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Bruch GM, Engel K, Schropp J, Grabherr S. Realistic three-dimensional imaging of injuries in forensic medicine - Survey-based method comparison of CRT and VRT. J Forensic Leg Med 2024; 103:102681. [PMID: 38588619 DOI: 10.1016/j.jflm.2024.102681] [Citation(s) in RCA: 0] [Impact Index Per Article: 0] [Reference Citation Analysis] [What about the content of this article? (0)] [Affiliation(s)] [Abstract] [Key Words] [Track Full Text] [Journal Information] [Subscribe] [Scholar Register] [Received: 02/09/2024] [Revised: 03/14/2024] [Accepted: 03/23/2024] [Indexed: 04/10/2024]
Abstract
OBJECTIVE A comparison between Cinematic Rendering Technique (CRT) and Volume Rendering Technique (VRT) in cases with postmortem CT-angiography (PMCTA) was carried out. METHODS For different injuries seen in PMCTA, a VRT and a CRT image of exactly the same pathological section was generated. Two questionnaires were created, one with CRT and one with VRT reconstructions, with the same questions per 3D-image. The questionnaires were sent to forensic pathologists, lawyers and police officers. In total eleven different injuries had to be analyzed. RESULTS In total 109 questionnaires were answered fully. Of these returnees, 36 stated that they were forensic pathologists. Seventy-three people were assigned to the group of medical laypersons, in the study this group consists mainly of police officers, judges and lawyers. Between the two software programs CRT and VRT that were compared, no significant difference could be identified in any of the participating groups with regard to the assessment of the life-threatening nature of the injury images shown. When asked about the comprehensibility of pathology, there was a significant difference in favour of CRT. This advantage was apparent to named medical laypersons and to forensic pathologists. CONCLUSIONS The study showed a positive trend that CRT may be more understandable than VRT. Not only the medical laypersons, but also the forensic physicians found CRT to be beneficial.
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Affiliation(s)
- G M Bruch
- Institut für Rechtsmedizin, Ludwig-Maximilians-Universität, Munich, Germany.
| | - K Engel
- Medical Imaging Technologies, Siemens Healthcare Technology Center, Erlangen, Germany
| | - J Schropp
- Jonas Schropp Consulting, Switzerland
| | - S Grabherr
- Centre Universitaire Romand de Médecine Légale, Hôpitaux Universitaires de Genève, Université de Genève, Switzerland; Centre Universitaire Romand de Médecine Légale, Centre Hospitalier Universitaire Vaudois, Université de Lausanne, Switzerland
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Brunet J, Cook AC, Walsh CL, Cranley J, Tafforeau P, Engel K, Berruyer C, O’Leary EB, Bellier A, Torii R, Werlein C, Jonigk DD, Ackermann M, Dollman K, Lee PD. Multidimensional Analysis of the Adult Human Heart in Health and Disease using Hierarchical Phase-Contrast Tomography (HiP-CT). bioRxiv 2023:2023.10.09.561474. [PMID: 37873359 PMCID: PMC10592740 DOI: 10.1101/2023.10.09.561474] [Citation(s) in RCA: 0] [Impact Index Per Article: 0] [Reference Citation Analysis] [What about the content of this article? (0)] [Affiliation(s)] [Abstract] [Grants] [Track Full Text] [Subscribe] [Scholar Register] [Indexed: 10/25/2023]
Abstract
Cardiovascular diseases (CVDs) are a leading cause of death worldwide. Current clinical imaging modalities provide resolution adequate for diagnosis but are unable to provide detail of structural changes in the heart, across length-scales, necessary for understanding underlying pathophysiology of disease. Hierarchical Phase-Contrast Tomography (HiP-CT), using new (4th) generation synchrotron sources, potentially overcomes this limitation, allowing micron resolution imaging of intact adult organs with unprecedented detail. In this proof of principle study (n=2), we show the utility of HiP-CT to image whole adult human hearts ex-vivo: one 'control' without known cardiac disease and one with multiple known cardiopulmonary pathologies. The resulting multiscale imaging was able to demonstrate exemplars of anatomy in each cardiac segment along with novel findings in the cardiac conduction system, from gross (20 um/voxel) to cellular scale (2.2 um/voxel), non-destructively, thereby bridging the gap between macroscopic and microscopic investigations. We propose that the technique represents a significant step in virtual autopsy methods for studying structural heart disease, facilitating research into abnormalities across scales and age-groups. It opens up possibilities for understanding and treating disease; and provides a cardiac 'blueprint' with potential for in-silico simulation, device design, virtual surgical training, and bioengineered heart in the future.
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Affiliation(s)
- J. Brunet
- Department of Mechanical Engineering, University College London, London, UK
- European Synchrotron Radiation Facility, Grenoble, France
| | - A. C. Cook
- UCL Institute of Cardiovascular Science, London, UK
| | - C. L. Walsh
- Department of Mechanical Engineering, University College London, London, UK
| | - J. Cranley
- Wellcome Sanger Institute, Wellcome Genome Campus, Hinxton, Cambridge, UK
| | - P. Tafforeau
- European Synchrotron Radiation Facility, Grenoble, France
| | - K. Engel
- Siemens Healthineers, Erlangen, Germany
| | - C. Berruyer
- Department of Mechanical Engineering, University College London, London, UK
- European Synchrotron Radiation Facility, Grenoble, France
| | - E. Burke O’Leary
- Department of Mechanical Engineering, University College London, London, UK
| | - A. Bellier
- Laboratoire d’Anatomie des Alpes Françaises (LADAF), Université Grenoble Alpes, Grenoble, F
| | - R. Torii
- Department of Mechanical Engineering, University College London, London, UK
| | - C. Werlein
- Institute of Pathology, Hannover Medical School, Hannover, Germany
- Biomedical Research in End-stage and Obstructive Lung Disease Hannover (BREATH), German Lung Research Centre (DZL), Hannover, Germany
| | - D. D. Jonigk
- Biomedical Research in End-stage and Obstructive Lung Disease Hannover (BREATH), German Lung Research Centre (DZL), Hannover, Germany
- Institute of Pathology, Aachen Medical University, RWTH Aachen, Germany
| | - M. Ackermann
- Institute of Pathology and Molecular Pathology, Helios University Clinic Wuppertal, University of Witten/Herdecke, Wuppertal, Germany
- Institute of Functional and Clinical Anatomy, University Medical Center of the Johannes Gutenberg-University Mainz, Mainz, Germany
| | - K. Dollman
- European Synchrotron Radiation Facility, Grenoble, France
| | - P. D. Lee
- Department of Mechanical Engineering, University College London, London, UK
- Research Complex at Harwell, Didcot, UK
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Pasini MPB, Engel E, Engel K, Mallmann AA, Link D. BIoecology of Oncideres cervina Thomson (Coleoptera: Cerambycidae) on Persea americana Mill. (Lauraceae). BRAZ J BIOL 2023; 83:e272252. [PMID: 37672434 DOI: 10.1590/1519-6984.272252] [Citation(s) in RCA: 0] [Impact Index Per Article: 0] [Reference Citation Analysis] [What about the content of this article? (0)] [Affiliation(s)] [Abstract] [MESH Headings] [Track Full Text] [Journal Information] [Subscribe] [Scholar Register] [Received: 02/21/2023] [Accepted: 06/20/2023] [Indexed: 09/08/2023] Open
Abstract
Cerambycidae beetles limit production and establishment of forest and fruit trees. Oncideres cervina Thomson, 1868 (Coleoptera: Cerambycidae) is one of the most important species. The objective was to record O. cervina girdling branches of Persea americana Mill. (Lauraceae) for the first time, check the number of oviposition incisions (Noi) as a function of the diameter of branch sections, period of emergence, and describe the larval-pupal chamber. Individuals of O. cervina were observed, for the first time, in P. americana orchards in Santa Maria, Rio Grande do Sul, Brazil. The middle section of branches (40-60 cm interval) had higher number of incisions. Girdled branches with a diameter of 40-50 mm had higher number of them. Adults emerged from November through January. Larval-pupal boreholes had diameters between 9 and 11 mm, and average tunnel length was 28 mm, with a mean volume of consumed wood of 4.3 mL. This information is useful for establishing integrated pest management practices against O. cervina in P. americana since this crop has a high added value and can be significantly compromised by attack by Cerambycidae beetles.
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Affiliation(s)
- M P B Pasini
- INTAGRO Consultoria, Pesquisa e Treinamentos, Cruz Alta, RS, Brasil
| | - E Engel
- Universidade de São Paulo, Escola Superior de Agricultura "Luiz de Queiroz", Departamento de Entomologia e Acarologia, Piracicaba, SP, Brasil
| | - K Engel
- Universidade Federal do Paraná - UFPR, Departamento de Engenharia Florestal, Curitiba, PR, Brasil
| | - A A Mallmann
- Universidade Federal do Paraná - UFPR, Departamento de Engenharia Florestal, Curitiba, PR, Brasil
| | - D Link
- Universidade Federal de Santa Maria, Centro de Ciências Rurais, Departamento de Defesa Fitossanitária, Santa Maria, RS, Brasil
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Albert A, Alfaro R, Alvarez C, Arteaga-Velázquez JC, Avila Rojas D, Ayala Solares HA, Babu R, Belmont-Moreno E, Brisbois C, Caballero-Mora KS, Capistrán T, Carramiñana A, Casanova S, Chaparro-Amaro O, Cotti U, Cotzomi J, Coutiño de León S, De la Fuente E, Diaz Hernandez R, Dingus BL, DuVernois MA, Durocher M, Díaz-Vélez JC, Ellsworth RW, Engel K, Espinoza C, Fan KL, Fang K, Fernández Alonso M, Fleischhack H, Fraija N, García-González JA, Garfias F, González MM, Goodman JA, Harding JP, Hernandez S, Hinton J, Huang D, Hueyotl-Zahuantitla F, Hüntemeyer P, Iriarte A, Joshi V, Kaufmann S, Lee J, Linnemann JT, Longinotti AL, Luis-Raya G, Malone K, Martinez O, Martínez-Castro J, Matthews JA, Miranda-Romagnoli P, Morales-Soto JA, Moreno E, Mostafá M, Nayerhoda A, Nellen L, Nisa MU, Noriega-Papaqui R, Olivera-Nieto L, Omodei N, Pérez Araujo Y, Pérez-Pérez EG, Rho CD, Rosa-González D, Ruiz-Velasco E, Salazar H, Salazar-Gallegos D, Sandoval A, Schneider M, Serna-Franco J, Smith AJ, Son Y, Springer RW, Tibolla O, Tollefson K, Torres I, Torres-Escobedo R, Turner R, Ureña-Mena F, Varela E, Villaseñor L, Wang X, Watson IJ, Willox E, Yun-Cárcamo S, Zhou H, de León C, Beacom JF, Linden T, Ng KCY, Peter AHG, Zhou B. Discovery of Gamma Rays from the Quiescent Sun with HAWC. Phys Rev Lett 2023; 131:051201. [PMID: 37595214 DOI: 10.1103/physrevlett.131.051201] [Citation(s) in RCA: 0] [Impact Index Per Article: 0] [Reference Citation Analysis] [What about the content of this article? (0)] [Affiliation(s)] [Abstract] [Track Full Text] [Subscribe] [Scholar Register] [Received: 12/06/2022] [Revised: 01/27/2023] [Accepted: 06/23/2023] [Indexed: 08/20/2023]
Abstract
We report the first detection of a TeV γ-ray flux from the solar disk (6.3σ), based on 6.1 years of data from the High Altitude Water Cherenkov (HAWC) observatory. The 0.5-2.6 TeV spectrum is well fit by a power law, dN/dE=A(E/1 TeV)^{-γ}, with A=(1.6±0.3)×10^{-12} TeV^{-1} cm^{-2} s^{-1} and γ=3.62±0.14. The flux shows a strong indication of anticorrelation with solar activity. These results extend the bright, hard GeV emission from the disk observed with Fermi-LAT, seemingly due to hadronic Galactic cosmic rays showering on nuclei in the solar atmosphere. However, current theoretical models are unable to explain the details of how solar magnetic fields shape these interactions. HAWC's TeV detection thus deepens the mysteries of the solar-disk emission.
