{"paper":{"title":"The Discovery of gamma-Ray Emission From The Blazar RGB J0710+591","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","headline":"","cross_cats":["astro-ph.CO"],"primary_cat":"astro-ph.HE","authors_text":"A. A. Moiseev, A. Bouvier, A. Cannon, A. Cesarini, A. Chekhtman, A. Falcone, A. Furniss, A. Imran, A. Konopelko, A. Lamerato, A. Makeev, A. McCann, A. Morselli, A. N. Otte, A. Pichel, A. P. Waite, A. Reimer, A. Sander, A. S. Johnson, A. Tramacere, A. Varlotta, A. W. Borgland, A. Weinstein, A. W. Smith, A. Y. Rodriguez, B. Berenji, B. Giebels, B. Lott, B. L. Winer, B. Zitzer, C. C. Cheung, C. Cecchi, C. D. Dermer, C. Duke, C. Farnier, C. Favuzzi, C. M. Hui, C. Monte, C. Sgr\\`o, D. A. Williams, D. Bastieri, D. Boltuch, D. Dumora, D. F. Torres, D. Gall, D. Gasparrini, D. Hanna, D. Horan, D. J. Suson, D. J. Thompson, D. Kieda, D. Pandel, D. Paneque, D. Petry, D. Sanchez, D. Steele, E. Aliu, E. Antolini, E. Bonamente, E. Cavazzuti, E. Charles, E. D. Bloom, E. do Couto e Silva, E. Hays, E. J. Siskind, E. Nuss, E. Orlando, E. Roache, F. de Palma, F. Gargano, F. Giordano, F. Krennrich, F. Longo, F. Loparco, F. Piron, G. A. Caliandro, G. Barbiellini, G. Demet Senturk, G. Finnegan, G. Godfrey, G. Gyuk, G. H. Gillanders, G. H. Sembroski, G. J\\'ohannesson, G. Maier, G. Spandre, G. Te\\v{s}i\\'c, G. Tosti, H. F.-W. Sadrozinski, H. J. Rose, H. Katagiri, H. Krawczynski, H. Takahashi, I. A. Grenier, I. V. Moskalenko, J. Ballet, J. Bregeon, J. B. Thayer, J. Chiang, J. Cohen-Tanugi, J. Conrad, J. D. Scargle, J. E. Grove, J. E. Ward, J. F. Ormes, J. Grube, J. G. Thayer, J. H. Buckley, J. Holder, J. H. Panetta, J. Kataoka, J. Kn\\\"odlseder, J. Lande, J. M. Casandjian, J. P. Finley, J. P. Norris, J. Quinn, J. Ripken, J. S. Perkins, K. Bechtol, K. Byrum, K. Gibbs, K. Ragan, K. S. Wood, L. Baldini, L. Ciupik, L. C. Reyes, L. Fortson, L. Latronico, L. Tibaldo, M. Ackermann, M. Ajello, M. Bautista, M. Beilicke, M. B\\\"ottcher, M. Brigida, M. E. Monzani, M. Frailis, M. Giroletti, M. J. Lang, M. Kertzman, M. Kuss, M. Llena Garde, M. McCutcheon, M. N. Lovellette, M. N. Mazziotta, M. Ohno, M. Pepe, M. Pesce-Rollins, M. Pohl, M. Razzano, M. Roth, M. Schroedter, M. S. Strickman, M. Theiling, M. Wood, M. Ziegler, N. Galante, N. Gehrels, N. Giglietto, N. Karlsson, N. Omodei, N. Vilchez, \\\"O. \\c{C}elik, O. Reimer, P. A. Caraveo, P. Bruel, P. D. Smith, P. F. Michelson, P. Fortin, P. Fusco, P. Kaaret, P. L. Nolan, P. Lubrano, P. Moriarty, P. Roustazadeh, P. S. Drell, P. Spinelli, P. T. Reynolds, P. Wang, R. A. Cameron, R. A. Ong, R. Bellazzini, R. Buehler, R. Claus, R. D. Blandford, R. Dickherber, R. Dubois, R. E. Hughes, R. Guenette, R. G. Wagner, R. Mukherjee, R. Rando, S. Buson, S. Carrigan, S. Ciprini, S. Funk, S. Germani, S. Godambe, S. Guiriec, S.-H. Lee, S. J. Fegan, S. LeBohec, S. M. Bradbury, S. McArthur, S. Murgia, S. P. Swordy, S. P. Wakely, S. Rain\\`o, S. Thibadeau, S. Vincent, S. Wissel, T. A. Porter, T. Arlen, T. Aune, T. B. Humensky, T. C. Weekes, T. Glanzman, T. Kamae, T. L. Usher, T. Mizuno, T. Ohsugi, T. Tanaka, T. Weisgarber, T. Ylinen, V. A. Acciari, V. Bugaev, V. Pelassa, V. Vasileiou, V. Vitale, V. V. Vassiliev, W. Benbow, W. Cui, W. Mitthumsiri, W. N. Johnson, Y. Fukazawa, Z. Yang","submitted_at":"2010-05-01T03:19:42Z","abstract_excerpt":"The high-frequency-peaked BL Lacertae object RGB J0710+591 was observed in the very high-energy (VHE; E > 100 GeV) wave band by the VERITAS array of atmospheric Cherenkov telescopes. The observations, taken between 2008 December and 2009 March and totaling 22.1 hr, yield the discovery of VHE gamma rays from the source. RGB J0710+591 is detected at a statistical significance of 5.5 standard deviations (5.5{\\sigma}) above the background, corresponding to an integral flux of (3.9 +/- 0.8) x 10-12 cm-2 s-1 (3% of the Crab Nebula's flux) above 300 GeV. The observed spectrum can be fit by a power la"},"claims":{"count":0,"items":[],"snapshot_sha256":"258153158e38e3291e3d48162225fcdb2d5a3ed65a07baac614ab91432fd4f57"},"source":{"id":"1005.0041","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"}