gravitationsphysik, D-30167 Hannover, Germany
| | - Z Frei
- MTA Eötvös University, 'Lendulet' A. R. G., Budapest 1117, Hungary
| | - A Freise
- University of Birmingham, Birmingham B15 2TT, United Kingdom
| | - R Frey
- University of Oregon, Eugene, Oregon 97403, USA
| | - T T Fricke
- Albert-Einstein-Institut, Max-Planck-Institut für Gravitationsphysik, D-30167 Hannover, Germany
| | - P Fritschel
- LIGO, Massachusetts Institute of Technology, Cambridge, Massachusetts 02139, USA
| | - V V Frolov
- LIGO Livingston Observatory, Livingston, Louisiana 70754, USA
| | - P Fulda
- University of Florida, Gainesville, Florida 32611, USA
| | - M Fyffe
- LIGO Livingston Observatory, Livingston, Louisiana 70754, USA
| | - J R Gair
- University of Cambridge, Cambridge CB2 1TN, United Kingdom
| | - L Gammaitoni
- INFN, Sezione di Perugia, I-06123 Perugia, Italy and Università di Perugia, I-06123 Perugia, Italy
| | - S Gaonkar
- Inter-University Centre for Astronomy and Astrophysics, Pune - 411007, India
| | - F Garufi
- INFN, Sezione di Napoli, Complesso Universitario di Monte S. Angelo, I-80126 Napoli, Italy and Università di Napoli 'Federico II', Complesso Universitario di Monte S. Angelo, I-80126 Napoli, Italy
| | - N Gehrels
- NASA/Goddard Space Flight Center, Greenbelt, Maryland 20771, USA
| | - G Gemme
- INFN, Sezione di Genova, I-16146 Genova, Italy
| | - B Gendre
- Université Nice-Sophia-Antipolis, CNRS, Observatoire de la Côte d'Azur, F-06304 Nice, France
| | - E Genin
- European Gravitational Observatory (EGO), I-56021 Cascina, Pisa, Italy
| | - A Gennai
- INFN, Sezione di Pisa, I-56127 Pisa, Italy
| | - S Ghosh
- Nikhef, Science Park, 1098 XG Amsterdam, The Netherlands and Department of Astrophysics/IMAPP, Radboud University Nijmegen, P.O. Box 9010, 6500 GL Nijmegen, The Netherlands
| | - J A Giaime
- Louisiana State University, Baton Rouge, Louisiana 70803, USA and LIGO Livingston Observatory, Livingston, Louisiana 70754, USA
| | - K D Giardina
- LIGO Livingston Observatory, Livingston, Louisiana 70754, USA
| | - A Giazotto
- INFN, Sezione di Pisa, I-56127 Pisa, Italy
| | - J Gleason
- University of Florida, Gainesville, Florida 32611, USA
| | - E Goetz
- Albert-Einstein-Institut, Max-Planck-Institut für Gravitationsphysik, D-30167 Hannover, Germany
| | - R Goetz
- University of Florida, Gainesville, Florida 32611, USA
| | - L Gondan
- MTA Eötvös University, 'Lendulet' A. R. G., Budapest 1117, Hungary
| | - G González
- Louisiana State University, Baton Rouge, Louisiana 70803, USA
| | - N Gordon
- SUPA, University of Glasgow, Glasgow G12 8QQ, United Kingdom
| | - M L Gorodetsky
- Faculty of Physics, Lomonosov Moscow State University, Moscow 119991, Russia
| | - S Gossan
- Caltech-CaRT, Pasadena, California 91125, USA
| | - S Goßler
- Albert-Einstein-Institut, Max-Planck-Institut für Gravitationsphysik, D-30167 Hannover, Germany
| | - R Gouaty
- Laboratoire d'Annecy-le-Vieux de Physique des Particules (LAPP), Université de Savoie, CNRS/IN2P3, F-74941 Annecy-le-Vieux, France
| | - C Gräf
- SUPA, University of Glasgow, Glasgow G12 8QQ, United Kingdom
| | - P B Graff
- NASA/Goddard Space Flight Center, Greenbelt, Maryland 20771, USA
| | - M Granata
- Laboratoire des Matériaux Avancés (LMA), IN2P3/CNRS, Université de Lyon, F-69622 Villeurbanne, Lyon, France
| | - A Grant
- SUPA, University of Glasgow, Glasgow G12 8QQ, United Kingdom
| | - S Gras
- LIGO, Massachusetts Institute of Technology, Cambridge, Massachusetts 02139, USA
| | - C Gray
- LIGO Hanford Observatory, Richland, Washington 99352, USA
| | - R J S Greenhalgh
- Rutherford Appleton Laboratory, HSIC, Chilton, Didcot, Oxon OX11 0QX, United Kingdom
| | - A M Gretarsson
- Embry-Riddle Aeronautical University, Prescott, Arizona 86301, USA
| | - P Groot
- Department of Astrophysics/IMAPP, Radboud University Nijmegen, P.O. Box 9010, 6500 GL Nijmegen, The Netherlands
| | - H Grote
- Albert-Einstein-Institut, Max-Planck-Institut für Gravitationsphysik, D-30167 Hannover, Germany
| | - K Grover
- University of Birmingham, Birmingham B15 2TT, United Kingdom
| | - S Grunewald
- Albert-Einstein-Institut, Max-Planck-Institut für Gravitationsphysik, D-14476 Golm, Germany
| | - G M Guidi
- Università degli Studi di Urbino 'Carlo Bo', I-61029 Urbino, Italy and INFN, Sezione di Firenze, I-50019 Sesto Fiorentino, Firenze, Italy
| | - C J Guido
- LIGO Livingston Observatory, Livingston, Louisiana 70754, USA
| | - K Gushwa
- LIGO, California Institute of Technology, Pasadena, California 91125, USA
| | - E K Gustafson
- LIGO, California Institute of Technology, Pasadena, California 91125, USA
| | - R Gustafson
- University of Michigan, Ann Arbor, Michigan 48109, USA
| | - J Ha
- Seoul National University, Seoul 151-742, Korea
| | - E D Hall
- LIGO, California Institute of Technology, Pasadena, California 91125, USA
| | - W Hamilton
- Louisiana State University, Baton Rouge, Louisiana 70803, USA
| | - D Hammer
- University of Wisconsin-Milwaukee, Milwaukee, Wisconsin 53201, USA
| | - G Hammond
- SUPA, University of Glasgow, Glasgow G12 8QQ, United Kingdom
| | - M Hanke
- Albert-Einstein-Institut, Max-Planck-Institut für Gravitationsphysik, D-30167 Hannover, Germany
| | - J Hanks
- LIGO Hanford Observatory, Richland, Washington 99352, USA
| | - C Hanna
- The Pennsylvania State University, University Park, Pennsylvania 16802, USA and Perimeter Institute for Theoretical Physics, Waterloo, Ontario N2 L 2Y5, Canada
| | - M D Hannam
- Cardiff University, Cardiff CF24 3AA, United Kingdom
| | - J Hanson
- LIGO Livingston Observatory, Livingston, Louisiana 70754, USA
| | - J Harms
- LIGO, California Institute of Technology, Pasadena, California 91125, USA
| | - G M Harry
- American University, Washington, DC 20016, USA
| | - I W Harry
- Syracuse University, Syracuse, New York 13244, USA
| | - E D Harstad
- University of Oregon, Eugene, Oregon 97403, USA
| | - M Hart
- SUPA, University of Glasgow, Glasgow G12 8QQ, United Kingdom
| | - M T Hartman
- University of Florida, Gainesville, Florida 32611, USA
| | - C-J Haster
- University of Birmingham, Birmingham B15 2TT, United Kingdom
| | - K Haughian
- SUPA, University of Glasgow, Glasgow G12 8QQ, United Kingdom
| | - A Heidmann
- Laboratoire Kastler Brossel, ENS, CNRS, UPMC, Université Pierre et Marie Curie, F-75005 Paris, France
| | - M Heintze
- University of Florida, Gainesville, Florida 32611, USA and LIGO Livingston Observatory, Livingston, Louisiana 70754, USA
| | - H Heitmann
- Université Nice-Sophia-Antipolis, CNRS, Observatoire de la Côte d'Azur, F-06304 Nice, France
| | - P Hello
- LAL, Université Paris-Sud, IN2P3/CNRS, F-91898 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
| | - A W Heptonstall
- LIGO, California Institute of Technology, Pasadena, California 91125, USA
| | - M Heurs
- Albert-Einstein-Institut, Max-Planck-Institut für Gravitationsphysik, D-30167 Hannover, Germany
| | - M Hewitson
- Albert-Einstein-Institut, Max-Planck-Institut für Gravitationsphysik, D-30167 Hannover, Germany
| | - S Hild
- SUPA, University of Glasgow, Glasgow G12 8QQ, United Kingdom
| | - D Hoak
- University of Massachusetts Amherst, Amherst, Massachusetts 01003, USA
| | - K A Hodge
- LIGO, California Institute of Technology, Pasadena, California 91125, USA
| | - D Hofman
- Laboratoire des Matériaux Avancés (LMA), IN2P3/CNRS, Université de Lyon, F-69622 Villeurbanne, Lyon, France
| | - K Holt
- LIGO Livingston Observatory, Livingston, Louisiana 70754, USA
| | - P Hopkins
- Cardiff University, Cardiff CF24 3AA, United Kingdom
| | - T Horrom
- College of William and Mary, Williamsburg, Virginia 23187, USA
| | - D Hoske
- University of Adelaide, Adelaide, South Australia 5005, Australia
| | - D J Hosken
- University of Adelaide, Adelaide, South Australia 5005, Australia
| | - J Hough
- SUPA, University of Glasgow, Glasgow G12 8QQ, United Kingdom
| | - E J Howell
- University of Western Australia, Crawley, Western Australia 6009, Australia
| | - Y Hu
- SUPA, University of Glasgow, Glasgow G12 8QQ, United Kingdom
| | - E Huerta
- Syracuse University, Syracuse, New York 13244, USA
| | - B Hughey
- Embry-Riddle Aeronautical University, Prescott, Arizona 86301, USA
| | - S Husa
- Universitat de les Illes Balears, E-07122 Palma de Mallorca, Spain
| | - S H Huttner
- SUPA, University of Glasgow, Glasgow G12 8QQ, United Kingdom
| | - M Huynh
- University of Wisconsin-Milwaukee, Milwaukee, Wisconsin 53201, USA
| | - T Huynh-Dinh
- LIGO Livingston Observatory, Livingston, Louisiana 70754, USA
| | - A Idrisy
- The Pennsylvania State University, University Park, Pennsylvania 16802, USA
| | - D R Ingram
- LIGO Hanford Observatory, Richland, Washington 99352, USA
| | - R Inta
- The Pennsylvania State University, University Park, Pennsylvania 16802, USA
| | - G Islas
- California State University Fullerton, Fullerton, California 92831, USA
| | - T Isogai
- LIGO, Massachusetts Institute of Technology, Cambridge, Massachusetts 02139, USA
| | - A Ivanov
- LIGO, California Institute of Technology, Pasadena, California 91125, USA
| | - B R Iyer
- Raman Research Institute, Bangalore, Karnataka 560080, India
| | - K Izumi
- LIGO Hanford Observatory, Richland, Washington 99352, USA
| | - M Jacobson
- LIGO, California Institute of Technology, Pasadena, California 91125, USA
| | - H Jang
- Korea Institute of Science and Technology Information, Daejeon 305-806, Korea
| | | | - Y Ji
- Tsinghua University, Beijing 100084, China
| | | | - W W Johnson
- Louisiana State University, Baton Rouge, Louisiana 70803, USA
| | - D I Jones
- University of Southampton, Southampton SO17 1BJ, United Kingdom
| | - R Jones
- SUPA, University of Glasgow, Glasgow G12 8QQ, United Kingdom
| | - R J G Jonker
- Nikhef, Science Park, 1098 XG Amsterdam, The Netherlands
| | - L Ju
- University of Western Australia, Crawley, Western Australia 6009, Australia
| | - K Haris
- IISER-TVM, CET Campus, Trivandrum, Kerala 695016, India
| | - P Kalmus
- LIGO, California Institute of Technology, Pasadena, California 91125, USA
| | - V Kalogera
- Northwestern University, Evanston, Illinois 60208, USA
| | - S Kandhasamy
- The University of Mississippi, University, Mississippi 38677, USA
| | - G Kang
- Korea Institute of Science and Technology Information, Daejeon 305-806, Korea
| | - J B Kanner
- LIGO, California Institute of Technology, Pasadena, California 91125, USA
| | - J Karlen
- University of Massachusetts Amherst, Amherst, Massachusetts 01003, USA
| | - M Kasprzack
- European Gravitational Observatory (EGO), I-56021 Cascina, Pisa, Italy and LAL, Université Paris-Sud, IN2P3/CNRS, F-91898 Orsay, France
| | - E Katsavounidis
- LIGO, Massachusetts Institute of Technology, Cambridge, Massachusetts 02139, USA
| | - W Katzman
- LIGO Livingston Observatory, Livingston, Louisiana 70754, USA
| | - H Kaufer
- Leibniz Universität Hannover, D-30167 Hannover, Germany
| | - S Kaufer
- Leibniz Universität Hannover, D-30167 Hannover, Germany
| | - T Kaur
- University of Western Australia, Crawley, Western Australia 6009, Australia
| | - K Kawabe
- LIGO Hanford Observatory, Richland, Washington 99352, USA
| | - F Kawazoe
- Albert-Einstein-Institut, Max-Planck-Institut für Gravitationsphysik, D-30167 Hannover, Germany
| | - F Kéfélian
- Université Nice-Sophia-Antipolis, CNRS, Observatoire de la Côte d'Azur, F-06304 Nice, France
| | - G M Keiser
- Stanford University, Stanford, California 94305, USA
| | - D Keitel
- Albert-Einstein-Institut, Max-Planck-Institut für Gravitationsphysik, D-30167 Hannover, Germany
| | - D B Kelley
- Syracuse University, Syracuse, New York 13244, USA
| | - W Kells
- LIGO, California Institute of Technology, Pasadena, California 91125, USA
| | - D G Keppel
- Albert-Einstein-Institut, Max-Planck-Institut für Gravitationsphysik, D-30167 Hannover, Germany
| | - A Khalaidovski
- Albert-Einstein-Institut, Max-Planck-Institut für Gravitationsphysik, D-30167 Hannover, Germany
| | - F Y Khalili
- Faculty of Physics, Lomonosov Moscow State University, Moscow 119991, Russia
| | - E A Khazanov
- Institute of Applied Physics, Nizhny Novgorod 603950, Russia
| | - C Kim
- Seoul National University, Seoul 151-742, Korea and Korea Institute of Science and Technology Information, Daejeon 305-806, Korea
| | - K Kim
- Hanyang University, Seoul 133-791, Korea
| | - N G Kim
- Korea Institute of Science and Technology Information, Daejeon 305-806, Korea
| | - N Kim
- Stanford University, Stanford, California 94305, USA
| | - S Kim
- Korea Institute of Science and Technology Information, Daejeon 305-806, Korea
| | - Y-M Kim
- Pusan National University, Busan 609-735, Korea
| | - E J King
- University of Adelaide, Adelaide, South Australia 5005, Australia
| | - P J King
- LIGO, California Institute of Technology, Pasadena, California 91125, USA
| | - D L Kinzel
- LIGO Livingston Observatory, Livingston, Louisiana 70754, USA
| | - J S Kissel
- LIGO Hanford Observatory, Richland, Washington 99352, USA
| | - S Klimenko
- University of Florida, Gainesville, Florida 32611, USA
| | - J Kline
- University of Wisconsin-Milwaukee, Milwaukee, Wisconsin 53201, USA
| | - S Koehlenbeck
- Albert-Einstein-Institut, Max-Planck-Institut für Gravitationsphysik, D-30167 Hannover, Germany
| | - K Kokeyama
- Louisiana State University, Baton Rouge, Louisiana 70803, USA
| | - V Kondrashov
- LIGO, California Institute of Technology, Pasadena, California 91125, USA
| | - S Koranda
- University of Wisconsin-Milwaukee, Milwaukee, Wisconsin 53201, USA
| | - W Z Korth
- LIGO, California Institute of Technology, Pasadena, California 91125, USA
| | - I Kowalska
- Astronomical Observatory Warsaw University, 00-478 Warsaw, Poland
| | - D B Kozak
- LIGO, California Institute of Technology, Pasadena, California 91125, USA
| | - V Kringel
- Albert-Einstein-Institut, Max-Planck-Institut für Gravitationsphysik, D-30167 Hannover, Germany
| | - B Krishnan
- Albert-Einstein-Institut, Max-Planck-Institut für Gravitationsphysik, D-30167 Hannover, Germany
| | - A Królak
- NCBJ, 05-400 Świerk-Otwock, Poland and IM-PAN, 00-956 Warsaw, Poland
| | - G Kuehn
- Albert-Einstein-Institut, Max-Planck-Institut für Gravitationsphysik, D-30167 Hannover, Germany
| | - A Kumar
- Institute for Plasma Research, Bhat, Gandhinagar 382428, India
| | - D Nanda Kumar
- University of Florida, Gainesville, Florida 32611, USA
| | - P Kumar
- Syracuse University, Syracuse, New York 13244, USA
| | - R Kumar
- SUPA, University of Glasgow, Glasgow G12 8QQ, United Kingdom
| | - L Kuo
- National Tsing Hua University, Hsinchu 300, Taiwan
| | | | - P K Lam
- Australian National University, Canberra, ACT 0200, Australia
| | - M Landry
- LIGO Hanford Observatory, Richland, Washington 99352, USA
| | - B Lantz
- Stanford University, Stanford, California 94305, USA
| | - S Larson
- Northwestern University, Evanston, Illinois 60208, USA
| | - P D Lasky
- The University of Melbourne, Parkville, VIC 3010, Australia
| | - A Lazzarini
- LIGO, California Institute of Technology, Pasadena, California 91125, USA
| | - C Lazzaro
- INFN, Sezione di Padova, I-35131 Padova, Italy
| | - P Leaci
- Albert-Einstein-Institut, Max-Planck-Institut für Gravitationsphysik, D-14476 Golm, Germany
| | - S Leavey
- SUPA, University of Glasgow, Glasgow G12 8QQ, United Kingdom
| | | | - C H Lee
- Pusan National University, Busan 609-735, Korea
| | - H K Lee
- Hanyang University, Seoul 133-791, Korea
| | - H M Lee
- Seoul National University, Seoul 151-742, Korea
| | - J Lee
- Hanyang University, Seoul 133-791, Korea
| | - P J Lee
- LIGO, Massachusetts Institute of Technology, Cambridge, Massachusetts 02139, USA
| | - M Leonardi
- Università di Trento, I-38050 Povo, Trento, Italy and INFN, Gruppo Collegato di Trento, I-38050 Povo, Trento, Italy
| | - J R Leong
- Albert-Einstein-Institut, Max-Planck-Institut für Gravitationsphysik, D-30167 Hannover, Germany
| | - I Leonor
- University of Oregon, Eugene, Oregon 97403, USA
| | - A Le Roux
- LIGO Livingston Observatory, Livingston, Louisiana 70754, USA
| | - N Leroy
- LAL, Université Paris-Sud, IN2P3/CNRS, F-91898 Orsay, France
| | - N Letendre
- Laboratoire d'Annecy-le-Vieux de Physique des Particules (LAPP), Université de Savoie, CNRS/IN2P3, F-74941 Annecy-le-Vieux, France
| | - Y Levin
- Monash University, Victoria 3800, Australia
| | - B Levine
- LIGO Hanford Observatory, Richland, Washington 99352, USA
| | - J Lewis
- LIGO, California Institute of Technology, Pasadena, California 91125, USA
| | - T G F Li
- LIGO, California Institute of Technology, Pasadena, California 91125, USA
| | - K Libbrecht
- LIGO, California Institute of Technology, Pasadena, California 91125, USA
| | - A Libson
- LIGO, Massachusetts Institute of Technology, Cambridge, Massachusetts 02139, USA
| | - A C Lin
- Stanford University, Stanford, California 94305, USA
| | | | - N A Lockerbie
- SUPA, University of Strathclyde, Glasgow G1 1XQ, United Kingdom
| | - V Lockett
- California State University Fullerton, Fullerton, California 92831, USA
| | - D Lodhia
- University of Birmingham, Birmingham B15 2TT, United Kingdom
| | - K Loew
- Embry-Riddle Aeronautical University, Prescott, Arizona 86301, USA
| | - J Logue
- SUPA, University of Glasgow, Glasgow G12 8QQ, United Kingdom
| | - A L Lombardi
- University of Massachusetts Amherst, Amherst, Massachusetts 01003, USA
| | - E Lopez
- Louisiana Tech University, Ruston, Louisiana 71272, USA
| | - M Lorenzini
- INFN, Sezione di Roma Tor Vergata, I-00133 Roma, Italy and Università di Roma Tor Vergata, I-00133 Roma, Italy
| | | | - M Lormand
- LIGO Livingston Observatory, Livingston, Louisiana 70754, USA
| | - G Losurdo
- INFN, Sezione di Firenze, I-50019 Sesto Fiorentino, Firenze, Italy
| | - J Lough
- Syracuse University, Syracuse, New York 13244, USA
| | - M J Lubinski
- LIGO Hanford Observatory, Richland, Washington 99352, USA
| | - H Lück
- Albert-Einstein-Institut, Max-Planck-Institut für Gravitationsphysik, D-30167 Hannover, Germany and Leibniz Universität Hannover, D-30167 Hannover, Germany
| | - A P Lundgren
- Albert-Einstein-Institut, Max-Planck-Institut für Gravitationsphysik, D-30167 Hannover, Germany
| | - Y Ma
- University of Western Australia, Crawley, Western Australia 6009, Australia
| | - E P Macdonald
- Cardiff University, Cardiff CF24 3AA, United Kingdom
| | - T MacDonald
- Stanford University, Stanford, California 94305, USA
| | - B Machenschalk
- Albert-Einstein-Institut, Max-Planck-Institut für Gravitationsphysik, D-30167 Hannover, Germany
| | - M MacInnis
- LIGO, Massachusetts Institute of Technology, Cambridge, Massachusetts 02139, USA
| | - D M Macleod
- Louisiana State University, Baton Rouge, Louisiana 70803, USA
| | | | - R Magee
- Washington State University, Pullman, Washington 99164, USA
| | - M Mageswaran
- LIGO, California Institute of Technology, Pasadena, California 91125, USA
| | - C Maglione
- Argentinian Gravitational Wave Group, Cordoba Cordoba 5000, Argentina
| | - K Mailand
- LIGO, California Institute of Technology, Pasadena, California 91125, USA
| | - E Majorana
- INFN, Sezione di Roma, I-00185 Roma, Italy
| | | | - V Malvezzi
- INFN, Sezione di Roma Tor Vergata, I-00133 Roma, Italy and Università di Roma Tor Vergata, I-00133 Roma, Italy
| | - N Man
- Université Nice-Sophia-Antipolis, CNRS, Observatoire de la Côte d'Azur, F-06304 Nice, France
| | - G M Manca
- Albert-Einstein-Institut, Max-Planck-Institut für Gravitationsphysik, D-30167 Hannover, Germany
| | - I Mandel
- University of Birmingham, Birmingham B15 2TT, United Kingdom
| | - V Mandic
- University of Minnesota, Minneapolis, Minnesota 55455, USA
| | - V Mangano
- INFN, Sezione di Roma, I-00185 Roma, Italy and Università di Roma 'La Sapienza', I-00185 Roma, Italy
| | - N M Mangini
- University of Massachusetts Amherst, Amherst, Massachusetts 01003, USA
| | - G Mansell
- Australian National University, Canberra, ACT 0200, Australia
| | | | - F Marchesoni
- INFN, Sezione di Perugia, I-06123 Perugia, Italy and Università di Camerino, Dipartimento di Fisica, I-62032 Camerino, Italy
| | - F Marion
- Laboratoire d'Annecy-le-Vieux de Physique des Particules (LAPP), Université de Savoie, CNRS/IN2P3, F-74941 Annecy-le-Vieux, France
| | - S Márka
- Columbia University, New York, New York 10027, USA
| | - Z Márka
- Columbia University, New York, New York 10027, USA
| | - A Markosyan
- Stanford University, Stanford, California 94305, USA
| | - E Maros
- LIGO, California Institute of Technology, Pasadena, California 91125, USA
| | - J Marque
- European Gravitational Observatory (EGO), I-56021 Cascina, Pisa, Italy
| | - F Martelli
- Università degli Studi di Urbino 'Carlo Bo', I-61029 Urbino, Italy and 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
- University of Florida, Gainesville, Florida 32611, USA
| | - L Martinelli
- Université Nice-Sophia-Antipolis, CNRS, Observatoire de la Côte d'Azur, F-06304 Nice, France
| | - D Martynov
- LIGO, California Institute of Technology, Pasadena, California 91125, USA
| | - J N Marx
- LIGO, California Institute of Technology, Pasadena, California 91125, USA
| | - K Mason
- LIGO, Massachusetts Institute of Technology, Cambridge, Massachusetts 02139, USA
| | - A Masserot
- Laboratoire d'Annecy-le-Vieux de Physique des Particules (LAPP), Université de Savoie, CNRS/IN2P3, F-74941 Annecy-le-Vieux, France
| | | | - F Matichard
- LIGO, Massachusetts Institute of Technology, Cambridge, Massachusetts 02139, USA
| | - L Matone
- Columbia University, New York, New York 10027, USA
| | - N Mavalvala
- LIGO, Massachusetts Institute of Technology, Cambridge, Massachusetts 02139, USA
| | - G May
- Louisiana State University, Baton Rouge, Louisiana 70803, USA
| | - N Mazumder
- IISER-TVM, CET Campus, Trivandrum, Kerala 695016, India
| | - G Mazzolo
- Albert-Einstein-Institut, Max-Planck-Institut für Gravitationsphysik, D-30167 Hannover, Germany
| | - R McCarthy
- LIGO Hanford Observatory, Richland, Washington 99352, USA
| | - D E McClelland
- Australian National University, Canberra, ACT 0200, Australia
| | - S C McGuire
- Southern University and A&M College, Baton Rouge, Louisiana 70813, USA
| | - G McIntyre
- LIGO, California Institute of Technology, Pasadena, California 91125, USA
| | - J McIver
- University of Massachusetts Amherst, Amherst, Massachusetts 01003, USA
| | - K McLin
- Sonoma State University, Rohnert Park, California 94928, USA
| | - D Meacher
- Université Nice-Sophia-Antipolis, CNRS, Observatoire de la Côte d'Azur, F-06304 Nice, France
| | - G D Meadors
- University of Michigan, Ann Arbor, Michigan 48109, USA
| | - M Mehmet
- Albert-Einstein-Institut, Max-Planck-Institut für Gravitationsphysik, D-30167 Hannover, Germany
| | - J Meidam
- Nikhef, Science Park, 1098 XG Amsterdam, The Netherlands
| | - M Meinders
- Leibniz Universität Hannover, D-30167 Hannover, Germany
| | - A Melatos
- The University of Melbourne, Parkville, VIC 3010, Australia
| | - G Mendell
- LIGO Hanford Observatory, Richland, Washington 99352, USA
| | - R A Mercer
- University of Wisconsin-Milwaukee, Milwaukee, Wisconsin 53201, USA
| | - S Meshkov
- LIGO, California Institute of Technology, Pasadena, California 91125, USA
| | - C Messenger
- SUPA, University of Glasgow, Glasgow G12 8QQ, United Kingdom
| | - M S Meyer
- LIGO Livingston Observatory, Livingston, Louisiana 70754, USA
| | - P M Meyers
- University of Minnesota, Minneapolis, Minnesota 55455, USA
| | - F Mezzani
- INFN, Sezione di Roma, I-00185 Roma, Italy and Università di Roma 'La Sapienza', I-00185 Roma, Italy
| | - H Miao
- Caltech-CaRT, Pasadena, California 91125, USA
| | - C Michel
- Laboratoire des Matériaux Avancés (LMA), IN2P3/CNRS, Université de Lyon, F-69622 Villeurbanne, Lyon, France
| | - E E Mikhailov
- College of William and Mary, Williamsburg, Virginia 23187, USA
| | - L Milano
- INFN, Sezione di Napoli, Complesso Universitario di Monte S. Angelo, I-80126 Napoli, Italy and Università di Napoli 'Federico II', Complesso Universitario di Monte S. Angelo, I-80126 Napoli, Italy
| | - J Miller
- LIGO, Massachusetts Institute of Technology, Cambridge, Massachusetts 02139, USA
| | - Y Minenkov
- INFN, Sezione di Roma Tor Vergata, I-00133 Roma, Italy
| | | | - C Mishra
- IISER-TVM, CET Campus, Trivandrum, Kerala 695016, India
| | - 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, Massachusetts Institute of Technology, Cambridge, Massachusetts 02139, USA
| | - B Moe
- University of Wisconsin-Milwaukee, Milwaukee, Wisconsin 53201, USA
| | - A Moggi
- INFN, Sezione di Pisa, I-56127 Pisa, Italy
| | - M Mohan
- European Gravitational Observatory (EGO), I-56021 Cascina, Pisa, Italy
| | | | - D Moraru
- LIGO Hanford Observatory, Richland, Washington 99352, USA
| | - G Moreno
- LIGO Hanford Observatory, Richland, Washington 99352, USA
| | - N Morgado
- Laboratoire des Matériaux Avancés (LMA), IN2P3/CNRS, Université de Lyon, F-69622 Villeurbanne, Lyon, France
| | - S R Morriss
- The University of Texas at Brownsville, Brownsville, Texas 78520, USA
| | - K Mossavi
- Albert-Einstein-Institut, Max-Planck-Institut für Gravitationsphysik, D-30167 Hannover, Germany
| | - B Mours
- Laboratoire d'Annecy-le-Vieux de Physique des Particules (LAPP), Université de Savoie, CNRS/IN2P3, F-74941 Annecy-le-Vieux, France
| | - C M Mow-Lowry
- Albert-Einstein-Institut, Max-Planck-Institut für Gravitationsphysik, D-30167 Hannover, Germany
| | - C L Mueller
- University of Florida, Gainesville, Florida 32611, USA
