{"as_of":"2026-08-23T17:50:00Z","caps":{"database_statements":6,"inbound":100,"outbound":100},"context_digest":"sha256:947d2db9e94a36e2cb9da89368d6ad55f019fc0c1297e484b1a1b57b8c432bb2","coverage":[{"denominator":93,"lane":"reference_resolution","note":"Typed states for the displayed outbound observations.","records_observed":93,"source":"paper_references, paper_reference_links","source_observed_at":"2026-07-08T21:06:26.923131Z","state":"measured"},{"denominator":93,"lane":"standing_notices","note":"One-hop event checks from named stored sources.","records_observed":93,"source":"scholarly_work_events, retraction_status_cache","source_observed_at":"2026-08-23T06:30:58.430688+00:00","state":"measured"},{"denominator":0,"lane":"inbound_itemization","note":"Pith citing papers itemized under the disclosed page cap.","records_observed":0,"source":"paper_references, paper_reference_links","source_observed_at":null,"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":[],"links":{"evidence":"/evidence","html":"/paper/2607.05909/citation-record","integrity":"/paper/2607.05909/integrity","json":"/paper/2607.05909/citation-record.json","paper":"/paper/2607.05909"},"outbound":[{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":"raw_reference","pith_arxiv_id":null,"snapshot_observed_at":"2026-07-08T21:15:39.453973Z","title":null,"venue":null,"work_id":"be6bff3f-7118-40e6-8d84-8b4142ed2846","year":2016},"citing_paper":{"arxiv_id":"2607.05909","last_updated":"2026-07-07T07:04:03Z","snapshot_observed_at":"2026-08-14T10:29:50.174311Z","submitted_at":"2026-07-07T07:04:03Z","title":"Probing near-zone magnetic fields with extreme mass-ratio inspirals","version":1},"reference_index":1,"source":"pdf_text","source_observed_at":"2026-07-08T21:06:26.923131Z"},"links":{"citing_paper":"/paper/2607.05909"},"observation_digest":"sha256:5f9c1901466073fde3d06fdae6240753f7c2eb0bdfff3b47c20ef1b425e1504d","observation_id":"1392425b-b3e7-4ead-9ec1-9d59d0861fe2","resolution":{"observed_at":"2026-07-08T21:15:39.455605Z","resolver_source":"raw_fallback","status":"unresolved"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-23T06:30:58.430688+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-23T06:30:58.430688+00:00","source":"crossref"},{"observed_at":"2026-08-23T06:30:53.778098+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":"2607.05909","last_updated":"2026-07-07T07:04:03Z","snapshot_observed_at":"2026-08-14T10:29:50.174311Z","submitted_at":"2026-07-07T07:04:03Z","title":"Probing near-zone magnetic fields with extreme mass-ratio inspirals","version":1},"reference_index":2,"source":"pdf_text","source_observed_at":"2026-07-08T21:06:26.923131Z"},"links":{"cited_paper":"/paper/1710.05832","citing_paper":"/paper/2607.05909"},"observation_digest":"sha256:f869f2be42d72a1513ebe74f4b1b17dc6590bf2b5db321e50a8ebaf7d28bc4aa","observation_id":"09176a0f-5d90-4663-ad85-4a7b01691fd3","resolution":{"observed_at":"2026-07-08T21:15:39.134466Z","resolver_source":"local_arxiv","status":"verified_exact"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-23T06:30:58.430688+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-23T06:30:58.430688+00:00","source":"crossref"},{"observed_at":"2026-08-23T06:30:53.778098+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":{"arxiv_id":"1702.00786","last_updated":"2017-02-23T05:33:01Z","snapshot_observed_at":"2026-08-20T08:25:18.189806Z","submitted_at":"2017-02-02T07:06:53Z","title":"Laser Interferometer Space Antenna","version":3},"cited_work":{"arxiv_id":"1702.00786","doi":"10.48550/arxiv.1702.00786","metadata_source":"pith","pith_arxiv_id":"1702.00786","snapshot_observed_at":"2026-08-05T02:28:24.338817Z","title":"Laser Interferometer Space Antenna","venue":"astro-ph.IM","work_id":"04a25305-b4d4-47f9-9613-efea8cc0292b","year":2017},"citing_paper":{"arxiv_id":"2607.05909","last_updated":"2026-07-07T07:04:03Z","snapshot_observed_at":"2026-08-14T10:29:50.174311Z","submitted_at":"2026-07-07T07:04:03Z","title":"Probing near-zone magnetic fields with extreme mass-ratio inspirals","version":1},"reference_index":3,"source":"pdf_text","source_observed_at":"2026-07-08T21:06:26.923131Z"},"links":{"cited_paper":"/paper/1702.00786","citing_paper":"/paper/2607.05909"},"observation_digest":"sha256:128296032fd6ee20f309726f4a8faef8d19bce715c624310a333de7b0ac3e861","observation_id":"d24cb512-09c0-40d7-a14f-2704cb49a9ca","resolution":{"observed_at":"2026-07-08T21:15:39.186266Z","resolver_source":"local_arxiv","status":"metadata_mismatch"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-23T06:30:58.430688+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-23T06:30:58.430688+00:00","source":"crossref"},{"observed_at":"2026-08-08T05:38:14.000717+00:00","source":"crossref_status_cache"},{"observed_at":"2026-08-08T05:38:14.000717+00:00","source":"openalex_status_cache"},{"observed_at":"2026-08-23T06:30:53.778098+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":"2026-07-08T21:15:39.458634Z","title":"Meiet al., Progress of Theoretical and Experimental Physics2021, 05A107 (2021)","venue":null,"work_id":"b9968a37-2ee3-40ae-bb0e-2ce81611a8db","year":2021},"citing_paper":{"arxiv_id":"2607.05909","last_updated":"2026-07-07T07:04:03Z","snapshot_observed_at":"2026-08-14T10:29:50.174311Z","submitted_at":"2026-07-07T07:04:03Z","title":"Probing near-zone magnetic fields with extreme mass-ratio inspirals","version":1},"reference_index":4,"source":"pdf_text","source_observed_at":"2026-07-08T21:06:26.923131Z"},"links":{"citing_paper":"/paper/2607.05909"},"observation_digest":"sha256:8e0ba35e21e0c5a8203e6fc0534124cb71085a4fcef313e82a9112c0768adaa7","observation_id":"6651c08a-98c0-4598-a3ef-3f9110bb2bfe","resolution":{"observed_at":"2026-07-08T21:15:39.459915Z","resolver_source":"raw_fallback","status":"verified_fuzzy"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-23T06:30:58.430688+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-23T06:30:58.430688+00:00","source":"crossref"},{"observed_at":"2026-08-23T06:30:53.778098+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":{"arxiv_id":"1807.09495","last_updated":"2020-06-04T08:56:43Z","snapshot_observed_at":"2026-08-19T13:24:47.714101Z","submitted_at":"2018-07-25T09:11:17Z","title":"Taiji Program: Gravitational-Wave Sources","version":3},"cited_work":{"arxiv_id":"1807.09495","doi":null,"metadata_source":"pith","pith_arxiv_id":"1807.09495","snapshot_observed_at":"2026-07-08T21:15:39.260607Z","title":"Ruan, Z.-K","venue":"gr-qc","work_id":"c402b754-ae04-41c8-96f1-c747b5cf1073","year":2018},"citing_paper":{"arxiv_id":"2607.05909","last_updated":"2026-07-07T07:04:03Z","snapshot_observed_at":"2026-08-14T10:29:50.174311Z","submitted_at":"2026-07-07T07:04:03Z","title":"Probing near-zone magnetic fields with extreme mass-ratio inspirals","version":1},"reference_index":5,"source":"pdf_text","source_observed_at":"2026-07-08T21:06:26.923131Z"},"links":{"cited_paper":"/paper/1807.09495","citing_paper":"/paper/2607.05909"},"observation_digest":"sha256:ea420624e89a5123fb7668a87c8e4bf547d02aa152bccaf0009ca0a3807c2434","observation_id":"169fd5f8-d241-4810-a530-d7ab3f9402ee","resolution":{"observed_at":"2026-07-08T21:15:39.261776Z","resolver_source":"local_arxiv","status":"verified_exact"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-23T06:30:58.430688+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-23T06:30:58.430688+00:00","source":"crossref"},{"observed_at":"2026-08-23T06:30:53.778098+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":{"arxiv_id":"1703.09722","last_updated":"2018-04-11T11:52:26Z","snapshot_observed_at":"2026-08-14T21:09:32.929806Z","submitted_at":"2017-03-28T18:00:17Z","title":"Science with the space-based interferometer LISA. V: Extreme mass-ratio inspirals","version":2},"cited_work":{"arxiv_id":"1703.09722","doi":null,"metadata_source":"pith","pith_arxiv_id":"1703.09722","snapshot_observed_at":"2026-07-10T10:47:02.104780Z","title":"Science with the space-based interferometer LISA. V: Extreme mass-ratio inspirals","venue":"gr-qc","work_id":"6de2ba37-5a0d-429f-a916-57b7cebf0da8","year":2017},"citing_paper":{"arxiv_id":"2607.05909","last_updated":"2026-07-07T07:04:03Z","snapshot_observed_at":"2026-08-14T10:29:50.174311Z","submitted_at":"2026-07-07T07:04:03Z","title":"Probing near-zone magnetic fields with extreme mass-ratio inspirals","version":1},"reference_index":6,"source":"pdf_text","source_observed_at":"2026-07-08T21:06:26.923131Z"},"links":{"cited_paper":"/paper/1703.09722","citing_paper":"/paper/2607.05909"},"observation_digest":"sha256:ec6082e59fa9e801002c046094318aa957e269cfcbe8b6c664f67eca8f5ed32b","observation_id":"0cb4d4e6-3511-4434-8cba-200804f18e46","resolution":{"observed_at":"2026-07-08T21:15:39.139828Z","resolver_source":"local_arxiv","status":"verified_exact"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-23T06:30:58.430688+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-23T06:30:58.430688+00:00","source":"crossref"},{"observed_at":"2026-08-23T06:30:53.778098+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":{"arxiv_id":"gr-qc/0510057","last_updated":"2005-10-11T21:39:07Z","snapshot_observed_at":"2026-07-06T02:11:23.670680Z","submitted_at":"2005-10-11T21:39:07Z","title":"Mapping spacetimes with LISA: inspiral of a test-body in a `quasi-Kerr' field","version":1},"cited_work":{"arxiv_id":"gr-qc/0510057","doi":null,"metadata_source":"pith","pith_arxiv_id":"gr-qc/0510057","snapshot_observed_at":"2026-07-08T21:15:39.179468Z","title":"Mapping spacetimes with LISA: inspiral of a test-body in a `quasi-Kerr' field","venue":"gr-qc","work_id":"8eeac176-9ccd-4cc4-83f6-12008749de51","year":2005},"citing_paper":{"arxiv_id":"2607.05909","last_updated":"2026-07-07T07:04:03Z","snapshot_observed_at":"2026-08-14T10:29:50.174311Z","submitted_at":"2026-07-07T07:04:03Z","title":"Probing near-zone magnetic fields with extreme mass-ratio inspirals","version":1},"reference_index":7,"source":"pdf_text","source_observed_at":"2026-07-08T21:06:26.923131Z"},"links":{"cited_paper":"/paper/gr-qc/0510057","citing_paper":"/paper/2607.05909"},"observation_digest":"sha256:cea1097406505861ab87f8758269dfb36bc48e83c6d5663d33d954ae5c2a8c04","observation_id":"45ef2659-1ca1-40f5-9d69-267a9b67e225","resolution":{"observed_at":"2026-07-08T21:15:39.181416Z","resolver_source":"local_arxiv","status":"verified_exact"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-23T06:30:58.430688+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-23T06:30:58.430688+00:00","source":"crossref"},{"observed_at":"2026-08-23T06:30:53.778098+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":{"arxiv_id":"gr-qc/0612029","last_updated":"2006-12-05T12:33:46Z","snapshot_observed_at":"2026-07-06T02:11:23.670680Z","submitted_at":"2006-12-05T12:33:46Z","title":"Using LISA EMRI sources to test off-Kerr deviations in the geometry of massive black holes","version":1},"cited_work":{"arxiv_id":"gr-qc/0612029","doi":null,"metadata_source":"pith","pith_arxiv_id":"gr-qc/0612029","snapshot_observed_at":"2026-07-08T21:15:39.266522Z","title":"Using LISA EMRI sources to test off-Kerr deviations in the geometry of massive black holes","venue":"gr-qc","work_id":"b412662f-97a4-4f77-8b90-58872289bb24","year":2006},"citing_paper":{"arxiv_id":"2607.05909","last_updated":"2026-07-07T07:04:03Z","snapshot_observed_at":"2026-08-14T10:29:50.174311Z","submitted_at":"2026-07-07T07:04:03Z","title":"Probing near-zone magnetic fields with extreme mass-ratio inspirals","version":1},"reference_index":8,"source":"pdf_text","source_observed_at":"2026-07-08T21:06:26.923131Z"},"links":{"cited_paper":"/paper/gr-qc/0612029","citing_paper":"/paper/2607.05909"},"observation_digest":"sha256:8afdd128fc3f64e6dca0074cd9b7615e297035ad5e5dad930635ddb090bacb97","observation_id":"9915877f-c33c-44fe-b9d0-5861e2b89e58","resolution":{"observed_at":"2026-07-08T21:15:39.267822Z","resolver_source":"local_arxiv","status":"verified_exact"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-23T06:30:58.430688+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-23T06:30:58.430688+00:00","source":"crossref"},{"observed_at":"2026-08-23T06:30:53.778098+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":{"arxiv_id":"1904.05363","last_updated":"2019-06-13T08:23:28Z","snapshot_observed_at":"2026-07-06T07:45:18.053726Z","submitted_at":"2019-04-10T18:00:05Z","title":"Testing the nature of dark compact objects: a status report","version":3},"cited_work":{"arxiv_id":"1904.05363","doi":null,"metadata_source":"pith","pith_arxiv_id":"1904.05363","snapshot_observed_at":"2026-07-08T21:15:39.269047Z","title":"Testing the nature of dark compact objects: a status report","venue":"gr-qc","work_id":"412b4dca-8cfc-4867-9b0e-a60ee7c67e0d","year":2019},"citing_paper":{"arxiv_id":"2607.05909","last_updated":"2026-07-07T07:04:03Z","snapshot_observed_at":"2026-08-14T10:29:50.174311Z","submitted_at":"2026-07-07T07:04:03Z","title":"Probing near-zone magnetic fields with extreme mass-ratio inspirals","version":1},"reference_index":9,"source":"pdf_text","source_observed_at":"2026-07-08T21:06:26.923131Z"},"links":{"cited_paper":"/paper/1904.05363","citing_paper":"/paper/2607.05909"},"observation_digest":"sha256:7ba5f2f415b3cdca69df8ab37657fdd23180b3c606b8d45d74d8e0c836dc4c27","observation_id":"069c85e4-b3a9-40fe-9f8b-07e1e44b520c","resolution":{"observed_at":"2026-07-08T21:15:39.270357Z","resolver_source":"local_arxiv","status":"verified_exact"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-23T06:30:58.430688+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-23T06:30:58.430688+00:00","source":"crossref"},{"observed_at":"2026-08-23T06:30:53.778098+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":{"arxiv_id":"2104.06047","last_updated":"2021-09-03T06:04:12Z","snapshot_observed_at":"2026-08-16T18:32:00.142889Z","submitted_at":"2021-04-13T09:21:43Z","title":"Science with the TianQin Observatory: Preliminary Results on Testing the No-hair Theorem with EMRI","version":2},"cited_work":{"arxiv_id":"2104.06047","doi":null,"metadata_source":"pith","pith_arxiv_id":"2104.06047","snapshot_observed_at":"2026-07-08T21:15:39.129986Z","title":"Zi, J.-D","venue":"gr-qc","work_id":"fbd16b1c-c51e-4bc5-bc7c-6e2ebff5d299","year":2021},"citing_paper":{"arxiv_id":"2607.05909","last_updated":"2026-07-07T07:04:03Z","snapshot_observed_at":"2026-08-14T10:29:50.174311Z","submitted_at":"2026-07-07T07:04:03Z","title":"Probing near-zone magnetic fields with extreme mass-ratio inspirals","version":1},"reference_index":10,"source":"pdf_text","source_observed_at":"2026-07-08T21:06:26.923131Z"},"links":{"cited_paper":"/paper/2104.06047","citing_paper":"/paper/2607.05909"},"observation_digest":"sha256:6c3993a24e2919cdcae71c74bf193e507c6ffd957645dc39e13640c70848e319","observation_id":"1de3e8a2-fdce-413f-a1fc-38c8f6d3c000","resolution":{"observed_at":"2026-07-08T21:15:39.131314Z","resolver_source":"local_arxiv","status":"verified_exact"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-23T06:30:58.430688+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-23T06:30:58.430688+00:00","source":"crossref"},{"observed_at":"2026-08-23T06:30:53.778098+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":{"arxiv_id":"2311.07279","last_updated":"2023-11-29T06:54:54Z","snapshot_observed_at":"2026-08-16T14:43:49.146192Z","submitted_at":"2023-11-13T12:23:02Z","title":"Gravitational waves from extreme-mass-ratio inspirals in the semiclassical gravity spacetime","version":2},"cited_work":{"arxiv_id":"2311.07279","doi":null,"metadata_source":"pith","pith_arxiv_id":"2311.07279","snapshot_observed_at":"2026-07-08T21:15:39.157407Z","title":"Gravitational waves from extreme-mass-ratio inspirals in the semiclassical grav- ity spacetime","venue":"gr-qc","work_id":"10d6417b-052d-42bf-917b-df77a8ae13db","year":2023},"citing_paper":{"arxiv_id":"2607.05909","last_updated":"2026-07-07T07:04:03Z","snapshot_observed_at":"2026-08-14T10:29:50.174311Z","submitted_at":"2026-07-07T07:04:03Z","title":"Probing near-zone magnetic fields with extreme mass-ratio inspirals","version":1},"reference_index":11,"source":"pdf_text","source_observed_at":"2026-07-08T21:06:26.923131Z"},"links":{"cited_paper":"/paper/2311.07279","citing_paper":"/paper/2607.05909"},"observation_digest":"sha256:48d0d5ce31ce3be7e4be7936f41910a2186162ec1f6eecfb43d4640d559a6ef1","observation_id":"2407cd38-d94c-46e3-836b-69c19b477061","resolution":{"observed_at":"2026-07-08T21:15:39.158681Z","resolver_source":"local_arxiv","status":"verified_exact"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-23T06:30:58.430688+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-23T06:30:58.430688+00:00","source":"crossref"},{"observed_at":"2026-08-23T06:30:53.778098+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":{"arxiv_id":"2306.02683","last_updated":"2023-09-17T12:56:24Z","snapshot_observed_at":"2026-08-16T15:26:37.800789Z","submitted_at":"2023-06-05T08:18:44Z","title":"Gravitational waves from extreme mass ratio inspirals around a hairy Kerr black hole","version":2},"cited_work":{"arxiv_id":"2306.02683","doi":null,"metadata_source":"pith","pith_arxiv_id":"2306.02683","snapshot_observed_at":"2026-07-08T21:15:39.233916Z","title":"Zi and P.