{"as_of":"2026-08-04T10:06:00Z","caps":{"database_statements":6,"inbound":100,"outbound":100},"context_digest":"sha256:50d06e9305044335f7385c261de293b3910652cefe945664754edd0f654e95a6","coverage":[{"denominator":77,"lane":"reference_resolution","note":"Typed states for the displayed outbound observations.","records_observed":77,"source":"paper_references, paper_reference_links","source_observed_at":"2026-05-18T18:16:19.200462Z","state":"measured"},{"denominator":79,"lane":"standing_notices","note":"One-hop event checks from named stored sources.","records_observed":79,"source":"scholarly_work_events, retraction_status_cache","source_observed_at":"2026-08-04T06:34:03.388597+00:00","state":"measured"},{"denominator":2,"lane":"inbound_itemization","note":"Pith citing papers itemized under the disclosed page cap.","records_observed":2,"source":"paper_references, paper_reference_links","source_observed_at":"2026-08-01T15:35:54.568869Z","state":"measured"},{"denominator":1,"lane":"external_citation_measurements","note":"A source-named dated measurement, never combined with another source.","records_observed":0,"source":"pith","source_observed_at":"2026-05-18T18:16:42.784704Z","state":"measured"}],"external_citation_measurements":[],"inbound":[{"citation":{"cited_paper":{"arxiv_id":"2509.09986","last_updated":"2026-04-08T06:08:20Z","snapshot_observed_at":"2026-07-06T22:29:06.119014Z","submitted_at":"2025-09-12T06:00:19Z","title":"Plunge spectra as discriminators of black hole mimickers","version":3},"cited_work":{"arxiv_id":"2509.09986","doi":null,"metadata_source":"pith","pith_arxiv_id":"2509.09986","snapshot_observed_at":"2026-06-05T21:23:00.469572Z","title":"Plunge spectra as discriminators of black hole mimickers","venue":"gr-qc","work_id":"d73ee60a-b4d7-45cf-9b4c-4109424c68bd","year":2025},"citing_paper":{"arxiv_id":"2509.09986","last_updated":"2026-04-08T06:08:20Z","snapshot_observed_at":"2026-07-06T22:29:06.119014Z","submitted_at":"2025-09-12T06:00:19Z","title":"Plunge spectra as discriminators of black hole mimickers","version":3},"reference_index":1,"source":"pdf_text","source_observed_at":"2026-05-18T18:16:19.200462Z"},"links":{"cited_paper":"/paper/2509.09986","citing_paper":"/paper/2509.09986"},"observation_digest":"sha256:3d292da338ea56f9a1edf4c5ca3280c3f463e14793fa70c4cad156b9a948ab43","observation_id":"a131d8a1-8dcc-4522-9bdd-4a2de2c5950f","resolution":{"observed_at":"2026-05-18T18:16:42.787238Z","resolver_source":"local_arxiv","status":"verified_exact"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-04T06:34:03.388597+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-04T06:34:03.388597+00:00","source":"crossref"},{"observed_at":"2026-08-04T06:33:57.428241+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":{"arxiv_id":"2509.09986","last_updated":"2026-04-08T06:08:20Z","snapshot_observed_at":"2026-07-06T22:29:06.119014Z","submitted_at":"2025-09-12T06:00:19Z","title":"Plunge spectra as discriminators of black hole mimickers","version":3},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2509.09986","snapshot_observed_at":"2026-08-01T15:35:54.568869Z","title":"Plunge spectra as discriminators of black- hole mimickers,","venue":null,"work_id":null,"year":2026},"citing_paper":{"arxiv_id":"2607.18405","last_updated":"2026-07-29T15:42:23Z","snapshot_observed_at":"2026-08-04T01:42:40.892447Z","submitted_at":"2026-07-20T18:00:44Z","title":"Extreme mass-ratio inspirals into Newtonian Proca stars","version":2},"reference_index":75,"source":"pdf_text","source_observed_at":"2026-08-01T15:35:54.568869Z"},"links":{"cited_paper":"/paper/2509.09986","citing_paper":"/paper/2607.18405"},"observation_digest":"sha256:7782343b4abae3eae70f76c4936d368d81d44dd9f58ceaabfd3f66d44c637f5d","observation_id":"66f797b4-7953-4cb8-bc5e-341128f7919e","resolution":{"observed_at":"2026-08-01T15:35:54.568869Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}}],"links":{"evidence":"/evidence","html":"/paper/2509.09986/citation-record","integrity":"/paper/2509.09986/integrity","json":"/paper/2509.09986/citation-record.json","paper":"/paper/2509.09986"},"outbound":[{"citation":{"cited_paper":{"arxiv_id":"2509.09986","last_updated":"2026-04-08T06:08:20Z","snapshot_observed_at":"2026-07-06T22:29:06.119014Z","submitted_at":"2025-09-12T06:00:19Z","title":"Plunge spectra as discriminators of black hole mimickers","version":3},"cited_work":{"arxiv_id":"2509.09986","doi":null,"metadata_source":"pith","pith_arxiv_id":"2509.09986","snapshot_observed_at":"2026-06-05T21:23:00.469572Z","title":"Plunge spectra as discriminators of black hole mimickers","venue":"gr-qc","work_id":"d73ee60a-b4d7-45cf-9b4c-4109424c68bd","year":2025},"citing_paper":{"arxiv_id":"2509.09986","last_updated":"2026-04-08T06:08:20Z","snapshot_observed_at":"2026-07-06T22:29:06.119014Z","submitted_at":"2025-09-12T06:00:19Z","title":"Plunge spectra as discriminators of black hole mimickers","version":3},"reference_index":1,"source":"pdf_text","source_observed_at":"2026-05-18T18:16:19.200462Z"},"links":{"cited_paper":"/paper/2509.09986","citing_paper":"/paper/2509.09986"},"observation_digest":"sha256:3d292da338ea56f9a1edf4c5ca3280c3f463e14793fa70c4cad156b9a948ab43","observation_id":"a131d8a1-8dcc-4522-9bdd-4a2de2c5950f","resolution":{"observed_at":"2026-05-18T18:16:42.787238Z","resolver_source":"local_arxiv","status":"verified_exact"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-04T06:34:03.388597+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-04T06:34:03.388597+00:00","source":"crossref"},{"observed_at":"2026-08-04T06:33:57.428241+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":"raw_reference","pith_arxiv_id":null,"snapshot_observed_at":"2026-06-05T21:23:00.469572Z","title":"We will start in Sec","venue":null,"work_id":"70bb7a1a-5c8d-459d-b078-16b64b4843bb","year":null},"citing_paper":{"arxiv_id":"2509.09986","last_updated":"2026-04-08T06:08:20Z","snapshot_observed_at":"2026-07-06T22:29:06.119014Z","submitted_at":"2025-09-12T06:00:19Z","title":"Plunge spectra as discriminators of black hole mimickers","version":3},"reference_index":2,"source":"pdf_text","source_observed_at":"2026-05-18T18:16:19.200462Z"},"links":{"citing_paper":"/paper/2509.09986"},"observation_digest":"sha256:baf297fe30a47557040c10456eae969ec31a47efd70a4fe4f3682d1d88c3b5f2","observation_id":"148379ce-b598-4517-8105-26e61a3f212b","resolution":{"observed_at":"2026-05-18T18:16:43.966561Z","resolver_source":"raw_fallback","status":"verified_fuzzy"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-04T06:34:03.388597+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-04T06:34:03.388597+00:00","source":"crossref"},{"observed_at":"2026-08-04T06:33:57.428241+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":"raw_reference","pith_arxiv_id":null,"snapshot_observed_at":"2026-06-05T21:23:00.469572Z","title":null,"venue":null,"work_id":"65d3d1a2-4144-4aca-ab90-43cbbfced78b","year":null},"citing_paper":{"arxiv_id":"2509.09986","last_updated":"2026-04-08T06:08:20Z","snapshot_observed_at":"2026-07-06T22:29:06.119014Z","submitted_at":"2025-09-12T06:00:19Z","title":"Plunge spectra as discriminators of black hole mimickers","version":3},"reference_index":3,"source":"pdf_text","source_observed_at":"2026-05-18T18:16:19.200462Z"},"links":{"citing_paper":"/paper/2509.09986"},"observation_digest":"sha256:2608ab6f02523cfe4725413aeaaf2ef32e9f2e32082671b679064416463d029a","observation_id":"16c1baee-ebf9-4291-b9e8-35aa6f929d54","resolution":{"observed_at":"2026-05-18T18:16:43.963534Z","resolver_source":"raw_fallback","status":"unresolved"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-04T06:34:03.388597+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-04T06:34:03.388597+00:00","source":"crossref"},{"observed_at":"2026-08-04T06:33:57.428241+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":"raw_reference","pith_arxiv_id":null,"snapshot_observed_at":"2026-06-05T21:23:00.469572Z","title":"(1), some- thing interesting happens whenM ω≳0.39","venue":null,"work_id":"3133600d-08f3-4187-86a6-18922d7a58fb","year":null},"citing_paper":{"arxiv_id":"2509.09986","last_updated":"2026-04-08T06:08:20Z","snapshot_observed_at":"2026-07-06T22:29:06.119014Z","submitted_at":"2025-09-12T06:00:19Z","title":"Plunge spectra as discriminators of black hole mimickers","version":3},"reference_index":4,"source":"pdf_text","source_observed_at":"2026-05-18T18:16:19.200462Z"},"links":{"citing_paper":"/paper/2509.09986"},"observation_digest":"sha256:963694567284956853ca89a637da66376d94ad3e16ce103b13b17303c98cda65","observation_id":"156d0b3d-497a-4d95-85e2-4f59e01837c5","resolution":{"observed_at":"2026-05-18T18:16:43.958999Z","resolver_source":"raw_fallback","status":"verified_fuzzy"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-04T06:34:03.388597+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-04T06:34:03.388597+00:00","source":"crossref"},{"observed_at":"2026-08-04T06:33:57.428241+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":{"arxiv_id":"1411.4547","last_updated":"2014-11-17T16:55:23Z","snapshot_observed_at":"2026-07-06T02:11:23.670680Z","submitted_at":"2014-11-17T16:55:23Z","title":"Advanced LIGO","version":1},"cited_work":{"arxiv_id":"1411.4547","doi":null,"metadata_source":"pith","pith_arxiv_id":"1411.4547","snapshot_observed_at":"2026-07-04T19:40:06.484660Z","title":"Advanced LIGO","venue":"gr-qc","work_id":"b93186e6-8d0a-440a-aa48-9de6dbff57b9","year":2014},"citing_paper":{"arxiv_id":"2509.09986","last_updated":"2026-04-08T06:08:20Z","snapshot_observed_at":"2026-07-06T22:29:06.119014Z","submitted_at":"2025-09-12T06:00:19Z","title":"Plunge spectra as discriminators of black hole mimickers","version":3},"reference_index":5,"source":"pdf_text","source_observed_at":"2026-05-18T18:16:19.200462Z"},"links":{"cited_paper":"/paper/1411.4547","citing_paper":"/paper/2509.09986"},"observation_digest":"sha256:b18d41cda583c5839a0f3fd68824aa123241a6d23f0521abac00c73358477dfd","observation_id":"154e1427-bc4b-49ba-9697-c4b841c3e7db","resolution":{"observed_at":"2026-05-18T18:16:42.902814Z","resolver_source":"local_arxiv","status":"verified_exact"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-04T06:34:03.388597+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-04T06:34:03.388597+00:00","source":"crossref"},{"observed_at":"2026-08-04T06:33:57.428241+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":{"arxiv_id":"1408.3978","last_updated":"2014-10-16T13:24:29Z","snapshot_observed_at":"2026-07-06T02:11:23.670680Z","submitted_at":"2014-08-18T11:19:22Z","title":"Advanced Virgo: a 2nd generation interferometric gravitational wave detector","version":3},"cited_work":{"arxiv_id":"1408.3978","doi":null,"metadata_source":"pith","pith_arxiv_id":"1408.3978","snapshot_observed_at":"2026-07-04T19:40:06.434742Z","title":"Advanced Virgo: a 2nd generation interferometric gravitational wave detector","venue":"gr-qc","work_id":"29d52a5a-6fd3-471b-8fec-d17c29cf9026","year":2014},"citing_paper":{"arxiv_id":"2509.09986","last_updated":"2026-04-08T06:08:20Z","snapshot_observed_at":"2026-07-06T22:29:06.119014Z","submitted_at":"2025-09-12T06:00:19Z","title":"Plunge spectra as discriminators of black hole