Author: "Michael Zacharias" - Searchworks@Jio Institute Digital Library Search Results

Your search keyword '"Michael Zacharias"' showing total 120 results

Start Over Author "Michael Zacharias"

120 results on '"Michael Zacharias"'

51. PULMONARY HYPERTENSION AND POST HEART TRANSPLANTATION OUTCOMES: A CONTEMPORARY ANALYSIS

Author: Meisam Moghbelli, Osama Mahmoud, Yasir Abu-Omar, Michael Zacharias, Eiran Z. Gorodeski, Monique Robinson, Marc P. Pelletier, Chantal ElAmm, and Yakov Elgudin
Subjects: Heart transplantation, medicine.medical_specialty, business.industry, Internal medicine, medicine.medical_treatment, Cardiology, Medicine, Cardiology and Cardiovascular Medicine, business, medicine.disease, Pulmonary hypertension
Published: 2021

52. LEFT VENTRICULAR ASSIST DEVICE TYPE AND POST-HEART TRANSPLANT SURVIVAL: A UNOS DATABASE ANALYSIS

Author: Yasir Abu-Omar, Osama Mahmoud, Chantal ElAmm, Yakov Elgudin, Monique Robinson, Marc P. Pelletier, Michael Zacharias, Eiran Z. Gorodeski, and Meisam Moghbelli
Subjects: medicine.medical_specialty, business.industry, Database analysis, Ventricular assist device, medicine.medical_treatment, Internal medicine, Cardiology, Medicine, Cardiology and Cardiovascular Medicine, business
Published: 2021

53. A NOVEL CASE REPORT ON TACROLIMUS INDUCED CHRONIC INFLAMMATORY DEMYELINATING POLYNEUROPATHY AFTER HEART TRANSPLANTATION

Author: Muhammad Wajih Ullah, Michael Zacharias, Ataul Qureshi, and Chander Shekhar
Subjects: Heart transplantation, medicine.medical_specialty, business.industry, Internal medicine, medicine.medical_treatment, medicine, Chronic inflammatory demyelinating polyneuropathy, Cardiology and Cardiovascular Medicine, business, medicine.disease, Gastroenterology, Tacrolimus
Published: 2021

54. Attenuation of TeV γ-rays by the starlight photon field of the host galaxy

Author: Stefan Wagner, Michael Zacharias, and Xuhui Chen
Subjects: Astrophysics::High Energy Astrophysical Phenomena, Astrophysics::Cosmology and Extragalactic Astrophysics, Astrophysics, 01 natural sciences, 0103 physical sciences, ddc:530, Interacting galaxy, 010306 general physics, Blazar, Absorption (electromagnetic radiation), 010303 astronomy & astrophysics, Astrophysics::Galaxy Astrophysics, Physics, Soft photon, Institut für Physik und Astronomie, Astronomy, Astronomy and Astrophysics, Type-cD galaxy, Astrophysics - Astrophysics of Galaxies, Galaxy, Redshift, Extragalactic background light, Space and Planetary Science, ddc:520, Astrophysics::Earth and Planetary Astrophysics, Astrophysics - High Energy Astrophysical Phenomena
Abstract: Monthly notices of the Royal Astronomical Society 465(3), 3767 - 3774 (2017). doi:10.1093/mnras/stw3032, The absorption of TeV $\gamma$-ray photons produced in relativistic jets by surrounding soft photon fields is a long-standing problem of jet physics. In some cases, the most likely emission site close to the central black hole is ruled out because of the high opacity caused by strong optical and infrared photon sources, such as the broad-line region. Mostly neglected for jet modelling is the absorption of $\gamma$-rays in the starlight photon field of the host galaxy. Analysing the absorption for arbitrary locations and observation angles of the $\gamma$-ray emission site within the host galaxy, we find that the distance to the galaxy centre, the observation angle, and the distribution of starlight in the galaxy are crucial for the amount of absorption. We derive the absorption value for a sample of 20 TeV-detected blazars with a redshift $z_r$ < 0.2. The absorption value of the $\gamma$-ray emission located in the galaxy centre may be as high as 20 per cent, with an average value of 6 per cent. This is important in order to determine the intrinsic blazar parameters. We see no significant trends in our sample between the degree of absorption and host properties, such as starlight emissivity, galactic size, half-light radius, and redshift. While the uncertainty of the spectral properties of the extragalactic background light exceeds the effect of absorption by stellar light from the host galaxy in distant objects, the latter is a dominant effect in nearby sources. It may also be revealed in a differential comparison of sources with similar redshifts., Published by Oxford Univ. Press, Oxford
Published: 2016

55. Incidence and risk of heart failure in systemic lupus erythematosus

Author: Michael Zacharias, Sadeer G. Al-Kindi, Guilherme H. Oliveira, Chang H. Kim, Ali D. Askari, and Bochra Jandali
Subjects: Male, Databases, Factual, 030204 cardiovascular system & hematology, 0302 clinical medicine, Risk Factors, Odds Ratio, Prevalence, Lupus Erythematosus, Systemic, Child, skin and connective tissue diseases, Prospective cohort study, Aged, 80 and over, education.field_of_study, Incidence, Incidence (epidemiology), Middle Aged, Prognosis, Child, Preschool, Female, Cardiology and Cardiovascular Medicine, Risk assessment, Adult, medicine.medical_specialty, Adolescent, Population, Risk Assessment, Young Adult, 03 medical and health sciences, Age Distribution, Internal medicine, medicine, Humans, Sex Distribution, education, Aged, Retrospective Studies, Heart Failure, 030203 arthritis & rheumatology, Chi-Square Distribution, Lupus erythematosus, business.industry, Infant, Newborn, Infant, Retrospective cohort study, Odds ratio, medicine.disease, United States, Logistic Models, Relative risk, Immunology, business
Abstract: Although case series suggest a higher burden of cardiovascular risk factors in patients with systemic lupus erythematosus (SLE) compared with the general population, the association between SLE and heart failure (HF) remains undefined. We sought to investigate the incidence and risk of HF in patients with SLE.In April 2016, we performed a retrospective cohort analysis using the Explorys platform, which provides aggregated electronic medical record data from 26 major integrated healthcare systems across the USA from 1999 to present. Demographic and regression analyses were performed to assess the impact of SLE on HF incidence.Among 45 284 540 individuals in the database, we identified 95 400 (0.21%) with SLE and 98 900 (0.22%) with a new diagnosis of HF between May 2015 and April 2016. HF incidence was markedly higher in the SLE group compared with controls (0.97% vs 0.22%, relative risk (RR): 4.6 (95% CI 4.3 to 4.9)), as were other cardiovascular risk factors. In regression analysis, SLE was an independent predictor of HF (adjusted OR: 3.17 (2.63 to 3.83), p0.0001). RR of HF was highest in young males with SLE (65.2 (35.3 to 120.5) for age 20-24), with an overall trend of increasing absolute risk but decreasing RR with advancing age in both sexes. Renal involvement in SLE correlated with earlier and higher incidence of HF.The findings of this study suggest that patients with SLE have significantly higher risk of developing HF and a worse cardiovascular risk profile compared with the general population. These results need to be confirmed by prospective studies.
Published: 2016

56. Predictive Preoperative Characteristics For Right Ventricular Failure After Left Ventricle Assist Device Placement

Author: Safwan Gaznabi, Tracy Schwab, Shu Lan Peng, Yasir Abu Omar, Raul Angel Garcia, Jennifer T. Dahm, Babaljeet Kaur, Kathir Balakumaran, Chantal El Amm, and Michael Zacharias
Subjects: Inotrope, medicine.medical_specialty, Bilirubin, business.industry, medicine.medical_treatment, Incidence (epidemiology), Central venous pressure, Hemodynamics, chemistry.chemical_compound, medicine.anatomical_structure, chemistry, Ventricle, Ventricular assist device, Internal medicine, medicine, Cardiology, Cardiology and Cardiovascular Medicine, business, Destination therapy
Abstract: Introduction The current literature reports a 10-40% occurrence rate of right ventricular (RV) failure after left ventricular assist device (LVAD) implantation. We assessed our institution's incidence of RV failure after LVAD implantation to determine specific predictive values for developing RV failure after LVAD implantation. Methods We conducted a retrospective analysis of patients who underwent LVAD implantation from 2013 to 2019 at a single academic hospital. RV failure was defined according to the INTERMACS definition, with elevated central venous pressure (CVP) documented by right atrial pressure > 16mmHg, and manifestations of elevated CVP including renal dysfunction, or elevated bilirubin. Based on the duration of inotropes, severity of RV failure was further risk stratified as mild ( 14 days). Preoperative demographic, hemodynamic, echocardiographic and laboratory characteristics were identified amongst each group. Using patients without RV failure as the control arm, comparisons were made with independent two sample t-tests and multivariate analysis. Results Between 2013 to 2019, there were a total of 136 LVAD implantations at our institution in which 22.1% were as bridge to transplant, and 77.9% as destination therapy. RV failure was diagnosed in 44.1% of patients, in which 14.7% were categorized as mild, 17.7% as moderate, and 11.8% as severe. Preoperative parameters that predicted RV failure after LVAD implantation included right atrial pressure (RAP) > 10mmHg (RR: 1.58, 95% CI: 1.08 to 2.32, p=0.0174), preoperative renal dysfunction with BUN > 20 mg/dL (RR: 2.22, 95% CI: 1.45 to 3.41, p=0.0003) or Cr > 1.3 mg/dL (RR: 1.83, 95% CI: 1.28 to 2.63, p = 0.001) and total bilirubin > 1.5mg/dL (RR: 1.73, 95% CI: 1.21 to 2.46, p=0.0025). Conclusions Postoperative RV failure is a common occurrence after LVAD implantation. We identified that patients with elevated CVP, renal dysfunction and elevated total bilirubin pre operatively are at higher risk for developing RV failure after LVAD, and these patients should have a low threshold for RV support at the time of LVAD surgery.
Published: 2020

57. Population study of Galactic supernova remnants at very high γ-ray energies with H.E.S.S

Author: Christo Venter, H. Iwasaki, Gilles Maurin, Q. Piel, J. F. Glicenstein, J. Becker Tjus, A. Zech, M. Büchele, Julien Lefaucheur, Nachiketa Chakraborty, R. Liu, C. Mariaud, L. O'c. Drury, A.M. Taylor, C. Perennes, T. Garrigoux, Riaan Steenkamp, Ruben Lopez-Coto, Pierre Brun, M. Lemoine-Goumard, A. Wörnlein, P.-O. Petrucci, H. Ndiyavala, G. Lamanna, S. J. Fegan, A. Djannati-Ataï, N. W. Pekeur, P. Wagner, Alison Mitchell, Dieter Horns, Jean-Pierre Ernenwein, Zorawar Wadiasingh, B. Condon, I. Shilon, M. Seglar-Arroyo, Jan Conrad, Marco Padovani, Clemens Hoischen, A. A. Zdziarski, Frank M. Rieger, Johannes Veh, D. Gottschall, D. A. Sanchez, J. Hawkes, Anne Lemiere, Gavin Rowell, M. Bryan, R. C. G. Chaves, E. O. Angüner, Reinhard Schlickeiser, D. Zaborov, D. Jankowsky, Monica Barnard, A. S. Seyffert, Axel Donath, R. de los Reyes, A. W. Chen, M. Tluczykont, D. Fernandez, V. Poireau, Cameron B Rulten, C. Romoli, K. Morå, F. Gaté, Felix Spanier, I. Jung-Richardt, Manuel Meyer, H. Abdalla, Christian Stegmann, I. Oya, Stefan Wagner, Yasunobu Uchiyama, D. Wouters, M. A. Kastendieck, G. Vasileiadis, Nu. Komin, Jim Hinton, Y. A. Gallant, Fabian Schüssler, Matteo Cerruti, Stefan Ohm, Markus Holler, Felix Jankowsky, J. Decock, M. Mayer, S. Pita, Dmitry Khangulyan, Dorit Glawion, E. Moulin, Tomasz Bulik, S. Nakashima, J. Zorn, Robert Wagner, Thomas Lohse, L. Mohrmann, Felix Aharonian, L. Dirson, C. Farnier, Ramin Marx, E. Leser, M. Panter, U. Katz, Stefano Gabici, J. Dyks, C. van Rensburg, Werner Hofmann, G. Emery, Samar Safi-Harb, Thomas Vuillaume, B. Khélifi, S. Saito, Justine Devin, M. Lorentz, S. Bonnefoy, Constantin Steppa, M. Füßling, S. Eschbach, Jacek Niemiec, G. Hermann, Regis Terrier, Stefan Klepser, A. Balzer, Heinrich J. Völk, M. Mohamed, Olaf Reimer, P. P. Krüger, F. Voisin, D. Klochkov, Alexandre Marcowith, D.A. Prokhorov, M. Renaud, F. Zefi, D. Kerszberg, Rachel Simoni, Helen Poon, M. Jingo, R. D. Parsons, D. J. van der Walt, L. Oakes, J. Bolmont, I. Sushch, A. Ivascenko, R. Blackwell, S. Colafrancesco, Michael Backes, H. Prokoph, Masanori Arakawa, Gianluca Giavitto, V. Marandon, K. Dutson, Thomas Murach, Joachim Hahn, J. Lau, M. Settimo, Andreas Quirrenbach, Sami Caroff, Włodek Kluźniak, M. Capasso, S. Krakau, V. Sahakian, P. Bordas, Michael Zacharias, F. Niederwanger, J. P. Lees, H. Odaka, Tim Holch, S. Raab, A. Abramowski, G. Heinzelmann, N. Maxted, Krzysztof Katarzynski, A. Jacholkowska, Naomi Tsuji, Tanya Edwards, K. Kosack, Konrad Bernlöhr, Jacco Vink, Catherine Boisson, L. Tibaldo, D. Berge, Christoph Deil, Sabrina Casanova, Gerard Fontaine, G. Pelletier, B. Peyaud, Ullrich Schwanke, G. Pühlhofer, Johan Bregeon, J.-P. Tavernet, Kleopas Shiningayamwe, R. J. White, A. Reimer, A. Viana, Domenico Tiziani, D. Malyshev, Łukasz Stawarz, S. Bernhard, B. van Soelen, Michal Ostrowski, B. Rudak, J.-P. Lenain, F. Ait Benkhali, P. T. O'Brien, M. V. Fernandes, Manami Sasaki, S. Schwemmer, Andrea Santangelo, Gilles Henri, C. van Eldik, Stefan Funk, Alicja Wierzcholska, Marek Jamrozy, Helene Sol, B. Giebels, R. J. Tuffs, L. Jouvin, Iryna Lypova, Yvonne Becherini, K. Egberts, J. Chevalier, R. Rauth, Thomas Tavernier, N. Shafi, Natalia Żywucka, M. de Naurois, Ruizhi Yang, Tadayuki Takahashi, A. Schulz, Isak Delberth Davids, A. Fiasson, Roberta Zanin, P. Willmann, C. Trichard, P. J. Meintjes, A. Ziegler, H. Laffon, M. Arrieta, P. deWilt, J. King, Marion Spir-Jacob, Maria Haupt, Michelle Tsirou, L. Rinchiuso, Rafal Moderski, A. Carosi, Francois Brun, P. Vincent, M.-H. Grondin, Markus Böttcher, M. Katsuragawa, Pierre-Henri Aubert, M. Kraus, Michael Punch, Laboratoire Univers et Théories ( LUTH ), Institut national des sciences de l'Univers ( INSU - CNRS ) -Observatoire de Paris-Université Paris Diderot - Paris 7 ( UPD7 ) -Centre National de la Recherche Scientifique ( CNRS ), Laboratoire d'Annecy de Physique des Particules ( LAPP/Laboratoire d'Annecy-le-Vieux de Physique des Particules ), Institut National de Physique Nucléaire et de Physique des Particules du CNRS ( IN2P3 ) -Université Savoie Mont Blanc ( USMB [Université de Savoie] [Université de Chambéry] ) -Centre National de la Recherche Scientifique ( CNRS ), Laboratoire de Physique Nucléaire et de Hautes Énergies ( LPNHE ), Université Pierre et Marie Curie - Paris 6 ( UPMC ) -Institut National de Physique Nucléaire et de Physique des Particules du CNRS ( IN2P3 ) -Université Paris Diderot - Paris 7 ( UPD7 ) -Centre National de la Recherche Scientifique ( CNRS ), Laboratoire Univers et Particules de Montpellier ( LUPM ), Centre National de la Recherche Scientifique ( CNRS ) -Institut National de Physique Nucléaire et de Physique des Particules du CNRS ( IN2P3 ) -Université Montpellier 2 - Sciences et Techniques ( UM2 ) -Université de Montpellier ( UM ), Centre d'Etudes Nucléaires de Bordeaux Gradignan ( CENBG ), Université Sciences et Technologies - Bordeaux 1-Institut National de Physique Nucléaire et de Physique des Particules du CNRS ( IN2P3 ) -Centre National de la Recherche Scientifique ( CNRS ), Institut de Recherches sur les lois Fondamentales de l'Univers ( IRFU ), Commissariat à l'énergie atomique et aux énergies alternatives ( CEA ) -Université Paris-Saclay, Laboratoire Leprince-Ringuet ( LLR ), Institut National de Physique Nucléaire et de Physique des Particules du CNRS ( IN2P3 ) -École polytechnique ( X ) -Centre National de la Recherche Scientifique ( CNRS ), AstroParticule et Cosmologie ( APC - UMR 7164 ), Centre National de la Recherche Scientifique ( CNRS ) -Institut National de Physique Nucléaire et de Physique des Particules du CNRS ( IN2P3 ) -Observatoire de Paris-Université Paris Diderot - Paris 7 ( UPD7 ) -Commissariat à l'énergie atomique et aux énergies alternatives ( CEA ), Centre de Physique des Particules de Marseille ( CPPM ), Centre National de la Recherche Scientifique ( CNRS ) -Institut National de Physique Nucléaire et de Physique des Particules du CNRS ( IN2P3 ) -Aix Marseille Université ( AMU ), Institut de Planétologie et d'Astrophysique de Grenoble ( IPAG ), Observatoire des Sciences de l'Univers de Grenoble ( OSUG ), Université Joseph Fourier - Grenoble 1 ( UJF ) -Institut national des sciences de l'Univers ( INSU - CNRS ) -Centre National de la Recherche Scientifique ( CNRS ) -Université Grenoble Alpes ( UGA ) -Université Joseph Fourier - Grenoble 1 ( UJF ) -Institut national des sciences de l'Univers ( INSU - CNRS ) -Centre National de la Recherche Scientifique ( CNRS ) -Université Grenoble Alpes ( UGA ) -Centre National de la Recherche Scientifique ( CNRS ), HESS, Laboratoire Univers et Théories (LUTH (UMR_8102)), Institut national des sciences de l'Univers (INSU - CNRS)-Observatoire de Paris, Université Paris sciences et lettres (PSL)-Université Paris sciences et lettres (PSL)-Université Paris Diderot - Paris 7 (UPD7)-Centre National de la Recherche Scientifique (CNRS), Laboratoire d'Annecy de Physique des Particules (LAPP), Institut National de Physique Nucléaire et de Physique des Particules du CNRS (IN2P3)-Université Savoie Mont Blanc (USMB [Université de Savoie] [Université de Chambéry])-Centre National de la Recherche Scientifique (CNRS), Laboratoire de Physique Nucléaire et de Hautes Énergies (LPNHE (UMR_7585)), Institut National de Physique Nucléaire et de Physique des Particules du CNRS (IN2P3)-Sorbonne Université (SU)-Centre National de la Recherche Scientifique (CNRS), Laboratoire Univers et Particules de Montpellier (LUPM), Institut National de Physique Nucléaire et de Physique des Particules du CNRS (IN2P3)-Université de Montpellier (UM)-Centre National de la Recherche Scientifique (CNRS), Centre d'Etudes Nucléaires de Bordeaux Gradignan (CENBG), Université Sciences et Technologies - Bordeaux 1 (UB)-Institut National de Physique Nucléaire et de Physique des Particules du CNRS (IN2P3)-Centre National de la Recherche Scientifique (CNRS), Institut de Recherches sur les lois Fondamentales de l'Univers (IRFU), Commissariat à l'énergie atomique et aux énergies alternatives (CEA)-Université Paris-Saclay, Laboratoire Leprince-Ringuet (LLR), Institut National de Physique Nucléaire et de Physique des Particules du CNRS (IN2P3)-École polytechnique (X)-Centre National de la Recherche Scientifique (CNRS), AstroParticule et Cosmologie (APC (UMR_7164)), Commissariat à l'énergie atomique et aux énergies alternatives (CEA)-Institut National de Physique Nucléaire et de Physique des Particules du CNRS (IN2P3)-Observatoire de Paris, Université Paris sciences et lettres (PSL)-Université Paris sciences et lettres (PSL)-Centre National de la Recherche Scientifique (CNRS)-Université Paris Cité (UPCité), Centre de Physique des Particules de Marseille (CPPM), Aix Marseille Université (AMU)-Institut National de Physique Nucléaire et de Physique des Particules du CNRS (IN2P3)-Centre National de la Recherche Scientifique (CNRS), Institut de Planétologie et d'Astrophysique de Grenoble (IPAG), Institut national des sciences de l'Univers (INSU - CNRS)-Centre National d'Études Spatiales [Toulouse] (CNES)-Centre National de la Recherche Scientifique (CNRS)-Observatoire des Sciences de l'Univers de Grenoble (OSUG ), Institut polytechnique de Grenoble - Grenoble Institute of Technology (Grenoble INP )-Institut national des sciences de l'Univers (INSU - CNRS)-Institut national de recherche en sciences et technologies pour l'environnement et l'agriculture (IRSTEA)-Université Savoie Mont Blanc (USMB [Université de Savoie] [Université de Chambéry])-Centre National de la Recherche Scientifique (CNRS)-Université Grenoble Alpes [2016-2019] (UGA [2016-2019])-Institut polytechnique de Grenoble - Grenoble Institute of Technology (Grenoble INP )-Institut national de recherche en sciences et technologies pour l'environnement et l'agriculture (IRSTEA)-Université Savoie Mont Blanc (USMB [Université de Savoie] [Université de Chambéry])-Centre National de la Recherche Scientifique (CNRS)-Université Grenoble Alpes [2016-2019] (UGA [2016-2019]), Université Paris sciences et lettres (PSL)-Université Paris sciences et lettres (PSL)-Centre National de la Recherche Scientifique (CNRS)-Université Paris Diderot - Paris 7 (UPD7), Institut National de Physique Nucléaire et de Physique des Particules du CNRS (IN2P3)-Sorbonne Université (SU)-Centre National de la Recherche Scientifique (CNRS)-Université de Paris (UP), Université Montpellier 2 - Sciences et Techniques (UM2)-Institut National de Physique Nucléaire et de Physique des Particules du CNRS (IN2P3)-Université de Montpellier (UM)-Centre National de la Recherche Scientifique (CNRS), Université Sciences et Technologies - Bordeaux 1-Institut National de Physique Nucléaire et de Physique des Particules du CNRS (IN2P3)-Centre National de la Recherche Scientifique (CNRS), Centre National de la Recherche Scientifique (CNRS)-École polytechnique (X)-Institut National de Physique Nucléaire et de Physique des Particules du CNRS (IN2P3), Université Paris sciences et lettres (PSL)-Université Paris sciences et lettres (PSL)-Centre National de la Recherche Scientifique (CNRS)-Université de Paris (UP), Centre National d'Études Spatiales [Toulouse] (CNES)-Observatoire des Sciences de l'Univers de Grenoble (OSUG ), Institut national des sciences de l'Univers (INSU - CNRS)-Université Savoie Mont Blanc (USMB [Université de Savoie] [Université de Chambéry])-Centre National de la Recherche Scientifique (CNRS)-Institut National de Recherche pour l’Agriculture, l’Alimentation et l’Environnement (INRAE)-Université Grenoble Alpes (UGA)-Institut national des sciences de l'Univers (INSU - CNRS)-Université Savoie Mont Blanc (USMB [Université de Savoie] [Université de Chambéry])-Centre National de la Recherche Scientifique (CNRS)-Institut National de Recherche pour l’Agriculture, l’Alimentation et l’Environnement (INRAE)-Université Grenoble Alpes (UGA), PSL Research University (PSL)-PSL Research University (PSL)-Université Paris Diderot - Paris 7 (UPD7)-Centre National de la Recherche Scientifique (CNRS), Laboratoire d'Annecy de Physique des Particules (LAPP/Laboratoire d'Annecy-le-Vieux de Physique des Particules), Institut National de Physique Nucléaire et de Physique des Particules du CNRS (IN2P3)-Université Paris Diderot - Paris 7 (UPD7)-Sorbonne Université (SU)-Centre National de la Recherche Scientifique (CNRS), Université de Montpellier (UM)-Université Montpellier 2 - Sciences et Techniques (UM2)-Institut National de Physique Nucléaire et de Physique des Particules du CNRS (IN2P3)-Centre National de la Recherche Scientifique (CNRS), Institut National de Physique Nucléaire et de Physique des Particules du CNRS (IN2P3)-Centre National de la Recherche Scientifique (CNRS)-Commissariat à l'énergie atomique et aux énergies alternatives (CEA)-Observatoire de Paris, PSL Research University (PSL)-PSL Research University (PSL)-Université Paris Diderot - Paris 7 (UPD7), Centre National de la Recherche Scientifique (CNRS)-Institut National de Physique Nucléaire et de Physique des Particules du CNRS (IN2P3)-Aix Marseille Université (AMU), Centre National d'Études Spatiales [Toulouse] (CNES)-Université Grenoble Alpes (UGA)-Centre National de la Recherche Scientifique (CNRS)-Institut national des sciences de l'Univers (INSU - CNRS)-Observatoire des Sciences de l'Univers de Grenoble (OSUG), Université Savoie Mont Blanc (USMB [Université de Savoie] [Université de Chambéry])-Institut polytechnique de Grenoble - Grenoble Institute of Technology (Grenoble INP)-Institut national de recherche en sciences et technologies pour l'environnement et l'agriculture (IRSTEA)-Université Joseph Fourier - Grenoble 1 (UJF)-Institut national des sciences de l'Univers (INSU - CNRS)-Centre National de la Recherche Scientifique (CNRS)-Université Grenoble Alpes (UGA)-Université Savoie Mont Blanc (USMB [Université de Savoie] [Université de Chambéry])-Institut polytechnique de Grenoble - Grenoble Institute of Technology (Grenoble INP)-Institut national de recherche en sciences et technologies pour l'environnement et l'agriculture (IRSTEA)-Université Joseph Fourier - Grenoble 1 (UJF)-Centre National de la Recherche Scientifique (CNRS), Centre National de la Recherche Scientifique (CNRS)-Université Savoie Mont Blanc (USMB [Université de Savoie] [Université de Chambéry])-Institut National de Physique Nucléaire et de Physique des Particules du CNRS (IN2P3), Observatoire de Paris, PSL Research University (PSL)-PSL Research University (PSL)-Université Paris Diderot - Paris 7 (UPD7)-Commissariat à l'énergie atomique et aux énergies alternatives (CEA)-Institut National de Physique Nucléaire et de Physique des Particules du CNRS (IN2P3)-Centre National de la Recherche Scientifique (CNRS), Centre National de la Recherche Scientifique (CNRS)-Université de Montpellier (UM)-Institut National de Physique Nucléaire et de Physique des Particules du CNRS (IN2P3)-Université Montpellier 2 - Sciences et Techniques (UM2), Faculty of Science, High Energy Astrophys. & Astropart. Phys (API, FNWI), and API Other Research (FNWI)
Subjects: electron, Milky Way, [ PHYS.ASTR ] Physics [physics]/Astrophysics [astro-ph], Astrophysics::High Energy Astrophysical Phenomena, Hochenergie-Astrophysik Theorie - Abteilung Hofmann, Infrarot-Astrophysik - Abteilung Hofmann, Cosmic ray, magnetic field, Astrophysics, Astrophysics::Cosmology and Extragalactic Astrophysics, Compact star, 7. Clean energy, 01 natural sciences, Luminosity, HESS, 0103 physical sciences, supernova, ddc:530, luminosity, flux: upper limit, cosmic radiation: acceleration, 010303 astronomy & astrophysics, HESS - Abteilung Hofmann, Astrophysics::Galaxy Astrophysics, ISM: supernova remnants, Astroparticle physics, Physics, radio wave, density, energy: high, cosmic radiation: spectrum, 010308 nuclear & particles physics, supernova remnants [ISM], Molecular cloud, shell model, Institut für Physik und Astronomie, Astronomy and Astrophysics, gamma rays: general, Galactic plane, Supernova, gamma ray: VHE, Space and Planetary Science, cosmic radiation: galaxy, ddc:520, Astrophysics - High Energy Astrophysical Phenomena, [PHYS.ASTR]Physics [physics]/Astrophysics [astro-ph], general [gamma rays]
Abstract: 著者人数: H.E.S.S. Collaboration 253名 (所属. 宇宙航空研究開発機構宇宙科学研究所(JAXA)(ISAS): 桂川, 美穂; 中島, 真也; 小高, 裕和; 高橋, 忠幸), Number of authors: H.E.S.S. Collaboration 253 (Affiliation. Institute of Space and Astronautical Science, Japan Aerospace Exploration Agency(JAXA)(ISAS): Katsuragawa, Miho; Nakashima, Shinya; Odaka, Hirokazu; Takahashi, Tadayuki), Accepted: 2018-02-08, 資料番号: SA1170368000
Published: 2018

58. The supernova remnant W49B as seen with H.E.S.S. and Fermi-LAT

Author: M. Jingo, Ullrich Schwanke, I. Jung-Richardt, Markus Holler, Victor Zabalza, A. G. Akhperjanian, Michael Punch, Felix Jankowsky, I. Shilon, K. Dutson, D. Jankowsky, Felix Spanier, N. Shafi, Natalia Żywucka, T. Garrigoux, M. de Naurois, Christian Stegmann, Stefan Wagner, Yasunobu Uchiyama, J. Dyks, Mateusz Janiak, Felix Aharonian, H. Laffon, S. Eschbach, F. Spies, Ruizhi Yang, Marco Padovani, L. Mohrmann, C. van Rensburg, Thomas Tavernier, F. Niederwanger, A. Marcowith, C. Mariaud, Dieter Horns, Clemens Hoischen, A. A. Zdziarski, M. Lorentz, A. Schulz, Christoph Deil, T. Jogler, Gavin Rowell, M. Bryan, D. Zaborov, R. de los Reyes, P. Bordas, Nachiketa Chakraborty, Jacco Vink, Sabrina Casanova, R. Liu, C. Romoli, David Salek, E. Moulin, Tomasz Bulik, G. Lamanna, A. Fiasson, Christo Venter, Daniel Kerszberg, Ruben Lopez-Coto, M. Lemoine-Goumard, J. Lau, A. Jacholkowska, P. Willmann, Francois Brun, M. Chrétien, R. Moderski, A. Zech, B. Condon, Riaan Steenkamp, P. Wagner, M. Mayer, David Sánchez, Jacek Niemiec, Maria Haupt, Olaf Reimer, J. Becker Tjus, Thomas Murach, J. Chevalier, J. Hawkes, Krzysztof Katarzynski, Gilles Fontaine, Frank M. Rieger, Denis Wouters, Julien Lefaucheur, J. Bregeon, P.-O. Petrucci, Guillaume Dubus, L. O'c. Drury, Matteo Cerruti, F. Krayzel, R. Chalme-Calvet, Reinhard Schlickeiser, A. S. Seyffert, W. Kluźniak, D. Klochkov, M.-H. Grondin, N. W. Pekeur, Markus Böttcher, F. Zefi, Alison Mitchell, Zorawar Wadiasingh, D.A. Prokhorov, Michal Ostrowski, R. C. G. Chaves, J.-P. Lenain, Stefan Ohm, K. Morå, R. Blackwell, E. O. Angüner, Werner Hofmann, J. Decock, Pierre-Henri Aubert, S. Pita, J. Jeffrey Carr, Monica Barnard, L. Dirson, S. Öttl, F. Voisin, G. Heinzelmann, S. Colafrancesco, Stefano Gabici, Regis Terrier, Jan Conrad, N. Maxted, Aion Viana, C. Perennes, Nu. Komin, K. Egberts, M. Kraus, B. Peyaud, G. Pelletier, M. Kieffer, P. deWilt, A. Wörnlein, H. Odaka, Andrew M. Taylor, Stefan Funk, Alicja Wierzcholska, Ramin Marx, M. Panter, J. King, F. Ait Benkhali, Manami Sasaki, U. Katz, S. Schwemmer, R. J. Tuffs, S. J. Fegan, A. Djannati-Ataï, Andrea Santangelo, L. Tibaldo, M. Füßling, F. Schüssler, A. Balzer, R. J. White, Marek Jamrozy, Helene Sol, Domenico Tiziani, C. Trichard, I. D. Davids, Olivier Hervet, C. B. Rulten, P. J. Meintjes, Mariangela Settimo, Pierre Brun, Y. Cui, Rachel Simoni, Helen Poon, Joachim Hahn, M. Capasso, A. Ziegler, S. Krakau, V. Sahakian, C. Boisson, C. Farnier, M. Gajdus, E. Leser, Jean-Pierre Ernenwein, G. Cologna, Daniela Hadasch, B. Khélifi, G. Hermann, Johannes Veh, V. Lefranc, Heinrich J. Völk, M. Renaud, S. Bernhard, B. van Soelen, B. Rudak, M. Tluczykont, B. Degrange, H. Abdalla, M. A. Kastendieck, D. Gottschall, Anne Lemiere, Stefan Klepser, G. Vasileiadis, A. Ivascenko, Gilles Maurin, Y. A. Gallant, Łukasz Stawarz, Andreas Quirrenbach, Robert Wagner, Thomas Lohse, Justine Devin, Michael Zacharias, Léa Jouvin, T. Andersson, D. Kolitzus, M. Arrieta, Pascal Vincent, T. Vuillaume, Heike Prokoph, A. Förster, K. Stycz, J. F. Glicenstein, D. J. van der Walt, L. Oakes, J. Bolmont, I. Sushch, Axel Donath, A. W. Chen, Gilles Henri, Q. Piel, R. D. Parsons, F. Stinzing, B. Giebels, Junichiro Katsuta, Gianluca Giavitto, I. Oya, Tanya Edwards, S. Rosier-Lees, G. Spengler, Jim Hinton, M. Mohamed, Michael Backes, W. Domainko, J. P. Lees, S. Raab, A. Abramowski, P. P. Krüger, V. Marandon, D. Berge, Arti Goyal, J.-P. Tavernet, Iryna Lypova, Yvonne Becherini, P. T. O'Brien, Manuel Meyer, M. V. Fernandes, Peter Eger, C. van Eldik, K. Kosack, Konrad Bernlöhr, G. Pühlhofer, A. Reimer, Faculty of Science, High Energy Astrophys. & Astropart. Phys (API, FNWI), API Other Research (FNWI), ATLAS (IHEF, IoP, FNWI), Laboratoire Univers et Théories (LUTH (UMR_8102)), Centre National de la Recherche Scientifique (CNRS)-Université Paris Diderot - Paris 7 (UPD7)-Observatoire de Paris, PSL Research University (PSL)-PSL Research University (PSL)-Institut national des sciences de l'Univers (INSU - CNRS), Laboratoire d'Annecy de Physique des Particules (LAPP/Laboratoire d'Annecy-le-Vieux de Physique des Particules), Institut National de Physique Nucléaire et de Physique des Particules du CNRS (IN2P3)-Université Savoie Mont Blanc (USMB [Université de Savoie] [Université de Chambéry])-Centre National de la Recherche Scientifique (CNRS), Laboratoire de Physique Nucléaire et de Hautes Énergies (LPNHE (UMR_7585)), Institut National de Physique Nucléaire et de Physique des Particules du CNRS (IN2P3)-Université Paris Diderot - Paris 7 (UPD7)-Sorbonne Université (SU)-Centre National de la Recherche Scientifique (CNRS), Laboratoire Univers et Particules de Montpellier (LUPM), Université de Montpellier (UM)-Université Montpellier 2 - Sciences et Techniques (UM2)-Institut National de Physique Nucléaire et de Physique des Particules du CNRS (IN2P3)-Centre National de la Recherche Scientifique (CNRS), Centre d'Etudes Nucléaires de Bordeaux Gradignan (CENBG), Université Sciences et Technologies - Bordeaux 1-Institut National de Physique Nucléaire et de Physique des Particules du CNRS (IN2P3)-Centre National de la Recherche Scientifique (CNRS), Institut de Recherches sur les lois Fondamentales de l'Univers (IRFU), Commissariat à l'énergie atomique et aux énergies alternatives (CEA)-Université Paris-Saclay, Centre de Physique des Particules de Marseille (CPPM), Centre National de la Recherche Scientifique (CNRS)-Institut National de Physique Nucléaire et de Physique des Particules du CNRS (IN2P3)-Aix Marseille Université (AMU), Laboratoire Leprince-Ringuet (LLR), Institut National de Physique Nucléaire et de Physique des Particules du CNRS (IN2P3)-École polytechnique (X)-Centre National de la Recherche Scientifique (CNRS), AstroParticule et Cosmologie (APC (UMR_7164)), Observatoire de Paris, PSL Research University (PSL)-PSL Research University (PSL)-Université Paris Diderot - Paris 7 (UPD7)-Commissariat à l'énergie atomique et aux énergies alternatives (CEA)-Institut National de Physique Nucléaire et de Physique des Particules du CNRS (IN2P3)-Centre National de la Recherche Scientifique (CNRS), Institut de Planétologie et d'Astrophysique de Grenoble (IPAG), Centre National d'Études Spatiales [Toulouse] (CNES)-Université Grenoble Alpes (UGA)-Centre National de la Recherche Scientifique (CNRS)-Institut national des sciences de l'Univers (INSU - CNRS)-Observatoire des Sciences de l'Univers de Grenoble (OSUG), Université Savoie Mont Blanc (USMB [Université de Savoie] [Université de Chambéry])-Institut polytechnique de Grenoble - Grenoble Institute of Technology (Grenoble INP)-Institut national de recherche en sciences et technologies pour l'environnement et l'agriculture (IRSTEA)-Université Joseph Fourier - Grenoble 1 (UJF)-Institut national des sciences de l'Univers (INSU - CNRS)-Centre National de la Recherche Scientifique (CNRS)-Université Grenoble Alpes (UGA)-Université Savoie Mont Blanc (USMB [Université de Savoie] [Université de Chambéry])-Institut polytechnique de Grenoble - Grenoble Institute of Technology (Grenoble INP)-Institut national de recherche en sciences et technologies pour l'environnement et l'agriculture (IRSTEA)-Université Joseph Fourier - Grenoble 1 (UJF)-Centre National de la Recherche Scientifique (CNRS), HESS, Institut national des sciences de l'Univers (INSU - CNRS)-Observatoire de Paris, PSL Research University (PSL)-PSL Research University (PSL)-Université Paris Diderot - Paris 7 (UPD7)-Centre National de la Recherche Scientifique (CNRS), Institut National de Physique Nucléaire et de Physique des Particules du CNRS (IN2P3)-Centre National de la Recherche Scientifique (CNRS)-Commissariat à l'énergie atomique et aux énergies alternatives (CEA)-Observatoire de Paris, PSL Research University (PSL)-PSL Research University (PSL)-Université Paris Diderot - Paris 7 (UPD7), Université Paris sciences et lettres (PSL)-Université Paris sciences et lettres (PSL)-Centre National de la Recherche Scientifique (CNRS)-Université Paris Diderot - Paris 7 (UPD7), Laboratoire d'Annecy de Physique des Particules (LAPP), Université Montpellier 2 - Sciences et Techniques (UM2)-Institut National de Physique Nucléaire et de Physique des Particules du CNRS (IN2P3)-Université de Montpellier (UM)-Centre National de la Recherche Scientifique (CNRS), Aix Marseille Université (AMU)-Institut National de Physique Nucléaire et de Physique des Particules du CNRS (IN2P3)-Centre National de la Recherche Scientifique (CNRS), Centre National de la Recherche Scientifique (CNRS)-École polytechnique (X)-Institut National de Physique Nucléaire et de Physique des Particules du CNRS (IN2P3), Université Paris sciences et lettres (PSL)-Université Paris sciences et lettres (PSL)-Commissariat à l'énergie atomique et aux énergies alternatives (CEA)-Université Paris Diderot - Paris 7 (UPD7)-Centre National de la Recherche Scientifique (CNRS)-Institut National de Physique Nucléaire et de Physique des Particules du CNRS (IN2P3), Institut national des sciences de l'Univers (INSU - CNRS)-Centre National d'Études Spatiales [Toulouse] (CNES)-Centre National de la Recherche Scientifique (CNRS)-Observatoire des Sciences de l'Univers de Grenoble (OSUG ), Institut polytechnique de Grenoble - Grenoble Institute of Technology (Grenoble INP )-Institut national des sciences de l'Univers (INSU - CNRS)-Institut national de recherche en sciences et technologies pour l'environnement et l'agriculture (IRSTEA)-Université Savoie Mont Blanc (USMB [Université de Savoie] [Université de Chambéry])-Centre National de la Recherche Scientifique (CNRS)-Université Grenoble Alpes [2016-2019] (UGA [2016-2019])-Institut polytechnique de Grenoble - Grenoble Institute of Technology (Grenoble INP )-Institut national de recherche en sciences et technologies pour l'environnement et l'agriculture (IRSTEA)-Université Savoie Mont Blanc (USMB [Université de Savoie] [Université de Chambéry])-Centre National de la Recherche Scientifique (CNRS)-Université Grenoble Alpes [2016-2019] (UGA [2016-2019]), Université Paris sciences et lettres (PSL)-Université Paris sciences et lettres (PSL)-Université Paris Diderot - Paris 7 (UPD7)-Centre National de la Recherche Scientifique (CNRS), Institut National de Physique Nucléaire et de Physique des Particules du CNRS (IN2P3)-Université de Montpellier (UM)-Centre National de la Recherche Scientifique (CNRS), Université Sciences et Technologies - Bordeaux 1 (UB)-Institut National de Physique Nucléaire et de Physique des Particules du CNRS (IN2P3)-Centre National de la Recherche Scientifique (CNRS), and Commissariat à l'énergie atomique et aux énergies alternatives (CEA)-Institut National de Physique Nucléaire et de Physique des Particules du CNRS (IN2P3)-Observatoire de Paris
Subjects: Astrophysics::High Energy Astrophysical Phenomena, Hochenergie-Astrophysik Theorie - Abteilung Hofmann, Infrarot-Astrophysik - Abteilung Hofmann, FOS: Physical sciences, Cosmic ray, Astrophysics, Astrophysics::Cosmology and Extragalactic Astrophysics, 01 natural sciences, 7. Clean energy, Spectral line, 0103 physical sciences, Binary star, ddc:530, Supernova remnant, 010303 astronomy & astrophysics, HESS - Abteilung Hofmann, Cherenkov radiation, Astrophysics::Galaxy Astrophysics, Astroparticle physics, Physics, High Energy Astrophysical Phenomena (astro-ph.HE), [SDU.ASTR]Sciences of the Universe [physics]/Astrophysics [astro-ph], 010308 nuclear & particles physics, Computer Science::Information Retrieval, supernova remnants [ISM], [SDU.ASTR.HE]Sciences of the Universe [physics]/Astrophysics [astro-ph]/High Energy Astrophysical Phenomena [astro-ph.HE], Institut für Physik und Astronomie, Astronomy and Astrophysics, Supernova, 13. Climate action, Space and Planetary Science, [SDU]Sciences of the Universe [physics], ddc:520, Astrophysics - High Energy Astrophysical Phenomena, general [gamma rays], clouds [ISM], Fermi Gamma-ray Space Telescope
Abstract: The supernova remnant (SNR) W49B originated from a core-collapse supernova that occurred between one and four thousand years ago, and subsequently evolved into a mixed-morphology remnant, which is interacting with molecular clouds (MC). $\gamma$-ray observations of SNR/MC associations are a powerful tool to constrain the origin of Galactic cosmic-rays, as they can probe the acceleration of hadrons through their interaction with the surrounding medium and subsequent emission of non-thermal photons. The detection of a $\gamma$-ray source coincident with W49B at very high energies (VHE; E > 100 GeV) with the H.E.S.S. Cherenkov telescopes is reported together with a study of the source with 5 years of Fermi-LAT high energy $\gamma$-ray (0.06 - 300 GeV) data. The smoothly-connected combined source spectrum, measured from 60 MeV to multi-TeV energies, shows two significant spectral breaks at $304\pm20$ MeV and $8.4_{-2.5}^{+2.2}$ GeV, the latter being constrained by the joint fit from the two instruments. The detected spectral features are similar to those observed in several other SNR/MC associations and are found to be indicative of $\gamma$-ray emission produced through neutral-pion decay., Comment: 10 pages, 6 figures. Accepted for publication in A&A
Published: 2018