-C","venue":"gr-qc","work_id":"850aeed3-a31f-40fd-a9f1-6e738a0a635c","year":2023},"citing_paper":{"arxiv_id":"2607.05909","last_updated":"2026-07-07T07:04:03Z","snapshot_observed_at":"2026-08-14T10:29:50.174311Z","submitted_at":"2026-07-07T07:04:03Z","title":"Probing near-zone magnetic fields with extreme mass-ratio inspirals","version":1},"reference_index":12,"source":"pdf_text","source_observed_at":"2026-07-08T21:06:26.923131Z"},"links":{"cited_paper":"/paper/2306.02683","citing_paper":"/paper/2607.05909"},"observation_digest":"sha256:40b01624556be360c17c309467e543aefe85242e4c5589c939c32e3e3ae2526f","observation_id":"21651888-c18f-4b73-8581-bb2431e2a37e","resolution":{"observed_at":"2026-07-08T21:15:39.235195Z","resolver_source":"local_arxiv","status":"verified_exact"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-23T06:30:58.430688+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-23T06:30:58.430688+00:00","source":"crossref"},{"observed_at":"2026-08-23T06:30:53.778098+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":{"arxiv_id":"2311.15532","last_updated":"2024-09-03T07:21:38Z","snapshot_observed_at":"2026-08-19T11:13:40.647530Z","submitted_at":"2023-11-27T04:29:41Z","title":"Detecting the tidal heating with the generic extreme-mass-ratio inspirals","version":6},"cited_work":{"arxiv_id":"2311.15532","doi":null,"metadata_source":"pith","pith_arxiv_id":"2311.15532","snapshot_observed_at":"2026-07-08T21:15:39.140983Z","title":"Detecting the tidal heating with the generic extreme-mass-ratio inspirals","venue":"gr-qc","work_id":"4d8e3098-fef4-40bc-8d2c-d11fb39d362f","year":2023},"citing_paper":{"arxiv_id":"2607.05909","last_updated":"2026-07-07T07:04:03Z","snapshot_observed_at":"2026-08-14T10:29:50.174311Z","submitted_at":"2026-07-07T07:04:03Z","title":"Probing near-zone magnetic fields with extreme mass-ratio inspirals","version":1},"reference_index":13,"source":"pdf_text","source_observed_at":"2026-07-08T21:06:26.923131Z"},"links":{"cited_paper":"/paper/2311.15532","citing_paper":"/paper/2607.05909"},"observation_digest":"sha256:67737fa50c4d93f92aa9ef5f432ff47559e4861653d33a5ab2f80214d2862f05","observation_id":"e738f0f4-aa94-4dc7-84c1-c4d2bd231eca","resolution":{"observed_at":"2026-07-08T21:15:39.142133Z","resolver_source":"local_arxiv","status":"verified_exact"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-23T06:30:58.430688+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-23T06:30:58.430688+00:00","source":"crossref"},{"observed_at":"2026-08-23T06:30:53.778098+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":{"arxiv_id":"2404.04013","last_updated":"2024-06-26T07:28:14Z","snapshot_observed_at":"2026-08-16T14:03:23.655454Z","submitted_at":"2024-04-05T10:40:20Z","title":"Tidal heating as a discriminator for horizons in equatorial eccentric extreme mass ratio inspirals","version":3},"cited_work":{"arxiv_id":"2404.04013","doi":null,"metadata_source":"pith","pith_arxiv_id":"2404.04013","snapshot_observed_at":"2026-07-08T21:15:39.279500Z","title":"Datta, R","venue":"gr-qc","work_id":"1c557cf2-b9ec-4a4c-a328-a69852581b28","year":2024},"citing_paper":{"arxiv_id":"2607.05909","last_updated":"2026-07-07T07:04:03Z","snapshot_observed_at":"2026-08-14T10:29:50.174311Z","submitted_at":"2026-07-07T07:04:03Z","title":"Probing near-zone magnetic fields with extreme mass-ratio inspirals","version":1},"reference_index":14,"source":"pdf_text","source_observed_at":"2026-07-08T21:06:26.923131Z"},"links":{"cited_paper":"/paper/2404.04013","citing_paper":"/paper/2607.05909"},"observation_digest":"sha256:3593de88bf3fea9688b00a319e1018d3ccfe88bf7ac31812a6ddf08015f8181b","observation_id":"dc890945-57a2-45cd-a9fd-42fea3276202","resolution":{"observed_at":"2026-07-08T21:15:39.280684Z","resolver_source":"local_arxiv","status":"verified_exact"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-23T06:30:58.430688+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-23T06:30:58.430688+00:00","source":"crossref"},{"observed_at":"2026-08-23T06:30:53.778098+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":{"arxiv_id":"2401.08085","last_updated":"2024-05-13T17:58:26Z","snapshot_observed_at":"2026-08-20T03:08:47.260345Z","submitted_at":"2024-01-16T03:25:01Z","title":"Testing gravity with Extreme-Mass-Ratio Inspirals","version":2},"cited_work":{"arxiv_id":"2401.08085","doi":null,"metadata_source":"pith","pith_arxiv_id":"2401.08085","snapshot_observed_at":"2026-07-08T21:15:39.110764Z","title":"C´ ardenas-Avenda˜ no and C","venue":"gr-qc","work_id":"290c2bf7-9a8d-4522-aa0d-81cf08f55ac4","year":2024},"citing_paper":{"arxiv_id":"2607.05909","last_updated":"2026-07-07T07:04:03Z","snapshot_observed_at":"2026-08-14T10:29:50.174311Z","submitted_at":"2026-07-07T07:04:03Z","title":"Probing near-zone magnetic fields with extreme mass-ratio inspirals","version":1},"reference_index":15,"source":"pdf_text","source_observed_at":"2026-07-08T21:06:26.923131Z"},"links":{"cited_paper":"/paper/2401.08085","citing_paper":"/paper/2607.05909"},"observation_digest":"sha256:bf9ae83a9778a12059bf79013feffa16be930b68645e52d2a8ce25591aa5f40a","observation_id":"c3d12eef-a701-468c-903b-d97933e37696","resolution":{"observed_at":"2026-07-08T21:15:39.111949Z","resolver_source":"local_arxiv","status":"verified_exact"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-23T06:30:58.430688+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-23T06:30:58.430688+00:00","source":"crossref"},{"observed_at":"2026-08-23T06:30:53.778098+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":"2026-07-08T21:15:39.429232Z","title":"Zi, Phys","venue":null,"work_id":"a1af939d-c1f3-4169-ade0-0371421f01cc","year":2024},"citing_paper":{"arxiv_id":"2607.05909","last_updated":"2026-07-07T07:04:03Z","snapshot_observed_at":"2026-08-14T10:29:50.174311Z","submitted_at":"2026-07-07T07:04:03Z","title":"Probing near-zone magnetic fields with extreme mass-ratio inspirals","version":1},"reference_index":16,"source":"pdf_text","source_observed_at":"2026-07-08T21:06:26.923131Z"},"links":{"citing_paper":"/paper/2607.05909"},"observation_digest":"sha256:c0eb98dee3a7b353703116374f74a7cac742c80c291981bf76cebd858969a9b0","observation_id":"77a37b2c-9886-4684-96e8-6f6b287129f1","resolution":{"observed_at":"2026-07-08T21:15:39.430573Z","resolver_source":"raw_fallback","status":"verified_fuzzy"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-23T06:30:58.430688+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-23T06:30:58.430688+00:00","source":"crossref"},{"observed_at":"2026-08-23T06:30:53.778098+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":{"arxiv_id":"2409.17765","last_updated":"2025-05-18T06:14:55Z","snapshot_observed_at":"2026-08-16T21:19:50.691025Z","submitted_at":"2024-09-26T11:59:58Z","title":"Eccentric extreme mass-ratio inspirals: A gateway to probe quantum gravity effects","version":2},"cited_work":{"arxiv_id":"2409.17765","doi":null,"metadata_source":"pith","pith_arxiv_id":"2409.17765","snapshot_observed_at":"2026-07-08T21:15:39.120721Z","title":"Zi and S","venue":"gr-qc","work_id":"3796df8f-4c0e-49c5-aed5-6298ae1ae498","year":2024},"citing_paper":{"arxiv_id":"2607.05909","last_updated":"2026-07-07T07:04:03Z","snapshot_observed_at":"2026-08-14T10:29:50.174311Z","submitted_at":"2026-07-07T07:04:03Z","title":"Probing near-zone magnetic fields with extreme mass-ratio inspirals","version":1},"reference_index":17,"source":"pdf_text","source_observed_at":"2026-07-08T21:06:26.923131Z"},"links":{"cited_paper":"/paper/2409.17765","citing_paper":"/paper/2607.05909"},"observation_digest":"sha256:69851bd61fc79ea94d355b6d6aa825afddbeb15630b9dc872eeb7a6c5ff0d9e8","observation_id":"0a814ffb-9ea9-4d9d-80f4-86b5aaee2274","resolution":{"observed_at":"2026-07-08T21:15:39.121898Z","resolver_source":"local_arxiv","status":"verified_exact"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-23T06:30:58.430688+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-23T06:30:58.430688+00:00","source":"crossref"},{"observed_at":"2026-08-23T06:30:53.778098+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":{"arxiv_id":"2403.16192","last_updated":"2024-06-12T21:30:54Z","snapshot_observed_at":"2026-08-16T14:06:56.576839Z","submitted_at":"2024-03-24T15:18:00Z","title":"Testing disformal non-circular deformation of Kerr black holes with LISA","version":2},"cited_work":{"arxiv_id":"2403.16192","doi":null,"metadata_source":"pith","pith_arxiv_id":"2403.16192","snapshot_observed_at":"2026-07-08T21:15:39.228798Z","title":"Testing disformal non-circular deformation of Kerr black holes with LISA","venue":"gr-qc","work_id":"5e1c05c8-b1a8-4877-8c46-426fc3f8d6c4","year":2024},"citing_paper":{"arxiv_id":"2607.05909","last_updated":"2026-07-07T07:04:03Z","snapshot_observed_at":"2026-08-14T10:29:50.174311Z","submitted_at":"2026-07-07T07:04:03Z","title":"Probing near-zone magnetic fields with extreme mass-ratio inspirals","version":1},"reference_index":18,"source":"pdf_text","source_observed_at":"2026-07-08T21:06:26.923131Z"},"links":{"cited_paper":"/paper/2403.16192","citing_paper":"/paper/2607.05909"},"observation_digest":"sha256:a0e8f145e39940606675506a5abbcce187ca6b475e5b929c2f4fac09a262739b","observation_id":"4b40f2c2-c959-4165-b68d-ce13e922e6df","resolution":{"observed_at":"2026-07-08T21:15:39.229971Z","resolver_source":"local_arxiv","status":"verified_exact"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-23T06:30:58.430688+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-23T06:30:58.430688+00:00","source":"crossref"},{"observed_at":"2026-08-23T06:30:53.778098+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":{"arxiv_id":"2507.03380","last_updated":"2026-06-26T06:16:22Z","snapshot_observed_at":"2026-08-13T03:25:54.634306Z","submitted_at":"2025-07-04T08:24:29Z","title":"Extreme mass-ratio inspirals and extra dimensions: Insights from modified Teukolsky framework","version":3},"cited_work":{"arxiv_id":"2507.03380","doi":null,"metadata_source":"pith","pith_arxiv_id":"2507.03380","snapshot_observed_at":"2026-07-08T21:15:39.226306Z","title":"Kumar, T","venue":"gr-qc","work_id":"6d7301b4-fd82-432f-b003-9746e4ca1206","year":2025},"citing_paper":{"arxiv_id":"2607.05909","last_updated":"2026-07-07T07:04:03Z","snapshot_observed_at":"2026-08-14T10:29:50.174311Z","submitted_at":"2026-07-07T07:04:03Z","title":"Probing near-zone magnetic fields with extreme mass-ratio inspirals","version":1},"reference_index":19,"source":"pdf_text","source_observed_at":"2026-07-08T21:06:26.923131Z"},"links":{"cited_paper":"/paper/2507.03380","citing_paper":"/paper/2607.05909"},"observation_digest":"sha256:41531450a08ebe33125c65d82604ba3080e77f9bbd9971d8477c7ecf474a4b36","observation_id":"5c0743dc-06d1-4820-b312-acdd5ac50252","resolution":{"observed_at":"2026-07-08T21:15:39.227621Z","resolver_source":"local_arxiv","status":"verified_exact"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-23T06:30:58.430688+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-23T06:30:58.430688+00:00","source":"crossref"},{"observed_at":"2026-08-23T06:30:53.778098+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":"2510.05166","doi":null,"metadata_source":"arxiv_reference","pith_arxiv_id":null,"snapshot_observed_at":"2026-07-08T21:15:39.112990Z","title":"Probing regular black holes with sub-Planckian curva- ture through periodic orbits and their gravitational wave radiation","venue":null,"work_id":"94d63f63-ddfc-48ca-9052-1fbc3141e490","year":2026},"citing_paper":{"arxiv_id":"2607.05909","last_updated":"2026-07-07T07:04:03Z","snapshot_observed_at":"2026-08-14T10:29:50.174311Z","submitted_at":"2026-07-07T07:04:03Z","title":"Probing near-zone magnetic fields with extreme mass-ratio inspirals","version":1},"reference_index":20,"source":"pdf_text","source_observed_at":"2026-07-08T21:06:26.923131Z"},"links":{"citing_paper":"/paper/2607.05909"},"observation_digest":"sha256:e9089a716e634444aeef6a5ded4ca4f94b449e9aba3a503b6764a16b4db6aea0","observation_id":"b535cf2b-9274-469c-9508-083ebeca080d","resolution":{"observed_at":"2026-07-08T21:15:39.114642Z","resolver_source":"arxiv_id","status":"verified_exact"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-23T06:30:58.430688+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-23T06:30:58.430688+00:00","source":"crossref"},{"observed_at":"2026-08-23T06:30:53.778098+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":"2510.16102","doi":null,"metadata_source":"arxiv_reference","pith_arxiv_id":null,"snapshot_observed_at":"2026-07-08T21:15:39.231366Z","title":"LaHaye, C","venue":null,"work_id":"932bb8d2-cb02-4dc6-b4fe-26d33fb00259","year":2026},"citing_paper":{"arxiv_id":"2607.05909","last_updated":"2026-07-07T07:04:03Z","snapshot_observed_at":"2026-08-14T10:29:50.174311Z","submitted_at":"2026-07-07T07:04:03Z","title":"Probing near-zone magnetic fields with extreme mass-ratio inspirals","version":1},"reference_index":21,"source":"pdf_text","source_observed_at":"2026-07-08T21:06:26.923131Z"},"links":{"citing_paper":"/paper/2607.05909"},"observation_digest":"sha256:9ab2f128697f9536068fab74c335e3d51bc2bca553fddeaf7cdd81e03a6d08f5","observation_id":"18efe5d7-95a1-4106-a50b-acec98e0bbe6","resolution":{"observed_at":"2026-07-08T21:15:39.232753Z","resolver_source":"arxiv_id","status":"verified_exact"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-23T06:30:58.430688+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-23T06:30:58.430688+00:00","source":"crossref"},{"observed_at":"2026-08-23T06:30:53.778098+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":"2503.06503","doi":null,"metadata_source":"arxiv_reference","pith_arxiv_id":null,"snapshot_observed_at":"2026-07-08T21:15:39.255203Z","title":null,"venue":null,"work_id":"bef9abf2-93dd-48b6-9697-67fe14fdb2a3","year":2025},"citing_paper":{"arxiv_id":"2607.05909","last_updated":"2026-07-07T07:04:03Z","snapshot_observed_at":"2026-08-14T10:29:50.174311Z","submitted_at":"2026-07-07T07:04:03Z","title":"Probing near-zone magnetic fields with extreme mass-ratio inspirals","version":1},"reference_index":22,"source":"pdf_text","source_observed_at":"2026-07-08T21:06:26.923131Z"},"links":{"citing_paper":"/paper/2607.05909"},"observation_digest":"sha256:4d4bc0eee5b24a5935065a4c4cc08b6dde378414bc38ed470451af32e2cd0ede","observation_id":"c133b974-bdd5-4fa8-b175-07fbdd410921","resolution":{"observed_at":"2026-07-08T21:15:39.256908Z","resolver_source":"arxiv_id","status":"verified_exact"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-23T06:30:58.430688+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-23T06:30:58.430688+00:00","source":"crossref"},{"observed_at":"2026-08-23T06:30:53.778098+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":{"arxiv_id":"2512.11911","last_updated":"2026-06-19T02:53:11Z","snapshot_observed_at":"2026-08-11T17:01:56.178916Z","submitted_at":"2025-12-11T01:04:43Z","title":"Gravitational