{"record_type":"pith_number_record","schema_url":"https://pith.science/schemas/pith-number/v1.json","pith_number":"pith:2013:5526R7E3THJ3VSARNFFHEMCZX2","short_pith_number":"pith:5526R7E3","schema_version":"1.0","canonical_sha256":"ef75e8fc9b99d3bac811694a723059beaff33d4409ef0564973c956ed5638ebf","source":{"kind":"arxiv","id":"1310.7549","version":2},"attestation_state":"computed","paper":{"title":"A New Accretion Disk Around the Missing Link Binary System PSR J1023+0038","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","headline":"","cross_cats":[],"primary_cat":"astro-ph.HE","authors_text":"A.G. Lyne (Manchester), A.M. Archibald (ASTRON), A. Patruno (Leiden/ASTRON), B.W. Stappers (Manchester), C.G. Bassa (ASTRON), G.H. Janssen (ASTRON), J.W.T. Hessels (ASTRON/Amsterdam), S. Bogdanov (Columbia), S. Tendulkar (Caltech), V.M. Kaspi (McGill)","submitted_at":"2013-10-28T19:36:41Z","abstract_excerpt":"PSR J1023+0038 is an exceptional system for understanding how slowly rotating neutron stars are spun up to millisecond rotational periods through accretion from a companion star. Observed as a radio pulsar from 2007-2013, optical data showed that the system had an accretion disk in 2000/2001. Starting at the end of 2013 June, the radio pulsar has become undetectable, suggesting a return to the previous accretion-disk state, where the system more closely resembles an X-ray binary. In this Letter we report the first targeted X-ray observations ever performed of the active phase and complement th"},"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":"1310.7549","kind":"arxiv","version":2},"metadata":{"license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","primary_cat":"astro-ph.HE","submitted_at":"2013-10-28T19:36:41Z","cross_cats_sorted":[],"title_canon_sha256":"7962b79313e26446cd71890c7867aeb6152acd39ea3668a8903aa8dd66b99b5a","abstract_canon_sha256":"82a688f9f4add6574067b59712f50fc12dccb671f62607e4a665b1ea58775b36"},"schema_version":"1.0"},"receipt":{"kind":"pith_receipt","key_id":"pith-v1-2026-05","algorithm":"ed25519","signed_at":"2026-05-18T01:46:48.459903Z","signature_b64":"xqbwQM5xNqPyqNnjBWMg1hoDPThbTDPhRvKZMcMRMQq0iQv0IhCdji+YlI3zr09JvwvVCZt98E6Saj26cGTcCw==","signed_message":"canonical_sha256_bytes","builder_version":"pith-number-builder-2026-05-17-v1","receipt_version":"0.3","canonical_sha256":"ef75e8fc9b99d3bac811694a723059beaff33d4409ef0564973c956ed5638ebf","last_reissued_at":"2026-05-18T01:46:48.459330Z","signature_status":"signed_v1","first_computed_at":"2026-05-18T01:46:48.459330Z","public_key_fingerprint":"8d4b5ee74e4693bcd1df2446408b0d54"},"graph_snapshot":{"paper":{"title":"A New Accretion Disk Around the Missing Link Binary System PSR J1023+0038","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","headline":"","cross_cats":[],"primary_cat":"astro-ph.HE","authors_text":"A.G. Lyne (Manchester), A.M. Archibald (ASTRON), A. Patruno (Leiden/ASTRON), B.W. Stappers (Manchester), C.G. Bassa (ASTRON), G.H. Janssen (ASTRON), J.W.T. Hessels (ASTRON/Amsterdam), S. Bogdanov (Columbia), S. Tendulkar (Caltech), V.M. Kaspi (McGill)","submitted_at":"2013-10-28T19:36:41Z","abstract_excerpt":"PSR J1023+0038 is an exceptional system for understanding how slowly rotating neutron stars are spun up to millisecond rotational periods through accretion from a companion star. Observed as a radio pulsar from 2007-2013, optical data showed that the system had an accretion disk in 2000/2001. Starting at the end of 2013 June, the radio pulsar has become undetectable, suggesting a return to the previous accretion-disk state, where the system more closely resembles an X-ray binary. In this Letter we report the first targeted X-ray observations ever performed of the active phase and complement th"},"claims":{"count":0,"items":[],"snapshot_sha256":"258153158e38e3291e3d48162225fcdb2d5a3ed65a07baac614ab91432fd4f57"},"source":{"id":"1310.7549","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":"1310.7549","created_at":"2026-05-18T01:46:48.459428+00:00"},{"alias_kind":"arxiv_version","alias_value":"1310.7549v2","created_at":"2026-05-18T01:46:48.459428+00:00"},{"alias_kind":"doi","alias_value":"10.48550/arxiv.1310.7549","created_at":"2026-05-18T01:46:48.459428+00:00"},{"alias_kind":"pith_short_12","alias_value":"5526R7E3THJ3","created_at":"2026-05-18T12:27:34.582898+00:00"},{"alias_kind":"pith_short_16","alias_value":"5526R7E3THJ3VSAR","created_at":"2026-05-18T12:27:34.582898+00:00"},{"alias_kind":"pith_short_8","alias_value":"5526R7E3","created_at":"2026-05-18T12:27:34.582898+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/5526R7E3THJ3VSARNFFHEMCZX2","json":"https://pith.science/pith/5526R7E3THJ3VSARNFFHEMCZX2.json","graph_json":"https://pith.science/api/pith-number/5526R7E3THJ3VSARNFFHEMCZX2/graph.json","events_json":"https://pith.science/api/pith-number/5526R7E3THJ3VSARNFFHEMCZX2/events.json","paper":"https://pith.science/paper/5526R7E3"},"agent_actions":{"view_html":"https://pith.science/pith/5526R7E3THJ3VSARNFFHEMCZX2","download_json":"https://pith.science/pith/5526R7E3THJ3VSARNFFHEMCZX2.json","view_paper":"https://pith.science/paper/5526R7E3","resolve_alias":"https://pith.science/api/pith-number/resolve?arxiv=1310.7549&json=true","fetch_graph":"https://pith.science/api/pith-number/5526R7E3THJ3VSARNFFHEMCZX2/graph.json","fetch_events":"https://pith.science/api/pith-number/5526R7E3THJ3VSARNFFHEMCZX2/events.json","actions":{"anchor_timestamp":"https://pith.science/pith/5526R7E3THJ3VSARNFFHEMCZX2/action/timestamp_anchor","attest_storage":"https://pith.science/pith/5526R7E3THJ3VSARNFFHEMCZX2/action/storage_attestation","attest_author":"https://pith.science/pith/5526R7E3THJ3VSARNFFHEMCZX2/action/author_attestation","sign_citation":"https://pith.science/pith/5526R7E3THJ3VSARNFFHEMCZX2/action/citation_signature","submit_replication":"https://pith.science/pith/5526R7E3THJ3VSARNFFHEMCZX2/action/replication_record"}},"created_at":"2026-05-18T01:46:48.459428+00:00","updated_at":"2026-05-18T01:46:48.459428+00:00"}