{"as_of":"2026-08-11T08:37:00Z","caps":{"database_statements":6,"inbound":100,"outbound":100},"context_digest":"sha256:630d6223404d3537813b24b7259827abe14241523ae3ba138ca96333ed790dac","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":"2026-08-11T06:34:44.6726+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":"2026-08-10T16:33:19.714349Z","state":"measured"},{"denominator":1,"lane":"external_citation_measurements","note":"A source-named dated measurement, never combined with another source.","records_observed":0,"source":"arxiv_reference","source_observed_at":"2026-07-09T08:05:16.230513Z","state":"measured"}],"external_citation_measurements":[],"inbound":[{"citation":{"cited_paper":{"arxiv_id":"2202.05161","last_updated":"2022-06-19T09:22:41Z","snapshot_observed_at":"2026-07-06T12:36:30.798420Z","submitted_at":"2022-01-31T19:18:54Z","title":"Dynamical tides in superfluid neutron stars","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2202.05161","snapshot_observed_at":"2026-08-10T16:33:19.714349Z","title":"Passamonti, N","venue":null,"work_id":null,"year":2022},"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":43,"source":"pdf_text","source_observed_at":"2026-08-10T16:33:19.714349Z"},"links":{"cited_paper":"/paper/2202.05161","citing_paper":"/paper/2501.13064"},"observation_digest":"sha256:8da45d7c8234e038f2a50e3101aaef53ae0ea44fd0e671d7bcbea1565b3e997a","observation_id":"15a1427b-8814-4387-8ffe-66b95791cdcb","resolution":{"observed_at":"2026-08-10T16:33:19.714349Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2202.05161","last_updated":"2022-06-19T09:22:41Z","snapshot_observed_at":"2026-07-06T12:36:30.798420Z","submitted_at":"2022-01-31T19:18:54Z","title":"Dynamical tides in superfluid neutron stars","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2202.05161","snapshot_observed_at":"2026-07-13T17:23:25.842886Z","title":"Dynamical tides in superfluid neutron stars,","venue":null,"work_id":null,"year":2022},"citing_paper":{"arxiv_id":"2603.26885","last_updated":"2026-05-29T07:50:42Z","snapshot_observed_at":"2026-08-03T05:39:04.714659Z","submitted_at":"2026-03-27T18:02:32Z","title":"TTE-CAM: Self-Explainable Class Activation Maps for Pretrained Black-Box CNNs","version":2},"reference_index":39,"source":"pdf_text","source_observed_at":"2026-07-13T17:23:25.842886Z"},"links":{"cited_paper":"/paper/2202.05161","citing_paper":"/paper/2603.26885"},"observation_digest":"sha256:30c78f5edf7f45fc81fa4fdb63204cbfe3f235c21ae43183165f5eb794c0a342","observation_id":"0b4a2083-3e5d-4902-9897-f03a52ef1a8a","resolution":{"observed_at":"2026-07-13T17:23:25.842886Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2202.05161","last_updated":"2022-06-19T09:22:41Z","snapshot_observed_at":"2026-07-06T12:36:30.798420Z","submitted_at":"2022-01-31T19:18:54Z","title":"Dynamical tides in superfluid neutron stars","version":2},"cited_work":{"arxiv_id":"2202.05161","doi":"10.1093/mnras/stac1380.arxiv:2202.05161","metadata_source":"arxiv_reference","pith_arxiv_id":"2202.05161","snapshot_observed_at":"2026-07-11T11:50:26.030339Z","title":"Passamonti, N","venue":null,"work_id":"aa828f22-8e0d-4cf2-a076-ef087e107b0b","year":2022},"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":88,"source":"pdf_text","source_observed_at":"2026-05-10T17:33:47.120981Z"},"links":{"cited_paper":"/paper/2202.05161","citing_paper":"/paper/2604.08653"},"observation_digest":"sha256:e241e930d8cd8635c758a900044f3f10cdb6940c1ebbac37a153f10846c28a24","observation_id":"a3c5c9ae-7d00-40b6-b327-eb3055b9e58d","resolution":{"observed_at":"2026-05-10T17:35:40.024532Z","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":"2202.05161","last_updated":"2022-06-19T09:22:41Z","snapshot_observed_at":"2026-07-06T12:36:30.798420Z","submitted_at":"2022-01-31T19:18:54Z","title":"Dynamical tides in superfluid neutron stars","version":2},"cited_work":{"arxiv_id":"2202.05161","doi":"10.1093/mnras/stac1380.arxiv:2202.05161","metadata_source":"arxiv_reference","pith_arxiv_id":"2202.05161","snapshot_observed_at":"2026-07-11T11:50:26.030339Z","title":"Passamonti, N","venue":null,"work_id":"aa828f22-8e0d-4cf2-a076-ef087e107b0b","year":2022},"citing_paper":{"arxiv_id":"2606.19446","last_updated":"2026-06-17T18:00:06Z","snapshot_observed_at":"2026-08-08T23:32:37.826386Z","submitted_at":"2026-06-17T18:00:06Z","title":"Dynamical Tidal Response of Neutron Stars: from Effective Field Theory to Gravitational Waveforms","version":1},"reference_index":24,"source":"pdf_text","source_observed_at":"2026-06-26T19:56:39.553970Z"},"links":{"cited_paper":"/paper/2202.05161","citing_paper":"/paper/2606.19446"},"observation_digest":"sha256:7f61667047bc6678cc25aa0bb838d4de28ca41340443b4fc1c8301890d0278e7","observation_id":"451097cd-b300-4c78-b87f-99e156183114","resolution":{"observed_at":"2026-07-04T02:09:23.173289Z","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"}}],"links":{"evidence":"/evidence","html":"/paper/2202.05161/citation-record","integrity":"/paper/2202.05161/integrity","json":"/paper/2202.05161/citation-record.json","paper":"/paper/2202.05161"},"outbound":[],"paper":{"arxiv_id":"2202.05161","last_updated":"2022-06-19T09:22:41Z","latest_version":2,"primary_category":"astro-ph.HE","snapshot_observed_at":"2026-07-06T12:36:30.798420Z","submitted_at":"2022-01-31T19:18:54Z","title":"Dynamical tides in superfluid 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 4 inbound Pith citation observations for arXiv:2202.05161."}