{"record_type":"pith_number_record","schema_url":"https://pith.science/schemas/pith-number/v1.json","pith_number":"pith:2011:DMO7Z52UUNM7NRDAXOFSBH6UOL","short_pith_number":"pith:DMO7Z52U","schema_version":"1.0","canonical_sha256":"1b1dfcf754a359f6c460bb8b209fd472c036269958fcacee38735e255ca13aa3","source":{"kind":"arxiv","id":"1102.1743","version":2},"attestation_state":"computed","paper":{"title":"A study of 315 glitches in the rotation of 102 pulsars","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","headline":"","cross_cats":[],"primary_cat":"astro-ph.HE","authors_text":"Andrew G. Lyne, Ben W. Stappers, Cristobal M. Espinoza, Michael Kramer","submitted_at":"2011-02-08T22:55:51Z","abstract_excerpt":"The rotation of more than 700 pulsars has been monitored using the 76-m Lovell Telescope at Jodrell Bank. Here we report on a new search for glitches in the observations, revealing 128 new glitches in the rotation of 63 pulsars. Combining these new data with those already published we present a database containing 315 glitches in 102 pulsars. The database was used to study the glitch activity among the pulsar population, finding that it peaks for pulsars with a characteristic age tau_c ~ 10kyr and decreases for longer values of tau_c, disappearing for objects with tau_c > 20Myr. The glitch act"},"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":"1102.1743","kind":"arxiv","version":2},"metadata":{"license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","primary_cat":"astro-ph.HE","submitted_at":"2011-02-08T22:55:51Z","cross_cats_sorted":[],"title_canon_sha256":"d767bdcc5634a299404e124c7838ffc44a404142124b2a8bbd68ad28d38dbad4","abstract_canon_sha256":"3e7bf9a2475650027e8135ae06aa6e0d1d5f0bf0eb373c66203c6599660748e4"},"schema_version":"1.0"},"receipt":{"kind":"pith_receipt","key_id":"pith-v1-2026-05","algorithm":"ed25519","signed_at":"2026-05-18T02:22:39.486074Z","signature_b64":"HVmhci5TrMEMWr3VoE2zMaAiZiFzyZ6OhcO8z8qMKl+MQbvZz9pFinOTsS3y5+vi4crm7Dua7/Xw541D4aNBDA==","signed_message":"canonical_sha256_bytes","builder_version":"pith-number-builder-2026-05-17-v1","receipt_version":"0.3","canonical_sha256":"1b1dfcf754a359f6c460bb8b209fd472c036269958fcacee38735e255ca13aa3","last_reissued_at":"2026-05-18T02:22:39.485398Z","signature_status":"signed_v1","first_computed_at":"2026-05-18T02:22:39.485398Z","public_key_fingerprint":"8d4b5ee74e4693bcd1df2446408b0d54"},"graph_snapshot":{"paper":{"title":"A study of 315 glitches in the rotation of 102 pulsars","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","headline":"","cross_cats":[],"primary_cat":"astro-ph.HE","authors_text":"Andrew G. Lyne, Ben W. Stappers, Cristobal M. Espinoza, Michael Kramer","submitted_at":"2011-02-08T22:55:51Z","abstract_excerpt":"The rotation of more than 700 pulsars has been monitored using the 76-m Lovell Telescope at Jodrell Bank. Here we report on a new search for glitches in the observations, revealing 128 new glitches in the rotation of 63 pulsars. Combining these new data with those already published we present a database containing 315 glitches in 102 pulsars. The database was used to study the glitch activity among the pulsar population, finding that it peaks for pulsars with a characteristic age tau_c ~ 10kyr and decreases for longer values of tau_c, disappearing for objects with tau_c > 20Myr. The glitch act"},"claims":{"count":0,"items":[],"snapshot_sha256":"258153158e38e3291e3d48162225fcdb2d5a3ed65a07baac614ab91432fd4f57"},"source":{"id":"1102.1743","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":""},"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":"1102.1743","created_at":"2026-05-18T02:22:39.485517+00:00"},{"alias_kind":"arxiv_version","alias_value":"1102.1743v2","created_at":"2026-05-18T02:22:39.485517+00:00"},{"alias_kind":"doi","alias_value":"10.48550/arxiv.1102.1743","created_at":"2026-05-18T02:22:39.485517+00:00"},{"alias_kind":"pith_short_12","alias_value":"DMO7Z52UUNM7","created_at":"2026-05-18T12:26:26.731475+00:00"},{"alias_kind":"pith_short_16","alias_value":"DMO7Z52UUNM7NRDA","created_at":"2026-05-18T12:26:26.731475+00:00"},{"alias_kind":"pith_short_8","alias_value":"DMO7Z52U","created_at":"2026-05-18T12:26:26.731475+00:00"}],"events":[],"event_summary":{},"paper_claims":[],"inbound_citations":{"count":2,"internal_anchor_count":1,"sample":[{"citing_arxiv_id":"1907.04654","citing_title":"Phase transitions in neutron stars and their links to gravitational waves","ref_index":142,"is_internal_anchor":true},{"citing_arxiv_id":"2604.08373","citing_title":"Stochastic problems in pulsar timing","ref_index":112,"is_internal_anchor":false}]},"formal_canon":{"evidence_count":0,"sample":[],"anchors":[]},"links":{"html":"https://pith.science/pith/DMO7Z52UUNM7NRDAXOFSBH6UOL","json":"https://pith.science/pith/DMO7Z52UUNM7NRDAXOFSBH6UOL.json","graph_json":"https://pith.science/api/pith-number/DMO7Z52UUNM7NRDAXOFSBH6UOL/graph.json","events_json":"https://pith.science/api/pith-number/DMO7Z52UUNM7NRDAXOFSBH6UOL/events.json","paper":"https://pith.science/paper/DMO7Z52U"},"agent_actions":{"view_html":"https://pith.science/pith/DMO7Z52UUNM7NRDAXOFSBH6UOL","download_json":"https://pith.science/pith/DMO7Z52UUNM7NRDAXOFSBH6UOL.json","view_paper":"https://pith.science/paper/DMO7Z52U","resolve_alias":"https://pith.science/api/pith-number/resolve?arxiv=1102.1743&json=true","fetch_graph":"https://pith.science/api/pith-number/DMO7Z52UUNM7NRDAXOFSBH6UOL/graph.json","fetch_events":"https://pith.science/api/pith-number/DMO7Z52UUNM7NRDAXOFSBH6UOL/events.json","actions":{"anchor_timestamp":"https://pith.science/pith/DMO7Z52UUNM7NRDAXOFSBH6UOL/action/timestamp_anchor","attest_storage":"https://pith.science/pith/DMO7Z52UUNM7NRDAXOFSBH6UOL/action/storage_attestation","attest_author":"https://pith.science/pith/DMO7Z52UUNM7NRDAXOFSBH6UOL/action/author_attestation","sign_citation":"https://pith.science/pith/DMO7Z52UUNM7NRDAXOFSBH6UOL/action/citation_signature","submit_replication":"https://pith.science/pith/DMO7Z52UUNM7NRDAXOFSBH6UOL/action/replication_record"}},"created_at":"2026-05-18T02:22:39.485517+00:00","updated_at":"2026-05-18T02:22:39.485517+00:00"}