{"as_of":"2026-08-05T20:38:00Z","caps":{"database_statements":6,"inbound":100,"outbound":100},"context_digest":"sha256:a75f875d3a0e3a03cb430b2ce84f412b34c610d2fba59e5f558b4fcb5315c0ce","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":6,"lane":"standing_notices","note":"One-hop event checks from named stored sources.","records_observed":6,"source":"scholarly_work_events, retraction_status_cache","source_observed_at":"2026-08-05T06:32:48.257954+00:00","state":"measured"},{"denominator":6,"lane":"inbound_itemization","note":"Pith citing papers itemized under the disclosed page cap.","records_observed":6,"source":"paper_references, paper_reference_links","source_observed_at":"2026-08-05T16:34:15.518159Z","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":"2026-06-29T01:02:55.899180Z","state":"measured"}],"external_citation_measurements":[],"inbound":[{"citation":{"cited_paper":{"arxiv_id":"2209.04060","last_updated":"2023-03-06T15:51:10Z","snapshot_observed_at":"2026-07-06T13:50:22.878139Z","submitted_at":"2022-09-08T23:27:37Z","title":"Priorities in gravitational waveforms for future space-borne detectors: vacuum accuracy or environment?","version":2},"cited_work":{"arxiv_id":"2209.04060","doi":null,"metadata_source":"arxiv_reference","pith_arxiv_id":"2209.04060","snapshot_observed_at":"2026-06-29T01:02:55.899180Z","title":"R., & Mayer, L","venue":null,"work_id":"3d132ec2-e5af-435c-99ea-c4be84266076","year":2023},"citing_paper":{"arxiv_id":"2303.16204","last_updated":"2026-04-24T16:42:31Z","snapshot_observed_at":"2026-07-06T15:09:08.648296Z","submitted_at":"2023-03-28T17:59:59Z","title":"The Decoupling of Binaries from Their Circumbinary Disks","version":3},"reference_index":63,"source":"pdf_text","source_observed_at":"2026-05-24T09:45:11.194350Z"},"links":{"cited_paper":"/paper/2209.04060","citing_paper":"/paper/2303.16204"},"observation_digest":"sha256:5bb5b84186570ca1a7d109c46c76e049829c60be3a3f1db7d804fe1aa21c52d4","observation_id":"502f5a4e-b9a0-4cb7-889b-5905fecd0340","resolution":{"observed_at":"2026-05-24T09:46:07.330955Z","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":"2209.04060","last_updated":"2023-03-06T15:51:10Z","snapshot_observed_at":"2026-07-06T13:50:22.878139Z","submitted_at":"2022-09-08T23:27:37Z","title":"Priorities in gravitational waveforms for future space-borne detectors: vacuum accuracy or environment?","version":2},"cited_work":{"arxiv_id":"2209.04060","doi":null,"metadata_source":"arxiv_reference","pith_arxiv_id":"2209.04060","snapshot_observed_at":"2026-06-29T01:02:55.899180Z","title":"R., & Mayer, L","venue":null,"work_id":"3d132ec2-e5af-435c-99ea-c4be84266076","year":2023},"citing_paper":{"arxiv_id":"2501.12213","last_updated":"2026-04-14T00:30:19Z","snapshot_observed_at":"2026-07-06T20:23:53.794006Z","submitted_at":"2025-01-21T15:30:36Z","title":"Black holes surrounded by dark matter spike: Spacetime metrics and gravitational wave ringdown waveforms","version":2},"reference_index":14,"source":"pdf_text","source_observed_at":"2026-05-23T04:50:40.516949Z"},"links":{"cited_paper":"/paper/2209.04060","citing_paper":"/paper/2501.12213"},"observation_digest":"sha256:7675534b89657964fd8eb173dc54d1f3b3a99a0c9aa299399e27a9a266b9b6ff","observation_id":"ba8f5217-749e-4b7e-b43a-e8583dbb8030","resolution":{"observed_at":"2026-05-23T04:52:34.099119Z","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":"2209.04060","last_updated":"2023-03-06T15:51:10Z","snapshot_observed_at":"2026-07-06T13:50:22.878139Z","submitted_at":"2022-09-08T23:27:37Z","title":"Priorities in gravitational waveforms for future space-borne detectors: vacuum accuracy or environment?","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2209.04060","snapshot_observed_at":"2026-08-05T16:34:15.518159Z","title":"Zwick, P","venue":null,"work_id":null,"year":2023},"citing_paper":{"arxiv_id":"2508.18362","last_updated":"2025-08-25T18:00:07Z","snapshot_observed_at":"2026-08-05T16:34:14.431436Z","submitted_at":"2025-08-25T18:00:07Z","title":"Scalar fields from nonlinear sigma models on black hole spacetimes","version":1},"reference_index":17,"source":"pdf_text","source_observed_at":"2026-08-05T16:34:15.518159Z"},"links":{"cited_paper":"/paper/2209.04060","citing_paper":"/paper/2508.18362"},"observation_digest":"sha256:f75fba3c7a9eb987c786d432fec056b44c6c22f025437d13f1e112f6a68f9e7d","observation_id":"4b4601c4-0111-4154-896e-8e2f25ba85a8","resolution":{"observed_at":"2026-08-05T16:34:15.518159Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2209.04060","last_updated":"2023-03-06T15:51:10Z","snapshot_observed_at":"2026-07-06T13:50:22.878139Z","submitted_at":"2022-09-08T23:27:37Z","title":"Priorities