59. A search for new supernova remnant shells in the Galactic plane with H.E.S.S

Author: Maria Haupt, Michael Backes, H. Iwasaki, Jacek Niemiec, Axel Donath, A. W. Chen, J. P. Lees, Ramin Marx, M. Panter, U. Katz, Gilles Henri, I. Oya, Tim Holch, Olaf Reimer, M.-H. Grondin, Nachiketa Chakraborty, K. Dutson, Markus Böttcher, F. Spies, S. Raab, A. Abramowski, G. Spengler, Thomas Tavernier, Naomi Tsuji, M. Mohamed, Nu. Komin, L. Jouvin, Włodek Kluźniak, G. Cologna, Rafal Moderski, S. Bonnefoy, P. T. O'Brien, M. V. Fernandes, W. Domainko, J. Carr, Matteo Cerruti, C. van Eldik, Gerard Fontaine, M. Jingo, Yasuo Fukui, Emmanuel Moulin, G. Lamanna, Konrad Bernlöhr, Clemens Hoischen, A. A. Zdziarski, G. Pühlhofer, Thomas Murach, Ullrich Schwanke, A. Reimer, Manuel Meyer, Arache Djannati-Ataï, M. Katsuragawa, Pierre-Henri Aubert, K. Egberts, Anne Lemiere, Heinrich J. Völk, M. Renaud, B. Giebels, H. Prokoph, Victor Zabalza, Christoph Deil, F. Niederwanger, C. Trichard, A. G. Akhperjanian, F. Zefi, M. Kraus, I. D. Davids, P. J. Meintjes, Y. Cui, Werner Hofmann, Tadayuki Takahashi, G. Pelletier, B. Peyaud, R. C. G. Chaves, E. O. Angüner, A. Ziegler, R. Liu, Jacco Vink, H. Laffon, Alexandre Marcowith, P. deWilt, Robert Wagner, Thomas Lohse, Stefan Klepser, I. Shilon, K. Morå, Sabrina Casanova, F. Ait Benkhali, J. King, M. Füßling, Ruben Lopez-Coto, Manami Sasaki, M. Lemoine-Goumard, S. Schwemmer, A. Balzer, D. Klochkov, P. Bordas, J. Chevalier, Stefan Ohm, A. Ivascenko, D. Berge, S. Pita, P. Wagner, M. Gajdus, Michael Punch, Andrea Santangelo, Marek Jamrozy, T. Andersson, D. Kolitzus, R. Blackwell, C. Farnier, Michal Ostrowski, Helene Sol, E. Leser, Stefano Gabici, Thomas Vuillaume, S. Nakashima, P. Eger, M. Arrieta, S. Saito, Aya Bamba, C. Romoli, J. Hawkes, A. Förster, Hidetoshi Sano, J.-P. Tavernet, J.-P. Lenain, M. Capasso, J. Dyks, Christo Venter, Andrew M. Taylor, D. Jankowsky, Aion Viana, Christian Stegmann, Stefan Wagner, Q. Piel, Johan Bregeon, Karl Kosack, M. Mayer, Felix Spanier, Arti Goyal, Iryna Lypova, Stefan Funk, Alicja Wierzcholska, Łukasz Stawarz, Yvonne Becherini, B. Khélifi, G. Hermann, Yasunobu Uchiyama, S. Krakau, L. Mohrmann, Regis Terrier, F. Schüssler, A. Zech, N. Shafi, Natalia Żywucka, N. Maxted, M. de Naurois, V. Sahakian, L. Oakes, R. J. White, V. Lefranc, J. Bolmont, I. Sushch, M. Janiak, C. van Rensburg, S. Bernhard, Francois Brun, B. van Soelen, B. Rudak, Dieter Horns, S. Richter, D. A. Sanchez, T. Garrigoux, P. Vincent, Joachim Hahn, B. Degrange, R. J. Tuffs, Frank M. Rieger, M. Seglar-Arroyo, Domenico Tiziani, Andreas Quirrenbach, M. Lorentz, Gilles Maurin, Riaan Steenkamp, H. Abdalla, D. Gottschall, D. Kerszberg, M. A. Kastendieck, K. Stycz, Michael Zacharias, C. Mariaud, J. Becker Tjus, Ruizhi Yang, G. Vasileiadis, Denis Wouters, Rachel Simoni, Helen Poon, J. Decock, P.-O. Petrucci, Masanori Arakawa, F. Voisin, J. F. Glicenstein, N. W. Pekeur, A. Schulz, S. Colafrancesco, D.A. Prokhorov, Cameron B Rulten, I. Jung-Richardt, A. Fiasson, Roberta Zanin, S. Öttl, Marco Padovani, Jim Hinton, P. Willmann, Dmitry Khangulyan, A. S. Seyffert, D. J. van der Walt, Gavin Rowell, M. Bryan, O. Hervet, D. Zaborov, Markus Holler, Jan Conrad, Felix Jankowsky, R. de los Reyes, A. Jacholkowska, G. Heinzelmann, Tanya Edwards, Felix Aharonian, David Salek, Tomasz Bulik, S. Eschbach, Julien Lefaucheur, M. Coffaro, R. D. Parsons, Alison Mitchell, Zorawar Wadiasingh, B. Condon, Gianluca Giavitto, Monica Barnard, M. Settimo, L. Tibaldo, H. Odaka, Reinhard Schlickeiser, Pierre Brun, Jean-Pierre Ernenwein, L. Dirson, Johannes Veh, M. Tluczykont, Y. A. Gallant, Justine Devin, J. Lau, Satoshi Yoshiike, Krzysztof Katarzynski, Catherine Boisson, T. Jogler, P. P. Krüger, M. Büchele, C. Perennes, A. Wörnlein, L. O. 'C. Drury, S. J. Fegan, V. Marandon, Laboratoire Univers et Théories (LUTH (UMR_8102)), Centre National de la Recherche Scientifique (CNRS)-Université Paris Diderot - Paris 7 (UPD7)-Observatoire de Paris, PSL Research University (PSL)-PSL Research University (PSL)-Institut national des sciences de l'Univers (INSU - CNRS), Laboratoire d'Annecy de Physique des Particules (LAPP/Laboratoire d'Annecy-le-Vieux de Physique des Particules), Institut National de Physique Nucléaire et de Physique des Particules du CNRS (IN2P3)-Université Savoie Mont Blanc (USMB [Université de Savoie] [Université de Chambéry])-Centre National de la Recherche Scientifique (CNRS), Laboratoire de Physique Nucléaire et de Hautes Énergies (LPNHE (UMR_7585)), Institut National de Physique Nucléaire et de Physique des Particules du CNRS (IN2P3)-Université Paris Diderot - Paris 7 (UPD7)-Sorbonne Université (SU)-Centre National de la Recherche Scientifique (CNRS), Laboratoire Univers et Particules de Montpellier (LUPM), Université Montpellier 2 - Sciences et Techniques (UM2)-Institut National de Physique Nucléaire et de Physique des Particules du CNRS (IN2P3)-Université de Montpellier (UM)-Centre National de la Recherche Scientifique (CNRS), Centre d'Etudes Nucléaires de Bordeaux Gradignan (CENBG), Université Sciences et Technologies - Bordeaux 1-Institut National de Physique Nucléaire et de Physique des Particules du CNRS (IN2P3)-Centre National de la Recherche Scientifique (CNRS), Institut de Recherches sur les lois Fondamentales de l'Univers (IRFU), Commissariat à l'énergie atomique et aux énergies alternatives (CEA)-Université Paris-Saclay, Centre de Physique des Particules de Marseille (CPPM), Centre National de la Recherche Scientifique (CNRS)-Institut National de Physique Nucléaire et de Physique des Particules du CNRS (IN2P3)-Aix Marseille Université (AMU), Laboratoire Leprince-Ringuet (LLR), Institut National de Physique Nucléaire et de Physique des Particules du CNRS (IN2P3)-École polytechnique (X)-Centre National de la Recherche Scientifique (CNRS), AstroParticule et Cosmologie (APC (UMR_7164)), Observatoire de Paris, PSL Research University (PSL)-PSL Research University (PSL)-Université Paris Diderot - Paris 7 (UPD7)-Commissariat à l'énergie atomique et aux énergies alternatives (CEA)-Institut National de Physique Nucléaire et de Physique des Particules du CNRS (IN2P3)-Centre National de la Recherche Scientifique (CNRS), Institut de Planétologie et d'Astrophysique de Grenoble (IPAG), Centre National d'Études Spatiales [Toulouse] (CNES)-Université Grenoble Alpes (UGA)-Centre National de la Recherche Scientifique (CNRS)-Institut national des sciences de l'Univers (INSU - CNRS)-Observatoire des Sciences de l'Univers de Grenoble (OSUG), Université Savoie Mont Blanc (USMB [Université de Savoie] [Université de Chambéry])-Institut polytechnique de Grenoble - Grenoble Institute of Technology (Grenoble INP)-Institut national de recherche en sciences et technologies pour l'environnement et l'agriculture (IRSTEA)-Université Joseph Fourier - Grenoble 1 (UJF)-Institut national des sciences de l'Univers (INSU - CNRS)-Centre National de la Recherche Scientifique (CNRS)-Université Grenoble Alpes (UGA)-Université Savoie Mont Blanc (USMB [Université de Savoie] [Université de Chambéry])-Institut polytechnique de Grenoble - Grenoble Institute of Technology (Grenoble INP)-Institut national de recherche en sciences et technologies pour l'environnement et l'agriculture (IRSTEA)-Université Joseph Fourier - Grenoble 1 (UJF)-Centre National de la Recherche Scientifique (CNRS), H.E.S.S., Institut national des sciences de l'Univers (INSU - CNRS)-Observatoire de Paris, PSL Research University (PSL)-PSL Research University (PSL)-Université Paris Diderot - Paris 7 (UPD7)-Centre National de la Recherche Scientifique (CNRS), Université de Montpellier (UM)-Université Montpellier 2 - Sciences et Techniques (UM2)-Institut National de Physique Nucléaire et de Physique des Particules du CNRS (IN2P3)-Centre National de la Recherche Scientifique (CNRS), Institut National de Physique Nucléaire et de Physique des Particules du CNRS (IN2P3)-Centre National de la Recherche Scientifique (CNRS)-Commissariat à l'énergie atomique et aux énergies alternatives (CEA)-Observatoire de Paris, PSL Research University (PSL)-PSL Research University (PSL)-Université Paris Diderot - Paris 7 (UPD7), Laboratoire Univers et Théories ( LUTH ), Institut national des sciences de l'Univers ( INSU - CNRS ) -Observatoire de Paris-Université Paris Diderot - Paris 7 ( UPD7 ) -Centre National de la Recherche Scientifique ( CNRS ), Laboratoire d'Annecy de Physique des Particules ( LAPP/Laboratoire d'Annecy-le-Vieux de Physique des Particules ), Institut National de Physique Nucléaire et de Physique des Particules du CNRS ( IN2P3 ) -Université Savoie Mont Blanc ( USMB [Université de Savoie] [Université de Chambéry] ) -Centre National de la Recherche Scientifique ( CNRS ), Laboratoire de Physique Nucléaire et de Hautes Énergies ( LPNHE ), Université Pierre et Marie Curie - Paris 6 ( UPMC ) -Institut National de Physique Nucléaire et de Physique des Particules du CNRS ( IN2P3 ) -Université Paris Diderot - Paris 7 ( UPD7 ) -Centre National de la Recherche Scientifique ( CNRS ), Laboratoire Univers et Particules de Montpellier ( LUPM ), Centre National de la Recherche Scientifique ( CNRS ) -Institut National de Physique Nucléaire et de Physique des Particules du CNRS ( IN2P3 ) -Université Montpellier 2 - Sciences et Techniques ( UM2 ) -Université de Montpellier ( UM ), Centre d'Etudes Nucléaires de Bordeaux Gradignan ( CENBG ), Université Sciences et Technologies - Bordeaux 1-Institut National de Physique Nucléaire et de Physique des Particules du CNRS ( IN2P3 ) -Centre National de la Recherche Scientifique ( CNRS ), Institut de Recherches sur les lois Fondamentales de l'Univers ( IRFU ), Commissariat à l'énergie atomique et aux énergies alternatives ( CEA ) -Université Paris-Saclay, Centre de Physique des Particules de Marseille ( CPPM ), Centre National de la Recherche Scientifique ( CNRS ) -Institut National de Physique Nucléaire et de Physique des Particules du CNRS ( IN2P3 ) -Aix Marseille Université ( AMU ), Laboratoire Leprince-Ringuet ( LLR ), Institut National de Physique Nucléaire et de Physique des Particules du CNRS ( IN2P3 ) -École polytechnique ( X ) -Centre National de la Recherche Scientifique ( CNRS ), AstroParticule et Cosmologie ( APC - UMR 7164 ), Centre National de la Recherche Scientifique ( CNRS ) -Institut National de Physique Nucléaire et de Physique des Particules du CNRS ( IN2P3 ) -Observatoire de Paris-Université Paris Diderot - Paris 7 ( UPD7 ) -Commissariat à l'énergie atomique et aux énergies alternatives ( CEA ), Institut de Planétologie et d'Astrophysique de Grenoble ( IPAG ), Observatoire des Sciences de l'Univers de Grenoble ( OSUG ), Université Joseph Fourier - Grenoble 1 ( UJF ) -Institut national des sciences de l'Univers ( INSU - CNRS ) -Centre National de la Recherche Scientifique ( CNRS ) -Université Grenoble Alpes ( UGA ) -Université Joseph Fourier - Grenoble 1 ( UJF ) -Institut national des sciences de l'Univers ( INSU - CNRS ) -Centre National de la Recherche Scientifique ( CNRS ) -Université Grenoble Alpes ( UGA ) -Centre National de la Recherche Scientifique ( CNRS ), Université Paris sciences et lettres (PSL)-Université Paris sciences et lettres (PSL)-Centre National de la Recherche Scientifique (CNRS)-Université Paris Diderot - Paris 7 (UPD7), Laboratoire d'Annecy de Physique des Particules (LAPP), Institut National de Physique Nucléaire et de Physique des Particules du CNRS (IN2P3)-Sorbonne Université (SU)-Centre National de la Recherche Scientifique (CNRS)-Université de Paris (UP), Aix Marseille Université (AMU)-Institut National de Physique Nucléaire et de Physique des Particules du CNRS (IN2P3)-Centre National de la Recherche Scientifique (CNRS), Centre National de la Recherche Scientifique (CNRS)-École polytechnique (X)-Institut National de Physique Nucléaire et de Physique des Particules du CNRS (IN2P3), Commissariat à l'énergie atomique et aux énergies alternatives (CEA)-Institut National de Physique Nucléaire et de Physique des Particules du CNRS (IN2P3)-Observatoire de Paris, Université Paris sciences et lettres (PSL)-Université Paris sciences et lettres (PSL)-Centre National de la Recherche Scientifique (CNRS)-Université de Paris (UP), Centre National d'Études Spatiales [Toulouse] (CNES)-Observatoire des Sciences de l'Univers de Grenoble (OSUG ), Institut national des sciences de l'Univers (INSU - CNRS)-Université Savoie Mont Blanc (USMB [Université de Savoie] [Université de Chambéry])-Centre National de la Recherche Scientifique (CNRS)-Institut National de Recherche pour l’Agriculture, l’Alimentation et l’Environnement (INRAE)-Université Grenoble Alpes (UGA)-Institut national des sciences de l'Univers (INSU - CNRS)-Université Savoie Mont Blanc (USMB [Université de Savoie] [Université de Chambéry])-Centre National de la Recherche Scientifique (CNRS)-Institut National de Recherche pour l’Agriculture, l’Alimentation et l’Environnement (INRAE)-Université Grenoble Alpes (UGA), Université Paris sciences et lettres (PSL)-Université Paris sciences et lettres (PSL)-Université Paris Diderot - Paris 7 (UPD7)-Centre National de la Recherche Scientifique (CNRS), Institut National de Physique Nucléaire et de Physique des Particules du CNRS (IN2P3)-Sorbonne Université (SU)-Centre National de la Recherche Scientifique (CNRS), Institut National de Physique Nucléaire et de Physique des Particules du CNRS (IN2P3)-Université de Montpellier (UM)-Centre National de la Recherche Scientifique (CNRS), Université Sciences et Technologies - Bordeaux 1 (UB)-Institut National de Physique Nucléaire et de Physique des Particules du CNRS (IN2P3)-Centre National de la Recherche Scientifique (CNRS), Université Paris sciences et lettres (PSL)-Université Paris sciences et lettres (PSL)-Centre National de la Recherche Scientifique (CNRS)-Université Paris Cité (UPCité), Institut national des sciences de l'Univers (INSU - CNRS)-Centre National d'Études Spatiales [Toulouse] (CNES)-Centre National de la Recherche Scientifique (CNRS)-Observatoire des Sciences de l'Univers de Grenoble (OSUG ), Institut polytechnique de Grenoble - Grenoble Institute of Technology (Grenoble INP )-Institut national des sciences de l'Univers (INSU - CNRS)-Institut national de recherche en sciences et technologies pour l'environnement et l'agriculture (IRSTEA)-Université Savoie Mont Blanc (USMB [Université de Savoie] [Université de Chambéry])-Centre National de la Recherche Scientifique (CNRS)-Université Grenoble Alpes [2016-2019] (UGA [2016-2019])-Institut polytechnique de Grenoble - Grenoble Institute of Technology (Grenoble INP )-Institut national de recherche en sciences et technologies pour l'environnement et l'agriculture (IRSTEA)-Université Savoie Mont Blanc (USMB [Université de Savoie] [Université de Chambéry])-Centre National de la Recherche Scientifique (CNRS)-Université Grenoble Alpes [2016-2019] (UGA [2016-2019]), Faculty of Science, High Energy Astrophys. & Astropart. Phys (API, FNWI), API Other Research (FNWI), and ATLAS (IHEF, IoP, FNWI)
Subjects: accelerator, Milky Way, [ PHYS.ASTR ] Physics [physics]/Astrophysics [astro-ph], Astrophysics::High Energy Astrophysical Phenomena, leptonic, Population, Hochenergie-Astrophysik Theorie - Abteilung Hofmann, Infrarot-Astrophysik - Abteilung Hofmann, FOS: Physical sciences, Cosmic ray, Astrophysics, Astrophysics::Cosmology and Extragalactic Astrophysics, 01 natural sciences, hadronic, cosmic rays, HESS, 0103 physical sciences, supernova, ddc:530, High Energy Stereoscopic System, Supernova remnant, education, 010303 astronomy & astrophysics, HESS - Abteilung Hofmann, Astrophysics::Galaxy Astrophysics, Computer Science::Information Theory, ISM: supernova remnants, High Energy Astrophysical Phenomena (astro-ph.HE), Astroparticle physics, Physics, education.field_of_study, radio wave, particle: relativistic, 010308 nuclear & particles physics, supernova remnants [ISM], Institut für Physik und Astronomie, Astronomy and Astrophysics, Galactic plane, Supernova, Space and Planetary Science, gamma ray, astroparticle physics, cosmic radiation: galaxy, ddc:520, Astrophysics - High Energy Astrophysical Phenomena, [PHYS.ASTR]Physics [physics]/Astrophysics [astro-ph]
Abstract: 著者人数: H.E.S.S. Collaboration 264名 (所属. 宇宙航空研究開発機構宇宙科学研究所(JAXA)(ISAS): 桂川, 美穂; 中島, 真也; 小高, 裕和; 高橋, 忠幸), Number of authors: H.E.S.S. Collaboration 264 (Affiliation. Institute of Space and Astronautical Science, Japan Aerospace Exploration Agency(JAXA)(ISAS): Katsuragawa, Miho; Nakashima, Shinya; Odaka, Hirokazu; Takahashi, Tadayuki), Accepted: 2017-12-11, 資料番号: SA1170364000
Published: 2018

60. Multi-wavelength observations of flaring blazars with ATOM and Fermi-LAT

Author: Omar M. Kurtanidze, Felix Jankowsky, Jean-Philippe Lenain, Markus Böttcher, S. J. Wagner, Alicja Wierzcholska, Michael Zacharias, 29092086 - Zacharias, Michael, and 24420530 - Böttcher, Markus
Subjects: Physics, Astrophysics::High Energy Astrophysical Phenomena, Astrophysics::Instrumentation and Methods for Astrophysics, Multi wavelength, Astrophysics::Cosmology and Extragalactic Astrophysics, Astrophysics, Optical telescope, law.invention, CTA-102, Telescope, law, Atom, Blazar, Fermi Gamma-ray Space Telescope
Abstract: The Automatic Telescope for Optical Monitoring is a 75cm optical telescope located at the H.E.S.S. site in Namibia. Since 2005, it monitors around 250 gamma-ray emitting AGN and has observed numerous blazar flares in several colour bands with multiple measurements during any given night. We present recent flaring events of two FSRQ – 3C 279 and CTA 102 – together with corresponding multi-wavelength data including Fermi-LAT, and examine possible correlations between energy bands.
Published: 2017

61. Monitoring of the FSRQ PKS 1510-089 with H.E.S.S

Author: Alicja Wierzcholska, Michael Zacharias, Stefan Wagner, Heike Prokoph, Mahmoud Mohamed, Felix Jankowsky, David Sanchez, Laboratoire d'Annecy de Physique des Particules (LAPP/Laboratoire d'Annecy-le-Vieux de Physique des Particules), Centre National de la Recherche Scientifique (CNRS)-Université Savoie Mont Blanc (USMB [Université de Savoie] [Université de Chambéry])-Institut National de Physique Nucléaire et de Physique des Particules du CNRS (IN2P3), H.E.S.S., Institut National de Physique Nucléaire et de Physique des Particules du CNRS (IN2P3)-Université Savoie Mont Blanc (USMB [Université de Savoie] [Université de Chambéry])-Centre National de la Recherche Scientifique (CNRS), and Laboratoire d'Annecy de Physique des Particules (LAPP)
Subjects: electron, Astrophysics::High Energy Astrophysical Phenomena, Flux, FOS: Physical sciences, Astrophysics, 01 natural sciences, 7. Clean energy, Radio spectrum, GLAST, VHE, blazar, X-ray, HESS, 0103 physical sciences, Radiative transfer, optical, Blazar, 010303 astronomy & astrophysics, Physics, High Energy Astrophysical Phenomena (astro-ph.HE), radio wave, energy: high, 010308 nuclear & particles physics, quasar: spectrum, Gamma ray, Quasar, acceleration, flux, monitoring, gamma ray, frequency, correlation, Astrophysics - High Energy Astrophysical Phenomena, [PHYS.ASTR]Physics [physics]/Astrophysics [astro-ph], absorption, Fermi Gamma-ray Space Telescope, Radio wave
Abstract: The flat spectrum radio quasar (FSRQ) PKS 1510-089 (z=0.361) is known for its complex multiwavelength behavior. It has been monitored regularly at very high energy (VHE, $E>100\,$GeV) gamma-rays with H.E.S.S. since its discovery in 2009 in order to study the unknown behavior of FSRQs in quiescence at VHE, as well as the flux evolution around flaring events. Given the expected strong cooling of electrons and the absorption of VHE emission within the broad-line region, a detection of PKS 1510-089 at VHE in a quiescent state would be an important result, implying an acceleration and emission region on scales beyond the broad-line region. The H.E.S.S. monitoring has been intensified since 2015 and is complemented by monitoring at high energy ($E>100\,$MeV) gamma-rays with Fermi, at X-rays with Swift-XRT, and at optical frequencies with ATOM. The dense lightcurves allow for the first time detailed comparison studies between these energy bands. The source has been active in several frequency bands for a large fraction of the observation time frames. Yet, we do not find obvious correlations between the VHE and the other bands over the observed time frame indicating a non-trivial interplay of the acceleration, cooling and radiative processes. It also implies a rich variety in flaring behavior, which makes this source difficult to interpret within a unique theoretical framework., To appear in Proceedings of 35th ICRC, Busan (Korea) 2017
Published: 2017

62. Implications of time-dependent injection in relativistic jets

Author: Michael Zacharias
Subjects: Physics, Energy loss, Jet (fluid), Astrophysical jet, Astrophysics::High Energy Astrophysical Phenomena, Astrophysics, Electron, Blazar, Absorption (electromagnetic radiation), Spectral line, Electron distribution
Abstract: Rapid blazar flaring events and their rich behavior require time-dependent modeling. One important approach is time-dependent injection causing non-linear cooling effects, since the inevitable SSC cooling depends on the time-dependent electron distribution function γ˙∝∫γ2n(γ,t)dγ. This results in a collective and faster energy loss of the electrons in the jet, which could explain the extremely short variability times. The most obvious result of the non-linear cooling is the appearance of unique breaks in the time-integrated SED, which would normally be attributed to a complicated electron distribution. The knowledge of the observation time is important to interpret the observed spectra, because of the non-trivial evolution of the time-dependent SED. Intrinsic gamma-gamma absorption processes in the emission region are only of minor importance.
Published: 2017