| | - G Mueller
- University of Florida, Gainesville, Florida 32611, USA
| | - S Mukherjee
- The University of Texas at Brownsville, Brownsville, Texas 78520, USA
| | - A Mullavey
- Louisiana State University, Baton Rouge, Louisiana 70803, USA
| | - J Munch
- University of Adelaide, Adelaide, South Australia 5005, Australia
| | - D Murphy
- Columbia University, New York, New York 10027, USA
| | - P G Murray
- SUPA, University of Glasgow, Glasgow G12 8QQ, United Kingdom
| | - A Mytidis
- University of Florida, Gainesville, Florida 32611, USA
| | - M F Nagy
- Wigner RCP, RMKI, H-1121 Budapest, Konkoly Thege Miklós út 29-33, Hungary
| | - I Nardecchia
- INFN, Sezione di Roma Tor Vergata, I-00133 Roma, Italy and Università di Roma Tor Vergata, I-00133 Roma, Italy
| | - L Naticchioni
- INFN, Sezione di Roma, I-00185 Roma, Italy and Università di Roma 'La Sapienza', I-00185 Roma, Italy
| | - R K Nayak
- IISER-Kolkata, Mohanpur, West Bengal 741252, India
| | - V Necula
- University of Florida, Gainesville, Florida 32611, USA
| | - G Nelemans
- Nikhef, Science Park, 1098 XG Amsterdam, The Netherlands and Department of Astrophysics/IMAPP, Radboud University Nijmegen, P.O. Box 9010, 6500 GL Nijmegen, The Netherlands
| | - I Neri
- INFN, Sezione di Perugia, I-06123 Perugia, Italy and Università di Perugia, I-06123 Perugia, Italy
| | - M Neri
- Università degli Studi di Genova, I-16146 Genova, Italy and INFN, Sezione di Genova, I-16146 Genova, Italy
| | - G Newton
- SUPA, University of Glasgow, Glasgow G12 8QQ, United Kingdom
| | - T Nguyen
- Australian National University, Canberra, ACT 0200, Australia
| | - A B Nielsen
- Albert-Einstein-Institut, Max-Planck-Institut für Gravitationsphysik, D-30167 Hannover, Germany
| | - S Nissanke
- Caltech-CaRT, Pasadena, California 91125, USA
| | - A H Nitz
- Syracuse University, Syracuse, New York 13244, USA
| | - F Nocera
- European Gravitational Observatory (EGO), I-56021 Cascina, Pisa, Italy
| | - D Nolting
- LIGO Livingston Observatory, Livingston, Louisiana 70754, USA
| | - M E N Normandin
- The University of Texas at Brownsville, Brownsville, Texas 78520, USA
| | - L K Nuttall
- University of Wisconsin-Milwaukee, Milwaukee, Wisconsin 53201, USA
| | - E Ochsner
- University of Wisconsin-Milwaukee, Milwaukee, Wisconsin 53201, USA
| | - J O'Dell
- Rutherford Appleton Laboratory, HSIC, Chilton, Didcot, Oxon OX11 0QX, United Kingdom
| | - E Oelker
- LIGO, Massachusetts Institute of Technology, Cambridge, Massachusetts 02139, USA
| | - J J Oh
- National Institute for Mathematical Sciences, Daejeon 305-390, Korea
| | - S H Oh
- National Institute for Mathematical Sciences, Daejeon 305-390, Korea
| | - F Ohme
- Cardiff University, Cardiff CF24 3AA, United Kingdom
| | - S Omar
- Stanford University, Stanford, California 94305, USA
| | - P Oppermann
- Albert-Einstein-Institut, Max-Planck-Institut für Gravitationsphysik, D-30167 Hannover, Germany
| | - R Oram
- LIGO Livingston Observatory, Livingston, Louisiana 70754, USA
| | - B O'Reilly
- LIGO Livingston Observatory, Livingston, Louisiana 70754, USA
| | - W Ortega
- Argentinian Gravitational Wave Group, Cordoba Cordoba 5000, Argentina
| | - R O'Shaughnessy
- University of Wisconsin-Milwaukee, Milwaukee, Wisconsin 53201, USA
| | - C Osthelder
- LIGO, California Institute of Technology, Pasadena, California 91125, USA
| | - D J Ottaway
- University of Adelaide, Adelaide, South Australia 5005, Australia
| | - R S Ottens
- University of Florida, Gainesville, Florida 32611, USA
| | - H Overmier
- LIGO Livingston Observatory, Livingston, Louisiana 70754, USA
| | - B J Owen
- The Pennsylvania State University, University Park, Pennsylvania 16802, USA
| | - C Padilla
- California State University Fullerton, Fullerton, California 92831, USA
| | - A Pai
- IISER-TVM, CET Campus, Trivandrum, Kerala 695016, India
| | - 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 300, Taiwan
| | - Y Pan
- University of Maryland, College Park, Maryland 20742, USA
| | - C Pankow
- University of Wisconsin-Milwaukee, Milwaukee, Wisconsin 53201, USA
| | - F Paoletti
- INFN, Sezione di Pisa, I-56127 Pisa, Italy and European Gravitational Observatory (EGO), I-56021 Cascina, Pisa, Italy
| | - M A Papa
- University of Wisconsin-Milwaukee, Milwaukee, Wisconsin 53201, USA and Albert-Einstein-Institut, Max-Planck-Institut für Gravitationsphysik, D-14476 Golm, Germany
| | - H Paris
- Stanford University, Stanford, California 94305, USA
| | - A Pasqualetti
- European Gravitational Observatory (EGO), I-56021 Cascina, Pisa, Italy
| | - R Passaquieti
- INFN, Sezione di Pisa, I-56127 Pisa, Italy and Università di Pisa, I-56127 Pisa, Italy
| | | | - M Pedraza
- LIGO, California Institute of Technology, Pasadena, California 91125, USA
| | - A Pele
- LIGO Hanford Observatory, Richland, Washington 99352, USA
| | - S Penn
- Hobart and William Smith Colleges, Geneva, New York 14456, USA
| | - A Perreca
- Syracuse University, Syracuse, New York 13244, USA
| | - M Phelps
- LIGO, California Institute of Technology, Pasadena, California 91125, USA
| | - M Pichot
- Université Nice-Sophia-Antipolis, CNRS, Observatoire de la Côte d'Azur, F-06304 Nice, France
| | - M Pickenpack
- Albert-Einstein-Institut, Max-Planck-Institut für Gravitationsphysik, D-30167 Hannover, Germany
| | - F Piergiovanni
- Università degli Studi di Urbino 'Carlo Bo', I-61029 Urbino, Italy and INFN, Sezione di Firenze, I-50019 Sesto Fiorentino, Firenze, Italy
| | - V Pierro
- University of Sannio at Benevento, I-82100 Benevento, Italy and INFN, Sezione di Napoli, I-80100 Napoli, Italy
| | - L Pinard
- Laboratoire des Matériaux Avancés (LMA), IN2P3/CNRS, Université de Lyon, F-69622 Villeurbanne, Lyon, France
| | - I M Pinto
- University of Sannio at Benevento, I-82100 Benevento, Italy and INFN, Sezione di Napoli, I-80100 Napoli, Italy
| | - M Pitkin
- SUPA, University of Glasgow, Glasgow G12 8QQ, United Kingdom
| | - J Poeld
- Albert-Einstein-Institut, Max-Planck-Institut für Gravitationsphysik, D-30167 Hannover, Germany
| | - R Poggiani
- INFN, Sezione di Pisa, I-56127 Pisa, Italy and Università di Pisa, I-56127 Pisa, Italy
| | - A Poteomkin
- Institute of Applied Physics, Nizhny Novgorod 603950, Russia
| | - J Powell
- SUPA, University of Glasgow, Glasgow G12 8QQ, United Kingdom
| | - J Prasad
- Inter-University Centre for Astronomy and Astrophysics, Pune - 411007, India
| | - V Predoi
- Cardiff University, Cardiff CF24 3AA, United Kingdom
| | | | - T Prestegard
- University of Minnesota, Minneapolis, Minnesota 55455, USA
| | - L R Price
- LIGO, California Institute of Technology, Pasadena, California 91125, USA
| | - M Prijatelj
- European Gravitational Observatory (EGO), I-56021 Cascina, Pisa, Italy
| | - S Privitera
- LIGO, California Institute of Technology, Pasadena, California 91125, USA
| | - G A Prodi
- Università di Trento, I-38050 Povo, Trento, Italy and INFN, Gruppo Collegato di Trento, I-38050 Povo, Trento, Italy
| | - L Prokhorov
- Faculty of Physics, Lomonosov Moscow State University, Moscow 119991, Russia
| | - O Puncken
- The University of Texas at Brownsville, Brownsville, Texas 78520, USA
| | - M Punturo
- INFN, Sezione di Perugia, I-06123 Perugia, Italy
| | - P Puppo
- INFN, Sezione di Roma, I-00185 Roma, Italy
| | - M Pürrer
- Cardiff University, Cardiff CF24 3AA, United Kingdom
| | - J Qin
- University of Western Australia, Crawley, Western Australia 6009, Australia
| | - V Quetschke
- The University of Texas at Brownsville, Brownsville, Texas 78520, USA
| | - E Quintero
- LIGO, California Institute of Technology, Pasadena, California 91125, USA
| | | | - F J Raab
- LIGO Hanford Observatory, Richland, Washington 99352, USA
| | - D S Rabeling
- Nikhef, Science Park, 1098 XG Amsterdam, The Netherlands and VU University Amsterdam, 1081 HV Amsterdam, The Netherlands
| | - I Rácz
- Wigner RCP, RMKI, H-1121 Budapest, Konkoly Thege Miklós út 29-33, Hungary
| | - H Radkins
- LIGO Hanford Observatory, Richland, Washington 99352, USA
| | - P Raffai
- MTA Eötvös University, 'Lendulet' A. R. G., Budapest 1117, Hungary
| | - S Raja
- RRCAT, Indore, Madhya Pradesh 452013, India
| | - G Rajalakshmi
- Tata Institute for Fundamental Research, Mumbai 400005, India
| | - M Rakhmanov
- The University of Texas at Brownsville, Brownsville, Texas 78520, USA
| | - C Ramet
- LIGO Livingston Observatory, Livingston, Louisiana 70754, USA
| | - K Ramirez
- The University of Texas at Brownsville, Brownsville, Texas 78520, USA
| | - P Rapagnani
- INFN, Sezione di Roma, I-00185 Roma, Italy and Università di Roma 'La Sapienza', I-00185 Roma, Italy
| | - V Raymond
- LIGO, California Institute of Technology, Pasadena, California 91125, USA
| | - M Razzano
- INFN, Sezione di Pisa, I-56127 Pisa, Italy and Università di Pisa, I-56127 Pisa, Italy
| | - V Re
- INFN, Sezione di Roma Tor Vergata, I-00133 Roma, Italy and Università di Roma Tor Vergata, I-00133 Roma, Italy
| | - S Recchia
- Università di Roma Tor Vergata, I-00133 Roma, Italy and INFN, Gran Sasso Science Institute, I-67100 L'Aquila, Italy
| | - C M Reed
- LIGO Hanford Observatory, Richland, Washington 99352, USA
| | - T Regimbau
- Université Nice-Sophia-Antipolis, CNRS, Observatoire de la Côte d'Azur, F-06304 Nice, France
| | - S Reid
- SUPA, University of the West of Scotland, Paisley PA1 2BE, United Kingdom
| | - D H Reitze
- LIGO, California Institute of Technology, Pasadena, California 91125, USA and University of Florida, Gainesville, Florida 32611, USA
| | - O Reula
- Argentinian Gravitational Wave Group, Cordoba Cordoba 5000, Argentina
| | - E Rhoades
- Embry-Riddle Aeronautical University, Prescott, Arizona 86301, USA
| | - F Ricci
- INFN, Sezione di Roma, I-00185 Roma, Italy and Università di Roma 'La Sapienza', I-00185 Roma, Italy
| | - R Riesen
- LIGO Livingston Observatory, Livingston, Louisiana 70754, USA
| | - K Riles
- University of Michigan, Ann Arbor, Michigan 48109, USA
| | - N A Robertson
- LIGO, California Institute of Technology, Pasadena, California 91125, USA and SUPA, University of Glasgow, Glasgow G12 8QQ, United Kingdom
| | - F Robinet
- LAL, Université Paris-Sud, IN2P3/CNRS, F-91898 Orsay, France
| | - A Rocchi
- INFN, Sezione di Roma Tor Vergata, I-00133 Roma, Italy
| | - S B Roddy
- LIGO Livingston Observatory, Livingston, Louisiana 70754, USA
| | - L Rolland
- Laboratoire d'Annecy-le-Vieux de Physique des Particules (LAPP), Université de Savoie, CNRS/IN2P3, F-74941 Annecy-le-Vieux, France
| | - J G Rollins
- LIGO, California Institute of Technology, Pasadena, California 91125, USA
| | - R Romano
- Università di Salerno, Fisciano, I-84084 Salerno, Italy and INFN, Sezione di Napoli, Complesso Universitario di Monte S. Angelo, I-80126 Napoli, Italy
| | - G Romanov
- College of William and Mary, Williamsburg, Virginia 23187, USA
| | - J H Romie
- LIGO Livingston Observatory, Livingston, Louisiana 70754, USA
| | - D Rosińska
- CAMK-PAN, 00-716 Warsaw, Poland and Institute of Astronomy, 65-265 Zielona Góra, Poland
| | - S Rowan
- SUPA, University of Glasgow, Glasgow G12 8QQ, United Kingdom
| | - A Rüdiger
- Albert-Einstein-Institut, Max-Planck-Institut für Gravitationsphysik, D-30167 Hannover, Germany
| | - P Ruggi
- European Gravitational Observatory (EGO), I-56021 Cascina, Pisa, Italy
| | - K Ryan
- LIGO Hanford Observatory, Richland, Washington 99352, USA
| | - F Salemi
- Albert-Einstein-Institut, Max-Planck-Institut für Gravitationsphysik, D-30167 Hannover, Germany
| | - L Sammut
- The University of Melbourne, Parkville, VIC 3010, Australia
| | - V Sandberg
- LIGO Hanford Observatory, Richland, Washington 99352, USA
| | - J R Sanders
- University of Michigan, Ann Arbor, Michigan 48109, USA
| | - S Sankar
- LIGO, Massachusetts Institute of Technology, Cambridge, Massachusetts 02139, USA
| | - V Sannibale
- LIGO, California Institute of Technology, Pasadena, California 91125, USA
| | | | - E Saracco
- Laboratoire des Matériaux Avancés (LMA), IN2P3/CNRS, Université de Lyon, F-69622 Villeurbanne, Lyon, France
| | - B Sassolas
- Laboratoire des Matériaux Avancés (LMA), IN2P3/CNRS, Université de Lyon, F-69622 Villeurbanne, Lyon, France
| | | | - P R Saulson
- Syracuse University, Syracuse, New York 13244, USA
| | - R Savage
- LIGO Hanford Observatory, Richland, Washington 99352, USA
| | - J Scheuer
- Northwestern University, Evanston, Illinois 60208, USA
| | - R Schilling
- Albert-Einstein-Institut, Max-Planck-Institut für Gravitationsphysik, D-30167 Hannover, Germany
| | - M Schilman
- Argentinian Gravitational Wave Group, Cordoba Cordoba 5000, Argentina
| | - P Schmidt
- Cardiff University, Cardiff CF24 3AA, United Kingdom
| | - R Schnabel
- Albert-Einstein-Institut, Max-Planck-Institut für Gravitationsphysik, D-30167 Hannover, Germany and Leibniz Universität Hannover, D-30167 Hannover, Germany
| | | | - E Schreiber
- Albert-Einstein-Institut, Max-Planck-Institut für Gravitationsphysik, D-30167 Hannover, Germany
| | - D Schuette
- Albert-Einstein-Institut, Max-Planck-Institut für Gravitationsphysik, D-30167 Hannover, Germany
| | - B F Schutz
- Cardiff University, Cardiff CF24 3AA, United Kingdom and Albert-Einstein-Institut, Max-Planck-Institut für Gravitationsphysik, D-14476 Golm, Germany
| | - J Scott
- SUPA, University of Glasgow, Glasgow G12 8QQ, United Kingdom
| | - S M Scott
- Australian National University, Canberra, ACT 0200, Australia
| | - D Sellers
- LIGO Livingston Observatory, Livingston, Louisiana 70754, USA
| | - A S Sengupta
- Indian Institute of Technology, Gandhinagar, Ahmedabad, Gujarat 382424, India
| | - D Sentenac
- European Gravitational Observatory (EGO), I-56021 Cascina, Pisa, Italy
| | - V Sequino
- INFN, Sezione di Roma Tor Vergata, I-00133 Roma, Italy and Università di Roma Tor Vergata, I-00133 Roma, Italy
| | - A Sergeev
- Institute of Applied Physics, Nizhny Novgorod 603950, Russia
| | - D A Shaddock
- Australian National University, Canberra, ACT 0200, Australia
| | - S Shah
- Nikhef, Science Park, 1098 XG Amsterdam, The Netherlands and Department of Astrophysics/IMAPP, Radboud University Nijmegen, P.O. Box 9010, 6500 GL Nijmegen, The Netherlands
| | - M S Shahriar
- Northwestern University, Evanston, Illinois 60208, USA
| | - M Shaltev
- Albert-Einstein-Institut, Max-Planck-Institut für Gravitationsphysik, D-30167 Hannover, Germany
| | - Z Shao
- LIGO, California Institute of Technology, Pasadena, California 91125, USA
| | - B Shapiro
- Stanford University, Stanford, California 94305, USA
| | - P Shawhan
- University of Maryland, College Park, Maryland 20742, USA
| | - D H Shoemaker
- LIGO, Massachusetts Institute of Technology, Cambridge, Massachusetts 02139, USA
| | - T L Sidery
- University of Birmingham, Birmingham B15 2TT, United Kingdom
| | - K Siellez
- Université Nice-Sophia-Antipolis, CNRS, Observatoire de la Côte d'Azur, F-06304 Nice, France
| | - X Siemens
- University of Wisconsin-Milwaukee, Milwaukee, Wisconsin 53201, USA
| | - D Sigg
- LIGO Hanford Observatory, Richland, Washington 99352, USA
| | - D Simakov
- Albert-Einstein-Institut, Max-Planck-Institut für Gravitationsphysik, D-30167 Hannover, Germany
| | - A Singer
- LIGO, California Institute of Technology, Pasadena, California 91125, USA
| | - L Singer
- LIGO, California Institute of Technology, Pasadena, California 91125, USA
| | - R Singh
- Louisiana State University, Baton Rouge, Louisiana 70803, USA
| | - A M Sintes
- Universitat de les Illes Balears, E-07122 Palma de Mallorca, Spain
| | - B J J Slagmolen
- Australian National University, Canberra, ACT 0200, Australia
| | - J Slutsky
- NASA/Goddard Space Flight Center, Greenbelt, Maryland 20771, USA
| | - J R Smith
- California State University Fullerton, Fullerton, California 92831, USA
| | - M R Smith
- LIGO, California Institute of Technology, Pasadena, California 91125, USA
| | - R J E Smith
- LIGO, California Institute of Technology, Pasadena, California 91125, USA
| | - N D Smith-Lefebvre
- LIGO, California Institute of Technology, Pasadena, California 91125, USA
| | - E J Son
- National Institute for Mathematical Sciences, Daejeon 305-390, Korea
| | - B Sorazu
- SUPA, University of Glasgow, Glasgow G12 8QQ, United Kingdom
| | - T Souradeep
- Inter-University Centre for Astronomy and Astrophysics, Pune - 411007, India
| | - A Staley
- Columbia University, New York, New York 10027, USA
| | - J Stebbins
- Stanford University, Stanford, California 94305, USA
| | - M Steinke
- Albert-Einstein-Institut, Max-Planck-Institut für Gravitationsphysik, D-30167 Hannover, Germany
| | - J Steinlechner
- Albert-Einstein-Institut, Max-Planck-Institut für Gravitationsphysik, D-30167 Hannover, Germany and SUPA, University of Glasgow, Glasgow G12 8QQ, United Kingdom
| | - S Steinlechner
- Albert-Einstein-Institut, Max-Planck-Institut für Gravitationsphysik, D-30167 Hannover, Germany and SUPA, University of Glasgow, Glasgow G12 8QQ, United Kingdom
| | - B C Stephens
- University of Wisconsin-Milwaukee, Milwaukee, Wisconsin 53201, USA
| | - S Steplewski
- Washington State University, Pullman, Washington 99164, USA
| | - S Stevenson
- University of Birmingham, Birmingham B15 2TT, United Kingdom
| | - R Stone
- The University of Texas at Brownsville, Brownsville, Texas 78520, USA
| | - D Stops
- University of Birmingham, Birmingham B15 2TT, United Kingdom
| | - K A Strain
- SUPA, University of Glasgow, Glasgow G12 8QQ, United Kingdom
| | - N Straniero
- Laboratoire des Matériaux Avancés (LMA), IN2P3/CNRS, Université de Lyon, F-69622 Villeurbanne, Lyon, France
| | - S Strigin
- Faculty of Physics, Lomonosov Moscow State University, Moscow 119991, Russia
| | - R Sturani
- Instituto de Física Teórica, Universidade Estadual Paulista/ICTP South American Institute for Fundamental Research, São Paulo, São Paulo 01140-070, Brazil
| | - A L Stuver
- LIGO Livingston Observatory, Livingston, Louisiana 70754, USA
| | | | - S Susmithan
- University of Western Australia, Crawley, Western Australia 6009, Australia
| | - P J Sutton
- Cardiff University, Cardiff CF24 3AA, United Kingdom
| | - B Swinkels
- European Gravitational Observatory (EGO), I-56021 Cascina, Pisa, Italy
| | - M Tacca
- APC, AstroParticule et Cosmologie, Université Paris Diderot, CNRS/IN2P3, CEA/Irfu, Observatoire de Paris, Sorbonne Paris Cité, 10, rue Alice Domon et Léonie Duquet, F-75205 Paris Cedex 13, France
| | - D Talukder
- University of Oregon, Eugene, Oregon 97403, USA
| | - D B Tanner
- University of Florida, Gainesville, Florida 32611, USA
| | - J Tao
- Louisiana State University, Baton Rouge, Louisiana 70803, USA
| | - S P Tarabrin
- Albert-Einstein-Institut, Max-Planck-Institut für Gravitationsphysik, D-30167 Hannover, Germany
| | - R Taylor
- LIGO, California Institute of Technology, Pasadena, California 91125, USA
| | - G Tellez
- The University of Texas at Brownsville, Brownsville, Texas 78520, USA
| | | | - M Thomas
- LIGO Livingston Observatory, Livingston, Louisiana 70754, USA
| | - P Thomas
- LIGO Hanford Observatory, Richland, Washington 99352, USA
| | - K A Thorne
- LIGO Livingston Observatory, Livingston, Louisiana 70754, USA
| | - K S Thorne
- Caltech-CaRT, Pasadena, California 91125, USA
| | - E Thrane
- LIGO, California Institute of Technology, Pasadena, California 91125, USA
| | - V Tiwari
- University of Florida, Gainesville, Florida 32611, USA
| | - K V Tokmakov
- SUPA, University of Strathclyde, Glasgow G1 1XQ, United Kingdom
| | - C Tomlinson
- The University of Sheffield, Sheffield S10 2TN, United Kingdom
| | - M Tonelli
- INFN, Sezione di Pisa, I-56127 Pisa, Italy and Università di Pisa, I-56127 Pisa, Italy
| | - C V Torres
- The University of Texas at Brownsville, Brownsville, Texas 78520, USA
| | - C I Torrie
- LIGO, California Institute of Technology, Pasadena, California 91125, USA and SUPA, University of Glasgow, Glasgow G12 8QQ, United Kingdom
| | - F Travasso
- INFN, Sezione di Perugia, I-06123 Perugia, Italy and Università di Perugia, I-06123 Perugia, Italy
| | - G Traylor
- LIGO Livingston Observatory, Livingston, Louisiana 70754, USA
| | - M Tse
- Columbia University, New York, New York 10027, USA
| | - D Tshilumba
- University of Brussels, Brussels 1050, Belgium
| | - H Tuennermann
- Albert-Einstein-Institut, Max-Planck-Institut für Gravitationsphysik, D-30167 Hannover, Germany
| | - D Ugolini
- Trinity University, San Antonio, Texas 78212, USA
| | | | - A L Urban
- University of Wisconsin-Milwaukee, Milwaukee, Wisconsin 53201, USA
| | - S A Usman
- Syracuse University, Syracuse, New York 13244, USA
| | - H Vahlbruch
- Leibniz Universität Hannover, D-30167 Hannover, Germany
| | - G Vajente
- INFN, Sezione di Pisa, I-56127 Pisa, Italy and Università di Pisa, I-56127 Pisa, Italy
| | - G Valdes
- The University of Texas at Brownsville, Brownsville, Texas 78520, USA
| | | | - M van Beuzekom
- Nikhef, Science Park, 1098 XG Amsterdam, The Netherlands
| | - J F J van den Brand
- Nikhef, Science Park, 1098 XG Amsterdam, The Netherlands and VU University Amsterdam, 1081 HV Amsterdam, The Netherlands
| | | | - M V van der Sluys
- Nikhef, Science Park, 1098 XG Amsterdam, The Netherlands and Department of Astrophysics/IMAPP, Radboud University Nijmegen, P.O. Box 9010, 6500 GL Nijmegen, The Netherlands
| | | | - A A van Veggel
- SUPA, University of Glasgow, Glasgow G12 8QQ, United Kingdom
| | - S Vass
- LIGO, California Institute of Technology, Pasadena, California 91125, USA
| | - M Vasúth
- Wigner RCP, RMKI, H-1121 Budapest, Konkoly Thege Miklós út 29-33, Hungary
| | - R Vaulin
- LIGO, Massachusetts Institute of Technology, Cambridge, Massachusetts 02139, USA
| | - A Vecchio
- University of Birmingham, Birmingham B15 2TT, United Kingdom
| | - G Vedovato
- INFN, Sezione di Padova, I-35131 Padova, Italy
| | - J Veitch
- Nikhef, Science Park, 1098 XG Amsterdam, The Netherlands
| | - P J Veitch
- University of Adelaide, Adelaide, South Australia 5005, Australia
| | - K Venkateswara
- University of Washington, Seattle, Washington 98195, USA
| | - D Verkindt
- Laboratoire d'Annecy-le-Vieux de Physique des Particules (LAPP), Université de Savoie, CNRS/IN2P3, F-74941 Annecy-le-Vieux, France
| | - F Vetrano
- Università degli Studi di Urbino 'Carlo Bo', I-61029 Urbino, Italy and INFN, Sezione di Firenze, I-50019 Sesto Fiorentino, Firenze, Italy
| | - A Viceré
- Università degli Studi di Urbino 'Carlo Bo', I-61029 Urbino, Italy and INFN, Sezione di Firenze, I-50019 Sesto Fiorentino, Firenze, Italy
| | - R Vincent-Finley
- Southern University and A&M College, Baton Rouge, Louisiana 70813, USA
| | - J-Y Vinet
- Université Nice-Sophia-Antipolis, CNRS, Observatoire de la Côte d'Azur, F-06304 Nice, France
| | - S Vitale
- LIGO, Massachusetts Institute of Technology, Cambridge, Massachusetts 02139, USA
| | - T Vo
- LIGO Hanford Observatory, Richland, Washington 99352, USA
| | - H Vocca
- INFN, Sezione di Perugia, I-06123 Perugia, Italy and Università di Perugia, I-06123 Perugia, Italy
| | - C Vorvick
- LIGO Hanford Observatory, Richland, Washington 99352, USA
| | - W D Vousden
- University of Birmingham, Birmingham B15 2TT, United Kingdom
| | - S P Vyachanin
- Faculty of Physics, Lomonosov Moscow State University, Moscow 119991, Russia
| | - A R Wade
- Australian National University, Canberra, ACT 0200, Australia
| | - L Wade
- University of Wisconsin-Milwaukee, Milwaukee, Wisconsin 53201, USA
| | - M Wade
- University of Wisconsin-Milwaukee, Milwaukee, Wisconsin 53201, USA
| | - M Walker
- Louisiana State University, Baton Rouge, Louisiana 70803, USA
| | - L Wallace
- LIGO, California Institute of Technology, Pasadena, California 91125, USA
| | - S Walsh
- University of Wisconsin-Milwaukee, Milwaukee, Wisconsin 53201, USA
| | - M Wang
- University of Birmingham, Birmingham B15 2TT, United Kingdom
| | - X Wang
- Tsinghua University, Beijing 100084, China
| | - R L Ward
- Australian National University, Canberra, ACT 0200, Australia
| | - M Was
- Albert-Einstein-Institut, Max-Planck-Institut für Gravitationsphysik, D-30167 Hannover, Germany
| | - B Weaver
- LIGO Hanford Observatory, Richland, Washington 99352, USA
| | - L-W Wei
- Université Nice-Sophia-Antipolis, CNRS, Observatoire de la Côte d'Azur, F-06304 Nice, France
| | - M Weinert
- Albert-Einstein-Institut, Max-Planck-Institut für Gravitationsphysik, D-30167 Hannover, Germany
| | - A J Weinstein
- LIGO, California Institute of Technology, Pasadena, California 91125, USA
| | - R Weiss
- LIGO, Massachusetts Institute of Technology, Cambridge, Massachusetts 02139, USA
| | - T Welborn
- LIGO Livingston Observatory, Livingston, Louisiana 70754, USA
| | - L Wen
- University of Western Australia, Crawley, Western Australia 6009, Australia
| | - P Wessels
- Albert-Einstein-Institut, Max-Planck-Institut für Gravitationsphysik, D-30167 Hannover, Germany
| | - M West
- Syracuse University, Syracuse, New York 13244, USA
| | - T Westphal
- Albert-Einstein-Institut, Max-Planck-Institut für Gravitationsphysik, D-30167 Hannover, Germany
| | - K Wette
- Albert-Einstein-Institut, Max-Planck-Institut für Gravitationsphysik, D-30167 Hannover, Germany
| | - J T Whelan
- Rochester Institute of Technology, Rochester, New York 14623, USA
| | - D J White
- The University of Sheffield, Sheffield S10 2TN, United Kingdom
| | - B F Whiting
- University of Florida, Gainesville, Florida 32611, USA
| | - K Wiesner
- Albert-Einstein-Institut, Max-Planck-Institut für Gravitationsphysik, D-30167 Hannover, Germany
