{"as_of":"2026-08-04T06:47:00Z","caps":{"database_statements":6,"inbound":100,"outbound":100},"context_digest":"sha256:6c8f728fed7ebebc8776958705da97329d620e3fdb9327d255531ad4c83c6c50","coverage":[{"denominator":74,"lane":"reference_resolution","note":"Typed states for the displayed outbound observations.","records_observed":74,"source":"paper_references, paper_reference_links","source_observed_at":"2026-07-11T11:50:26.030339Z","state":"measured"},{"denominator":76,"lane":"standing_notices","note":"One-hop event checks from named stored sources.","records_observed":76,"source":"scholarly_work_events, retraction_status_cache","source_observed_at":"2026-08-04T06:34:03.388597+00:00","state":"measured"},{"denominator":2,"lane":"inbound_itemization","note":"Pith citing papers itemized under the disclosed page cap.","records_observed":2,"source":"paper_references, paper_reference_links","source_observed_at":"2026-08-02T22:32:35.151035Z","state":"measured"},{"denominator":1,"lane":"external_citation_measurements","note":"A source-named dated measurement, never combined with another source.","records_observed":0,"source":"cited_works","source_observed_at":null,"state":"measured"}],"external_citation_measurements":[],"inbound":[{"citation":{"cited_paper":{"arxiv_id":"2510.04703","last_updated":"2026-04-06T04:55:34Z","snapshot_observed_at":"2026-07-06T22:31:49.574184Z","submitted_at":"2025-10-06T11:16:49Z","title":"Testing black hole metrics with binary black hole inspirals","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2510.04703","snapshot_observed_at":"2026-08-02T22:32:35.151035Z","title":null,"venue":null,"work_id":null,"year":2025},"citing_paper":{"arxiv_id":"2602.16562","last_updated":"2026-06-03T18:19:23Z","snapshot_observed_at":"2026-08-02T22:32:30.780856Z","submitted_at":"2026-02-18T16:03:08Z","title":"Testing non-circular black hole spacetime with X-ray reflection","version":2},"reference_index":40,"source":"pdf_text","source_observed_at":"2026-08-02T22:32:35.151035Z"},"links":{"cited_paper":"/paper/2510.04703","citing_paper":"/paper/2602.16562"},"observation_digest":"sha256:d3b88883cb598ea4714a25b020b7ee325953257181a4d63ddc564bd71d269352","observation_id":"034ea00f-cffc-4661-a134-bab50b0b18ed","resolution":{"observed_at":"2026-08-02T22:32:35.151035Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2510.04703","last_updated":"2026-04-06T04:55:34Z","snapshot_observed_at":"2026-07-06T22:31:49.574184Z","submitted_at":"2025-10-06T11:16:49Z","title":"Testing black hole metrics with binary black hole inspirals","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2510.04703","snapshot_observed_at":"2026-07-11T20:43:45.414683Z","title":null,"venue":null,"work_id":null,"year":2025},"citing_paper":{"arxiv_id":"2607.04238","last_updated":"2026-07-05T11:29:11Z","snapshot_observed_at":"2026-08-02T10:24:46.301044Z","submitted_at":"2026-07-05T11:29:11Z","title":"Tests of general relativity using analytic derivatives of parametrized post-Einsteinian gravitational waveforms within the Fisher-matrix framework","version":1},"reference_index":65,"source":"pdf_text","source_observed_at":"2026-07-11T20:43:45.414683Z"},"links":{"cited_paper":"/paper/2510.04703","citing_paper":"/paper/2607.04238"},"observation_digest":"sha256:9750ae45ba4429b27cce8125fa430aac91f3582844507ba050676dce68d8dd8b","observation_id":"a3ad9596-949a-427e-ac7b-933247f66e27","resolution":{"observed_at":"2026-07-11T20:43:45.414683Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}}],"links":{"evidence":"/evidence","html":"/paper/2510.04703/citation-record","integrity":"/paper/2510.04703/integrity","json":"/paper/2510.04703/citation-record.json","paper":"/paper/2510.04703"},"outbound":[{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":"chicago/9780226","doi":"10.7208/chicago/9780226039206.001.0001","metadata_source":"arxiv_reference","pith_arxiv_id":null,"snapshot_observed_at":"2026-07-11T11:50:26.030339Z","title":"General Relativity","venue":null,"work_id":"36a84b1a-56ac-42a9-b70b-23335de647d5","year":1984},"citing_paper":{"arxiv_id":"2510.04703","last_updated":"2026-04-06T04:55:34Z","snapshot_observed_at":"2026-07-06T22:31:49.574184Z","submitted_at":"2025-10-06T11:16:49Z","title":"Testing black hole metrics with binary black hole inspirals","version":2},"reference_index":1,"source":"pdf_text","source_observed_at":"2026-05-18T09:47:38.064359Z"},"links":{"citing_paper":"/paper/2510.04703"},"observation_digest":"sha256:5c1684c11828660acf015dc4466546e47d02958cc63d4e0f8aae7d754f520b79","observation_id":"39126e21-43fc-4f89-b987-ad0967cc29c2","resolution":{"observed_at":"2026-05-18T09:51:12.688901Z","resolver_source":"arxiv_id","status":"metadata_mismatch"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-04T06:34:03.388597+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-04T06:34:03.388597+00:00","source":"crossref"},{"observed_at":"2026-08-04T06:33:57.428241+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":"10.1007/978-981-99-0022-0","metadata_source":"doi_reference","pith_arxiv_id":null,"snapshot_observed_at":"2026-06-05T21:23:00.469572Z","title":"Liang, B","venue":null,"work_id":"ad1c1a96-16d1-4688-9a75-3180d6aeae57","year":2023},"citing_paper":{"arxiv_id":"2510.04703","last_updated":"2026-04-06T04:55:34Z","snapshot_observed_at":"2026-07-06T22:31:49.574184Z","submitted_at":"2025-10-06T11:16:49Z","title":"Testing black hole metrics with binary black hole inspirals","version":2},"reference_index":2,"source":"pdf_text","source_observed_at":"2026-05-18T09:47:38.064359Z"},"links":{"citing_paper":"/paper/2510.04703"},"observation_digest":"sha256:edc0ec46192fc7b30a421cbcf75ab5d72c5df025878b17a0c465814624fcbe87","observation_id":"f5c3f144-df0c-41a5-8da1-1dd5ad5dcb22","resolution":{"observed_at":"2026-05-18T09:51:12.540764Z","resolver_source":"doi","status":"verified_exact"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-04T06:34:03.388597+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-04T06:34:03.388597+00:00","source":"crossref"},{"observed_at":"2026-08-04T06:33:57.428241+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":{"arxiv_id":"1602.03837","last_updated":"2016-02-11T19:26:44Z","snapshot_observed_at":"2026-07-09T16:56:15.649302Z","submitted_at":"2016-02-11T19:26:44Z","title":"Observation of Gravitational Waves from a Binary Black Hole Merger","version":1},"cited_work":{"arxiv_id":"1602.03837","doi":null,"metadata_source":"pith","pith_arxiv_id":"1602.03837","snapshot_observed_at":"2026-07-11T00:07:39.821374Z","title":"Observation of Gravitational Waves from a Binary Black Hole Merger","venue":"gr-qc","work_id":"ab878228-151c-4a29-8026-a4308b076d30","year":2016},"citing_paper":{"arxiv_id":"2510.04703","last_updated":"2026-04-06T04:55:34Z","snapshot_observed_at":"2026-07-06T22:31:49.574184Z","submitted_at":"2025-10-06T11:16:49Z","title":"Testing black hole metrics with binary black hole inspirals","version":2},"reference_index":3,"source":"pdf_text","source_observed_at":"2026-07-11T11:50:26.030339Z"},"links":{"cited_paper":"/paper/1602.03837","citing_paper":"/paper/2510.04703"},"observation_digest":"sha256:d49d7bc4d93be0ade009732a8da1f22679aed32fdc0ae59edac6ad3042282bf6","observation_id":"082ef2b2-9541-4706-8d23-362d07b39578","resolution":{"observed_at":"2026-05-18T09:51:12.643196Z","resolver_source":"local_arxiv","status":"verified_exact"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-04T06:34:03.388597+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-04T06:34:03.388597+00:00","source":"crossref"},{"observed_at":"2026-08-04T06:33:57.428241+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":{"arxiv_id":"1710.05832","last_updated":"2017-10-16T16:57:17Z","snapshot_observed_at":"2026-07-09T17:52:08.260915Z","submitted_at":"2017-10-16T16:57:17Z","title":"GW170817: Observation of Gravitational Waves from a Binary Neutron Star Inspiral","version":1},"cited_work":{"arxiv_id":"1710.05832","doi":"10.1103/physrevlett.119.161106","metadata_source":"pith","pith_arxiv_id":"1710.05832","snapshot_observed_at":"2026-07-11T11:50:26.030339Z","title":"GW170817: Observation of Gravitational Waves from a Binary Neutron Star Inspiral","venue":"gr-qc","work_id":"a19136e8-99c2-49be-b029-60af2e20c6ee","year":2017},"citing_paper":{"arxiv_id":"2510.04703","last_updated":"2026-04-06T04:55:34Z","snapshot_observed_at":"2026-07-06T22:31:49.574184Z","submitted_at":"2025-10-06T11:16:49Z","title":"Testing black hole metrics with binary black hole inspirals","version":2},"reference_index":4,"source":"pdf_text","source_observed_at":"2026-07-11T11:50:26.030339Z"},"links":{"cited_paper":"/paper/1710.05832","citing_paper":"/paper/2510.04703"},"observation_digest":"sha256:5cb6327100cb77f250a2fb5baa0af896480cca3a32fe7eea4be8c8ee83da6847","observation_id":"7e1455c5-30d7-4033-80fa-9dd0fd9dfc32","resolution":{"observed_at":"2026-05-18T09:51:12.584287Z","resolver_source":"local_arxiv","status":"metadata_mismatch"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-04T06:34:03.388597+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-04T06:34:03.388597+00:00","source":"crossref"},{"observed_at":"2026-08-04T06:33:57.428241+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":"oso/9780198","doi":"10.1093/acprof:oso/9780198237907.003.0008","metadata_source":"arxiv_reference","pith_arxiv_id":null,"snapshot_observed_at":"2026-07-11T11:50:26.030339Z","title":"Oxford Univer- sity Press (2018).https://doi.org/10.1093/oso/9780198814788.001.0001","venue":null,"work_id":"a1b77a81-dfdc-490e-805b-591b44077c3d","year":2016},"citing_paper":{"arxiv_id":"2510.04703","last_updated":"2026-04-06T04:55:34Z","snapshot_observed_at":"2026-07-06T22:31:49.574184Z","submitted_at":"2025-10-06T11:16:49Z","title":"Testing black hole metrics with binary black hole inspirals","version":2},"reference_index":5,"source":"pdf_text","source_observed_at":"2026-05-18T09:47:38.064359Z"},"links":{"citing_paper":"/paper/2510.04703"},"observation_digest":"sha256:30d4b3e7ab372b4efb857d27dcd202769c70cb6d5144c1643c2e5e23e95c3766","observation_id":"1a4db495-79d0-4518-a555-0213735f3cab","resolution":{"observed_at":"2026-05-18T09:51:12.525172Z","resolver_source":"arxiv_id","status":"metadata_mismatch"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-04T06:34:03.388597+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-04T06:34:03.388597+00:00","source":"crossref"},{"observed_at":"2026-08-04T06:33:57.428241+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":"10.1103/physrevd.105.124047","metadata_source":"doi_reference","pith_arxiv_id":null,"snapshot_observed_at":"2026-06-05T21:23:00.469572Z","title":"Perkins and N","venue":null,"work_id":"e2e695f2-3cac-4917-afce-3701032f9a4a","year":2022},"citing_paper":{"arxiv_id":"2510.04703","last_updated":"2026-04-06T04:55:34Z","snapshot_observed_at":"2026-07-06T22:31:49.574184Z","submitted_at":"2025-10-06T11:16:49Z","title":"Testing black hole metrics with binary black hole inspirals","version":2},"reference_index":6,"source":"pdf_text","source_observed_at":"2026-05-18T09:47:38.064359Z"},"links":{"citing_paper":"/paper/2510.04703"},"observation_digest":"sha256:3917da2dfe117c16727215972d0b48ac246989898fa7ca930e551dff541ac1df","observation_id":"a274df4f-bf4b-475e-bfb6-559d43251684","resolution":{"observed_at":"2026-05-18T09:51:12.751298Z","resolver_source":"doi","status":"verified_exact"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-04T06:34:03.388597+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-04T06:34:03.388597+00:00","source":"crossref"},{"observed_at":"2026-08-04T06:33:57.428241+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":{"arxiv_id":"0802.4047","last_updated":"2008-02-27T17:04:27Z","snapshot_observed_at":"2026-07-06T01:35:38.620403Z","submitted_at":"2008-02-27T17:04:27Z","title":"Introductory lectures on the Effective One Body formalism","version":1},"cited_work":{"arxiv_id":"0802.4047","doi":"10.1142/s0217751x08039992","metadata_source":"pith","pith_arxiv_id":"0802.4047","snapshot_observed_at":"2026-07-11T11:50:26.030339Z","title":"Introductory lectures on the Effective One Body formalism","venue":"gr-qc","work_id":"7e2a9578-412b-4594-b974-a15a92b9ebb5","year":2008},"citing_paper":{"arxiv_id":"2510.04703","last_updated":"2026-04-06T04:55:34Z","snapshot_observed_at":"2026-07-06T22:31:49.574184Z","submitted_at":"2025-10-06T11:16:49Z","title":"Testing black hole metrics with binary black hole inspirals","version":2},"reference_index":7,"source":"pdf_text","source_observed_at":"2026-07-11T11:50:26.030339Z"},"links":{"cited_paper":"/paper/0802.4047","citing_paper":"/paper/2510.04703"},"observation_digest":"sha256:408218942e801ba0f8b2098d2def28c7d81c1a30c61c137f1a84d64845b873ec","observation_id":"64764e50-5dde-4b48-b2b0-4f370fe0391f","resolution":{"observed_at":"2026-05-18T09:51:12.756054Z","resolver_source":"local_arxiv","status":"verified_exact"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-04T06:34:03.388597+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-04T06:34:03.388597+00:00","source":"crossref"},{"observed_at":"2026-08-04T06:33:57.428241+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":{"arxiv_id":"1310.1528","last_updated":"2024-07-12T19:24:23Z","snapshot_observed_at":"2026-07-06T03:24:52.562608Z","submitted_at":"2013-10-06T02:23:37Z","title":"Post-Newtonian