{"as_of":"2026-08-09T08:19:00Z","caps":{"database_statements":6,"inbound":100,"outbound":100},"context_digest":"sha256:badf1197b10df9d6fbb0bc1329212d42e9d77dc031e40099be35d45034c1ebdc","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":5,"lane":"standing_notices","note":"One-hop event checks from named stored sources.","records_observed":5,"source":"scholarly_work_events, retraction_status_cache","source_observed_at":"2026-08-09T06:31:02.800959+00:00","state":"measured"},{"denominator":5,"lane":"inbound_itemization","note":"Pith citing papers itemized under the disclosed page cap.","records_observed":5,"source":"paper_references, paper_reference_links","source_observed_at":"2026-08-06T16:49:31.555882Z","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":"2026-07-10T07:56:57.845097Z","state":"measured"}],"external_citation_measurements":[],"inbound":[{"citation":{"cited_paper":{"arxiv_id":"2503.23028","last_updated":"2025-03-29T09:49:27Z","snapshot_observed_at":"2026-08-07T16:28:44.557776Z","submitted_at":"2025-03-29T09:49:27Z","title":"Relativistic mean-field predictions for dense matter equation of state and application to neutron stars","version":1},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2503.23028","snapshot_observed_at":"2026-08-06T16:49:31.555882Z","title":"Relativistic mean-field predictions for dense matter equation of state and application to neutron stars,","venue":null,"work_id":null,"year":2025},"citing_paper":{"arxiv_id":"2507.12540","last_updated":"2025-07-16T18:00:09Z","snapshot_observed_at":"2026-08-08T17:36:40.109662Z","submitted_at":"2025-07-16T18:00:09Z","title":"Systematics from NICER Pulse Profiles Drive Uncertainty in Multi-Messenger Inference of the Neutron Star Equation of State","version":1},"reference_index":57,"source":"pdf_text","source_observed_at":"2026-08-06T16:49:31.555882Z"},"links":{"cited_paper":"/paper/2503.23028","citing_paper":"/paper/2507.12540"},"observation_digest":"sha256:0973b694f9ccb86a7af37caa998d11a15a499ae335a64ed6e7d9798bab896305","observation_id":"d01933d7-0b97-4c25-9c76-57cf4be4a116","resolution":{"observed_at":"2026-08-06T16:49:31.555882Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2503.23028","last_updated":"2025-03-29T09:49:27Z","snapshot_observed_at":"2026-08-07T16:28:44.557776Z","submitted_at":"2025-03-29T09:49:27Z","title":"Relativistic mean-field predictions for dense matter equation of state and application to neutron stars","version":1},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2503.23028","snapshot_observed_at":"2026-08-05T11:14:11.711821Z","title":"Relativistic mean-field predictions for dense matter equation of state and application to neutron stars,","venue":null,"work_id":null,"year":2025},"citing_paper":{"arxiv_id":"2509.03069","last_updated":"2025-09-03T07:04:12Z","snapshot_observed_at":"2026-08-05T11:14:05.347345Z","submitted_at":"2025-09-03T07:04:12Z","title":"The equation of state for neutron stars with speed of sound constraints via Bayesian inference","version":1},"reference_index":61,"source":"pdf_text","source_observed_at":"2026-08-05T11:14:11.711821Z"},"links":{"cited_paper":"/paper/2503.23028","citing_paper":"/paper/2509.03069"},"observation_digest":"sha256:5dba7418e30f8b286a0bfd0cc732da55f55b5f201f660b043d79a9a89dd7c723","observation_id":"38610576-08f5-48af-b2b4-62dd92eaaa08","resolution":{"observed_at":"2026-08-05T11:14:11.711821Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2503.23028","last_updated":"2025-03-29T09:49:27Z","snapshot_observed_at":"2026-08-07T16:28:44.557776Z","submitted_at":"2025-03-29T09:49:27Z","title":"Relativistic mean-field predictions for dense matter equation of state and application to neutron stars","version":1},"cited_work":{"arxiv_id":"2503.23028","doi":null,"metadata_source":"pith","pith_arxiv_id":"2503.23028","snapshot_observed_at":"2026-07-10T07:56:57.845097Z","title":"Relativistic mean-field predictions for dense matter equation of state and application to neutron