Very high-energy γ -ray observations of novae and dwarf novae with the MAGIC telescopes

被引：0

作者：

Ahnen, M.L. ^{[1
]}

Ansoldi, S. ^{[2
]}

Antonelli, L.A. ^{[3
]}

Antoranz, P. ^{[4
]}

Babic, A. ^{[5
]}

Banerjee, B. ^{[6
]}

Bangale, P. ^{[7
]}

Barres De Almeida, U. ^{[7
,26
]}

Barrio, J.A. ^{[8
]}

Becerra González, J. ^{[9
,27
,33
]}

Bednarek, W. ^{[10
]}

Bernardini, E. ^{[11
,28
]}

Biasuzzi, B. ^{[2
]}

Biland, A. ^{[1
]}

Blanch, O. ^{[12
]}

Bonnefoy, S. ^{[8
]}

Bonnoli, G. ^{[3
]}

Borracci, F. ^{[7
]}

Bretz, T. ^{[13
,29
]}

Carmona, E. ^{[14
]}

Carosi, A. ^{[3
]}

Chatterjee, A. ^{[6
]}

Clavero, R. ^{[33
]}

Colin, P. ^{[7
]}

Colombo, E. ^{[9
]}

Contreras, J.L. ^{[8
]}

Cortina, J. ^{[12
]}

Covino, S. ^{[3
]}

Da Vela, P. ^{[4
]}

Dazzi, F. ^{[7
]}

De Angelis, A. ^{[15
]}

De Caneva, G. ^{[11
]}

De Lotto, B. ^{[2
]}

De Oña Wilhelmi, E. ^{[16
]}

Delgado Mendez, C. ^{[14
]}

Di Pierro, F. ^{[3
]}

Dominis Prester, D. ^{[5
]}

Dorner, D. ^{[13
]}

Doro, M. ^{[15
]}

Einecke, S. ^{[17
]}

Eisenacher Glawion, D. ^{[13
]}

Elsaesser, D. ^{[13
]}

Fernández-Barral, A. ^{[12
]}

Fidalgo, D. ^{[8
]}

Fonseca, M.V. ^{[8
]}

Font, L. ^{[18
]}

Frantzen, K. ^{[17
]}

Fruck, C. ^{[7
]}

Galindo, D. ^{[19
]}

García López, R.J. ^{[9
]}

机构：

[1] ETH Zurich, Zurich,8093, Switzerland

[2] Università di Udine and INFN Trieste, Udine,33100, Italy

[3] INAF National Institute for Astrophysics, Rome,00136, Italy

[4] Università di Siena and INFN Pisa, Siena,53100, Italy

[5] Croatian MAGIC Consortium, Rudjer Boskovic Institute, University of Rijeka and University of Split, Zagreb,10000, Croatia

[6] Saha Institute of Nuclear Physics, 1AF Bidhannagar, Sector-1, Salt Lake, Kolkata,700064, India

[7] Max-Planck-Institut für Physik, München,80805, Germany

[8] Universidad Complutense, Madrid,28040, Spain

[9] Inst. de Astrofísica de Canarias, La Laguna, Tenerife,38200, Spain

[10] University of Lódź, Lodz,90236, Poland

[11] Deutsches Elektronen-Synchrotron (DESY), Zeuthen,15738, Germany

[12] IFAE, Campus UAB, Bellaterra,08193, Spain

[13] Universität Würzburg, Würzburg,97074, Germany

[14] Centro de Investigaciones Energéticas, Medioambientales y Tecnológicas, Madrid,28040, Spain

[15] Università di Padova and INFN, Padova,35131, Italy

[16] Institute of Space Sciences, Barcelona,08193, Spain

[17] Technische Universität Dortmund, Dortmund,44221, Germany

[18] Unitat de Física de les Radiacions, Departament de Física, CERES-IEEC, Universitat Autònoma de Barcelona, Bellaterra,08193, Spain

