{"as_of":"2026-08-11T13:45:00Z","caps":{"database_statements":6,"inbound":100,"outbound":100},"context_digest":"sha256:e778b8554d6cefb8f333ec99ded4e9c94f1c429f3e65c32bc3a7dd419acd2c88","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":"2026-08-11T06:34:44.6726+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":"2026-08-10T16:33:19.844614Z","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":"2026-07-10T15:07:19.539771Z","state":"measured"}],"external_citation_measurements":[],"inbound":[{"citation":{"cited_paper":{"arxiv_id":"1509.06975","last_updated":"2016-03-07T17:25:41Z","snapshot_observed_at":"2026-08-07T19:20:24.004295Z","submitted_at":"2015-09-22T00:50:45Z","title":"Growth rate of the tidal p-mode g-mode instability in coalescing binary neutron stars","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"1509.06975","snapshot_observed_at":"2026-08-10T16:33:19.844614Z","title":null,"venue":null,"work_id":null,"year":2016},"citing_paper":{"arxiv_id":"2501.13064","last_updated":"2025-03-07T22:36:49Z","snapshot_observed_at":"2026-08-10T16:40:19.014391Z","submitted_at":"2025-01-22T18:18:47Z","title":"Effective-one-body model for coalescing binary neutron stars: Incorporating tidal spin and enhanced radiation from dynamical tides","version":2},"reference_index":57,"source":"pdf_text","source_observed_at":"2026-08-10T16:33:19.844614Z"},"links":{"cited_paper":"/paper/1509.06975","citing_paper":"/paper/2501.13064"},"observation_digest":"sha256:2e472cb34aee948fd666bd24d177fa49572a5b8f2dcfb2232b09c0c6d4c5a543","observation_id":"2565f0e0-2f87-4eb6-b47d-3b2108097e8b","resolution":{"observed_at":"2026-08-10T16:33:19.844614Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"1509.06975","last_updated":"2016-03-07T17:25:41Z","snapshot_observed_at":"2026-08-07T19:20:24.004295Z","submitted_at":"2015-09-22T00:50:45Z","title":"Growth rate of the tidal p-mode g-mode instability in coalescing binary neutron stars","version":2},"cited_work":{"arxiv_id":"1509.06975","doi":"10.3847/0004-637x/819/2/109.arxiv:1509.06975","metadata_source":"pith","pith_arxiv_id":"1509.06975","snapshot_observed_at":"2026-07-11T11:50:26.030339Z","title":"Growth rate of the tidal p-mode g-mode instability in coalescing binary neutron stars","venue":"astro-ph.SR","work_id":"af203387-7044-48f3-8009-65adefe5926c","year":2015},"citing_paper":{"arxiv_id":"2604.08653","last_updated":"2026-04-09T18:00:01Z","snapshot_observed_at":"2026-07-06T02:11:23.670680Z","submitted_at":"2026-04-09T18:00:01Z","title":"Love numbers of black holes and compact objects","version":1},"reference_index":96,"source":"pdf_text","source_observed_at":"2026-05-10T17:33:47.120981Z"},"links":{"cited_paper":"/paper/1509.06975","citing_paper":"/paper/2604.08653"},"observation_digest":"sha256:64fb382c525f9537f1241cb55066657310123a63179bc1278838a5bd082fe923","observation_id":"23262401-c3cb-444b-918e-f7a0131c7f24","resolution":{"observed_at":"2026-07-04T20:53:26.410752Z","resolver_source":"arxiv_id","status":"verified_exact"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-11T06:34:44.6726+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-11T06:34:44.6726+00:00","source":"crossref"},{"observed_at":"2026-08-11T06:34:36.301508+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":{"arxiv_id":"1509.06975","last_updated":"2016-03-07T17:25:41Z","snapshot_observed_at":"2026-08-07T19:20:24.004295Z","submitted_at":"2015-09-22T00:50:45Z","title":"Growth rate of the tidal p-mode g-mode instability in coalescing binary neutron stars","version":2},"cited_work":{"arxiv_id":"1509.06975","doi":"10.3847/0004-637x/819/2/109.arxiv:1509.06975","metadata_source":"pith","pith_arxiv_id":"1509.06975","snapshot_observed_at":"2026-07-11T11:50:26.030339Z","title":"Growth rate of the tidal p-mode g-mode instability in coalescing binary neutron stars","venue":"astro-ph.SR","work_id":"af203387-7044-48f3-8009-65adefe5926c","year":2015},"citing_paper":{"arxiv_id":"2607.07943","last_updated":"2026-07-08T21:42:21Z","snapshot_observed_at":"2026-08-03T10:13:10.859235Z","submitted_at":"2026-07-08T21:42:21Z","title":"Nonlinear hydrodynamics in spinning neutron stars: Theoretical universal relations and equilibrium solutions","version":1},"reference_index":55,"source":"pdf_text","source_observed_at":"2026-07-10T15:01:14.878332Z"},"links":{"cited_paper":"/paper/1509.06975","citing_paper":"/paper/2607.07943"},"observation_digest":"sha256:5da2f5753d3e8f0837b97d99bfc0fc8e7f3531605ec7690c3e38143c06b933b5","observation_id":"331664e0-c73a-4e4f-ad68-e2f58f514744","resolution":{"observed_at":"2026-07-10T15:07:19.540988Z","resolver_source":"local_arxiv","status":"verified_exact"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-11T06:34:44.6726+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-11T06:34:44.6726+00:00","source":"crossref"},{"observed_at":"2026-08-11T06:34:36.301508+00:00","source":"retraction_watch"}],"state":"measured"}}],"links":{"evidence":"/evidence","html":"/paper/1509.06975/citation-record","integrity":"/paper/1509.06975/integrity","json":"/paper/1509.06975/citation-record.json","paper":"/paper/1509.06975"},"outbound":[],"paper":{"arxiv_id":"1509.06975","last_updated":"2016-03-07T17:25:41Z","latest_version":2,"primary_category":"astro-ph.SR","snapshot_observed_at":"2026-08-07T19:20:24.004295Z","submitted_at":"2015-09-22T00:50:45Z","title":"Growth rate of the tidal p-mode g-mode instability in coalescing binary neutron stars"},"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":"2026-08-11T06:34:44.6726+00:00","source":"crossref"},{"observed_at":"2026-08-11T06:34:36.301508+00:00","source":"retraction_watch"}],"thesis":"As of 11 August 2026, this Paper Citation Record lists 0 of 0 outbound references and 3 inbound Pith citation observations for arXiv:1509.06975."}