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Affiliation(s)
- A Albert
- Physics Division, Los Alamos National Laboratory, Los Alamos, NM 87544, USA
| | - R Alfaro
- Instituto de F'isica, Universidad Nacional Autónoma de México, Ciudad de Mexico, Mexico
| | - C Alvarez
- Universidad Autónoma de Chiapas, Tuxtla Gutiérrez, Chiapas, México
| | | | - D Avila Rojas
- Instituto de F'isica, Universidad Nacional Autónoma de México, Ciudad de Mexico, Mexico
| | - H A Ayala Solares
- Department of Physics, Pennsylvania State University, University Park, PA, USA
| | - R Babu
- Department of Physics, Michigan Technological University, Houghton, MI, USA
| | - E Belmont-Moreno
- Instituto de F'isica, Universidad Nacional Autónoma de México, Ciudad de Mexico, Mexico
| | - C Brisbois
- Department of Physics, University of Maryland, College Park, MD, USA
| | | | - T Capistrán
- Instituto de Astronom'ia, Universidad Nacional Autónoma de México, Ciudad de Mexico, Mexico
| | - A Carramiñana
- Instituto Nacional de Astrof'isica, Óptica y Electrónica, Puebla, Mexico
| | - S Casanova
- Instytut Fizyki Jadrowej im Henryka Niewodniczanskiego Polskiej Akademii Nauk, IFJ-PAN, Krakow, Poland
| | - O Chaparro-Amaro
- Centro de Investigaci'on en Computaci'on, Instituto Polit'ecnico Nacional, M'exico City, M'exico
| | - U Cotti
- Universidad Michoacana de San Nicolás de Hidalgo, Morelia, Mexico
| | - J Cotzomi
- Facultad de Ciencias F'isico Matemáticas, Benemérita Universidad Autónoma de Puebla, Puebla, Mexico
| | - S Coutiño de León
- Department of Physics, University of Wisconsin-Madison, Madison, WI, USA
| | - E De la Fuente
- Departamento de F'isica, Centro Universitario de Ciencias Exactase Ingenierias, Universidad de Guadalajara, Guadalajara, Mexico
| | - R Diaz Hernandez
- Instituto Nacional de Astrof'isica, Óptica y Electrónica, Puebla, Mexico
| | - B L Dingus
- Physics Division, Los Alamos National Laboratory, Los Alamos, NM 87544, USA
- Department of Physics, University of Maryland, College Park, MD, USA
| | - M A DuVernois
- Department of Physics, University of Wisconsin-Madison, Madison, WI, USA
| | - M Durocher
- Physics Division, Los Alamos National Laboratory, Los Alamos, NM 87544, USA
| | - J C Díaz-Vélez
- Departamento de F'isica, Centro Universitario de Ciencias Exactase Ingenierias, Universidad de Guadalajara, Guadalajara, Mexico
| | - R W Ellsworth
- Department of Physics, University of Maryland, College Park, MD, USA
| | - K Engel
- Department of Physics, University of Maryland, College Park, MD, USA
| | - C Espinoza
- Instituto de F'isica, Universidad Nacional Autónoma de México, Ciudad de Mexico, Mexico
| | - K L Fan
- Department of Physics, University of Maryland, College Park, MD, USA
| | - K Fang
- Department of Physics, University of Wisconsin-Madison, Madison, WI, USA
| | - M Fernández Alonso
- Department of Physics, Pennsylvania State University, University Park, PA, USA
| | - H Fleischhack
- Department of Physics, Catholic University of America, 620 Michigan Avenue NE, Washington, DC 20064
- NASA Goddard Space Flight Center, Greenbelt, MD 20771, USA
- Center for Research and Exploration in Space Science and Technology, NASA/GSFC, Greenbelt, MD 20771
| | - N Fraija
- Instituto de Astronom'ia, Universidad Nacional Autónoma de México, Ciudad de Mexico, Mexico
| | - J A García-González
- Tecnologico de Monterrey, Escuela de Ingeniería y Ciencias, Avenue Eugenio Garza Sada 2501, Monterrey, N.L., Mexico, 64849
| | - F Garfias
- Instituto de Astronom'ia, Universidad Nacional Autónoma de México, Ciudad de Mexico, Mexico
| | - M M González
- Instituto de Astronom'ia, Universidad Nacional Autónoma de México, Ciudad de Mexico, Mexico
| | - J A Goodman
- Department of Physics, University of Maryland, College Park, MD, USA
| | - J P Harding
- Physics Division, Los Alamos National Laboratory, Los Alamos, NM 87544, USA
| | - S Hernandez
- Instituto de F'isica, Universidad Nacional Autónoma de México, Ciudad de Mexico, Mexico
| | - J Hinton
- Max-Planck Institute for Nuclear Physics, 69117 Heidelberg, Germany
| | - D Huang
- Department of Physics, Michigan Technological University, Houghton, MI, USA
| | | | - P Hüntemeyer
- Department of Physics, Michigan Technological University, Houghton, MI, USA
| | - A Iriarte
- Instituto de Astronom'ia, Universidad Nacional Autónoma de México, Ciudad de Mexico, Mexico
| | - V Joshi
- Erlangen Centre for Astroparticle Physics, Friedrich-Alexander-Universität Erlangen-Nürnberg, Erlangen, Germany
| | - S Kaufmann
- Universidad Politecnica de Pachuca, Pachuca, Hgo, Mexico
| | - J Lee
- University of Seoul, Seoul, Rep. of Korea
| | - J T Linnemann
- Department of Physics and Astronomy, Michigan State University, East Lansing, MI, USA
| | - A L Longinotti
- Instituto de Astronom'ia, Universidad Nacional Autónoma de México, Ciudad de Mexico, Mexico
| | - G Luis-Raya
- Universidad Politecnica de Pachuca, Pachuca, Hgo, Mexico
| | - K Malone
- Space Science and Applications Group, Los Alamos National Laboratory, Los Alamos, NM 87544, USA
| | - O Martinez
- Facultad de Ciencias F'isico Matemáticas, Benemérita Universidad Autónoma de Puebla, Puebla, Mexico
| | - J Martínez-Castro
- Centro de Investigaci'on en Computaci'on, Instituto Polit'ecnico Nacional, M'exico City, M'exico
| | - J A Matthews
- Dept of Physics and Astronomy, University of New Mexico, Albuquerque, NM, USA
| | | | - J A Morales-Soto
- Universidad Michoacana de San Nicolás de Hidalgo, Morelia, Mexico
| | - E Moreno
- Facultad de Ciencias F'isico Matemáticas, Benemérita Universidad Autónoma de Puebla, Puebla, Mexico
| | - M Mostafá
- Department of Physics, Pennsylvania State University, University Park, PA, USA
| | - A Nayerhoda
- Instytut Fizyki Jadrowej im Henryka Niewodniczanskiego Polskiej Akademii Nauk, IFJ-PAN, Krakow, Poland
| | - L Nellen
- Instituto de Ciencias Nucleares, Universidad Nacional Autónoma de Mexico, Ciudad de Mexico, Mexico
| | - M U Nisa
- Department of Physics and Astronomy, Michigan State University, East Lansing, MI, USA
| | | | - L Olivera-Nieto
- Max-Planck Institute for Nuclear Physics, 69117 Heidelberg, Germany
| | - N Omodei
- Department of Physics, Stanford University: Stanford, CA 94305-4060, USA
| | - Y Pérez Araujo
- Instituto de Astronom'ia, Universidad Nacional Autónoma de México, Ciudad de Mexico, Mexico
| | | | - C D Rho
- Department of Physics, Sungkyunkwan University, Suwon 16419, South Korea
| | - D Rosa-González
- Instituto Nacional de Astrof'isica, Óptica y Electrónica, Puebla, Mexico
| | - E Ruiz-Velasco
- Max-Planck Institute for Nuclear Physics, 69117 Heidelberg, Germany
| | - H Salazar
- Facultad de Ciencias F'isico Matemáticas, Benemérita Universidad Autónoma de Puebla, Puebla, Mexico
| | - D Salazar-Gallegos
- Department of Physics and Astronomy, Michigan State University, East Lansing, MI, USA
| | - A Sandoval
- Instituto de F'isica, Universidad Nacional Autónoma de México, Ciudad de Mexico, Mexico
| | - M Schneider
- Department of Physics, University of Maryland, College Park, MD, USA
| | - J Serna-Franco
- Instituto de F'isica, Universidad Nacional Autónoma de México, Ciudad de Mexico, Mexico
| | - A J Smith
- Department of Physics, University of Maryland, College Park, MD, USA
| | - Y Son
- University of Seoul, Seoul, Rep. of Korea
| | - R W Springer
- Department of Physics and Astronomy, University of Utah, Salt Lake City, UT, USA
| | - O Tibolla
- Universidad Politecnica de Pachuca, Pachuca, Hgo, Mexico
| | - K Tollefson
- Department of Physics and Astronomy, Michigan State University, East Lansing, MI, USA
| | - I Torres
- Instituto Nacional de Astrof'isica, Óptica y Electrónica, Puebla, Mexico
| | - R Torres-Escobedo
- Tsung-Dao Lee Institute & School of Physics and Astronomy, Shanghai Jiao Tong University, Shanghai, People's Republic of China
| | - R Turner
- Department of Physics, Michigan Technological University, Houghton, MI, USA
| | - F Ureña-Mena
- Instituto Nacional de Astrof'isica, Óptica y Electrónica, Puebla, Mexico
| | - E Varela
- Facultad de Ciencias F'isico Matemáticas, Benemérita Universidad Autónoma de Puebla, Puebla, Mexico
| | - L Villaseñor
- Facultad de Ciencias F'isico Matemáticas, Benemérita Universidad Autónoma de Puebla, Puebla, Mexico
| | - X Wang
- Department of Physics, Michigan Technological University, Houghton, MI, USA
| | - I J Watson
- University of Seoul, Seoul, Rep. of Korea
| | - E Willox
- Department of Physics, University of Maryland, College Park, MD, USA
| | - S Yun-Cárcamo
- Department of Physics, University of Maryland, College Park, MD, USA
| | - H Zhou
- Tsung-Dao Lee Institute & School of Physics and Astronomy, Shanghai Jiao Tong University, Shanghai, People's Republic of China
| | - C de León
- Universidad Michoacana de San Nicolás de Hidalgo, Morelia, Mexico
| | - J F Beacom
- Center for Cosmology and AstroParticle Physics (CCAPP), Ohio State University, Columbus, Ohio 43210, USA
- Department of Physics, Ohio State University, Columbus, Ohio 43210, USA
- Department of Astronomy, Ohio State University, Columbus, Ohio 43210, USA
| | - T Linden
- The Oskar Klein Centre, Department of Physics, Stockholm University, AlbaNova, SE-10691 Stockholm, Sweden
| | - K C Y Ng
- Department of Physics, The Chinese University of Hong Kong, Sha Tin, Hong Kong, China
| | - A H G Peter
- Center for Cosmology and AstroParticle Physics (CCAPP), Ohio State University, Columbus, Ohio 43210, USA
- Department of Physics, Ohio State University, Columbus, Ohio 43210, USA
- Department of Astronomy, Ohio State University, Columbus, Ohio 43210, USA
- School of Natural Sciences, Institute for Advanced Study, 1 Einstein Drive, Princeton, NJ 08540, USA
| | - B Zhou
- William H. Miller III Department of Physics and Astronomy, Johns Hopkins University, Baltimore, Maryland 21218, USA
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Lange P, Engel K, Schleid T. Cs 3La[AsS 4] 2: a caesium-containing lanthanum thioarsenate(V). Acta Cryst Sect A 2022. [DOI: 10.1107/s2053273322092117] [Citation(s) in RCA: 0] [Impact Index Per Article: 0] [Reference Citation Analysis] [What about the content of this article? (0)] [Track Full Text] [Subscribe] [Scholar Register] [Indexed: 03/19/2023]
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Pachowsky M, Morf H, Simon D, Schönau V, Valor L, Knitza J, Engel K, Uder M, Hueber A, Schett G, Kleyer A. OP0293 PHOTOREALISTIC DEPICTION OF RHEUMATIC PATHOLOGIES BY CINEMATIC RENDERING FACILITATES DISEASE UNDERSTANDING OF PATIENTS WITH RHEUMATIC DISEASES. Ann Rheum Dis 2022. [DOI: 10.1136/annrheumdis-2022-eular.1463] [Citation(s) in RCA: 0] [Impact Index Per Article: 0] [Reference Citation Analysis] [What about the content of this article? (0)] [Abstract] [Track Full Text] [Journal Information] [Subscribe] [Scholar Register] [Indexed: 11/04/2022]
Abstract
BackgroundTreatment success of a rheumatic disease crucially depends on whether a patient is sufficiently informed about the disease[1]. Visual methods are suitable for explaining diseases[2]. Cinematic rendering (CR) is a new method that allows to segment standard medical images into images that illustrate disease pathologies in a photorealistic way. As such, CR provides new opportunities to visualize diseases and but could therefore be a valuable tool for patients with rheumatic and musculoskeletal disease (RMD).[3]ObjectivesWe questioned, if it is possible to apply CR on images from structural lesions of patients with rheumatoid arthritis (RA), Psoriatic Arthritis (PsA) and axial Spondyloarthritis (axSpA) and to test whether such images are helpful to patients with RMDs to understand their disease process. application in doctor-patient communication.MethodsWe selected conventional computed tomography (CT) and high-resolution peripheral CT (HR-pQCT) from patients with rheumatoid arthritis (RA), Psoriatic Arthritis (PsA) and axial Spondyloarthritis (axSpA) that showed typical changes of the respective disease. HR-pQCT measurements were performed in RA and PsA at the Rheumatology Department. CT Measurements of the spine in an axSpA patient was provided from AH. All images were segmented to CR images using a prototype software by the manufacturer Siemens Healthineers. In a prospective study on consecutive patients with RA, PsA, axSpA these images were used to explain the depicted pathognomonic pathologies and compared to conventional imaging in a structured doctor-patient interview. In the last step, patients filled in a quantitative questionnaire (Likert Scale 1-5) about their perspectives answering following questions: Did you understand your disease in the provided Cinematic Rendering images? Did you understand your disease better through the presentation using Cinematic Rendering images than with a normal X-ray image? Do you think it would be reasonable to use this type of Cinematic Rendering to improve patients’ understanding of their disease? Descriptive statistical methods were used.ResultsCR images of rheumatic diseases were successfully generated from above mentioned imaging data (CT, HR-pQCT). Bone erosions, osteophytes, enthesiophytes, osteoporosis and ankylosis of the spine could be visualized in photorealistic detail. Figure 1 shows examples of a images of a patient with RA and axSpA with typical bone changes.65 patients (23 RA/23 PsA/19 axSpA; f 55%) were guided through CR images of their respective disease by an experienced rheumatologist, followed by completing the questionnaire mentioned above. Patients stated that CR was very helpful to understand their disease process (4.39±0.15), that understanding diseases by CR was better than the one obtained by conventional radiographs (4.43±0.20) and that they considered such technology helpful for improving disease understanding (4.35±0.09).ConclusionCR seems to be a promising teaching tool for RMD patients facilitating an improved understanding of their disease process and in consequence my also improve adherence of RMD patients to their anti-rheumatic treatment.References[1]Ritschl, V., et al., 2020 EULAR points to consider for the prevention, screening, assessment and management of non-adherence to treatment in people with rheumatic and musculoskeletal diseases for use in clinical practice. Ann Rheum Dis, 2020.[2]Kleyer, A., et al., Development of three-dimensional prints of arthritic joints for supporting patients’ awareness to structural damage. Arthritis Res Ther, 2017. 19(1): p. 34.[3]Berger, F., et al., Application of Cinematic Rendering in Clinical Routine CT Examination of Ankle Sprains. AJR Am J Roentgenol, 2018. 211(4): p. 887-890.AcknowledgementsSiemens Healthineers /Dr.Klaus Engel for providing CR expertiseDisclosure of InterestsNone declared
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Simon D, Tascilar K, Kleyer A, Bayat S, Kampylafka E, Hueber A, Rech J, Schuster L, Engel K, Sticherling M, Schett G. OP0051 STRUCTURAL ENTHESEAL LESIONS IN PSORIASIS PATIENTS ARE ASSOCIATED WITH AN INCREASED RISK OF PROGRESSION TO PSORIATIC ARTHRITIS - A PROSPECTIVE COHORT STUDY. Ann Rheum Dis 2020. [DOI: 10.1136/annrheumdis-2020-eular.1524] [Citation(s) in RCA: 3] [Impact Index Per Article: 0.8] [Reference Citation Analysis] [What about the content of this article? (0)] [Abstract] [Track Full Text] [Journal Information] [Subscribe] [Scholar Register] [Indexed: 11/04/2022]
Abstract
Background:We have previously reported that the presence of musculoskeletal pain in psoriasis patients is associated with a higher risk of developing psoriatic arthritis (PsA) (1). Furthermore, a subset of psoriasis patients shows evidence for structural entheseal lesions (SEL) in their hand joints (2), sometimes also referred as “Deep Koebner Phenomenon”, which are highly specific for psoriatic disease and virtually absent in healthy controls, rheumatoid arthritis and hand osteoarthritis patients (2-4). However, it remains unclear whether SEL alone or in combination with musculoskeletal pain are associated with the development of PsA.Objectives:To test whether the presence of SEL in psoriasis patients increases the risk for progression to PsA and how this is related to the presence of musculoskeletal pain.Methods:Psoriasis patients without evidence of PsA were enrolled in a prospective cohort study between 2011 and 2018. All patients underwent baseline assessment of SEL in their 2ndand 3rdMCP joints by high-resolution peripheral quantitative computed tomography (HR-pQCT). The risk of PsA development associated with SEL and arthralgia was explored using survival analyses and multivariable Cox regression models.Results:114 psoriasis patients (72 men/42 women) with a mean (SD) follow-up duration of 28.2 (17.7) months were included, 24 of whom developed PsA (9.7 /100 patient-years, 95%CI 6.2 to 14.5) during the observation period. Patients with SEL (N=41) were at higher risk of developing PsA compared to patients without such lesions (21.4/100 patient-years, 95%CI 12.5 to 34.3, HR 5.10, 95%CI 1.53 to 16.99, p=0.008) (Kaplan Meier plot A). Furthermore, while patients without arthralgia and without SEL had a very low progression rate to PsA (1/29; 3.4%), patients with arthralgia but no SEL showed higher progression (5/33; 15.2%), which was in line with previous observations (1) (Kaplan Meier plot B). Presence of SEL further enhanced the risk for progression to PsA both in the absence (6/16; 37.5%) and presence (6/14; 42.8%) of arthralgia with the highest progression rate in those subjects with both arthralgia and SEL (p<0.001 by log rank test for trend) (Kaplan Meier plot B).Conclusion:Presence of SEL is associated with an increased risk of developing PsA in patients with psoriasis. If used together with pain, SEL allow defining subsets of psoriasis patients with very low and very high risk to develop PsA.References:[1]Faustini F et al. Ann Rheum Dis. 2016;75:2068-2074[2]Simon D et al. Ann Rheum Dis. 2016;75:660-6[3]Finzel S et al. Ann Rheum Dis. 2011;70:122-7[4]Finzel S et al. Arthritis Rheum. 2011;63:1231-6Disclosure of Interests:David Simon Grant/research support from: Else Kröner-Memorial Scholarship, Novartis, Consultant of: Novartis, Lilly, Koray Tascilar: None declared, Arnd Kleyer Consultant of: Lilly, Gilead, Novartis,Abbvie, Speakers bureau: Novartis, Lilly, Sara Bayat Speakers bureau: Novartis, Eleni Kampylafka Speakers bureau: Novartis, BMS, Janssen, Axel Hueber Grant/research support from: Novartis, Lilly, Pfizer, Consultant of: Abbvie, BMS, Celgene, Gilead, GSK, Lilly, Novartis, Speakers bureau: GSK, Lilly, Novartis, Jürgen Rech Consultant of: BMS, Celgene, Novartis, Roche, Chugai, Speakers bureau: AbbVie, Biogen, BMS, Celgene, MSD, Novartis, Roche, Chugai, Pfizer, Lilly, Louis Schuster: None declared, Klaus Engel: None declared, Michael Sticherling Grant/research support from: Novartis, Consultant of: Advisory boards Abbvie, Celgene, Janssen Cilag, Lilly, Pfizer, MSD, Novartis, Amgen, Leo, Sanofi, UCB, Speakers bureau: Abbvie, Celgene, Janssen Cilag, Leo, MSD, Novartis, Pfizer, Georg Schett Speakers bureau: AbbVie, BMS, Celgene, Janssen, Eli Lilly, Novartis, Roche and UCB
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Albert A, Alfaro R, Alvarez C, Angeles Camacho JR, Arteaga-Velázquez JC, Arunbabu KP, Avila Rojas D, Ayala Solares HA, Baghmanyan V, Belmont-Moreno E, BenZvi SY, Brisbois C, Caballero-Mora KS, Capistrán T, Carramiñana A, Casanova S, Cotti U, Cotzomi J, Coutiño de León S, De la Fuente E, de León C, Dingus BL, DuVernois MA, Díaz-Vélez JC, Ellsworth RW, Engel K, Espinoza C, Fleischhack H, Fraija N, Galván-Gámez A, Garcia D, García-González JA, Garfias F, González MM, Goodman JA, Harding JP, Hernandez S, Hona B, Huang D, Hueyotl-Zahuantitla F, Hüntemeyer P, Iriarte A, Joshi V, Lara A, Lee WH, León Vargas H, Linnemann JT, Longinotti AL, Luis-Raya G, Lundeen J, López-Coto R, Malone K, Marinelli SS, Martinez-Castellanos I, Martínez-Castro J, Martínez-Huerta H, Matthews JA, Miranda-Romagnoli P, Morales-Soto JA, Moreno E, Nayerhoda A, Nellen L, Newbold M, Nisa MU, Noriega-Papaqui R, Omodei N, Peisker A, Pérez-Pérez EG, Rho CD, Rivière C, Rosa-González D, Rosenberg M, Ruiz-Velasco E, Salazar H, Salesa Greus F, Sandoval A, Schneider M, Schoorlemmer H, Sinnis G, Smith AJ, Springer RW, Surajbali P, Tabachnick E, Tanner M, Tibolla O, Tollefson K, Torres I, Torres-Escobedo R, Weisgarber T, Yodh G, Zepeda A, Zhou H. Constraints on Lorentz Invariance Violation from HAWC Observations of Gamma Rays above 100 TeV. Phys Rev Lett 2020; 124:131101. [PMID: 32302173 DOI: 10.1103/physrevlett.124.131101] [Citation(s) in RCA: 9] [Impact Index Per Article: 2.3] [Reference Citation Analysis] [What about the content of this article? (0)] [Affiliation(s)] [Abstract] [Track Full Text] [Subscribe] [Scholar Register] [Received: 11/18/2019] [Revised: 02/07/2020] [Accepted: 03/04/2020] [Indexed: 06/11/2023]
Abstract
Because of the high energies and long distances to the sources, astrophysical observations provide a unique opportunity to test possible signatures of Lorentz invariance violation (LIV). Superluminal LIV enables the decay of photons at high energy. The high altitude water Cherenkov (HAWC) observatory is among the most sensitive gamma-ray instruments currently operating above 10 TeV. HAWC finds evidence of 100 TeV photon emission from at least four astrophysical sources. These observations exclude, for the strongest of the limits set, the LIV energy scale to 2.2×10^{31} eV, over 1800 times the Planck energy and an improvement of 1 to 2 orders of magnitude over previous limits.
