{"as_of":"2026-08-05T08:33:00Z","caps":{"database_statements":6,"inbound":100,"outbound":100},"context_digest":"sha256:6e617fa22f3aaf07cc0babe876c28f48aeb3469a471abc41d583968ee65ff5ec","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":16,"lane":"standing_notices","note":"One-hop event checks from named stored sources.","records_observed":16,"source":"scholarly_work_events, retraction_status_cache","source_observed_at":"2026-08-05T06:32:48.257954+00:00","state":"measured"},{"denominator":16,"lane":"inbound_itemization","note":"Pith citing papers itemized under the disclosed page cap.","records_observed":16,"source":"paper_references, paper_reference_links","source_observed_at":"2026-08-04T13:34:57.618208Z","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":"2026-07-04T18:50:05.359321Z","state":"measured"}],"external_citation_measurements":[],"inbound":[{"citation":{"cited_paper":{"arxiv_id":"2302.11257","last_updated":"2023-11-09T05:08:48Z","snapshot_observed_at":"2026-07-06T14:54:29.901460Z","submitted_at":"2023-02-22T10:10:45Z","title":"Defining eccentricity for gravitational wave astronomy","version":3},"cited_work":{"arxiv_id":"2302.11257","doi":null,"metadata_source":"arxiv_reference","pith_arxiv_id":"2302.11257","snapshot_observed_at":"2026-07-04T18:50:05.359321Z","title":"Defining eccentricity for gravitational wave astronomy","venue":null,"work_id":"6d35a5e8-5ca5-4dbd-bf1e-838041195f5d","year":2023},"citing_paper":{"arxiv_id":"2404.14286","last_updated":"2026-05-05T08:23:34Z","snapshot_observed_at":"2026-07-06T02:11:23.670680Z","submitted_at":"2024-04-22T15:37:08Z","title":"Evidence for eccentricity in the population of binary black holes observed by LIGO-Virgo-KAGRA","version":3},"reference_index":132,"source":"pdf_text","source_observed_at":"2026-05-24T01:34:53.946159Z"},"links":{"cited_paper":"/paper/2302.11257","citing_paper":"/paper/2404.14286"},"observation_digest":"sha256:2fa2061f22b6a371c12f2360062a2da2cde45be5e615460f9afa23ff25509628","observation_id":"156facb0-882e-4078-bfb4-af80768a00a0","resolution":{"observed_at":"2026-05-24T01:35:55.736864Z","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":"2302.11257","last_updated":"2023-11-09T05:08:48Z","snapshot_observed_at":"2026-07-06T14:54:29.901460Z","submitted_at":"2023-02-22T10:10:45Z","title":"Defining eccentricity for gravitational wave astronomy","version":3},"cited_work":{"arxiv_id":"2302.11257","doi":null,"metadata_source":"arxiv_reference","pith_arxiv_id":"2302.11257","snapshot_observed_at":"2026-07-04T18:50:05.359321Z","title":"Defining eccentricity for gravitational wave astronomy","venue":null,"work_id":"6d35a5e8-5ca5-4dbd-bf1e-838041195f5d","year":2023},"citing_paper":{"arxiv_id":"2502.06952","last_updated":"2026-04-10T20:47:12Z","snapshot_observed_at":"2026-07-06T20:34:20.957561Z","submitted_at":"2025-02-10T19:00:04Z","title":"Non-adiabatic dynamics of eccentric black-hole binaries in post-Newtonian theory","version":3},"reference_index":11,"source":"pdf_text","source_observed_at":"2026-05-23T03:23:04.626466Z"},"links":{"cited_paper":"/paper/2302.11257","citing_paper":"/paper/2502.06952"},"observation_digest":"sha256:fe9402360d59eca0b621d209414de6eef71fe1861946c110da285807aa18521f","observation_id":"41c615a6-6567-4127-a32f-aa5b2ed903f4","resolution":{"observed_at":"2026-05-23T03:25:20.684009Z","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":"2302.11257","last_updated":"2023-11-09T05:08:48Z","snapshot_observed_at":"2026-07-06T14:54:29.901460Z","submitted_at":"2023-02-22T10:10:45Z","title":"Defining