التفاصيل البيبلوغرافية
العنوان:
Multiwavelength observations of Mrk 501 in 2008
المؤلفون:
MAGIC Collaboration , J. Aleksić(IFAE, Edifici Cn., Campus UAB, E-08193 Bellaterra, Spain) , S. Ansoldi(Università di Udine, and INFN Trieste, I-33100 Udine, Italy) , L. A. Antonelli(INAF National Institute for Astrophysics, I-00136 Rome, Italy) , P. Antoranz(Università di Siena, and INFN Pisa, I-53100 Siena, Italy) , A. Babic(Croatian MAGIC Consortium, Rudjer Boskovic Institute, University of Rijeka and University of Split, HR-10000 Zagreb, Croatia) , P. Bangale(Max-Planck-Institut für Physik, D-80805 München, Germany) , U. Barres de Almeida(Max-Planck-Institut für Physik, D-80805 München, Germany) , J. A. Barrio(Universidad Complutense, E-28040 Madrid, Spain) , J. Becerra González(Inst. de Astrofísica de Canarias, E-38200 La Laguna, Tenerife, Spain) , W. Bednarek(University of Lodz, PL-90236 Lodz, Poland) , K. Berger(Inst. de Astrofísica de Canarias, E-38200 La Laguna, Tenerife, Spain) , E. Bernardini(Deutsches Elektronen-Synchrotron) , A. Biland(ETH Zurich, CH-8093 Zurich, Switzerland) , O. Blanch(IFAE, Edifici Cn., Campus UAB, E-08193 Bellaterra, Spain) , R. K. Bock(Max-Planck-Institut für Physik, D-80805 München, Germany) , S. Bonnefoy(Universidad Complutense, E-28040 Madrid, Spain) , G. Bonnoli(INAF National Institute for Astrophysics, I-00136 Rome, Italy) , F. Borracci(Max-Planck-Institut für Physik, D-80805 München, Germany) , T. Bretz(Universität Würzburg, D-97074 Würzburg, Germany) , E. Carmona(Centro de Investigaciones Energéticas, Medioambientales y Tecnológicas, E-28040 Madrid, Spain) , A. Carosi(INAF National Institute for Astrophysics, I-00136 Rome, Italy) , D. Carreto Fidalgo(Universität Würzburg, D-97074 Würzburg, Germany) , P. Colin(Max-Planck-Institut für Physik, D-80805 München, Germany) , E. Colombo(Inst. de Astrofísica de Canarias, E-38200 La Laguna, Tenerife, Spain) , J. L. Contreras(Universidad Complutense, E-28040 Madrid, Spain) , J. Cortina(IFAE, Edifici Cn., Campus UAB, E-08193 Bellaterra, Spain) , S. Covino(INAF National Institute for Astrophysics, I-00136 Rome, Italy) , P. Da Vela(Università di Siena, and INFN Pisa, I-53100 Siena, Italy) , F. Dazzi(Università di Udine, and INFN Trieste, I-33100 Udine, Italy) , A. De Angelis(Università di Udine, and INFN Trieste, I-33100 Udine, Italy) , G. De Caneva(Deutsches Elektronen-Synchrotron) , B. De Lotto(Università di Udine, and INFN Trieste, I-33100 Udine, Italy) , C. Delgado Mendez(Centro de Investigaciones Energéticas, Medioambientales y Tecnológicas, E-28040 Madrid, Spain) , M. Doert(Technische Universität Dortmund, D-44221 Dortmund, Germany) , A. Domínguez(Inst. de Astrofísica de Andalucía) , D. Dominis Prester(Croatian MAGIC Consortium, Rudjer Boskovic Institute, University of Rijeka and University of Split, HR-10000 Zagreb, Croatia) , D. Dorner(Universität Würzburg, D-97074 Würzburg, Germany) , M. Doro(Università di Padova and INFN, I-35131 Padova, Italy) , S. Einecke(Technische Universität Dortmund, D-44221 Dortmund, Germany) , D. Eisenacher(Universität Würzburg, D-97074 Würzburg, Germany) , D. Elsaesser(Universität Würzburg, D-97074 