{"as_of":"2026-08-14T16:54:00Z","caps":{"database_statements":6,"inbound":100,"outbound":100},"context_digest":"sha256:f8b24229e32b2f5ff103cd121fb0528b07da56fa6269536eb4fe8abdb85f0809","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":"2026-08-14T06:32:32.682623+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":"2026-08-11T10:36:09.870800Z","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":"2026-07-10T07:56:57.905630Z","state":"measured"}],"external_citation_measurements":[],"inbound":[{"citation":{"cited_paper":{"arxiv_id":"2105.08688","last_updated":"2021-10-25T13:31:14Z","snapshot_observed_at":"2026-08-14T15:47:00.084695Z","submitted_at":"2021-05-18T17:17:18Z","title":"Nuclear-Physics Multi-Messenger Astrophysics Constraints on the Neutron-Star Equation of State: Adding NICER's PSR J0740+6620 Measurement","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2105.08688","snapshot_observed_at":"2026-08-11T10:36:09.870800Z","title":null,"venue":null,"work_id":null,"year":2021},"citing_paper":{"arxiv_id":"2412.16513","last_updated":"2025-04-28T02:09:34Z","snapshot_observed_at":"2026-08-14T09:58:44.401775Z","submitted_at":"2024-12-21T07:25:36Z","title":"Bayesian constraints on covariant density functional equations of state of compact stars with new NICER mass-radius measurements","version":2},"reference_index":17,"source":"pdf_text","source_observed_at":"2026-08-11T10:36:09.870800Z"},"links":{"cited_paper":"/paper/2105.08688","citing_paper":"/paper/2412.16513"},"observation_digest":"sha256:156504aae048b3a6992379948f3e8de0030f5c24fcca36bc4082c1da7bc26d61","observation_id":"104afd18-6d24-44bd-bf3a-a87c0a1cdb80","resolution":{"observed_at":"2026-08-11T10:36:09.870800Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2105.08688","last_updated":"2021-10-25T13:31:14Z","snapshot_observed_at":"2026-08-14T15:47:00.084695Z","submitted_at":"2021-05-18T17:17:18Z","title":"Nuclear-Physics Multi-Messenger Astrophysics Constraints on the Neutron-Star Equation of State: Adding NICER's PSR J0740+6620 Measurement","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2105.08688","snapshot_observed_at":"2026-08-10T14:01:08.658261Z","title":null,"venue":null,"work_id":null,"year":2021},"citing_paper":{"arxiv_id":"2501.15810","last_updated":"2025-04-30T02:15:27Z","snapshot_observed_at":"2026-08-14T02:13:05.174190Z","submitted_at":"2025-01-27T06:34:32Z","title":"Towards constraining QCD phase transitions in neutron star interiors: Bayesian Inference with TOV linear response analysis","version":2},"reference_index":35,"source":"pdf_text","source_observed_at":"2026-08-10T14:01:08.658261Z"},"links":{"cited_paper":"/paper/2105.08688","citing_paper":"/paper/2501.15810"},"observation_digest":"sha256:3ecc415aabc7e310825375706353daf4b37e62e3248aada371eba6c56a335b58","observation_id":"5fed7279-2d06-4adf-92b4-7a80e34fb192","resolution":{"observed_at":"2026-08-10T14:01:08.658261Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2105.08688","last_updated":"2021-10-25T13:31:14Z","snapshot_observed_at":"2026-08-14T15:47:00.084695Z","submitted_at":"2021-05-18T17:17:18Z","title":"Nuclear-Physics Multi-Messenger Astrophysics Constraints on the Neutron-Star Equation of State: Adding NICER's PSR J0740+6620 Measurement","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2105.08688","snapshot_observed_at":"2026-08-07T11:39:47.302256Z","title":null,"venue":null,"work_id":null,"year":2021},"citing_paper":{"arxiv_id":"2506.02115","last_updated":"2025-06-02T18:00:04Z","snapshot_observed_at":"2026-08-09T15:07:34.142230Z","submitted_at":"2025-06-02T18:00:04Z","title":"The error budget of binary neutron star merger simulations for configurations with high