63. Prospects for Cherenkov Telescope Array Observations of the Young Supernova Remnant RX J1713.7−3946

Author: Csaba Balázs, M. Servillat, F. D'Ammando, D. Nosek, T. Yamamoto, A. Bilinsky, H.-S. Zechlin, Francesco Dazzi, A. Fernández-Barral, Satoshi Yoshiike, Catherine Boisson, Philippe Laporte, K. Nishijima, Yutaka Fujita, T. Armstrong, A. Shalchi, S. Kimura, D. Nakajima, Fuyuki Tokanai, Francesco Longo, S. Pavy, Philip Kaaret, W. van Driel, Gianpiero Tagliaferri, L. Nogués, F. Di Pierro, Wystan Benbow, T. Stolarczyk, Marco Padovani, T. Di Girolamo, Johan Bregeon, J. Rico, R. Wischnewski, A. Sillanpää, T. Grabarczyk, E. Pueschel, P. Blasi, S. D. Vergani, A. De Franco, C. Bonavolontà, J. Prast, J. Zorn, Elisabetta Bissaldi, Giuseppe Malaguti, A. Pe'Er, Stefano Covino, Akira Okumura, Takashi Saito, C. Aramo, Hermine Landt, R. Zanin, E. Fedorova, Shinji Hara, Yutaka Ohira, Petr Janecek, Petar Temnikov, T. B. Humensky, E. Fiandrini, C. Townsley, R. J. White, A. Fiasson, Koji Noda, Takanori Yoshikoshi, Y. Ikeno, Elena Amato, Yasuo Fukui, J. P. Lees, M. Nievas-Rosillo, Vito Conforti, Kazunori Kohri, I. Oya, M. Trifoglio, Gavin Rowell, Jacek Niemiec, Juan Abel Barrio, R. Walter, Stefan Wagner, Teresa Mineo, J. J. Watson, Reiko Orito, Masahiro Teshima, Jim Hinton, A. Pisarski, G. Rodriguez Fernandez, F. De Frondat, Robert Wagner, Pedro L. Luque-Escamilla, G. Morlino, Thomas Lohse, B. Rudak, Olaf Reimer, Josep Martí, Subir Sarkar, Martin White, Johann Cohen-Tanugi, Michiyuki Chikawa, Dusan Mandat, T. Montaruli, M. Mohammed, M. Iori, Oscar Blanch, Giovanni Bonanno, Benjamin Koch, M. A. Lopez, Julien Rousselle, M. Heller, Yusuke Konno, G. Maurin, J. Palacio, S. Gunji, C. Di Giulio, M. Zavrtanik, J.-P. Lenain, Adrian Biland, Michael Backes, Miroslav Filipovic, M. I. Martínez, M. Vazquez Acosta, Nicola Giglietto, J. M. Paredes, G. Fontaine, R. Moderski, A.A. Zdziarski, D. Tescaro, V. Vassiliev, C. van Eldik, H. Siejkowski, Stefan Kimeswenger, Shu Koyama, A. Bonardi, R. Gnatyk, S. Vorobiov, Oleh Petruk, M. Del Santo, Michał Szanecki, C. Delgado, Carole Mundell, Tomasz Szepieniec, Michael G. Burton, Bohdan Hnatyk, M. Capalbi, Kunihito Ioka, Jonathan Granot, Bohdan Novosyadlyj, Petr Schovanek, A. Weinstein, M. Stephan, Vikram V. Dwarkadas, L. Valore, Sabrina Einecke, P. Goldoni, J. Jacquemier, Hiroshi Muraishi, Andreas Quirrenbach, Takeshi Nakamori, Stefan Ohm, G. Busetto, Marcos Santander, A. Wierzcholska, Jaime Rosado, M. Yoshida, M. Huetten, S. Eschbach, Tatsuo Yoshida, Tomasz Bulik, Gino Tosti, Valentina Fioretti, Makoto Sawada, D. Zavrtanik, P. A. Caraveo, Mohamed Rameez, Sylvain Chaty, Nu. Komin, D. Dumas, Michael Zacharias, J. M. Huet, Reshmi Mukherjee, F. Lucarelli, L. Di Venere, Shuta J. Tanaka, F. de Palma, Shiu-Hang Lee, A. W. Chen, A. Giuliani, R. L. C. Starling, V. Beshley, Jonathan S. Lapington, Gilles Ferrand, Giovanni Covone, Rodrigo Nemmen, Tsuyoshi Inoue, R. C. Shellard, P. Cumani, G. Lamanna, Stefan Funk, Michele Doro, Koji Mori, G. Pühlhofer, Hidetoshi Sano, Susumu Inoue, Luis Ángel Tejedor, G. Kukec Mezek, Anderson Caproni, L. Freixas Coromina, M. de Naurois, D. Jankowsky, Yoshiyuki Inoue, Elina Lindfors, Saverio Lombardi, D. della Volpe, Giancarlo Cusumano, Andrea Orlati, S. Mangano, Samar Safi-Harb, Alexandre Marcowith, R. López-Coto, Martin Pohl, J. Lefaucheur, Vincenzo Rizi, Masayuki Tanaka, Shigehiro Nagataki, J. L. Rodriguez, Diego Falceta-Gonçalves, J. E. Ward, Petr Travnicek, I. Sadeh, Dominik Elsässer, P. Wilcox, Tsunefumi Mizuno, Kohta Murase, K. Lalik, M. Ostrowski, Vincenzo Testa, Tsuguya Naito, Matteo Cerruti, N. La Palombara, Yukikatsu Terada, Emmanuel Moulin, A. Balzer, M. Palatka, Samo Stanič, D. D'Urso, Łukasz Stawarz, D. Simone, Giuseppe Romeo, Francesco Giordano, Luca Zampieri, Michiko Ohishi, Giuseppe Leto, J.F. Glicenstein, G. De Cesare, Eleonora Torresi, R. A. Cameron, Katsuaki Asano, Ricardo Graciani, Gernot Maier, Paweł Wójcik, R. A. Ong, Jörg R. Hörandel, Carlo Vigorito, S. P. Wakely, Valerio Vagelli, Andrea Bulgarelli, J. Takeda, S. Brau-Nogué, Garret Cotter, Claudio Melioli, Hiroaki Yamamoto, M. Vrastil, Ryo Yamazaki, G. Maneva, N. Maxted, David A. Williams, K. Kosack, Konrad Bernlöhr, Markus Böttcher, Andreas Zech, Jürgen Knödlseder, Daniel Nieto, Paola Grandi, Maria Concetta Maccarone, Y. Inome, I. Telezhinsky, Fabio Acero, Michael C. B. Ashley, D. A. Sanchez, C. de Lisio, Francisco J. Franco, J. L. Dournaux, M. Kraus, G. Bonnoli, Xian Chen, Massimo Persic, Jonathan Blazek, Giacomo Principe, Louis Antonelli, H. Hakobyan, A. De Angelis, Marek Nikolajuk, F. Schüssler, T. Nagayoshi, P.-O. Petrucci, P. Sangiorgi, N. Sakaki, Anthony M. Brown, S. Tsujimoto, J. J. Rodríguez Vázquez, A. Morselli, B. De Lotto, Juan Carlos Helo, S. Nozaki, M. Takahashi, Lili Yang, H. Schoorlemmer, Catherine Braiding, Justin Vandenbroucke, J. A. Graham, P. Vallania, Stanislav Stefanik, M. Fesquet, Roberto Aloisio, Diego F. Torres, Ciro Bigongiari, C. Díaz, Shohei Yanagita, M. Garczarczyk, Abelardo Moralejo, Hideaki Katagiri, R. de los Reyes Lopez, A. Burtovoi, M. Hussein, Hiroyasu Tajima, M. Prouza, M. Renaud, C. Trichard, M. K. Daniel, Maria Chernyakova, Tarek M. Hassan, A. Ziegler, E. M. de Gouveia Dal Pino, Ll. Font, J. Kocot, Jiri Chudoba, J. P. Amans, Enrico Junior Schioppa, Alessandro Costa, Aya Bamba, A. Förster, F. Arqueros, Jan Ebr, M. Hayashida, A. J. Green, Marc Ribó, Olga Sergijenko, Hidetoshi Kubo, A. Porcelli, Tomohiro Inada, J. Biteau, J. Kushida, Jose Luis Contreras, S. Colafrancesco, Nestor Mirabal, V. Bugaev, R. J. García López, Vitalii Sliusar, I. Jung, Kathrin Egberts, G. Fasola, Maxim V. Barkov, Seiji Masuda, P. Romano, Enrico Cascone, V. I. Zhdanov, Elisa Prandini, Helene Sol, Rodolfo Carosi, S. Vercellone, Manuela Vecchi, German Martinez, A. Gadola, S. Griffiths, Satyendra Thoudam, Département d'Astrophysique (ex SAP) (DAP), Institut de Recherches sur les lois Fondamentales de l'Univers (IRFU), Commissariat à l'énergie atomique et aux énergies alternatives (CEA)-Université Paris-Saclay-Commissariat à l'énergie atomique et aux énergies alternatives (CEA)-Université Paris-Saclay, Laboratoire Univers et Théories (LUTH (UMR_8102)), Institut national des sciences de l'Univers (INSU - CNRS)-Observatoire de Paris, Université Paris sciences et lettres (PSL)-Université Paris sciences et lettres (PSL)-Centre National de la Recherche Scientifique (CNRS)-Université Paris Diderot - Paris 7 (UPD7), Institut de Physique Nucléaire d'Orsay (IPNO), Centre National de la Recherche Scientifique (CNRS)-Institut National de Physique Nucléaire et de Physique des Particules du CNRS (IN2P3)-Université Paris-Sud - Paris 11 (UP11), Institut de recherche en astrophysique et planétologie (IRAP), Institut national des sciences de l'Univers (INSU - CNRS)-Université Toulouse III - Paul Sabatier (UT3), Université Fédérale Toulouse Midi-Pyrénées-Université Fédérale Toulouse Midi-Pyrénées-Observatoire Midi-Pyrénées (OMP), Météo France-Centre National d'Études Spatiales [Toulouse] (CNES)-Université Fédérale Toulouse Midi-Pyrénées-Centre National de la Recherche Scientifique (CNRS)-Institut de Recherche pour le Développement (IRD)-Météo France-Centre National d'Études Spatiales [Toulouse] (CNES)-Centre National de la Recherche Scientifique (CNRS)-Institut de Recherche pour le Développement (IRD)-Centre National de la Recherche Scientifique (CNRS), Laboratoire Univers et Particules de Montpellier (LUPM), Centre National de la Recherche Scientifique (CNRS)-Université de Montpellier (UM)-Institut National de Physique Nucléaire et de Physique des Particules du CNRS (IN2P3)-Université Montpellier 2 - Sciences et Techniques (UM2), Laboratoire Leprince-Ringuet (LLR), Centre National de la Recherche Scientifique (CNRS)-École polytechnique (X)-Institut National de Physique Nucléaire et de Physique des Particules du CNRS (IN2P3), Commissariat à l'énergie atomique et aux énergies alternatives (CEA)-Université Paris-Saclay, Laboratoire d'Annecy de Physique des Particules (LAPP), Institut National de Physique Nucléaire et de Physique des Particules du CNRS (IN2P3)-Université Savoie Mont Blanc (USMB [Université de Savoie] [Université de Chambéry])-Centre National de la Recherche Scientifique (CNRS), Département de Physique des Particules (ex SPP) (DPP), AstroParticule et Cosmologie (APC (UMR_7164)), Commissariat à l'énergie atomique et aux énergies alternatives (CEA)-Institut National de Physique Nucléaire et de Physique des Particules du CNRS (IN2P3)-Observatoire de Paris, Université Paris sciences et lettres (PSL)-Université Paris sciences et lettres (PSL)-Centre National de la Recherche Scientifique (CNRS)-Université de Paris (UP), Laboratoire de Physique Nucléaire et de Hautes Énergies (LPNHE (UMR_7585)), Institut National de Physique Nucléaire et de Physique des Particules du CNRS (IN2P3)-Sorbonne Université (SU)-Centre National de la Recherche Scientifique (CNRS)-Université de Paris (UP), Institut de Planétologie et d'Astrophysique de Grenoble (IPAG), Centre National d'Études Spatiales [Toulouse] (CNES)-Observatoire des Sciences de l'Univers de Grenoble (OSUG ), Institut national des sciences de l'Univers (INSU - CNRS)-Université Savoie Mont Blanc (USMB [Université de Savoie] [Université de Chambéry])-Centre National de la Recherche Scientifique (CNRS)-Institut National de Recherche pour l’Agriculture, l’Alimentation et l’Environnement (INRAE)-Université Grenoble Alpes (UGA)-Institut national des sciences de l'Univers (INSU - CNRS)-Université Savoie Mont Blanc (USMB [Université de Savoie] [Université de Chambéry])-Centre National de la Recherche Scientifique (CNRS)-Institut National de Recherche pour l’Agriculture, l’Alimentation et l’Environnement (INRAE)-Université Grenoble Alpes (UGA), Centre de Physique des Particules de Marseille (CPPM), Aix Marseille Université (AMU)-Institut National de Physique Nucléaire et de Physique des Particules du CNRS (IN2P3)-Centre National de la Recherche Scientifique (CNRS), CTA Consortium, High Energy Astrophys. & Astropart. Phys (API, FNWI), Acero F., Aloisio R., Amans J., Amato E., Antonelli L. A., Aramo C., Armstrong T., Arqueros F., Asano K., Ashley M., Backes M., Balazs C., Balzer A., Bamba A., Barkov M., Barrio J. A., Benbow W., Bernlöhr K., Beshley V., Bigongiari C., Biland A., Bilinsky A., Bissaldi E., Biteau J., Blanch O., Blasi P., Blazek J., Boisson C., Bonanno G., Bonardi A., Bonavolontà C., Bonnoli G., Braiding C., Brau-Nogué S., Bregeon J., Brown A. M., Bugaev V., Bulgarelli A., Bulik T., Burton M., Burtovoi A., Busetto G., Böttcher M., Cameron R., Capalbi M., Caproni A., Caraveo P., Carosi R., Cascone E., Cerruti M., Chaty S., Chen A., Chen X., Chernyakova M., Chikawa M., Chudoba J., Cohen-Tanugi J., Colafrancesco S., Conforti V., Contreras J. L., Costa A., Cotter G., Covino S., Covone G., Cumani P., Cusumano G., D’Ammando F., D’Urso D., Daniel M., Dazzi F., De Angelis A., De Cesare G., De Franco A., De Frondat F., de Gouveia Dal Pino E. M., De Lisio C., de los Reyes Lopez R., De Lotto B., de Naurois M., De Palma F., Del Santo M., Delgado C., della Volpe D., Di Girolamo T., Di Giulio C., Di Pierro F., Di Venere L., Doro M., Dournaux J., Dumas D., Dwarkadas V., Díaz C., Ebr J., Egberts K., Einecke S., Elsässer D., Eschbach S., Falceta-Goncalves D., Fasola G., Fedorova E., Fernández-Barral A., Ferrand G., Fesquet M., Fiandrini E., Fiasson A., Filipovíc M. D., Fioretti V., Font L., Fontaine G., Franco F. J., Coromina L. Freixa, Fujita Y., Fukui Y., Funk S., Förster A., Gadola A., López R. Garcia, Garczarczyk M., Giglietto N., Giordano F., Giuliani A., Glicenstein J., Gnatyk R., Goldoni P., Grabarczyk T., Graciani R., Graham J., Grandi P., Granot J., Green A. J., Griffiths S., Gunji S., Hakobyan H., Hara S., Hassan T., Hayashida M., Heller M., Helo J. C., Hinton J., Hnatyk B., Huet J., Huetten M., Humensky T. B., Hussein M., Hörandel J., Ikeno Y., Inada T., Inome Y., Inoue S., Inoue T., Inoue Y., Ioka K., Iori M., Jacquemier J., Janecek P., Jankowsky D., Jung I., Kaaret P., Katagiri H., Kimeswenger S., Kimura S., Knödlseder J., Koch B., Kocot J., Kohri K., Komin N., Konno Y., Kosack K., Koyama S., Kraus M., Kubo H., Mezek G. Kukec, Kushida J., Palombara N. La, Lalik K., Lamanna G., Landt H., Lapington J., Laporte P., Lee S., Lees J., Lefaucheur J., Lenain J.-P., Leto G., Lindfors E., Lohse T., Lombardi S., Longo F., Lopez M., Lucarelli F., Luque-Escamilla P. L., López-Coto R., Maccarone M. C., Maier G., Malaguti G., Mandat D., Maneva G., Mangano S., Marcowith A., Martí J., Martínez M., Martínez G., Masuda S., Maurin G., Maxted N., Melioli C., Mineo T., Mirabal N., Mizuno T., Moderski R., Mohammed M., Montaruli T., Moralejo A., Mori K., Morlino G., Morselli A., Moulin E., Mukherjee R., Mundell C., Muraishi H., Murase K., Nagataki S., Nagayoshi T., Naito T., Nakajima D., Nakamori T., Nemmen R., Niemiec J., Nieto D., Nievas-Rosillo M., Nikołajuk M., Nishijima K., Noda K., Nogues L., Nosek D., Novosyadlyj B., Nozaki S., Ohira Y., Ohishi M., Ohm S., Okumura A., Ong R. A., Orito R., Orlati A., Ostrowski M., Oya I., Padovani M., Palacio J., Palatka M., Paredes J. M., Pavy S., Pe’Er A., Persic M., Petrucci P., Petruk O., Pisarski A., Pohl M., Porcelli A., Prandini E., Prast J., Principe G., Prouza M., Pueschel E., Pühlhofer G., Quirrenbach A., Rameez M., Reimer O., Renaud M., Ribó M., Rico J., Rizi V., Rodriguez J., Fernandez G. Rodriguez, Vázquez J. J. Rodríguez, Romano P., Romeo G., Rosado J., Rousselle J., Rowell G., Rudak B., Sadeh I., Safi-Harb S., Saito T., Sakaki N., Sanchez D., Sangiorgi P., Sano H., Santander M., Sarkar S., Sawada M., Schioppa E. J., Schoorlemmer H., Schovanek P., Schussler F., Sergijenko O., Servillat M., Shalchi A., Shellard R. C., Siejkowski H., Sillanpää A., Simone D., Sliusar V., Sol H., Stanič S., Starling R., Stawarz Ł., Stefanik S., Stephan M., Stolarczyk T., Szanecki M., Szepieniec T., Tagliaferri G., Tajima H., Takahashi M., Takeda J., Tanaka M., Tanaka S., Tejedor L. A., Telezhinsky I., Temnikov P., Terada Y., Tescaro D., Teshima M., Testa V., Thoudam S., Tokanai F., Torres D. F., Torresi E., Tosti G., Townsley C., Travnicek P., Trichard C., Trifoglio M., Tsujimoto S., Vagelli V., Vallania P., Valore L., van Driel W., van Eldik C., Vandenbroucke J., Vassiliev V., Vecchi M., Vercellone S., Vergani S., Vigorito C., Vorobiov S., Vrastil M., Acosta M. L. Vázquez, Wagner S. J., Wagner R., Wakely S. P., Walter R., Ward J. E., Watson J. J., Weinstein A., White M., White R., Wierzcholska A., Wilcox P., Williams D. A., Wischnewski R., Wojcik P., Yamamoto T., Yamamoto H., Yamazaki R., Yanagita S., Yang L., Yoshida T., Yoshida M., Yoshiike S., Yoshikoshi T., Zacharias M., Zampieri L., Zanin R., Zavrtanik M., Zavrtanik D., Zdziarski A., Zech A., Zechlin H., Zhdanov V., Ziegler A., Zorn J., Acero, F., Aloisio, R., Amans, J., Amato, E., Antonelli, L. A., Aramo, C., Armstrong, T., Arqueros, F., Asano, K., Ashley, M., Backes, M., Balazs, C., Balzer, A., Bamba, A., Barkov, M., Barrio, J. A., Benbow, W., Bernlöhr, K., Beshley, V., Bigongiari, C., Biland, A., Bilinsky, A., Bissaldi, E., Biteau, J., Blanch, O., Blasi, P., Blazek, J., Boisson, C., Bonanno, G., Bonardi, A., Bonavolontà, C., Bonnoli, G., Braiding, C., Brau Nogué, S., Bregeon, J., Brown, A. M., Bugaev, V., Bulgarelli, A., Bulik, T., Burton, M., Burtovoi, A., Busetto, G., Böttcher, M., Cameron, R., Capalbi, M., Caproni, A., Caraveo, P., Carosi, R., Cascone, E., Cerruti, M., Chaty, S., Chen, A., Chen, X., Chernyakova, M., Chikawa, M., Chudoba, J., Cohen Tanugi, J., Colafrancesco, S., Conforti, V., Contreras, J. L., Costa, A., Cotter, G., Covino, S., Covone, G., Cumani, P., Cusumano, G., D’Ammando, F., D’Urso, D., Daniel, M., Dazzi, F., De Angelis, A., De Cesare, G., De Franco, A., De Frondat, F., de Gouveia Dal Pino, E. M., De Lisio, C., de los Reyes Lopez, R., De Lotto, B., de Naurois, M., De Palma, F., Del Santo, M., Delgado, C., della Volpe, D., Di Girolamo, T., Di Giulio, C., Di Pierro, F., Di Venere, L., Doro, M., Dournaux, J., Dumas, D., Dwarkadas, V., Díaz, C., Ebr, J., Egberts, K., Einecke, S., Elsässer, D., Eschbach, S., Falceta Goncalves, D., Fasola, G., Fedorova, E., Fernández Barral, A., Ferrand, G., Fesquet, M., Fiandrini, E., Fiasson, A., Filipovíc, M. D., Fioretti, V., Font, L., Fontaine, G., Franco, F. J., Coromina, L. Freixa, Fujita, Y., Fukui, Y., Funk, S., Förster, A., Gadola, A., López, R. Garcia, Garczarczyk, M., Giglietto, N., Giordano, F., Giuliani, A., Glicenstein, J., Gnatyk, R., Goldoni, P., Grabarczyk, T., Graciani, R., Graham, J., Grandi, P., Granot, J., Green, A. J., Griffiths, S., Gunji, S., Hakobyan, H., Hara, S., Hassan, T., Hayashida, M., Heller, M., Helo, J. C., Hinton, J., Hnatyk, B., Huet, J., Huetten, M., Humensky, T. B., Hussein, M., Hörandel, J., Ikeno, Y., Inada, T., Inome, Y., Inoue, S., Inoue, T., Inoue, Y., Ioka, K., Iori, M., Jacquemier, J., Janecek, P., Jankowsky, D., Jung, I., Kaaret, P., Katagiri, H., Kimeswenger, S., Kimura, S., Knödlseder, J., Koch, B., Kocot, J., Kohri, K., Komin, N., Konno, Y., Kosack, K., Koyama, S., Kraus, M., Kubo, H., Mezek, G. Kukec, Kushida, J., Palombara, N. La, Lalik, K., Lamanna, G., Landt, H., Lapington, J., Laporte, P., Lee, S., Lees, J., Lefaucheur, J., Lenain, J. P., Leto, G., Lindfors, E., Lohse, T., Lombardi, S., Longo, Francesco, Lopez, M., Lucarelli, F., Luque Escamilla, P. L., López Coto, R., Maccarone, M. C., Maier, G., Malaguti, G., Mandat, D., Maneva, G., Mangano, S., Marcowith, A., Martí, J., Martínez, M., Martínez, G., Masuda, S., Maurin, G., Maxted, N., Melioli, C., Mineo, T., Mirabal, N., Mizuno, T., Moderski, R., Mohammed, M., Montaruli, T., Moralejo, A., Mori, K., Morlino, G., Morselli, A., Moulin, E., Mukherjee, R., Mundell, C., Muraishi, H., Murase, K., Nagataki, S., Nagayoshi, T., Naito, T., Nakajima, D., Nakamori, T., Nemmen, R., Niemiec, J., Nieto, D., Nievas Rosillo, M., Nikołajuk, M., Nishijima, K., Noda, K., Nogues, L., Nosek, D., Novosyadlyj, B., Nozaki, S., Ohira, Y., Ohishi, M., Ohm, S., Okumura, A., Ong, R. A., Orito, R., Orlati, A., Ostrowski, M., Oya, I., Padovani, M., Palacio, J., Palatka, M., Paredes, J. M., Pavy, S., Pe’Er, A., Persic, M., Petrucci, P., Petruk, O., Pisarski, A., Pohl, M., Porcelli, A., Prandini, E., Prast, J., Principe, G., Prouza, M., Pueschel, E., Pühlhofer, G., Quirrenbach, A., Rameez, M., Reimer, O., Renaud, M., Ribó, M., Rico, J., Rizi, V., Rodriguez, J., Fernandez, G. Rodriguez, Vázquez, J. J. Rodríguez, Romano, P., Romeo, G., Rosado, J., Rousselle, J., Rowell, G., Rudak, B., Sadeh, I., Safi Harb, S., Saito, T., Sakaki, N., Sanchez, D., Sangiorgi, P., Sano, H., Santander, M., Sarkar, S., Sawada, M., Schioppa, E. J., Schoorlemmer, H., Schovanek, P., Schussler, F., Sergijenko, O., Servillat, M., Shalchi, A., Shellard, R. C., Siejkowski, H., Sillanpää, A., Simone, D., Sliusar, V., Sol, H., Stanič, S., Starling, R., Stawarz, Ł., Stefanik, S., Stephan, M., Stolarczyk, T., Szanecki, M., Szepieniec, T., Tagliaferri, G., Tajima, H., Takahashi, M., Takeda, J., Tanaka, M., Tanaka, S., Tejedor, L. A., Telezhinsky, I., Temnikov, P., Terada, Y., Tescaro, D., Teshima, M., Testa, V., Thoudam, S., Tokanai, F., Torres, D. F., Torresi, E., Tosti, G., Townsley, C., Travnicek, P., Trichard, C., Trifoglio, M., Tsujimoto, S., Vagelli, V., Vallania, P., Valore, L., van Driel, W., van Eldik, C., Vandenbroucke, J., Vassiliev, V., Vecchi, M., Vercellone, S., Vergani, S., Vigorito, C., Vorobiov, S., Vrastil, M., Acosta, M. L. Vázquez, Wagner, S. J., Wagner, R., Wakely, S. P., Walter, R., Ward, J. E., Watson, J. J., Weinstein, A., White, M., White, R., Wierzcholska, A., Wilcox, P., Williams, D. A., Wischnewski, R., Wojcik, P., Yamamoto, T., Yamamoto, H., Yamazaki, R., Yanagita, S., Yang, L., Yoshida, T., Yoshida, M., Yoshiike, S., Yoshikoshi, T., Zacharias, M., Zampieri, L., Zanin, R., Zavrtanik, M., Zavrtanik, D., Zdziarski, A., Zech, A., Zechlin, H., Zhdanov, V., Ziegler, A., Zorn, J., Acero et al, F., PSL Research University (PSL)-PSL Research University (PSL)-Université Paris Diderot - Paris 7 (UPD7)-Centre National de la Recherche Scientifique (CNRS), Université Paris-Sud - Paris 11 (UP11)-Institut National de Physique Nucléaire et de Physique des Particules du CNRS (IN2P3)-Centre National de la Recherche Scientifique (CNRS), Université Toulouse III - Paul Sabatier (UT3), Université Fédérale Toulouse Midi-Pyrénées-Centre National de la Recherche Scientifique (CNRS), Université de Montpellier (UM)-Université Montpellier 2 - Sciences et Techniques (UM2)-Institut National de Physique Nucléaire et de Physique des Particules du CNRS (IN2P3)-Centre National de la Recherche Scientifique (CNRS), Institut National de Physique Nucléaire et de Physique des Particules du CNRS (IN2P3)-École polytechnique (X)-Centre National de la Recherche Scientifique (CNRS), Laboratoire d'Annecy de Physique des Particules (LAPP/Laboratoire d'Annecy-le-Vieux de Physique des Particules), Centre National de la Recherche Scientifique (CNRS)-Université Savoie Mont Blanc (USMB [Université de Savoie] [Université de Chambéry])-Institut National de Physique Nucléaire et de Physique des Particules du CNRS (IN2P3), Observatoire de Paris, PSL Research University (PSL)-PSL Research University (PSL)-Université Paris Diderot - Paris 7 (UPD7)-Commissariat à l'énergie atomique et aux énergies alternatives (CEA)-Institut National de Physique Nucléaire et de Physique des Particules du CNRS (IN2P3)-Centre National de la Recherche Scientifique (CNRS), Institut National de Physique Nucléaire et de Physique des Particules du CNRS (IN2P3)-Université Paris Diderot - Paris 7 (UPD7)-Sorbonne Université (SU)-Centre National de la Recherche Scientifique (CNRS), Centre National d'Études Spatiales [Toulouse] (CNES)-Université Grenoble Alpes (UGA)-Centre National de la Recherche Scientifique (CNRS)-Institut national des sciences de l'Univers (INSU - CNRS)-Observatoire des Sciences de l'Univers de Grenoble (OSUG), Université Savoie Mont Blanc (USMB [Université de Savoie] [Université de Chambéry])-Institut polytechnique de Grenoble - Grenoble Institute of Technology (Grenoble INP)-Institut national de recherche en sciences et technologies pour l'environnement et l'agriculture (IRSTEA)-Université Joseph Fourier - Grenoble 1 (UJF)-Institut national des sciences de l'Univers (INSU - CNRS)-Centre National de la Recherche Scientifique (CNRS)-Université Grenoble Alpes (UGA)-Université Savoie Mont Blanc (USMB [Université de Savoie] [Université de Chambéry])-Institut polytechnique de Grenoble - Grenoble Institute of Technology (Grenoble INP)-Institut national de recherche en sciences et technologies pour l'environnement et l'agriculture (IRSTEA)-Université Joseph Fourier - Grenoble 1 (UJF)-Centre National de la Recherche Scientifique (CNRS), Centre National de la Recherche Scientifique (CNRS)-Institut National de Physique Nucléaire et de Physique des Particules du CNRS (IN2P3)-Aix Marseille Université (AMU), Institut National de Physique Nucléaire et de Physique des Particules du CNRS (IN2P3)-Centre National de la Recherche Scientifique (CNRS)-Commissariat à l'énergie atomique et aux énergies alternatives (CEA)-Observatoire de Paris, PSL Research University (PSL)-PSL Research University (PSL)-Université Paris Diderot - Paris 7 (UPD7), Galaxies, Etoiles, Physique, Instrumentation (GEPI), Université Paris sciences et lettres (PSL)-Université Paris sciences et lettres (PSL)-Université Paris Diderot - Paris 7 (UPD7)-Centre National de la Recherche Scientifique (CNRS), Université de Toulouse (UT)-Université de Toulouse (UT)-Institut national des sciences de l'Univers (INSU - CNRS)-Observatoire Midi-Pyrénées (OMP), Institut de Recherche pour le Développement (IRD)-Université Toulouse III - Paul Sabatier (UT3), Université de Toulouse (UT)-Université de Toulouse (UT)-Institut national des sciences de l'Univers (INSU - CNRS)-Centre National d'Études Spatiales [Toulouse] (CNES)-Centre National de la Recherche Scientifique (CNRS)-Météo-France -Institut de Recherche pour le Développement (IRD)-Institut national des sciences de l'Univers (INSU - CNRS)-Centre National d'Études Spatiales [Toulouse] (CNES)-Centre National de la Recherche Scientifique (CNRS)-Météo-France -Centre National de la Recherche Scientifique (CNRS), Institut National de Physique Nucléaire et de Physique des Particules du CNRS (IN2P3)-Université de Montpellier (UM)-Centre National de la Recherche Scientifique (CNRS), Département de Physique des Particules (ex SPP) (DPhP), Université Paris sciences et lettres (PSL)-Université Paris sciences et lettres (PSL)-Centre National de la Recherche Scientifique (CNRS)-Université Paris Cité (UPCité), Institut National de Physique Nucléaire et de Physique des Particules du CNRS (IN2P3)-Sorbonne Université (SU)-Centre National de la Recherche Scientifique (CNRS), Institut national des sciences de l'Univers (INSU - CNRS)-Centre National d'Études Spatiales [Toulouse] (CNES)-Centre National de la Recherche Scientifique (CNRS)-Observatoire des Sciences de l'Univers de Grenoble (OSUG ), Institut polytechnique de Grenoble - Grenoble Institute of Technology (Grenoble INP )-Institut national des sciences de l'Univers (INSU - CNRS)-Institut national de recherche en sciences et technologies pour l'environnement et l'agriculture (IRSTEA)-Université Savoie Mont Blanc (USMB [Université de Savoie] [Université de Chambéry])-Centre National de la Recherche Scientifique (CNRS)-Université Grenoble Alpes [2016-2019] (UGA [2016-2019])-Institut polytechnique de Grenoble - Grenoble Institute of Technology (Grenoble INP )-Institut national de recherche en sciences et technologies pour l'environnement et l'agriculture (IRSTEA)-Université Savoie Mont Blanc (USMB [Université de Savoie] [Université de Chambéry])-Centre National de la Recherche Scientifique (CNRS)-Université Grenoble Alpes [2016-2019] (UGA [2016-2019]), Acero, F, Aloisio, R, Amans, J, De Lisio, C, Di Girolamo, T, Valore, L, Covone, G, and Al., Et
Subjects: electron, Supernova Remnants, PARTICLE-ACCELERATION, Cherenkov Telescope Array, Astronomy, leptonic, Telescope Array Experiment, pi, Astrophysics, 01 natural sciences, Supernova Remnant, LARGE-AREA TELESCOPE, Spectral line, spectrum, ISM: individual objects, HESS, Supernova remnant, 010303 astronomy & astrophysics, cosmic ray, Physics, cosmic rays gamma rays: ISM ISM: individual objects (RX J1713.7-3946, G347.3-0.5), spatial distribution, Gamma Ray, Cherenkov radiation, MAGNETIC-FIELD, Gamma ray, COSMIC-RAYS, ISM: individual objects (RX J1713.7–3946, G347.3–0.5), Supernova, cosmic rays, gamma rays: ISM, ISM: individual objects (RX J1713.7-3946, G347.3-0.5), Astronomy and Astrophysics, Space and Planetary Science, gamma ray: emission, G347.3–0.5, ComputingMethodologies_DOCUMENTANDTEXTPROCESSING, DIFFUSIVE SHOCK ACCELERATION, Electrónica, Física nuclear, Electricidad, individual objects: RX J1713.7–3946 [ISM], Compton scattering, Gamma Rays, G347.3-0.5), NONTHERMAL, accelerator, X-RAYS, Astrophysics::High Energy Astrophysical Phenomena, INSTABILITY, Cosmic ray, hadronic, GLAST, ISM: individual objects (RX J1713.7-3946, ISM [gamma rays], gas, 0103 physical sciences, supernova, ddc:530, X-ray: emission, GAMMA-RAY EMISSION, AMPLIFICATION, BROAD-BAND EMISSION, MOLECULAR CLOUDS, STREAMING, Astrophysics::Galaxy Astrophysics, Astroparticle physics, 010308 nuclear & particles physics, p: relativistic, Institut für Physik und Astronomie, ASTROFÍSICA, gamma ray: VHE, ddc:520, time dependence, [PHYS.ASTR]Physics [physics]/Astrophysics [astro-ph], RAIOS CÓSMICOS
Abstract: 著者人数: 382名 (JAXA職員: 井上, 芳幸 : 小山, 志勇 : Lee, Shiu-Hang), Accepted: 2017-04-12, 資料番号: SA1170071000
Published: 2017

64. A polarized fast radio burst at low Galactic latitude

Author: M. de Jong, Michael Punch, Mansi M. Kasliwal, T. A. Pritchard, S. Galatà, K. Egberts, S. Loucatos, C. Tönnis, S. Öttl, G. Pelletier, Ivan Felis, Mitchell B. Mickaliger, Jacek Niemiec, G. Cologna, Robert Wagner, A. Gleixner, C. Racca, P. J. Meintjes, Thomas Lohse, Jamie Farnes, Olaf Reimer, F. Ait Benkhali, L. O'c. Drury, P. de Wilt, R. Chalme-Calvet, I. Salvadori, Kay Graf, Karel Melis, A. Vizzoca, I. El Bojaddaini, G. Heinzelmann, C. B. Rulten, Bruny Baret, Heinrich J. Völk, Manami Sasaki, S. Schwemmer, Q. Piel, Andrea Santangelo, Thomas Vuillaume, Guillaume Dubus, A. Jacholkowska, Simon Johnston, J. Chevalier, Julien Lefaucheur, M. Renaud, K. Dutson, F. Spies, D. Dornic, C. Farnier, A. Trovato, E. Leser, Tanya Edwards, Jean-Pierre Macquart, L. Tibaldo, Thomas Murach, C. Lachaud, A. Marinelli, I. D. Davids, Ramin Marx, M. Panter, U. Katz, Silvia Celli, Timothée Grégoire, D. Kiessling, Antoine Kouchner, Marco Padovani, Matthias Kadler, Francois Brun, A. Ivascenko, E. D. Barr, C. W. James, Daniela Hadasch, C. Perrina, Maria Tselengidou, G. Hermann, Regis Terrier, D. Klochkov, Johan Bregeon, W. Kluzniak, M. Kieffer, P. Vincent, Y. Cui, S. Bernhard, L. Stawarz, A. Ziegler, M.C. Bouwhuis, C. Romoli, Dieter Horns, Mateusz Janiak, B. van Soelen, B. Rudak, T. Michael, Nachiketa Chakraborty, Caterina Tiburzi, N. Zywucka, Alison Mitchell, B. Degrange, Santiago Pita, R. Blackwell, Reinhard Schlickeiser, I. Kreykenbohm, Annarita Margiotta, Jutta Schnabel, M. Jingo, R. J. White, Thomas Eberl, H. Laffon, M. Lotze, Christo Venter, Tommaso Chiarusi, M. Anghinolfi, Maura McLaughlin, Zorawar Wadiasingh, B. Condon, D. A. Sanchez, M. Mayer, V. Lefranc, H. Abdalla, M. A. Kastendieck, S. Bourret, G. Vasileiadis, Iryna Lypova, Yvonne Becherini, G. Illuminati, Clemens Hoischen, A. A. Zdziarski, S. Geisselsoder, I. Shilon, E. O. Angüner, Domenico Tiziani, K. Kosack, Konrad Bernlöhr, A. Enzenhöfer, R. Moderski, V. S. Dhillon, Evan Keane, G. Lamanna, Riaan Steenkamp, Matthew Bailes, M. Füssling, A. Zech, V. Van Elewyck, M. Taiuti, J. Decock, Ullrich Schwanke, Monica Barnard, D. Zaborov, O. Kalekin, M. Circella, Y. A. Gallant, N. D. R. Bhat, A. Creusot, Victor Zabalza, Th. Stolarczyk, B. Vallage, N. Maxted, Dominique Lefèvre, L. Dirson, E. Petroff, D. Jankowsky, M.-H. Grondin, C. Perennes, Markus Böttcher, E. Nezri, A. G. Akhperjanian, Maria Haupt, Jürgen Brunner, G. Pühlhofer, S. Klepser, A. Wörnlein, Denis Wouters, Armin Rest, A. Possenti, R. C. G. Chaves, C. Mueller, P. Coyle, F. Zefi, Poonam Chandra, F. Niederwanger, R. D. Parsons, Anne Deschamps, T. Seitz, Daniele Vivolo, D. J. Champion, C. Sieger, J. Dyks, F. Schüssler, L. Caramete, A. Reimer, Felix Spanier, Dominik Elsässer, H. van Haren, S. R. Bernard, T. Garrigoux, K. Morå, I. Di Palma, L. K. Hardy, David Salek, E. Moulin, Justine Devin, Michal Ostrowski, Tomasz Bulik, J.-P. Lenain, Luigi Antonio Fusco, Thomas Tavernier, Matteo Sanguineti, A. Sánchez-Losa, M. Capasso, S. J. Fegan, A. Djannati-Ataï, G. Riccobene, Gianluca Giavitto, Benjamin Stappers, Gilles Maurin, I. Oya, L. Quinn, Axel Donath, Jacco Vink, A. W. Chen, J. Zúñiga, A. S. Seyffert, R. Miller, Pierre-Henri Aubert, Nu. Komin, Sabrina Casanova, Andrew M. Taylor, Jörn Wilms, M. Kreter, Mark Sullivan, Michael Kramer, S. Krakau, V. Sahakian, R. Bruijn, Andreas Quirrenbach, J-J. Aubert, R. Borrnuth, M. Saldaña, Aion Viana, C. Mariaud, Joao A B Coelho, J. P. Lees, P. Migliozzi, D. J. van der Walt, M. Settimo, C. Vallée, Christian Stegmann, Stefan Wagner, Gisela Anton, Bruno Khelifi, Jan Conrad, M. Marcelin, V. Giordano, M. Lorentz, M. Kraus, D. Kerszberg, T. Avgitas, Rachel Simoni, Helen Poon, J.A. Martínez-Mora, Alexis Coleiro, Antonia Rowlinson, S. Raab, Stefan Funk, Alicja Wierzcholska, B. Peyaud, Yasunobu Uchiyama, R. J. Tuffs, L. Mohrmann, Juan José Hernández-Rey, T. Jogler, D.A. Prokhorov, Michel André, Frank M. Rieger, J.D. Zornoza, A. Schulz, T. Pradier, S. Wagner, A. Abramowski, R. Mele, S. Rosier-Lees, G. Spengler, Yann Hello, J. Lau, C. van Rensburg, M. Holler, R. Coniglione, Arnauld Albert, Emanuele Leonora, A. Balzer, Michael Zacharias, M. Mohamed, Yahya Tayalati, J. Carr, I. Jung-Richardt, A. Mathieu, A. Fiasson, Roberta Zanin, P. Willmann, Hervé Glotin, K. Geyer, K. Roensch, Michael Backes, Alexandre Marcowith, J. King, J. Hofestädt, P. P. Krüger, K. Stycz, Jeff Cooke, S. P. Littlefair, H. Odaka, Felix Jankowsky, N. Shafi, M. de Naurois, Krzysztof Katarzynski, Jim Hinton, Matteo Cerruti, P. Bordas, Robert Lahmann, F. Krayzel, V. Bertin, J. Barrios-Martí, R. Liu, Stefan Ohm, W. van Straten, Christoph Deil, J. Hossl, P. Jaroenjittichai, Léa Jouvin, R. Gracia-Ruiz, T. Andersson, W. Domainko, Gerard Fontaine, Felix Aharonian, J. F. Glicenstein, Maurizio Spurio, V. Popa, Catherine Boisson, D. Drouhin, Paolo Piattelli, Olivier Hervet, Pierre Brun, F. Voisin, M. Jongen, D. Kolitzus, C. Trichard, M. Arrieta, Utane Sawangwit, Heike Prokoph, P. T. O'Brien, Paolo Sapienza, A. Förster, Ruben Lopez-Coto, M. Lemoine-Goumard, Abdelilah Moussa, S. Eschbach, M. V. Fernandes, A.J. Heijboer, Steffen Hallmann, C. Hugon, Ruizhi Yang, D. Turpin, Werner Hofmann, Stefano Gabici, S.F. Biagi, P. Wagner, V. Marandon, Jean-Pierre Ernenwein, C. Distefano, S. Colafrancesco, D. F. E. Samtleben, Vladimir Kulikovskiy, Marek Jamrozy, I. Andreoni, Corinne Donzaud, Vikram Ravi, Joachim Hahn, Shivani Bhandari, L. Oakes, Johannes Veh, M. Tluczykont, M. Caleb, Gilles Henri, J. Bolmont, J. Hawkes, I. Sushch, S. Basa, M. Chrétien, Sarah Burke-Spolaor, M. Gajdus, G.E. Păvălaş, C. Pellegrino, H. Costantini, Peter Eger, F. Stinzing, C. van Eldik, D. Berge, G. De Bonis, B. Giebels, A. Capone, Helene Sol, J. Busto, J. Becker Tjus, J.-P. Tavernet, Gavin Rowell, M. Bryan, R. de los Reyes, P.-O. Petrucci, N. W. Pekeur, Manuel Meyer, A. Goya, M. Burgay, Miguel Ardid, D. Gottschall, Anne Lemiere, Laboratoire Univers et Théories (LUTH (UMR_8102)), Institut national des sciences de l'Univers (INSU - CNRS)-Observatoire de Paris, Université Paris sciences et lettres (PSL)-Université Paris sciences et lettres (PSL)-Centre National de la Recherche Scientifique (CNRS)-Université Paris Diderot - Paris 7 (UPD7), AstroParticule et Cosmologie (APC (UMR_7164)), Observatoire de Paris, Université Paris sciences et lettres (PSL)-Université Paris sciences et lettres (PSL)-Commissariat à l'énergie atomique et aux énergies alternatives (CEA)-Université Paris Diderot - Paris 7 (UPD7)-Centre National de la Recherche Scientifique (CNRS)-Institut National de Physique Nucléaire et de Physique des Particules du CNRS (IN2P3), Laboratoire d'Astrophysique de Marseille (LAM), Centre National de la Recherche Scientifique (CNRS)-Institut national des sciences de l'Univers (INSU - CNRS)-Aix Marseille Université (AMU)-Centre National d'Études Spatiales [Toulouse] (CNES), Petroff, E, Burke-Spolaor, S, Keane, Ef, Mclaughlin, Ma, Miller, R, Andreoni, I, Bailes, M, Barr, Ed, Bernard, Sr, Bhandari, S, Bhat, Ndr, Burgay, M, Caleb, M, Champion, D, Chandra, P, Cooke, J, Dhillon, V, Farnes, J, Hardy, Lk, Jaroenjittichai, P, Johnston, S, Kasliwal, M, Kramer, M, Littlefair, Sp, Macquart, Jp, Mickaliger, M, Possenti, A, Pritchard, T, Ravi, V, Rest, A, Rowlinson, A, Sawangwit, U, Stappers, B, Sullivan, M, Tiburzi, C, van Straten, W, Albert, A, Andre, M, Anghinolfi, M, Anton, G, Ardid, M, Aubert, Jj, Avgitas, T, Baret, B, Barrios-Marti, J, Basa, S, Bertin, V, Biagi, S, Borrnuth, R, Bourret, S, Bouwhuis, Mc, Bruijn, R, Brunner, J, Busto, J, Capone, A, Caramete, L, Carr, J, Celli, S, Chiarusi, T, Circella, M, Coelho, Jab, Coleiro, A, Coniglione, R, Costantini, H, Coyle, P, Creusot, A, Deschamps, A, De Bonis, G, Distefano, C, Di Palma, I, Donzaud, C, Dornic, D, Drouhin, D, Eberl, T, El Bojaddaini, I, Elsasser, D, Enzenhofer, A, Felis, I, Fusco, La, Galata, S, Gay, P, Geisselsoder, S, Geyer, K, Giordano, V, Gleixner, A, Glotin, H, Gregoire, T, Gracia-Ruiz, R, Graf, K, Hallmann, S, van Haren, H, Heijboer, Aj, Hello, Y, Hernandez-Rey, Jj, Hossl, J, Hofestadt, J, Hugon, C, Illuminati, G, James, Cwcw, de Jong, M, Jongen, M, Kadler, M, Kalekin, O, Katz, U, Kiessling, D, Kouchner, A, Kreter, M, Kreykenbohm, I, Kulikovskiy, V, Lachaud, C, Lahmann, R, Lefevre, D, Leonora, E, Lotze, M, Loucatos, S, Marcelin, M, Margiotta, A, Marinelli, A, Martinez-Mora, Ja, Mathieu, A, Mele, R, Melis, K, Michael, T, Migliozzi, P, Moussa, A, Mueller, C, Nezri, E, Pavalas, Ge, Pellegrino, C, Perrina, C, Piattelli, P, Popa, V, Pradier, T, Quinn, L, Racca, C, Riccobene, G, Roensch, K, Sanchez-Losa, A, Saldana, M, Salvadori, I, Samtleben, Dfe, Sanguineti, M, Sapienza, P, Schnabel, J, Seitz, T, Sieger, C, Spurio, M, Stolarczyk, T, Taiuti, M, Tayalati, Y, Trovato, A, Tselengidou, M, Turpin, D, Tonnis, C, Vallage, B, Vallee, C, Van Elewyck, V, Vivolo, D, Vizzoca, A, Wagner, S, Wilms, J, Zornoza, Jd, Zuniga, J, Abdalla, H, Abramowski, A, Aharonian, F, Benkhali, Fa, Akhperjanian, Ag, Andersson, T, Anguner, Eo, Arrieta, M, Aubert, P, Backes, M, Balzer, A, Barnard, M, Becherini, Y, Tjus, Jb, Berge, D, Bernhard, S, Bernlohr, K, Blackwell, R, Bottcher, M, Boisson, C, Bolmont, J, Bordas, P, Bregeon, J, Brun, F, Brun, P, Bryan, M, Bulik, T, Capasso, M, Casanova, S, Cerruti, M, Chakraborty, N, Chalme-Calvet, R, Chaves, Rcg, Chen, A, Chevalier, J, Chretien, M, Colafrancesco, S, Cologna, G, Condon, B, Conrad, J, Cui, Y, Davids, Id, Decock, J, Degrange, B, Deil, C, Devin, J, de Wilt, P, Dirson, L, Djannati-Atai, A, Domainko, W, Donath, A, Drury, Lo, Dubus, G, Dutson, K, Dyks, J, Edwards, T, Egberts, K, Eger, P, Ernenwein, Jp, Eschbach, S, Farnier, C, Fegan, S, Fernandes, Mv, Fiasson, A, Fontaine, G, Forster, A, Funk, S, Fussling, M, Gabici, S, Gajdus, M, Gallant, Ya, Garrigoux, T, Giavitto, G, Giebels, B, Glicenstein, Jf, Gottschall, D, Goya, A, Grondin, Mh, Hadasch, D, Hahn, J, Haupt, M, Hawkes, J, Heinzelmann, G, Henri, G, Hermann, G, Hervet, O, Hinton, Ja, Hofmann, W, Hoischen, C, Holler, M, Horns, D, Ivascenko, A, Jacholkowska, A, Jamrozy, M, Janiak, M, Jankowsky, D, Jankowsky, F, Jingo, M, Jogler, T, Jouvin, L, Jung-Richardt, I, Kastendieck, Ma, Katarzynski, K, Kerszberg, D, Khelifi, B, Kieffer, M, King, J, Klepser, S, Klochkov, D, Kluzniak, W, Kolitzus, D, Komin, N, Kosack, K, Krakau, S, Kraus, M, Krayzel, F, Kruger, Pp, Laffon, H, Lamanna, G, Lau, J, Lees, Jp, Lefaucheur, J, Lefranc, V, Lemiere, A, Lemoine-Goumard, M, Lenain, Jp, Leser, E, Lohse, T, Lorentz, M, Liu, R, Lopez-Coto, R, Lypova, I, Marandon, V, Marcowith, A, Mariaud, C, Marx, R, Maurin, G, Maxted, N, Mayer, M, Meintjes, Pj, Meyer, M, Mitchell, Amw, Moderski, R, Mohamed, M, Mohrmann, L, Mora, K, Moulin, E, Murach, T, de Naurois, M, Niederwanger, F, Niemiec, J, Oakes, L, O'Brien, P, Odaka, H, Ottl, S, Ohm, S, Ostrowski, M, Oya, I, Padovani, M, Panter, M, Parsons, Rd, Pekeur, Nw, Pelletier, G, Perennes, C, Petrucci, Po, Peyaud, B, Piel, Q, Pita, S, Poon, H, Prokhorov, D, Prokoph, H, Puhlhofer, G, Punch, M, Quirrenbach, A, Raab, S, Reimer, A, Reimer, O, Renaud, M, de los Reyes, R, Rieger, F, Romoli, C, Rosier-Lees, S, Rowell, G, Rudak, B, Rulten, Cb, Sahakian, V, Salek, D, Sanchez, Da, Santangelo, A, Sasaki, M, Schlickeiser, R, Schulz, A, Schussler, F, Schwanke, U, Schwemmer, S, Settimo, M, Seyffert, A, Shafi, N, Shilon, I, Simoni, R, Sol, H, Spanier, F, Spengler, G, Spies, F, Stawarz, L, Steenkamp, R, Stegmann, C, Stinzing, F, Stycz, K, Sushch, I, Tavernet, Jp, Tavernier, T, Taylor, Am, Terrier, R, Tibaldo, L, Tiziani, D, Tluczykont, M, Trichard, C, Tuffs, R, Uchiyama, Y, van der Walt, Dj, van Eldik, C, van Rensburg, C, van Soelen, B, Vasileiadis, G, Veh, J, Venter, C, Viana, A, Vincent, P, Vink, J, Voisin, F, Volk, Hj, Vuillaume, T, Wadiasingh, Z, Wagner, Sj, Wagner, P, Wagner, Rm, White, R, Wierzcholska, A, Willmann, P, Wornlein, A, Wouters, D, Yang, R, Zabalza, V, Zaborov, D, Zacharias, M, Zanin, R, Zdziarski, Aa, Zech, A, Zefi, F, Ziegler, A, Zywucka, N, PSL Research University (PSL)-PSL Research University (PSL)-Université Paris Diderot - Paris 7 (UPD7)-Centre National de la Recherche Scientifique (CNRS), Institut National de Physique Nucléaire et de Physique des Particules du CNRS (IN2P3)-Centre National de la Recherche Scientifique (CNRS)-Commissariat à l'énergie atomique et aux énergies alternatives (CEA)-Observatoire de Paris, PSL Research University (PSL)-PSL Research University (PSL)-Université Paris Diderot - Paris 7 (UPD7), Petroff, E., Burke-Spolaor, S., Keane, E. F., Mclaughlin, M. A., Miller, R., Andreoni, I., Bailes, M., Barr, E. D., Bernard, S. R., Bhandari, S., Bhat, N. D. R., Burgay, M., Caleb, M., Champion, D., Chandra, P., Cooke, J., Dhillon, V. S., Farnes, J. S., Hardy, L. K., Jaroenjittichai, P., Johnston, S., Kasliwal, M., Kramer, M., Littlefair, S. P., Macquart, J. P., Mickaliger, M., Possenti, A., Pritchard, T., Ravi, V., Rest, A., Rowlinson, A., Sawangwit, U., Stappers, B., Sullivan, M., Tiburzi, C., van Straten, W., Albert, A., André, M., Anghinolfi, M., Anton, G., Ardid, M., Aubert, J.-J., Avgitas, T., Baret, B., Barrios-Martí, J., Basa, S., Bertin, V., Biagi, S., Bormuth, R., Bourret, S., Bouwhuis, M.C., Bruijn, R., Brunner, J., Busto, J., Capone, A., Caramete, L., Carr, J., Celli, S., Chiarusi, T., Circella, M., Coelho, J.A.B., Coleiro, A., Coniglione, R., Costantini, H., Coyle, P., Creusot, A., Deschamps, A., De Bonis, G., Distefano, C., Palma, I. Di, Donzaud, C., Dornic, D., Drouhin, D., Eberl, T., El Bojaddaini, I., Elsässer, D., Enzenhöfer, A., Felis, I., Fusco, L.A., Galatà, S., Gay, P., Geißelsöder, S., Geyer, K., Giordano, V., Gleixner, A., Glotin, H., Grégoire, T., Gracia-Ruiz, R., Graf, K., Hallmann, S., van Haren, H., Heijboer, A.J., Hello, Y., Hernández-Rey, J.J., Hößl, J., Hofestädt, J., Hugon, C., Illuminati, G., James, C.W, de Jong, M., Jongen, M., Kadler, M., Kalekin, O., Katz, U., Kießling, D., Kouchner, A., Kreter, M., Kreykenbohm, I., Kulikovskiy, V., Lachaud, C., Lahmann, R., Lefèvre, D., Leonora, E., Lotze, M., Loucatos, S., Marcelin, M., Margiotta, A., Marinelli, A., Martínez-Mora, J.A., Mathieu, A., Mele, R., Melis, K., Michael, T., Migliozzi, P., Moussa, A., Mueller, C., Nezri, E., Păvălaş, G.E., Pellegrino, C., Perrina, C., Piattelli, P., Popa, V., Pradier, T., Quinn, L., Racca, C., Riccobene, G., Roensch, K., Sánchez-Losa, A., Saldaña, M., Salvadori, I., Samtleben, D. F. E., Sanguineti, M., Sapienza, P., Schnabel, J., Seitz, T., Sieger, C., Spurio, M., Stolarczyk, Th., Taiuti, M., Tayalati, Y., Trovato, A., Tselengidou, M., Turpin, D., Tönnis, C., Vallage, B., Vallée, C., Van Elewyck, V., Vivolo, D., Vizzoca, A., Wagner, S., Wilms, J., Zornoza, J.D., Zúñiga, J., Abdalla, H., Abramowski, A., Aharonian, F., Benkhali, F. Ait, Akhperjanian, A.G., Andersson, T., Angüner, E.O., Arrieta, M., Aubert, P., Backes, M., Balzer, A., Barnard, M., Becherini, Y., Becker Tjus, J., Berge, D., Bernhard, S., Bernlöhr, K., Blackwell, R., Böttcher, M., Boisson, C., Bolmont, J., Bordas, P., Bregeon, J., Brun, F., Brun, P., Bryan, M., Bulik, T., Capasso, M., Casanova, S., Cerruti, M., Chakraborty, N., Chalme-Calvet, R., Chaves, R.C.G., Chen, A., Chevalier, J., Chrétien, M., Colafrancesco, S., Cologna, G., Condon, B., Conrad, J., Cui, Y., Davids, I.D., Decock, J., Degrange, B., Deil, C., Devin, J., Dewilt, P., Dirson, L., Djannati-Ataï, A., Domainko, W., Donath, A., Drury, L.O’C., Dubus, G., Dutson, K., Dyks, J., Edwards, T., Egberts, K., Eger, P., Ernenwein, J.-P., Eschbach, S., Farnier, C., Fegan, S., Fernandes, M.V., Fiasson, A., Fontaine, G., Förster, A., Funk, S., Füßling, M., Gabici, S., Gajdus, M., Gallant, Y.A., Garrigoux, T., Giavitto, G., Giebels, B., Glicenstein, J.F., Gottschall, D., Goyal, A., Grondin, M.-H., Hadasch, D., Hahn, J., Haupt, M., Hawkes, J., Heinzelmann, G., Henri, G., Hermann, G., Hervet, O., Hinton, J.A., Hofmann, W., Hoischen, C., Holler, M., Horns, D., Ivascenko, A., Jacholkowska, A., Jamrozy, M., Janiak, M., Jankowsky, D., Jankowsky, F., Jingo, M., Jogler, T., Jouvin, L., Jung-Richardt, I., Kastendieck, M.A., Katarzyński, K., Kerszberg, D., Khélifi, B., Kieffer, M., King, J., Klepser, S., Klochkov, D., Kluźniak, W., Kolitzus, D., Komin, Nu., Kosack, K., Krakau, S., Kraus, M., Krayzel, F., Krüger, P.P., Laffon, H., Lamanna, G., Lau, J., Lees, J.-P., Lefaucheur, J., Lefranc, V., Lemière, A., Lemoine-Goumard, M., Lenain, J.-P., Leser, E., Lohse, T., Lorentz, M., Liu, R., López-Coto, R., Lypova, I., Marandon, V., Marcowith, A., Mariaud, C., Marx, R., Maurin, G., Maxted, N., Mayer, M., Meintjes, P.J., Meyer, M., Mitchell, A.M.W., Moderski, R., Mohamed, M., Mohrmann, L., Morå, K., Moulin, E., Murach, T., de Naurois, M., Niederwanger, F., Niemiec, J., Oakes, L., O’Brien, P., Odaka, H., Öttl, S., Ohm, S., Ostrowski, M., Oya, I., Padovani, M., Panter, M., Parsons, R.D., Pekeur, N.W., Pelletier, G., Perennes, C., Petrucci, P.-O., Peyaud, B., Piel, Q., Pita, S., Poon, H., Prokhorov, D., Prokoph, H., Pühlhofer, G., Punch, M., Quirrenbach, A., Raab, S., Reimer, A., Reimer, O., Renaud, M., Reyes, R. de lo, Rieger, F., Romoli, C., Rosier-Lees, S., Rowell, G., Rudak, B., Rulten, C.B., Sahakian, V., Salek, D., Sanchez, D.A., Santangelo, A., Sasaki, M., Schlickeiser, R., Schulz, A., Schüssler, F., Schwanke, U., Schwemmer, S., Settimo, M., Seyffert, A.S., Shafi, N., Shilon, I., Simoni, R., Sol, H., Spanier, F., Spengler, G., Spies, F., Stawarz, Ł., Steenkamp, R., Stegmann, C., Stinzing, F., Stycz, K., Sushch, I., Tavernet, J.-P., Tavernier, T., Taylor, A.M., Terrier, R., Tibaldo, L., Tiziani, D., Tluczykont, M., Trichard, C., Tuffs, R., Uchiyama, Y., Walt, D.J. van der, van Eldik, C., van Rensburg, C., van Soelen, B., Vasileiadis, G., Veh, J., Venter, C., Viana, A., Vincent, P., Vink, J., Voisin, F., Völk, H.J., Vuillaume, T., Wadiasingh, Z., Wagner, S.J., Wagner, P., Wagner, R.M., White, R., Wierzcholska, A., Willmann, P., Wörnlein, A., Wouters, D., Yang, R., Zabalza, V., Zaborov, D., Zacharias, M., Zanin, R., Zdziarski, A.A., Zech, A., Zefi, F., Ziegler, A., Żywucka, N., High Energy Astrophys. & Astropart. Phys (API, FNWI), KM3NeT (IHEF, IoP, FNWI), Faculty of Science, Gravitation and Astroparticle Physics Amsterdam, ATLAS (IHEF, IoP, FNWI), GRAPPA (ITFA, IoP, FNWI), Université Paris sciences et lettres (PSL)-Université Paris sciences et lettres (PSL)-Université Paris Diderot - Paris 7 (UPD7)-Centre National de la Recherche Scientifique (CNRS), Commissariat à l'énergie atomique et aux énergies alternatives (CEA)-Institut National de Physique Nucléaire et de Physique des Particules du CNRS (IN2P3)-Observatoire de Paris, Centre de Physique des Particules de Marseille (CPPM), Aix Marseille Université (AMU)-Institut National de Physique Nucléaire et de Physique des Particules du CNRS (IN2P3)-Centre National de la Recherche Scientifique (CNRS), Aix Marseille Université (AMU)-Institut national des sciences de l'Univers (INSU - CNRS)-Centre National d'Études Spatiales [Toulouse] (CNES)-Centre National de la Recherche Scientifique (CNRS), Andre, M., Aubert, J. -J., Barrios-Marti, J., Bouwhuis, M. C., Coelho, J. A. B., Di Palma, I., Elsasser, D., Enzenhofer, A., Fusco, L. A., Galata, S., Geisselsoder, S., Gregoire, T., Heijboer, A. J., Hernandez-Rey, J. J., Hobl, J., Hofestadt, J., James, C. W., Kiebling, D., Lefevre, D., Martinez-Mora, J. A., Pavalas, G. E., Sanchez-Losa, A., Saldana, M., Stolarczyk, T., Tonnis, C., Vallee, C., Zornoza, J. D., Zuniga, J., Ait Benkhali, F., Akhperjanian, A. G., Anguner, E. O., Bernlohr, K., Bottcher, M., Chaves, R. C. G., Chretien, M., Davids, I. D., Djannati-Atai, A., Drury, L. O'C., Ernenwein, J. -P., Fernandes, M. V., Forster, A., Fubling, M., Gallant, Y. A., Glicenstein, J. F., Grondin, M. -H., Hinton, J. A., Kastendieck, M. A., Katarzynski, K., Khelifi, B., Kluzniak, W., Komin, N., Kruger, P. P., Lees, J. -P., Lemiere, A., Lenain, J. -P., Lopez-Coto, R., Meintjes, P. J., Mitchell, A. M. W., Mora, K., O'Brien, P., Ottl, S., Parsons, R. D., Pekeur, N. W., Petrucci, P. -O., Puhlhofer, G., de los Reyes, R., Rulten, C. B., Sanchez, D. A., Schussler, F., Seyffert, A. S., Stawarz, L., Tavernet, J. -P., Taylor, A. M., van der Walt, D. J., Volk, H. J., Wagner, S. J., Wagner, R. M., Wornlein, A., Zdziarski, A. A., Zywucka, N., Centre Tecnològic de Vilanova i la Geltrú, and Universitat Politècnica de Catalunya. LAB - Laboratori d'Aplicacions Bioacústiques
Subjects: Astrofísica, Astronomy, Astrophysics, Surveys, ISM: structure, Methods: data analysis, Polarization, Astronomy and Astrophysics, Space and Planetary Science, 01 natural sciences, Radio telescopes, data analysis [Methods], 010303 astronomy & astrophysics, High Energy Astrophysical Phenomena (astro-ph.HE), Physics, Line-of-sight, [SDU.ASTR]Sciences of the Universe [physics]/Astrophysics [astro-ph], Linear polarization, Fast radio burst, Galactic Center, ComputingMethodologies_DOCUMENTANDTEXTPROCESSING, Astrophysics - High Energy Astrophysical Phenomena, polarization–methods, dataanalysis–surveys–ISM, structure, Milky Way, Astrophysics::High Energy Astrophysical Phenomena, FOS: Physical sciences, Astrophysics::Cosmology and Extragalactic Astrophysics, Radio telescope, 0103 physical sciences, Neutrins, Neutrinos, Astrophysics::Galaxy Astrophysics, Astroparticle physics, Telescopis, 010308 nuclear & particles physics, Galactic plane, Física::Astronomia i astrofísica [Àrees temàtiques de la UPC], FISICA APLICADA, ddc:520, polarization – methods: data analysis – surveys – ISM: structure, structure [ISM], Methods: data analysi
Abstract: Monthly notices of the Royal Astronomical Society 469(4), 4465 – 4482 (2017). doi:10.1093/mnras/stx1098, We report on the discovery of a new fast radio burst (FRB), FRB 150215, with the Parkes radio telescope on 2015 February 15. The burst was detected in real time with a dispersion measure (DM) of 1105.6 ± 0.8 pc cm$^{−3}$, a pulse duration of 2.8 $^{+1.2}_{-0.5}$ ms, and a measured peak flux density assuming that the burst was at beam centre of 0.7$^{+0.2}_{-0.1}$ Jy. The FRB originated at a Galactic longitude and latitude of 24.66°, 5.28° and 25° away from the Galactic Center. The burst was found to be 43 ± 5 per cent linearly polarized with a rotation measure (RM) in the range −9, Published by Oxford Univ. Press, Oxford
Published: 2017