| | - C Wilkinson
- LIGO Hanford Observatory, Richland, Washington 99352, USA
| | - K Williams
- Southern University and A&M College, Baton Rouge, Louisiana 70813, USA
| | - L Williams
- University of Florida, Gainesville, Florida 32611, USA
| | - R Williams
- LIGO, California Institute of Technology, Pasadena, California 91125, USA
| | - T D Williams
- Southeastern Louisiana University, Hammond, Louisiana 70402, USA
| | | | - J L Willis
- Abilene Christian University, Abilene, Texas 79699, USA
| | - B Willke
- Albert-Einstein-Institut, Max-Planck-Institut für Gravitationsphysik, D-30167 Hannover, Germany and Leibniz Universität Hannover, D-30167 Hannover, Germany
| | - M Wimmer
- Albert-Einstein-Institut, Max-Planck-Institut für Gravitationsphysik, D-30167 Hannover, Germany
| | - W Winkler
- Albert-Einstein-Institut, Max-Planck-Institut für Gravitationsphysik, D-30167 Hannover, Germany
| | - C C Wipf
- LIGO, Massachusetts Institute of Technology, Cambridge, Massachusetts 02139, USA
| | - A G Wiseman
- University of Wisconsin-Milwaukee, Milwaukee, Wisconsin 53201, USA
| | - H Wittel
- Albert-Einstein-Institut, Max-Planck-Institut für Gravitationsphysik, D-30167 Hannover, Germany
| | - G Woan
- SUPA, University of Glasgow, Glasgow G12 8QQ, United Kingdom
| | - N Wolovick
- Argentinian Gravitational Wave Group, Cordoba Cordoba 5000, Argentina
| | - J Worden
- LIGO Hanford Observatory, Richland, Washington 99352, USA
| | - Y Wu
- University of Florida, Gainesville, Florida 32611, USA
| | - J Yablon
- Northwestern University, Evanston, Illinois 60208, USA
| | - I Yakushin
- LIGO Livingston Observatory, Livingston, Louisiana 70754, USA
| | - W Yam
- LIGO, Massachusetts Institute of Technology, Cambridge, Massachusetts 02139, USA
| | - H Yamamoto
- LIGO, California Institute of Technology, Pasadena, California 91125, USA
| | - C C Yancey
- University of Maryland, College Park, Maryland 20742, USA
| | - H Yang
- Caltech-CaRT, Pasadena, California 91125, USA
| | - S Yoshida
- Southeastern Louisiana University, Hammond, Louisiana 70402, USA
| | - M Yvert
- Laboratoire d'Annecy-le-Vieux de Physique des Particules (LAPP), Université de Savoie, CNRS/IN2P3, F-74941 Annecy-le-Vieux, France
| | | | - M Zanolin
- Embry-Riddle Aeronautical University, Prescott, Arizona 86301, USA
| | - J-P Zendri
- INFN, Sezione di Padova, I-35131 Padova, Italy
| | - Fan Zhang
- LIGO, Massachusetts Institute of Technology, Cambridge, Massachusetts 02139, USA and Tsinghua University, Beijing 100084, China
| | - L Zhang
- LIGO, California Institute of Technology, Pasadena, California 91125, USA
| | - C Zhao
- University of Western Australia, Crawley, Western Australia 6009, Australia
| | - H Zhu
- The Pennsylvania State University, University Park, Pennsylvania 16802, USA
| | - X J Zhu
- University of Western Australia, Crawley, Western Australia 6009, Australia
| | - M E Zucker
- LIGO, Massachusetts Institute of Technology, Cambridge, Massachusetts 02139, USA
| | - S Zuraw
- University of Massachusetts Amherst, Amherst, Massachusetts 01003, USA
| | - J Zweizig
- LIGO, California Institute of Technology, Pasadena, California 91125, USA
| | - R L Aptekar
- Ioffe Physical-Technical Institute, Saint Petersburg, 194021, Russian Federation
| | - J L Atteia
- Université de Toulouse, UPS-OMP, IRAP, Toulouse, France and CNRS, IRAP, 14, Avenue Edouard Belin, F-31400 Toulouse, France
| | - T Cline
- NASA/Goddard Space Flight Center, Greenbelt, Maryland 20771, USA
| | - V Connaughton
- CSPAR, University of Alabama in Huntsville, Huntsville, Alabama 35899, USA
| | - D D Frederiks
- Ioffe Physical-Technical Institute, Saint Petersburg, 194021, Russian Federation
| | - S V Golenetskii
- Ioffe Physical-Technical Institute, Saint Petersburg, 194021, Russian Federation
| | - K Hurley
- University of California-Berkeley, Space Sciences Lab, 7 Gauss Way, Berkeley, California 94720, USA
| | - H A Krimm
- Center for Research and Exploration in Space Science and Technology (CRESST) and NASA Goddard Space Flight Center, Greenbelt, Maryland 20771, USA and Universities Space Research Association, 7178 Columbia Gateway Drive Columbia, Maryland 21046, USA
| | - M Marisaldi
- INAF-IASF Bologna, Via Piero Gobetti 101, 40129 Bologna, Italy
| | - V D Pal'shin
- Ioffe Physical-Technical Institute, Saint Petersburg, 194021, Russian Federation and Saint Petersburg State Polytechnical University, 195251, Saint Petersburg, Russia
| | - D Palmer
- Los Alamos National Laboratory, Los Alamos, New Mexico 87545, USA
| | - D S Svinkin
- Ioffe Physical-Technical Institute, Saint Petersburg, 194021, Russian Federation
| | - Y Terada
- Graduate School of Science and Engineering, Saitama University, Saitama City, Japan
| | - A von Kienlin
- Max-Planck-Institut für extraterrestrische Physik, Giessenbachstrasse 1, 85748 Garching, Germany
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Aasi J, Abbott BP, Abbott R, Abbott T, Abernathy MR, Acernese F, Ackley K, Adams C, Adams T, Addesso P, Adhikari RX, Affeldt C, Agathos M, Aggarwal N, Aguiar OD, Ajith P, Alemic A, Allen B, Allocca A, Amariutei D, Andersen M, Anderson RA, Anderson SB, Anderson WG, Arai K, Araya MC, Arceneaux C, Areeda JS, Ast S, Aston SM, Astone P, Aufmuth P, Augustus H, Aulbert C, Aylott BE, Babak S, Baker PT, Ballardin G, Ballmer SW, Barayoga JC, Barbet M, Barish BC, Barker D, Barone F, Barr B, Barsotti L, Barsuglia M, Barton MA, Bartos I, Bassiri R, Basti A, Batch JC, Bauchrowitz J, Bauer TS, Baune C, Bavigadda V, Behnke B, Bejger M, Beker MG, Belczynski C, Bell AS, Bell C, Bergmann G, Bersanetti D, Bertolini A, Betzwieser J, Bilenko IA, Billingsley G, Birch J, Biscans S, Bitossi M, Biwer C, Bizouard MA, Black E, Blackburn JK, Blackburn L, Blair D, Bloemen S, Bock O, Bodiya TP, Boer M, Bogaert G, Bogan C, Bond C, Bondu F, Bonelli L, Bonnand R, Bork R, Born M, Boschi V, Bose S, Bosi L, Bradaschia C, Brady PR, Braginsky VB, Branchesi M, Brau JE, Briant T, Bridges DO, Brillet A, Brinkmann M, Brisson V, Brooks AF, Brown DA, Brown DD, Brückner F, Buchman S, Buikema A, Bulik T, Bulten HJ, Buonanno A, Burman R, Buskulic D, Buy C, Cadonati L, Cagnoli G, Calderón Bustillo J, Calloni E, Camp JB, Campsie P, Cannon KC, Canuel B, Cao J, Capano CD, Carbognani F, Carbone L, Caride S, Castaldi G, Caudill S, Cavaglià M, Cavalier F, Cavalieri R, Celerier C, Cella G, Cepeda C, Cesarini E, Chakraborty R, Chalermsongsak T, Chamberlin SJ, Chao S, Charlton P, Chassande-Mottin E, Chen X, Chen Y, Chincarini A, Chiummo A, Cho HS, Cho M, Chow JH, Christensen N, Chu Q, Chua SSY, Chung S, Ciani G, Clara F, Clark DE, Clark JA, Clayton JH, Cleva F, Coccia E, Cohadon PF, Colla A, Collette C, Colombini M, Cominsky L, Constancio M, Conte A, Cook D, Corbitt TR, Cornish N, Corsi A, Costa CA, Coughlin MW, Coulon JP, Countryman S, Couvares P, Coward DM, Cowart MJ, Coyne DC, Coyne R, Craig K, Creighton JDE, Croce RP, Crowder SG, Cumming A, Cunningham L, Cuoco E, Cutler C, Dahl K, Dal Canton T, Damjanic M, Danilishin SL, D'Antonio S, Danzmann K, Dattilo V, Daveloza H, Davier M, Davies GS, Daw EJ, Day R, Dayanga T, DeBra D, Debreczeni G, Degallaix J, Deléglise S, Del Pozzo W, Denker T, Dent T, Dereli H, Dergachev V, De Rosa R, DeRosa RT, DeSalvo R, Dhurandhar S, Díaz M, Dickson J, Di Fiore L, Di Lieto A, Di Palma I, Di Virgilio A, Dolique V, Dominguez E, Donovan F, Dooley KL, Doravari S, Douglas R, Downes TP, Drago M, Drever RWP, Driggers JC, Du Z, Ducrot M, Dwyer S, Eberle T, Edo T, Edwards M, Effler A, Eggenstein HB, Ehrens P, Eichholz J, Eikenberry SS, Endrőczi G, Essick R, Etzel T, Evans M, Evans T, Factourovich M, Fafone V, Fairhurst S, Fan X, Fang Q, Farinon S, Farr B, Farr WM, Favata M, Fazi D, Fehrmann H, Fejer MM, Feldbaum D, Feroz F, Ferrante I, Ferreira EC, Ferrini F, Fidecaro F, Finn LS, Fiori I, Fisher RP, Flaminio R, Fournier JD, Franco S, Frasca S, Frasconi F, Frede M, Frei Z, Freise A, Frey R, Fricke TT, Fritschel P, Frolov VV, Fulda P, Fyffe M, Gair JR, Gammaitoni L, Gaonkar S, Garufi F, Gehrels N, Gemme G, Gendre B, Genin E, Gennai A, Ghosh S, Giaime JA, Giardina KD, Giazotto A, Gleason J, Goetz E, Goetz R, Gondan L, González G, Gordon N, Gorodetsky ML, Gossan S, Goßler S, Gouaty R, Gräf C, Graff PB, Granata M, Grant A, Gras S, Gray C, Greenhalgh RJS, Gretarsson AM, Groot P, Grote H, Grover K, Grunewald S, Guidi GM, Guido CJ, Gushwa K, Gustafson EK, Gustafson R, Ha J, Hall ED, Hamilton W, Hammer D, Hammond G, Hanke M, Hanks J, Hanna C, Hannam MD, Hanson J, Harms J, Harry GM, Harry IW, Harstad ED, Hart M, Hartman MT, Haster CJ, Haughian K, Heidmann A, Heintze M, Heitmann H, Hello P, Hemming G, Hendry M, Heng IS, Heptonstall AW, Heurs M, Hewitson M, Hild S, Hoak D, Hodge KA, Hofman D, Holt K, Hopkins P, Horrom T, Hoske D, Hosken DJ, Hough J, Howell EJ, Hu Y, Huerta E, Hughey B, Husa S, Huttner SH, Huynh M, Huynh-Dinh T, Idrisy A, Ingram DR, Inta R, Islas G, Isogai T, Ivanov A, Iyer BR, Izumi K, Jacobson M, Jang H, Jaranowski P, Ji Y, Jiménez-Forteza F, Johnson WW, Jones DI, Jones R, Jonker RJG, Ju L, Haris K, Kalmus P, Kalogera V, Kandhasamy S, Kang G, Kanner JB, Karlen J, Kasprzack M, Katsavounidis E, Katzman W, Kaufer H, Kaufer S, Kaur T, Kawabe K, Kawazoe F, Kéfélian F, Keiser GM, Keitel D, Kelley DB, Kells W, Keppel DG, Khalaidovski A, Khalili FY, Khazanov EA, Kim C, Kim K, Kim NG, Kim N, Kim S, Kim YM, King EJ, King PJ, Kinzel DL, Kissel JS, Klimenko S, Kline J, Koehlenbeck S, Kokeyama K, Kondrashov V, Koranda S, Korth WZ, Kowalska I, Kozak DB, Kringel V, Krishnan B, Królak A, Kuehn G, Kumar A, Kumar DN, Kumar P, Kumar R, Kuo L, Kutynia A, Lam PK, Landry M, Lantz B, Larson S, Lasky PD, Lazzarini A, Lazzaro C, Leaci P, Leavey S, Lebigot EO, Lee CH, Lee HK, Lee HM, Lee J, Lee PJ, Leonardi M, Leong JR, Leonor I, Le Roux A, Leroy N, Letendre N, Levin Y, Levine B, Lewis J, Li TGF, Libbrecht K, Libson A, Lin AC, Littenberg TB, Lockerbie NA, 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Mittleman R, Moe B, Moggi A, Mohan M, Mohapatra SRP, Moraru D, Moreno G, Morgado N, Morriss SR, Mossavi K, Mours B, Mow-Lowry CM, Mueller CL, Mueller G, Mukherjee S, Mullavey A, Munch J, Murphy D, Murray PG, Mytidis A, Nagy MF, Nardecchia I, Naticchioni L, Nayak RK, Necula V, Nelemans G, Neri I, Neri M, Newton G, Nguyen T, Nielsen AB, Nissanke S, Nitz AH, Nocera F, Nolting D, Normandin MEN, Nuttall LK, Ochsner E, O'Dell J, Oelker E, Oh JJ, Oh SH, Ohme F, Omar S, Oppermann P, Oram R, O'Reilly B, Ortega W, O'Shaughnessy R, Osthelder C, Ottaway DJ, Ottens RS, Overmier H, Owen BJ, Padilla C, Pai A, Palashov O, Palomba C, Pan H, Pan Y, Pankow C, Paoletti F, Papa MA, Paris H, Pasqualetti A, Passaquieti R, Passuello D, Pedraza M, Pele A, Penn S, Perreca A, Phelps M, Pichot M, Pickenpack M, Piergiovanni F, Pierro V, Pinard L, Pinto IM, Pitkin M, Poeld J, Poggiani R, Poteomkin A, Powell J, Prasad J, Predoi V, Premachandra S, Prestegard T, Price LR, Prijatelj M, Privitera S, Prodi GA, Prokhorov 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Search for gravitational waves associated with γ-ray bursts detected by the interplanetary network. Phys Rev Lett 2014; 113:011102. [PMID: 25032916 DOI: 10.1103/physrevd.89.122004] [Citation(s) in RCA: 8] [Impact Index Per Article: 0.8] [Reference Citation Analysis] [What about the content of this article? (0)] [Affiliation(s)] [Abstract] [Track Full Text] [Subscribe] [Scholar Register] [Received: 04/07/2014] [Indexed: 05/21/2023]
Abstract
We present the results of a search for gravitational waves associated with 223 γ-ray bursts (GRBs) detected by the InterPlanetary Network (IPN) in 2005-2010 during LIGO's fifth and sixth science runs and Virgo's first, second, and third science runs. The IPN satellites provide accurate times of the bursts and sky localizations that vary significantly from degree scale to hundreds of square degrees. We search for both a well-modeled binary coalescence signal, the favored progenitor model for short GRBs, and for generic, unmodeled gravitational wave bursts. Both searches use the event time and sky localization to improve the gravitational wave search sensitivity as compared to corresponding all-time, all-sky searches. We find no evidence of a gravitational wave signal associated with any of the IPN GRBs in the sample, nor do we find evidence for a population of weak gravitational wave signals associated with the GRBs. For all IPN-detected GRBs, for which a sufficient duration of quality gravitational wave data are available, we place lower bounds on the distance to the source in accordance with an optimistic assumption of gravitational wave emission energy of 10(-2)M⊙c(2) at 150 Hz, and find a median of 13 Mpc. For the 27 short-hard GRBs we place 90% confidence exclusion distances to two source models: a binary neutron star coalescence, with a median distance of 12 Mpc, or the coalescence of a neutron star and black hole, with a median distance of 22 Mpc. Finally, we combine this search with previously published results to provide a population statement for GRB searches in first-generation LIGO and Virgo gravitational wave detectors and a resulting examination of prospects for the advanced gravitational wave detectors.
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Affiliation(s)
- J Aasi
- LIGO, California Institute of Technology, Pasadena, California 91125, USA
| | - B P Abbott
- LIGO, California Institute of Technology, Pasadena, California 91125, USA
| | - R Abbott
- LIGO, California Institute of Technology, Pasadena, California 91125, USA
| | - T Abbott
- Louisiana State University, Baton Rouge, Louisiana 70803, USA
| | - M R Abernathy
- LIGO, California Institute of Technology, Pasadena, California 91125, USA
| | - F Acernese
- Università di Salerno, Fisciano, I-84084 Salerno, Italy and INFN, Sezione di Napoli, Complesso Universitario di Monte S. Angelo, I-80126 Napoli, Italy
| | - K Ackley
- University of Florida, Gainesville, Florida 32611, USA
| | - C Adams
- LIGO Livingston Observatory, Livingston, Louisiana 70754, USA
| | - T Adams
- Cardiff University, Cardiff CF24 3AA, United Kingdom
| | - P Addesso
- University of Sannio at Benevento, I-82100 Benevento, Italy and INFN, Sezione di Napoli, I-80100 Napoli, Italy
| | - R X Adhikari
- LIGO, California Institute of Technology, Pasadena, California 91125, USA
| | - C Affeldt
- Albert-Einstein-Institut, Max-Planck-Institut für Gravitationsphysik, D-30167 Hannover, Germany
| | - M Agathos
- Nikhef, Science Park, 1098 XG Amsterdam, The Netherlands
| | - N Aggarwal
- LIGO, Massachusetts Institute of Technology, Cambridge, Massachusetts 02139, USA
| | - O D Aguiar
- Instituto Nacional de Pesquisas Espaciais, 12227-010 - São José dos Campos, São Paulo, Brazil
| | - P Ajith
- International Centre for Theoretical Sciences, Tata Institute of Fundamental Research, Bangalore 560012, India
| | - A Alemic
- Syracuse University, Syracuse, New York 13244, USA
| | - B Allen
- Albert-Einstein-Institut, Max-Planck-Institut für Gravitationsphysik, D-30167 Hannover, Germany and University of Wisconsin-Milwaukee, Milwaukee, Wisconsin 53201, USA and Leibniz Universität Hannover, D-30167 Hannover, Germany
| | - A Allocca
- Università di Siena, I-53100 Siena, Italy and INFN, Sezione di Pisa, I-56127 Pisa, Italy
| | - D Amariutei
- University of Florida, Gainesville, Florida 32611, USA
| | - M Andersen
- Stanford University, Stanford, California 94305, USA
| | - R A Anderson
- LIGO, California Institute of Technology, Pasadena, California 91125, USA
| | - S B Anderson
- LIGO, California Institute of Technology, Pasadena, California 91125, USA
| | - W G Anderson
- University of Wisconsin-Milwaukee, Milwaukee, Wisconsin 53201, USA
| | - K Arai
- LIGO, California Institute of Technology, Pasadena, California 91125, USA
| | - M C Araya
- LIGO, California Institute of Technology, Pasadena, California 91125, USA
| | - C Arceneaux
- The University of Mississippi, University, Mississippi 38677, USA
| | - J S Areeda
- California State University Fullerton, Fullerton, California 92831, USA
| | - S Ast
- Leibniz Universität Hannover, D-30167 Hannover, Germany
| | - S M Aston
- LIGO Livingston Observatory, Livingston, Louisiana 70754, USA
| | - P Astone
- INFN, Sezione di Roma, I-00185 Roma, Italy
| | - P Aufmuth
- Leibniz Universität Hannover, D-30167 Hannover, Germany
| | - H Augustus
- University of Birmingham, Birmingham B15 2TT, United Kingdom
| | - C Aulbert
- Albert-Einstein-Institut, Max-Planck-Institut für Gravitationsphysik, D-30167 Hannover, Germany
| | - B E Aylott
- University of Birmingham, Birmingham B15 2TT, United Kingdom
| | - S Babak
- Albert-Einstein-Institut, Max-Planck-Institut für Gravitationsphysik, D-14476 Golm, Germany
| | - P T Baker
- Montana State University, Bozeman, Montana 59717, USA
| | - G Ballardin
- European Gravitational Observatory (EGO), I-56021 Cascina, Pisa, Italy
| | - S W Ballmer
- Syracuse University, Syracuse, New York 13244, USA
| | - J C Barayoga
- LIGO, California Institute of Technology, Pasadena, California 91125, USA
| | - M Barbet
- University of Florida, Gainesville, Florida 32611, USA
| | - B C Barish
- LIGO, California Institute of Technology, Pasadena, California 91125, USA
| | - D Barker
- LIGO Hanford Observatory, Richland, Washington 99352, USA
| | - F Barone
- Università di Salerno, Fisciano, I-84084 Salerno, Italy and INFN, Sezione di Napoli, Complesso Universitario di Monte S. Angelo, I-80126 Napoli, Italy
| | - B Barr
- SUPA, University of Glasgow, Glasgow G12 8QQ, United Kingdom
| | - L Barsotti
- LIGO, Massachusetts Institute of Technology, Cambridge, Massachusetts 02139, USA
| | - M Barsuglia
- APC, AstroParticule et Cosmologie, Université Paris Diderot, CNRS/IN2P3, CEA/Irfu, Observatoire de Paris, Sorbonne Paris Cité, 10, rue Alice Domon et Léonie Duquet, F-75205 Paris Cedex 13, France
| | - M A Barton
- LIGO Hanford Observatory, Richland, Washington 99352, USA
| | - I Bartos
- Columbia University, New York, New York 10027, USA
| | - R Bassiri
- Stanford University, Stanford, California 94305, USA
| | - A Basti
- INFN, Sezione di Pisa, I-56127 Pisa, Italy and Università di Pisa, I-56127 Pisa, Italy
| | - J C Batch
- LIGO Hanford Observatory, Richland, Washington 99352, USA
| | - J Bauchrowitz
- Albert-Einstein-Institut, Max-Planck-Institut für Gravitationsphysik, D-30167 Hannover, Germany
| | - Th S Bauer
- Nikhef, Science Park, 1098 XG Amsterdam, The Netherlands
| | - C Baune
- Albert-Einstein-Institut, Max-Planck-Institut für Gravitationsphysik, D-30167 Hannover, Germany
| | - V Bavigadda
- European Gravitational Observatory (EGO), I-56021 Cascina, Pisa, Italy
| | - B Behnke
- Albert-Einstein-Institut, Max-Planck-Institut für Gravitationsphysik, D-14476 Golm, Germany
| | | | - M G Beker
- Nikhef, Science Park, 1098 XG Amsterdam, The Netherlands
| | - C Belczynski
- Astronomical Observatory Warsaw University, 00-478 Warsaw, Poland
| | - A S Bell
- SUPA, University of Glasgow, Glasgow G12 8QQ, United Kingdom
| | - C Bell
- SUPA, University of Glasgow, Glasgow G12 8QQ, United Kingdom
| | - G Bergmann
- Albert-Einstein-Institut, Max-Planck-Institut für Gravitationsphysik, D-30167 Hannover, Germany
| | - D Bersanetti
- Università degli Studi di Genova, I-16146 Genova, Italy and INFN, Sezione di Genova, I-16146 Genova, Italy
| | - A Bertolini
- Nikhef, Science Park, 1098 XG Amsterdam, The Netherlands
| | - J Betzwieser
- LIGO Livingston Observatory, Livingston, Louisiana 70754, USA
| | - I A Bilenko
- Faculty of Physics, Lomonosov Moscow State University, Moscow 119991, Russia
| | - G Billingsley
- LIGO, California Institute of Technology, Pasadena, California 91125, USA
| | - J Birch
- LIGO Livingston Observatory, Livingston, Louisiana 70754, USA
| | - S Biscans
- LIGO, Massachusetts Institute of Technology, Cambridge, Massachusetts 02139, USA
| | - M Bitossi
- INFN, Sezione di Pisa, I-56127 Pisa, Italy
| | - C Biwer
- Syracuse University, Syracuse, New York 13244, USA
| | - M A Bizouard
- LAL, Université Paris-Sud, IN2P3/CNRS, F-91898 Orsay, France
| | - E Black
- LIGO, California Institute of Technology, Pasadena, California 91125, USA
| | - J K Blackburn
- LIGO, California Institute of Technology, Pasadena, California 91125, USA
| | - L Blackburn
- NASA/Goddard Space Flight Center, Greenbelt, Maryland 20771, USA
| | - D Blair
- University of Western Australia, Crawley, Western Australia 6009, Australia
| | - S Bloemen
- Nikhef, Science Park, 1098 XG Amsterdam, The Netherlands and Department of Astrophysics/IMAPP, Radboud University Nijmegen, P.O. Box 9010, 6500 GL Nijmegen, The Netherlands
| | - O Bock
- Albert-Einstein-Institut, Max-Planck-Institut für Gravitationsphysik, D-30167 Hannover, Germany
| | - T P Bodiya
- LIGO, Massachusetts Institute of Technology, Cambridge, Massachusetts 02139, USA
| | - M Boer
- Université Nice-Sophia-Antipolis, CNRS, Observatoire de la Côte d'Azur, F-06304 Nice, France
| | - G Bogaert
- Université Nice-Sophia-Antipolis, CNRS, Observatoire de la Côte d'Azur, F-06304 Nice, France
| | - C Bogan
- Albert-Einstein-Institut, Max-Planck-Institut für Gravitationsphysik, D-30167 Hannover, Germany
| | - C Bond
- University of Birmingham, Birmingham B15 2TT, United Kingdom
| | - F Bondu
- Institut de Physique de Rennes, CNRS, Université de Rennes 1, F-35042 Rennes, France
| | - L Bonelli
- INFN, Sezione di Pisa, I-56127 Pisa, Italy and Università di Pisa, I-56127 Pisa, Italy
| | - R Bonnand
- Laboratoire d'Annecy-le-Vieux de Physique des Particules (LAPP), Université de Savoie, CNRS/IN2P3, F-74941 Annecy-le-Vieux, France
| | - R Bork
- LIGO, California Institute of Technology, Pasadena, California 91125, USA
| | - M Born
- Albert-Einstein-Institut, Max-Planck-Institut für Gravitationsphysik, D-30167 Hannover, Germany
| | - V Boschi
- INFN, Sezione di Pisa, I-56127 Pisa, Italy
| | - Sukanta Bose
- Washington State University, Pullman, Washington 99164, USA and Inter-University Centre for Astronomy and Astrophysics, Pune - 411007, India
| | - L Bosi
- INFN, Sezione di Perugia, I-06123 Perugia, Italy
| | | | - P R Brady
- University of Wisconsin-Milwaukee, Milwaukee, Wisconsin 53201, USA and Yukawa Institute for Theoretical Physics, Kyoto University, Kyoto 606-8502, Japan
| | - V B Braginsky
- Faculty of Physics, Lomonosov Moscow State University, Moscow 119991, Russia
| | - M Branchesi
- Università degli Studi di Urbino 'Carlo Bo', I-61029 Urbino, Italy and INFN, Sezione di Firenze, I-50019 Sesto Fiorentino, Firenze, Italy
| | - J E Brau
- University of Oregon, Eugene, Oregon 97403, USA
| | - T Briant
- Laboratoire Kastler Brossel, ENS, CNRS, UPMC, Université Pierre et Marie Curie, F-75005 Paris, France
| | - D O Bridges
- LIGO Livingston Observatory, Livingston, Louisiana 70754, USA
| | - A Brillet
- Université Nice-Sophia-Antipolis, CNRS, Observatoire de la Côte d'Azur, F-06304 Nice, France
| | - M Brinkmann
- Albert-Einstein-Institut, Max-Planck-Institut für Gravitationsphysik, D-30167 Hannover, Germany
| | - V Brisson
- LAL, Université Paris-Sud, IN2P3/CNRS, F-91898 Orsay, France
| | - A F Brooks
- LIGO, California Institute of Technology, Pasadena, California 91125, USA
| | - D A Brown
- Syracuse University, Syracuse, New York 13244, USA
| | - D D Brown
- University of Birmingham, Birmingham B15 2TT, United Kingdom
| | - F Brückner
- University of Birmingham, Birmingham B15 2TT, United Kingdom
| | - S Buchman
- Stanford University, Stanford, California 94305, USA
| | - A Buikema
- LIGO, Massachusetts Institute of Technology, Cambridge, Massachusetts 02139, USA
| | - T Bulik
- Astronomical Observatory Warsaw University, 00-478 Warsaw, Poland
| | - H J Bulten
- Nikhef, Science Park, 1098 XG Amsterdam, The Netherlands and VU University Amsterdam, 1081 HV Amsterdam, The Netherlands
| | - A Buonanno
- University of Maryland, College Park, Maryland 20742, USA
| | - R Burman
- University of Western Australia, Crawley, Western Australia 6009, Australia
| | - D Buskulic
- Laboratoire d'Annecy-le-Vieux de Physique des Particules (LAPP), Université de Savoie, CNRS/IN2P3, F-74941 Annecy-le-Vieux, France
| | - C Buy
- APC, AstroParticule et Cosmologie, Université Paris Diderot, CNRS/IN2P3, CEA/Irfu, Observatoire de Paris, Sorbonne Paris Cité, 10, rue Alice Domon et Léonie Duquet, F-75205 Paris Cedex 13, France
| | - L Cadonati
- Cardiff University, Cardiff CF24 3AA, United Kingdom and University of Massachusetts Amherst, Amherst, Massachusetts 01003, USA
| | - G Cagnoli
- Laboratoire des Matériaux Avancés (LMA), IN2P3/CNRS, Université de Lyon, F-69622 Villeurbanne, Lyon, France
| | | | - E Calloni
- INFN, Sezione di Napoli, Complesso Universitario di Monte S. Angelo, I-80126 Napoli, Italy and Università di Napoli 'Federico II', Complesso Universitario di Monte S. Angelo, I-80126 Napoli, Italy
| | - J B Camp
- NASA/Goddard Space Flight Center, Greenbelt, Maryland 20771, USA
| | - P Campsie
- SUPA, University of Glasgow, Glasgow G12 8QQ, United Kingdom
| | - K C Cannon
- Canadian Institute for Theoretical Astrophysics, University of Toronto, Toronto, Ontario, M5S 3H8, Canada
| | - B Canuel
- European Gravitational Observatory (EGO), I-56021 Cascina, Pisa, Italy
| | - J Cao
- Tsinghua University, Beijing 100084, China
| | - C D Capano
- University of Maryland, College Park, Maryland 20742, USA
| | - F Carbognani
- European Gravitational Observatory (EGO), I-56021 Cascina, Pisa, Italy