mimickers","version":3},"reference_index":6,"source":"pdf_text","source_observed_at":"2026-05-18T18:16:19.200462Z"},"links":{"cited_paper":"/paper/1408.3978","citing_paper":"/paper/2509.09986"},"observation_digest":"sha256:5de55583e1f90e3ebcf850d88571477453bc5c1d43218ca9ad7e7e9b93f77bcc","observation_id":"c92db411-263c-4e7f-9d37-17fbf1944373","resolution":{"observed_at":"2026-05-18T18:16:42.991491Z","resolver_source":"local_arxiv","status":"verified_exact"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-04T06:34:03.388597+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-04T06:34:03.388597+00:00","source":"crossref"},{"observed_at":"2026-08-04T06:33:57.428241+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":{"arxiv_id":"1602.03837","last_updated":"2016-02-11T19:26:44Z","snapshot_observed_at":"2026-07-09T16:56:15.649302Z","submitted_at":"2016-02-11T19:26:44Z","title":"Observation of Gravitational Waves from a Binary Black Hole Merger","version":1},"cited_work":{"arxiv_id":"1602.03837","doi":null,"metadata_source":"pith","pith_arxiv_id":"1602.03837","snapshot_observed_at":"2026-07-11T00:07:39.821374Z","title":"Observation of Gravitational Waves from a Binary Black Hole Merger","venue":"gr-qc","work_id":"ab878228-151c-4a29-8026-a4308b076d30","year":2016},"citing_paper":{"arxiv_id":"2509.09986","last_updated":"2026-04-08T06:08:20Z","snapshot_observed_at":"2026-07-06T22:29:06.119014Z","submitted_at":"2025-09-12T06:00:19Z","title":"Plunge spectra as discriminators of black hole mimickers","version":3},"reference_index":7,"source":"pdf_text","source_observed_at":"2026-05-18T18:16:19.200462Z"},"links":{"cited_paper":"/paper/1602.03837","citing_paper":"/paper/2509.09986"},"observation_digest":"sha256:c123f8124c4a02e489cf5a35b9ad92188ee9528b77315ac395d958a77f5c771f","observation_id":"48c58eac-0a38-41dd-9ab6-a583a7e84450","resolution":{"observed_at":"2026-05-18T18:16:42.950208Z","resolver_source":"local_arxiv","status":"verified_exact"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-04T06:34:03.388597+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-04T06:34:03.388597+00:00","source":"crossref"},{"observed_at":"2026-08-04T06:33:57.428241+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":{"arxiv_id":"1811.12907","last_updated":"2019-10-04T08:10:25Z","snapshot_observed_at":"2026-07-06T02:11:23.670680Z","submitted_at":"2018-11-30T17:34:09Z","title":"GWTC-1: A Gravitational-Wave Transient Catalog of Compact Binary Mergers Observed by LIGO and Virgo during the First and Second Observing Runs","version":3},"cited_work":{"arxiv_id":"1811.12907","doi":null,"metadata_source":"pith","pith_arxiv_id":"1811.12907","snapshot_observed_at":"2026-07-09T20:06:29.259645Z","title":"GWTC-1: A Gravitational-Wave Transient Catalog of Compact Binary Mergers Observed by LIGO and Virgo during the First and Second Observing Runs","venue":"astro-ph.HE","work_id":"ed2ab6af-3b84-426b-a8d5-c1f2cb6b0af7","year":2018},"citing_paper":{"arxiv_id":"2509.09986","last_updated":"2026-04-08T06:08:20Z","snapshot_observed_at":"2026-07-06T22:29:06.119014Z","submitted_at":"2025-09-12T06:00:19Z","title":"Plunge spectra as discriminators of black hole mimickers","version":3},"reference_index":8,"source":"pdf_text","source_observed_at":"2026-05-18T18:16:19.200462Z"},"links":{"cited_paper":"/paper/1811.12907","citing_paper":"/paper/2509.09986"},"observation_digest":"sha256:ccf4ca30000b044cc854b931e091079c5097d33a2958f1f332657664707cfbf0","observation_id":"5e218552-672d-4fa5-8748-2e16f94514f3","resolution":{"observed_at":"2026-05-18T18:16:43.070368Z","resolver_source":"local_arxiv","status":"verified_exact"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-04T06:34:03.388597+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-04T06:34:03.388597+00:00","source":"crossref"},{"observed_at":"2026-08-04T06:33:57.428241+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":{"arxiv_id":"2010.14527","last_updated":"2021-03-08T18:36:29Z","snapshot_observed_at":"2026-07-06T02:11:23.670680Z","submitted_at":"2020-10-27T18:01:31Z","title":"GWTC-2: Compact Binary Coalescences Observed by LIGO and Virgo During the First Half of the Third Observing Run","version":3},"cited_work":{"arxiv_id":"2010.14527","doi":null,"metadata_source":"pith","pith_arxiv_id":"2010.14527","snapshot_observed_at":"2026-07-10T13:17:05.780253Z","title":"GWTC-2: Compact Binary Coalescences Observed by LIGO and Virgo During the First Half of the Third Observing Run","venue":"gr-qc","work_id":"7410f8dd-43ce-418e-a2fe-baea0cf36999","year":2020},"citing_paper":{"arxiv_id":"2509.09986","last_updated":"2026-04-08T06:08:20Z","snapshot_observed_at":"2026-07-06T22:29:06.119014Z","submitted_at":"2025-09-12T06:00:19Z","title":"Plunge spectra as discriminators of black hole mimickers","version":3},"reference_index":9,"source":"pdf_text","source_observed_at":"2026-05-18T18:16:19.200462Z"},"links":{"cited_paper":"/paper/2010.14527","citing_paper":"/paper/2509.09986"},"observation_digest":"sha256:91c9abd732b6bdaf22b08d278015c32ebd9c6255464eaf01ea87a7355212d007","observation_id":"b1705907-2ead-4269-9584-71b7e968fc32","resolution":{"observed_at":"2026-05-18T18:16:43.037905Z","resolver_source":"local_arxiv","status":"verified_exact"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-04T06:34:03.388597+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-04T06:34:03.388597+00:00","source":"crossref"},{"observed_at":"2026-08-04T06:33:57.428241+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":"2005.05574","doi":null,"metadata_source":"arxiv_reference","pith_arxiv_id":null,"snapshot_observed_at":"2026-07-03T22:29:00.083174Z","title":"Akutsuet al.(KAGRA), PTEP2021, 05A101 (2021), arXiv:2005.05574 [physics.ins-det]","venue":null,"work_id":"5d6cbaec-f994-4631-bca0-649752990e3b","year":2021},"citing_paper":{"arxiv_id":"2509.09986","last_updated":"2026-04-08T06:08:20Z","snapshot_observed_at":"2026-07-06T22:29:06.119014Z","submitted_at":"2025-09-12T06:00:19Z","title":"Plunge spectra as discriminators of black hole mimickers","version":3},"reference_index":10,"source":"pdf_text","source_observed_at":"2026-05-18T18:16:19.200462Z"},"links":{"citing_paper":"/paper/2509.09986"},"observation_digest":"sha256:c2d0f6adce917d7a4b41f9aa01c5afd14b1538d31c986b623b6f5baf6a0990b5","observation_id":"20bf19f8-4fd6-432d-a7e9-0419c550a49e","resolution":{"observed_at":"2026-05-18T18:16:42.959612Z","resolver_source":"arxiv_id","status":"verified_exact"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-04T06:34:03.388597+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-04T06:34:03.388597+00:00","source":"crossref"},{"observed_at":"2026-08-04T06:33:57.428241+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":{"arxiv_id":"2111.03606","last_updated":"2023-10-23T13:37:50Z","snapshot_observed_at":"2026-08-02T06:32:23.817229Z","submitted_at":"2021-11-05T16:43:17Z","title":"GWTC-3: Compact Binary Coalescences Observed by LIGO and Virgo During the Second Part of the Third Observing Run","version":3},"cited_work":{"arxiv_id":"2111.03606","doi":"10.48550/arxiv.2111.03606","metadata_source":"pith","pith_arxiv_id":"2111.03606","snapshot_observed_at":"2026-07-10T06:15:00.866473Z","title":"GWTC-3: Compact Binary Coalescences Observed by LIGO and Virgo During the Second Part of the Third Observing Run","venue":"gr-qc","work_id":"da52a8d9-11a6-46c6-a2f5-89dab8381497","year":2021},"citing_paper":{"arxiv_id":"2509.09986","last_updated":"2026-04-08T06:08:20Z","snapshot_observed_at":"2026-07-06T22:29:06.119014Z","submitted_at":"2025-09-12T06:00:19Z","title":"Plunge spectra as discriminators of black hole mimickers","version":3},"reference_index":11,"source":"pdf_text","source_observed_at":"2026-05-18T18:16:19.200462Z"},"links":{"cited_paper":"/paper/2111.03606","citing_paper":"/paper/2509.09986"},"observation_digest":"sha256:d21965922a61fa10c976f1329ea17cc4cb12f4b463937424494163e61bb279ae","observation_id":"7aa72ed6-666a-4d34-84d8-5f8dad3e6cca","resolution":{"observed_at":"2026-05-18T18:16:42.945195Z","resolver_source":"local_arxiv","status":"verified_exact"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-04T06:34:03.388597+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-04T06:34:03.388597+00:00","source":"crossref"},{"observed_at":"2026-05-25T07:54:10.687378+00:00","source":"crossref_status_cache"},{"observed_at":"2026-05-25T07:54:10.687378+00:00","source":"openalex_status_cache"},{"observed_at":"2026-08-04T06:33:57.428241+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":{"arxiv_id":"1602.03841","last_updated":"2018-10-23T15:08:45Z","snapshot_observed_at":"2026-07-06T04:45:55.047976Z","submitted_at":"2016-02-11T19:26:48Z","title":"Tests of general relativity with GW150914","version":3},"cited_work":{"arxiv_id":"1602.03841","doi":null,"metadata_source":"pith","pith_arxiv_id":"1602.03841","snapshot_observed_at":"2026-07-10T23:37:42.489501Z","title":"Tests of general relativity with GW150914","venue":"gr-qc","work_id":"6360cb89-3e23-4c10-b265-09130bfbf688","year":2016},"citing_paper":{"arxiv_id":"2509.09986","last_updated":"2026-04-08T06:08:20Z","snapshot_observed_at":"2026-07-06T22:29:06.119014Z","submitted_at":"2025-09-12T06:00:19Z","title":"Plunge spectra as discriminators of black hole mimickers","version":3},"reference_index":12,"source":"pdf_text","source_observed_at":"2026-05-18T18:16:19.200462Z"},"links":{"cited_paper":"/paper/1602.03841","citing_paper":"/paper/2509.09986"},"observation_digest":"sha256:c2c41c79ce937b677adf78c61eba63658c3e6a5bff49c89f40deb0c043a0b7ee","observation_id":"74610721-00fd-4b80-ac79-10c6486a271d","resolution":{"observed_at":"2026-05-18T18:16:42.939694Z","resolver_source":"local_arxiv","status":"verified_exact"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-04T06:34:03.388597+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-04T06:34:03.388597+00:00","source":"crossref"},{"observed_at":"2026-08-04T06:33:57.428241+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":{"arxiv_id":"1811.00364","last_updated":"2019-07-29T15:54:28Z","snapshot_observed_at":"2026-07-06T07:12:00.243292Z","submitted_at":"2018-11-01T13:23:52Z","title":"Tests of General Relativity with GW170817","version":3},"cited_work":{"arxiv_id":"1811.00364","doi":null,"metadata_source":"pith","pith_arxiv_id":"1811.00364","snapshot_observed_at":"2026-07-09T20:56:34.422948Z","title":"Tests of General Relativity with GW170817","venue":"gr-qc","work_id":"1229a152-7a3c-4f8f-9e6c-b08a17aa5966","year":2018},"citing_paper":{"arxiv_id":"2509.09986","last_updated":"2026-04-08T06:08:20Z","snapshot_observed_at":"2026-07-06T22:29:06.119014Z","submitted_at":"2025-09-12T06:00:19Z","title":"Plunge spectra as discriminators of black hole mimickers","version":3},"reference_index":13,"source":"pdf_text","source_observed_at":"2026-05-18T18:16:19.200462Z"},"links":{"cited_paper":"/paper/1811.00364","citing_paper":"/paper/2509.09986"},"observation_digest":"sha256:ea1a6bd3b76d717918c455dd642cd915482daf7771293609d2ab709810c065f0","observation_id":"e35e6835-00df-4945-86be-09fbb1e90743","resolution":{"observed_at":"2026-05-18T18:16:43.059823Z","resolver_source":"local_arxiv","status":"verified_exact"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-04T06:34:03.388597+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-04T06:34:03.388597+00:00","source":"crossref"},{"observed_at":"2026-08-04T06:33:57.428241+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":{"arxiv_id":"1903.04467","last_updated":"2019-10-09T09:03:41Z","snapshot_observed_at":"2026-07-06T07:38:28.188454Z","submitted_at":"2019-03-11T17:43:43Z","title":"Tests of General Relativity with the Binary Black Hole Signals from the LIGO-Virgo Catalog