{"paper":{"title":"Detection of bridge emission above 50 GeV from the Crab pulsar with the MAGIC telescopes","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","headline":"","cross_cats":[],"primary_cat":"astro-ph.HE","authors_text":"A. Babic, A. Biland, A. Carosi, A. De Angelis, 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. Biasuzzi, B. De Lotto, B. Marcote, C. Delgado Mendez, C. Fruck, C. Schultz, D. Dominis Prester, D. Dorner, D. Eisenacher, D. Elsaesser, D. Ferenc, D. Fidalgo, 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. Spanier, F. Tavecchio, 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. Frantzen, K. Hirotani, 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. Palatiello, M. Persic, M. Rib\\'o, M. Strzys, 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, S. Ansoldi, S. Bonnefoy, 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. Schweizer, T. Steinbring, T. Suri\\'c, T. Terzi\\'c, T. Toyama, T.Y. Saito, U. Barres de Almeida, U. Menzel, V. Kadenius, V. Scalzotto, V. Scapin, V. Stamatescu, W. Bednarek, W. Idec, W. Rhode, X. Paredes-Fortuny, Y. Konno","submitted_at":"2014-02-18T03:32:42Z","abstract_excerpt":"The Crab pulsar is the only astronomical pulsed source detected at very high energy (VHE, E>100GeV) gamma-rays. The emission mechanism of VHE pulsation is not yet fully understood, although several theoretical models have been proposed. In order to test the new models, we measured the light curve and the spectra of the Crab pulsar with high precision by means of deep observations. We analyzed 135 hours of selected MAGIC data taken between 2009 and 2013 in stereoscopic mode. In order to discuss the spectral shape in connection with lower energies, 4.6 years of {\\it Fermi}-LAT data were also ana"},"claims":{"count":0,"items":[],"snapshot_sha256":"258153158e38e3291e3d48162225fcdb2d5a3ed65a07baac614ab91432fd4f57"},"source":{"id":"1402.4219","kind":"arxiv","version":2},"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"}