| | - L Carbone
- University of Birmingham, Birmingham B15 2TT, United Kingdom
| | - S Caride
- University of Michigan, Ann Arbor, Michigan 48109, USA
| | - G Castaldi
- University of Sannio at Benevento, I-82100 Benevento, Italy and INFN, Sezione di Napoli, I-80100 Napoli, Italy
| | - S Caudill
- University of Wisconsin-Milwaukee, Milwaukee, Wisconsin 53201, USA
| | - M Cavaglià
- The University of Mississippi, University, Mississippi 38677, USA
| | - F Cavalier
- LAL, Université Paris-Sud, IN2P3/CNRS, F-91898 Orsay, France
| | - R Cavalieri
- European Gravitational Observatory (EGO), I-56021 Cascina, Pisa, Italy
| | - C Celerier
- Stanford University, Stanford, California 94305, USA
| | - G Cella
- INFN, Sezione di Pisa, I-56127 Pisa, Italy
| | - C Cepeda
- LIGO, California Institute of Technology, Pasadena, California 91125, USA
| | - E Cesarini
- INFN, Sezione di Roma Tor Vergata, I-00133 Roma, Italy
| | - R Chakraborty
- LIGO, California Institute of Technology, Pasadena, California 91125, USA
| | - T Chalermsongsak
- LIGO, California Institute of Technology, Pasadena, California 91125, USA
| | - S J Chamberlin
- University of Wisconsin-Milwaukee, Milwaukee, Wisconsin 53201, USA
| | - S Chao
- National Tsing Hua University, Hsinchu 300, Taiwan
| | - P Charlton
- Charles Sturt University, Wagga Wagga, New South Wales 2678, Australia
| | - E Chassande-Mottin
- APC, AstroParticule et Cosmologie, Université Paris Diderot, CNRS/IN2P3, CEA/Irfu, Observatoire de Paris, Sorbonne Paris Cité, 10, rue Alice Domon et Léonie Duquet, F-75205 Paris Cedex 13, France
| | - X Chen
- University of Western Australia, Crawley, Western Australia 6009, Australia
| | - Y Chen
- Caltech-CaRT, Pasadena, California 91125, USA
| | | | - A Chiummo
- European Gravitational Observatory (EGO), I-56021 Cascina, Pisa, Italy
| | - H S Cho
- Pusan National University, Busan 609-735, Korea
| | - M Cho
- University of Maryland, College Park, Maryland 20742, USA
| | - J H Chow
- Australian National University, Canberra, ACT 0200, Australia
| | | | - Q Chu
- University of Western Australia, Crawley, Western Australia 6009, Australia
| | - S S Y Chua
- Australian National University, Canberra, ACT 0200, Australia
| | - S Chung
- University of Western Australia, Crawley, Western Australia 6009, Australia
| | - G Ciani
- University of Florida, Gainesville, Florida 32611, USA
| | - F Clara
- LIGO Hanford Observatory, Richland, Washington 99352, USA
| | - D E Clark
- Stanford University, Stanford, California 94305, USA
| | - J A Clark
- University of Massachusetts Amherst, Amherst, Massachusetts 01003, USA
| | - J H Clayton
- University of Wisconsin-Milwaukee, Milwaukee, Wisconsin 53201, USA
| | - F Cleva
- Université Nice-Sophia-Antipolis, CNRS, Observatoire de la Côte d'Azur, F-06304 Nice, France
| | - E Coccia
- Università di Roma Tor Vergata, I-00133 Roma, Italy and INFN, Gran Sasso Science Institute, I-67100 L'Aquila, Italy
| | - P-F Cohadon
- Laboratoire Kastler Brossel, ENS, CNRS, UPMC, Université Pierre et Marie Curie, F-75005 Paris, France
| | - A Colla
- INFN, Sezione di Roma, I-00185 Roma, Italy and Università di Roma 'La Sapienza', I-00185 Roma, Italy
| | - C Collette
- University of Brussels, Brussels 1050, Belgium
| | - M Colombini
- INFN, Sezione di Perugia, I-06123 Perugia, Italy
| | - L Cominsky
- Sonoma State University, Rohnert Park, California 94928, USA
| | - M Constancio
- Instituto Nacional de Pesquisas Espaciais, 12227-010 - São José dos Campos, São Paulo, Brazil
| | - A Conte
- INFN, Sezione di Roma, I-00185 Roma, Italy and Università di Roma 'La Sapienza', I-00185 Roma, Italy
| | - D Cook
- LIGO Hanford Observatory, Richland, Washington 99352, USA
| | - T R Corbitt
- Louisiana State University, Baton Rouge, Louisiana 70803, USA
| | - N Cornish
- Montana State University, Bozeman, Montana 59717, USA
| | - A Corsi
- The George Washington University, Washington, DC 20052, USA
| | - C A Costa
- Instituto Nacional de Pesquisas Espaciais, 12227-010 - São José dos Campos, São Paulo, Brazil
| | - M W Coughlin
- University of Cambridge, Cambridge CB2 1TN, United Kingdom
| | - J-P Coulon
- Université Nice-Sophia-Antipolis, CNRS, Observatoire de la Côte d'Azur, F-06304 Nice, France
| | - S Countryman
- Columbia University, New York, New York 10027, USA
| | - P Couvares
- Syracuse University, Syracuse, New York 13244, USA
| | - D M Coward
- University of Western Australia, Crawley, Western Australia 6009, Australia
| | - M J Cowart
- LIGO Livingston Observatory, Livingston, Louisiana 70754, USA
| | - D C Coyne
- LIGO, California Institute of Technology, Pasadena, California 91125, USA
| | - R Coyne
- The George Washington University, Washington, DC 20052, USA
| | - K Craig
- SUPA, University of Glasgow, Glasgow G12 8QQ, United Kingdom
| | - J D E Creighton
- University of Wisconsin-Milwaukee, Milwaukee, Wisconsin 53201, USA
| | - R P Croce
- University of Sannio at Benevento, I-82100 Benevento, Italy and INFN, Sezione di Napoli, I-80100 Napoli, Italy
| | - S G Crowder
- University of Minnesota, Minneapolis, Minnesota 55455, USA
| | - A Cumming
- SUPA, University of Glasgow, Glasgow G12 8QQ, United Kingdom
| | - L Cunningham
- SUPA, University of Glasgow, Glasgow G12 8QQ, United Kingdom
| | - E Cuoco
- European Gravitational Observatory (EGO), I-56021 Cascina, Pisa, Italy
| | - C Cutler
- Caltech-CaRT, Pasadena, California 91125, USA
| | - K Dahl
- Albert-Einstein-Institut, Max-Planck-Institut für Gravitationsphysik, D-30167 Hannover, Germany
| | - T Dal Canton
- Albert-Einstein-Institut, Max-Planck-Institut für Gravitationsphysik, D-30167 Hannover, Germany
| | - M Damjanic
- Albert-Einstein-Institut, Max-Planck-Institut für Gravitationsphysik, D-30167 Hannover, Germany
| | - S L Danilishin
- University of Western Australia, Crawley, Western Australia 6009, Australia
| | - S D'Antonio
- INFN, Sezione di Roma Tor Vergata, I-00133 Roma, Italy
| | - K Danzmann
- Albert-Einstein-Institut, Max-Planck-Institut für Gravitationsphysik, D-30167 Hannover, Germany and Leibniz Universität Hannover, D-30167 Hannover, Germany
| | - V Dattilo
- European Gravitational Observatory (EGO), I-56021 Cascina, Pisa, Italy
| | - H Daveloza
- The University of Texas at Brownsville, Brownsville, Texas 78520, USA
| | - M Davier
- LAL, Université Paris-Sud, IN2P3/CNRS, F-91898 Orsay, France
| | - G S Davies
- SUPA, University of Glasgow, Glasgow G12 8QQ, United Kingdom
| | - E J Daw
- The University of Sheffield, Sheffield S10 2TN, United Kingdom
| | - R Day
- European Gravitational Observatory (EGO), I-56021 Cascina, Pisa, Italy
| | - T Dayanga
- Washington State University, Pullman, Washington 99164, USA
| | - D DeBra
- Stanford University, Stanford, California 94305, USA
| | - G Debreczeni
- Wigner RCP, RMKI, H-1121 Budapest, Konkoly Thege Miklós út 29-33, Hungary
| | - J Degallaix
- Laboratoire des Matériaux Avancés (LMA), IN2P3/CNRS, Université de Lyon, F-69622 Villeurbanne, Lyon, France
| | - S Deléglise
- Laboratoire Kastler Brossel, ENS, CNRS, UPMC, Université Pierre et Marie Curie, F-75005 Paris, France
| | - W Del Pozzo
- Nikhef, Science Park, 1098 XG Amsterdam, The Netherlands and University of Birmingham, Birmingham B15 2TT, United Kingdom
| | - T Denker
- Albert-Einstein-Institut, Max-Planck-Institut für Gravitationsphysik, D-30167 Hannover, Germany
| | - T Dent
- Albert-Einstein-Institut, Max-Planck-Institut für Gravitationsphysik, D-30167 Hannover, Germany
| | - H Dereli
- Université Nice-Sophia-Antipolis, CNRS, Observatoire de la Côte d'Azur, F-06304 Nice, France
| | - V Dergachev
- LIGO, California Institute of Technology, Pasadena, California 91125, USA
| | - R De Rosa
- INFN, Sezione di Napoli, Complesso Universitario di Monte S. Angelo, I-80126 Napoli, Italy and Università di Napoli 'Federico II', Complesso Universitario di Monte S. Angelo, I-80126 Napoli, Italy
| | - R T DeRosa
- Louisiana State University, Baton Rouge, Louisiana 70803, USA
| | - R DeSalvo
- University of Sannio at Benevento, I-82100 Benevento, Italy and INFN, Sezione di Napoli, I-80100 Napoli, Italy
| | - S Dhurandhar
- Inter-University Centre for Astronomy and Astrophysics, Pune - 411007, India
| | - M Díaz
- The University of Texas at Brownsville, Brownsville, Texas 78520, USA
| | - J Dickson
- Australian National University, Canberra, ACT 0200, Australia
| | - L Di Fiore
- INFN, Sezione di Napoli, Complesso Universitario di Monte S. Angelo, I-80126 Napoli, Italy
| | - A Di Lieto
- INFN, Sezione di Pisa, I-56127 Pisa, Italy and Università di Pisa, I-56127 Pisa, Italy
| | - I Di Palma
- Albert-Einstein-Institut, Max-Planck-Institut für Gravitationsphysik, D-30167 Hannover, Germany
| | | | - V Dolique
- Laboratoire des Matériaux Avancés (LMA), IN2P3/CNRS, Université de Lyon, F-69622 Villeurbanne, Lyon, France
| | - E Dominguez
- Argentinian Gravitational Wave Group, Cordoba Cordoba 5000, Argentina
| | - F Donovan
- LIGO, Massachusetts Institute of Technology, Cambridge, Massachusetts 02139, USA
| | - K L Dooley
- Albert-Einstein-Institut, Max-Planck-Institut für Gravitationsphysik, D-30167 Hannover, Germany
| | - S Doravari
- LIGO Livingston Observatory, Livingston, Louisiana 70754, USA
| | - R Douglas
- SUPA, University of Glasgow, Glasgow G12 8QQ, United Kingdom
| | - T P Downes
- University of Wisconsin-Milwaukee, Milwaukee, Wisconsin 53201, USA
| | - M Drago
- Università di Trento, I-38050 Povo, Trento, Italy and INFN, Gruppo Collegato di Trento, I-38050 Povo, Trento, Italy
| | - R W P Drever
- LIGO, California Institute of Technology, Pasadena, California 91125, USA
| | - J C Driggers
- LIGO, California Institute of Technology, Pasadena, California 91125, USA
| | - Z Du
- Tsinghua University, Beijing 100084, China
| | - M Ducrot
- Laboratoire d'Annecy-le-Vieux de Physique des Particules (LAPP), Université de Savoie, CNRS/IN2P3, F-74941 Annecy-le-Vieux, France
| | - S Dwyer
- LIGO Hanford Observatory, Richland, Washington 99352, USA
| | - T Eberle
- Albert-Einstein-Institut, Max-Planck-Institut für Gravitationsphysik, D-30167 Hannover, Germany
| | - T Edo
- The University of Sheffield, Sheffield S10 2TN, United Kingdom
| | - M Edwards
- Cardiff University, Cardiff CF24 3AA, United Kingdom
| | - A Effler
- Louisiana State University, Baton Rouge, Louisiana 70803, USA
| | - H-B Eggenstein
- Albert-Einstein-Institut, Max-Planck-Institut für Gravitationsphysik, D-30167 Hannover, Germany
| | - P Ehrens
- LIGO, California Institute of Technology, Pasadena, California 91125, USA
| | - J Eichholz
- University of Florida, Gainesville, Florida 32611, USA
| | | | - G Endrőczi
- Wigner RCP, RMKI, H-1121 Budapest, Konkoly Thege Miklós út 29-33, Hungary
| | - R Essick
- LIGO, Massachusetts Institute of Technology, Cambridge, Massachusetts 02139, USA
| | - T Etzel
- LIGO, California Institute of Technology, Pasadena, California 91125, USA
| | - M Evans
- LIGO, Massachusetts Institute of Technology, Cambridge, Massachusetts 02139, USA
| | - T Evans
- LIGO Livingston Observatory, Livingston, Louisiana 70754, USA
| | | | - V Fafone
- INFN, Sezione di Roma Tor Vergata, I-00133 Roma, Italy and Università di Roma Tor Vergata, I-00133 Roma, Italy
| | - S Fairhurst
- Cardiff University, Cardiff CF24 3AA, United Kingdom
| | - X Fan
- SUPA, University of Glasgow, Glasgow G12 8QQ, United Kingdom
| | - Q Fang
- University of Western Australia, Crawley, Western Australia 6009, Australia
| | - S Farinon
- INFN, Sezione di Genova, I-16146 Genova, Italy
| | - B Farr
- Northwestern University, Evanston, Illinois 60208, USA
| | - W M Farr
- University of Birmingham, Birmingham B15 2TT, United Kingdom
| | - M Favata
- Montclair State University, Montclair, New Jersey 07043, USA
| | - D Fazi
- Northwestern University, Evanston, Illinois 60208, USA
| | - H Fehrmann
- Albert-Einstein-Institut, Max-Planck-Institut für Gravitationsphysik, D-30167 Hannover, Germany
| | - M M Fejer
- Stanford University, Stanford, California 94305, USA
| | - D Feldbaum
- University of Florida, Gainesville, Florida 32611, USA and LIGO Livingston Observatory, Livingston, Louisiana 70754, USA
| | - F Feroz
- University of Cambridge, Cambridge CB2 1TN, United Kingdom
| | - I Ferrante
- INFN, Sezione di Pisa, I-56127 Pisa, Italy and Università di Pisa, I-56127 Pisa, Italy
| | - E C Ferreira
- Instituto Nacional de Pesquisas Espaciais, 12227-010 - São José dos Campos, São Paulo, Brazil
| | - F Ferrini
- European Gravitational Observatory (EGO), I-56021 Cascina, Pisa, Italy
| | - F Fidecaro
- INFN, Sezione di Pisa, I-56127 Pisa, Italy and Università di Pisa, I-56127 Pisa, Italy
| | - L S Finn
- The Pennsylvania State University, University Park, Pennsylvania 16802, USA
| | - I Fiori
- European Gravitational Observatory (EGO), I-56021 Cascina, Pisa, Italy
| | - R P Fisher
- Syracuse University, Syracuse, New York 13244, USA
| | - R Flaminio
- Laboratoire des Matériaux Avancés (LMA), IN2P3/CNRS, Université de Lyon, F-69622 Villeurbanne, Lyon, France
| | - J-D Fournier
- Université Nice-Sophia-Antipolis, CNRS, Observatoire de la Côte d'Azur, F-06304 Nice, France
| | - S Franco
- LAL, Université Paris-Sud, IN2P3/CNRS, F-91898 Orsay, France
| | - S Frasca
- INFN, Sezione di Roma, I-00185 Roma, Italy and Università di Roma 'La Sapienza', I-00185 Roma, Italy
| | - F Frasconi
- INFN, Sezione di Pisa, I-56127 Pisa, Italy
| | - M Frede
- Albert-Einstein-Institut, Max-Planck-Institut für Gravitationsphysik, D-30167 Hannover, Germany
| | - Z Frei
- MTA Eötvös University, 'Lendulet' A. R. G., Budapest 1117, Hungary
| | - A Freise
- University of Birmingham, Birmingham B15 2TT, United Kingdom
| | - R Frey
- University of Oregon, Eugene, Oregon 97403, USA
| | - T T Fricke
- Albert-Einstein-Institut, Max-Planck-Institut für Gravitationsphysik, D-30167 Hannover, Germany
| | - P Fritschel
- LIGO, Massachusetts Institute of Technology, Cambridge, Massachusetts 02139, USA
| | - V V Frolov
- LIGO Livingston Observatory, Livingston, Louisiana 70754, USA
| | - P Fulda
- University of Florida, Gainesville, Florida 32611, USA
| | - M Fyffe
- LIGO Livingston Observatory, Livingston, Louisiana 70754, USA
| | - J R Gair
- University of Cambridge, Cambridge CB2 1TN, United Kingdom
| | - L Gammaitoni
- INFN, Sezione di Perugia, I-06123 Perugia, Italy and Università di Perugia, I-06123 Perugia, Italy
| | - S Gaonkar
- Inter-University Centre for Astronomy and Astrophysics, Pune - 411007, India
| | - F Garufi
- INFN, Sezione di Napoli, Complesso Universitario di Monte S. Angelo, I-80126 Napoli, Italy and Università di Napoli 'Federico II', Complesso Universitario di Monte S. Angelo, I-80126 Napoli, Italy
| | - N Gehrels
- NASA/Goddard Space Flight Center, Greenbelt, Maryland 20771, USA
| | - G Gemme
- INFN, Sezione di Genova, I-16146 Genova, Italy
| | - B Gendre
- Université Nice-Sophia-Antipolis, CNRS, Observatoire de la Côte d'Azur, F-06304 Nice, France
| | - E Genin
- European Gravitational Observatory (EGO), I-56021 Cascina, Pisa, Italy
| | - A Gennai
- INFN, Sezione di Pisa, I-56127 Pisa, Italy
| | - S Ghosh
- Nikhef, Science Park, 1098 XG Amsterdam, The Netherlands and Department of Astrophysics/IMAPP, Radboud University Nijmegen, P.O. Box 9010, 6500 GL Nijmegen, The Netherlands
| | - J A Giaime
- Louisiana State University, Baton Rouge, Louisiana 70803, USA and LIGO Livingston Observatory, Livingston, Louisiana 70754, USA
| | - K D Giardina
- LIGO Livingston Observatory, Livingston, Louisiana 70754, USA
| | - A Giazotto
- INFN, Sezione di Pisa, I-56127 Pisa, Italy
| | - J Gleason
- University of Florida, Gainesville, Florida 32611, USA
| | - E Goetz
- Albert-Einstein-Institut, Max-Planck-Institut für Gravitationsphysik, D-30167 Hannover, Germany
| | - R Goetz
- University of Florida, Gainesville, Florida 32611, USA
| | - L Gondan
- MTA Eötvös University, 'Lendulet' A. R. G., Budapest 1117, Hungary
| | - G González
- Louisiana State University, Baton Rouge, Louisiana 70803, USA
| | - N Gordon
- SUPA, University of Glasgow, Glasgow G12 8QQ, United Kingdom
| | - M L Gorodetsky
- Faculty of Physics, Lomonosov Moscow State University, Moscow 119991, Russia
| | - S Gossan
- Caltech-CaRT, Pasadena, California 91125, USA
| | - S Goßler
- Albert-Einstein-Institut, Max-Planck-Institut für Gravitationsphysik, D-30167 Hannover, Germany
| | - R Gouaty
- Laboratoire d'Annecy-le-Vieux de Physique des Particules (LAPP), Université de Savoie, CNRS/IN2P3, F-74941 Annecy-le-Vieux, France
| | - C Gräf
- SUPA, University of Glasgow, Glasgow G12 8QQ, United Kingdom
| | - P B Graff
- NASA/Goddard Space Flight Center, Greenbelt, Maryland 20771, USA
| | - M Granata
- Laboratoire des Matériaux Avancés (LMA), IN2P3/CNRS, Université de Lyon, F-69622 Villeurbanne, Lyon, France
| | - A Grant
- SUPA, University of Glasgow, Glasgow G12 8QQ, United Kingdom
| | - S Gras
- LIGO, Massachusetts Institute of Technology, Cambridge, Massachusetts 02139, USA
| | - C Gray
- LIGO Hanford Observatory, Richland, Washington 99352, USA
| | - R J S Greenhalgh
- Rutherford Appleton Laboratory, HSIC, Chilton, Didcot, Oxon OX11 0QX, United Kingdom
| | - A M Gretarsson
- Embry-Riddle Aeronautical University, Prescott, Arizona 86301, USA
| | - P Groot
- Department of Astrophysics/IMAPP, Radboud University Nijmegen, P.O. Box 9010, 6500 GL Nijmegen, The Netherlands
| | - H Grote
- Albert-Einstein-Institut, Max-Planck-Institut für Gravitationsphysik, D-30167 Hannover, Germany
| | - K Grover
- University of Birmingham, Birmingham B15 2TT, United Kingdom
| | - S Grunewald
- Albert-Einstein-Institut, Max-Planck-Institut für Gravitationsphysik, D-14476 Golm, Germany
| | - G M Guidi
- Università degli Studi di Urbino 'Carlo Bo', I-61029 Urbino, Italy and INFN, Sezione di Firenze, I-50019 Sesto Fiorentino, Firenze, Italy
| | - C J Guido
- LIGO Livingston Observatory, Livingston, Louisiana 70754, USA
| | - K Gushwa
- LIGO, California Institute of Technology, Pasadena, California 91125, USA
| | - E K Gustafson
- LIGO, California Institute of Technology, Pasadena, California 91125, USA
| | - R Gustafson
- University of Michigan, Ann Arbor, Michigan 48109, USA
| | - J Ha
- Seoul National University, Seoul 151-742, Korea
| | - E D Hall
- LIGO, California Institute of Technology, Pasadena, California 91125, USA
| | - W Hamilton
- Louisiana State University, Baton Rouge, Louisiana 70803, USA
| | - D Hammer
- University of Wisconsin-Milwaukee, Milwaukee, Wisconsin 53201, USA
| | - G Hammond
- SUPA, University of Glasgow, Glasgow G12 8QQ, United Kingdom
| | - M Hanke
- Albert-Einstein-Institut, Max-Planck-Institut für Gravitationsphysik, D-30167 Hannover, Germany
| | - J Hanks
- LIGO Hanford Observatory, Richland, Washington 99352, USA
| | - C Hanna
- The Pennsylvania State University, University Park, Pennsylvania 16802, USA and Perimeter Institute for Theoretical Physics, Waterloo, Ontario N2 L 2Y5, Canada
| | - M D Hannam
- Cardiff University, Cardiff CF24 3AA, United Kingdom
| | - J Hanson
- LIGO Livingston Observatory, Livingston, Louisiana 70754, USA
| | - J Harms
- LIGO, California Institute of Technology, Pasadena, California 91125, USA
| | - G M Harry
- American University, Washington, DC 20016, USA
| | - I W Harry
- Syracuse University, Syracuse, New York 13244, USA
| | - E D Harstad
- University of Oregon, Eugene, Oregon 97403, USA
| | - M Hart
- SUPA, University of Glasgow, Glasgow G12 8QQ, United Kingdom
| | - M T Hartman
- University of Florida, Gainesville, Florida 32611, USA
| | - C-J Haster
- University of Birmingham, Birmingham B15 2TT, United Kingdom
| | - K Haughian
- SUPA, University of Glasgow, Glasgow G12 8QQ, United Kingdom
| | - A Heidmann
- Laboratoire Kastler Brossel, ENS, CNRS, UPMC, Université Pierre et Marie Curie, F-75005 Paris, France
| | - M Heintze
- University of Florida, Gainesville, Florida 32611, USA and LIGO Livingston Observatory, Livingston, Louisiana 70754, USA
| | - H Heitmann
- Université Nice-Sophia-Antipolis, CNRS, Observatoire de la Côte d'Azur, F-06304 Nice, France
| | - P Hello
- LAL, Université Paris-Sud, IN2P3/CNRS, F-91898 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
| | - A W Heptonstall
- LIGO, California Institute of Technology, Pasadena, California 91125, USA
| | - M Heurs
- Albert-Einstein-Institut, Max-Planck-Institut für Gravitationsphysik, D-30167 Hannover, Germany
| | - M Hewitson
- Albert-Einstein-Institut, Max-Planck-Institut für Gravitationsphysik, D-30167 Hannover, Germany
| | - S Hild
- SUPA, University of Glasgow, Glasgow G12 8QQ, United Kingdom
| | - D Hoak
- University of Massachusetts Amherst, Amherst, Massachusetts 01003, USA
| | - K A Hodge
- LIGO, California Institute of Technology, Pasadena, California 91125, USA
| | - D Hofman
- Laboratoire des Matériaux Avancés (LMA), IN2P3/CNRS, Université de Lyon, F-69622 Villeurbanne, Lyon, France
| | - K Holt
- LIGO Livingston Observatory, Livingston, Louisiana 70754, USA
| | - P Hopkins
- Cardiff University, Cardiff CF24 3AA, United Kingdom
| | - T Horrom
- College of William and Mary, Williamsburg, Virginia 23187, USA
| | - D Hoske
- University of Adelaide, Adelaide, South Australia 5005, Australia
| | - D J Hosken
- University of Adelaide, Adelaide, South Australia 5005, Australia
| | - J Hough
- SUPA, University of Glasgow, Glasgow G12 8QQ, United Kingdom
| | - E J Howell
- University of Western Australia, Crawley, Western Australia 6009, Australia
| | - Y Hu
- SUPA, University of Glasgow, Glasgow G12 8QQ, United Kingdom
| | - E Huerta
- Syracuse University, Syracuse, New York 13244, USA
| | - B Hughey
- Embry-Riddle Aeronautical University, Prescott, Arizona 86301, USA
| | - S Husa
- Universitat de les Illes Balears, E-07122 Palma de Mallorca, Spain
| | - S H Huttner
- SUPA, University of Glasgow, Glasgow G12 8QQ, United Kingdom
| | - M Huynh
- University of Wisconsin-Milwaukee, Milwaukee, Wisconsin 53201, USA
| | - T Huynh-Dinh
- LIGO Livingston Observatory, Livingston, Louisiana 70754, USA
| | - A Idrisy
- The Pennsylvania State University, University Park, Pennsylvania 16802, USA
| | - D R Ingram
- LIGO Hanford Observatory, Richland, Washington 99352, USA
| | - R Inta
- The Pennsylvania State University, University Park, Pennsylvania 16802, USA
| | - G Islas
- California State University Fullerton, Fullerton, California 92831, USA
| | - T Isogai
- LIGO, Massachusetts Institute of Technology, Cambridge, Massachusetts 02139, USA
| | - A Ivanov
- LIGO, California Institute of Technology, Pasadena, California 91125, USA
| | - B R Iyer
- Raman Research Institute, Bangalore, Karnataka 560080, India
| | - K Izumi
- LIGO Hanford Observatory, Richland, Washington 99352, USA
| | - M Jacobson
- LIGO, California Institute of Technology, Pasadena, California 91125, USA
| | - H Jang
- Korea Institute of Science and Technology Information, Daejeon 305-806, Korea
| | | | - Y Ji
- Tsinghua University, Beijing 100084, China
| | | | - W W Johnson
- Louisiana State University, Baton Rouge, Louisiana 70803, USA
| | - D I Jones
- University of Southampton, Southampton SO17 1BJ, United Kingdom
| | - R Jones
- SUPA, University of Glasgow, Glasgow G12 8QQ, United Kingdom
| | - R J G Jonker
- Nikhef, Science Park, 1098 XG Amsterdam, The Netherlands
| | - L Ju
- University of Western Australia, Crawley, Western Australia 6009, Australia
| | - K Haris
- IISER-TVM, CET Campus, Trivandrum, Kerala 695016, India
| | - P Kalmus
- LIGO, California Institute of Technology, Pasadena, California 91125, USA
| | - V Kalogera
- Northwestern University, Evanston, Illinois 60208, USA
| | - S Kandhasamy
- The University of Mississippi, University, Mississippi 38677, USA
| | - G Kang
- Korea Institute of Science and Technology Information, Daejeon 305-806, Korea
| | - J B Kanner
- LIGO, California Institute of Technology, Pasadena, California 91125, USA
| | - J Karlen
- University of Massachusetts Amherst, Amherst, Massachusetts 01003, USA
| | - M Kasprzack
- European Gravitational Observatory (EGO), I-56021 Cascina, Pisa, Italy and LAL, Université Paris-Sud, IN2P3/CNRS, F-91898 Orsay, France
| | - E Katsavounidis
- LIGO, Massachusetts Institute of Technology, Cambridge, Massachusetts 02139, USA
| | - W Katzman
- LIGO Livingston Observatory, Livingston, Louisiana 70754, USA
| | - H Kaufer
- Leibniz Universität Hannover, D-30167 Hannover, Germany
| | - S Kaufer
- Leibniz Universität Hannover, D-30167 Hannover, Germany
| | - T Kaur
- University of Western Australia, Crawley, Western Australia 6009, Australia
| | - K Kawabe
- LIGO Hanford Observatory, Richland, Washington 99352, USA
| | - F Kawazoe
- Albert-Einstein-Institut, Max-Planck-Institut für Gravitationsphysik, D-30167 Hannover, Germany
| | - F Kéfélian
- Université Nice-Sophia-Antipolis, CNRS, Observatoire de la Côte d'Azur, F-06304 Nice, France
| | - G M Keiser
- Stanford University, Stanford, California 94305, USA
| | - D Keitel
- Albert-Einstein-Institut, Max-Planck-Institut für Gravitationsphysik, D-30167 Hannover, Germany
| | - D B Kelley
- Syracuse University, Syracuse, New York 13244, USA
| | - W Kells
- LIGO, California Institute of Technology, Pasadena, California 91125, USA
| | - D G Keppel
- Albert-Einstein-Institut, Max-Planck-Institut für Gravitationsphysik, D-30167 Hannover, Germany
| | - A Khalaidovski
- Albert-Einstein-Institut, Max-Planck-Institut für Gravitationsphysik, D-30167 Hannover, Germany
| | - F Y Khalili
- Faculty of Physics, Lomonosov Moscow State University, Moscow 119991, Russia