Theory for Gravitational Waves","version":6},"cited_work":{"arxiv_id":"1310.1528","doi":null,"metadata_source":"pith","pith_arxiv_id":"1310.1528","snapshot_observed_at":"2026-07-04T19:40:06.527864Z","title":"Post-Newtonian Theory for Gravitational Waves","venue":"gr-qc","work_id":"6cb2442c-e284-4ded-a540-4da7a2454980","year":2013},"citing_paper":{"arxiv_id":"2510.04703","last_updated":"2026-04-06T04:55:34Z","snapshot_observed_at":"2026-07-06T22:31:49.574184Z","submitted_at":"2025-10-06T11:16:49Z","title":"Testing black hole metrics with binary black hole inspirals","version":2},"reference_index":8,"source":"pdf_text","source_observed_at":"2026-07-11T11:50:26.030339Z"},"links":{"cited_paper":"/paper/1310.1528","citing_paper":"/paper/2510.04703"},"observation_digest":"sha256:41e14ac82308086daad1bccacc65ce3bfe079997737d8e63e9a173d8a0cc9b73","observation_id":"8f0bc754-f902-4ba1-ba8f-09de1ca5ea29","resolution":{"observed_at":"2026-05-18T09:51:12.407545Z","resolver_source":"local_arxiv","status":"metadata_mismatch"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-04T06:34:03.388597+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-04T06:34:03.388597+00:00","source":"crossref"},{"observed_at":"2026-08-04T06:33:57.428241+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":{"arxiv_id":"gr-qc/9811091","last_updated":"1998-11-26T20:44:21Z","snapshot_observed_at":"2026-07-07T03:29:43.892120Z","submitted_at":"1998-11-26T20:44:21Z","title":"Effective one-body approach to general relativistic two-body dynamics","version":1},"cited_work":{"arxiv_id":"gr-qc/9811091","doi":null,"metadata_source":"pith","pith_arxiv_id":"gr-qc/9811091","snapshot_observed_at":"2026-07-10T15:07:19.604012Z","title":"Effective one-body approach to general relativistic two-body dynamics","venue":"gr-qc","work_id":"4a250095-9d3f-4aab-8936-948711e6dc74","year":1998},"citing_paper":{"arxiv_id":"2510.04703","last_updated":"2026-04-06T04:55:34Z","snapshot_observed_at":"2026-07-06T22:31:49.574184Z","submitted_at":"2025-10-06T11:16:49Z","title":"Testing black hole metrics with binary black hole inspirals","version":2},"reference_index":9,"source":"pdf_text","source_observed_at":"2026-07-11T11:50:26.030339Z"},"links":{"cited_paper":"/paper/gr-qc/9811091","citing_paper":"/paper/2510.04703"},"observation_digest":"sha256:035d92f29e3aebeaf79d930e0f35ddaf164c4ff79bc87e214040e2291bb8734b","observation_id":"97ed46a0-5c95-45d0-83b0-5120d06861c8","resolution":{"observed_at":"2026-05-18T09:51:12.546111Z","resolver_source":"local_arxiv","status":"verified_exact"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-04T06:34:03.388597+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-04T06:34:03.388597+00:00","source":"crossref"},{"observed_at":"2026-08-04T06:33:57.428241+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":"10.1103/physrevd.64.124013","metadata_source":"doi_reference","pith_arxiv_id":null,"snapshot_observed_at":"2026-06-29T16:03:33.424973Z","title":"Damour, Phys","venue":null,"work_id":"b91788cc-13fa-43e6-968c-02af1ede6cfc","year":2001},"citing_paper":{"arxiv_id":"2510.04703","last_updated":"2026-04-06T04:55:34Z","snapshot_observed_at":"2026-07-06T22:31:49.574184Z","submitted_at":"2025-10-06T11:16:49Z","title":"Testing black hole metrics with binary black hole inspirals","version":2},"reference_index":10,"source":"pdf_text","source_observed_at":"2026-05-18T09:47:38.064359Z"},"links":{"citing_paper":"/paper/2510.04703"},"observation_digest":"sha256:da2da3efed602a363dae16732f7715cfb01ff84318322e6a9b26d6142e03552a","observation_id":"9c63f6c3-4d49-4893-bcb3-3cb1c7d81ffa","resolution":{"observed_at":"2026-05-18T09:51:12.647606Z","resolver_source":"doi","status":"verified_exact"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-04T06:34:03.388597+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-04T06:34:03.388597+00:00","source":"crossref"},{"observed_at":"2026-08-03T19:38:13.372414+00:00","source":"crossref_status_cache"},{"observed_at":"2026-08-03T19:38:13.372414+00:00","source":"openalex_status_cache"},{"observed_at":"2026-08-04T06:33:57.428241+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":"10.1103/physrevd.111.044026","metadata_source":"doi_reference","pith_arxiv_id":null,"snapshot_observed_at":"2026-06-05T21:23:00.469572Z","title":null,"venue":null,"work_id":"89adcddc-cb10-4720-ace5-eae6114b2166","year":2025},"citing_paper":{"arxiv_id":"2510.04703","last_updated":"2026-04-06T04:55:34Z","snapshot_observed_at":"2026-07-06T22:31:49.574184Z","submitted_at":"2025-10-06T11:16:49Z","title":"Testing black hole metrics with binary black hole inspirals","version":2},"reference_index":11,"source":"pdf_text","source_observed_at":"2026-05-18T09:47:38.064359Z"},"links":{"citing_paper":"/paper/2510.04703"},"observation_digest":"sha256:011edd02b8e60e965d8b0f7ee38fcc528d6caf757f081e1ed8019d1e4aaf30a9","observation_id":"d5417a5d-3fb2-4ac4-9003-88e0b56694af","resolution":{"observed_at":"2026-05-18T09:51:12.447817Z","resolver_source":"doi","status":"verified_exact"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-04T06:34:03.388597+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-04T06:34:03.388597+00:00","source":"crossref"},{"observed_at":"2026-08-04T06:33:57.428241+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":{"arxiv_id":"0909.3328","last_updated":"2009-12-07T17:14:47Z","snapshot_observed_at":"2026-07-06T01:57:40.790524Z","submitted_at":"2009-09-17T22:16:20Z","title":"Fundamental Theoretical Bias in Gravitational Wave Astrophysics and the Parameterized Post-Einsteinian Framework","version":2},"cited_work":{"arxiv_id":"0909.3328","doi":null,"metadata_source":"pith","pith_arxiv_id":"0909.3328","snapshot_observed_at":"2026-07-09T20:56:34.441065Z","title":"Fundamental Theoretical Bias in Gravitational Wave Astrophysics and the Parameterized Post-Einsteinian Framework","venue":"gr-qc","work_id":"85dae841-6297-42d3-868a-061fde84933e","year":2009},"citing_paper":{"arxiv_id":"2510.04703","last_updated":"2026-04-06T04:55:34Z","snapshot_observed_at":"2026-07-06T22:31:49.574184Z","submitted_at":"2025-10-06T11:16:49Z","title":"Testing black hole metrics with binary black hole inspirals","version":2},"reference_index":12,"source":"pdf_text","source_observed_at":"2026-07-11T11:50:26.030339Z"},"links":{"cited_paper":"/paper/0909.3328","citing_paper":"/paper/2510.04703"},"observation_digest":"sha256:15f36cd928d2c7eac20a939e523f339693290403c4f59f718b4d4b7c6d0b1af0","observation_id":"aedfddd7-d865-42d7-ae8f-e547dbd1eb2e","resolution":{"observed_at":"2026-05-18T09:51:12.474977Z","resolver_source":"local_arxiv","status":"verified_exact"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-04T06:34:03.388597+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-04T06:34:03.388597+00:00","source":"crossref"},{"observed_at":"2026-08-04T06:33:57.428241+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":"10.1088/1361-6382/ab8f64","metadata_source":"doi_reference","pith_arxiv_id":null,"snapshot_observed_at":"2026-06-05T21:23:00.469572Z","title":"Cardenas-Avendano, S","venue":null,"work_id":"2f23e29e-a067-46f8-a8eb-16d8fe84d109","year":2020},"citing_paper":{"arxiv_id":"2510.04703","last_updated":"2026-04-06T04:55:34Z","snapshot_observed_at":"2026-07-06T22:31:49.574184Z","submitted_at":"2025-10-06T11:16:49Z","title":"Testing black hole metrics with binary black hole inspirals","version":2},"reference_index":13,"source":"pdf_text","source_observed_at":"2026-05-18T09:47:38.064359Z"},"links":{"citing_paper":"/paper/2510.04703"},"observation_digest":"sha256:0fc637c9a14e67722d6b01c388e7a15e60846e8d521a0a72f0d4171470397b47","observation_id":"63cc1777-4c5c-469d-a00b-a00db5e8f9b9","resolution":{"observed_at":"2026-05-18T09:51:12.379214Z","resolver_source":"doi","status":"verified_exact"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-04T06:34:03.388597+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-04T06:34:03.388597+00:00","source":"crossref"},{"observed_at":"2026-08-04T06:33:57.428241+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":"10.1103/physrevd.105.104004","metadata_source":"doi_reference","pith_arxiv_id":null,"snapshot_observed_at":"2026-06-05T21:23:00.469572Z","title":"Shashank and C","venue":null,"work_id":"8670aeb1-0320-4316-a7cb-9dfd2bacc9ab","year":2022},"citing_paper":{"arxiv_id":"2510.04703","last_updated":"2026-04-06T04:55:34Z","snapshot_observed_at":"2026-07-06T22:31:49.574184Z","submitted_at":"2025-10-06T11:16:49Z","title":"Testing black hole metrics with binary black hole inspirals","version":2},"reference_index":14,"source":"pdf_text","source_observed_at":"2026-05-18T09:47:38.064359Z"},"links":{"citing_paper":"/paper/2510.04703"},"observation_digest":"sha256:21351ab415966fc55d7e98f7f56da4693121ec712e2a1e648a85fdcfab6f8dbb","observation_id":"19c519ca-59ef-445e-aa9d-728aefcedbdb","resolution":{"observed_at":"2026-05-18T09:51:12.600109Z","resolver_source":"doi","status":"verified_exact"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-04T06:34:03.388597+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-04T06:34:03.388597+00:00","source":"crossref"},{"observed_at":"2026-08-04T06:33:57.428241+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":"10.1140/epjc/s10052-","metadata_source":"doi_reference","pith_arxiv_id":null,"snapshot_observed_at":"2026-07-11T00:07:38.750706Z","title":"Jumaniyozov, S","venue":null,"work_id":"a2dfea1d-cc9f-4fc5-9dee-a95e25aa43c8","year":2011},"citing_paper":{"arxiv_id":"2510.04703","last_updated":"2026-04-06T04:55:34Z","snapshot_observed_at":"2026-07-06T22:31:49.574184Z","submitted_at":"2025-10-06T11:16:49Z","title":"Testing black hole metrics with binary black hole inspirals","version":2},"reference_index":15,"source":"pdf_text","source_observed_at":"2026-05-18T09:47:38.064359Z"},"links":{"citing_paper":"/paper/2510.04703"},"observation_digest":"sha256:d72b0af04ecaac0df602dff830b22db6abb5d3be4e5e4c19a5e01d3304d5129b","observation_id":"5e698c40-6f49-4f37-bc17-0d3cd93bbba8","resolution":{"observed_at":"2026-05-18T09:51:12.388194Z","resolver_source":"doi_truncated","status":"malformed_identifier"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-04T06:34:03.388597+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-04T06:34:03.388597+00:00","source":"crossref"},{"observed_at":"2026-08-04T06:33:57.428241+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":"10.1007/s41114-022-00041-y","metadata_source":"doi_reference","pith_arxiv_id":null,"snapshot_observed_at":"2026-07-02T09:06:48.204848Z","title":"Living Reviews in Relativity , keywords =","venue":null,"work_id":"0f255515-c5d4-44a4-a0bf-a990aeaabec5","year":2023},"citing_paper":{"arxiv_id":"2510.04703","last_updated":"2026-04-06T04:55:34Z","snapshot_observed_at":"2026-07-06T22:31:49.574184Z","submitted_at":"2025-10-06T11:16:49Z","title":"Testing black hole metrics with binary black hole inspirals","version":2},"reference_index":16,"source":"pdf_text","source_observed_at":"2026-05-18T09:47:38.064359Z"},"links":{"citing_paper":"/paper/2510.04703"},"observation_digest":"sha256:d8b15022dd3aad361343859499fb135da2401cf4159ec602ecc45761de7d8b5c","observation_id":"44b77f9d-8602-4519-86f1-dd904c084bf3","resolution":{"observed_at":"2026-05-18T09:51:12.609850Z","resolver_source":"doi","status":"verified_exact"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-04T06:34:03.388597+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-04T06:34:03.388597+00:00","source":"crossref"},{"observed_at":"2026-07-16T20:21:11.615612+00:00","source":"crossref_status_cache"},{"observed_at":"2026-07-16T20:21:11.615612+00:00","source":"openalex_status_cache"},{"observed_at":"2026-08-04T06:33:57.428241+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":"raw_reference","pith_arxiv_id":null,"snapshot_observed_at":"2026-06-05T21:23:00.469572Z","title":"Blanchet, Living Rev","venue":null,"work_id":"11332ac0-8336-4ac4-94a9-544e6a594057","year":2006},"citing_paper":{"arxiv_id":"2510.04703","last_updated":"2026-04-06T04:55:34Z","snapshot_observed_at":"2026-07-06T22:31:49.574184Z","submitted_at":"2025-10-06T11:16:49Z","title":"Testing black hole metrics with binary black hole inspirals","version":2},"reference_index":17,"source":"pdf_text","source_observed_at":"2026-05-18T09:47:38.064359Z"},"links":{"citing_paper":"/paper/2510.04703"},"observation_digest":"sha256:f84b393667e20322dd33eee4c376a0b66c48da2949d42041445d3b3503023b4d","observation_id":"b547a31e-d785-4610-93fc-5aab5963d0eb","resolution":{"observed_at":"2026-05-18T09:52:31.795886Z","resolver_source":"raw_fallback","status":"verified_fuzzy"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-04T06:34:03.388597+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-04T06:34:03.388597+00:00","source":"crossref"},{"observed_at":"2026-08-04T06:33:57.428241+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":{"arxiv_id":"1707.08426","last_updated":"2018-01-05T15:16:35Z","snapshot_observed_at":"2026-07-06T05:52:47.361285Z","submitted_at":"2017-07-26T13:22:23Z","title":"Foundations of an effective-one-body model for coalescing binaries on eccentric orbits","version":2},"cited_work":{"arxiv_id":"1707.08426","doi":null,"metadata_source":"pith","pith_arxiv_id":"1707.08426","snapshot_observed_at":"2026-06-30T16:24:58.768985Z","title":"Foundations