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Affiliation(s)
- A Albert
- Physics Division, Los Alamos National Laboratory, Los Alamos, New Mexico 87545, USA
| | - R Alfaro
- Instituto de Física, Universidad Nacional Autónoma de México, Ciudad de Mexico 04510, Mexico
| | - C Alvarez
- Universidad Autónoma de Chiapas, Tuxtla Gutiérrez, Chiapas 29050, Mexico
| | - J R Angeles Camacho
- Instituto de Física, Universidad Nacional Autónoma de México, Ciudad de Mexico 04510, Mexico
| | | | - K P Arunbabu
- Instituto de Geofísica, Universidad Nacional Autónoma de México, Ciudad de Mexico 04510, Mexico
| | - D Avila Rojas
- Instituto de Física, Universidad Nacional Autónoma de México, Ciudad de Mexico 04510, Mexico
| | - H A Ayala Solares
- Department of Physics, Pennsylvania State University, University Park, Pennsylvania 16802, USA
| | - V Baghmanyan
- Institute of Nuclear Physics Polish Academy of Sciences, PL-31342 IFJ-PAN, Krakow 31342, Poland
| | - E Belmont-Moreno
- Instituto de Física, Universidad Nacional Autónoma de México, Ciudad de Mexico 04510, Mexico
| | - S Y BenZvi
- Department of Physics & Astronomy, University of Rochester, Rochester, New York 14627, USA
| | - C Brisbois
- Department of Physics, Michigan Technological University, Houghton, Michigan 49931-1295, USA
| | - K S Caballero-Mora
- Universidad Autónoma de Chiapas, Tuxtla Gutiérrez, Chiapas 29050, Mexico
| | - T Capistrán
- Instituto Nacional de Astrofísica, Óptica y Electrónica, Puebla 72840, Mexico
| | - A Carramiñana
- Instituto Nacional de Astrofísica, Óptica y Electrónica, Puebla 72840, Mexico
| | - S Casanova
- Institute of Nuclear Physics Polish Academy of Sciences, PL-31342 IFJ-PAN, Krakow 31342, Poland
| | - U Cotti
- Universidad Michoacana de San Nicolás de Hidalgo, Morelia 58040, Mexico
| | - J Cotzomi
- Facultad de Ciencias Físico Matemáticas, Benemérita Universidad Autónoma de Puebla, Puebla 72570, Mexico
| | - S Coutiño de León
- Instituto Nacional de Astrofísica, Óptica y Electrónica, Puebla 72840, Mexico
| | - E De la Fuente
- Departamento de Física, CUCEI, Universidad de Guadalajara, Guadalajara 44430, Mexico
| | - C de León
- Universidad Michoacana de San Nicolás de Hidalgo, Morelia 58040, Mexico
| | - B L Dingus
- Physics Division, Los Alamos National Laboratory, Los Alamos, New Mexico 87545, USA
| | - M A DuVernois
- Department of Physics, University of Wisconsin-Madison, Madison, Wisconsin 53706, USA
| | - J C Díaz-Vélez
- Departamento de Física, Centro Universitario de los Valles, Universidad de Guadalajara, Guadalajara 46600, Mexico
| | - R W Ellsworth
- Department of Physics, University of Maryland, College Park, Maryland 20742-4111, USA
| | - K Engel
- Department of Physics, University of Maryland, College Park, Maryland 20742-4111, USA
| | - C Espinoza
- Instituto de Física, Universidad Nacional Autónoma de México, Ciudad de Mexico 04510, Mexico
| | - H Fleischhack
- Department of Physics, Michigan Technological University, Houghton, Michigan 49931-1295, USA
| | - N Fraija
- Instituto de Astronomía, Universidad Nacional Autónoma de México, Ciudad de Mexico 04510, Mexico
| | - A Galván-Gámez
- Instituto de Astronomía, Universidad Nacional Autónoma de México, Ciudad de Mexico 04510, Mexico
| | - D Garcia
- Instituto de Física, Universidad Nacional Autónoma de México, Ciudad de Mexico 04510, Mexico
| | - J A García-González
- Instituto de Física, Universidad Nacional Autónoma de México, Ciudad de Mexico 04510, Mexico
| | - F Garfias
- Instituto de Astronomía, Universidad Nacional Autónoma de México, Ciudad de Mexico 04510, Mexico
| | - M M González
- Instituto de Astronomía, Universidad Nacional Autónoma de México, Ciudad de Mexico 04510, Mexico
| | - J A Goodman
- Department of Physics, University of Maryland, College Park, Maryland 20742-4111, USA
| | - J P Harding
- Physics Division, Los Alamos National Laboratory, Los Alamos, New Mexico 87545, USA
| | - S Hernandez
- Instituto de Física, Universidad Nacional Autónoma de México, Ciudad de Mexico 04510, Mexico
| | - B Hona
- Department of Physics, Michigan Technological University, Houghton, Michigan 49931-1295, USA
| | - D Huang
- Department of Physics, Michigan Technological University, Houghton, Michigan 49931-1295, USA
| | | | - P Hüntemeyer
- Department of Physics, Michigan Technological University, Houghton, Michigan 49931-1295, USA
| | - A Iriarte
- Instituto de Astronomía, Universidad Nacional Autónoma de México, Ciudad de Mexico 04510, Mexico
| | - V Joshi
- Erlangen Centre for Astroparticle Physics, Friedrich-Alexander-Universität Erlangen-Nürnberg, 91058 Erlangen, Germany
| | - A Lara
- Instituto de Geofísica, Universidad Nacional Autónoma de México, Ciudad de Mexico 04510, Mexico
| | - W H Lee
- Instituto de Astronomía, Universidad Nacional Autónoma de México, Ciudad de Mexico 04510, Mexico
| | - H León Vargas
- Instituto de Física, Universidad Nacional Autónoma de México, Ciudad de Mexico 04510, Mexico
| | - J T Linnemann
- Department of Physics and Astronomy, Michigan State University, East Lansing, Michigan 48824, USA
| | - A L Longinotti
- Instituto Nacional de Astrofísica, Óptica y Electrónica, Puebla 72840, Mexico
| | - G Luis-Raya
- Universidad Politecnica de Pachuca, Pachuca, Hgo 42083, Mexico
| | - J Lundeen
- Department of Physics and Astronomy, Michigan State University, East Lansing, Michigan 48824, USA
| | - R López-Coto
- INFN and Universita di Padova, via Marzolo 8, I-35131, Padova, Italy
| | - K Malone
- Physics Division, Los Alamos National Laboratory, Los Alamos, New Mexico 87545, USA
| | - S S Marinelli
- Department of Physics and Astronomy, Michigan State University, East Lansing, Michigan 48824, USA
| | | | - J Martínez-Castro
- Centro de Investigación en Computación, Instituto Politécnico Nacional, México City 07738, Mexico
| | - H Martínez-Huerta
- Instituto de Física de São Carlos, Universidade de São Paulo, São Carlos, Sao Paolo 13566-590, Brasil
| | - J A Matthews
- Dept of Physics and Astronomy, University of New Mexico, Albuquerque, New Mexico 87131, USA
| | | | - J A Morales-Soto
- Universidad Michoacana de San Nicolás de Hidalgo, Morelia 58040, Mexico
| | - E Moreno
- Facultad de Ciencias Físico Matemáticas, Benemérita Universidad Autónoma de Puebla, Puebla 72570, Mexico
| | - A Nayerhoda
- Institute of Nuclear Physics Polish Academy of Sciences, PL-31342 IFJ-PAN, Krakow 31342, Poland
| | - L Nellen
- Instituto de Ciencias Nucleares, Universidad Nacional Autónoma de Mexico, Ciudad de Mexico 04510, Mexico
| | - M Newbold
- Department of Physics and Astronomy, University of Utah, Salt Lake City, Utah 84112, USA
| | - M U Nisa
- Department of Physics and Astronomy, Michigan State University, East Lansing, Michigan 48824, USA
| | | | - N Omodei
- Stanford University, Stanford, California 94305, USA
| | - A Peisker
- Department of Physics and Astronomy, Michigan State University, East Lansing, Michigan 48824, USA
| | - E G Pérez-Pérez
- Universidad Politecnica de Pachuca, Pachuca, Hgo 42083, Mexico
| | - C D Rho
- Department of Physics & Astronomy, University of Rochester, Rochester, New York 14627, USA
| | - C Rivière
- Department of Physics, University of Maryland, College Park, Maryland 20742-4111, USA
| | - D Rosa-González
- Instituto Nacional de Astrofísica, Óptica y Electrónica, Puebla 72840, Mexico
| | - M Rosenberg
- Department of Physics, Pennsylvania State University, University Park, Pennsylvania 16802, USA
| | - E Ruiz-Velasco
- Max-Planck Institute for Nuclear Physics, 69117 Heidelberg, Germany
| | - H Salazar
- Facultad de Ciencias Físico Matemáticas, Benemérita Universidad Autónoma de Puebla, Puebla 72570, Mexico
| | - F Salesa Greus
- Institute of Nuclear Physics Polish Academy of Sciences, PL-31342 IFJ-PAN, Krakow 31342, Poland
| | - A Sandoval
- Instituto de Física, Universidad Nacional Autónoma de México, Ciudad de Mexico 04510, Mexico
| | - M Schneider
- Department of Physics, University of Maryland, College Park, Maryland 20742-4111, USA
| | - H Schoorlemmer
- Max-Planck Institute for Nuclear Physics, 69117 Heidelberg, Germany
| | - G Sinnis
- Physics Division, Los Alamos National Laboratory, Los Alamos, New Mexico 87545, USA
| | - A J Smith
- Department of Physics, University of Maryland, College Park, Maryland 20742-4111, USA
| | - R W Springer
- Department of Physics and Astronomy, University of Utah, Salt Lake City, Utah 84112, USA
| | - P Surajbali
- Max-Planck Institute for Nuclear Physics, 69117 Heidelberg, Germany
| | - E Tabachnick
- Department of Physics, University of Maryland, College Park, Maryland 20742-4111, USA
| | - M Tanner
- Department of Physics, Pennsylvania State University, University Park, Pennsylvania 16802, USA
| | - O Tibolla
- Universidad Politecnica de Pachuca, Pachuca, Hgo 42083, Mexico
| | - K Tollefson
- Department of Physics and Astronomy, Michigan State University, East Lansing, Michigan 48824, USA
| | - I Torres
- Instituto Nacional de Astrofísica, Óptica y Electrónica, Puebla 72840, Mexico
| | - R Torres-Escobedo
- Departamento de Física, CUCEI, Universidad de Guadalajara, Guadalajara 44430, Mexico
- Department of Physics and Astronomy, Texas Tech University, Lubbock, Texas 79409-1051, USA
| | - T Weisgarber
- Department of Physics, University of Wisconsin-Madison, Madison, Wisconsin 53706, USA
| | - G Yodh
- Department of Physics and Astronomy, University of California, Irvine, Irvine, California 92697, USA
| | - A Zepeda
- Physics Department, Centro de Investigacion y de Estudios Avanzados del IPN, Mexico City 07360, Mexico
| | - H Zhou
- Physics Division, Los Alamos National Laboratory, Los Alamos, New Mexico 87545, USA
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9
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Abeysekara AU, Albert A, Alfaro R, Angeles Camacho JR, Arteaga-Velázquez JC, Arunbabu KP, Avila Rojas D, Ayala Solares HA, Baghmanyan V, Belmont-Moreno E, BenZvi SY, Brisbois C, Caballero-Mora KS, Capistrán T, Carramiñana A, Casanova S, Cotti U, Cotzomi J, Coutiño de León S, De la Fuente E, de León C, Dichiara S, Dingus BL, DuVernois MA, Díaz-Vélez JC, Ellsworth RW, Engel K, Espinoza C, Fleischhack H, Fraija N, Galván-Gámez A, Garcia D, García-González JA, Garfias F, González MM, Goodman JA, Harding JP, Hernandez S, Hinton J, Hona B, Huang D, Hueyotl-Zahuantitla F, Hüntemeyer P, Iriarte A, Jardin-Blicq A, Joshi V, Kaufmann S, Kieda D, Lara A, Lee WH, León Vargas H, Linnemann JT, Longinotti AL, Luis-Raya G, Lundeen J, López-Coto R, Malone K, Marinelli SS, Martinez O, Martinez-Castellanos I, Martínez-Castro J, Martínez-Huerta H, Matthews JA, Miranda-Romagnoli P, Morales-Soto JA, Moreno E, Mostafá M, Nayerhoda A, Nellen L, Newbold M, Nisa MU, Noriega-Papaqui R, Peisker A, Pérez-Pérez EG, Pretz J, Ren Z, Rho CD, Rivière C, Rosa-González D, Rosenberg M, Ruiz-Velasco E, Salesa Greus F, Sandoval A, Schneider M, Schoorlemmer H, Sinnis G, Smith AJ, Springer RW, Surajbali P, Tabachnick E, Tanner M, Tibolla O, Tollefson K, Torres I, Torres-Escobedo R, Villaseñor L, Weisgarber T, Wood J, Yapici T, Zhang H, Zhou H. Multiple Galactic Sources with Emission Above 56 TeV Detected by HAWC. Phys Rev Lett 2020; 124:021102. [PMID: 32004015 DOI: 10.1103/physrevlett.124.021102] [Citation(s) in RCA: 7] [Impact Index Per Article: 1.8] [Reference Citation Analysis] [What about the content of this article? (0)] [Affiliation(s)] [Abstract] [Track Full Text] [Subscribe] [Scholar Register] [Received: 09/18/2019] [Revised: 11/21/2019] [Indexed: 06/10/2023]
Abstract
We present the first catalog of gamma-ray sources emitting above 56 and 100 TeV with data from the High Altitude Water Cherenkov Observatory, a wide field-of-view observatory capable of detecting gamma rays up to a few hundred TeV. Nine sources are observed above 56 TeV, all of which are likely galactic in origin. Three sources continue emitting past 100 TeV, making this the highest-energy gamma-ray source catalog to date. We report the integral flux of each of these objects. We also report spectra for three highest-energy sources and discuss the possibility that they are PeVatrons.