Würzburg, Germany) , E. Farina(Università dell'Insubria, Como, I-22100 Como, Italy) , D. Ferenc(Croatian MAGIC Consortium, Rudjer Boskovic Institute, University of Rijeka and University of Split, HR-10000 Zagreb, Croatia) , M. V. Fonseca(Universidad Complutense, E-28040 Madrid, Spain) , L. Font(Unitat de Física de les Radiacions, Departament de Física, and CERES-IEEC, Universitat Autònoma de Barcelona, E-08193 Bellaterra, Spain) , K. Frantzen(Technische Universität Dortmund, D-44221 Dortmund, Germany) , C. Fruck(Max-Planck-Institut für Physik, D-80805 München, Germany) , R. J. García López(Inst. de Astrofísica de Canarias, E-38200 La Laguna, Tenerife, Spain) , M. Garczarczyk(Deutsches Elektronen-Synchrotron) , D. Garrido Terrats(Unitat de Física de les Radiacions, Departament de Física, and CERES-IEEC, Universitat Autònoma de Barcelona, E-08193 Bellaterra, Spain) , M. Gaug(Unitat de Física de les Radiacions, Departament de Física, and CERES-IEEC, Universitat Autònoma de Barcelona, E-08193 Bellaterra, Spain) , G. Giavitto(IFAE, Edifici Cn., Campus UAB, E-08193 Bellaterra, Spain) , N. Godinović(Croatian MAGIC Consortium, Rudjer Boskovic Institute, University of Rijeka and University of Split, HR-10000 Zagreb, Croatia) , A. González Muñoz(IFAE, Edifici Cn., Campus UAB, E-08193 Bellaterra, Spain) , S. R. Gozzini(Deutsches Elektronen-Synchrotron) , A. Hadamek(Technische Universität Dortmund, D-44221 Dortmund, Germany) , D. Hadasch(Institut de Ciències de l'Espai) , A. Herrero(Inst. de Astrofísica de Canarias, E-38200 La Laguna, Tenerife, Spain) , D. Hildebrand(ETH Zurich, CH-8093 Zurich, Switzerland) , J. Hose(Max-Planck-Institut für Physik, D-80805 München, Germany) , D. Hrupec(Croatian MAGIC Consortium, Rudjer Boskovic Institute, University of Rijeka and University of Split, HR-10000 Zagreb, Croatia) , W. Idec(University of Lodz, PL-90236 Lodz, Poland) , V. Kadenius(Finnish MAGIC Consortium, Tuorla Observatory, University of Turku and Department of Physics, University of Oulu, Finland) , H. Kellermann(Max-Planck-Institut für Physik, D-80805 München, Germany) , M. L. Knoetig(ETH Zurich, CH-8093 Zurich, Switzerland) , J. Krause(Max-Planck-Institut für Physik, D-80805 München, Germany) , J. Kushida(Japanese MAGIC Consortium, Division of Physics and Astronomy, Kyoto University, Japan) , A. La Barbera(INAF National Institute for Astrophysics, I-00136 Rome, Italy) , D. Lelas(Croatian MAGIC Consortium, Rudjer Boskovic Institute, University of Rijeka and University of Split, HR-10000 Zagreb, Croatia) , N. Lewandowska(Universität Würzburg, D-97074 Würzburg, Germany) , E. Lindfors(Finnish MAGIC Consortium, Tuorla Observatory, University of Turku and Department of Physics, University of Oulu, Finland) , S. Lombardi(INAF National Institute for Astrophysics, I-00136 Rome, Italy) , M. López(Universidad Complutense, E-28040 Madrid, Spain) , R. López-Coto(IFAE, Edifici Cn., Campus UAB, E-08193 Bellaterra, Spain) , A. López-Oramas(IFAE, Edifici Cn., Campus UAB, E-08193 Bellaterra, Spain) , E. Lorenz(Max-Planck-Institut für Physik, D-80805 München, Germany) , I. Lozano(Universidad Complutense, E-28040 