{"as_of":"2026-08-05T10:25:00Z","caps":{"database_statements":6,"inbound":100,"outbound":100},"context_digest":"sha256:ffb0dae6b9d513f12d8a56b3cddb26be630fc6d183e814c3b04b409fb4b626e2","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":"2026-08-05T06:32:48.257954+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":"2026-05-24T08:53:31.777812Z","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":"2026-05-24T08:54:15.785878Z","state":"measured"}],"external_citation_measurements":[],"inbound":[{"citation":{"cited_paper":{"arxiv_id":"1204.1043","last_updated":"2012-09-28T16:40:29Z","snapshot_observed_at":"2026-07-06T02:45:46.840279Z","submitted_at":"2012-04-04T19:33:03Z","title":"The third and a half post-Newtonian gravitational wave quadrupole mode for quasi-circular inspiralling compact binaries","version":2},"cited_work":{"arxiv_id":"1204.1043","doi":null,"metadata_source":"pith","pith_arxiv_id":"1204.1043","snapshot_observed_at":"2026-06-05T21:23:00.469572Z","title":"The third and a half post-Newtonian gravitational wave quadrupole mode for quasi-circular inspiralling compact binaries","venue":"gr-qc","work_id":"e4a27147-325f-4c50-8bf9-41108c870f8d","year":2012},"citing_paper":{"arxiv_id":"2305.15473","last_updated":"2026-04-04T14:44:55Z","snapshot_observed_at":"2026-07-06T15:32:54.279309Z","submitted_at":"2023-05-24T18:00:04Z","title":"Worldline effective field theory of inspiralling black hole binaries in presence of dark photon and axionic dark matter","version":4},"reference_index":17,"source":"pdf_text","source_observed_at":"2026-05-24T08:53:31.777812Z"},"links":{"cited_paper":"/paper/1204.1043","citing_paper":"/paper/2305.15473"},"observation_digest":"sha256:1c3710102cfc0d56333ca640f75e615df1cea4be68b2abbe8c66d13387f6b348","observation_id":"35deb553-46ed-45f5-b536-c8a583c81f68","resolution":{"observed_at":"2026-05-24T08:54:15.788477Z","resolver_source":"local_arxiv","status":"verified_exact"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-05T06:32:48.257954+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-05T06:32:48.257954+00:00","source":"crossref"},{"observed_at":"2026-08-05T06:32:44.755628+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":{"arxiv_id":"1204.1043","last_updated":"2012-09-28T16:40:29Z","snapshot_observed_at":"2026-07-06T02:45:46.840279Z","submitted_at":"2012-04-04T19:33:03Z","title":"The third and a half post-Newtonian gravitational wave quadrupole mode for quasi-circular inspiralling compact binaries","version":2},"cited_work":{"arxiv_id":"1204.1043","doi":null,"metadata_source":"pith","pith_arxiv_id":"1204.1043","snapshot_observed_at":"2026-06-05T21:23:00.469572Z","title":"The third and a half post-Newtonian gravitational wave quadrupole mode for quasi-circular inspiralling compact binaries","venue":"gr-qc","work_id":"e4a27147-325f-4c50-8bf9-41108c870f8d","year":2012},"citing_paper":{"arxiv_id":"2605.08798","last_updated":"2026-05-09T08:44:16Z","snapshot_observed_at":"2026-07-06T23:20:57.084438Z","submitted_at":"2026-05-09T08:44:16Z","title":"Gravitational waveform from radial infall at the third-and-half Post-Newtonian order","version":1},"reference_index":34,"source":"pdf_text","source_observed_at":"2026-05-12T01:40:05.664304Z"},"links":{"cited_paper":"/paper/1204.1043","citing_paper":"/paper/2605.08798"},"observation_digest":"sha256:cf3aa9848ea853472c2f7b0b301b2159bbc63f44bb8c30c00e3623ba8599310d","observation_id":"4c6c94a4-2aed-4c28-a4ea-43733983e0da","resolution":{"observed_at":"2026-05-12T01:41:20.138632Z","resolver_source":"arxiv_id","status":"verified_exact"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-05T06:32:48.257954+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-05T06:32:48.257954+00:00","source":"crossref"},{"observed_at":"2026-08-05T06:32:44.755628+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":{"arxiv_id":"1204.1043","last_updated":"2012-09-28T16:40:29Z","snapshot_observed_at":"2026-07-06T02:45:46.840279Z","submitted_at":"2012-04-04T19:33:03Z","title":"The third and a half post-Newtonian gravitational wave quadrupole mode for quasi-circular inspiralling compact binaries","version":2},"cited_work":{"arxiv_id":"1204.1043","doi":null,"metadata_source":"pith","pith_arxiv_id":"1204.1043","snapshot_observed_at":"2026-06-05T21:23:00.469572Z","title":"The third and a half post-Newtonian gravitational wave quadrupole mode for quasi-circular inspiralling compact binaries","venue":"gr-qc","work_id":"e4a27147-325f-4c50-8bf9-41108c870f8d","year":2012},"citing_paper":{"arxiv_id":"2605.20562","last_updated":"2026-05-19T23:44:55Z","snapshot_observed_at":"2026-07-06T23:31:08.671011Z","submitted_at":"2026-05-19T23:44:55Z","title":"Convergence of post-Newtonian for quasi-circular non-precessing comparable mass ratios BBHs","version":1},"reference_index":43,"source":"pdf_text","source_observed_at":"2026-05-21T06:22:04.929858Z"},"links":{"cited_paper":"/paper/1204.1043","citing_paper":"/paper/2605.20562"},"observation_digest":"sha256:9a06ad68cbd790aa4dcf6165d50c5846d5eb5d4227242e7d69ce72c83eae9d03","observation_id":"2e518248-8694-410f-a2b5-64f4898430c5","resolution":{"observed_at":"2026-05-21T06:24:00.587439Z","resolver_source":"local_arxiv","status":"verified_exact"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-05T06:32:48.257954+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-05T06:32:48.257954+00:00","source":"crossref"},{"observed_at":"2026-08-05T06:32:44.755628+00:00","source":"retraction_watch"}],"state":"measured"}}],"links":{"evidence":"/evidence","html":"/paper/1204.1043/citation-record","integrity":"/paper/1204.1043/integrity","json":"/paper/1204.1043/citation-record.json","paper":"/paper/1204.1043"},"outbound":[],"paper":{"arxiv_id":"1204.1043","last_updated":"2012-09-28T16:40:29Z","latest_version":2,"primary_category":"gr-qc","snapshot_observed_at":"2026-07-06T02:45:46.840279Z","submitted_at":"2012-04-04T19:33:03Z","title":"The third and a half post-Newtonian gravitational wave quadrupole mode for quasi-circular inspiralling compact binaries"},"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":"2026-08-05T06:32:48.257954+00:00","source":"crossref"},{"observed_at":"2026-08-05T06:32:44.755628+00:00","source":"retraction_watch"}],"thesis":"As of 5 August 2026, this Paper Citation Record lists 0 of 0 outbound references and 3 inbound Pith citation observations for arXiv:1204.1043."}