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Affiliation(s)
- A U Abeysekara
- Department of Physics and Astronomy, University of Utah, Salt Lake City, Utah, USA
| | - A Albert
- Physics Division, Los Alamos National Laboratory, Los Alamos, New Mexico, USA
| | - R Alfaro
- Instituto de Física, Universidad Nacional Autónoma de México, Ciudad de Mexico, Mexico
| | - J R Angeles Camacho
- Instituto de Física, Universidad Nacional Autónoma de México, Ciudad de Mexico, Mexico
| | | | - K P Arunbabu
- Instituto de Geofísica, Universidad Nacional Autónoma de México, Ciudad de Mexico, Mexico
| | - D Avila Rojas
- Instituto de Física, Universidad Nacional Autónoma de México, Ciudad de Mexico, Mexico
| | - H A Ayala Solares
- Department of Physics, Pennsylvania State University, University Park, Pennsylvania, USA
| | - V Baghmanyan
- Institute of Nuclear Physics Polish Academy of Sciences, IFJ-PAN, Krakow, Poland
| | - E Belmont-Moreno
- Instituto de Física, Universidad Nacional Autónoma de México, Ciudad de Mexico, Mexico
| | - S Y BenZvi
- Department of Physics & Astronomy, University of Rochester, Rochester, New York, USA
| | - C Brisbois
- Department of Physics, University of Maryland, College Park, Maryland, USA
| | | | - T Capistrán
- Instituto Nacional de Astrofísica, Óptica y Electrónica, Puebla, Mexico
| | - A Carramiñana
- Instituto Nacional de Astrofísica, Óptica y Electrónica, Puebla, Mexico
| | - S Casanova
- Institute of Nuclear Physics Polish Academy of Sciences, IFJ-PAN, Krakow, Poland
| | - U Cotti
- Universidad Michoacana de San Nicolás de Hidalgo, Morelia, Mexico
| | - J Cotzomi
- Facultad de Ciencias Físico Matemáticas, Benemérita Universidad Autónoma de Puebla, Puebla, Mexico
| | - S Coutiño de León
- Instituto Nacional de Astrofísica, Óptica y Electrónica, Puebla, Mexico
| | - E De la Fuente
- Departamento de Física, Centro Universitario de Ciencias Exactase Ingenierias, Universidad de Guadalajara, Guadalajara, Mexico
- Department of Physics and Astronomy, Texas Tech University, Lubbock, Texas, USA
| | - C de León
- Universidad Michoacana de San Nicolás de Hidalgo, Morelia, Mexico
| | - S Dichiara
- Instituto de Astronomía, Universidad Nacional Autónoma de México, Ciudad de Mexico, Mexico
| | - B L Dingus
- Physics Division, Los Alamos National Laboratory, Los Alamos, New Mexico, USA
| | - M A DuVernois
- Department of Physics, University of Wisconsin-Madison, Madison, Wisconsin, USA
| | - J C Díaz-Vélez
- Departamento de Física, Centro Universitario de Ciencias Exactase Ingenierias, Universidad de Guadalajara, Guadalajara, Mexico
- Department of Physics and Astronomy, Texas Tech University, Lubbock, Texas, USA
| | - R W Ellsworth
- Department of Physics, University of Maryland, College Park, Maryland, USA
| | - K Engel
- Department of Physics, University of Maryland, College Park, Maryland, USA
| | - C Espinoza
- Instituto de Física, Universidad Nacional Autónoma de México, Ciudad de Mexico, Mexico
| | - H Fleischhack
- Department of Physics, Michigan Technological University, Houghton, Michigan, USA
| | - N Fraija
- Instituto de Astronomía, Universidad Nacional Autónoma de México, Ciudad de Mexico, Mexico
| | - A Galván-Gámez
- Instituto de Astronomía, Universidad Nacional Autónoma de México, Ciudad de Mexico, Mexico
| | - D Garcia
- Instituto de Física, Universidad Nacional Autónoma de México, Ciudad de Mexico, Mexico
| | - J A García-González
- Instituto de Física, Universidad Nacional Autónoma de México, Ciudad de Mexico, Mexico
| | - F Garfias
- Instituto de Astronomía, Universidad Nacional Autónoma de México, Ciudad de Mexico, Mexico
| | - M M González
- Instituto de Astronomía, Universidad Nacional Autónoma de México, Ciudad de Mexico, Mexico
| | - J A Goodman
- Department of Physics, University of Maryland, College Park, Maryland, USA
| | - J P Harding
- Physics Division, Los Alamos National Laboratory, Los Alamos, New Mexico, USA
| | - S Hernandez
- Instituto de Física, Universidad Nacional Autónoma de México, Ciudad de Mexico, Mexico
| | - J Hinton
- Max-Planck Institute for Nuclear Physics, Heidelberg, Germany
| | - B Hona
- Department of Physics, Michigan Technological University, Houghton, Michigan, USA
| | - D Huang
- Department of Physics, Michigan Technological University, Houghton, Michigan, USA
| | | | - P Hüntemeyer
- Department of Physics, Michigan Technological University, Houghton, Michigan, USA
| | - A Iriarte
- Instituto de Astronomía, Universidad Nacional Autónoma de México, Ciudad de Mexico, Mexico
| | - A Jardin-Blicq
- Max-Planck Institute for Nuclear Physics, Heidelberg, Germany
| | - V Joshi
- Erlangen Centre for Astroparticle Physics, Friedrich-Alexander-Universität Erlangen-Nürnberg, Erlangen, Germany
| | - S Kaufmann
- Universidad Politecnica de Pachuca, Pachuca, Hgo, Mexico
| | - D Kieda
- Department of Physics and Astronomy, University of Utah, Salt Lake City, Utah, USA
| | - A Lara
- Instituto de Geofísica, Universidad Nacional Autónoma de México, Ciudad de Mexico, Mexico
| | - W H Lee
- Instituto de Astronomía, Universidad Nacional Autónoma de México, Ciudad de Mexico, Mexico
| | - H León Vargas
- Instituto de Física, Universidad Nacional Autónoma de México, Ciudad de Mexico, Mexico
| | - J T Linnemann
- Department of Physics and Astronomy, Michigan State University, East Lansing, Michigan, USA
| | - A L Longinotti
- Instituto Nacional de Astrofísica, Óptica y Electrónica, Puebla, Mexico
| | - G Luis-Raya
- Universidad Politecnica de Pachuca, Pachuca, Hgo, Mexico
| | - J Lundeen
- Department of Physics and Astronomy, Michigan State University, East Lansing, Michigan, USA
| | - R López-Coto
- INFN and Universita di Padova, via Marzolo 8, Padova, Italy
| | - K Malone
- Physics Division, Los Alamos National Laboratory, Los Alamos, New Mexico, USA
- Department of Physics, Pennsylvania State University, University Park, Pennsylvania, USA
| | - S S Marinelli
- Department of Physics and Astronomy, Michigan State University, East Lansing, Michigan, USA
| | - O Martinez
- Facultad de Ciencias Físico Matemáticas, Benemérita Universidad Autónoma de Puebla, Puebla, Mexico
| | | | - J Martínez-Castro
- Centro de Investigación en Computación, Instituto Politécnico Nacional, México City, México
| | - H Martínez-Huerta
- Instituto de Física de São Carlos, Universidade de São Paulo, São Carlos, São Paulo, Brasil
| | - J A Matthews
- Dept of Physics and Astronomy, University of New Mexico, Albuquerque, New Mexico, USA
| | | | - J A Morales-Soto
- Universidad Michoacana de San Nicolás de Hidalgo, Morelia, Mexico
| | - E Moreno
- Facultad de Ciencias Físico Matemáticas, Benemérita Universidad Autónoma de Puebla, Puebla, Mexico
| | - M Mostafá
- Department of Physics, Pennsylvania State University, University Park, Pennsylvania, USA
| | - A Nayerhoda
- Institute of Nuclear Physics Polish Academy of Sciences, IFJ-PAN, Krakow, Poland
| | - L Nellen
- Instituto de Ciencias Nucleares, Universidad Nacional Autónoma de Mexico, Ciudad de Mexico, Mexico
| | - M Newbold
- Department of Physics and Astronomy, University of Utah, Salt Lake City, Utah, USA
| | - M U Nisa
- Department of Physics and Astronomy, Michigan State University, East Lansing, Michigan, USA
| | | | - A Peisker
- Department of Physics and Astronomy, Michigan State University, East Lansing, Michigan, USA
| | | | - J Pretz
- Department of Physics, Pennsylvania State University, University Park, Pennsylvania, USA
| | - Z Ren
- Dept of Physics and Astronomy, University of New Mexico, Albuquerque, New Mexico, USA
| | - C D Rho
- Department of Physics & Astronomy, University of Rochester, Rochester, New York, USA
| | - C Rivière
- Department of Physics, University of Maryland, College Park, Maryland, USA
| | - D Rosa-González
- Instituto Nacional de Astrofísica, Óptica y Electrónica, Puebla, Mexico
| | - M Rosenberg
- Department of Physics, Pennsylvania State University, University Park, Pennsylvania, USA
| | - E Ruiz-Velasco
- Max-Planck Institute for Nuclear Physics, Heidelberg, Germany
| | - F Salesa Greus
- Institute of Nuclear Physics Polish Academy of Sciences, IFJ-PAN, Krakow, Poland
| | - A Sandoval
- Instituto de Física, Universidad Nacional Autónoma de México, Ciudad de Mexico, Mexico
| | - M Schneider
- Department of Physics, University of Maryland, College Park, Maryland, USA
| | - H Schoorlemmer
- Max-Planck Institute for Nuclear Physics, Heidelberg, Germany
| | - G Sinnis
- Physics Division, Los Alamos National Laboratory, Los Alamos, New Mexico, USA
| | - A J Smith
- Department of Physics, University of Maryland, College Park, Maryland, USA
| | - R W Springer
- Department of Physics and Astronomy, University of Utah, Salt Lake City, Utah, USA
| | - P Surajbali
- Max-Planck Institute for Nuclear Physics, Heidelberg, Germany
| | - E Tabachnick
- Department of Physics, University of Maryland, College Park, Maryland, USA
| | - M Tanner
- Department of Physics, Pennsylvania State University, University Park, Pennsylvania, USA
| | - O Tibolla
- Universidad Politecnica de Pachuca, Pachuca, Hgo, Mexico
| | - K Tollefson
- Department of Physics and Astronomy, Michigan State University, East Lansing, Michigan, USA
| | - I Torres
- Instituto Nacional de Astrofísica, Óptica y Electrónica, Puebla, Mexico
| | - R Torres-Escobedo
- Departamento de Física, Centro Universitario de Ciencias Exactase Ingenierias, Universidad de Guadalajara, Guadalajara, Mexico
- Department of Physics and Astronomy, Texas Tech University, Lubbock, Texas, USA
| | - L Villaseñor
- Facultad de Ciencias Físico Matemáticas, Benemérita Universidad Autónoma de Puebla, Puebla, Mexico
| | - T Weisgarber
- Department of Physics, University of Wisconsin-Madison, Madison, Wisconsin, USA
| | - J Wood
- NASA Marshall Space Flight Center, Hunstville, Alabama, USA
| | - T Yapici
- Department of Physics & Astronomy, University of Rochester, Rochester, New York, USA
| | - H Zhang
- Department of Physics and Astronomy, Purdue University, West Lafayette, Indiana, USA
| | - H Zhou
- Physics Division, Los Alamos National Laboratory, Los Alamos, New Mexico, USA
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Abeysekara AU, Albert A, Alfaro R, Alvarez C, Álvarez JD, Arceo R, Arteaga-Velázquez JC, Avila Rojas D, Ayala Solares HA, Belmont-Moreno E, BenZvi SY, Brisbois C, Caballero-Mora KS, Capistrán T, Carramiñana A, Casanova S, Castillo M, Cotti U, Cotzomi J, Coutiño de León S, De León C, De la Fuente E, Díaz-Vélez JC, Dichiara S, Dingus BL, DuVernois MA, Ellsworth RW, Engel K, Espinoza C, Fang K, Fleischhack H, Fraija N, Galván-Gámez A, García-González JA, Garfias F, González-Muñoz A, González MM, Goodman JA, Hampel-Arias Z, Harding JP, Hernandez S, Hinton J, Hona B, Hueyotl-Zahuantitla F, Hui CM, Hüntemeyer P, Iriarte A, Jardin-Blicq A, Joshi V, Kaufmann S, Kar P, Kunde GJ, Lauer RJ, Lee WH, León Vargas H, Li H, Linnemann JT, Longinotti AL, Luis-Raya G, López-Coto R, Malone K, Marinelli SS, Martinez O, Martinez-Castellanos I, Martínez-Castro J, Matthews JA, Miranda-Romagnoli P, Moreno E, Mostafá M, Nayerhoda A, Nellen L, Newbold M, Nisa MU, Noriega-Papaqui R, Pretz J, Pérez-Pérez EG, Ren Z, Rho CD, Rivière C, Rosa-González D, Rosenberg M, Ruiz-Velasco E, Salesa Greus F, Sandoval A, Schneider M, Schoorlemmer H, Seglar Arroyo M, Sinnis G, Smith AJ, Springer RW, Surajbali P, Taboada I, Tibolla O, Tollefson K, Torres I, Vianello G, Villaseñor L, Weisgarber T, Werner F, Westerhoff S, Wood J, Yapici T, Yodh G, Zepeda A, Zhang H, Zhou H. Publisher Correction: Very-high-energy particle acceleration powered by the jets of the microquasar SS 433. Nature 2018; 564:E38. [PMID: 30482938 DOI: 10.1038/s41586-018-0688-8] [Citation(s) in RCA: 2] [Impact Index Per Article: 0.3] [Reference Citation Analysis] [What about the content of this article? (0)] [Affiliation(s)] [Abstract] [Track Full Text] [Journal Information] [Subscribe] [Scholar Register] [Indexed: 11/09/2022]
Abstract
In this Letter, owing to a production error, the penultimate version of the PDF was published. The HTML version was always correct. The PDF has been corrected online.
