{"record_type":"pith_number_record","schema_url":"https://pith.science/schemas/pith-number/v1.json","pith_number":"pith:2011:7GQERXKW6D6LCLUUPQ5WOO2IWK","short_pith_number":"pith:7GQERXKW","schema_version":"1.0","canonical_sha256":"f9a048dd56f0fcb12e947c3b673b48b2a91556990774d87e8d3fbdd43f46edc2","source":{"kind":"arxiv","id":"1106.0897","version":1},"attestation_state":"computed","paper":{"title":"Five and a half roads to form a millisecond pulsar","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","headline":"","cross_cats":["astro-ph.SR"],"primary_cat":"astro-ph.HE","authors_text":"Thomas M. Tauris","submitted_at":"2011-06-05T13:20:49Z","abstract_excerpt":"In this review I discuss the characteristics and the formation of all classes of millisecond pulsars (MSPs). The main focus is on the stellar astrophysics of X-ray binaries leading to the production of fully recycled MSPs with white dwarf (WD) or substellar semi-degenerate companions. Depending on the nature of the companion star MSPs are believed to form from either low-mass X-ray binaries (LMXBs) or intermediate-mass X-ray binaries (IMXBs). For each of these two classes of X-ray binaries the evolutionary status of the donor star -- or equivalently, the orbital period -- at the onset of the R"},"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":"1106.0897","kind":"arxiv","version":1},"metadata":{"license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","primary_cat":"astro-ph.HE","submitted_at":"2011-06-05T13:20:49Z","cross_cats_sorted":["astro-ph.SR"],"title_canon_sha256":"755dbb32ca796a95b799e0ab31c3c7f78aebac71147f726aca38a7b884c25a00","abstract_canon_sha256":"5ff7d60aa6795d3adaf68bce38f27fc02df1d389a9508f3e9dd6220ed13a40e1"},"schema_version":"1.0"},"receipt":{"kind":"pith_receipt","key_id":"pith-v1-2026-05","algorithm":"ed25519","signed_at":"2026-05-18T02:21:44.116863Z","signature_b64":"cePoNlu0nnGiH0F/ju7YCWU0ugQw8Bal2gKKMo6B1WUXUOeHfVBD2DTqxqu3uMdXlQ+92NG9mw2z/XOJOWUFCw==","signed_message":"canonical_sha256_bytes","builder_version":"pith-number-builder-2026-05-17-v1","receipt_version":"0.3","canonical_sha256":"f9a048dd56f0fcb12e947c3b673b48b2a91556990774d87e8d3fbdd43f46edc2","last_reissued_at":"2026-05-18T02:21:44.116494Z","signature_status":"signed_v1","first_computed_at":"2026-05-18T02:21:44.116494Z","public_key_fingerprint":"8d4b5ee74e4693bcd1df2446408b0d54"},"graph_snapshot":{"paper":{"title":"Five and a half roads to form a millisecond pulsar","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","headline":"","cross_cats":["astro-ph.SR"],"primary_cat":"astro-ph.HE","authors_text":"Thomas M. Tauris","submitted_at":"2011-06-05T13:20:49Z","abstract_excerpt":"In this review I discuss the characteristics and the formation of all classes of millisecond pulsars (MSPs). The main focus is on the stellar astrophysics of X-ray binaries leading to the production of fully recycled MSPs with white dwarf (WD) or substellar semi-degenerate companions. Depending on the nature of the companion star MSPs are believed to form from either low-mass X-ray binaries (LMXBs) or intermediate-mass X-ray binaries (IMXBs). For each of these two classes of X-ray binaries the evolutionary status of the donor star -- or equivalently, the orbital period -- at the onset of the R"},"claims":{"count":0,"items":[],"snapshot_sha256":"258153158e38e3291e3d48162225fcdb2d5a3ed65a07baac614ab91432fd4f57"},"source":{"id":"1106.0897","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":"1106.0897","created_at":"2026-05-18T02:21:44.116551+00:00"},{"alias_kind":"arxiv_version","alias_value":"1106.0897v1","created_at":"2026-05-18T02:21:44.116551+00:00"},{"alias_kind":"doi","alias_value":"10.48550/arxiv.1106.0897","created_at":"2026-05-18T02:21:44.116551+00:00"},{"alias_kind":"pith_short_12","alias_value":"7GQERXKW6D6L","created_at":"2026-05-18T12:26:22.705136+00:00"},{"alias_kind":"pith_short_16","alias_value":"7GQERXKW6D6LCLUU","created_at":"2026-05-18T12:26:22.705136+00:00"},{"alias_kind":"pith_short_8","alias_value":"7GQERXKW","created_at":"2026-05-18T12:26:22.705136+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/7GQERXKW6D6LCLUUPQ5WOO2IWK","json":"https://pith.science/pith/7GQERXKW6D6LCLUUPQ5WOO2IWK.json","graph_json":"https://pith.science/api/pith-number/7GQERXKW6D6LCLUUPQ5WOO2IWK/graph.json","events_json":"https://pith.science/api/pith-number/7GQERXKW6D6LCLUUPQ5WOO2IWK/events.json","paper":"https://pith.science/paper/7GQERXKW"},"agent_actions":{"view_html":"https://pith.science/pith/7GQERXKW6D6LCLUUPQ5WOO2IWK","download_json":"https://pith.science/pith/7GQERXKW6D6LCLUUPQ5WOO2IWK.json","view_paper":"https://pith.science/paper/7GQERXKW","resolve_alias":"https://pith.science/api/pith-number/resolve?arxiv=1106.0897&json=true","fetch_graph":"https://pith.science/api/pith-number/7GQERXKW6D6LCLUUPQ5WOO2IWK/graph.json","fetch_events":"https://pith.science/api/pith-number/7GQERXKW6D6LCLUUPQ5WOO2IWK/events.json","actions":{"anchor_timestamp":"https://pith.science/pith/7GQERXKW6D6LCLUUPQ5WOO2IWK/action/timestamp_anchor","attest_storage":"https://pith.science/pith/7GQERXKW6D6LCLUUPQ5WOO2IWK/action/storage_attestation","attest_author":"https://pith.science/pith/7GQERXKW6D6LCLUUPQ5WOO2IWK/action/author_attestation","sign_citation":"https://pith.science/pith/7GQERXKW6D6LCLUUPQ5WOO2IWK/action/citation_signature","submit_replication":"https://pith.science/pith/7GQERXKW6D6LCLUUPQ5WOO2IWK/action/replication_record"}},"created_at":"2026-05-18T02:21:44.116551+00:00","updated_at":"2026-05-18T02:21:44.116551+00:00"}