radiations from periodic orbits around a black hole in the effective field theory extension of general relativity","version":3},"cited_work":{"arxiv_id":"2512.11911","doi":null,"metadata_source":"pith","pith_arxiv_id":"2512.11911","snapshot_observed_at":"2026-07-08T21:15:39.198012Z","title":"Gravitational radiations from periodic orbits around a black hole in the effective field theory extension of general relativity","venue":"gr-qc","work_id":"3d6089bc-21bf-47c2-b2b3-195927393518","year":2025},"citing_paper":{"arxiv_id":"2607.05909","last_updated":"2026-07-07T07:04:03Z","snapshot_observed_at":"2026-08-14T10:29:50.174311Z","submitted_at":"2026-07-07T07:04:03Z","title":"Probing near-zone magnetic fields with extreme mass-ratio inspirals","version":1},"reference_index":23,"source":"pdf_text","source_observed_at":"2026-07-08T21:06:26.923131Z"},"links":{"cited_paper":"/paper/2512.11911","citing_paper":"/paper/2607.05909"},"observation_digest":"sha256:31ca51055d5278823df3572d4fd770c49080014dbe8241d99b07c64c84abb19e","observation_id":"692a0f9f-820a-47f4-967b-3159d5cb4027","resolution":{"observed_at":"2026-07-08T21:15:39.199387Z","resolver_source":"local_arxiv","status":"verified_exact"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-23T06:30:58.430688+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-23T06:30:58.430688+00:00","source":"crossref"},{"observed_at":"2026-08-23T06:30:53.778098+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":"2602.11039","doi":null,"metadata_source":"arxiv_reference","pith_arxiv_id":null,"snapshot_observed_at":"2026-07-08T21:15:39.214334Z","title":null,"venue":null,"work_id":"4e08d10a-c2dd-4837-8ab9-fc7ce7f5f49f","year":2026},"citing_paper":{"arxiv_id":"2607.05909","last_updated":"2026-07-07T07:04:03Z","snapshot_observed_at":"2026-08-14T10:29:50.174311Z","submitted_at":"2026-07-07T07:04:03Z","title":"Probing near-zone magnetic fields with extreme mass-ratio inspirals","version":1},"reference_index":24,"source":"pdf_text","source_observed_at":"2026-07-08T21:06:26.923131Z"},"links":{"citing_paper":"/paper/2607.05909"},"observation_digest":"sha256:5867008a841994d8e9bc2a2d2e457e79bcb213f333c40e0b38491449a8044896","observation_id":"e0527e0d-3453-4ed7-8b51-1f9e1db7b154","resolution":{"observed_at":"2026-07-08T21:15:39.215610Z","resolver_source":"arxiv_id","status":"verified_exact"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-23T06:30:58.430688+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-23T06:30:58.430688+00:00","source":"crossref"},{"observed_at":"2026-08-23T06:30:53.778098+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":{"arxiv_id":"2605.05362","last_updated":"2026-06-04T15:01:39Z","snapshot_observed_at":"2026-07-06T02:11:23.670680Z","submitted_at":"2026-05-06T18:40:43Z","title":"Constraining Lorentz symmetry breaking in bumblebee gravity with extreme mass-ratio inspirals","version":3},"cited_work":{"arxiv_id":"2605.05362","doi":null,"metadata_source":"pith","pith_arxiv_id":"2605.05362","snapshot_observed_at":"2026-07-08T21:15:39.145638Z","title":"Constraining Lorentz symmetry breaking in bumblebee gravity with extreme mass-ratio inspirals","venue":"gr-qc","work_id":"1bfa6e50-56de-462f-aa61-b2b5c4de4256","year":2026},"citing_paper":{"arxiv_id":"2607.05909","last_updated":"2026-07-07T07:04:03Z","snapshot_observed_at":"2026-08-14T10:29:50.174311Z","submitted_at":"2026-07-07T07:04:03Z","title":"Probing near-zone magnetic fields with extreme mass-ratio inspirals","version":1},"reference_index":25,"source":"pdf_text","source_observed_at":"2026-07-08T21:06:26.923131Z"},"links":{"cited_paper":"/paper/2605.05362","citing_paper":"/paper/2607.05909"},"observation_digest":"sha256:65d8974a20a92544cf674c5ed609c0b84c08c9b35dcbe3ef7507a76919aec659","observation_id":"3140d427-fba8-466f-9a61-0c1df7bce342","resolution":{"observed_at":"2026-07-08T21:15:39.146805Z","resolver_source":"local_arxiv","status":"verified_exact"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-23T06:30:58.430688+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-23T06:30:58.430688+00:00","source":"crossref"},{"observed_at":"2026-08-23T06:30:53.778098+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":{"arxiv_id":"2604.06053","last_updated":"2026-04-09T13:09:44Z","snapshot_observed_at":"2026-08-18T03:25:50.535598Z","submitted_at":"2026-04-07T16:41:35Z","title":"Probing Kerr Symmetry Breaking with LISA Extreme-Mass-Ratio Inspirals","version":2},"cited_work":{"arxiv_id":"2604.06053","doi":null,"metadata_source":"pith","pith_arxiv_id":"2604.06053","snapshot_observed_at":"2026-07-08T21:15:39.143226Z","title":"Probing Kerr Symmetry Breaking with LISA Extreme-Mass-Ratio Inspirals","venue":"gr-qc","work_id":"95d8d118-5dca-4229-971b-910aac06d9dc","year":2026},"citing_paper":{"arxiv_id":"2607.05909","last_updated":"2026-07-07T07:04:03Z","snapshot_observed_at":"2026-08-14T10:29:50.174311Z","submitted_at":"2026-07-07T07:04:03Z","title":"Probing near-zone magnetic fields with extreme mass-ratio inspirals","version":1},"reference_index":26,"source":"pdf_text","source_observed_at":"2026-07-08T21:06:26.923131Z"},"links":{"cited_paper":"/paper/2604.06053","citing_paper":"/paper/2607.05909"},"observation_digest":"sha256:8174ab24bcf837ed09ae361c39dfcd645adc637bf8b48ee31e4c93e83526dcb6","observation_id":"34899e1b-c412-44b4-86fd-0eb8f8436f54","resolution":{"observed_at":"2026-07-08T21:15:39.144485Z","resolver_source":"local_arxiv","status":"verified_exact"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-23T06:30:58.430688+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-23T06:30:58.430688+00:00","source":"crossref"},{"observed_at":"2026-08-23T06:30:53.778098+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":{"arxiv_id":"1104.2322","last_updated":"2011-04-12T20:00:00Z","snapshot_observed_at":"2026-08-15T07:25:16.288892Z","submitted_at":"2011-04-12T20:00:00Z","title":"Observable Signatures of EMRI Black Hole Binaries Embedded in Thin Accretion Disks","version":1},"cited_work":{"arxiv_id":"1104.2322","doi":null,"metadata_source":"pith","pith_arxiv_id":"1104.2322","snapshot_observed_at":"2026-07-08T21:15:39.150375Z","title":"Observable Signatures of EMRI Black Hole Binaries Embedded in Thin Accretion Disks","venue":"astro-ph.GA","work_id":"5cc822b1-d6df-4033-86a1-414006a5b182","year":2011},"citing_paper":{"arxiv_id":"2607.05909","last_updated":"2026-07-07T07:04:03Z","snapshot_observed_at":"2026-08-14T10:29:50.174311Z","submitted_at":"2026-07-07T07:04:03Z","title":"Probing near-zone magnetic fields with extreme mass-ratio inspirals","version":1},"reference_index":27,"source":"pdf_text","source_observed_at":"2026-07-08T21:06:26.923131Z"},"links":{"cited_paper":"/paper/1104.2322","citing_paper":"/paper/2607.05909"},"observation_digest":"sha256:88736b25ee9e4e5818165a0d3b14e175a3aa7828e7e9f234e21f725790331770","observation_id":"d355f74b-1934-4e0c-be0f-27e595ffb09b","resolution":{"observed_at":"2026-07-08T21:15:39.151552Z","resolver_source":"local_arxiv","status":"verified_exact"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-23T06:30:58.430688+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-23T06:30:58.430688+00:00","source":"crossref"},{"observed_at":"2026-08-23T06:30:53.778098+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":{"arxiv_id":"1404.7149","last_updated":"2014-05-24T00:33:48Z","snapshot_observed_at":"2026-08-14T23:36:00.477660Z","submitted_at":"2014-04-28T20:00:58Z","title":"Can environmental effects spoil precision gravitational-wave astrophysics?","version":2},"cited_work":{"arxiv_id":"1404.7149","doi":null,"metadata_source":"pith","pith_arxiv_id":"1404.7149","snapshot_observed_at":"2026-07-08T21:15:39.289646Z","title":"Can environmental effects spoil precision gravitational-wave astrophysics?","venue":"gr-qc","work_id":"b86edaf3-7f8d-4107-8fc7-efff113907ad","year":2014},"citing_paper":{"arxiv_id":"2607.05909","last_updated":"2026-07-07T07:04:03Z","snapshot_observed_at":"2026-08-14T10:29:50.174311Z","submitted_at":"2026-07-07T07:04:03Z","title":"Probing near-zone magnetic fields with extreme mass-ratio inspirals","version":1},"reference_index":28,"source":"pdf_text","source_observed_at":"2026-07-08T21:06:26.923131Z"},"links":{"cited_paper":"/paper/1404.7149","citing_paper":"/paper/2607.05909"},"observation_digest":"sha256:b55e631809de10fe692ad88bbb882f354954c3a697e19bcf048b45a8e53bb2e7","observation_id":"043344f4-dea5-4cff-9113-c4e1b854d21b","resolution":{"observed_at":"2026-07-08T21:15:39.290872Z","resolver_source":"local_arxiv","status":"verified_exact"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-23T06:30:58.430688+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-23T06:30:58.430688+00:00","source":"crossref"},{"observed_at":"2026-08-23T06:30:53.778098+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":{"arxiv_id":"2104.01208","last_updated":"2021-09-03T18:13:59Z","snapshot_observed_at":"2026-08-16T18:34:10.193462Z","submitted_at":"2021-04-02T19:17:10Z","title":"Wet Extreme Mass Ratio Inspirals May Be More Common For Spaceborne Gravitational Wave Detection","version":2},"cited_work":{"arxiv_id":"2104.01208","doi":null,"metadata_source":"pith","pith_arxiv_id":"2104.01208","snapshot_observed_at":"2026-07-08T21:15:39.287127Z","title":"Wet Extreme Mass Ratio Inspirals May Be More Common For Spaceborne Gravitational Wave Detection","venue":"astro-ph.HE","work_id":"0458894e-b169-43e9-92a2-63df934ff738","year":2021},"citing_paper":{"arxiv_id":"2607.05909","last_updated":"2026-07-07T07:04:03Z","snapshot_observed_at":"2026-08-14T10:29:50.174311Z","submitted_at":"2026-07-07T07:04:03Z","title":"Probing near-zone magnetic fields with extreme mass-ratio inspirals","version":1},"reference_index":29,"source":"pdf_text","source_observed_at":"2026-07-08T21:06:26.923131Z"},"links":{"cited_paper":"/paper/2104.01208","citing_paper":"/paper/2607.05909"},"observation_digest":"sha256:636dea61c503be8c888e91aef60d42d01f6a34d56fb660f9f20e64a4ff1ab4b9","observation_id":"4eaf4f86-bd58-473c-a713-7a99aa25f736","resolution":{"observed_at":"2026-07-08T21:15:39.288376Z","resolver_source":"local_arxiv","status":"verified_exact"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-23T06:30:58.430688+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-23T06:30:58.430688+00:00","source":"crossref"},{"observed_at":"2026-08-23T06:30:53.778098+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":{"arxiv_id":"2205.01597","last_updated":"2022-05-03T16:20:16Z","snapshot_observed_at":"2026-08-16T17:02:52.550577Z","submitted_at":"2022-05-03T16:20:16Z","title":"New Horizons for Fundamental Physics with LISA","version":1},"cited_work":{"arxiv_id":"2205.01597","doi":null,"metadata_source":"pith","pith_arxiv_id":"2205.01597","snapshot_observed_at":"2026-07-08T21:15:39.262945Z","title":"Arun et al","venue":"gr-qc","work_id":"24248c69-f237-4237-9cc2-0803e27716fc","year":2022},"citing_paper":{"arxiv_id":"2607.05909","last_updated":"2026-07-07T07:04:03Z","snapshot_observed_at":"2026-08-14T10:29:50.174311Z","submitted_at":"2026-07-07T07:04:03Z","title":"Probing near-zone magnetic fields with extreme mass-ratio inspirals","version":1},"reference_index":30,"source":"pdf_text","source_observed_at":"2026-07-08T21:06:26.923131Z"},"links":{"cited_paper":"/paper/2205.01597","citing_paper":"/paper/2607.05909"},"observation_digest":"sha256:f5bb72ed23f02256e692b17892b3f61b2ad6aad9a3abdc7d95cf8eac87d598d2","observation_id":"613a7c14-a375-4813-9598-9e2e61b1390e","resolution":{"observed_at":"2026-07-08T21:15:39.264135Z","resolver_source":"local_arxiv","status":"verified_exact"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-23T06:30:58.430688+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-23T06:30:58.430688+00:00","source":"crossref"},{"observed_at":"2026-08-23T06:30:53.778098+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":{"arxiv_id":"2210.01133","last_updated":"2022-11-21T14:31:26Z","snapshot_observed_at":"2026-08-16T16:27:14.500036Z","submitted_at":"2022-10-03T18:00:01Z","title":"Gravitational waves from extreme-mass-ratio systems in astrophysical environments","version":2},"cited_work":{"arxiv_id":"2210.01133","doi":null,"metadata_source":"pith","pith_arxiv_id":"2210.01133","snapshot_observed_at":"2026-07-08T21:15:39.216758Z","title":"Cardoso, K","venue":"gr-qc","work_id":"682b6693-c7b6-4b27-9f70-709be62f270f","year":2022},"citing_paper":{"arxiv_id":"2607.05909","last_updated":"2026-07-07T07:04:03Z","snapshot_observed_at":"2026-08-14T10:29:50.174311Z","submitted_at":"2026-07-07T07:04:03Z","title":"Probing near-zone magnetic fields with extreme mass-ratio inspirals","version":1},"reference_index":31,"source":"pdf_text","source_observed_at":"2026-07-08T21:06:26.923131Z"},"links":{"cited_paper":"/paper/2210.01133","citing_paper":"/paper/2607.05909"},"observation_digest":"sha256:79190cbc43b2ba1430b9e855114731e178e7d09a1dee1fb1e38d27a4e9230ae6","observation_id":"3c7c335f-fdc7-44a5-ba17-94ffb80c1ab4","resolution":{"observed_at":"2026-07-08T21:15:39.217967Z","resolver_source":"local_arxiv","status":"verified_exact"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-23T06:30:58.430688+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-23T06:30:58.430688+00:00","source":"crossref"},{"observed_at":"2026-08-23T06:30:53.778098+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":{"arxiv_id":"2207.10086","last_updated":"2023-08-14T09:43:26Z","snapshot_observed_at":"2026-08-16T16:44:29.109525Z","submitted_at":"2022-07-20T18:00:00Z","title":"Probing Accretion Physics with Gravitational Waves","version":3},"cited_work":{"arxiv_id":"2207.10086","doi":null,"metadata_source":"pith","pith_arxiv_id":"2207.10086","snapshot_observed_at":"2026-07-08T21:15:39.281908Z","title":"Speri, A","venue":"gr-qc","work_id":"9d37619c-d6a0-4222-99e6-16a351a04dcd","year":2022},"citing_paper":{"arxiv_id":"2607.05909","last_updated":"2026-07-07T07:04:03Z","snapshot_observed_at":"2026-08-14T10:29:50.174311Z","submitted_at":"2026-07-07T07:04:03Z","title":"Probing near-zone magnetic fields with extreme mass-ratio inspirals","version":1},"reference_index":32,"source":"pdf_text","source_observed_at":"2026-07-08T21:06:26.923131Z"},"links":{"cited_paper":"/paper/2207.10086","citing_paper":"/paper/2607.05909"},"observation_digest":"sha256:b72d21220ab3a3d612d567bb5e821714330d8d8e23c0fce3d22412b804c929be","observation_id":"92d7786e-6ee0-4902-9f83-c21d22777f7d","resolution":{"observed_at":"2026-07-08T21:15:39.283101Z","resolver_source":"local_arxiv","status":"verified_exact"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-23T06:30:58.430688+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-23T06:30:58.430688+00:00","source":"crossref"},{"observed_at":"2026-08-23T06:30:53.778098+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":{"arxiv_id":"2301.05088","last_updated":"2024-10-31T00:59:24Z","snapshot_observed_at":"2026-08-16T16:02:50.481161Z","submitted_at":"2023-01-12T15:35:58Z","title":"Extreme mass ratio inspirals in galaxies with dark matter halos","version":2},"cited_work":{"arxiv_id":"2301.05088","doi":null,"metadata_source":"pith","pith_arxiv_id":"2301.05088","snapshot_observed_at":"2026-07-08T21:15:39.223982Z","title":"Extreme mass ratio inspirals in galaxies with dark matter halos","venue":"gr-qc","work_id":"4073f472-752b-4850-8192-47ee4383e00d","year":2023},"citing_paper":{"arxiv_id":"2607.05909","last_updated":"2026-07-07T07:04:03Z","snapshot_observed_at":"2026-08-14T10:29:50.174311Z","submitted_at":"2026-07-07T07:04:03Z","title":"Probing near-zone magnetic fields with extreme mass-ratio