{"record_type":"pith_number_record","schema_url":"https://pith.science/schemas/pith-number/v1.json","pith_number":"pith:2024:HO3XNW7V7JYTHRZXQ3KDOLOKGZ","short_pith_number":"pith:HO3XNW7V","schema_version":"1.0","canonical_sha256":"3bb776dbf5fa7133c73786d4372dca3678baaf6c5f21a23658eb05b13adf9140","source":{"kind":"arxiv","id":"2408.15022","version":2},"attestation_state":"computed","paper":{"title":"A multi-band study of pulsar glitches with Fermi-LAT and Parkes","license":"http://creativecommons.org/licenses/by/4.0/","headline":"","cross_cats":["nucl-th"],"primary_cat":"astro-ph.HE","authors_text":"A. Li, D. Li, E. G\\\"ugercino\\u{g}lu, J.-P. Yuan, M.-Y. Ge, N. Wang, P. Liu, P. Wang, S.-J. Dang, S.-Q. Zhou, W.-T. Ye, Z. H. Tu, Z.-R. Zhou","submitted_at":"2024-08-27T12:55:02Z","abstract_excerpt":"Pulsar glitch is a phenomenon characterized by abrupt changes in the spin period over less than a minute. We present a comprehensive analysis of glitches in four gamma-ray pulsars by combining the timing observation data from \\textit{Fermi} Large Area Telescope (\\textit{Fermi}-LAT) and Parkes 64 m radio telescope. The timing data of five pulsars, namely PSRs J1028$-$5819, J1420$-$6048, J1509$-$5850, J1709$-$4429 (B1706$-$44) and J1718$-$3825, are examined over 14 yr of observations for each. A total of 12 glitches are identified in four pulsars, including a previously unreported glitch. That i"},"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":"2408.15022","kind":"arxiv","version":2},"metadata":{"license":"http://creativecommons.org/licenses/by/4.0/","primary_cat":"astro-ph.HE","submitted_at":"2024-08-27T12:55:02Z","cross_cats_sorted":["nucl-th"],"title_canon_sha256":"cb630e8cec80100c93163e09cdfd20f442125d4af90415361eef620c2a00d3a8","abstract_canon_sha256":"1d3b137142bc22297478a10f849a4e84fb19e29ed7cc9ca9ef832150ef28ed5c"},"schema_version":"1.0"},"receipt":{"kind":"pith_receipt","key_id":"pith-v1-2026-05","algorithm":"ed25519","signed_at":"2026-07-05T10:01:35.924111Z","signature_b64":"iOIw+bFvHyKBT3FxiIlJ74Cs1gG3wP/LKaAaKzKCgarub0jlpu4s6zym8DqHM1MjRLYV1ooW3A94wGENH7aZBw==","signed_message":"canonical_sha256_bytes","builder_version":"pith-number-builder-2026-05-17-v1","receipt_version":"0.3","canonical_sha256":"3bb776dbf5fa7133c73786d4372dca3678baaf6c5f21a23658eb05b13adf9140","last_reissued_at":"2026-07-05T10:01:35.923603Z","signature_status":"signed_v1","first_computed_at":"2026-07-05T10:01:35.923603Z","public_key_fingerprint":"8d4b5ee74e4693bcd1df2446408b0d54"},"graph_snapshot":{"paper":{"title":"A multi-band study of pulsar glitches with Fermi-LAT and Parkes","license":"http://creativecommons.org/licenses/by/4.0/","headline":"","cross_cats":["nucl-th"],"primary_cat":"astro-ph.HE","authors_text":"A. Li, D. Li, E. G\\\"ugercino\\u{g}lu, J.-P. Yuan, M.-Y. Ge, N. Wang, P. Liu, P. Wang, S.-J. Dang, S.-Q. Zhou, W.-T. Ye, Z. H. Tu, Z.