of an effective-one-body model for coalescing binaries on eccentric orbits","venue":"gr-qc","work_id":"250a57f3-2be6-4696-86cf-4eb712ba7afb","year":2017},"citing_paper":{"arxiv_id":"2510.04703","last_updated":"2026-04-06T04:55:34Z","snapshot_observed_at":"2026-07-06T22:31:49.574184Z","submitted_at":"2025-10-06T11:16:49Z","title":"Testing black hole metrics with binary black hole inspirals","version":2},"reference_index":18,"source":"pdf_text","source_observed_at":"2026-07-11T11:50:26.030339Z"},"links":{"cited_paper":"/paper/1707.08426","citing_paper":"/paper/2510.04703"},"observation_digest":"sha256:98ccb099ec1b20847eb80e13cc61e9803a1e8a8df2474e50138c6b7a6debd045","observation_id":"56d01236-652d-4d78-a22c-761f0d697a6b","resolution":{"observed_at":"2026-05-18T09:51:12.634880Z","resolver_source":"local_arxiv","status":"verified_exact"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-04T06:34:03.388597+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-04T06:34:03.388597+00:00","source":"crossref"},{"observed_at":"2026-08-04T06:33:57.428241+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":{"arxiv_id":"1508.07253","last_updated":"2015-09-25T12:59:37Z","snapshot_observed_at":"2026-07-06T04:28:02.506375Z","submitted_at":"2015-08-28T15:58:53Z","title":"Frequency-domain gravitational waves from non-precessing black-hole binaries. II. A phenomenological model for the advanced detector era","version":2},"cited_work":{"arxiv_id":"1508.07253","doi":null,"metadata_source":"pith","pith_arxiv_id":"1508.07253","snapshot_observed_at":"2026-07-04T07:19:38.056764Z","title":"Frequency-domain gravitational waves from non-precessing black-hole binaries. II. A phenomenological model for the advanced detector era","venue":"gr-qc","work_id":"dd1b67ec-f336-41e8-bca4-418afe4815d6","year":2015},"citing_paper":{"arxiv_id":"2510.04703","last_updated":"2026-04-06T04:55:34Z","snapshot_observed_at":"2026-07-06T22:31:49.574184Z","submitted_at":"2025-10-06T11:16:49Z","title":"Testing black hole metrics with binary black hole inspirals","version":2},"reference_index":19,"source":"pdf_text","source_observed_at":"2026-07-11T11:50:26.030339Z"},"links":{"cited_paper":"/paper/1508.07253","citing_paper":"/paper/2510.04703"},"observation_digest":"sha256:443159c5f5a398e5fb4abeaf57d76300c6ebc114b0361ceea7cb273c64a4092c","observation_id":"d109d16a-221b-45aa-950e-d710ec2db7fc","resolution":{"observed_at":"2026-05-18T09:51:12.605437Z","resolver_source":"local_arxiv","status":"verified_exact"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-04T06:34:03.388597+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-04T06:34:03.388597+00:00","source":"crossref"},{"observed_at":"2026-08-04T06:33:57.428241+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":"10.1103/physrevd.104.063041","metadata_source":"doi_reference","pith_arxiv_id":null,"snapshot_observed_at":"2026-06-05T21:23:00.469572Z","title":null,"venue":null,"work_id":"010b69f2-26a3-47a7-97bc-e60704bd1fac","year":2021},"citing_paper":{"arxiv_id":"2510.04703","last_updated":"2026-04-06T04:55:34Z","snapshot_observed_at":"2026-07-06T22:31:49.574184Z","submitted_at":"2025-10-06T11:16:49Z","title":"Testing black hole metrics with binary black hole inspirals","version":2},"reference_index":20,"source":"pdf_text","source_observed_at":"2026-05-18T09:47:38.064359Z"},"links":{"citing_paper":"/paper/2510.04703"},"observation_digest":"sha256:8277c82da44e1fcea5e7f2a34d20428cc32e2254ae1235b07704d41bf5a11687","observation_id":"4ef49448-edb6-4d27-a441-f4eefa161a37","resolution":{"observed_at":"2026-05-18T09:51:12.708430Z","resolver_source":"doi","status":"verified_exact"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-04T06:34:03.388597+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-04T06:34:03.388597+00:00","source":"crossref"},{"observed_at":"2026-08-04T06:33:57.428241+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":"10.1103/physrevlett.11.237","metadata_source":"doi_reference","pith_arxiv_id":null,"snapshot_observed_at":"2026-07-03T08:47:49.367982Z","title":"Gravitational field of a spinning mass as an example of algebraically special metrics","venue":null,"work_id":"08aa2457-2fc9-4d0a-83a5-2b87e8c8008f","year":1963},"citing_paper":{"arxiv_id":"2510.04703","last_updated":"2026-04-06T04:55:34Z","snapshot_observed_at":"2026-07-06T22:31:49.574184Z","submitted_at":"2025-10-06T11:16:49Z","title":"Testing black hole metrics with binary black hole inspirals","version":2},"reference_index":21,"source":"pdf_text","source_observed_at":"2026-05-18T09:47:38.064359Z"},"links":{"citing_paper":"/paper/2510.04703"},"observation_digest":"sha256:2b2e9f914c6c17a688974cf588c0e67ab0f4c1b8f9121604d36b123a96ff573e","observation_id":"6809cf40-0434-4756-bd0b-0f760c09d69f","resolution":{"observed_at":"2026-05-18T09:51:12.703321Z","resolver_source":"doi","status":"verified_exact"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-04T06:34:03.388597+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-04T06:34:03.388597+00:00","source":"crossref"},{"observed_at":"2026-08-04T06:33:57.428241+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":"10.1063/1.1704350","metadata_source":"doi_reference","pith_arxiv_id":null,"snapshot_observed_at":"2026-06-30T13:04:39.083380Z","title":"T., & Janis, A","venue":null,"work_id":"2bf408b9-c09a-4b83-a6e7-cd6cd5e1a6f4","year":1965},"citing_paper":{"arxiv_id":"2510.04703","last_updated":"2026-04-06T04:55:34Z","snapshot_observed_at":"2026-07-06T22:31:49.574184Z","submitted_at":"2025-10-06T11:16:49Z","title":"Testing black hole metrics with binary black hole inspirals","version":2},"reference_index":22,"source":"pdf_text","source_observed_at":"2026-05-18T09:47:38.064359Z"},"links":{"citing_paper":"/paper/2510.04703"},"observation_digest":"sha256:2da3c2b368091c0e5603c218086bea9fed9a74c0e0d20208ce4de676c54092e2","observation_id":"4fc11c26-c845-40e6-a524-731b45e00471","resolution":{"observed_at":"2026-05-18T09:51:12.496245Z","resolver_source":"doi","status":"verified_exact"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-04T06:34:03.388597+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-04T06:34:03.388597+00:00","source":"crossref"},{"observed_at":"2026-07-13T12:50:31.326421+00:00","source":"crossref_status_cache"},{"observed_at":"2026-07-13T12:50:31.326421+00:00","source":"openalex_status_cache"},{"observed_at":"2026-08-04T06:33:57.428241+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":{"arxiv_id":"2205.07787","last_updated":"2023-05-26T11:55:37Z","snapshot_observed_at":"2026-07-06T13:10:28.094958Z","submitted_at":"2022-05-16T16:22:56Z","title":"Horizon-scale tests of gravity theories and fundamental physics from the Event Horizon Telescope image of Sagittarius A$^*$","version":3},"cited_work":{"arxiv_id":"2205.07787","doi":null,"metadata_source":"pith","pith_arxiv_id":"2205.07787","snapshot_observed_at":"2026-07-09T09:36:09.253132Z","title":"Horizon-scale tests of gravity theories and fundamental physics from the Event Horizon Telescope image of Sagittarius A$^*$","venue":"gr-qc","work_id":"081a5c35-17fb-4820-babf-cb9164748a63","year":2022},"citing_paper":{"arxiv_id":"2510.04703","last_updated":"2026-04-06T04:55:34Z","snapshot_observed_at":"2026-07-06T22:31:49.574184Z","submitted_at":"2025-10-06T11:16:49Z","title":"Testing black hole metrics with binary black hole inspirals","version":2},"reference_index":23,"source":"pdf_text","source_observed_at":"2026-07-11T11:50:26.030339Z"},"links":{"cited_paper":"/paper/2205.07787","citing_paper":"/paper/2510.04703"},"observation_digest":"sha256:53e233a294650d5b1434f2735d69ca97a6db4f9737f3865e34a732153329b55d","observation_id":"de60e454-2648-486e-bb15-3079cf09283a","resolution":{"observed_at":"2026-05-18T09:51:12.414190Z","resolver_source":"local_arxiv","status":"malformed_identifier"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-04T06:34:03.388597+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-04T06:34:03.388597+00:00","source":"crossref"},{"observed_at":"2026-08-04T06:33:57.428241+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":{"arxiv_id":"0812.1328","last_updated":"2009-02-03T08:10:51Z","snapshot_observed_at":"2026-07-06T01:47:43.289296Z","submitted_at":"2008-12-07T05:57:00Z","title":"Apparent shape of super-spinning black holes","version":3},"cited_work":{"arxiv_id":"0812.1328","doi":"10.1103/physrevd.79.043002","metadata_source":"pith","pith_arxiv_id":"0812.1328","snapshot_observed_at":"2026-07-11T11:50:26.030339Z","title":"Apparent shape of super-spinning black holes","venue":"astro-ph","work_id":"34c818fa-dd3d-4acd-ae4e-01625474de24","year":2008},"citing_paper":{"arxiv_id":"2510.04703","last_updated":"2026-04-06T04:55:34Z","snapshot_observed_at":"2026-07-06T22:31:49.574184Z","submitted_at":"2025-10-06T11:16:49Z","title":"Testing black hole metrics with binary black hole inspirals","version":2},"reference_index":24,"source":"pdf_text","source_observed_at":"2026-07-11T11:50:26.030339Z"},"links":{"cited_paper":"/paper/0812.1328","citing_paper":"/paper/2510.04703"},"observation_digest":"sha256:e738a472584520c7dca929d16a6323377a9d61f9d87a401842aca5a8d414a052","observation_id":"6fd28fab-2ee7-4f90-a23a-5d0894acd950","resolution":{"observed_at":"2026-05-18T09:51:12.624180Z","resolver_source":"local_arxiv","status":"verified_exact"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-04T06:34:03.388597+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-04T06:34:03.388597+00:00","source":"crossref"},{"observed_at":"2026-07-13T12:50:21.584655+00:00","source":"crossref_status_cache"},{"observed_at":"2026-07-13T12:50:21.584655+00:00","source":"openalex_status_cache"},{"observed_at":"2026-08-04T06:33:57.428241+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":{"arxiv_id":"1607.00596","last_updated":"2017-05-19T20:13:18Z","snapshot_observed_at":"2026-07-06T05:02:13.102277Z","submitted_at":"2016-07-03T05:46:12Z","title":"Testing the Kerr black hole hypothesis using X-ray reflection spectroscopy","version":2},"cited_work":{"arxiv_id":"1607.00596","doi":null,"metadata_source":"pith","pith_arxiv_id":"1607.00596","snapshot_observed_at":"2026-06-05T21:23:00.469572Z","title":"Testing the Kerr black hole hypothesis using X-ray reflection spectroscopy","venue":"gr-qc","work_id":"fca115f4-50a1-43c4-9854-90c970808523","year":2016},"citing_paper":{"arxiv_id":"2510.04703","last_updated":"2026-04-06T04:55:34Z","snapshot_observed_at":"2026-07-06T22:31:49.574184Z","submitted_at":"2025-10-06T11:16:49Z","title":"Testing black hole metrics with binary black hole inspirals","version":2},"reference_index":25,"source":"pdf_text","source_observed_at":"2026-07-11T11:50:26.030339Z"},"links":{"cited_paper":"/paper/1607.00596","citing_paper":"/paper/2510.04703"},"observation_digest":"sha256:1fe118a170d04005d1db35782473392e73675be919ef3a53bbe1cecb667eb802","observation_id":"98ba17d8-a37e-4160-867c-a4acf1435837","resolution":{"observed_at":"2026-05-18T09:51:12.511613Z","resolver_source":"local_arxiv","status":"verified_exact"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-04T06:34:03.388597+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-04T06:34:03.388597+00:00","source":"crossref"},{"observed_at":"2026-08-04T06:33:57.428241+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":{"arxiv_id":"1902.09665","last_updated":"2019-06-18T14:46:26Z","snapshot_observed_at":"2026-07-06T07:35:24.412482Z","submitted_at":"2019-02-25T23:53:38Z","title":"Public Release of RELXILL_NK: A Relativistic Reflection Model for Testing Einstein's Gravity","version":2},"cited_work":{"arxiv_id":"1902.09665","doi":"10.3847/1538-4357/ab1f89","metadata_source":"pith","pith_arxiv_id":"1902.09665","snapshot_observed_at":"2026-07-11T11:50:26.030339Z","title":"Public Release of RELXILL_NK: A Relativistic Reflection Model for Testing Einstein's Gravity","venue":"gr-qc","work_id":"fe94b084-3918-4dc4-b3f9-04d4edc689b3","year":2019},"citing_paper":{"arxiv_id":"2510.04703","last_updated":"2026-04-06T04:55:34Z","snapshot_observed_at":"2026-07-06T22:31:49.574184Z","submitted_at":"2025-10-06T11:16:49Z","title":"Testing black hole metrics with binary black hole inspirals","version":2},"reference_index":26,"source":"pdf_text","source_observed_at":"2026-07-11T11:50:26.030339Z"},"links":{"cited_paper":"/paper/1902.09665","citing_paper":"/paper/2510.04703"},"observation_digest":"sha256:02162cefa407eaf74673cb73164a6bab8c12728e3888a73f1c7303c691d1703f","observation_id":"b7dfbfc9-f805-4362-9e21-533d528fc7c9","resolution":{"observed_at":"2026-05-18T09:51:12.453294Z","resolver_source":"local_arxiv","status":"verified_exact"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-04T06:34:03.388597+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-04T06:34:03.388597+00:00","source":"crossref"},{"observed_at":"2026-07-13T10:19:37.408057+00:00","source":"crossref_status_cache"},{"observed_at":"2026-07-13T10:19:37.408057+00:00","source":"openalex_status_cache"},{"observed_at":"2026-08-04T06:33:57.428241+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":"10.3847/1538-4357/aba625","metadata_source":"doi_reference","pith_arxiv_id":null,"snapshot_observed_at":"2026-06-05T21:23:00.469572Z","title":"B., Ayzenberg, D., Bambi, C., et