{"paper":{"title":"Insights into the emission of the blazar 1ES 1011+496 through unprecedented broadband observations during 2011 and 2012","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","headline":"","cross_cats":[],"primary_cat":"astro-ph.HE","authors_text":"A. Babic, A. Biland, A. B. Pushkarev, A. Carosi, A. C. S. Readhead, A. De Angelis, A. Fern\\'andez-Barral, A. Gonz\\'alez Mu. noz, A. La Barbera, A. L\\\"ahteenm\\\"aki, A. L\\'opez-Oramas, A. Moralejo, A. Niedzwiecki, A. Overkemping, A. Sillanp\\\"a\\\"a, A. Stamerra, A. Treves, B. Biasuzzi, B. De Lotto, B. Marcote, C. Arcaro, C. Delgado Mendez, C. Fruck, C. Mundell, D. A. Sanchez, D. Dominis Prester, D. Dorner, D. Eisenacher, D. Elsaesser, D. Fidalgo, D. F. Torres, D. Galindo, D. Garrido Terrats, D. Hadasch, D. Hrupec, D. Lelas, D. Mazin, D. Nakajima, D. Paneque, D. Sobczynska, D. Tescaro, E. Bernardini, E. Carmona, E. Colombo, E. de O. na Wilhelmi, E. Lindfors, E. Lorenz, E. Prandini, E. Rastorgueva-Foi, F. Borracci, F. D'Ammando, F. Dazzi, F. Di Pierro, F. Longo, F. Tavecchio, G. Bonnoli, G. De Caneva, G. Maneva, H. Kellermann, H. Kubo, H. Takami, I. Lozano, I. Puljak, I. Snidaric, I. Steele, J. A. Barrio, J. Aleksi\\'c, J. Becerra Gonz\\'alez, J. Cortina, J. Herrera, J. Hose, J. Krause, J. Kushida, J. L. Contreras, J. L. Richards, J. M. Miranda, J. M. Paredes, J. Poutanen, J. Rico, J. Rodriguez Garcia, J. Sitarek, J. Tammi, J. Thaele, K. Frantzen, K. Kodani, K. Mallot, K. Mannheim, K. Nilsson, K. Nishijima, K. Noda, K. Saito, K. Satalecka, L. A. Antonelli, L. Font, L. Maraschi, L. Takalo, M. Doro, M. Garczarczyk, M. Gaug, M. Hayashida, M. L. Knoetig, M. L. Lister, M. L\\'opez, M. Makariev, M. Mariotti, M. Mart\\'inez, M. Nievas Rosillo, M. Palatiello, M. Persic, M. Rib\\'o, M. Strzys, M. Teshima, M. Tornikoski, M. V. Fonseca, M. Will, N. Godinovi\\'c, N. Lewandowska, O. Blanch, P. Antoranz, P. Bangale, P. Colin, P. Da Vela, P. G. Prada Moroni, P. Munar-Adrover, P. Temnikov, P. Vogler, R. J. Garc\\'ia L\\'opez, R. L\\'opez-Coto, R. Mirzoyan, R. Orito, R. Paoletti, R. Reinthal, R. Zanin, S. Ansoldi, S. Bonnefoy, S. Buson, S. Covino, S. Einecke, S. Lombardi, S. N. Shore, S. Paiano, S. R. Gozzini, T. Bretz, T. Hovatta, T. Saito, T. Savolainen, T. Schweizer, T. Steinbring, T. Terzi\\'c, T. Toyama, U. Barres de Almeida, U. Menzel, V. Kadenius, V. Neustroev, V. Scalzotto, V. Scapin, W. Bednarek, W. Idec, W. Max-Moerbeck, W. Rhode, X. Paredes-Fortuny, Y. Hanabata, Y. Konno, Y. Y. Kovalev","submitted_at":"2016-03-22T13:19:51Z","abstract_excerpt":"1ES 1011+496 $(z=0.212)$ was discovered in very high energy (VHE, E >100 GeV) $\\gamma$-rays with MAGIC in 2007. The absence of simultaneous data at lower energies led to a rather incomplete characterization of the broadband spectral energy distribution (SED). We study the source properties and the emission mechanisms, probing whether a simple one-zone synchrotron-self-Compton (SSC) scenario is able to explain the observed broadband spectrum. We analyzed VHE to radio data from 2011 and 2012 collected by MAGIC, $Fermi$-LAT, $Swift$, KVA, OVRO, and Mets\\\"ahovi in addition to optical polarimetry d"},"claims":{"count":0,"items":[],"snapshot_sha256":"258153158e38e3291e3d48162225fcdb2d5a3ed65a07baac614ab91432fd4f57"},"source":{"id":"1603.06776","kind":"arxiv","version":4},"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"}