Madrid, Spain) , M. Makariev(Inst. for Nucl. Research and Nucl. Energy, BG-1784 Sofia, Bulgaria) , K. Mallot(Deutsches Elektronen-Synchrotron) , G. Maneva(Inst. for Nucl. Research and Nucl. Energy, BG-1784 Sofia, Bulgaria) , N. Mankuzhiyil(2,*) , K. Mannheim(Universität Würzburg, D-97074 Würzburg, Germany) , L. Maraschi(INAF National Institute for Astrophysics, I-00136 Rome, Italy) , B. Marcote(Universitat de Barcelona) , M. Mariotti(Università di Padova and INFN, I-35131 Padova, Italy) , M. Martínez(IFAE, Edifici Cn., Campus UAB, E-08193 Bellaterra, Spain) , D. Mazin(Max-Planck-Institut für Physik, D-80805 München, Germany) , U. Menzel(Max-Planck-Institut für Physik, D-80805 München, Germany) , M. Meucci(Università di Siena, and INFN Pisa, I-53100 Siena, Italy) , J. M. Miranda(Università di Siena, and INFN Pisa, I-53100 Siena, Italy) , R. Mirzoyan(Max-Planck-Institut für Physik, D-80805 München, Germany) , A. Moralejo(IFAE, Edifici Cn., Campus UAB, E-08193 Bellaterra, Spain) , P. Munar-Adrover(Universitat de Barcelona) , D. Nakajima(Japanese MAGIC Consortium, Division of Physics and Astronomy, Kyoto University, Japan) , A. Niedzwiecki(University of Lodz, PL-90236 Lodz, Poland) , K. Nilsson(Finnish MAGIC Consortium, Tuorla Observatory, University of Turku and Department of Physics, University of Oulu, Finland) , N. Nowak(Max-Planck-Institut für Physik, D-80805 München, Germany) , R. Orito(Japanese MAGIC Consortium, Division of Physics and Astronomy, Kyoto University, Japan) , A. Overkemping(Technische Universität Dortmund, D-44221 Dortmund, Germany) , S. Paiano(Università di Padova and INFN, I-35131 Padova, Italy) , M. Palatiello(Università di Udine, and INFN Trieste, I-33100 Udine, Italy) , D. Paneque(6,*) , R. Paoletti(Università di Siena, and INFN Pisa, I-53100 Siena, Italy) , J. M. Paredes(Universitat de Barcelona) , X. Paredes-Fortuny(Universitat de Barcelona) , S. Partini(Università di Siena, and INFN Pisa, I-53100 Siena, Italy) , M. Persic(Università di Udine, and INFN Trieste, I-33100 Udine, Italy) , F. Prada(Inst. de Astrofísica de Andalucía) , P. G. Prada Moroni(Università di Pisa, and INFN Pisa, I-56126 Pisa, Italy) , E. Prandini(Università di Padova and INFN, I-35131 Padova, Italy) , S. Preziuso(Università di Siena, and INFN Pisa, I-53100 Siena, Italy) , I. Puljak(Croatian MAGIC Consortium, Rudjer Boskovic Institute, University of Rijeka and University of Split, HR-10000 Zagreb, Croatia) , R. Reinthal(Finnish MAGIC Consortium, Tuorla Observatory, University of Turku and Department of Physics, University of Oulu, Finland) , W. Rhode(Technische Universität Dortmund, D-44221 Dortmund, Germany) , M. Ribó(Universitat de Barcelona) , J. Rico(IFAE, Edifici Cn., Campus UAB, E-08193 Bellaterra, Spain) , J. Rodriguez Garcia(Max-Planck-Institut für Physik, D-80805 München, Germany) , S. Rügamer(Universität Würzburg, D-97074 Würzburg, Germany) , A. Saggion(Università di Padova and INFN, I-35131 Padova, Italy) , T. Saito(Japanese MAGIC Consortium, Division of Physics and Astronomy, Kyoto University, Japan) , K. Saito(Japanese MAGIC Consortium, Division of Physics and Astronomy, Kyoto University, Japan) , M. Salvati(INAF