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Affiliation(s)
- A U Abeysekara
- Department of Physics and Astronomy, University of Utah, Salt Lake City, UT, USA
| | - A Albert
- Physics and Theoretical Divisions, Los Alamos National Laboratory, Los Alamos, NM, USA
| | - R Alfaro
- Instituto de Física, Universidad Nacional Autónoma de México, Mexico City, Mexico
| | - C Alvarez
- Universidad Autónoma de Chiapas, Tuxtla Gutiérrez, Mexico
| | - J D Álvarez
- Universidad Michoacana de San Nicolás de Hidalgo, Morelia, Mexico
| | - R Arceo
- Universidad Autónoma de Chiapas, Tuxtla Gutiérrez, Mexico
| | | | - D Avila Rojas
- Instituto de Física, Universidad Nacional Autónoma de México, Mexico City, Mexico
| | - H A Ayala Solares
- Department of Physics, Pennsylvania State University, University Park, PA, USA
| | - E Belmont-Moreno
- Instituto de Física, Universidad Nacional Autónoma de México, Mexico City, Mexico
| | - S Y BenZvi
- Department of Physics and Astronomy, University of Rochester, Rochester, NY, USA
| | - C Brisbois
- Department of Physics, Michigan Technological University, Houghton, MI, USA
| | | | - T Capistrán
- Instituto Nacional de Astrofísica, Óptica y Electrónica, Puebla, Mexico
| | - A Carramiñana
- Instituto Nacional de Astrofísica, Óptica y Electrónica, Puebla, Mexico
| | - S Casanova
- Institute of Nuclear Physics Polish Academy of Sciences, IFJ-PAN, Krakow, Poland.,Max-Planck Institute for Nuclear Physics, Heidelberg, Germany
| | - M Castillo
- Universidad Michoacana de San Nicolás de Hidalgo, Morelia, Mexico
| | - U Cotti
- Universidad Michoacana de San Nicolás de Hidalgo, Morelia, Mexico
| | - J Cotzomi
- Facultad de Ciencias Físico Matemáticas, Benemérita Universidad Autónoma de Puebla, Puebla, Mexico
| | - S Coutiño de León
- Instituto Nacional de Astrofísica, Óptica y Electrónica, Puebla, Mexico
| | - C De León
- Facultad de Ciencias Físico Matemáticas, Benemérita Universidad Autónoma de Puebla, Puebla, Mexico
| | - E De la Fuente
- Departamento de Física, Centro Universitario de Ciencias Exactas e Ingenierías, Universidad de Guadalajara, Guadalajara, Mexico
| | - J C Díaz-Vélez
- Departamento de Física, Centro Universitario de Ciencias Exactas e Ingenierías, Universidad de Guadalajara, Guadalajara, Mexico.,Department of Physics and Wisconsin IceCube Particle Astrophysics Center, University of Wisconsin-Madison, Madison, WI, USA
| | - S Dichiara
- Instituto de Astronomía, Universidad Nacional Autónoma de México, Mexico City, Mexico
| | - B L Dingus
- Physics and Theoretical Divisions, Los Alamos National Laboratory, Los Alamos, NM, USA
| | - M A DuVernois
- Department of Physics and Wisconsin IceCube Particle Astrophysics Center, University of Wisconsin-Madison, Madison, WI, USA
| | - R W Ellsworth
- School of Physics, Astronomy, and Computational Sciences, George Mason University, Fairfax, VA, USA
| | - K Engel
- Department of Physics, University of Maryland, College Park, MD, USA
| | - C Espinoza
- Instituto de Física, Universidad Nacional Autónoma de México, Mexico City, Mexico
| | - K Fang
- Department of Astronomy, University of Maryland, College Park, MD, USA.,Joint Space-Science Institute, University of Maryland, College Park, MD, USA
| | - H Fleischhack
- Department of Physics, Michigan Technological University, Houghton, MI, USA
| | - N Fraija
- Instituto de Astronomía, Universidad Nacional Autónoma de México, Mexico City, Mexico
| | - A Galván-Gámez
- Instituto de Astronomía, Universidad Nacional Autónoma de México, Mexico City, Mexico
| | - J A García-González
- Instituto de Física, Universidad Nacional Autónoma de México, Mexico City, Mexico
| | - F Garfias
- Instituto de Astronomía, Universidad Nacional Autónoma de México, Mexico City, Mexico
| | - A González-Muñoz
- Departamento de Física, Centro Universitario de Ciencias Exactas e Ingenierías, Universidad de Guadalajara, Guadalajara, Mexico
| | - M M González
- Instituto de Astronomía, Universidad Nacional Autónoma de México, Mexico City, Mexico
| | - J A Goodman
- Department of Physics, University of Maryland, College Park, MD, USA
| | - Z Hampel-Arias
- Department of Physics and Wisconsin IceCube Particle Astrophysics Center, University of Wisconsin-Madison, Madison, WI, USA.,Inter-university Institute for High Energies, Université Libre de Bruxelles, Brussels, Belgium
| | - J P Harding
- Physics and Theoretical Divisions, Los Alamos National Laboratory, Los Alamos, NM, USA
| | - S Hernandez
- Instituto de Física, Universidad Nacional Autónoma de México, Mexico City, Mexico
| | - J Hinton
- Max-Planck Institute for Nuclear Physics, Heidelberg, Germany
| | - B Hona
- Department of Physics, Michigan Technological University, Houghton, MI, USA
| | | | - C M Hui
- NASA Marshall Space Flight Center, Astrophysics Office, Huntsville, AL, USA
| | - P Hüntemeyer
- Department of Physics, Michigan Technological University, Houghton, MI, USA
| | - A Iriarte
- Instituto de Astronomía, Universidad Nacional Autónoma de México, Mexico City, Mexico
| | - A Jardin-Blicq
- Max-Planck Institute for Nuclear Physics, Heidelberg, Germany
| | - V Joshi
- Max-Planck Institute for Nuclear Physics, Heidelberg, Germany
| | - S Kaufmann
- Universidad Autónoma de Chiapas, Tuxtla Gutiérrez, Mexico
| | - P Kar
- Department of Physics and Astronomy, University of Utah, Salt Lake City, UT, USA
| | - G J Kunde
- Physics and Theoretical Divisions, Los Alamos National Laboratory, Los Alamos, NM, USA
| | - R J Lauer
- Department of Physics and Astronomy, University of New Mexico, Albuquerque, NM, USA
| | - W H Lee
- Instituto de Astronomía, Universidad Nacional Autónoma de México, Mexico City, Mexico
| | - H León Vargas
- Instituto de Física, Universidad Nacional Autónoma de México, Mexico City, Mexico
| | - H Li
- Physics and Theoretical Divisions, Los Alamos National Laboratory, Los Alamos, NM, USA
| | - J T Linnemann
- Department of Physics and Astronomy, Michigan State University, East Lansing, MI, USA
| | - A L Longinotti
- Instituto Nacional de Astrofísica, Óptica y Electrónica, Puebla, Mexico
| | - G Luis-Raya
- Universidad Politecnica de Pachuca, Pachuca, Mexico
| | | | - K Malone
- Department of Physics, Pennsylvania State University, University Park, PA, USA
| | - S S Marinelli
- Department of Physics and Astronomy, Michigan State University, East Lansing, MI, USA
| | - O Martinez
- Facultad de Ciencias Físico Matemáticas, Benemérita Universidad Autónoma de Puebla, Puebla, Mexico
| | | | - J Martínez-Castro
- Centro de Investigación en Computación, Instituto Politécnico Nacional, Mexico City, Mexico
| | - J A Matthews
- Department of Physics and Astronomy, University of New Mexico, Albuquerque, NM, USA
| | | | - E Moreno
- Facultad de Ciencias Físico Matemáticas, Benemérita Universidad Autónoma de Puebla, Puebla, Mexico
| | - M Mostafá
- Department of Physics, Pennsylvania State University, University Park, PA, USA
| | - A Nayerhoda
- Institute of Nuclear Physics Polish Academy of Sciences, IFJ-PAN, Krakow, Poland
| | - L Nellen
- Instituto de Ciencias Nucleares, Universidad Nacional Autónoma de Mexico, Mexico City, Mexico
| | - M Newbold
- Department of Physics and Astronomy, University of Utah, Salt Lake City, UT, USA
| | - M U Nisa
- Department of Physics and Astronomy, University of Rochester, Rochester, NY, USA
| | | | - J Pretz
- Department of Physics, Pennsylvania State University, University Park, PA, USA
| | | | - Z Ren
- Department of Physics and Astronomy, University of New Mexico, Albuquerque, NM, USA
| | - C D Rho
- Department of Physics and Astronomy, University of Rochester, Rochester, NY, USA.
| | - C Rivière
- Department of Physics, University of Maryland, College Park, MD, USA
| | - D Rosa-González
- Instituto Nacional de Astrofísica, Óptica y Electrónica, Puebla, Mexico
| | - M Rosenberg
- Department of Physics, Pennsylvania State University, University Park, PA, USA
| | - E Ruiz-Velasco
- Max-Planck Institute for Nuclear Physics, Heidelberg, Germany
| | - F Salesa Greus
- Institute of Nuclear Physics Polish Academy of Sciences, IFJ-PAN, Krakow, Poland
| | - A Sandoval
- Instituto de Física, Universidad Nacional Autónoma de México, Mexico City, Mexico
| | - M Schneider
- Santa Cruz Institute for Particle Physics, University of California, Santa Cruz, Santa Cruz, CA, USA
| | - H Schoorlemmer
- Max-Planck Institute for Nuclear Physics, Heidelberg, Germany
| | - M Seglar Arroyo
- Department of Physics, Pennsylvania State University, University Park, PA, USA
| | - G Sinnis
- Physics and Theoretical Divisions, Los Alamos National Laboratory, Los Alamos, NM, USA
| | - A J Smith
- Department of Physics, University of Maryland, College Park, MD, USA
| | - R W Springer
- Department of Physics and Astronomy, University of Utah, Salt Lake City, UT, USA
| | - P Surajbali
- Max-Planck Institute for Nuclear Physics, Heidelberg, Germany
| | - I Taboada
- School of Physics and Center for Relativistic Astrophysics, Georgia Institute of Technology, Atlanta, GA, USA
| | - O Tibolla
- Universidad Autónoma de Chiapas, Tuxtla Gutiérrez, Mexico
| | - K Tollefson
- Department of Physics and Astronomy, Michigan State University, East Lansing, MI, USA
| | - I Torres
- Instituto Nacional de Astrofísica, Óptica y Electrónica, Puebla, Mexico
| | - G Vianello
- Department of Physics, Stanford University, Stanford, CA, USA
| | - L Villaseñor
- Facultad de Ciencias Físico Matemáticas, Benemérita Universidad Autónoma de Puebla, Puebla, Mexico
| | - T Weisgarber
- Department of Physics and Wisconsin IceCube Particle Astrophysics Center, University of Wisconsin-Madison, Madison, WI, USA
| | - F Werner
- Max-Planck Institute for Nuclear Physics, Heidelberg, Germany
| | - S Westerhoff
- Department of Physics and Wisconsin IceCube Particle Astrophysics Center, University of Wisconsin-Madison, Madison, WI, USA
| | - J Wood
- Department of Physics and Wisconsin IceCube Particle Astrophysics Center, University of Wisconsin-Madison, Madison, WI, USA
| | - T Yapici
- Department of Physics and Astronomy, University of Rochester, Rochester, NY, USA
| | - G Yodh
- Department of Physics and Astronomy, University of California, Irvine, Irvine, CA, USA
| | - A Zepeda
- Universidad Autónoma de Chiapas, Tuxtla Gutiérrez, Mexico.,Physics Department, Centro de Investigación y de Estudios Avanzados del IPN, Mexico City, Mexico
| | - H Zhang
- Department of Physics and Astronomy, Purdue University, West Lafayette, IN, USA
| | - H Zhou
- Physics and Theoretical Divisions, Los Alamos National Laboratory, Los Alamos, NM, USA.
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Abeysekara A, Albert A, Alfaro R, Alvarez C, Álvarez J, Arceo R, Arteaga-Velázquez J, Avila Rojas D, Ayala Solares H, Belmont-Moreno E, BenZvi S, Braun J, Brisbois C, Caballero-Mora K, Capistrán T, Carramiñana A, Casanova S, Castillo M, Cotti U, Cotzomi J, Coutiño de León S, De León C, De la Fuente E, Diaz Hernandez R, Dichiara S, Dingus B, DuVernois M, Ellsworth R, Engel K, Enríquez-Rivera O, Fleischhack H, Fraija N, Galván-Gámez A, García-González J, González Muñoz A, González M, Hampel-Arias Z, Harding J, Hernandez S, Hona B, Hueyotl-Zahuantitla F, Hui C, Hüntemeyer P, Iriarte A, Jardin-Blicq A, Joshi V, Kaufmann S, Lara A, Lee W, León Vargas H, Linnemann J, Longinotti A, Luis-Raya G, Luna-García R, López-Coto R, Malone K, Marinelli S, Martinez O, Martinez-Castellanos I, Martínez-Castro J, Martínez-Huerta H, Matthews J, Miranda-Romagnoli P, Moreno E, Mostafá M, Nellen L, Newbold M, Nisa M, Noriega-Papaqui R, Pelayo R, Pretz J, Pérez-Pérez E, Ren Z, Rho C, Rivière C, Rosa-González D, Rosenberg M, Ruiz-Velasco E, Salesa Greus F, Sandoval A, Schneider M, Schoorlemmer H, Seglar Arroyo M, Sinnis G, Smith A, Springer R, Surajbali P, Taboada I, Tibolla O, Torres I, Villaseñor L, Weisgarber T, Westerhoff S, Wood J, Yapici T, Yodh G, Zepeda A, Zhou H. Constraining the
p¯/p
ratio in TeV cosmic rays with observations of the Moon shadow by HAWC. Int J Clin Exp Med 2018. [DOI: 10.1103/physrevd.97.102005] [Citation(s) in RCA: 5] [Impact Index Per Article: 0.8] [Reference Citation Analysis] [What about the content of this article? (0)] [Track Full Text] [Journal Information] [Subscribe] [Scholar Register] [Indexed: 11/07/2022]
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13
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Abeysekara AU, Albert A, Alfaro R, Alvarez C, Álvarez JD, Arceo R, Arteaga-Velázquez JC, Avila Rojas D, Ayala Solares HA, Barber AS, Bautista-Elivar N, Becerril A, Belmont-Moreno E, BenZvi SY, Berley D, Bernal A, Braun J, Brisbois C, Caballero-Mora KS, Capistrán T, Carramiñana A, Casanova S, Castillo M, Cotti U, Cotzomi J, Coutiño de León S, De León C, De la Fuente E, Dingus BL, DuVernois MA, Díaz-Vélez JC, Ellsworth RW, Engel K, Enríquez-Rivera O, Fiorino DW, Fraija N, García-González JA, Garfias F, Gerhardt M, González Muñoz A, González MM, Goodman JA, Hampel-Arias Z, Harding JP, Hernández S, Hernández-Almada A, Hinton J, Hona B, Hui CM, Hüntemeyer P, Iriarte A, Jardin-Blicq A, Joshi V, Kaufmann S, Kieda D, Lara A, Lauer RJ, Lee WH, Lennarz D, Vargas HL, Linnemann JT, Longinotti AL, Luis Raya G, Luna-García R, López-Coto R, Malone K, Marinelli SS, Martinez O, Martinez-Castellanos I, Martínez-Castro J, Martínez-Huerta H, Matthews JA, Miranda-Romagnoli P, Moreno E, Mostafá M, Nellen L, Newbold M, Nisa MU, Noriega-Papaqui R, Pelayo R, Pretz J, Pérez-Pérez EG, Ren Z, Rho CD, Rivière C, Rosa-González D, Rosenberg M, Ruiz-Velasco E, Salazar H, Salesa Greus F, Sandoval A, Schneider M, Schoorlemmer H, Sinnis G, Smith AJ, Springer RW, Surajbali P, Taboada I, Tibolla O, Tollefson K, Torres I, Ukwatta TN, Vianello G, Weisgarber T, Westerhoff S, Wisher IG, Wood J, Yapici T, Yodh G, Younk PW, Zepeda A, Zhou H, Guo F, Hahn J, Li H, Zhang H. Extended gamma-ray sources around pulsars constrain the origin of the positron flux at Earth. Science 2018; 358:911-914. [PMID: 29146808 DOI: 10.1126/science.aan4880] [Citation(s) in RCA: 211] [Impact Index Per Article: 35.2] [Reference Citation Analysis] [What about the content of this article? (0)] [Affiliation(s)] [Abstract] [Track Full Text] [Journal Information] [Subscribe] [Scholar Register] [Received: 04/20/2017] [Accepted: 10/09/2017] [Indexed: 11/02/2022]
Abstract
The unexpectedly high flux of cosmic-ray positrons detected at Earth may originate from nearby astrophysical sources, dark matter, or unknown processes of cosmic-ray secondary production. We report the detection, using the High-Altitude Water Cherenkov Observatory (HAWC), of extended tera-electron volt gamma-ray emission coincident with the locations of two nearby middle-aged pulsars (Geminga and PSR B0656+14). The HAWC observations demonstrate that these pulsars are indeed local sources of accelerated leptons, but the measured tera-electron volt emission profile constrains the diffusion of particles away from these sources to be much slower than previously assumed. We demonstrate that the leptons emitted by these objects are therefore unlikely to be the origin of the excess positrons, which may have a more exotic origin.
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Affiliation(s)
- A U Abeysekara
- Department of Physics and Astronomy, University of Utah, Salt Lake City, UT, USA
| | - A Albert
- Los Alamos National Laboratory, Los Alamos, NM, USA
| | - R Alfaro
- Instituto de Física, Universidad Nacional Autónoma de México, Mexico City, Mexico
| | - C Alvarez
- Universidad Autónoma de Chiapas, Tuxtla Gutiérrez, Chiapas, Mexico
| | - J D Álvarez
- Universidad Michoacana de San Nicolás de Hidalgo, Morelia, Mexico
| | - R Arceo
- Universidad Autónoma de Chiapas, Tuxtla Gutiérrez, Chiapas, Mexico
| | | | - D Avila Rojas
- Instituto de Física, Universidad Nacional Autónoma de México, Mexico City, Mexico
| | - H A Ayala Solares
- Department of Physics, Michigan Technological University, Houghton, MI, USA
| | - A S Barber
- Department of Physics and Astronomy, University of Utah, Salt Lake City, UT, USA
| | | | - A Becerril
- Instituto de Física, Universidad Nacional Autónoma de México, Mexico City, Mexico
| | - E Belmont-Moreno
- Instituto de Física, Universidad Nacional Autónoma de México, Mexico City, Mexico
| | - S Y BenZvi
- Department of Physics and Astronomy, University of Rochester, Rochester, NY, USA
| | - D Berley
- Department of Physics, University of Maryland, College Park, MD, USA
| | - A Bernal
- Instituto de Astronomía, Universidad Nacional Autónoma de México, Mexico City, Mexico
| | - J Braun
- Department of Physics, University of Wisconsin-Madison, Madison, WI, USA
| | - C Brisbois
- Department of Physics, Michigan Technological University, Houghton, MI, USA
| | | | - T Capistrán
- Instituto Nacional de Astrofísica, Óptica y Electrónica, Puebla, Mexico
| | - A Carramiñana
- Instituto Nacional de Astrofísica, Óptica y Electrónica, Puebla, Mexico
| | - S Casanova
- Institute of Nuclear Physics Polish Academy of Sciences, Krakow, Poland.,Max-Planck Institute for Nuclear Physics, Heidelberg, Germany
| | - M Castillo
- Universidad Michoacana de San Nicolás de Hidalgo, Morelia, Mexico
| | - U Cotti
- Universidad Michoacana de San Nicolás de Hidalgo, Morelia, Mexico
| | - J Cotzomi
- Facultad de Ciencias Físico Matemáticas, Benemérita Universidad Autónoma de Puebla, Puebla, Mexico
| | - S Coutiño de León
- Instituto Nacional de Astrofísica, Óptica y Electrónica, Puebla, Mexico
| | - C De León
- Facultad de Ciencias Físico Matemáticas, Benemérita Universidad Autónoma de Puebla, Puebla, Mexico
| | - E De la Fuente
- Departamento de Física, Centro Universitario de Ciencias Exactas e Ingenierías, Universidad de Guadalajara, Guadalajara, Mexico
| | - B L Dingus
- Los Alamos National Laboratory, Los Alamos, NM, USA
| | - M A DuVernois
- Department of Physics, University of Wisconsin-Madison, Madison, WI, USA
| | - J C Díaz-Vélez
- Departamento de Física, Centro Universitario de Ciencias Exactas e Ingenierías, Universidad de Guadalajara, Guadalajara, Mexico
| | - R W Ellsworth
- School of Physics, Astronomy, and Computational Sciences, George Mason University, Fairfax, VA, USA
| | - K Engel
- Department of Physics, University of Maryland, College Park, MD, USA
| | - O Enríquez-Rivera
- Instituto de Geofísica, Universidad Nacional Autónoma de México, Mexico City, Mexico
| | - D W Fiorino
- Department of Physics, University of Maryland, College Park, MD, USA
| | - N Fraija
- Instituto de Astronomía, Universidad Nacional Autónoma de México, Mexico City, Mexico
| | - J A García-González
- Instituto de Física, Universidad Nacional Autónoma de México, Mexico City, Mexico
| | - F Garfias
- Instituto de Astronomía, Universidad Nacional Autónoma de México, Mexico City, Mexico
| | - M Gerhardt
- Department of Physics, Michigan Technological University, Houghton, MI, USA
| | - A González Muñoz
- Instituto de Física, Universidad Nacional Autónoma de México, Mexico City, Mexico
| | - M M González
- Instituto de Astronomía, Universidad Nacional Autónoma de México, Mexico City, Mexico
| | - J A Goodman
- Department of Physics, University of Maryland, College Park, MD, USA
| | - Z Hampel-Arias
- Department of Physics, University of Wisconsin-Madison, Madison, WI, USA
| | - J P Harding
- Los Alamos National Laboratory, Los Alamos, NM, USA
| | - S Hernández
- Instituto de Física, Universidad Nacional Autónoma de México, Mexico City, Mexico
| | - A Hernández-Almada
- Instituto de Física, Universidad Nacional Autónoma de México, Mexico City, Mexico
| | - J Hinton
- Max-Planck Institute for Nuclear Physics, Heidelberg, Germany
| | - B Hona
- Department of Physics, Michigan Technological University, Houghton, MI, USA
| | - C M Hui
- Astrophysics Office, NASA Marshall Space Flight Center Huntsville, AL, USA
| | - P Hüntemeyer
- Department of Physics, Michigan Technological University, Houghton, MI, USA
| | - A Iriarte
- Instituto de Astronomía, Universidad Nacional Autónoma de México, Mexico City, Mexico
| | - A Jardin-Blicq
- Max-Planck Institute for Nuclear Physics, Heidelberg, Germany
| | - V Joshi
- Max-Planck Institute for Nuclear Physics, Heidelberg, Germany
| | - S Kaufmann
- Universidad Autónoma de Chiapas, Tuxtla Gutiérrez, Chiapas, Mexico
| | - D Kieda
- Department of Physics and Astronomy, University of Utah, Salt Lake City, UT, USA
| | - A Lara
- Instituto de Geofísica, Universidad Nacional Autónoma de México, Mexico City, Mexico
| | - R J Lauer
- Department of Physics and Astronomy, University of New Mexico, Albuquerque, NM, USA
| | - W H Lee
- Instituto de Astronomía, Universidad Nacional Autónoma de México, Mexico City, Mexico
| | - D Lennarz
- School of Physics and Center for Relativistic Astrophysics, Georgia Institute of Technology, Atlanta, GA, USA
| | - H León Vargas
- Instituto de Física, Universidad Nacional Autónoma de México, Mexico City, Mexico
| | - J T Linnemann
- Department of Physics and Astronomy, Michigan State University, East Lansing, MI, USA
| | - A L Longinotti
- Instituto Nacional de Astrofísica, Óptica y Electrónica, Puebla, Mexico
| | - G Luis Raya
- Universidad Politecnica de Pachuca, Pachuca, Hidalgo, Mexico
| | - R Luna-García
- Centro de Investigación en Computación, Instituto Politécnico Nacional, Mexico City, Mexico
| | - R López-Coto
- Max-Planck Institute for Nuclear Physics, Heidelberg, Germany.