eccentricity for gravitational wave astronomy","version":3},"cited_work":{"arxiv_id":"2302.11257","doi":null,"metadata_source":"arxiv_reference","pith_arxiv_id":"2302.11257","snapshot_observed_at":"2026-07-04T18:50:05.359321Z","title":"Defining eccentricity for gravitational wave astronomy","venue":null,"work_id":"6d35a5e8-5ca5-4dbd-bf1e-838041195f5d","year":2023},"citing_paper":{"arxiv_id":"2507.22862","last_updated":"2026-05-01T13:55:06Z","snapshot_observed_at":"2026-07-06T22:05:17.795002Z","submitted_at":"2025-07-30T17:38:27Z","title":"Parameter Estimation with Targeted Eccentric Numerical-Relativity Simulations for GW200208_22 and GW190620","version":2},"reference_index":83,"source":"pdf_text","source_observed_at":"2026-05-19T02:51:11.710911Z"},"links":{"cited_paper":"/paper/2302.11257","citing_paper":"/paper/2507.22862"},"observation_digest":"sha256:7008d031ff320f0b38a9aeadb1414a410a93fb714285cd3b231a1de43a6c22e2","observation_id":"4ec1f72a-871c-40aa-9870-ca9bf163f3e1","resolution":{"observed_at":"2026-05-19T02:52:00.064690Z","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":"2302.11257","last_updated":"2023-11-09T05:08:48Z","snapshot_observed_at":"2026-07-06T14:54:29.901460Z","submitted_at":"2023-02-22T10:10:45Z","title":"Defining eccentricity for gravitational wave astronomy","version":3},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2302.11257","snapshot_observed_at":"2026-08-04T13:34:57.618208Z","title":null,"venue":null,"work_id":null,"year":2023},"citing_paper":{"arxiv_id":"2510.00116","last_updated":"2026-07-21T22:58:27Z","snapshot_observed_at":"2026-08-04T13:34:48.887952Z","submitted_at":"2025-09-30T18:00:25Z","title":"Chase Orbits, not Time: A Scalable Paradigm for Long-Duration Eccentric Gravitational-Wave Surrogates","version":3},"reference_index":119,"source":"pdf_text","source_observed_at":"2026-08-04T13:34:57.618208Z"},"links":{"cited_paper":"/paper/2302.11257","citing_paper":"/paper/2510.00116"},"observation_digest":"sha256:2ef535a5c2303ef9a5339efd255e40010766fdac38eee872e374ec1cf142ad08","observation_id":"329bb256-5a4a-4ace-ade3-debc751c7d5c","resolution":{"observed_at":"2026-08-04T13:34:57.618208Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2302.11257","last_updated":"2023-11-09T05:08:48Z","snapshot_observed_at":"2026-07-06T14:54:29.901460Z","submitted_at":"2023-02-22T10:10:45Z","title":"Defining eccentricity for gravitational wave astronomy","version":3},"cited_work":{"arxiv_id":"2302.11257","doi":null,"metadata_source":"arxiv_reference","pith_arxiv_id":"2302.11257","snapshot_observed_at":"2026-07-04T18:50:05.359321Z","title":"Defining eccentricity for gravitational wave astronomy","venue":null,"work_id":"6d35a5e8-5ca5-4dbd-bf1e-838041195f5d","year":2023},"citing_paper":{"arxiv_id":"2510.04332","last_updated":"2026-05-12T13:46:37Z","snapshot_observed_at":"2026-07-06T22:31:44.964774Z","submitted_at":"2025-10-05T19:29:41Z","title":"Biased parameter inference of eccentric, spin-precessing binary black holes","version":2},"reference_index":137,"source":"pdf_text","source_observed_at":"2026-05-18T09:50:50.035204Z"},"links":{"cited_paper":"/paper/2302.11257","citing_paper":"/paper/2510.04332"},"observation_digest":"sha256:448c015732da23ca93f6c94c5ee9321d1ea78f410fbac8eb9608f9e6eb4677cf","observation_id":"1c4ad6a3-0605-4d4d-a263-20c0003babe3","resolution":{"observed_at":"2026-05-18T09:51:13.232027Z","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":"2302.11257","last_updated":"2023-11-09T05:08:48Z","snapshot_observed_at":"2026-07-06T14:54:29.901460Z","submitted_at":"2023-02-22T10:10:45Z","title":"Defining