{"record_type":"pith_number_record","schema_url":"https://pith.science/schemas/pith-number/v1.json","pith_number":"pith:2010:R4HDTSAI7CD6F5G3CYC6HH3OQL","short_pith_number":"pith:R4HDTSAI","schema_version":"1.0","canonical_sha256":"8f0e39c808f887e2f4db1605e39f6e82f43e81310605c9b41374d0fa2aa6081a","source":{"kind":"arxiv","id":"1007.2183","version":1},"attestation_state":"computed","paper":{"title":"Pulsar Results with the Fermi Large Area Telescope","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","headline":"","cross_cats":[],"primary_cat":"astro-ph.HE","authors_text":"Pablo M. Saz Parkinson, Paul S. Ray","submitted_at":"2010-07-13T20:00:01Z","abstract_excerpt":"The launch of the Fermi Gamma-ray Space Telescope has heralded a new era in the study of gamma-ray pulsars. The population of confirmed gamma-ray pulsars has gone from 6-7 to more than 60, and the superb sensitivity of the Large Area Telescope (LAT) on Fermi has allowed the detailed study of their spectra and light curves. Twenty-four of these pulsars were discovered in blind searches of the gamma-ray data, and twenty-one of these are, at present, radio quiet, despite deep radio follow-up observations. In addition, millisecond pulsars have been confirmed as a class of gamma-ray emitters, both "},"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":"1007.2183","kind":"arxiv","version":1},"metadata":{"license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","primary_cat":"astro-ph.HE","submitted_at":"2010-07-13T20:00:01Z","cross_cats_sorted":[],"title_canon_sha256":"795a9a5d40324ecd4ca936744abe394bd84e9e3c73c927f57ad1bd57b0a03d21","abstract_canon_sha256":"9f0813cf39fdbdf5d652ac89a787a4f51bccc51a3ec3cc93278ffa42136cc5f9"},"schema_version":"1.0"},"receipt":{"kind":"pith_receipt","key_id":"pith-v1-2026-05","algorithm":"ed25519","signed_at":"2026-05-18T02:06:22.354748Z","signature_b64":"QDwVw2OPVYIHwTZYxoh3EdeGBU0Nzn0fXDMjlBbtNWcTj7cQ2uUA5gCFvxsWcWomZYizYHZH6aJkdcOh0KDiAw==","signed_message":"canonical_sha256_bytes","builder_version":"pith-number-builder-2026-05-17-v1","receipt_version":"0.3","canonical_sha256":"8f0e39c808f887e2f4db1605e39f6e82f43e81310605c9b41374d0fa2aa6081a","last_reissued_at":"2026-05-18T02:06:22.354091Z","signature_status":"signed_v1","first_computed_at":"2026-05-18T02:06:22.354091Z","public_key_fingerprint":"8d4b5ee74e4693bcd1df2446408b0d54"},"graph_snapshot":{"paper":{"title":"Pulsar Results with the Fermi Large Area Telescope","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","headline":"","cross_cats":[],"primary_cat":"astro-ph.HE","authors_text":"Pablo M. Saz Parkinson, Paul S. Ray","submitted_at":"2010-07-13T20:00:01Z","abstract_excerpt":"The launch of the Fermi Gamma-ray Space Telescope has heralded a new era in the study of gamma-ray pulsars. The population of confirmed gamma-ray pulsars has gone from 6-7 to more than 60, and the superb sensitivity of the Large Area Telescope (LAT) on Fermi has allowed the detailed study of their spectra and light curves. Twenty-four of these pulsars were discovered in blind searches of the gamma-ray data, and twenty-one of these are, at present, radio quiet, despite deep radio follow-up observations. In addition, millisecond pulsars have been confirmed as a class of gamma-ray emitters, both "},"claims":{"count":0,"items":[],"snapshot_sha256":"258153158e38e3291e3d48162225fcdb2d5a3ed65a07baac614ab91432fd4f57"},"source":{"id":"1007.2183","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":"1007.2183","created_at":"2026-05-18T02:06:22.354186+00:00"},{"alias_kind":"arxiv_version","alias_value":"1007.2183v1","created_at":"2026-05-18T02:06:22.354186+00:00"},{"alias_kind":"doi","alias_value":"10.48550/arxiv.1007.2183","created_at":"2026-05-18T02:06:22.354186+00:00"},{"alias_kind":"pith_short_12","alias_value":"R4HDTSAI7CD6","created_at":"2026-05-18T12:26:13.927090+00:00"},{"alias_kind":"pith_short_16","alias_value":"R4HDTSAI7CD6F5G3","created_at":"2026-05-18T12:26:13.927090+00:00"},{"alias_kind":"pith_short_8","alias_value":"R4HDTSAI","created_at":"2026-05-18T12:26:13.927090+00:00"}],"events":[],"event_summary":{},"paper_claims":[],"inbound_citations":{"count":0,"internal_anchor_count":0,"sample":[]},"formal_canon":{"evidence_count":0,"sample":[],"anchors":[]},"links":{"html":"https://pith.science/pith/R4HDTSAI7CD6F5G3CYC6HH3OQL","json":"https://pith.science/pith/R4HDTSAI7CD6F5G3CYC6HH3OQL.json","graph_json":"https://pith.science/api/pith-number/R4HDTSAI7CD6F5G3CYC6HH3OQL/graph.json","events_json":"https://pith.science/api/pith-number/R4HDTSAI7CD6F5G3CYC6HH3OQL/events.json","paper":"https://pith.science/paper/R4HDTSAI"},"agent_actions":{"view_html":"https://pith.science/pith/R4HDTSAI7CD6F5G3CYC6HH3OQL","download_json":"https://pith.science/pith/R4HDTSAI7CD6F5G3CYC6HH3OQL.json","view_paper":"https://pith.science/paper/R4HDTSAI","resolve_alias":"https://pith.science/api/pith-number/resolve?arxiv=1007.2183&json=true","fetch_graph":"https://pith.science/api/pith-number/R4HDTSAI7CD6F5G3CYC6HH3OQL/graph.json","fetch_events":"https://pith.science/api/pith-number/R4HDTSAI7CD6F5G3CYC6HH3OQL/events.json","actions":{"anchor_timestamp":"https://pith.science/pith/R4HDTSAI7CD6F5G3CYC6HH3OQL/action/timestamp_anchor","attest_storage":"https://pith.science/pith/R4HDTSAI7CD6F5G3CYC6HH3OQL/action/storage_attestation","attest_author":"https://pith.science/pith/R4HDTSAI7CD6F5G3CYC6HH3OQL/action/author_attestation","sign_citation":"https://pith.science/pith/R4HDTSAI7CD6F5G3CYC6HH3OQL/action/citation_signature","submit_replication":"https://pith.science/pith/R4HDTSAI7CD6F5G3CYC6HH3OQL/action/replication_record"}},"created_at":"2026-05-18T02:06:22.354186+00:00","updated_at":"2026-05-18T02:06:22.354186+00:00"}