stars","venue":"nucl-th","work_id":"3aa93f2b-c046-476d-866e-ace488b1ac45","year":2025},"citing_paper":{"arxiv_id":"2606.21435","last_updated":"2026-06-19T13:51:27Z","snapshot_observed_at":"2026-08-06T05:56:14.769876Z","submitted_at":"2026-06-19T13:51:27Z","title":"Is the coexistence of strange quark stars and hadronic stars favored by astrophysical data? A Bayesian analysis","version":1},"reference_index":73,"source":"pdf_text","source_observed_at":"2026-06-26T12:50:53.032717Z"},"links":{"cited_paper":"/paper/2503.23028","citing_paper":"/paper/2606.21435"},"observation_digest":"sha256:d089baf97fa444ed7e388c50b0a9b6beb4b886cef60164e20cc158dd95d442a9","observation_id":"ad39d0fa-5088-4304-81c1-f4343f2fbe02","resolution":{"observed_at":"2026-07-04T07:49:39.121611Z","resolver_source":"arxiv_id","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"}},{"citation":{"cited_paper":{"arxiv_id":"2503.23028","last_updated":"2025-03-29T09:49:27Z","snapshot_observed_at":"2026-08-07T16:28:44.557776Z","submitted_at":"2025-03-29T09:49:27Z","title":"Relativistic mean-field predictions for dense matter equation of state and application to neutron stars","version":1},"cited_work":{"arxiv_id":"2503.23028","doi":null,"metadata_source":"pith","pith_arxiv_id":"2503.23028","snapshot_observed_at":"2026-07-10T07:56:57.845097Z","title":"Relativistic mean-field predictions for dense matter equation of state and application to neutron stars","venue":"nucl-th","work_id":"3aa93f2b-c046-476d-866e-ace488b1ac45","year":2025},"citing_paper":{"arxiv_id":"2607.08412","last_updated":"2026-07-09T12:36:36Z","snapshot_observed_at":"2026-08-06T06:25:07.687890Z","submitted_at":"2026-07-09T12:36:36Z","title":"Relativistic Mean Field Approach with Chiral Symmetry Breaking and Quark Confinement in the light of Astrophysical Observations","version":1},"reference_index":131,"source":"pdf_text","source_observed_at":"2026-07-10T07:51:26.601892Z"},"links":{"cited_paper":"/paper/2503.23028","citing_paper":"/paper/2607.08412"},"observation_digest":"sha256:aefc2eb1d8c8c587bd154e6bb615352182de8272ef32073ff2b42708bc62d7d5","observation_id":"246fb29f-fbf4-46c6-acbd-6786fa0800ad","resolution":{"observed_at":"2026-07-10T07:56:57.847030Z","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"}},{"citation":{"cited_paper":{"arxiv_id":"2503.23028","last_updated":"2025-03-29T09:49:27Z","snapshot_observed_at":"2026-08-07T16:28:44.557776Z","submitted_at":"2025-03-29T09:49:27Z","title":"Relativistic mean-field predictions for dense matter equation of state and application to neutron stars","version":1},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2503.23028","snapshot_observed_at":"2026-07-13T05:17:12.889672Z","title":"Passarella, J","venue":null,"work_id":null,"year":2025},"citing_paper":{"arxiv_id":"2607.09119","last_updated":"2026-07-10T06:16:49Z","snapshot_observed_at":"2026-08-08T02:18:59.676855Z","submitted_at":"2026-07-10T06:16:49Z","title":"Effects of dark matter and magnetic field on neutron star properties in relativistic mean-field theory: A single-fluid approach","version":1},"reference_index":47,"source":"pdf_text","source_observed_at":"2026-07-13T05:17:12.889672Z"},"links":{"cited_paper":"/paper/2503.23028","citing_paper":"/paper/2607.09119"},"observation_digest":"sha256:b8e5edbfb64070ec601702f990628ce9afa5150593ae4aad4590226e449488e5","observation_id":"bda7010c-3be7-42cf-9e25-637c537e3516","resolution":{"observed_at":"2026-07-13T05:17:12.889672Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}}],"links":{"evidence":"/evidence","html":"/paper/2503.23028/citation-record","integrity":"/paper/2503.23028/integrity","json":"/paper/2503.23028/citation-record.json","paper":"/paper/2503.23028"},"outbound":[],"paper":{"arxiv_id":"2503.23028","last_updated":"2025-03-29T09:49:27Z","latest_version":1,"primary_category":"nucl-th","snapshot_observed_at":"2026-08-07T16:28:44.557776Z","submitted_at":"2025-03-29T09:49:27Z","title":"Relativistic mean-field predictions for dense matter equation of state and application to neutron stars"},"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 5 inbound Pith citation observations for arXiv:2503.23028."}