{"record_type":"pith_number_record","schema_url":"https://pith.science/schemas/pith-number/v1.json","pith_number":"pith:2013:ZPT5PJG34Y44HCC5KIZZF6U7IA","short_pith_number":"pith:ZPT5PJG3","schema_version":"1.0","canonical_sha256":"cbe7d7a4dbe639c3885d523392fa9f400edbfac649a28f20be6b3e8f25af39ae","source":{"kind":"arxiv","id":"1304.6022","version":2},"attestation_state":"computed","paper":{"title":"Long-term evolution of the neutron-star spin period of SXP 1062","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","headline":"","cross_cats":[],"primary_cat":"astro-ph.HE","authors_text":"A. Udalski, F. Haberl, J. S. Gallagher III, L. M. Oskinova, M. P. E. Schurch, R. Sturm, V. H\\'enault-Brunet","submitted_at":"2013-04-22T17:12:19Z","abstract_excerpt":"The Be/X-ray binary SXP1062 is of especial interest owing to the large spin period of the neutron star, its large spin-down rate, and the association with a supernova remnant constraining its age. This makes the source an important probe for accretion physics. To investigate the long-term evolution of the spin period and associated spectral variations, we performed an XMM-Newton target-of-opportunity observation of SXP1062 during X-ray outburst. Spectral and timing analysis of the XMM-Newton data was compared with previous studies, as well as complementary Swift/XRT monitoring and optical spec"},"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":"1304.6022","kind":"arxiv","version":2},"metadata":{"license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","primary_cat":"astro-ph.HE","submitted_at":"2013-04-22T17:12:19Z","cross_cats_sorted":[],"title_canon_sha256":"6375394b790480889d68f795ba151045eb889b71b410915d14529b4ec5a504ac","abstract_canon_sha256":"6b4d1936546a2b62b38f87ca123263934dd4b6de9327abd0d07b828ab05f58ab"},"schema_version":"1.0"},"receipt":{"kind":"pith_receipt","key_id":"pith-v1-2026-05","algorithm":"ed25519","signed_at":"2026-05-18T01:50:23.557754Z","signature_b64":"NKwhHu91A3JTt+NEr5OAacIHRQdJby7nxor79yNN2N6jLrEhl4xJ7mPe22B8xjPTDBiujunuliu+V17WsTMHAw==","signed_message":"canonical_sha256_bytes","builder_version":"pith-number-builder-2026-05-17-v1","receipt_version":"0.3","canonical_sha256":"cbe7d7a4dbe639c3885d523392fa9f400edbfac649a28f20be6b3e8f25af39ae","last_reissued_at":"2026-05-18T01:50:23.557061Z","signature_status":"signed_v1","first_computed_at":"2026-05-18T01:50:23.557061Z","public_key_fingerprint":"8d4b5ee74e4693bcd1df2446408b0d54"},"graph_snapshot":{"paper":{"title":"Long-term evolution of the neutron-star spin period of SXP 1062","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","headline":"","cross_cats":[],"primary_cat":"astro-ph.HE","authors_text":"A. Udalski, F. Haberl, J. S. Gallagher III, L. M. Oskinova, M. P. E. Schurch, R. Sturm, V. H\\'enault-Brunet","submitted_at":"2013-04-22T17:12:19Z","abstract_excerpt":"The Be/X-ray binary SXP1062 is of especial interest owing to the large spin period of the neutron star, its large spin-down rate, and the association with a supernova remnant constraining its age. This makes the source an important probe for accretion physics. To investigate the long-term evolution of the spin period and associated spectral variations, we performed an XMM-Newton target-of-opportunity observation of SXP1062 during X-ray outburst. Spectral and timing analysis of the XMM-Newton data was compared with previous studies, as well as complementary Swift/XRT monitoring and optical spec"},"claims":{"count":0,"items":[],"snapshot_sha256":"258153158e38e3291e3d48162225fcdb2d5a3ed65a07baac614ab91432fd4f57"},"source":{"id":"1304.6022","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":"1304.6022","created_at":"2026-05-18T01:50:23.557164+00:00"},{"alias_kind":"arxiv_version","alias_value":"1304.6022v2","created_at":"2026-05-18T01:50:23.557164+00:00"},{"alias_kind":"doi","alias_value":"10.48550/arxiv.1304.6022","created_at":"2026-05-18T01:50:23.557164+00:00"},{"alias_kind":"pith_short_12","alias_value":"ZPT5PJG34Y44","created_at":"2026-05-18T12:28:09.283467+00:00"},{"alias_kind":"pith_short_16","alias_value":"ZPT5PJG34Y44HCC5","created_at":"2026-05-18T12:28:09.283467+00:00"},{"alias_kind":"pith_short_8","alias_value":"ZPT5PJG3","created_at":"2026-05-18T12:28:09.283467+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/ZPT5PJG34Y44HCC5KIZZF6U7IA","json":"https://pith.science/pith/ZPT5PJG34Y44HCC5KIZZF6U7IA.json","graph_json":"https://pith.science/api/pith-number/ZPT5PJG34Y44HCC5KIZZF6U7IA/graph.json","events_json":"https://pith.science/api/pith-number/ZPT5PJG34Y44HCC5KIZZF6U7IA/events.json","paper":"https://pith.science/paper/ZPT5PJG3"},"agent_actions":{"view_html":"https://pith.science/pith/ZPT5PJG34Y44HCC5KIZZF6U7IA","download_json":"https://pith.science/pith/ZPT5PJG34Y44HCC5KIZZF6U7IA.json","view_paper":"https://pith.science/paper/ZPT5PJG3","resolve_alias":"https://pith.science/api/pith-number/resolve?arxiv=1304.6022&json=true","fetch_graph":"https://pith.science/api/pith-number/ZPT5PJG34Y44HCC5KIZZF6U7IA/graph.json","fetch_events":"https://pith.science/api/pith-number/ZPT5PJG34Y44HCC5KIZZF6U7IA/events.json","actions":{"anchor_timestamp":"https://pith.science/pith/ZPT5PJG34Y44HCC5KIZZF6U7IA/action/timestamp_anchor","attest_storage":"https://pith.science/pith/ZPT5PJG34Y44HCC5KIZZF6U7IA/action/storage_attestation","attest_author":"https://pith.science/pith/ZPT5PJG34Y44HCC5KIZZF6U7IA/action/author_attestation","sign_citation":"https://pith.science/pith/ZPT5PJG34Y44HCC5KIZZF6U7IA/action/citation_signature","submit_replication":"https://pith.science/pith/ZPT5PJG34Y44HCC5KIZZF6U7IA/action/replication_record"}},"created_at":"2026-05-18T01:50:23.557164+00:00","updated_at":"2026-05-18T01:50:23.557164+00:00"}