{"record_type":"pith_number_record","schema_url":"https://pith.science/schemas/pith-number/v1.json","pith_number":"pith:2016:LO5RIJ5L7APPEBPXJDWIOVPCUK","short_pith_number":"pith:LO5RIJ5L","schema_version":"1.0","canonical_sha256":"5bbb1427abf81ef205f748ec8755e2a293be7d673dd796d87baf442e57b324ae","source":{"kind":"arxiv","id":"1602.00606","version":1},"attestation_state":"computed","paper":{"title":"Young and middle age pulsar light-curve morphology: Comparison of Fermi observations with gamma-ray and radio emission geometries","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","headline":"","cross_cats":[],"primary_cat":"astro-ph.HE","authors_text":"A. K. Harding, I. A. Grenier, M. Pierbattista, P. L. Gonthier","submitted_at":"2016-02-01T17:37:42Z","abstract_excerpt":"Thanks to the huge amount of gamma-ray pulsar photons collected by the Fermi Large Area Telescope since June 2008, it is now possible to constrain gamma-ray geometrical models by comparing simulated and observed light-curve morphological characteristics. We assumed vacuum-retarded dipole pulsar magnetic field and tested simulated and observed morphological light-curve characteristics in the framework of two pole emission geometries, Polar Cap (PC), radio, and Slot Gap (SG), and Outer Gap (OG)/One Pole Caustic (OPC) emission geometries. We compared simulated and observed/estimated light-curve m"},"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":"1602.00606","kind":"arxiv","version":1},"metadata":{"license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","primary_cat":"astro-ph.HE","submitted_at":"2016-02-01T17:37:42Z","cross_cats_sorted":[],"title_canon_sha256":"81c168364a1dad180426216810ba820638366edca3d8575baf0b0dda2f6076a6","abstract_canon_sha256":"0a0eaab37076b8e87fd1222aa3fa66759144de2e8f28f8573f3f77c3e5242670"},"schema_version":"1.0"},"receipt":{"kind":"pith_receipt","key_id":"pith-v1-2026-05","algorithm":"ed25519","signed_at":"2026-05-18T01:17:41.754131Z","signature_b64":"18QI+i3TcNvW1/7nWpLuyB75S/QH/SlOMoRyafCsKnDSCSrQW/Kg0n62c4c0J70WDp+sEhhQIKeIjTbB5kL7Bw==","signed_message":"canonical_sha256_bytes","builder_version":"pith-number-builder-2026-05-17-v1","receipt_version":"0.3","canonical_sha256":"5bbb1427abf81ef205f748ec8755e2a293be7d673dd796d87baf442e57b324ae","last_reissued_at":"2026-05-18T01:17:41.753454Z","signature_status":"signed_v1","first_computed_at":"2026-05-18T01:17:41.753454Z","public_key_fingerprint":"8d4b5ee74e4693bcd1df2446408b0d54"},"graph_snapshot":{"paper":{"title":"Young and middle age pulsar light-curve morphology: Comparison of Fermi observations with gamma-ray and radio emission geometries","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","headline":"","cross_cats":[],"primary_cat":"astro-ph.HE","authors_text":"A. K. Harding, I. A. Grenier, M. Pierbattista, P. L. Gonthier","submitted_at":"2016-02-01T17:37:42Z","abstract_excerpt":"Thanks to the huge amount of gamma-ray pulsar photons collected by the Fermi Large Area Telescope since June 2008, it is now possible to constrain gamma-ray geometrical models by comparing simulated and observed light-curve morphological characteristics. We assumed vacuum-retarded dipole pulsar magnetic field and tested simulated and observed morphological light-curve characteristics in the framework of two pole emission geometries, Polar Cap (PC), radio, and Slot Gap (SG), and Outer Gap (OG)/One Pole Caustic (OPC) emission geometries. We compared simulated and observed/estimated light-curve m"},"claims":{"count":0,"items":[],"snapshot_sha256":"258153158e38e3291e3d48162225fcdb2d5a3ed65a07baac614ab91432fd4f57"},"source":{"id":"1602.00606","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":"1602.00606","created_at":"2026-05-18T01:17:41.753561+00:00"},{"alias_kind":"arxiv_version","alias_value":"1602.00606v1","created_at":"2026-05-18T01:17:41.753561+00:00"},{"alias_kind":"doi","alias_value":"10.48550/arxiv.1602.00606","created_at":"2026-05-18T01:17:41.753561+00:00"},{"alias_kind":"pith_short_12","alias_value":"LO5RIJ5L7APP","created_at":"2026-05-18T12:30:29.479603+00:00"},{"alias_kind":"pith_short_16","alias_value":"LO5RIJ5L7APPEBPX","created_at":"2026-05-18T12:30:29.479603+00:00"},{"alias_kind":"pith_short_8","alias_value":"LO5RIJ5L","created_at":"2026-05-18T12:30:29.479603+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/LO5RIJ5L7APPEBPXJDWIOVPCUK","json":"https://pith.science/pith/LO5RIJ5L7APPEBPXJDWIOVPCUK.json","graph_json":"https://pith.science/api/pith-number/LO5RIJ5L7APPEBPXJDWIOVPCUK/graph.json","events_json":"https://pith.science/api/pith-number/LO5RIJ5L7APPEBPXJDWIOVPCUK/events.json","paper":"https://pith.science/paper/LO5RIJ5L"},"agent_actions":{"view_html":"https://pith.science/pith/LO5RIJ5L7APPEBPXJDWIOVPCUK","download_json":"https://pith.science/pith/LO5RIJ5L7APPEBPXJDWIOVPCUK.json","view_paper":"https://pith.science/paper/LO5RIJ5L","resolve_alias":"https://pith.science/api/pith-number/resolve?arxiv=1602.00606&json=true","fetch_graph":"https://pith.science/api/pith-number/LO5RIJ5L7APPEBPXJDWIOVPCUK/graph.json","fetch_events":"https://pith.science/api/pith-number/LO5RIJ5L7APPEBPXJDWIOVPCUK/events.json","actions":{"anchor_timestamp":"https://pith.science/pith/LO5RIJ5L7APPEBPXJDWIOVPCUK/action/timestamp_anchor","attest_storage":"https://pith.science/pith/LO5RIJ5L7APPEBPXJDWIOVPCUK/action/storage_attestation","attest_author":"https://pith.science/pith/LO5RIJ5L7APPEBPXJDWIOVPCUK/action/author_attestation","sign_citation":"https://pith.science/pith/LO5RIJ5L7APPEBPXJDWIOVPCUK/action/citation_signature","submit_replication":"https://pith.science/pith/LO5RIJ5L7APPEBPXJDWIOVPCUK/action/replication_record"}},"created_at":"2026-05-18T01:17:41.753561+00:00","updated_at":"2026-05-18T01:17:41.753561+00:00"}