GWTC-1","version":3},"cited_work":{"arxiv_id":"1903.04467","doi":null,"metadata_source":"pith","pith_arxiv_id":"1903.04467","snapshot_observed_at":"2026-07-10T23:37:41.405750Z","title":"Tests of General Relativity with the Binary Black Hole Signals from the LIGO-Virgo Catalog GWTC-1","venue":"gr-qc","work_id":"f83ceb1b-d07d-4ffc-bdc6-8f2da0284397","year":2019},"citing_paper":{"arxiv_id":"2509.09986","last_updated":"2026-04-08T06:08:20Z","snapshot_observed_at":"2026-07-06T22:29:06.119014Z","submitted_at":"2025-09-12T06:00:19Z","title":"Plunge spectra as discriminators of black hole mimickers","version":3},"reference_index":14,"source":"pdf_text","source_observed_at":"2026-05-18T18:16:19.200462Z"},"links":{"cited_paper":"/paper/1903.04467","citing_paper":"/paper/2509.09986"},"observation_digest":"sha256:759910ea4c498afdef94d5ce7670021e0ede8e5e3d3ab35bcc6c5388a198fb70","observation_id":"ccd80d0b-ec2b-4e42-8a2a-d7a69077fefe","resolution":{"observed_at":"2026-05-18T18:16:42.892360Z","resolver_source":"local_arxiv","status":"verified_exact"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-04T06:34:03.388597+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-04T06:34:03.388597+00:00","source":"crossref"},{"observed_at":"2026-08-04T06:33:57.428241+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":{"arxiv_id":"2010.14529","last_updated":"2025-09-10T17:43:53Z","snapshot_observed_at":"2026-07-06T02:11:23.670680Z","submitted_at":"2020-10-27T18:01:34Z","title":"Tests of General Relativity with Binary Black Holes from the second LIGO-Virgo Gravitational-Wave Transient Catalog","version":3},"cited_work":{"arxiv_id":"2010.14529","doi":null,"metadata_source":"pith","pith_arxiv_id":"2010.14529","snapshot_observed_at":"2026-07-09T20:56:34.492954Z","title":"Tests of General Relativity with Binary Black Holes from the second LIGO-Virgo Gravitational-Wave Transient Catalog","venue":"gr-qc","work_id":"62bb917e-cb23-4dd7-970e-02affb9488c2","year":2020},"citing_paper":{"arxiv_id":"2509.09986","last_updated":"2026-04-08T06:08:20Z","snapshot_observed_at":"2026-07-06T22:29:06.119014Z","submitted_at":"2025-09-12T06:00:19Z","title":"Plunge spectra as discriminators of black hole mimickers","version":3},"reference_index":15,"source":"pdf_text","source_observed_at":"2026-05-18T18:16:19.200462Z"},"links":{"cited_paper":"/paper/2010.14529","citing_paper":"/paper/2509.09986"},"observation_digest":"sha256:5fecc9abb7b212ec808a787d00c08d2376105e4c715548825f080ebc50f561df","observation_id":"048e41c1-9861-4af3-9010-a220b4c3fd29","resolution":{"observed_at":"2026-05-18T18:16:42.909001Z","resolver_source":"local_arxiv","status":"verified_exact"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-04T06:34:03.388597+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-04T06:34:03.388597+00:00","source":"crossref"},{"observed_at":"2026-08-04T06:33:57.428241+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":{"arxiv_id":"2112.06861","last_updated":"2025-11-17T15:05:31Z","snapshot_observed_at":"2026-08-02T22:41:06.793496Z","submitted_at":"2021-12-13T18:19:04Z","title":"Tests of General Relativity with GWTC-3","version":3},"cited_work":{"arxiv_id":"2112.06861","doi":"10.48550/arxiv.2112.06861","metadata_source":"pith","pith_arxiv_id":"2112.06861","snapshot_observed_at":"2026-07-10T23:37:41.449573Z","title":"Tests of General Relativity with GWTC-3","venue":"gr-qc","work_id":"a1a21d1d-87a3-4fbe-be6f-efe2ea2acb33","year":2021},"citing_paper":{"arxiv_id":"2509.09986","last_updated":"2026-04-08T06:08:20Z","snapshot_observed_at":"2026-07-06T22:29:06.119014Z","submitted_at":"2025-09-12T06:00:19Z","title":"Plunge spectra as discriminators of black hole mimickers","version":3},"reference_index":16,"source":"pdf_text","source_observed_at":"2026-05-18T18:16:19.200462Z"},"links":{"cited_paper":"/paper/2112.06861","citing_paper":"/paper/2509.09986"},"observation_digest":"sha256:ae7be9e62e7c074851fec705ea328256b4b0c3130f7f6920b34ce80e4a9a4acd","observation_id":"02960c6b-d07d-4bf9-9cab-171698a15c21","resolution":{"observed_at":"2026-05-18T18:16:42.918796Z","resolver_source":"local_arxiv","status":"verified_exact"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-04T06:34:03.388597+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-04T06:34:03.388597+00:00","source":"crossref"},{"observed_at":"2026-08-04T06:33:57.428241+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":{"arxiv_id":"gr-qc/0109035","last_updated":"2023-02-15T18:05:46Z","snapshot_observed_at":"2026-07-07T03:14:39.685358Z","submitted_at":"2001-09-11T04:27:23Z","title":"Gravitational Condensate Stars: An Alternative to Black Holes","version":6},"cited_work":{"arxiv_id":"gr-qc/0109035","doi":null,"metadata_source":"pith","pith_arxiv_id":"gr-qc/0109035","snapshot_observed_at":"2026-07-09T06:26:02.257520Z","title":"Gravitational Condensate Stars: An Alternative to Black Holes","venue":"gr-qc","work_id":"8fabb909-8758-46d6-8e39-bbe330778bae","year":2001},"citing_paper":{"arxiv_id":"2509.09986","last_updated":"2026-04-08T06:08:20Z","snapshot_observed_at":"2026-07-06T22:29:06.119014Z","submitted_at":"2025-09-12T06:00:19Z","title":"Plunge spectra as discriminators of black hole mimickers","version":3},"reference_index":17,"source":"pdf_text","source_observed_at":"2026-05-18T18:16:19.200462Z"},"links":{"cited_paper":"/paper/gr-qc/0109035","citing_paper":"/paper/2509.09986"},"observation_digest":"sha256:04af98ed5a5b9c27065572118b6c50542f9ea85daf0f83cb33072cf4261f8df7","observation_id":"35ff9c45-33f4-4220-b6d6-ea564f654b87","resolution":{"observed_at":"2026-05-18T18:16:42.986735Z","resolver_source":"arxiv_id","status":"verified_exact"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-04T06:34:03.388597+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-04T06:34:03.388597+00:00","source":"crossref"},{"observed_at":"2026-08-04T06:33:57.428241+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":"raw_reference","pith_arxiv_id":null,"snapshot_observed_at":"2026-06-05T21:23:00.469572Z","title":"Visser and D","venue":null,"work_id":"31988000-24f7-40fa-aa5b-1436c24b7b95","year":2004},"citing_paper":{"arxiv_id":"2509.09986","last_updated":"2026-04-08T06:08:20Z","snapshot_observed_at":"2026-07-06T22:29:06.119014Z","submitted_at":"2025-09-12T06:00:19Z","title":"Plunge spectra as discriminators of black hole mimickers","version":3},"reference_index":18,"source":"pdf_text","source_observed_at":"2026-05-18T18:16:19.200462Z"},"links":{"citing_paper":"/paper/2509.09986"},"observation_digest":"sha256:6122184e2c7e34f406c3f7574647bf30d8051e6db58c844aa52579cfe3da12a7","observation_id":"cecafdc6-f9e5-4cf1-a0c8-9bc77d00b33b","resolution":{"observed_at":"2026-05-18T18:16:43.999382Z","resolver_source":"raw_fallback","status":"verified_fuzzy"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-04T06:34:03.388597+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-04T06:34:03.388597+00:00","source":"crossref"},{"observed_at":"2026-08-04T06:33:57.428241+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":"raw_reference","pith_arxiv_id":null,"snapshot_observed_at":"2026-06-05T21:23:00.469572Z","title":"Jetzer,Boson stars,Phys","venue":null,"work_id":"84cb6d38-2432-44df-8f13-99ee4d7f400d","year":1992},"citing_paper":{"arxiv_id":"2509.09986","last_updated":"2026-04-08T06:08:20Z","snapshot_observed_at":"2026-07-06T22:29:06.119014Z","submitted_at":"2025-09-12T06:00:19Z","title":"Plunge spectra as discriminators of black hole mimickers","version":3},"reference_index":19,"source":"pdf_text","source_observed_at":"2026-05-18T18:16:19.200462Z"},"links":{"citing_paper":"/paper/2509.09986"},"observation_digest":"sha256:e00bc1808f1be1162cbbc1acc8e3b4457abc462c74c15d5c4e7627e5e69f120d","observation_id":"789e0e5f-aac5-4e84-a6d9-7c9e34639692","resolution":{"observed_at":"2026-05-18T18:16:44.002855Z","resolver_source":"raw_fallback","status":"verified_fuzzy"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-04T06:34:03.388597+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-04T06:34:03.388597+00:00","source":"crossref"},{"observed_at":"2026-08-04T06:33:57.428241+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":"raw_reference","pith_arxiv_id":null,"snapshot_observed_at":"2026-06-05T21:23:00.469572Z","title":null,"venue":null,"work_id":"89dbabc1-2b76-4aa6-bb00-6f948b6bdebe","year":2003},"citing_paper":{"arxiv_id":"2509.09986","last_updated":"2026-04-08T06:08:20Z","snapshot_observed_at":"2026-07-06T22:29:06.119014Z","submitted_at":"2025-09-12T06:00:19Z","title":"Plunge spectra as discriminators of black hole mimickers","version":3},"reference_index":20,"source":"pdf_text","source_observed_at":"2026-05-18T18:16:19.200462Z"},"links":{"citing_paper":"/paper/2509.09986"},"observation_digest":"sha256:dc10659d4949149b896be7a408b96946ab7043b213bd4295e89f75304c1a10e8","observation_id":"3697888a-d284-4873-97eb-3d853be1ab6a","resolution":{"observed_at":"2026-05-18T18:16:44.005902Z","resolver_source":"raw_fallback","status":"unresolved"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-04T06:34:03.388597+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-04T06:34:03.388597+00:00","source":"crossref"},{"observed_at":"2026-08-04T06:33:57.428241+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":"raw_reference","pith_arxiv_id":null,"snapshot_observed_at":"2026-06-05T21:23:00.469572Z","title":null,"venue":null,"work_id":"35334cdd-2d79-4f04-81bd-2f700b0445e1","year":2012},"citing_paper":{"arxiv_id":"2509.09986","last_updated":"2026-04-08T06:08:20Z","snapshot_observed_at":"2026-07-06T22:29:06.119014Z","submitted_at":"2025-09-12T06:00:19Z","title":"Plunge spectra as discriminators of black hole mimickers","version":3},"reference_index":21,"source":"pdf_text","source_observed_at":"2026-05-18T18:16:19.200462Z"},"links":{"citing_paper":"/paper/2509.09986"},"observation_digest":"sha256:ae52798eb07346bd7e55d759d127e5c96c631ce86e7611591e660f83b3918606","observation_id":"78c0654f-9fd4-49cb-bc01-9932906076ce","resolution":{"observed_at":"2026-05-18T18:16:44.010280Z","resolver_source":"raw_fallback","status":"unresolved"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-04T06:34:03.388597+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-04T06:34:03.388597+00:00","source":"crossref"},{"observed_at":"2026-08-04T06:33:57.428241+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":"raw_reference","pith_arxiv_id":null,"snapshot_observed_at":"2026-06-05T21:23:00.469572Z","title":null,"venue":null,"work_id":"da89353e-a607-49f7-98fb-d77318ac12b3","year":1974},"citing_paper":{"arxiv_id":"2509.09986","last_updated":"2026-04-08T06:08:20Z","snapshot_observed_at":"2026-07-06T22:29:06.119014Z","submitted_at":"2025-09-12T06:00:19Z","title":"Plunge spectra as discriminators of black hole mimickers","version":3},"reference_index":22,"source":"pdf_text","source_observed_at":"2026-05-18T18:16:19.200462Z"},"links":{"citing_paper":"/paper/2509.09986"},"observation_digest":"sha256:2b6da4709778dc54800960638a5f54bf09a6d788e65a205cc608536142eeb37f","observation_id":"16586ca1-ee3f-4d19-a74b-38e1ffae4b36","resolution":{"observed_at":"2026-05-18T18:16:43.992992Z","resolver_source":"raw_fallback","status":"unresolved"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-04T06:34:03.388597+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-04T06:34:03.388597+00:00","source":"crossref"},{"observed_at":"2026-08-04T06:33:57.428241+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":"raw_reference","pith_arxiv_id":null,"snapshot_observed_at":"2026-06-05T21:23:00.469572Z","title":null,"venue":null,"work_id":"140d3b34-18c0-4da0-b435-0b8ceb36a201","year":1995},"citing_paper":{"arxiv_id":"2509.09986","last_updated":"2026-04-08T06:08:20Z","snapshot_observed_at":"2026-07-06T22:29:06.119014Z","submitted_at":"2025-09-12T06:00:19Z","title":"Plunge