al","venue":null,"work_id":"c9e74ff2-9fb8-41f9-82c3-8c08ef328439","year":2020},"citing_paper":{"arxiv_id":"2510.04703","last_updated":"2026-04-06T04:55:34Z","snapshot_observed_at":"2026-07-06T22:31:49.574184Z","submitted_at":"2025-10-06T11:16:49Z","title":"Testing black hole metrics with binary black hole inspirals","version":2},"reference_index":27,"source":"pdf_text","source_observed_at":"2026-05-18T09:47:38.064359Z"},"links":{"citing_paper":"/paper/2510.04703"},"observation_digest":"sha256:1196286e3969d26ed9904a71806aac3a18d04d730a72fd4fafb2da91a820e26e","observation_id":"2a7f5488-197a-4668-9964-4bec086f23d2","resolution":{"observed_at":"2026-05-18T09:51:12.730272Z","resolver_source":"doi","status":"verified_exact"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-04T06:34:03.388597+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-04T06:34:03.388597+00:00","source":"crossref"},{"observed_at":"2026-07-13T10:19:37.72162+00:00","source":"crossref_status_cache"},{"observed_at":"2026-07-13T10:19:37.72162+00:00","source":"openalex_status_cache"},{"observed_at":"2026-08-04T06:33:57.428241+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":{"arxiv_id":"1509.03884","last_updated":"2017-04-06T21:41:09Z","snapshot_observed_at":"2026-07-06T04:29:43.654622Z","submitted_at":"2015-09-13T19:05:18Z","title":"Testing black hole candidates with electromagnetic radiation","version":4},"cited_work":{"arxiv_id":"1509.03884","doi":null,"metadata_source":"pith","pith_arxiv_id":"1509.03884","snapshot_observed_at":"2026-06-05T21:23:00.469572Z","title":"Testing black hole candidates with electromagnetic radiation","venue":"gr-qc","work_id":"82757738-97c6-439d-9ce5-cf540b455624","year":2015},"citing_paper":{"arxiv_id":"2510.04703","last_updated":"2026-04-06T04:55:34Z","snapshot_observed_at":"2026-07-06T22:31:49.574184Z","submitted_at":"2025-10-06T11:16:49Z","title":"Testing black hole metrics with binary black hole inspirals","version":2},"reference_index":28,"source":"pdf_text","source_observed_at":"2026-07-11T11:50:26.030339Z"},"links":{"cited_paper":"/paper/1509.03884","citing_paper":"/paper/2510.04703"},"observation_digest":"sha256:77504fa9f4caac446d9c7fdc7bc30a848bd1a554fc40f0251c28e6b2264ed31b","observation_id":"40d555f2-6cf5-4c95-8682-efb8113b3736","resolution":{"observed_at":"2026-05-18T09:51:12.517634Z","resolver_source":"local_arxiv","status":"verified_exact"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-04T06:34:03.388597+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-04T06:34:03.388597+00:00","source":"crossref"},{"observed_at":"2026-08-04T06:33:57.428241+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":{"arxiv_id":"1709.00219","last_updated":"2018-02-02T00:23:20Z","snapshot_observed_at":"2026-07-06T05:57:41.376252Z","submitted_at":"2017-09-01T09:43:43Z","title":"Testing general relativity with the reflection spectrum of the supermassive black hole in 1H0707$-$495","version":2},"cited_work":{"arxiv_id":"1709.00219","doi":null,"metadata_source":"pith","pith_arxiv_id":"1709.00219","snapshot_observed_at":"2026-06-05T21:23:00.469572Z","title":"Testing general relativity with the reflection spectrum of the supermassive black hole in 1H0707$-$495","venue":"gr-qc","work_id":"1d59e9d5-3a02-4a23-ae9e-cadac8603caa","year":2017},"citing_paper":{"arxiv_id":"2510.04703","last_updated":"2026-04-06T04:55:34Z","snapshot_observed_at":"2026-07-06T22:31:49.574184Z","submitted_at":"2025-10-06T11:16:49Z","title":"Testing black hole metrics with binary black hole inspirals","version":2},"reference_index":29,"source":"pdf_text","source_observed_at":"2026-07-11T11:50:26.030339Z"},"links":{"cited_paper":"/paper/1709.00219","citing_paper":"/paper/2510.04703"},"observation_digest":"sha256:6722f935533c1e3108cf14804527e242174302bc79ad9ff76d25c35d65a687bb","observation_id":"f804842f-5a00-4d16-a527-e51fbc4cf54f","resolution":{"observed_at":"2026-05-18T09:51:12.735762Z","resolver_source":"local_arxiv","status":"verified_exact"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-04T06:34:03.388597+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-04T06:34:03.388597+00:00","source":"crossref"},{"observed_at":"2026-08-04T06:33:57.428241+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":{"arxiv_id":"1901.03064","last_updated":"2019-04-02T22:05:53Z","snapshot_observed_at":"2026-08-02T13:57:52.564061Z","submitted_at":"2019-01-10T09:06:38Z","title":"Constraints on the spacetime metric around seven \"bare\" AGNs using X-ray reflection spectroscopy","version":2},"cited_work":{"arxiv_id":"1901.03064","doi":null,"metadata_source":"pith","pith_arxiv_id":"1901.03064","snapshot_observed_at":"2026-06-05T21:23:00.469572Z","title":"Constraints on the spacetime metric around seven \"bare\" AGNs using X-ray reflection spectroscopy","venue":"gr-qc","work_id":"69dc5ba7-1e43-44e7-9dfa-074c0446aacf","year":2019},"citing_paper":{"arxiv_id":"2510.04703","last_updated":"2026-04-06T04:55:34Z","snapshot_observed_at":"2026-07-06T22:31:49.574184Z","submitted_at":"2025-10-06T11:16:49Z","title":"Testing black hole metrics with binary black hole inspirals","version":2},"reference_index":30,"source":"pdf_text","source_observed_at":"2026-07-11T11:50:26.030339Z"},"links":{"cited_paper":"/paper/1901.03064","citing_paper":"/paper/2510.04703"},"observation_digest":"sha256:fe5b7f4d2219b7b7dd51800532ff57aad0ba50e75511748a894ed62eedfbd6d4","observation_id":"2049217e-5b84-4347-9c6f-1e94374ea9ca","resolution":{"observed_at":"2026-05-18T09:51:12.551993Z","resolver_source":"local_arxiv","status":"verified_exact"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-04T06:34:03.388597+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-04T06:34:03.388597+00:00","source":"crossref"},{"observed_at":"2026-08-04T06:33:57.428241+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":{"arxiv_id":"1811.08148","last_updated":"2019-04-17T00:04:08Z","snapshot_observed_at":"2026-07-31T03:24:37.324944Z","submitted_at":"2018-11-20T09:39:50Z","title":"Towards precision tests of general relativity with black hole X-ray reflection spectroscopy","version":2},"cited_work":{"arxiv_id":"1811.08148","doi":null,"metadata_source":"pith","pith_arxiv_id":"1811.08148","snapshot_observed_at":"2026-06-05T21:23:00.469572Z","title":"Towards precision tests of general relativity with black hole X-ray reflection spectroscopy","venue":"gr-qc","work_id":"4e85b85d-d53d-4c78-9d1c-e09cc3e7c7ce","year":2018},"citing_paper":{"arxiv_id":"2510.04703","last_updated":"2026-04-06T04:55:34Z","snapshot_observed_at":"2026-07-06T22:31:49.574184Z","submitted_at":"2025-10-06T11:16:49Z","title":"Testing black hole metrics with binary black hole inspirals","version":2},"reference_index":31,"source":"pdf_text","source_observed_at":"2026-07-11T11:50:26.030339Z"},"links":{"cited_paper":"/paper/1811.08148","citing_paper":"/paper/2510.04703"},"observation_digest":"sha256:3858dedb580b5c089588453c9563522467896ddf3175eb3325f02cdc6304882e","observation_id":"fef8a9cc-f882-4a2b-a9ff-310c1b4f3f4c","resolution":{"observed_at":"2026-05-18T09:51:12.742427Z","resolver_source":"local_arxiv","status":"verified_exact"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-04T06:34:03.388597+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-04T06:34:03.388597+00:00","source":"crossref"},{"observed_at":"2026-08-04T06:33:57.428241+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":"10.3847/1538-4357/abf6cd","metadata_source":"doi_reference","pith_arxiv_id":null,"snapshot_observed_at":"2026-06-27T16:01:01.049786Z","title":"Tripathi, Y","venue":null,"work_id":"2f6a53f7-be07-4ac1-9583-08890041b1b8","year":2021},"citing_paper":{"arxiv_id":"2510.04703","last_updated":"2026-04-06T04:55:34Z","snapshot_observed_at":"2026-07-06T22:31:49.574184Z","submitted_at":"2025-10-06T11:16:49Z","title":"Testing black hole metrics with binary black hole inspirals","version":2},"reference_index":32,"source":"pdf_text","source_observed_at":"2026-05-18T09:47:38.064359Z"},"links":{"citing_paper":"/paper/2510.04703"},"observation_digest":"sha256:e442bf96b8fedf8702a7946fb73ec7aeffe3f986999b31800992410e5c75ab6f","observation_id":"0b672c56-8116-43c5-9df1-fde64eb26ca0","resolution":{"observed_at":"2026-05-18T09:51:12.723073Z","resolver_source":"doi","status":"verified_exact"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-04T06:34:03.388597+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-04T06:34:03.388597+00:00","source":"crossref"},{"observed_at":"2026-07-13T10:19:35.044704+00:00","source":"crossref_status_cache"},{"observed_at":"2026-07-13T10:19:35.044704+00:00","source":"openalex_status_cache"},{"observed_at":"2026-08-04T06:33:57.428241+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":"raw_reference","pith_arxiv_id":null,"snapshot_observed_at":"2026-06-05T21:23:00.469572Z","title":null,"venue":null,"work_id":"11c214a1-e111-4c2d-8654-642146196575","year":1968},"citing_paper":{"arxiv_id":"2510.04703","last_updated":"2026-04-06T04:55:34Z","snapshot_observed_at":"2026-07-06T22:31:49.574184Z","submitted_at":"2025-10-06T11:16:49Z","title":"Testing black hole metrics with binary black hole inspirals","version":2},"reference_index":33,"source":"pdf_text","source_observed_at":"2026-05-18T09:47:38.064359Z"},"links":{"citing_paper":"/paper/2510.04703"},"observation_digest":"sha256:c30b0c7fcea2292a639ce3d69f20c1e9e19c7836c1db1b2e38c0bc848250beb7","observation_id":"070268e2-bd00-4cae-850a-2425f07a0b9a","resolution":{"observed_at":"2026-05-18T09:52:31.793277Z","resolver_source":"raw_fallback","status":"unresolved"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-04T06:34:03.388597+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-04T06:34:03.388597+00:00","source":"crossref"},{"observed_at":"2026-08-04T06:33:57.428241+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":{"arxiv_id":"gr-qc/0009077","last_updated":"2000-09-22T00:44:55Z","snapshot_observed_at":"2026-08-02T20:26:14.413721Z","submitted_at":"2000-09-22T00:44:55Z","title":"The Bardeen Model as a Nonlinear Magnetic Monopole","version":1},"cited_work":{"arxiv_id":"gr-qc/0009077","doi":"10.1016/s0370-2693(00)01125-","metadata_source":"pith","pith_arxiv_id":"gr-qc/0009077","snapshot_observed_at":"2026-07-11T11:50:26.030339Z","title":"The Bardeen Model as a Nonlinear Magnetic Monopole","venue":"gr-qc","work_id":"72742531-704a-4d91-a991-b8f4fdf35f82","year":2000},"citing_paper":{"arxiv_id":"2510.04703","last_updated":"2026-04-06T04:55:34Z","snapshot_observed_at":"2026-07-06T22:31:49.574184Z","submitted_at":"2025-10-06T11:16:49Z","title":"Testing black hole metrics with binary black hole inspirals","version":2},"reference_index":34,"source":"pdf_text","source_observed_at":"2026-07-11T11:50:26.030339Z"},"links":{"cited_paper":"/paper/gr-qc/0009077","citing_paper":"/paper/2510.04703"},"observation_digest":"sha256:e5b3433d6145ad07f689a563e0e9fcbaef3295c481fbde45e8fd81dd207be23f","observation_id":"da33af3d-86e0-46a2-87b3-46c5c1dbe9cd","resolution":{"observed_at":"2026-05-18T09:51:12.562712Z","resolver_source":"local_arxiv","status":"malformed_identifier"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-04T06:34:03.388597+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-04T06:34:03.388597+00:00","source":"crossref"},{"observed_at":"2026-08-04T06:33:57.428241+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":{"arxiv_id":"hep-th/0403229","last_updated":"2005-05-05T17:29:38Z","snapshot_observed_at":"2026-07-07T04:50:08.532517Z","submitted_at":"2004-03-23T02:26:58Z","title":"Four Parametric Regular Black Hole Solution","version":2},"cited_work":{"arxiv_id":"hep-th/0403229","doi":null,"metadata_source":"pith","pith_arxiv_id":"hep-th/0403229","snapshot_observed_at":"2026-07-10T03:56:44.499089Z","title":"Four Parametric Regular Black Hole Solution","venue":"hep-th","work_id":"35b9e417-02cd-4c59-989a-1304f1761810","year":2004},"citing_paper":{"arxiv_id":"2510.04703","last_updated":"2026-04-06T04:55:34Z","snapshot_observed_at":"2026-07-06T22:31:49.574184Z","submitted_at":"2025-10-06T11:16:49Z","title":"Testing black hole metrics with binary black hole inspirals","version":2},"reference_index":35,"source":"pdf_text","source_observed_at":"2026-07-11T11:50:26.030339Z"},"links":{"cited_paper":"/paper/hep-th/0403229","citing_paper":"/paper/2510.04703"},"observation_digest":"sha256:643931ea6c9dd6accd515cca23ba8e1454890321d993b2fb9662139b5f3b7cfc","observation_id":"fcb815ea-8f86-46b4-9ba6-f964180cec5b","resolution":{"observed_at":"2026-05-18T09:51:12.433597Z","resolver_source":"local_arxiv","status":"verified_exact"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-04T06:34:03.388597+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-04T06:34:03.388597+00:00","source":"crossref"},{"observed_at":"2026-08-04T06:33:57.428241+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":{"arxiv_id":"1801.08872","last_updated":"2018-12-05T13:42:59Z","snapshot_observed_at":"2026-07-06T06:20:26.483102Z","submitted_at":"2018-01-26T18:53:58Z","title":"Bardeen regular black hole as a quantum-corrected Schwarzschild black hole","version":2},"cited_work":{"arxiv_id":"1801.08872","doi":"10.1142/s0218271819500482","metadata_source":"pith","pith_arxiv_id":"1801.08872","snapshot_observed_at":"2026-07-11T11:50:26.030339Z","title":"Bardeen regular