eccentricity for gravitational wave astronomy","version":3},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2302.11257","snapshot_observed_at":"2026-08-03T18:57:08.508390Z","title":null,"venue":null,"work_id":null,"year":2023},"citing_paper":{"arxiv_id":"2512.02943","last_updated":"2025-12-02T17:11:26Z","snapshot_observed_at":"2026-08-05T08:12:39.544541Z","submitted_at":"2025-12-02T17:11:26Z","title":"Can Eccentric Binary Black Hole Signals Mimic Gravitational-Wave Microlensing?","version":1},"reference_index":98,"source":"pdf_text","source_observed_at":"2026-08-03T18:57:08.508390Z"},"links":{"cited_paper":"/paper/2302.11257","citing_paper":"/paper/2512.02943"},"observation_digest":"sha256:839c13131eec4d34883eeb2caf40d3f42d625ae02bc96a18356b8466072d5726","observation_id":"c5973580-3e72-4233-99b4-06fe9ff3b6fd","resolution":{"observed_at":"2026-08-03T18:57:08.508390Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2302.11257","last_updated":"2023-11-09T05:08:48Z","snapshot_observed_at":"2026-07-06T14:54:29.901460Z","submitted_at":"2023-02-22T10:10:45Z","title":"Defining eccentricity for gravitational wave astronomy","version":3},"cited_work":{"arxiv_id":"2302.11257","doi":null,"metadata_source":"arxiv_reference","pith_arxiv_id":"2302.11257","snapshot_observed_at":"2026-07-04T18:50:05.359321Z","title":"Defining eccentricity for gravitational wave astronomy","venue":null,"work_id":"6d35a5e8-5ca5-4dbd-bf1e-838041195f5d","year":2023},"citing_paper":{"arxiv_id":"2604.11903","last_updated":"2026-04-13T18:00:35Z","snapshot_observed_at":"2026-08-04T03:18:15.061469Z","submitted_at":"2026-04-13T18:00:35Z","title":"Post-Newtonian inspiral waveform model for eccentric precessing binaries with higher-order modes and matter effects","version":1},"reference_index":133,"source":"pdf_text","source_observed_at":"2026-05-10T15:00:29.655032Z"},"links":{"cited_paper":"/paper/2302.11257","citing_paper":"/paper/2604.11903"},"observation_digest":"sha256:7bf0c18d1178105f4765e465add963dc76c631f286133545de59393870d4a80a","observation_id":"24bf5e81-82b1-4f70-95bf-c70f3eee7fe4","resolution":{"observed_at":"2026-05-10T15:00:31.310132Z","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":"2302.11257","last_updated":"2023-11-09T05:08:48Z","snapshot_observed_at":"2026-07-06T14:54:29.901460Z","submitted_at":"2023-02-22T10:10:45Z","title":"Defining eccentricity for gravitational wave astronomy","version":3},"cited_work":{"arxiv_id":"2302.11257","doi":null,"metadata_source":"arxiv_reference","pith_arxiv_id":"2302.11257","snapshot_observed_at":"2026-07-04T18:50:05.359321Z","title":"Defining eccentricity for gravitational wave astronomy","venue":null,"work_id":"6d35a5e8-5ca5-4dbd-bf1e-838041195f5d","year":2023},"citing_paper":{"arxiv_id":"2604.15431","last_updated":"2026-04-16T18:00:02Z","snapshot_observed_at":"2026-08-02T05:54:54.327009Z","submitted_at":"2026-04-16T18:00:02Z","title":"Highly eccentric non-spinning binary black hole mergers: quadrupolar post-merger waveforms","version":1},"reference_index":153,"source":"pdf_text","source_observed_at":"2026-05-10T10:16:15.923894Z"},"links":{"cited_paper":"/paper/2302.11257","citing_paper":"/paper/2604.15431"},"observation_digest":"sha256:389df2c9bb89eb55109dab0666e385b65ff5ecf6f3749ecbf8834fb83aaf3086","observation_id":"15de655b-4359-437b-81e6-3107b4a0d5f9","resolution":{"observed_at":"2026-05-10T10:19:21.242685Z","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":"2302.11257","last_updated":"2023-11-09T05:08:48Z","snapshot_observed_at":"2026-07-06T14:54:29.901460Z","submitted_at":"2023-02-22T10:10:45Z","title":"Defining