65. The extended jet in AP Librae as the source of the VHE γ-ray emission

Author: Michael Zacharias and Stefan Wagner
Subjects: Physics, Jet (fluid), Photon, Astrophysics::High Energy Astrophysical Phenomena, Cosmic microwave background, Compton scattering, Gamma ray, Astrophysics::Cosmology and Extragalactic Astrophysics, Astrophysics, Astrophysics - Astrophysics of Galaxies, Spectral energy distribution, Astrophysics - High Energy Astrophysical Phenomena, Blazar, BL Lac object
Abstract: Most modeling attempts of blazars use a small emission zone located close to the central black hole in order to explain the broad-band spectral energy distribution. Here we present a case where additionally to the small region a $>$kpc-scale jet is required to successfully reproduce the spectrum and especially the TeV emission, namely the low-frequeny peaked BL Lac object AP Librae detected in the TeV domain by the H.E.S.S. experiment. Given that other parts of the spectral energy distribution follow the characteristics implied by the source classification, the inverse Compton component spans 10 orders of magnitude, which cannot be reproduced by the one-zone model. Additionally, observational constraints in both the synchrotron and inverse Compton compoenent strongly constrain the parameters of a self-consistent model ruling out the possibility of TeV photon production in the vicinity of the galactic center. We discuss the possibility that the TeV radiation is emitted by highly energetic particles in the extended, arcsec-scale jet, which has been detected at radio and X-ray energies. The slope of the jet X-ray spectrum indicates an inverse Compton origin, and an extrapolation to higher energies coincides with a break feature in the $\gamma$-ray band. Modeling the jet emission with inverse Compton scattering of the cosmic microwave background results in an excellent fit of the radio, X-ray and TeV emission. Implications will be discussed, such as properties of the jet, acceleration scenarios, and observations to test the model. If confirmed, large scale jets are able to efficiently accelerate particles and to keep relativistic speeds up to distances of several 100kpc., Comment: 5 pages, 1 figure, to appear in the AIP Conference proceedings of the "High Energy Gamma-Ray Astronomy (Gamma2016)", edited by F. Aharonian, W. Hofmann, F. Rieger
Published: 2017

66. Inverse Compton light curves of blazars under non-linear, time-dependent synchrotron-self Compton cooling

Author: Michael Zacharias
Subjects: High Energy Astrophysical Phenomena (astro-ph.HE), Physics, Astrophysics::High Energy Astrophysical Phenomena, FOS: Physical sciences, Flux, Inverse, Astronomy and Astrophysics, Astrophysics, Electron, Light curve, Synchrotron, law.invention, Space and Planetary Science, law, Spectral energy distribution, Monochromatic color, Astrophysics - High Energy Astrophysical Phenomena, Blazar
Abstract: Blazars exhibit flares with a doubling time scale on the order of minutes. Such rapid flares are theoretically challenging and several {models} have been put forward to explain the fast variability. In this paper we continue the discussion concerning the effects of non-linear, time-dependent synchrotron self-Compton (SSC) cooling. In previous papers we were able to show that the non-linearity{, introduced by a time-dependent electron injection,} has severe consequences for both the spectral energy distribution (SED) and the monochromatic synchrotron light curve. The non-linear cooling introduces novel breaks in the SED, which are usually explained by complicated underlying electron distributions, while the much faster cooling of the SSC process {causes significant differences in the synchrotron light curves}. In this paper we calculate the inverse Compton light curves, taking into account both the SSC and the external Compton process. The light curves are calculated from the monochromatic intensities by introducing the retardation due to the finite size of the emission region and the geometry of the source. Even though some of the obvious effects of the SSC cooling are washed out by the retardation, there are still several observational constraints which could help to discriminate between the non-linear and the usual linear models, such as different flux states, temporal shapes or faster variability of the light curves at different energies., Comment: 23 pages, 5 figures, accepted for publication in MNRAS
Published: 2014

67. Acute Myocarditis Following Influenza Vaccine in a Heart Transplant Patient

Author: Chantal ElAmm, Mohamed Khayata, Michael Zacharias, and Linda Njoroge
Subjects: Heart transplantation, medicine.medical_specialty, Ejection fraction, Myocarditis, business.industry, Influenza vaccine, medicine.medical_treatment, Cardiac index, medicine.disease, Tacrolimus, medicine.anatomical_structure, Ventricle, Internal medicine, medicine, Cardiology, Plasmapheresis, Cardiology and Cardiovascular Medicine, business
Abstract: Introduction Seasonal influenza vaccine is recommended in heart transplant patients. While it is typically well tolerated, there have been reports of low level histologic rejections . The influenza vaccine itself has been linked to inflammatory myopathies and has also been implicated in a case of myocarditis in a previously healthy individual . We present the first suspected case of myocarditis after influenza vaccine in a heart transplant patient. Case Report A 30-year-old African-American male with familial cardiomyopathy status post heart transplantation 18 months ago developed recurrent significant left ventricular dysfunction. Immediately post transplantation, he had acute graft dysfunction without evidence of acute cellular or antibody mediated rejection and negative donor specific antibodies. He received steroids, IVIG and plasmapheresis with restoration of graft function. 16 moths post-transplant, he had acute cellular rejection in the setting of subtherapeutic tacrolimus levels and was treated with pulse dose steroids with resolution. At 18 months, his EF dropped from 55-60% to 30-35% with a low cardiac index of 1.8, felt to be secondary to a non HLA antibodies given a negative endomyocardial biopsy. Pulse dose steroids resulted in recovery of his LV function by cardiac MRI (LVEF 52%). As part of his care he received the seasonal influenza vaccine. 3 weeks later he presented with dyspnea and fatigue. An echocardiogram at that time showed an ejection fraction of 35-40%. EMB was negative for rejection. A repeat cardiac MRI showed acute myocarditis. Although the EMB was negative for myocarditis, the sensitivity would have increased if a sample from the left ventricle was obtained. Summary This is the first case of a heart transplant patient with suspected acute myocarditis after receiving the influenza vaccine. Although alternative diagnoses cannot be excluded, the proximity of the vaccine and imaging evidence supports a direct correlation.
Published: 2018

68. Neurocognitive Deficits are Prevalent in Ambulatory Patients Living with Left Ventricular Assist Devices

Author: Michael Zacharias, Mahazarin Ginwalla, S. Al-Kindi, C. El Amm, L. Meece, H. Khalid, M. Moghbelli, R. Benatti, M.R. Robinson, and Guilherme H. Oliveira
Subjects: Pulmonary and Respiratory Medicine, Transplantation, medicine.medical_specialty, Physical medicine and rehabilitation, business.industry, Ambulatory, Medicine, Surgery, Cardiology and Cardiovascular Medicine, business, Neurocognitive
Published: 2018

69. Outcomes of Patients with Cardiogenic Shock Requiring Early vs Late Renal Replacement Therapy during Extracorporeal Membrane Oxygenation (ECMO) Support

Author: Francis Lytle, Nour Tashtish, Erica Zanath, Sadeer G. Al-Kindi, Chantal ElAmm, Rana Hejal, Michael Zacharias, Mohamad Karnib, Benjamin Medalion, and Nada Abou Hassan
Subjects: Inpatient mortality, business.industry, Cardiogenic shock, medicine.medical_treatment, Acute kidney injury, Mean age, medicine.disease, University hospital, Anesthesia, Baseline characteristics, medicine, Extracorporeal membrane oxygenation, Renal replacement therapy, Cardiology and Cardiovascular Medicine, business
Abstract: Introduction Acute kidney injury is common in patients with cardiogenic shock supported with extracorporeal membrane oxygenation (ECMO), and it is associated with mortality. Hypothesis We hypothesized that mortality is not different between patients who require early (within 48 hours) vs late (≥48 hours of ECMO) initiation of continuous renal replacement therapy (CRRT). Methods We retrospectively reviewed all patients with cardiogenic shock who underwent veno-arterial ECMO at University Hospitals, between 2015 and 2018. Patients who required CRRT during ECMO support were divided into early vs late CRRT initiation. Inpatient mortality, one-year mortality and length of stay were compared between the two patient groups. Results Out of 127 patients supported with ECMO, 56 (44%) required CRRT (40 early and 16 late CRRT). Among patients requiring CRRT, mean age was 57±14 years, 74% were male, median SAVE score was -9 [-14, -5], and median lactate was 7.6 [4.2, 12.4] mmol/L. There were no statistically-significant differences in baseline characteristics (demographics, comorbidities, laboratory values, or hemodynamic measurements) between early and late CRRT (P>0.05 for all comparisons). There were no statistically-significant differences between early and late CRRT with respect to inpatient mortality (62% vs 64%, P>0.99), 1-year mortality (78% vs 67%, P=0.71) or length of stay (median 20 vs 16 days, P=0.61). There was no association between time of CRRT and risk of inpatient mortality (OR 1.00, 95% CI: 0.88-1.15, P=0.95), or one-year mortality (HR 0.96, 9% CI: 0.89-1.05, P=0.39). Conclusions Mortality is high among patients who require CRRT during ECMO support. There was no difference between early (
Published: 2019

70. Model for End-Stage Liver Disease (MELD) Does Not Predict Mortality after Veno-Arterial Extracorporeal Membrane Oxygenation Support

Author: Soon J. Park, Benjamin Medalion, Michael Zacharias, J. Sohn, Basar Sareyyupoglu, T. Schwab, Francis Lytle, Mohamad Amer Alaiti, Erica Zanath, Salil V. Deo, A.M. Johnson, Chantal ElAmm, L. Chaaban, Yakov Elgudin, Nour Tashtish, S. Al-Kindi, Hiram G. Bezerra, Mohamad Karnib, and Guilherme H. Oliveira
Subjects: Pulmonary and Respiratory Medicine, Transplantation, medicine.medical_specialty, business.industry, medicine.medical_treatment, Cardiogenic shock, Organ dysfunction, Logistic regression, medicine.disease, Liver disease, Model for End-Stage Liver Disease, Internal medicine, Heart failure, medicine, Extracorporeal membrane oxygenation, Cardiology, Surgery, Hemodialysis, medicine.symptom, Cardiology and Cardiovascular Medicine, business
Abstract: Purpose The Model of End-Stage Liver Disease (MELD) score incorporates measures of kidney and liver dysfunction . MELD score has been shown to predict mortality in patients with advanced heart failure or cardiogenic shock (CS). Prior small single-center studies have shown that MELD score predicts mortality in patients supported with Venoarterial Extracorporeal Membrane Oxygenation (VA-ECMO). The Purpose of our was to reassess the role of MELD score predicting Mortality After (VA-ECMO). Methods We reviewed 105 consecutive patients with (CS) who received VA-ECMO between 8/2014 and 6/2018 in our hospital. We calculated MELD, MELD excluding INR (MELDXI), MELD with sodium -MELDNa- (calculated at a mean of 7 hours prior to VA-ECMO initiation), and SAVE score. We identified the association between each score and short-term mortality using logistic regression and Kaplan-Meier with Cox proportional hazard models . Results Our patient had Mean age was 57.1 ± 13.8 years and 32% female. Mean MELD score was 19.5 ± 8.3, MELDXI 18.9 ± 7.1, MELDNa 20.5 ± 8.3, SAVE -8.6 ± 6.5. Inpatient mortality was 68%. SAVE score was associated with short-term (OR 0.91 per 1 unit, 95% CI: 0.84-0.98, P=0.011) and long-term mortality (HR 0.95, 95% CI: 0.91-0.98, P=0.002) (Figure 1). There was no association between MELD (OR 1.02, 95% CI: 0.97-1.08, P=0.41), MELDXI (OR 1.01, 95% CI: 0.95-1.07, P=0.86), or MELDNa (OR 1.02, 95% CI: 0.97-1.08, P=0.41), with inpatient mortality. MELD (OR 1.07, 1.01-1.13, P=0.02), MELDXI (OR 1.12 [1.05-1.20], P=0.001) and MELDNa (OR 1.06, 95% CI: 1.01-1.12, P=0.03) were all associated with need for hemodialysis after ECMO. Conclusion In this single-center study of patients with VA ECMO, neither MELD, nor MELDXI or MELDNa, were associated with short-term or long-term mortality. SAVE score was able to modestly predict inpatient mortality. Further studies are needed to delineate the impact of bystander organ dysfunction to predict mortality in patients supported with VA-ECMO.
Published: 2019

71. The Long-Lasting Activity in the Flat Spectrum Radio Quasar (FSRQ) CTA 102

Author: Felix Jankowsky, Jean-Philippe Lenain, Michael Zacharias, Markus Böttcher, Alicja Wierzcholska, Stefan Wagner, Laboratoire de Physique Nucléaire et de Hautes Énergies (LPNHE (UMR_7585)), Institut National de Physique Nucléaire et de Physique des Particules du CNRS (IN2P3)-Université Paris Diderot - Paris 7 (UPD7)-Sorbonne Université (SU)-Centre National de la Recherche Scientifique (CNRS), 24420530 - Böttcher, Markus, and 29092086 - Zacharias, Michael
Subjects: Long lasting, Active galactic nucleus, lcsh:Astronomy, Astrophysics::High Energy Astrophysical Phenomena, FOS: Physical sciences, Multi wavelength, Astrophysics, blazar variability, 01 natural sciences, blazar modeling, lcsh:QB1-991, 0103 physical sciences, Astrophysics::Solar and Stellar Astrophysics, Blazar modeling, 10. No inequality, 010303 astronomy & astrophysics, Astrophysics::Galaxy Astrophysics, High Energy Astrophysical Phenomena (astro-ph.HE), Physics, Active galactic nuclei, Multi-wavelength, Jet (fluid), 010308 nuclear & particles physics, Active Galactic Nuclei, Astronomy and Astrophysics, Observable, Quasar, Light curve, Astrophysics - Astrophysics of Galaxies, CTA-102, Multi-Wavelength, 13. Climate action, Astrophysics of Galaxies (astro-ph.GA), Blazar variability, Astrophysics - High Energy Astrophysical Phenomena, [PHYS.ASTR]Physics [physics]/Astrophysics [astro-ph]
Abstract: The flat spectrum radio quasar CTA 102 ($z = 1.032$) went through a tremendous phase of variability. Since early 2016 the gamma-ray flux level has been significantly higher than in previous years. It was topped by a four month long giant outburst, where peak fluxes were more than 100 times higher than the quiescence level. Similar trends are observable in optical and X-ray energies. We have explained the giant outburst as the ablation of a gas cloud by the relativistic jet that injects additional matter into the jet and can self-consistently explain the long-term light curve. Here, we argue that the cloud responsible for the giant outburst is part of a larger system that collides with the jet and is responsible for the years-long activity in CTA 102., 9 pages, 5 figures, accepted by Galaxies as part of the special issue "Monitoring the non-thermal Universe", a conference held in Cochem, Germany, 17th - 21st September 2018
Published: 2019

72. First-in-Human Experience With Transcatheter Mitral Valve-in-Valve Implantation During Left Ventricular Assist Device Placement

Author: Guilherme F. Attizzani, Mahmoud Farhoud, Guilherme H. Oliveira, Soon J. Park, Mahazarin Ginwalla, Sadeer G. Al-Kindi, Michael Zacharias, Benjamin Medalion, Salil V. Deo, Monique R. Robinson, Basar Sareyyupoglu, Gabriela Orasanu, and Chantal ElAmm
Subjects: Male, medicine.medical_specialty, Cardiac Catheterization, medicine.medical_treatment, 030204 cardiovascular system & hematology, Prosthesis Design, Ventricular Function, Left, 03 medical and health sciences, 0302 clinical medicine, Mitral valve stenosis, Internal medicine, Mitral valve, medicine, Humans, Mitral Valve Stenosis, cardiovascular diseases, Aged, Bioprosthesis, Heart Failure, Heart Valve Prosthesis Implantation, Mitral regurgitation, Ejection fraction, business.industry, Mitral valve replacement, Hemodynamics, Recovery of Function, medicine.disease, Dor procedure, Surgery, Left Ventricular Aneurysm, medicine.anatomical_structure, Treatment Outcome, 030228 respiratory system, Ventricular assist device, Heart Valve Prosthesis, cardiovascular system, Cardiology, Mitral Valve, Heart-Assist Devices, Cardiology and Cardiovascular Medicine, business, Tomography, X-Ray Computed, Echocardiography, Transesophageal
Abstract: Valvular disease is common in patients undergoing left ventricular assist device (LVAD) implantation. Concomitant valve surgery increases procedural complexity and cardiopulmonary bypass time and may lead to worse outcomes.1 Although mitral regurgitation is the most common mitral valve dysfunction in patients undergoing LVAD implantation, mitral stenosis (MS) is occasionally encountered. MS can lead to restricted LVAD flow; therefore, mitral valve replacement is considered to be reasonable in patients with hemodynamically significant MS undergoing LVAD implantation. We describe a successful transcatheter mitral valve replacement (TMVR) via a transapical approach with concomitant LVAD implantation in a patient with bioprosthetic MS. Our patient is a 67-year-old male with ischemic cardiomyopathy, stage D heart failure with reduced ejection fraction, and left ventricular ejection fraction 15%. He had prior 6-vessel coronary artery bypass grafting, bioprosthetic mitral valve replacement (Medtronic Mosaic porcine mitral valve, 29-mm size) for severe mitral regurgitation, and a modified endoventricular circular patch plasty (Dor procedure) for left ventricular aneurysm repair. He had cardiac resynchronization therapy and defibrillator therapy and was paced 99% but remained symptomatic with low output symptoms, as confirmed by hemodynamic assessment. By the time of referral to our institution, he had been hospitalized multiple times in the preceding 6 months with acutely decompensated heart failure, severe ascites, and malnutrition and was maintained on home inotropic therapy with Milrinone at …
Published: 2016

73. The Complex VHE And Multiwavelength Flaring Activity Of The FSRQ PKS 1510-089 In May 2015

Author: Markus Böttcher, Alicja Wierzcholska, Nachiketa Chakraborty, Michael Zacharias, Stefan Wagner, G. Cologna, Mahmoud Mohamed, Felix Jankowsky, Heike Prokoph, Jean-Philippe Lenain, D. Zaborov, Laboratoire de Physique Nucléaire et de Hautes Énergies (LPNHE (UMR_7585)), Institut National de Physique Nucléaire et de Physique des Particules du CNRS (IN2P3)-Université Paris Diderot - Paris 7 (UPD7)-Sorbonne Université (SU)-Centre National de la Recherche Scientifique (CNRS), Laboratoire Leprince-Ringuet (LLR), Centre National de la Recherche Scientifique (CNRS)-École polytechnique (X)-Institut National de Physique Nucléaire et de Physique des Particules du CNRS (IN2P3), H.E.S.S., Institut National de Physique Nucléaire et de Physique des Particules du CNRS (IN2P3)-École polytechnique (X)-Centre National de la Recherche Scientifique (CNRS), Laboratoire de Physique Nucléaire et de Hautes Énergies ( LPNHE ), Université Pierre et Marie Curie - Paris 6 ( UPMC ) -Institut National de Physique Nucléaire et de Physique des Particules du CNRS ( IN2P3 ) -Université Paris Diderot - Paris 7 ( UPD7 ) -Centre National de la Recherche Scientifique ( CNRS ), Laboratoire Leprince-Ringuet ( LLR ), and Institut National de Physique Nucléaire et de Physique des Particules du CNRS ( IN2P3 ) -École polytechnique ( X ) -Centre National de la Recherche Scientifique ( CNRS )
Subjects: [ PHYS.ASTR ] Physics [physics]/Astrophysics [astro-ph], Astrophysics::High Energy Astrophysical Phenomena, satellite, FOS: Physical sciences, Astrophysics, Astrophysics::Cosmology and Extragalactic Astrophysics, 01 natural sciences, Spectral line, VHE, blazar, Target of opportunity, HESS, 0103 physical sciences, Optical depth (astrophysics), optical, quasar, structure, Blazar, 010303 astronomy & astrophysics, Line (formation), High Energy Astrophysical Phenomena (astro-ph.HE), Physics, Soft photon, 010308 nuclear & particles physics, photon, Quasar, acceleration, electromagnetic, Cherenkov counter, time dependence, Astrophysics - High Energy Astrophysical Phenomena, [PHYS.ASTR]Physics [physics]/Astrophysics [astro-ph], absorption, Fermi Gamma-ray Space Telescope
Abstract: The blazar PKS 1510-089 was the first of the flat spectrum radio quasar type, which had been detected simultaneously by a ground based Cherenkov telescope (H.E.S.S.) and the LAT instrument on board the Fermi satellite. Given the strong broad line region emission defining this blazar class, and the resulting high optical depth for VHE ($E>100\,$GeV) $\gamma$-rays, it was surprising to detect VHE emission from such an object. In May 2015, PKS 1510-089 exhibited high states throughout the electromagnetic spectrum. Target of Opportunity observations with the H.E.S.S. experiment revealed strong and unprecedented variability of this source. Comparison with the lightcurves obtained with the \textit{Fermi}-LAT in HE $\gamma$-rays ($100\,$MeV$, Comment: 5 pages, 2 figures, to be published in the AIP Conference Proceedings of the "High Energy Gamma-Ray Astronomy (Gamma2016)", edited by F. Aharonian, W. Hofmann, F. Rieger
Published: 2016

74. Heart failure in patients with human immunodeficiency virus infection: Epidemiology and management disparities

Author: R. Benatti, Chantal ElAmm, Emile Mehanna, Sadeer G. Al-Kindi, Michael Zacharias, Mahazarin Ginwalla, Chris T. Longenecker, and Guilherme H. Oliveira
Subjects: Adult, Male, medicine.medical_specialty, Databases, Factual, HIV Infections, Disease, 030204 cardiovascular system & hematology, Article, Cohort Studies, 03 medical and health sciences, Young Adult, 0302 clinical medicine, Acquired immunodeficiency syndrome (AIDS), Internal medicine, Epidemiology, Medicine, Electronic Health Records, Humans, 030212 general & internal medicine, Registries, Young adult, Healthcare Disparities, Aged, Retrospective Studies, Heart Failure, business.industry, Medical record, Disease Management, Cardiovascular Agents, Middle Aged, medicine.disease, United States, Anti-Retroviral Agents, Relative risk, Cardiovascular agent, Immunology, Female, Cardiology and Cardiovascular Medicine, business, Cohort study
Abstract: Persons living with HIV are at a higher risk of cardiovascular disease despite effective antiretroviral therapy and dramatic reductions in AIDS-related conditions. We sought to identify the epidemiology of heart failure (HF) among persons living with HIV in the United States in an era of contemporary antiretroviral therapy.Explorys is an electronic healthcare database that aggregates medical records from 23 healthcare systems nationwide. Using systemized nomenclature of medicine-clinical terms (SNOMED-CT), we identified adult patients (age18), who had active records over the past year (September 2014-September 2015). We described the prevalence of HF in HIV patients by demographics and treatment and compared them to HIV-uninfected controls.Overall, there were 36,400 patients with HIV and 12,208,430 controls. The overall prevalence of HF was 7.2% in HIV and 4.4% in controls (RR 1.66 [1.60-1.72], p0.0001). The relative risk of HF associated with HIV infection was higher among women and younger age groups. Patients receiving antiretroviral therapy had only marginally lower risk (6.4% vs. 7.7%, p0.0001) of HF compared to those who were untreated. Compared to uninfected patients with HF, HIV patients with HF were less likely to receive antiplatelet drugs, statins, diuretics, and ACE/ARBs (p0.0001 for all comparisons). For patients with HIV and HF, receiving care from a cardiologist was associated with higher use of antiplatelets, statins, betablockers, ACE/ARBs, and diuretics.Persons with HIV are at higher risk for HF in this large contemporary sample that includes both men and women. Although the prevalence of heart failure is higher in older HIV patients, the relative risk associated with HIV is highest in young people and in women. HIV patients are less likely to have HF optimally treated, but cardiology referral was associated with higher treatment rates.
Published: 2016

75. The extended jet of AP Librae: Origin of the very high-energy gamma-ray emission?

Author: Michael Zacharias and Stefan Wagner
Subjects: Physics, High Energy Astrophysical Phenomena (astro-ph.HE), Jet (fluid), High energy, 010308 nuclear & particles physics, Astrophysics::High Energy Astrophysical Phenomena, FOS: Physical sciences, Astronomy and Astrophysics, Astrophysics, 01 natural sciences, Space and Planetary Science, 0103 physical sciences, Astrophysics - High Energy Astrophysical Phenomena, 010303 astronomy & astrophysics
Abstract: The low-frequency peaked BL Lac object (LBL) AP Librae exhibits very-high-energy (VHE, $E>100$GeV) $\gamma$-ray emission and hosts an extended jet, which has been detected in radio and X-rays. The jet X-ray spectral index implies an inverse Compton origin. These observations are unusual for LBLs calling for a consistent explanation of this extraordinary source. The observationally constrained parameters necessary to describe the core emission within the standard one-zone model are unable to explain the broad-band spectrum, even if observationally unconstrained external photon fields are taken into account. We demonstrate that the addition of the extended jet emission successfully reproduces the total spectral energy distribution. In particular, the VHE radiation is produced in the $>100\,$kpc long extended jet via inverse Compton scattering of cosmic microwave background photons by highly relativistic electrons. We present several ways to test this theory. The extended jet is weakly magnetized ($B_0 = 2.5\,\mu$G), while its minimum and maximum electron Lorentz factors are $\gamma_{min}=60$ and $\gamma_{max}=5\times 10^6$, respectively. The electron spectral index is $s=2.6$. These parameters are comparable to parameters of other blazars with extended X-ray jets dominated by inverse Compton scattering., Comment: 12 pages, 6 figures. Accepted for publication by Astronomy & Astrophysics, V2: using traditional abstract style
Published: 2016

76. HESS observations of the Carina nebula and its enigmatic colliding wind binary Eta Carinae

Author: E. Birsin, G. Cologna, Nu. Komin, K. Egberts, Anna Szostek, S. J. Nolan, Joachim Hahn, Petter Hofverberg, K. Kosack, Konrad Bernlöhr, Heinrich J. Völk, M. Renaud, W. Kluźniak, P.-O. Petrucci, N. W. Pekeur, D. Nekrassov, G. Pühlhofer, M.-H. Grondin, J. Perez, A. Reimer, M. Naumann-Godo, M. Paz Arribas, P. Bordas, Dirk Lennarz, E. Moulin, A. Jacholkowska, Fabio Acero, A. Charbonnier, F. Feinstein, S. Heinz, C.-C. Lu, Andreas Quirrenbach, A. A. Zdziarski, Igor Oya, M. K. Daniel, S. Schwarzburg, M. Füßling, Stefan Ohm, Sarah Kaufmann, Ullrich Schwanke, Michael Zacharias, S. Pita, T. Bulik, I. Büsching, M. Dalton, L. Gérard, B. Glück, Anna Barnacka, Riaan Steenkamp, Matteo Cerruti, T. J. L. McComb, J. K. Becker, F. Krayzel, J. Dyks, A. G. Akhperjanian, G. Pelletier, S. Rosier-Lees, G. Heinzelmann, M. Mohamed, Regis Terrier, D. Klochkov, M. C. Medina, R. Kossakowski, Yvonne Becherini, B. Peyaud, A. Bochow, Werner Hofmann, Gilles Maurin, J. L. Skilton, Christo Venter, Marek Jamrozy, Andreas Hillert, M. V. Fernandes, D. Göring, R. White, A. Marcowith, Joachim Ripken, C. Jahn, Helene Sol, E. de Oña Wilhelmi, S. Häffner, A. Balzer, J. Bolmont, N. Nguyen, N. Maxted, I. Sushch, Michael Punch, Julien Masbou, Reinhard Schlickeiser, R. Moderski, J. Harris, A. Zech, Christian Stegmann, Isak Delberth Davids, M. Ostrowski, Peter Eger, Gisela Anton, A. Fiasson, Jim Hinton, L. Fallon, S. Schwemmer, Andrea Santangelo, C. van Eldik, V. Marandon, Hugh Dickinson, C. L. Naumann, David Sánchez, Gavin Rowell, Y. A. Gallant, H.-S. Zechlin, Daniel Hampf, M. Hauser, R. de los Reyes, Sabrina Casanova, F. Sheidaei, P. Espigat, Frank M. Rieger, Michal Dyrda, A. Abramowski, Ł. Stawarz, Francois Brun, G. Spengler, Francesca Volpe, J. D. Hague, B. Nicholas, André Schulz, J.-P. Tavernet, S. J. Fegan, A. Djannati-Ataï, Dieter Horns, J. Mehault, W. Domainko, Jacek Niemiec, Henning Gast, Pascal Vincent, A. Cheesebrough, Gerard Fontaine, Olaf Reimer, M. Mayer, K. Stycz, Jan Conrad, I. Jung, B. Rudak, A. Lopatin, B. Degrange, L. O'c. Drury, Anna Zajczyk, J. F. Glicenstein, Thierry Montmerle, M. de Naurois, Gilles Henri, J.-P. Lenain, F. Stinzing, Alicja Wierzcholska, B. Giebels, T. Garrigoux, Serguei Vorobiov, Krzysztof Katarzynski, M. J. Vorster, Markus Holler, Felix Aharonian, Pierre Brun, H. Laffon, K. Valerius, D. Nedbal, Thomas Lohse, M. Panter, U. Katz, M. Tluczykont, V. Sahakian, Martin Ward, C. B. Rulten, C. Boisson, B. Khélifi, G. Hermann, J. Brucker, G. Lamanna, R. C. G. Chaves, Aion Viana, B. Opitz, Jonathan Biteau, Guillaume Dubus, K. Dutson, Christoph Deil, T. Kneiske, L. Rob, Stefan Wagner, M. A. Kastendieck, G. Vasileiadis, P. M. Chadwick, A. Förster, Martin Raue, and Svenja Carrigan
Subjects: Physics, Colliding-wind binary, Spectral index, Nebula, 010308 nuclear & particles physics, Astrophysics::High Energy Astrophysical Phenomena, Flux, Astronomy and Astrophysics, Astrophysics, 01 natural sciences, Particle acceleration, Cover (topology), Space and Planetary Science, 0103 physical sciences, Absorption (logic), Supernova remnant, 010303 astronomy & astrophysics, Astrophysics::Galaxy Astrophysics
Abstract: The massive binary system Eta Carinae and the surrounding HII complex, the Carina Nebula, are potential particle acceleration sites from which very-high-energy (VHE; E > 100 GeV) \gamma-ray emission could be expected. This paper presents data collected during VHE \gamma-ray observations with the H.E.S.S. telescope array from 2004 to 2010, which cover a full orbit of Eta Carinae. In the 33.1-hour data set no hint of significant \gamma-ray emission from Eta Carinae has been found and an upper limit on the \gamma-ray flux of 7.7 x 10-13 ph cm-2 s-1 (99% confidence level) is derived above the energy threshold of 470 GeV. Together with the detection of high-energy (HE; 0.1 GeV > E > 100 GeV) \gamma-ray emission by the Fermi-LAT up to 100 GeV, and assuming a continuation of the average HE spectral index into the VHE domain, these results imply a cut-off in the \gamma-ray spectrum between the HE and VHE \gamma-ray range. This could be caused either by a cut-off in the accelerated particle distribution or by severe \gamma-\gamma\ absorption losses in the wind collision region. Furthermore, the search for extended \gamma-ray emission from the Carina Nebula resulted in an upper limit on the \gamma-ray flux of 4.2 x 10-12 ph cm-2 s-1 (99% confidence level). The derived upper limit of ~23 on the cosmic-ray enhancement factor is compared with results found for the old-age mixed-morphology supernova remnant W 28.
Published: 2012

77. A new ordering parameter of spectral energy distributions from synchrotron self-Compton emitting blazars

Author: Michael Zacharias and Reinhard Schlickeiser
Subjects: Physics, Astrophysics::High Energy Astrophysical Phenomena, Spectral density, Synchrotron radiation, Astronomy and Astrophysics, Electron, Radiation, Spectral line, Synchrotron, Computational physics, law.invention, Space and Planetary Science, law, Kinetic equations, Blazar
Abstract: The broad-band SEDs of blazars exhibit two broad spectral components, which in leptonic emission models are attributed to synchrotron radiation and synchrotron self-Compton (SSC) radiation of relativistic electrons. During high-state phases, the high-frequency SSC component often dominates the low-frequency synchrotron component, implying that the inverse-Compton SSC losses of electrons are at least equal to or greater than the synchrotron losses of electrons. We calculate from the analytical solution of the kinetic equation of relativistic electrons, subject to the combined linear synchrotron and non-linear SSC cooling, for monoenergetic injection the time-integrated total synchrotron and SSC radiation fluences and spectral energy distributions (SEDs). Depending on the ratio of the initial cooling terms, displayed by the injection parameter α, we find for α≪ 1, implying complete linear cooling, that the synchrotron peak dominates the inverse-Compton peak and the usual results of the spectra are recovered. For α≫ 1, the SSC peak dominates the synchrotron peak, proving our assumption that in such a case the cooling becomes initially non-linear. The spectra also show some unique features, which can be attributed directly to the non-linear cooling. To show the potential of the model, we apply it to outbursts of 3C 279 and 3C 454.3, successfully reproducing the SEDs. The results of our analysis are promising, and we argue that this non-equilibrium model should be considered in future modelling attempts for blazar flares.
Published: 2011

78. Weight and Mortality Following Heart Failure Hospitalization among Diabetic Patients

Author: Darleen M. Lessard, Jane S. Saczynski, Joel M. Gore, Molly E. Waring, Robert J. Goldberg, Michael Zacharias, and David D. McManus
Subjects: Male, medicine.medical_specialty, Type 2 diabetes, Overweight, Article, Diabetes Complications, Thinness, Risk Factors, Cause of Death, Internal medicine, Diabetes mellitus, Odds Ratio, medicine, Humans, Obesity, Risk factor, Intensive care medicine, Aged, Proportional Hazards Models, Aged, 80 and over, Heart Failure, business.industry, Body Weight, General Medicine, Middle Aged, Prognosis, medicine.disease, Survival Analysis, Hospitalization, Diabetes Mellitus, Type 2, Massachusetts, Heart failure, Acute Disease, Female, Underweight, medicine.symptom, business, Body mass index
Abstract: BACKGROUND: Type 2 diabetes is an important risk factor for heart failure and is common among patients with heart failure. The impact of weight on prognosis after hospitalization for acute heart failure among patients with diabetes is unknown. The objective of this study was to examine all-cause mortality in relation to weight status among patients with type 2 diabetes hospitalized for decompensated heart failure. METHODS: The Worcester Heart Failure Study included adults admitted with acute heart failure to all metropolitan Worcester medical centers in 1995 and 2000. The weight status of 1644 patients with diabetes (history of type 2 diabetes in medical record or admission serum glucose 200 mg/dL) was categorized using body mass index calculated from height and weight at admission. Survival status was ascertained at 1 and 5 years after hospital admission. RESULTS: Sixty-five percent of patients were overweight or obese and 3% were underweight. Underweight patients had 50% higher odds of all-cause mortality within 5 years of hospitalization for acute heart failure than normal weight patients. Class I and II obesity were associated with 20% and 40% lower odds of dying. Overweight and Class III obesity were not associated with mortality. Results were similar for mortality within 1 year of hospitalization for acute heart failure. CONCLUSIONS: The mechanisms underlying the association between weight status and mortality are not fully understood. Additional research is needed to explore the effects of body composition, recent weight changes, and prognosis after hospitalization for heart failure among patients with diabetes.
Published: 2011

79. Preoperative MELD-XI is not Associated with Mortality after LVAD

Author: Muhammad S. Panhwar, Benjamin Medalian, Salil V. Deo, Linda Njoroge, Mohamed Khayata, Michael Zacharias, Monique R. Robinson, Sadeer G. Al-Kindi, Chantal ElAmm, Guilherme H. Oliveira, and Mahazarin Ginwalla
Subjects: Heart transplantation, medicine.medical_specialty, Heartmate ii, business.industry, medicine.medical_treatment, Mean age, 030204 cardiovascular system & hematology, medicine.disease, body regions, 03 medical and health sciences, Liver disease, 0302 clinical medicine, Heart failure, Internal medicine, medicine, Cardiology, Referral center, In patient, 030212 general & internal medicine, Liver dysfunction, Cardiology and Cardiovascular Medicine, business
Abstract: Background Kidney and liver dysfunction are common in patients with advanced heart failure undergoing left ventricular assistant device (LVAD) implantation. We have previously shown that Model of End-Stage Liver Disease excluding INR (MELD-XI) scores can predict poor outcomes after heart transplantation. Whether MELD-XI predicts outcomes after LVAD implantation is not well understood. Methods All patients who underwent LVAD implantation at a tertiary referral center (2007-2017) were included and preoperative MELD-XI was calculated. Cox proportional hazard models and Kaplan Meier method were used to describe association with overall post-implant mortality. Penalized smoothed splines were used to visualize the association between continuous MELDXI and mortality. Results A total of 94 patients were included. Mean age was 60±13 years, 78% males, 64% Caucasian, 76% had the HeartMate II. Median MELD-XI was 12.4(9.9-15.9). At a median follow-up of 2.8 years, 31 patients died. There was no difference between patients with MELD-XI >12.4 and MELD-XI ≤12.4 in overall mortality ( P =0.14), figure (panel A). There was no association between continuous MELD-XI and mortality (HR 1.04; 95% CI: 0.96-1.13, P =0.32), figure (panel B). Conclusion Our findings showed that MELD-XI is not associated with mortality after LVAD implantation. These findings need to be validated in a larger group registry to identify best bridging strategy in patients with advanced heart failure and combined kidney-liver dysfunction.
Published: 2018