| | - E A Khazanov
- Institute of Applied Physics, Nizhny Novgorod 603950, Russia
| | - C Kim
- Seoul National University, Seoul 151-742, Korea and Korea Institute of Science and Technology Information, Daejeon 305-806, Korea
| | - K Kim
- Hanyang University, Seoul 133-791, Korea
| | - N G Kim
- Korea Institute of Science and Technology Information, Daejeon 305-806, Korea
| | - N Kim
- Stanford University, Stanford, California 94305, USA
| | - S Kim
- Korea Institute of Science and Technology Information, Daejeon 305-806, Korea
| | - Y-M Kim
- Pusan National University, Busan 609-735, Korea
| | - E J King
- University of Adelaide, Adelaide, South Australia 5005, Australia
| | - P J King
- LIGO, California Institute of Technology, Pasadena, California 91125, USA
| | - D L Kinzel
- LIGO Livingston Observatory, Livingston, Louisiana 70754, USA
| | - J S Kissel
- LIGO Hanford Observatory, Richland, Washington 99352, USA
| | - S Klimenko
- University of Florida, Gainesville, Florida 32611, USA
| | - J Kline
- University of Wisconsin-Milwaukee, Milwaukee, Wisconsin 53201, USA
| | - S Koehlenbeck
- Albert-Einstein-Institut, Max-Planck-Institut für Gravitationsphysik, D-30167 Hannover, Germany
| | - K Kokeyama
- Louisiana State University, Baton Rouge, Louisiana 70803, USA
| | - V Kondrashov
- LIGO, California Institute of Technology, Pasadena, California 91125, USA
| | - S Koranda
- University of Wisconsin-Milwaukee, Milwaukee, Wisconsin 53201, USA
| | - W Z Korth
- LIGO, California Institute of Technology, Pasadena, California 91125, USA
| | - I Kowalska
- Astronomical Observatory Warsaw University, 00-478 Warsaw, Poland
| | - D B Kozak
- LIGO, California Institute of Technology, Pasadena, California 91125, USA
| | - V Kringel
- Albert-Einstein-Institut, Max-Planck-Institut für Gravitationsphysik, D-30167 Hannover, Germany
| | - B Krishnan
- Albert-Einstein-Institut, Max-Planck-Institut für Gravitationsphysik, D-30167 Hannover, Germany
| | - A Królak
- NCBJ, 05-400 Świerk-Otwock, Poland and IM-PAN, 00-956 Warsaw, Poland
| | - G Kuehn
- Albert-Einstein-Institut, Max-Planck-Institut für Gravitationsphysik, D-30167 Hannover, Germany
| | - A Kumar
- Institute for Plasma Research, Bhat, Gandhinagar 382428, India
| | - D Nanda Kumar
- University of Florida, Gainesville, Florida 32611, USA
| | - P Kumar
- Syracuse University, Syracuse, New York 13244, USA
| | - R Kumar
- SUPA, University of Glasgow, Glasgow G12 8QQ, United Kingdom
| | - L Kuo
- National Tsing Hua University, Hsinchu 300, Taiwan
| | | | - P K Lam
- Australian National University, Canberra, ACT 0200, Australia
| | - M Landry
- LIGO Hanford Observatory, Richland, Washington 99352, USA
| | - B Lantz
- Stanford University, Stanford, California 94305, USA
| | - S Larson
- Northwestern University, Evanston, Illinois 60208, USA
| | - P D Lasky
- The University of Melbourne, Parkville, VIC 3010, Australia
| | - A Lazzarini
- LIGO, California Institute of Technology, Pasadena, California 91125, USA
| | - C Lazzaro
- INFN, Sezione di Padova, I-35131 Padova, Italy
| | - P Leaci
- Albert-Einstein-Institut, Max-Planck-Institut für Gravitationsphysik, D-14476 Golm, Germany
| | - S Leavey
- SUPA, University of Glasgow, Glasgow G12 8QQ, United Kingdom
| | | | - C H Lee
- Pusan National University, Busan 609-735, Korea
| | - H K Lee
- Hanyang University, Seoul 133-791, Korea
| | - H M Lee
- Seoul National University, Seoul 151-742, Korea
| | - J Lee
- Hanyang University, Seoul 133-791, Korea
| | - P J Lee
- LIGO, Massachusetts Institute of Technology, Cambridge, Massachusetts 02139, USA
| | - M Leonardi
- Università di Trento, I-38050 Povo, Trento, Italy and INFN, Gruppo Collegato di Trento, I-38050 Povo, Trento, Italy
| | - J R Leong
- Albert-Einstein-Institut, Max-Planck-Institut für Gravitationsphysik, D-30167 Hannover, Germany
| | - I Leonor
- University of Oregon, Eugene, Oregon 97403, USA
| | - A Le Roux
- LIGO Livingston Observatory, Livingston, Louisiana 70754, USA
| | - N Leroy
- LAL, Université Paris-Sud, IN2P3/CNRS, F-91898 Orsay, France
| | - N Letendre
- Laboratoire d'Annecy-le-Vieux de Physique des Particules (LAPP), Université de Savoie, CNRS/IN2P3, F-74941 Annecy-le-Vieux, France
| | - Y Levin
- Monash University, Victoria 3800, Australia
| | - B Levine
- LIGO Hanford Observatory, Richland, Washington 99352, USA
| | - J Lewis
- LIGO, California Institute of Technology, Pasadena, California 91125, USA
| | - T G F Li
- LIGO, California Institute of Technology, Pasadena, California 91125, USA
| | - K Libbrecht
- LIGO, California Institute of Technology, Pasadena, California 91125, USA
| | - A Libson
- LIGO, Massachusetts Institute of Technology, Cambridge, Massachusetts 02139, USA
| | - A C Lin
- Stanford University, Stanford, California 94305, USA
| | | | - N A Lockerbie
- SUPA, University of Strathclyde, Glasgow G1 1XQ, United Kingdom
| | - V Lockett
- California State University Fullerton, Fullerton, California 92831, USA
| | - D Lodhia
- University of Birmingham, Birmingham B15 2TT, United Kingdom
| | - K Loew
- Embry-Riddle Aeronautical University, Prescott, Arizona 86301, USA
| | - J Logue
- SUPA, University of Glasgow, Glasgow G12 8QQ, United Kingdom
| | - A L Lombardi
- University of Massachusetts Amherst, Amherst, Massachusetts 01003, USA
| | - E Lopez
- Louisiana Tech University, Ruston, Louisiana 71272, USA
| | - M Lorenzini
- INFN, Sezione di Roma Tor Vergata, I-00133 Roma, Italy and Università di Roma Tor Vergata, I-00133 Roma, Italy
| | | | - M Lormand
- LIGO Livingston Observatory, Livingston, Louisiana 70754, USA
| | - G Losurdo
- INFN, Sezione di Firenze, I-50019 Sesto Fiorentino, Firenze, Italy
| | - J Lough
- Syracuse University, Syracuse, New York 13244, USA
| | - M J Lubinski
- LIGO Hanford Observatory, Richland, Washington 99352, USA
| | - H Lück
- Albert-Einstein-Institut, Max-Planck-Institut für Gravitationsphysik, D-30167 Hannover, Germany and Leibniz Universität Hannover, D-30167 Hannover, Germany
| | - A P Lundgren
- Albert-Einstein-Institut, Max-Planck-Institut für Gravitationsphysik, D-30167 Hannover, Germany
| | - Y Ma
- University of Western Australia, Crawley, Western Australia 6009, Australia
| | - E P Macdonald
- Cardiff University, Cardiff CF24 3AA, United Kingdom
| | - T MacDonald
- Stanford University, Stanford, California 94305, USA
| | - B Machenschalk
- Albert-Einstein-Institut, Max-Planck-Institut für Gravitationsphysik, D-30167 Hannover, Germany
| | - M MacInnis
- LIGO, Massachusetts Institute of Technology, Cambridge, Massachusetts 02139, USA
| | - D M Macleod
- Louisiana State University, Baton Rouge, Louisiana 70803, USA
| | | | - R Magee
- Washington State University, Pullman, Washington 99164, USA
| | - M Mageswaran
- LIGO, California Institute of Technology, Pasadena, California 91125, USA
| | - C Maglione
- Argentinian Gravitational Wave Group, Cordoba Cordoba 5000, Argentina
| | - K Mailand
- LIGO, California Institute of Technology, Pasadena, California 91125, USA
| | - E Majorana
- INFN, Sezione di Roma, I-00185 Roma, Italy
| | | | - V Malvezzi
- INFN, Sezione di Roma Tor Vergata, I-00133 Roma, Italy and Università di Roma Tor Vergata, I-00133 Roma, Italy
| | - N Man
- Université Nice-Sophia-Antipolis, CNRS, Observatoire de la Côte d'Azur, F-06304 Nice, France
| | - G M Manca
- Albert-Einstein-Institut, Max-Planck-Institut für Gravitationsphysik, D-30167 Hannover, Germany
| | - I Mandel
- University of Birmingham, Birmingham B15 2TT, United Kingdom
| | - V Mandic
- University of Minnesota, Minneapolis, Minnesota 55455, USA
| | - V Mangano
- INFN, Sezione di Roma, I-00185 Roma, Italy and Università di Roma 'La Sapienza', I-00185 Roma, Italy
| | - N M Mangini
- University of Massachusetts Amherst, Amherst, Massachusetts 01003, USA
| | - G Mansell
- Australian National University, Canberra, ACT 0200, Australia
| | | | - F Marchesoni
- INFN, Sezione di Perugia, I-06123 Perugia, Italy and Università di Camerino, Dipartimento di Fisica, I-62032 Camerino, Italy
| | - F Marion
- Laboratoire d'Annecy-le-Vieux de Physique des Particules (LAPP), Université de Savoie, CNRS/IN2P3, F-74941 Annecy-le-Vieux, France
| | - S Márka
- Columbia University, New York, New York 10027, USA
| | - Z Márka
- Columbia University, New York, New York 10027, USA
| | - A Markosyan
- Stanford University, Stanford, California 94305, USA
| | - E Maros
- LIGO, California Institute of Technology, Pasadena, California 91125, USA
| | - J Marque
- European Gravitational Observatory (EGO), I-56021 Cascina, Pisa, Italy
| | - F Martelli
- Università degli Studi di Urbino 'Carlo Bo', I-61029 Urbino, Italy and 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
- University of Florida, Gainesville, Florida 32611, USA
| | - L Martinelli
- Université Nice-Sophia-Antipolis, CNRS, Observatoire de la Côte d'Azur, F-06304 Nice, France
| | - D Martynov
- LIGO, California Institute of Technology, Pasadena, California 91125, USA
| | - J N Marx
- LIGO, California Institute of Technology, Pasadena, California 91125, USA
| | - K Mason
- LIGO, Massachusetts Institute of Technology, Cambridge, Massachusetts 02139, USA
| | - A Masserot
- Laboratoire d'Annecy-le-Vieux de Physique des Particules (LAPP), Université de Savoie, CNRS/IN2P3, F-74941 Annecy-le-Vieux, France
| | | | - F Matichard
- LIGO, Massachusetts Institute of Technology, Cambridge, Massachusetts 02139, USA
| | - L Matone
- Columbia University, New York, New York 10027, USA
| | - N Mavalvala
- LIGO, Massachusetts Institute of Technology, Cambridge, Massachusetts 02139, USA
| | - G May
- Louisiana State University, Baton Rouge, Louisiana 70803, USA
| | - N Mazumder
- IISER-TVM, CET Campus, Trivandrum, Kerala 695016, India
| | - G Mazzolo
- Albert-Einstein-Institut, Max-Planck-Institut für Gravitationsphysik, D-30167 Hannover, Germany
| | - R McCarthy
- LIGO Hanford Observatory, Richland, Washington 99352, USA
| | - D E McClelland
- Australian National University, Canberra, ACT 0200, Australia
| | - S C McGuire
- Southern University and A&M College, Baton Rouge, Louisiana 70813, USA
| | - G McIntyre
- LIGO, California Institute of Technology, Pasadena, California 91125, USA
| | - J McIver
- University of Massachusetts Amherst, Amherst, Massachusetts 01003, USA
| | - K McLin
- Sonoma State University, Rohnert Park, California 94928, USA
| | - D Meacher
- Université Nice-Sophia-Antipolis, CNRS, Observatoire de la Côte d'Azur, F-06304 Nice, France
| | - G D Meadors
- University of Michigan, Ann Arbor, Michigan 48109, USA
| | - M Mehmet
- Albert-Einstein-Institut, Max-Planck-Institut für Gravitationsphysik, D-30167 Hannover, Germany
| | - J Meidam
- Nikhef, Science Park, 1098 XG Amsterdam, The Netherlands
| | - M Meinders
- Leibniz Universität Hannover, D-30167 Hannover, Germany
| | - A Melatos
- The University of Melbourne, Parkville, VIC 3010, Australia
| | - G Mendell
- LIGO Hanford Observatory, Richland, Washington 99352, USA
| | - R A Mercer
- University of Wisconsin-Milwaukee, Milwaukee, Wisconsin 53201, USA
| | - S Meshkov
- LIGO, California Institute of Technology, Pasadena, California 91125, USA
| | - C Messenger
- SUPA, University of Glasgow, Glasgow G12 8QQ, United Kingdom
| | - M S Meyer
- LIGO Livingston Observatory, Livingston, Louisiana 70754, USA
| | - P M Meyers
- University of Minnesota, Minneapolis, Minnesota 55455, USA
| | - F Mezzani
- INFN, Sezione di Roma, I-00185 Roma, Italy and Università di Roma 'La Sapienza', I-00185 Roma, Italy
| | - H Miao
- Caltech-CaRT, Pasadena, California 91125, USA
| | - C Michel
- Laboratoire des Matériaux Avancés (LMA), IN2P3/CNRS, Université de Lyon, F-69622 Villeurbanne, Lyon, France
| | - E E Mikhailov
- College of William and Mary, Williamsburg, Virginia 23187, USA
| | - L Milano
- INFN, Sezione di Napoli, Complesso Universitario di Monte S. Angelo, I-80126 Napoli, Italy and Università di Napoli 'Federico II', Complesso Universitario di Monte S. Angelo, I-80126 Napoli, Italy
| | - J Miller
- LIGO, Massachusetts Institute of Technology, Cambridge, Massachusetts 02139, USA
| | - Y Minenkov
- INFN, Sezione di Roma Tor Vergata, I-00133 Roma, Italy
| | | | - C Mishra
- IISER-TVM, CET Campus, Trivandrum, Kerala 695016, India
| | - 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, Massachusetts Institute of Technology, Cambridge, Massachusetts 02139, USA
| | - B Moe
- University of Wisconsin-Milwaukee, Milwaukee, Wisconsin 53201, USA
| | - A Moggi
- INFN, Sezione di Pisa, I-56127 Pisa, Italy
| | - M Mohan
- European Gravitational Observatory (EGO), I-56021 Cascina, Pisa, Italy
| | | | - D Moraru
- LIGO Hanford Observatory, Richland, Washington 99352, USA
| | - G Moreno
- LIGO Hanford Observatory, Richland, Washington 99352, USA
| | - N Morgado
- Laboratoire des Matériaux Avancés (LMA), IN2P3/CNRS, Université de Lyon, F-69622 Villeurbanne, Lyon, France
| | - S R Morriss
- The University of Texas at Brownsville, Brownsville, Texas 78520, USA
| | - K Mossavi
- Albert-Einstein-Institut, Max-Planck-Institut für Gravitationsphysik, D-30167 Hannover, Germany
| | - B Mours
- Laboratoire d'Annecy-le-Vieux de Physique des Particules (LAPP), Université de Savoie, CNRS/IN2P3, F-74941 Annecy-le-Vieux, France
| | - C M Mow-Lowry
- Albert-Einstein-Institut, Max-Planck-Institut für Gravitationsphysik, D-30167 Hannover, Germany
| | - C L Mueller
- University of Florida, Gainesville, Florida 32611, USA
| | - G Mueller
- University of Florida, Gainesville, Florida 32611, USA
| | - S Mukherjee
- The University of Texas at Brownsville, Brownsville, Texas 78520, USA
| | - A Mullavey
- Louisiana State University, Baton Rouge, Louisiana 70803, USA
| | - J Munch
- University of Adelaide, Adelaide, South Australia 5005, Australia
| | - D Murphy
- Columbia University, New York, New York 10027, USA
| | - P G Murray
- SUPA, University of Glasgow, Glasgow G12 8QQ, United Kingdom
| | - A Mytidis
- University of Florida, Gainesville, Florida 32611, USA
| | - M F Nagy
- Wigner RCP, RMKI, H-1121 Budapest, Konkoly Thege Miklós út 29-33, Hungary
| | - I Nardecchia
- INFN, Sezione di Roma Tor Vergata, I-00133 Roma, Italy and Università di Roma Tor Vergata, I-00133 Roma, Italy
| | - L Naticchioni
- INFN, Sezione di Roma, I-00185 Roma, Italy and Università di Roma 'La Sapienza', I-00185 Roma, Italy
| | - R K Nayak
- IISER-Kolkata, Mohanpur, West Bengal 741252, India
| | - V Necula
- University of Florida, Gainesville, Florida 32611, USA
| | - G Nelemans
- Nikhef, Science Park, 1098 XG Amsterdam, The Netherlands and Department of Astrophysics/IMAPP, Radboud University Nijmegen, P.O. Box 9010, 6500 GL Nijmegen, The Netherlands
| | - I Neri
- INFN, Sezione di Perugia, I-06123 Perugia, Italy and Università di Perugia, I-06123 Perugia, Italy
| | - M Neri
- Università degli Studi di Genova, I-16146 Genova, Italy and INFN, Sezione di Genova, I-16146 Genova, Italy
| | - G Newton
- SUPA, University of Glasgow, Glasgow G12 8QQ, United Kingdom
| | - T Nguyen
- Australian National University, Canberra, ACT 0200, Australia
| | - A B Nielsen
- Albert-Einstein-Institut, Max-Planck-Institut für Gravitationsphysik, D-30167 Hannover, Germany
| | - S Nissanke
- Caltech-CaRT, Pasadena, California 91125, USA
| | - A H Nitz
- Syracuse University, Syracuse, New York 13244, USA
| | - F Nocera
- European Gravitational Observatory (EGO), I-56021 Cascina, Pisa, Italy
| | - D Nolting
- LIGO Livingston Observatory, Livingston, Louisiana 70754, USA
| | - M E N Normandin
- The University of Texas at Brownsville, Brownsville, Texas 78520, USA
| | - L K Nuttall
- University of Wisconsin-Milwaukee, Milwaukee, Wisconsin 53201, USA
| | - E Ochsner
- University of Wisconsin-Milwaukee, Milwaukee, Wisconsin 53201, USA
| | - J O'Dell
- Rutherford Appleton Laboratory, HSIC, Chilton, Didcot, Oxon OX11 0QX, United Kingdom
| | - E Oelker
- LIGO, Massachusetts Institute of Technology, Cambridge, Massachusetts 02139, USA
| | - J J Oh
- National Institute for Mathematical Sciences, Daejeon 305-390, Korea
| | - S H Oh
- National Institute for Mathematical Sciences, Daejeon 305-390, Korea
| | - F Ohme
- Cardiff University, Cardiff CF24 3AA, United Kingdom
| | - S Omar
- Stanford University, Stanford, California 94305, USA
| | - P Oppermann
- Albert-Einstein-Institut, Max-Planck-Institut für Gravitationsphysik, D-30167 Hannover, Germany
| | - R Oram
- LIGO Livingston Observatory, Livingston, Louisiana 70754, USA
| | - B O'Reilly
- LIGO Livingston Observatory, Livingston, Louisiana 70754, USA
| | - W Ortega
- Argentinian Gravitational Wave Group, Cordoba Cordoba 5000, Argentina
| | - R O'Shaughnessy
- University of Wisconsin-Milwaukee, Milwaukee, Wisconsin 53201, USA
| | - C Osthelder
- LIGO, California Institute of Technology, Pasadena, California 91125, USA
| | - D J Ottaway
- University of Adelaide, Adelaide, South Australia 5005, Australia
| | - R S Ottens
- University of Florida, Gainesville, Florida 32611, USA
| | - H Overmier
- LIGO Livingston Observatory, Livingston, Louisiana 70754, USA
| | - B J Owen
- The Pennsylvania State University, University Park, Pennsylvania 16802, USA
| | - C Padilla
- California State University Fullerton, Fullerton, California 92831, USA
| | - A Pai
- IISER-TVM, CET Campus, Trivandrum, Kerala 695016, India
| | - 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 300, Taiwan
| | - Y Pan
- University of Maryland, College Park, Maryland 20742, USA
| | - C Pankow
- University of Wisconsin-Milwaukee, Milwaukee, Wisconsin 53201, USA
| | - F Paoletti
- INFN, Sezione di Pisa, I-56127 Pisa, Italy and European Gravitational Observatory (EGO), I-56021 Cascina, Pisa, Italy
| | - M A Papa
- University of Wisconsin-Milwaukee, Milwaukee, Wisconsin 53201, USA and Albert-Einstein-Institut, Max-Planck-Institut für Gravitationsphysik, D-14476 Golm, Germany
| | - H Paris
- Stanford University, Stanford, California 94305, USA
| | - A Pasqualetti
- European Gravitational Observatory (EGO), I-56021 Cascina, Pisa, Italy
| | - R Passaquieti
- INFN, Sezione di Pisa, I-56127 Pisa, Italy and Università di Pisa, I-56127 Pisa, Italy
| | | | - M Pedraza
- LIGO, California Institute of Technology, Pasadena, California 91125, USA
| | - A Pele
- LIGO Hanford Observatory, Richland, Washington 99352, USA
| | - S Penn
- Hobart and William Smith Colleges, Geneva, New York 14456, USA
| | - A Perreca
- Syracuse University, Syracuse, New York 13244, USA
| | - M Phelps
- LIGO, California Institute of Technology, Pasadena, California 91125, USA
| | - M Pichot
- Université Nice-Sophia-Antipolis, CNRS, Observatoire de la Côte d'Azur, F-06304 Nice, France
| | - M Pickenpack
- Albert-Einstein-Institut, Max-Planck-Institut für Gravitationsphysik, D-30167 Hannover, Germany
| | - F Piergiovanni
- Università degli Studi di Urbino 'Carlo Bo', I-61029 Urbino, Italy and INFN, Sezione di Firenze, I-50019 Sesto Fiorentino, Firenze, Italy
| | - V Pierro
- University of Sannio at Benevento, I-82100 Benevento, Italy and INFN, Sezione di Napoli, I-80100 Napoli, Italy
| | - L Pinard
- Laboratoire des Matériaux Avancés (LMA), IN2P3/CNRS, Université de Lyon, F-69622 Villeurbanne, Lyon, France
| | - I M Pinto
- University of Sannio at Benevento, I-82100 Benevento, Italy and INFN, Sezione di Napoli, I-80100 Napoli, Italy
| | - M Pitkin
- SUPA, University of Glasgow, Glasgow G12 8QQ, United Kingdom
| | - J Poeld
- Albert-Einstein-Institut, Max-Planck-Institut für Gravitationsphysik, D-30167 Hannover, Germany
| | - R Poggiani
- INFN, Sezione di Pisa, I-56127 Pisa, Italy and Università di Pisa, I-56127 Pisa, Italy
| | - A Poteomkin
- Institute of Applied Physics, Nizhny Novgorod 603950, Russia
| | - J Powell
- SUPA, University of Glasgow, Glasgow G12 8QQ, United Kingdom
| | - J Prasad
- Inter-University Centre for Astronomy and Astrophysics, Pune - 411007, India
| | - V Predoi
- Cardiff University, Cardiff CF24 3AA, United Kingdom
| | | | - T Prestegard
- University of Minnesota, Minneapolis, Minnesota 55455, USA
| | - L R Price
- LIGO, California Institute of Technology, Pasadena, California 91125, USA
| | - M Prijatelj
- European Gravitational Observatory (EGO), I-56021 Cascina, Pisa, Italy
| | - S Privitera
- LIGO, California Institute of Technology, Pasadena, California 91125, USA
| | - G A Prodi
- Università di Trento, I-38050 Povo, Trento, Italy and INFN, Gruppo Collegato di Trento, I-38050 Povo, Trento, Italy
| | - L Prokhorov
- Faculty of Physics, Lomonosov Moscow State University, Moscow 119991, Russia
| | - O Puncken
- The University of Texas at Brownsville, Brownsville, Texas 78520, USA
| | - M Punturo
- INFN, Sezione di Perugia, I-06123 Perugia, Italy
| | - P Puppo
- INFN, Sezione di Roma, I-00185 Roma, Italy
| | - M Pürrer
- Cardiff University, Cardiff CF24 3AA, United Kingdom
| | - J Qin
- University of Western Australia, Crawley, Western Australia 6009, Australia
| | - V Quetschke
- The University of Texas at Brownsville, Brownsville, Texas 78520, USA
| | - E Quintero
- LIGO, California Institute of Technology, Pasadena, California 91125, USA
| | | | - F J Raab
- LIGO Hanford Observatory, Richland, Washington 99352, USA
| | - D S Rabeling
- Nikhef, Science Park, 1098 XG Amsterdam, The Netherlands and VU University Amsterdam, 1081 HV Amsterdam, The Netherlands
| | - I Rácz
- Wigner RCP, RMKI, H-1121 Budapest, Konkoly Thege Miklós út 29-33, Hungary
| | - H Radkins
- LIGO Hanford Observatory, Richland, Washington 99352, USA
| | - P Raffai
- MTA Eötvös University, 'Lendulet' A. R. G., Budapest 1117, Hungary
| | - S Raja
- RRCAT, Indore, Madhya Pradesh 452013, India
| | - G Rajalakshmi
- Tata Institute for Fundamental Research, Mumbai 400005, India
| | - M Rakhmanov
- The University of Texas at Brownsville, Brownsville, Texas 78520, USA
| | - C Ramet
- LIGO Livingston Observatory, Livingston, Louisiana 70754, USA
| | - K Ramirez
- The University of Texas at Brownsville, Brownsville, Texas 78520, USA
| | - P Rapagnani
- INFN, Sezione di Roma, I-00185 Roma, Italy and Università di Roma 'La Sapienza', I-00185 Roma, Italy
| | - V Raymond
- LIGO, California Institute of Technology, Pasadena, California 91125, USA
| | - M Razzano
- INFN, Sezione di Pisa, I-56127 Pisa, Italy and Università di Pisa, I-56127 Pisa, Italy
| | - V Re
- INFN, Sezione di Roma Tor Vergata, I-00133 Roma, Italy and Università di Roma Tor Vergata, I-00133 Roma, Italy
| | - S Recchia
- Università di Roma Tor Vergata, I-00133 Roma, Italy and INFN, Gran Sasso Science Institute, I-67100 L'Aquila, Italy
| | - C M Reed
- LIGO Hanford Observatory, Richland, Washington 99352, USA
| | - T Regimbau
- Université Nice-Sophia-Antipolis, CNRS, Observatoire de la Côte d'Azur, F-06304 Nice, France
| | - S Reid
- SUPA, University of the West of Scotland, Paisley PA1 2BE, United Kingdom
| | - D H Reitze
- LIGO, California Institute of Technology, Pasadena, California 91125, USA and University of Florida, Gainesville, Florida 32611, USA
| | - O Reula
- Argentinian Gravitational Wave Group, Cordoba Cordoba 5000, Argentina
| | - E Rhoades
- Embry-Riddle Aeronautical University, Prescott, Arizona 86301, USA
| | - F Ricci
- INFN, Sezione di Roma, I-00185 Roma, Italy and Università di Roma 'La Sapienza', I-00185 Roma, Italy
| | - R Riesen
- LIGO Livingston Observatory, Livingston, Louisiana 70754, USA
| | - K Riles
- University of Michigan, Ann Arbor, Michigan 48109, USA
| | - N A Robertson
- LIGO, California Institute of Technology, Pasadena, California 91125, USA and SUPA, University of Glasgow, Glasgow G12 8QQ, United Kingdom
| | - F Robinet
- LAL, Université Paris-Sud, IN2P3/CNRS, F-91898 Orsay, France
| | - A Rocchi
- INFN, Sezione di Roma Tor Vergata, I-00133 Roma, Italy
| | - S B Roddy
- LIGO Livingston Observatory, Livingston, Louisiana 70754, USA
| | - L Rolland
- Laboratoire d'Annecy-le-Vieux de Physique des Particules (LAPP), Université de Savoie, CNRS/IN2P3, F-74941 Annecy-le-Vieux, France
| | - J G Rollins
- LIGO, California Institute of Technology, Pasadena, California 91125, USA
| | - R Romano
- Università di Salerno, Fisciano, I-84084 Salerno, Italy and INFN, Sezione di Napoli, Complesso Universitario di Monte S. Angelo, I-80126 Napoli, Italy
| | - G Romanov
- College of William and Mary, Williamsburg, Virginia 23187, USA
| | - J H Romie
- LIGO Livingston Observatory, Livingston, Louisiana 70754, USA
| | - D Rosińska
- CAMK-PAN, 00-716 Warsaw, Poland and Institute of Astronomy, 65-265 Zielona Góra, Poland
| | - S Rowan
- SUPA, University of Glasgow, Glasgow G12 8QQ, United Kingdom
| | - A Rüdiger
- Albert-Einstein-Institut, Max-Planck-Institut für Gravitationsphysik, D-30167 Hannover, Germany
| | - P Ruggi
- European Gravitational Observatory (EGO), I-56021 Cascina, Pisa, Italy
| | - K Ryan
- LIGO Hanford Observatory, Richland, Washington 99352, USA
| | - F Salemi
- Albert-Einstein-Institut, Max-Planck-Institut für Gravitationsphysik, D-30167 Hannover, Germany
| | - L Sammut
- The University of Melbourne, Parkville, VIC 3010, Australia
| | - V Sandberg
- LIGO Hanford Observatory, Richland, Washington 99352, USA
| | - J R Sanders
- University of Michigan, Ann Arbor, Michigan 48109, USA
| | - S Sankar
- LIGO, Massachusetts Institute of Technology, Cambridge, Massachusetts 02139, USA
| | - V Sannibale
- LIGO, California Institute of Technology, Pasadena, California 91125, USA
| | | | - E Saracco
- Laboratoire des Matériaux Avancés (LMA), IN2P3/CNRS, Université de Lyon, F-69622 Villeurbanne, Lyon, France
