{"paper":{"title":"The second catalog of flaring gamma-ray sources from the Fermi All-sky Variability Analysis","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","headline":"","cross_cats":[],"primary_cat":"astro-ph.HE","authors_text":"A. Albert, A. Chekhtman, A. Desai, A. Franckowiak, A. Manfreda, A. Morselli, A. Reimer, A. S. Johnson, B. Donaggio, C. C. Cheung, C. Cecchi, C. Favuzzi, C. Sgr\\`o, D. Bastieri, D. Costantin, D. F. Torres, D. Gasparrini, D. Green, D. Horan, D. J. Suson, D. J. Thompson, D. Kocevski, D. Paneque, D. Simone, E. Bissaldi, E. Bottacini, E. Cavazzuti, E. C. Ferrara, E. D. Bloom, E. Hays, E. J. Siskind, E. Nuss, E. Orlando, E. Torresi, E. Troja, F. Costanza, F. D'Ammando, F. de Palma, F. Gargano, F. Giordano, F. Longo, F. Loparco, F. Piron, F. Spada, G. Barbiellini, G. Chiaro, G. J\\'ohannesson, G. La Mura, G. Principe, G. Spandre, G. Tosti, G. Vianello, I. A. Grenier, I. V. Moskalenko, J. Ballet, J. Becerra Gonzalez, J. Bregeon, J. B. Thayer, J. Conrad, J. D. Magill, J. E. Grove, J. Li, J. S. Perkins, K. S. Wood, K. Tanaka, L. Baldini, L. Di Venere, L. Guillemot, L. Latronico, L. Stawarz, M. Ackermann, M. Ajello, M. Caragiulo, M. Di Mauro, M. E. Monzani, M. Giomi, M. Giroletti, M. Kuss, M. Mayer, M. Negro, M. N. Lovellette, M. N. Mazziotta, M. Orienti, M. Persic, M. Pesce-Rollins, M. Razzano, M. Takahashi, N. Di Lalla, N. Giglietto, N. Omodei, O. Reimer, P. A. Caraveo, P. Bruel, P. F. Michelson, P. Fusco, P. Lubrano, P. S. Drell, P. Spinelli, R. A. Cameron, R. Bellazzini, R. Bonino, R. Buehler, R. D. Blandford, R. Desiante, R. Rando, S. Abdollahi, S. Buson, S. Ciprini, S. Cutini, S. Funk, S. Guiriec, S. J. Fegan, S. Larsson, S. Maldera, S. Rain\\`o, S. Razzaque, S. W. Digel, T. A. Porter, T. Glanzman, T. Jogler, T. Mizuno, T. Ohsugi, V. Petrosian, V. S. Paliya, W. B. Focke, W. Mitthumsiri, Y. Fukazawa","submitted_at":"2016-12-09T20:59:58Z","abstract_excerpt":"We present the second catalog of flaring gamma-ray sources (2FAV) detected with the Fermi All-sky Variability Analysis (FAVA), a tool that blindly searches for transients over the entire sky observed by the Large Area Telescope (LAT) on board the \\textit{Fermi} Gamma-ray Space Telescope. With respect to the first FAVA catalog, this catalog benefits from a larger data set, the latest LAT data release (Pass 8), as well as from an improved analysis that includes likelihood techniques for a more precise localization of the transients. Applying this analysis on the first 7.4 years of \\textit{Fermi}"},"claims":{"count":0,"items":[],"snapshot_sha256":"258153158e38e3291e3d48162225fcdb2d5a3ed65a07baac614ab91432fd4f57"},"source":{"id":"1612.03165","kind":"arxiv","version":3},"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"}