{"paper":{"title":"Discovery of very high energy gamma-ray emission from the blazar 1ES 0033+595 by the MAGIC telescopes","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","headline":"","cross_cats":["astro-ph.CO","astro-ph.GA"],"primary_cat":"astro-ph.HE","authors_text":"A. Babic, A. Biland, A. Carosi, A. De Angelis, A. Dom\\'inguez, A. Gonz\\'alez Mu\\~noz, A. Herrero, A. La Barbera, A. L\\'opez-Oramas, A. Moralejo, A. Niedzwiecki, A. Overkemping, A. Saggion, A. Sillanp\\\"a\\\"a, A. Stamerra, A. Treves, B. De Lotto, B. Marcote, C. Delgado Mendez, C. Fruck, C. Schultz, D. Carreto Fidalgo, D. Dominis Prester, D. Dorner, D. Eisenacher, D. Elsaesser, D. Ferenc, D. F. Torres, D. Garrido Terrats, D. Hadasch, D. Hildebrand, D. Hrupec, D. Lelas, D. Mazin, D. Nakajima, D. Paneque, D. Sobczynska, D. Tescaro, E. Bernardini, E. Carmona, E. Colombo, E. Farina, E. Lindfors, E. Lorenz, E. Prandini, F. Borracci, F. Dazzi, F. Prada, F. Spanier, F. Tavecchio, F. Zandanel, G. Bonnoli, G. De Caneva, G. Maneva, H. Kellermann, H. Kubo, H. Takami, I. Lozano, I. Puljak, I. Snidaric, J. A. Barrio, J. Aleksi\\'c, J. Becerra Gonz\\'alez, J. Cortina, J. Herrera, J. Hose, J. Krause, J. Kushida, J. L. Contreras, J. M. Miranda, J. M. Paredes, J. Rico, J. Rodriguez Garcia, J. Sitarek, J. Storz, J. Thaele, K. Berger, 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. Doert, M. Doro, M. Garczarczyk, M. Gaug, M. Hayashida, M. L\\'opez, M. Makariev, M. Mariotti, M. Mart\\'inez, M. Meucci, M. Palatiello, M. Persic, M. Rib\\'o, M. Teshima, M. Uellenbeck, M. V. Fonseca, N. Godinovi\\'c, N. Lewandowska, N. Mankuzhiyil, N. Nowak, O. Blanch, O. Tibolla, 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. M. Wagner, R. Orito, R. Paoletti, R. Reinthal, R. Zanin (MAGIC collaboration), S. Ansoldi, S. Bonnefoy, S. Buson, S. Covino, S. Einecke, S. Lombardi, S. N. Shore, S. Paiano, S. Partini, S. Preziuso, S. R. Gozzini, S. R\\\"ugamer, S. Sun, T. Bretz, T. Saito, T. Schweizer, T. Steinbring, T. Suri\\'c, T. Terzi\\'c, T. Toyama, U. Barres de Almeida, U. Menzel, V. Kadenius, V. Scalzotto, V. Scapin, V. Stamatescu, V. Tronconi, W. Bednarek, W. Idec, W. Rhode, X. Paredes-Fortuny, Y. Konno","submitted_at":"2014-10-26T16:59:44Z","abstract_excerpt":"The number of known very high energy (VHE) blazars is $\\sim\\,50$, which is very small in comparison to the number of blazars detected in other frequencies. This situation is a handicap for population studies of blazars, which emit about half of their luminosity in the $\\gamma$-ray domain. Moreover, VHE blazars, if distant, allow for the study of the environment that the high-energy $\\gamma$-rays traverse in their path towards the Earth, like the extragalactic background light (EBL) and the intergalactic magnetic field (IGMF), and hence they have a special interest for the astrophysics communit"},"claims":{"count":0,"items":[],"snapshot_sha256":"258153158e38e3291e3d48162225fcdb2d5a3ed65a07baac614ab91432fd4f57"},"source":{"id":"1410.7059","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"}