{"paper":{"title":"Spectral Energy Distribution of Markarian 501: Quiescent State vs. Extreme Outburst","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","headline":"","cross_cats":[],"primary_cat":"astro-ph.HE","authors_text":"A. Berdyugin, A. Biland, A. Boller, A. Cannon, A. Carosi, A. Cesarini, A. De Angelis, A. Diago Ortega, A. Dom\\'inguez, A. Falcone, A. Furniss, A. Herrero, A. Imran, A. Konopelko, A. La Barbera, A. McCann, A. Moralejo, A. N. Otte, A. Pichel, A. Saggion, A. Sierpowska-Bartosik, A. Sillanp\\\"a\\\"a, A. S Madhavan, A. Stamerra, A. Varlotta, A. Weinstein, B. De Lotto, B. Steinke, B. Zitzer, C. Delgado Mendez, C. Duke, C. M. Hui, C. Schultz, D. A. Williams, D. Bastieri, D. Boltuch, D. Borla Tridon, D. Bose, D. Dominis Prester, D. Dorner, D. Elsaesser, D. Ferenc, D. F. Torres, D. Gall, D. Hadasch, D. Hanna, D. Hildebrand, D. H\\\"ohne-M\\\"onch, D. Hrupec, D. Huang, D. Kieda, D. Kranich, D. Mazin, D. Nieto, D. Pandel, D. Paneque, D. Sobczynska, D. Steele, D. Tescaro, E. Bernardini, E. Carmona, E. Colombo, E. de Cea del Pozo, E. Leonardo, E. Lindfors, E. Lorenz, E. Prandini, E. Roache, F. Dazzi, F. De Sabata, F. Krennrich, F. Longo, F. Pauss, F. Prada, F. Spanier, F. Tavecchio, F. Zandanel, G. Bonnoli, G. Finnegan, G. Giavitto, G. Gyuk, G. H. Sembroski, G. Maier, G. Maneva, H. J. Rose, H. Krawczynski, H. Miyamoto, H. Vankov, I. Braun, I. Oya, I. Puljak, I. Reichardt, J. A. Barrio, J. Becerra Gonz\\'alez, J. Cortina, J. C. Struebig, J. E. Ward, J. Grube, J. H. Buckley, J. Holder, J. Hose, J. Krause, J. L. Contreras, J. M. Miranda, J. Mold\\'on, J. M. Paredes, J. P. Finley, J. Pochon, J. Quinn, J. Rico, J. Sitarek, J. S. Perkins, J. Storz, K. Berger, K. Mannheim, K. Nilsson, K. Ragan, K. Saito, K. Satalecka, L. A. Antonelli, L. Ciupik, L. C. Reyes, L. Font, L. Fortson, L. Maraschi, L. Peruzzo, L. Takalo, M. A. Perez-Torres, M. Backes, M. Beilicke, M. B\\\"ottcher, M. Camara, M. De Maria, M. Doert, M. Doro, M. Errando, M. Garczarczyk, M. Gaug, M. Hayashida, M. Kertzman, M. L\\'opez, M. Makariev, M. Mariotti, M. Mart\\'inez, M. Meucci, M. Pasanen, M. Persic, M. Pohl, M. Rib\\'o, M. Rissi, M. Salvati, M. S\\'anchez-Conde, M. Schroedter, M. Shayduk, M. Teshima, M. Theiling, M. V. Fonseca, M. Wood, N. Galante, N. Godinovi\\'c, N. Karlsson, N. Mankuzhiyil, N. Puchades, N. Strah, O. Blanch, P. Antoranz, P. Bordas, P. Colin, P. G. Prada Moroni, P. Kaaret, P. Majumdar, P. Moriarty, P. Temnikov, P. T. Reynolds, Q. Weitzel, R. A. Ong, R. Dickherber, R. G. Pegna, R. Guenette, R. J. Garc\\'ia L\\'opez, R. K. Bock, R. Mirzoyan, R. M. Wagner, R. Orito, R. Paoletti, R. Reinthal, R. Zanin, S. Covino, S. Godambe, S. Klepser, S. Lombardi, S. M. Bradbury, S. McArthur, S. N. Shore, S. Partini, S. P. Swordy, S. P. Wakely, S. R\\\"ugamer, S. Spiro, S. Thibadeau, S. Vincent, T. Arlen, T. Aune, T. B. Humensky, T. Bretz, T. C. Weekes, The MAGIC Collaboration: J. Aleksi\\'c, The VERITAS Collaboration: V. A. Acciari, T. Jogler, T. Kr\\\"ahenb\\\"uhl, T. Schweizer, T. Suric, T. Terzi\\'c, T. Weisgarber, T. Y. Saito, V. Bosch-Ramon, V. Bugaev, V. Scalzotto, V. Scapin, V. V. Vassiliev, V. Zabalza, W. Bednarek, W. Benbow, W. Cui, W. Rhode","submitted_at":"2010-12-10T08:13:28Z","abstract_excerpt":"The very high energy (VHE; E > 100 GeV) blazar Markarian 501 has a well-studied history of extreme spectral variability and is an excellent laboratory for studying the physical processes within the jets of active galactic nuclei. However, there are few detailed multiwavelength studies of Markarian 501 during its quiescent state, due to its low luminosity. A short-term multiwavelength study of Markarian 501 was coordinated in March 2009, focusing around a multi-day observation with the Suzaku X-ray satellite and including {\\gamma}-ray data from VERITAS, MAGIC, and the Fermi Gamma-ray Space Tele"},"claims":{"count":0,"items":[],"snapshot_sha256":"258153158e38e3291e3d48162225fcdb2d5a3ed65a07baac614ab91432fd4f57"},"source":{"id":"1012.2200","kind":"arxiv","version":1},"verdict":{"id":null,"model_set":{},"created_at":null,"strongest_claim":"","one_line_summary":"","pipeline_version":null,"weakest_assumption":"","pith_extraction_headline":""},"references":{"count":0,"sample":[],"resolved_work":0,"snapshot_sha256":"258153158e38e3291e3d48162225fcdb2d5a3ed65a07baac614ab91432fd4f57","internal_anchors":0},"formal_canon":{"evidence_count":0,"snapshot_sha256":"258153158e38e3291e3d48162225fcdb2d5a3ed65a07baac614ab91432fd4f57"},"author_claims":{"count":0,"strong_count":0,"snapshot_sha256":"258153158e38e3291e3d48162225fcdb2d5a3ed65a07baac614ab91432fd4f57"},"builder_version":"pith-number-builder-2026-05-17-v1"}