in gravitational waveforms for future space-borne detectors: vacuum accuracy or environment?","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2209.04060","snapshot_observed_at":"2026-08-03T01:15:25.129977Z","title":"Zwick, P","venue":null,"work_id":null,"year":2023},"citing_paper":{"arxiv_id":"2602.10579","last_updated":"2026-06-16T11:09:53Z","snapshot_observed_at":"2026-08-05T04:56:08.228942Z","submitted_at":"2026-02-11T07:08:30Z","title":"Geometric properties of slowly rotating black holes embedded in matter environments","version":2},"reference_index":7,"source":"pdf_text","source_observed_at":"2026-08-03T01:15:25.129977Z"},"links":{"cited_paper":"/paper/2209.04060","citing_paper":"/paper/2602.10579"},"observation_digest":"sha256:b8d3cd062c5f8e68e7bad72ab76aeee46c94b979f4e6769d9b34b5e4fafc6bb3","observation_id":"33bea11c-4cba-4c39-a992-a6e471327142","resolution":{"observed_at":"2026-08-03T01:15:25.129977Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2209.04060","last_updated":"2023-03-06T15:51:10Z","snapshot_observed_at":"2026-07-06T13:50:22.878139Z","submitted_at":"2022-09-08T23:27:37Z","title":"Priorities in gravitational waveforms for future space-borne detectors: vacuum accuracy or environment?","version":2},"cited_work":{"arxiv_id":"2209.04060","doi":null,"metadata_source":"arxiv_reference","pith_arxiv_id":"2209.04060","snapshot_observed_at":"2026-06-29T01:02:55.899180Z","title":"R., & Mayer, L","venue":null,"work_id":"3d132ec2-e5af-435c-99ea-c4be84266076","year":2023},"citing_paper":{"arxiv_id":"2604.06053","last_updated":"2026-04-09T13:09:44Z","snapshot_observed_at":"2026-07-06T02:11:23.670680Z","submitted_at":"2026-04-07T16:41:35Z","title":"Probing Kerr Symmetry Breaking with LISA Extreme-Mass-Ratio Inspirals","version":2},"reference_index":157,"source":"pdf_text","source_observed_at":"2026-05-10T19:16:55.664160Z"},"links":{"cited_paper":"/paper/2209.04060","citing_paper":"/paper/2604.06053"},"observation_digest":"sha256:431adfb2e9a9a6d97ef60147c8221883308f58e2094654b8c4a0af2e2fc84292","observation_id":"5bae6afd-8f96-4f3f-a941-cab1d2eb3398","resolution":{"observed_at":"2026-05-10T23:10:55.192725Z","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":"2209.04060","last_updated":"2023-03-06T15:51:10Z","snapshot_observed_at":"2026-07-06T13:50:22.878139Z","submitted_at":"2022-09-08T23:27:37Z","title":"Priorities in gravitational waveforms for future space-borne detectors: vacuum accuracy or environment?","version":2},"cited_work":{"arxiv_id":"2209.04060","doi":null,"metadata_source":"arxiv_reference","pith_arxiv_id":"2209.04060","snapshot_observed_at":"2026-06-29T01:02:55.899180Z","title":"R., & Mayer, L","venue":null,"work_id":"3d132ec2-e5af-435c-99ea-c4be84266076","year":2023},"citing_paper":{"arxiv_id":"2606.27526","last_updated":"2026-06-25T20:19:24Z","snapshot_observed_at":"2026-08-01T01:50:16.703668Z","submitted_at":"2026-06-25T20:19:24Z","title":"Dynamics of Relativistic Binaries in Structured and Stochastic Environments: A Lagrange-Fourier-Hansen Framework","version":1},"reference_index":103,"source":"pdf_text","source_observed_at":"2026-06-29T00:58:22.089350Z"},"links":{"cited_paper":"/paper/2209.04060","citing_paper":"/paper/2606.27526"},"observation_digest":"sha256:d4d3a0d56bfeb95fce066ce6d7fd0d02a805eb2e2344cd3dd1748ea19ada45df","observation_id":"dd1c9424-c2c4-44b2-99a7-55fe3fb26418","resolution":{"observed_at":"2026-06-29T01:02:55.900696Z","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"}}],"links":{"evidence":"/evidence","html":"/paper/2209.04060/citation-record","integrity":"/paper/2209.04060/integrity","json":"/paper/2209.04060/citation-record.json","paper":"/paper/2209.04060"},"outbound":[],"paper":{"arxiv_id":"2209.04060","last_updated":"2023-03-06T15:51:10Z","latest_version":2,"primary_category":"gr-qc","snapshot_observed_at":"2026-07-06T13:50:22.878139Z","submitted_at":"2022-09-08T23:27:37Z","title":"Priorities in gravitational waveforms for future space-borne detectors: vacuum accuracy or environment?"},"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 6 inbound Pith citation observations for arXiv:2209.04060."}