{"as_of":"2026-08-21T04:10:00Z","caps":{"database_statements":6,"inbound":100,"outbound":100},"context_digest":"sha256:a18508d8ebab59870835a7c546898d06a835e0c6ca0b6d059345eaac677035b8","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":"2026-08-20T06:33:59.587034+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":"2026-08-15T16:43:43.247476Z","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":"2026-08-06T17:02:29.112081Z","state":"measured"}],"external_citation_measurements":[],"inbound":[{"citation":{"cited_paper":{"arxiv_id":"2112.10439","last_updated":"2022-08-08T18:13:16Z","snapshot_observed_at":"2026-08-19T09:09:18.089168Z","submitted_at":"2021-12-20T10:48:30Z","title":"Universal relations for rapidly rotating cold and hot hybrid star","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2112.10439","snapshot_observed_at":"2026-08-11T18:36:55.019809Z","title":null,"venue":null,"work_id":null,"year":2022},"citing_paper":{"arxiv_id":"2412.07758","last_updated":"2025-08-01T16:22:13Z","snapshot_observed_at":"2026-08-19T11:39:49.765495Z","submitted_at":"2024-12-10T18:54:39Z","title":"Fastest spinning millisecond pulsars: indicators for quark matter in neutron stars?","version":2},"reference_index":31,"source":"pdf_text","source_observed_at":"2026-08-11T18:36:55.019809Z"},"links":{"cited_paper":"/paper/2112.10439","citing_paper":"/paper/2412.07758"},"observation_digest":"sha256:0c30cac38b3e927023f4ac61560652af38f4d59557c69dbabcd38244df7a7f8e","observation_id":"b4e384c0-612a-4aa8-83ee-2e7dba75f26b","resolution":{"observed_at":"2026-08-11T18:36:55.019809Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2112.10439","last_updated":"2022-08-08T18:13:16Z","snapshot_observed_at":"2026-08-19T09:09:18.089168Z","submitted_at":"2021-12-20T10:48:30Z","title":"Universal relations for rapidly rotating cold and hot hybrid star","version":2},"cited_work":{"arxiv_id":"2112.10439","doi":null,"metadata_source":"pith","pith_arxiv_id":"2112.10439","snapshot_observed_at":"2026-08-06T17:02:29.112081Z","title":"Universal relations for rapidly rotating cold and hot hybrid star","venue":"astro-ph.HE","work_id":"e4ca992e-817c-406f-807f-9c0fdc41d99a","year":2021},"citing_paper":{"arxiv_id":"2507.11956","last_updated":"2025-07-16T06:42:48Z","snapshot_observed_at":"2026-08-15T14:26:09.034158Z","submitted_at":"2025-07-16T06:42:48Z","title":"Investigating Universal Relations in Compact Stars featuring $\\Delta-$Admixed Exotic Dense Matter","version":1},"reference_index":38,"source":"pdf_text","source_observed_at":"2026-08-06T17:02:27.090998Z"},"links":{"cited_paper":"/paper/2112.10439","citing_paper":"/paper/2507.11956"},"observation_digest":"sha256:211233f1bd5acde976e4b5f55be541f59749fb89cf03332d199e4e504beaf062","observation_id":"fdc753f2-71f0-4af0-b780-fd37c974745c","resolution":{"observed_at":"2026-08-06T17:02:29.160663Z","resolver_source":"local_arxiv","status":"verified_exact"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-20T06:33:59.587034+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-20T06:33:59.587034+00:00","source":"crossref"},{"observed_at":"2026-08-20T06:33:54.927442+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":{"arxiv_id":"2112.10439","last_updated":"2022-08-08T18:13:16Z","snapshot_observed_at":"2026-08-19T09:09:18.089168Z","submitted_at":"2021-12-20T10:48:30Z","title":"Universal relations for rapidly rotating cold and hot hybrid star","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2112.10439","snapshot_observed_at":"2026-08-15T16:43:43.247476Z","title":null,"venue":null,"work_id":null,"year":2022},"citing_paper":{"arxiv_id":"2509.02554","last_updated":"2025-09-02T17:50:38Z","snapshot_observed_at":"2026-08-16T13:05:49.605770Z","submitted_at":"2025-09-02T17:50:38Z","title":"Bayesian inference favors quark matter in neutron star interiors","version":1},"reference_index":70,"source":"pdf_text","source_observed_at":"2026-08-15T16:43:43.247476Z"},"links":{"cited_paper":"/paper/2112.10439","citing_paper":"/paper/2509.02554"},"observation_digest":"sha256:4543c63d3b5e9294990f68a4ccf5e8464b3943dff1fdc128806ff7711484dcbe","observation_id":"a8bd2425-d296-4105-8c52-06776751dd6f","resolution":{"observed_at":"2026-08-15T16:43:43.247476Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2112.10439","last_updated":"2022-08-08T18:13:16Z","snapshot_observed_at":"2026-08-19T09:09:18.089168Z","submitted_at":"2021-12-20T10:48:30Z","title":"Universal relations for rapidly rotating cold and hot hybrid star","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2112.10439","snapshot_observed_at":"2026-08-03T17:54:34.413940Z","title":null,"venue":null,"work_id":null,"year":2022},"citing_paper":{"arxiv_id":"2512.07977","last_updated":"2025-12-08T19:10:30Z","snapshot_observed_at":"2026-08-14T19:40:16.335967Z","submitted_at":"2025-12-08T19:10:30Z","title":"Rapidly Spinning Massive Pulsars as an Indicator of Quark Deconfinement","version":1},"reference_index":10,"source":"pdf_text","source_observed_at":"2026-08-03T17:54:34.413940Z"},"links":{"cited_paper":"/paper/2112.10439","citing_paper":"/paper/2512.07977"},"observation_digest":"sha256:6abe600dae7a8074814ee064c976eed8818a576cc9b6412f2156901533ae0508","observation_id":"9dea90b6-6159-4657-a6b1-d18962f3ca9c","resolution":{"observed_at":"2026-08-03T17:54:34.413940Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}}],"links":{"evidence":"/evidence","html":"/paper/2112.10439/citation-record","integrity":"/paper/2112.10439/integrity","json":"/paper/2112.10439/citation-record.json","paper":"/paper/2112.10439"},"outbound":[],"paper":{"arxiv_id":"2112.10439","last_updated":"2022-08-08T18:13:16Z","latest_version":2,"primary_category":"astro-ph.HE","snapshot_observed_at":"2026-08-19T09:09:18.089168Z","submitted_at":"2021-12-20T10:48:30Z","title":"Universal relations for rapidly rotating cold and hot hybrid star"},"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":"2026-08-20T06:33:59.587034+00:00","source":"crossref"},{"observed_at":"2026-08-20T06:33:54.927442+00:00","source":"retraction_watch"}],"thesis":"As of 21 August 2026, this Paper Citation Record lists 0 of 0 outbound references and 4 inbound Pith citation observations for arXiv:2112.10439."}