black hole as a quantum-corrected Schwarzschild black hole","venue":"gr-qc","work_id":"33787205-167d-421b-bdca-37c7295a197e","year":2018},"citing_paper":{"arxiv_id":"2510.04703","last_updated":"2026-04-06T04:55:34Z","snapshot_observed_at":"2026-07-06T22:31:49.574184Z","submitted_at":"2025-10-06T11:16:49Z","title":"Testing black hole metrics with binary black hole inspirals","version":2},"reference_index":36,"source":"pdf_text","source_observed_at":"2026-07-11T11:50:26.030339Z"},"links":{"cited_paper":"/paper/1801.08872","citing_paper":"/paper/2510.04703"},"observation_digest":"sha256:4a04ca012dd9f78953e771eb9206d8ae5bfde08b4c87b0f1ff2663bae5517e22","observation_id":"5056ced3-1ea9-4398-bff6-a37befebf971","resolution":{"observed_at":"2026-05-18T09:51:12.694256Z","resolver_source":"local_arxiv","status":"verified_exact"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-04T06:34:03.388597+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-04T06:34:03.388597+00:00","source":"crossref"},{"observed_at":"2026-08-04T06:33:57.428241+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":{"arxiv_id":"1302.6075","last_updated":"2013-03-26T14:31:07Z","snapshot_observed_at":"2026-07-06T02:11:23.670680Z","submitted_at":"2013-02-25T12:29:05Z","title":"Rotating regular black holes","version":2},"cited_work":{"arxiv_id":"1302.6075","doi":null,"metadata_source":"pith","pith_arxiv_id":"1302.6075","snapshot_observed_at":"2026-07-10T03:56:44.590682Z","title":"Rotating regular black holes","venue":"gr-qc","work_id":"75a6fd09-a706-4511-ad8f-80afc0b8f5e1","year":2013},"citing_paper":{"arxiv_id":"2510.04703","last_updated":"2026-04-06T04:55:34Z","snapshot_observed_at":"2026-07-06T22:31:49.574184Z","submitted_at":"2025-10-06T11:16:49Z","title":"Testing black hole metrics with binary black hole inspirals","version":2},"reference_index":37,"source":"pdf_text","source_observed_at":"2026-07-11T11:50:26.030339Z"},"links":{"cited_paper":"/paper/1302.6075","citing_paper":"/paper/2510.04703"},"observation_digest":"sha256:fa3871ee46a19d93b144e6bff089d5012327ef29bf2bb137bf6ffdf0f4178a0c","observation_id":"45198888-b926-407b-b58f-a3bfb2ca4e5e","resolution":{"observed_at":"2026-05-18T09:51:12.614918Z","resolver_source":"local_arxiv","status":"verified_exact"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-04T06:34:03.388597+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-04T06:34:03.388597+00:00","source":"crossref"},{"observed_at":"2026-08-04T06:33:57.428241+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":{"arxiv_id":"1401.4640","last_updated":"2014-01-25T19:53:51Z","snapshot_observed_at":"2026-08-02T06:58:40.425030Z","submitted_at":"2014-01-19T06:57:26Z","title":"Testing the Bardeen metric with the black hole candidate in Cygnus X-1","version":2},"cited_work":{"arxiv_id":"1401.4640","doi":null,"metadata_source":"pith","pith_arxiv_id":"1401.4640","snapshot_observed_at":"2026-06-05T21:23:00.469572Z","title":"Testing the Bardeen metric with the black hole candidate in Cygnus X-1","venue":"gr-qc","work_id":"e18489f3-7db4-499b-98be-c1ed84b120d1","year":2014},"citing_paper":{"arxiv_id":"2510.04703","last_updated":"2026-04-06T04:55:34Z","snapshot_observed_at":"2026-07-06T22:31:49.574184Z","submitted_at":"2025-10-06T11:16:49Z","title":"Testing black hole metrics with binary black hole inspirals","version":2},"reference_index":38,"source":"pdf_text","source_observed_at":"2026-07-11T11:50:26.030339Z"},"links":{"cited_paper":"/paper/1401.4640","citing_paper":"/paper/2510.04703"},"observation_digest":"sha256:e7e489d4790e0f1f316fda2f679e5069f302a14422b6b30aec1b2b22b96741ec","observation_id":"04a4aaf0-d3a0-4ac3-8b3a-30167ea4d518","resolution":{"observed_at":"2026-05-18T09:51:12.683533Z","resolver_source":"local_arxiv","status":"verified_exact"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-04T06:34:03.388597+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-04T06:34:03.388597+00:00","source":"crossref"},{"observed_at":"2026-08-04T06:33:57.428241+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":"10.1103/physrevlett.96.031103","metadata_source":"doi_reference","pith_arxiv_id":null,"snapshot_observed_at":"2026-07-09T03:05:54.779250Z","title":"Formation and evaporation of nonsingular black holes","venue":null,"work_id":"8ac6b2c1-de6b-4728-83b1-ed150e7f18ef","year":2006},"citing_paper":{"arxiv_id":"2510.04703","last_updated":"2026-04-06T04:55:34Z","snapshot_observed_at":"2026-07-06T22:31:49.574184Z","submitted_at":"2025-10-06T11:16:49Z","title":"Testing black hole metrics with binary black hole inspirals","version":2},"reference_index":39,"source":"pdf_text","source_observed_at":"2026-05-18T09:47:38.064359Z"},"links":{"citing_paper":"/paper/2510.04703"},"observation_digest":"sha256:cba777be357c7502f029c442c845b882f91c0bb95cd400b79c412216115d4db3","observation_id":"40f42fe1-90f8-4153-a853-8ecbefe3e520","resolution":{"observed_at":"2026-05-18T09:51:12.698578Z","resolver_source":"doi","status":"verified_exact"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-04T06:34:03.388597+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-04T06:34:03.388597+00:00","source":"crossref"},{"observed_at":"2026-07-16T22:51:36.054213+00:00","source":"crossref_status_cache"},{"observed_at":"2026-07-16T22:51:36.054213+00:00","source":"openalex_status_cache"},{"observed_at":"2026-08-04T06:33:57.428241+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":{"arxiv_id":"hep-th/0002196","last_updated":"2000-02-23T11:40:36Z","snapshot_observed_at":"2026-07-07T04:35:58.689626Z","submitted_at":"2000-02-23T11:40:36Z","title":"Renormalization group improved black hole spacetimes","version":1},"cited_work":{"arxiv_id":"hep-th/0002196","doi":null,"metadata_source":"pith","pith_arxiv_id":"hep-th/0002196","snapshot_observed_at":"2026-07-10T11:07:02.072897Z","title":"Renormalization group improved black hole spacetimes","venue":"hep-th","work_id":"23d2379e-05d2-482d-afb6-2305a4e8f7eb","year":2000},"citing_paper":{"arxiv_id":"2510.04703","last_updated":"2026-04-06T04:55:34Z","snapshot_observed_at":"2026-07-06T22:31:49.574184Z","submitted_at":"2025-10-06T11:16:49Z","title":"Testing black hole metrics with binary black hole inspirals","version":2},"reference_index":40,"source":"pdf_text","source_observed_at":"2026-07-11T11:50:26.030339Z"},"links":{"cited_paper":"/paper/hep-th/0002196","citing_paper":"/paper/2510.04703"},"observation_digest":"sha256:e3cdc74502108b98a302dfea690b4a38022dbd2abc08ed185eb2760dd919e9f7","observation_id":"0e7151b6-9a09-4696-b87c-126d2e9be695","resolution":{"observed_at":"2026-05-18T09:51:12.530596Z","resolver_source":"local_arxiv","status":"verified_exact"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-04T06:34:03.388597+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-04T06:34:03.388597+00:00","source":"crossref"},{"observed_at":"2026-08-04T06:33:57.428241+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":{"arxiv_id":"1702.03567","last_updated":"2017-05-16T16:41:11Z","snapshot_observed_at":"2026-07-06T05:29:43.545440Z","submitted_at":"2017-02-12T20:10:46Z","title":"Non-singular quantum improved rotating black holes and their maximal extension","version":2},"cited_work":{"arxiv_id":"1702.03567","doi":"10.1007/s10714-017-2236-5","metadata_source":"pith","pith_arxiv_id":"1702.03567","snapshot_observed_at":"2026-07-11T11:50:26.030339Z","title":"Non-singular quantum improved rotating black holes and their maximal extension","venue":"gr-qc","work_id":"53f63a43-1b83-4ed5-8937-1259a1d67cae","year":2017},"citing_paper":{"arxiv_id":"2510.04703","last_updated":"2026-04-06T04:55:34Z","snapshot_observed_at":"2026-07-06T22:31:49.574184Z","submitted_at":"2025-10-06T11:16:49Z","title":"Testing black hole metrics with binary black hole inspirals","version":2},"reference_index":41,"source":"pdf_text","source_observed_at":"2026-07-11T11:50:26.030339Z"},"links":{"cited_paper":"/paper/1702.03567","citing_paper":"/paper/2510.04703"},"observation_digest":"sha256:7495cbf65e01c4a6cb49a1af18d1ad511c5d922265fdf679fb842b6ec0ef401b","observation_id":"a702abc6-9ae2-494c-85f3-a0ffae5f1194","resolution":{"observed_at":"2026-05-18T09:51:12.427934Z","resolver_source":"local_arxiv","status":"verified_exact"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-04T06:34:03.388597+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-04T06:34:03.388597+00:00","source":"crossref"},{"observed_at":"2026-08-04T06:33:57.428241+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":"10.1088/1475-7516/2021/01/047","metadata_source":"doi_reference","pith_arxiv_id":null,"snapshot_observed_at":"2026-06-05T21:23:00.469572Z","title":null,"venue":null,"work_id":"5da086fe-fed8-44c7-9c99-073d0361ac95","year":2021},"citing_paper":{"arxiv_id":"2510.04703","last_updated":"2026-04-06T04:55:34Z","snapshot_observed_at":"2026-07-06T22:31:49.574184Z","submitted_at":"2025-10-06T11:16:49Z","title":"Testing black hole metrics with binary black hole inspirals","version":2},"reference_index":42,"source":"pdf_text","source_observed_at":"2026-05-18T09:47:38.064359Z"},"links":{"citing_paper":"/paper/2510.04703"},"observation_digest":"sha256:15b3746ddc99781a81ed165c8292df1f161bf9026c3b8ae67ffbea46fd390ee2","observation_id":"115d440c-ed91-47dd-b451-a580bec85712","resolution":{"observed_at":"2026-05-18T09:51:12.491865Z","resolver_source":"doi","status":"verified_exact"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-04T06:34:03.388597+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-04T06:34:03.388597+00:00","source":"crossref"},{"observed_at":"2026-08-04T06:33:57.428241+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":"2021.136390","doi":"10.1016/j.physletb.2021.136390","metadata_source":"arxiv_reference","pith_arxiv_id":null,"snapshot_observed_at":"2026-07-11T11:50:26.030339Z","title":"Bodendorfer, F","venue":null,"work_id":"29f6ec58-7607-4e36-bc29-129451156c48","year":2021},"citing_paper":{"arxiv_id":"2510.04703","last_updated":"2026-04-06T04:55:34Z","snapshot_observed_at":"2026-07-06T22:31:49.574184Z","submitted_at":"2025-10-06T11:16:49Z","title":"Testing black hole metrics with binary black hole inspirals","version":2},"reference_index":43,"source":"pdf_text","source_observed_at":"2026-05-18T09:47:38.064359Z"},"links":{"citing_paper":"/paper/2510.04703"},"observation_digest":"sha256:29e915ad7aa20c8c570f2bebf3092513fb6faaebd3e449ce01f5531150a491f4","observation_id":"f77c241c-ca7e-4e79-9c9a-6cfa77ea5503","resolution":{"observed_at":"2026-05-18T09:51:12.440041Z","resolver_source":"arxiv_id","status":"verified_exact"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-04T06:34:03.388597+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-04T06:34:03.388597+00:00","source":"crossref"},{"observed_at":"2026-08-04T06:33:57.428241+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":"10.1088/1361-6382/abe05d","metadata_source":"doi_reference","pith_arxiv_id":null,"snapshot_observed_at":"2026-06-05T21:23:00.469572Z","title":"Bodendorfer, F","venue":null,"work_id":"8102adb0-980f-4fe0-8fc8-0d158d367a7b","year":2021},"citing_paper":{"arxiv_id":"2510.04703","last_updated":"2026-04-06T04:55:34Z","snapshot_observed_at":"2026-07-06T22:31:49.574184Z","submitted_at":"2025-10-06T11:16:49Z","title":"Testing black hole metrics with binary black hole inspirals","version":2},"reference_index":44,"source":"pdf_text","source_observed_at":"2026-05-18T09:47:38.064359Z"},"links":{"citing_paper":"/paper/2510.04703"},"observation_digest":"sha256:1291d947c8a5f46c809276f5305565f5f86e7f2a19ee9bf5a014e560e98ed0fd","observation_id":"6939d7c5-3437-487f-acbb-009bcf06d596","resolution":{"observed_at":"2026-05-18T09:51:12.468672Z","resolver_source":"doi","status":"verified_exact"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-04T06:34:03.388597+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-04T06:34:03.388597+00:00","source":"crossref"},{"observed_at":"2026-08-04T06:33:57.428241+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":"10.1103/physrevlett.126.181301","metadata_source":"doi_reference","pith_arxiv_id":null,"snapshot_observed_at":"2026-06-30T13:04:39.100040Z","title":"Brahma, C","venue":null,"work_id":"b77a5860-8fb3-45cb-b7bb-3d2368074e8d","year":2021},"citing_paper":{"arxiv_id":"2510.04703","last_updated":"2026-04-06T04:55:34Z","snapshot_observed_at":"2026-07-06T22:31:49.574184Z","submitted_at":"2025-10-06T11:16:49Z","title":"Testing black hole metrics with binary black hole inspirals","version":2},"reference_index":45,"source":"pdf_text","source_observed_at":"2026-05-18T09:47:38.064359Z"},"links":{"citing_paper":"/paper/2510.04703"},"observation_digest":"sha256:b59ca14182c1bbe810e259b4488d6e1e74c2a8e41bd7584a9bbcc335100b2e7d","observation_id":"b12ee059-6d97-40d0-ba1d-fda1321b1796","resolution":{"observed_at":"2026-05-18T09:51:12.588656Z","resolver_source":"doi","status":"verified_exact"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-04T06:34:03.388597+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-04T06:34:03.388597+00:00","source":"crossref"},{"observed_at":"2026-08-04T06:33:57.428241+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":"10.3847/1538-","metadata_source":"doi_reference","pith_arxiv_id":null,"snapshot_observed_at":"2026-07-09T15:56:19.393046Z","title":"S., Bindi, V., Zhang, M., Feng, X., 