| | - K Malone
- Department of Physics, Pennsylvania State University, University Park, PA, USA
| | - S S Marinelli
- Department of Physics and Astronomy, Michigan State University, East Lansing, MI, USA
| | - O Martinez
- Facultad de Ciencias Físico Matemáticas, Benemérita Universidad Autónoma de Puebla, Puebla, Mexico
| | | | - J Martínez-Castro
- Centro de Investigación en Computación, Instituto Politécnico Nacional, Mexico City, Mexico
| | - H Martínez-Huerta
- Physics Department, Centro de Investigacion y de Estudios Avanzados del IPN, Mexico City, Mexico
| | - J A Matthews
- Department of Physics and Astronomy, University of New Mexico, Albuquerque, NM, USA
| | | | - E Moreno
- Facultad de Ciencias Físico Matemáticas, Benemérita Universidad Autónoma de Puebla, Puebla, Mexico
| | - M Mostafá
- Department of Physics, Pennsylvania State University, University Park, PA, USA
| | - L Nellen
- Instituto de Ciencias Nucleares, Universidad Nacional Autónoma de México, Mexico City, Mexico
| | - M Newbold
- Department of Physics and Astronomy, University of Utah, Salt Lake City, UT, USA
| | - M U Nisa
- Department of Physics and Astronomy, University of Rochester, Rochester, NY, USA
| | | | - R Pelayo
- Centro de Investigación en Computación, Instituto Politécnico Nacional, Mexico City, Mexico
| | - J Pretz
- Department of Physics, Pennsylvania State University, University Park, PA, USA
| | - E G Pérez-Pérez
- Universidad Politecnica de Pachuca, Pachuca, Hidalgo, Mexico
| | - Z Ren
- Department of Physics and Astronomy, University of New Mexico, Albuquerque, NM, USA
| | - C D Rho
- Department of Physics and Astronomy, University of Rochester, Rochester, NY, USA
| | - C Rivière
- Department of Physics, University of Maryland, College Park, MD, USA
| | - D Rosa-González
- Instituto Nacional de Astrofísica, Óptica y Electrónica, Puebla, Mexico
| | - M Rosenberg
- Department of Physics, Pennsylvania State University, University Park, PA, USA
| | - E Ruiz-Velasco
- Instituto de Física, Universidad Nacional Autónoma de México, Mexico City, Mexico
| | - H Salazar
- Facultad de Ciencias Físico Matemáticas, Benemérita Universidad Autónoma de Puebla, Puebla, Mexico
| | - F Salesa Greus
- Institute of Nuclear Physics Polish Academy of Sciences, Krakow, Poland.
| | - A Sandoval
- Instituto de Física, Universidad Nacional Autónoma de México, Mexico City, Mexico
| | - M Schneider
- Santa Cruz Institute for Particle Physics, University of California, Santa Cruz, Santa Cruz, CA, USA
| | - H Schoorlemmer
- Max-Planck Institute for Nuclear Physics, Heidelberg, Germany
| | - G Sinnis
- Los Alamos National Laboratory, Los Alamos, NM, USA
| | - A J Smith
- Department of Physics, University of Maryland, College Park, MD, USA
| | - R W Springer
- Department of Physics and Astronomy, University of Utah, Salt Lake City, UT, USA
| | - P Surajbali
- Max-Planck Institute for Nuclear Physics, Heidelberg, Germany
| | - I Taboada
- School of Physics and Center for Relativistic Astrophysics, Georgia Institute of Technology, Atlanta, GA, USA
| | - O Tibolla
- Universidad Autónoma de Chiapas, Tuxtla Gutiérrez, Chiapas, Mexico
| | - K Tollefson
- Department of Physics and Astronomy, Michigan State University, East Lansing, MI, USA
| | - I Torres
- Instituto Nacional de Astrofísica, Óptica y Electrónica, Puebla, Mexico
| | - T N Ukwatta
- Los Alamos National Laboratory, Los Alamos, NM, USA
| | - G Vianello
- Hansen Experimental Physics Laboratory Stanford University, Stanford, CA, USA
| | - T Weisgarber
- Department of Physics, University of Wisconsin-Madison, Madison, WI, USA
| | - S Westerhoff
- Department of Physics, University of Wisconsin-Madison, Madison, WI, USA
| | - I G Wisher
- Department of Physics, University of Wisconsin-Madison, Madison, WI, USA
| | - J Wood
- Department of Physics, University of Wisconsin-Madison, Madison, WI, USA
| | - T Yapici
- Department of Physics and Astronomy, Michigan State University, East Lansing, MI, USA
| | - G Yodh
- Department of Physics and Astronomy, University of California, Irvine, Irvine, CA, USA
| | - P W Younk
- Los Alamos National Laboratory, Los Alamos, NM, USA
| | - A Zepeda
- Physics Department, Centro de Investigacion y de Estudios Avanzados del IPN, Mexico City, Mexico.,Universidad Autónoma de Chiapas, Tuxtla Gutiérrez, Chiapas, Mexico
| | - H Zhou
- Los Alamos National Laboratory, Los Alamos, NM, USA.
| | - F Guo
- Los Alamos National Laboratory, Los Alamos, NM, USA
| | - J Hahn
- Max-Planck Institute for Nuclear Physics, Heidelberg, Germany
| | - H Li
- Los Alamos National Laboratory, Los Alamos, NM, USA
| | - H Zhang
- Los Alamos National Laboratory, Los Alamos, NM, USA
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Abstract
Summary
Objectives:
To meet the challenge for high quality and efficient care, highly specialized and distributed healthcare establishments have to communicate and co-operate in a semantically interoperable way. Information and communication technology must be open, flexible, scalable, knowledge-based and service-oriented as well as secure and safe.
Methods:
For enabling semantic interoperability, a unified process for defining and implementing the architecture, i.e. structure and functions of the cooperating systems’ components, as well as the approach for knowledge representation, i.e. the used information and its interpretation, algorithms, etc. have to be defined in a harmonized way. Deploying the Generic Component Model, systems and their components, underlying concepts and applied constraints must be formally modeled, strictly separating platform-independent from platform-specific models.
Results:
As HL7 Version 3 claims to represent the most successful standard for semantic interoperability, HL7 has been analyzed regarding the requirements for model-driven, service-oriented design of semantic interoperable information systems, thereby moving from a communication to an architecture paradigm. The approach is compared with advanced architectural approaches for information systems such as OMG’s CORBA 3 or EHR systems such as GEHR/openEHR and CEN EN 13606 Electronic Health Record Communication.
Conclusion:
HL7 Version 3 is maturing towards an architectural approach for semantic interoperability. Despite current differences, there is a close collaboration between the teams involved guaranteeing a convergence between competing approaches.
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Stachs A, Engel K, Reimer T, Voigt J, Kundt G, Gerber B. Does computed tomography scan predict suboptimal primary cytoreduktion in patients with advanced ovarian cancer? Geburtshilfe Frauenheilkd 2017. [DOI: 10.1055/s-0037-1606155] [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: 10/18/2022] Open
Affiliation(s)
- A Stachs
- Universitätsfrauenklinik Rostock, Rostock
| | - K Engel
- Universitätsfrauenklinik Rostock, Rostock
| | - T Reimer
- Universitätsfrauenklinik Rostock, Rostock
| | - J Voigt
- Radiologische Praxis am Klinikum Südstadt Rostock, Rostock
| | - G Kundt
- Institut für Biostatistik und Informatik der Universität Rostock, Rostock
| | - B Gerber
- Universitätsfrauenklinik Rostock, Rostock
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Li VA, Dorrill R, Duvall MJ, Koblanski J, Negrashov S, Sakai M, Wipperfurth SA, Engel K, Jocher GR, Learned JG, Macchiarulo L, Matsuno S, McDonough WF, Mumm HP, Murillo J, Nishimura K, Rosen M, Usman SM, Varner GS. Invited Article: miniTimeCube. Rev Sci Instrum 2016; 87:021301. [PMID: 26931826 DOI: 10.1063/1.4942243] [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: 06/05/2023]
Abstract
We present the development of the miniTimeCube (mTC), a novel compact neutrino detector. The mTC is a multipurpose detector, aiming to detect not only neutrinos but also fast/thermal neutrons. Potential applications include the counterproliferation of nuclear materials and the investigation of antineutrino short-baseline effects. The mTC is a plastic 0.2% (10)B-doped scintillator (13 cm)(3) cube surrounded by 24 Micro-Channel Plate (MCP) photon detectors, each with an 8 × 8 anode totaling 1536 individual channels/pixels viewing the scintillator. It uses custom-made electronics modules which mount on top of the MCPs, making our detector compact and able to both distinguish different types of events and reject noise in real time. The detector is currently deployed and being tested at the National Institute of Standards and Technology Center for Neutron Research nuclear reactor (20 MWth) in Gaithersburg MD. A shield for further tests is being constructed, and calibration and upgrades are ongoing. The mTC's improved spatiotemporal resolution will allow for determination of incident particle directions beyond previous capabilities.
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Affiliation(s)
- V A Li
- Department of Physics and Astronomy, University of Hawaii at Manoa, Honolulu, Hawaii 96822, USA
| | - R Dorrill
- Department of Physics and Astronomy, University of Hawaii at Manoa, Honolulu, Hawaii 96822, USA
| | - M J Duvall
- Department of Physics and Astronomy, University of Hawaii at Manoa, Honolulu, Hawaii 96822, USA
| | - J Koblanski
- Department of Physics and Astronomy, University of Hawaii at Manoa, Honolulu, Hawaii 96822, USA
| | - S Negrashov
- Department of Physics and Astronomy, University of Hawaii at Manoa, Honolulu, Hawaii 96822, USA
| | - M Sakai
- Department of Physics and Astronomy, University of Hawaii at Manoa, Honolulu, Hawaii 96822, USA
| | - S A Wipperfurth
- Department of Geology, University of Maryland, College Park, Maryland 20742, USA
| | - K Engel
- Department of Geology, University of Maryland, College Park, Maryland 20742, USA
| | - G R Jocher
- Ultralytics LLC, Arlington, Virginia 22203, USA
| | - J G Learned
- Department of Physics and Astronomy, University of Hawaii at Manoa, Honolulu, Hawaii 96822, USA
| | - L Macchiarulo
- Department of Physics and Astronomy, University of Hawaii at Manoa, Honolulu, Hawaii 96822, USA
| | - S Matsuno
- Department of Physics and Astronomy, University of Hawaii at Manoa, Honolulu, Hawaii 96822, USA
| | - W F McDonough
- Department of Geology, University of Maryland, College Park, Maryland 20742, USA
| | - H P Mumm
- National Institute of Standards and Technology, 100 Bureau Dr., Gaithersburg, Maryland 20899, USA
| | - J Murillo
- Department of Physics and Astronomy, University of Hawaii at Manoa, Honolulu, Hawaii 96822, USA
| | - K Nishimura
- Ultralytics LLC, Arlington, Virginia 22203, USA
| | - M Rosen
- Department of Physics and Astronomy, University of Hawaii at Manoa, Honolulu, Hawaii 96822, USA
| | - S M Usman
- Exploratory Science and Technology Branch, National Geospatial-Intelligence Agency, Springfield, Virginia 22150, USA
| | - G S Varner
- Department of Physics and Astronomy, University of Hawaii at Manoa, Honolulu, Hawaii 96822, USA
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Kirn V, Thangarajah F, Richters L, Afheldt B, Bergauer F, Engel K, Schmidt-Petruschkat S, Theune M, Patzke J, Einzmann T, Mallmann P. Der „auffällige“ Pap-Abstrich: Belastung und Informationsbedürfnisse betroffener Frauen. Geburtshilfe Frauenheilkd 2014. [DOI: 10.1055/s-0034-1388311] [Citation(s) in RCA: 0] [Impact Index Per Article: 0] [Reference Citation Analysis] [What about the content of this article? (0)] [Track Full Text] [Journal Information] [Subscribe] [Scholar Register] [Indexed: 10/24/2022] Open
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Yang PFF, Engel K, Sanno M, Dargel J, Wegmann K, Brüggemann GP, Rittweger J. Tibia segment deformation in response to simulated muscle forces: a cadaveric study with a novel optical segment tracking (OST) approach. J Musculoskelet Neuronal Interact 2014; 14:267-275. [PMID: 25198221] [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] [Subscribe] [Scholar Register] [Indexed: 06/03/2023]
Abstract
OBJECTIVES A novel optical segment tracking (OST) approach reliant upon motion capturing was previously proposed to assess human tibia segment deformation. The purposes of the present study were to validate the OST approach and assess the contribution of muscular forces to the bone deformation in a well-defined ex vivo human model. METHODS A custom-made Lower Extremity Loading Device (LELD) was developed to simulate physiological muscle contractions in six human cadaveric lower extremities. Tibia segment deformation was measured by tracking the relative movement between two marker clusters which were affixed into the proximal and distal tibia, respectively. RESULTS Compared to the physiological norms, the simulated muscle forces remained at a low level. When quadriceps muscle was loaded with forces from 198 N to 505 N, posterior bending (0.12°-0.25°) and lateral bending (0.06°-0.21°) of the tibia segment were found. Large tibia bending angles were found when simulating the co-contraction of upper leg muscles and plantar flexors, and of all leg muscles, respectively. The standard deviations of the deformation angles between the repetitions remained at a low level. CONCLUSIONS We conclude that the OST approach has the potential to be applied in vivo and quantify muscle-induced bone deformations.
