{"as_of":"2026-08-13T08:15:00Z","caps":{"database_statements":6,"inbound":100,"outbound":100},"context_digest":"sha256:d4d13f2e0dc623b3454b033d49fd470304ebeb2768b2f4a43255534eb5857d6f","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":4,"lane":"standing_notices","note":"One-hop event checks from named stored sources.","records_observed":4,"source":"scholarly_work_events, retraction_status_cache","source_observed_at":"2026-08-13T06:32:02.005865+00:00","state":"measured"},{"denominator":4,"lane":"inbound_itemization","note":"Pith citing papers itemized under the disclosed page cap.","records_observed":4,"source":"paper_references, paper_reference_links","source_observed_at":"2026-08-11T04:21:33.061008Z","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":"2026-05-22T01:40:54.117211Z","state":"measured"}],"external_citation_measurements":[],"inbound":[{"citation":{"cited_paper":{"arxiv_id":"2208.04294","last_updated":"2023-04-13T13:46:36Z","snapshot_observed_at":"2026-08-02T17:53:27.551573Z","submitted_at":"2022-08-08T17:35:26Z","title":"Degeneracy in the inference of phase transitions in the neutron star equation of state from gravitational wave data","version":2},"cited_work":{"arxiv_id":"2208.04294","doi":null,"metadata_source":"arxiv_reference","pith_arxiv_id":"2208.04294","snapshot_observed_at":"2026-06-05T21:23:00.469572Z","title":null,"venue":null,"work_id":"83bc37c2-31d1-4e8b-857c-80e3aa4a8165","year":2023},"citing_paper":{"arxiv_id":"2505.16929","last_updated":"2026-04-14T09:24:59Z","snapshot_observed_at":"2026-08-13T05:14:11.917440Z","submitted_at":"2025-05-22T17:22:16Z","title":"Properties of the neutron star crust informed by nuclear structure data","version":2},"reference_index":35,"source":"pdf_text","source_observed_at":"2026-05-22T01:36:22.187463Z"},"links":{"cited_paper":"/paper/2208.04294","citing_paper":"/paper/2505.16929"},"observation_digest":"sha256:fa112f1059a2306fbb7a5cbe28f0ac1adcd1197e809fb87c94256b6a62f35e3b","observation_id":"498080f6-0d3c-445e-b728-db9e0a293b67","resolution":{"observed_at":"2026-05-22T01:40:54.120432Z","resolver_source":"arxiv_id","status":"verified_exact"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-13T06:32:02.005865+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-13T06:32:02.005865+00:00","source":"crossref"},{"observed_at":"2026-08-13T06:31:53.387327+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":{"arxiv_id":"2208.04294","last_updated":"2023-04-13T13:46:36Z","snapshot_observed_at":"2026-08-02T17:53:27.551573Z","submitted_at":"2022-08-08T17:35:26Z","title":"Degeneracy in the inference of phase transitions in the neutron star equation of state from gravitational wave data","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2208.04294","snapshot_observed_at":"2026-08-07T05:14:55.014803Z","title":null,"venue":null,"work_id":null,"year":2023},"citing_paper":{"arxiv_id":"2506.08658","last_updated":"2025-06-10T10:19:43Z","snapshot_observed_at":"2026-08-12T15:48:14.233455Z","submitted_at":"2025-06-10T10:19:43Z","title":"Crust (Unified) Tool for Equation-of-state Reconstruction (CUTER) v2","version":1},"reference_index":36,"source":"pdf_text","source_observed_at":"2026-08-07T05:14:55.014803Z"},"links":{"cited_paper":"/paper/2208.04294","citing_paper":"/paper/2506.08658"},"observation_digest":"sha256:bd3d16bf30e6d6980d07c2d0587d0841fe21c551b04ccc5dc0efc8ef2a4bc0ee","observation_id":"6dfb030b-e3bd-408c-86cb-8ace4896e286","resolution":{"observed_at":"2026-08-07T05:14:55.014803Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2208.04294","last_updated":"2023-04-13T13:46:36Z","snapshot_observed_at":"2026-08-02T17:53:27.551573Z","submitted_at":"2022-08-08T17:35:26Z","title":"Degeneracy in the inference of phase transitions in the neutron star equation of state from gravitational wave data","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2208.04294","snapshot_observed_at":"2026-08-07T23:28:59.300353Z","title":null,"venue":null,"work_id":null,"year":2023},"citing_paper":{"arxiv_id":"2608.05794","last_updated":"2026-08-08T19:08:50Z","snapshot_observed_at":"2026-08-13T08:10:47.106973Z","submitted_at":"2026-08-06T09:30:26Z","title":"How Loud Must a Neutron-Star Merger Be to Reveal Its Equation of State?","version":1},"reference_index":25,"source":"pdf_text","source_observed_at":"2026-08-07T23:28:59.300353Z"},"links":{"cited_paper":"/paper/2208.04294","citing_paper":"/paper/2608.05794"},"observation_digest":"sha256:5c7046b6076eaa0e25016957bff994771efb1f65ceaaf936c4db553a72b5ccfe","observation_id":"66546818-a14b-4f08-bdf0-e40073cfe10a","resolution":{"observed_at":"2026-08-07T23:28:59.300353Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2208.04294","last_updated":"2023-04-13T13:46:36Z","snapshot_observed_at":"2026-08-02T17:53:27.551573Z","submitted_at":"2022-08-08T17:35:26Z","title":"Degeneracy in the inference of phase transitions in the neutron star equation of state from gravitational wave data","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2208.04294","snapshot_observed_at":"2026-08-11T04:21:33.061008Z","title":null,"venue":null,"work_id":null,"year":2023},"citing_paper":{"arxiv_id":"2608.05794","last_updated":"2026-08-08T19:08:50Z","snapshot_observed_at":"2026-08-13T08:10:47.106973Z","submitted_at":"2026-08-06T09:30:26Z","title":"How Loud Must a Neutron-Star Merger Be to Reveal Its Equation of State?","version":2},"reference_index":25,"source":"pdf_text","source_observed_at":"2026-08-11T04:21:33.061008Z"},"links":{"cited_paper":"/paper/2208.04294","citing_paper":"/paper/2608.05794"},"observation_digest":"sha256:be418f07d57a861621903acbccfa78678692a83d276d47e3bf2dfcc62ca1aa90","observation_id":"f9848189-373f-4307-8077-01d652507479","resolution":{"observed_at":"2026-08-11T04:21:33.061008Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}}],"links":{"evidence":"/evidence","html":"/paper/2208.04294/citation-record","integrity":"/paper/2208.04294/integrity","json":"/paper/2208.04294/citation-record.json","paper":"/paper/2208.04294"},"outbound":[],"paper":{"arxiv_id":"2208.04294","last_updated":"2023-04-13T13:46:36Z","latest_version":2,"primary_category":"astro-ph.HE","snapshot_observed_at":"2026-08-02T17:53:27.551573Z","submitted_at":"2022-08-08T17:35:26Z","title":"Degeneracy in the inference of phase transitions in the neutron star equation of state from gravitational wave data"},"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":"2026-08-13T06:32:02.005865+00:00","source":"crossref"},{"observed_at":"2026-08-13T06:31:53.387327+00:00","source":"retraction_watch"}],"thesis":"As of 13 August 2026, this Paper Citation Record lists 0 of 0 outbound references and 4 inbound Pith citation observations for arXiv:2208.04294."}