{"as_of":"2026-08-16T11:11:00Z","caps":{"database_statements":6,"inbound":100,"outbound":100},"context_digest":"sha256:24f02637581eb73b4cbff6528825482c77fe4193658d36f2f0c231e65dca73f4","coverage":[{"denominator":0,"lane":"reference_resolution","note":"Typed states for the displayed outbound observations.","records_observed":0,"source":"paper_references, paper_reference_links","source_observed_at":null,"state":"measured"},{"denominator":3,"lane":"standing_notices","note":"One-hop event checks from named stored sources.","records_observed":3,"source":"scholarly_work_events, retraction_status_cache","source_observed_at":"2026-08-16T06:30:59.297886+00:00","state":"measured"},{"denominator":3,"lane":"inbound_itemization","note":"Pith citing papers itemized under the disclosed page cap.","records_observed":3,"source":"paper_references, paper_reference_links","source_observed_at":"2026-08-12T18:32:10.867839Z","state":"measured"},{"denominator":1,"lane":"external_citation_measurements","note":"A source-named dated measurement, never combined with another source.","records_observed":0,"source":"pith","source_observed_at":"2026-07-13T14:39:39.609319Z","state":"measured"}],"external_citation_measurements":[],"inbound":[{"citation":{"cited_paper":{"arxiv_id":"2006.10448","last_updated":"2020-08-24T18:30:05Z","snapshot_observed_at":"2026-08-04T11:56:11.954838Z","submitted_at":"2020-06-18T11:55:16Z","title":"Relativistic rotating vector model for X-ray millisecond pulsars","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2006.10448","snapshot_observed_at":"2026-08-07T05:18:36.581733Z","title":"Poutanen ,\\ 10.1051/0004-6361/202038689 journal journal \\ volume 641 ,\\ eid A166 ( year 2020 ) ,\\ http://arxiv.org/abs/2006.10448 arXiv:2006.10448 [astro-ph.HE] NoStop","venue":null,"work_id":null,"year":2020},"citing_paper":{"arxiv_id":"2506.08369","last_updated":"2025-09-08T08:13:57Z","snapshot_observed_at":"2026-08-14T07:11:05.914769Z","submitted_at":"2025-06-10T02:28:03Z","title":"Physics of Strong Magnetism with eXTP","version":2},"reference_index":36,"source":"arxiv_source","source_observed_at":"2026-08-07T05:18:36.581733Z"},"links":{"cited_paper":"/paper/2006.10448","citing_paper":"/paper/2506.08369"},"observation_digest":"sha256:85b70d669facb7cade0b2057ce26c3b080ced3d02b3e25dd537f731754d69aac","observation_id":"b776c4c8-3e89-42e9-9089-85f9db293628","resolution":{"observed_at":"2026-08-07T05:18:36.581733Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2006.10448","last_updated":"2020-08-24T18:30:05Z","snapshot_observed_at":"2026-08-04T11:56:11.954838Z","submitted_at":"2020-06-18T11:55:16Z","title":"Relativistic rotating vector model for X-ray millisecond pulsars","version":2},"cited_work":{"arxiv_id":"2006.10448","doi":null,"metadata_source":"pith","pith_arxiv_id":"2006.10448","snapshot_observed_at":"2026-07-13T14:39:39.609319Z","title":"Relativistic rotating vector model for X-ray millisecond pulsars","venue":"astro-ph.HE","work_id":"20978b3e-0205-4249-8b6f-5ad6fa33f3f4","year":2020},"citing_paper":{"arxiv_id":"2604.01219","last_updated":"2026-04-01T17:57:47Z","snapshot_observed_at":"2026-08-14T17:43:52.011218Z","submitted_at":"2026-04-01T17:57:47Z","title":"Information content of JWST transmission spectroscopy of the exoplanet HAT-P-12b from the optical to the mid-infrared","version":1},"reference_index":46,"source":"pdf_text","source_observed_at":"2026-07-13T14:30:13.573690Z"},"links":{"cited_paper":"/paper/2006.10448","citing_paper":"/paper/2604.01219"},"observation_digest":"sha256:da11d225607cbcb078b7dd0af34bab6645fa1247ed4811b1a2ccbef43d4c8a45","observation_id":"c94cf2b9-b437-4ee2-8ef4-0f0c665f7f0b","resolution":{"observed_at":"2026-07-13T14:39:39.611376Z","resolver_source":"local_arxiv","status":"verified_exact"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-16T06:30:59.297886+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-16T06:30:59.297886+00:00","source":"crossref"},{"observed_at":"2026-08-16T06:30:54.164669+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":{"arxiv_id":"2006.10448","last_updated":"2020-08-24T18:30:05Z","snapshot_observed_at":"2026-08-04T11:56:11.954838Z","submitted_at":"2020-06-18T11:55:16Z","title":"Relativistic rotating vector model for X-ray millisecond pulsars","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2006.10448","snapshot_observed_at":"2026-08-12T18:32:10.867839Z","title":", keywords =","venue":null,"work_id":null,"year":2006},"citing_paper":{"arxiv_id":"2608.10733","last_updated":"2026-08-11T09:53:11Z","snapshot_observed_at":"2026-08-15T09:06:37.337125Z","submitted_at":"2026-08-11T09:53:11Z","title":"Real-time observations of the transition to the quiescent state in an accreting magnetised neutron star: No propeller required?","version":1},"reference_index":71,"source":"arxiv_source","source_observed_at":"2026-08-12T18:32:10.867839Z"},"links":{"cited_paper":"/paper/2006.10448","citing_paper":"/paper/2608.10733"},"observation_digest":"sha256:f5c2834c2fb26740c717a40e96c3fae4c0b3f5786ef82b804a1caa3572a3a83d","observation_id":"37c35596-86b0-41c9-a35f-f3f9602e74ba","resolution":{"observed_at":"2026-08-12T18:32:10.867839Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}}],"links":{"evidence":"/evidence","html":"/paper/2006.10448/citation-record","integrity":"/paper/2006.10448/integrity","json":"/paper/2006.10448/citation-record.json","paper":"/paper/2006.10448"},"outbound":[],"paper":{"arxiv_id":"2006.10448","last_updated":"2020-08-24T18:30:05Z","latest_version":2,"primary_category":"astro-ph.HE","snapshot_observed_at":"2026-08-04T11:56:11.954838Z","submitted_at":"2020-06-18T11:55:16Z","title":"Relativistic rotating vector model for X-ray millisecond pulsars"},"reference_resolution":{"displayed":0,"state_counts":{"malformed_identifier":0,"metadata_mismatch":0,"parse_uncertain":0,"unresolved":0,"verified_exact":0,"verified_fuzzy":0},"total_outbound_references":0},"refusal":"A citation records a reference. It does not transfer a finding from one paper to another.","schema":"pith.paper-citation-record.v1","standing_sources":[{"observed_at":"2026-08-16T06:30:59.297886+00:00","source":"crossref"},{"observed_at":"2026-08-16T06:30:54.164669+00:00","source":"retraction_watch"}],"thesis":"As of 16 August 2026, this Paper Citation Record lists 0 of 0 outbound references and 3 inbound Pith citation observations for arXiv:2006.10448."}