{"paper":{"title":"GeV Observations of Star-forming Galaxies with \\textit{Fermi} LAT","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","headline":"","cross_cats":[],"primary_cat":"astro-ph.HE","authors_text":"A. Allafort, A. Bouvier, A. Chekhtman, A. Drlica-Wagner, A. Morselli, A. N. Cillis, A. Okumura, A. P. Waite, A. Reimer, A. S. Johnson, A. W. Borgland, A. W. Strong, B. Berenji, B. Lott, C. C. Cheung, C. Cecchi, C. D. Dermer, C. Favuzzi, C. Monte, C. Sbarra, C. Sgr\\`o, D. Bastieri, D. F. Torres, D. Gasparrini, D. Hadasch, D. Parent, E. Bonamente, E. Charles, E. D. Bloom, E. do Couto e Silva, E. Hays, E. J. Siskind, E. Nuss, E. Orlando, E. Troja, F. de Palma, Fermi LAT Collaboration: M. Ackermann, F. Gargano, F. Giordano, F. Longo, F. Loparco, F. Piron, G. A. Caliandro, G. Godfrey, G. J\\'ohannesson, G. M. Madejski, G. Pivato, G. Spandre, G. Tosti, G. Vianello, H. Katagiri, H. Takahashi, I. A. Grenier, I. V. Moskalenko, J. Ballet, J. Bregeon, J. B. Thayer, J. Chiang, J. Cohen-Tanugi, J. Conrad, J. E. McEnery, J. Kataoka, J. Kn\\\"odlseder, J. Lande, J. M. Casandjian, J. P. Norris, J. Vandenbroucke, K. Bechtol, L. Baldini, L. Tibaldo, \\{L}ukasz Stawarz, M. Ajello, M. Brigida, M. E. Monzani, M. Gustafsson, M. Hayashida, M. Kuss, M. N. Lovellette, M. N. Mazziotta, M. Ohno, M. Ozaki, M. Persic, M. Pesce-Rollins, M. Pierbattista, M. Razzano, M. Roth, M. Tinivella, M. Wood, N. Giglietto, N. Omodei, O. Reimer, P. A. Caraveo, P. Bruel, P. F. Michelson, P. Fortin, P. Fusco, P. Lubrano, P. Martin, P. S. Drell, P. Spinelli, R. A. Cameron, R. Bellazzini, R. Buehler, R. Claus, R. E. Hughes, R. Rando, S. Buson, S. Ciprini, S. Cutini, S. Funk, S. Germani, S. Guiriec, S. J. Fegan, S. Murgia, S. Nishino, S. Rain\\`o, S. Ritz, S. W. Digel, T. A. Porter, T. Glanzman, T. Kamae, T. Mizuno, T. Ohsugi, T. Tanaka, V. Petrosian, V. Vitale, Y. Fukazawa, Y. Uchiyama, Z. Yang","submitted_at":"2012-06-06T20:47:20Z","abstract_excerpt":"Recent detections of the starburst galaxies M82 and NGC 253 by gamma-ray telescopes suggest that galaxies rapidly forming massive stars are more luminous at gamma-ray energies compared to their quiescent relatives. Building upon those results, we examine a sample of 69 dwarf, spiral, and luminous and ultraluminous infrared galaxies at photon energies 0.1-100 GeV using 3 years of data collected by the Large Area Telescope (LAT) on the \\textit{Fermi Gamma-ray Space Telescope} (\\textit{Fermi}). Measured fluxes from significantly detected sources and flux upper limits for the remaining galaxies ar"},"claims":{"count":0,"items":[],"snapshot_sha256":"258153158e38e3291e3d48162225fcdb2d5a3ed65a07baac614ab91432fd4f57"},"source":{"id":"1206.1346","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"}