{"as_of":"2026-08-11T15:22:00Z","caps":{"database_statements":6,"inbound":100,"outbound":100},"context_digest":"sha256:aca4e62b33b65d14458cf49beadb5e173daed3d16611f946a27273df161086bd","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":2,"lane":"standing_notices","note":"One-hop event checks from named stored sources.","records_observed":2,"source":"scholarly_work_events, retraction_status_cache","source_observed_at":"2026-08-11T06:34:44.6726+00:00","state":"measured"},{"denominator":2,"lane":"inbound_itemization","note":"Pith citing papers itemized under the disclosed page cap.","records_observed":2,"source":"paper_references, paper_reference_links","source_observed_at":"2026-08-08T12:40:54.737873Z","state":"measured"},{"denominator":1,"lane":"external_citation_measurements","note":"A source-named dated measurement, never combined with another source.","records_observed":0,"source":"arxiv_reference","source_observed_at":"2026-05-24T22:25:01.609084Z","state":"measured"}],"external_citation_measurements":[],"inbound":[{"citation":{"cited_paper":{"arxiv_id":"1904.07012","last_updated":"2019-04-15T13:00:46Z","snapshot_observed_at":"2026-08-10T03:18:56.022954Z","submitted_at":"2019-04-15T13:00:46Z","title":"Constraining the neutron star equation of state using Pulse Profile Modeling","version":1},"cited_work":{"arxiv_id":"1904.07012","doi":null,"metadata_source":"arxiv_reference","pith_arxiv_id":"1904.07012","snapshot_observed_at":"2026-06-05T21:23:00.469572Z","title":"Constraining the neutron star equation of state using Pulse Proﬁle Modeling","venue":null,"work_id":"d33073cc-73cb-4c66-bc42-586ed63b43c9","year":2019},"citing_paper":{"arxiv_id":"1907.05841","last_updated":"2019-07-12T17:03:45Z","snapshot_observed_at":"2026-08-06T21:47:38.893542Z","submitted_at":"2019-07-12T17:03:45Z","title":"Compact star properties from an extended linear sigma model","version":1},"reference_index":20,"source":"pdf_text","source_observed_at":"2026-05-24T22:20:27.323938Z"},"links":{"cited_paper":"/paper/1904.07012","citing_paper":"/paper/1907.05841"},"observation_digest":"sha256:89bfe117337e9bb4805a79d56118d37d4c0cf0c61fff4af1dea4b3900b5f2884","observation_id":"1496aa53-495f-4e1c-af27-31e2258add41","resolution":{"observed_at":"2026-05-24T22:25:01.612104Z","resolver_source":"arxiv_id","status":"verified_exact"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-11T06:34:44.6726+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-11T06:34:44.6726+00:00","source":"crossref"},{"observed_at":"2026-08-11T06:34:36.301508+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":{"arxiv_id":"1904.07012","last_updated":"2019-04-15T13:00:46Z","snapshot_observed_at":"2026-08-10T03:18:56.022954Z","submitted_at":"2019-04-15T13:00:46Z","title":"Constraining the neutron star equation of state using Pulse Profile Modeling","version":1},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"1904.07012","snapshot_observed_at":"2026-08-08T12:40:54.737873Z","title":"L., 2019, in Xiamen-CUSTIPEN Workshop on the Equation of State of Dense Neutron-Rich Matter in the Era of Gravitational Wave Astronomy","venue":null,"work_id":null,"year":2019},"citing_paper":{"arxiv_id":"2502.07471","last_updated":"2025-02-11T11:26:20Z","snapshot_observed_at":"2026-08-10T03:09:46.892514Z","submitted_at":"2025-02-11T11:26:20Z","title":"Scaling relations for the uncertainty in neutron star radius inferred from pulse profile modelling: the effect of spin rate","version":1},"reference_index":48,"source":"arxiv_source","source_observed_at":"2026-08-08T12:40:54.737873Z"},"links":{"cited_paper":"/paper/1904.07012","citing_paper":"/paper/2502.07471"},"observation_digest":"sha256:2a5b4da5cd5761464ffa76e4e83ee995b6dbb8ff4874c0b4f6d24aced8dcff21","observation_id":"12341ece-e14e-4819-9b01-91c0d736a254","resolution":{"observed_at":"2026-08-08T12:40:54.737873Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}}],"links":{"evidence":"/evidence","html":"/paper/1904.07012/citation-record","integrity":"/paper/1904.07012/integrity","json":"/paper/1904.07012/citation-record.json","paper":"/paper/1904.07012"},"outbound":[],"paper":{"arxiv_id":"1904.07012","last_updated":"2019-04-15T13:00:46Z","latest_version":1,"primary_category":"astro-ph.HE","snapshot_observed_at":"2026-08-10T03:18:56.022954Z","submitted_at":"2019-04-15T13:00:46Z","title":"Constraining the neutron star equation of state using Pulse Profile Modeling"},"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":"2026-08-11T06:34:44.6726+00:00","source":"crossref"},{"observed_at":"2026-08-11T06:34:36.301508+00:00","source":"retraction_watch"}],"thesis":"As of 11 August 2026, this Paper Citation Record lists 0 of 0 outbound references and 2 inbound Pith citation observations for arXiv:1904.07012."}