spectra as discriminators of black hole mimickers","version":3},"reference_index":23,"source":"pdf_text","source_observed_at":"2026-05-18T18:16:19.200462Z"},"links":{"citing_paper":"/paper/2509.09986"},"observation_digest":"sha256:ab346bb9e98fe6e788b41a43b1b785b68f6d6321d7e2582ae263ea2c785c0428","observation_id":"384cbd0b-5569-4152-a8fa-143d25674563","resolution":{"observed_at":"2026-05-18T18:16:43.996164Z","resolver_source":"raw_fallback","status":"unresolved"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-04T06:34:03.388597+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-04T06:34:03.388597+00:00","source":"crossref"},{"observed_at":"2026-08-04T06:33:57.428241+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":"raw_reference","pith_arxiv_id":null,"snapshot_observed_at":"2026-06-05T21:23:00.469572Z","title":"Ashtekar, J","venue":null,"work_id":"836c5b92-86e2-4dbf-af19-e5c6aa73cbb9","year":1998},"citing_paper":{"arxiv_id":"2509.09986","last_updated":"2026-04-08T06:08:20Z","snapshot_observed_at":"2026-07-06T22:29:06.119014Z","submitted_at":"2025-09-12T06:00:19Z","title":"Plunge spectra as discriminators of black hole mimickers","version":3},"reference_index":24,"source":"pdf_text","source_observed_at":"2026-05-18T18:16:19.200462Z"},"links":{"citing_paper":"/paper/2509.09986"},"observation_digest":"sha256:22b335d1c628defe9dce5d5533d2c66c6039b42659336f0580e4f5a44d323f4a","observation_id":"f409dec6-f6b8-4c4a-a552-b99a1f6b5441","resolution":{"observed_at":"2026-05-18T18:16:43.988017Z","resolver_source":"raw_fallback","status":"verified_fuzzy"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-04T06:34:03.388597+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-04T06:34:03.388597+00:00","source":"crossref"},{"observed_at":"2026-08-04T06:33:57.428241+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":{"arxiv_id":"hep-th/0502050","last_updated":"2005-02-03T22:40:11Z","snapshot_observed_at":"2026-07-07T04:53:11.180776Z","submitted_at":"2005-02-03T22:40:11Z","title":"The fuzzball proposal for black holes: an elementary review","version":1},"cited_work":{"arxiv_id":"hep-th/0502050","doi":null,"metadata_source":"pith","pith_arxiv_id":"hep-th/0502050","snapshot_observed_at":"2026-07-04T02:09:22.627515Z","title":"The fuzzball proposal for black holes: an elementary review","venue":"hep-th","work_id":"c6f0e995-1e9b-4273-ac01-3bfb1badf430","year":2005},"citing_paper":{"arxiv_id":"2509.09986","last_updated":"2026-04-08T06:08:20Z","snapshot_observed_at":"2026-07-06T22:29:06.119014Z","submitted_at":"2025-09-12T06:00:19Z","title":"Plunge spectra as discriminators of black hole mimickers","version":3},"reference_index":25,"source":"pdf_text","source_observed_at":"2026-05-18T18:16:19.200462Z"},"links":{"cited_paper":"/paper/hep-th/0502050","citing_paper":"/paper/2509.09986"},"observation_digest":"sha256:34f4db9a21a891deb238ecce385725ed621539121710c42211a00c89bf5dabab","observation_id":"3a0fc8a3-ed95-4e1c-be83-737810b55eed","resolution":{"observed_at":"2026-05-18T18:16:43.011939Z","resolver_source":"local_arxiv","status":"verified_exact"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-04T06:34:03.388597+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-04T06:34:03.388597+00:00","source":"crossref"},{"observed_at":"2026-08-04T06:33:57.428241+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":"raw_reference","pith_arxiv_id":null,"snapshot_observed_at":"2026-06-05T21:23:00.469572Z","title":null,"venue":null,"work_id":"a271a81c-7c3b-4333-91ee-eebf912479a8","year":1988},"citing_paper":{"arxiv_id":"2509.09986","last_updated":"2026-04-08T06:08:20Z","snapshot_observed_at":"2026-07-06T22:29:06.119014Z","submitted_at":"2025-09-12T06:00:19Z","title":"Plunge spectra as discriminators of black hole mimickers","version":3},"reference_index":26,"source":"pdf_text","source_observed_at":"2026-05-18T18:16:19.200462Z"},"links":{"citing_paper":"/paper/2509.09986"},"observation_digest":"sha256:3d58ce08284e61bf4a72a2063f560f95725188cc8a2f8c144f48cb4da5fa45e8","observation_id":"cde344e1-fad6-401d-9a60-3ee9821ec227","resolution":{"observed_at":"2026-05-18T18:16:43.985222Z","resolver_source":"raw_fallback","status":"unresolved"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-04T06:34:03.388597+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-04T06:34:03.388597+00:00","source":"crossref"},{"observed_at":"2026-08-04T06:33:57.428241+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":{"arxiv_id":"1612.04889","last_updated":"2017-01-13T19:31:47Z","snapshot_observed_at":"2026-07-06T05:22:46.074568Z","submitted_at":"2016-12-15T00:15:06Z","title":"Not quite a black hole","version":2},"cited_work":{"arxiv_id":"1612.04889","doi":null,"metadata_source":"pith","pith_arxiv_id":"1612.04889","snapshot_observed_at":"2026-06-05T21:23:00.469572Z","title":"Not quite a black hole","venue":"gr-qc","work_id":"f20d9a4c-38c1-41b7-a0a3-847f8884b1bc","year":2016},"citing_paper":{"arxiv_id":"2509.09986","last_updated":"2026-04-08T06:08:20Z","snapshot_observed_at":"2026-07-06T22:29:06.119014Z","submitted_at":"2025-09-12T06:00:19Z","title":"Plunge spectra as discriminators of black hole mimickers","version":3},"reference_index":27,"source":"pdf_text","source_observed_at":"2026-05-18T18:16:19.200462Z"},"links":{"cited_paper":"/paper/1612.04889","citing_paper":"/paper/2509.09986"},"observation_digest":"sha256:cbecf722674de361690d402683dbc839bcd2a04bb326d110ce83775147b3922c","observation_id":"477fe151-f709-49c1-b951-0915b76ae6a5","resolution":{"observed_at":"2026-05-18T18:16:43.001841Z","resolver_source":"local_arxiv","status":"verified_exact"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-04T06:34:03.388597+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-04T06:34:03.388597+00:00","source":"crossref"},{"observed_at":"2026-08-04T06:33:57.428241+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":{"arxiv_id":"1811.07917","last_updated":"2019-05-15T14:18:41Z","snapshot_observed_at":"2026-07-06T07:15:51.575438Z","submitted_at":"2018-11-19T19:00:16Z","title":"Anisotropic stars as ultracompact objects in General Relativity","version":2},"cited_work":{"arxiv_id":"1811.07917","doi":null,"metadata_source":"pith","pith_arxiv_id":"1811.07917","snapshot_observed_at":"2026-07-04T02:09:22.326184Z","title":"Anisotropic stars as ultracompact objects in General Relativity","venue":"gr-qc","work_id":"d3dff4b9-f4c2-462f-afe3-94a95154204b","year":2018},"citing_paper":{"arxiv_id":"2509.09986","last_updated":"2026-04-08T06:08:20Z","snapshot_observed_at":"2026-07-06T22:29:06.119014Z","submitted_at":"2025-09-12T06:00:19Z","title":"Plunge spectra as discriminators of black hole mimickers","version":3},"reference_index":28,"source":"pdf_text","source_observed_at":"2026-05-18T18:16:19.200462Z"},"links":{"cited_paper":"/paper/1811.07917","citing_paper":"/paper/2509.09986"},"observation_digest":"sha256:011cecd029b6caadb97c4f7b5fbd65254a6a4cc5bce36fbabf6b0a2703246b92","observation_id":"8f880bd0-de65-48e1-89ea-3adf6b5b9cb9","resolution":{"observed_at":"2026-05-18T18:16:42.970393Z","resolver_source":"local_arxiv","status":"verified_exact"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-04T06:34:03.388597+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-04T06:34:03.388597+00:00","source":"crossref"},{"observed_at":"2026-08-04T06:33:57.428241+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":{"arxiv_id":"2006.14628","last_updated":"2020-09-09T21:29:00Z","snapshot_observed_at":"2026-07-06T09:32:51.851813Z","submitted_at":"2020-06-25T18:00:01Z","title":"How does a dark compact object ringdown?","version":2},"cited_work":{"arxiv_id":"2006.14628","doi":null,"metadata_source":"arxiv_reference","pith_arxiv_id":"2006.14628","snapshot_observed_at":"2026-07-02T09:26:50.670702Z","title":"Maggio, L","venue":null,"work_id":"526bcd52-541c-4da5-97b0-4a95ec92dd86","year":2020},"citing_paper":{"arxiv_id":"2509.09986","last_updated":"2026-04-08T06:08:20Z","snapshot_observed_at":"2026-07-06T22:29:06.119014Z","submitted_at":"2025-09-12T06:00:19Z","title":"Plunge spectra as discriminators of black hole mimickers","version":3},"reference_index":29,"source":"pdf_text","source_observed_at":"2026-05-18T18:16:19.200462Z"},"links":{"cited_paper":"/paper/2006.14628","citing_paper":"/paper/2509.09986"},"observation_digest":"sha256:5ef25fe16d01fea080eb34be9c2e0e6ae891499667dcacde6bfbe964ec859810","observation_id":"eb2bcbc3-5094-4a86-a070-54453caaeeb0","resolution":{"observed_at":"2026-05-18T18:16:43.049082Z","resolver_source":"arxiv_id","status":"verified_exact"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-04T06:34:03.388597+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-04T06:34:03.388597+00:00","source":"crossref"},{"observed_at":"2026-08-04T06:33:57.428241+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":"raw_reference","pith_arxiv_id":null,"snapshot_observed_at":"2026-06-05T21:23:00.469572Z","title":"Laghi, G","venue":null,"work_id":"1452d3f2-189c-4a90-a61f-1c0924501670","year":2021},"citing_paper":{"arxiv_id":"2509.09986","last_updated":"2026-04-08T06:08:20Z","snapshot_observed_at":"2026-07-06T22:29:06.119014Z","submitted_at":"2025-09-12T06:00:19Z","title":"Plunge spectra as discriminators of black hole mimickers","version":3},"reference_index":30,"source":"pdf_text","source_observed_at":"2026-05-18T18:16:19.200462Z"},"links":{"citing_paper":"/paper/2509.09986"},"observation_digest":"sha256:2ce5a8169dff06a2031bc11a3152ed23949229cb82f67b58322affb2f2ff38cc","observation_id":"9b9b7617-9be6-4563-87d5-1d8ada4777a4","resolution":{"observed_at":"2026-05-18T18:16:43.979466Z","resolver_source":"raw_fallback","status":"verified_fuzzy"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-04T06:34:03.388597+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-04T06:34:03.388597+00:00","source":"crossref"},{"observed_at":"2026-08-04T06:33:57.428241+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":"raw_reference","pith_arxiv_id":null,"snapshot_observed_at":"2026-06-05T21:23:00.469572Z","title":null,"venue":null,"work_id":"a23b620e-68f6-4c74-af0f-b015ac5ef6bb","year":2024},"citing_paper":{"arxiv_id":"2509.09986","last_updated":"2026-04-08T06:08:20Z","snapshot_observed_at":"2026-07-06T22:29:06.119014Z","submitted_at":"2025-09-12T06:00:19Z","title":"Plunge spectra as discriminators of black hole mimickers","version":3},"reference_index":31,"source":"pdf_text","source_observed_at":"2026-05-18T18:16:19.200462Z"},"links":{"citing_paper":"/paper/2509.09986"},"observation_digest":"sha256:396d9c52381a0818c94f8d2c7846efb7c9047fef5fdd3909d0f646413e2308cd","observation_id":"f253583c-148b-4311-884e-c1b6c27bda34","resolution":{"observed_at":"2026-05-18T18:16:43.982255Z","resolver_source":"raw_fallback","status":"unresolved"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-04T06:34:03.388597+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-04T06:34:03.388597+00:00","source":"crossref"},{"observed_at":"2026-08-04T06:33:57.428241+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":"raw_reference","pith_arxiv_id":null,"snapshot_observed_at":"2026-06-05T21:23:00.469572Z","title":"Cardoso, E","venue":null,"work_id":"e0f0f691-f3b3-47a9-8b32-2f5b49bfe5e2","year":2017},"citing_paper":{"arxiv_id":"2509.09986","last_updated":"2026-04-08T06:08:20Z","snapshot_observed_at":"2026-07-06T22:29:06.119014Z","submitted_at":"2025-09-12T06:00:19Z","title":"Plunge