inspirals","version":1},"reference_index":33,"source":"pdf_text","source_observed_at":"2026-07-08T21:06:26.923131Z"},"links":{"cited_paper":"/paper/2301.05088","citing_paper":"/paper/2607.05909"},"observation_digest":"sha256:e8dc0961f2cb658f8973e5155bc7ca96a277f81fdd34334e7d1ddf05294d2f28","observation_id":"fc317fd9-a5ef-40f4-b804-69d7a851b491","resolution":{"observed_at":"2026-07-08T21:15:39.225158Z","resolver_source":"local_arxiv","status":"verified_exact"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-23T06:30:58.430688+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-23T06:30:58.430688+00:00","source":"crossref"},{"observed_at":"2026-08-23T06:30:53.778098+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":"2026-07-08T21:15:39.439324Z","title":null,"venue":null,"work_id":"3a9c9b5b-1767-43c4-aee4-ec0662e84f56","year":2023},"citing_paper":{"arxiv_id":"2607.05909","last_updated":"2026-07-07T07:04:03Z","snapshot_observed_at":"2026-08-14T10:29:50.174311Z","submitted_at":"2026-07-07T07:04:03Z","title":"Probing near-zone magnetic fields with extreme mass-ratio inspirals","version":1},"reference_index":34,"source":"pdf_text","source_observed_at":"2026-07-08T21:06:26.923131Z"},"links":{"citing_paper":"/paper/2607.05909"},"observation_digest":"sha256:f5add95bdb4a6f30d23a03c616d70dfb672dd5acff0c7f21e27d2979cf1c1ec8","observation_id":"6920b2f2-1a77-4f5b-b214-348ef5d7a97f","resolution":{"observed_at":"2026-07-08T21:15:39.440976Z","resolver_source":"raw_fallback","status":"unresolved"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-23T06:30:58.430688+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-23T06:30:58.430688+00:00","source":"crossref"},{"observed_at":"2026-08-23T06:30:53.778098+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":"2410.06882","doi":null,"metadata_source":"arxiv_reference","pith_arxiv_id":null,"snapshot_observed_at":"2026-07-08T21:15:39.271837Z","title":null,"venue":null,"work_id":"36b38a4d-9c3c-4f0f-a1ac-d227e1c96002","year":2025},"citing_paper":{"arxiv_id":"2607.05909","last_updated":"2026-07-07T07:04:03Z","snapshot_observed_at":"2026-08-14T10:29:50.174311Z","submitted_at":"2026-07-07T07:04:03Z","title":"Probing near-zone magnetic fields with extreme mass-ratio inspirals","version":1},"reference_index":35,"source":"pdf_text","source_observed_at":"2026-07-08T21:06:26.923131Z"},"links":{"citing_paper":"/paper/2607.05909"},"observation_digest":"sha256:322af75c3021a62d990680474df5a76e24eb64028c87718d31234f32ad59c10e","observation_id":"dcd72b89-5df7-460c-9f98-b44597052dd4","resolution":{"observed_at":"2026-07-08T21:15:39.273099Z","resolver_source":"arxiv_id","status":"verified_exact"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-23T06:30:58.430688+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-23T06:30:58.430688+00:00","source":"crossref"},{"observed_at":"2026-08-23T06:30:53.778098+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":"2026-07-08T21:15:39.450677Z","title":"Jiang and W.-B","venue":null,"work_id":"dfa8d7c1-590a-4b58-9ca3-867df6a75a83","year":2024},"citing_paper":{"arxiv_id":"2607.05909","last_updated":"2026-07-07T07:04:03Z","snapshot_observed_at":"2026-08-14T10:29:50.174311Z","submitted_at":"2026-07-07T07:04:03Z","title":"Probing near-zone magnetic fields with extreme mass-ratio inspirals","version":1},"reference_index":36,"source":"pdf_text","source_observed_at":"2026-07-08T21:06:26.923131Z"},"links":{"citing_paper":"/paper/2607.05909"},"observation_digest":"sha256:7cc8169431ff94da79675a9b0e925994c04a33b10e89584215c749cf2bddd3ed","observation_id":"e91692cf-2766-4cb1-a0a0-ade39ef12796","resolution":{"observed_at":"2026-07-08T21:15:39.452208Z","resolver_source":"raw_fallback","status":"verified_fuzzy"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-23T06:30:58.430688+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-23T06:30:58.430688+00:00","source":"crossref"},{"observed_at":"2026-08-23T06:30:53.778098+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":{"arxiv_id":"2505.04697","last_updated":"2025-08-18T00:00:03Z","snapshot_observed_at":"2026-08-18T00:22:38.418616Z","submitted_at":"2025-05-07T18:00:03Z","title":"Extreme mass ratio inspirals in rotating dark matter spikes","version":2},"cited_work":{"arxiv_id":"2505.04697","doi":null,"metadata_source":"pith","pith_arxiv_id":"2505.04697","snapshot_observed_at":"2026-07-08T21:15:39.159890Z","title":"Mitra, N","venue":"gr-qc","work_id":"d7618433-0655-4ae9-ac78-1d7ea13a7692","year":2025},"citing_paper":{"arxiv_id":"2607.05909","last_updated":"2026-07-07T07:04:03Z","snapshot_observed_at":"2026-08-14T10:29:50.174311Z","submitted_at":"2026-07-07T07:04:03Z","title":"Probing near-zone magnetic fields with extreme mass-ratio inspirals","version":1},"reference_index":37,"source":"pdf_text","source_observed_at":"2026-07-08T21:06:26.923131Z"},"links":{"cited_paper":"/paper/2505.04697","citing_paper":"/paper/2607.05909"},"observation_digest":"sha256:04c558c4134b9e46299e1e0b7d3157b633c9c7736edcb54cf2226aeea171d001","observation_id":"41f5c358-4262-4c6b-9640-25e3ecceb4d8","resolution":{"observed_at":"2026-07-08T21:15:39.161139Z","resolver_source":"local_arxiv","status":"verified_exact"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-23T06:30:58.430688+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-23T06:30:58.430688+00:00","source":"crossref"},{"observed_at":"2026-08-23T06:30:53.778098+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":"2505.09715","doi":null,"metadata_source":"arxiv_reference","pith_arxiv_id":null,"snapshot_observed_at":"2026-07-08T21:15:39.190572Z","title":"Vicente, T","venue":null,"work_id":"2a12c126-2c21-4ccf-973f-70df123c8e5d","year":2025},"citing_paper":{"arxiv_id":"2607.05909","last_updated":"2026-07-07T07:04:03Z","snapshot_observed_at":"2026-08-14T10:29:50.174311Z","submitted_at":"2026-07-07T07:04:03Z","title":"Probing near-zone magnetic fields with extreme mass-ratio inspirals","version":1},"reference_index":38,"source":"pdf_text","source_observed_at":"2026-07-08T21:06:26.923131Z"},"links":{"citing_paper":"/paper/2607.05909"},"observation_digest":"sha256:bfe259ce879c61819f22299a230b25eed43dd495ec858bd2e59f56f42dcee33c","observation_id":"454c7039-ab0a-475f-8b57-db07fcd182d7","resolution":{"observed_at":"2026-07-08T21:15:39.191907Z","resolver_source":"arxiv_id","status":"verified_exact"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-23T06:30:58.430688+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-23T06:30:58.430688+00:00","source":"crossref"},{"observed_at":"2026-08-23T06:30:53.778098+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":"2026-07-08T21:15:39.436962Z","title":null,"venue":null,"work_id":"904f7ba6-c255-4509-8dc4-8dce9a6b75d3","year":2025},"citing_paper":{"arxiv_id":"2607.05909","last_updated":"2026-07-07T07:04:03Z","snapshot_observed_at":"2026-08-14T10:29:50.174311Z","submitted_at":"2026-07-07T07:04:03Z","title":"Probing near-zone magnetic fields with extreme mass-ratio inspirals","version":1},"reference_index":39,"source":"pdf_text","source_observed_at":"2026-07-08T21:06:26.923131Z"},"links":{"citing_paper":"/paper/2607.05909"},"observation_digest":"sha256:f87ad3a47c06db016522211697b68e3e226affd1076bd347647acd39d3b63808","observation_id":"57580d22-c4c2-4147-b41d-bfe73332228a","resolution":{"observed_at":"2026-07-08T21:15:39.438383Z","resolver_source":"raw_fallback","status":"unresolved"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-23T06:30:58.430688+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-23T06:30:58.430688+00:00","source":"crossref"},{"observed_at":"2026-08-23T06:30:53.778098+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":"2507.15720","doi":null,"metadata_source":"arxiv_reference","pith_arxiv_id":null,"snapshot_observed_at":"2026-07-08T21:15:39.115787Z","title":"Polcar and V","venue":null,"work_id":"0f181c3b-6fc7-4fdb-aac8-cb3c174e427c","year":2025},"citing_paper":{"arxiv_id":"2607.05909","last_updated":"2026-07-07T07:04:03Z","snapshot_observed_at":"2026-08-14T10:29:50.174311Z","submitted_at":"2026-07-07T07:04:03Z","title":"Probing near-zone magnetic fields with extreme mass-ratio inspirals","version":1},"reference_index":40,"source":"pdf_text","source_observed_at":"2026-07-08T21:06:26.923131Z"},"links":{"citing_paper":"/paper/2607.05909"},"observation_digest":"sha256:467a8aa365982cc8dd8f3e4e21d4239578e6ca545cd74065601a0be644b319b3","observation_id":"f01baceb-3079-40f3-ae94-ebac68495567","resolution":{"observed_at":"2026-07-08T21:15:39.117143Z","resolver_source":"arxiv_id","status":"verified_exact"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-23T06:30:58.430688+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-23T06:30:58.430688+00:00","source":"crossref"},{"observed_at":"2026-08-23T06:30:53.778098+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":"2510.17398","doi":null,"metadata_source":"arxiv_reference","pith_arxiv_id":null,"snapshot_observed_at":"2026-07-08T21:15:39.118207Z","title":"Kejriwal, E","venue":null,"work_id":"97a7795f-1541-48a5-ac02-08f321d36dd9","year":2026},"citing_paper":{"arxiv_id":"2607.05909","last_updated":"2026-07-07T07:04:03Z","snapshot_observed_at":"2026-08-14T10:29:50.174311Z","submitted_at":"2026-07-07T07:04:03Z","title":"Probing near-zone magnetic fields with extreme mass-ratio inspirals","version":1},"reference_index":41,"source":"pdf_text","source_observed_at":"2026-07-08T21:06:26.923131Z"},"links":{"citing_paper":"/paper/2607.05909"},"observation_digest":"sha256:7d6c40925cf7fa5712fc4d26bce91c9a72c78782d776e2b9e6dac347a0ef4f7b","observation_id":"eacdb570-68be-42c9-9843-c86979f18c5a","resolution":{"observed_at":"2026-07-08T21:15:39.119548Z","resolver_source":"arxiv_id","status":"verified_exact"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-23T06:30:58.430688+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-23T06:30:58.430688+00:00","source":"crossref"},{"observed_at":"2026-08-23T06:30:53.778098+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":{"arxiv_id":"2502.20138","last_updated":"2026-05-25T10:43:21Z","snapshot_observed_at":"2026-08-20T04:09:23.790872Z","submitted_at":"2025-02-27T14:31:17Z","title":"Fundamental Physics and Cosmology with TianQin","version":2},"cited_work":{"arxiv_id":"2502.20138","doi":null,"metadata_source":"pith","pith_arxiv_id":"2502.20138","snapshot_observed_at":"2026-07-10T22:27:37.048467Z","title":"Luo et al","venue":"gr-qc","work_id":"0644d710-91f8-480f-b116-aeed0a397d98","year":2025},"citing_paper":{"arxiv_id":"2607.05909","last_updated":"2026-07-07T07:04:03Z","snapshot_observed_at":"2026-08-14T10:29:50.174311Z","submitted_at":"2026-07-07T07:04:03Z","title":"Probing near-zone magnetic fields with extreme mass-ratio inspirals","version":1},"reference_index":42,"source":"pdf_text","source_observed_at":"2026-07-08T21:06:26.923131Z"},"links":{"cited_paper":"/paper/2502.20138","citing_paper":"/paper/2607.05909"},"observation_digest":"sha256:a421ca9948e869ed349680abce9c11d2978c9ddb64f3e0923a7e45fd39b40e1b","observation_id":"45616a6a-ca45-4076-adbb-5b32f668e4b2","resolution":{"observed_at":"2026-07-08T21:15:39.137412Z","resolver_source":"local_arxiv","status":"verified_exact"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-23T06:30:58.430688+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-23T06:30:58.430688+00:00","source":"crossref"},{"observed_at":"2026-08-23T06:30:53.778098+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":{"arxiv_id":"2501.09806","last_updated":"2025-01-16T19:32:12Z","snapshot_observed_at":"2026-08-20T08:55:09.565662Z","submitted_at":"2025-01-16T19:32:12Z","title":"Environmental effects in extreme mass ratio inspirals: perturbations to the environment in Kerr","version":1},"cited_work":{"arxiv_id":"2501.09806","doi":null,"metadata_source":"pith","pith_arxiv_id":"2501.09806","snapshot_observed_at":"2026-07-08T21:15:39.211997Z","title":"Dyson, T","venue":"gr-qc","work_id":"66c4da66-6f77-44ec-a68c-2c872d278c07","year":2025},"citing_paper":{"arxiv_id":"2607.05909","last_updated":"2026-07-07T07:04:03Z","snapshot_observed_at":"2026-08-14T10:29:50.174311Z","submitted_at":"2026-07-07T07:04:03Z","title":"Probing near-zone magnetic fields with extreme mass-ratio inspirals","version":1},"reference_index":43,"source":"pdf_text","source_observed_at":"2026-07-08T21:06:26.923131Z"},"links":{"cited_paper":"/paper/2501.09806","citing_paper":"/paper/2607.05909"},"observation_digest":"sha256:e29b6fa6a833dedafb26afdb1ebfaea1763a775e834e0c2e915b2cb4718e86a4","observation_id":"715b33e8-5fe7-4924-a6b6-f053f944673d","resolution":{"observed_at":"2026-07-08T21:15:39.213237Z","resolver_source":"local_arxiv","status":"verified_exact"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-23T06:30:58.430688+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-23T06:30:58.430688+00:00","source":"crossref"},{"observed_at":"2026-08-23T06:30:53.778098+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":{"arxiv_id":"2502.09171","last_updated":"2025-08-28T13:56:48Z","snapshot_observed_at":"2026-08-20T02:21:31.790178Z","submitted_at":"2025-02-13T10:54:45Z","title":"Periodic orbits and their gravitational wave radiations in black hole with dark matter halo","version":2},"cited_work":{"arxiv_id":"2502.09171","doi":null,"metadata_source":"pith","pith_arxiv_id":"2502.09171","snapshot_observed_at":"2026-07-08T21:15:39.182638Z","title":"Periodic orbits and their gravi- tational wave radiations in black hole with dark matter halo","venue":"gr-qc","work_id":"886bcb4f-0f5e-4d16-bc55-d42a232dfac2","year":2025},"citing_paper":{"arxiv_id":"2607.05909","last_updated":"2026-07-07T07:04:03Z","snapshot_observed_at":"2026-08-14T10:29:50.174311Z","submitted_at":"2026-07-07T07:04:03Z","title":"Probing near-zone magnetic fields with extreme mass-ratio inspirals","version":1},"reference_index":44,"source":"pdf_text","source_observed_at":"2026-07-08T21:06:26.923131Z"},"links":{"cited_paper":"/paper/2502.09171","citing_paper":"/paper/2607.05909"},"observation_digest":"sha256:3b22ff985e1c0d842cbb6bdec0f5602c0fedc677737af4bed3e095341910b6c8","observation_id":"71ddf8cf-1024-406d-b8d0-e0e4e90d76d8","resolution":{"observed_at":"2026-07-08T21:15:39.183926Z","resolver_source":"local_arxiv","status":"verified_exact"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-23T06:30:58.430688+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-23T06:30:58.430688+00:00","source":"crossref"},{"observed_at":"2026-08-23T06:30:53.778098+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":"2512.04848","doi":null,"metadata_source":"arxiv_reference","pith_arxiv_id":null,"snapshot_observed_at":"2026-07-08T21:15:39.209639Z","title":null,"venue":null,"work_id":"95de9fbb-f584-46b7-afd5-9722c3f259a7","year":2025},"citing_paper":{"arxiv_id":"2607.05909","last_updated":"2026-07-07T07:04:03Z","snapshot_observed_at":"2026-08-14T10:29:50.174311Z","submitted_at":"2026-07-07T07:04:03Z","title":"Probing near-zone magnetic fields with extreme mass-ratio inspirals","version":1},"reference_index":45,"source":"pdf_text","source_observed_at":"2026-07-08T21:06:26.923131Z"},"links":{"citing_paper":"/paper/2607.05909"},"observation_digest":"sha256:81cdf54ffea14f30dd713f94166aeb373e1a5822d148fd1f928b07d7fdc3e7bd","observation_id":"9bf1da52-7d3b-413e-a937-266ead4eea73","resolution":{"observed_at":"2026-07-08T21:15:39.210908Z","resolver_source":"arxiv_id","status":"verified_exact"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-23T06:30:58.430688+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-23T06:30:58.430688+00:00","source":"crossref"},{"observed_at":"2026-08-23T06:30:53.778098+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":"2507.06923","doi":null,"metadata_source":"arxiv_reference","pith_arxiv_id":null,"snapshot_observed_at":"2026-07-08T21:15:39.236359Z","title":"Rahman and T","venue":null,"work_id":"1413ea2d-b1f7-41f4-be71-b8a83875184a","year":2026},"citing_paper":{"arxiv_id":"2607.05909","last_updated":"2026-07-07T07:04:03Z","snapshot_observed_at":"2026-08-14T10:29:50.174311Z","submitted_at":"2026-07-07T07:04:03Z","title":"Probing near-zone magnetic fields with extreme mass-ratio