{"as_of":"2026-08-08T08:26:00Z","caps":{"database_statements":6,"inbound":100,"outbound":100},"context_digest":"sha256:f45523d0045e9255fb1e22a24e207a6b39d8f7018a3b84013c57675cc8d76c7f","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":"2026-08-08T06:32:00.761636+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":"2026-08-07T15:31:32.591640Z","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":"2026-07-04T16:19:57.295694Z","state":"measured"}],"external_citation_measurements":[],"inbound":[{"citation":{"cited_paper":{"arxiv_id":"2306.06180","last_updated":"2024-05-12T22:24:52Z","snapshot_observed_at":"2026-07-06T15:40:58.515223Z","submitted_at":"2023-06-09T18:10:57Z","title":"Isospin Equilibration in Neutron Star Mergers","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2306.06180","snapshot_observed_at":"2026-08-07T15:31:32.591640Z","title":null,"venue":null,"work_id":null,"year":2024},"citing_paper":{"arxiv_id":"2505.14921","last_updated":"2025-05-20T21:15:29Z","snapshot_observed_at":"2026-08-08T07:38:50.103324Z","submitted_at":"2025-05-20T21:15:29Z","title":"An Overview of the MUSES Calculation Engine and How It Can Be Used to Describe Neutron Stars","version":1},"reference_index":18,"source":"pdf_text","source_observed_at":"2026-08-07T15:31:32.591640Z"},"links":{"cited_paper":"/paper/2306.06180","citing_paper":"/paper/2505.14921"},"observation_digest":"sha256:4be909c679c845b8dc7a38efab186b2410cbb1466a5c5da8a5df92ac98021518","observation_id":"c4ac166c-e850-480c-8b5d-9a95267b4e30","resolution":{"observed_at":"2026-08-07T15:31:32.591640Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2306.06180","last_updated":"2024-05-12T22:24:52Z","snapshot_observed_at":"2026-07-06T15:40:58.515223Z","submitted_at":"2023-06-09T18:10:57Z","title":"Isospin Equilibration in Neutron Star Mergers","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2306.06180","snapshot_observed_at":"2026-08-05T10:17:56.717226Z","title":null,"venue":null,"work_id":null,"year":2024},"citing_paper":{"arxiv_id":"2509.04240","last_updated":"2025-09-04T14:14:59Z","snapshot_observed_at":"2026-08-06T19:56:10.597732Z","submitted_at":"2025-09-04T14:14:59Z","title":"Neutrino absorption in two-flavor color-superconducting quark matter","version":1},"reference_index":5,"source":"pdf_text","source_observed_at":"2026-08-05T10:17:56.717226Z"},"links":{"cited_paper":"/paper/2306.06180","citing_paper":"/paper/2509.04240"},"observation_digest":"sha256:cb655db2e644e864534fa7f136274ddba97ca899e5a647e788edb21a17485779","observation_id":"7d2de5bf-bf90-4557-afec-7e4817dd5605","resolution":{"observed_at":"2026-08-05T10:17:56.717226Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2306.06180","last_updated":"2024-05-12T22:24:52Z","snapshot_observed_at":"2026-07-06T15:40:58.515223Z","submitted_at":"2023-06-09T18:10:57Z","title":"Isospin Equilibration in Neutron Star Mergers","version":2},"cited_work":{"arxiv_id":"2306.06180","doi":null,"metadata_source":"arxiv_reference","pith_arxiv_id":"2306.06180","snapshot_observed_at":"2026-07-04T16:19:57.295694Z","title":null,"venue":null,"work_id":"1fc49f49-bc19-4114-8afa-eaf2d748509b","year":2024},"citing_paper":{"arxiv_id":"2509.25838","last_updated":"2026-04-16T18:51:06Z","snapshot_observed_at":"2026-07-06T22:31:10.099674Z","submitted_at":"2025-09-30T06:23:26Z","title":"Bulk viscosity from neutron decays to dark baryons in neutron star matter","version":2},"reference_index":78,"source":"pdf_text","source_observed_at":"2026-05-18T12:44:55.766757Z"},"links":{"cited_paper":"/paper/2306.06180","citing_paper":"/paper/2509.25838"},"observation_digest":"sha256:3f7287dc48559c0ebcf2ea9d90d841a3e6aebba4d3cf86f5d38b20e1319fccb1","observation_id":"63085b82-f25e-438b-a7f2-e2bcc94221eb","resolution":{"observed_at":"2026-05-18T12:46:23.739436Z","resolver_source":"arxiv_id","status":"verified_exact"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-08T06:32:00.761636+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-08T06:32:00.761636+00:00","source":"crossref"},{"observed_at":"2026-08-08T06:31:55.24221+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":{"arxiv_id":"2306.06180","last_updated":"2024-05-12T22:24:52Z","snapshot_observed_at":"2026-07-06T15:40:58.515223Z","submitted_at":"2023-06-09T18:10:57Z","title":"Isospin