National Institute for Astrophysics, I-00136 Rome, Italy) , K. Satalecka(7,*) , V. Scalzotto(Università di Padova and INFN, I-35131 Padova, Italy) , V. Scapin(Universidad Complutense, E-28040 Madrid, Spain) , C. Schultz(Università di Padova and INFN, I-35131 Padova, Italy) , T. Schweizer(Max-Planck-Institut für Physik, D-80805 München, Germany) , S. N. Shore(Università di Pisa, and INFN Pisa, I-56126 Pisa, Italy) , A. Sillanpää(Finnish MAGIC Consortium, Tuorla Observatory, University of Turku and Department of Physics, University of Oulu, Finland) , J. Sitarek(IFAE, Edifici Cn., Campus UAB, E-08193 Bellaterra, Spain) , I. Snidaric(Croatian MAGIC Consortium, Rudjer Boskovic Institute, University of Rijeka and University of Split, HR-10000 Zagreb, Croatia) , D. Sobczynska(University of Lodz, PL-90236 Lodz, Poland) , F. Spanier(Universität Würzburg, D-97074 Würzburg, Germany) , V. Stamatescu(IFAE, Edifici Cn., Campus UAB, E-08193 Bellaterra, Spain) , A. Stamerra(INAF National Institute for Astrophysics, I-00136 Rome, Italy) , T. Steinbring(Universität Würzburg, D-97074 Würzburg, Germany) , J. Storz(Universität Würzburg, D-97074 Würzburg, Germany) , S. Sun(Max-Planck-Institut für Physik, D-80805 München, Germany) , T. Surić(Croatian MAGIC Consortium, Rudjer Boskovic Institute, University of Rijeka and University of Split, HR-10000 Zagreb, Croatia) , L. Takalo(Finnish MAGIC Consortium, Tuorla Observatory, University of Turku and Department of Physics, University of Oulu, Finland) , F. Tavecchio(INAF National Institute for Astrophysics, I-00136 Rome, Italy) , P. Temnikov(Inst. for Nucl. Research and Nucl. Energy, BG-1784 Sofia, Bulgaria) , T. Terzić(Croatian MAGIC Consortium, Rudjer Boskovic Institute, University of Rijeka and University of Split, HR-10000 Zagreb, Croatia) , D. Tescaro(Inst. de Astrofísica de Canarias, E-38200 La Laguna, Tenerife, Spain) , M. Teshima(Max-Planck-Institut für Physik, D-80805 München, Germany) , J. Thaele(Technische Universität Dortmund, D-44221 Dortmund, Germany) , O. Tibolla(Universität Würzburg, D-97074 Würzburg, Germany) , D. F. Torres(Institut de Ciències de l'Espai) , T. Toyama(Max-Planck-Institut für Physik, D-80805 München, Germany) , A. Treves(Università dell'Insubria, Como, I-22100 Como, Italy) , M. Uellenbeck(Technische Universität Dortmund, D-44221 Dortmund, Germany) , P. Vogler(ETH Zurich, CH-8093 Zurich, Switzerland) , R. M. Wagner(Max-Planck-Institut für Physik, D-80805 München, Germany) , F. Zandanel(Inst. de Astrofísica de Andalucía) , R. Zanin(Universitat de Barcelona) , VERITAS Collaboration(Deutsches Elektronen-Synchrotron) , (Deutsches Elektronen-Synchrotron) , B. Behera(Deutsches Elektronen-Synchrotron) , M. Beilicke(Department of Physics, Washington University, St. Louis, MO 63130, USA) , W. Benbow(Fred Lawrence Whipple Observatory, Harvard-Smithsonian Center for Astrophysics, Amado, AZ 85645, USA) , R. Bird(School of Physics, University College Dublin, Belfield, Dublin 4, Ireland) , A. Bouvier(Santa Cruz Institute for Particle Physics and Department of Physics, University of California, Santa Cruz, CA 95064, USA) , V. Bugaev(Department of