| | - B Sassolas
- Laboratoire des Matériaux Avancés (LMA), IN2P3/CNRS, Université de Lyon, F-69622 Villeurbanne, Lyon, France
| | | | - P R Saulson
- Syracuse University, Syracuse, New York 13244, USA
| | - R Savage
- LIGO Hanford Observatory, Richland, Washington 99352, USA
| | - J Scheuer
- Northwestern University, Evanston, Illinois 60208, USA
| | - R Schilling
- Albert-Einstein-Institut, Max-Planck-Institut für Gravitationsphysik, D-30167 Hannover, Germany
| | - M Schilman
- Argentinian Gravitational Wave Group, Cordoba Cordoba 5000, Argentina
| | - P Schmidt
- Cardiff University, Cardiff CF24 3AA, United Kingdom
| | - R Schnabel
- Albert-Einstein-Institut, Max-Planck-Institut für Gravitationsphysik, D-30167 Hannover, Germany and Leibniz Universität Hannover, D-30167 Hannover, Germany
| | | | - E Schreiber
- Albert-Einstein-Institut, Max-Planck-Institut für Gravitationsphysik, D-30167 Hannover, Germany
| | - D Schuette
- Albert-Einstein-Institut, Max-Planck-Institut für Gravitationsphysik, D-30167 Hannover, Germany
| | - B F Schutz
- Cardiff University, Cardiff CF24 3AA, United Kingdom and Albert-Einstein-Institut, Max-Planck-Institut für Gravitationsphysik, D-14476 Golm, Germany
| | - J Scott
- SUPA, University of Glasgow, Glasgow G12 8QQ, United Kingdom
| | - S M Scott
- Australian National University, Canberra, ACT 0200, Australia
| | - D Sellers
- LIGO Livingston Observatory, Livingston, Louisiana 70754, USA
| | - A S Sengupta
- Indian Institute of Technology, Gandhinagar, Ahmedabad, Gujarat 382424, India
| | - D Sentenac
- European Gravitational Observatory (EGO), I-56021 Cascina, Pisa, Italy
| | - V Sequino
- INFN, Sezione di Roma Tor Vergata, I-00133 Roma, Italy and Università di Roma Tor Vergata, I-00133 Roma, Italy
| | - A Sergeev
- Institute of Applied Physics, Nizhny Novgorod 603950, Russia
| | - D A Shaddock
- Australian National University, Canberra, ACT 0200, Australia
| | - S Shah
- Nikhef, Science Park, 1098 XG Amsterdam, The Netherlands and Department of Astrophysics/IMAPP, Radboud University Nijmegen, P.O. Box 9010, 6500 GL Nijmegen, The Netherlands
| | - M S Shahriar
- Northwestern University, Evanston, Illinois 60208, USA
| | - M Shaltev
- Albert-Einstein-Institut, Max-Planck-Institut für Gravitationsphysik, D-30167 Hannover, Germany
| | - Z Shao
- LIGO, California Institute of Technology, Pasadena, California 91125, USA
| | - B Shapiro
- Stanford University, Stanford, California 94305, USA
| | - P Shawhan
- University of Maryland, College Park, Maryland 20742, USA
| | - D H Shoemaker
- LIGO, Massachusetts Institute of Technology, Cambridge, Massachusetts 02139, USA
| | - T L Sidery
- University of Birmingham, Birmingham B15 2TT, United Kingdom
| | - K Siellez
- Université Nice-Sophia-Antipolis, CNRS, Observatoire de la Côte d'Azur, F-06304 Nice, France
| | - X Siemens
- University of Wisconsin-Milwaukee, Milwaukee, Wisconsin 53201, USA
| | - D Sigg
- LIGO Hanford Observatory, Richland, Washington 99352, USA
| | - D Simakov
- Albert-Einstein-Institut, Max-Planck-Institut für Gravitationsphysik, D-30167 Hannover, Germany
| | - A Singer
- LIGO, California Institute of Technology, Pasadena, California 91125, USA
| | - L Singer
- LIGO, California Institute of Technology, Pasadena, California 91125, USA
| | - R Singh
- Louisiana State University, Baton Rouge, Louisiana 70803, USA
| | - A M Sintes
- Universitat de les Illes Balears, E-07122 Palma de Mallorca, Spain
| | - B J J Slagmolen
- Australian National University, Canberra, ACT 0200, Australia
| | - J Slutsky
- NASA/Goddard Space Flight Center, Greenbelt, Maryland 20771, USA
| | - J R Smith
- California State University Fullerton, Fullerton, California 92831, USA
| | - M R Smith
- LIGO, California Institute of Technology, Pasadena, California 91125, USA
| | - R J E Smith
- LIGO, California Institute of Technology, Pasadena, California 91125, USA
| | - N D Smith-Lefebvre
- LIGO, California Institute of Technology, Pasadena, California 91125, USA
| | - E J Son
- National Institute for Mathematical Sciences, Daejeon 305-390, Korea
| | - B Sorazu
- SUPA, University of Glasgow, Glasgow G12 8QQ, United Kingdom
| | - T Souradeep
- Inter-University Centre for Astronomy and Astrophysics, Pune - 411007, India
| | - A Staley
- Columbia University, New York, New York 10027, USA
| | - J Stebbins
- Stanford University, Stanford, California 94305, USA
| | - M Steinke
- Albert-Einstein-Institut, Max-Planck-Institut für Gravitationsphysik, D-30167 Hannover, Germany
| | - J Steinlechner
- Albert-Einstein-Institut, Max-Planck-Institut für Gravitationsphysik, D-30167 Hannover, Germany and SUPA, University of Glasgow, Glasgow G12 8QQ, United Kingdom
| | - S Steinlechner
- Albert-Einstein-Institut, Max-Planck-Institut für Gravitationsphysik, D-30167 Hannover, Germany and SUPA, University of Glasgow, Glasgow G12 8QQ, United Kingdom
| | - B C Stephens
- University of Wisconsin-Milwaukee, Milwaukee, Wisconsin 53201, USA
| | - S Steplewski
- Washington State University, Pullman, Washington 99164, USA
| | - S Stevenson
- University of Birmingham, Birmingham B15 2TT, United Kingdom
| | - R Stone
- The University of Texas at Brownsville, Brownsville, Texas 78520, USA
| | - D Stops
- University of Birmingham, Birmingham B15 2TT, United Kingdom
| | - K A Strain
- SUPA, University of Glasgow, Glasgow G12 8QQ, United Kingdom
| | - N Straniero
- Laboratoire des Matériaux Avancés (LMA), IN2P3/CNRS, Université de Lyon, F-69622 Villeurbanne, Lyon, France
| | - S Strigin
- Faculty of Physics, Lomonosov Moscow State University, Moscow 119991, Russia
| | - R Sturani
- Instituto de Física Teórica, Universidade Estadual Paulista/ICTP South American Institute for Fundamental Research, São Paulo, São Paulo 01140-070, Brazil
| | - A L Stuver
- LIGO Livingston Observatory, Livingston, Louisiana 70754, USA
| | | | - S Susmithan
- University of Western Australia, Crawley, Western Australia 6009, Australia
| | - P J Sutton
- Cardiff University, Cardiff CF24 3AA, United Kingdom
| | - B Swinkels
- European Gravitational Observatory (EGO), I-56021 Cascina, Pisa, Italy
| | - M Tacca
- APC, AstroParticule et Cosmologie, Université Paris Diderot, CNRS/IN2P3, CEA/Irfu, Observatoire de Paris, Sorbonne Paris Cité, 10, rue Alice Domon et Léonie Duquet, F-75205 Paris Cedex 13, France
| | - D Talukder
- University of Oregon, Eugene, Oregon 97403, USA
| | - D B Tanner
- University of Florida, Gainesville, Florida 32611, USA
| | - J Tao
- Louisiana State University, Baton Rouge, Louisiana 70803, USA
| | - S P Tarabrin
- Albert-Einstein-Institut, Max-Planck-Institut für Gravitationsphysik, D-30167 Hannover, Germany
| | - R Taylor
- LIGO, California Institute of Technology, Pasadena, California 91125, USA
| | - G Tellez
- The University of Texas at Brownsville, Brownsville, Texas 78520, USA
| | | | - M Thomas
- LIGO Livingston Observatory, Livingston, Louisiana 70754, USA
| | - P Thomas
- LIGO Hanford Observatory, Richland, Washington 99352, USA
| | - K A Thorne
- LIGO Livingston Observatory, Livingston, Louisiana 70754, USA
| | - K S Thorne
- Caltech-CaRT, Pasadena, California 91125, USA
| | - E Thrane
- LIGO, California Institute of Technology, Pasadena, California 91125, USA
| | - V Tiwari
- University of Florida, Gainesville, Florida 32611, USA
| | - K V Tokmakov
- SUPA, University of Strathclyde, Glasgow G1 1XQ, United Kingdom
| | - C Tomlinson
- The University of Sheffield, Sheffield S10 2TN, United Kingdom
| | - M Tonelli
- INFN, Sezione di Pisa, I-56127 Pisa, Italy and Università di Pisa, I-56127 Pisa, Italy
| | - C V Torres
- The University of Texas at Brownsville, Brownsville, Texas 78520, USA
| | - C I Torrie
- LIGO, California Institute of Technology, Pasadena, California 91125, USA and SUPA, University of Glasgow, Glasgow G12 8QQ, United Kingdom
| | - F Travasso
- INFN, Sezione di Perugia, I-06123 Perugia, Italy and Università di Perugia, I-06123 Perugia, Italy
| | - G Traylor
- LIGO Livingston Observatory, Livingston, Louisiana 70754, USA
| | - M Tse
- Columbia University, New York, New York 10027, USA
| | - D Tshilumba
- University of Brussels, Brussels 1050, Belgium
| | - H Tuennermann
- Albert-Einstein-Institut, Max-Planck-Institut für Gravitationsphysik, D-30167 Hannover, Germany
| | - D Ugolini
- Trinity University, San Antonio, Texas 78212, USA
| | | | - A L Urban
- University of Wisconsin-Milwaukee, Milwaukee, Wisconsin 53201, USA
| | - S A Usman
- Syracuse University, Syracuse, New York 13244, USA
| | - H Vahlbruch
- Leibniz Universität Hannover, D-30167 Hannover, Germany
| | - G Vajente
- INFN, Sezione di Pisa, I-56127 Pisa, Italy and Università di Pisa, I-56127 Pisa, Italy
| | - G Valdes
- The University of Texas at Brownsville, Brownsville, Texas 78520, USA
| | | | - M van Beuzekom
- Nikhef, Science Park, 1098 XG Amsterdam, The Netherlands
| | - J F J van den Brand
- Nikhef, Science Park, 1098 XG Amsterdam, The Netherlands and VU University Amsterdam, 1081 HV Amsterdam, The Netherlands
| | | | - M V van der Sluys
- Nikhef, Science Park, 1098 XG Amsterdam, The Netherlands and Department of Astrophysics/IMAPP, Radboud University Nijmegen, P.O. Box 9010, 6500 GL Nijmegen, The Netherlands
| | | | - A A van Veggel
- SUPA, University of Glasgow, Glasgow G12 8QQ, United Kingdom
| | - S Vass
- LIGO, California Institute of Technology, Pasadena, California 91125, USA
| | - M Vasúth
- Wigner RCP, RMKI, H-1121 Budapest, Konkoly Thege Miklós út 29-33, Hungary
| | - R Vaulin
- LIGO, Massachusetts Institute of Technology, Cambridge, Massachusetts 02139, USA
| | - A Vecchio
- University of Birmingham, Birmingham B15 2TT, United Kingdom
| | - G Vedovato
- INFN, Sezione di Padova, I-35131 Padova, Italy
| | - J Veitch
- Nikhef, Science Park, 1098 XG Amsterdam, The Netherlands
| | - P J Veitch
- University of Adelaide, Adelaide, South Australia 5005, Australia
| | - K Venkateswara
- University of Washington, Seattle, Washington 98195, USA
| | - D Verkindt
- Laboratoire d'Annecy-le-Vieux de Physique des Particules (LAPP), Université de Savoie, CNRS/IN2P3, F-74941 Annecy-le-Vieux, France
| | - F Vetrano
- Università degli Studi di Urbino 'Carlo Bo', I-61029 Urbino, Italy and INFN, Sezione di Firenze, I-50019 Sesto Fiorentino, Firenze, Italy
| | - A Viceré
- Università degli Studi di Urbino 'Carlo Bo', I-61029 Urbino, Italy and INFN, Sezione di Firenze, I-50019 Sesto Fiorentino, Firenze, Italy
| | - R Vincent-Finley
- Southern University and A&M College, Baton Rouge, Louisiana 70813, USA
| | - J-Y Vinet
- Université Nice-Sophia-Antipolis, CNRS, Observatoire de la Côte d'Azur, F-06304 Nice, France
| | - S Vitale
- LIGO, Massachusetts Institute of Technology, Cambridge, Massachusetts 02139, USA
| | - T Vo
- LIGO Hanford Observatory, Richland, Washington 99352, USA
| | - H Vocca
- INFN, Sezione di Perugia, I-06123 Perugia, Italy and Università di Perugia, I-06123 Perugia, Italy
| | - C Vorvick
- LIGO Hanford Observatory, Richland, Washington 99352, USA
| | - W D Vousden
- University of Birmingham, Birmingham B15 2TT, United Kingdom
| | - S P Vyachanin
- Faculty of Physics, Lomonosov Moscow State University, Moscow 119991, Russia
| | - A R Wade
- Australian National University, Canberra, ACT 0200, Australia
| | - L Wade
- University of Wisconsin-Milwaukee, Milwaukee, Wisconsin 53201, USA
| | - M Wade
- University of Wisconsin-Milwaukee, Milwaukee, Wisconsin 53201, USA
| | - M Walker
- Louisiana State University, Baton Rouge, Louisiana 70803, USA
| | - L Wallace
- LIGO, California Institute of Technology, Pasadena, California 91125, USA
| | - S Walsh
- University of Wisconsin-Milwaukee, Milwaukee, Wisconsin 53201, USA
| | - M Wang
- University of Birmingham, Birmingham B15 2TT, United Kingdom
| | - X Wang
- Tsinghua University, Beijing 100084, China
| | - R L Ward
- Australian National University, Canberra, ACT 0200, Australia
| | - M Was
- Albert-Einstein-Institut, Max-Planck-Institut für Gravitationsphysik, D-30167 Hannover, Germany
| | - B Weaver
- LIGO Hanford Observatory, Richland, Washington 99352, USA
| | - L-W Wei
- Université Nice-Sophia-Antipolis, CNRS, Observatoire de la Côte d'Azur, F-06304 Nice, France
| | - M Weinert
- Albert-Einstein-Institut, Max-Planck-Institut für Gravitationsphysik, D-30167 Hannover, Germany
| | - A J Weinstein
- LIGO, California Institute of Technology, Pasadena, California 91125, USA
| | - R Weiss
- LIGO, Massachusetts Institute of Technology, Cambridge, Massachusetts 02139, USA
| | - T Welborn
- LIGO Livingston Observatory, Livingston, Louisiana 70754, USA
| | - L Wen
- University of Western Australia, Crawley, Western Australia 6009, Australia
| | - P Wessels
- Albert-Einstein-Institut, Max-Planck-Institut für Gravitationsphysik, D-30167 Hannover, Germany
| | - M West
- Syracuse University, Syracuse, New York 13244, USA
| | - T Westphal
- Albert-Einstein-Institut, Max-Planck-Institut für Gravitationsphysik, D-30167 Hannover, Germany
| | - K Wette
- Albert-Einstein-Institut, Max-Planck-Institut für Gravitationsphysik, D-30167 Hannover, Germany
| | - J T Whelan
- Rochester Institute of Technology, Rochester, New York 14623, USA
| | - D J White
- The University of Sheffield, Sheffield S10 2TN, United Kingdom
| | - B F Whiting
- University of Florida, Gainesville, Florida 32611, USA
| | - K Wiesner
- Albert-Einstein-Institut, Max-Planck-Institut für Gravitationsphysik, D-30167 Hannover, Germany
| | - C Wilkinson
- LIGO Hanford Observatory, Richland, Washington 99352, USA
| | - K Williams
- Southern University and A&M College, Baton Rouge, Louisiana 70813, USA
| | - L Williams
- University of Florida, Gainesville, Florida 32611, USA
| | - R Williams
- LIGO, California Institute of Technology, Pasadena, California 91125, USA
| | - T D Williams
- Southeastern Louisiana University, Hammond, Louisiana 70402, USA
| | | | - J L Willis
- Abilene Christian University, Abilene, Texas 79699, USA
| | - B Willke
- Albert-Einstein-Institut, Max-Planck-Institut für Gravitationsphysik, D-30167 Hannover, Germany and Leibniz Universität Hannover, D-30167 Hannover, Germany
| | - M Wimmer
- Albert-Einstein-Institut, Max-Planck-Institut für Gravitationsphysik, D-30167 Hannover, Germany
| | - W Winkler
- Albert-Einstein-Institut, Max-Planck-Institut für Gravitationsphysik, D-30167 Hannover, Germany
| | - C C Wipf
- LIGO, Massachusetts Institute of Technology, Cambridge, Massachusetts 02139, USA
| | - A G Wiseman
- University of Wisconsin-Milwaukee, Milwaukee, Wisconsin 53201, USA
| | - H Wittel
- Albert-Einstein-Institut, Max-Planck-Institut für Gravitationsphysik, D-30167 Hannover, Germany
| | - G Woan
- SUPA, University of Glasgow, Glasgow G12 8QQ, United Kingdom
| | - N Wolovick
- Argentinian Gravitational Wave Group, Cordoba Cordoba 5000, Argentina
| | - J Worden
- LIGO Hanford Observatory, Richland, Washington 99352, USA
| | - Y Wu
- University of Florida, Gainesville, Florida 32611, USA
| | - J Yablon
- Northwestern University, Evanston, Illinois 60208, USA
| | - I Yakushin
- LIGO Livingston Observatory, Livingston, Louisiana 70754, USA
| | - W Yam
- LIGO, Massachusetts Institute of Technology, Cambridge, Massachusetts 02139, USA
| | - H Yamamoto
- LIGO, California Institute of Technology, Pasadena, California 91125, USA
| | - C C Yancey
- University of Maryland, College Park, Maryland 20742, USA
| | - H Yang
- Caltech-CaRT, Pasadena, California 91125, USA
| | - S Yoshida
- Southeastern Louisiana University, Hammond, Louisiana 70402, USA
| | - M Yvert
- Laboratoire d'Annecy-le-Vieux de Physique des Particules (LAPP), Université de Savoie, CNRS/IN2P3, F-74941 Annecy-le-Vieux, France
| | | | - M Zanolin
- Embry-Riddle Aeronautical University, Prescott, Arizona 86301, USA
| | - J-P Zendri
- INFN, Sezione di Padova, I-35131 Padova, Italy
| | - Fan Zhang
- LIGO, Massachusetts Institute of Technology, Cambridge, Massachusetts 02139, USA and Tsinghua University, Beijing 100084, China
| | - L Zhang
- LIGO, California Institute of Technology, Pasadena, California 91125, USA
| | - C Zhao
- University of Western Australia, Crawley, Western Australia 6009, Australia
| | - H Zhu
- The Pennsylvania State University, University Park, Pennsylvania 16802, USA
| | - X J Zhu
- University of Western Australia, Crawley, Western Australia 6009, Australia
| | - M E Zucker
- LIGO, Massachusetts Institute of Technology, Cambridge, Massachusetts 02139, USA
| | - S Zuraw
- University of Massachusetts Amherst, Amherst, Massachusetts 01003, USA
| | - J Zweizig
- LIGO, California Institute of Technology, Pasadena, California 91125, USA
| | - R L Aptekar
- Ioffe Physical-Technical Institute, Saint Petersburg, 194021, Russian Federation
| | - J L Atteia
- Université de Toulouse, UPS-OMP, IRAP, Toulouse, France and CNRS, IRAP, 14, Avenue Edouard Belin, F-31400 Toulouse, France
| | - T Cline
- NASA/Goddard Space Flight Center, Greenbelt, Maryland 20771, USA
| | - V Connaughton
- CSPAR, University of Alabama in Huntsville, Huntsville, Alabama 35899, USA
| | - D D Frederiks
- Ioffe Physical-Technical Institute, Saint Petersburg, 194021, Russian Federation
| | - S V Golenetskii
- Ioffe Physical-Technical Institute, Saint Petersburg, 194021, Russian Federation
| | - K Hurley
- University of California-Berkeley, Space Sciences Lab, 7 Gauss Way, Berkeley, California 94720, USA
| | - H A Krimm
- Center for Research and Exploration in Space Science and Technology (CRESST) and NASA Goddard Space Flight Center, Greenbelt, Maryland 20771, USA and Universities Space Research Association, 7178 Columbia Gateway Drive Columbia, Maryland 21046, USA
| | - M Marisaldi
- INAF-IASF Bologna, Via Piero Gobetti 101, 40129 Bologna, Italy
| | - V D Pal'shin
- Ioffe Physical-Technical Institute, Saint Petersburg, 194021, Russian Federation and Saint Petersburg State Polytechnical University, 195251, Saint Petersburg, Russia
| | - D Palmer
- Los Alamos National Laboratory, Los Alamos, New Mexico 87545, USA
| | - D S Svinkin
- Ioffe Physical-Technical Institute, Saint Petersburg, 194021, Russian Federation
| | - Y Terada
- Graduate School of Science and Engineering, Saitama University, Saitama City, Japan
| | - A von Kienlin
- Max-Planck-Institut für extraterrestrische Physik, Giessenbachstrasse 1, 85748 Garching, Germany
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Tanigawa S, Lee CH, Lin CS, Ku CC, Hasegawa H, Qin S, Kawahara A, Korenori Y, Miyamori K, Noguchi M, Lee LH, Lin YC, Lin CLS, Nakamura Y, Jin C, Yamaguchi N, Eckner R, Hou DX, Yokoyama KK. Erratum: Jun dimerization protein 2 is a critical component of the Nrf2/MafK complex regulating the response to ROS homeostasis. Cell Death Dis 2014. [PMCID: PMC4123110 DOI: 10.1038/cddis.2014.322] [Citation(s) in RCA: 0] [Impact Index Per Article: 0] [Reference Citation Analysis] [What about the content of this article? (0)] [Track Full Text] [Download PDF] [Figures] [Journal Information] [Subscribe] [Scholar Register] [Indexed: 11/09/2022]
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115
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Hwang JK, Erkhembaatar M, Gu DR, Lee SH, Lee CH, Shin DM, Lee YR, Kim MS. Glechoma hederacea Suppresses RANKL-mediated Osteoclastogenesis. J Dent Res 2014; 93:685-90. [PMID: 24850617 DOI: 10.1177/0022034514536579] [Citation(s) in RCA: 15] [Impact Index Per Article: 1.5] [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: 02/04/2014] [Accepted: 04/23/2014] [Indexed: 11/17/2022] Open
Abstract
Glechoma hederacea (GH), commonly known as ground-ivy or gill-over-the-ground, has been extensively used in folk remedies for relieving symptoms of inflammatory disorders. However, the molecular mechanisms underlying the therapeutic action of GH are poorly understood. Here, we demonstrate that GH constituents inhibit osteoclastogenesis by abrogating receptor activator of nuclear κ-B ligand (RANKL)-induced free cytosolic Ca(2+) ([Ca(2+)]i) oscillations. To evaluate the effect of GH on osteoclastogenesis, we assessed the formation of multi-nucleated cells (MNCs), enzymatic activity of tartrate-resistant acidic phosphatase (TRAP), expression of nuclear factor of activated T-cells cytoplasmic 1 (NFATc1), and [Ca(2+)]i alterations in response to treatment with GH ethanol extract (GHE) in primarily cultured bone marrow-derived macrophages (BMMs). Treatment of RANKL-stimulated or non-stimulated BMMs with GHE markedly suppressed MNC formation, TRAP activity, and NFATc1 expression in a dose-dependent manner. Additionally, GHE treatment induced a large transient elevation in [Ca(2+)]i while suppressing RANKL-induced [Ca(2+)]i oscillations, which are essential for NFATc1 activation. GHE-evoked increase in [Ca(2+)]i was dependent on extracellular Ca(2+) and was inhibited by 1,4-dihydropyridine (DHP), inhibitor of voltage-gated Ca(2+) channels (VGCCs), but was independent of store-operated Ca(2+) channels. Notably, after transient [Ca(2+)] elevation, treatment with GHE desensitized the VGCCs, resulting in an abrogation of RANKL-induced [Ca(2+)]i oscillations and MNC formation. These findings demonstrate that treatment of BMMs with GHE suppresses RANKL-mediated osteoclastogenesis by activating and then desensitizing DHP-sensitive VGCCs, suggesting potential applications of GH in the treatment of bone disorders, such as periodontitis, osteoporosis, and rheumatoid arthritis.
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Affiliation(s)
- J K Hwang
- Center for Metabolic Function Regulation (CMFR), Wonkwang University School of Medicine, Iksan 570-749, Republic of Korea Department of Oral Biochemistry, College of Dentistry, Wonkwang University, 344-2 Shinyong-dong, Iksan 570-749, Republic of Korea
| | - M Erkhembaatar
- Department of Oral Physiology, College of Dentistry, Wonkwang University, Iksan 570-749, Republic of Korea
| | - D R Gu
- Center for Metabolic Function Regulation (CMFR), Wonkwang University School of Medicine, Iksan 570-749, Republic of Korea Department of Oral Microbiology and Immunology, College of Dentistry, Wonkwang University, Iksan 570-749, Republic of Korea
| | - S H Lee
- Center for Metabolic Function Regulation (CMFR), Wonkwang University School of Medicine, Iksan 570-749, Republic of Korea Department of Oral Microbiology and Immunology, College of Dentistry, Wonkwang University, Iksan 570-749, Republic of Korea
| | - C H Lee
- Microelectronics and Display, Next Generation Industrial Radiation Technology RIC, Wonkwang University, Iksan 570-749, Republic of Korea
| | - D M Shin
- Department of Oral Biology, BK21 PLUS Project, Yonsei University College of Dentistry, Seoul 120-752
| | - Y R Lee
- Center for Metabolic Function Regulation (CMFR), Wonkwang University School of Medicine, Iksan 570-749, Republic of Korea Department of Oral Biochemistry, College of Dentistry, Wonkwang University, 344-2 Shinyong-dong, Iksan 570-749, Republic of Korea
| | - M S Kim
- Department of Oral Physiology, College of Dentistry, Wonkwang University, Iksan 570-749, Republic of Korea Microelectronics and Display, Next Generation Industrial Radiation Technology RIC, Wonkwang University, Iksan 570-749, Republic of Korea
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116
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Kosik RO, Tran DT, Fan APC, Mandell GA, Tarng DC, Hsu HS, Chen YS, Su TP, Wang SJ, Chiu AW, Lee CH, Hou MC, Lee FY, Chen WS, Chen Q. Physician Scientist Training in the United States: A Survey of the Current Literature. Eval Health Prof 2014; 39:3-20. [PMID: 24686746 DOI: 10.1177/0163278714527290] [Citation(s) in RCA: 43] [Impact Index Per Article: 4.3] [Reference Citation Analysis] [What about the content of this article? (0)] [Affiliation(s)] [Abstract] [Key Words] [Track Full Text] [Journal Information] [Subscribe] [Scholar Register] [Indexed: 11/16/2022]
Abstract
The declining number of physician scientists is an alarming issue. A systematic review of all existing programs described in the literature was performed, so as to highlight which programs may serve as the best models for the training of successful physician scientists. Multiple databases were searched, and 1,294 articles related to physician scientist training were identified. Preference was given to studies that looked at number of confirmed publications and/or research grants as primary outcomes. Thirteen programs were identified in nine studies. Eighty-three percent of Medical Scientist Training Program (MSTP) graduates, 77% of Clinician Investigator Training Program (CI) graduates, and only 16% of Medical Fellows Program graduates entered a career in academics. Seventy-eight percent of MSTP graduates succeeded in obtaining National Institute of Health (NIH) grants, while only 15% of Mayo Clinic National Research Service Award-T32 graduates obtained NIH grants. MSTP physician scientists who graduated in 1990 had 13.5 ± 12.5 publications, while MSTP physician scientists who graduated in 1975 had 51.2 ± 38.3 publications. Additionally, graduates from the Mayo Clinic's MD-PhD Program, the CI Program, and the NSRA Program had 18.2 ± 20.1, 26.5 ± 24.5, and 17.9 ± 26.3 publications, respectively. MSTP is a successful model for the training of physician scientists in the United States, but training at the postgraduate level also shows promising outcomes. An increase in the number of positions available for training at the postgraduate level should be considered.
