{"record_type":"pith_number_record","schema_url":"https://pith.science/schemas/pith-number/v1.json","pith_number":"pith:2009:PSDMP4DX6TUADLRBBLEOHIJJJA","short_pith_number":"pith:PSDMP4DX","schema_version":"1.0","canonical_sha256":"7c86c7f077f4e801ae210ac8e3a12948165f52f12f050140f20bfac2240e3e6f","source":{"kind":"arxiv","id":"0912.2040","version":1},"attestation_state":"computed","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,"},"verification_status":{"content_addressed":true,"pith_receipt":true,"author_attested":false,"weak_author_claims":0,"strong_author_claims":0,"externally_anchored":false,"storage_verified":false,"citation_signatures":0,"replication_records":0,"graph_snapshot":true,"references_resolved":false,"formal_links_present":false},"canonical_record":{"source":{"id":"0912.2040","kind":"arxiv","version":1},"metadata":{"license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","primary_cat":"astro-ph.CO","submitted_at":"2009-12-10T16:38:42Z","cross_cats_sorted":[],"title_canon_sha256":"7934f512315cac80087fad077d5ce000615a4548979c58acfdaebded4a866f83","abstract_canon_sha256":"461d622e128fed662064da0fad99f850d6e3a4bdff8bc588cf3bfaead4e20e93"},"schema_version":"1.0"},"receipt":{"kind":"pith_receipt","key_id":"pith-v1-2026-05","algorithm":"ed25519","signed_at":"2026-05-18T02:33:56.945158Z","signature_b64":"M6+P9vXQ5QyJbIj6mjsq89xUklQTSgq0RLLkyv3ADkgBsRmU3WkoUvSzFc8+2RCargRqdRo7+t6CiI93TdYtDQ==","signed_message":"canonical_sha256_bytes","builder_version":"pith-number-builder-2026-05-17-v1","receipt_version":"0.3","canonical_sha256":"7c86c7f077f4e801ae210ac8e3a12948165f52f12f050140f20bfac2240e3e6f","last_reissued_at":"2026-05-18T02:33:56.944737Z","signature_status":"signed_v1","first_computed_at":"2026-05-18T02:33:56.944737Z","public_key_fingerprint":"8d4b5ee74e4693bcd1df2446408b0d54"},"graph_snapshot":{"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"},"aliases":[{"alias_kind":"arxiv","alias_value":"0912.2040","created_at":"2026-05-18T02:33:56.944798+00:00"},{"alias_kind":"arxiv_version","alias_value":"0912.2040v1","created_at":"2026-05-18T02:33:56.944798+00:00"},{"alias_kind":"doi","alias_value":"10.48550/arxiv.0912.2040","created_at":"2026-05-18T02:33:56.944798+00:00"},{"alias_kind":"pith_short_12","alias_value":"PSDMP4DX6TUA","created_at":"2026-05-18T12:26:01.383474+00:00"},{"alias_kind":"pith_short_16","alias_value":"PSDMP4DX6TUADLRB","created_at":"2026-05-18T12:26:01.383474+00:00"},{"alias_kind":"pith_short_8","alias_value":"PSDMP4DX","created_at":"2026-05-18T12:26:01.383474+00:00"}],"events":[],"event_summary":{},"paper_claims":[],"inbound_citations":{"count":1,"internal_anchor_count":1,"sample":[{"citing_arxiv_id":"2605.12602","citing_title":"Tracking down the broadband polarimetric properties of PG 1553+113","ref_index":132,"is_internal_anchor":true}]},"formal_canon":{"evidence_count":0,"sample":[],"anchors":[]},"links":{"html":"https://pith.science/pith/PSDMP4DX6TUADLRBBLEOHIJJJA","json":"https://pith.science/pith/PSDMP4DX6TUADLRBBLEOHIJJJA.json","graph_json":"https://pith.science/api/pith-number/PSDMP4DX6TUADLRBBLEOHIJJJA/graph.json","events_json":"https://pith.science/api/pith-number/PSDMP4DX6TUADLRBBLEOHIJJJA/events.json","paper":"https://pith.science/paper/PSDMP4DX"},"agent_actions":{"view_html":"https://pith.science/pith/PSDMP4DX6TUADLRBBLEOHIJJJA","download_json":"https://pith.science/pith/PSDMP4DX6TUADLRBBLEOHIJJJA.json","view_paper":"https://pith.science/paper/PSDMP4DX","resolve_alias":"https://pith.science/api/pith-number/resolve?arxiv=0912.2040&json=true","fetch_graph":"https://pith.science/api/pith-number/PSDMP4DX6TUADLRBBLEOHIJJJA/graph.json","fetch_events":"https://pith.science/api/pith-number/PSDMP4DX6TUADLRBBLEOHIJJJA/events.json","actions":{"anchor_timestamp":"https://pith.science/pith/PSDMP4DX6TUADLRBBLEOHIJJJA/action/timestamp_anchor","attest_storage":"https://pith.science/pith/PSDMP4DX6TUADLRBBLEOHIJJJA/action/storage_attestation","attest_author":"https://pith.science/pith/PSDMP4DX6TUADLRBBLEOHIJJJA/action/author_attestation","sign_citation":"https://pith.science/pith/PSDMP4DX6TUADLRBBLEOHIJJJA/action/citation_signature","submit_replication":"https://pith.science/pith/PSDMP4DX6TUADLRBBLEOHIJJJA/action/replication_record"}},"created_at":"2026-05-18T02:33:56.944798+00:00","updated_at":"2026-05-18T02:33:56.944798+00:00"}