spectra as discriminators of black hole mimickers","version":3},"reference_index":32,"source":"pdf_text","source_observed_at":"2026-05-18T18:16:19.200462Z"},"links":{"citing_paper":"/paper/2509.09986"},"observation_digest":"sha256:0367f861b4f94642d555b0fdccf262a74f5f814d23e205f87244a133d3e710e3","observation_id":"5852f4b0-0876-4f10-bb60-b23d6a5ca8e7","resolution":{"observed_at":"2026-05-18T18:16:43.976572Z","resolver_source":"raw_fallback","status":"verified_fuzzy"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-04T06:34:03.388597+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-04T06:34:03.388597+00:00","source":"crossref"},{"observed_at":"2026-08-04T06:33:57.428241+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":{"arxiv_id":"2208.06235","last_updated":"2023-06-26T10:19:33Z","snapshot_observed_at":"2026-08-03T04:18:29.385309Z","submitted_at":"2022-08-12T12:10:21Z","title":"Dynamical Love for area quantized black holes","version":2},"cited_work":{"arxiv_id":"2208.06235","doi":null,"metadata_source":"arxiv_reference","pith_arxiv_id":"2208.06235","snapshot_observed_at":"2026-07-04T18:10:01.570896Z","title":"Dynamical Love numbers for area quantized black holes","venue":null,"work_id":"609a4403-afc6-424c-a348-3cd73465e0b9","year":2023},"citing_paper":{"arxiv_id":"2509.09986","last_updated":"2026-04-08T06:08:20Z","snapshot_observed_at":"2026-07-06T22:29:06.119014Z","submitted_at":"2025-09-12T06:00:19Z","title":"Plunge spectra as discriminators of black hole mimickers","version":3},"reference_index":33,"source":"pdf_text","source_observed_at":"2026-05-18T18:16:19.200462Z"},"links":{"cited_paper":"/paper/2208.06235","citing_paper":"/paper/2509.09986"},"observation_digest":"sha256:f1b2a63978294ddc637536754f1f0a303dede280ff6cb13d70e0938ef19f4af5","observation_id":"f5e19778-c3c4-493e-b9ba-6e08a5c5d8ae","resolution":{"observed_at":"2026-05-18T18:16:42.996733Z","resolver_source":"arxiv_id","status":"verified_exact"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-04T06:34:03.388597+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-04T06:34:03.388597+00:00","source":"crossref"},{"observed_at":"2026-08-04T06:33:57.428241+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":{"arxiv_id":"2310.06023","last_updated":"2024-10-14T11:41:47Z","snapshot_observed_at":"2026-07-06T16:30:04.288241Z","submitted_at":"2023-10-09T18:00:01Z","title":"Dynamical tidal Love numbers of Kerr-like compact objects","version":2},"cited_work":{"arxiv_id":"2310.06023","doi":null,"metadata_source":"arxiv_reference","pith_arxiv_id":"2310.06023","snapshot_observed_at":"2026-06-05T21:23:00.469572Z","title":"Chakraborty, E","venue":null,"work_id":"3c382144-0ab0-4aba-8316-93b1951d2f0f","year":2024},"citing_paper":{"arxiv_id":"2509.09986","last_updated":"2026-04-08T06:08:20Z","snapshot_observed_at":"2026-07-06T22:29:06.119014Z","submitted_at":"2025-09-12T06:00:19Z","title":"Plunge spectra as discriminators of black hole mimickers","version":3},"reference_index":34,"source":"pdf_text","source_observed_at":"2026-05-18T18:16:19.200462Z"},"links":{"cited_paper":"/paper/2310.06023","citing_paper":"/paper/2509.09986"},"observation_digest":"sha256:9ed0653d7b432ce00b222575cb60488983b7704c521ee0a4e3a99e491b26d448","observation_id":"59ec7337-079e-4d58-92ad-00d8d565bd81","resolution":{"observed_at":"2026-05-18T18:16:42.976410Z","resolver_source":"arxiv_id","status":"verified_exact"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-04T06:34:03.388597+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-04T06:34:03.388597+00:00","source":"crossref"},{"observed_at":"2026-08-04T06:33:57.428241+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":{"arxiv_id":"2404.06979","last_updated":"2024-06-06T08:07:15Z","snapshot_observed_at":"2026-07-06T17:58:16.989442Z","submitted_at":"2024-04-10T12:49:31Z","title":"Tidal Love numbers and approximate universal relations for fermion soliton stars","version":2},"cited_work":{"arxiv_id":"2404.06979","doi":null,"metadata_source":"arxiv_reference","pith_arxiv_id":"2404.06979","snapshot_observed_at":"2026-06-05T21:23:00.469572Z","title":"Berti, V","venue":null,"work_id":"96947528-60e0-4e54-840e-d8114dea4acb","year":2024},"citing_paper":{"arxiv_id":"2509.09986","last_updated":"2026-04-08T06:08:20Z","snapshot_observed_at":"2026-07-06T22:29:06.119014Z","submitted_at":"2025-09-12T06:00:19Z","title":"Plunge spectra as discriminators of black hole mimickers","version":3},"reference_index":35,"source":"pdf_text","source_observed_at":"2026-05-18T18:16:19.200462Z"},"links":{"cited_paper":"/paper/2404.06979","citing_paper":"/paper/2509.09986"},"observation_digest":"sha256:1b36ba69dbd43e7a18332da7b9f0ab5ac8b2e4c8bd3750c8a0cda38bc4269950","observation_id":"da831826-25eb-414d-b455-6d55659952c3","resolution":{"observed_at":"2026-05-18T18:16:42.981401Z","resolver_source":"arxiv_id","status":"verified_exact"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-04T06:34:03.388597+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-04T06:34:03.388597+00:00","source":"crossref"},{"observed_at":"2026-08-04T06:33:57.428241+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":{"arxiv_id":"2506.16516","last_updated":"2025-06-25T09:44:50Z","snapshot_observed_at":"2026-07-06T21:44:57.091757Z","submitted_at":"2025-06-19T18:00:22Z","title":"One Membrane to Love them all: Tidal deformations of compact objects from the membrane paradigm","version":2},"cited_work":{"arxiv_id":"2506.16516","doi":null,"metadata_source":"arxiv_reference","pith_arxiv_id":"2506.16516","snapshot_observed_at":"2026-06-05T21:23:00.469572Z","title":"Silvestrini, E","venue":null,"work_id":"b3e0b479-b8cc-4140-9178-24b05d0ea10a","year":2025},"citing_paper":{"arxiv_id":"2509.09986","last_updated":"2026-04-08T06:08:20Z","snapshot_observed_at":"2026-07-06T22:29:06.119014Z","submitted_at":"2025-09-12T06:00:19Z","title":"Plunge spectra as discriminators of black hole mimickers","version":3},"reference_index":36,"source":"pdf_text","source_observed_at":"2026-05-18T18:16:19.200462Z"},"links":{"cited_paper":"/paper/2506.16516","citing_paper":"/paper/2509.09986"},"observation_digest":"sha256:98a5120414c17ac1b44c974c4d03529db9c8ca8215c1a271bd11d7a52d42be57","observation_id":"bca1f8e4-2053-41b8-88ab-ee1119362918","resolution":{"observed_at":"2026-05-18T18:16:42.882311Z","resolver_source":"arxiv_id","status":"verified_exact"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-04T06:34:03.388597+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-04T06:34:03.388597+00:00","source":"crossref"},{"observed_at":"2026-08-04T06:33:57.428241+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":{"arxiv_id":"1709.01525","last_updated":"2017-09-05T18:00:26Z","snapshot_observed_at":"2026-07-06T05:58:15.108179Z","submitted_at":"2017-09-05T18:00:26Z","title":"Tests for the existence of horizons through gravitational wave echoes","version":1},"cited_work":{"arxiv_id":"1709.01525","doi":null,"metadata_source":"pith","pith_arxiv_id":"1709.01525","snapshot_observed_at":"2026-07-04T02:09:22.742288Z","title":"Tests for the existence of horizons through gravitational wave echoes","venue":"gr-qc","work_id":"aa925302-92c9-40fc-9a92-f49e9b143ffc","year":2017},"citing_paper":{"arxiv_id":"2509.09986","last_updated":"2026-04-08T06:08:20Z","snapshot_observed_at":"2026-07-06T22:29:06.119014Z","submitted_at":"2025-09-12T06:00:19Z","title":"Plunge spectra as discriminators of black hole mimickers","version":3},"reference_index":37,"source":"pdf_text","source_observed_at":"2026-05-18T18:16:19.200462Z"},"links":{"cited_paper":"/paper/1709.01525","citing_paper":"/paper/2509.09986"},"observation_digest":"sha256:f113f0b67742ea9935f061572af2b31018b5f48efdffb328bf5b4f0fab5caaaa","observation_id":"9d9ab36c-7443-4d5f-aa5c-90bbebc2160e","resolution":{"observed_at":"2026-05-18T18:16:42.823609Z","resolver_source":"local_arxiv","status":"verified_exact"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-04T06:34:03.388597+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-04T06:34:03.388597+00:00","source":"crossref"},{"observed_at":"2026-08-04T06:33:57.428241+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":{"arxiv_id":"1706.06155","last_updated":"2017-06-19T20:01:01Z","snapshot_observed_at":"2026-07-06T05:47:30.057781Z","submitted_at":"2017-06-19T20:01:01Z","title":"A recipe for echoes from exotic compact objects","version":1},"cited_work":{"arxiv_id":"1706.06155","doi":null,"metadata_source":"pith","pith_arxiv_id":"1706.06155","snapshot_observed_at":"2026-07-04T02:09:22.722815Z","title":"A recipe for echoes from exotic compact objects","venue":"gr-qc","work_id":"90fa0482-dc17-451b-8715-b060f0d0ca0a","year":2017},"citing_paper":{"arxiv_id":"2509.09986","last_updated":"2026-04-08T06:08:20Z","snapshot_observed_at":"2026-07-06T22:29:06.119014Z","submitted_at":"2025-09-12T06:00:19Z","title":"Plunge spectra as discriminators of black hole mimickers","version":3},"reference_index":38,"source":"pdf_text","source_observed_at":"2026-05-18T18:16:19.200462Z"},"links":{"cited_paper":"/paper/1706.06155","citing_paper":"/paper/2509.09986"},"observation_digest":"sha256:7a670052f557f497b5553c911fb3fc19a964e132d2ef16da2ab925e42caf6901","observation_id":"2b2201cb-bef4-4c22-881d-6c7433b21f5e","resolution":{"observed_at":"2026-05-18T18:16:42.964931Z","resolver_source":"local_arxiv","status":"verified_exact"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-04T06:34:03.388597+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-04T06:34:03.388597+00:00","source":"crossref"},{"observed_at":"2026-08-04T06:33:57.428241+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":{"arxiv_id":"1910.07841","last_updated":"2020-01-14T15:48:51Z","snapshot_observed_at":"2026-07-06T08:30:16.047619Z","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":"2509.09986","last_updated":"2026-04-08T06:08:20Z","snapshot_observed_at":"2026-07-06T22:29:06.119014Z","submitted_at":"2025-09-12T06:00:19Z","title":"Plunge spectra as discriminators of black hole mimickers","version":3},"reference_index":39,"source":"pdf_text","source_observed_at":"2026-05-18T18:16:19.200462Z"},"links":{"cited_paper":"/paper/1910.07841","citing_paper":"/paper/2509.09986"},"observation_digest":"sha256:03028336cafbe8a104227d613ae62a7fd80106d74ba373edde8d87a24faf8dfb","observation_id":"9b9d470b-5dcf-4db5-ab08-a8777ed57636","resolution":{"observed_at":"2026-05-18T18:16:42.852670Z","resolver_source":"arxiv_id","status":"verified_exact"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-04T06:34:03.388597+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-04T06:34:03.388597+00:00","source":"crossref"},{"observed_at":"2026-08-04T06:33:57.428241+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":{"arxiv_id":"1912.05419","last_updated":"2020-03-17T23:34:59Z","snapshot_observed_at":"2026-07-06T08:43:46.907186Z","submitted_at":"2019-12-11T16:23:03Z","title":"Spicing up the recipe for echoes from exotic compact objects: orbital differences and corrections in rotating