{"as_of":"2026-08-21T10:50:00Z","caps":{"database_statements":6,"inbound":100,"outbound":100},"context_digest":"sha256:b68bb7363555f9c2aad49c5c3a018017587ea78a78825e2b10cbdd87ce2fb8c7","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":"2026-08-21T06:32:19.484+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":"2026-08-03T02:15:32.555287Z","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":"2026-07-02T09:26:51.428207Z","state":"measured"}],"external_citation_measurements":[],"inbound":[{"citation":{"cited_paper":{"arxiv_id":"1911.10440","last_updated":"2020-07-09T23:37:10Z","snapshot_observed_at":"2026-07-06T08:39:29.458110Z","submitted_at":"2019-11-24T00:59:04Z","title":"Gravitational waveforms of binary neutron star inspirals using post-Newtonian tidal splicing","version":2},"cited_work":{"arxiv_id":"1911.10440","doi":null,"metadata_source":"arxiv_reference","pith_arxiv_id":"1911.10440","snapshot_observed_at":"2026-07-02T09:26:51.428207Z","title":"Gravitational waveforms of binary neutron star inspirals using post-Newtonian tidal splicing","venue":null,"work_id":"a37df593-9d4c-481a-bf4c-dd642fb4d22d","year":2020},"citing_paper":{"arxiv_id":"2601.23019","last_updated":"2026-05-05T14:01:09Z","snapshot_observed_at":"2026-08-14T10:26:00.239666Z","submitted_at":"2026-01-30T14:27:25Z","title":"Toward claiming a detection of gravitational memory","version":2},"reference_index":121,"source":"pdf_text","source_observed_at":"2026-05-16T09:18:23.702726Z"},"links":{"cited_paper":"/paper/1911.10440","citing_paper":"/paper/2601.23019"},"observation_digest":"sha256:a1333ac5fbefed8ae6865be67f367c61acccde3a978bdd97c472b099979fea49","observation_id":"44ea3fc5-a706-4adf-b3eb-c1f81b917f68","resolution":{"observed_at":"2026-05-16T09:20:47.973495Z","resolver_source":"arxiv_id","status":"verified_exact"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-21T06:32:19.484+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-21T06:32:19.484+00:00","source":"crossref"},{"observed_at":"2026-08-21T06:32:16.066871+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":{"arxiv_id":"1911.10440","last_updated":"2020-07-09T23:37:10Z","snapshot_observed_at":"2026-07-06T08:39:29.458110Z","submitted_at":"2019-11-24T00:59:04Z","title":"Gravitational waveforms of binary neutron star inspirals using post-Newtonian tidal splicing","version":2},"cited_work":{"arxiv_id":"1911.10440","doi":null,"metadata_source":"arxiv_reference","pith_arxiv_id":"1911.10440","snapshot_observed_at":"2026-07-02T09:26:51.428207Z","title":"Gravitational waveforms of binary neutron star inspirals using post-Newtonian tidal splicing","venue":null,"work_id":"a37df593-9d4c-481a-bf4c-dd642fb4d22d","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":56,"source":"pdf_text","source_observed_at":"2026-06-28T05:31:01.574505Z"},"links":{"cited_paper":"/paper/1911.10440","citing_paper":"/paper/2606.04810"},"observation_digest":"sha256:46f255bcfca662e7eff0e02a3fe88d6ea3413e69da7a70dba3ddf747528adf84","observation_id":"79a87ab6-d99d-498c-9530-404b6eb919aa","resolution":{"observed_at":"2026-07-02T09:26:51.429562Z","resolver_source":"arxiv_id","status":"verified_exact"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-21T06:32:19.484+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-21T06:32:19.484+00:00","source":"crossref"},{"observed_at":"2026-08-21T06:32:16.066871+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":{"arxiv_id":"1911.10440","last_updated":"2020-07-09T23:37:10Z","snapshot_observed_at":"2026-07-06T08:39:29.458110Z","submitted_at":"2019-11-24T00:59:04Z","title":"Gravitational waveforms of binary neutron star inspirals using post-Newtonian tidal splicing","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"1911.10440","snapshot_observed_at":"2026-08-03T02:15:32.555287Z","title":"Barkett, Y","venue":null,"work_id":null,"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":2},"reference_index":56,"source":"pdf_text","source_observed_at":"2026-08-03T02:15:32.555287Z"},"links":{"cited_paper":"/paper/1911.10440","citing_paper":"/paper/2606.04810"},"observation_digest":"sha256:4f73e9f108f18483fcb0186abf770e9d0ed8eb684c9e8535265cf0961042c66d","observation_id":"ce799bed-e831-42d1-a63b-d71f38b7f926","resolution":{"observed_at":"2026-08-03T02:15:32.555287Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}}],"links":{"evidence":"/evidence","html":"/paper/1911.10440/citation-record","integrity":"/paper/1911.10440/integrity","json":"/paper/1911.10440/citation-record.json","paper":"/paper/1911.10440"},"outbound":[],"paper":{"arxiv_id":"1911.10440","last_updated":"2020-07-09T23:37:10Z","latest_version":2,"primary_category":"gr-qc","snapshot_observed_at":"2026-07-06T08:39:29.458110Z","submitted_at":"2019-11-24T00:59:04Z","title":"Gravitational waveforms of binary neutron star inspirals using post-Newtonian tidal splicing"},"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":"2026-08-21T06:32:19.484+00:00","source":"crossref"},{"observed_at":"2026-08-21T06:32:16.066871+00:00","source":"retraction_watch"}],"thesis":"As of 21 August 2026, this Paper Citation Record lists 0 of 0 outbound references and 3 inbound Pith citation observations for arXiv:1911.10440."}