{"record_type":"pith_number_record","schema_url":"https://pith.science/schemas/pith-number/v1.json","pith_number":"pith:2009:IBMP2H57LG6NZTYNF2B4MPZMJU","short_pith_number":"pith:IBMP2H57","schema_version":"1.0","canonical_sha256":"4058fd1fbf59bcdccf0d2e83c63f2c4d21a69b544eccba0c46d3e794d9a91bcd","source":{"kind":"arxiv","id":"0902.1340","version":2},"attestation_state":"computed","paper":{"title":"Fermi Large Area Telescope Bright Gamma-ray Source List","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","headline":"","cross_cats":[],"primary_cat":"astro-ph.HE","authors_text":"A. A. Abdo, et al","submitted_at":"2009-02-08T21:36:37Z","abstract_excerpt":"Following its launch in June 2008, the Fermi Gamma-ray Space Telescope (Fermi) began a sky survey in August. The Large Area Telescope (LAT) on Fermi in 3 months produced a deeper and better-resolved map of the gamma-ray sky than any previous space mission. We present here initial results for energies above 100 MeV for the 205 most significant (statistical significance greater than ~10-sigma) gamma-ray sources in these data. These are the best-characterized and best-localized point-like (i.e., spatially unresolved) gamma-ray sources in the early-mission data."},"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":"0902.1340","kind":"arxiv","version":2},"metadata":{"license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","primary_cat":"astro-ph.HE","submitted_at":"2009-02-08T21:36:37Z","cross_cats_sorted":[],"title_canon_sha256":"27947ef3ebf323756963b846f5637efc9f9089c3008a0009400f843740272e07","abstract_canon_sha256":"88ab8842ee0b3a0148f39bac33fa15b8235772569832f697dbefd8d59a37b245"},"schema_version":"1.0"},"receipt":{"kind":"pith_receipt","key_id":"pith-v1-2026-05","algorithm":"ed25519","signed_at":"2026-07-04T15:45:29.707245Z","signature_b64":"k/qRb2X44Ekh1064GmfCNVF9ey0I/cqA2cDdU17EkDoidiU9F+1BO44VAA7KBx8H33Ugh7QFRxKhT4TQhVBNBA==","signed_message":"canonical_sha256_bytes","builder_version":"pith-number-builder-2026-05-17-v1","receipt_version":"0.3","canonical_sha256":"4058fd1fbf59bcdccf0d2e83c63f2c4d21a69b544eccba0c46d3e794d9a91bcd","last_reissued_at":"2026-07-04T15:45:29.706848Z","signature_status":"signed_v1","first_computed_at":"2026-07-04T15:45:29.706848Z","public_key_fingerprint":"8d4b5ee74e4693bcd1df2446408b0d54"},"graph_snapshot":{"paper":{"title":"Fermi Large Area Telescope Bright Gamma-ray Source List","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","headline":"","cross_cats":[],"primary_cat":"astro-ph.HE","authors_text":"A. A. Abdo, et al","submitted_at":"2009-02-08T21:36:37Z","abstract_excerpt":"Following its launch in June 2008, the Fermi Gamma-ray Space Telescope (Fermi) began a sky survey in August. The Large Area Telescope (LAT) on Fermi in 3 months produced a deeper and better-resolved map of the gamma-ray sky than any previous space mission. We present here initial results for energies above 100 MeV for the 205 most significant (statistical significance greater than ~10-sigma) gamma-ray sources in these data. These are the best-characterized and best-localized point-like (i.e., spatially unresolved) gamma-ray sources in the early-mission data."},"claims":{"count":0,"items":[],"snapshot_sha256":"258153158e38e3291e3d48162225fcdb2d5a3ed65a07baac614ab91432fd4f57"},"source":{"id":"0902.1340","kind":"arxiv","version":2},"verdict":{"id":null,"model_set":{},"created_at":null,"strongest_claim":"","one_line_summary":"","pipeline_version":null,"weakest_assumption":"","pith_extraction_headline":""},"integrity":{"clean":true,"summary":{"advisory":0,"critical":0,"by_detector":{},"informational":0},"endpoint":"/pith/0902.1340/integrity.json","findings":[],"available":true,"detectors_run":[],"snapshot_sha256":"c28c3603d3b5d939e8dc4c7e95fa8dfce3d595e45f758748cecf8e644a296938"},"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":"0902.1340","created_at":"2026-07-04T15:45:29.706906+00:00"},{"alias_kind":"arxiv_version","alias_value":"0902.1340v2","created_at":"2026-07-04T15:45:29.706906+00:00"},{"alias_kind":"doi","alias_value":"10.48550/arxiv.0902.1340","created_at":"2026-07-04T15:45:29.706906+00:00"},{"alias_kind":"pith_short_12","alias_value":"IBMP2H57LG6N","created_at":"2026-07-04T15:45:29.706906+00:00"},{"alias_kind":"pith_short_16","alias_value":"IBMP2H57LG6NZTYN","created_at":"2026-07-04T15:45:29.706906+00:00"},{"alias_kind":"pith_short_8","alias_value":"IBMP2H57","created_at":"2026-07-04T15:45:29.706906+00:00"}],"events":[],"event_summary":{},"paper_claims":[],"inbound_citations":{"count":1,"internal_anchor_count":1,"sample":[{"citing_arxiv_id":"1908.06162","citing_title":"The Cherenkov Telescope Array view of the Galactic Center region","ref_index":5,"is_internal_anchor":true}]},"formal_canon":{"evidence_count":0,"sample":[],"anchors":[]},"links":{"html":"https://pith.science/pith/IBMP2H57LG6NZTYNF2B4MPZMJU","json":"https://pith.science/pith/IBMP2H57LG6NZTYNF2B4MPZMJU.json","graph_json":"https://pith.science/api/pith-number/IBMP2H57LG6NZTYNF2B4MPZMJU/graph.json","events_json":"https://pith.science/api/pith-number/IBMP2H57LG6NZTYNF2B4MPZMJU/events.json","paper":"https://pith.science/paper/IBMP2H57"},"agent_actions":{"view_html":"https://pith.science/pith/IBMP2H57LG6NZTYNF2B4MPZMJU","download_json":"https://pith.science/pith/IBMP2H57LG6NZTYNF2B4MPZMJU.json","view_paper":"https://pith.science/paper/IBMP2H57","resolve_alias":"https://pith.science/api/pith-number/resolve?arxiv=0902.1340&json=true","fetch_graph":"https://pith.science/api/pith-number/IBMP2H57LG6NZTYNF2B4MPZMJU/graph.json","fetch_events":"https://pith.science/api/pith-number/IBMP2H57LG6NZTYNF2B4MPZMJU/events.json","actions":{"anchor_timestamp":"https://pith.science/pith/IBMP2H57LG6NZTYNF2B4MPZMJU/action/timestamp_anchor","attest_storage":"https://pith.science/pith/IBMP2H57LG6NZTYNF2B4MPZMJU/action/storage_attestation","attest_author":"https://pith.science/pith/IBMP2H57LG6NZTYNF2B4MPZMJU/action/author_attestation","sign_citation":"https://pith.science/pith/IBMP2H57LG6NZTYNF2B4MPZMJU/action/citation_signature","submit_replication":"https://pith.science/pith/IBMP2H57LG6NZTYNF2B4MPZMJU/action/replication_record"}},"created_at":"2026-07-04T15:45:29.706906+00:00","updated_at":"2026-07-04T15:45:29.706906+00:00"}