{"record_type":"pith_number_record","schema_url":"https://pith.science/schemas/pith-number/v1.json","pith_number":"pith:2013:TVMH3VHR2RZNE47VRO77WOO67U","short_pith_number":"pith:TVMH3VHR","schema_version":"1.0","canonical_sha256":"9d587dd4f1d472d273f58bbffb39defd2ed9bb03811df72c771728b2b7dd627c","source":{"kind":"arxiv","id":"1305.4385","version":3},"attestation_state":"computed","paper":{"title":"The Second Fermi Large Area Telescope Catalog of Gamma-ray Pulsars","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","headline":"","cross_cats":[],"primary_cat":"astro-ph.HE","authors_text":"The Fermi-LAT Collaboration","submitted_at":"2013-05-19T17:57:51Z","abstract_excerpt":"This catalog summarizes 117 high-confidence > 0.1 GeV gamma-ray pulsar detections using three years of data acquired by the Large Area Telescope (LAT) on the Fermi satellite. Half are neutron stars discovered using LAT data, through periodicity searches in gamma-ray and radio data around LAT unassociated source positions. The 117 pulsars are evenly divided into three groups: millisecond pulsars, young radio-loud pulsars, and young radio-quiet pulsars. We characterize the pulse profiles and energy spectra and derive luminosities when distance information exists. Spectral analysis of the off-pea"},"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":"1305.4385","kind":"arxiv","version":3},"metadata":{"license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","primary_cat":"astro-ph.HE","submitted_at":"2013-05-19T17:57:51Z","cross_cats_sorted":[],"title_canon_sha256":"67e116be67c7cc6dd7043b6242fbb5d23c6ec3457e93e0a450e9bf9a64db4a1a","abstract_canon_sha256":"4c35307d8aa64e9b676ae3b3318556619f65eb545b980d826c6ecff48c234553"},"schema_version":"1.0"},"receipt":{"kind":"pith_receipt","key_id":"pith-v1-2026-05","algorithm":"ed25519","signed_at":"2026-05-18T03:12:32.798765Z","signature_b64":"ezkNfdEiLo+ImsE5yJg2XbyODejCz+nnDGcrMt66ax6YvZgRfRZeuvmg4e93L42ZuhGWs7W+YPSTcfon16PxDg==","signed_message":"canonical_sha256_bytes","builder_version":"pith-number-builder-2026-05-17-v1","receipt_version":"0.3","canonical_sha256":"9d587dd4f1d472d273f58bbffb39defd2ed9bb03811df72c771728b2b7dd627c","last_reissued_at":"2026-05-18T03:12:32.797982Z","signature_status":"signed_v1","first_computed_at":"2026-05-18T03:12:32.797982Z","public_key_fingerprint":"8d4b5ee74e4693bcd1df2446408b0d54"},"graph_snapshot":{"paper":{"title":"The Second Fermi Large Area Telescope Catalog of Gamma-ray Pulsars","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","headline":"","cross_cats":[],"primary_cat":"astro-ph.HE","authors_text":"The Fermi-LAT Collaboration","submitted_at":"2013-05-19T17:57:51Z","abstract_excerpt":"This catalog summarizes 117 high-confidence > 0.1 GeV gamma-ray pulsar detections using three years of data acquired by the Large Area Telescope (LAT) on the Fermi satellite. Half are neutron stars discovered using LAT data, through periodicity searches in gamma-ray and radio data around LAT unassociated source positions. The 117 pulsars are evenly divided into three groups: millisecond pulsars, young radio-loud pulsars, and young radio-quiet pulsars. We characterize the pulse profiles and energy spectra and derive luminosities when distance information exists. Spectral analysis of the off-pea"},"claims":{"count":0,"items":[],"snapshot_sha256":"258153158e38e3291e3d48162225fcdb2d5a3ed65a07baac614ab91432fd4f57"},"source":{"id":"1305.4385","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"},"aliases":[{"alias_kind":"arxiv","alias_value":"1305.4385","created_at":"2026-05-18T03:12:32.798094+00:00"},{"alias_kind":"arxiv_version","alias_value":"1305.4385v3","created_at":"2026-05-18T03:12:32.798094+00:00"},{"alias_kind":"doi","alias_value":"10.48550/arxiv.1305.4385","created_at":"2026-05-18T03:12:32.798094+00:00"},{"alias_kind":"pith_short_12","alias_value":"TVMH3VHR2RZN","created_at":"2026-05-18T12:28:02.375192+00:00"},{"alias_kind":"pith_short_16","alias_value":"TVMH3VHR2RZNE47V","created_at":"2026-05-18T12:28:02.375192+00:00"},{"alias_kind":"pith_short_8","alias_value":"TVMH3VHR","created_at":"2026-05-18T12:28:02.375192+00:00"}],"events":[],"event_summary":{},"paper_claims":[],"inbound_citations":{"count":1,"internal_anchor_count":1,"sample":[{"citing_arxiv_id":"2605.21331","citing_title":"Searching for links between energetic millisecond pulsars and repeating fast radio bursts","ref_index":10,"is_internal_anchor":true}]},"formal_canon":{"evidence_count":0,"sample":[],"anchors":[]},"links":{"html":"https://pith.science/pith/TVMH3VHR2RZNE47VRO77WOO67U","json":"https://pith.science/pith/TVMH3VHR2RZNE47VRO77WOO67U.json","graph_json":"https://pith.science/api/pith-number/TVMH3VHR2RZNE47VRO77WOO67U/graph.json","events_json":"https://pith.science/api/pith-number/TVMH3VHR2RZNE47VRO77WOO67U/events.json","paper":"https://pith.science/paper/TVMH3VHR"},"agent_actions":{"view_html":"https://pith.science/pith/TVMH3VHR2RZNE47VRO77WOO67U","download_json":"https://pith.science/pith/TVMH3VHR2RZNE47VRO77WOO67U.json","view_paper":"https://pith.science/paper/TVMH3VHR","resolve_alias":"https://pith.science/api/pith-number/resolve?arxiv=1305.4385&json=true","fetch_graph":"https://pith.science/api/pith-number/TVMH3VHR2RZNE47VRO77WOO67U/graph.json","fetch_events":"https://pith.science/api/pith-number/TVMH3VHR2RZNE47VRO77WOO67U/events.json","actions":{"anchor_timestamp":"https://pith.science/pith/TVMH3VHR2RZNE47VRO77WOO67U/action/timestamp_anchor","attest_storage":"https://pith.science/pith/TVMH3VHR2RZNE47VRO77WOO67U/action/storage_attestation","attest_author":"https://pith.science/pith/TVMH3VHR2RZNE47VRO77WOO67U/action/author_attestation","sign_citation":"https://pith.science/pith/TVMH3VHR2RZNE47VRO77WOO67U/action/citation_signature","submit_replication":"https://pith.science/pith/TVMH3VHR2RZNE47VRO77WOO67U/action/replication_record"}},"created_at":"2026-05-18T03:12:32.798094+00:00","updated_at":"2026-05-18T03:12:32.798094+00:00"}