inspirals","version":1},"reference_index":46,"source":"pdf_text","source_observed_at":"2026-07-08T21:06:26.923131Z"},"links":{"citing_paper":"/paper/2607.05909"},"observation_digest":"sha256:6cc809b4993ffee43eb4563dc82deaaef7df1c9a70e2bf09c6e13a9d07662bd3","observation_id":"0ce41bd1-361c-4513-85ab-6e6f1760174f","resolution":{"observed_at":"2026-07-08T21:15:39.237663Z","resolver_source":"arxiv_id","status":"verified_exact"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-23T06:30:58.430688+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-23T06:30:58.430688+00:00","source":"crossref"},{"observed_at":"2026-08-23T06:30:53.778098+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":"2509.20457","doi":null,"metadata_source":"arxiv_reference","pith_arxiv_id":null,"snapshot_observed_at":"2026-07-08T21:15:39.243870Z","title":"Hegade K","venue":null,"work_id":"1633e2f3-a11c-4d56-89cd-d84d50178879","year":2025},"citing_paper":{"arxiv_id":"2607.05909","last_updated":"2026-07-07T07:04:03Z","snapshot_observed_at":"2026-08-14T10:29:50.174311Z","submitted_at":"2026-07-07T07:04:03Z","title":"Probing near-zone magnetic fields with extreme mass-ratio inspirals","version":1},"reference_index":47,"source":"pdf_text","source_observed_at":"2026-07-08T21:06:26.923131Z"},"links":{"citing_paper":"/paper/2607.05909"},"observation_digest":"sha256:275755c2d85d03170c51ddb861bf8a6f580f8947d1068cd021658c97f6e1111f","observation_id":"ac496826-db0a-48fa-b2e1-34affb229a90","resolution":{"observed_at":"2026-07-08T21:15:39.245136Z","resolver_source":"arxiv_id","status":"verified_exact"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-23T06:30:58.430688+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-23T06:30:58.430688+00:00","source":"crossref"},{"observed_at":"2026-08-23T06:30:53.778098+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":"2602.12022","doi":null,"metadata_source":"arxiv_reference","pith_arxiv_id":null,"snapshot_observed_at":"2026-07-08T21:15:39.177115Z","title":"Zhao and Y","venue":null,"work_id":"7191d4fa-a3dc-4891-b074-e5ac59b6bf0c","year":2026},"citing_paper":{"arxiv_id":"2607.05909","last_updated":"2026-07-07T07:04:03Z","snapshot_observed_at":"2026-08-14T10:29:50.174311Z","submitted_at":"2026-07-07T07:04:03Z","title":"Probing near-zone magnetic fields with extreme mass-ratio inspirals","version":1},"reference_index":48,"source":"pdf_text","source_observed_at":"2026-07-08T21:06:26.923131Z"},"links":{"citing_paper":"/paper/2607.05909"},"observation_digest":"sha256:5f8789de3e418a11a7743664808ac661c7ca522e8b021a700921f0985c8856c9","observation_id":"15879fbe-1a70-4146-b909-7ea99bae1c90","resolution":{"observed_at":"2026-07-08T21:15:39.178396Z","resolver_source":"arxiv_id","status":"verified_exact"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-23T06:30:58.430688+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-23T06:30:58.430688+00:00","source":"crossref"},{"observed_at":"2026-08-23T06:30:53.778098+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":"2601.03374","doi":null,"metadata_source":"arxiv_reference","pith_arxiv_id":null,"snapshot_observed_at":"2026-07-08T21:15:39.219058Z","title":"Probing beyond-vacuum general relativistic effects with extreme mass-ratio inspirals,","venue":null,"work_id":"2f777945-50ec-4e04-9192-a005a9c918b3","year":2026},"citing_paper":{"arxiv_id":"2607.05909","last_updated":"2026-07-07T07:04:03Z","snapshot_observed_at":"2026-08-14T10:29:50.174311Z","submitted_at":"2026-07-07T07:04:03Z","title":"Probing near-zone magnetic fields with extreme mass-ratio inspirals","version":1},"reference_index":49,"source":"pdf_text","source_observed_at":"2026-07-08T21:06:26.923131Z"},"links":{"citing_paper":"/paper/2607.05909"},"observation_digest":"sha256:1505146669acd4f109b482ed1f2ea497599dbe642ad7d7dd75acae5a241fbd9c","observation_id":"170f2b88-d1ce-49b8-8d09-81ae4e6730d4","resolution":{"observed_at":"2026-07-08T21:15:39.220462Z","resolver_source":"arxiv_id","status":"verified_exact"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-23T06:30:58.430688+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-23T06:30:58.430688+00:00","source":"crossref"},{"observed_at":"2026-08-23T06:30:53.778098+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":{"arxiv_id":"2602.19541","last_updated":"2026-06-29T16:28:05Z","snapshot_observed_at":"2026-08-21T23:10:17.569877Z","submitted_at":"2026-02-23T06:29:03Z","title":"Chaotic imprints of dark matter in extreme mass-ratio inspirals","version":2},"cited_work":{"arxiv_id":"2602.19541","doi":null,"metadata_source":"pith","pith_arxiv_id":"2602.19541","snapshot_observed_at":"2026-07-08T21:15:39.221619Z","title":"Chaotic imprints of dark matter in extreme mass-ratio inspirals","venue":"gr-qc","work_id":"91557ec1-4a94-411a-80aa-8d194c12509e","year":2026},"citing_paper":{"arxiv_id":"2607.05909","last_updated":"2026-07-07T07:04:03Z","snapshot_observed_at":"2026-08-14T10:29:50.174311Z","submitted_at":"2026-07-07T07:04:03Z","title":"Probing near-zone magnetic fields with extreme mass-ratio inspirals","version":1},"reference_index":50,"source":"pdf_text","source_observed_at":"2026-07-08T21:06:26.923131Z"},"links":{"cited_paper":"/paper/2602.19541","citing_paper":"/paper/2607.05909"},"observation_digest":"sha256:8f09a1a7a422486dc92f2701da37da87bdd29d4a851c8919deeda072c2c513e8","observation_id":"422dbf64-ae2d-4716-9ff5-2a7d48fac423","resolution":{"observed_at":"2026-07-08T21:15:39.222833Z","resolver_source":"local_arxiv","status":"verified_exact"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-23T06:30:58.430688+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-23T06:30:58.430688+00:00","source":"crossref"},{"observed_at":"2026-08-23T06:30:53.778098+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":"2026-07-08T21:15:39.476596Z","title":null,"venue":null,"work_id":"454abd80-8f78-479a-ab5d-0eae68268cd5","year":1975},"citing_paper":{"arxiv_id":"2607.05909","last_updated":"2026-07-07T07:04:03Z","snapshot_observed_at":"2026-08-14T10:29:50.174311Z","submitted_at":"2026-07-07T07:04:03Z","title":"Probing near-zone magnetic fields with extreme mass-ratio inspirals","version":1},"reference_index":51,"source":"pdf_text","source_observed_at":"2026-07-08T21:06:26.923131Z"},"links":{"citing_paper":"/paper/2607.05909"},"observation_digest":"sha256:7a9cad956b521d2db278553b74cb56bc5754fe7d9776bc8865267e6cb5d24a39","observation_id":"f2e6aff2-cc9e-40c4-8a8e-0ac37f4fd849","resolution":{"observed_at":"2026-07-08T21:15:39.477679Z","resolver_source":"raw_fallback","status":"unresolved"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-23T06:30:58.430688+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-23T06:30:58.430688+00:00","source":"crossref"},{"observed_at":"2026-08-23T06:30:53.778098+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":"2026-07-08T21:15:39.447177Z","title":null,"venue":null,"work_id":"64496fd3-0dd0-4553-a1d0-5c64cdc330b7","year":1977},"citing_paper":{"arxiv_id":"2607.05909","last_updated":"2026-07-07T07:04:03Z","snapshot_observed_at":"2026-08-14T10:29:50.174311Z","submitted_at":"2026-07-07T07:04:03Z","title":"Probing near-zone magnetic fields with extreme mass-ratio inspirals","version":1},"reference_index":52,"source":"pdf_text","source_observed_at":"2026-07-08T21:06:26.923131Z"},"links":{"citing_paper":"/paper/2607.05909"},"observation_digest":"sha256:8fc890462594602771126a79c36d6318aa60919dc5943b3912f189b5169d953f","observation_id":"9e2f32b6-913f-413c-9f54-db0c9c7621f4","resolution":{"observed_at":"2026-07-08T21:15:39.449535Z","resolver_source":"raw_fallback","status":"unresolved"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-23T06:30:58.430688+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-23T06:30:58.430688+00:00","source":"crossref"},{"observed_at":"2026-08-23T06:30:53.778098+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":{"arxiv_id":"2105.01169","last_updated":"2021-05-03T21:12:04Z","snapshot_observed_at":"2026-08-19T04:43:09.989457Z","submitted_at":"2021-05-03T21:12:04Z","title":"First M87 Event Horizon Telescope Results. VII. Polarization of the Ring","version":1},"cited_work":{"arxiv_id":"2105.01169","doi":null,"metadata_source":"pith","pith_arxiv_id":"2105.01169","snapshot_observed_at":"2026-07-08T21:15:39.207270Z","title":"First M87 Event Horizon Telescope Results. VII. Polariza- tion of the Ring","venue":"astro-ph.HE","work_id":"455e4c9f-bcf5-4d02-96cd-a12b0f54d52c","year":2021},"citing_paper":{"arxiv_id":"2607.05909","last_updated":"2026-07-07T07:04:03Z","snapshot_observed_at":"2026-08-14T10:29:50.174311Z","submitted_at":"2026-07-07T07:04:03Z","title":"Probing near-zone magnetic fields with extreme mass-ratio inspirals","version":1},"reference_index":53,"source":"pdf_text","source_observed_at":"2026-07-08T21:06:26.923131Z"},"links":{"cited_paper":"/paper/2105.01169","citing_paper":"/paper/2607.05909"},"observation_digest":"sha256:22153d3421206637e5e3a230aceb44fdf013ada89cb0fc9e6315abeb70ba2f24","observation_id":"8ce1cbed-6d9b-4717-9f2a-dc6e847f8cf2","resolution":{"observed_at":"2026-07-08T21:15:39.208506Z","resolver_source":"local_arxiv","status":"verified_exact"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-23T06:30:58.430688+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-23T06:30:58.430688+00:00","source":"crossref"},{"observed_at":"2026-08-23T06:30:53.778098+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":{"arxiv_id":"2105.01173","last_updated":"2021-05-05T12:39:47Z","snapshot_observed_at":"2026-08-19T20:44:55.211814Z","submitted_at":"2021-05-03T21:22:13Z","title":"First M87 Event Horizon Telescope Results. VIII. Magnetic Field Structure near The Event Horizon","version":2},"cited_work":{"arxiv_id":"2105.01173","doi":null,"metadata_source":"pith","pith_arxiv_id":"2105.01173","snapshot_observed_at":"2026-07-08T21:15:39.193060Z","title":"Akiyama et al","venue":"astro-ph.HE","work_id":"cfa0b111-14c8-4001-9ab3-52e562b247a1","year":2021},"citing_paper":{"arxiv_id":"2607.05909","last_updated":"2026-07-07T07:04:03Z","snapshot_observed_at":"2026-08-14T10:29:50.174311Z","submitted_at":"2026-07-07T07:04:03Z","title":"Probing near-zone magnetic fields with extreme mass-ratio inspirals","version":1},"reference_index":54,"source":"pdf_text","source_observed_at":"2026-07-08T21:06:26.923131Z"},"links":{"cited_paper":"/paper/2105.01173","citing_paper":"/paper/2607.05909"},"observation_digest":"sha256:7bf73c8a53d36f53aee620054ca913f1e4c74bb935835864c0ca2164c41e1e37","observation_id":"4ea06c0a-4821-4223-bee1-79262cdac47b","resolution":{"observed_at":"2026-07-08T21:15:39.194272Z","resolver_source":"local_arxiv","status":"verified_exact"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-23T06:30:58.430688+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-23T06:30:58.430688+00:00","source":"crossref"},{"observed_at":"2026-08-23T06:30:53.778098+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":{"arxiv_id":"1308.3147","last_updated":"2013-08-14T14:56:26Z","snapshot_observed_at":"2026-08-18T01:16:05.472000Z","submitted_at":"2013-08-14T14:56:26Z","title":"A strong magnetic field around the supermassive black hole at the centre of the Galaxy","version":1},"cited_work":{"arxiv_id":"1308.3147","doi":null,"metadata_source":"pith","pith_arxiv_id":"1308.3147","snapshot_observed_at":"2026-07-08T21:15:39.241488Z","title":"A strong magnetic field around the supermassive black hole at the centre of the Galaxy","venue":"astro-ph.GA","work_id":"55cd30b5-ae8c-4578-8dab-c99e4e62f71a","year":2013},"citing_paper":{"arxiv_id":"2607.05909","last_updated":"2026-07-07T07:04:03Z","snapshot_observed_at":"2026-08-14T10:29:50.174311Z","submitted_at":"2026-07-07T07:04:03Z","title":"Probing near-zone magnetic fields with extreme mass-ratio inspirals","version":1},"reference_index":55,"source":"pdf_text","source_observed_at":"2026-07-08T21:06:26.923131Z"},"links":{"cited_paper":"/paper/1308.3147","citing_paper":"/paper/2607.05909"},"observation_digest":"sha256:5c2a5dba8f482590e2230ec9bc0102520dcf038fda8aed053d5c63a8c290e604","observation_id":"193c0549-f6ef-4afd-a4d0-1be629dd796f","resolution":{"observed_at":"2026-07-08T21:15:39.242735Z","resolver_source":"local_arxiv","status":"verified_exact"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-23T06:30:58.430688+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-23T06:30:58.430688+00:00","source":"crossref"},{"observed_at":"2026-08-23T06:30:53.778098+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":{"arxiv_id":"1212.2040","last_updated":"2012-12-10T11:58:15Z","snapshot_observed_at":"2026-08-15T00:36:35.459752Z","submitted_at":"2012-12-10T11:58:15Z","title":"The magnetic field in the X-ray corona of Cygnus X-1","version":1},"cited_work":{"arxiv_id":"1212.2040","doi":null,"metadata_source":"pith","pith_arxiv_id":"1212.2040","snapshot_observed_at":"2026-07-08T21:15:39.164709Z","title":"The magnetic field in the X-ray corona of Cygnus X-1","venue":"astro-ph.HE","work_id":"6ec067d7-c1c3-4cad-b098-c53322d97072","year":2012},"citing_paper":{"arxiv_id":"2607.05909","last_updated":"2026-07-07T07:04:03Z","snapshot_observed_at":"2026-08-14T10:29:50.174311Z","submitted_at":"2026-07-07T07:04:03Z","title":"Probing near-zone magnetic fields with extreme mass-ratio inspirals","version":1},"reference_index":56,"source":"pdf_text","source_observed_at":"2026-07-08T21:06:26.923131Z"},"links":{"cited_paper":"/paper/1212.2040","citing_paper":"/paper/2607.05909"},"observation_digest":"sha256:20dcc7793933955e764268de09e1888f5587444e195573651f4a6ebf7ce1cdc5","observation_id":"b7320b5b-f750-4db9-89b6-7053c5ac548d","resolution":{"observed_at":"2026-07-08T21:15:39.166077Z","resolver_source":"local_arxiv","status":"verified_exact"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-23T06:30:58.430688+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-23T06:30:58.430688+00:00","source":"crossref"},{"observed_at":"2026-08-23T06:30:53.778098+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":"2026-07-08T21:15:39.460591Z","title":null,"venue":null,"work_id":"ccc92532-6d01-47da-b900-3b14fdcb0448","year":1976},"citing_paper":{"arxiv_id":"2607.05909","last_updated":"2026-07-07T07:04:03Z","snapshot_observed_at":"2026-08-14T10:29:50.174311Z","submitted_at":"2026-07-07T07:04:03Z","title":"Probing near-zone magnetic fields with extreme mass-ratio inspirals","version":1},"reference_index":57,"source":"pdf_text","source_observed_at":"2026-07-08T21:06:26.923131Z"},"links":{"citing_paper":"/paper/2607.05909"},"observation_digest":"sha256:03d638bfc3cf94a6283d4706656308ae839dc72c661d63d6e53b9bc6e7862fbc","observation_id":"4186c88e-b925-473c-ad37-2755a6902238","resolution":{"observed_at":"2026-07-08T21:15:39.462566Z","resolver_source":"raw_fallback","status":"unresolved"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-23T06:30:58.430688+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-23T06:30:58.430688+00:00","source":"crossref"},{"observed_at":"2026-08-23T06:30:53.778098+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":"2026-07-08T21:15:39.463624Z","title":null,"venue":null,"work_id":"95b18426-4fdf-49f7-a328-0cdc8c9564fe","year":1964},"citing_paper":{"arxiv_id":"2607.05909","last_updated":"2026-07-07T07:04:03Z","snapshot_observed_at":"2026-08-14T10:29:50.174311Z","submitted_at":"2026-07-07T07:04:03Z","title":"Probing near-zone magnetic fields with extreme mass-ratio inspirals","version":1},"reference_index":58,"source":"pdf_text","source_observed_at":"2026-07-08T21:06:26.923131Z"},"links":{"citing_paper":"/paper/2607.05909"},"observation_digest":"sha256:d89668bfe5f7c8cd2daa4d5ec029acdbf3951b48e095ad1e4eb606dbe3cc3939","observation_id":"44964352-7eb0-4118-9891-2b22d8f05d32","resolution":{"observed_at":"2026-07-08T21:15:39.468046Z","resolver_source":"raw_fallback","status":"unresolved"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-23T06:30:58.430688+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-23T06:30:58.430688+00:00","source":"crossref"},{"observed_at":"2026-08-23T06:30:53.778098+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":"2026-07-08T21:15:39.474390Z","title":null,"venue":null,"work_id":"801e8b01-8470-47d0-9224-0871fbc69777","year":1968},"citing_paper":{"arxiv_id":"2607.05909","last_updated":"2026-07-07T07:04:03Z","snapshot_observed_at":"2026-08-14T10:29:50.174311Z","submitted_at":"2026-07-07T07:04:03Z","title":"Probing