{"as_of":"2026-08-09T17:13:00Z","caps":{"database_statements":6,"inbound":100,"outbound":100},"context_digest":"sha256:8aece810fcbb5f93a13755b0bcc37ee5f1b65b08de1e1685ae030827788d0a7b","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":"2026-08-09T06:31:02.800959+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":"2026-08-09T04:46:12.850987Z","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":"2026-08-07T15:35:21.142399Z","state":"measured"}],"external_citation_measurements":[],"inbound":[{"citation":{"cited_paper":{"arxiv_id":"2002.00562","last_updated":"2020-02-03T05:20:07Z","snapshot_observed_at":"2026-07-06T08:54:25.868963Z","submitted_at":"2020-02-03T05:20:07Z","title":"Effects of symmetry energy on the radius and tidal deformability of neutron stars in relativistic mean-field model","version":1},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2002.00562","snapshot_observed_at":"2026-08-09T04:46:12.850987Z","title":null,"venue":null,"work_id":null,"year":2020},"citing_paper":{"arxiv_id":"2502.03463","last_updated":"2025-02-05T18:59:08Z","snapshot_observed_at":"2026-08-09T10:58:57.963124Z","submitted_at":"2025-02-05T18:59:08Z","title":"Cosmic Calipers: Precise and Accurate Neutron Star Radius Measurements with Next-Generation Gravitational Wave Detectors","version":1},"reference_index":32,"source":"pdf_text","source_observed_at":"2026-08-09T04:46:12.850987Z"},"links":{"cited_paper":"/paper/2002.00562","citing_paper":"/paper/2502.03463"},"observation_digest":"sha256:14f2805e5d852ea9f6dcc13dfdceba2efafd59266c54f933fc6a96fb6202dbd4","observation_id":"31637bf7-8cdf-477f-9b97-56970487aba5","resolution":{"observed_at":"2026-08-09T04:46:12.850987Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2002.00562","last_updated":"2020-02-03T05:20:07Z","snapshot_observed_at":"2026-07-06T08:54:25.868963Z","submitted_at":"2020-02-03T05:20:07Z","title":"Effects of symmetry energy on the radius and tidal deformability of neutron stars in relativistic mean-field model","version":1},"cited_work":{"arxiv_id":"2002.00562","doi":null,"metadata_source":"pith","pith_arxiv_id":"2002.00562","snapshot_observed_at":"2026-08-07T15:35:21.142399Z","title":"Effects of symmetry energy on the radius and tidal deformability of neutron stars in relativistic mean-field model","venue":"nucl-th","work_id":"8b19d14b-f883-4cd8-809f-e2d203ecd22a","year":2020},"citing_paper":{"arxiv_id":"2505.14822","last_updated":"2025-05-20T18:39:26Z","snapshot_observed_at":"2026-08-09T16:20:07.906050Z","submitted_at":"2025-05-20T18:39:26Z","title":"Model-Independent Determination of the Tidal Deformability of a 1.4 $M_{\\odot}$ Neutron Star from Gravitational-Wave Measurements","version":1},"reference_index":32,"source":"pdf_text","source_observed_at":"2026-08-07T15:35:19.175245Z"},"links":{"cited_paper":"/paper/2002.00562","citing_paper":"/paper/2505.14822"},"observation_digest":"sha256:4eca72138cb798e4806020095107be11a75033197fc3bf5df54241b8c39c7c39","observation_id":"6f9153d1-5e7b-441c-a2ab-b963c29272fd","resolution":{"observed_at":"2026-08-07T15:35:21.150969Z","resolver_source":"local_arxiv","status":"verified_exact"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-09T06:31:02.800959+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-09T06:31:02.800959+00:00","source":"crossref"},{"observed_at":"2026-08-09T06:30:57.326959+00:00","source":"retraction_watch"}],"state":"measured"}}],"links":{"evidence":"/evidence","html":"/paper/2002.00562/citation-record","integrity":"/paper/2002.00562/integrity","json":"/paper/2002.00562/citation-record.json","paper":"/paper/2002.00562"},"outbound":[],"paper":{"arxiv_id":"2002.00562","last_updated":"2020-02-03T05:20:07Z","latest_version":1,"primary_category":"nucl-th","snapshot_observed_at":"2026-07-06T08:54:25.868963Z","submitted_at":"2020-02-03T05:20:07Z","title":"Effects of symmetry energy on the radius and tidal deformability of neutron stars in relativistic mean-field model"},"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":"2026-08-09T06:31:02.800959+00:00","source":"crossref"},{"observed_at":"2026-08-09T06:30:57.326959+00:00","source":"retraction_watch"}],"thesis":"As of 9 August 2026, this Paper Citation Record lists 0 of 0 outbound references and 2 inbound Pith citation observations for arXiv:2002.00562."}