eccentricity for gravitational wave astronomy","version":3},"cited_work":{"arxiv_id":"2302.11257","doi":null,"metadata_source":"arxiv_reference","pith_arxiv_id":"2302.11257","snapshot_observed_at":"2026-07-04T18:50:05.359321Z","title":"Defining eccentricity for gravitational wave astronomy","venue":null,"work_id":"6d35a5e8-5ca5-4dbd-bf1e-838041195f5d","year":2023},"citing_paper":{"arxiv_id":"2604.17868","last_updated":"2026-04-20T06:28:06Z","snapshot_observed_at":"2026-07-06T23:04:50.935335Z","submitted_at":"2026-04-20T06:28:06Z","title":"Including higher-order modes in a quadrupolar eccentric numerical relativity surrogate using universal eccentric modulation functions","version":1},"reference_index":93,"source":"pdf_text","source_observed_at":"2026-05-10T04:38:37.066802Z"},"links":{"cited_paper":"/paper/2302.11257","citing_paper":"/paper/2604.17868"},"observation_digest":"sha256:7f8b77ed11469b7892d120f272c0f6633627116ad8924d794a1e7a9e4985b1c9","observation_id":"fcec5b64-41a6-4369-b702-e7f3b5c65f2a","resolution":{"observed_at":"2026-05-10T12:10:22.443185Z","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":"2302.11257","last_updated":"2023-11-09T05:08:48Z","snapshot_observed_at":"2026-07-06T14:54:29.901460Z","submitted_at":"2023-02-22T10:10:45Z","title":"Defining eccentricity for gravitational wave astronomy","version":3},"cited_work":{"arxiv_id":"2302.11257","doi":null,"metadata_source":"arxiv_reference","pith_arxiv_id":"2302.11257","snapshot_observed_at":"2026-07-04T18:50:05.359321Z","title":"Defining eccentricity for gravitational wave astronomy","venue":null,"work_id":"6d35a5e8-5ca5-4dbd-bf1e-838041195f5d","year":2023},"citing_paper":{"arxiv_id":"2605.00124","last_updated":"2026-05-20T21:35:50Z","snapshot_observed_at":"2026-07-06T23:13:38.354733Z","submitted_at":"2026-04-30T18:25:52Z","title":"Merger remnant and eccentricity dynamics surrogates for eccentric nonspinning black hole binaries","version":1},"reference_index":36,"source":"pdf_text","source_observed_at":"2026-05-09T20:41:09.388195Z"},"links":{"cited_paper":"/paper/2302.11257","citing_paper":"/paper/2605.00124"},"observation_digest":"sha256:4e90315d8a38cfbd0ca47aab7e5e2cadfd89a65ce80fbf93bd9a1f0f99af2853","observation_id":"41efa1ab-378f-4707-b63d-21fa9788eff0","resolution":{"observed_at":"2026-05-11T15:01:09.111469Z","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":"2302.11257","last_updated":"2023-11-09T05:08:48Z","snapshot_observed_at":"2026-07-06T14:54:29.901460Z","submitted_at":"2023-02-22T10:10:45Z","title":"Defining eccentricity for gravitational wave astronomy","version":3},"cited_work":{"arxiv_id":"2302.11257","doi":null,"metadata_source":"arxiv_reference","pith_arxiv_id":"2302.11257","snapshot_observed_at":"2026-07-04T18:50:05.359321Z","title":"Defining eccentricity for gravitational wave astronomy","venue":null,"work_id":"6d35a5e8-5ca5-4dbd-bf1e-838041195f5d","year":2023},"citing_paper":{"arxiv_id":"2605.00124","last_updated":"2026-05-20T21:35:50Z","snapshot_observed_at":"2026-07-06T23:13:38.354733Z","submitted_at":"2026-04-30T18:25:52Z","title":"Merger remnant and eccentricity dynamics surrogates for eccentric nonspinning black hole