spin","version":1},"reference_index":33,"source":"pdf_text","source_observed_at":"2026-08-07T11:39:47.302256Z"},"links":{"cited_paper":"/paper/2105.08688","citing_paper":"/paper/2506.02115"},"observation_digest":"sha256:aadb2216cf6822ef77c1f2ff6f6faff5d60e36d50af303568bbb39829e289f5f","observation_id":"1d0afbd3-35e3-4151-bd73-61017ffbd96d","resolution":{"observed_at":"2026-08-07T11:39:47.302256Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2105.08688","last_updated":"2021-10-25T13:31:14Z","snapshot_observed_at":"2026-08-14T15:47:00.084695Z","submitted_at":"2021-05-18T17:17:18Z","title":"Nuclear-Physics Multi-Messenger Astrophysics Constraints on the Neutron-Star Equation of State: Adding NICER's PSR J0740+6620 Measurement","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2105.08688","snapshot_observed_at":"2026-08-03T20:20:20.083030Z","title":"Astrophys","venue":null,"work_id":null,"year":2021},"citing_paper":{"arxiv_id":"2511.20378","last_updated":"2026-06-28T03:18:05Z","snapshot_observed_at":"2026-08-06T06:55:09.797555Z","submitted_at":"2025-11-25T14:59:28Z","title":"Toward a Unified Understanding of the Dense Matter Equation of State","version":2},"reference_index":247,"source":"pdf_text","source_observed_at":"2026-08-03T20:20:20.083030Z"},"links":{"cited_paper":"/paper/2105.08688","citing_paper":"/paper/2511.20378"},"observation_digest":"sha256:9b11a724decd2399dd26dc62a00a9dd82eee6ba50d5e3e2a777ddbb1d2abfb3f","observation_id":"ab346078-1175-47e0-ba07-3e2d3b849be7","resolution":{"observed_at":"2026-08-03T20:20:20.083030Z","resolver_source":null,"status":"malformed_identifier"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2105.08688","last_updated":"2021-10-25T13:31:14Z","snapshot_observed_at":"2026-08-14T15:47:00.084695Z","submitted_at":"2021-05-18T17:17:18Z","title":"Nuclear-Physics Multi-Messenger Astrophysics Constraints on the Neutron-Star Equation of State: Adding NICER's PSR J0740+6620 Measurement","version":2},"cited_work":{"arxiv_id":"2105.08688","doi":null,"metadata_source":"pith","pith_arxiv_id":"2105.08688","snapshot_observed_at":"2026-07-10T07:56:57.905630Z","title":"Nuclear-Physics Multi-Messenger Astrophysics Constraints on the Neutron-Star Equation of State: Adding NICER's PSR J0740+6620 Measurement","venue":"astro-ph.HE","work_id":"f5abbbc3-a744-432e-a8d0-88ec32ab4443","year":2021},"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":80,"source":"pdf_text","source_observed_at":"2026-07-10T07:51:26.601892Z"},"links":{"cited_paper":"/paper/2105.08688","citing_paper":"/paper/2607.08412"},"observation_digest":"sha256:01b5e17c2d27a423b668fe968b4c2ca81613bc658c34497b74135c552e4deff3","observation_id":"96a85bf3-7b3e-4a49-8c7c-eda0aae67b9f","resolution":{"observed_at":"2026-07-10T07:56:57.907611Z","resolver_source":"local_arxiv","status":"verified_exact"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-14T06:32:32.682623+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-14T06:32:32.682623+00:00","source":"crossref"},{"observed_at":"2026-08-14T06:32:18.44784+00:00","source":"retraction_watch"}],"state":"measured"}}],"links":{"evidence":"/evidence","html":"/paper/2105.08688/citation-record","integrity":"/paper/2105.08688/integrity","json":"/paper/2105.08688/citation-record.json","paper":"/paper/2105.08688"},"outbound":[],"paper":{"arxiv_id":"2105.08688","last_updated":"2021-10-25T13:31:14Z","latest_version":2,"primary_category":"astro-ph.HE","snapshot_observed_at":"2026-08-14T15:47:00.084695Z","submitted_at":"2021-05-18T17:17:18Z","title":"Nuclear-Physics Multi-Messenger Astrophysics Constraints on the Neutron-Star Equation of State: Adding NICER's PSR J0740+6620 Measurement"},"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":"2026-08-14T06:32:32.682623+00:00","source":"crossref"},{"observed_at":"2026-08-14T06:32:18.44784+00:00","source":"retraction_watch"}],"thesis":"As of 14 August 2026, this Paper Citation Record lists 0 of 0 outbound references and 5 inbound Pith citation observations for arXiv:2105.08688."}