{"record_type":"pith_number_record","schema_url":"https://pith.science/schemas/pith-number/v1.json","pith_number":"pith:2000:ZRHHHCRZ4NGZ7BIZRN2C74XYRU","short_pith_number":"pith:ZRHHHCRZ","schema_version":"1.0","canonical_sha256":"cc4e738a39e34d9f85198b742ff2f88d3eeac25411d54eb79e4189a2c80e47fc","source":{"kind":"arxiv","id":"astro-ph/0005561","version":1},"attestation_state":"computed","paper":{"title":"Glitches in Southern Pulsars","license":"","headline":"","cross_cats":[],"primary_cat":"astro-ph","authors_text":"A. G. Lyne, B. W. Stappers, M. Bailes, N. Wang, R. N. Manchester, R. T. Pace, V. M. Kaspi","submitted_at":"2000-05-30T04:48:37Z","abstract_excerpt":"Timing observations of 40 mostly young pulsars using the ATNF Parkes radio telescope between 1990 January and 1998 December are reported. In total, 20 previously unreported glitches and ten other glitches were detected in 11 pulsars. These included 12 glitches in PSR J1341$- $6220, corresponding to a glitch rate of 1.5 glitches per year. We also detected the largest known glitch, in PSR J1614$-$5047, with $\\Delta\\nu_g/\\nu \\approx 6.5 \\times 10^{-6}$ where $\\nu = 1/P$ is the pulse frequency. Glitch parameters were determined both by extrapolating timing solutions to inter-glitch intervals and b"},"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":"astro-ph/0005561","kind":"arxiv","version":1},"metadata":{"license":"","primary_cat":"astro-ph","submitted_at":"2000-05-30T04:48:37Z","cross_cats_sorted":[],"title_canon_sha256":"39acebf7bec17d2a52ff3365d9056991754a73db60ab1efed9ee0109ee949cc5","abstract_canon_sha256":"b773aa78e670885b289d558962a50868cf5615a284c1f4d958ce00d794a0e88e"},"schema_version":"1.0"},"receipt":{"kind":"pith_receipt","key_id":"pith-v1-2026-05","algorithm":"ed25519","signed_at":"2026-07-04T16:16:44.251733Z","signature_b64":"fN5Z6pHltLH6YJtMwmIbXO7H5ymFQz7jf0kdUh0HxW9ezKZvoaGjTj/fngVAHLNpNBI/D83zaRZXzUvKJMKFDA==","signed_message":"canonical_sha256_bytes","builder_version":"pith-number-builder-2026-05-17-v1","receipt_version":"0.3","canonical_sha256":"cc4e738a39e34d9f85198b742ff2f88d3eeac25411d54eb79e4189a2c80e47fc","last_reissued_at":"2026-07-04T16:16:44.251280Z","signature_status":"signed_v1","first_computed_at":"2026-07-04T16:16:44.251280Z","public_key_fingerprint":"8d4b5ee74e4693bcd1df2446408b0d54"},"graph_snapshot":{"paper":{"title":"Glitches in Southern Pulsars","license":"","headline":"","cross_cats":[],"primary_cat":"astro-ph","authors_text":"A. G. Lyne, B. W. Stappers, M. Bailes, N. Wang, R. N. Manchester, R. T. Pace, V. M. Kaspi","submitted_at":"2000-05-30T04:48:37Z","abstract_excerpt":"Timing observations of 40 mostly young pulsars using the ATNF Parkes radio telescope between 1990 January and 1998 December are reported. In total, 20 previously unreported glitches and ten other glitches were detected in 11 pulsars. These included 12 glitches in PSR J1341$- $6220, corresponding to a glitch rate of 1.5 glitches per year. We also detected the largest known glitch, in PSR J1614$-$5047, with $\\Delta\\nu_g/\\nu \\approx 6.5 \\times 10^{-6}$ where $\\nu = 1/P$ is the pulse frequency. Glitch parameters were determined both by extrapolating timing solutions to inter-glitch intervals and b"},"claims":{"count":0,"items":[],"snapshot_sha256":"258153158e38e3291e3d48162225fcdb2d5a3ed65a07baac614ab91432fd4f57"},"source":{"id":"astro-ph/0005561","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":""},"integrity":{"clean":true,"summary":{"advisory":0,"critical":0,"by_detector":{},"informational":0},"endpoint":"/pith/astro-ph/0005561/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":"astro-ph/0005561","created_at":"2026-07-04T16:16:44.251371+00:00"},{"alias_kind":"arxiv_version","alias_value":"astro-ph/0005561v1","created_at":"2026-07-04T16:16:44.251371+00:00"},{"alias_kind":"doi","alias_value":"10.48550/arxiv.astro-ph/0005561","created_at":"2026-07-04T16:16:44.251371+00:00"},{"alias_kind":"pith_short_12","alias_value":"ZRHHHCRZ4NGZ","created_at":"2026-07-04T16:16:44.251371+00:00"},{"alias_kind":"pith_short_16","alias_value":"ZRHHHCRZ4NGZ7BIZ","created_at":"2026-07-04T16:16:44.251371+00:00"},{"alias_kind":"pith_short_8","alias_value":"ZRHHHCRZ","created_at":"2026-07-04T16:16:44.251371+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/ZRHHHCRZ4NGZ7BIZRN2C74XYRU","json":"https://pith.science/pith/ZRHHHCRZ4NGZ7BIZRN2C74XYRU.json","graph_json":"https://pith.science/api/pith-number/ZRHHHCRZ4NGZ7BIZRN2C74XYRU/graph.json","events_json":"https://pith.science/api/pith-number/ZRHHHCRZ4NGZ7BIZRN2C74XYRU/events.json","paper":"https://pith.science/paper/ZRHHHCRZ"},"agent_actions":{"view_html":"https://pith.science/pith/ZRHHHCRZ4NGZ7BIZRN2C74XYRU","download_json":"https://pith.science/pith/ZRHHHCRZ4NGZ7BIZRN2C74XYRU.json","view_paper":"https://pith.science/paper/ZRHHHCRZ","resolve_alias":"https://pith.science/api/pith-number/resolve?arxiv=astro-ph/0005561&json=true","fetch_graph":"https://pith.science/api/pith-number/ZRHHHCRZ4NGZ7BIZRN2C74XYRU/graph.json","fetch_events":"https://pith.science/api/pith-number/ZRHHHCRZ4NGZ7BIZRN2C74XYRU/events.json","actions":{"anchor_timestamp":"https://pith.science/pith/ZRHHHCRZ4NGZ7BIZRN2C74XYRU/action/timestamp_anchor","attest_storage":"https://pith.science/pith/ZRHHHCRZ4NGZ7BIZRN2C74XYRU/action/storage_attestation","attest_author":"https://pith.science/pith/ZRHHHCRZ4NGZ7BIZRN2C74XYRU/action/author_attestation","sign_citation":"https://pith.science/pith/ZRHHHCRZ4NGZ7BIZRN2C74XYRU/action/citation_signature","submit_replication":"https://pith.science/pith/ZRHHHCRZ4NGZ7BIZRN2C74XYRU/action/replication_record"}},"created_at":"2026-07-04T16:16:44.251371+00:00","updated_at":"2026-07-04T16:16:44.251371+00:00"}