Physics, Washington University, St. Louis, MO 63130, USA) , M. Cerruti(Fred Lawrence Whipple Observatory, Harvard-Smithsonian Center for Astrophysics, Amado, AZ 85645, USA) , X. Chen(Institute of Physics and Astronomy, University of Potsdam, 14476 Potsdam-Golm, Germany) , L. Ciupik(Astronomy Department, Adler Planetarium and Astronomy Museum, Chicago, IL 60605, USA) , E. Collins-Hughes(School of Physics, University College Dublin, Belfield, Dublin 4, Ireland) , W. Cui(Department of Physics, Purdue University, West Lafayette, IN 47907, USA) , C. Duke(Department of Physics, Grinnell College, Grinnell, IA 50112-1690, USA) , J. Dumm(School of Physics and Astronomy, University of Minnesota, Minneapolis, MN 55455, USA) , A. Falcone(Department of Astronomy and Astrophysics, 525 Davey Lab, Pennsylvania State University, University Park, PA 16802, USA) , S. Federici(now at GRAPPA Institute, University of Amsterdam, 1098XH) , Q. Feng(Department of Physics, Purdue University, West Lafayette, IN 47907, USA) , J. P. Finley(Department of Physics, Purdue University, West Lafayette, IN 47907, USA) , L. Fortson(School of Physics and Astronomy, University of Minnesota, Minneapolis, MN 55455, USA) , A. Furniss(Santa Cruz Institute for Particle Physics and Department of Physics, University of California, Santa Cruz, CA 95064, USA) , N. Galante(Fred Lawrence Whipple Observatory, Harvard-Smithsonian Center for Astrophysics, Amado, AZ 85645, USA) , G. H. Gillanders(School of Physics, National University of Ireland Galway, University Road, Galway, Ireland) , S. Griffin(Physics Department, McGill University, Montreal, QC H3A 2T8, Canada) , S. T. Griffiths(Department of Physics and Astronomy, University of Iowa, Van Allen Hall, Iowa City, IA 52242, USA) , J. Grube(Astronomy Department, Adler Planetarium and Astronomy Museum, Chicago, IL 60605, USA) , G. Gyuk(Astronomy Department, Adler Planetarium and Astronomy Museum, Chicago, IL 60605, USA) , D. Hanna(Physics Department, McGill University, Montreal, QC H3A 2T8, Canada) , J. Holder(Department of Physics and Astronomy and the Bartol Research Institute, University of Delaware, Newark, DE 19716, USA) , C. A. Johnson(Santa Cruz Institute for Particle Physics and Department of Physics, University of California, Santa Cruz, CA 95064, USA) , P. Kaaret(Department of Physics and Astronomy, University of Iowa, Van Allen Hall, Iowa City, IA 52242, USA) , M. Kertzman(Department of Physics and Astronomy, DePauw University, Greencastle, IN 46135-0037, USA) , D. Kieda(Department of Physics and Astronomy, University of Utah, Salt Lake City, UT 84112, USA) , H. Krawczynski(Department of Physics, Washington University, St. Louis, MO 63130, USA) , M. J. Lang(School of Physics, National University of Ireland Galway, University Road, Galway, Ireland) , A. S Madhavan(Department of Physics and Astronomy, Iowa State University, Ames, IA 50011, USA) , G. Maier(Deutsches Elektronen-Synchrotron) , P. Majumdar(Department of Physics and Astronomy, University of California, Los Angeles, CA 90095, USA) , K. Meagher(School of Physics and Center for Relativistic Astrophysics, Georgia Institute of Technology, 