{"as_of":"2026-08-17T18:03:00Z","caps":{"database_statements":6,"inbound":100,"outbound":100},"context_digest":"sha256:fd11a199159f0f6a50f24cbbb08c0d114a9f925b0db6dd51d9b62e0a1ecabf6c","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":2,"lane":"standing_notices","note":"One-hop event checks from named stored sources.","records_observed":2,"source":"scholarly_work_events, retraction_status_cache","source_observed_at":"2026-08-17T06:30:58.91139+00:00","state":"measured"},{"denominator":2,"lane":"inbound_itemization","note":"Pith citing papers itemized under the disclosed page cap.","records_observed":2,"source":"paper_references, paper_reference_links","source_observed_at":"2026-08-15T23:10:59.601512Z","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":"2026-06-29T20:33:58.120782Z","state":"measured"}],"external_citation_measurements":[],"inbound":[{"citation":{"cited_paper":{"arxiv_id":"1312.4532","last_updated":"2014-05-17T15:55:02Z","snapshot_observed_at":"2026-08-14T23:51:26.880922Z","submitted_at":"2013-12-16T21:00:00Z","title":"Three-Hair Relations for Rotating Stars: Nonrelativistic Limit","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"1312.4532","snapshot_observed_at":"2026-08-15T23:10:59.601512Z","title":null,"venue":null,"work_id":null,"year":2014},"citing_paper":{"arxiv_id":"2505.05429","last_updated":"2025-07-14T15:36:29Z","snapshot_observed_at":"2026-08-17T12:11:52.400416Z","submitted_at":"2025-05-08T17:19:11Z","title":"Theoretical modeling of approximate universality of tidally deformed neutron stars","version":2},"reference_index":52,"source":"pdf_text","source_observed_at":"2026-08-15T23:10:59.601512Z"},"links":{"cited_paper":"/paper/1312.4532","citing_paper":"/paper/2505.05429"},"observation_digest":"sha256:299de7be8637a7524d85c2a8fc6298b97d8127c0eb717e381cbacd9048eca08e","observation_id":"12781114-f2e9-49e4-a334-ae60df973122","resolution":{"observed_at":"2026-08-15T23:10:59.601512Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"1312.4532","last_updated":"2014-05-17T15:55:02Z","snapshot_observed_at":"2026-08-14T23:51:26.880922Z","submitted_at":"2013-12-16T21:00:00Z","title":"Three-Hair Relations for Rotating Stars: Nonrelativistic Limit","version":2},"cited_work":{"arxiv_id":"1312.4532","doi":null,"metadata_source":"pith","pith_arxiv_id":"1312.4532","snapshot_observed_at":"2026-06-29T20:33:58.120782Z","title":"Three-Hair Relations for Rotating Stars: Nonrelativistic Limit","venue":"gr-qc","work_id":"996d2cad-ca4b-4262-bcd3-d9f8ac3b318d","year":2013},"citing_paper":{"arxiv_id":"2605.26228","last_updated":"2026-05-25T18:00:28Z","snapshot_observed_at":"2026-08-01T21:44:38.475132Z","submitted_at":"2026-05-25T18:00:28Z","title":"Donutization Inside Neutron Stars: Shell-Localized Scalar Fields","version":1},"reference_index":89,"source":"pdf_text","source_observed_at":"2026-06-29T20:33:28.058638Z"},"links":{"cited_paper":"/paper/1312.4532","citing_paper":"/paper/2605.26228"},"observation_digest":"sha256:ff50e3d48292eb7801a12cae2ea89a8490faa79347cb90d175297fd1eb1c5a55","observation_id":"444dca37-03cf-43f7-92a3-b5689473ea58","resolution":{"observed_at":"2026-06-29T20:33:58.122212Z","resolver_source":"local_arxiv","status":"verified_exact"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-17T06:30:58.91139+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-17T06:30:58.91139+00:00","source":"crossref"},{"observed_at":"2026-08-17T06:30:54.323127+00:00","source":"retraction_watch"}],"state":"measured"}}],"links":{"evidence":"/evidence","html":"/paper/1312.4532/citation-record","integrity":"/paper/1312.4532/integrity","json":"/paper/1312.4532/citation-record.json","paper":"/paper/1312.4532"},"outbound":[],"paper":{"arxiv_id":"1312.4532","last_updated":"2014-05-17T15:55:02Z","latest_version":2,"primary_category":"gr-qc","snapshot_observed_at":"2026-08-14T23:51:26.880922Z","submitted_at":"2013-12-16T21:00:00Z","title":"Three-Hair Relations for Rotating Stars: Nonrelativistic Limit"},"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":"2026-08-17T06:30:58.91139+00:00","source":"crossref"},{"observed_at":"2026-08-17T06:30:54.323127+00:00","source":"retraction_watch"}],"thesis":"As of 17 August 2026, this Paper Citation Record lists 0 of 0 outbound references and 2 inbound Pith citation observations for arXiv:1312.4532."}