{"as_of":"2026-08-18T18:12:00Z","caps":{"database_statements":6,"inbound":100,"outbound":100},"context_digest":"sha256:4165b71ca206dd4f65ee5f16e8c3f379e1c258d317ae687fa354cd77e63aebc2","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":"2026-08-18T06:34:40.430872+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":"2026-07-11T05:52:28.674753Z","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":"2305.05999","last_updated":"2023-05-11T08:20:38Z","snapshot_observed_at":"2026-08-16T15:34:13.763369Z","submitted_at":"2023-05-10T09:19:27Z","title":"Detectability of a phase transition in neutron star matter with third-generation gravitational wave interferometers","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2305.05999","snapshot_observed_at":"2026-07-11T05:52:28.674753Z","title":"Mondal, M","venue":null,"work_id":null,"year":2023},"citing_paper":{"arxiv_id":"2607.05555","last_updated":"2026-07-06T18:48:17Z","snapshot_observed_at":"2026-07-31T03:57:30.597074Z","submitted_at":"2026-07-06T18:48:17Z","title":"Can average speed of sound and thermodynamic response functions signal the exotic phases in neutron star cores?","version":1},"reference_index":42,"source":"pdf_text","source_observed_at":"2026-07-11T05:52:28.674753Z"},"links":{"cited_paper":"/paper/2305.05999","citing_paper":"/paper/2607.05555"},"observation_digest":"sha256:b919ac7760c61e46813e60739aa831bb632b87da739f3e7b3e1a84f87287ef7b","observation_id":"ea83f584-d2ad-4264-b3dc-771d0ec7f44a","resolution":{"observed_at":"2026-07-11T05:52:28.674753Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}}],"links":{"evidence":"/evidence","html":"/paper/2305.05999/citation-record","integrity":"/paper/2305.05999/integrity","json":"/paper/2305.05999/citation-record.json","paper":"/paper/2305.05999"},"outbound":[],"paper":{"arxiv_id":"2305.05999","last_updated":"2023-05-11T08:20:38Z","latest_version":2,"primary_category":"astro-ph.HE","snapshot_observed_at":"2026-08-16T15:34:13.763369Z","submitted_at":"2023-05-10T09:19:27Z","title":"Detectability of a phase transition in neutron star matter with third-generation gravitational wave interferometers"},"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":"2026-08-18T06:34:40.430872+00:00","source":"crossref"},{"observed_at":"2026-08-18T06:34:34.496301+00:00","source":"retraction_watch"}],"thesis":"As of 18 August 2026, this Paper Citation Record lists 0 of 0 outbound references and 1 inbound Pith citation observation for arXiv:2305.05999."}