2019, A Numerical Study of Cosmic Proton Modulation Using AMS-02 Observations , Astrophys","venue":null,"work_id":"02c51af2-7d22-4018-b41a-9de4b65b7c4a","year":2019},"citing_paper":{"arxiv_id":"2510.04703","last_updated":"2026-04-06T04:55:34Z","snapshot_observed_at":"2026-07-06T22:31:49.574184Z","submitted_at":"2025-10-06T11:16:49Z","title":"Testing black hole metrics with binary black hole inspirals","version":2},"reference_index":46,"source":"pdf_text","source_observed_at":"2026-05-18T09:47:38.064359Z"},"links":{"citing_paper":"/paper/2510.04703"},"observation_digest":"sha256:b280127fd824bb95c5abd231a058a5da7f463e761f2ed3ce3c97edba9e9bf491","observation_id":"12932867-95bb-4821-97c4-b22202226dd3","resolution":{"observed_at":"2026-05-18T09:51:12.618763Z","resolver_source":"doi_truncated","status":"malformed_identifier"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-04T06:34:03.388597+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-04T06:34:03.388597+00:00","source":"crossref"},{"observed_at":"2026-08-04T06:33:57.428241+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":{"arxiv_id":"0801.4074","last_updated":"2008-05-21T12:17:10Z","snapshot_observed_at":"2026-07-06T01:34:45.604137Z","submitted_at":"2008-01-26T12:26:08Z","title":"Hawking Radiation as Quantum Tunneling from Noncommutative Schwarzschild Black Hole","version":3},"cited_work":{"arxiv_id":"0801.4074","doi":null,"metadata_source":"pith","pith_arxiv_id":"0801.4074","snapshot_observed_at":"2026-06-05T21:23:00.469572Z","title":"Hawking Radiation as Quantum Tunneling from Noncommutative Schwarzschild Black Hole","venue":"gr-qc","work_id":"e1e2920e-d64a-4494-b9a0-5c8e2fde975a","year":2008},"citing_paper":{"arxiv_id":"2510.04703","last_updated":"2026-04-06T04:55:34Z","snapshot_observed_at":"2026-07-06T22:31:49.574184Z","submitted_at":"2025-10-06T11:16:49Z","title":"Testing black hole metrics with binary black hole inspirals","version":2},"reference_index":47,"source":"pdf_text","source_observed_at":"2026-07-11T11:50:26.030339Z"},"links":{"cited_paper":"/paper/0801.4074","citing_paper":"/paper/2510.04703"},"observation_digest":"sha256:216276492771a368a5d325a855b491af7cd171585dcdd99f75f49192b155c49d","observation_id":"99806a38-7c9a-4a5e-b370-7e9bc749b895","resolution":{"observed_at":"2026-05-18T09:51:12.464977Z","resolver_source":"local_arxiv","status":"malformed_identifier"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-04T06:34:03.388597+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-04T06:34:03.388597+00:00","source":"crossref"},{"observed_at":"2026-08-04T06:33:57.428241+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":"2020.135334","doi":"10.1016/j.physletb.2020.135334","metadata_source":"arxiv_reference","pith_arxiv_id":null,"snapshot_observed_at":"2026-07-11T11:50:26.030339Z","title":null,"venue":null,"work_id":"15dccd3e-8e79-4b31-8d96-3ed84a563412","year":2020},"citing_paper":{"arxiv_id":"2510.04703","last_updated":"2026-04-06T04:55:34Z","snapshot_observed_at":"2026-07-06T22:31:49.574184Z","submitted_at":"2025-10-06T11:16:49Z","title":"Testing black hole metrics with binary black hole inspirals","version":2},"reference_index":48,"source":"pdf_text","source_observed_at":"2026-05-18T09:47:38.064359Z"},"links":{"citing_paper":"/paper/2510.04703"},"observation_digest":"sha256:f651592460994a4e574018fcd5773111e3a3f2c3ba0ff65e8ca16f097cc3fcee","observation_id":"28e3f152-6127-4902-8551-42cc1d9689fb","resolution":{"observed_at":"2026-05-18T09:51:12.420428Z","resolver_source":"arxiv_id","status":"verified_exact"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-04T06:34:03.388597+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-04T06:34:03.388597+00:00","source":"crossref"},{"observed_at":"2026-08-04T06:33:57.428241+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":"2024.101796","doi":"10.1016/j.dark.2024.101796","metadata_source":"arxiv_reference","pith_arxiv_id":null,"snapshot_observed_at":"2026-07-11T11:50:26.030339Z","title":null,"venue":null,"work_id":"2860187c-a31a-41ac-88c5-682720a7cbd3","year":2025},"citing_paper":{"arxiv_id":"2510.04703","last_updated":"2026-04-06T04:55:34Z","snapshot_observed_at":"2026-07-06T22:31:49.574184Z","submitted_at":"2025-10-06T11:16:49Z","title":"Testing black hole metrics with binary black hole inspirals","version":2},"reference_index":49,"source":"pdf_text","source_observed_at":"2026-05-18T09:47:38.064359Z"},"links":{"citing_paper":"/paper/2510.04703"},"observation_digest":"sha256:97cecb5b1ee5f99eb5cc4fb373f11b9cb55a79c284f74301bc6d2d78ea98e609","observation_id":"d7bf0a39-744c-4552-9675-7f74cd7bf6fb","resolution":{"observed_at":"2026-05-18T09:51:12.578638Z","resolver_source":"arxiv_id","status":"verified_exact"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-04T06:34:03.388597+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-04T06:34:03.388597+00:00","source":"crossref"},{"observed_at":"2026-08-04T06:33:57.428241+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":{"arxiv_id":"1107.1424","last_updated":"2012-08-22T20:09:59Z","snapshot_observed_at":"2026-07-06T02:30:32.520614Z","submitted_at":"2011-07-07T15:26:20Z","title":"Quantum corrections to gravity","version":2},"cited_work":{"arxiv_id":"1107.1424","doi":null,"metadata_source":"pith","pith_arxiv_id":"1107.1424","snapshot_observed_at":"2026-07-04T14:29:54.412192Z","title":"Quantum corrections to gravity","venue":"gr-qc","work_id":"c92b3e43-7c43-4345-9571-df055442c5c7","year":2011},"citing_paper":{"arxiv_id":"2510.04703","last_updated":"2026-04-06T04:55:34Z","snapshot_observed_at":"2026-07-06T22:31:49.574184Z","submitted_at":"2025-10-06T11:16:49Z","title":"Testing black hole metrics with binary black hole inspirals","version":2},"reference_index":50,"source":"pdf_text","source_observed_at":"2026-05-18T09:47:38.064359Z"},"links":{"cited_paper":"/paper/1107.1424","citing_paper":"/paper/2510.04703"},"observation_digest":"sha256:5fd534b2a6340252fc52a26ec2671d91c3dd3ecac9f6a2518cdc0f99eb8a4168","observation_id":"0e1cce41-be17-4885-90db-175d6ea14af6","resolution":{"observed_at":"2026-05-18T09:51:13.694347Z","resolver_source":"local_arxiv","status":"metadata_mismatch"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-04T06:34:03.388597+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-04T06:34:03.388597+00:00","source":"crossref"},{"observed_at":"2026-08-04T06:33:57.428241+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":"10.1088/1475-7516/2020/07/053","metadata_source":"doi_reference","pith_arxiv_id":null,"snapshot_observed_at":"2026-06-30T13:04:39.312558Z","title":"Kumar and S","venue":null,"work_id":"827c7b99-cb81-4194-9fb2-1667b74d2288","year":2020},"citing_paper":{"arxiv_id":"2510.04703","last_updated":"2026-04-06T04:55:34Z","snapshot_observed_at":"2026-07-06T22:31:49.574184Z","submitted_at":"2025-10-06T11:16:49Z","title":"Testing black hole metrics with binary black hole inspirals","version":2},"reference_index":51,"source":"pdf_text","source_observed_at":"2026-05-18T09:47:38.064359Z"},"links":{"citing_paper":"/paper/2510.04703"},"observation_digest":"sha256:166bee711fbc92d83738626c7e97e1beb4f28d530fcec8cb31294955613a1bef","observation_id":"f9bfaae9-f268-4057-9e21-d81a7f368c10","resolution":{"observed_at":"2026-05-18T09:51:12.486480Z","resolver_source":"doi","status":"verified_exact"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-04T06:34:03.388597+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-04T06:34:03.388597+00:00","source":"crossref"},{"observed_at":"2026-07-13T12:50:30.264123+00:00","source":"crossref_status_cache"},{"observed_at":"2026-07-13T12:50:30.264123+00:00","source":"openalex_status_cache"},{"observed_at":"2026-08-04T06:33:57.428241+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":"10.1103/physrevlett.54.502","metadata_source":"doi_reference","pith_arxiv_id":null,"snapshot_observed_at":"2026-06-28T12:02:06.530676Z","title":"Gross, J.A","venue":null,"work_id":"8f4dc734-ee26-48cc-a990-981f340d2a8b","year":1985},"citing_paper":{"arxiv_id":"2510.04703","last_updated":"2026-04-06T04:55:34Z","snapshot_observed_at":"2026-07-06T22:31:49.574184Z","submitted_at":"2025-10-06T11:16:49Z","title":"Testing black hole metrics with binary black hole inspirals","version":2},"reference_index":52,"source":"pdf_text","source_observed_at":"2026-05-18T09:47:38.064359Z"},"links":{"citing_paper":"/paper/2510.04703"},"observation_digest":"sha256:93632028fc5229c0a8e040bf0bbb4bf6b3bcd7cf4c0a0c492461aa33d928ed72","observation_id":"2acc3341-30cd-4696-8784-a159f0a349ca","resolution":{"observed_at":"2026-05-18T09:51:12.658144Z","resolver_source":"doi","status":"verified_exact"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-04T06:34:03.388597+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-04T06:34:03.388597+00:00","source":"crossref"},{"observed_at":"2026-08-04T06:33:57.428241+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":"10.1103/physrevlett.69.1006","metadata_source":"doi_reference","pith_arxiv_id":null,"snapshot_observed_at":"2026-06-29T11:13:20.361518Z","title":"Rotating charged black hole solution in heterotic string theory.Phys","venue":null,"work_id":"dfc7c60c-0cfd-4d1e-af68-f3f889fa97cd","year":1992},"citing_paper":{"arxiv_id":"2510.04703","last_updated":"2026-04-06T04:55:34Z","snapshot_observed_at":"2026-07-06T22:31:49.574184Z","submitted_at":"2025-10-06T11:16:49Z","title":"Testing black hole metrics with binary black hole inspirals","version":2},"reference_index":53,"source":"pdf_text","source_observed_at":"2026-05-18T09:47:38.064359Z"},"links":{"citing_paper":"/paper/2510.04703"},"observation_digest":"sha256:5aa0f82d62e547e5c73c9ba5ade3f1e3f6c84d4154934a74c60a876c2afae5b2","observation_id":"6e4d8f41-b421-4c03-8281-78c9fce2210a","resolution":{"observed_at":"2026-05-18T09:51:12.678443Z","resolver_source":"doi","status":"verified_exact"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-04T06:34:03.388597+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-04T06:34:03.388597+00:00","source":"crossref"},{"observed_at":"2026-08-04T06:33:57.428241+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":"10.1023/a:1002080003862","metadata_source":"doi_reference","pith_arxiv_id":null,"snapshot_observed_at":"2026-06-05T21:23:00.469572Z","title":"Yazadjiev, Gen","venue":null,"work_id":"f1b87acc-738e-4a90-9c4e-42d97da0256e","year":2000},"citing_paper":{"arxiv_id":"2510.04703","last_updated":"2026-04-06T04:55:34Z","snapshot_observed_at":"2026-07-06T22:31:49.574184Z","submitted_at":"2025-10-06T11:16:49Z","title":"Testing black hole metrics with binary black hole inspirals","version":2},"reference_index":54,"source":"pdf_text","source_observed_at":"2026-05-18T09:47:38.064359Z"},"links":{"citing_paper":"/paper/2510.04703"},"observation_digest":"sha256:aa4c8db19030995cfceb20e8ece89358bf85e38db272adfe2302faede6ffe797","observation_id":"2d08186b-6eb7-4b29-9542-3d790313aab7","resolution":{"observed_at":"2026-05-18T09:51:12.671491Z","resolver_source":"doi","status":"verified_exact"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-04T06:34:03.388597+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-04T06:34:03.388597+00:00","source":"crossref"},{"observed_at":"2026-08-04T06:33:57.428241+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":"10.1088/1475-7516/2021/07/002","metadata_source":"doi_reference","pith_arxiv_id":null,"snapshot_observed_at":"2026-06-05T21:23:00.469572Z","title":"Tripathi, B","venue":null,"work_id":"75ee631b-c706-45ef-a424-bbfe9b41d089","year":2021},"citing_paper":{"arxiv_id":"2510.04703","last_updated":"2026-04-06T04:55:34Z","snapshot_observed_at":"2026-07-06T22:31:49.574184Z","submitted_at":"2025-10-06T11:16:49Z","title":"Testing black hole metrics with binary black hole inspirals","version":2},"reference_index":55,"source":"pdf_text","source_observed_at":"2026-05-18T09:47:38.064359Z"},"links":{"citing_paper":"/paper/2510.04703"},"observation_digest":"sha256:d020634840e35cabb51667f641181d31c10bd425068ef019fde9366c78cbaa20","observation_id":"11c7ee55-07d4-46a9-8ac8-8a4f4b42911a","resolution":{"observed_at":"2026-05-18T09:51:12.572664Z","resolver_source":"doi","status":"verified_exact"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-04T06:34:03.388597+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-04T06:34:03.388597+00:00","source":"crossref"},{"observed_at":"2026-08-04T06:33:57.428241+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":"2021.168619","doi":"10.1016/j.aop.2021.168619","metadata_source":"arxiv_reference","pith_arxiv_id":null,"snapshot_observed_at":"2026-07-11T11:50:26.030339Z","title":null,"venue":null,"work_id":"95819eef-f49c-480e-ae00-338e35b51d5d","year":2021},"citing_paper":{"arxiv_id":"2510.04703","last_updated":"2026-04-06T04:55:34Z","snapshot_observed_at":"2026-07-06T22:31:49.574184Z","submitted_at":"2025-10-06T11:16:49Z","title":"Testing black hole metrics with binary black hole