near-zone magnetic fields with extreme mass-ratio inspirals","version":1},"reference_index":59,"source":"pdf_text","source_observed_at":"2026-07-08T21:06:26.923131Z"},"links":{"citing_paper":"/paper/2607.05909"},"observation_digest":"sha256:f78e444a7d0866a26c698c4e358a3cc5a266fdc4a809f0f47cdfb2d284447c42","observation_id":"8fc76a94-5b42-484e-ab6b-7a13aea4b8dd","resolution":{"observed_at":"2026-07-08T21:15:39.475807Z","resolver_source":"raw_fallback","status":"unresolved"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-23T06:30:58.430688+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-23T06:30:58.430688+00:00","source":"crossref"},{"observed_at":"2026-08-23T06:30:53.778098+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":"2026-07-08T21:15:39.456320Z","title":null,"venue":null,"work_id":"d0e9fe1e-30fe-431c-9531-2c3cd166e6d4","year":1976},"citing_paper":{"arxiv_id":"2607.05909","last_updated":"2026-07-07T07:04:03Z","snapshot_observed_at":"2026-08-14T10:29:50.174311Z","submitted_at":"2026-07-07T07:04:03Z","title":"Probing near-zone magnetic fields with extreme mass-ratio inspirals","version":1},"reference_index":60,"source":"pdf_text","source_observed_at":"2026-07-08T21:06:26.923131Z"},"links":{"citing_paper":"/paper/2607.05909"},"observation_digest":"sha256:2cade0a6cb5fb7b81d005cb5f19437ff7eea04ef4f4fbc0541c72434c425c8ff","observation_id":"ca6e2ff2-70c6-4fbc-aa8e-47343c37d558","resolution":{"observed_at":"2026-07-08T21:15:39.457896Z","resolver_source":"raw_fallback","status":"unresolved"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-23T06:30:58.430688+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-23T06:30:58.430688+00:00","source":"crossref"},{"observed_at":"2026-08-23T06:30:53.778098+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":{"arxiv_id":"2011.13586","last_updated":"2021-12-01T03:37:57Z","snapshot_observed_at":"2026-08-19T18:51:02.788005Z","submitted_at":"2020-11-27T07:23:23Z","title":"Gravitational and electromagnetic radiation from binary black holes with electric and magnetic charges: Elliptical orbits on a cone","version":2},"cited_work":{"arxiv_id":"2011.13586","doi":null,"metadata_source":"pith","pith_arxiv_id":"2011.13586","snapshot_observed_at":"2026-07-08T21:15:39.095883Z","title":"Gravitational and electromagnetic radiation from binary black holes with electric and magnetic charges: Elliptical orbits on a cone","venue":"gr-qc","work_id":"780c2547-da7c-4b6a-bc76-1e39d69927a9","year":2020},"citing_paper":{"arxiv_id":"2607.05909","last_updated":"2026-07-07T07:04:03Z","snapshot_observed_at":"2026-08-14T10:29:50.174311Z","submitted_at":"2026-07-07T07:04:03Z","title":"Probing near-zone magnetic fields with extreme mass-ratio inspirals","version":1},"reference_index":61,"source":"pdf_text","source_observed_at":"2026-07-08T21:06:26.923131Z"},"links":{"cited_paper":"/paper/2011.13586","citing_paper":"/paper/2607.05909"},"observation_digest":"sha256:95e0d8b4fbf77f1a4c21f3208912c35be334e90363dc5e46a2061fa152111be3","observation_id":"4e20b5ae-ea76-4015-8352-5b8f9785f902","resolution":{"observed_at":"2026-07-08T21:15:39.097140Z","resolver_source":"local_arxiv","status":"verified_exact"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-23T06:30:58.430688+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-23T06:30:58.430688+00:00","source":"crossref"},{"observed_at":"2026-08-23T06:30:53.778098+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":{"arxiv_id":"2406.03371","last_updated":"2024-10-31T17:16:48Z","snapshot_observed_at":"2026-08-16T13:45:50.531220Z","submitted_at":"2024-06-05T15:25:16Z","title":"Orbits of particles with magnetic dipole moment around magnetized Schwarzschild black holes: Applications to S2 star orbit","version":2},"cited_work":{"arxiv_id":"2406.03371","doi":null,"metadata_source":"pith","pith_arxiv_id":"2406.03371","snapshot_observed_at":"2026-07-08T21:15:39.122998Z","title":"Orbits of particles with magnetic dipole moment around magnetized Schwarzschild black holes: Applications to S2 star orbit","venue":"gr-qc","work_id":"7ac83bb4-a54e-4899-b6f8-45b856def8f3","year":2024},"citing_paper":{"arxiv_id":"2607.05909","last_updated":"2026-07-07T07:04:03Z","snapshot_observed_at":"2026-08-14T10:29:50.174311Z","submitted_at":"2026-07-07T07:04:03Z","title":"Probing near-zone magnetic fields with extreme mass-ratio inspirals","version":1},"reference_index":62,"source":"pdf_text","source_observed_at":"2026-07-08T21:06:26.923131Z"},"links":{"cited_paper":"/paper/2406.03371","citing_paper":"/paper/2607.05909"},"observation_digest":"sha256:197ba1219174de868a4cf3c1bb17639c1ba7af50d86cccb64b14015248b402e2","observation_id":"55aa9d37-0a8e-4173-a45f-ca45cc90fe3a","resolution":{"observed_at":"2026-07-08T21:15:39.126385Z","resolver_source":"local_arxiv","status":"verified_exact"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-23T06:30:58.430688+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-23T06:30:58.430688+00:00","source":"crossref"},{"observed_at":"2026-08-23T06:30:53.778098+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":"2507.05199","doi":null,"metadata_source":"arxiv_reference","pith_arxiv_id":null,"snapshot_observed_at":"2026-07-08T21:15:39.246226Z","title":"Podolsky and H","venue":null,"work_id":"d51c0bff-1e54-48c1-8c17-dfd0843b7abc","year":2025},"citing_paper":{"arxiv_id":"2607.05909","last_updated":"2026-07-07T07:04:03Z","snapshot_observed_at":"2026-08-14T10:29:50.174311Z","submitted_at":"2026-07-07T07:04:03Z","title":"Probing near-zone magnetic fields with extreme mass-ratio inspirals","version":1},"reference_index":63,"source":"pdf_text","source_observed_at":"2026-07-08T21:06:26.923131Z"},"links":{"citing_paper":"/paper/2607.05909"},"observation_digest":"sha256:7eeeeb47dc5620940549c752c11f1d1e6317bc1566b005f4432fe5f15d24e67b","observation_id":"99d7fb43-f653-4a97-b983-8465f866085d","resolution":{"observed_at":"2026-07-08T21:15:39.247562Z","resolver_source":"arxiv_id","status":"verified_exact"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-23T06:30:58.430688+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-23T06:30:58.430688+00:00","source":"crossref"},{"observed_at":"2026-08-23T06:30:53.778098+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":"2507.22494","doi":null,"metadata_source":"arxiv_reference","pith_arxiv_id":null,"snapshot_observed_at":"2026-07-08T21:15:39.248837Z","title":"Geodesics and shadows in the Kerr-Bertotti-Robinson black hole space- time,","venue":null,"work_id":"878d7a8e-3555-4d37-bf98-a00ab8a90602","year":2026},"citing_paper":{"arxiv_id":"2607.05909","last_updated":"2026-07-07T07:04:03Z","snapshot_observed_at":"2026-08-14T10:29:50.174311Z","submitted_at":"2026-07-07T07:04:03Z","title":"Probing near-zone magnetic fields with extreme mass-ratio inspirals","version":1},"reference_index":64,"source":"pdf_text","source_observed_at":"2026-07-08T21:06:26.923131Z"},"links":{"citing_paper":"/paper/2607.05909"},"observation_digest":"sha256:990342861237ff6eabfa7dbf3b2c2ef81e00e12e70a60c9644e21fca0bae926e","observation_id":"b146c5cb-176d-41c8-8a7d-d16746966774","resolution":{"observed_at":"2026-07-08T21:15:39.254093Z","resolver_source":"arxiv_id","status":"verified_exact"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-23T06:30:58.430688+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-23T06:30:58.430688+00:00","source":"crossref"},{"observed_at":"2026-08-23T06:30:53.778098+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":"2512.02921","doi":null,"metadata_source":"arxiv_reference","pith_arxiv_id":null,"snapshot_observed_at":"2026-07-08T21:15:39.162242Z","title":"Li, H.-P","venue":null,"work_id":"ff615f3f-fa6e-4758-8418-28960c7e759a","year":2026},"citing_paper":{"arxiv_id":"2607.05909","last_updated":"2026-07-07T07:04:03Z","snapshot_observed_at":"2026-08-14T10:29:50.174311Z","submitted_at":"2026-07-07T07:04:03Z","title":"Probing near-zone magnetic fields with extreme mass-ratio inspirals","version":1},"reference_index":65,"source":"pdf_text","source_observed_at":"2026-07-08T21:06:26.923131Z"},"links":{"citing_paper":"/paper/2607.05909"},"observation_digest":"sha256:63155d4a802b6118d8be4313583dd2d1f6781ccd6ae02112edb89693fdbc1684","observation_id":"68e232f3-defa-4b2f-8f16-a749565fc3a0","resolution":{"observed_at":"2026-07-08T21:15:39.163529Z","resolver_source":"arxiv_id","status":"verified_exact"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-23T06:30:58.430688+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-23T06:30:58.430688+00:00","source":"crossref"},{"observed_at":"2026-08-23T06:30:53.778098+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":"2603.00653","doi":null,"metadata_source":"arxiv_reference","pith_arxiv_id":null,"snapshot_observed_at":"2026-07-08T21:15:39.296973Z","title":null,"venue":null,"work_id":"76708f69-c35d-449f-ba4b-00c52c9d845a","year":2026},"citing_paper":{"arxiv_id":"2607.05909","last_updated":"2026-07-07T07:04:03Z","snapshot_observed_at":"2026-08-14T10:29:50.174311Z","submitted_at":"2026-07-07T07:04:03Z","title":"Probing near-zone magnetic fields with extreme mass-ratio inspirals","version":1},"reference_index":66,"source":"pdf_text","source_observed_at":"2026-07-08T21:06:26.923131Z"},"links":{"citing_paper":"/paper/2607.05909"},"observation_digest":"sha256:bf5da0bbd28521fa5f5f1056cf13246a2ae4e9c792db7d94ef6fd068e6751b0a","observation_id":"77ea0976-5451-43cb-b4a7-a36cb873ffcf","resolution":{"observed_at":"2026-07-08T21:15:39.298382Z","resolver_source":"arxiv_id","status":"verified_exact"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-23T06:30:58.430688+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-23T06:30:58.430688+00:00","source":"crossref"},{"observed_at":"2026-08-23T06:30:53.778098+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":{"arxiv_id":"2507.21777","last_updated":"2025-08-19T07:13:27Z","snapshot_observed_at":"2026-08-19T05:44:00.546033Z","submitted_at":"2025-07-29T13:01:44Z","title":"Energy Extraction From the Kerr-Bertotti-Robinson Black Hole via Magnetic Reconnection under Circular Plasma and Plunging Plasma","version":2},"cited_work":{"arxiv_id":"2507.21777","doi":null,"metadata_source":"pith","pith_arxiv_id":"2507.21777","snapshot_observed_at":"2026-07-08T21:15:39.195480Z","title":"Energy extraction from the Kerr-Bertotti-Robinson black hole via magnetic reconnection in a circular and a plunging plasma","venue":"gr-qc","work_id":"68a0429c-804e-4a5d-83c9-dc2e1e259b0c","year":2025},"citing_paper":{"arxiv_id":"2607.05909","last_updated":"2026-07-07T07:04:03Z","snapshot_observed_at":"2026-08-14T10:29:50.174311Z","submitted_at":"2026-07-07T07:04:03Z","title":"Probing near-zone magnetic fields with extreme mass-ratio inspirals","version":1},"reference_index":67,"source":"pdf_text","source_observed_at":"2026-07-08T21:06:26.923131Z"},"links":{"cited_paper":"/paper/2507.21777","citing_paper":"/paper/2607.05909"},"observation_digest":"sha256:d62e6ec6baac95288ee4f22bdc579358b34417be7669c0bd1d1c2a77c67a1c4d","observation_id":"1aaf4375-36a6-4410-afd9-e965d71baeee","resolution":{"observed_at":"2026-07-08T21:15:39.196826Z","resolver_source":"local_arxiv","status":"verified_exact"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-23T06:30:58.430688+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-23T06:30:58.430688+00:00","source":"crossref"},{"observed_at":"2026-08-23T06:30:53.778098+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":"2512.04806","doi":null,"metadata_source":"arxiv_reference","pith_arxiv_id":null,"snapshot_observed_at":"2026-07-08T21:15:39.187522Z","title":"Inspiraling binary charged black holes in an external magnetic field: Appli- cation of post-newtonian dynamics in einstein-maxwell theory","venue":null,"work_id":"d4df7dff-49c7-4bac-9432-16171412d723","year":2026},"citing_paper":{"arxiv_id":"2607.05909","last_updated":"2026-07-07T07:04:03Z","snapshot_observed_at":"2026-08-14T10:29:50.174311Z","submitted_at":"2026-07-07T07:04:03Z","title":"Probing near-zone magnetic fields with extreme mass-ratio inspirals","version":1},"reference_index":68,"source":"pdf_text","source_observed_at":"2026-07-08T21:06:26.923131Z"},"links":{"citing_paper":"/paper/2607.05909"},"observation_digest":"sha256:a30172d955d846b233912b267934a4929407449d5c37cf2fc8482210fe3a6acc","observation_id":"16d23e9d-0ba2-473b-a265-26f49b27381e","resolution":{"observed_at":"2026-07-08T21:15:39.189032Z","resolver_source":"arxiv_id","status":"verified_exact"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-23T06:30:58.430688+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-23T06:30:58.430688+00:00","source":"crossref"},{"observed_at":"2026-08-23T06:30:53.778098+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":"2602.03161","doi":null,"metadata_source":"arxiv_reference","pith_arxiv_id":null,"snapshot_observed_at":"2026-07-08T21:15:39.098241Z","title":"Wang, X.-C","venue":null,"work_id":"ce639e48-6d48-41d2-a257-2cdc6f8bbe8c","year":2026},"citing_paper":{"arxiv_id":"2607.05909","last_updated":"2026-07-07T07:04:03Z","snapshot_observed_at":"2026-08-14T10:29:50.174311Z","submitted_at":"2026-07-07T07:04:03Z","title":"Probing near-zone magnetic fields with extreme mass-ratio inspirals","version":1},"reference_index":69,"source":"pdf_text","source_observed_at":"2026-07-08T21:06:26.923131Z"},"links":{"citing_paper":"/paper/2607.05909"},"observation_digest":"sha256:2d76036e5686fc304a5d1a2421e25e5b913b0d00df9a037e23fc231760e4c91c","observation_id":"fe218a46-8c6f-4fc1-9166-9ad4d30df28f","resolution":{"observed_at":"2026-07-08T21:15:39.099487Z","resolver_source":"arxiv_id","status":"verified_exact"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-23T06:30:58.430688+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-23T06:30:58.430688+00:00","source":"crossref"},{"observed_at":"2026-08-23T06:30:53.778098+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":{"arxiv_id":"2511.06017","last_updated":"2026-05-23T11:35:15Z","snapshot_observed_at":"2026-08-20T03:41:16.953177Z","submitted_at":"2025-11-08T14:09:16Z","title":"A Universal Framework for Horizon-Scale Tests of Gravity with Black Hole Shadows","version":3},"cited_work":{"arxiv_id":"2511.06017","doi":null,"metadata_source":"pith","pith_arxiv_id":"2511.06017","snapshot_observed_at":"2026-07-08T21:15:39.292069Z","title":"A Universal Framework for Horizon-Scale Tests of Gravity with Black Hole Shadows","venue":"gr-qc","work_id":"792c95b9-9cd5-4318-a2c3-b0c537e91c65","year":2025},"citing_paper":{"arxiv_id":"2607.05909","last_updated":"2026-07-07T07:04:03Z","snapshot_observed_at":"2026-08-14T10:29:50.174311Z","submitted_at":"2026-07-07T07:04:03Z","title":"Probing near-zone magnetic fields with extreme mass-ratio inspirals","version":1},"reference_index":70,"source":"pdf_text","source_observed_at":"2026-07-08T21:06:26.923131Z"},"links":{"cited_paper":"/paper/2511.06017","citing_paper":"/paper/2607.05909"},"observation_digest":"sha256:3c96a83f595d197c32b295ba18e0c1dbe6ec4f368be6435801e2ce385f5fee5d","observation_id":"51c5a74c-1764-4b84-a9b6-15a6b235532b","resolution":{"observed_at":"2026-07-08T21:15:39.293277Z","resolver_source":"local_arxiv","status":"verified_exact"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-23T06:30:58.430688+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-23T06:30:58.430688+00:00","source":"crossref"},{"observed_at":"2026-08-23T06:30:53.778098+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":"2510.07914","doi":null,"metadata_source":"arxiv_reference","pith_arxiv_id":null,"snapshot_observed_at":"2026-07-08T21:15:39.274227Z","title":"Zhang and S.