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Affiliation(s)
- R O Kosik
- Santa Clara Valley Medical Center, San Jose, CA, USA
| | - D T Tran
- Department of Nephrology and Endocrinology, Children's Hospital 2, HoChiMinh City, Vietnam
| | | | - G A Mandell
- Santa Clara Valley Medical Center, San Jose, CA, USA
| | - D C Tarng
- School of Medicine, National Yang-Ming University, Taipei, Taiwan
| | - H S Hsu
- School of Medicine, National Yang-Ming University, Taipei, Taiwan
| | - Y S Chen
- School of Medicine, National Yang-Ming University, Taipei, Taiwan
| | - T P Su
- School of Medicine, National Yang-Ming University, Taipei, Taiwan
| | - S J Wang
- School of Medicine, National Yang-Ming University, Taipei, Taiwan
| | - A W Chiu
- School of Medicine, National Yang-Ming University, Taipei, Taiwan
| | - C H Lee
- School of Medicine, National Yang-Ming University, Taipei, Taiwan
| | - M C Hou
- School of Medicine, National Yang-Ming University, Taipei, Taiwan
| | - F Y Lee
- School of Medicine, National Yang-Ming University, Taipei, Taiwan
| | - W S Chen
- Santa Clara Valley Medical Center, San Jose, CA, USA
| | - Q Chen
- School of Medicine, Nanjin Medical University, Nanjin, China
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117
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Lee CH, Belanger JE, Kassam Z, Smieja M, Higgins D, Broukhanski G, Kim PT. The outcome and long-term follow-up of 94 patients with recurrent and refractory Clostridium difficile infection using single to multiple fecal microbiota transplantation via retention enema. Eur J Clin Microbiol Infect Dis 2014; 33:1425-8. [PMID: 24627239 DOI: 10.1007/s10096-014-2088-9] [Citation(s) in RCA: 83] [Impact Index Per Article: 8.3] [Reference Citation Analysis] [What about the content of this article? (0)] [Affiliation(s)] [Abstract] [Track Full Text] [Journal Information] [Subscribe] [Scholar Register] [Received: 01/21/2014] [Accepted: 03/02/2014] [Indexed: 12/12/2022]
Abstract
Clostridium difficile infection (CDI) is one of the most frequent causes of healthcare-associated infections, and its rates are also increasing in the community. The management of CDI has become a major challenge, given growing rates of recurrences and failures with standard antibiotic therapy. Mounting evidence suggests that fecal microbiota transplantation (FMT) may be effective; however, as there is a paucity of data with regard to repeat FMT for primary non-response to this treatment, this study examined the outcome of multiple FMTs for recurrent CDI. Case records were reviewed for 94 patients who underwent FMT via retention enema for recurrent or refractory CDI during the period 2008-2012. Demographic information, treatment data, and clinical resolution rates were examined for single FMT and cumulative resolution was assessed for multiple FMTs in the context of ongoing symptoms. The cumulative clinical resolution following four or more FMTs was 86%. When antibiotic therapy was used between FMTs, the clinical resolution rate increased to 92%. There were no reported adverse events and no patients who were cured with FMT had further episodes of CDI at 6-24 months follow-up. Multiple FMTs administered through enemas is an effective, safe, and simple therapy for the management of recurrent or refractory CDI.
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Affiliation(s)
- C H Lee
- Department of Pathology and Molecular Medicine, McMaster University, St Joseph's Healthcare, 50 Charlton Avenue East, 424 Luke Wing, Hamilton, ON, L8N 4A6, Canada,
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118
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Kim WC, Ma C, Li WM, Chohan M, Wilson III DM, Lee CH. Altered endoribonuclease activity of apurinic/apyrimidinic endonuclease 1 variants identified in the human population. PLoS One 2014; 9:e90837. [PMID: 24595156 PMCID: PMC3942487 DOI: 10.1371/journal.pone.0090837] [Citation(s) in RCA: 6] [Impact Index Per Article: 0.6] [Reference Citation Analysis] [What about the content of this article? (0)] [Affiliation(s)] [Abstract] [MESH Headings] [Grants] [Track Full Text] [Download PDF] [Figures] [Journal Information] [Subscribe] [Scholar Register] [Received: 11/21/2013] [Accepted: 02/05/2014] [Indexed: 11/30/2022] Open
Abstract
Apurinic/apyrimidinic endonuclease 1 (APE1) is the major mammalian enzyme in the DNA base excision repair pathway and cleaves the DNA phosphodiester backbone immediately 5′ to abasic sites. APE1 also has 3′-5′ DNA exonuclease and 3′ DNA phosphodiesterase activities, and regulates transcription factor DNA binding through its redox regulatory function. The human APE1 has recently been shown to endonucleolytically cleave single-stranded regions of RNA. Towards understanding the biological significance of the endoribonuclease activity of APE1, we examined eight different amino acid substitution variants of APE1 previously identified in the human population. Our study shows that six APE1 variants, D148E, Q51H, I64V, G241R, R237A, and G306A, exhibit a 76–85% reduction in endoribonuclease activity against a specific coding region of the c-myc RNA, yet fully retain the ability to cleave apurinic/apyrimidinic DNA. We found that two APE1 variants, L104R and E126D, exhibit a unique RNase inhibitor-resistant endoribonuclease activity, where the proteins cleave c-myc RNA 3′ of specific single-stranded guanosine residues. Expression of L104R and E126D APE1 variants in bacterial Origami cells leads to a 60–80% reduction in colony formation and a 1.5-fold increase in cell doubling time, whereas the other variants, which exhibit diminished endoribonuclease activity, had no effect. These data indicate that two human APE1 variants exhibit a unique endoribonuclease activity, which correlates with their ability to induce cytotoxicity or slow down growth in bacterial cells and supports the notion of their biological functionality.
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Affiliation(s)
- Wan Cheol Kim
- Chemistry Program, University of Northern British Columbia, Prince George, British Columbia, Canada
| | - Conan Ma
- Chemistry Program, University of Northern British Columbia, Prince George, British Columbia, Canada
| | - Wai-Ming Li
- Chemistry Program, University of Northern British Columbia, Prince George, British Columbia, Canada
| | - Manbir Chohan
- Chemistry Program, University of Northern British Columbia, Prince George, British Columbia, Canada
| | - David M. Wilson III
- Laboratory of Molecular Gerontology, National Institute on Aging, National Institutes of Health, Baltimore, Maryland, United States of America
| | - Chow H. Lee
- Chemistry Program, University of Northern British Columbia, Prince George, British Columbia, Canada
- * E-mail:
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119
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Abstract
The ability to repair damaged DNA and to maintain genome stability is the utmost importance for the survival of any species. Hence, it is not surprising to find that DNA repair mechanisms are evolutionarily conserved and are expected to evolve to maintain the existence of species. In the last few years, there has been an exponential increase in the evidence linking RNA processing with DNA repair programs. For instance, the well-studied DNA base excision repair (BER) enzyme apurinic/apyrimidinic endonuclease 1 can cleave RNA molecules, regulate mRNA levels, and associate physically with proteins involved in RNA processing. It is now clear that not only the expression of noncoding RNAs are changed upon DNA damage, they can modulate the expression of genes involved in the genome stability programs. The five reviews in this Forum provide the up-to-date knowledge on DNA repair, with a focus on BER, and a perspective on how the two ancient biochemical pathways are linked. The contributions demonstrate the complexity of such interactions, but also pointed out the opportunities for new therapeutic interventions. Future in vivo studies on the link between DNA repair processes and RNA metabolism should contribute to our basic understanding of physiology, disease, and treatment strategies.
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Affiliation(s)
- Chow H Lee
- Chemistry Program, University of Northern British Columbia , Prince George, Canada
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120
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Oyungerel B, Lim H, Lee CH, Choi EH, Li GH, Choi KD. Anti-inflammatory Effects of Magnolia sieboldii Extract in Lipopolysaccharide-Stimulated RAW264.7 Macrophages. TROP J PHARM RES 2014. [DOI: 10.4314/tjpr.v12i6.8] [Citation(s) in RCA: 9] [Impact Index Per Article: 0.9] [Reference Citation Analysis] [What about the content of this article? (0)] [Track Full Text] [Journal Information] [Subscribe] [Scholar Register] [Indexed: 11/17/2022] Open
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121
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Hyun MH, Lee CH, Kim HJ, Tong Y, Park SS. Systematic review and meta-analysis of robotic surgery compared with conventional laparoscopic and open resections for gastric carcinoma. Br J Surg 2014; 100:1566-78. [PMID: 24264778 DOI: 10.1002/bjs.9242] [Citation(s) in RCA: 74] [Impact Index Per Article: 7.4] [Reference Citation Analysis] [What about the content of this article? (0)] [Affiliation(s)] [Abstract] [Track Full Text] [Journal Information] [Subscribe] [Scholar Register] [Accepted: 06/26/2013] [Indexed: 02/06/2023]
Abstract
BACKGROUND Robot-assisted gastrectomy (RAG) has been developed in the hope of improving surgical quality and overcoming the limitations of conventional laparoscopically assisted gastrectomy (LAG) and open gastrectomy (OG) for gastric cancer. The aim of this study was to determine the extent of evidence in support of these ideals. METHODS A systematic review of the three operation types (RAG, LAG and OG) was carried out to evaluate short-term outcomes including duration of operation, retrieved lymph nodes, estimated blood loss, resection margin status, technical postoperative complications and hospital stay. RESULTS Nine non-randomized observational clinical studies involving 7200 patients satisfied the eligibility criteria. RAG was associated with longer operating times than LAG and OG (weighted mean difference 61.99 and 65.73 min respectively; P ≤ 0.001). The number of retrieved lymph nodes and the resection margin length in RAG were comparable with those of LAG and OG. Estimated blood loss as significantly less in RAG than in OG (P = 0.002), but not LAG. Mean hospital stay for RAG was similar to that for LAG (P = 0.14). In contrast, hospital stay was significantly shorter, by a mean of 2.18 days, for RAG compared with OG (P < 0.001). Postoperative complications were similar for all three operative approaches. CONCLUSION Short-term oncological outcomes of RAG were comparable with those of the other approaches. LAG was a shorter procedure and less expensive than RAG. Future studies involving RAG should focus on minimizing duration of operation and reducing cost.
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Affiliation(s)
- M H Hyun
- Division of Upper Gastrointestinal Surgery, Department of Surgery, and
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122
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Park JS, Oh IH, Lee CH, Kim GH, Kang CM. The rate of decline of glomerular filtration rate is a predictor of long-term graft outcome after kidney transplantation. Transplant Proc 2013; 45:1438-41. [PMID: 23726591 DOI: 10.1016/j.transproceed.2012.10.052] [Citation(s) in RCA: 7] [Impact Index Per Article: 0.6] [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: 10/05/2012] [Accepted: 10/30/2012] [Indexed: 02/07/2023]
Abstract
BACKGROUND To improve the long-term outcome of kidney transplantation (KT), it is important to identify and take active steps to reduce the number or severity of novel risk factors. We investigated whether changes in estimated glomerular filtration rate over the first year after KT (ΔeGFR12-3) was associated with long-term renal allograft function and survival. METHODS Four hundred twenty-eight allograft recipients transplanted between 1990 and 2001 underwent ΔeGFR12-3 calculation using the equation: ΔeGFR12-3 = ([eGFR at 12 months post-KT - eGFR at 3 months post-KT]/[eGFR at 3 months post-KT]) × 100%. Recipients were divided into 3 groups according to their ΔeGFR12-3: group I (n = 150), ΔeGFR12-3 ≥ 10%; group II (n = 151), 10 > ΔeGFR12-3 ≥ -10%; and group III (n = 127), ΔeGFR12-3 < -10%. Multiple linear regression analysis was used to adjust for confounding variables that may affect long-term renal allograft function, and Kaplan-Meier analysis, to compare allograft survival. RESULTS At a mean follow-up of 120 ± 58 months, we observed 112 renal allograft losses. The ΔeGFR over 10 years post-KT (ΔeGFR120-3) was significantly associated with the serum uric acid levels at 3 months post-transplantation and ΔeGFR12-3. Group III showed poor renal allograft survival; group I, 194 ± 8 months; group II, 197 ± 7 month and; group III, 163 ± 4 months; (log-rank test, P < .05). A Cox proportional hazard model revealed ΔeGFR12-3 to be independently associated with future renal allograft loss (hazard ratio, 0.981; 95% confidence interval, 0.974-0.992). CONCLUSION Our results suggested that ΔeGFR12-3 may be an independent predictor of kidney allograft survival. Routine application of eGFR is strongly recommended to identify patients at risk for chronic allograft dysfunction.
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Affiliation(s)
- J-S Park
- Department of Internal Medicine, Hanyang University College of Medicine, Seoul, South Korea
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123
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Lee CH, Steffens P, Qureshi N, Nakajima M, Kihou K, Iyo A, Eisaki H, Braden M. Universality of the dispersive spin-resonance mode in superconducting BaFe2As2. Phys Rev Lett 2013; 111:167002. [PMID: 24182293 DOI: 10.1103/physrevlett.111.167002] [Citation(s) in RCA: 3] [Impact Index Per Article: 0.3] [Reference Citation Analysis] [What about the content of this article? (0)] [Affiliation(s)] [Abstract] [Track Full Text] [Subscribe] [Scholar Register] [Received: 06/19/2013] [Revised: 09/09/2013] [Indexed: 06/02/2023]
Abstract
Spin fluctuations in superconducting BaFe2(As(1-x)P(x))2 (x=0.34, T(c)=29.5 K) are studied using inelastic neutron scattering. Well-defined commensurate magnetic signals are observed at (π, 0), which is consistent with the nesting vector of the Fermi surface. Antiferromagnetic (AFM) spin fluctuations in the normal state exhibit a three-dimensional character reminiscent of the AFM order in nondoped BaFe2As2. A clear spin gap is observed in the superconducting phase forming a peak whose energy is significantly dispersed along the c axis. The bandwidth of dispersion becomes larger with approaching the AFM ordered phase universally in all superconducting BaFe2As2, indicating that the dispersive feature is attributed to three-dimensional AFM correlations. The results suggest a strong relationship between the magnetism and superconductivity.
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Affiliation(s)
- C H Lee
- National Institute of Advanced Industrial Science and Technology (AIST), Tsukuba, Ibaraki 305-8568, Japan and Transformative Research-Project on Iron Pnictides (TRIP), JST, Chiyoda, Tokyo 102-0075, Japan
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124
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Abstract
We retrospectively studied the radiological and clinical results of a simple hemiresection arthroplasty, a modification of previous oblique distal ulnar resections, in 62 patients with rheumatoid arthritis (68 wrists) over a mean follow-up of 103 (range 60-173) months. Fourteen wrists (20%) became fused at the radiocarpal joint and 28 wrists fused (41%) at the midcarpal joints during follow-up. Severe ulnar translocation of the carpus was observed in two wrists (3%), radio-ulnar convergence in five wrists (7%), as well as a significant decrease of carpal height ratio, without any radiological findings of stylocarpal impingement. Improvements in forearm pronation and supination, and reduction in pain were maintained at the last follow-up. Grip strength was not significantly improved. The Jebsen-Taylor hand function test showed improvements in writing, card turning, and simulated feeding. Fifty-two patients (58 wrists, 85%) were satisfied with the results at the last follow-up. Simple hemiresection arthroplasty showed good long-term results with few complications.
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Affiliation(s)
- C H Lee
- Department of Orthopaedic Surgery, Hanil General Hospital, Seoul, Korea
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125
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Lee SM, Kim WH, Ahn HJ, Kim JA, Yang MK, Lee CH, Lee JH, Kim YR, Choi JW. The effects of prolonged inspiratory time during one-lung ventilation: a randomised controlled trial. Anaesthesia 2013; 68:908-16. [PMID: 23789714 DOI: 10.1111/anae.12318] [Citation(s) in RCA: 19] [Impact Index Per Article: 1.7] [Reference Citation Analysis] [What about the content of this article? (0)] [Affiliation(s)] [Abstract] [Track Full Text] [Journal Information] [Subscribe] [Scholar Register] [Accepted: 04/27/2013] [Indexed: 11/28/2022]
Abstract
We evaluated the effects of a prolonged inspiratory time on gas exchange in subjects undergoing one-lung ventilation for thoracic surgery. One hundred patients were randomly assigned to Group I:E = 1:2 or Group I:E = 1:1. Arterial blood gas analysis and respiratory mechanics measurements were performed 10 min after anaesthesia induction, 30 and 60 min after initiation of one-lung ventilation, and 15 min after restoration of conventional two-lung ventilation. The mean (SD) ratio of the partial pressure of arterial oxygen to fraction of inspired oxygen after 60 min of one-lung ventilation was significantly lower in Group I:E = 1:2 compared with Group I:E = 1:1 (27.7 (13.2) kPa vs 35.2 (22.1) kPa, respectively, p = 0.043). Mean (SD) physiological dead space-to-tidal volume ratio after 60 min of one-lung ventilation was significantly higher in Group I:E = 1:2 compared with Group I:E = 1:1 (0.46 (0.04) vs 0.43 (0.04), respectively, p = 0.008). Median (IQR [range]) peak inspiratory pressure was higher in Group I:E = 1:2 compared with Group I:E = 1:1 after 60 min of one-lung ventilation (23 (22-25 [18-29]) cmH2O vs 20 (18-21 [16-27]) cmH2O, respectively, p < 0.001) and median (IQR [range]) mean airway pressure was lower in Group I:E = 1:2 compared with Group I:E = 1:1 (10 (8-11 [5-15]) cmH2O vs 11 (10-13 [5-16]) cmH2O, respectively, p < 0.001). We conclude that, compared with an I:E ratio of 1:2, an I:E ratio of 1:1 resulted in a modest improvement in oxygenation and decreased shunt fraction during one-lung ventilation.
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Affiliation(s)
- S M Lee
- Department of Anaesthesia and Pain Medicine, Samsung Medical Center, Sungkyunkwan University School of Medicine, Seoul, Korea
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126
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Ishida S, Nakajima M, Liang T, Kihou K, Lee CH, Iyo A, Eisaki H, Kakeshita T, Tomioka Y, Ito T, Uchida S. Anisotropy of the in-plane resistivity of underdoped Ba(Fe(1-x)Co(x))2As2 superconductors induced by impurity scattering in the antiferromagnetic orthorhombic phase. Phys Rev Lett 2013; 110:207001. [PMID: 25167441 DOI: 10.1103/physrevlett.110.207001] [Citation(s) in RCA: 8] [Impact Index Per Article: 0.7] [Reference Citation Analysis] [What about the content of this article? (0)] [Affiliation(s)] [Abstract] [Track Full Text] [Subscribe] [Scholar Register] [Received: 10/17/2012] [Indexed: 06/03/2023]
Abstract
We investigated the in-plane resistivity anisotropy for underdoped Ba(Fe(1-x)Co(x))(2)As(2) single crystals with improved quality. We demonstrate that the anisotropy in resistivity in the magnetostructural ordered phase arises from the anisotropy in the residual component which increases in proportion to the Co concentration x. This gives evidence that the anisotropy originates from the impurity scattering by Co atoms substituted for the Fe sites, rather than the so far proposed mechanisms such as the anisotropy of Fermi velocities of reconstructed Fermi surface pockets. As doping proceeds to the paramagnetic-tetragonal phase, a Co impurity transforms to a weak and isotropic scattering center.
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Affiliation(s)
- S Ishida
- Department of Physics, University of Tokyo, Tokyo 113-0033, Japan and National Institute of Advanced Industrial Science and Technology, Tsukuba 305-8568, Japan and JST, Transformative Research-Project on Iron Pnictides, Tokyo 102-0075, Japan
| | - M Nakajima
- Department of Physics, University of Tokyo, Tokyo 113-0033, Japan and National Institute of Advanced Industrial Science and Technology, Tsukuba 305-8568, Japan and JST, Transformative Research-Project on Iron Pnictides, Tokyo 102-0075, Japan
| | - T Liang
- Department of Physics, University of Tokyo, Tokyo 113-0033, Japan and National Institute of Advanced Industrial Science and Technology, Tsukuba 305-8568, Japan and JST, Transformative Research-Project on Iron Pnictides, Tokyo 102-0075, Japan
| | - K Kihou
- National Institute of Advanced Industrial Science and Technology, Tsukuba 305-8568, Japan and JST, Transformative Research-Project on Iron Pnictides, Tokyo 102-0075, Japan
| | - C H Lee
- National Institute of Advanced Industrial Science and Technology, Tsukuba 305-8568, Japan and JST, Transformative Research-Project on Iron Pnictides, Tokyo 102-0075, Japan
| | - A Iyo
- National Institute of Advanced Industrial Science and Technology, Tsukuba 305-8568, Japan and JST, Transformative Research-Project on Iron Pnictides, Tokyo 102-0075, Japan
| | - H Eisaki
- National Institute of Advanced Industrial Science and Technology, Tsukuba 305-8568, Japan and JST, Transformative Research-Project on Iron Pnictides, Tokyo 102-0075, Japan
| | - T Kakeshita
- Department of Physics, University of Tokyo, Tokyo 113-0033, Japan and JST, Transformative Research-Project on Iron Pnictides, Tokyo 102-0075, Japan
| | - Y Tomioka
- National Institute of Advanced Industrial Science and Technology, Tsukuba 305-8568, Japan and JST, Transformative Research-Project on Iron Pnictides, Tokyo 102-0075, Japan
| | - T Ito
- National Institute of Advanced Industrial Science and Technology, Tsukuba 305-8568, Japan and JST, Transformative Research-Project on Iron Pnictides, Tokyo 102-0075, Japan
| | - S Uchida
- Department of Physics, University of Tokyo, Tokyo 113-0033, Japan and JST, Transformative Research-Project on Iron Pnictides, Tokyo 102-0075, Japan
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127
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Amorosa LF, Lee CH, Aydemir AB, Nizami S, Hsu A, Patel NR, Gardner TR, Navalgund A, Kim DG, Park SH, Mao JJ, Lee FY. Physiologic load-bearing characteristics of autografts, allografts, and polymer-based scaffolds in a critical sized segmental defect of long bone: an experimental study. Int J Nanomedicine 2013; 8:1637-43. [PMID: 23637532 PMCID: PMC3639117 DOI: 10.2147/ijn.s42855] [Citation(s) in RCA: 23] [Impact Index Per Article: 2.1] [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] [Indexed: 12/03/2022] Open
Abstract
Background To address the challenge of treating critical sized intercalary defects, we hypothesized that under physiologic cyclic loading, autografts, allografts, and scaffolds loaded with and without human mesenchymal stem cells (hMSCs) would have different biomechanical characteristics. Methods Using a rat femoral defect model, 46 rats were assigned to four groups, ie, autograft (n = 12), allograft (n = 10), scaffold (n = 13), and scaffold with hMSCs (n = 11). The scaffold groups used a 5 mm segment of scaffold composed of 80% poly-ε-caprolactone and 20% hydroxyapatite. Rats were sacrificed 4 months postoperatively, and the repairs were assessed radiographically and biomechanically. Results Autograft and allograft groups exhibited the most bridging callus, while the scaffold/hMSCs group had more callus than the scaffold repairs. Although signs of radiographic healing did not accurately reflect restoration of mechanical properties, addition of hMSCs on the scaffold enhanced bone formation. The scaffold alone group had significantly lower elastic and viscous stiffness and higher phase angles than other repairs and the contralateral controls. Addition of hMSCs increased the elastic and viscous stiffness of the repair, while decreasing the phase angle. Conclusion Further comparative analysis is needed to optimize clinical use of scaffolds and hMSCs for critical sized defect repairs. However, our results suggest that addition of hMSCs to scaffolds enhances mechanical simulation of native host bone.
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Affiliation(s)
- L F Amorosa
- Center for Orthopaedic Research, Columbia University Medical Center, New York, NY 10032, USA
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Lee HY, Seong MW, Park SS, Hwang SS, Lee J, Park YS, Lee CH, Lee SM, Yoo CG, Kim YW, Han SK, Yim JJ. Diagnostic accuracy of Xpert® MTB/RIF on bronchoscopy specimens in patients with suspected pulmonary tuberculosis. Int J Tuberc Lung Dis 2013; 17:917-21. [PMID: 23621953 DOI: 10.5588/ijtld.12.0885] [Citation(s) in RCA: 50] [Impact Index Per Article: 4.5] [Reference Citation Analysis] [What about the content of this article? (0)] [Affiliation(s)] [Abstract] [Track Full Text] [Journal Information] [Subscribe] [Scholar Register] [Indexed: 11/10/2022] Open
Abstract
OBJECTIVE To determine the diagnostic accuracy of the Xpert® MTB/RIF assay using samples obtained through bronchoscopy in patients with suspected pulmonary tuberculosis (PTB). DESIGN We retrospectively reviewed the records of patients with suspected PTB for whom the Xpert MTB/RIF assay was performed on bronchoscopy specimens. The sensitivity, specificity, positive predictive value (PPV) and negative predictive value (NPV) for the diagnosis of active PTB were calculated for acid-fast bacilli (AFB) smear microscopy and the Xpert assay using culture of Mycobacterium tuberculosis from sputum or bronchoscopy specimens as a reference standard. RESULTS A total of 132 patients were included in the final analysis. Of these, 38 had culture-confirmed PTB. The sensitivity of the Xpert assay using bronchial washing or bronchoalveolar lavage (BAL) fluid for the diagnosis of PTB was 81.6%, and specificity was 100%. The PPV and NPV were 100% and 92.1%, respectively. The sensitivity and specificity of AFB smear microscopy were respectively 13.2% and 98.8%. CONCLUSION The Xpert assay on bronchoscopy specimens provided an accurate diagnosis of PTB in patients who had a negative AFB smear or who could not produce sputum.
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Affiliation(s)
- H Y Lee
- Division of Pulmonary and Critical Care Medicine, Department of Internal Medicine and Lung Institute, Seoul National University College of Medicine, Seoul, Republic of Korea
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Chaou CH, Lin CC, Chen HY, Lee CH, Chen THH. Chlorpyrifos is associated with slower serum cholinesterase recovery in acute organophosphate-poisoned patients. Clin Toxicol (Phila) 2013; 51:402-8. [PMID: 23590812 DOI: 10.3109/15563650.2013.782035] [Citation(s) in RCA: 8] [Impact Index Per Article: 0.7] [Reference Citation Analysis] [What about the content of this article? (0)] [Affiliation(s)] [Abstract] [Track Full Text] [Journal Information] [Subscribe] [Scholar Register] [Indexed: 11/13/2022]
Abstract
PURPOSE Organophosphate poisoning (OPP) accounts for 200,000 deaths annually in developing countries. Serum cholinesterase (SChE) is of diagnostic value in patients with OPP and is checked repeatedly during the course of treatment. This study aimed to investigate the recovery pattern in patients with OPP using linear mixed models. METHODS Using a retrospective cohort study design, we included 212 adult OPP patients who had visited the emergency department (ED) in a tertiary medical center between 2000 and 2010. One hundred and thirty-one patients were available for analysis, as 81 patients did not meet the criteria and were excluded. Information regarding basic personal characteristics, initial vital signs and severity scores, laboratory data, type and amount of organophosphate ingested, treatment, and serial SChE values was collected. A random coefficient model with a random intercept and a random slope of time were added to address the dynamic relationships of SChE with time and other associated factors. RESULTS The initial SChE activity and recovery rates varied among patients with OPP. The type of organophosphate, the first SChE activity, and the initial APACHE II score were significantly related to the SChE recovery trend. Chlorpyrifos and methamidophos had significantly slower and faster SChE recovery rates, respectively, than other organophosphates. Sex, dose of Pralidoxim (2-PAM), and delay in obtaining medical assistance did not significantly affect SChE recovery. CONCLUSIONS This study demonstrated the pattern and associated correlates of SChE activity recovery in patients with acute OPP. Chlorpyrifos appeared to have a slower SChE activity recovery rate than other organophosphates.
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Affiliation(s)
- C H Chaou
- Department of Emergency Medicine, Chang Gung Memorial Hospital and Chang Gung University College of Medicine , Taoyuan , Taiwan
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130
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Steffens P, Lee CH, Qureshi N, Kihou K, Iyo A, Eisaki H, Braden M. Splitting of resonance excitations in nearly optimally doped Ba(Fe0.94Co0.06)2As2: an inelastic neutron scattering study with polarization analysis. Phys Rev Lett 2013; 110:137001. [PMID: 23581359 DOI: 10.1103/physrevlett.110.137001] [Citation(s) in RCA: 4] [Impact Index Per Article: 0.4] [Reference Citation Analysis] [What about the content of this article? (0)] [Affiliation(s)] [Abstract] [Track Full Text] [Subscribe] [Scholar Register] [Received: 10/24/2012] [Revised: 02/19/2013] [Indexed: 06/02/2023]
Abstract
Magnetic excitations in Ba(Fe0.94Co0.06)2As2: are studied by polarized inelastic neutron scattering above and below the superconducting transition. In the superconducting state, we find clear evidence for two resonancelike excitations. At a higher energy of about 8 meV, there is an isotropic resonance mode with weak dispersion along the c direction. In addition, we find a lower excitation at 4 meV that appears only in the c-polarized channel and whose intensity strongly varies with the l component of the scattering vector. These resonance excitations behave remarkably similar to the gap modes in the antiferromagnetic phase of the parent compound BaFe2As2.
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Affiliation(s)
- P Steffens
- Institut Laue Langevin, 6 Rue Jules Horowitz, BP 156, F-38042 Grenoble Cedex 9, France.
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131
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Ideta S, Yoshida T, Nishi I, Fujimori A, Kotani Y, Ono K, Nakashima Y, Yamaichi S, Sasagawa T, Nakajima M, Kihou K, Tomioka Y, Lee CH, Iyo A, Eisaki H, Ito T, Uchida S, Arita R. Dependence of carrier doping on the impurity potential in transition-metal-substituted FeAs-based superconductors. Phys Rev Lett 2013; 110:107007. [PMID: 23521287 DOI: 10.1103/physrevlett.110.107007] [Citation(s) in RCA: 6] [Impact Index Per Article: 0.5] [Reference Citation Analysis] [What about the content of this article? (0)] [Affiliation(s)] [Abstract] [Track Full Text] [Subscribe] [Scholar Register] [Received: 05/08/2012] [Revised: 01/14/2013] [Indexed: 06/01/2023]
Abstract
In order to examine to what extent the rigid-band-like electron doping scenario is applicable to the transition metal-substituted Fe-based superconductors, we have performed angle-resolved photoemission spectroscopy studies of Ba(Fe(1-x)Ni(x))(2)As(2) (Ni-122) and Ba(Fe(1-x)Cu(x))(2)As(2) (Cu-122), and compared the results with Ba(Fe(1-x)Co(x))(2)As(2) (Co-122). We find that Ni 3d-derived features are formed below the Fe 3d band and that Cu 3d-derived ones further below it. The electron and hole Fermi surface (FS) volumes are found to increase and decrease with substitution, respectively, qualitatively consistent with the rigid-band model. However, the total extra electron number estimated from the FS volumes (the total electron FS volume minus the total hole FS volume) is found to decrease in going from Co-, Ni-, to Cu-122 for a fixed nominal extra electron number, that is, the number of electrons that participate in the formation of FS decreases with increasing impurity potential. We find that the Néel temperature T(N) and the critical temperature T(c) maximum are determined by the FS volumes rather than the nominal extra electron concentration or the substituted atom concentration.