Equilibration in Neutron Star Mergers","version":2},"cited_work":{"arxiv_id":"2306.06180","doi":null,"metadata_source":"arxiv_reference","pith_arxiv_id":"2306.06180","snapshot_observed_at":"2026-07-04T16:19:57.295694Z","title":null,"venue":null,"work_id":"1fc49f49-bc19-4114-8afa-eaf2d748509b","year":2024},"citing_paper":{"arxiv_id":"2510.09104","last_updated":"2026-05-21T12:53:58Z","snapshot_observed_at":"2026-08-02T16:10:55.190085Z","submitted_at":"2025-10-10T07:58:38Z","title":"Thermal and Magnetic effects on Bulk Viscosity in Binary Neutron Star Mergers","version":3},"reference_index":50,"source":"pdf_text","source_observed_at":"2026-05-22T12:52:58.423553Z"},"links":{"cited_paper":"/paper/2306.06180","citing_paper":"/paper/2510.09104"},"observation_digest":"sha256:0a9b2e8bb56da6443a8fd49961b3b7ba3ce6a9f981d326e95609603a7e34a95c","observation_id":"6448eb7a-83f9-4974-8daa-e5ed2906b1eb","resolution":{"observed_at":"2026-05-22T12:54:52.625219Z","resolver_source":"arxiv_id","status":"verified_exact"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-08T06:32:00.761636+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-08T06:32:00.761636+00:00","source":"crossref"},{"observed_at":"2026-08-08T06:31:55.24221+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":{"arxiv_id":"2306.06180","last_updated":"2024-05-12T22:24:52Z","snapshot_observed_at":"2026-07-06T15:40:58.515223Z","submitted_at":"2023-06-09T18:10:57Z","title":"Isospin Equilibration in Neutron Star Mergers","version":2},"cited_work":{"arxiv_id":"2306.06180","doi":null,"metadata_source":"arxiv_reference","pith_arxiv_id":"2306.06180","snapshot_observed_at":"2026-07-04T16:19:57.295694Z","title":null,"venue":null,"work_id":"1fc49f49-bc19-4114-8afa-eaf2d748509b","year":2024},"citing_paper":{"arxiv_id":"2606.26326","last_updated":"2026-06-24T19:12:40Z","snapshot_observed_at":"2026-08-03T00:30:24.951043Z","submitted_at":"2026-06-24T19:12:40Z","title":"Studying the QCD Matter produced in Heavy-Ion Collisions using the MUSES Calculation Engine","version":1},"reference_index":156,"source":"pdf_text","source_observed_at":"2026-06-26T00:47:21.247516Z"},"links":{"cited_paper":"/paper/2306.06180","citing_paper":"/paper/2606.26326"},"observation_digest":"sha256:781a187a5b69f42875dada654aa2638ca89a6dde924541f62a4ac8680267c0db","observation_id":"40923a05-9622-4462-ad05-4fd59fb8ffc4","resolution":{"observed_at":"2026-07-04T16:19:57.297108Z","resolver_source":"arxiv_id","status":"verified_exact"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-08T06:32:00.761636+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-08T06:32:00.761636+00:00","source":"crossref"},{"observed_at":"2026-08-08T06:31:55.24221+00:00","source":"retraction_watch"}],"state":"measured"}}],"links":{"evidence":"/evidence","html":"/paper/2306.06180/citation-record","integrity":"/paper/2306.06180/integrity","json":"/paper/2306.06180/citation-record.json","paper":"/paper/2306.06180"},"outbound":[],"paper":{"arxiv_id":"2306.06180","last_updated":"2024-05-12T22:24:52Z","latest_version":2,"primary_category":"nucl-th","snapshot_observed_at":"2026-07-06T15:40:58.515223Z","submitted_at":"2023-06-09T18:10:57Z","title":"Isospin Equilibration in Neutron Star Mergers"},"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":"2026-08-08T06:32:00.761636+00:00","source":"crossref"},{"observed_at":"2026-08-08T06:31:55.24221+00:00","source":"retraction_watch"}],"thesis":"As of 8 August 2026, this Paper Citation Record lists 0 of 0 outbound references and 5 inbound Pith citation observations for arXiv:2306.06180."}