-W","venue":null,"work_id":"45b23104-80fa-4cc7-bf4e-9612149c7b43","year":2026},"citing_paper":{"arxiv_id":"2607.05909","last_updated":"2026-07-07T07:04:03Z","snapshot_observed_at":"2026-08-14T10:29:50.174311Z","submitted_at":"2026-07-07T07:04:03Z","title":"Probing near-zone magnetic fields with extreme mass-ratio inspirals","version":1},"reference_index":71,"source":"pdf_text","source_observed_at":"2026-07-08T21:06:26.923131Z"},"links":{"citing_paper":"/paper/2607.05909"},"observation_digest":"sha256:4df9f1136538386129e0b9ff91b9e1968598f713fa1790413912c63f15be0fff","observation_id":"f352b135-7476-4b79-b023-49e70b7ee7ac","resolution":{"observed_at":"2026-07-08T21:15:39.275569Z","resolver_source":"arxiv_id","status":"verified_exact"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-23T06:30:58.430688+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-23T06:30:58.430688+00:00","source":"crossref"},{"observed_at":"2026-08-23T06:30:53.778098+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":{"arxiv_id":"2603.05084","last_updated":"2026-04-28T13:39:56Z","snapshot_observed_at":"2026-08-13T03:54:32.604656Z","submitted_at":"2026-03-05T11:56:51Z","title":"Distinguishability of magnetic massive black holes from environmental mimics with inspiral gravitational waves","version":2},"cited_work":{"arxiv_id":"2603.05084","doi":null,"metadata_source":"pith","pith_arxiv_id":"2603.05084","snapshot_observed_at":"2026-07-08T21:15:39.284371Z","title":"Distinguishability of magnetic massive black holes from environmental mimics with inspiral gravitational waves","venue":"gr-qc","work_id":"0a49e513-0042-45c1-823a-46da35816295","year":2026},"citing_paper":{"arxiv_id":"2607.05909","last_updated":"2026-07-07T07:04:03Z","snapshot_observed_at":"2026-08-14T10:29:50.174311Z","submitted_at":"2026-07-07T07:04:03Z","title":"Probing near-zone magnetic fields with extreme mass-ratio inspirals","version":1},"reference_index":72,"source":"pdf_text","source_observed_at":"2026-07-08T21:06:26.923131Z"},"links":{"cited_paper":"/paper/2603.05084","citing_paper":"/paper/2607.05909"},"observation_digest":"sha256:3070c3f64d1fd5ecfd10b03061146cebefbf3c9abb9d98b6b96a518faba832ae","observation_id":"e07d04f9-20a0-4f27-aa3c-f4cfd401d9e3","resolution":{"observed_at":"2026-07-08T21:15:39.285762Z","resolver_source":"local_arxiv","status":"verified_exact"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-23T06:30:58.430688+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-23T06:30:58.430688+00:00","source":"crossref"},{"observed_at":"2026-08-23T06:30:53.778098+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":"2508.21100","doi":null,"metadata_source":"arxiv_reference","pith_arxiv_id":null,"snapshot_observed_at":"2026-07-08T21:15:39.238798Z","title":"Vachher, A","venue":null,"work_id":"2a771df1-db3c-4e2b-a526-6837aa767d51","year":null},"citing_paper":{"arxiv_id":"2607.05909","last_updated":"2026-07-07T07:04:03Z","snapshot_observed_at":"2026-08-14T10:29:50.174311Z","submitted_at":"2026-07-07T07:04:03Z","title":"Probing near-zone magnetic fields with extreme mass-ratio inspirals","version":1},"reference_index":73,"source":"pdf_text","source_observed_at":"2026-07-08T21:06:26.923131Z"},"links":{"citing_paper":"/paper/2607.05909"},"observation_digest":"sha256:78143278b5f8fffe2cca9e418934f915f266d3555e23c99c128f63df85957c53","observation_id":"f9091e2d-bb36-472e-b6ee-4fa83c3a1c13","resolution":{"observed_at":"2026-07-08T21:15:39.240332Z","resolver_source":"arxiv_id","status":"verified_exact"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-23T06:30:58.430688+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-23T06:30:58.430688+00:00","source":"crossref"},{"observed_at":"2026-08-23T06:30:53.778098+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":"2512.12533","doi":null,"metadata_source":"arxiv_reference","pith_arxiv_id":null,"snapshot_observed_at":"2026-07-08T21:15:39.152679Z","title":null,"venue":null,"work_id":"42768854-8a3a-4b83-a4eb-f67d0a1a34f5","year":2026},"citing_paper":{"arxiv_id":"2607.05909","last_updated":"2026-07-07T07:04:03Z","snapshot_observed_at":"2026-08-14T10:29:50.174311Z","submitted_at":"2026-07-07T07:04:03Z","title":"Probing near-zone magnetic fields with extreme mass-ratio inspirals","version":1},"reference_index":74,"source":"pdf_text","source_observed_at":"2026-07-08T21:06:26.923131Z"},"links":{"citing_paper":"/paper/2607.05909"},"observation_digest":"sha256:9b643487b64525806d48bb879f19ab3d8c4ea77ca3f4865140d9062c4af8f342","observation_id":"be227152-444d-47b4-a4ca-947bbaf3150b","resolution":{"observed_at":"2026-07-08T21:15:39.153982Z","resolver_source":"arxiv_id","status":"verified_exact"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-23T06:30:58.430688+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-23T06:30:58.430688+00:00","source":"crossref"},{"observed_at":"2026-08-23T06:30:53.778098+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":"2602.09453","doi":null,"metadata_source":"arxiv_reference","pith_arxiv_id":null,"snapshot_observed_at":"2026-07-08T21:15:39.127471Z","title":"Xamidov, S","venue":null,"work_id":"609cb708-0846-40f9-accf-d6caef5cfa21","year":2026},"citing_paper":{"arxiv_id":"2607.05909","last_updated":"2026-07-07T07:04:03Z","snapshot_observed_at":"2026-08-14T10:29:50.174311Z","submitted_at":"2026-07-07T07:04:03Z","title":"Probing near-zone magnetic fields with extreme mass-ratio inspirals","version":1},"reference_index":75,"source":"pdf_text","source_observed_at":"2026-07-08T21:06:26.923131Z"},"links":{"citing_paper":"/paper/2607.05909"},"observation_digest":"sha256:bf80eae8c0d13d4f46792951bfef339ed134fa2d133fb2841b9e62a18efb246e","observation_id":"2f7a263c-f441-4b36-be62-a2d8eccbce8d","resolution":{"observed_at":"2026-07-08T21:15:39.128786Z","resolver_source":"arxiv_id","status":"verified_exact"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-23T06:30:58.430688+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-23T06:30:58.430688+00:00","source":"crossref"},{"observed_at":"2026-08-23T06:30:53.778098+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":"2603.18129","doi":null,"metadata_source":"arxiv_reference","pith_arxiv_id":null,"snapshot_observed_at":"2026-07-08T21:15:39.203073Z","title":"Rehman, S","venue":null,"work_id":"fa6a41d5-783b-4ed0-b1df-af62f00dc3ab","year":2026},"citing_paper":{"arxiv_id":"2607.05909","last_updated":"2026-07-07T07:04:03Z","snapshot_observed_at":"2026-08-14T10:29:50.174311Z","submitted_at":"2026-07-07T07:04:03Z","title":"Probing near-zone magnetic fields with extreme mass-ratio inspirals","version":1},"reference_index":76,"source":"pdf_text","source_observed_at":"2026-07-08T21:06:26.923131Z"},"links":{"citing_paper":"/paper/2607.05909"},"observation_digest":"sha256:f0231eecbf74056766a479392045a2b40c9141372c5a458cb0ed4f53806bd68f","observation_id":"f50d0f7c-661e-4fc8-867b-402df3706e85","resolution":{"observed_at":"2026-07-08T21:15:39.206048Z","resolver_source":"arxiv_id","status":"verified_exact"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-23T06:30:58.430688+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-23T06:30:58.430688+00:00","source":"crossref"},{"observed_at":"2026-08-23T06:30:53.778098+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":{"arxiv_id":"2605.09593","last_updated":"2026-05-10T15:11:12Z","snapshot_observed_at":"2026-08-15T03:10:55.382660Z","submitted_at":"2026-05-10T15:11:12Z","title":"Optical Appearance of the Kerr-Bertotti-Robinson Black Hole with a Magnetically Driven Synchrotron Emissivity Model","version":1},"cited_work":{"arxiv_id":"2605.09593","doi":null,"metadata_source":"pith","pith_arxiv_id":"2605.09593","snapshot_observed_at":"2026-07-08T21:15:39.172210Z","title":"Optical Appearance of the Kerr-Bertotti-Robinson Black Hole with a Magnetically Driven Synchrotron Emissivity Model","venue":"astro-ph.HE","work_id":"71788a55-b9cf-46b1-8f6e-cfb40b458b3c","year":2026},"citing_paper":{"arxiv_id":"2607.05909","last_updated":"2026-07-07T07:04:03Z","snapshot_observed_at":"2026-08-14T10:29:50.174311Z","submitted_at":"2026-07-07T07:04:03Z","title":"Probing near-zone magnetic fields with extreme mass-ratio inspirals","version":1},"reference_index":77,"source":"pdf_text","source_observed_at":"2026-07-08T21:06:26.923131Z"},"links":{"cited_paper":"/paper/2605.09593","citing_paper":"/paper/2607.05909"},"observation_digest":"sha256:f399bdb9156dd4f08ff03d40c2b3153e57bab99febf8079c0ab57afc71784640","observation_id":"00ad1601-4576-462f-982f-60fd5be73e28","resolution":{"observed_at":"2026-07-08T21:15:39.173455Z","resolver_source":"local_arxiv","status":"verified_exact"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-23T06:30:58.430688+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-23T06:30:58.430688+00:00","source":"crossref"},{"observed_at":"2026-08-23T06:30:53.778098+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":{"arxiv_id":"2603.18821","last_updated":"2026-08-18T16:16:48Z","snapshot_observed_at":"2026-08-21T22:11:20.290309Z","submitted_at":"2026-03-19T12:18:51Z","title":"Thermodynamics of Kerr-Bertotti-Robinson black hole","version":3},"cited_work":{"arxiv_id":"2603.18821","doi":null,"metadata_source":"arxiv_reference","pith_arxiv_id":"2603.18821","snapshot_observed_at":"2026-07-27T01:19:57.967013Z","title":"Thermodynamics of Kerr-Bertotti-Robinson black hole","venue":null,"work_id":"09ee4410-88bc-4d5e-bf47-26d30cf3e19c","year":2026},"citing_paper":{"arxiv_id":"2607.05909","last_updated":"2026-07-07T07:04:03Z","snapshot_observed_at":"2026-08-14T10:29:50.174311Z","submitted_at":"2026-07-07T07:04:03Z","title":"Probing near-zone magnetic fields with extreme mass-ratio inspirals","version":1},"reference_index":78,"source":"pdf_text","source_observed_at":"2026-07-08T21:06:26.923131Z"},"links":{"cited_paper":"/paper/2603.18821","citing_paper":"/paper/2607.05909"},"observation_digest":"sha256:7854d5ac435cbdb02de478cd3d60f1961e8fce3bf68a31ae45b5733b2b8707c1","observation_id":"108f4b7b-87b2-464a-83d3-074d9b138d3c","resolution":{"observed_at":"2026-07-27T01:19:57.967013Z","resolver_source":"arxiv_id","status":"verified_exact"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-23T06:30:58.430688+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-23T06:30:58.430688+00:00","source":"crossref"},{"observed_at":"2026-08-23T06:30:53.778098+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":{"arxiv_id":"2603.25049","last_updated":"2026-07-27T06:09:59Z","snapshot_observed_at":"2026-08-17T01:29:27.447279Z","submitted_at":"2026-03-26T05:32:03Z","title":"Critical Behavior of Photon Rings in Kerr-Bertotti-Robinson Spacetime","version":2},"cited_work":{"arxiv_id":"2603.25049","doi":null,"metadata_source":"arxiv_reference","pith_arxiv_id":"2603.25049","snapshot_observed_at":"2026-07-28T02:23:29.036882Z","title":null,"venue":null,"work_id":"48d8bba7-eb91-4fd8-aa04-8275a79f5319","year":2026},"citing_paper":{"arxiv_id":"2607.05909","last_updated":"2026-07-07T07:04:03Z","snapshot_observed_at":"2026-08-14T10:29:50.174311Z","submitted_at":"2026-07-07T07:04:03Z","title":"Probing near-zone magnetic fields with extreme mass-ratio inspirals","version":1},"reference_index":79,"source":"pdf_text","source_observed_at":"2026-07-08T21:06:26.923131Z"},"links":{"cited_paper":"/paper/2603.25049","citing_paper":"/paper/2607.05909"},"observation_digest":"sha256:024fbe9cf63c32b20542b7f3b929c27d84d53294175307f0026195016df12f32","observation_id":"25bcb086-a658-4d5a-a756-788e1bae6e0f","resolution":{"observed_at":"2026-07-28T02:23:29.036882Z","resolver_source":"arxiv_id","status":"verified_exact"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-23T06:30:58.430688+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-23T06:30:58.430688+00:00","source":"crossref"},{"observed_at":"2026-08-23T06:30:53.778098+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":"2026-07-08T21:15:39.431524Z","title":null,"venue":null,"work_id":"c0028c8a-493f-417a-9e5d-d9d7c81126ba","year":1974},"citing_paper":{"arxiv_id":"2607.05909","last_updated":"2026-07-07T07:04:03Z","snapshot_observed_at":"2026-08-14T10:29:50.174311Z","submitted_at":"2026-07-07T07:04:03Z","title":"Probing near-zone magnetic fields with extreme mass-ratio inspirals","version":1},"reference_index":80,"source":"pdf_text","source_observed_at":"2026-07-08T21:06:26.923131Z"},"links":{"citing_paper":"/paper/2607.05909"},"observation_digest":"sha256:6608bc2afeaf00dc11cb18a95cd9153e523df84a8831958507ca8f4476460c26","observation_id":"456806ab-872b-47f8-9068-4d9702e7badc","resolution":{"observed_at":"2026-07-08T21:15:39.433122Z","resolver_source":"raw_fallback","status":"unresolved"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-23T06:30:58.430688+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-23T06:30:58.430688+00:00","source":"crossref"},{"observed_at":"2026-08-23T06:30:53.778098+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":"2026-07-08T21:15:39.434847Z","title":null,"venue":null,"work_id":"f8655fb7-0447-4eab-90ce-cb63add0cc28","year":1995},"citing_paper":{"arxiv_id":"2607.05909","last_updated":"2026-07-07T07:04:03Z","snapshot_observed_at":"2026-08-14T10:29:50.174311Z","submitted_at":"2026-07-07T07:04:03Z","title":"Probing near-zone magnetic fields with extreme mass-ratio inspirals","version":1},"reference_index":81,"source":"pdf_text","source_observed_at":"2026-07-08T21:06:26.923131Z"},"links":{"citing_paper":"/paper/2607.05909"},"observation_digest":"sha256:2503cbc6b562f41803f907fd61f93ec07357e00fd85a587f83b2714fc6e25ff0","observation_id":"406694ec-2bc4-43a8-9024-50922b6a9019","resolution":{"observed_at":"2026-07-08T21:15:39.436332Z","resolver_source":"raw_fallback","status":"unresolved"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-23T06:30:58.430688+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-23T06:30:58.430688+00:00","source":"crossref"},{"observed_at":"2026-08-23T06:30:53.778098+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":{"arxiv_id":"1405.6976","last_updated":"2014-05-27T17:02:46Z","snapshot_observed_at":"2026-08-14T23:32:32.997690Z","submitted_at":"2014-05-27T17:02:46Z","title":"Orbital and epicyclic frequencies around rapidly rotating compact stars in scalar-tensor theories of gravity","version":1},"cited_work":{"arxiv_id":"1405.6976","doi":null,"metadata_source":"pith","pith_arxiv_id":"1405.6976","snapshot_observed_at":"2026-07-08T21:15:39.276753Z","title":"Orbital and epicyclic frequencies around rapidly rotating compact stars in scalar-tensor theories of gravity","venue":"astro-ph.HE","work_id":"b6195dad-1890-4735-b130-62893602f3c3","year":2014},"citing_paper":{"arxiv_id":"2607.05909","last_updated":"2026-07-07T07:04:03Z","snapshot_observed_at":"2026-08-14T10:29:50.174311Z","submitted_at":"2026-07-07T07:04:03Z","title":"Probing near-zone magnetic fields with extreme mass-ratio inspirals","version":1},"reference_index":82,"source":"pdf_text","source_observed_at":"2026-07-08T21:06:26.923131Z"},"links":{"cited_paper":"/paper/1405.6976","citing_paper":"/paper/2607.05909"},"observation_digest":"sha256:562102472fda552d2ab9d005fc0cce38ae90bb1f36658ee48dabdadcd706ba49","observation_id":"95caf208-60ef-4ce2-83fe-b7b6e609b817","resolution":{"observed_at":"2026-07-08T21:15:39.277989Z","resolver_source":"local_arxiv","status":"verified_exact"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-23T06:30:58.430688+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-23T06:30:58.430688+00:00","source":"crossref"},{"observed_at":"2026-08-23T06:30:53.778098+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":{"arxiv_id":"astro-ph/0411709","last_updated":"2004-11-26T13:44:09Z","snapshot_observed_at":"2026-08-08T00:16:28.055909Z","submitted_at":"2004-11-26T13:44:09Z","title":"Epicyclic frequencies derived from the effective potential: simple and practical formulae","version":1},"cited_work":{"arxiv_id":"astro-ph/0411709","doi":null,"metadata_source":"pith","pith_arxiv_id":"astro-ph/0411709","snapshot_observed_at":"2026-07-08T21:15:39.258088Z","title":"Epicyclic