837 State Street NW, Atlanta, GA 30332-0430) , P. Moriarty(Department of Life and Physical Sciences, Galway-Mayo Institute of Technology, Dublin Road, Galway, Ireland) , R. Mukherjee(Department of Physics and Astronomy, Barnard College, Columbia University, NY 10027, USA) , D. Nieto(Physics Department, Columbia University, New York, NY 10027, USA) , A. O'Faoláin de Bhróithe(School of Physics, University College Dublin, Belfield, Dublin 4, Ireland) , R. A. Ong(Department of Physics and Astronomy, University of California, Los Angeles, CA 90095, USA) , A. N. Otte(School of Physics and Center for Relativistic Astrophysics, Georgia Institute of Technology, 837 State Street NW, Atlanta, GA 30332-0430) , A. Pichel(Instituto de Astronomia y Fisica del Espacio, Casilla de Correo 67 - Sucursal 28) , M. Pohl(Institute of Physics and Astronomy, University of Potsdam, 14476 Potsdam-Golm, Germany) , A. Popkow(Department of Physics and Astronomy, University of California, Los Angeles, CA 90095, USA) , H. Prokoph(Deutsches Elektronen-Synchrotron) , J. Quinn(School of Physics, University College Dublin, Belfield, Dublin 4, Ireland) , J. Rajotte(Physics Department, McGill University, Montreal, QC H3A 2T8, Canada) , G. Ratliff(Astronomy Department, Adler Planetarium and Astronomy Museum, Chicago, IL 60605, USA) , L. C. Reyes(Physics Department, California Polytechnic State University, San Luis Obispo, CA 94307, USA) , P. T. Reynolds(Department of Applied Physics and Instrumentation, Cork Institute of Technology, Bishopstown, Cork, Ireland) , G. T. Richards(School of Physics and Center for Relativistic Astrophysics, Georgia Institute of Technology, 837 State Street NW, Atlanta, GA 30332-0430) , E. Roache(Fred Lawrence Whipple Observatory, Harvard-Smithsonian Center for Astrophysics, Amado, AZ 85645, USA) , G. H. Sembroski(Department of Physics, Purdue University, West Lafayette, IN 47907, USA) , K. Shahinyan(School of Physics and Astronomy, University of Minnesota, Minneapolis, MN 55455, USA) , F. Sheidaei(Department of Physics and Astronomy, University of Utah, Salt Lake City, UT 84112, USA) , A. W. Smith(Department of Physics and Astronomy, University of Utah, Salt Lake City, UT 84112, USA) , D. Staszak(Physics Department, McGill University, Montreal, QC H3A 2T8, Canada) , I. Telezhinsky(Institute of Physics and Astronomy, University of Potsdam, 14476 Potsdam-Golm, Germany) , M. Theiling(Department of Physics, Purdue University, West Lafayette, IN 47907, USA) , J. Tyler(Physics Department, McGill University, Montreal, QC H3A 2T8, Canada) , A. Varlotta(Department of Physics, Purdue University, West Lafayette, IN 47907, USA) , S. Vincent(Deutsches Elektronen-Synchrotron) , S. P. Wakely(Enrico Fermi Institute, University of Chicago, Chicago, IL 60637, USA) , T. C. Weekes(Fred Lawrence Whipple Observatory, Harvard-Smithsonian Center for Astrophysics, Amado, AZ 85645, USA) , R. Welsing(Deutsches Elektronen-Synchrotron) , D. A. Williams(Santa Cruz Institute for Particle Physics and Department of Physics, University of California, Santa Cruz, CA 95064, USA) , A. Zajczyk(Department of Physics, Washington University, St. Louis, MO 