inspirals","version":2},"reference_index":56,"source":"pdf_text","source_observed_at":"2026-05-18T09:47:38.064359Z"},"links":{"citing_paper":"/paper/2510.04703"},"observation_digest":"sha256:8b5ef714e828ea7a667a30f04a4a71478c8dc024dc2c6cedda9bc16d5aa31402","observation_id":"55c610d6-6de7-4bf2-92d9-b4e62f725001","resolution":{"observed_at":"2026-05-18T09:51:12.596679Z","resolver_source":"arxiv_id","status":"verified_exact"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-04T06:34:03.388597+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-04T06:34:03.388597+00:00","source":"crossref"},{"observed_at":"2026-08-04T06:33:57.428241+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":{"arxiv_id":"hep-th/9310150","last_updated":"1993-10-27T17:16:25Z","snapshot_observed_at":"2026-07-07T05:04:09.561864Z","submitted_at":"1993-10-19T08:16:15Z","title":"On Quantum Deformation of the Schwarzschild Solution","version":4},"cited_work":{"arxiv_id":"hep-th/9310150","doi":null,"metadata_source":"pith","pith_arxiv_id":"hep-th/9310150","snapshot_observed_at":"2026-06-05T21:23:00.469572Z","title":"On Quantum Deformation of the Schwarzschild Solution","venue":"hep-th","work_id":"b87b812b-60a9-4478-b83e-926fe460cfe6","year":1993},"citing_paper":{"arxiv_id":"2510.04703","last_updated":"2026-04-06T04:55:34Z","snapshot_observed_at":"2026-07-06T22:31:49.574184Z","submitted_at":"2025-10-06T11:16:49Z","title":"Testing black hole metrics with binary black hole inspirals","version":2},"reference_index":57,"source":"pdf_text","source_observed_at":"2026-07-11T11:50:26.030339Z"},"links":{"cited_paper":"/paper/hep-th/9310150","citing_paper":"/paper/2510.04703"},"observation_digest":"sha256:d587ac51c3faa0fce6aa2823dc15d9bbf2ff82cbedb31db62ef150499d354cc8","observation_id":"e37ffd97-9658-4458-8e97-31a3f04cf657","resolution":{"observed_at":"2026-05-18T09:51:12.398483Z","resolver_source":"local_arxiv","status":"malformed_identifier"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-04T06:34:03.388597+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-04T06:34:03.388597+00:00","source":"crossref"},{"observed_at":"2026-08-04T06:33:57.428241+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":"10.1103/physrevd.102.064058","metadata_source":"doi_reference","pith_arxiv_id":null,"snapshot_observed_at":"2026-06-05T21:23:00.469572Z","title":"Kocherlakota and L","venue":null,"work_id":"4153b9c2-4f6e-40b0-af87-236b33888bcb","year":2020},"citing_paper":{"arxiv_id":"2510.04703","last_updated":"2026-04-06T04:55:34Z","snapshot_observed_at":"2026-07-06T22:31:49.574184Z","submitted_at":"2025-10-06T11:16:49Z","title":"Testing black hole metrics with binary black hole inspirals","version":2},"reference_index":58,"source":"pdf_text","source_observed_at":"2026-05-18T09:47:38.064359Z"},"links":{"citing_paper":"/paper/2510.04703"},"observation_digest":"sha256:353e0df0c733bc8e395f5495ae326ee1dc874a27ea68ce3ed7ba82b3582b5fb8","observation_id":"9b222eef-022c-42c6-bb63-a7ce139dd71f","resolution":{"observed_at":"2026-05-18T09:51:12.629795Z","resolver_source":"doi","status":"verified_exact"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-04T06:34:03.388597+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-04T06:34:03.388597+00:00","source":"crossref"},{"observed_at":"2026-08-04T06:33:57.428241+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":"10.1140/epjc/s10052-021-09635-2","metadata_source":"doi_reference","pith_arxiv_id":null,"snapshot_observed_at":"2026-06-05T21:23:00.469572Z","title":"Xu and M","venue":null,"work_id":"976c184e-aecd-4d4a-ac7c-7c6f254872dc","year":2021},"citing_paper":{"arxiv_id":"2510.04703","last_updated":"2026-04-06T04:55:34Z","snapshot_observed_at":"2026-07-06T22:31:49.574184Z","submitted_at":"2025-10-06T11:16:49Z","title":"Testing black hole metrics with binary black hole inspirals","version":2},"reference_index":59,"source":"pdf_text","source_observed_at":"2026-05-18T09:47:38.064359Z"},"links":{"citing_paper":"/paper/2510.04703"},"observation_digest":"sha256:25bdece3815cb6d0fdac2387671eaaef09dfaa6009ef08428368b034aebc94a8","observation_id":"a2bf4bc6-d76f-4cd7-bc47-e9d0d7bd482c","resolution":{"observed_at":"2026-05-18T09:51:12.443947Z","resolver_source":"doi","status":"verified_exact"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-04T06:34:03.388597+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-04T06:34:03.388597+00:00","source":"crossref"},{"observed_at":"2026-08-04T06:33:57.428241+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":"10.3390/universe8040210","metadata_source":"doi_reference","pith_arxiv_id":null,"snapshot_observed_at":"2026-06-05T21:23:00.469572Z","title":"Jusufi, M","venue":null,"work_id":"97d50da6-03c0-455d-849f-fe3d329d2682","year":2022},"citing_paper":{"arxiv_id":"2510.04703","last_updated":"2026-04-06T04:55:34Z","snapshot_observed_at":"2026-07-06T22:31:49.574184Z","submitted_at":"2025-10-06T11:16:49Z","title":"Testing black hole metrics with binary black hole inspirals","version":2},"reference_index":60,"source":"pdf_text","source_observed_at":"2026-05-18T09:47:38.064359Z"},"links":{"citing_paper":"/paper/2510.04703"},"observation_digest":"sha256:8352ad04cb451e1a7c15534979dd0baa44e40318e1847d6cde8cabab27877438","observation_id":"83bbf4d6-ed47-46d8-9ac8-dc22e435d6a2","resolution":{"observed_at":"2026-05-18T09:51:12.506036Z","resolver_source":"doi","status":"verified_exact"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-04T06:34:03.388597+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-04T06:34:03.388597+00:00","source":"crossref"},{"observed_at":"2026-08-04T06:33:57.428241+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":{"arxiv_id":"1408.0306","last_updated":"2014-12-10T18:59:50Z","snapshot_observed_at":"2026-07-06T02:11:23.670680Z","submitted_at":"2014-08-01T21:08:40Z","title":"Regular black holes with a nonlinear electrodynamics source","version":2},"cited_work":{"arxiv_id":"1408.0306","doi":null,"metadata_source":"pith","pith_arxiv_id":"1408.0306","snapshot_observed_at":"2026-07-10T23:07:46.550101Z","title":"Regular black holes with a nonlinear electrodynamics source","venue":"gr-qc","work_id":"7cc8675b-0549-4b59-b45b-c45d4878eeae","year":2014},"citing_paper":{"arxiv_id":"2510.04703","last_updated":"2026-04-06T04:55:34Z","snapshot_observed_at":"2026-07-06T22:31:49.574184Z","submitted_at":"2025-10-06T11:16:49Z","title":"Testing black hole metrics with binary black hole inspirals","version":2},"reference_index":61,"source":"pdf_text","source_observed_at":"2026-07-11T11:50:26.030339Z"},"links":{"cited_paper":"/paper/1408.0306","citing_paper":"/paper/2510.04703"},"observation_digest":"sha256:12c0febda22cf7d2a46cf734a1b9fa474b51437242ac7fd13b5da941fe47f005","observation_id":"d96a8030-980d-4aa4-82a1-ce256a1834a2","resolution":{"observed_at":"2026-05-18T09:51:12.458640Z","resolver_source":"local_arxiv","status":"verified_exact"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-04T06:34:03.388597+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-04T06:34:03.388597+00:00","source":"crossref"},{"observed_at":"2026-08-04T06:33:57.428241+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":{"arxiv_id":"1408.3334","last_updated":"2015-10-30T13:47:58Z","snapshot_observed_at":"2026-07-06T03:51:44.523089Z","submitted_at":"2014-08-14T16:37:59Z","title":"On a regular charged black hole with a nonlinear electric source","version":4},"cited_work":{"arxiv_id":"1408.3334","doi":null,"metadata_source":"pith","pith_arxiv_id":"1408.3334","snapshot_observed_at":"2026-07-10T23:07:46.169109Z","title":"On a regular charged black hole with a nonlinear electric source","venue":"gr-qc","work_id":"15ef997d-83f6-4c3c-8f09-29132b807cce","year":2014},"citing_paper":{"arxiv_id":"2510.04703","last_updated":"2026-04-06T04:55:34Z","snapshot_observed_at":"2026-07-06T22:31:49.574184Z","submitted_at":"2025-10-06T11:16:49Z","title":"Testing black hole metrics with binary black hole inspirals","version":2},"reference_index":62,"source":"pdf_text","source_observed_at":"2026-07-11T11:50:26.030339Z"},"links":{"cited_paper":"/paper/1408.3334","citing_paper":"/paper/2510.04703"},"observation_digest":"sha256:1a983c743e4bc599bfeddf77fbb1be30916e8b6efec516cc791f7fed33fa4816","observation_id":"ea58cdaf-6f54-4a1e-90fe-4c53cd794a51","resolution":{"observed_at":"2026-05-18T09:51:12.747497Z","resolver_source":"local_arxiv","status":"verified_exact"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-04T06:34:03.388597+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-04T06:34:03.388597+00:00","source":"crossref"},{"observed_at":"2026-08-04T06:33:57.428241+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":{"arxiv_id":"1408.5668","last_updated":"2015-10-17T03:37:58Z","snapshot_observed_at":"2026-07-06T03:52:31.542932Z","submitted_at":"2014-08-25T06:35:46Z","title":"A nonsingular rotating black hole","version":4},"cited_work":{"arxiv_id":"1408.5668","doi":"10.1140/epjc/s10052-015-3740-y","metadata_source":"pith","pith_arxiv_id":"1408.5668","snapshot_observed_at":"2026-07-11T11:50:26.030339Z","title":"A nonsingular rotating black hole","venue":"gr-qc","work_id":"64cd1fc5-6a9a-4cd8-8099-8cb50eeacefd","year":2014},"citing_paper":{"arxiv_id":"2510.04703","last_updated":"2026-04-06T04:55:34Z","snapshot_observed_at":"2026-07-06T22:31:49.574184Z","submitted_at":"2025-10-06T11:16:49Z","title":"Testing black hole metrics with binary black hole inspirals","version":2},"reference_index":63,"source":"pdf_text","source_observed_at":"2026-07-11T11:50:26.030339Z"},"links":{"cited_paper":"/paper/1408.5668","citing_paper":"/paper/2510.04703"},"observation_digest":"sha256:22ab1db897cd875dbee6637de4ee87395ea386c42fb87ded9fcbe06f988e3dfd","observation_id":"260695a7-5375-4741-a1d6-d370a994b0a7","resolution":{"observed_at":"2026-05-18T09:51:12.481947Z","resolver_source":"local_arxiv","status":"verified_exact"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-04T06:34:03.388597+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-04T06:34:03.388597+00:00","source":"crossref"},{"observed_at":"2026-08-04T06:33:57.428241+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":{"arxiv_id":"1512.09164","last_updated":"2015-12-30T22:04:41Z","snapshot_observed_at":"2026-07-06T04:41:29.846747Z","submitted_at":"2015-12-30T22:04:41Z","title":"The Shadow of Generalized Kerr Black Holes with Exotic Matter","version":1},"cited_work":{"arxiv_id":"1512.09164","doi":"10.6122/cjp.20150810","metadata_source":"pith","pith_arxiv_id":"1512.09164","snapshot_observed_at":"2026-07-11T11:50:26.030339Z","title":"The Shadow of Generalized Kerr Black Holes with Exotic Matter","venue":"gr-qc","work_id":"7f95a5b0-fd13-4f14-8082-5ba2a6617a9e","year":2015},"citing_paper":{"arxiv_id":"2510.04703","last_updated":"2026-04-06T04:55:34Z","snapshot_observed_at":"2026-07-06T22:31:49.574184Z","submitted_at":"2025-10-06T11:16:49Z","title":"Testing black hole metrics with binary black hole inspirals","version":2},"reference_index":64,"source":"pdf_text","source_observed_at":"2026-07-11T11:50:26.030339Z"},"links":{"cited_paper":"/paper/1512.09164","citing_paper":"/paper/2510.04703"},"observation_digest":"sha256:7a185d3c575824cbedf2a2505777051dc71ee24006e792024aacfbfc1d831fc1","observation_id":"6b57d42e-5e3d-48fc-ba39-020d8ec8df05","resolution":{"observed_at":"2026-05-18T09:51:12.536511Z","resolver_source":"local_arxiv","status":"verified_exact"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-04T06:34:03.388597+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-04T06:34:03.388597+00:00","source":"crossref"},{"observed_at":"2026-08-04T06:33:57.428241+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":"10.1103/physrev.47.877","metadata_source":"doi_reference","pith_arxiv_id":null,"snapshot_observed_at":"2026-06-05T21:23:00.469572Z","title":"Hoffmann, Phys","venue":null,"work_id":"4ede7712-874b-4ca4-85d4-2dc3163dbba5","year":1935},"citing_paper":{"arxiv_id":"2510.04703","last_updated":"2026-04-06T04:55:34Z","snapshot_observed_at":"2026-07-06T22:31:49.574184Z","submitted_at":"2025-10-06T11:16:49Z","title":"Testing black hole metrics with binary black hole inspirals","version":2},"reference_index":65,"source":"pdf_text","source_observed_at":"2026-05-18T09:47:38.064359Z"},"links":{"citing_paper":"/paper/2510.04703"},"observation_digest":"sha256:7c1c0914dde0c33285f1c562355d6ca08dbc715b1e531e690b3f5ed5e4b7277b","observation_id":"3925d413-c947-4b9f-908b-af2a69774646","resolution":{"observed_at":"2026-05-18T09:51:12.712385Z","resolver_source":"doi","status":"verified_exact"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-04T06:34:03.388597+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-04T06:34:03.388597+00:00","source":"crossref"},{"observed_at":"2026-08-04T06:33:57.428241+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":{"arxiv_id":"hep-th/9604177","last_updated":"1996-04-28T21:42:31Z","snapshot_observed_at":"2026-07-07T05:10:37.867666Z","submitted_at":"1996-04-28T21:42:31Z","title":"Dyson Pairs and Zero-Mass Black Holes","version":1},"cited_work":{"arxiv_id":"hep-th/9604177","doi":null,"metadata_source":"pith","pith_arxiv_id":"hep-th/9604177","snapshot_observed_at":"2026-06-05T21:23:00.469572Z","title":"Dyson Pairs and Zero-Mass Black Holes","venue":"hep-th","work_id":"e7821ab1-48d7-4852-98c0-34571812d40b","year":1996},"citing_paper":{"arxiv_id":"2510.04703","last_updated":"2026-04-06T04:55:34Z","snapshot_observed_at":"2026-07-06T22:31:49.574184Z","submitted_at":"2025-10-06T11:16:49Z","title":"Testing black hole metrics with binary black hole