[19] Universitat de Barcelona, ICC, IEEC-UB, Barcelona,08028, Spain

[20] Japanese MAGIC Consortium, ICRR, University of Tokyo, Department of Physics and Hakubi Center, Kyoto University, Tokai University, University of Tokushima, KEK, Tokushima,770-0855, Japan

[21] Finnish MAGIC Consortium, Tuorla Observatory, University of Turku and Department of Physics, University of Oulu, Oulu,90014, Finland

[22] Inst. for Nucl. Research and Nucl. Energy, Sofia,1784, Bulgaria

[23] Università di Pisa, INFN Pisa, Pisa,56126, Italy

[24] ICREA and Institute of Space Sciences, Barcelona,08193, Spain

[25] Università dell'Insubria and INFN Milano Bicocca, Como, Como,22100, Italy

[26] Centro Brasileiro de Pesquisas Físicas (CBPFMCTI), R. Dr. Xavier Sigaud, 150 - Urca, Rio de Janeiro - RJ,22290-180, Brazil

[27] NASA Goddard Space Flight Center, Greenbelt,MD,20771, United States

[28] Humboldt University of Berlin, Institut für Physik Newtonstr. 15, Berlin,12489, Germany

[29] École Polytechnique Fédérale de Lausanne (EPFL), Lausanne, Switzerland

[30] Finnish Centre for Astronomy with ESO (FINCA), Turku, Finland

[31] INAF, Trieste, Italy

[32] ISDC - Science Data Center for Astrophysics, Versoix (Geneva),1290, Switzerland

[33] Department of Physics and Department of Astronomy, University of Maryland, College Park,MD,20742, United States

来源：

Astronomy and Astrophysics | 2015年 / 582卷

关键词：

The MAGIC Collaboration would like to thank the Instituto de Astrofísica de Canarias for the excellent working conditions at the Observatorio del Roque de los Muchachos in La Palma. The financial support of the German BMBF and MPG; the Italian INFN and INAF; the Swiss National Fund SNF; the ERDF under the Spanish MINECO; and the Japanese [!text type='JS']JS[!/text]PS and MEXT is gratefully acknowledged. This work was also supported by the Centro de Excelencia Severo Ochoa SEV-2012-0234; CPAN CSD2007-00042; and MultiDark CSD2009-00064 projects of the Spanish Consolider-Ingenio 2010 programme; by grant 268740 of the Academy of Finland; by the Croatian Science Foundation (HrZZ) Project 09/176 and the University of Rijeka Project 13.12.1.3.02; by the DFG Collaborative Research Centers SFB823/C4 and SFB876/C3; and by the Polish MNiSzW grant 745/N-HESS-MAGIC/2010/0 and NCN 2011/01/B/ST9/00411. J.S. is supported by Fundacja UL. We thank M.A. Pérez-Torres for the information about nova ASASSN-13ax. The Fermi-LAT Collaboration acknowledges generous ongoing support from a number of agencies and institutes that have supported both the development and the operation of the LAT as well as scientific data analysis. These include the National Aeronautics and Space Administration and the Department of Energy in the United States; the Commissariat à l’Énergie Atomique and the Centre National de la Recherche Scientifique/Institut National de Physique Nucléaire et de Physique des Particules in France; the Agenzia Spaziale Italiana and the Istituto Nazionale di Fisica Nucleare in Italy; the Ministry of Education; Culture; Sports; Science and Technology (MEXT); High Energy Accelerator Research Organization (KEK) and Japan Aerospace Exploration Agency (JAXA) in Japan; and the K. A. Wallenberg Foundation; the Swedish Research Council and the Swedish National Space Board in Sweden. Additional support for science analysis during the operations phase is gratefully acknowledged from the Istituto Nazionale di Astrofisica in Italy and the Centre National d’Études Spatiales in France. Authors would like to thank S. N. Shore for scientific discussions and providing an optical spectrum of V339 Del and UV spectrum of OS And. We would also like to thank the anonymous referee for comments that helped to improve the paper;

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