{"as_of":"2026-08-14T06:46:00Z","caps":{"database_statements":6,"inbound":100,"outbound":100},"context_digest":"sha256:996efd5a62fc73c5eef78714de7237d9373ad476368c1bcae0d4ff3214d91b8e","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":1,"lane":"standing_notices","note":"One-hop event checks from named stored sources.","records_observed":1,"source":"scholarly_work_events, retraction_status_cache","source_observed_at":"2026-08-14T06:32:32.682623+00:00","state":"measured"},{"denominator":1,"lane":"inbound_itemization","note":"Pith citing papers itemized under the disclosed page cap.","records_observed":1,"source":"paper_references, paper_reference_links","source_observed_at":"2026-08-01T07:01:56.885136Z","state":"measured"},{"denominator":1,"lane":"external_citation_measurements","note":"A source-named dated measurement, never combined with another source.","records_observed":0,"source":"cited_works","source_observed_at":null,"state":"measured"}],"external_citation_measurements":[],"inbound":[{"citation":{"cited_paper":{"arxiv_id":"1212.2532","last_updated":"2012-12-11T16:47:00Z","snapshot_observed_at":"2026-07-06T03:01:45.479586Z","submitted_at":"2012-12-11T16:47:00Z","title":"The accretion flow to the intermittent accreting ms pulsar, HETE J1900.1-2455, as observed by XMM-Newton and RXTE","version":1},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"1212.2532","snapshot_observed_at":"2026-08-01T07:01:56.885136Z","title":", keywords =","venue":null,"work_id":null,"year":null},"citing_paper":{"arxiv_id":"2607.21587","last_updated":"2026-07-23T17:57:52Z","snapshot_observed_at":"2026-08-09T14:04:39.476184Z","submitted_at":"2026-07-23T17:57:52Z","title":"XMM-Newton and Swift Unveil Another X-Ray Transient in NGC 4945, XMM J130514.64-493311.27","version":1},"reference_index":8,"source":"arxiv_source","source_observed_at":"2026-08-01T07:01:56.885136Z"},"links":{"cited_paper":"/paper/1212.2532","citing_paper":"/paper/2607.21587"},"observation_digest":"sha256:a0fa843181d676180efb3dff932d1da764a6f6a1ed8b77314105c5d73f1395f7","observation_id":"4bd4a916-ccdf-438c-bba6-5a48ea2cd832","resolution":{"observed_at":"2026-08-01T07:01:56.885136Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}}],"links":{"evidence":"/evidence","html":"/paper/1212.2532/citation-record","integrity":"/paper/1212.2532/integrity","json":"/paper/1212.2532/citation-record.json","paper":"/paper/1212.2532"},"outbound":[],"paper":{"arxiv_id":"1212.2532","last_updated":"2012-12-11T16:47:00Z","latest_version":1,"primary_category":"astro-ph.HE","snapshot_observed_at":"2026-07-06T03:01:45.479586Z","submitted_at":"2012-12-11T16:47:00Z","title":"The accretion flow to the intermittent accreting ms pulsar, HETE J1900.1-2455, as observed by XMM-Newton and RXTE"},"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":"2026-08-14T06:32:32.682623+00:00","source":"crossref"},{"observed_at":"2026-08-14T06:32:18.44784+00:00","source":"retraction_watch"}],"thesis":"As of 14 August 2026, this Paper Citation Record lists 0 of 0 outbound references and 1 inbound Pith citation observation for arXiv:1212.2532."}