63130, USA) , B. Zitzer(Argonne National Laboratory, 9700 S. Cass Avenue, Argonne, IL 60439, USA) , External Collaborators(INAF, Osservatorio Astronomico di Torino, I-10025 Pino Torinese) , (INAF, Osservatorio Astronomico di Torino, I-10025 Pino Torinese) , M. Villata(INAF, Osservatorio Astronomico di Torino, I-10025 Pino Torinese) , C. M. Raiteri(INAF, Osservatorio Astronomico di Torino, I-10025 Pino Torinese) , M. Ajello(Space Sciences Laboratory, 7 Gauss Way, University of California, Berkeley, CA 94720-7450, USA) , M. Perri(ASI-Science Data Center, Via del Politecnico, I-00133 Rome, Italy) , H. D. Aller(Department of Astronomy, University of Michigan, Ann Arbor, MI 48109-1042, USA) , M. F. Aller(Department of Astronomy, University of Michigan, Ann Arbor, MI 48109-1042, USA) , V. M. Larionov(Astron. Inst., St.-Petersburg State Univ., Russia) , N. V. Efimova(Astron. Inst., St.-Petersburg State Univ., Russia) , T. S. Konstantinova(Astron. Inst., St.-Petersburg State Univ., Russia) , E. N. Kopatskaya(Astron. Inst., St.-Petersburg State Univ., Russia) , W. P. Chen(Graduate Institute of Astronomy, National Central University, 300 Jhongda Rd., Jhongli 32001, Taiwan) , E. Koptelova(Graduate Institute of Astronomy, National Central University, 300 Jhongda Rd., Jhongli 32001, Taiwan) , H. Y. Hsiao(Graduate Institute of Astronomy, National Central University, 300 Jhongda Rd., Jhongli 32001, Taiwan) , O. M. Kurtanidze(Abastumani Observatory, Mt. Kanobili, 0301 Abastumani, Georgia) , M. G. Nikolashvili(Abastumani Observatory, Mt. Kanobili, 0301 Abastumani, Georgia) , G. N. Kimeridze(Abastumani Observatory, Mt. Kanobili, 0301 Abastumani, Georgia) , B. Jordan(School of Cosmic Physics, Dublin Institute For Advanced Studies, Ireland) , P. Leto(INAF - Osservatorio Astrofisico di Catania, Italy) , C. S. Buemi(INAF - Osservatorio Astrofisico di Catania, Italy) , C. Trigilio(INAF - Osservatorio Astrofisico di Catania, Italy) , G. Umana(INAF - Osservatorio Astrofisico di Catania, Italy) , A. Lahtenmaki(Aalto University Metsähovi Radio Observatory Metsähovintie 114 FIN-02540 Kylmälä Finland) , E. Nieppola(Aalto University Metsähovi Radio Observatory Metsähovintie 114 FIN-02540 Kylmälä Finland) , M. Tornikoski(Aalto University Metsähovi Radio Observatory Metsähovintie 114 FIN-02540 Kylmälä Finland) , J. Sainio(Finnish MAGIC Consortium, Tuorla Observatory, University of Turku and Department of Physics, University of Oulu, Finland) , M. Giroletti(INAF Istituto di Radioastronomia, 40129 Bologna, Italy) , A. Cesarini(University of Trento, Department of Physics, I38050 Povo, Trento, Italy) , L. Fuhrmann(Max-Planck-Institut für Radioastronomie, Auf dem Hügel 69, 53121 Bonn, Germany) , Yu. A. Kovalev(Astro Space Center of the Lebedev Physical Institute, 117997) , Y. Y. Kovalev(Max-Planck-Institut für Radioastronomie, Auf dem Hügel 69, 53121 Bonn, Germany)
المساهمون:
Anne Lähteenmäki Group, Department of Radio Science and Engineering, Aalto-yliopisto, Aalto University, Universitat de Barcelona, School services, ELEC, ~
المصدر:
E-Prints Complutense: Archivo Institucional de la UCM
بيانات النشر:
Edp Sciences, 2015.