80. Cloud Ablation by a Relativistic Jet and the Extended Flare in CTA 102 in 2016 and 2017

Author: Felix Jankowsky, Alicja Wierzcholska, Markus Böttcher, J.-P. Lenain, Stefan Wagner, Michael Zacharias, Laboratoire de Physique Nucléaire et de Hautes Énergies (LPNHE (UMR_7585)), Institut National de Physique Nucléaire et de Physique des Particules du CNRS (IN2P3)-Université Paris Diderot - Paris 7 (UPD7)-Sorbonne Université (SU)-Centre National de la Recherche Scientifique (CNRS), Laboratoire de Physique Nucléaire et de Hautes Énergies ( LPNHE ), Université Pierre et Marie Curie - Paris 6 ( UPMC ) -Institut National de Physique Nucléaire et de Physique des Particules du CNRS ( IN2P3 ) -Université Paris Diderot - Paris 7 ( UPD7 ) -Centre National de la Recherche Scientifique ( CNRS ), 24420530 - Böttcher, Markus, and 29092086 - Zacharias, Michael
Subjects: active [Galaxies], Particle number, [ PHYS.ASTR ] Physics [physics]/Astrophysics [astro-ph], Astrophysics::High Energy Astrophysical Phenomena, medicine.medical_treatment, galaxies: active, FOS: Physical sciences, Flux, Astrophysics, 01 natural sciences, law.invention, law, 0103 physical sciences, medicine, quasars: individual, 010303 astronomy & astrophysics, relativistic processes, High Energy Astrophysical Phenomena (astro-ph.HE), Physics, Jet (fluid), non-thermal [Radiation mechanisms], 010308 nuclear & particles physics, Relativistic processes, individual (CTA 102) [Quasars], Astronomy and Astrophysics, Quasar, radiation mechanisms: non-thermal, Ablation, Astrophysics - Astrophysics of Galaxies, CTA-102, 13. Climate action, Space and Planetary Science, Astrophysics of Galaxies (astro-ph.GA), Astrophysics - High Energy Astrophysical Phenomena, [PHYS.ASTR]Physics [physics]/Astrophysics [astro-ph], Event (particle physics), Flare
Abstract: In late 2016 and early 2017 the flat spectrum radio quasar CTA 102 exhibited a very strong and long-lasting outburst. The event can be described by a roughly 2 months long increase of the baseline flux in the monitored energy bands (optical to $\gamma$ rays) by a factor 8, and a subsequent decrease over another 2 months back to pre-flare levels. The long-term trend was superseded by short but very strong flares, resulting in a peak flux that was a factor 50 above pre-flare levels in the $\gamma$-ray domain and almost a factor 100 above pre-flare levels in the optical domain. In this paper we explain the long-term evolution of the outburst by the ablation of a gas cloud penetrating the relativistic jet. The slice-by-slice ablation results in a gradual increase of the particle injection until the center of the cloud is reached, after which the injected number of particles decreases again. With reasonable cloud parameters we obtain excellent fits of the long-term trend., Comment: 9 pages, 5 figures; accepted for publication in The Astrophysical Journal
Published: 2017

81. Synchrotron fluence of nonlinearly cooled relativistic electrons with instantaneous flat power law injection

Author: Michael Zacharias and Reinhard Schlickeiser
Subjects: Physics, Spectral index, Astrophysics::High Energy Astrophysical Phenomena, Astronomy and Astrophysics, Electron, Astrophysics, Radiation, Kinetic energy, Fluence, Power law, Synchrotron, Magnetic field, law.invention, Space and Planetary Science, law, Atomic physics
Abstract: Context. In powerful cosmic nonthermal radiation sources with a dominant magnetic field self generation, partition between the energy densities in magnetic fields and relativistic electrons is expected. As the electrons cool by synchrotron emission, the magnetic field strength becomes time-dependent and adjusts itself to the actual kinetic energy density of the radiating electrons. Aims. For the case of instantaneous injection of power law distributed electrons with a flat power law spectral index, the nonlinear synchrotron fluence is calculated. Methods. Results. For flat (spectral index 1 < s < 2) injected power laws the nonlinear synchrotron fluence at small frequencies approaches a power law ∝v ―0.6 , independent of the value of s, which is identical to the synchrotron fluence behaviour for steep injected power laws.
Published: 2009

82. Discovery of the VHE gamma-ray source HESS J1832-093 in the vicinity of SNR G22.7-0.2

Author: Julien Lefaucheur, J. Biteau, Matteo Cerruti, M. Holler, Matthias Weidinger, F. Krayzel, Tanya Edwards, M. Paz Arribas, Christo Venter, Dirk Lennarz, K. Dutson, F. Spies, Mateusz Janiak, Alexandre Marcowith, C. Jahn, S. Raab, A. Abramowski, C. L. Naumann, R. C. G. Chaves, M. K. Daniel, C. Stegmann, U. F. Katz, R. Moderski, A. Zech, Frank M. Rieger, Gilles Henri, G. Fontaine, Ullrich Schwanke, Iurii Sushch, Werner Hofmann, P. M. Chadwick, Nu. Komin, S. Krakau, Pierre-Olivier Petrucci, A. Fiasson, S. Häffner, Pierre Brun, Ramin Marx, M. Mohamed, A. G. Akhperjanian, Christoph Deil, M. Kieffer, Denis Wouters, T. Kneiske, Stefan Ohm, Aion Viana, V. Sahakian, M. de Naurois, Martin Ward, Jim Hinton, P. Willmann, S. Pita, F. Stinzing, Michal Dyrda, R. Steenkamp, F. Ait Benkhali, S. Schwemmer, B. Opitz, B. Giebels, S. Schwarzburg, Cameron B Rulten, L. O'c. Drury, P. deWilt, E. de Oña Wilhelmi, W. Kluźniak, Sarah Kaufmann, K. Katarzyński, S. J. Nolan, S. Balenderan, S. Klepser, A. C. Clapson, Joachim Hahn, Andrea Santangelo, S. Colafrancesco, Guillaume Dubus, C. Couturier, L. Oakes, M. Tluczykont, Marek Jamrozy, J. Dyks, Andreas Quirrenbach, Łukasz Stawarz, Felix Aharonian, Manuel Meyer, Michael Zacharias, Heinrich J. Völk, Stefan Wagner, Gisela Anton, M. Mayer, Helene Sol, J. Brucker, P.P. Krüger, K. Valerius, R. Chalme-Calvet, M. Panter, R. D. Parsons, J. Harris, Quirin Weitzel, A. Cheesebrough, M. Gajdus, C. Romoli, L. Rob, Elisabetta Bissaldi, Daniel Sánchez, Konrad Bernlöhr, Jan Conrad, K. Stycz, P. Vincent, M. J. Vorster, J. F. Glicenstein, Tomasz Bulik, D. Fernandez, Vincent Marandon, Victor Zabalza, U. Menzler, Gianluca Giavitto, G. Cologna, C. van Eldik, B. van Soelen, I. Jung, B. Rudak, Kathrin Egberts, M. A. Kastendieck, B. Degrange, I. D. Davids, G. Pühlhofer, Markus Böttcher, G. Spengler, M. Füßling, G. Vasileiadis, J. Perez, Y. Cui, Karl Kosack, A. Jacholkowska, A. Reimer, Catherine Boisson, Felix Jankowsky, Fabio Acero, T. J. L. McComb, S. Rosier-Lees, H. Laffon, Andreas Hillert, J. Becker Tjus, T. Vuillaume, Michał Ostrowski, G. Lamanna, W. Domainko, M. Renaud, A. Balzer, M. V. Fernandes, Sabrina Casanova, B. Peyaud, Y. A. Gallant, H.-S. Zechlin, R. White, C. Trichard, Thomas Lohse, A. Wörnlein, M. Grudzińska, P. J. Meintjes, Francois Brun, M. Chrétien, Chia-Chun Lu, Anna Zajczyk, N. W. Pekeur, D. Kolitzus, M. Dalton, Gavin Rowell, A. Djannati-Ataï, Peter Eger, P. Wagner, Guy Pelletier, A. Förster, R. de los Reyes, C. Farnier, Martin Raue, Andrew M. Taylor, B. Khélifi, G. Hermann, Regis Terrier, F. Schüssler, T. Garrigoux, O. Hervet, P. Espigat, D. Klochkov, Marianne Lemoine-Goumard, I. Oya, Jacek Niemiec, A. Lemière, Olaf Reimer, Michael Punch, N. Maxted, Anna Szostek, S. J. Fegan, Thomas Murach, Svenja Carrigan, E. Birsin, Petter Hofverberg, Emmanuel Moulin, André Schulz, J. Méhault, F. Feinstein, Dieter Horns, A. A. Zdziarski, J.-P. Tavernet, Yvonne Becherini, G. Maurin, M. H. Grondin, Francesca Volpe, Helen Poon, A. Lopatin, J.-P. Lenain, Reinhard Schlickeiser, Pol Bordas, Hugh Dickinson, E. O. Angüner, G. Heinzelmann, J. Bolmont, Anna Barnacka, Alicja Wierzcholska, T. Tavernier, Institut für Experimentalphysik [Hamburg], Universität Hamburg (UHH), CEA- Saclay (CEA), Commissariat à l'énergie atomique et aux énergies alternatives (CEA), Max Planck Institute for Nuclear Physics (MPIK), Max-Planck-Gesellschaft, Dublin Institute for Advanced Studies (DIAS), National Academy of Sciences of the Republic of Armenia [Yerevan] (NAS RA), Humboldt-Universität zu Berlin, Physikalisches Institut [Erlangen], Friedrich-Alexander Universität Erlangen-Nürnberg (FAU), Department of Physics [Durham], University of New Hampshire (UNH), Deutsches Elektronen-Synchrotron [Zeuthen] (DESY), Helmholtz-Gemeinschaft = Helmholtz Association, Universität Potsdam, Astronomical Observatory [Warsaw], Faculty of Physics [Warsaw] (FUW), University of Warsaw (UW)-University of Warsaw (UW), Linnaeus University, Institut für Theoretische Physik IV [Bochum] (ITP4), Ruhr-Universität Bochum [Bochum], Institut f¨ur Astro- und Teilchenphysik and Institut f¨ur Theoretische Physik, Leopold-Franzens Universitat Innsbruck, Laboratoire Leprince-Ringuet (LLR), Centre National de la Recherche Scientifique (CNRS)-École polytechnique (X)-Institut National de Physique Nucléaire et de Physique des Particules du CNRS (IN2P3), North-West University [South Aftrica] (NWU), Laboratoire Univers et Théories (LUTH (UMR_8102)), Centre National de la Recherche Scientifique (CNRS)-Université de Paris (UP)-Observatoire de Paris, Université Paris sciences et lettres (PSL)-Université Paris sciences et lettres (PSL)-Institut national des sciences de l'Univers (INSU - CNRS), Laboratoire de Physique Nucléaire et de Hautes Énergies (LPNHE), Centre National de la Recherche Scientifique (CNRS)-Université Paris Diderot - Paris 7 (UPD7)-Institut National de Physique Nucléaire et de Physique des Particules du CNRS (IN2P3)-Université Pierre et Marie Curie - Paris 6 (UPMC), Institut für Astronomie und Astrophysik [Tübingen] (IAAT), Eberhard Karls Universität Tübingen = Eberhard Karls University of Tuebingen, Institut de Recherches sur les lois Fondamentales de l'Univers (IRFU), Commissariat à l'énergie atomique et aux énergies alternatives (CEA)-Université Paris-Saclay, Institut national des sciences de l'Univers (INSU - CNRS)-Observatoire de Paris, Université Paris sciences et lettres (PSL)-Université Paris sciences et lettres (PSL)-Centre National de la Recherche Scientifique (CNRS)-Université Paris Diderot - Paris 7 (UPD7), Harvard-Smithsonian Center for Astrophysics (CfA), Smithsonian Institution-Harvard University [Cambridge], University of the Witwatersrand [Johannesburg] (WITS), Landessternwarte Königstuhl [ZAH] (LSW), Universität Heidelberg [Heidelberg], Stockholm University, Centre d'Etudes Nucléaires de Bordeaux Gradignan (CENBG), Université Sciences et Technologies - Bordeaux 1-Institut National de Physique Nucléaire et de Physique des Particules du CNRS (IN2P3)-Centre National de la Recherche Scientifique (CNRS), Namibia University of Science and Technology (NUST), University of Adelaide, Oskar Klein Centre [Stockholm], AstroParticule et Cosmologie (APC (UMR_7164)), Observatoire de Paris, Université Paris sciences et lettres (PSL)-Université Paris sciences et lettres (PSL)-Commissariat à l'énergie atomique et aux énergies alternatives (CEA)-Université Paris Diderot - Paris 7 (UPD7)-Centre National de la Recherche Scientifique (CNRS)-Institut National de Physique Nucléaire et de Physique des Particules du CNRS (IN2P3), Institut de Planétologie et d'Astrophysique de Grenoble (IPAG ), Centre National d'Études Spatiales [Toulouse] (CNES)-Centre National de la Recherche Scientifique (CNRS)-Observatoire des Sciences de l'Univers de Grenoble (OSUG), Université Joseph Fourier - Grenoble 1 (UJF)-Institut polytechnique de Grenoble - Grenoble Institute of Technology (Grenoble INP )-Institut national des sciences de l'Univers (INSU - CNRS)-Institut national de recherche en sciences et technologies pour l'environnement et l'agriculture (IRSTEA)-Université Savoie Mont Blanc (USMB [Université de Savoie] [Université de Chambéry])-Centre National de la Recherche Scientifique (CNRS)-Université Joseph Fourier - Grenoble 1 (UJF)-Institut polytechnique de Grenoble - Grenoble Institute of Technology (Grenoble INP )-Institut national des sciences de l'Univers (INSU - CNRS)-Institut national de recherche en sciences et technologies pour l'environnement et l'agriculture (IRSTEA)-Université Savoie Mont Blanc (USMB [Université de Savoie] [Université de Chambéry])-Centre National de la Recherche Scientifique (CNRS), Department of Physics and Astronomy [Leicester], University of Leicester, Instytut Fizyki Jądrowej PAN (IFJ), Polskiej Akademii Nauk, Laboratoire Univers et Particules de Montpellier (LUPM), Centre National de la Recherche Scientifique (CNRS)-Université de Montpellier (UM)-Institut National de Physique Nucléaire et de Physique des Particules du CNRS (IN2P3)-Université Montpellier 2 - Sciences et Techniques (UM2), Laboratoire d'Annecy de Physique des Particules (LAPP), Institut National de Physique Nucléaire et de Physique des Particules du CNRS (IN2P3)-Université Savoie Mont Blanc (USMB [Université de Savoie] [Université de Chambéry])-Centre National de la Recherche Scientifique (CNRS), Institut für Physik und Astrophysik [Potsdam], Obserwatorium Astronomiczne, Uniwersytet Jagiello?ski, Torun Centre for Astronomy (TCfA), Nicolaus Copernicus University [Toruń], University of the Free State [South Africa], Université Pierre et Marie Curie - Paris 6 - UFR de Médecine Pierre et Marie Curie (UPMC), Université Pierre et Marie Curie - Paris 6 (UPMC), Astronomical Observatory [Kraków], Uniwersytet Jagielloński w Krakowie = Jagiellonian University (UJ), Institut für Experimentalphysik [Innsbruck], Universität Innsbruck [Innsbruck], Institute of Astronomy [Prague], Charles University [Prague] (CU), HESS, H.E.S.S. Collaboration, Humboldt University Of Berlin, University of Potsdam = Universität Potsdam, Institut National de Physique Nucléaire et de Physique des Particules du CNRS (IN2P3)-École polytechnique (X)-Centre National de la Recherche Scientifique (CNRS), Université Paris sciences et lettres (PSL)-Université Paris sciences et lettres (PSL)-Centre National de la Recherche Scientifique (CNRS)-Université Paris Cité (UPCité), Université Pierre et Marie Curie - Paris 6 (UPMC)-Institut National de Physique Nucléaire et de Physique des Particules du CNRS (IN2P3)-Université Paris Diderot - Paris 7 (UPD7)-Centre National de la Recherche Scientifique (CNRS), Université Paris sciences et lettres (PSL)-Université Paris sciences et lettres (PSL)-Université Paris Diderot - Paris 7 (UPD7)-Centre National de la Recherche Scientifique (CNRS), Harvard University-Smithsonian Institution, Universität Heidelberg [Heidelberg] = Heidelberg University, Université Sciences et Technologies - Bordeaux 1 (UB)-Institut National de Physique Nucléaire et de Physique des Particules du CNRS (IN2P3)-Centre National de la Recherche Scientifique (CNRS), Commissariat à l'énergie atomique et aux énergies alternatives (CEA)-Institut National de Physique Nucléaire et de Physique des Particules du CNRS (IN2P3)-Observatoire de Paris, Observatoire des Sciences de l'Univers de Grenoble (OSUG), Université Joseph Fourier - Grenoble 1 (UJF)-Institut polytechnique de Grenoble - Grenoble Institute of Technology (Grenoble INP )-Institut national des sciences de l'Univers (INSU - CNRS)-Institut national de recherche en sciences et technologies pour l'environnement et l'agriculture (IRSTEA)-Université Savoie Mont Blanc (USMB [Université de Savoie] [Université de Chambéry])-Centre National de la Recherche Scientifique (CNRS)-Université Joseph Fourier - Grenoble 1 (UJF)-Institut polytechnique de Grenoble - Grenoble Institute of Technology (Grenoble INP )-Institut national des sciences de l'Univers (INSU - CNRS)-Institut national de recherche en sciences et technologies pour l'environnement et l'agriculture (IRSTEA)-Université Savoie Mont Blanc (USMB [Université de Savoie] [Université de Chambéry])-Centre National de la Recherche Scientifique (CNRS)-Centre National d'Études Spatiales [Toulouse] (CNES)-Centre National de la Recherche Scientifique (CNRS), Institut National de Physique Nucléaire et de Physique des Particules du CNRS (IN2P3)-Université de Montpellier (UM)-Centre National de la Recherche Scientifique (CNRS), University of the Free State [South Africa] (UFS), 24420530 - Böttcher, Markus, 23909196 - Casanova, Sabrina, 13146629 - Davids, Isak Delberth, 11749903 - Krüger, Petrus Paulus, 22050574 - Pekeur, Nicolette Whilna, 24922986 - Sushch, Iurii, 12006653 - Venter, Christo, and 12792322 - Vorster, Michael Johannes
Subjects: Photon, ISM: individual objects: HESS J1832−093, Point source, Astrophysics::High Energy Astrophysical Phenomena, Hochenergie-Astrophysik Theorie - Abteilung Hofmann, Gamma rays: general, FOS: Physical sciences, Cosmic ray, Astrophysics, individual objects: HESS J1832−093 [ISM], Pulsar wind nebula, general. [Gamma-rays], Astroparticle physics, Gamma-rays: general, ISM: individual objects: HESS J1832-093, ISM: individual objects: SNR G22.7-0.2, Astronomy and Astrophysics, Space and Planetary Science, individual objects: SNR G22.7−0.2 [ISM], Supernova remnant, HESS - Abteilung Hofmann, Astrophysics::Galaxy Astrophysics, Physics, High Energy Astrophysical Phenomena (astro-ph.HE), Molecular cloud, [SDU.ASTR.HE]Sciences of the Universe [physics]/Astrophysics [astro-ph]/High Energy Astrophysical Phenomena [astro-ph.HE], Gamma ray, Institut für Physik und Astronomie, Astronomy, ddc:520, High Energy Physics::Experiment, ISM: individual objects: SNR G22.7−0.2, Astrophysics - High Energy Astrophysical Phenomena, general [gamma-rays]
Abstract: Monthly notices of the Royal Astronomical Society 446(2), 1163 - 1169 (2015). doi:10.1093/mnras/stu2148, The region around the supernova remnant (SNR) W41 contains several TeV sources and has prompted the HESS Collaboration to perform deep observations of this field of view. This resulted in the discovery of the new very high energy (VHE) source HESS J1832−093, at the position $RA=18^{h}32^{m}50^{s} \pm 3^{s}_{stat}\pm2^{s}_{syst},Dec=−9^\circ22^{\prime} 36^{\prime\prime} \pm 32^{\prime\prime}_{stat} \pm 20^{\prime\prime}_{syst}(J2000)$, spatially coincident with a part of the radio shell of the neighbouring remnant G22.7−0.2. The photon spectrum is well described by a power law of index Γ = 2.6 $\pm$ 0.3$_{stat}$ $\pm$ 0.1$_{syst}$ and a normalization at 1 TeV of Φ$_{0}=(4.8 \pm 0.8_{stat} \pm 1.0_{syst}) ×10^{−13}cm^{−2}s^{−1}TeV^{−1}$. The location of the gamma-ray emission on the edge of the SNR rim first suggested a signature of escaping cosmic rays illuminating a nearby molecular cloud. Then a dedicated XMM–Newton observation led to the discovery of a new X-ray point source spatially coincident with the TeV excess. Two other scenarios were hence proposed to identify the nature of HESS J1832−093. Gamma-rays from inverse Compton radiation in the framework of a pulsar wind nebula scenario or the possibility of gamma-ray production within a binary system are therefore also considered. Deeper multiwavelength observations will help to shed new light on this intriguing VHE source., Published by Oxford Univ. Press, Oxford
Published: 2015

83. Search for dark matter annihilation signatures in H.E.S.S. observations of dwarf spheroidal galaxies

Author: S. Rosier-Lees, Jacco Vink, Sabrina Casanova, H. Sano, D. Gottschall, P. Vincent, M. J. Vorster, Marie-Hélène Grondin, Christo Venter, V. Sahakian, M. de Naurois, S. J. Fegan, Petter Hofverberg, Denis Wouters, Michael Punch, Stefano Gabici, C. Jahn, Svenja Carrigan, Tanya Edwards, R. Moderski, A. Zech, Quirin Weitzel, G. Fontaine, A. Jacholkowska, J. Lau, A. Ivascenko, I. D. Davids, Y. Cui, E. Birsin, Y. A. Gallant, H.-S. Zechlin, Robert Wagner, Thomas Lohse, W. Kluźniak, J. Becker Tjus, T. Vuillaume, I. Reichardt, H. Laffon, F. Feinstein, Andreas Quirrenbach, F. Krayzel, S. Krakau, G. Heinzelmann, J. Bolmont, Alicja Wierzcholska, Ramin Marx, C. Couturier, D. Fernandez, M. Grudzińska, N. W. Pekeur, Axel Donath, Christian Stegmann, Stefan Wagner, S. Schwarzburg, M. Kieffer, Martin Ward, Cameron B Rulten, P. Wagner, S. Balenderan, P. Willmann, Vincent Marandon, Michal Dyrda, F. Ait Benkhali, M. A. Kastendieck, A. Fiasson, Markus Holler, Andrew M. Taylor, P. P. Krueger, Nachiketa Chakraborty, André Schulz, J. Méhault, Michael Zacharias, S. Schwemmer, Werner Hofmann, Michał Ostrowski, Michael Backes, Emmanuel Moulin, Felix Aharonian, G. Vasileiadis, Dieter Horns, J. Dyks, Anna Barnacka, Ł. Stawarz, O. Hervet, T. Garrigoux, J. Biteau, R. D. Parsons, Jan Conrad, Andrea Santangelo, A. A. Zdziarski, R. C. G. Chaves, K. Valerius, Heinrich J. Völk, Alexandre Marcowith, D. Kolitzus, Pierre Brun, Julien Lefaucheur, Manuel Meyer, Mateusz Janiak, K. Morå, Helen Poon, Gilles Henri, Marek Jamrozy, Pierre-Olivier Petrucci, W. Domainko, A. Wörnlein, M. Panter, A. Balzer, David Berge, Gianluca Giavitto, A. Lopatin, David Sanchez, Guy Pelletier, Ruizhi Yang, L. O'c. Drury, D. Klochkov, A. Djannati-Ataï, A. Förster, S. Häffner, Helene Sol, Stefan Ohm, Uli Katz, S. Pita, J.-P. Lenain, S. Bernhard, Aion Viana, Alison Mitchell, B. van Soelen, B. Rudak, Kathrin Egberts, S. Klepser, B. Degrange, Frank M. Rieger, J. Harris, C. Romoli, Guillaume Dubus, K. Bernloehr, Gavin Rowell, M. Bryan, Matthias Weidinger, David Salek, S. Colafrancesco, Reinhard Schlickeiser, Karl Kosack, Tomasz Bulik, B. Opitz, D. Zaborov, T. Tavernier, R. de los Reyes, Pol Bordas, Yvonne Becherini, F. Stinzing, M. Dalton, B. Giebels, Johan Bregeon, P. M. Chadwick, J.-P. Tavernet, G. Maurin, E. O. Angüner, M. Paz Arribas, M. Mayer, M. Tluczykont, C. Farnier, U. Menzler, K. Dutson, F. Spies, L. Oakes, Ullrich Schwanke, N. Maxted, Francesca Volpe, M. Gajdus, B. Khélifi, Y. Fukui, G. Hermann, Regis Terrier, F. Schüssler, Marianne Lemoine-Goumard, S. J. Nolan, Joachim Hahn, V. Lefranc, Victor Zabalza, A. G. Akhperjanian, R. Chalme-Calvet, Satoshi Yoshiike, Andreas Hillert, R. Steenkamp, K. Stycz, Christoph Deil, S. Raab, A. Abramowski, Catherine Boisson, J. F. Glicenstein, Jim Hinton, Nu. Komin, H. Odaka, M. Füßling, Sarah Kaufmann, J. Veh, Markus Böttcher, T. J. L. McComb, B. Peyaud, R. White, P. J. Meintjes, Francois Brun, M. Chrétien, P. deWilt, K. Katarzyński, P. Espigat, I. Jung-Richardt, I. Oya, Jacek Niemiec, A. Lemière, Olaf Reimer, Thomas Murach, G. Lamanna, Felix Spanier, G. Cologna, C. van Eldik, Felix Jankowsky, M. Renaud, Chia-Chun Lu, G. Pühlhofer, A. Reimer, Iurii Sushch, T. Fukuda, D. Hadasch, G. Spengler, M. Mohamed, M. V. Fernandes, C. Trichard, Peter Eger, H.E.S.S. Collaboration, Laboratoire Leprince-Ringuet (LLR), Centre National de la Recherche Scientifique (CNRS)-École polytechnique (X)-Institut National de Physique Nucléaire et de Physique des Particules du CNRS (IN2P3), Laboratoire Univers et Théories (LUTH (UMR_8102)), Institut national des sciences de l'Univers (INSU - CNRS)-Observatoire de Paris, Université Paris sciences et lettres (PSL)-Université Paris sciences et lettres (PSL)-Centre National de la Recherche Scientifique (CNRS)-Université Paris Diderot - Paris 7 (UPD7), Laboratoire de Physique Nucléaire et de Hautes Énergies (LPNHE (UMR_7585)), Institut National de Physique Nucléaire et de Physique des Particules du CNRS (IN2P3)-Université Paris Diderot - Paris 7 (UPD7)-Sorbonne Université (SU)-Centre National de la Recherche Scientifique (CNRS), Laboratoire Univers et Particules de Montpellier (LUPM), Université Montpellier 2 - Sciences et Techniques (UM2)-Institut National de Physique Nucléaire et de Physique des Particules du CNRS (IN2P3)-Université de Montpellier (UM)-Centre National de la Recherche Scientifique (CNRS), Centre d'Etudes Nucléaires de Bordeaux Gradignan (CENBG), Université Sciences et Technologies - Bordeaux 1-Institut National de Physique Nucléaire et de Physique des Particules du CNRS (IN2P3)-Centre National de la Recherche Scientifique (CNRS), AstroParticule et Cosmologie (APC (UMR_7164)), Observatoire de Paris, Université Paris sciences et lettres (PSL)-Université Paris sciences et lettres (PSL)-Commissariat à l'énergie atomique et aux énergies alternatives (CEA)-Université Paris Diderot - Paris 7 (UPD7)-Centre National de la Recherche Scientifique (CNRS)-Institut National de Physique Nucléaire et de Physique des Particules du CNRS (IN2P3), Laboratoire d'Annecy de Physique des Particules (LAPP), Institut National de Physique Nucléaire et de Physique des Particules du CNRS (IN2P3)-Université Savoie Mont Blanc (USMB [Université de Savoie] [Université de Chambéry])-Centre National de la Recherche Scientifique (CNRS), Laboratoire d'Annecy-le-Vieux de Physique Théorique (LAPTH), Université Savoie Mont Blanc (USMB [Université de Savoie] [Université de Chambéry])-Centre National de la Recherche Scientifique (CNRS), HESS, Institut National de Physique Nucléaire et de Physique des Particules du CNRS (IN2P3)-École polytechnique (X)-Centre National de la Recherche Scientifique (CNRS), Université Paris sciences et lettres (PSL)-Université Paris sciences et lettres (PSL)-Université Paris Diderot - Paris 7 (UPD7)-Centre National de la Recherche Scientifique (CNRS), Laboratoire de Physique Nucléaire et de Hautes Énergies (LPNHE), Université Pierre et Marie Curie - Paris 6 (UPMC)-Institut National de Physique Nucléaire et de Physique des Particules du CNRS (IN2P3)-Université Paris Diderot - Paris 7 (UPD7)-Centre National de la Recherche Scientifique (CNRS), Université Montpellier 2 - Sciences et Techniques (UM2)-Institut National de Physique Nucléaire et de Physique des Particules du CNRS (IN2P3)-Centre National de la Recherche Scientifique (CNRS), Université Sciences et Technologies - Bordeaux 1 (UB)-Institut National de Physique Nucléaire et de Physique des Particules du CNRS (IN2P3)-Centre National de la Recherche Scientifique (CNRS), Commissariat à l'énergie atomique et aux énergies alternatives (CEA)-Institut National de Physique Nucléaire et de Physique des Particules du CNRS (IN2P3)-Observatoire de Paris, Université de Montpellier (UM)-Université Montpellier 2 - Sciences et Techniques (UM2)-Institut National de Physique Nucléaire et de Physique des Particules du CNRS (IN2P3)-Centre National de la Recherche Scientifique (CNRS), Institut National de Physique Nucléaire et de Physique des Particules du CNRS (IN2P3)-Centre National de la Recherche Scientifique (CNRS)-Commissariat à l'énergie atomique et aux énergies alternatives (CEA)-Observatoire de Paris, PSL Research University (PSL)-PSL Research University (PSL)-Université Paris Diderot - Paris 7 (UPD7), and Laboratoire d'Annecy de Physique des Particules (LAPP/Laboratoire d'Annecy-le-Vieux de Physique des Particules)
Subjects: Nuclear and High Energy Physics, Milky Way, Astrophysics::High Energy Astrophysical Phenomena, Dwarf galaxy problem, Hochenergie-Astrophysik Theorie - Abteilung Hofmann, FOS: Physical sciences, Astrophysics, Astrophysics::Cosmology and Extragalactic Astrophysics, 01 natural sciences, Black dwarf, Galaxy group, 0103 physical sciences, Astrophysics::Solar and Stellar Astrophysics, ddc:530, 010303 astronomy & astrophysics, HESS - Abteilung Hofmann, Astrophysics::Galaxy Astrophysics, Dwarf galaxy, Physics, High Energy Astrophysical Phenomena (astro-ph.HE), 010308 nuclear & particles physics, [SDU.ASTR.HE]Sciences of the Universe [physics]/Astrophysics [astro-ph]/High Energy Astrophysical Phenomena [astro-ph.HE], Institut für Physik und Astronomie, Astronomy, Galaxy, Dwarf spheroidal galaxy, Elliptical galaxy, Astrophysics::Earth and Planetary Astrophysics, Astrophysics - High Energy Astrophysical Phenomena
Abstract: Dwarf spheroidal galaxies of the Local Group are close satellites of the Milky Way characterized by a large mass-to-light ratio and are not expected to be the site of non-thermal high-energy gamma-ray emission or intense star formation. Therefore they are amongst the most promising candidates for indirect dark matter searches. During the last years the High Energy Stereoscopic System (H.E.S.S.) of imaging atmospheric Cherenkov telescopes observed five of these dwarf galaxies for more than 140 hours in total, searching for TeV gamma-ray emission from annihilation of dark matter particles. The new results of the deep exposure of the Sagittarius dwarf spheroidal galaxy, the first observations of the Coma Berenices and Fornax dwarves and the re-analysis of two more dwarf spheroidal galaxies already published by the H.E.S.S. Collaboration, Carina and Sculptor, are presented. In the absence of a significant signal new constraints on the annihilation cross-section applicable to Weakly Interacting Massive Particles (WIMPs) are derived by combining the observations of the five dwarf galaxies. The combined exclusion limit depends on the WIMP mass and the best constraint is reached at 1-2 TeV masses with a cross-section upper bound of ~3.9x10-24 cm^3 s-1 at a 95% confidence level., Comment: to be published in Physical Review D journal; Contact authors: E. Birsin, C. Farnier, G. Lamanna
Published: 2014

84. Blazars and Optical Depth in a non-linear, time-dependent injection and cooling scenario

Author: Michael Zacharias
Subjects: High Energy Astrophysical Phenomena (astro-ph.HE), Physics, Soft photon, Photon, Field (physics), business.industry, Astrophysics::High Energy Astrophysical Phenomena, FOS: Physical sciences, Astronomy and Astrophysics, Radiation, Synchrotron, law.invention, Optics, Space and Planetary Science, law, business, Absorption (electromagnetic radiation), Blazar, Astrophysics - High Energy Astrophysical Phenomena, Optical depth
Abstract: In this paper the optical depths in blazars due to photo-pair production is calculated for a time-dependent, non-linear injection model. Several target photon fields are taken into account, namely the internal synchrotron, synchrotron-self Compton and external Compton radiation, as well as a constant external soft photon field. By applying the optical depths to theoretical blazar spectra only the constant external photon field turns out to significantly influence the radiation at high energies. The impact of the internal time-dependent radiation fields is either minor or requires extreme parameter settings. Additionally, the synchrotron-self absorption turn-over energy for low synchrotron energies is calculated, which is inherently time-dependent. It would be challenging to use it to constrain free parameters, since precise knowledge of the observation time relative to the injection time is needed. In conclusion, optical depth does not significantly influence the non-linear, time-dependent injection and cooling model., accepted by MNRAS, 14 pages, 7 figures
Published: 2014

85. Body Mass Index Adversely Affects Survival in Left Ventricular Assist Device Bridged Patients Undergoing Heart Transplantation

Author: R. Benatti, Mahazarin Ginwalla, Guilherme H. Oliveira, Salah E. Altarabsheh, J. Kerner, Michael Zacharias, Salil V. Deo, Soon J. Park, Benjamin Medalion, Chantal ElAmm, J. Benavides, Basar Sareyyupoglu, Yakov Elgudin, Gregg C. Fonarow, and Sachin Kumar
Subjects: Pulmonary and Respiratory Medicine, Heart transplantation, Transplantation, medicine.medical_specialty, business.industry, medicine.medical_treatment, Surgery, Internal medicine, Ventricular assist device, medicine, Cardiology, Cardiology and Cardiovascular Medicine, business, Body mass index
Published: 2016

86. Obesity and Wait-List Outcomes in Patients with Continuous Flow Left Ventricular Assist Devices as Bridge to Transplantation

Author: R. Benatti, Guilherme H. Oliveira, M. Farhoud, Mahazarin Ginwalla, Sadeer G. Al-Kindi, Chantal ElAmm, M. Kattea, Soon J. Park, Benjamin Medalion, Basar Sareyyupoglu, Michael Zacharias, and Salil V. Deo
Subjects: Pulmonary and Respiratory Medicine, Transplantation, medicine.medical_specialty, business.industry, Continuous flow, Medicine, Surgery, In patient, Bridge to transplantation, Cardiology and Cardiovascular Medicine, business, Intensive care medicine
Published: 2016

87. Impact of Number of Pregnancies on Allosensitization and Heart Transplant Outcomes

Author: Michael Zacharias, R. Benatti, Soon J. Park, Guilherme H. Oliveira, P. Thakker, Benjamin Medalion, Basar Sareyyupoglu, Salil V. Deo, Sadeer G. Al-Kindi, Mahazarin Ginwalla, Chantal ElAmm, M. Kattea, and M. Farhoud
Subjects: Pulmonary and Respiratory Medicine, Transplantation, medicine.medical_specialty, business.industry, Allosensitization, Medicine, Surgery, Cardiology and Cardiovascular Medicine, business, Intensive care medicine
Published: 2016

88. Results of Adult Heart Transplant While Supported on Extra-Corporeal Membrane Oxygenator Support: Evidence from a National Registry

Author: R. Benatti, Salil V. Deo, Benjamin Medalion, M.R. Robinson, Basar Sareyyupoglu, Mahazarin Ginwalla, Soon J. Park, Chantal ElAmm, Michael Zacharias, Yakov Elgudin, and Guilherme H. Oliveira
Subjects: Pulmonary and Respiratory Medicine, Transplantation, medicine.medical_specialty, Membrane oxygenator, business.industry, medicine, Surgery, National registry, Cardiology and Cardiovascular Medicine, Intensive care medicine, business
Published: 2017

89. Percutaneous treatment of severe aortic insufficiency in a patient with left ventricular assist device: friend or foe

Author: Michael, Zacharias and Ravi, Dhingra
Subjects: Adult, Heart Failure, Male, Cardiac Catheterization, Septal Occluder Device, Aortic Valve Insufficiency, Hemodynamics, Prosthesis Design, Severity of Illness Index, Ventricular Function, Left, Treatment Outcome, Foreign-Body Migration, Risk Factors, Aortic Valve, Heart Transplantation, Humans, Heart-Assist Devices, Tomography, X-Ray Computed
Published: 2014

