{"as_of":"2026-08-06T19:51:00Z","caps":{"database_statements":6,"inbound":100,"outbound":100},"context_digest":"sha256:53ee57a1f639ba2ff8735c09b6529e17cc2e4205c1155ddaca764d239eecb448","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":"2026-08-06T06:34:29.942622+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":"2026-08-03T02:15:27.935223Z","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":"2026-07-02T19:07:18.453209Z","state":"measured"}],"external_citation_measurements":[],"inbound":[{"citation":{"cited_paper":{"arxiv_id":"2007.08493","last_updated":"2026-06-09T12:42:57Z","snapshot_observed_at":"2026-07-06T09:38:53.228850Z","submitted_at":"2020-07-16T17:45:08Z","title":"GW190814 as a massive rapidly-rotating neutron star with exotic degrees of freedom","version":3},"cited_work":{"arxiv_id":"2007.08493","doi":null,"metadata_source":"pith","pith_arxiv_id":"2007.08493","snapshot_observed_at":"2026-07-02T19:07:18.453209Z","title":"GW190814 as a massive rapidly-rotating neutron star with exotic degrees of freedom","venue":"astro-ph.HE","work_id":"3d767dfa-8285-43d1-a383-7ac697a0a9c8","year":2020},"citing_paper":{"arxiv_id":"2606.04810","last_updated":"2026-07-31T09:53:50Z","snapshot_observed_at":"2026-08-05T23:10:45.274273Z","submitted_at":"2026-06-03T12:35:35Z","title":"Fast gravitational waveform models for quasi-circular coalescences of neutron star--black hole binaries","version":1},"reference_index":19,"source":"pdf_text","source_observed_at":"2026-06-28T05:31:01.574505Z"},"links":{"cited_paper":"/paper/2007.08493","citing_paper":"/paper/2606.04810"},"observation_digest":"sha256:97673fdf99b1e4028c6b94b9315b5ebb006d59f9ab773418e41f2fb17a8653ca","observation_id":"482be2f7-577b-49e2-9f35-20e8e538258f","resolution":{"observed_at":"2026-07-02T09:26:51.423904Z","resolver_source":"local_arxiv","status":"verified_exact"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-06T06:34:29.942622+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-06T06:34:29.942622+00:00","source":"crossref"},{"observed_at":"2026-08-06T06:34:23.284952+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":{"arxiv_id":"2007.08493","last_updated":"2026-06-09T12:42:57Z","snapshot_observed_at":"2026-07-06T09:38:53.228850Z","submitted_at":"2020-07-16T17:45:08Z","title":"GW190814 as a massive rapidly-rotating neutron star with exotic degrees of freedom","version":3},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2007.08493","snapshot_observed_at":"2026-08-03T02:15:27.935223Z","title":"Dexheimer, R","venue":null,"work_id":null,"year":2021},"citing_paper":{"arxiv_id":"2606.04810","last_updated":"2026-07-31T09:53:50Z","snapshot_observed_at":"2026-08-05T23:10:45.274273Z","submitted_at":"2026-06-03T12:35:35Z","title":"Fast gravitational waveform models for quasi-circular coalescences of neutron star--black hole binaries","version":2},"reference_index":19,"source":"pdf_text","source_observed_at":"2026-08-03T02:15:27.935223Z"},"links":{"cited_paper":"/paper/2007.08493","citing_paper":"/paper/2606.04810"},"observation_digest":"sha256:2cd55799c39e3dd779d124ff51b82cd4fce3c939f9ab59a3090c0fcfb8d7e0f2","observation_id":"ff734b9e-224a-48b9-ba6e-06daacee619d","resolution":{"observed_at":"2026-08-03T02:15:27.935223Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2007.08493","last_updated":"2026-06-09T12:42:57Z","snapshot_observed_at":"2026-07-06T09:38:53.228850Z","submitted_at":"2020-07-16T17:45:08Z","title":"GW190814 as a massive rapidly-rotating neutron star with exotic degrees of freedom","version":3},"cited_work":{"arxiv_id":"2007.08493","doi":null,"metadata_source":"pith","pith_arxiv_id":"2007.08493","snapshot_observed_at":"2026-07-02T19:07:18.453209Z","title":"GW190814 as a massive rapidly-rotating neutron star with exotic degrees of freedom","venue":"astro-ph.HE","work_id":"3d767dfa-8285-43d1-a383-7ac697a0a9c8","year":2020},"citing_paper":{"arxiv_id":"2606.07742","last_updated":"2026-06-05T18:00:04Z","snapshot_observed_at":"2026-07-06T23:47:19.773490Z","submitted_at":"2026-06-05T18:00:04Z","title":"Core Composition Effects on the QCD Axion Mass Limit from Neutron Star