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Affiliation(s)
- S Ideta
- Department of Physics, University of Tokyo, Bunkyo-ku, Tokyo 113-0033, Japan
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132
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Chung BY, Kim HO, Kim JH, Cho SI, Lee CH, Park CW. The proactive treatment of atopic dermatitis with tacrolimus ointment in Korean patients: a comparative study between once-weekly and thrice-weekly applications. Br J Dermatol 2013; 168:908-10. [PMID: 23110605 DOI: 10.1111/bjd.12115] [Citation(s) in RCA: 10] [Impact Index Per Article: 0.9] [Reference Citation Analysis] [What about the content of this article? (0)] [MESH Headings] [Track Full Text] [Journal Information] [Subscribe] [Scholar Register] [Indexed: 11/28/2022]
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Lee JK, Lee CH, Choi CH. QCT bone mineral density responses to 1 year of oral bisphosphonate after total knee replacement for knee osteoarthritis. Osteoporos Int 2013; 24:287-92. [PMID: 22358316 DOI: 10.1007/s00198-012-1925-x] [Citation(s) in RCA: 8] [Impact Index Per Article: 0.7] [Reference Citation Analysis] [What about the content of this article? (0)] [Affiliation(s)] [Abstract] [MESH Headings] [Track Full Text] [Journal Information] [Submit a Manuscript] [Subscribe] [Scholar Register] [Received: 08/04/2011] [Accepted: 01/31/2012] [Indexed: 11/25/2022]
Abstract
UNLABELLED Bone mineral density (BMD) declined in more than half (53.7%) of post-total knee arthroplasty (TKA) patients (44 of the 82) after 1 year of oral bisphosphonate treatment, and that this decline was significant in bilateral TKA patients. INTRODUCTION TKA has proven to be an extremely successful procedure in terms of improving ambulatory function. However, the effects of such improvements in ambulatory function and of bisphosphonate on axial BMD have not been established. The purpose of this study was to determine the effect of 1 year of oral bisphosphonate in postmenopausal patients that have undergone TKA and to identify factors related to BMD changes using lumbar spine quantitative computed tomography (QCT). METHODS Eighty-two postmenopausal women that underwent primary TKA for knee osteoarthritis and who received once-weekly oral alendronate 70 mg for 12 months after TKA were enrolled. The effect of 1 year of oral bisphosphonate treatment post-TKA and the factors related to general lumbar spine BMD changes by using QCT were determined. RESULTS Some 53.7% of patients (44 of the 82) experienced an average lumbar spine QCT BMD decline of -6 mg/ml (range -15 to -0.5 mg/ml) after 1 year of oral bisphosphonate treatment, whereas the remaining 38 patients (46.3%) experienced an average increase of 6.8 mg/ml (range 0.6 to 15.7 mg/ml). Logistic and linear regression analysis showed that bilateral TKA was significantly related to a BMD decline (p < 0.05). Other factors, such as, age, body mass index, number of comorbidities, and Knee Society scores were not found to be significantly related to BMD response. CONCLUSIONS BMD declined in more than half (53.7%) of the patients after bisphosphonate treatment, and that this decline was significant in bilateral TKA patients. We believe that reduced mobility during rehabilitation was probably responsible for these BMD reductions.
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Affiliation(s)
- J K Lee
- Department of Orthopaedic Surgery, Hanyang University College of Medicine, Seoul, Republic of Korea
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134
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Nakajima M, Ishida S, Tomioka Y, Kihou K, Lee CH, Iyo A, Ito T, Kakeshita T, Eisaki H, Uchida S. Effect of Co doping on the in-plane anisotropy in the optical spectrum of underdoped Ba(Fe(1-x)Co(x))2As2. Phys Rev Lett 2012; 109:217003. [PMID: 23215609 DOI: 10.1103/physrevlett.109.217003] [Citation(s) in RCA: 4] [Impact Index Per Article: 0.3] [Reference Citation Analysis] [What about the content of this article? (0)] [Affiliation(s)] [Abstract] [Track Full Text] [Subscribe] [Scholar Register] [Received: 07/02/2012] [Indexed: 06/01/2023]
Abstract
We investigate the anisotropy in the in-plane optical spectra of detwinned Ba(Fe(1-x)Co(x))(2)As(2). The optical conductivity spectrum of BaFe(2)As(2) shows appreciable anisotropy in the magnetostructural ordered phase, whereas the dc (ω = 0) resistivity is nearly isotropic at low temperatures. Upon Co doping, the resistivity becomes highly anisotropic, while the finite-energy intrinsic anisotropy is suppressed. It is found that anisotropy in resistivity arises from anisotropic impurity scattering due to the presence of doped Co atoms, and it is extrinsic in origin. The intensity of a specific optical phonon mode is also found to show striking anisotropy in the ordered phase. The anisotropy induced by the Co impurity and that observed in the optical phonon mode are hallmarks of the highly polarizable electronic state in the ordered phase.
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Affiliation(s)
- M Nakajima
- Department of Physics, University of Tokyo, Tokyo 113-0033, Japan.
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135
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Lim D, Wang WL, Lee CH, Dodge T, Gilks B, Oliva E. Old versus new FIGO staging systems in predicting overall survival in patients with uterine leiomyosarcoma: a study of 86 cases. Gynecol Oncol 2012; 128:322-6. [PMID: 23153591 DOI: 10.1016/j.ygyno.2012.11.009] [Citation(s) in RCA: 15] [Impact Index Per Article: 1.3] [Reference Citation Analysis] [What about the content of this article? (0)] [Affiliation(s)] [Abstract] [Track Full Text] [Journal Information] [Subscribe] [Scholar Register] [Received: 07/12/2012] [Revised: 11/05/2012] [Accepted: 11/07/2012] [Indexed: 01/21/2023]
Abstract
OBJECTIVES Uterine leiomyosarcoma (uLMS) was staged using the FIGO system for endometrial cancers. The new FIGO system takes into consideration tumor size disregarding myometrial and cervical involvement. We aimed to compare the two systems and see which more accurately predicts overall survival (OS). METHODS 86 patients with uLMS (1984-2010) were retrospectively staged using both FIGO systems. Mean OS rates were estimated using the Kaplan-Meier method. RESULTS More patients had stage-I disease by the new FIGO system (42 versus 33). Five versus 18 and 27 versus 5 had old and new stage-II and III diseases respectively. Five and 4 patients with old stage II and III uLMS respectively were downstaged to stage I while 18 with old stage III were downstaged to stage II. Median follow-up was 23.5 months with a median OS of 114 (95% CI, 61-166) months. Although patients with stage I tumors had a higher mean OS rate compared to those with higher stage disease by either system, patients with old stage II-IV disease showed similar mean OS rates, with stage III-IV patients having a slightly better mean OS and a similar trend was observed with the new system. Patients with new FIGO stage III had a higher mean OS rate than those with stage II or IV disease (37.6 versus 28.1 and 34.3 months). Nonetheless, no statistical significant differences were seen in OS according to stage using either system (p=0.786 and p=0.400 respectively). CONCLUSION Neither FIGO staging system is ideal in classifying patients into four clinically significant stages.
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Affiliation(s)
- D Lim
- Department of Pathology, National University Health System, Singapore
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136
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Juang DF, Lee CH, Hsueh SC. Comparison of electrogenic capabilities of microbial fuel cell with different light power on algae grown cathode. Bioresour Technol 2012; 123:23-9. [PMID: 22929741 DOI: 10.1016/j.biortech.2012.07.041] [Citation(s) in RCA: 11] [Impact Index Per Article: 0.9] [Reference Citation Analysis] [What about the content of this article? (0)] [Affiliation(s)] [Abstract] [MESH Headings] [Track Full Text] [Subscribe] [Scholar Register] [Received: 05/08/2012] [Revised: 07/11/2012] [Accepted: 07/13/2012] [Indexed: 05/07/2023]
Abstract
Electricity generation capabilities of microbial fuel cell with different light power on algae grown cathode were compared. Results showed that microbial fuel cell with 6 and 12W power of light always produced higher voltage and power density than with 18 and 26W. Similarly, microbial fuel cell with 6 and 12W of light power always displayed higher Coulombic efficiency and specific power than the one with 18 and 26W. The results also showed that microbial fuel cell with covered anodic chamber always displayed higher voltage, power density, Coulombic efficiency and specific power than the one without covered anodic chamber. Binary quadratic equations can be used to express the relationships between the light power and the voltage, power density, Coulombic efficiency and specific power. Although lower power of light on algae grown cathode and covering anodic chamber will increase system's electricity production, they will not significantly reduce its internal resistance.
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Affiliation(s)
- D F Juang
- Department of Health Business Administration, Meiho University, 23, Pingguang Rd., Neipu, Pingtung 912, Taiwan, ROC.
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137
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Kim S, Cha JM, Lee CH, Shin HP, Park JJ, Joo KR, Lee JI, Jeun JW, Lim K, Lim JU, Choi JH. Rectal perforation due to benign stricture caused by rectal burns associated with hot coffee enemas. Endoscopy 2012; 44 Suppl 2 UCTN:E32-3. [PMID: 22396264 DOI: 10.1055/s-0031-1291512] [Citation(s) in RCA: 5] [Impact Index Per Article: 0.4] [Reference Citation Analysis] [What about the content of this article? (0)] [Affiliation(s)] [Track Full Text] [Journal Information] [Submit a Manuscript] [Subscribe] [Scholar Register] [Indexed: 12/10/2022]
Affiliation(s)
- S Kim
- Department of Internal Medicine, Kyung Hee University Hospital at Gang Dong, Kyung Hee University College of Medicine, Seoul, Republic of Korea
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Kim MH, Yun CH, Lee CH, Ha JK. The effects of fermented soybean meal on immunophysiological and stress-related parameters in Holstein calves after weaning. J Dairy Sci 2012; 95:5203-5212. [PMID: 22916926 DOI: 10.3168/jds.2012-5317] [Citation(s) in RCA: 27] [Impact Index Per Article: 2.3] [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: 01/03/2012] [Accepted: 05/14/2012] [Indexed: 11/19/2022]
Abstract
The present experiment was conducted to investigate the effects of partial substitution of soybean meal (SBM) with fermented SBM (FSBM) on immunophysiological and stress-related parameters in Holstein calves after weaning. Eighteen Holstein calves were randomly assigned to receive either SBM or FSBM (5% of SBM was replaced with FSBM) calf starter and calves were weaned at 42 d of age. It was noted that FSBM contained a lower content of trypsin inhibitor but higher crude protein, amino acids, and small-sized peptides than those of SBM. The group fed FSBM calf starter significantly increased body weight gain and intakes of both feed and milk, when compared with those fed SBM calf starter at 4 wk of age. Calves fed the FSBM calf starter had significantly lower fecal scores than those fed the SBM calf starter during both pre- and postweaning periods. Calves also had better health scores when fed the FSBM calf starter than those fed SBM during the preweaning period. Weaning challenge significantly increased proinflammatory cytokines, tumor necrosis factor α, IL-1β, and IL-6 levels at 1d postweaning (DPW). The TNF-α and IL-6 levels of the SBM group were significantly higher compared with those of the FSBM group at 3 DPW. Acute phase proteins (serum amyloid A and haptoglobin) in the serum were increased after weaning. Concentrations of serum amyloid A and haptoglobin in calves fed FSBM calf starter were significantly lower than those fed the SBM calf starter at 3 and 5 DPW, respectively. The concentration of cortisol was significantly lower in the FSBM group than that of the SBM group at 3 DPW. Weaning stress did not cause drastic changes in the total serum immunoglobulin levels and composition of peripheral lymphocytes. Our results indicate that FSBM may not only improve growth performance, feed intake, and health conditions during the preweaning period, but also alleviate stress responses, which was indicated by reduced induction of stress hormone, proinflammatory cytokines, and acute phase proteins in Holstein calves after weaning.
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Affiliation(s)
- M H Kim
- Department of Agricultural Biotechnology and Research Institute for Agriculture and Life Sciences, College of Agriculture and Life Sciences, Seoul National University, Seoul 151-921, Republic of Korea
| | - C H Yun
- Department of Agricultural Biotechnology and Research Institute for Agriculture and Life Sciences, College of Agriculture and Life Sciences, Seoul National University, Seoul 151-921, Republic of Korea; Center for Agricultural Biomaterials, Seoul National University, 599 Gwanangno, Gwanak-gu, Seoul 151-921, Republic of Korea
| | - C H Lee
- Genebiotech Co. Ltd., Gongju, Republic of Korea
| | - J K Ha
- Department of Agricultural Biotechnology and Research Institute for Agriculture and Life Sciences, College of Agriculture and Life Sciences, Seoul National University, Seoul 151-921, Republic of Korea.
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Reid JP, Tanatar MA, Juneau-Fecteau A, Gordon RT, de Cotret SR, Doiron-Leyraud N, Saito T, Fukazawa H, Kohori Y, Kihou K, Lee CH, Iyo A, Eisaki H, Prozorov R, Taillefer L. Universal heat conduction in the iron arsenide superconductor KFe2As2: evidence of a d-wave state. Phys Rev Lett 2012; 109:087001. [PMID: 23002766 DOI: 10.1103/physrevlett.109.087001] [Citation(s) in RCA: 9] [Impact Index Per Article: 0.8] [Reference Citation Analysis] [What about the content of this article? (0)] [Affiliation(s)] [Abstract] [Track Full Text] [Subscribe] [Scholar Register] [Received: 01/16/2012] [Indexed: 06/01/2023]
Abstract
The thermal conductivity κ of the iron arsenide superconductor KFe2As2 was measured down to 50 mK for a heat current parallel and perpendicular to the tetragonal c axis. A residual linear term at T→0, κ(0)/T is observed for both current directions, confirming the presence of nodes in the superconducting gap. Our value of κ(0)/T in the plane is equal to that reported by Dong et al. [Phys. Rev. Lett. 104, 087005 (2010)] for a sample whose residual resistivity ρ(0) was 10 times larger. This independence of κ(0)/T on impurity scattering is the signature of universal heat transport, a property of superconducting states with symmetry-imposed line nodes. This argues against an s-wave state with accidental nodes. It favors instead a d-wave state, an assignment consistent with five additional properties: the magnitude of the critical scattering rate Γ(c) for suppressing T(c) to zero; the magnitude of κ(0)/T, and its dependence on current direction and on magnetic field; the temperature dependence of κ(T).
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Affiliation(s)
- J-Ph Reid
- Département de physique and RQMP, Université de Sherbrooke, Sherbrooke, Québec, Canada
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Matsuda M, Fishman RS, Hong T, Lee CH, Ushiyama T, Yanagisawa Y, Tomioka Y, Ito T. magnetic dispersion and anisotropy in multiferroic BiFeO3. Phys Rev Lett 2012; 109:067205. [PMID: 23006302 DOI: 10.1103/physrevlett.109.067205] [Citation(s) in RCA: 5] [Impact Index Per Article: 0.4] [Reference Citation Analysis] [What about the content of this article? (0)] [Affiliation(s)] [Abstract] [Track Full Text] [Subscribe] [Scholar Register] [Received: 03/05/2012] [Indexed: 06/01/2023]
Abstract
We have determined the full magnetic dispersion relations of multiferroic BiFeO3. In particular, two excitation gaps originating from magnetic anisotropies have been clearly observed. The direct observation of the gaps enables us to accurately determine the Dzyaloshinskii-Moriya (DM) interaction and the single ion anisotropy. The DM interaction supports a sizable magnetoelectric coupling in this compound.
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Affiliation(s)
- M Matsuda
- Quantum Condensed Matter Division, Oak Ridge National Laboratory, Oak Ridge, Tennessee 37831, USA
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141
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Blackstone BN, Willard JJ, Lee CH, Nelson MT, Hart RT, Lannutti JJ, Powell HM. Plasma surface modification of electrospun fibers for adhesion-based cancer cell sorting. Integr Biol (Camb) 2012; 4:1112-21. [PMID: 22832548 DOI: 10.1039/c2ib20025b] [Citation(s) in RCA: 13] [Impact Index Per Article: 1.1] [Reference Citation Analysis] [What about the content of this article? (0)] [Affiliation(s)] [Abstract] [Track Full Text] [Journal Information] [Subscribe] [Scholar Register] [Indexed: 12/31/2022]
Abstract
Personalized cancer therapies drive the need for devices that rapidly and accurately segregate cancer cells from solid tumors. One potential sorting strategy is to segregate populations of cells based on their relative strength of adhesion. To investigate the effect of surface hydrophilicity and cell phenotype on adhesion, primary human breast skin fibroblasts and keratinocytes and MCF-7 breast cancer cells were seeded onto air and CF(4) plasma-treated nanofibers followed by exposure to three shear stresses (200, 275 and 350 dynes per cm(2)) 1 hour after inoculation. No difference in strength of adhesion was measured in either fibroblasts or keratinocytes on either plasma treated-surface: all exhibited >60% of the initial cell count after a 5 minute exposure to 350 dynes per cm(2) of shear stress. In contrast, a significant difference between relative strength of adhesion on air versus CF(4) plasma-treated surfaces was observed for MCF-7 cells: 26% and 6.6% of cells remained on the air and CF(4) plasma-treated surfaces, respectively. The ability to sort this cancer cell line from two non-cancerous primary human cells was evaluated by inoculating a mixture of all three cell types simultaneously onto CF(4) treated nanofibers followed by 1 hour of culture and exposure to 350 dynes per cm(2) shear stress. The majority of MCF-7 cells were removed (0.7% remained) while a majority of fibroblasts and keratinocytes remained adhered (74 and 57%). Post-sorted MCF-7 viability and morphology remained unchanged, preserving the possibility of post-separation and analysis. These data suggest that the plasma treatment of electrospun scaffolds provides a tool useful in sorting cancer cells from a mixed cell population based on adhesion strength.
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Affiliation(s)
- B N Blackstone
- Department of Biomedical Engineering, The Ohio State University, Columbus, OH 43210, USA
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142
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Oyama KI, Lee CH, Fang HK, Cheng CZ. Means to remove electrode contamination effect of Langmuir probe measurement in space. Rev Sci Instrum 2012; 83:055113. [PMID: 22667663 DOI: 10.1063/1.4722167] [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: 06/01/2023]
Abstract
Precaution to remove the serious effect of electrode contamination in Langmuir probe experiments has not been taken in many space measurements because the effect is either not understood or ignored. We stress here that one should pay extra attention to the electrode contamination effect to get accurate and reliable plasma measurements so that the long time effort for sounding rocket/satellite missions does not end in vain or becomes less fruitful. In this paper, we describe two main features of voltage-current characteristic curves associated with the contaminated Langmuir probe, which are predicted from the equivalent circuit model, which we proposed in 1970's. We then show that fast sweeping dc Langmuir probes can give reliable results in the steady state regime. The fast sweeping probe can also give reliable results in transient situations such as satellite moves through plasma bubble in the ionosphere where the electron density drastically changes. This fact was first confirmed in our laboratory experiment.
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Affiliation(s)
- K-I Oyama
- Plasma and Space Science Center, National Cheng Kung University, No.1 Ta-Hsueh Rd., Tainan 70101, Taiwan
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Kim YD, Kim YH, Cho YM, Kim DK, Ahn SW, Lee JM, Chanda D, Shong M, Lee CH, Choi HS. Metformin ameliorates IL-6-induced hepatic insulin resistance via induction of orphan nuclear receptor small heterodimer partner (SHP) in mouse models. Diabetologia 2012; 55:1482-94. [PMID: 22349108 DOI: 10.1007/s00125-012-2494-4] [Citation(s) in RCA: 51] [Impact Index Per Article: 4.3] [Reference Citation Analysis] [What about the content of this article? (0)] [Affiliation(s)] [Abstract] [MESH Headings] [Track Full Text] [Journal Information] [Submit a Manuscript] [Subscribe] [Scholar Register] [Received: 11/23/2011] [Accepted: 01/09/2012] [Indexed: 01/14/2023]
Abstract
AIMS/HYPOTHESIS IL-6 is a proinflammatory cytokine associated with the pathogenesis of hepatic diseases. Metformin is an anti-diabetic drug used for the treatment of type 2 diabetes, and orphan nuclear receptor small heterodimer partner (SHP, also known as NR0B2), a transcriptional co-repressor, plays an important role in maintaining metabolic homeostasis. Here, we demonstrate that metformin-mediated activation of AMP-activated protein kinase (AMPK) increases SHP protein production and regulates IL-6-induced hepatic insulin resistance. METHODS We investigated metformin-mediated SHP production improved insulin resistance through the regulation of an IL-6-dependent pathway (involving signal transducer and activator of transcription 3 [STAT3] and suppressor of cytokine signalling 3 [SOCS3]) in both Shp knockdown and Shp null mice. RESULTS IL-6-induced STAT3 transactivation and SOCS3 production were significantly repressed by metformin, adenoviral constitutively active AMPK (Ad-CA-AMPK), and adenoviral SHP (Ad-SHP), but not in Shp knockdown, or with the adenoviral dominant negative form of AMPK (Ad-DN-AMPK). Chromatin immunoprecipitation (ChIP), co-immunoprecipitation (Co-IP) and protein localisation studies showed that SHP inhibits DNA binding of STAT3 on the Socs3 gene promoter via interaction and colocalisation within the nucleus. Upregulation of inflammatory genes and downregulation of hepatic insulin signalling by acute IL-6 treatment were observed in wild-type mice but not in Shp null mice. Finally, chronic IL-6 exposure caused hepatic insulin resistance, leading to impaired insulin tolerance and elevated gluconeogenesis, and these phenomena were aggravated in Shp null mice. CONCLUSIONS/INTERPRETATION Our results demonstrate that SHP upregulation by metformin may prevent hepatic disorders by regulating the IL-6-dependent pathway, and that this pathway can help to ameliorate the pathogenesis of cytokine-mediated metabolic dysfunction.
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Affiliation(s)
- Y D Kim
- National Creative Research Initiatives Center for Nuclear Receptor Signals, Hormone Research Center, School of Biological Sciences and Technology, Chonnam National University, Gwangju 500-757, Republic of Korea
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Kim JH, Kang YJ, Kim DS, Lee CH, Jeon YS, Lee NK, Oh MH. The relationship between mast cell density and tumour grade in transitional cell carcinoma of the bladder. J Int Med Res 2012; 39:1675-81. [PMID: 22117967 DOI: 10.1177/147323001103900509] [Citation(s) in RCA: 9] [Impact Index Per Article: 0.8] [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] Open
Abstract
This study investigated the relationship between mast cell numbers and the grade of bladder transitional cell carcinoma (TCC). Bladder TCC biopsies were obtained via transurethral resection and 45 stage T1 specimens were included in the study. Specimens were sorted into two groups, low grade (grade I) and high grade (grades II and III). Samples were stained using haematoxylin and eosin, toluidine blue and immunohistochemical staining for tryptase. Mast cells were examined by light microscopy and cell density was recorded. Mast cell density was significantly higher in high-grade TCC than low-grade TCC. There was also a significant relationship between the number of mast cells identified using toluidine blue staining or immunohistochemical staining for tryptase. Detailed studies of mast cell function will enable the development of more effective antitumour therapies via mast cell manipulation.
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Affiliation(s)
- J H Kim
- Department of Urology, Korea University Hospital, Korea University College of Medicine, Ansan, Republic of Korea
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Paterson-Beedle M, Jeong BC, Lee CH, Jee KY, Kim WH, Renshaw JC, Macaskie LE. Radiotolerance of phosphatases of a Serratia sp.: potential for the use of this organism in the biomineralization of wastes containing radionuclides. Biotechnol Bioeng 2012; 109:1937-46. [PMID: 22422344 DOI: 10.1002/bit.24467] [Citation(s) in RCA: 10] [Impact Index Per Article: 0.8] [Reference Citation Analysis] [What about the content of this article? (0)] [Affiliation(s)] [Abstract] [Track Full Text] [Journal Information] [Subscribe] [Scholar Register] [Received: 09/22/2011] [Revised: 01/29/2012] [Accepted: 02/01/2012] [Indexed: 11/05/2022]
Abstract
Aqueous wastes from nuclear fuel reprocessing present special problems of radiotoxicity of the active species. Cells of Serratia sp. were found previously to accumulate high levels of hydrogen uranyl phosphate (HUP) via the activity of a phosphatase enzyme. Uranium is of relatively low radiotoxicity whereas radionuclide fission products such as (90)Sr and (137)Cs are highly radiotoxic. These radionuclides can be co-crystallized, held within the bio-HUP "host" lattice on the bacterial cells and thereby removed from contaminated solution, depending on continued phosphatase activity. Radiostability tests using a commercial (60)Co γ-source showed that while cell viability and activity of purified phosphatase were lost within a few hours on irradiation, whole-cell phosphatase retained 80% of the initial activity, even after loss of cell culturability, which was increased to 100% by the incorporation of mercaptoethanol as an example radioprotectant, beyond an accumulated dose of >1.3 MGy. Using this co-crystallization approach (without mercaptoethanol) (137)Cs(+) and (85)Sr(2+) were removed from a simulated waste selectively against a 33-fold excess of Na(+).
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Affiliation(s)
- M Paterson-Beedle
- School of Biosciences, University of Birmingham, Edgbaston, Birmingham B15 2TT, UK
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146
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Affiliation(s)
- Y H Kim
- Seoul National University College of Medicine, Neurosurgery, Seoul, Republic of Korea
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147
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Xie CB, Chan MY, Teo SG, Low AF, Tan HC, Lee CH. Acute myocardial infarction in young Asian women: a comparative study on Chinese, Malay and Indian ethnic groups. Singapore Med J 2011; 52:835-839. [PMID: 22173254] [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] [Journal Information] [Subscribe] [Scholar Register] [Indexed: 05/31/2023]
Abstract
INTRODUCTION There is a paucity of data on acute myocardial infarction (AMI) in young Asian women and of comparative data among various ethnic groups with respect to risk factor profile and clinical outcomes. We present a comprehensive overview of the clinical characteristics of young Asian women with AMI and a comparative analysis among Chinese, Malay and Indian women in a multi-ethnic Asian country. METHODS We studied 45 Asian female patients aged 50 years and below who were admitted to our hospital with a diagnosis of ST-segment elevation myocardial infarction (STEMI) or non-ST-segment elevation myocardial infarction (NSTEMI). RESULTS Overall, diabetes mellitus, hypertension and hyperlipidaemia were prevalent in the study population. Hyperlipidaemia was more prevalent among Indian patients, while diabetes mellitus was more common among Malay patients. Only a minority of the study patients were current smokers. Among the 20 patients admitted with STEMI, 17 (85 percent) received urgent reperfusion therapy. The mean symptom-to-balloon time and door-to-balloon time for the Malay patients were longer compared to those for other ethnic groups. Among the 25 patients admitted with NSTEMI, 12 (48 percent) underwent coronary revascularisation therapy. The average duration of hospital stay was 4 +/- 4.1 days, with no significant difference observed among the various ethnic groups. CONCLUSION Many young Asian women with AMI have identifiable risk factors that are different from those found in the Western population. There seems to be an ethnic effect on the prevalence of these risk factors and door-to-balloon time.
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Affiliation(s)
- C B Xie
- Department of Medicine, Yong Loo Lin School of Medicine, National University of Singapore, National University Health System, Level 10 NUHS Tower Block, Kent Ridge Road, Singapore 119228
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Chau PH, Woo J, Lee CH, Cheung WL, Chen J, Chan WM, Hui L, McGhee SM. Older people with diabetes have higher risk of depression, cognitive and functional impairments: implications for diabetes services. J Nutr Health Aging 2011; 15:751-5. [PMID: 22089223 DOI: 10.1007/s12603-011-0071-z] [Citation(s) in RCA: 20] [Impact Index Per Article: 1.5] [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: 01/01/2023]
Abstract
OBJECTIVES To examine the relationship between diabetes and impairments in functional and cognitive status as well as depression in older people. DESIGN Cross-sectional study. SETTING Elderly Health Centres (EHC) in Hong Kong. PARTICIPANTS 66,813 older people receiving baseline assessment at EHC in 1998 to 2001. MEASUREMENTS Diabetes status was defined by self-report and blood glucose tests. Functional status was assessed by 5 items of instrumental activities of daily living (IADL) and 7 items of activities of daily living (ADL). Cognitive status was screened by the Abbreviated Mental Test-Hong Kong version (AMT). Depressive symptoms were screened by the Geriatric Depression Scale-Chinese version (GDS). RESULTS Among the subjects, 10.4% reported having regular treatment for diabetes, 3.4% had diabetes but were not receiving regular treatment, and 86.2% did not have diabetes. After controlling for age, sex and education level, those having regular treatment for diabetes were 1.7 times more likely (OR=1.65, 95% CI: 1.51-1.80) to have functional impairment, 1.3 times more likely (OR=1.28, 95% CI: 1.11-1.48) to have cognitive impairment and 1.3 times more likely (OR=1.35, 95% CI: 1.25-1.46) to have depression, than older people without diabetes. CONCLUSION Older people with diabetes may be less capable of managing the disease than the younger ones as a result of increased risk of both physical and cognitive impairment. This study provided further evidence for the need of an international consensus statement regarding care of diabetes in older people.
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Affiliation(s)
- P H Chau
- Faculty of Social Sciences, The University of Hong Kong, Hong Kong.
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Lee CH, Chan WP. Foramen of Winslow hernia. Acta Clin Belg 2011; 66:453. [PMID: 22338311 DOI: 10.2143/acb.66.6.2062614] [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] [Journal Information] [Subscribe] [Scholar Register] [Indexed: 05/31/2023]
Affiliation(s)
- C H Lee
- Department of Radiology, Wan Fang Hospital, Taipei Medical University, Tapei, Taiwan
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Lee CH, Chan WP. Bilateral carotid body tumours. Acta Clin Belg 2011; 66:454. [PMID: 22338312 DOI: 10.2143/acb.66.6.2062615] [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] [Journal Information] [Subscribe] [Scholar Register] [Indexed: 05/31/2023]
Affiliation(s)
- C H Lee
- Department of Radiology, Wan Fang Hospital, Taipei Medical University, Tapei, Taiwan
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