سنة النشر:
2015
مصطلحات موضوعية:
extragalactic background light , Ciencias Físicas , Flux , Electron , Astrophysics , 7. Clean energy , law.invention , purl.org/becyt/ford/1 [https] , Raigs gamma , bl lacertae objects , law , individual: Mrk 501 [BL Lacertae objects] , Physics , High Energy Astrophysical Phenomena (astro-ph.HE) , astro-ph.HE , 213 Electronic, automation and communications engineering, electronics , Astroparticle physics , BL Lacertae objects: individual: Mrk 501 , Gamma rays: general , Astronomy and Astrophysics , Space and Planetary Science , Synchrotron , individual: Mrk 50 [BL Lacertae objects] , Homogeneous , astroparticle physics , Spectral energy distribution , Electrónica , Física nuclear , Electricidad , Astrophysics - High Energy Astrophysical Phenomena , CIENCIAS NATURALES Y EXACTAS , 1171 Geosciences , Astrophysics::High Energy Astrophysical Phenomena , emitting electrons , FOS: Physical sciences , Astrophysics::Cosmology and Extragalactic Astrophysics , 114 Physical sciences , bl lacertae objects: individual: mrk 501 , crab-nebula , Blazar , Astrophysics::Galaxy Astrophysics , tev blazars , variability , 221 Nanotechnology , Gamma rays , Individual: Mrk 501 , Institut für Physik und Astronomie , purl.org/becyt/ford/1.3 [https] , gamma rays: general , Galaxies , gamma-ray emission , telescope system , Galàxies , Active Galaxies , blazars , gamma-rays , Mrk 501 , Astronomía , Crab Nebula , x-ray , 115 Astronomy and space science , Low emission , 216 Materials engineering , Galàxies actives , active galactic nuclei , Active galaxies , ddc:520 , general [gamma rays]
الوصف:
Mrk 501 is one of the brightest blazars at TeV energies and has been extensively studied since its first VHE detection in 1996. Our goal is to characterize in detail the source gamma-ray emission, together with the radio-to-X-ray emission, during the non-flaring (low) activity, which is less often studied than the occasional flaring (high) activity. We organized a multiwavelength (MW) campaign on Mrk 501 between March and May 2008. This multi-instrument effort included the most sensitive VHE gamma-ray instruments in the northern hemisphere, namely the imaging atmospheric Cherenkov telescopes MAGIC and VERITAS, as well as Swift, RXTE, the F-GAMMA, GASP-WEBT, and other collaborations and instruments. Mrk 501 was found to be in a low state of activity during the campaign, with a VHE flux in the range of 10%-20% of the Crab nebula flux. Nevertheless, significant flux variations were detected with various instruments, with a trend of increasing variability with energy. The broadband spectral energy distribution during the two different emission states of the campaign can be adequately described within the homogeneous one-zone synchrotron self-Compton model, with the (slightly) higher state described by an increase in the electron number density. This agrees with previous studies of the broadband emission of this source during flaring and non-flaring states. We report for the first time a tentative X-ray-to-VHE correlation during a low VHE activity. Although marginally significant, this positive correlation between X-ray and VHE, which has been reported many times during flaring activity, suggests that the mechanisms that dominate the X-ray/VHE emission during non-flaring-activity are not substantially different from those that are responsible for the emission during flaring activity.
وصف الملف:
application/pdf
اللغة:
English
الوصول الحر:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::32e69b9aa5312790ae4b8fdfb73c70d8Test https://www.aanda.org/articles/aa/abs/2015/01/aa22906-13/aa22906-13.htmlTest
حقوق:
OPEN
رقم الانضمام:
edsair.doi.dedup.....32e69b9aa5312790ae4b8fdfb73c70d8
قاعدة البيانات:
OpenAIRE