backgrounds","version":2},"cited_work":{"arxiv_id":"1912.05419","doi":null,"metadata_source":"arxiv_reference","pith_arxiv_id":"1912.05419","snapshot_observed_at":"2026-06-05T21:23:00.469572Z","title":null,"venue":null,"work_id":"98f184bb-3069-4f97-882d-4f06f63bede2","year":2020},"citing_paper":{"arxiv_id":"2509.09986","last_updated":"2026-04-08T06:08:20Z","snapshot_observed_at":"2026-07-06T22:29:06.119014Z","submitted_at":"2025-09-12T06:00:19Z","title":"Plunge spectra as discriminators of black hole mimickers","version":3},"reference_index":40,"source":"pdf_text","source_observed_at":"2026-05-18T18:16:19.200462Z"},"links":{"cited_paper":"/paper/1912.05419","citing_paper":"/paper/2509.09986"},"observation_digest":"sha256:0ae477477688f32fdaae7769cc5fde1ff94194613b9bc48a7eee55f332d5807f","observation_id":"8f145b91-b723-47bf-9783-3393d8b286b6","resolution":{"observed_at":"2026-05-18T18:16:42.858709Z","resolver_source":"arxiv_id","status":"verified_exact"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-04T06:34:03.388597+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-04T06:34:03.388597+00:00","source":"crossref"},{"observed_at":"2026-08-04T06:33:57.428241+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":{"arxiv_id":"2002.04480","last_updated":"2021-05-24T06:32:45Z","snapshot_observed_at":"2026-07-06T08:56:30.534634Z","submitted_at":"2020-02-11T15:31:10Z","title":"Tidal heating of Quantum Black Holes and their imprints on gravitational waves","version":3},"cited_work":{"arxiv_id":"2002.04480","doi":null,"metadata_source":"arxiv_reference","pith_arxiv_id":"2002.04480","snapshot_observed_at":"2026-06-05T21:23:00.469572Z","title":"Datta, Tidal heating of Quantum Black Holes and their imprints on gravitational waves, Phys","venue":null,"work_id":"ea14b7cf-2236-41b4-b696-2b3384beef58","year":2020},"citing_paper":{"arxiv_id":"2509.09986","last_updated":"2026-04-08T06:08:20Z","snapshot_observed_at":"2026-07-06T22:29:06.119014Z","submitted_at":"2025-09-12T06:00:19Z","title":"Plunge spectra as discriminators of black hole mimickers","version":3},"reference_index":41,"source":"pdf_text","source_observed_at":"2026-05-18T18:16:19.200462Z"},"links":{"cited_paper":"/paper/2002.04480","citing_paper":"/paper/2509.09986"},"observation_digest":"sha256:f7b7567f04a78e626aca92397a61506d0a34b77344de9322101fefbc6e37729d","observation_id":"1cfb5296-f573-4632-bfce-32a2abde0d6f","resolution":{"observed_at":"2026-05-18T18:16:42.924052Z","resolver_source":"arxiv_id","status":"verified_exact"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-04T06:34:03.388597+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-04T06:34:03.388597+00:00","source":"crossref"},{"observed_at":"2026-08-04T06:33:57.428241+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":"raw_reference","pith_arxiv_id":null,"snapshot_observed_at":"2026-06-05T21:23:00.469572Z","title":"Agullo, V","venue":null,"work_id":"e020acb0-e7b8-4771-940a-3b31da4214a9","year":2021},"citing_paper":{"arxiv_id":"2509.09986","last_updated":"2026-04-08T06:08:20Z","snapshot_observed_at":"2026-07-06T22:29:06.119014Z","submitted_at":"2025-09-12T06:00:19Z","title":"Plunge spectra as discriminators of black hole mimickers","version":3},"reference_index":42,"source":"pdf_text","source_observed_at":"2026-05-18T18:16:19.200462Z"},"links":{"citing_paper":"/paper/2509.09986"},"observation_digest":"sha256:4c5c1d1c8bf3a93dd466c6bce41ada6317353bdeba83414ae68847e10110f9a1","observation_id":"48e6d2a7-574e-4d40-a4ca-0295c54e6a17","resolution":{"observed_at":"2026-05-18T18:16:43.969041Z","resolver_source":"raw_fallback","status":"verified_fuzzy"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-04T06:34:03.388597+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-04T06:34:03.388597+00:00","source":"crossref"},{"observed_at":"2026-08-04T06:33:57.428241+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":"raw_reference","pith_arxiv_id":null,"snapshot_observed_at":"2026-06-05T21:23:00.469572Z","title":"Chakraborty, E","venue":null,"work_id":"4fdc45a7-8576-4f62-9294-0ef5af020995","year":2022},"citing_paper":{"arxiv_id":"2509.09986","last_updated":"2026-04-08T06:08:20Z","snapshot_observed_at":"2026-07-06T22:29:06.119014Z","submitted_at":"2025-09-12T06:00:19Z","title":"Plunge spectra as discriminators of black hole mimickers","version":3},"reference_index":43,"source":"pdf_text","source_observed_at":"2026-05-18T18:16:19.200462Z"},"links":{"citing_paper":"/paper/2509.09986"},"observation_digest":"sha256:d7a6fc37bee2984b7d0ec8359f84f5501027045b1c47c9ca4d215f4b9e374ff9","observation_id":"8c8d1295-8a49-4a87-a799-22cb7bacf79b","resolution":{"observed_at":"2026-05-18T18:16:43.973947Z","resolver_source":"raw_fallback","status":"verified_fuzzy"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-04T06:34:03.388597+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-04T06:34:03.388597+00:00","source":"crossref"},{"observed_at":"2026-08-04T06:33:57.428241+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":{"arxiv_id":"2310.18022","last_updated":"2023-10-27T09:58:40Z","snapshot_observed_at":"2026-07-06T16:39:24.839340Z","submitted_at":"2023-10-27T09:58:40Z","title":"Formation and Stability of Area Quantized Black Holes","version":1},"cited_work":{"arxiv_id":"2310.18022","doi":null,"metadata_source":"arxiv_reference","pith_arxiv_id":"2310.18022","snapshot_observed_at":"2026-06-05T21:23:00.469572Z","title":"Chakravarti, R","venue":null,"work_id":"22b3f14d-62d8-40c2-baa9-2fe871b0a2f9","year":2024},"citing_paper":{"arxiv_id":"2509.09986","last_updated":"2026-04-08T06:08:20Z","snapshot_observed_at":"2026-07-06T22:29:06.119014Z","submitted_at":"2025-09-12T06:00:19Z","title":"Plunge spectra as discriminators of black hole mimickers","version":3},"reference_index":44,"source":"pdf_text","source_observed_at":"2026-05-18T18:16:19.200462Z"},"links":{"cited_paper":"/paper/2310.18022","citing_paper":"/paper/2509.09986"},"observation_digest":"sha256:6113f4081953b7a4963ad8ccdec42e30ce4c3218d280206b1d7d280905e02b17","observation_id":"a64527ba-cb0f-45f1-9609-cb2dec8ff60f","resolution":{"observed_at":"2026-05-18T18:16:42.887336Z","resolver_source":"arxiv_id","status":"verified_exact"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-04T06:34:03.388597+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-04T06:34:03.388597+00:00","source":"crossref"},{"observed_at":"2026-08-04T06:33:57.428241+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":{"arxiv_id":"2404.04013","last_updated":"2024-06-26T07:28:14Z","snapshot_observed_at":"2026-08-02T23:25:19.431718Z","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":"2509.09986","last_updated":"2026-04-08T06:08:20Z","snapshot_observed_at":"2026-07-06T22:29:06.119014Z","submitted_at":"2025-09-12T06:00:19Z","title":"Plunge spectra as discriminators of black hole mimickers","version":3},"reference_index":45,"source":"pdf_text","source_observed_at":"2026-05-18T18:16:19.200462Z"},"links":{"cited_paper":"/paper/2404.04013","citing_paper":"/paper/2509.09986"},"observation_digest":"sha256:b7a6116b0131c98afcb58709c521184cf4bae8d12d5350227f664d2fefa45749","observation_id":"00dab415-02b3-48f1-9f19-64ed2bfa094d","resolution":{"observed_at":"2026-05-18T18:16:42.913772Z","resolver_source":"arxiv_id","status":"verified_exact"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-04T06:34:03.388597+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-04T06:34:03.388597+00:00","source":"crossref"},{"observed_at":"2026-08-04T06:33:57.428241+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":{"arxiv_id":"2505.09014","last_updated":"2025-05-13T23:07:32Z","snapshot_observed_at":"2026-08-02T04:20:02.624757Z","submitted_at":"2025-05-13T23:07:32Z","title":"Black hole mimickers: from theory to observation","version":1},"cited_work":{"arxiv_id":"2505.09014","doi":null,"metadata_source":"arxiv_reference","pith_arxiv_id":"2505.09014","snapshot_observed_at":"2026-07-04T18:00:01.231524Z","title":"Bambi et al., Black hole mimickers: from theory to observation , 5, 2025 [ 2505.09014]","venue":null,"work_id":"1cb8042e-3b12-407b-88d2-78b8970c29c9","year":2025},"citing_paper":{"arxiv_id":"2509.09986","last_updated":"2026-04-08T06:08:20Z","snapshot_observed_at":"2026-07-06T22:29:06.119014Z","submitted_at":"2025-09-12T06:00:19Z","title":"Plunge spectra as discriminators of black hole mimickers","version":3},"reference_index":46,"source":"pdf_text","source_observed_at":"2026-05-18T18:16:19.200462Z"},"links":{"cited_paper":"/paper/2505.09014","citing_paper":"/paper/2509.09986"},"observation_digest":"sha256:ed6edc2d1f838ee83d30113d4aed7ce7602b69abe9b17618980b75deb0afe8e9","observation_id":"f539afa3-622d-4cd0-881c-eda081b9e316","resolution":{"observed_at":"2026-05-18T18:16:42.898306Z","resolver_source":"arxiv_id","status":"verified_exact"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-04T06:34:03.388597+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-04T06:34:03.388597+00:00","source":"crossref"},{"observed_at":"2026-08-04T06:33:57.428241+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":"raw_reference","pith_arxiv_id":null,"snapshot_observed_at":"2026-06-05T21:23:00.469572Z","title":"Cardoso, A","venue":null,"work_id":"f039b865-bf76-4c30-af30-355dcd528f06","year":2019},"citing_paper":{"arxiv_id":"2509.09986","last_updated":"2026-04-08T06:08:20Z","snapshot_observed_at":"2026-07-06T22:29:06.119014Z","submitted_at":"2025-09-12T06:00:19Z","title":"Plunge spectra as discriminators of black hole mimickers","version":3},"reference_index":47,"source":"pdf_text","source_observed_at":"2026-05-18T18:16:19.200462Z"},"links":{"citing_paper":"/paper/2509.09986"},"observation_digest":"sha256:0ca32e50570cfdb51d53e39db7d14c01b21488cba40f40ec9b541cb4f85ddb31","observation_id":"0fa89e7b-2abf-4d92-90b7-70912e09b726","resolution":{"observed_at":"2026-05-18T18:16:44.013883Z","resolver_source":"raw_fallback","status":"verified_fuzzy"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-04T06:34:03.388597+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-04T06:34:03.388597+00:00","source":"crossref"},{"observed_at":"2026-08-04T06:33:57.428241+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":"raw_reference","pith_arxiv_id":null,"snapshot_observed_at":"2026-06-05T21:23:00.469572Z","title":"Maggio, M","venue":null,"work_id":"f627add8-7f3f-4211-b2ba-17178c4609ce","year":2021},"citing_paper":{"arxiv_id":"2509.09986","last_updated":"2026-04-08T06:08:20Z","snapshot_observed_at":"2026-07-06T22:29:06.119014Z","submitted_at":"2025-09-12T06:00:19Z","title":"Plunge spectra as discriminators of black hole mimickers","version":3},"reference_index":48,"source":"pdf_text","source_observed_at":"2026-05-18T18:16:19.200462Z"},"links":{"citing_paper":"/paper/2509.09986"},"observation_digest":"sha256:262bacb3d4aa0f6144fd34f9e7e25667ea22ce21c017fe2601bfec98dd473562","observation_id":"72d9ac41-9dff-461d-a473-b529052cdc63","resolution":{"observed_at":"2026-05-18T18:16:44.017722Z","resolver_source":"raw_fallback","status":"verified_fuzzy"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-04T06:34:03.388597+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-04T06:34:03.388597+00:00","source":"crossref"},{"observed_at":"2026-08-04T06:33:57.428241+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":"raw_reference","pith_arxiv_id":null,"snapshot_observed_at":"2026-06-05T21:23:00.469572Z","title":null,"venue":null,"work_id":"6b77637b-6943-4088-8bc7-39628f7454cc","year":1978},"citing_paper":{"arxiv_id":"2509.09986","last_updated":"2026-04-08T06:08:20Z","snapshot_observed_at":"2026-07-06T22:29:06.119014Z","submitted_at":"2025-09-12T06:00:19Z","title":"Plunge