frequencies derived from the effective potential: simple and practical formulae","venue":"astro-ph","work_id":"a05dfbce-ef72-4a2c-bcc8-84c8ea84f706","year":2004},"citing_paper":{"arxiv_id":"2607.05909","last_updated":"2026-07-07T07:04:03Z","snapshot_observed_at":"2026-08-14T10:29:50.174311Z","submitted_at":"2026-07-07T07:04:03Z","title":"Probing near-zone magnetic fields with extreme mass-ratio inspirals","version":1},"reference_index":83,"source":"pdf_text","source_observed_at":"2026-07-08T21:06:26.923131Z"},"links":{"cited_paper":"/paper/astro-ph/0411709","citing_paper":"/paper/2607.05909"},"observation_digest":"sha256:670108cb811136a95ee59db5fbaee65c9ba76e3e4938a9277be0aea850aa2bbc","observation_id":"a12147e9-4f13-431a-9dba-c413c181a757","resolution":{"observed_at":"2026-07-08T21:15:39.259370Z","resolver_source":"local_arxiv","status":"verified_exact"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-23T06:30:58.430688+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-23T06:30:58.430688+00:00","source":"crossref"},{"observed_at":"2026-08-23T06:30:53.778098+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":{"arxiv_id":"gr-qc/0502028","last_updated":"2005-02-08T16:58:57Z","snapshot_observed_at":"2026-08-21T05:26:42.270246Z","submitted_at":"2005-02-08T16:58:57Z","title":"Gravitational perturbations of the Schwarzschild spacetime: A practical covariant and gauge-invariant formalism","version":1},"cited_work":{"arxiv_id":"gr-qc/0502028","doi":null,"metadata_source":"pith","pith_arxiv_id":"gr-qc/0502028","snapshot_observed_at":"2026-07-08T21:15:39.100644Z","title":"Gravitational perturbations of the Schwarzschild spacetime: A practical covariant and gauge-invariant formalism","venue":"gr-qc","work_id":"22d0ea2a-46da-408e-a209-1ff40b61443c","year":2005},"citing_paper":{"arxiv_id":"2607.05909","last_updated":"2026-07-07T07:04:03Z","snapshot_observed_at":"2026-08-14T10:29:50.174311Z","submitted_at":"2026-07-07T07:04:03Z","title":"Probing near-zone magnetic fields with extreme mass-ratio inspirals","version":1},"reference_index":84,"source":"pdf_text","source_observed_at":"2026-07-08T21:06:26.923131Z"},"links":{"cited_paper":"/paper/gr-qc/0502028","citing_paper":"/paper/2607.05909"},"observation_digest":"sha256:322500225bb76754e86357008b19d4960deb258cbc21a9645cb9df89095db05d","observation_id":"e35aa7e9-a5cd-4222-b0cf-14b60587dab0","resolution":{"observed_at":"2026-07-08T21:15:39.101813Z","resolver_source":"local_arxiv","status":"verified_exact"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-23T06:30:58.430688+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-23T06:30:58.430688+00:00","source":"crossref"},{"observed_at":"2026-08-23T06:30:53.778098+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":"qc/0311017","doi":null,"metadata_source":"arxiv_reference","pith_arxiv_id":null,"snapshot_observed_at":"2026-07-08T21:15:39.102887Z","title":"Martel, Phys","venue":null,"work_id":"af099249-1607-4750-b8ba-8c33dcc8f8aa","year":2004},"citing_paper":{"arxiv_id":"2607.05909","last_updated":"2026-07-07T07:04:03Z","snapshot_observed_at":"2026-08-14T10:29:50.174311Z","submitted_at":"2026-07-07T07:04:03Z","title":"Probing near-zone magnetic fields with extreme mass-ratio inspirals","version":1},"reference_index":85,"source":"pdf_text","source_observed_at":"2026-07-08T21:06:26.923131Z"},"links":{"citing_paper":"/paper/2607.05909"},"observation_digest":"sha256:52915a035292a74fc6d771d085b1c4be267210d4f8155b0153b101bd1ca26cf7","observation_id":"5b416a26-de5d-4c76-9c51-1242c5e11a2d","resolution":{"observed_at":"2026-07-08T21:15:39.107238Z","resolver_source":"arxiv_id","status":"verified_exact"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-23T06:30:58.430688+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-23T06:30:58.430688+00:00","source":"crossref"},{"observed_at":"2026-08-23T06:30:53.778098+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":{"arxiv_id":"1910.07841","last_updated":"2020-01-14T15:48:51Z","snapshot_observed_at":"2026-08-19T07:18:51.844950Z","submitted_at":"2019-10-17T11:51:30Z","title":"Tidal heating as a discriminator for horizons in extreme mass ratio inspirals","version":2},"cited_work":{"arxiv_id":"1910.07841","doi":null,"metadata_source":"pith","pith_arxiv_id":"1910.07841","snapshot_observed_at":"2026-07-08T21:15:39.147991Z","title":"Datta, R","venue":"gr-qc","work_id":"8ee2fefc-42ad-44c0-a985-160d6bff6f4e","year":2019},"citing_paper":{"arxiv_id":"2607.05909","last_updated":"2026-07-07T07:04:03Z","snapshot_observed_at":"2026-08-14T10:29:50.174311Z","submitted_at":"2026-07-07T07:04:03Z","title":"Probing near-zone magnetic fields with extreme mass-ratio inspirals","version":1},"reference_index":86,"source":"pdf_text","source_observed_at":"2026-07-08T21:06:26.923131Z"},"links":{"cited_paper":"/paper/1910.07841","citing_paper":"/paper/2607.05909"},"observation_digest":"sha256:3c9ca9195818cb262286524e8ff2b0dbbd218f1946a10ae01e9d28aea573487e","observation_id":"087e224a-cf2b-4e07-88f1-ac3d4efa0a85","resolution":{"observed_at":"2026-07-08T21:15:39.149194Z","resolver_source":"local_arxiv","status":"verified_exact"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-23T06:30:58.430688+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-23T06:30:58.430688+00:00","source":"crossref"},{"observed_at":"2026-08-23T06:30:53.778098+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":"2026-07-08T21:15:39.444170Z","title":null,"venue":null,"work_id":"3fa31ea7-e293-4281-b050-ad27794264c4","year":1967},"citing_paper":{"arxiv_id":"2607.05909","last_updated":"2026-07-07T07:04:03Z","snapshot_observed_at":"2026-08-14T10:29:50.174311Z","submitted_at":"2026-07-07T07:04:03Z","title":"Probing near-zone magnetic fields with extreme mass-ratio inspirals","version":1},"reference_index":87,"source":"pdf_text","source_observed_at":"2026-07-08T21:06:26.923131Z"},"links":{"citing_paper":"/paper/2607.05909"},"observation_digest":"sha256:e38cd5ab1b7f3cd3aed063252ef2edd086bb81d68fed2a2e1c669eeeb35e618a","observation_id":"9f97ed91-c13b-464b-8a9e-b16bed2f9798","resolution":{"observed_at":"2026-07-08T21:15:39.445523Z","resolver_source":"raw_fallback","status":"unresolved"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-23T06:30:58.430688+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-23T06:30:58.430688+00:00","source":"crossref"},{"observed_at":"2026-08-23T06:30:53.778098+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":"qc/9703068","doi":null,"metadata_source":"arxiv_reference","pith_arxiv_id":null,"snapshot_observed_at":"2026-07-08T21:15:39.155028Z","title":"Cutler, Angular resolution of the LISA gravitational wave detector, Phys","venue":null,"work_id":"6b1cd433-4d31-4155-a592-e09cc3baed15","year":1998},"citing_paper":{"arxiv_id":"2607.05909","last_updated":"2026-07-07T07:04:03Z","snapshot_observed_at":"2026-08-14T10:29:50.174311Z","submitted_at":"2026-07-07T07:04:03Z","title":"Probing near-zone magnetic fields with extreme mass-ratio inspirals","version":1},"reference_index":88,"source":"pdf_text","source_observed_at":"2026-07-08T21:06:26.923131Z"},"links":{"citing_paper":"/paper/2607.05909"},"observation_digest":"sha256:d7430a88624efb1477a6056c926aeb8d3bc8397c495908cf11c9a193f6ff4de2","observation_id":"f064621c-7aa3-4e40-931a-9f73c078816e","resolution":{"observed_at":"2026-07-08T21:15:39.156243Z","resolver_source":"arxiv_id","status":"verified_exact"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-23T06:30:58.430688+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-23T06:30:58.430688+00:00","source":"crossref"},{"observed_at":"2026-08-23T06:30:53.778098+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":"2026-07-08T21:15:39.442267Z","title":null,"venue":null,"work_id":"436f4171-f509-4a1c-8228-03d246abd04f","year":1994},"citing_paper":{"arxiv_id":"2607.05909","last_updated":"2026-07-07T07:04:03Z","snapshot_observed_at":"2026-08-14T10:29:50.174311Z","submitted_at":"2026-07-07T07:04:03Z","title":"Probing near-zone magnetic fields with extreme mass-ratio inspirals","version":1},"reference_index":89,"source":"pdf_text","source_observed_at":"2026-07-08T21:06:26.923131Z"},"links":{"citing_paper":"/paper/2607.05909"},"observation_digest":"sha256:0a96c3f74a4bc39b3bd17e0129a6283029653bcc58068739e32f8d1c6037e6bd","observation_id":"906591aa-43d8-4c7a-a497-3c30c7005f9e","resolution":{"observed_at":"2026-07-08T21:15:39.443453Z","resolver_source":"raw_fallback","status":"unresolved"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-23T06:30:58.430688+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-23T06:30:58.430688+00:00","source":"crossref"},{"observed_at":"2026-08-23T06:30:53.778098+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":{"arxiv_id":"gr-qc/0310125","last_updated":"2004-09-02T09:29:13Z","snapshot_observed_at":"2026-08-15T11:00:41.031793Z","submitted_at":"2003-10-30T01:27:41Z","title":"LISA Capture Sources: Approximate Waveforms, Signal-to-Noise Ratios, and Parameter Estimation Accuracy","version":3},"cited_work":{"arxiv_id":"gr-qc/0310125","doi":null,"metadata_source":"pith","pith_arxiv_id":"gr-qc/0310125","snapshot_observed_at":"2026-07-08T21:15:39.294452Z","title":"LISA Capture Sources: Approximate Waveforms, Signal-to-Noise Ratios, and Parameter Estimation Accuracy","venue":"gr-qc","work_id":"32d0596b-e5a8-47c4-a307-5ce5578033c6","year":2003},"citing_paper":{"arxiv_id":"2607.05909","last_updated":"2026-07-07T07:04:03Z","snapshot_observed_at":"2026-08-14T10:29:50.174311Z","submitted_at":"2026-07-07T07:04:03Z","title":"Probing near-zone magnetic fields with extreme mass-ratio inspirals","version":1},"reference_index":90,"source":"pdf_text","source_observed_at":"2026-07-08T21:06:26.923131Z"},"links":{"cited_paper":"/paper/gr-qc/0310125","citing_paper":"/paper/2607.05909"},"observation_digest":"sha256:cbf3c0628bd64fb39d73160e22c2255269558f42b58b9adccf95971d3fa9f006","observation_id":"ce6ee77a-4a55-460d-ae51-6c41a1027da6","resolution":{"observed_at":"2026-07-08T21:15:39.295775Z","resolver_source":"local_arxiv","status":"verified_exact"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-23T06:30:58.430688+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-23T06:30:58.430688+00:00","source":"crossref"},{"observed_at":"2026-08-23T06:30:53.778098+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":{"arxiv_id":"1803.01944","last_updated":"2018-10-15T16:27:32Z","snapshot_observed_at":"2026-08-14T19:39:16.581930Z","submitted_at":"2018-03-05T21:56:12Z","title":"The construction and use of LISA sensitivity curves","version":2},"cited_work":{"arxiv_id":"1803.01944","doi":null,"metadata_source":"pith","pith_arxiv_id":"1803.01944","snapshot_observed_at":"2026-07-10T10:47:02.038442Z","title":"The construction and use of LISA sensitivity curves","venue":"astro-ph.HE","work_id":"be579bfb-0138-4c35-9292-f00f32ccaca3","year":2018},"citing_paper":{"arxiv_id":"2607.05909","last_updated":"2026-07-07T07:04:03Z","snapshot_observed_at":"2026-08-14T10:29:50.174311Z","submitted_at":"2026-07-07T07:04:03Z","title":"Probing near-zone magnetic fields with extreme mass-ratio inspirals","version":1},"reference_index":91,"source":"pdf_text","source_observed_at":"2026-07-08T21:06:26.923131Z"},"links":{"cited_paper":"/paper/1803.01944","citing_paper":"/paper/2607.05909"},"observation_digest":"sha256:582d70264e9b6b4bf33aba374995f7cbab571e8c0965cdb9087de50943faa307","observation_id":"38cac58a-b220-45bb-a6ec-4f741b0ef32d","resolution":{"observed_at":"2026-07-08T21:15:39.109603Z","resolver_source":"local_arxiv","status":"verified_exact"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-23T06:30:58.430688+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-23T06:30:58.430688+00:00","source":"crossref"},{"observed_at":"2026-08-23T06:30:53.778098+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":{"arxiv_id":"0809.3844","last_updated":"2008-11-05T17:07:03Z","snapshot_observed_at":"2026-08-19T21:46:09.241551Z","submitted_at":"2008-09-23T03:35:04Z","title":"Model Waveform Accuracy Standards for Gravitational Wave Data Analysis","version":2},"cited_work":{"arxiv_id":"0809.3844","doi":null,"metadata_source":"pith","pith_arxiv_id":"0809.3844","snapshot_observed_at":"2026-07-08T21:15:39.167234Z","title":"Model Waveform Accuracy Standards for Gravitational Wave Data Analysis","venue":"gr-qc","work_id":"ec0d1933-467c-4368-8b46-92fd847e85b5","year":2008},"citing_paper":{"arxiv_id":"2607.05909","last_updated":"2026-07-07T07:04:03Z","snapshot_observed_at":"2026-08-14T10:29:50.174311Z","submitted_at":"2026-07-07T07:04:03Z","title":"Probing near-zone magnetic fields with extreme mass-ratio inspirals","version":1},"reference_index":92,"source":"pdf_text","source_observed_at":"2026-07-08T21:06:26.923131Z"},"links":{"cited_paper":"/paper/0809.3844","citing_paper":"/paper/2607.05909"},"observation_digest":"sha256:0e577c125314c80103ad41e3d29b03ff4319daad69ae07037adc4296e59e7b79","observation_id":"c0b3ac51-d26d-47d3-b8ff-3333d1b24580","resolution":{"observed_at":"2026-07-08T21:15:39.168342Z","resolver_source":"local_arxiv","status":"verified_exact"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-23T06:30:58.430688+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-23T06:30:58.430688+00:00","source":"crossref"},{"observed_at":"2026-08-23T06:30:53.778098+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":{"arxiv_id":"gr-qc/9710129","last_updated":"1997-10-30T18:14:35Z","snapshot_observed_at":"2026-08-22T05:17:13.885610Z","submitted_at":"1997-10-30T18:14:35Z","title":"Measuring gravitational waves from binary black hole coalescences: II. the waves' information and its extraction, with and without templates","version":1},"cited_work":{"arxiv_id":"gr-qc/9710129","doi":null,"metadata_source":"pith","pith_arxiv_id":"gr-qc/9710129","snapshot_observed_at":"2026-07-08T21:15:39.200613Z","title":"Measuring gravitat ional waves from binary black hole coalescences. II. The wave’s information and its ex- traction, with and without templates","venue":"gr-qc","work_id":"5d1e6ae6-72c2-437d-a643-a4efba56388a","year":1997},"citing_paper":{"arxiv_id":"2607.05909","last_updated":"2026-07-07T07:04:03Z","snapshot_observed_at":"2026-08-14T10:29:50.174311Z","submitted_at":"2026-07-07T07:04:03Z","title":"Probing near-zone magnetic fields with extreme mass-ratio inspirals","version":1},"reference_index":93,"source":"pdf_text","source_observed_at":"2026-07-08T21:06:26.923131Z"},"links":{"cited_paper":"/paper/gr-qc/9710129","citing_paper":"/paper/2607.05909"},"observation_digest":"sha256:358b2b29125a624801b98b9abeccb2948e5190db3693858b1be49c8d7da9d78b","observation_id":"0d4dae8c-3817-4b34-af7c-7c96ce996379","resolution":{"observed_at":"2026-07-08T21:15:39.201965Z","resolver_source":"local_arxiv","status":"verified_exact"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-23T06:30:58.430688+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-23T06:30:58.430688+00:00","source":"crossref"},{"observed_at":"2026-08-23T06:30:53.778098+00:00","source":"retraction_watch"}],"state":"measured"}}],"paper":{"arxiv_id":"2607.05909","last_updated":"2026-07-07T07:04:03Z","latest_version":1,"primary_category":"gr-qc","snapshot_observed_at":"2026-08-14T10:29:50.174311Z","submitted_at":"2026-07-07T07:04:03Z","title":"Probing near-zone magnetic fields with extreme mass-ratio inspirals"},"reference_resolution":{"displayed":93,"state_counts":{"malformed_identifier":0,"metadata_mismatch":1,"parse_uncertain":0,"unresolved":13,"verified_exact":76,"verified_fuzzy":3},"total_outbound_references":93},"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":"2026-08-23T06:30:58.430688+00:00","source":"crossref"},{"observed_at":"2026-08-23T06:30:53.778098+00:00","source":"retraction_watch"}],"thesis":"As of 23 August 2026, this Paper Citation Record lists 93 of 93 outbound references and 0 inbound Pith citation observations for arXiv:2607.05909."}