-R. Zhou","submitted_at":"2024-08-27T12:55:02Z","abstract_excerpt":"Pulsar glitch is a phenomenon characterized by abrupt changes in the spin period over less than a minute. We present a comprehensive analysis of glitches in four gamma-ray pulsars by combining the timing observation data from \\textit{Fermi} Large Area Telescope (\\textit{Fermi}-LAT) and Parkes 64 m radio telescope. The timing data of five pulsars, namely PSRs J1028$-$5819, J1420$-$6048, J1509$-$5850, J1709$-$4429 (B1706$-$44) and J1718$-$3825, are examined over 14 yr of observations for each. A total of 12 glitches are identified in four pulsars, including a previously unreported glitch. That i"},"claims":{"count":0,"items":[],"snapshot_sha256":"258153158e38e3291e3d48162225fcdb2d5a3ed65a07baac614ab91432fd4f57"},"source":{"id":"2408.15022","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/2408.15022/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":"2408.15022","created_at":"2026-07-05T10:01:35.923672+00:00"},{"alias_kind":"arxiv_version","alias_value":"2408.15022v2","created_at":"2026-07-05T10:01:35.923672+00:00"},{"alias_kind":"doi","alias_value":"10.48550/arxiv.2408.15022","created_at":"2026-07-05T10:01:35.923672+00:00"},{"alias_kind":"pith_short_12","alias_value":"HO3XNW7V7JYT","created_at":"2026-07-05T10:01:35.923672+00:00"},{"alias_kind":"pith_short_16","alias_value":"HO3XNW7V7JYTHRZX","created_at":"2026-07-05T10:01:35.923672+00:00"},{"alias_kind":"pith_short_8","alias_value":"HO3XNW7V","created_at":"2026-07-05T10:01:35.923672+00:00"}],"events":[],"event_summary":{},"paper_claims":[],"inbound_citations":{"count":1,"internal_anchor_count":0,"sample":[{"citing_arxiv_id":"2605.02467","citing_title":"Modeling large glitches with core superfluidity in a Hybrid star","ref_index":6,"is_internal_anchor":false}]},"formal_canon":{"evidence_count":0,"sample":[],"anchors":[]},"links":{"html":"https://pith.science/pith/HO3XNW7V7JYTHRZXQ3KDOLOKGZ","json":"https://pith.science/pith/HO3XNW7V7JYTHRZXQ3KDOLOKGZ.json","graph_json":"https://pith.science/api/pith-number/HO3XNW7V7JYTHRZXQ3KDOLOKGZ/graph.json","events_json":"https://pith.science/api/pith-number/HO3XNW7V7JYTHRZXQ3KDOLOKGZ/events.json","paper":"https://pith.science/paper/HO3XNW7V"},"agent_actions":{"view_html":"https://pith.science/pith/HO3XNW7V7JYTHRZXQ3KDOLOKGZ","download_json":"https://pith.science/pith/HO3XNW7V7JYTHRZXQ3KDOLOKGZ.json","view_paper":"https://pith.science/paper/HO3XNW7V","resolve_alias":"https://pith.science/api/pith-number/resolve?arxiv=2408.15022&json=true","fetch_graph":"https://pith.science/api/pith-number/HO3XNW7V7JYTHRZXQ3KDOLOKGZ/graph.json","fetch_events":"https://pith.science/api/pith-number/HO3XNW7V7JYTHRZXQ3KDOLOKGZ/events.json","actions":{"anchor_timestamp":"https://pith.science/pith/HO3XNW7V7JYTHRZXQ3KDOLOKGZ/action/timestamp_anchor","attest_storage":"https://pith.science/pith/HO3XNW7V7JYTHRZXQ3KDOLOKGZ/action/storage_attestation","attest_author":"https://pith.science/pith/HO3XNW7V7JYTHRZXQ3KDOLOKGZ/action/author_attestation","sign_citation":"https://pith.science/pith/HO3XNW7V7JYTHRZXQ3KDOLOKGZ/action/citation_signature","submit_replication":"https://pith.science/pith/HO3XNW7V7JYTHRZXQ3KDOLOKGZ/action/replication_record"}},"created_at":"2026-07-05T10:01:35.923672+00:00","updated_at":"2026-07-05T10:01:35.923672+00:00"}