{"paper":{"title":"The Spectral Energy Distribution of Fermi bright blazars","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","headline":"","cross_cats":[],"primary_cat":"astro-ph.CO","authors_text":"A. A. Abdo, A. Borgland, A. Brez, A. Chekhtman, A. De Angelis, A. K. Harding, A. Makeev, A. S. Johnson, B. Berenji, B. Giebels, B. Lott, B. M. Baughman, C. Cecchi, C. D. Dermer, C. Farnier, C. Favuzzi, C. Meurer, D. Bastieri, D. Dumora, D. Gasparrini, D. Hadasch, D. Horan, E. Bonamente, E. Cavazzuti, E. Charles, E. D. Bloom, E. do Couto e Silva, E. Hays, et al, F. de Palma, F. Gargano, F. Giordano, F. Longo, F. Loparco, G. A. Caliandro, G. Barbiellini, G. Godfrey, G. Johannesson, G. M. Madejski, H. Katagiri, I. A. Grenier, J. Ballet, J. Bregeon, J. Chiang, J. Cohen-Tanugi, J. Conrad, J. E. Grove, J. E. McEnery, J. Kataoka, J. Knodlseder, J. Lande, J. M. Casandjian, K. Bechtol, L. Baldini, L. Costamante, L. Fuhrmann, L. Guillemot, L. Latronico, L. R. Cominsky, M. Ackermann, M. Ajello, M. Axelsson, M. Brigida, M. Frailis, M. Hayashida, M. Kadler, M. Kerr, M. Kuss, M. L. Kocian, M. N. Lovellette, M. N. Mazziotta, M. S. Jackson, N. Gehrels, N. Giglietto, N. Kawai, O. Celik, P. A. Caraveo, P. Bruel, P. F. Michelson, P. Fortin, P. Fusco, P. Giommi, P. Lubrano, P. S. Drell, R. A. Cameron, R. Bellazzini, R. Claus, R. D. Blandford, R. Dubois, R. E. Hughes, R. Itoh, S. Buson, S. Chaty, S. Ciprini, S. Colafrancesco, S. Cutini, S. E. Healey, S. Funk, S. Germani, S. Guiriec, S. J. Fegan, S. W. Digel, T. Glanzman, T. H. Burnett, T. Kamae, W. B. Focke, W. Max-Moerbeck, W. McConville, W. N. Johnson, Y. Fukazawa, Y. Hanabata","submitted_at":"2009-12-10T16:38:42Z","abstract_excerpt":"(Abridged) We have conducted a detailed investigation of the broad-band spectral properties of the \\gamma-ray selected blazars of the Fermi LAT Bright AGN Sample (LBAS). By combining our accurately estimated Fermi gamma-ray spectra with Swift, radio, infra-red, optical and other hard X-ray/gamma-ray data, collected within three months of the LBAS data taking period, we were able to assemble high-quality and quasi-simultaneous Spectral Energy Distributions (SED) for 48 LBAS blazars.The SED of these gamma-ray sources is similar to that of blazars discovered at other wavelengths, clearly showing,"},"claims":{"count":0,"items":[],"snapshot_sha256":"258153158e38e3291e3d48162225fcdb2d5a3ed65a07baac614ab91432fd4f57"},"source":{"id":"0912.2040","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"}