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Affiliation(s)
- P-F F Yang
- Key Laboratory for Space Bioscience and Biotechnology, School of Life Sciences, Northwestern Polytechnical University, Xi'an, China
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Engel K, Bassermann F. Das Ubiquitin-Proteasom-System und seine Bedeutung in der Onkologie. Dtsch Med Wochenschr 2013; 138:1178-82. [DOI: 10.1055/s-0033-1343110] [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: 10/26/2022]
Affiliation(s)
- K. Engel
- III. Medizinische Klinik, Klinikum rechts der Isar, Technische Universität München
| | - F. Bassermann
- III. Medizinische Klinik, Klinikum rechts der Isar, Technische Universität München
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Gauer T, Kiesel A, Engel K, Gargioni E, Petersen C. EP-1508 VALIDATION OF A LEAF SEQUENCING MODEL FOR ELECTRON IMRT PROVIDING EFFICIENT AND ROBUST DOSE DELIVERY IN BREAST CANCER. Radiother Oncol 2012. [DOI: 10.1016/s0167-8140(12)71841-8] [Citation(s) in RCA: 0] [Impact Index Per Article: 0] [Reference Citation Analysis] [What about the content of this article? (0)] [Track Full Text] [Journal Information] [Subscribe] [Scholar Register] [Indexed: 11/17/2022]
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Neufeld JD, Engel K, Cheng J, Moreno-Hagelsieb G, Rose DR, Charles TC. Open resource metagenomics: a model for sharing metagenomic libraries. Stand Genomic Sci 2011; 5:203-10. [PMID: 22180823 PMCID: PMC3235511 DOI: 10.4056/sigs.1974654] [Citation(s) in RCA: 18] [Impact Index Per Article: 1.4] [Reference Citation Analysis] [What about the content of this article? (0)] [Abstract] [Key Words] [Track Full Text] [Download PDF] [Figures] [Journal Information] [Subscribe] [Scholar Register] [Indexed: 11/20/2022] Open
Abstract
Both sequence-based and activity-based exploitation of environmental DNA have provided unprecedented access to the genomic content of cultivated and uncultivated microorganisms. Although researchers deposit microbial strains in culture collections and DNA sequences in databases, activity-based metagenomic studies typically only publish sequences from the hits retrieved from specific screens. Physical metagenomic libraries, conceptually similar to entire sequence datasets, are usually not straightforward to obtain by interested parties subsequent to publication. In order to facilitate unrestricted distribution of metagenomic libraries, we propose the adoption of open resource metagenomics, in line with the trend towards open access publishing, and similar to culture- and mutant-strain collections that have been the backbone of traditional microbiology and microbial genetics. The concept of open resource metagenomics includes preparation of physical DNA libraries, preferably in versatile vectors that facilitate screening in a diversity of host organisms, and pooling of clones so that single aliquots containing complete libraries can be easily distributed upon request. Database deposition of associated metadata and sequence data for each library provides researchers with information to select the most appropriate libraries for further research projects. As a starting point, we have established the Canadian MetaMicroBiome Library (CM(2)BL [1]). The CM(2)BL is a publicly accessible collection of cosmid libraries containing environmental DNA from soils collected from across Canada, spanning multiple biomes. The libraries were constructed such that the cloned DNA can be easily transferred to Gateway® compliant vectors, facilitating functional screening in virtually any surrogate microbial host for which there are available plasmid vectors. The libraries, which we are placing in the public domain, will be distributed upon request without restriction to members of both the academic research community and industry. This article invites the scientific community to adopt this philosophy of open resource metagenomics to extend the utility of functional metagenomics beyond initial publication, circumventing the need to start from scratch with each new research project.
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Zumpe C, Engel K, Wiedemann N, Metzger A, Pischetsrieder M, Bachmann C. Development of a STAT5 Phosphorylation Assay as a Rapid Bioassay to Assess Interleukin-7 Potency. Curr Pharm Biotechnol 2011; 12:1580-8. [DOI: 10.2174/138920111798357294] [Citation(s) in RCA: 1] [Impact Index Per Article: 0.1] [Reference Citation Analysis] [What about the content of this article? (0)] [Track Full Text] [Journal Information] [Subscribe] [Scholar Register] [Received: 07/22/2010] [Accepted: 01/12/2011] [Indexed: 11/22/2022]
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Gargioni E, Cremers F, Gauer T, Engel K, Goy Y, Petersen C. 317 oral DOSIMETRIC COMPARISON OF IMRT USING HELICAL PHOTON BEAMS VERSUS RANGE-MODULATED ELECTRON BEAMS IN RADIOTHERAPY OF BREAST AND CHEST WALL CANCER. Radiother Oncol 2011. [DOI: 10.1016/s0167-8140(11)70439-x] [Citation(s) in RCA: 0] [Impact Index Per Article: 0] [Reference Citation Analysis] [What about the content of this article? (0)] [Track Full Text] [Journal Information] [Subscribe] [Scholar Register] [Indexed: 10/18/2022]
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Mercimek-Mahmutoglu S, Moeslinger D, Häberle J, Engel K, Herle M, Strobl MW, Scheibenreiter S, Muehl A, Stöckler-Ipsiroglu S. Long-term outcome of patients with argininosuccinate lyase deficiency diagnosed by newborn screening in Austria. Mol Genet Metab 2010; 100:24-8. [PMID: 20236848 DOI: 10.1016/j.ymgme.2010.01.013] [Citation(s) in RCA: 43] [Impact Index Per Article: 3.1] [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: 01/23/2010] [Accepted: 01/24/2010] [Indexed: 11/16/2022]
Abstract
Twenty-three patients with late onset argininosuccinate lyase deficiency (ASLD) were identified during a 27-year period of newborn screening in Austria (1:95,600, 95% CI=1:68,036-1:162,531). One additional patient was identified outside the newborn screening with neonatal hyperammonemia. Long-term outcome data were available in 17 patients (median age 13 years) ascertained by newborn screening. Patients were treated with protein restricted diet and oral arginine supplementation during infancy and childhood. IQ was average/above average in 11 (65%), low average in 5 (29%), and in the mild intellectual disability range in 1 (6%) patients. Four patients had an abnormal EEG without evidence of clinical seizures and three had abnormal liver function tests and/or evidence of hepatic steatosis. Plasma citrulline levels were elevated in four patients. Plasma ammonia levels were within normal range prior and after a protein load in all patients. Seven different mutations were identified in the 16 alleles investigated. Four mutations were novel (p.E189G, p.R168C, p.R126P, and p.D423H). All mutations were associated with low argininosuccinate lyase activities (0-15%) in red blood cells. Newborn screening might be beneficial in the prevention of chronic neurologic and intellectual sequelae in late onset ASLD, but a proportion of benign variants might have contributed to the overall favorable outcome as well.
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Affiliation(s)
- S Mercimek-Mahmutoglu
- Department of Pediatrics, Division of Biochemical Diseases, British Columbia University, Vancouver, BC, Canada
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Gnoth MJ, Sandmann S, Engel K, Radtke M. In vitro to in vivo comparison of the substrate characteristics of sorafenib tosylate toward P-glycoprotein. Drug Metab Dispos 2010; 38:1341-6. [PMID: 20413726 DOI: 10.1124/dmd.110.032052] [Citation(s) in RCA: 33] [Impact Index Per Article: 2.4] [Reference Citation Analysis] [What about the content of this article? (0)] [Affiliation(s)] [Abstract] [Track Full Text] [Journal Information] [Subscribe] [Scholar Register] [Indexed: 02/02/2023] Open
Abstract
Sorafenib (Nexavar) is a novel oral Raf kinase and vascular endothelial growth factor receptor inhibitor. Most anticancer drugs are substrates for ATP-binding cassette efflux pumps especially for P-glycoprotein (P-gp). To evaluate the influence of P-gp on the pharmacokinetics of sorafenib substrate properties for this transporter were investigated. Therefore, permeability of sorafenib across Caco-2 and P-gp-overexpressing cells was determined. To determine the in vivo relevance of these in vitro findings, pharmacokinetics of sorafenib in mdr1a/1b(-/-) and wild-type (WT) mice was studied. Sorafenib is highly permeable and exhibits a slight efflux across Caco-2 cells. In P-gp-overexpressing cells, a small concentration-dependent efflux was observed, which was completely blocked by the addition of ivermectin. In mdr1a/1b(-/-) and WT mice, unchanged compound represented by far the majority of radioactivity in plasma. After intravenous and oral administration, brain/plasma concentration ratios in mdr1a/1b(-/-) mice were 1.3- to 1.5-fold higher than those in WT mice. However, after intravenous or oral administration, plasma concentrations were similar in both mouse strains. In conclusion, sorafenib is highly permeable and a weak P-gp substrate in vitro. These findings were confirmed by the small factor of 1.3 to 1.5 observed for the brain/plasma ratios in mdr1a/1b(-/-) versus WT mice in vivo. Based on these in vitro and in vivo results, it is unlikely that P-gp has a major effect on the plasma concentrations of sorafenib in humans. Because of the high permeability and low P-gp-mediated transport, sorafenib might be able to cross the blood-brain barrier and target tumors within the brain.
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Affiliation(s)
- M J Gnoth
- Drug Metabolism and Pharmacokinetics, Bayer Schering Pharma AG, Wuppertal, Germany.
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Klaus V, Vermeulen T, Minassian B, Israelian N, Engel K, Lund AM, Roebrock K, Christensen E, Häberle J. Highly variable clinical phenotype of carbamylphosphate synthetase 1 deficiency in one family: an effect of allelic variation in gene expression? Clin Genet 2010; 76:263-9. [PMID: 19793055 DOI: 10.1111/j.1399-0004.2009.01216.x] [Citation(s) in RCA: 21] [Impact Index Per Article: 1.5] [Reference Citation Analysis] [What about the content of this article? (0)] [Affiliation(s)] [Abstract] [Track Full Text] [Journal Information] [Subscribe] [Scholar Register] [Indexed: 11/27/2022]
Abstract
Deficiency of the urea cycle enzyme carbamylphosphate synthetase 1 (CPS1) causes hyperammonemia with a vast range of clinical severity from neonatal onset with early lethality to onset after age 40 with rare episodes of hyperammonemic confusion. The cause for this variability is not understood. We report two patients from one family with highly divergent clinical course, one presenting neonatally with a fatal form and the other at age 45 with benign diet-responsive disease. The patients are compound heterozygous for two mutations of the CPS1 gene, c.3558 + 1G > C and c.4101 + 2T > C. The haplotypes containing each mutation are identical between the two patients, as are the sequences of CPS1 exons and flanking introns. Transcriptional experiments show that the abnormal CPS1 transcripts generated by both mutations are identical in these two patients. We characterize promoter and enhancer sequences of the CPS1 gene and find also in these regions no sequence differences between patients. Finally, we perform cloning experiments and find that in the neonatal-onset case, clones of messenger RNA (mRNA) expressed from the allele carrying the c.4101 + 2T > C mutation are threefold more than clones of mRNA from the allele with the c.3558 + 1G > C mutation, whereas in the adult-onset case the two types of clones are equal, indicating skewed expression towards the c.4101 + 2T > C allele in the neonatal case. Although we are yet to understand the mechanism of this differential expression, our work suggests that allelic imbalance may explain clinical variability in CPS1 deficiency in some families.
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Affiliation(s)
- V Klaus
- Universitätsklinikum Münster, Klinik und Poliklinik für Kinder- und Jugendmedizin, 48129 Münster, Germany
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Niemier K, Schmidt S, Engel K, Steinmetz A, Herms K, Herms K, Liefring V, Maulhardt A, Wetterling T, Kosup S, Casser R, Jäger G, Törkott S, Bieneck K, Rotter G, Marnitz U, Klein A, Jahr S, Reishauer A, Seidel W. Funktionelle Diagnostik der Bewegungssteuerung, Bewegungsstabilisation und Hypermobilität. Orthopäde 2009; 38:847-54. [DOI: 10.1007/s00132-009-1474-y] [Citation(s) in RCA: 6] [Impact Index Per Article: 0.4] [Reference Citation Analysis] [What about the content of this article? (0)] [Track Full Text] [Subscribe] [Scholar Register] [Indexed: 11/28/2022]
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Engel K, Kildeberg PA, Fine BP, Winters RW. Effects of Acute Respiratory Acidosis on Blood Lactate Concentration. Scandinavian Journal of Clinical and Laboratory Investigation 2009. [DOI: 10.3109/00365516709076940] [Citation(s) in RCA: 8] [Impact Index Per Article: 0.5] [Reference Citation Analysis] [What about the content of this article? (0)] [Track Full Text] [Subscribe] [Scholar Register] [Indexed: 11/13/2022]
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Bandelow B, Engel K, Wedekind D. [Evidence-based medicine in therapy of anxiety disorders]. MMW Fortschr Med 2009; 151:89-91. [PMID: 19504830] [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: 05/27/2023]
Affiliation(s)
- B Bandelow
- Klinik für Psychiatrie und Psychotherapie der Universität Göttingen.
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Wedekind D, Sprute A, Broocks A, Hüther G, Engel K, Falkai P, Bandelow B. Nocturnal urinary cortisol excretion over a randomized controlled trial with paroxetine vs. placebo combined with relaxation training or aerobic exercise in panic disorder. Curr Pharm Des 2009; 14:3518-24. [PMID: 19075728 DOI: 10.2174/138161208786848757] [Citation(s) in RCA: 10] [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: 11/22/2022]
Abstract
INTRODUCTION Data on basal hypothalamo-pituitary-adrenomedullary (HPA) function over controlled treatment trials with serotonergic drugs in anxiety disorders are still rare. METHODS 29 patients with panic disorder participating in a 10 week randomized, controlled trial (paroxetine vs. placebo with exercise or relaxation; N=60) collected urine for cortisol excretion over 3 consecutive nights before start and before termination of the treatment episode. Urinary cortisol was measured by radioimmunoassay. Efficacy measures were the Clinical Global Impression Scale (CGI) and the Panic and Agoraphobia Scale (P&A). 83% were female (p<.05 vs. males). 55% received additional aerobic exercise, and 45% relaxation. 55% received paroxetine treatment, and 45% placebo. Significantly fewer males received placebo treatment (p<.05). RESULTS All subjects improved significantly. Cortisol excretion did not differ between treatment groups or at pre-/post measurements. Females showed a significantly higher variability of cortisol excretion compared to males, at pre-(p<.005) and post (p=.015) assessments. Males displayed a trend to lower basal HPA function at end of treatment (p=.08). HPA variability after treatment showed a trend to be higher in the paroxetine (p=.052) -who clinically improved significantly better- compared to the placebo group. No relationship between HPA activity and treatment response or with exercise was detected. DISCUSSION HPA function shows significant gender differences, with females having a higher HPA function variability. Future studies on HPA function in treatment trials should address gender and medication effects.
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Affiliation(s)
- D Wedekind
- Department of Psychiatry and Psychotherapy, University of Goettingen, Von-Siebold-Strasse 5, D-37075 Goettingen, Germany.
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Oexle K, Engel K, Tinschert S, Haas D, Lee-Kirsch MA. Three-generational alkaptonuria in a non-consanguineous family. J Inherit Metab Dis 2008; 31 Suppl 2:S425-30. [PMID: 19096913 DOI: 10.1007/s10545-008-0994-7] [Citation(s) in RCA: 7] [Impact Index Per Article: 0.4] [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: 07/07/2008] [Revised: 11/10/2008] [Accepted: 11/11/2008] [Indexed: 11/28/2022]
Abstract
OBJECTIVE Alkaptonuria (AKU) is a rare inborn error of metabolism of aromatic amino acids and considered to be an autosomal recessive trait caused by mutations in the homogentisate 1,2-dioxygenase (HGD) gene. A dominant pattern of inheritance has been reported but was attributed to extended consanguinity in many cases. However, we have observed a non-consanguineous family segregating AKU in a dominant manner over three generations. RESULTS All affected individuals presented with typical features of AKU including darkening of the urine, ochronosis, arthropathy, and elevated urinary excretion of homogentisic acid. Sequence analysis of the HGD gene from genomic DNA of two affected individuals, uncle and niece, revealed a heterozygous missense mutation (M368V) in the uncle that was not present in his niece. Microsatellite genotyping demonstrated that both were heterozygous at the HGD locus and shared one haplotype. This haplotype did not contain a detectable HGD mutation. The haplotype was also found in a healthy son of the niece, making a dominant HGD mutation unlikely. Moreover, sequencing of cDNA from lymphoblastoid cells of the niece did not reveal an HGD mRNA with a potentially dominant-negative effect. CONCLUSION Rare causes of the uncommon AKU inheritance in this family have to be considered, ranging from the coincidence of undetectable HGD mutations to a dominant mutation of a second, hitherto unknown AKU gene.
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Affiliation(s)
- K Oexle
- Institute of Human Genetics, Technical University Munich, Trogerstr. 32, D-81675, München, Germany.