binaries","version":2},"reference_index":36,"source":"pdf_text","source_observed_at":"2026-05-22T10:37:23.693585Z"},"links":{"cited_paper":"/paper/2302.11257","citing_paper":"/paper/2605.00124"},"observation_digest":"sha256:081f54167934932a81ba94b5c147e24dc7642433060dc3093f83b61fbfb16076","observation_id":"61601b2a-3eb4-4036-b3ba-ddc9440e78dd","resolution":{"observed_at":"2026-05-22T10:41:25.628269Z","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":"2302.11257","last_updated":"2023-11-09T05:08:48Z","snapshot_observed_at":"2026-07-06T14:54:29.901460Z","submitted_at":"2023-02-22T10:10:45Z","title":"Defining eccentricity for gravitational wave astronomy","version":3},"cited_work":{"arxiv_id":"2302.11257","doi":null,"metadata_source":"arxiv_reference","pith_arxiv_id":"2302.11257","snapshot_observed_at":"2026-07-04T18:50:05.359321Z","title":"Defining eccentricity for gravitational wave astronomy","venue":null,"work_id":"6d35a5e8-5ca5-4dbd-bf1e-838041195f5d","year":2023},"citing_paper":{"arxiv_id":"2605.05537","last_updated":"2026-05-07T00:35:22Z","snapshot_observed_at":"2026-07-06T23:18:07.750358Z","submitted_at":"2026-05-07T00:35:22Z","title":"Implications of the LISA stochastic signal from eccentric stellar mass black hole binaries in vacuum","version":1},"reference_index":66,"source":"pdf_text","source_observed_at":"2026-05-08T07:48:04.948543Z"},"links":{"cited_paper":"/paper/2302.11257","citing_paper":"/paper/2605.05537"},"observation_digest":"sha256:c80fbe2a4c7d20901f56933a21643562f4332e45dd36f4e78d5cd8452aa7dfe3","observation_id":"0acac5d3-fb2e-45ca-8cf6-81e43c608633","resolution":{"observed_at":"2026-05-11T20:51:12.945677Z","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":"2302.11257","last_updated":"2023-11-09T05:08:48Z","snapshot_observed_at":"2026-07-06T14:54:29.901460Z","submitted_at":"2023-02-22T10:10:45Z","title":"Defining eccentricity for gravitational wave astronomy","version":3},"cited_work":{"arxiv_id":"2302.11257","doi":null,"metadata_source":"arxiv_reference","pith_arxiv_id":"2302.11257","snapshot_observed_at":"2026-07-04T18:50:05.359321Z","title":"Defining eccentricity for gravitational wave astronomy","venue":null,"work_id":"6d35a5e8-5ca5-4dbd-bf1e-838041195f5d","year":2023},"citing_paper":{"arxiv_id":"2605.12818","last_updated":"2026-05-12T23:23:08Z","snapshot_observed_at":"2026-07-06T23:24:27.821980Z","submitted_at":"2026-05-12T23:23:08Z","title":"Assessing the imprint of eccentricity in GW signatures using two independent waveform models","version":1},"reference_index":71,"source":"pdf_text","source_observed_at":"2026-05-14T19:19:56.792712Z"},"links":{"cited_paper":"/paper/2302.11257","citing_paper":"/paper/2605.12818"},"observation_digest":"sha256:1f149f3775ea690e0e2ab9383c49a8f7586dda968f8a840c93ff4b69c685ede5","observation_id":"1064b5a9-da9a-49ee-a56a-5e8769f51cda","resolution":{"observed_at":"2026-05-14T19:22:50.879364Z","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":"2302.11257","last_updated":"2023-11-09T05:08:48Z","snapshot_observed_at":"2026-07-06T14:54:29.901460Z","submitted_at":"2023-02-22T10:10:45Z","title":"Defining eccentricity for gravitational wave astronomy","version":3},"cited_work":{"arxiv_id":"2302.11257","doi":null,"metadata_source":"arxiv_reference","pith_arxiv_id":"2302.11257","snapshot_observed_at":"2026-07-04T18:50:05.359321Z","title":"Defining eccentricity for gravitational wave astronomy","venue":null,"work_id":"6d35a5e8-5ca5-4dbd-bf1e-838041195f5d","year":2023},"citing_paper":{"arxiv_id":"2605.18742","last_updated":"2026-05-18T17:58:22Z","snapshot_observed_at":"2026-07-06T23:29:33.702647Z","submitted_at":"2026-05-18T17:58:22Z","title":"A universal framework to identify eccentric binary mergers: GW200105 