{"record_type":"pith_number_record","schema_url":"https://pith.science/schemas/pith-number/v1.json","pith_number":"pith:2013:LJLLYW3TS4J7AP5IMF4DMSMI3Z","short_pith_number":"pith:LJLLYW3T","schema_version":"1.0","canonical_sha256":"5a56bc5b739713f03fa86178364988de742b27be468e3f11fa90d94b4fed84ee","source":{"kind":"arxiv","id":"1306.5214","version":1},"attestation_state":"computed","paper":{"title":"Glitch recoveries in radio-pulsars and magnetars","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","headline":"","cross_cats":["astro-ph.HE"],"primary_cat":"astro-ph.SR","authors_text":"Brynmor Haskell, Danai Antonopoulou","submitted_at":"2013-06-21T18:55:42Z","abstract_excerpt":"Pulsar glitches are sudden increases in the spin frequency of an otherwise steadily spinning down neutron star. These events are thought to represent a direct probe of the dynamics of the superfluid interior of the star. However glitches can differ significantly from one another, not only in size and frequency, but also in the post-glitch response of the star. Some appear as simple steps in frequency, while others also display an increase in spin-down rate after the glitch. Others still show several exponentially relaxing components in the post-glitch recovery. We show that if glitches are ind"},"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":"1306.5214","kind":"arxiv","version":1},"metadata":{"license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","primary_cat":"astro-ph.SR","submitted_at":"2013-06-21T18:55:42Z","cross_cats_sorted":["astro-ph.HE"],"title_canon_sha256":"9d453f776253ee9e5b13a26ba553e238ae6d19e193d10c11cfca6f2f5e25a8b3","abstract_canon_sha256":"f78087838a5220d9b21263d84bd262ae6dca6bcdfed09acd61c786369f398766"},"schema_version":"1.0"},"receipt":{"kind":"pith_receipt","key_id":"pith-v1-2026-05","algorithm":"ed25519","signed_at":"2026-05-18T01:49:13.876023Z","signature_b64":"r47jhzuSEIL4ovzhbNVTqJfg+IyP6u+PSjrNkKr3JpiNpS9ceyLqklNxbs9R6RKF4Cf9dERFVBAzr2Znx64xDA==","signed_message":"canonical_sha256_bytes","builder_version":"pith-number-builder-2026-05-17-v1","receipt_version":"0.3","canonical_sha256":"5a56bc5b739713f03fa86178364988de742b27be468e3f11fa90d94b4fed84ee","last_reissued_at":"2026-05-18T01:49:13.875347Z","signature_status":"signed_v1","first_computed_at":"2026-05-18T01:49:13.875347Z","public_key_fingerprint":"8d4b5ee74e4693bcd1df2446408b0d54"},"graph_snapshot":{"paper":{"title":"Glitch recoveries in radio-pulsars and magnetars","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","headline":"","cross_cats":["astro-ph.HE"],"primary_cat":"astro-ph.SR","authors_text":"Brynmor Haskell, Danai Antonopoulou","submitted_at":"2013-06-21T18:55:42Z","abstract_excerpt":"Pulsar glitches are sudden increases in the spin frequency of an otherwise steadily spinning down neutron star. These events are thought to represent a direct probe of the dynamics of the superfluid interior of the star. However glitches can differ significantly from one another, not only in size and frequency, but also in the post-glitch response of the star. Some appear as simple steps in frequency, while others also display an increase in spin-down rate after the glitch. Others still show several exponentially relaxing components in the post-glitch recovery. We show that if glitches are ind"},"claims":{"count":0,"items":[],"snapshot_sha256":"258153158e38e3291e3d48162225fcdb2d5a3ed65a07baac614ab91432fd4f57"},"source":{"id":"1306.5214","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":"1306.5214","created_at":"2026-05-18T01:49:13.875446+00:00"},{"alias_kind":"arxiv_version","alias_value":"1306.5214v1","created_at":"2026-05-18T01:49:13.875446+00:00"},{"alias_kind":"doi","alias_value":"10.48550/arxiv.1306.5214","created_at":"2026-05-18T01:49:13.875446+00:00"},{"alias_kind":"pith_short_12","alias_value":"LJLLYW3TS4J7","created_at":"2026-05-18T12:27:51.066281+00:00"},{"alias_kind":"pith_short_16","alias_value":"LJLLYW3TS4J7AP5I","created_at":"2026-05-18T12:27:51.066281+00:00"},{"alias_kind":"pith_short_8","alias_value":"LJLLYW3T","created_at":"2026-05-18T12:27:51.066281+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/LJLLYW3TS4J7AP5IMF4DMSMI3Z","json":"https://pith.science/pith/LJLLYW3TS4J7AP5IMF4DMSMI3Z.json","graph_json":"https://pith.science/api/pith-number/LJLLYW3TS4J7AP5IMF4DMSMI3Z/graph.json","events_json":"https://pith.science/api/pith-number/LJLLYW3TS4J7AP5IMF4DMSMI3Z/events.json","paper":"https://pith.science/paper/LJLLYW3T"},"agent_actions":{"view_html":"https://pith.science/pith/LJLLYW3TS4J7AP5IMF4DMSMI3Z","download_json":"https://pith.science/pith/LJLLYW3TS4J7AP5IMF4DMSMI3Z.json","view_paper":"https://pith.science/paper/LJLLYW3T","resolve_alias":"https://pith.science/api/pith-number/resolve?arxiv=1306.5214&json=true","fetch_graph":"https://pith.science/api/pith-number/LJLLYW3TS4J7AP5IMF4DMSMI3Z/graph.json","fetch_events":"https://pith.science/api/pith-number/LJLLYW3TS4J7AP5IMF4DMSMI3Z/events.json","actions":{"anchor_timestamp":"https://pith.science/pith/LJLLYW3TS4J7AP5IMF4DMSMI3Z/action/timestamp_anchor","attest_storage":"https://pith.science/pith/LJLLYW3TS4J7AP5IMF4DMSMI3Z/action/storage_attestation","attest_author":"https://pith.science/pith/LJLLYW3TS4J7AP5IMF4DMSMI3Z/action/author_attestation","sign_citation":"https://pith.science/pith/LJLLYW3TS4J7AP5IMF4DMSMI3Z/action/citation_signature","submit_replication":"https://pith.science/pith/LJLLYW3TS4J7AP5IMF4DMSMI3Z/action/replication_record"}},"created_at":"2026-05-18T01:49:13.875446+00:00","updated_at":"2026-05-18T01:49:13.875446+00:00"}