{"as_of":"2026-08-13T02:11:00Z","caps":{"database_statements":6,"inbound":100,"outbound":100},"context_digest":"sha256:96ead7f5f6b0d84a79bc80475f1287f64ccf9691b5c54930e155dd18933c991a","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":"2026-08-12T06:34:41.77262+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":"2026-08-11T21:11:05.914800Z","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":"2026-05-11T08:30:57.699984Z","state":"measured"}],"external_citation_measurements":[],"inbound":[{"citation":{"cited_paper":{"arxiv_id":"1610.06344","last_updated":"2016-10-20T09:59:12Z","snapshot_observed_at":"2026-07-06T05:15:21.042868Z","submitted_at":"2016-10-20T09:59:12Z","title":"Strong correlations of neutron star radii with the slopes of nuclear matter incompressibility and symmetry energy at saturation","version":1},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"1610.06344","snapshot_observed_at":"2026-08-11T21:11:05.914800Z","title":null,"venue":null,"work_id":null,"year":2016},"citing_paper":{"arxiv_id":"2412.04946","last_updated":"2024-12-06T11:06:01Z","snapshot_observed_at":"2026-08-11T21:04:17.814148Z","submitted_at":"2024-12-06T11:06:01Z","title":"Impact of the Scalar Isovector $\\delta$-meson on the description of nuclear matter and neutron star properties","version":1},"reference_index":34,"source":"pdf_text","source_observed_at":"2026-08-11T21:11:05.914800Z"},"links":{"cited_paper":"/paper/1610.06344","citing_paper":"/paper/2412.04946"},"observation_digest":"sha256:b2824ae61b6ba2fe662594ad08f77ff438bdb4e0622e71d9cb8b49a06c00ed90","observation_id":"44d7200d-646c-4ffa-8fd0-b7cb53ccdf2d","resolution":{"observed_at":"2026-08-11T21:11:05.914800Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"1610.06344","last_updated":"2016-10-20T09:59:12Z","snapshot_observed_at":"2026-07-06T05:15:21.042868Z","submitted_at":"2016-10-20T09:59:12Z","title":"Strong correlations of neutron star radii with the slopes of nuclear matter incompressibility and symmetry energy at saturation","version":1},"cited_work":{"arxiv_id":"1610.06344","doi":null,"metadata_source":"arxiv_reference","pith_arxiv_id":"1610.06344","snapshot_observed_at":"2026-07-04T21:32:26.663190Z","title":null,"venue":null,"work_id":"b394174b-0197-4436-bd48-5d930e5e980e","year":2016},"citing_paper":{"arxiv_id":"2604.11046","last_updated":"2026-04-13T06:22:40Z","snapshot_observed_at":"2026-08-13T01:13:16.603938Z","submitted_at":"2026-04-13T06:22:40Z","title":"Sensitivity of Neutron Star Observables to Transition Density in Hybrid Equation-of-State Models","version":1},"reference_index":79,"source":"pdf_text","source_observed_at":"2026-05-10T16:35:52.640568Z"},"links":{"cited_paper":"/paper/1610.06344","citing_paper":"/paper/2604.11046"},"observation_digest":"sha256:6fc45cc856e92c18e19354a71ad64db411c10d7f3625212ae7bd079d1b947225","observation_id":"de5be808-3622-42b6-b89f-a4c7c6e4d761","resolution":{"observed_at":"2026-07-04T21:32:26.663190Z","resolver_source":"arxiv_id","status":"verified_exact"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-12T06:34:41.77262+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-12T06:34:41.77262+00:00","source":"crossref"},{"observed_at":"2026-08-12T06:34:36.333875+00:00","source":"retraction_watch"}],"state":"measured"}}],"links":{"evidence":"/evidence","html":"/paper/1610.06344/citation-record","integrity":"/paper/1610.06344/integrity","json":"/paper/1610.06344/citation-record.json","paper":"/paper/1610.06344"},"outbound":[],"paper":{"arxiv_id":"1610.06344","last_updated":"2016-10-20T09:59:12Z","latest_version":1,"primary_category":"nucl-th","snapshot_observed_at":"2026-07-06T05:15:21.042868Z","submitted_at":"2016-10-20T09:59:12Z","title":"Strong correlations of neutron star radii with the slopes of nuclear matter incompressibility and symmetry energy at saturation"},"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":"2026-08-12T06:34:41.77262+00:00","source":"crossref"},{"observed_at":"2026-08-12T06:34:36.333875+00:00","source":"retraction_watch"}],"thesis":"As of 13 August 2026, this Paper Citation Record lists 0 of 0 outbound references and 2 inbound Pith citation observations for arXiv:1610.06344."}