case study","version":1},"reference_index":72,"source":"pdf_text","source_observed_at":"2026-05-20T08:51:43.355150Z"},"links":{"cited_paper":"/paper/2302.11257","citing_paper":"/paper/2605.18742"},"observation_digest":"sha256:ae550361663728fcfd1c7503f02873db2b74395629f625117f7ba5878798e278","observation_id":"44b4b37e-baed-410e-996a-8020ce4d55fe","resolution":{"observed_at":"2026-05-20T08:53:09.887559Z","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":"2302.11257","last_updated":"2023-11-09T05:08:48Z","snapshot_observed_at":"2026-07-06T14:54:29.901460Z","submitted_at":"2023-02-22T10:10:45Z","title":"Defining eccentricity for gravitational wave astronomy","version":3},"cited_work":{"arxiv_id":"2302.11257","doi":null,"metadata_source":"arxiv_reference","pith_arxiv_id":"2302.11257","snapshot_observed_at":"2026-07-04T18:50:05.359321Z","title":"Defining eccentricity for gravitational wave astronomy","venue":null,"work_id":"6d35a5e8-5ca5-4dbd-bf1e-838041195f5d","year":2023},"citing_paper":{"arxiv_id":"2605.28716","last_updated":"2026-05-27T16:38:48Z","snapshot_observed_at":"2026-08-02T19:42:11.441558Z","submitted_at":"2026-05-27T16:38:48Z","title":"Eccentric and unbound compact binaries in the LIGO-Virgo-KAGRA catalog: parameter estimation and waveform systematics with SEOBNRv6EHM","version":1},"reference_index":121,"source":"pdf_text","source_observed_at":"2026-06-29T10:35:54.691849Z"},"links":{"cited_paper":"/paper/2302.11257","citing_paper":"/paper/2605.28716"},"observation_digest":"sha256:b719d5f36e968f97a529c024e99665086c5b15aba70dc384d6923a072c8700db","observation_id":"474e2dab-ba0a-4a4f-9e7b-b1744f394adc","resolution":{"observed_at":"2026-06-29T13:13:28.220485Z","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":"2302.11257","last_updated":"2023-11-09T05:08:48Z","snapshot_observed_at":"2026-07-06T14:54:29.901460Z","submitted_at":"2023-02-22T10:10:45Z","title":"Defining eccentricity for gravitational wave astronomy","version":3},"cited_work":{"arxiv_id":"2302.11257","doi":null,"metadata_source":"arxiv_reference","pith_arxiv_id":"2302.11257","snapshot_observed_at":"2026-07-04T18:50:05.359321Z","title":"Defining eccentricity for gravitational wave astronomy","venue":null,"work_id":"6d35a5e8-5ca5-4dbd-bf1e-838041195f5d","year":2023},"citing_paper":{"arxiv_id":"2606.24816","last_updated":"2026-06-23T17:02:02Z","snapshot_observed_at":"2026-08-02T22:27:04.722600Z","submitted_at":"2026-06-23T17:02:02Z","title":"The Bondi--Sachs gauge, BMS frames, and memory in black hole perturbation theory","version":1},"reference_index":11,"source":"pdf_text","source_observed_at":"2026-06-25T22:19:51.278679Z"},"links":{"cited_paper":"/paper/2302.11257","citing_paper":"/paper/2606.24816"},"observation_digest":"sha256:350c147c8dbb8fc60c0dcfccc91351e1a9e70e3e611a925df22d8244f5e50a74","observation_id":"f17e964e-01b3-4288-aec2-56af6232d512","resolution":{"observed_at":"2026-07-04T18:50:05.360674Z","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/2302.11257/citation-record","integrity":"/paper/2302.11257/integrity","json":"/paper/2302.11257/citation-record.json","paper":"/paper/2302.11257"},"outbound":[],"paper":{"arxiv_id":"2302.11257","last_updated":"2023-11-09T05:08:48Z","latest_version":3,"primary_category":"gr-qc","snapshot_observed_at":"2026-07-06T14:54:29.901460Z","submitted_at":"2023-02-22T10:10:45Z","title":"Defining eccentricity for gravitational wave astronomy"},"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 16 inbound Pith citation observations for arXiv:2302.11257."}