inspirals","version":2},"reference_index":67,"source":"pdf_text","source_observed_at":"2026-07-11T11:50:26.030339Z"},"links":{"cited_paper":"/paper/hep-th/9604177","citing_paper":"/paper/2510.04703"},"observation_digest":"sha256:a0388b926a2d658770ac9e47fc9963e084f85ba23e217e30289bcfa1318a8aba","observation_id":"796804a7-1c09-4581-ab96-c7ae33f8da97","resolution":{"observed_at":"2026-05-18T09:51:12.652710Z","resolver_source":"local_arxiv","status":"malformed_identifier"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-04T06:34:03.388597+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-04T06:34:03.388597+00:00","source":"crossref"},{"observed_at":"2026-08-04T06:33:57.428241+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":"10.1103/physrevd.62.105007","metadata_source":"doi_reference","pith_arxiv_id":null,"snapshot_observed_at":"2026-06-05T21:23:00.469572Z","title":"Chruscinski, Phys","venue":null,"work_id":"e4b10b51-adff-45e9-bda0-e59b403e6938","year":2000},"citing_paper":{"arxiv_id":"2510.04703","last_updated":"2026-04-06T04:55:34Z","snapshot_observed_at":"2026-07-06T22:31:49.574184Z","submitted_at":"2025-10-06T11:16:49Z","title":"Testing black hole metrics with binary black hole inspirals","version":2},"reference_index":68,"source":"pdf_text","source_observed_at":"2026-05-18T09:47:38.064359Z"},"links":{"citing_paper":"/paper/2510.04703"},"observation_digest":"sha256:7c65b764e2452560345822212cada6eaf80416afcb4ff5ca8745083bdcf0312a","observation_id":"76074a04-d0c6-480b-b021-4c3b4ac3c845","resolution":{"observed_at":"2026-05-18T09:51:12.674732Z","resolver_source":"doi","status":"verified_exact"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-04T06:34:03.388597+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-04T06:34:03.388597+00:00","source":"crossref"},{"observed_at":"2026-08-04T06:33:57.428241+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":{"arxiv_id":"hep-th/9709190","last_updated":"1997-09-26T10:19:12Z","snapshot_observed_at":"2026-07-07T05:14:47.090495Z","submitted_at":"1997-09-26T10:19:12Z","title":"Symmetry Properties of Self-Dual Fields","version":1},"cited_work":{"arxiv_id":"hep-th/9709190","doi":null,"metadata_source":"pith","pith_arxiv_id":"hep-th/9709190","snapshot_observed_at":"2026-06-05T21:23:00.469572Z","title":"Symmetry Properties of Self-Dual Fields","venue":"hep-th","work_id":"20c19bbb-26b4-421b-976a-84481b8dc2b5","year":1997},"citing_paper":{"arxiv_id":"2510.04703","last_updated":"2026-04-06T04:55:34Z","snapshot_observed_at":"2026-07-06T22:31:49.574184Z","submitted_at":"2025-10-06T11:16:49Z","title":"Testing black hole metrics with binary black hole inspirals","version":2},"reference_index":69,"source":"pdf_text","source_observed_at":"2026-05-18T09:47:38.064359Z"},"links":{"cited_paper":"/paper/hep-th/9709190","citing_paper":"/paper/2510.04703"},"observation_digest":"sha256:8b2aeefab5b03600b4218b404d1090274e674e36866482f432f396d52c73f58a","observation_id":"c22fc87b-4655-4836-87a1-5260babed9a7","resolution":{"observed_at":"2026-05-18T09:51:13.689243Z","resolver_source":"local_arxiv","status":"verified_exact"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-04T06:34:03.388597+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-04T06:34:03.388597+00:00","source":"crossref"},{"observed_at":"2026-08-04T06:33:57.428241+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":{"arxiv_id":"gr-qc/0612063","last_updated":"2006-12-11T12:44:29Z","snapshot_observed_at":"2026-07-07T03:23:24.597961Z","submitted_at":"2006-12-11T12:44:29Z","title":"The Newman-Janis Algorithm, Rotating Solutions and Einstein-Born-Infeld Black Holes","version":1},"cited_work":{"arxiv_id":"gr-qc/0612063","doi":null,"metadata_source":"pith","pith_arxiv_id":"gr-qc/0612063","snapshot_observed_at":"2026-06-05T21:23:00.469572Z","title":"The Newman-Janis Algorithm, Rotating Solutions and Einstein-Born-Infeld Black Holes","venue":"gr-qc","work_id":"8137028f-c347-4045-867e-a4137b18bab8","year":2006},"citing_paper":{"arxiv_id":"2510.04703","last_updated":"2026-04-06T04:55:34Z","snapshot_observed_at":"2026-07-06T22:31:49.574184Z","submitted_at":"2025-10-06T11:16:49Z","title":"Testing black hole metrics with binary black hole inspirals","version":2},"reference_index":70,"source":"pdf_text","source_observed_at":"2026-07-11T11:50:26.030339Z"},"links":{"cited_paper":"/paper/gr-qc/0612063","citing_paper":"/paper/2510.04703"},"observation_digest":"sha256:d02eb7a407d367ccb1384c60d14d73c31ce8d4811e7dfffa7dd8ce93f02abfce","observation_id":"5c0eb9e6-7c7a-48e8-a07c-238088c23c64","resolution":{"observed_at":"2026-05-18T09:51:12.718539Z","resolver_source":"local_arxiv","status":"verified_exact"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-04T06:34:03.388597+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-04T06:34:03.388597+00:00","source":"crossref"},{"observed_at":"2026-08-04T06:33:57.428241+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":{"arxiv_id":"1506.03690","last_updated":"2015-06-17T11:29:45Z","snapshot_observed_at":"2026-07-06T04:20:37.335944Z","submitted_at":"2015-06-11T14:36:49Z","title":"Horizon structure of rotating Einstein-Born-Infeld black holes and shadow","version":2},"cited_work":{"arxiv_id":"1506.03690","doi":"10.1140/epjc/s10052-016-4122-9","metadata_source":"pith","pith_arxiv_id":"1506.03690","snapshot_observed_at":"2026-07-11T11:50:26.030339Z","title":"Horizon structure of rotating Einstein-Born-Infeld black holes and shadow","venue":"gr-qc","work_id":"f333bc48-2466-4a32-bb48-e4c643cb2ecb","year":2015},"citing_paper":{"arxiv_id":"2510.04703","last_updated":"2026-04-06T04:55:34Z","snapshot_observed_at":"2026-07-06T22:31:49.574184Z","submitted_at":"2025-10-06T11:16:49Z","title":"Testing black hole metrics with binary black hole inspirals","version":2},"reference_index":71,"source":"pdf_text","source_observed_at":"2026-07-11T11:50:26.030339Z"},"links":{"cited_paper":"/paper/1506.03690","citing_paper":"/paper/2510.04703"},"observation_digest":"sha256:300e90b48a633ad8f2fe4ea87db6de805f8f4c9d947c60eb47518ffa6a787311","observation_id":"e1d527d6-3a55-44a4-8a9d-f879db970bc6","resolution":{"observed_at":"2026-05-18T09:51:12.557587Z","resolver_source":"local_arxiv","status":"verified_exact"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-04T06:34:03.388597+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-04T06:34:03.388597+00:00","source":"crossref"},{"observed_at":"2026-08-04T06:33:57.428241+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":{"arxiv_id":"hep-th/9911174","last_updated":"1999-11-22T19:47:27Z","snapshot_observed_at":"2026-07-07T05:21:30.904101Z","submitted_at":"1999-11-22T19:47:27Z","title":"New Regular Black Hole Solution from Nonlinear Electrodynamics","version":1},"cited_work":{"arxiv_id":"hep-th/9911174","doi":null,"metadata_source":"pith","pith_arxiv_id":"hep-th/9911174","snapshot_observed_at":"2026-07-10T11:07:02.063177Z","title":"New Regular Black Hole Solution from Nonlinear Electrodynamics","venue":"hep-th","work_id":"b023c21d-84c5-4e1a-b7cc-7364914f9baf","year":1999},"citing_paper":{"arxiv_id":"2510.04703","last_updated":"2026-04-06T04:55:34Z","snapshot_observed_at":"2026-07-06T22:31:49.574184Z","submitted_at":"2025-10-06T11:16:49Z","title":"Testing black hole metrics with binary black hole inspirals","version":2},"reference_index":72,"source":"pdf_text","source_observed_at":"2026-07-11T11:50:26.030339Z"},"links":{"cited_paper":"/paper/hep-th/9911174","citing_paper":"/paper/2510.04703"},"observation_digest":"sha256:42274e396024f19afb86cc32aed9a05d46b9e435f2104690762887b02b2788ee","observation_id":"e44ac147-dc15-404f-a31c-2a504cac9cdd","resolution":{"observed_at":"2026-05-18T09:51:12.665384Z","resolver_source":"local_arxiv","status":"verified_exact"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-04T06:34:03.388597+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-04T06:34:03.388597+00:00","source":"crossref"},{"observed_at":"2026-08-04T06:33:57.428241+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":"10.7935/903s-gx73","metadata_source":"doi_reference","pith_arxiv_id":null,"snapshot_observed_at":"2026-06-05T21:23:00.469572Z","title":"Tests of general relativity with binary black holes from the second ligo–virgo gravitational- wave transient catalog - full posterior sample data release","venue":null,"work_id":"217b189b-38b8-4362-b648-6936e9ac2d77","year":2021},"citing_paper":{"arxiv_id":"2510.04703","last_updated":"2026-04-06T04:55:34Z","snapshot_observed_at":"2026-07-06T22:31:49.574184Z","submitted_at":"2025-10-06T11:16:49Z","title":"Testing black hole metrics with binary black hole inspirals","version":2},"reference_index":73,"source":"pdf_text","source_observed_at":"2026-05-18T09:47:38.064359Z"},"links":{"citing_paper":"/paper/2510.04703"},"observation_digest":"sha256:2deee8b30c1441a2146fa6f8aa222fd6ab10745c0d399aa4c64ba7199b0650b3","observation_id":"8f390236-0321-4ef6-afe6-69cdc2ceb846","resolution":{"observed_at":"2026-05-18T09:51:12.383593Z","resolver_source":"doi","status":"verified_exact"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-04T06:34:03.388597+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-04T06:34:03.388597+00:00","source":"crossref"},{"observed_at":"2026-08-04T06:33:57.428241+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":{"arxiv_id":"1811.12907","last_updated":"2019-10-04T08:10:25Z","snapshot_observed_at":"2026-07-06T02:11:23.670680Z","submitted_at":"2018-11-30T17:34:09Z","title":"GWTC-1: A Gravitational-Wave Transient Catalog of Compact Binary Mergers Observed by LIGO and Virgo during the First and Second Observing Runs","version":3},"cited_work":{"arxiv_id":"1811.12907","doi":null,"metadata_source":"pith","pith_arxiv_id":"1811.12907","snapshot_observed_at":"2026-07-09T20:06:29.259645Z","title":"GWTC-1: A Gravitational-Wave Transient Catalog of Compact Binary Mergers Observed by LIGO and Virgo during the First and Second Observing Runs","venue":"astro-ph.HE","work_id":"ed2ab6af-3b84-426b-a8d5-c1f2cb6b0af7","year":2018},"citing_paper":{"arxiv_id":"2510.04703","last_updated":"2026-04-06T04:55:34Z","snapshot_observed_at":"2026-07-06T22:31:49.574184Z","submitted_at":"2025-10-06T11:16:49Z","title":"Testing black hole metrics with binary black hole inspirals","version":2},"reference_index":74,"source":"pdf_text","source_observed_at":"2026-07-11T11:50:26.030339Z"},"links":{"cited_paper":"/paper/1811.12907","citing_paper":"/paper/2510.04703"},"observation_digest":"sha256:10967acdaf0bfcc0a3048cab5a204e6f561582802598215fe4fce6ecf3e1a558","observation_id":"ee558c49-9d42-462c-b59b-739cc6e5f275","resolution":{"observed_at":"2026-05-18T09:51:12.502163Z","resolver_source":"local_arxiv","status":"verified_exact"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-04T06:34:03.388597+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-04T06:34:03.388597+00:00","source":"crossref"},{"observed_at":"2026-08-04T06:33:57.428241+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":{"arxiv_id":"1711.05578","last_updated":"2017-11-15T14:07:43Z","snapshot_observed_at":"2026-07-06T06:09:37.457486Z","submitted_at":"2017-11-15T14:07:43Z","title":"GW170608: Observation of a 19-solar-mass Binary Black Hole Coalescence","version":1},"cited_work":{"arxiv_id":"1711.05578","doi":null,"metadata_source":"pith","pith_arxiv_id":"1711.05578","snapshot_observed_at":"2026-06-29T10:23:18.056230Z","title":"GW170608: Observation of a 19-solar-mass Binary Black Hole Coalescence","venue":"astro-ph.HE","work_id":"1e7d169f-3550-42bd-9958-a49acc1fd3d7","year":2017},"citing_paper":{"arxiv_id":"2510.04703","last_updated":"2026-04-06T04:55:34Z","snapshot_observed_at":"2026-07-06T22:31:49.574184Z","submitted_at":"2025-10-06T11:16:49Z","title":"Testing black hole metrics with binary black hole inspirals","version":2},"reference_index":75,"source":"pdf_text","source_observed_at":"2026-07-11T11:50:26.030339Z"},"links":{"cited_paper":"/paper/1711.05578","citing_paper":"/paper/2510.04703"},"observation_digest":"sha256:d9ccab9ed57bb071d8d7354e6923256b76867b27d3d51b69cab7f09a4636ab47","observation_id":"51d7598e-1c4f-4c87-b267-adbc16336f7c","resolution":{"observed_at":"2026-05-18T09:51:12.569191Z","resolver_source":"local_arxiv","status":"verified_exact"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-04T06:34:03.388597+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-04T06:34:03.388597+00:00","source":"crossref"},{"observed_at":"2026-08-04T06:33:57.428241+00:00","source":"retraction_watch"}],"state":"measured"}}],"paper":{"arxiv_id":"2510.04703","last_updated":"2026-04-06T04:55:34Z","latest_version":2,"primary_category":"gr-qc","snapshot_observed_at":"2026-07-06T22:31:49.574184Z","submitted_at":"2025-10-06T11:16:49Z","title":"Testing black hole metrics with binary black hole inspirals"},"reference_resolution":{"displayed":74,"state_counts":{"malformed_identifier":7,"metadata_mismatch":5,"parse_uncertain":0,"unresolved":1,"verified_exact":60,"verified_fuzzy":1},"total_outbound_references":74},"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":"2026-08-04T06:34:03.388597+00:00","source":"crossref"},{"observed_at":"2026-08-04T06:33:57.428241+00:00","source":"retraction_watch"}],"thesis":"As of 4 August 2026, this Paper Citation Record lists 74 of 74 outbound references and 2 inbound Pith citation observations for arXiv:2510.04703."}