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Wedekind D, Engel K, Bandelow B. [Social anxiety disorder--diagnostics and treatment options]. Fortschr Neurol Psychiatr 2008; 76:616-624. [PMID: 18833508 DOI: 10.1055/s-2008-1038201] [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] [Subscribe] [Scholar Register] [Indexed: 05/26/2023]
Affiliation(s)
- D Wedekind
- Klinik für Psychiatrie und Psychotherapie der Georg-August-Universität Göttingen.
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Engel K, Reuter J, Seiler C, Mönting JS, Jakob T, Schempp CM. Anti-inflammatory effect of pimecrolimus in the sodium lauryl sulphate test. J Eur Acad Dermatol Venereol 2008; 22:447-50. [DOI: 10.1111/j.1468-3083.2007.02477.x] [Citation(s) in RCA: 22] [Impact Index Per Article: 1.4] [Reference Citation Analysis] [What about the content of this article? (0)] [Track Full Text] [Journal Information] [Subscribe] [Scholar Register] [Indexed: 11/26/2022]
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Engel K, Klaus V, Keyvani K, Hörnig-Franz I, Rellensmann G, Häberle J. Neugeborenes mit Knochenbrüchen: Nemaline Myopathie ist eine Differentialdiagnose zur Osteogenesis imperfecta. Z Geburtshilfe Neonatol 2008. [DOI: 10.1055/s-2008-1079045] [Citation(s) in RCA: 0] [Impact Index Per Article: 0] [Reference Citation Analysis] [What about the content of this article? (0)] [Track Full Text] [Journal Information] [Subscribe] [Scholar Register] [Indexed: 10/21/2022]
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Abstract
Anxiety disorders represent a widespread illness. Those affected with initial symptoms usually seek the help of their family doctor. In many cases, considerable time passes before the diagnosis has been established and specialised treatment applied, with the result that chronification is furthered. Physical symptoms of an anxiety disorder, and fears of contracting somatic disease are almost always the first to be described. In patients abusing alcohol and/or hypnotics consideration must always be given to an anxiety disorder. Previously existing symptoms almost always include depressive moods or avoidance behavior. Stressful life events and other psychosocial stressful factors may also point the way to the early diagnosis of an anxiety disorder.
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Affiliation(s)
- D Wedekind
- Klinik für Psychiatrie und Psychotherapie, Georg-August-Universität Göttingen.
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Jacobi U, Engel K, Patzelt A, Worm M, Sterry W, Lademann J. Penetration of Pollen Proteins into the Skin. Skin Pharmacol Physiol 2007; 20:297-304. [PMID: 17851273 DOI: 10.1159/000108101] [Citation(s) in RCA: 26] [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] [Received: 02/01/2007] [Accepted: 06/15/2007] [Indexed: 11/19/2022]
Abstract
Atopic dermatitis is a chronic remittent skin disease. In the extrinsic form of atopic dermatitis, type IgE-mediated reactions play an important pathophysiological role. The aim of the present study was to examine whether type I allergens can penetrate into the skin. Therefore, pollen proteins were labeled with fluorescein isothiocyanate (FITC), and their penetration profile was studied qualitatively. Solutions of FITC-labeled pollen proteins were applied in vitro on porcine skin and in vivo on human skin. In vitro, the FITC-labeled proteins were observed within the complete stratum corneum (SC) and inside the hair follicles even 15 min after application. They were also distributed inside the dermis around the hair follicles. In vivo, a similar pattern of distribution within the SC and the hair follicles was observed. These results indicate penetration via the SC lipid layers and a faster penetration via the hair follicles. The FITC-labeled proteins entered the dermis via the follicular pathway. Therefore, the follicular penetration should be considered in the development of skin protection strategies. To evaluate such strategies, the developed method can be used, and further studies in atopic dermatitis patients are necessary to determine whether the penetration of type I allergens is increased.
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Affiliation(s)
- U Jacobi
- Department of Dermatology and Allergology, Charité - Universitätsmedizin Berlin, Berlin, Germany
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Engel K, Schmidt U, Reuter J, Weckesser S, Simon-Haarhaus B, Schempp CM. Usnea barbata extract prevents ultraviolet-B induced prostaglandin E2 synthesis and COX-2 expression in HaCaT keratinocytes. J Photochem Photobiol B 2007; 89:9-14. [PMID: 17766140 DOI: 10.1016/j.jphotobiol.2007.08.002] [Citation(s) in RCA: 17] [Impact Index Per Article: 1.0] [Reference Citation Analysis] [What about the content of this article? (0)] [Affiliation(s)] [Abstract] [MESH Headings] [Track Full Text] [Subscribe] [Scholar Register] [Received: 05/09/2007] [Revised: 08/01/2007] [Accepted: 08/01/2007] [Indexed: 10/23/2022]
Abstract
Usnea barbata and its major constituent usnic acid are potent antimicrobial agents. Here, we have investigated anti-inflammatory properties of an U. barbata extract (UBE) containing 4% usnic acid in an ultraviolet-B (UVB) model with HaCaT keratinocytes. UVB irradiation induced PGE(2) production and COX-2 expression in a time and dose-dependent manner. UBE inhibited PGE(2) production at a half-maximal concentration of 60 microg/ml (2.4 microg/ml usnic acid) that did not affect the UVB-induced upregulation of COX-2, suggesting an effect on enzyme activity rather than on protein expression. The inhibition of PGE(2) production by UBE was not due to cytotoxicity. Besides its known antimicrobial properties, UBE displays specific UVB protective effects that might be useful in the topical treatment of UVB-mediated inflammatory skin conditions.
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Affiliation(s)
- K Engel
- Department of Dermatology, University Medical Center Freiburg, Hauptstr. 7, D-79104 Freiburg, Germany
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Weckesser S, Engel K, Simon-Haarhaus B, Wittmer A, Pelz K, Schempp CM. Screening of plant extracts for antimicrobial activity against bacteria and yeasts with dermatological relevance. Phytomedicine 2007; 14:508-16. [PMID: 17291738 DOI: 10.1016/j.phymed.2006.12.013] [Citation(s) in RCA: 119] [Impact Index Per Article: 7.0] [Reference Citation Analysis] [What about the content of this article? (0)] [Affiliation(s)] [Abstract] [MESH Headings] [Track Full Text] [Subscribe] [Scholar Register] [Received: 04/06/2006] [Accepted: 10/13/2006] [Indexed: 05/09/2023]
Abstract
There is cumulative resistance against antibiotics of many bacteria. Therefore, the development of new antiseptics and antimicrobial agents for the treatment of skin infections is of increasing interest. We have screened six plant extracts and isolated compounds for antimicrobial effects on bacteria and yeasts with dermatological relevance. The following plant extracts have been tested: Gentiana lutea, Harpagophytum procumbens, Boswellia serrata (dry extracts), Usnea barbata, Rosmarinus officinalis and Salvia officinalis (supercritical carbon dioxide [CO2] extracts). Additionally, the following characteristic plant substances were tested: usnic acid, carnosol, carnosic acid, ursolic acid, oleanolic acid, harpagoside, boswellic acid and gentiopicroside. The extracts and compounds were tested against 29 aerobic and anaerobic bacteria and yeasts in the agar dilution test. U. barbata-extract and usnic acid were the most active compounds, especially in anaerobic bacteria. Usnea CO2-extract effectively inhibited the growth of several Gram-positive bacteria like Staphylococcus aureus (including methicillin-resistant strains - MRSA), Propionibacterium acnes and Corynebacterium species. Growth of the dimorphic yeast Malassezia furfur was also inhibited by Usnea-extract. Besides the Usnea-extract, Rosmarinus-, Salvia-, Boswellia- and Harpagophytum-extracts proved to be effective against a panel of bacteria. It is concluded that due to their antimicrobial effects some of the plant extracts may be used for the topical treatment of skin disorders like acne vulgaris and seborrhoic eczema.
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Affiliation(s)
- S Weckesser
- Department of Dermatology, University of Freiburg, Hauptstrasse 7, 79104 Freiburg, Germany
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Blobel BGME, Engel K, Pharow P. Semantic interoperability--HL7 Version 3 compared to advanced architecture standards. Methods Inf Med 2006; 45:343-53. [PMID: 16964348] [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: 05/11/2023]
Abstract
OBJECTIVES To meet the challenge for high quality and efficient care, highly specialized and distributed healthcare establishments have to communicate and co-operate in a semantically interoperable way. Information and communication technology must be open, flexible, scalable, knowledge-based and service-oriented as well as secure and safe. METHODS For enabling semantic interoperability, a unified process for defining and implementing the architecture, i.e. structure and functions of the cooperating systems' components, as well as the approach for knowledge representation, i.e. the used information and its interpretation, algorithms, etc. have to be defined in a harmonized way. Deploying the Generic Component Model, systems and their components, underlying concepts and applied constraints must be formally modeled, strictly separating platform-independent from platform-specific models. RESULTS As HL7 Version 3 claims to represent the most successful standard for semantic interoperability, HL7 has been analyzed regarding the requirements for model-driven, service-oriented design of semantic interoperable information systems, thereby moving from a communication to an architecture paradigm. The approach is compared with advanced architectural approaches for information systems such as OMG's CORBA 3 or EHR systems such as GEHR/openEHR and CEN EN 13606 Electronic Health Record Communication. CONCLUSION HL7 Version 3 is maturing towards an architectural approach for semantic interoperability. Despite current differences, there is a close collaboration between the teams involved guaranteeing a convergence between competing approaches.
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Affiliation(s)
- B G M E Blobel
- eHealth Competence Center, University of Regensburg Medical Center, 93042 Regensburg, Germany.
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Garms-Homolová V, Engel K. Verfahren zur wirksamen Kontrolle der Pflegedokumentation und Pflegeplanung. Gesundheitswesen 2005. [DOI: 10.1055/s-2005-920514] [Citation(s) in RCA: 0] [Impact Index Per Article: 0] [Reference Citation Analysis] [What about the content of this article? (0)] [Track Full Text] [Journal Information] [Subscribe] [Scholar Register] [Indexed: 10/28/2022]
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Schories B, Engel K, Dörken B, Gossen M, Bommert K. Characterization of apoptosis-induced Mcm3 and Cdc6 cleavage reveals a proapoptotic effect for one Mcm3 fragment. Cell Death Differ 2005; 11:940-2. [PMID: 15002044 DOI: 10.1038/sj.cdd.4401411] [Citation(s) in RCA: 16] [Impact Index Per Article: 0.8] [Reference Citation Analysis] [What about the content of this article? (0)] [MESH Headings] [Track Full Text] [Journal Information] [Subscribe] [Scholar Register] [Indexed: 11/09/2022] Open
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Affiliation(s)
- K Engel
- Hautklinik der Albert-Ludwigs-Universität Freiburg
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Engel K. Das Resident Assessment Instrument (RAI) – Anwendung des Instrumentes als Qualitätsinstrument in der Pflege. Gesundheitswesen 2004. [DOI: 10.1055/s-2004-833756] [Citation(s) in RCA: 0] [Impact Index Per Article: 0] [Reference Citation Analysis] [What about the content of this article? (0)] [Track Full Text] [Journal Information] [Subscribe] [Scholar Register] [Indexed: 10/19/2022]
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Abstract
OBJECTIVE In previous studies of the renal response to acute NH4Cl acidosis no correlation was found between systemic acid-base status and the traditionally used quantity, renal net acid excretion (NAE). If NAE is to be considered a physiologically meaningful quantity then this is surprising, as the extracellular acid-base status would be expected to be the key physiological trigger for renal NAE. The object of this study was to investigate the renal response to acute non-carbonic acid loading using a quantitative organ physiological approach. MATERIAL AND METHODS Five-h NH4Cl loading studies were performed in 10 healthy men using a randomized, placebo-controlled, crossover design. Arterialized capillary blood, serum and urine were collected hourly during the loading studies for the measurement of electrolytes and acid-base status. Concentrations of non-metabolizable base (NB) and acid (NA) were calculated from measured concentrations of non-metabolizable ions according to Kildeberg. RESULTS In the steady state (placebo) the rate of renal excretion of NA (=-NB) was close to zero, indicating that the net extrarenal input of NA (endogeneous production, gastrointestinal absorption. skeletal release, etc.) was likewise about zero. An inverse correlation was found between blood pH and the rate of renal excretion of NA. Only a small amount of the acid load (approximately 8%) was excreted during the 5-h study period and this was accompanied by massive calciuria, indicating that mobilization of NB from bone contributed substantially to the current net extrarenal NA input. CONCLUSION From a physiological point of view, NB can be regarded as the actual substrate for renal acid-base control, and measurement of renal turnover of NB may give a more precise description of renal acid-base metabolism during acid loading than previously described methods.
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Affiliation(s)
- P J Osther
- Centre for Kidney Stones and Endourology, Department of Urology, Fredericia Hospital, Fredericia, Denmark.
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Planche T, Dzeing A, Emmerson AC, Onanga M, Kremsner PG, Engel K, Kombila M, Ngou-Milama E, Krishna S. Plasma glutamine and glutamate concentrations in Gabonese children with Plasmodium falciparum infection. QJM 2002; 95:89-97. [PMID: 11861956 DOI: 10.1093/qjmed/95.2.89] [Citation(s) in RCA: 23] [Impact Index Per Article: 1.0] [Reference Citation Analysis] [What about the content of this article? (0)] [Affiliation(s)] [Abstract] [MESH Headings] [Track Full Text] [Journal Information] [Submit a Manuscript] [Subscribe] [Scholar Register] [Indexed: 11/14/2022] Open
Abstract
BACKGROUND Low plasma glutamine levels in critical illness, neonates and burns patients are associated with poor outcome and increased risk of intercurrent infection. AIM To investigate the relationship between plasma glutamine/glutamate levels and severity/outcome of malaria. DESIGN Two-hospital prospective study, with both febrile and healthy controls. METHODS We measured plasma glutamine and glutamate concentrations in 239 Gabonese patients: 145 children with malaria (86 with severe, 36 with moderate and 23 with uncomplicated disease), 42 healthy children, 44 febrile controls and eight healthy adults, and related findings to conventional markers of disease severity such as plasma lactate. RESULTS Median (IQR) plasma glutamine was lower in uncomplicated falciparum malaria and in moderate malaria than in healthy controls: 353 (287-474) and 379 (293-448) vs. 485 (428-531) micromol/l, respectively; p<0.01 for both malaria groups vs. controls. In contrast, plasma glutamine was within the normal range in those with severe malaria and in febrile control children: 431 (342-525) and 472 (338-547) micromol/l, respectively. Furthermore, plasma glutamine was significantly higher in the children who died with malaria than in survivors: 514 (374-813) (n=12) vs. 399 (316-475) micromol/l (n=133), respectively; p=0.001. There were no significant differences in plasma glutamate concentrations between any of the study groups. DISCUSSION In severe malaria, there was a positive correlation between plasma glutamine and lactate levels (p=0.009, r=0.281). This correlation may reflect impaired gluconeogenesis. Glutamine supplementation is probably not justified in severe P. falciparum infection.
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Affiliation(s)
- T Planche
- Department of Infectious Diseases, St George's Hospital Medical School, Cranmer Terrace, London, UK
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Blobel B, Pharow P, Spiegel V, Engel K, Engelbrecht R. Securing interoperability between chip card based medical information systems and health networks. Int J Med Inform 2001; 64:401-15. [PMID: 11734401 DOI: 10.1016/s1386-5056(01)00193-9] [Citation(s) in RCA: 13] [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] [Indexed: 11/17/2022]
Abstract
Health information systems supporting shared care are going to be distributed and interoperable. Dealing with sensitive personal medical information, such information systems have to provide appropriate security services, allowing only authorised users restricted access rights to the patients' data according to the 'need to know' principle. Especially in healthcare, chip card based information systems occur in the shape of patient data cards providing informational self determination and mobility of the users as well as quality, integrity, accountability, and availability of the data stored on the card, thus improving the shared care of patients. The DIABCARD project aims at the implementation and evaluation of a chip card based medical information system (CCMIS) for facilitating communication and co-operation between health professionals in different organisations or departments caring the same patient with diabetes as an example. In co-operation with the EC-funded TrustHealth(2) project, communication and application security services needed are provided like strong authentication as well as the derived services such as authorisation, access control, accountability, confidentiality, etc. The solution is based on Health Professional Cards and Trusted Third Party services. In addition to the secure handling of the patient's chip card and data in DIABCARD workstations, the secure communication between these workstations and related departmental systems has been implemented. Based on the results of this feasibility study, an enhanced security services specification for the DIABCARD example of a CCMIS is provided which will be implemented in the framework of a health network being established in the German federal state Bavaria. Beside the preferred solution of a combination of Patient Identification Card and Patient Data Card, lower level alternatives using card-verifiable certificates are explained in some details. Finally, a few legal issues, future trends like the XML standard set and their implications for the solution presented as well as for distributed health information systems in general are shortly discussed.
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Affiliation(s)
- B Blobel
- Department of Medical Informatics, Medical Faculty, Institute of Biometry and Medical Informatics, Otto-von-Guericke University Magdeburg, Leipziger Str. 44, D-39120 Magdeburg, Saxony-Anhalt, Germany.
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