Cooling","version":1},"reference_index":48,"source":"pdf_text","source_observed_at":"2026-06-27T21:37:55.919953Z"},"links":{"cited_paper":"/paper/2007.08493","citing_paper":"/paper/2606.07742"},"observation_digest":"sha256:be5342f9bd973ce42ae9b0513876b5e600a48da6602f3bb0dda5d5e35d98f8fb","observation_id":"d92524a4-5507-4247-8b43-0e343fdd1da7","resolution":{"observed_at":"2026-07-02T19:07:18.454397Z","resolver_source":"local_arxiv","status":"verified_exact"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-06T06:34:29.942622+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-06T06:34:29.942622+00:00","source":"crossref"},{"observed_at":"2026-08-06T06:34:23.284952+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":{"arxiv_id":"2007.08493","last_updated":"2026-06-09T12:42:57Z","snapshot_observed_at":"2026-07-06T09:38:53.228850Z","submitted_at":"2020-07-16T17:45:08Z","title":"GW190814 as a massive rapidly-rotating neutron star with exotic degrees of freedom","version":3},"cited_work":{"arxiv_id":"2007.08493","doi":null,"metadata_source":"pith","pith_arxiv_id":"2007.08493","snapshot_observed_at":"2026-07-02T19:07:18.453209Z","title":"GW190814 as a massive rapidly-rotating neutron star with exotic degrees of freedom","venue":"astro-ph.HE","work_id":"3d767dfa-8285-43d1-a383-7ac697a0a9c8","year":2020},"citing_paper":{"arxiv_id":"2606.18081","last_updated":"2026-07-12T08:39:11Z","snapshot_observed_at":"2026-08-02T05:46:42.848412Z","submitted_at":"2026-06-16T15:45:58Z","title":"The Chirp-Mass Ladder: A New Rung Emerges","version":1},"reference_index":88,"source":"arxiv_source","source_observed_at":"2026-07-11T11:50:26.030339Z"},"links":{"cited_paper":"/paper/2007.08493","citing_paper":"/paper/2606.18081"},"observation_digest":"sha256:1642e61dea9626e7f7004d748da502d9ec29d1a3b80461d4cf6cc225361202e9","observation_id":"2bf7d07b-5b19-4a47-9e89-656825ca6275","resolution":{"observed_at":"2026-06-26T23:10:14.402857Z","resolver_source":"local_arxiv","status":"verified_exact"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-06T06:34:29.942622+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-06T06:34:29.942622+00:00","source":"crossref"},{"observed_at":"2026-08-06T06:34:23.284952+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":{"arxiv_id":"2007.08493","last_updated":"2026-06-09T12:42:57Z","snapshot_observed_at":"2026-07-06T09:38:53.228850Z","submitted_at":"2020-07-16T17:45:08Z","title":"GW190814 as a massive rapidly-rotating neutron star with exotic degrees of freedom","version":3},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2007.08493","snapshot_observed_at":"2026-08-02T05:44:17.488757Z","title":"Dexheimer, R","venue":null,"work_id":null,"year":2021},"citing_paper":{"arxiv_id":"2607.13268","last_updated":"2026-07-14T21:03:17Z","snapshot_observed_at":"2026-08-06T00:54:46.121673Z","submitted_at":"2026-07-14T21:03:17Z","title":"Neural-Accelerated Bayesian Calibration of Chiral Mean-Field Models to Nuclear Saturation and Vacuum Properties","version":1},"reference_index":24,"source":"pdf_text","source_observed_at":"2026-08-02T05:44:17.488757Z"},"links":{"cited_paper":"/paper/2007.08493","citing_paper":"/paper/2607.13268"},"observation_digest":"sha256:b6cda6499336ba22aada4a0f0fe0446741bc6a0fcc731848d51958710f3a75b4","observation_id":"74ab5cb9-ce16-4864-85eb-14fb9637e621","resolution":{"observed_at":"2026-08-02T05:44:17.488757Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}}],"links":{"evidence":"/evidence","html":"/paper/2007.08493/citation-record","integrity":"/paper/2007.08493/integrity","json":"/paper/2007.08493/citation-record.json","paper":"/paper/2007.08493"},"outbound":[],"paper":{"arxiv_id":"2007.08493","last_updated":"2026-06-09T12:42:57Z","latest_version":3,"primary_category":"astro-ph.HE","snapshot_observed_at":"2026-07-06T09:38:53.228850Z","submitted_at":"2020-07-16T17:45:08Z","title":"GW190814 as a massive rapidly-rotating neutron star with exotic degrees of freedom"},"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":"2026-08-06T06:34:29.942622+00:00","source":"crossref"},{"observed_at":"2026-08-06T06:34:23.284952+00:00","source":"retraction_watch"}],"thesis":"As of 6 August 2026, this Paper Citation Record lists 0 of 0 outbound references and 5 inbound Pith citation observations for arXiv:2007.08493."}