90. TeV γ-ray observations of the young synchrotron-dominated SNRs G1.9+0.3 and G330.2+1.0 with H.E.S.S

Author: P. deWilt, K. Katarzyński, M. Dalton, Anna Szostek, Elisabetta Bissaldi, C. Farnier, Gavin Rowell, Y. A. Gallant, H.-S. Zechlin, Petter Hofverberg, R. de los Reyes, Michael Punch, Emma de Ona Wilhelmi, Konrad Bernlöhr, B. Khélifi, K. Stycz, Daniel Sánchez, Regis Terrier, G. Pühlhofer, F. Schüssler, G. Spengler, W. Domainko, A. Balzer, J. Perez, A. Reimer, J. F. Glicenstein, Stefan Wagner, Gisela Anton, M. Mayer, V. Sahakian, P.P. Krüger, S. Rosier-Lees, M. V. Fernandes, C. Trichard, C. Stegmann, Nu. Komin, André Schulz, J. Méhault, Gilles Henri, Sabrina Casanova, G. Heinzelmann, Andreas Quirrenbach, Dirk Lennarz, J. Bolmont, R. C. G. Chaves, P. J. Meintjes, Francois Brun, M. Chrétien, Peter Eger, O. Hervet, Guillaume Dubus, S. Raab, A. Abramowski, M. Paz Arribas, Christo Venter, G. Cologna, C. van Eldik, Alicja Wierzcholska, Pierre-Olivier Petrucci, Michael Zacharias, Dieter Horns, G. Lamanna, S. Kaufmann, Iurii Sushch, S. Schwarzburg, M. K. Daniel, Ullrich Schwanke, C. Jahn, G. Maurin, Aion Viana, U. F. Katz, M. Mohamed, K. Dutson, F. Spies, A. A. Zdziarski, J. Brucker, G. Fontaine, B. Opitz, R. Moderski, A. Zech, F. Feinstein, F. Stinzing, B. Giebels, J. Dyks, Tanya Edwards, Tomasz Bulik, Yvonne Becherini, Anna Barnacka, Victor Zabalza, U. Menzler, M. Kieffer, Vincent Marandon, Felix Jankowsky, M. Renaud, Chia-Chun Lu, A. G. Akhperjanian, S. Krakau, P. Vincent, Marianne Lemoine-Goumard, Francesca Volpe, S. Schwemmer, R. Steenkamp, Christoph Deil, T. Kneiske, I. D. Davids, B. van Soelen, J. Becker Tjus, T. Vuillaume, I. Jung, B. Rudak, Kathrin Egberts, Andrea Santangelo, Markus Böttcher, Catherine Boisson, Ramin Marx, A. Fiasson, Helen Poon, Andreas Hillert, M. Grudzińska, N. W. Pekeur, Pierre Brun, A. Lopatin, M. Panter, Quirin Weitzel, Y. Cui, Martin Ward, Marek Jamrozy, B. Degrange, L. O'c. Drury, P. Willmann, Frank M. Rieger, C. Romoli, L. Rob, Michal Dyrda, Julien Lefaucheur, J.-P. Lenain, Helene Sol, S. Klepser, Reinhard Schlickeiser, H. Laffon, P. Espigat, Gianluca Giavitto, Pol Bordas, Łukasz Stawarz, M. Tluczykont, D. Fernandez, Stefan Ohm, J. Harris, T. J. L. McComb, M. A. Kastendieck, Hugh Dickinson, G. Vasileiadis, Karl Kosack, Matthias Weidinger, E. O. Angüner, Heinrich J. Völk, S. Pita, German Hermann, Anna Zajczyk, M. Holler, Faical Ait Benkhali, Marie-Hélène Grondin, P. Wagner, Jim Hinton, Cameron B Rulten, D. Kolitzus, Alexandre Marcowith, C. L. Naumann, S. Balenderan, S. J. Nolan, Guy Pelletier, B. Peyaud, R. White, A. Förster, S. Colafrancesco, Denis Wouters, M. de Naurois, Andrew M. Taylor, Felix Aharonian, I. Oya, Jacek Niemiec, A. Lemière, Joachim Hahn, T. Tavernier, K. Valerius, P. M. Chadwick, Olaf Reimer, T. Garrigoux, L. Oakes, A. Cheesebrough, M. J. Vorster, R. Chalme-Calvet, W. Kluźniak, Thomas Murach, A. Jacholkowska, Jan Conrad, Thomas Lohse, Manuel Meyer, C. Couturier, M. Füßling, J.-P. Tavernet, J. Biteau, Mateusz Janiak, S. Häffner, D. Klochkov, M. Gajdus, D. Parsons, Michał Ostrowski, A. Wörnlein, N. Maxted, S. J. Fegan, A. Djannati-Ataï, Svenja Carrigan, Martin Raue, E. Birsin, Matteo Cerruti, F. Krayzel, Werner Hofmann, Emmanuel Moulin, H. E. S. S. Collaboration, H.E.S.S. Collaboration, Laboratoire Leprince-Ringuet (LLR), Centre National de la Recherche Scientifique (CNRS)-École polytechnique (X)-Institut National de Physique Nucléaire et de Physique des Particules du CNRS (IN2P3), Laboratoire Univers et Théories (LUTH (UMR_8102)), Institut national des sciences de l'Univers (INSU - CNRS)-Observatoire de Paris, Université Paris sciences et lettres (PSL)-Université Paris sciences et lettres (PSL)-Centre National de la Recherche Scientifique (CNRS)-Université Paris Diderot - Paris 7 (UPD7), Laboratoire de Physique Nucléaire et de Hautes Énergies (LPNHE), Centre National de la Recherche Scientifique (CNRS)-Université Paris Diderot - Paris 7 (UPD7)-Institut National de Physique Nucléaire et de Physique des Particules du CNRS (IN2P3)-Université Pierre et Marie Curie - Paris 6 (UPMC), Institut de Recherches sur les lois Fondamentales de l'Univers (IRFU), Commissariat à l'énergie atomique et aux énergies alternatives (CEA)-Université Paris-Saclay, FERMI, Centre d'Etudes Nucléaires de Bordeaux Gradignan (CENBG), Université Sciences et Technologies - Bordeaux 1-Institut National de Physique Nucléaire et de Physique des Particules du CNRS (IN2P3)-Centre National de la Recherche Scientifique (CNRS)-Université Sciences et Technologies - Bordeaux 1-Institut National de Physique Nucléaire et de Physique des Particules du CNRS (IN2P3)-Centre National de la Recherche Scientifique (CNRS), APC - Astrophysique des Hautes Energies (APC - AHE), AstroParticule et Cosmologie (APC (UMR_7164)), Observatoire de Paris, Université Paris sciences et lettres (PSL)-Université Paris sciences et lettres (PSL)-Commissariat à l'énergie atomique et aux énergies alternatives (CEA)-Université Paris Diderot - Paris 7 (UPD7)-Centre National de la Recherche Scientifique (CNRS)-Institut National de Physique Nucléaire et de Physique des Particules du CNRS (IN2P3)-Observatoire de Paris, Université Paris sciences et lettres (PSL)-Université Paris sciences et lettres (PSL)-Commissariat à l'énergie atomique et aux énergies alternatives (CEA)-Université Paris Diderot - Paris 7 (UPD7)-Centre National de la Recherche Scientifique (CNRS)-Institut National de Physique Nucléaire et de Physique des Particules du CNRS (IN2P3)-Dipartimento di Astronomia, Universita degli Studi di Bologna, Alma Mater Studiorum Università di Bologna [Bologna] (UNIBO)-Alma Mater Studiorum Università di Bologna [Bologna] (UNIBO), Université Paris sciences et lettres (PSL)-Université Paris sciences et lettres (PSL)-Commissariat à l'énergie atomique et aux énergies alternatives (CEA)-Université Paris Diderot - Paris 7 (UPD7)-Centre National de la Recherche Scientifique (CNRS)-Institut National de Physique Nucléaire et de Physique des Particules du CNRS (IN2P3), Laboratoire Univers et Particules de Montpellier (LUPM), Université Montpellier 2 - Sciences et Techniques (UM2)-Institut National de Physique Nucléaire et de Physique des Particules du CNRS (IN2P3)-Université de Montpellier (UM)-Centre National de la Recherche Scientifique (CNRS), Laboratoire d'Annecy de Physique des Particules (LAPP), Institut National de Physique Nucléaire et de Physique des Particules du CNRS (IN2P3)-Université Savoie Mont Blanc (USMB [Université de Savoie] [Université de Chambéry])-Centre National de la Recherche Scientifique (CNRS), HESS, Institut National de Physique Nucléaire et de Physique des Particules du CNRS (IN2P3)-École polytechnique (X)-Centre National de la Recherche Scientifique (CNRS), Université Paris sciences et lettres (PSL)-Université Paris sciences et lettres (PSL)-Université Paris Diderot - Paris 7 (UPD7)-Centre National de la Recherche Scientifique (CNRS), Université Pierre et Marie Curie - Paris 6 (UPMC)-Institut National de Physique Nucléaire et de Physique des Particules du CNRS (IN2P3)-Université Paris Diderot - Paris 7 (UPD7)-Centre National de la Recherche Scientifique (CNRS), Université Sciences et Technologies - Bordeaux 1 (UB)-Institut National de Physique Nucléaire et de Physique des Particules du CNRS (IN2P3)-Centre National de la Recherche Scientifique (CNRS)-Université Sciences et Technologies - Bordeaux 1 (UB)-Institut National de Physique Nucléaire et de Physique des Particules du CNRS (IN2P3)-Centre National de la Recherche Scientifique (CNRS), Commissariat à l'énergie atomique et aux énergies alternatives (CEA)-Institut National de Physique Nucléaire et de Physique des Particules du CNRS (IN2P3)-Observatoire de Paris, Université Paris sciences et lettres (PSL)-Université Paris sciences et lettres (PSL)-Université Paris Diderot - Paris 7 (UPD7)-Centre National de la Recherche Scientifique (CNRS)-Commissariat à l'énergie atomique et aux énergies alternatives (CEA)-Institut National de Physique Nucléaire et de Physique des Particules du CNRS (IN2P3)-Observatoire de Paris, Université Paris sciences et lettres (PSL)-Université Paris sciences et lettres (PSL)-Université Paris Diderot - Paris 7 (UPD7)-Centre National de la Recherche Scientifique (CNRS)-Alma Mater Studiorum Università di Bologna [Bologna] (UNIBO), Université Montpellier 2 - Sciences et Techniques (UM2)-Institut National de Physique Nucléaire et de Physique des Particules du CNRS (IN2P3)-Centre National de la Recherche Scientifique (CNRS), Institut National de Physique Nucléaire et de Physique des Particules du CNRS (IN2P3)-Centre National de la Recherche Scientifique (CNRS)-Commissariat à l'énergie atomique et aux énergies alternatives (CEA)-Observatoire de Paris, PSL Research University (PSL)-PSL Research University (PSL)-Université Paris Diderot - Paris 7 (UPD7)-Institut National de Physique Nucléaire et de Physique des Particules du CNRS (IN2P3)-Centre National de la Recherche Scientifique (CNRS)-Commissariat à l'énergie atomique et aux énergies alternatives (CEA)-Observatoire de Paris, PSL Research University (PSL)-PSL Research University (PSL)-Université Paris Diderot - Paris 7 (UPD7)-Dipartimento di Astronomia, Universita degli Studi di Bologna, Università di Bologna [Bologna] (UNIBO)-Università di Bologna [Bologna] (UNIBO), PSL Research University (PSL)-PSL Research University (PSL)-Université Paris Diderot - Paris 7 (UPD7), Université de Montpellier (UM)-Université Montpellier 2 - Sciences et Techniques (UM2)-Institut National de Physique Nucléaire et de Physique des Particules du CNRS (IN2P3)-Centre National de la Recherche Scientifique (CNRS), and Laboratoire d'Annecy de Physique des Particules (LAPP/Laboratoire d'Annecy-le-Vieux de Physique des Particules)
Subjects: [PHYS.ASTR.HE]Physics [physics]/Astrophysics [astro-ph]/High Energy Astrophysical Phenomena [astro-ph.HE], Radiation mechanisms: non-thermal, individual objects: SNR G1.9+0.3 [ISM], Hochenergie-Astrophysik Theorie - Abteilung Hofmann, FOS: Physical sciences, Gamma-rays: ISM, Context (language use), Astrophysics, individual objects: SNR G330.2+1.0 [ISM], ISM. [Gamma-rays], High Energy Stereoscopic System, ISM [gamma-rays], HESS - Abteilung Hofmann, ISM: supernova remnants, High Energy Astrophysical Phenomena (astro-ph.HE), Astroparticle physics, Physics, Spectral index, non-thermal [Radiation mechanisms], ISM: magnetic fields, Astronomy and Astrophysics, Space and Planetary Science, [SDU.ASTR.HE]Sciences of the Universe [physics]/Astrophysics [astro-ph]/High Energy Astrophysical Phenomena [astro-ph.HE], supernova remnants [ISM], magnetic fields [ISM], Astronomy, Institut für Physik und Astronomie, Cherenkov Telescope Array, Galaxy, Particle acceleration, Supernova, 13. Climate action, ddc:520, Astrophysics - High Energy Astrophysical Phenomena
Abstract: The non-thermal nature of the X-ray emission from the shell-type supernova remnants (SNRs) G1.9+0.3 and G330.2+1.0 is an indication of intense particle acceleration in the shock fronts of both objects. This suggests that the SNRs are prime candidates for very-high-energy (VHE; E $>$ 0.1 TeV) {\gamma}-ray observations. G1.9+0.3, recently established as the youngest known SNR in the Galaxy, also offers a unique opportunity to study the earliest stages of SNR evolution in the VHE domain. The purpose of this work is to probe the level of VHE {\gamma}-ray emission from both SNRs and use this to constrain their physical properties. Observations were conducted with the H.E.S.S. (High Energy Stereoscopic System) Cherenkov telescope array over a more than six-year period spanning 2004-2010. The obtained data have effective livetimes of 67 h for G1.9+0.3 and 16 h for G330.2+1.0. The data are analyzed in the context of the multi-wavelength observations currently available and in the framework of both leptonic and hadronic particle acceleration scenarios. No significant {\gamma}-ray signal from G1.9+0.3 or G330.2+1.0 was detected. Upper limits (99% confidence level) to the TeV flux from G1.9+0.3 and G330.2+1.0 for the assumed spectral index {\Gamma} = 2.5 were set at 5.6 $\times$ 10$^{-13}$ cm$^{-2}$ s$^{-1}$ above 0.26 TeV and 3.2 $\times$ 10$^{-12}$ cm$^{-2}$ s$^{-1}$ above 0.38 TeV, respectively. In a one-zone leptonic scenario, these upper limits imply lower limits on the interior magnetic field to B$_{\mathrm{G1.9}}$ $\gtrsim$ 11 {\mu}G for G1.9+0.3 and to B$_{\mathrm{G330}}$ $\gtrsim$ 8 {\mu}G for G330.2+1.0. In a hadronic scenario, the low ambient densities and the large distances to the SNRs result in very low predicted fluxes, for which the H.E.S.S. upper limits are not constraining., Comment: 9 pages, 2 figures, 4 tables. Accepted for publication in MNRAS
Published: 2014

91. Erratum: 'Search for Dark Matter Annihilation Signals from the Fornax Galaxy Cluster with H.E.S.S.' (2012, ApJ, 750, 123)

Author: A. Schulz, L. O'c. Drury, J. Becker Tjus, K. Katarzyński, Nu. Komin, S. Bernhard, S. J. Fegan, P.-O. Petrucci, Svenja Carrigan, E. Birsin, Y. Cui, Yvonne Becherini, E. O. Angüner, Guillaume Dubus, S. Klepser, Axel Donath, P. Vincent, Anne Lemiere, M. J. Vorster, J. Lau, M. Füßling, P. Espigat, Vincent Marandon, Christo Venter, D. Berge, I. Jung-Richardt, C. Jahn, M. Gajdus, Satoshi Yoshiike, Y. A. Gallant, H.-S. Zechlin, Catherine Boisson, Michael Punch, A. Jacholkowska, U. F. Katz, T. Tavernier, R. Moderski, A. Zech, D. Gottschall, S. J. Nolan, K. Morå, T. Murach, B. Peyaud, C. Romoli, Emmanuel Moulin, U. Menzler, Joachim Hahn, M. Janiak, P. P. Krueger, I. Oya, Jacek Niemiec, Pierre Brun, M. Mohamed, R. Chalme-Calvet, S. Raab, A. Abramowski, Robert Wagner, Olaf Reimer, C. Trichard, Quirin Weitzel, Thomas Lohse, M. Paz Arribas, S. Pita, Johannes Veh, M. Tluczykont, R. C. G. Chaves, A. M. W. Mitchell, P. J. Meintjes, T. Garrigoux, M. Panter, Ullrich Schwanke, Christian Farnier, M. Dalton, G. Pühlhofer, A. Balzer, M. de Naurois, Stefan Wagner, M. Lemoine-Goumard, M. Mayer, Jan Conrad, M. Bryan, A. Djannati-Ataï, A. G. Akhperjanian, D. Fernandez, Dieter Horns, D. Klochkov, A. Reimer, Tomasz Bulik, M. A. Kastendieck, T. Fukuda, R. Steenkamp, I. Reichardt, Jim Hinton, S. Gabici, Ruizhi Yang, F. Schüssler, Aion Viana, Stefan Ohm, A. A. Zdziarski, G. Vasileiadis, G. Heinzelmann, A.M. Taylor, K. Dutson, Marek Jamrozy, S. Krakau, G. Fontaine, David Sanchez, M. Böttcher, Helene Sol, J. Bolmont, Iurii Sushch, P. deWilt, S. Schwarzburg, B. Opitz, Ramin Marx, Karl Kosack, G. Giavitto, C. Couturier, Alicja Wierzcholska, G. Spengler, S. Kaufmann, B. Khélifi, P. Willmann, Michal Dyrda, Christoph Deil, F. Spies, G. Lamanna, Y. Fukui, G. Hermann, Regis Terrier, L. Oakes, J. Dyks, N. Maxted, Hidetoshi Sano, Michał Ostrowski, M. V. Fernandes, J. Lefaucheur, J.-P. Lenain, J. Vink, I. D. Davids, W. Domainko, D. Salek, Reinhard Schlickeiser, J.-P. Tavernet, Pol Bordas, J. Harris, R. D. Parsons, Nachiketa Chakraborty, Peter Eger, Petter Hofverberg, A. Wörnlein, A. Ivascenko, S. Colafrancesco, S. Schwemmer, Anna Barnacka, Andrea Santangelo, Alexandre Marcowith, F. Krayzel, Helen Poon, M. Grudzińska, A. Lopatin, Werner Hofmann, F. Feinstein, H. Odaka, J. Mehault, Tanya Edwards, M. Backes, A. Fiasson, P. M. Chadwick, Gilles Henri, F. Jankowsky, Gavin Rowell, D. Zaborov, R. de los Reyes, Guy Pelletier, A. Förster, Victor Zabalza, F. Stinzing, B. Giebels, Andreas Hillert, V. Sahakian, Andreas Quirrenbach, T. Vuillaume, Michael Zacharias, K. Stycz, J. F. Glicenstein, Łukasz Stawarz, Heinrich J. Völk, M. Kieffer, D. Hadasch, F. Ait Benkhali, P. Wagner, Martin Ward, Francesca Volpe, Cameron B Rulten, S. Balenderan, J. Biteau, Markus Holler, Felix Aharonian, H. Laffon, M. Chrétien, S. Häffner, K. Valerius, Marie-Hélène Grondin, Denis Wouters, O. Hervet, W. Kluźniak, Matthias Weidinger, V. Lefranc, S. Rosier-Lees, Sabrina Casanova, C. Stegmann, B. van Soelen, B. Rudak, Kathrin Egberts, B. Degrange, Frank M. Rieger, F. Spanier, K. Bernloehr, Gilles Maurin, N. W. Pekeur, Michael Meyer, Francois Brun, G. Cologna, C. van Eldik, J. Bregeon, M. Renaud, T. J. L. McComb, D. Kolitzus, Chia-Chun Lu, R. White, and H.E.S.S. Collaboration
Subjects: Physics, Annihilation, Space and Planetary Science, Dark matter, Hochenergie-Astrophysik Theorie - Abteilung Hofmann, Astronomy, Astronomy and Astrophysics, Astrophysics, HESS - Abteilung Hofmann, Galaxy cluster
Published: 2014

92. Diffuse Galactic gamma-ray emission with H.E.S.S

Author: Jim Hinton, J. Veh, Svenja Carrigan, E. Birsin, P. P. Krueger, M. Holler, P. Espigat, Hidetoshi Sano, Felix Spanier, M. Gajdus, Jacek Niemiec, Nachiketa Chakraborty, Axel Donath, Olaf Reimer, Michał Ostrowski, Yasuo Fukui, G. Lamanna, Manuel Meyer, Tanya Edwards, Y. A. Gallant, H.-S. Zechlin, K. Kosack, S. J. Nolan, G. Fontaine, K. Dutson, R. C. G. Chaves, F. Spies, Włodek Kluźniak, K. Morå, Jan Conrad, Uli Katz, Joachim Hahn, G. Pühlhofer, Michael Backes, Thomas Murach, T. Fukuda, A. Reimer, Michael Punch, M. Kieffer, Ramin Marx, A. Fiasson, D. Gottschall, Anne Lemiere, M. J. Vorster, Pascal Vincent, Christo Venter, S. Schwarzburg, Aion Viana, B. Opitz, P. Willmann, C. Jahn, O. Hervet, Stefan Ohm, S. Pita, D. Klochkov, F. Ait Benkhali, S. Schwemmer, R. D. Parsons, Michal Dyrda, W. Domainko, A. Balzer, J. Becker Tjus, S. Bernhard, B. van Soelen, S. Rosier-Lees, P. J. Meintjes, C. Trichard, Christoph Deil, Ignasi Reichardt, Francois Brun, M. Chrétien, Andrea Santangelo, G. Spengler, M. Grudzińska, A. Zech, A. Wörnlein, Gilles Maurin, Stefano Gabici, M. Panter, S. J. Fegan, A. Djannati-Ataï, M. Mohamed, Robert Wagner, Gianluca Giavitto, N. W. Pekeur, J. Dyks, I. D. Davids, Kathrin Egberts, B. Degrange, B. Rudak, A. Marcowith, Frank M. Rieger, Thomas Lohse, Ł. Stawarz, Y. Cui, C. Romoli, J. Lau, N. Maxted, S. Häffner, A. Wierzcholska, A. Barnacka, M. V. Fernandes, Jonathan Biteau, P. Wagner, Ruizhi Yang, J. Bregeon, K. Bernloehr, L. Oakes, J.-P. Lenain, Andrew M. Taylor, Vincent Marandon, S. Krakau, Satoshi Yoshiike, V. Sahakian, J. Bolmont, I. Sushch, P. deWilt, Thomas Vuillaume, Peter Eger, Christian Stegmann, Stefan Wagner, David Salek, E. Moulin, M. Mayer, Tomasz Bulik, Guillaume Dubus, C. van Eldik, A. Jacholkowska, M. Lemoine-Goumard, P. M. Chadwick, L. O'c. Drury, K. Katarzyński, D. Hadasch, J. Mehault, Francesca Volpe, Catherine Boisson, S. Klepser, F. Krayzel, André Schulz, S. Colafrancesco, D. Kolitzus, C. B. Rulten, R. Chalme-Calvet, S. Raab, A. Abramowski, G. Cologna, Quirin Weitzel, C. Farnier, Martin Ward, Julien Lefaucheur, Felix Jankowsky, Werner Hofmann, M. Renaud, Pierre Brun, Jacco Vink, B. Khélifi, G. Hermann, Regis Terrier, Marie-Hélène Grondin, Andrzej A. Zdziarski, Dieter Horns, Sabrina Casanova, Chia-Chun Lu, V. Lefranc, Igor Oya, Denis Wouters, Markus Böttcher, D. Fernandez, Guy Pelletier, A. Förster, M. A. Kastendieck, Marek Jamrozy, C. Couturier, G. Vasileiadis, T. J. L. McComb, David Sanchez, Alison Mitchell, B. Peyaud, Matthias Weidinger, R. White, M. Tluczykont, Helene Sol, I. Jung-Richardt, J.-P. Tavernet, S. Balenderan, J. Harris, Felix Aharonian, H. Laffon, K. Valerius, M. Paz Arribas, Ullrich Schwanke, M. Dalton, Victor Zabalza, A. G. Akhperjanian, R. Steenkamp, P.-O. Petrucci, Yvonne Becherini, Rafał Moderski, Thomas Tavernier, M. de Naurois, Petter Hofverberg, Andreas Quirrenbach, Michael Zacharias, F. Feinstein, Nu. Komin, H. Odaka, David Berge, Gavin Rowell, M. Bryan, D. Zaborov, R. de los Reyes, M. Füßling, T. Garrigoux, Sarah Kaufmann, U. Menzler, Andreas Hillert, Gilles Henri, F. Schüssler, F. Stinzing, B. Giebels, A. Ivascenko, Helen Poon, A. Lopatin, Heinrich J. Völk, G. Heinzelmann, M. Janiak, K. Stycz, J. F. Glicenstein, Reinhard Schlickeiser, Pol Bordas, E. O. Angüner, Laboratoire Leprince-Ringuet (LLR), Centre National de la Recherche Scientifique (CNRS)-École polytechnique (X)-Institut National de Physique Nucléaire et de Physique des Particules du CNRS (IN2P3), Laboratoire Univers et Théories (LUTH (UMR_8102)), Institut national des sciences de l'Univers (INSU - CNRS)-Observatoire de Paris, Université Paris sciences et lettres (PSL)-Université Paris sciences et lettres (PSL)-Centre National de la Recherche Scientifique (CNRS)-Université Paris Diderot - Paris 7 (UPD7), Laboratoire de Physique Nucléaire et de Hautes Énergies (LPNHE), Centre National de la Recherche Scientifique (CNRS)-Université Paris Diderot - Paris 7 (UPD7)-Institut National de Physique Nucléaire et de Physique des Particules du CNRS (IN2P3)-Université Pierre et Marie Curie - Paris 6 (UPMC), Laboratoire Univers et Particules de Montpellier (LUPM), Centre National de la Recherche Scientifique (CNRS)-Université de Montpellier (UM)-Institut National de Physique Nucléaire et de Physique des Particules du CNRS (IN2P3)-Université Montpellier 2 - Sciences et Techniques (UM2), Institut de Recherches sur les lois Fondamentales de l'Univers (IRFU), Commissariat à l'énergie atomique et aux énergies alternatives (CEA)-Université Paris-Saclay, AstroParticule et Cosmologie (APC (UMR_7164)), Observatoire de Paris, Université Paris sciences et lettres (PSL)-Université Paris sciences et lettres (PSL)-Commissariat à l'énergie atomique et aux énergies alternatives (CEA)-Université Paris Diderot - Paris 7 (UPD7)-Centre National de la Recherche Scientifique (CNRS)-Institut National de Physique Nucléaire et de Physique des Particules du CNRS (IN2P3), Laboratoire d'Annecy de Physique des Particules (LAPP), Institut National de Physique Nucléaire et de Physique des Particules du CNRS (IN2P3)-Université Savoie Mont Blanc (USMB [Université de Savoie] [Université de Chambéry])-Centre National de la Recherche Scientifique (CNRS), Centre d'Etudes Nucléaires de Bordeaux Gradignan (CENBG), Université Sciences et Technologies - Bordeaux 1-Institut National de Physique Nucléaire et de Physique des Particules du CNRS (IN2P3)-Centre National de la Recherche Scientifique (CNRS), HESS, Institut National de Physique Nucléaire et de Physique des Particules du CNRS (IN2P3)-École polytechnique (X)-Centre National de la Recherche Scientifique (CNRS), Université Paris sciences et lettres (PSL)-Université Paris sciences et lettres (PSL)-Université Paris Diderot - Paris 7 (UPD7)-Centre National de la Recherche Scientifique (CNRS), Université Pierre et Marie Curie - Paris 6 (UPMC)-Institut National de Physique Nucléaire et de Physique des Particules du CNRS (IN2P3)-Université Paris Diderot - Paris 7 (UPD7)-Centre National de la Recherche Scientifique (CNRS), Université Montpellier 2 - Sciences et Techniques (UM2)-Institut National de Physique Nucléaire et de Physique des Particules du CNRS (IN2P3)-Centre National de la Recherche Scientifique (CNRS), Commissariat à l'énergie atomique et aux énergies alternatives (CEA)-Institut National de Physique Nucléaire et de Physique des Particules du CNRS (IN2P3)-Observatoire de Paris, Université Sciences et Technologies - Bordeaux 1 (UB)-Institut National de Physique Nucléaire et de Physique des Particules du CNRS (IN2P3)-Centre National de la Recherche Scientifique (CNRS), H.E.S.S. Collaboration, Université de Montpellier (UM)-Université Montpellier 2 - Sciences et Techniques (UM2)-Institut National de Physique Nucléaire et de Physique des Particules du CNRS (IN2P3)-Centre National de la Recherche Scientifique (CNRS), Laboratoire d'Annecy de Physique des Particules (LAPP/Laboratoire d'Annecy-le-Vieux de Physique des Particules), Institut National de Physique Nucléaire et de Physique des Particules du CNRS (IN2P3)-Centre National de la Recherche Scientifique (CNRS)-Commissariat à l'énergie atomique et aux énergies alternatives (CEA)-Observatoire de Paris, PSL Research University (PSL)-PSL Research University (PSL)-Université Paris Diderot - Paris 7 (UPD7), and Laboratoire de Physique Théorique et Astroparticules (LPTA)
Subjects: Nuclear and High Energy Physics, [PHYS.ASTR.HE]Physics [physics]/Astrophysics [astro-ph]/High Energy Astrophysical Phenomena [astro-ph.HE], Astrophysics::High Energy Astrophysical Phenomena, Hochenergie-Astrophysik Theorie - Abteilung Hofmann, FOS: Physical sciences, Cosmic ray, Astrophysics, Astrophysics::Cosmology and Extragalactic Astrophysics, 01 natural sciences, [PHYS.ASTR.CO]Physics [physics]/Astrophysics [astro-ph]/Cosmology and Extra-Galactic Astrophysics [astro-ph.CO], Pion, 0103 physical sciences, 010303 astronomy & astrophysics, HESS - Abteilung Hofmann, Cherenkov radiation, Astrophysics::Galaxy Astrophysics, High Energy Astrophysical Phenomena (astro-ph.HE), Astroparticle physics, Physics, 010308 nuclear & particles physics, Gamma ray, Astronomy, Institut für Physik und Astronomie, Galactic plane, Galaxy, Infrared cirrus, Astrophysics - High Energy Astrophysical Phenomena
Abstract: Diffuse $\gamma$-ray emission is the most prominent observable signature of celestial cosmic-ray interactions at high energies. While already being investigated at GeV energies over several decades, assessments of diffuse $\gamma$-ray emission at TeV energies remain sparse. After completion of the systematic survey of the inner Galaxy, the H.E.S.S. experiment is in a prime position to observe large-scale diffuse emission at TeV energies. Data of the H.E.S.S. Galactic Plane Survey are investigated in regions off known $\gamma$-ray sources. Corresponding $\gamma$-ray flux measurements were made over an extensive grid of celestial locations. Longitudinal and latitudinal profiles of the observed $\gamma$-ray fluxes show characteristic excess emission not attributable to known $\gamma$-ray sources. For the first time large-scale $\gamma$-ray emission along the Galactic Plane using imaging atmospheric Cherenkov telescopes has been observed. While the background subtraction technique limits the ability to recover modest variation on the scale of the H.E.S.S. field of view or larger, which is characteristic of the inverse Compton scatter-induced Galactic diffuse emission, contributions of neutral pion decay as well as emission from unresolved $\gamma$-ray sources can be recovered in the observed signal to a large fraction. Calculations show that the minimum $\gamma$-ray emission from $\pi^0$-decay represents a significant contribution to the total signal. This detection is interpreted as a mix of diffuse Galactic $\gamma$-ray emission and unresolved sources., Comment: 8 pages, 2 figures, accepted for publication in Physical Review D
Published: 2014

93. HESS J1640-465 - an exceptionally luminous TeV ${\gamma}$-ray supernova remnant

Author: G. Cologna, C. van Eldik, R. C. G. Chaves, S. Rosier-Lees, S. Raab, A. Abramowski, P. M. Chadwick, Felix Jankowsky, M. J. Vorster, Jacco Vink, Pierre-Olivier Petrucci, M. Renaud, Sabrina Casanova, Quirin Weitzel, A. Jacholkowska, D. Klochkov, L. O'c. Drury, S. Klepser, M. H. Grondin, Chia-Chun Lu, R. Chalme-Calvet, Christo Venter, G. Maurin, Michał Ostrowski, Tanya Edwards, C. Jahn, L. Rob, U. F. Katz, R. Moderski, A. Zech, Aion Viana, Francesca Volpe, A. A. Zdziarski, M. Dalton, D. Fernandez, G. Lamanna, B. Opitz, S. J. Nolan, Joachim Hahn, A. Wörnlein, Thomas Lohse, Markus Böttcher, C. Farnier, M. A. Kastendieck, A. Cheesebrough, Jan Conrad, Stefan Ohm, A. Fiasson, G. Vasileiadis, A. Djannati-Ataï, S. Pita, N. Maxted, Helen Poon, A. Lopatin, B. van Soelen, I. Jung, B. Rudak, Kathrin Egberts, D. Kolitzus, S. Schwarzburg, Martin Raue, F. Feinstein, B. Degrange, Michael Punch, J. Biteau, Guy Pelletier, A. Förster, T. Tavernier, B. Khélifi, G. Hermann, Regis Terrier, F. Schüssler, Mateusz Janiak, Anna Zajczyk, P. Wagner, Andrew M. Taylor, Stefan Wagner, Gisela Anton, M. Mayer, Frank M. Rieger, P.P. Krüger, T. Garrigoux, J. Dyks, R. D. Parsons, J.-P. Lenain, S. Häffner, Reinhard Schlickeiser, Pol Bordas, L. Oakes, I. D. Davids, Daniel Sánchez, Tomasz Bulik, Guillaume Dubus, Gianluca Giavitto, T. J. L. McComb, Hugh Dickinson, E. O. Angüner, Denis Wouters, Y. Cui, André Schulz, J. Méhault, G. Spengler, J. Brucker, H. Laffon, Dieter Horns, B. Peyaud, R. White, W. Kluźniak, W. Domainko, A. Balzer, Vincent Marandon, C. Couturier, S. Colafrancesco, J. Becker Tjus, T. Vuillaume, K. Dutson, F. Spies, G. Heinzelmann, J. Bolmont, P. J. Meintjes, Francois Brun, M. Chrétien, Jim Hinton, M. Grudzińska, N. W. Pekeur, Christoph Deil, Alexandre Marcowith, C. L. Naumann, T. Kneiske, P. deWilt, K. Katarzyński, Victor Zabalza, U. Menzler, Andreas Hillert, V. Sahakian, Andreas Quirrenbach, Michael Zacharias, Gavin Rowell, R. de los Reyes, Elisabetta Bissaldi, K. Stycz, J. F. Glicenstein, M. Holler, Łukasz Stawarz, Heinrich J. Völk, Gilles Henri, F. Stinzing, B. Giebels, S. J. Fegan, Svenja Carrigan, E. Birsin, Emmanuel Moulin, P. Espigat, Matteo Cerruti, F. Krayzel, Werner Hofmann, G. Fontaine, M. V. Fernandes, M. Gajdus, I. Oya, Jacek Niemiec, A. Lemière, Olaf Reimer, Ramin Marx, C. Trichard, Thomas Murach, P. Willmann, Michal Dyrda, M. de Naurois, Peter Eger, C. Stegmann, Nu. Komin, M. Panter, S. Krakau, P. Vincent, Martin Ward, Cameron B Rulten, S. Balenderan, E. de Oña Wilhelmi, C. Romoli, Konrad Bernlöhr, Felix Aharonian, K. Valerius, Julien Lefaucheur, Anna Barnacka, Matthias Weidinger, G. Pühlhofer, Dirk Lennarz, J. Perez, M. K. Daniel, A. Reimer, M. Kieffer, F. Ait Benkhali, S. Schwemmer, Andrea Santangelo, Yvonne Becherini, Anna Szostek, Petter Hofverberg, Iurii Sushch, M. Mohamed, Marianne Lemoine-Goumard, M. Füßling, J.-P. Tavernet, Manuel Meyer, Pierre Brun, M. Tluczykont, Y. A. Gallant, H.-S. Zechlin, O. Hervet, Catherine Boisson, Alicja Wierzcholska, S. Kaufmann, M. Paz Arribas, Ullrich Schwanke, A. G. Akhperjanian, R. Steenkamp, Marek Jamrozy, Helene Sol, J. Harris, Karl Kosack, H. E. S. S. Collaboration, Institut für Experimentalphysik [Hamburg], Universität Hamburg (UHH), Max Planck Institute for Nuclear Physics (MPIK), Max-Planck-Gesellschaft, National Academy of Sciences of the Republic of Armenia [Yerevan] (NAS RA), Yerevan Physics Institute, Yerevan State University, Humboldt-Universität zu Berlin, Physikalisches Institut [Erlangen], Friedrich-Alexander Universität Erlangen-Nürnberg (FAU), Department of Physics [Durham], University of New Hampshire (UNH), Deutsches Elektronen-Synchrotron [Zeuthen] (DESY), Helmholtz-Gemeinschaft = Helmholtz Association, Astronomical Observatory [Warsaw], Faculty of Physics [Warsaw] (FUW), University of Warsaw (UW)-University of Warsaw (UW), School of Computer Science, Physics and Mathematics [Linnaeus University], Linnaeus University, Institut für Theoretische Physik IV [Bochum] (ITP4), Ruhr-Universität Bochum [Bochum], Institut f¨ur Astro- und Teilchenphysik and Institut f¨ur Theoretische Physik, Leopold-Franzens Universitat Innsbruck, Laboratoire Leprince-Ringuet (LLR), Centre National de la Recherche Scientifique (CNRS)-École polytechnique (X)-Institut National de Physique Nucléaire et de Physique des Particules du CNRS (IN2P3), North-West University [South Aftrica] (NWU), Laboratoire Univers et Théories (LUTH (UMR_8102)), Institut national des sciences de l'Univers (INSU - CNRS)-Observatoire de Paris, Université Paris sciences et lettres (PSL)-Université Paris sciences et lettres (PSL)-Centre National de la Recherche Scientifique (CNRS)-Université Paris Diderot - Paris 7 (UPD7), Laboratoire de Physique Nucléaire et de Hautes Énergies (LPNHE), Centre National de la Recherche Scientifique (CNRS)-Université Paris Diderot - Paris 7 (UPD7)-Institut National de Physique Nucléaire et de Physique des Particules du CNRS (IN2P3)-Université Pierre et Marie Curie - Paris 6 (UPMC), Institut für Astronomie und Astrophysik [Tübingen] (IAAT), Eberhard Karls Universität Tübingen = Eberhard Karls University of Tuebingen, Institut de Recherches sur les lois Fondamentales de l'Univers (IRFU), Commissariat à l'énergie atomique et aux énergies alternatives (CEA)-Université Paris-Saclay, Astroparticules (ASTRO), Centre d'Etudes Nucléaires de Bordeaux Gradignan (CENBG), Université Sciences et Technologies - Bordeaux 1-Institut National de Physique Nucléaire et de Physique des Particules du CNRS (IN2P3)-Centre National de la Recherche Scientifique (CNRS)-Université Sciences et Technologies - Bordeaux 1-Institut National de Physique Nucléaire et de Physique des Particules du CNRS (IN2P3)-Centre National de la Recherche Scientifique (CNRS), APC - Astrophysique des Hautes Energies (APC - AHE), AstroParticule et Cosmologie (APC (UMR_7164)), Observatoire de Paris, Université Paris sciences et lettres (PSL)-Université Paris sciences et lettres (PSL)-Commissariat à l'énergie atomique et aux énergies alternatives (CEA)-Université Paris Diderot - Paris 7 (UPD7)-Centre National de la Recherche Scientifique (CNRS)-Institut National de Physique Nucléaire et de Physique des Particules du CNRS (IN2P3)-Observatoire de Paris, Université Paris sciences et lettres (PSL)-Université Paris sciences et lettres (PSL)-Commissariat à l'énergie atomique et aux énergies alternatives (CEA)-Université Paris Diderot - Paris 7 (UPD7)-Centre National de la Recherche Scientifique (CNRS)-Institut National de Physique Nucléaire et de Physique des Particules du CNRS (IN2P3)-Dipartimento di Astronomia, Universita degli Studi di Bologna, Alma Mater Studiorum Università di Bologna [Bologna] (UNIBO)-Alma Mater Studiorum Università di Bologna [Bologna] (UNIBO), Dublin Institute for Advanced Studies (DIAS), Université Paris sciences et lettres (PSL)-Université Paris sciences et lettres (PSL)-Commissariat à l'énergie atomique et aux énergies alternatives (CEA)-Université Paris Diderot - Paris 7 (UPD7)-Centre National de la Recherche Scientifique (CNRS)-Institut National de Physique Nucléaire et de Physique des Particules du CNRS (IN2P3), Laboratoire Univers et Particules de Montpellier (LUPM), Université Montpellier 2 - Sciences et Techniques (UM2)-Institut National de Physique Nucléaire et de Physique des Particules du CNRS (IN2P3)-Université de Montpellier (UM)-Centre National de la Recherche Scientifique (CNRS), Laboratoire d'Annecy de Physique des Particules (LAPP), Institut National de Physique Nucléaire et de Physique des Particules du CNRS (IN2P3)-Université Savoie Mont Blanc (USMB [Université de Savoie] [Université de Chambéry])-Centre National de la Recherche Scientifique (CNRS), Universität Potsdam, Department of Physics [Durham University], Durham University, HESS, Institut National de Physique Nucléaire et de Physique des Particules du CNRS (IN2P3)-École polytechnique (X)-Centre National de la Recherche Scientifique (CNRS), Université Pierre et Marie Curie - Paris 6 (UPMC)-Institut National de Physique Nucléaire et de Physique des Particules du CNRS (IN2P3)-Université Paris Diderot - Paris 7 (UPD7)-Centre National de la Recherche Scientifique (CNRS), Institut National de Physique Nucléaire et de Physique des Particules du CNRS (IN2P3)-Centre National de la Recherche Scientifique (CNRS)-Commissariat à l'énergie atomique et aux énergies alternatives (CEA)-Observatoire de Paris, PSL Research University (PSL)-PSL Research University (PSL)-Université Paris Diderot - Paris 7 (UPD7)-Institut National de Physique Nucléaire et de Physique des Particules du CNRS (IN2P3)-Centre National de la Recherche Scientifique (CNRS)-Commissariat à l'énergie atomique et aux énergies alternatives (CEA)-Observatoire de Paris, PSL Research University (PSL)-PSL Research University (PSL)-Université Paris Diderot - Paris 7 (UPD7)-Dipartimento di Astronomia, Universita degli Studi di Bologna, Università di Bologna [Bologna] (UNIBO)-Università di Bologna [Bologna] (UNIBO), PSL Research University (PSL)-PSL Research University (PSL)-Université Paris Diderot - Paris 7 (UPD7), Université de Montpellier (UM)-Université Montpellier 2 - Sciences et Techniques (UM2)-Institut National de Physique Nucléaire et de Physique des Particules du CNRS (IN2P3)-Centre National de la Recherche Scientifique (CNRS), Laboratoire d'Annecy de Physique des Particules (LAPP/Laboratoire d'Annecy-le-Vieux de Physique des Particules), High Energy Astrophys. & Astropart. Phys (API, FNWI), Humboldt University Of Berlin, Universität Innsbruck [Innsbruck], Université Paris sciences et lettres (PSL)-Université Paris sciences et lettres (PSL)-Université Paris Diderot - Paris 7 (UPD7)-Centre National de la Recherche Scientifique (CNRS), Université Sciences et Technologies - Bordeaux 1 (UB)-Institut National de Physique Nucléaire et de Physique des Particules du CNRS (IN2P3)-Centre National de la Recherche Scientifique (CNRS)-Université Sciences et Technologies - Bordeaux 1 (UB)-Institut National de Physique Nucléaire et de Physique des Particules du CNRS (IN2P3)-Centre National de la Recherche Scientifique (CNRS), Commissariat à l'énergie atomique et aux énergies alternatives (CEA)-Institut National de Physique Nucléaire et de Physique des Particules du CNRS (IN2P3)-Observatoire de Paris, Université Paris sciences et lettres (PSL)-Université Paris sciences et lettres (PSL)-Université Paris Diderot - Paris 7 (UPD7)-Centre National de la Recherche Scientifique (CNRS)-Commissariat à l'énergie atomique et aux énergies alternatives (CEA)-Institut National de Physique Nucléaire et de Physique des Particules du CNRS (IN2P3)-Observatoire de Paris, Université Paris sciences et lettres (PSL)-Université Paris sciences et lettres (PSL)-Université Paris Diderot - Paris 7 (UPD7)-Centre National de la Recherche Scientifique (CNRS)-Alma Mater Studiorum Università di Bologna [Bologna] (UNIBO), Université Montpellier 2 - Sciences et Techniques (UM2)-Institut National de Physique Nucléaire et de Physique des Particules du CNRS (IN2P3)-Centre National de la Recherche Scientifique (CNRS), and University of Potsdam = Universität Potsdam
Subjects: [PHYS.ASTR.HE]Physics [physics]/Astrophysics [astro-ph]/High Energy Astrophysical Phenomena [astro-ph.HE], Photon, Radiation mechanisms: non-thermal, Supernova remnants, Astrophysics::High Energy Astrophysical Phenomena, Hadron, Hochenergie-Astrophysik Theorie - Abteilung Hofmann, FOS: Physical sciences, Astrophysics, Astrophysics::Cosmology and Extragalactic Astrophysics, 7. Clean energy, 01 natural sciences, Power law, Spectral line, ISM: individual objects: G338.3−0.0, G338.3-0.0-ISM, Individual objects, Non-thermal-ISM, Radiation mechanisms, Astronomy and Astrophysics, Space and Planetary Science, 0103 physical sciences, High Energy Stereoscopic System, Supernova remnant, 010303 astronomy & astrophysics, HESS - Abteilung Hofmann, ISM: supernova remnant, High Energy Astrophysical Phenomena, Astroparticle physics, Physics, High Energy Astrophysical Phenomena (astro-ph.HE), non-thermal [Radiation mechanisms], 010308 nuclear & particles physics, supernova remnants [ISM], [SDU.ASTR.HE]Sciences of the Universe [physics]/Astrophysics [astro-ph]/High Energy Astrophysical Phenomena [astro-ph.HE], Institut für Physik und Astronomie, Astronomy, individual objects: G338.3−0.0 [ISM], Supernova, supernova remnants. [ISM], ddc:520, High Energy Physics::Experiment, Astrophysics - High Energy Astrophysical Phenomena
Abstract: The results of follow-up observations of the TeV gamma-ray source HESSJ 1640-465 from 2004 to 2011 with the High Energy Stereoscopic System (H.E.S.S.) are reported in this work. The spectrum is well described by an exponential cut-off power law with photon index Gamma=2.11 +/- 0.09_stat +/- 0.10_sys, and a cut-off energy of E_c = (6.0 +2.0 -1.2) TeV. The TeV emission is significantly extended and overlaps with the north-western part of the shell of the SNR G338.3-0.0. The new H.E.S.S. results, a re-analysis of archival XMM-Newton data, and multi-wavelength observations suggest that a significant part of the gamma-ray emission from HESS J1640-465 originates in the SNR shell. In a hadronic scenario, as suggested by the smooth connection of the GeV and TeV spectra, the product of total proton energy and mean target density could be as high as W_p n_H ~ 4 x 10^52 (d/10kpc)^2 erg cm^-3., accepted for publication in MNRAS, 9 pages, 5 figures, added Spitzer citation and acknowledgement
Published: 2014

94. Percutaneous Treatment of Severe Aortic Insufficiency in a Patient With Left Ventricular Assist Device

Author: Michael Zacharias and Ravi Dhingra
Subjects: medicine.medical_specialty, Percutaneous, Heartmate ii, business.industry, medicine.medical_treatment, equipment and supplies, Surgery, Congenitally corrected transposition, Great arteries, Internal medicine, Ventricular assist device, medicine, Cardiology, Right ventricular failure, Septal Occluder, New York Heart Association Class IV, Cardiology and Cardiovascular Medicine, business
Abstract: A 29-year-old man with congenitally corrected transposition of the great arteries underwent implantation of a HeartMate II left ventricular assist device (LVAD) (Thoratec Corp, Pleasanton, California) as a result of worsening systemic right ventricular failure and New York Heart Association class IV
Published: 2015