spectra as discriminators of black hole mimickers","version":3},"reference_index":49,"source":"pdf_text","source_observed_at":"2026-05-18T18:16:19.200462Z"},"links":{"citing_paper":"/paper/2509.09986"},"observation_digest":"sha256:61d354e7887aa80b4f89177b75f24fc29e643b60cb3b48b865fb583dd5c646fe","observation_id":"cbbe2ff9-321c-47e5-a410-0bf8cf412372","resolution":{"observed_at":"2026-05-18T18:16:44.021349Z","resolver_source":"raw_fallback","status":"unresolved"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-04T06:34:03.388597+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-04T06:34:03.388597+00:00","source":"crossref"},{"observed_at":"2026-08-04T06:33:57.428241+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":{"arxiv_id":"gr-qc/9412027","last_updated":"1994-12-08T18:50:20Z","snapshot_observed_at":"2026-07-07T03:25:05.188192Z","submitted_at":"1994-12-08T18:50:20Z","title":"Gravitational radiation from a particle in circular orbit around a black hole. V. Black-hole absorption and tail corrections","version":1},"cited_work":{"arxiv_id":"gr-qc/9412027","doi":null,"metadata_source":"pith","pith_arxiv_id":"gr-qc/9412027","snapshot_observed_at":"2026-07-04T02:09:22.637872Z","title":"Gravitational radiation from a particle in circular orbit around a black hole. V. Black-hole absorption and tail corrections","venue":"gr-qc","work_id":"26d5d3b0-507e-427b-81c1-60533af7903c","year":1994},"citing_paper":{"arxiv_id":"2509.09986","last_updated":"2026-04-08T06:08:20Z","snapshot_observed_at":"2026-07-06T22:29:06.119014Z","submitted_at":"2025-09-12T06:00:19Z","title":"Plunge spectra as discriminators of black hole mimickers","version":3},"reference_index":50,"source":"pdf_text","source_observed_at":"2026-05-18T18:16:19.200462Z"},"links":{"cited_paper":"/paper/gr-qc/9412027","citing_paper":"/paper/2509.09986"},"observation_digest":"sha256:d55a61211d7d2e881e3b674b26fc3056f3e07e6de597a5038884136d92e0aa8f","observation_id":"4e73eb4b-cb44-4a34-bf50-f5e983d2b0be","resolution":{"observed_at":"2026-05-18T18:16:43.054292Z","resolver_source":"local_arxiv","status":"verified_exact"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-04T06:34:03.388597+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-04T06:34:03.388597+00:00","source":"crossref"},{"observed_at":"2026-08-04T06:33:57.428241+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":{"arxiv_id":"gr-qc/0003032","last_updated":"2000-03-08T18:55:53Z","snapshot_observed_at":"2026-07-07T03:12:11.561349Z","submitted_at":"2000-03-08T18:55:53Z","title":"The Transition from Inspiral to Plunge for a Compact Body in a Circular Equatorial Orbit Around a Massive, Spinning Black Hole","version":1},"cited_work":{"arxiv_id":"gr-qc/0003032","doi":null,"metadata_source":"pith","pith_arxiv_id":"gr-qc/0003032","snapshot_observed_at":"2026-06-05T21:23:00.469572Z","title":"The Transition from Inspiral to Plunge for a Compact Body in a Circular Equatorial Orbit Around a Massive, Spinning Black Hole","venue":"gr-qc","work_id":"a4d1f495-a24a-4266-b60e-7202c660d316","year":2000},"citing_paper":{"arxiv_id":"2509.09986","last_updated":"2026-04-08T06:08:20Z","snapshot_observed_at":"2026-07-06T22:29:06.119014Z","submitted_at":"2025-09-12T06:00:19Z","title":"Plunge spectra as discriminators of black hole mimickers","version":3},"reference_index":51,"source":"pdf_text","source_observed_at":"2026-05-18T18:16:19.200462Z"},"links":{"cited_paper":"/paper/gr-qc/0003032","citing_paper":"/paper/2509.09986"},"observation_digest":"sha256:29cd8e38f35186417c8d01d8c3ab7433426d4623e78dbdaf9148d42f3fa110c0","observation_id":"266576e4-7a92-4fa1-b269-7c0d3805b3ae","resolution":{"observed_at":"2026-05-18T18:16:42.875921Z","resolver_source":"local_arxiv","status":"verified_exact"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-04T06:34:03.388597+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-04T06:34:03.388597+00:00","source":"crossref"},{"observed_at":"2026-08-04T06:33:57.428241+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":{"arxiv_id":"gr-qc/0211023","last_updated":"2002-11-07T03:47:47Z","snapshot_observed_at":"2026-07-07T03:16:37.248186Z","submitted_at":"2002-11-07T03:47:47Z","title":"Transition from inspiral to plunge for eccentric equatorial Kerr orbits","version":1},"cited_work":{"arxiv_id":"gr-qc/0211023","doi":null,"metadata_source":"pith","pith_arxiv_id":"gr-qc/0211023","snapshot_observed_at":"2026-06-05T21:23:00.469572Z","title":"Transition from inspiral to plunge for eccentric equatorial Kerr orbits","venue":"gr-qc","work_id":"557298b8-409f-43c8-8573-711893f534c2","year":2002},"citing_paper":{"arxiv_id":"2509.09986","last_updated":"2026-04-08T06:08:20Z","snapshot_observed_at":"2026-07-06T22:29:06.119014Z","submitted_at":"2025-09-12T06:00:19Z","title":"Plunge spectra as discriminators of black hole mimickers","version":3},"reference_index":52,"source":"pdf_text","source_observed_at":"2026-05-18T18:16:19.200462Z"},"links":{"cited_paper":"/paper/gr-qc/0211023","citing_paper":"/paper/2509.09986"},"observation_digest":"sha256:5c4e7bedcec69a7971f10701203158fa85f94d709a7dff194b0d6e9626282f62","observation_id":"8355e978-40af-4a81-b39a-5ae536cc6077","resolution":{"observed_at":"2026-05-18T18:16:43.006985Z","resolver_source":"local_arxiv","status":"verified_exact"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-04T06:34:03.388597+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-04T06:34:03.388597+00:00","source":"crossref"},{"observed_at":"2026-08-04T06:33:57.428241+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":{"arxiv_id":"0803.4482","last_updated":"2008-05-08T15:45:12Z","snapshot_observed_at":"2026-07-06T01:35:51.632580Z","submitted_at":"2008-03-31T15:38:54Z","title":"The transition from adiabatic inspiral to geodesic plunge for a compact object around a massive Kerr black hole: Generic orbits","version":3},"cited_work":{"arxiv_id":"0803.4482","doi":null,"metadata_source":"pith","pith_arxiv_id":"0803.4482","snapshot_observed_at":"2026-06-05T21:23:00.469572Z","title":"The transition from adiabatic inspiral to geodesic plunge for a compact object around a massive Kerr black hole: Generic orbits","venue":"gr-qc","work_id":"a5ba8a09-c0cc-4972-8695-55279a2c1aaa","year":2008},"citing_paper":{"arxiv_id":"2509.09986","last_updated":"2026-04-08T06:08:20Z","snapshot_observed_at":"2026-07-06T22:29:06.119014Z","submitted_at":"2025-09-12T06:00:19Z","title":"Plunge spectra as discriminators of black hole mimickers","version":3},"reference_index":53,"source":"pdf_text","source_observed_at":"2026-05-18T18:16:19.200462Z"},"links":{"cited_paper":"/paper/0803.4482","citing_paper":"/paper/2509.09986"},"observation_digest":"sha256:c6795a546da6e04642dfdced2349c6214d5b92851596d56d6ba71de266776bfc","observation_id":"8f82c783-4d4a-403a-b0e9-3b441d8ba6a7","resolution":{"observed_at":"2026-05-18T18:16:43.032563Z","resolver_source":"local_arxiv","status":"verified_exact"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-04T06:34:03.388597+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-04T06:34:03.388597+00:00","source":"crossref"},{"observed_at":"2026-08-04T06:33:57.428241+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":{"arxiv_id":"0902.0573","last_updated":"2009-04-22T12:42:51Z","snapshot_observed_at":"2026-07-06T01:50:54.859348Z","submitted_at":"2009-02-03T18:10:58Z","title":"Gravitational self-force correction to the innermost stable circular orbit of a Schwarzschild black hole","version":2},"cited_work":{"arxiv_id":"0902.0573","doi":null,"metadata_source":"pith","pith_arxiv_id":"0902.0573","snapshot_observed_at":"2026-06-05T21:23:00.469572Z","title":"Gravitational self-force correction to the innermost stable circular orbit of a Schwarzschild black hole","venue":"gr-qc","work_id":"747f003a-ca47-46a4-87b6-380b7030132d","year":2009},"citing_paper":{"arxiv_id":"2509.09986","last_updated":"2026-04-08T06:08:20Z","snapshot_observed_at":"2026-07-06T22:29:06.119014Z","submitted_at":"2025-09-12T06:00:19Z","title":"Plunge spectra as discriminators of black hole mimickers","version":3},"reference_index":54,"source":"pdf_text","source_observed_at":"2026-05-18T18:16:19.200462Z"},"links":{"cited_paper":"/paper/0902.0573","citing_paper":"/paper/2509.09986"},"observation_digest":"sha256:3dd2a6455003a31245709090245ed181555d1bfd3d8d74af91948f4d91970e05","observation_id":"2a503ef1-dc58-4ec7-9337-6004a043a899","resolution":{"observed_at":"2026-05-18T18:16:42.846837Z","resolver_source":"local_arxiv","status":"verified_exact"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-04T06:34:03.388597+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-04T06:34:03.388597+00:00","source":"crossref"},{"observed_at":"2026-08-04T06:33:57.428241+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":{"arxiv_id":"0911.3899","last_updated":"2011-04-06T17:35:39Z","snapshot_observed_at":"2026-08-02T12:13:56.218511Z","submitted_at":"2009-11-20T13:49:32Z","title":"Post-ISCO Ringdown Amplitudes in Extreme Mass Ratio Inspiral","version":4},"cited_work":{"arxiv_id":"0911.3899","doi":null,"metadata_source":"pith","pith_arxiv_id":"0911.3899","snapshot_observed_at":"2026-07-02T19:57:19.352715Z","title":"Post-ISCO Ringdown Amplitudes in Extreme Mass Ratio Inspiral","venue":"gr-qc","work_id":"badb9df2-e33b-4bf7-99a3-1ac16f1033b0","year":2009},"citing_paper":{"arxiv_id":"2509.09986","last_updated":"2026-04-08T06:08:20Z","snapshot_observed_at":"2026-07-06T22:29:06.119014Z","submitted_at":"2025-09-12T06:00:19Z","title":"Plunge spectra as discriminators of black hole mimickers","version":3},"reference_index":55,"source":"pdf_text","source_observed_at":"2026-05-18T18:16:19.200462Z"},"links":{"cited_paper":"/paper/0911.3899","citing_paper":"/paper/2509.09986"},"observation_digest":"sha256:abfc23bbec54dcee18064135eb4628d2f04be6c1397771b99b4977a326196af2","observation_id":"887233a3-748b-44b0-a4dc-f854a250206f","resolution":{"observed_at":"2026-05-18T18:16:42.864307Z","resolver_source":"local_arxiv","status":"verified_exact"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-04T06:34:03.388597+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-04T06:34:03.388597+00:00","source":"crossref"},{"observed_at":"2026-08-04T06:33:57.428241+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":{"arxiv_id":"2204.11738","last_updated":"2022-10-25T14:02:30Z","snapshot_observed_at":"2026-07-06T13:03:32.889984Z","submitted_at":"2022-04-25T15:50:27Z","title":"Extreme Mass-Ratio Binary Black Hole Merger: Characteristics of the Test-Particle Limit","version":2},"cited_work":{"arxiv_id":"2204.11738","doi":null,"metadata_source":"arxiv_reference","pith_arxiv_id":"2204.11738","snapshot_observed_at":"2026-06-05T21:23:00.469572Z","title":"Rom and R","venue":null,"work_id":"578339da-b6ca-481a-8009-c343654a511a","year":2022},"citing_paper":{"arxiv_id":"2509.09986","last_updated":"2026-04-08T06:08:20Z","snapshot_observed_at":"2026-07-06T22:29:06.119014Z","submitted_at":"2025-09-12T06:00:19Z","title":"Plunge spectra as discriminators of black hole