{"as_of":"2026-08-16T15:19:00Z","caps":{"database_statements":6,"inbound":100,"outbound":100},"context_digest":"sha256:92ad0a551207f8594341bbcf08a573a0e10e096bcf66a2ee4212ec8dcba8ad56","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":3,"lane":"standing_notices","note":"One-hop event checks from named stored sources.","records_observed":3,"source":"scholarly_work_events, retraction_status_cache","source_observed_at":"2026-08-16T06:30:59.297886+00:00","state":"measured"},{"denominator":3,"lane":"inbound_itemization","note":"Pith citing papers itemized under the disclosed page cap.","records_observed":3,"source":"paper_references, paper_reference_links","source_observed_at":"2026-08-16T04:38:46.954357Z","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":"2026-08-15T15:58:54.575035Z","state":"measured"}],"external_citation_measurements":[],"inbound":[{"citation":{"cited_paper":{"arxiv_id":"2007.02513","last_updated":"2020-09-01T00:29:15Z","snapshot_observed_at":"2026-07-06T09:35:35.885280Z","submitted_at":"2020-07-06T03:44:43Z","title":"GW190814's secondary component with mass $(2.50-2.67)$ M$_{\\odot}$ as a super-fast pulsar","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2007.02513","snapshot_observed_at":"2026-08-16T04:38:46.954357Z","title":"Zhang and B.-A","venue":null,"work_id":null,"year":2020},"citing_paper":{"arxiv_id":"2505.00911","last_updated":"2025-07-03T08:25:05Z","snapshot_observed_at":"2026-08-16T07:13:43.337592Z","submitted_at":"2025-05-01T23:15:31Z","title":"Bayesian inferences on covariant density functionals from multimessenger astrophysical data: The impacts of likelihood functions of low density matter constraints","version":2},"reference_index":14,"source":"pdf_text","source_observed_at":"2026-08-16T04:38:46.954357Z"},"links":{"cited_paper":"/paper/2007.02513","citing_paper":"/paper/2505.00911"},"observation_digest":"sha256:1b72373210e79c4779ad521b308a51b0154f83febd24bfddf52a2bd017bc24c9","observation_id":"7575fbd4-9f82-48dc-9671-5841f83aaf71","resolution":{"observed_at":"2026-08-16T04:38:46.954357Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2007.02513","last_updated":"2020-09-01T00:29:15Z","snapshot_observed_at":"2026-07-06T09:35:35.885280Z","submitted_at":"2020-07-06T03:44:43Z","title":"GW190814's secondary component with mass $(2.50-2.67)$ M$_{\\odot}$ as a super-fast pulsar","version":2},"cited_work":{"arxiv_id":"2007.02513","doi":null,"metadata_source":"pith","pith_arxiv_id":"2007.02513","snapshot_observed_at":"2026-08-15T15:58:54.575035Z","title":"GW190814's secondary component with mass $(2.50-2.67)$ M$_{\\odot}$ as a super-fast pulsar","venue":"astro-ph.HE","work_id":"1203ce43-81c9-4ffd-a513-490901b2c850","year":2020},"citing_paper":{"arxiv_id":"2509.10420","last_updated":"2025-09-12T17:18:32Z","snapshot_observed_at":"2026-08-16T09:15:47.099026Z","submitted_at":"2025-09-12T17:18:32Z","title":"Testing the nature of compact objects in the lower mass gap using gravitational wave observations","version":1},"reference_index":87,"source":"pdf_text","source_observed_at":"2026-08-15T15:58:53.841699Z"},"links":{"cited_paper":"/paper/2007.02513","citing_paper":"/paper/2509.10420"},"observation_digest":"sha256:665e69966f85286ad9ac9b5c67454a14bf0837c153c8b25267b15fc56b20199f","observation_id":"50699409-aa04-446b-add7-4784aaa9df43","resolution":{"observed_at":"2026-08-15T15:58:54.588334Z","resolver_source":"local_arxiv","status":"verified_exact"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-16T06:30:59.297886+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-16T06:30:59.297886+00:00","source":"crossref"},{"observed_at":"2026-08-16T06:30:54.164669+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":{"arxiv_id":"2007.02513","last_updated":"2020-09-01T00:29:15Z","snapshot_observed_at":"2026-07-06T09:35:35.885280Z","submitted_at":"2020-07-06T03:44:43Z","title":"GW190814's secondary component with mass $(2.50-2.67)$ M$_{\\odot}$ as a super-fast pulsar","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2007.02513","snapshot_observed_at":"2026-08-16T00:09:07.067617Z","title":"GW190814's Secondary Component with Mass 2.50 2.67 M _ as a Superfast Pulsar","venue":null,"work_id":null,"year":2020},"citing_paper":{"arxiv_id":"2608.12632","last_updated":"2026-08-12T22:44:40Z","snapshot_observed_at":"2026-08-16T15:12:45.446848Z","submitted_at":"2026-08-12T22:44:40Z","title":"How Neutron Star Radii Encode the Dense-Matter Equation of State and Hadron-Quark Transition","version":1},"reference_index":143,"source":"arxiv_source","source_observed_at":"2026-08-16T00:09:07.067617Z"},"links":{"cited_paper":"/paper/2007.02513","citing_paper":"/paper/2608.12632"},"observation_digest":"sha256:151ca471d188ab1c89d6abb0748cc0ffb8ab337179e3440e9ce7f16a3982fe2c","observation_id":"911a7b46-f40a-4726-b136-1d815e7e5dd2","resolution":{"observed_at":"2026-08-16T00:09:07.067617Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}}],"links":{"evidence":"/evidence","html":"/paper/2007.02513/citation-record","integrity":"/paper/2007.02513/integrity","json":"/paper/2007.02513/citation-record.json","paper":"/paper/2007.02513"},"outbound":[],"paper":{"arxiv_id":"2007.02513","last_updated":"2020-09-01T00:29:15Z","latest_version":2,"primary_category":"astro-ph.HE","snapshot_observed_at":"2026-07-06T09:35:35.885280Z","submitted_at":"2020-07-06T03:44:43Z","title":"GW190814's secondary component with mass $(2.50-2.67)$ M$_{\\odot}$ as a super-fast pulsar"},"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":"2026-08-16T06:30:59.297886+00:00","source":"crossref"},{"observed_at":"2026-08-16T06:30:54.164669+00:00","source":"retraction_watch"}],"thesis":"As of 16 August 2026, this Paper Citation Record lists 0 of 0 outbound references and 3 inbound Pith citation observations for arXiv:2007.02513."}