95. A Case of LV 'Pseudo' Pseudodyskinesis

Author: Michael Zacharias, Dennis A. Tighe, and Gerard P. Aurigemma
Subjects: Aged, 80 and over, Male, medicine.medical_specialty, Movement Disorders, Aortic Aneurysm, Thoracic, business.industry, Diagnosis, Differential, Ventricular Dysfunction, Left, Echocardiography, Internal medicine, medicine, Cardiology, Humans, Radiology, Nuclear Medicine and imaging, Cardiology and Cardiovascular Medicine, business
Published: 2013

96. Introducing the CTA concept

Author: A. Mathieu, R. G. Wagner, K. Panagiotidis, S Rosier Lees, Julien Rousselle, M. Gómez Berisso, Michela Uslenghi, Stephen Maxfield, R. C. Shellard, Ivica Puljak, T. Le Flour, Thomas Schanz, Tobias C. Walther, Juanan Aguilar, Pierre Colin, M. Chikawa, N. Fouque, Mosè Mariotti, G. Fontaine, Merja Tornikoski, V. Diez-Blanco, Enrico Giro, A. Krepps, G. Koss, J. M. Martin, Sergio Billotta, E. de Oña Wilhelmi, Keitaro Takahashi, S. Buson, P. Brook, S. Steiner, M. Dyrda, Joseph Silk, Sera Markoff, P. Lubinski, U. Schwanke, Sauvik Bhattacharyya, J. Ripken, T. Haubold, C. Zurbach, H. Wetteskind, R. Hermel, J. Darling, J. Nicolau-Kukliński, Konstancja Satalecka, M. Videla, Stefan Funk, P. Conconi, S. Bajtlik, Lukasz Stawarz, J. M. Paredes, K. Reitberger, Stefan Wagner, Teresa Mineo, David Kieda, G. Pareschi, Shigeto Kabuki, Makoto Sawada, Antonio Stamerra, Rodolfo Canestrari, N. Baby, G. Crimi, P. Kostka, J. Grube, R. Zanin, I. K. Kominis, L. Mc Comb, R. Sternberger, M. Fesquet, M. Tokarz, David Fink, Daniela Dorner, N. Hamer Heras, A. Moralejo Olaizola, M. de Naurois, Diego F. Torres, Claes Fransson, K. Nishijima, Yutaka Fujita, L. Fresnillo, B. García, R. Kossakowski, A. Masserot, H. von Gunten, Alkiviadis F. Bais, Ciro Bigongiari, A. Saggion, G. Papyan, I. Mrusek, K. Farakos, J. Michałowski, A. Franckowiak, Fernando Martinez, M. Doert, R. Wawrzaszek, Michele Doro, L. Sapozhnikov, Claudia Lavalley, D. Thuermann, A.A. Zdziarski, Cristina Knapic, Karen Byrum, N. Neyroud, Petr Schovanek, W. Domainko, D. Kastana, E. Birsin, Adrian Biland, F. Sánchez, Alexandre Marcowith, M. Errando, R. L. C. Starling, J. Schultze, A. Weinstein, B. B. Singh, Yassir Moudden, Jelena Aleksić, C. L. Naumann, V. Waegebaert, M. Shayduk, U. F. Katz, Gianpiero Tagliaferri, M. Schroedter, A. Vollhardt, O. Reimann, Hideyuki Ohoka, Vincenzo Testa, C. Jablonski, Tsuguya Naito, J. Schäfer, Stavros Maltezos, A. Wierzcholska, P. Wawer, L. Nellen, F. Mirabel, Tatsuo Yoshida, P. H. Carton, Nina Nowak, L. Platos, Riccardo Rando, P. P. Krueger, R. Wischnewski, W. Romaszkan, E. Fede, Martino Marisaldi, Markus Gaug, Richard Willingale, J. H. Buckley, U. De AlmeidaBarres, J. Knapp, Saverio Lombardi, D. della Volpe, A. Herrero, A. Bottani, E. Delagnes, Martin J. Hardcastle, C. Morello, Anna Lipniacka, T. Greenshaw, M. Renaud, Giancarlo Cusumano, Jonathan Biteau, M. Sowiński, J. R. T. de Mello Neto, T. B. Humensky, Michael G. Richer, G. Parks, G. Grasseau, H. Baba, Gino Tosti, Damir Lelas, H. Krawzcynski, David Paneque, M. Barcelo, R. Dickherber, P. Ferrando, Shinji Hara, D. Florin, Hideaki Katagiri, T. Shibata, Fuyuki Tokanai, N. A. McCubbin, J. Gomez-Ortega, D. Nakajima, A. Liolios, P. Laporte, Orjan Dale, A. Sillanpää, Dainis Dravins, Timothée Grégoire, Nu. Komin, A. Mihailidis, L. Sidoli, Shiu-Hang Lee, A. W. Chen, J. M. Illa, A. Kuznetsov, P. Munar-Adrover, D. Dominis Prester, Marcos Daniel Actis, Abraham D. Falcone, L. Journet, D. Hadasch, N. Galante, A. Murphy, C. J. Todero Peixoto, S. Wiesand, A. Aravantinos, A. C. Rovero, J. L. Dournaux, P. Romano, M. Hrabovsky, R. de los Reyes Lopez, M. Ostrowski, J. Pallota, Geza Gyuk, Petar Temnikov, R. Dubois, Jan Ebr, R. Koul, David J. Smith, S. Schwarzburg, P. Manigot, Chad Finley, Tarek M. Hassan, Giuseppe Sottile, Evgeni Ovcharov, P. J. Rajda, F. Krennrich, Peter L. Moore, W. B. Focke, W. Bednarek, Elena Amato, Kazunori Kohri, J. Gamez-Garcia, I. Oya, A. Shibuya, German Hermann, William H. Lee, Dorota Sobczyńska, X. Zhou, C. Balkowski, G. Vallejo, M. Hayashida, M. Bitossi, Loukas Vlahos, H. Lockart, N. Geffroy, L. Tibaldo, Marek Jamrozy, Luke O'c. Drury, Pratik Majumdar, P. Sutcliffe, S. Schlenstedt, M. Palatka, Christophe Champion, H. Ueno, M. Rupiński, P. Giommi, J. Schwarz, G. Pühlhofer, Takashi Saito, W. van Driel, C. van Eldik, Q. Xiong, Yasuo Fukui, A. Donat, A. Ibarra, R. S. Warwick, Michiko Ohishi, A. W. Smith, J.-P. Lenain, Aion Viana, Terry Ashton, Guillaume Dubus, Jacek Niemiec, K. Kodani, Luis Ángel Tejedor, A. Wörnlein, Takanori Yoshikoshi, Masahiro Teshima, W. Gäbele, Ll. Font, Olaf Reimer, J. F. Valdés-Galicia, Lucy Fortson, J. P. Osborne, Mattia Fornasa, Keith Bechtol, Masayuki Tanaka, Shigehiro Nagataki, M. Rataj, M. Ribordy, Emmanuel Moulin, I. de la Calle, K. Winiarski, C. Jeanney, I. Mognet, I. Vegas, C. Juffroy, Yutaka Ohira, A. Jacholkowska, Matthew Wood, A. E. Suárez, J. Bähr, K. M. Schure, J. Maya, M. Dafonseca, J. Tasan, R. Sugawara, M. Bourgeat, A. Mancilla, D. Pelat, Olga Botner, D. Nedbal, G. Depaola, Robert Wagner, T. Okuda, H. Arnaldi, Josep Martí, P. Corona, T. Bonev, D. Yelos, J. Sieiro, V. Scalzotto, Jacco Vink, D. Languignon, Marco Ajello, J. Vandenbrouke, Philipp Mertsch, M. Mordalska, P. Wegner, P. Ziółkowski, P. T. O'Brien, A. Nozato, Robert D. Preece, B. Huber, Matteo Balbo, J.R. Bogart, R. Kankanyan, K. Mori, T. Jogler, Seth Digel, Claudio Vuerli, Hiromitsu Takahashi, Thomas Lohse, K. Saito, A. W. Borgland, Elisa Prandini, Helene Sol, Ryan Heller, M. Bogdan, D. Dumas, M. Stodulski, Y. Awane, Piercarlo Bonifacio, Pedro L. Luque-Escamilla, Judith H. Croston, Fabio Pizzolato, P. M. Chadwick, M. K. Daniel, Riccardo Paoletti, Reiko Orito, Katsuaki Asano, R. Frei, G. Disset, Valerie Connaughton, Juhani Huovelin, Hiroyasu Tajima, S. Vercellone, F. Feinstein, G. Decerprit, Riccardo Smareglia, S. Spyrou, Gustavo E. Romero, J. Shi, J. Carr, N. Girard, Dirk L. Hoffmann, Andreas Zech, Markus Boettcher, Osvaldo Catalano, Akira Okumura, M. Dohmke, C. Föhr, Sabrina Casanova, R. A. Cameron, Jan Conrad, K. Umehara, K. K. Yadav, A. Paizis, John L. Quinn, L. Pogosyan, C. Farnier, William J. Potter, Domenico Impiombato, Tadashi Kifune, Jonathan Granot, Gernot Maier, M. Cieślar, S. Palanque, G.W. Fraser, J. Prast, R. Bose, Heidi Sandaker, G. Lamanna, Dusan Mandat, J.F. Glicenstein, J. Harris, D. Naumann, J. Ziolkowski, Michał Szanecki, C. Delgado, J. Kocot, W. Lustermann, Sabine Elles, J. Schmoll, L. Gérard, M. López, Norita Kawanaka, V. Gika, B. Lieunard, A. Pichel, Martin Pohl, Mariusz Sterzel, S. Vincent, Paolo De Coppi, J. Lande, O. Blanch Bigas, Gianluca Giavitto, Yusuke Konno, Julian Sitarek, M. Panter, P.-O. Petrucci, F. Henault, M. Prouza, Philip Kaaret, Josep Colomé, Luciano Nicastro, German Martinez, L. Gebremedhin, J. M. Yebras, Apostolos Mastichiadis, A. S. Madhavan, Thomas J. Maccarone, K. Berger, R. Buehler, P. Jean, N. Sartore, F. Toussenel, Aris Karastergiou, W. Kluźniak, A. Djannati-Ataï, S. J. Fegan, Louis Antonelli, A. González Muñoz, J. Berdugo, S. S. Upadhya, M. Sidz, F. Mottez, Patrick Vogler, F. Di Pierro, Wystan Benbow, B. Sacco, L. Chiappetti, J. Dumm, R. Firpo Curcoll, David Gascon, V. Boccone, J. Krause, J. P. Avernet, B. Peyaud, B. De Lotto, Ana Babić, T. O. B. Schmidt, I. M. McHardy, T. Schweizer, S. P. Wakely, Daniel Gall, Frank M. Rieger, E. Sant'Ambrogio, M. Kagaya, P. Vincent, R. C. Rannot, Sandro Mereghetti, A. De Angelis, M. Scarcioffolo, R. White, G. H. Sembroski, Takeshi Nakamori, C. Medina, M. A. De Oliveira Leigui, Subir Sarkar, A. Marszałek, Reshmi Mukherjee, K. Nakayama, A. Fiasson, S. Giarrusso, T. Bernardino, J. P. Finley, D. Neise, L. O. Takalo, F. Grañena, Nikola Godinovic, H. Sasaki, P. Zychowski, Francesco Dazzi, B. Courty, A. Basili, Vitaly Neustroev, B. Khélifi, T. Glanzman, M. Trifoglio, Regis Terrier, R. A. Ong, E. M. Santos, M. Minuti, Thomas Bretz, R. Moderski, J. Kushida, S. Royer, Emilio Molinari, Etienne Lyard, J. Houles, Juan Abel Barrio, T. Lerch, S. Rivoire, T. Kishimoto, M. Cailles, M. Casiraghi, Nikolaos Stergioulas, J. Gaweda, S. Koyama, Ingomar Allekotte, E. Ismailova, Elina Giannakaki, S. Schwemmer, Ryo Yamazaki, G. Fasola, Christoph Deil, Jose Luis Contreras, T. Bird, Miguel A. Sánchez-Conde, J. Dick, E. Edy, D. Parsons, R. Pyzioł, R. Mirzoyan, Manjuli R. Sharma, J. Borkowski, Jonathan S. Lapington, Cameron B Rulten, Rino Bandiera, Volker Beckmann, Jun Kakuwa, Dimitris Balis, Kenji Toma, Anna Barnacka, Andrea Santangelo, L. Padilla, Peter Eger, G. Decock, Karol Seweryn, N. Sakaki, Darko Veberič, Andrea Bulgarelli, B. Rudak, M. Pérez, H. Koppel, Felix Spanier, M. I. Martínez, D. Horville, Marco Molinaro, R. Walter, P. Ramon, S. Brau-Nogue, J. Camprecios, K. Kärcher, John H. Seiradakis, S. Criswell, D. J. Leopold, V. J. Guarino, R. Gredig, S. Vorobiov, Viktor Gruev, Gareth Hughes, Daniele Spiga, Quirin Weitzel, N. Håkansson, Susumu Inoue, U. Straumann, Juan Cortina, B. Behera, Jürgen Knödlseder, Daniel Nieto, Tomasz Szepieniec, H. Prokoph, Jerzy Grygorczuk, G. De La Vega, Jim Hinton, E. Chabanne, M. Mahabir, R. Krobot, M. Capalbi, Miroslav Pech, C. Díaz, J. Ludwin, F. Gianotti, Garret Cotter, Claudio Melioli, Hiroaki Yamamoto, C. Veyssiere, Kunihito Ioka, S. Sun, J. M. Parraud, L. Rob, Felix Aharonian, G. Maneva, D. Melkumyan, T. Schwab, J. Kasperek, J. M. Huet, E. Lorenz, S. Tanaka, Y. A. Gallant, S. Couturier, B.W. Favill, J. Boix Gargallo, Andrea Tiengo, Leszek Bogacz, Andreu Sanuy, Christian Fruck, J. Sykes, C. Martens, A. Yoshida, Marek Sikora, E. Racero, G. Rouaix, N. Bhat, A. Salini, A. S. Barber, Mauro Ghigo, Jan Ridky, K. Kosack, Konrad Bernlöhr, C. Tenzer, Alice Allafort, M. Torres, Catherine Boisson, Grzegorz Kowal, M. Karczewski, G. Agnetta, Victor Stamatescu, Anthony H. Gonzalez, S. Rousselle, Giovanni Bonanno, A. Zajczyk, A. Gadola, P. Martin, V. Zitelli, I. Manthos, N. Maragos, A. Dettlaff, F. Profeti, S. Colonges, S. Gunji, S. Cazaux, S. Colafrancesco, M. Paz Arribas, Rika Hagiwara, Darell Engelhaupt, Nestor Mirabal, Johann Cohen-Tanugi, S. Grunewald, Abby M. Green, I. D. Davids, D. Nosek, T. Yamamoto, Gagik Tovmassian, R. Sakonaka, Miguel Alcubierre, C. Baixeras, T. L. Usher, Kazufumi Torii, H. Lüdecke, L. Wiśniewski, B. Kellner-Leidel, P. Demange, F. Gonzalez, B. Moal, V. De Caprio, V. Golev, K. Katarzyński, V. Bugaev, A. Reimer, J. Koziol, G. Pojmanski, Alessandro Carosi, J. Bolmont, A. Nikolaidis, R. J. García López, V. A. Kudryavtsev, C. Stegmann, J.-P. Ernenwein, M. Fiorini, Ivone F. M. Albuquerque, Marco Tavani, P. Korohoda, A. Giuliani, E. Carmona, C. Bauer, Kostas D. Kokkotas, O. Tibolla, G. Deleglise, Pierre Brun, Dinko Dimitrov, I. Jung, R. Steenkamp, Marc Ribó, Kathrin Egberts, P. Reardon, Adriano Ghedina, Stefan Rosén, N. Hidaka, Trygve Buanes, A. Segreto, H. Huan, Juri Poutanen, Ruben Lopez-Coto, S. Cavazzani, Massimiliano Belluso, A. Kretzschmann, F. De Frondat, A. Riviere, J. F. Olive, Tsunefumi Mizuno, Serena Mattiazzo, M. González, D. Fantinel, Matteo Cerruti, S. Vergani, Sabrina Einecke, N. La Palombara, Reinhard Schlickeiser, P. Antoranz, Pol Bordas, D. Paillot, V. de Souza, Yasushi Fukazawa, Phil Evans, Werner Hofmann, Hugh Dickinson, F. Roy, Yvonne Becherini, E. O. Angüner, D. Corti, T. C. Arlen, Francesco Russo, V. R. Chitnis, D. Ross, R. Gabriele, Massimo Persic, E. Fokitis, A. Bonardi, D. Garrido, A. Niedźwiecki, L. Cossio, Hidetoshi Kubo, Y. de Oliveira, F. Mattana, Anna Szostek, M. Compin, S. Blake, F. Lucarelli, Petter Hofverberg, Felix Ryde, M. Gougerot, C. Boutonnet, Dimitrios Emmanoulopoulos, A. Mangano, P. Vallania, Jose Miguel Miranda, A. Manalaysay, M. Raue, A. Bouvier, Shohei Yanagita, Nektarios Vlahakis, Joni Tammi, M. Naumann-Godo, Kohta Murase, E. Fillin-Martino, Jiri Chudoba, K. Hatanaka, A. Lopatin, N. Otte, G. Rojas, Tomonori Totani, K. S. Gothe, J. P. Vialle, D. Kolitzus, K. Warda, Hironori Matsumoto, J. Rico, P. Ringegni, James Chiang, R. McKay, A. Bobkov, Aya Bamba, H. Takami, B. Giebels, O. Grimm, S. Basso, F. Dubois, Victor Zabalza, A. Förster, Pasquale Blasi, Alexandros Papayannis, A. G. Akhperjanian, Eckhard Kendziorra, James A. Anderson, Giuseppe Malaguti, R. Welsing, S. Pita, A. Ozieblo, Heide Costantini, D. Tezier, J.-H. Köhne, M. Tluczykont, Ll. Garrido, Alexander Varón Sandoval, Matthew R. Orr, Dominique Durand, F. Chollet, O. Luz, E. O. Saemann, Jun Kataoka, M. Proyetti, C. Barbier, Jürgen Barnstedt, L. Bouchet, Hiroshi Muraishi, Anton N. Baushev, L. A. Otero, Denis Bastieri, S. Incorvaia, Tihomir Surić, V. La Parola, Nathan Smith, Karl-Heinz Sulanke, F. Bernard, Luca Stringhetti, S. Paiano, S. Federici, Hector Flores, Karl Mannheim, Michael S. Briggs, Giovanna Pedaletti, E. M. de Gouveia Dal Pino, J. D. Smith, G. La Rosa, Alicia López-Oramas, M. Janiak, Gary Drake, G. Talbot, Petr Travnicek, Elisabetta Bissaldi, Mario Meucci, R. Northrop, V. Scapin, Vito Conforti, J. D. Ponz, T. Aghajani, J. J. Jimenez, A. D. Supanitsky, Hernán Asorey, M. Werner, Brian Reville, A. Haupt, C. Skole, Gilles Henri, Daniele Gardiol, V. Vassiliev, R. Platzer, Y. Saito, A. La Barbera, Allan Hallgren, C. Eleftheriadis, S. Cantu, G. Maurin, K. Lacombe, A. Le Padellec, F. Stinzing, T. Hayakawa, A. Cillis, M. Suchenek, I. Monteiro, V. Sahakian, A. Di Paola, Grzegorz Madejski, A. De Luca, Andreas Quirrenbach, P. A. Caraveo, N. A. Webb, Michael Zacharias, J. Vanderwalt, Dario Hrupec, K. Ziȩtara, T. Armstrong, A. Lorca, T. Krähenbühl, A. Etchegoyen, Stefano Covino, C. Kalkuhl, K. Kitamoto, Tomasz Bulik, R. Rohlfs, D. Allan, A. Zhao, Luisa Arrabito, B. S. Acharya, T. Johnson, C. Schultz, G. Vasileiadis, Eleen Shum, Daniel Ferenc, Paola Grandi, Maria Concetta Maccarone, E. Strazzeri, H. Kelly, E. J. Quel, H. Vankov, Ruben Alfaro, I. Telezhinsky, J. Becker Tjus, C. Dufour, F. Köck, Ilana M. Braun, Jamie Holder, Ryoji Enomoto, Luigi Lessio, Michael Punch, Stefano Gabici, I. Puerto-Gimenez, S. Karkar, P. Nayman, M. Grudzińska, E. Aliu, Yoshiyuki Inoue, Elina Lindfors, J. Becerra, Daniel Mazin, Yukikatsu Terada, André Schulz, Teresa Montaruli, G. Bonnoli, S. Renner, Dieter Horns, J. Dyks, V. Pelassa, Mark I. Wilkinson, Ricardo Graciani, I. Troyano, P. Ristori, Thomas Kihm, P. Micolon, S. J. Nolan, Torsten Bringmann, David A. Williams, Joachim Hahn, L. Brunetti, U. Roeser, Wolfgang Rhode, Kanaris Tsinganos, Stefan Ohm, J. L. Panazol, G. Busetto, B. S., Acharya, M., Acti, T., Aghajani, G., Agnetta, J., Aguilar, F., Aharonian, M., Ajello, A., Akhperjanian, M., Alcubierre, J., Aleksic, R., Alfaro, E., Aliu, A. J., Allafort, D., Allan, I., Allekotte, E., Amato, J., Anderson, E. O., Anguener, L. A., Antonelli, P., Antoranz, A., Aravantino, T., Arlen, T., Armstrong, H., Arnaldi, L., Arrabito, K., Asano, T., Ashton, H. G., Asorey, Y., Awane, H., Baba, A., Babic, N., Baby, J., Baehr, A., Bai, C., Baixera, S., Bajtlik, M., Balbo, D., Bali, C., Balkowski, A., Bamba, R., Bandiera, A., Barber, C., Barbier, M., Barcelo, A., Barnacka, J., Barnstedt, U. B., De, J. A., Barrio, A., Basili, S., Basso, D., Bastieri, C., Bauer, A., Baushev, J., Becerra, Y., Becherini, K. C., Bechtol, J. B., Tju, V., Beckmann, W., Bednarek, B., Behera, M., Belluso, W., Benbow, J., Berdugo, K., Berger, F., Bernard, T., Bernardino, K., Bernloehr, N., Bhat, S., Bhattacharyya, C., Bigongiari, A., Biland, S., Billotta, T., Bird, E., Birsin, Bissaldi, Elisabetta, J., Biteau, M., Bitossi, S., Blake, O. B., Biga, P., Blasi, A., Bobkov, V., Boccone, M., Boettcher, L., Bogacz, J., Bogart, M., Bogdan, C., Boisson, J. B., Gargallo, J., Bolmont, G., Bonanno, A., Bonardi, T., Bonev, P., Bonifacio, G., Bonnoli, P., Borda, A., Borgland, J., Borkowski, R., Bose, O., Botner, A., Bottani, L., Bouchet, M., Bourgeat, C., Boutonnet, A., Bouvier, S., Brau Nogue, I., Braun, T., Bretz, M., Brigg, T., Bringmann, P., Brook, P., Brun, L., Brunetti, T., Buane, J., Buckley, R., Buehler, V., Bugaev, A., Bulgarelli, T., Bulik, G., Busetto, S., Buson, K., Byrum, M., Caille, R., Cameron, J., Camprecio, R., Canestrari, S., Cantu, M., Capalbi, P., Caraveo, E., Carmona, A., Carosi, J., Carr, P. . ., H., S., Casanova, M., Casiraghi, O., Catalano, S., Cavazzani, S., Cazaux, M., Cerruti, E., Chabanne, P., Chadwick, C., Champion, A., Chen, J., Chiang, L., Chiappetti, M., Chikawa, V. R., Chitni, F., Chollet, J., Chudoba, M., Cieslar, A., Cilli, J., Cohen Tanugi, S., Colafrancesco, P., Colin, J., Calome, S., Colonge, M., Compin, P., Conconi, V., Conforti, V., Connaughton, J., Conrad, J. L., Contrera, P., Coppi, P., Corona, D., Corti, J., Cortina, L., Cossio, H., Costantini, G., Cotter, B., Courty, S., Couturier, S., Covino, G., Crimi, S. J., Criswell, J., Croston, G., Cusumano, M., Dafonseca, O., Dale, M., Daniel, J., Darling, I., David, F., Dazzi, A. D., Angeli, V. D., Caprio, F. D., Frondat, E. M., De, I. d., La, G. A., De, R. d., Lo, B. D., Lotto, A. D., Luca, J. R., T., M. d., Nauroi, Y. d., Oliveira, E. d., Ona, V. d., Souza, G., Decerprit, G., Decock, C., Deil, E., Delagne, G., Deleglise, C., Delgado, D. D., Volpe, P., Demange, G., Depaola, A., Dettlaff, A. D., Paola, F. D., Pierro, C., Diaz, J., Dick, R., Dickherber, H., Dickinson, V., Diez Blanco, S., Digel, D., Dimitrov, G., Disset, A., Djannati Atai, M., Doert, M., Dohmke, W., Domainko, D. D., Prester, A., Donat, D., Dorner, M., Doro, J. . ., L., G., Drake, D., Dravin, L., Drury, F., Duboi, R., Duboi, G., Dubu, C., Dufour, D., Duma, J., Dumm, D., Durand, J., Dyk, M., Dyrda, J., Ebr, E., Edy, K., Egbert, P., Eger, S., Einecke, C., Eleftheriadi, S., Elle, D., Emmanoulopoulo, D., Engelhaupt, R., Enomoto, J. . ., P., M., Errando, A., Etchegoyen, P., Evan, A., Falcone, D., Fantinel, K., Farako, C., Farnier, G., Fasola, B., Favill, E., Fede, S., Federici, S., Fegan, F., Feinstein, D., Ferenc, P., Ferrando, M., Fesquet, A., Fiasson, E., Fillin Martino, D., Fink, C., Finley, J. P., Finley, M., Fiorini, R. F., Curcoll, H., Flore, D., Florin, W., Focke, C., Foehr, E., Fokiti, L., Font, G., Fontaine, M., Fornasa, A., Foerster, L., Fortson, N., Fouque, A., Franckowiak, C., Fransson, G., Fraser, R., Frei, I. F., M., L., Fresnillo, C., Fruck, Y., Fujita, Y., Fukazawa, Y., Fukui, S., Funk, W., Gaebele, S., Gabici, R., Gabriele, A., Gadola, N., Galante, D., Gall, Y., Gallant, J., Gamez Garcia, B., Garcia, R. G., Lopez, D., Gardiol, D., Garrido, L., Garrido, D., Gascon, M., Gaug, J., Gaweda, L., Gebremedhin, N., Geffroy, L., Gerard, A., Ghedina, M., Ghigo, E., Giannakaki, F., Gianotti, S., Giarrusso, G., Giavitto, B., Giebel, V., Gika, P., Giommi, N., Girard, E., Giro, A., Giuliani, T., Glanzman, J. . ., F., N., Godinovic, V., Golev, M. G., Berisso, J., Gomez Ortega, M. M., Gonzalez, A., Gonzalez, F., Gonzalez, A. G., Munoz, K. S., Gothe, M., Gougerot, R., Graciani, P., Grandi, F., Granena, J., Granot, G., Grasseau, R., Gredig, A., Green, T., Greenshaw, T., Gregoire, O., Grimm, J., Grube, M., Grudzinska, V., Gruev, S., Gruenewald, J., Grygorczuk, V., Guarino, S., Gunji, G., Gyuk, D., Hadasch, R., Hagiwara, J., Hahn, N., Hakansson, A., Hallgren, N. H., Hera, S., Hara, M. J., Hardcastle, J., Harri, T., Hassan, K., Hatanaka, T., Haubold, A., Haupt, T., Hayakawa, M., Hayashida, R., Heller, F., Henault, G., Henri, G., Hermann, R., Hermel, A., Herrero, N., Hidaka, J., Hinton, D., Hoffmann, W., Hofmann, P., Hofverberg, J., Holder, D., Horn, D., Horville, J., Houle, M., Hrabovsky, D., Hrupec, H., Huan, B., Huber, J. . ., M., G., Hughe, T. B., Humensky, J., Huovelin, A., Ibarra, J. M., Illa, D., Impiombato, S., Incorvaia, S., Inoue, Y., Inoue, K., Ioka, E., Ismailova, C., Jablonski, A., Jacholkowska, M., Jamrozy, M., Janiak, P., Jean, C., Jeanney, J. J., Jimenez, T., Jogler, T., Johnson, L., Journet, C., Juffroy, I., Jung, P., Kaaret, S., Kabuki, M., Kagaya, J., Kakuwa, C., Kalkuhl, R., Kankanyan, A., Karastergiou, K., Kaercher, M., Karczewski, S., Karkar, A., Kasperek, D., Kastana, H., Katagiri, J., Kataoka, K., Katarzynski, U., Katz, N., Kawanaka, B., Kellner Leidel, H., Kelly, E., Kendziorra, B., Khelifi, D. B., Kieda, T., Kifune, T., Kihm, T., Kishimoto, K., Kitamoto, W., Kluzniak, C., Knapic, J. w., Knapp, J., Knoedlseder, F., Koeck, J., Kocot, K., Kodani, J. . ., H., K., Kohri, K., Kokkota, D., Kolitzu, N., Komin, I., Komini, Y., Konno, H., Koeppel, P., Korohoda, K., Kosack, G., Ko, R., Kossakowski, P., Kostka, R., Koul, G., Kowal, S., Koyama, J., Koziol, T., Kraehenbuehl, J., Krause, H., Krawzcynski, F., Krennrich, A., Krepp, A., Kretzschmann, R., Krobot, P., Krueger, H., Kubo, V. A., Kudryavtsev, J., Kushida, A., Kuznetsov, A. L., Barbera, N. L., Palombara, V. L., Parola, G. L., Rosa, K., Lacombe, G., Lamanna, J., Lande, D., Languignon, J., Lapington, P., Laporte, C., Lavalley, T. L., Flour, A. L., Padellec, S. . ., H., W. H., Lee, M. A., Leigui, D., Lela, D. J., Leopold, T., Lerch, L., Lessio, B., Lieunard, E., Lindfor, A., Liolio, A., Lipniacka, H., Lockart, T., Lohse, S., Lombardi, A., Lopatin, M., Lopez, R., Lopez Coto, A., Lopez Orama, A., Lorca, E., Lorenz, P., Lubinski, F., Lucarelli, H., Luedecke, J., Ludwin, P. L., Luque Escamilla, W., Lustermann, O., Luz, E., Lyard, M. C., Maccarone, T. J., Maccarone, G. M., Madejski, A., Madhavan, M., Mahabir, G., Maier, P., Majumdar, G., Malaguti, S., Maltezo, A., Manalaysay, A., Mancilla, D., Mandat, G., Maneva, A., Mangano, P., Manigot, K., Mannheim, I., Mantho, N., Marago, A., Marcowith, M., Mariotti, M., Marisaldi, S., Markoff, A., Marszalek, C., Marten, J., Marti, P., Martin, G., Martinez, F., Martinez, M., Martinez, A., Masserot, A., Mastichiadi, A., Mathieu, H., Matsumoto, F., Mattana, S., Mattiazzo, G., Maurin, S., Maxfield, J., Maya, D., Mazin, L. M., Comb, N., Mccubbin, I., Mchardy, R., Mckay, C., Medina, C., Melioli, D., Melkumyan, S., Mereghetti, P., Mertsch, M., Meucci, J., Michalowski, P., Micolon, A., Mihailidi, T., Mineo, M., Minuti, N., Mirabal, F., Mirabel, J. M., Miranda, R., Mirzoyan, T., Mizuno, B., Moal, R., Moderski, I., Mognet, E., Molinari, M., Molinaro, T., Montaruli, I., Monteiro, P., Moore, A. M., Olaizola, M., Mordalska, C., Morello, K., Mori, F., Mottez, Y., Moudden, E., Moulin, I., Mrusek, R., Mukherjee, P., Munar Adrover, H., Muraishi, K., Murase, A., Murphy, S., Nagataki, T., Naito, D., Nakajima, T., Nakamori, K., Nakayama, C., Naumann, D., Naumann, M., Naumann Godo, P., Nayman, D., Nedbal, D., Neise, L., Nellen, V., Neustroev, N., Neyroud, L., Nicastro, J., Nicolau Kuklinski, A., Niedzwiecki, J., Niemiec, D., Nieto, A., Nikolaidi, K., Nishijima, S., Nolan, R., Northrop, D., Nosek, N., Nowak, A., Nozato, P., O'Brien, Y., Ohira, M., Ohishi, S., Ohm, H., Ohoka, T., Okuda, A., Okumura, R. A., Ong, R., Orito, M., Orr, J., Osborne, M., Ostrowski, L. A., Otero, N., Otte, E., Ovcharov, I., Oya, A., Ozieblo, L., Padilla, S., Paiano, D., Paillot, A., Paizi, S., Palanque, M., Palatka, J., Pallota, K., Panagiotidi, D., Paneque, M., Panter, R., Paoletti, A., Papayanni, G., Papyan, J. M., Parede, G., Pareschi, G., Park, D., Parson, M. P., Arriba, M., Pech, G., Pedaletti, V., Pelassa, D., Pelat, M. D., C., M., Persic, P. . ., O., B., Peyaud, A., Pichel, S., Pita, F., Pizzolato, L., Plato, R., Platzer, L., Pogosyan, M., Pohl, G., Pojmanski, J. D., Ponz, W., Potter, J., Poutanen, E., Prandini, J., Prast, R., Preece, F., Profeti, H., Prokoph, M., Prouza, M., Proyetti, I., Puerto Gimenez, G., Puehlhofer, I., Puljak, M., Punch, R., Pyziol, E. J., Quel, J., Quinn, A., Quirrenbach, E., Racero, P. J., Rajda, P., Ramon, R., Rando, R. C., Rannot, M., Rataj, M., Raue, P., Reardon, O., Reimann, A., Reimer, O., Reimer, K., Reitberger, M., Renaud, S., Renner, B., Reville, W., Rhode, M., Ribo, M., Ribordy, M. G., Richer, J., Rico, J., Ridky, F., Rieger, P., Ringegni, J., Ripken, P. R., Ristori, A., Riviere, S., Rivoire, L., Rob, U., Roeser, R., Rohlf, G., Roja, P., Romano, W., Romaszkan, G. E., Romero, S., Rosen, S. R., Lee, D., Ro, G., Rouaix, J., Rousselle, S., Rousselle, A. C., Rovero, F., Roy, S., Royer, B., Rudak, C., Rulten, M., Rupinski, F., Russo, F., Ryde, B., Sacco, E. O., Saemann, A., Saggion, V., Safiakian, K., Saito, T., Saito, Y., Saito, N., Sakaki, R., Sakonaka, A., Salini, F., Sanchez, M., Sanchez Conde, A., Sandoval, H., Sandaker, E., Sant'Ambrogio, A., Santangelo, E. M., Santo, A., Sanuy, L., Sapozhnikov, S., Sarkar, N., Sartore, H., Sasaki, K., Satalecka, M., Sawada, V., Scalzotto, V., Scapin, M., Scarcioffolo, J., Schafer, T., Schanz, S., Schlenstedt, R., Schlickeiser, T., Schmidt, J., Schmoll, P., Schovanek, M., Schroedter, C., Schultz, J., Schultze, A., Schulz, K., Schure, T., Schwab, U., Schwanke, J., Schwarz, S., Schwarzburg, T., Schweizer, S., Schwemmer, A., Segreto, G. H., Sembroski, K., Seweryn, M., Sharma, M., Shayduk, R. C., Shellard, J., Shi, T., Shibata, A., Shibuya, E., Shum, L., Sidoli, M., Sidz, J., Sieiro, M., Sikora, J., Silk, A., Sillanpaa, B. B., Singh, J., Sitarek, C., Skole, R., Smareglia, A., Smith, D., Smith, J., Smith, N., Smith, D., Sobczynska, H., Sol, G., Sottile, M., Sowinski, F., Spanier, D., Spiga, S., Spyrou, V., Stamatescu, A., Stamerra, R., Starling, L., Stawarz, R., Steenkamp, C., Stegmann, S., Steiner, N., Stergioula, R., Sternberger, M., Sterzel, F., Stinzing, M., Stodulski, U., Straumann, E., Strazzeri, L., Stringhetti, A., Suarez, M., Suchenek, R., Sugawara, K. . ., H., S., Sun, A. D., Supanitsky, T., Suric, P., Sutcliffe, J., Syke, M., Szanecki, T., Szepieniec, A., Szostek, G., Tagliaferri, H., Tajima, H., Takahashi, K., Takahashi, L., Takalo, H., Takami, C., Talbot, J., Tammi, M., Tanaka, S., Tanaka, J., Tasan, M., Tavani, L. A., Tejedor, I., Telezhinsky, P., Temnikov, C., Tenzer, Y., Terada, R., Terrier, M., Teshima, V., Testa, D., Tezier, D., Thuermann, L., Tibaldo, O., Tibolla, A., Tiengo, M., Tluczykont, C. J., Todero, F., Tokanai, M., Tokarz, K., Toma, K., Torii, M., Tornikoski, D. F., Torre, M., Torre, G., Tosti, T., Totani, C., Toussenel, G., Tovmassian, P., Travnicek, M., Trifoglio, I., Troyano, K., Tsingano, H., Ueno, K., Umehara, S. S., Upadhya, T., Usher, M., Uslenghi, J. F., Valdes Galicia, P., Vallania, G., Vallejo, W. v., Driel, C. v., Eldik, J., Vandenbrouke, J., Vanderwalt, H., Vankov, G., Vasileiadi, V., Vassiliev, D., Veberic, I., Vega, S., Vercellone, S., Vergani, C., Veyssiere, J. P., Vialle, A., Viana, M., Videla, P., Vincent, S., Vincent, J., Vink, N., Vlahaki, L., Vlaho, P., Vogler, A., Vollhardt, H. . ., P., S., Vorobiov, C., Vuerli, V., Waegebaert, R., Wagner, R. G., Wagner, S., Wagner, S. P., Wakely, R., Walter, T., Walther, K., Warda, R., Warwick, P., Wawer, R., Wawrzaszek, N., Webb, P., Wegner, A., Weinstein, Q., Weitzel, R., Welsing, M., Werner, H., Wetteskind, R., White, A., Wierzcholska, S., Wiesand, M., Wilkinson, D. A., William, R., Willingale, K., Winiarski, R., Wischnewski, L., Wisniewski, M., Wood, A., Woernlein, Q., Xiong, K. K., Yadav, H., Yamamoto, T., Yamamoto, R., Yamazaki, S., Yanagita, J. M., Yebra, D., Yelo, A., Yoshida, T., Yoshida, T., Yoshikoshi, V., Zabalza, M., Zacharia, A., Zajczyk, R., Zanin, A., Zdziarski, A., Zech, A., Zhao, X., Zhou, K., Zietara, J., Ziolkowski, P., Ziolkowski, V., Zitelli, C., Zurbach, P., Zychowski, Laboratoire d'Annecy de Physique des Particules (LAPP/Laboratoire d'Annecy-le-Vieux de Physique des Particules), Institut National de Physique Nucléaire et de Physique des Particules du CNRS (IN2P3)-Université Savoie Mont Blanc (USMB [Université de Savoie] [Université de Chambéry])-Centre National de la Recherche Scientifique (CNRS), AstroParticule et Cosmologie (APC (UMR_7164)), Institut National de Physique Nucléaire et de Physique des Particules du CNRS (IN2P3)-Centre National de la Recherche Scientifique (CNRS)-Commissariat à l'énergie atomique et aux énergies alternatives (CEA)-Observatoire de Paris, PSL Research University (PSL)-PSL Research University (PSL)-Université Paris Diderot - Paris 7 (UPD7), APC - Astrophysique des Hautes Energies (APC - AHE), PSL Research University (PSL)-PSL Research University (PSL)-Université Paris Diderot - Paris 7 (UPD7)-Institut National de Physique Nucléaire et de Physique des Particules du CNRS (IN2P3)-Centre National de la Recherche Scientifique (CNRS)-Commissariat à l'énergie atomique et aux énergies alternatives (CEA)-Observatoire de Paris, PSL Research University (PSL)-PSL Research University (PSL)-Université Paris Diderot - Paris 7 (UPD7)-Dipartimento di Astronomia, Universita degli Studi di Bologna, Università di Bologna [Bologna] (UNIBO)-Università di Bologna [Bologna] (UNIBO), Centre de Physique des Particules de Marseille (CPPM), Centre National de la Recherche Scientifique (CNRS)-Institut National de Physique Nucléaire et de Physique des Particules du CNRS (IN2P3)-Aix Marseille Université (AMU), Institut de Recherches sur les lois Fondamentales de l'Univers (IRFU), Commissariat à l'énergie atomique et aux énergies alternatives (CEA)-Université Paris-Saclay, CTA, Laboratoire Univers et Théories (LUTH (UMR_8102)), Institut national des sciences de l'Univers (INSU - CNRS)-Observatoire de Paris, Université Paris sciences et lettres (PSL)-Université Paris sciences et lettres (PSL)-Université Paris Diderot - Paris 7 (UPD7)-Centre National de la Recherche Scientifique (CNRS), Galaxies, Etoiles, Physique, Instrumentation (GEPI), Laboratoire d'Annecy de Physique des Particules (LAPP), Commissariat à l'énergie atomique et aux énergies alternatives (CEA)-Institut National de Physique Nucléaire et de Physique des Particules du CNRS (IN2P3)-Observatoire de Paris, Université Paris sciences et lettres (PSL)-Université Paris sciences et lettres (PSL)-Université Paris Diderot - Paris 7 (UPD7)-Centre National de la Recherche Scientifique (CNRS)-Commissariat à l'énergie atomique et aux énergies alternatives (CEA)-Institut National de Physique Nucléaire et de Physique des Particules du CNRS (IN2P3)-Observatoire de Paris, Université Paris sciences et lettres (PSL)-Université Paris sciences et lettres (PSL)-Université Paris Diderot - Paris 7 (UPD7)-Centre National de la Recherche Scientifique (CNRS)-Alma Mater Studiorum Università di Bologna [Bologna] (UNIBO), Aix Marseille Université (AMU)-Institut National de Physique Nucléaire et de Physique des Particules du CNRS (IN2P3)-Centre National de la Recherche Scientifique (CNRS), Université Paris sciences et lettres (PSL)-Université Paris sciences et lettres (PSL)-Centre National de la Recherche Scientifique (CNRS)-Université Paris Diderot - Paris 7 (UPD7), Observatoire de Paris, Université Paris sciences et lettres (PSL)-Université Paris sciences et lettres (PSL)-Commissariat à l'énergie atomique et aux énergies alternatives (CEA)-Université Paris Diderot - Paris 7 (UPD7)-Centre National de la Recherche Scientifique (CNRS)-Institut National de Physique Nucléaire et de Physique des Particules du CNRS (IN2P3), Université Paris sciences et lettres (PSL)-Université Paris sciences et lettres (PSL)-Commissariat à l'énergie atomique et aux énergies alternatives (CEA)-Université Paris Diderot - Paris 7 (UPD7)-Centre National de la Recherche Scientifique (CNRS)-Institut National de Physique Nucléaire et de Physique des Particules du CNRS (IN2P3)-Observatoire de Paris, Université Paris sciences et lettres (PSL)-Université Paris sciences et lettres (PSL)-Commissariat à l'énergie atomique et aux énergies alternatives (CEA)-Université Paris Diderot - Paris 7 (UPD7)-Centre National de la Recherche Scientifique (CNRS)-Institut National de Physique Nucléaire et de Physique des Particules du CNRS (IN2P3)-Dipartimento di Astronomia, Universita degli Studi di Bologna, Alma Mater Studiorum Università di Bologna [Bologna] (UNIBO)-Alma Mater Studiorum Università di Bologna [Bologna] (UNIBO), and High Energy Astrophys. & Astropart. Phys (API, FNWI)
Subjects: Next generation Cherenkov telescopes, Ciencias Físicas, 01 natural sciences, 7. Clean energy, TeV GAMMA-RAY ASTRONOMY, Observatory, Air showers, HESS, Cherenkov Telescopes, 010303 astronomy & astrophysics, MISSION, SUPERNOVA REMNANT W44, TELESCOPE, ASTRONOMY, EMISSION, Physics, ta213, [SDU.ASTR.HE]Sciences of the Universe [physics]/Astrophysics [astro-ph]/High Energy Astrophysical Phenomena [astro-ph.HE], Settore FIS/01 - Fisica Sperimentale, Astrophysics::Instrumentation and Methods for Astrophysics, TeV gamma-ray astronomy, ddc:540, CIENCIAS NATURALES Y EXACTAS, [PHYS.ASTR.HE]Physics [physics]/Astrophysics [astro-ph]/High Energy Astrophysical Phenomena [astro-ph.HE], [PHYS.ASTR.IM]Physics [physics]/Astrophysics [astro-ph]/Instrumentation and Methods for Astrophysic [astro-ph.IM], Air shower, AIR SHOWERS, Astrophysics::High Energy Astrophysical Phenomena, 0103 physical sciences, Preparatory phase, ta115, TeV gamma-ray astronomy Air showers Cherenkov Telescopes, 010308 nuclear & particles physics, business.industry, CHERENKOV TELESCOPES, Física, Astronomy, Institut für Physik und Astronomie, Astronomy and Astrophysics, ASTROFÍSICA, Cherenkov Telescope Array, [SDU.ASTR.IM]Sciences of the Universe [physics]/Astrophysics [astro-ph]/Instrumentation and Methods for Astrophysic [astro-ph.IM], Astronomía, Design study, Telecommunications, business
Abstract: The Cherenkov Telescope Array (CTA) is a new observatory for very high-energy (VHE) gamma rays. CTA has ambitions science goals, for which it is necessary to achieve full-sky coverage, to improve the sensitivity by about an order of magnitude, to span about four decades of energy, from a few tens of GeV to above 100 TeV with enhanced angular and energy resolutions over existing VHE gamma-ray observatories. An international collaboration has formed with more than 1000 members from 27 countries in Europe, Asia, Africa and North and South America. In 2010 the CTA Consortium completed a Design Study and started a three-year Preparatory Phase which leads to production readiness of CTA in 2014. In this paper we introduce the science goals and the concept of CTA, and provide an overview of the project., La lista completa de autores puede consultarse en el documento o en la página web de la revista., Facultad de Ingeniería
Published: 2013

97. Search for Photon-Linelike Signatures from Dark Matter Annihilations with H.E.S.S

Author: S. Schwarzburg, J. Dyks, G. Heinzelmann, M. C. Medina, Y. A. Gallant, H.-S. Zechlin, Reinhard Schlickeiser, J.-P. Tavernet, Daniel Hampf, Michael Punch, Sabrina Casanova, Marek Jamrozy, Christo Venter, C. Jahn, Francois Brun, Gilles Henri, J. Becker Tjus, U. F. Katz, M. J. Vorster, Hugh Dickinson, C. L. Naumann, Helene Sol, R. D. Parsons, Matteo Cerruti, A. Zech, G. Cologna, C. van Eldik, Pascal Vincent, P.-O. Petrucci, F. Krayzel, F. Sheidaei, J. Harris, A. Marcowith, N. W. Pekeur, Anna Szostek, D. Göring, L. Fallon, S. Häffner, R. C. G. Chaves, Petter Hofverberg, M. V. Fernandes, Joachim Ripken, Werner Hofmann, Michał Ostrowski, A. Abramowski, D. Nekrassov, Dmitry Klochkov, Pierre Brun, Alicja Wierzcholska, S. Kaufmann, Daniel Sánchez, Thomas Lohse, Frank M. Rieger, L. O'c. Drury, Svenja Carrigan, Julien Lefaucheur, M. Renaud, P. Bordas, R. Steenkamp, S. Klepser, A. Barnacka, J. D. Hague, F. Stinzing, André Schulz, M. H. Grondin, P. M. Chadwick, M. Tluczykont, M. Paz Arribas, B. Giebels, J. Perez, F. Feinstein, E. Birsin, Dieter Horns, Julien Masbou, S. Heinz, Chia-Chun Lu, S. J. Fegan, A. Djannati-Ataï, Aion Viana, Ullrich Schwanke, J. Mehault, S. J. Nolan, G. Spengler, Henning Gast, P. Espigat, M. Dalton, Stefan Ohm, Joachim Hahn, S. Colafrancesco, Gavin Rowell, A. A. Zdziarski, Peter Eger, C. Stegmann, A. Lopatin, S. Pita, B. Opitz, A. G. Akhperjanian, M. Holler, Gilles Maurin, Nu. Komin, R. de los Reyes, A. Cheesebrough, I. Oya, Jacek Niemiec, Krzysztof Katarzynski, T. J. L. McComb, R. Moderski, Olaf Reimer, Jan Conrad, Catherine Boisson, Regis Terrier, Anna Zajczyk, D. Nedbal, C. Farnier, R. White, B. Peyaud, J.-P. Lenain, P. Dewilt, K. Stycz, J. Bolmont, W. Domainko, R. Kossakowski, A. Balzer, U. Menzler, B. Khélifi, J. F. Glicenstein, Iurii Sushch, M. Füßling, T. Garrigoux, Emmanuel Moulin, G. Hermann, E. de Oña Wilhelmi, G. Fontaine, I. Jung, B. Rudak, Kathrin Egberts, S. Rosier-Lees, B. Degrange, G. Lamanna, Tomasz Bulik, B. Glück, Andreas Hillert, A. Jacholkowska, M. Mohamed, M. Gajdus, V. Sahakian, I. D. Davids, Jim Hinton, Łukasz Stawarz, A. Fiasson, Heinrich J. Völk, A. Bochow, Stefan Wagner, Gisela Anton, M. Mayer, Yvonne Becherini, P.P. Krüger, K. Kosack, J. Brucker, Konrad Bernlöhr, Andreas Quirrenbach, Vincent Marandon, G. Pühlhofer, A. Reimer, M. Naumann-Godo, Fabio Acero, Michal Dyrda, Michael Zacharias, M. de Naurois, M. Panter, Martin Ward, Cameron B Rulten, S. Balenderan, Dirk Lennarz, Serguei Vorobiov, M. K. Daniel, G. Pelletier, C. Trichard, Felix Aharonian, H. Laffon, J. L. Skilton, Jonathan Biteau, K. Valerius, S. Schwemmer, Andrea Santangelo, Guillaume Dubus, A. Förster, Martin Raue, L. Rob, D. Fernandez, N. Nguyen, M. A. Kastendieck, N. Maxted, G. Vasileiadis, K. Dutson, Christoph Deil, T. Kneiske, M. Lemoine-Goumard, Francesca Volpe, Denis Wouters, W. Kluźniak, C. Couturier, Institut für Experimentalphysik [Hamburg], Universität Hamburg (UHH), Laboratoire Univers et Particules de Montpellier (LUPM), Université Montpellier 2 - Sciences et Techniques (UM2)-Institut National de Physique Nucléaire et de Physique des Particules du CNRS (IN2P3)-Centre National de la Recherche Scientifique (CNRS), Max-Planck-Institut für Kernphysik (MPIK), Max-Planck-Gesellschaft, Dublin Institute for Advanced Studies (DIAS), National Academy of Sciences of the Republic of Armenia [Yerevan] (NAS RA), Yerevan Physics Institute, Yerevan State University, Friedrich-Alexander Universität Erlangen-Nürnberg (FAU), Department of Physics [Durham University], Durham University, Deutsches Elektronen-Synchrotron [Zeuthen] (DESY), Helmholtz-Gemeinschaft = Helmholtz Association, University of Potsdam = Universität Potsdam, Nicolaus Copernicus University [Toruń], Laboratoire Leprince-Ringuet (LLR), Institut National de Physique Nucléaire et de Physique des Particules du CNRS (IN2P3)-École polytechnique (X)-Centre National de la Recherche Scientifique (CNRS), AstroParticule et Cosmologie (APC (UMR_7164)), Commissariat à l'énergie atomique et aux énergies alternatives (CEA)-Institut National de Physique Nucléaire et de Physique des Particules du CNRS (IN2P3)-Observatoire de Paris, Université Paris sciences et lettres (PSL)-Université Paris sciences et lettres (PSL)-Université Paris Diderot - Paris 7 (UPD7)-Centre National de la Recherche Scientifique (CNRS), Astronomisches Institut der Ruhr-Universität Bochum, Ruhr-Universität Bochum [Bochum], Humboldt University Of Berlin, Laboratoire Univers et Théories (LUTH (UMR_8102)), Institut national des sciences de l'Univers (INSU - CNRS)-Observatoire de Paris, Laboratoire de Physique Nucléaire et de Hautes Énergies (LPNHE), Université Pierre et Marie Curie - Paris 6 (UPMC)-Institut National de Physique Nucléaire et de Physique des Particules du CNRS (IN2P3)-Université Paris Diderot - Paris 7 (UPD7)-Centre National de la Recherche Scientifique (CNRS), Institut für Astronomie und Astrophysik [Tübingen] (IAAT), Eberhard Karls Universität Tübingen = Eberhard Karls University of Tuebingen, CEA- Saclay (CEA), Commissariat à l'énergie atomique et aux énergies alternatives (CEA), Astronomical Observatory [Warsaw], Faculty of Physics [Warsaw] (FUW), University of Warsaw (UW)-University of Warsaw (UW), North-West University [Potchefstroom] (NWU), University of the Witwatersrand [Johannesburg] (WITS), Zentrum für Astronomie der Universität Heidelberg (ZAH), Universität Heidelberg [Heidelberg] = Heidelberg University, Oskar Klein Centre [Stockholm], Stockholm University, Centre d'Etudes Nucléaires de Bordeaux Gradignan (CENBG), Université Sciences et Technologies - Bordeaux 1 (UB)-Institut National de Physique Nucléaire et de Physique des Particules du CNRS (IN2P3)-Centre National de la Recherche Scientifique (CNRS), Namibia University of Science and Technology (NUST), University of South Australia [Adelaide], APC - Astrophysique des Hautes Energies (APC - AHE), Université Paris sciences et lettres (PSL)-Université Paris sciences et lettres (PSL)-Université Paris Diderot - Paris 7 (UPD7)-Centre National de la Recherche Scientifique (CNRS)-Commissariat à l'énergie atomique et aux énergies alternatives (CEA)-Institut National de Physique Nucléaire et de Physique des Particules du CNRS (IN2P3)-Observatoire de Paris, Université Paris sciences et lettres (PSL)-Université Paris sciences et lettres (PSL)-Université Paris Diderot - Paris 7 (UPD7)-Centre National de la Recherche Scientifique (CNRS)-Alma Mater Studiorum Università di Bologna [Bologna] (UNIBO), Institut de Planétologie et d'Astrophysique de Grenoble (IPAG ), Observatoire des Sciences de l'Univers de Grenoble (OSUG), Université Joseph Fourier - Grenoble 1 (UJF)-Institut polytechnique de Grenoble - Grenoble Institute of Technology (Grenoble INP )-Institut national des sciences de l'Univers (INSU - CNRS)-Institut national de recherche en sciences et technologies pour l'environnement et l'agriculture (IRSTEA)-Université Savoie Mont Blanc (USMB [Université de Savoie] [Université de Chambéry])-Centre National de la Recherche Scientifique (CNRS)-Université Joseph Fourier - Grenoble 1 (UJF)-Institut polytechnique de Grenoble - Grenoble Institute of Technology (Grenoble INP )-Institut national des sciences de l'Univers (INSU - CNRS)-Institut national de recherche en sciences et technologies pour l'environnement et l'agriculture (IRSTEA)-Université Savoie Mont Blanc (USMB [Université de Savoie] [Université de Chambéry])-Centre National de la Recherche Scientifique (CNRS)-Centre National d'Études Spatiales [Toulouse] (CNES)-Centre National de la Recherche Scientifique (CNRS), Department of Physics and Astronomy [Leicester], University of Leicester, Instytut Fizyki Jądrowej PAN (IFJ), Polskiej Akademii Nauk, Leopold Franzens Universität Innsbruck - University of Innsbruck, Laboratoire d'Annecy de Physique des Particules (LAPP), Institut National de Physique Nucléaire et de Physique des Particules du CNRS (IN2P3)-Université Savoie Mont Blanc (USMB [Université de Savoie] [Université de Chambéry])-Centre National de la Recherche Scientifique (CNRS), Max Planck Institute for Astronomy (MPIA), Uniwersytet Jagielloński w Krakowie = Jagiellonian University (UJ), Torun Centre for Astronomy (TCfA), Physikalisches Institut [Erlangen], Institut für Theoretische Physik IV [Bochum] (ITP4), Space Research Centre [Torun], Polska Akademia Nauk = Polish Academy of Sciences (PAN), Astronomical Institute of Charles University, Charles University [Prague] (CU), Space Research Centre [Leicester], HESS, Université de Montpellier (UM)-Université Montpellier 2 - Sciences et Techniques (UM2)-Institut National de Physique Nucléaire et de Physique des Particules du CNRS (IN2P3)-Centre National de la Recherche Scientifique (CNRS), Institut National de Physique Nucléaire et de Physique des Particules du CNRS (IN2P3)-Centre National de la Recherche Scientifique (CNRS)-Commissariat à l'énergie atomique et aux énergies alternatives (CEA)-Observatoire de Paris, PSL Research University (PSL)-PSL Research University (PSL)-Université Paris Diderot - Paris 7 (UPD7), PSL Research University (PSL)-PSL Research University (PSL)-Université Paris Diderot - Paris 7 (UPD7)-Institut National de Physique Nucléaire et de Physique des Particules du CNRS (IN2P3)-Centre National de la Recherche Scientifique (CNRS)-Commissariat à l'énergie atomique et aux énergies alternatives (CEA)-Observatoire de Paris, PSL Research University (PSL)-PSL Research University (PSL)-Université Paris Diderot - Paris 7 (UPD7)-Dipartimento di Astronomia, Universita degli Studi di Bologna, Università di Bologna [Bologna] (UNIBO)-Università di Bologna [Bologna] (UNIBO), Laboratoire d'Annecy de Physique des Particules (LAPP/Laboratoire d'Annecy-le-Vieux de Physique des Particules), GLAST, Université Sciences et Technologies - Bordeaux 1-Institut National de Physique Nucléaire et de Physique des Particules du CNRS (IN2P3)-Centre National de la Recherche Scientifique (CNRS)-Université Sciences et Technologies - Bordeaux 1-Institut National de Physique Nucléaire et de Physique des Particules du CNRS (IN2P3)-Centre National de la Recherche Scientifique (CNRS), Université Montpellier 2 - Sciences et Techniques (UM2)-Institut National de Physique Nucléaire et de Physique des Particules du CNRS (IN2P3)-Université de Montpellier (UM)-Centre National de la Recherche Scientifique (CNRS), Universität Potsdam, Centre National de la Recherche Scientifique (CNRS)-École polytechnique (X)-Institut National de Physique Nucléaire et de Physique des Particules du CNRS (IN2P3), Observatoire de Paris, Université Paris sciences et lettres (PSL)-Université Paris sciences et lettres (PSL)-Commissariat à l'énergie atomique et aux énergies alternatives (CEA)-Université Paris Diderot - Paris 7 (UPD7)-Centre National de la Recherche Scientifique (CNRS)-Institut National de Physique Nucléaire et de Physique des Particules du CNRS (IN2P3), Humboldt-Universität zu Berlin, Université Paris sciences et lettres (PSL)-Université Paris sciences et lettres (PSL)-Centre National de la Recherche Scientifique (CNRS)-Université Paris Diderot - Paris 7 (UPD7), Centre National de la Recherche Scientifique (CNRS)-Université Paris Diderot - Paris 7 (UPD7)-Institut National de Physique Nucléaire et de Physique des Particules du CNRS (IN2P3)-Université Pierre et Marie Curie - Paris 6 (UPMC), Unit for Space Physics, North-West University, South-Africa, Unit for Space Physics, North-West University, APC - Cosmologie, Université Paris sciences et lettres (PSL)-Université Paris sciences et lettres (PSL)-Centre National de la Recherche Scientifique (CNRS)-Université de Paris (UP)-Commissariat à l'énergie atomique et aux énergies alternatives (CEA)-Institut National de Physique Nucléaire et de Physique des Particules du CNRS (IN2P3)-Observatoire de Paris, Université Paris sciences et lettres (PSL)-Université Paris sciences et lettres (PSL)-Centre National de la Recherche Scientifique (CNRS)-Université de Paris (UP), Universität Heidelberg [Heidelberg], Laboratoire de Physique Nucléaire et de Hautes Énergies (LPNHE (UMR_7585)), Institut National de Physique Nucléaire et de Physique des Particules du CNRS (IN2P3)-Sorbonne Université (SU)-Centre National de la Recherche Scientifique (CNRS)-Université de Paris (UP), Université Sciences et Technologies - Bordeaux 1-Institut National de Physique Nucléaire et de Physique des Particules du CNRS (IN2P3)-Centre National de la Recherche Scientifique (CNRS), Université Paris sciences et lettres (PSL)-Université Paris sciences et lettres (PSL)-Commissariat à l'énergie atomique et aux énergies alternatives (CEA)-Université Paris Diderot - Paris 7 (UPD7)-Centre National de la Recherche Scientifique (CNRS)-Institut National de Physique Nucléaire et de Physique des Particules du CNRS (IN2P3)-Observatoire de Paris, Université Paris sciences et lettres (PSL)-Université Paris sciences et lettres (PSL)-Commissariat à l'énergie atomique et aux énergies alternatives (CEA)-Université Paris Diderot - Paris 7 (UPD7)-Centre National de la Recherche Scientifique (CNRS)-Institut National de Physique Nucléaire et de Physique des Particules du CNRS (IN2P3)-Dipartimento di Astronomia, Universita degli Studi di Bologna, Alma Mater Studiorum Università di Bologna [Bologna] (UNIBO)-Alma Mater Studiorum Università di Bologna [Bologna] (UNIBO), Centre National d'Études Spatiales [Toulouse] (CNES)-Centre National de la Recherche Scientifique (CNRS)-Observatoire des Sciences de l'Univers de Grenoble (OSUG), Université Joseph Fourier - Grenoble 1 (UJF)-Institut polytechnique de Grenoble - Grenoble Institute of Technology (Grenoble INP )-Institut national des sciences de l'Univers (INSU - CNRS)-Institut national de recherche en sciences et technologies pour l'environnement et l'agriculture (IRSTEA)-Université Savoie Mont Blanc (USMB [Université de Savoie] [Université de Chambéry])-Centre National de la Recherche Scientifique (CNRS)-Université Joseph Fourier - Grenoble 1 (UJF)-Institut polytechnique de Grenoble - Grenoble Institute of Technology (Grenoble INP )-Institut national des sciences de l'Univers (INSU - CNRS)-Institut national de recherche en sciences et technologies pour l'environnement et l'agriculture (IRSTEA)-Université Savoie Mont Blanc (USMB [Université de Savoie] [Université de Chambéry])-Centre National de la Recherche Scientifique (CNRS), 11749903 - Krüger, Petrus Paulus, 22050574 - Pekeur, Nicolette Whilna, 12006653 - Venter, Christo, 22164405 - Sheidaei, Farzaneh, 12792322 - Vorster, Michael Johannes, and 23909196 - Casanova, Sabrina
Subjects: [PHYS.ASTR.HE]Physics [physics]/Astrophysics [astro-ph]/High Energy Astrophysical Phenomena [astro-ph.HE], 95.85.Pw, Ciencias Físicas, Milky Way, Astrophysics::High Energy Astrophysical Phenomena, Dark matter, General Physics and Astronomy, FOS: Physical sciences, Astrophysics, Astrophysics::Cosmology and Extragalactic Astrophysics, 7. Clean energy, 01 natural sciences, Gamma-ray, purl.org/becyt/ford/1 [https], 0103 physical sciences, ddc:550, 010306 general physics, Astrophysics::Galaxy Astrophysics, Line (formation), Astroparticle physics, Physics, High Energy Astrophysical Phenomena (astro-ph.HE), Annihilation, 010308 nuclear & particles physics, [SDU.ASTR.HE]Sciences of the Universe [physics]/Astrophysics [astro-ph]/High Energy Astrophysical Phenomena [astro-ph.HE], Gamma ray, Institut für Physik und Astronomie, purl.org/becyt/ford/1.3 [https], Gamma-Rays, Astronomía, Dark Matter Annihilations, Dark matter halo, 95.35.+d, Halo, Astrophysics - High Energy Astrophysical Phenomena, CIENCIAS NATURALES Y EXACTAS
Abstract: Gamma-ray line signatures can be expected in the very-high-energy (VHE; E_\gamma > 100 GeV) domain due to self-annihilation or decay of dark matter (DM) particles in space. Such a signal would be readily distinguishable from astrophysical \gamma-ray sources that in most cases produce continuous spectra which span over several orders of magnitude in energy. Using data collected with the H.E.S.S. \gamma-ray instrument, upper limits on line-like emission are obtained in the energy range between ~500 GeV and ~25 TeV for the central part of the Milky Way halo and for extragalactic observations, complementing recent limits obtained with the Fermi-LAT instrument at lower energies. No statistically significant signal could be found. For monochromatic \gamma-ray line emission, flux limits of (2x10^-7 - 2x10^-5) m^-2 s^-1 sr^-1 and (1x10^-8 - 2x10^-6) m^-2 s^-1 sr^-1 are obtained for the central part of the Milky Way halo and extragalactic observations, respectively. For a DM particle mass of 1 TeV, limits on the velocity-averaged DM annihilation cross section < \sigma v >(\chi\chi -> \gamma\gamma) reach ~10^-27 cm^3 s^-1, based on the Einasto parametrization of the Galactic DM halo density profile., Comment: 6 pages, 4 figures, accepted for publication in Phys. Rev. Lett
Published: 2013

98. HESS and Fermi-LAT discovery of gamma-rays from the blazar 1ES 1312-423

Author: J. Biteau, Michael Punch, G. Fontaine, Mateusz Janiak, S. J. Fegan, M. Weidinger, Svenja Carrigan, E. Birsin, Gilles Henri, André Schulz, Christian Farnier, G. Lamanna, D. Goering, Dieter Horns, Anna Zajczyk, P. Wagner, K. Dutson, A. Woernlein, Emmanuel Moulin, F. Stinzing, B. Giebels, Alexandre Marcowith, C. L. Naumann, A. A. Zdziarski, M. J. Vorster, A. Jacholkowska, P. Willmann, Michal Dyrda, Thomas Lohse, G. Puehlhofer, T. Garrigoux, Christo Venter, J. Brucker, Gavin Rowell, Dirk Lennarz, R. de los Reyes, Denis Wouters, V. Sahakian, Christoph Deil, Jamie Stevens, M. K. Daniel, Elisabetta Bissaldi, T. Kneiske, J. S. Perkins, S. Haeffner, C. Jahn, U. F. Katz, R. Moderski, A. Zech, Vincent Marandon, D. Klochkov, S. Schwarzburg, H. J. Voelk, P. Espigat, C. Stegmann, Nu. Komin, K. Stycz, F. Schuessler, Tanya Edwards, Luke O'c. Drury, Andreas Quirrenbach, C. Couturier, M. Gajdus, Guillaume Dubus, J. F. Glicenstein, K. Bernloehr, Catherine Boisson, Stefan Ohm, I. Oya, Jacek Niemiec, M. Kieffer, S. Pita, M. Holler, Michael Zacharias, M. Dalton, A. Cheesebrough, Pierre Brun, J. Perez, Philip G. Edwards, Olaf Reimer, S. Schwemmer, Jan Conrad, Matthias Kadler, N. Maxted, Manuel Meyer, J. Dyks, E. de Oña Wilhelmi, A. Reimer, Fabio Acero, Andrea Santangelo, Francois Brun, M. Chrétien, L. Rob, A. Fiasson, D. Fernandez, Matteo Cerruti, M. Panter, M. de Naurois, G. Maurin, Thomas Murach, U. Menzler, F. Krayzel, S. Klepser, Anna Barnacka, B. Khélifi, Roopesh Ojha, G. Hermann, M. A. Kastendieck, Regis Terrier, M. Tluczykont, G. Vasileiadis, M. V. Fernandes, M. Paz Arribas, Francesca Volpe, C. Trichard, M. Fuessling, Werner Hofmann, Michał Ostrowski, P. P. Krueger, F. Feinstein, G. Cologna, C. van Eldik, Jim Hinton, Andreas Hillert, J. D. Hague, M. C. Medina, Y. A. Gallant, H.-S. Zechlin, Felix Jankowsky, Peter Eger, Ullrich Schwanke, C-C Lu, A. Djannati-Ataï, L. Oakes, Henning Gast, M. Renaud, Martin Raue, A. G. Akhperjanian, O. Hervet, R. Steenkamp, I. D. Davids, Iurii Sushch, R. D. Parsons, S. Rosier-Lees, P. deWilt, K. Katarzyński, Marek Jamrozy, M. Mohamed, Helene Sol, J. Harris, Sabrina Casanova, Karl Kosack, Frank M. Rieger, J. Mehault, F. Spiess, S. Raab, A. Abramowski, J.-P. Tavernet, W. Kluzniak, T. J. L. McComb, P-O. Petrucci, B. Peyaud, R. White, S. Colafrancesco, I. Jung, B. Rudak, Kathrin Egberts, P. M. Chadwick, B. Degrange, Marianne Lemoine-Goumard, R. Chalme-Calvet, R. C. G. Chaves, Yvonne Becherini, Anna Szostek, Petter Hofverberg, Aion Viana, B. Opitz, A. Foerster, E. O. Anguener, D. Kolitzus, G. Heinzelmann, J. Bolmont, Guy Pelletier, Alicja Wierzcholska, S. Kaufmann, M. H. Grondin, Helen Poon, A. Lopatin, J.-P. Lenain, Reinhard Schlickeiser, Pol Bordas, Hugh Dickinson, J. Becker Tjus, Daniel Sánchez, M. Grudzińska, N. W. Pekeur, Tomasz Bulik, G. Spengler, S. J. Nolan, Joachim Hahn, W. Domainko, A. Balzer, Stefan Wagner, Gisela Anton, M. Mayer, Cameron B Rulten, S. Balenderan, Felix Aharonian, H. Laffon, K. Valerius, Julien Lefaucheur, D. Nedbal, L. Stawarz, P. Vincent, S. Krakau, Martin Ward, Laboratoire Univers et Particules de Montpellier (LUPM), Centre National de la Recherche Scientifique (CNRS)-Université de Montpellier (UM)-Institut National de Physique Nucléaire et de Physique des Particules du CNRS (IN2P3)-Université Montpellier 2 - Sciences et Techniques (UM2), AstroParticule et Cosmologie (APC (UMR_7164)), Observatoire de Paris, Université Paris sciences et lettres (PSL)-Université Paris sciences et lettres (PSL)-Commissariat à l'énergie atomique et aux énergies alternatives (CEA)-Université Paris Diderot - Paris 7 (UPD7)-Centre National de la Recherche Scientifique (CNRS)-Institut National de Physique Nucléaire et de Physique des Particules du CNRS (IN2P3), Laboratoire Univers et Théories (LUTH (UMR_8102)), Institut national des sciences de l'Univers (INSU - CNRS)-Observatoire de Paris, Université Paris sciences et lettres (PSL)-Université Paris sciences et lettres (PSL)-Centre National de la Recherche Scientifique (CNRS)-Université Paris Diderot - Paris 7 (UPD7), Laboratoire Leprince-Ringuet (LLR), Centre National de la Recherche Scientifique (CNRS)-École polytechnique (X)-Institut National de Physique Nucléaire et de Physique des Particules du CNRS (IN2P3), Laboratoire de Physique Nucléaire et de Hautes Énergies (LPNHE), Centre National de la Recherche Scientifique (CNRS)-Université Paris Diderot - Paris 7 (UPD7)-Institut National de Physique Nucléaire et de Physique des Particules du CNRS (IN2P3)-Université Pierre et Marie Curie - Paris 6 (UPMC), FERMI, Centre d'Etudes Nucléaires de Bordeaux Gradignan (CENBG), Université Sciences et Technologies - Bordeaux 1-Institut National de Physique Nucléaire et de Physique des Particules du CNRS (IN2P3)-Centre National de la Recherche Scientifique (CNRS)-Université Sciences et Technologies - Bordeaux 1-Institut National de Physique Nucléaire et de Physique des Particules du CNRS (IN2P3)-Centre National de la Recherche Scientifique (CNRS), Laboratoire d'Annecy de Physique des Particules (LAPP), Institut National de Physique Nucléaire et de Physique des Particules du CNRS (IN2P3)-Université Savoie Mont Blanc (USMB [Université de Savoie] [Université de Chambéry])-Centre National de la Recherche Scientifique (CNRS), APC - Astrophysique des Hautes Energies (APC - AHE), Université Paris sciences et lettres (PSL)-Université Paris sciences et lettres (PSL)-Commissariat à l'énergie atomique et aux énergies alternatives (CEA)-Université Paris Diderot - Paris 7 (UPD7)-Centre National de la Recherche Scientifique (CNRS)-Institut National de Physique Nucléaire et de Physique des Particules du CNRS (IN2P3)-Observatoire de Paris, Université Paris sciences et lettres (PSL)-Université Paris sciences et lettres (PSL)-Commissariat à l'énergie atomique et aux énergies alternatives (CEA)-Université Paris Diderot - Paris 7 (UPD7)-Centre National de la Recherche Scientifique (CNRS)-Institut National de Physique Nucléaire et de Physique des Particules du CNRS (IN2P3)-Dipartimento di Astronomia, Universita degli Studi di Bologna, Alma Mater Studiorum Università di Bologna [Bologna] (UNIBO)-Alma Mater Studiorum Università di Bologna [Bologna] (UNIBO), HESS, Université Montpellier 2 - Sciences et Techniques (UM2)-Institut National de Physique Nucléaire et de Physique des Particules du CNRS (IN2P3)-Centre National de la Recherche Scientifique (CNRS), Commissariat à l'énergie atomique et aux énergies alternatives (CEA)-Institut National de Physique Nucléaire et de Physique des Particules du CNRS (IN2P3)-Observatoire de Paris, Université Paris sciences et lettres (PSL)-Université Paris sciences et lettres (PSL)-Université Paris Diderot - Paris 7 (UPD7)-Centre National de la Recherche Scientifique (CNRS), Institut National de Physique Nucléaire et de Physique des Particules du CNRS (IN2P3)-École polytechnique (X)-Centre National de la Recherche Scientifique (CNRS), Université Pierre et Marie Curie - Paris 6 (UPMC)-Institut National de Physique Nucléaire et de Physique des Particules du CNRS (IN2P3)-Université Paris Diderot - Paris 7 (UPD7)-Centre National de la Recherche Scientifique (CNRS), Université Sciences et Technologies - Bordeaux 1 (UB)-Institut National de Physique Nucléaire et de Physique des Particules du CNRS (IN2P3)-Centre National de la Recherche Scientifique (CNRS)-Université Sciences et Technologies - Bordeaux 1 (UB)-Institut National de Physique Nucléaire et de Physique des Particules du CNRS (IN2P3)-Centre National de la Recherche Scientifique (CNRS), Université Paris sciences et lettres (PSL)-Université Paris sciences et lettres (PSL)-Université Paris Diderot - Paris 7 (UPD7)-Centre National de la Recherche Scientifique (CNRS)-Commissariat à l'énergie atomique et aux énergies alternatives (CEA)-Institut National de Physique Nucléaire et de Physique des Particules du CNRS (IN2P3)-Observatoire de Paris, Université Paris sciences et lettres (PSL)-Université Paris sciences et lettres (PSL)-Université Paris Diderot - Paris 7 (UPD7)-Centre National de la Recherche Scientifique (CNRS)-Alma Mater Studiorum Università di Bologna [Bologna] (UNIBO), Université de Montpellier (UM)-Université Montpellier 2 - Sciences et Techniques (UM2)-Institut National de Physique Nucléaire et de Physique des Particules du CNRS (IN2P3)-Centre National de la Recherche Scientifique (CNRS), Institut National de Physique Nucléaire et de Physique des Particules du CNRS (IN2P3)-Centre National de la Recherche Scientifique (CNRS)-Commissariat à l'énergie atomique et aux énergies alternatives (CEA)-Observatoire de Paris, PSL Research University (PSL)-PSL Research University (PSL)-Université Paris Diderot - Paris 7 (UPD7), Laboratoire d'Annecy de Physique des Particules (LAPP/Laboratoire d'Annecy-le-Vieux de Physique des Particules), PSL Research University (PSL)-PSL Research University (PSL)-Université Paris Diderot - Paris 7 (UPD7)-Institut National de Physique Nucléaire et de Physique des Particules du CNRS (IN2P3)-Centre National de la Recherche Scientifique (CNRS)-Commissariat à l'énergie atomique et aux énergies alternatives (CEA)-Observatoire de Paris, PSL Research University (PSL)-PSL Research University (PSL)-Université Paris Diderot - Paris 7 (UPD7)-Dipartimento di Astronomia, Universita degli Studi di Bologna, Università di Bologna [Bologna] (UNIBO)-Università di Bologna [Bologna] (UNIBO), 10103449 - Krüger, Petrus Paulus, 22050574 - Pekeur, Nicolette Whilna, 12006653 - Venter, Christo, 12792322 - Vorster, Michael Johannes, 24922986 - Sushch, Iurii, 23909196 - Casanova, Sabrina, A., Abramowski, F., Acero, F., Aharonian, A. G., Akhperjanian, E., Anguener, G., Anton, S., Balenderan, A., Balzer, A., Barnacka, Y., Becherini, J. B., Tju, K., Bernloehr, E., Birsin, Bissaldi, Elisabetta, J., Biteau, C., Boisson, J., Bolmont, P., Borda, J., Brucker, F., Brun, P., Brun, T., Bulik, S., Carrigan, S., Casanova, M., Cerruti, P. M., Chadwick, R., Chalme Calvet, R. C., G., A., Cheesebrough, M., Chretien, S., Colafrancesco, G., Cologna, J., Conrad, C., Couturier, M., Dalton, M. K., Daniel, I. D., David, B., Degrange, C., Deil, P., Dewilt, H. J., Dickinson, A., Djannati Atai, W., Domainko, L. O., '., G., Dubu, K., Dutson, J., Dyk, M., Dyrda, T., Edward, K., Egbert, P., Eger, P., Espigat, C., Farnier, S., Fegan, F., Feinstein, M. V., Fernande, D., Fernandez, A., Fiasson, G., Fontaine, A., Foerster, M., Fuessling, M., Gajdu, Y. A., Gallant, T., Garrigoux, H., Gast, B., Giebel, J. F., Glicenstein, D., Goering, M. . ., H., M., Grudzinska, S., Haeffner, J. D., Hague, J., Hahn, J., Harri, G., Heinzelmann, G., Henri, G., Hermann, O., Hervet, A., Hillert, J. A., Hinton, W., Hofmann, P., Hofverberg, M., Holler, D., Horn, A., Jacholkowska, C., Jahn, M., Jamrozy, M., Janiak, F., Jankowsky, I., Jung, M. A., Kastendieck, K., Katarzynski, U., Katz, S., Kaufmann, B., Khelifi, M., Kieffer, S., Klepser, D., Klochkov, W., Kluzniak, T., Kneiske, D., Kolitzu, N., Komin, K., Kosack, S., Krakau, F., Krayzel, P. P., Krueger, H., Laffon, G., Lamanna, J., Lefaucheur, M., Lemoine Goumard, J. . ., P., D., Lennarz, T., Lohse, A., Lopatin, C. . ., C., V., Marandon, A., Marcowith, G., Maurin, N., Maxted, M., Mayer, T. J., L., M. C., Medina, J., Mehault, U., Menzler, M., Meyer, R., Moderski, M., Mohamed, E., Moulin, T., Murach, C. L., Naumann, M. d., Nauroi, D., Nedbal, J., Niemiec, S. J., Nolan, L., Oake, S., Ohm, E. d., Ona, B., Opitz, M., Ostrowski, I., Oya, M., Panter, R. D., Parson, M. P., Arriba, N. W., Pekeur, G., Pelletier, J., Perez, P. . ., O., B., Peyaud, S., Pita, H., Poon, G., Puehlhofer, M., Punch, A., Quirrenbach, S., Raab, M., Raue, A., Reimer, O., Reimer, M., Renaud, R. d., Lo, F., Rieger, L., Rob, S., Rosier Lee, G., Rowell, B., Rudak, C. B., Rulten, V., Sahakian, D. A., Sanchez, A., Santangelo, R., Schlickeiser, F., Schuessler, A., Schulz, U., Schwanke, S., Schwarzburg, S., Schwemmer, H., Sol, G., Spengler, F., Spie, L., Stawarz, R., Steenkamp, C., Stegmann, F., Stinzing, K., Stycz, I., Sushch, A., Szostek, R., Terrier, M., Tluczykont, C., Trichard, K., Valeriu, C. v., Eldik, G., Vasileiadi, C., Venter, A., Viana, P., Vincent, H. J., Voelk, F., Volpe, M., Vorster, S. J., Wagner, P., Wagner, M., Ward, M., Weidinger, R., White, A., Wierzcholska, P., Willmann, A., Woernlein, D., Wouter, M., Zacharia, A., Zajczyk, A. A., Zdziarski, A., Zech, H. . ., S., J. S., Perkin, R., Ojha, J., Steven, P. G., Edward, and M., Kadler
Subjects: [PHYS.ASTR.HE]Physics [physics]/Astrophysics [astro-ph]/High Energy Astrophysical Phenomena [astro-ph.HE], gamma-rays: galaxies, Radio galaxy, BL Lacertae objects: individual: 1ES 1312-423, Astrophysics::High Energy Astrophysical Phenomena, Centaurus A, galaxies: active, jets [galaxies], FOS: Physical sciences, Astrophysics, Astrophysics::Cosmology and Extragalactic Astrophysics, 7. Clean energy, 01 natural sciences, radiation mechanisms: non-thermal, galaxies: jets, 0103 physical sciences, High Energy Stereoscopic System, Blazar, 010303 astronomy & astrophysics, individual: 1ES 1312-423 [BL Lacertae objects], Astrophysics::Galaxy Astrophysics, Physics, High Energy Astrophysical Phenomena (astro-ph.HE), Spectral index, 010308 nuclear & particles physics, [SDU.ASTR.HE]Sciences of the Universe [physics]/Astrophysics [astro-ph]/High Energy Astrophysical Phenomena [astro-ph.HE], Astronomy, Institut für Physik und Astronomie, Astronomy and Astrophysics, non-thermal [radiation mechanisms], Crab Nebula, galaxies [gamma-rays], jet [galaxies], 13. Climate action, Space and Planetary Science, individual: 1ES 1312–423 [BL Lacertae objects], active [galaxies], ddc:520, Spectral energy distribution, High Energy Physics::Experiment, Astrophysics - High Energy Astrophysical Phenomena, Bl Lacertae objects: individual: 1ES 1312-423, Galaxies: active, Galaxies: jets, Gamma-rays: galaxies, Radiation mechanisms: non-thermal, Fermi Gamma-ray Space Telescope
Abstract: A deep observation campaign carried out by the High Energy Stereoscopic System (H.E.S.S.) on Centaurus A enabled the discovery of gamma rays from the blazar 1ES 1312-423, two degrees away from the radio galaxy. With a differential flux at 1 TeV of (1.9 +/-0.6(stat) +/-0.4(sys)) x 10^{-13} /cm^2 /s /TeV corresponding to 0.5% of the Crab nebula differential flux and a spectral index of 2.9 +/- 0.5 (stat) +/- 0.2 (sys), 1ES 1312-423 is one of the faintest sources ever detected in the very high energy (E>100 GeV) extragalactic sky. A careful analysis using three and a half years of Fermi-LAT data allows the discovery at high energies (E>100 MeV) of a hard spectrum (index of 1.4 +/- 0.4 (stat) +/- 0.2 (sys)) source coincident with 1ES 1312-423. Radio, optical, UV and X-ray observations complete the spectral energy distribution of this blazar, now covering 16 decades in energy. The emission is successfully fitted with a synchrotron self Compton model for the non-thermal component, combined with a black-body spectrum for the optical emission from the host galaxy., 12 pages, 10 figures, accepted in MNRAS
Published: 2013

99. Synchrotron Lightcurves of blazars in a time-dependent synchrotron-self Compton cooling scenario

Author: Michael Zacharias and Reinhard Schlickeiser
Subjects: Physics, High Energy Astrophysical Phenomena (astro-ph.HE), Astrophysics::High Energy Astrophysical Phenomena, Flux, FOS: Physical sciences, Astronomy and Astrophysics, Quasar, Astrophysics, Electron, Synchrotron, Radio spectrum, law.invention, Space and Planetary Science, law, Thermal radiation, Spectral energy distribution, Blazar, Astrophysics - High Energy Astrophysical Phenomena
Abstract: Blazars emit non-thermal radiation in all frequency bands from radio to \gamma-rays. Additionally, they often exhibit rapid flaring events at all frequencies with doubling time scale of the TeV and X-ray flux on the order of minutes, and such rapid flaring events are hard to explain theoretically. We explore the effect of the synchrotron-self Compton cooling, which is inherently time-dependent, leading to a rapid cooling of the electrons. Having discussed intensively the resulting effects of this cooling scenario on the spectral energy distribution of blazars in previous papers, the effects of the time-dependent approach on the synchrotron lightcurve are investigated here. Taking into account the retardation due to the finite size of the source and the source geometry, we show that the time-dependent synchrotron-self Compton (SSC) cooling still has profound effects on the lightcurve compared to the usual linear (synchrotron and external Compton) cooling terms. This is most obvious if the SSC cooling takes longer than the light crossing time scale. Then in most frequency bands the variability time scale is up to an order of magnitude shorter than under linear cooling conditions. This is yet another strong indication that the time-dependent approach should be taken into account for modeling blazar flares from compact emission regions., Comment: Accepted by The Astrophysical Journal, 11pages, 5 figures
Published: 2013
Full Text: View/download PDF

100. Evaluating the Role of Palliative Medicine in an Advanced Heart Failure Cohort at a Tertiary Care Center

Author: JaMia Washington, Guilherme H. Oliveira, Monique Robinson, Christine Koniaris, Sadeer G. Al-Kindi, Michael Zacharias, and Lauren Donnelly
Subjects: medicine.medical_specialty, business.industry, Heart failure, Emergency medicine, Cohort, medicine, Center (algebra and category theory), Cardiology and Cardiovascular Medicine, medicine.disease, business, Tertiary care
Published: 2016

Catalog

Books, media, physical & digital resources

See catalog results

Searchworks

Select search scope, currently: Articles Catalog books, media & more in Jio Institute collections Articles journal articles & other e-resources

Search

Search Constraints

Refine your results

Search Limiters

Topic

Publication Year Range

Language

Publication Type

Journal

Database

Publisher

120 results on '"Michael Zacharias"'

Search Results

Catalog

Select search scope, currently: Articles

Catalog

books, media & more in Jio Institute collections

Articles

journal articles & other e-resources