mimickers","version":3},"reference_index":56,"source":"pdf_text","source_observed_at":"2026-05-18T18:16:19.200462Z"},"links":{"cited_paper":"/paper/2204.11738","citing_paper":"/paper/2509.09986"},"observation_digest":"sha256:35dc66b00be8c2e042694a22a5c58133015917c355f8138f7e74e7284fa36146","observation_id":"09050522-bd50-4f67-bd7b-e68c400aa73c","resolution":{"observed_at":"2026-05-18T18:16:42.797915Z","resolver_source":"arxiv_id","status":"verified_exact"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-04T06:34:03.388597+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-04T06:34:03.388597+00:00","source":"crossref"},{"observed_at":"2026-08-04T06:33:57.428241+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":{"arxiv_id":"2506.22363","last_updated":"2026-05-10T17:37:43Z","snapshot_observed_at":"2026-07-06T21:48:45.170162Z","submitted_at":"2025-06-27T16:25:24Z","title":"Binary black holes in the heat of merger","version":2},"cited_work":{"arxiv_id":"2506.22363","doi":null,"metadata_source":"pith","pith_arxiv_id":"2506.22363","snapshot_observed_at":"2026-07-03T11:48:04.616091Z","title":"Binary black holes in the heat of merger","venue":"gr-qc","work_id":"fd5a5b0c-bb63-4e1c-9ad7-0828caea2638","year":2025},"citing_paper":{"arxiv_id":"2509.09986","last_updated":"2026-04-08T06:08:20Z","snapshot_observed_at":"2026-07-06T22:29:06.119014Z","submitted_at":"2025-09-12T06:00:19Z","title":"Plunge spectra as discriminators of black hole mimickers","version":3},"reference_index":57,"source":"pdf_text","source_observed_at":"2026-05-18T18:16:19.200462Z"},"links":{"cited_paper":"/paper/2506.22363","citing_paper":"/paper/2509.09986"},"observation_digest":"sha256:c50bb27130b092370e146a3cca3652266356f1ccfed3b986637cd77f52e84297","observation_id":"ad06f2ac-d084-4334-83db-1b38005e1a65","resolution":{"observed_at":"2026-05-18T18:16:42.792323Z","resolver_source":"local_arxiv","status":"verified_exact"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-04T06:34:03.388597+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-04T06:34:03.388597+00:00","source":"crossref"},{"observed_at":"2026-08-04T06:33:57.428241+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":{"arxiv_id":"1702.00786","last_updated":"2017-02-23T05:33:01Z","snapshot_observed_at":"2026-07-06T02:11:23.670680Z","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":"2026-07-10T10:47:02.063679Z","title":"Laser Interferometer Space Antenna","venue":"astro-ph.IM","work_id":"04a25305-b4d4-47f9-9613-efea8cc0292b","year":2017},"citing_paper":{"arxiv_id":"2509.09986","last_updated":"2026-04-08T06:08:20Z","snapshot_observed_at":"2026-07-06T22:29:06.119014Z","submitted_at":"2025-09-12T06:00:19Z","title":"Plunge spectra as discriminators of black hole mimickers","version":3},"reference_index":58,"source":"pdf_text","source_observed_at":"2026-05-18T18:16:19.200462Z"},"links":{"cited_paper":"/paper/1702.00786","citing_paper":"/paper/2509.09986"},"observation_digest":"sha256:5f45312e96caa8b668ff55414a3c07ea5b9c8f76eb1747d036038be3ea4b48dc","observation_id":"40f0ac20-8f78-4864-82d5-5d234ef5d88b","resolution":{"observed_at":"2026-05-18T18:16:42.803828Z","resolver_source":"local_arxiv","status":"verified_exact"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-04T06:34:03.388597+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-04T06:34:03.388597+00:00","source":"crossref"},{"observed_at":"2026-08-01T05:08:47.011282+00:00","source":"crossref_status_cache"},{"observed_at":"2026-08-01T05:08:47.011282+00:00","source":"openalex_status_cache"},{"observed_at":"2026-08-04T06:33:57.428241+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":{"arxiv_id":"2205.01597","last_updated":"2022-05-03T16:20:16Z","snapshot_observed_at":"2026-07-31T23:30:08.084874Z","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":"2509.09986","last_updated":"2026-04-08T06:08:20Z","snapshot_observed_at":"2026-07-06T22:29:06.119014Z","submitted_at":"2025-09-12T06:00:19Z","title":"Plunge spectra as discriminators of black hole mimickers","version":3},"reference_index":59,"source":"pdf_text","source_observed_at":"2026-05-18T18:16:19.200462Z"},"links":{"cited_paper":"/paper/2205.01597","citing_paper":"/paper/2509.09986"},"observation_digest":"sha256:7c96c45697223730f12ab26a8f7d55684d32e9ab221f77e39f0868b9340ac18a","observation_id":"5b67e922-07ef-40b4-b8a2-41f9b9b2b434","resolution":{"observed_at":"2026-05-18T18:16:42.934581Z","resolver_source":"arxiv_id","status":"verified_exact"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-04T06:34:03.388597+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-04T06:34:03.388597+00:00","source":"crossref"},{"observed_at":"2026-08-04T06:33:57.428241+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":{"arxiv_id":"2402.07571","last_updated":"2024-02-12T11:06:12Z","snapshot_observed_at":"2026-08-02T13:54:50.876049Z","submitted_at":"2024-02-12T11:06:12Z","title":"LISA Definition Study Report","version":1},"cited_work":{"arxiv_id":"2402.07571","doi":"10.1086/511063","metadata_source":"pith","pith_arxiv_id":"2402.07571","snapshot_observed_at":"2026-07-11T11:50:26.030339Z","title":"LISA Definition Study Report","venue":"astro-ph.CO","work_id":"0417ec60-d1d3-40b8-8dd8-853e19bc7adf","year":2024},"citing_paper":{"arxiv_id":"2509.09986","last_updated":"2026-04-08T06:08:20Z","snapshot_observed_at":"2026-07-06T22:29:06.119014Z","submitted_at":"2025-09-12T06:00:19Z","title":"Plunge spectra as discriminators of black hole mimickers","version":3},"reference_index":60,"source":"pdf_text","source_observed_at":"2026-05-18T18:16:19.200462Z"},"links":{"cited_paper":"/paper/2402.07571","citing_paper":"/paper/2509.09986"},"observation_digest":"sha256:68368cefabeaff4f6fdbfe2d8e590fd5485524b6441d0fb5344ba699dacb8281","observation_id":"219b8c6a-b525-43f3-9293-748c2abe6679","resolution":{"observed_at":"2026-05-18T18:16:42.929045Z","resolver_source":"local_arxiv","status":"verified_exact"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-04T06:34:03.388597+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-04T06:34:03.388597+00:00","source":"crossref"},{"observed_at":"2026-07-13T22:21:41.501094+00:00","source":"crossref_status_cache"},{"observed_at":"2026-07-13T22:21:41.501094+00:00","source":"openalex_status_cache"},{"observed_at":"2026-08-04T06:33:57.428241+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":{"arxiv_id":"1703.09722","last_updated":"2018-04-11T11:52:26Z","snapshot_observed_at":"2026-07-06T02:11:23.670680Z","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":"2509.09986","last_updated":"2026-04-08T06:08:20Z","snapshot_observed_at":"2026-07-06T22:29:06.119014Z","submitted_at":"2025-09-12T06:00:19Z","title":"Plunge spectra as discriminators of black hole mimickers","version":3},"reference_index":61,"source":"pdf_text","source_observed_at":"2026-05-18T18:16:19.200462Z"},"links":{"cited_paper":"/paper/1703.09722","citing_paper":"/paper/2509.09986"},"observation_digest":"sha256:16ea15bc7bacf83c13f7dc94a083f440b15ac2d8338a042c323b819c0059e6b3","observation_id":"f079037e-5c84-4541-bbb8-9bb32a3c7555","resolution":{"observed_at":"2026-05-18T18:16:42.809454Z","resolver_source":"local_arxiv","status":"verified_exact"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-04T06:34:03.388597+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-04T06:34:03.388597+00:00","source":"crossref"},{"observed_at":"2026-08-04T06:33:57.428241+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":{"arxiv_id":"1701.05808","last_updated":"2017-01-20T14:39:34Z","snapshot_observed_at":"2026-07-06T05:26:56.912030Z","submitted_at":"2017-01-20T14:39:34Z","title":"Black hole spectroscopy with coherent mode stacking","version":1},"cited_work":{"arxiv_id":"1701.05808","doi":null,"metadata_source":"pith","pith_arxiv_id":"1701.05808","snapshot_observed_at":"2026-07-04T18:00:01.222683Z","title":"Black hole spectroscopy with coherent mode stacking","venue":"gr-qc","work_id":"8cef2b0f-9be7-4b4f-8c68-7b60bc142b26","year":2017},"citing_paper":{"arxiv_id":"2509.09986","last_updated":"2026-04-08T06:08:20Z","snapshot_observed_at":"2026-07-06T22:29:06.119014Z","submitted_at":"2025-09-12T06:00:19Z","title":"Plunge spectra as discriminators of black hole mimickers","version":3},"reference_index":62,"source":"pdf_text","source_observed_at":"2026-05-18T18:16:19.200462Z"},"links":{"cited_paper":"/paper/1701.05808","citing_paper":"/paper/2509.09986"},"observation_digest":"sha256:1e393af772e6ec320e4f544cad281ef03e54d93f7dbd29dfe0874b404ec308fe","observation_id":"48c5bbee-2fbe-4b81-9cf0-005a8f10155f","resolution":{"observed_at":"2026-05-18T18:16:43.064336Z","resolver_source":"local_arxiv","status":"verified_exact"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-04T06:34:03.388597+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-04T06:34:03.388597+00:00","source":"crossref"},{"observed_at":"2026-08-04T06:33:57.428241+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":{"arxiv_id":"gr-qc/0307104","last_updated":"2003-07-23T22:24:58Z","snapshot_observed_at":"2026-07-07T03:18:10.155739Z","submitted_at":"2003-07-23T22:24:58Z","title":"Electromagnetic radiation from collisions at almost the speed of light: an extremely relativistic charged particle falling into a Schwarzschild black hole","version":1},"cited_work":{"arxiv_id":"gr-qc/0307104","doi":null,"metadata_source":"pith","pith_arxiv_id":"gr-qc/0307104","snapshot_observed_at":"2026-06-05T21:23:00.469572Z","title":"Electromagnetic radiation from collisions at almost the speed of light: an extremely relativistic charged particle falling into a Schwarzschild black hole","venue":"gr-qc","work_id":"302cf8ac-cbc7-46b4-aba8-e44bfffc7071","year":2003},"citing_paper":{"arxiv_id":"2509.09986","last_updated":"2026-04-08T06:08:20Z","snapshot_observed_at":"2026-07-06T22:29:06.119014Z","submitted_at":"2025-09-12T06:00:19Z","title":"Plunge spectra as discriminators of black hole mimickers","version":3},"reference_index":63,"source":"pdf_text","source_observed_at":"2026-05-18T18:16:19.200462Z"},"links":{"cited_paper":"/paper/gr-qc/0307104","citing_paper":"/paper/2509.09986"},"observation_digest":"sha256:78dd85accbf0c4e467f1c9b85e283e9e08728eb199144f9118067dba2925e343","observation_id":"ab8e3de3-1bf8-4bfe-9998-e350457f53a6","resolution":{"observed_at":"2026-05-18T18:16:42.829684Z","resolver_source":"local_arxiv","status":"verified_exact"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-04T06:34:03.388597+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-04T06:34:03.388597+00:00","source":"crossref"},{"observed_at":"2026-08-04T06:33:57.428241+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":"raw_reference","pith_arxiv_id":null,"snapshot_observed_at":"2026-06-05T21:23:00.469572Z","title":"Regge and J","venue":null,"work_id":"661c987d-6824-42ca-b47d-218cb5b5a40e","year":1957},"citing_paper":{"arxiv_id":"2509.09986","last_updated":"2026-04-08T06:08:20Z","snapshot_observed_at":"2026-07-06T22:29:06.119014Z","submitted_at":"2025-09-12T06:00:19Z","title":"Plunge spectra as discriminators of black hole mimickers","version":3},"reference_index":65,"source":"pdf_text","source_observed_at":"2026-05-18T18:16:19.200462Z"},"links":{"citing_paper":"/paper/2509.09986"},"observation_digest":"sha256:f6cdb85eaeed046d868753c4cbb386887eaaa1dedac720b416cb36763007dbab","observation_id":"5f16a3f1-5851-4aa6-91f7-a44f57d1bd66","resolution":{"observed_at":"2026-05-18T18:16:43.953097Z","resolver_source":"raw_fallback","status":"verified_fuzzy"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-04T06:34:03.388597+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-04T06:34:03.388597+00:00","source":"crossref"},{"observed_at":"2026-08-04T06:33:57.428241+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":"raw_reference","pith_arxiv_id":null,"snapshot_observed_at":"2026-06-05T21:23:00.469572Z","title":null,"venue":null,"work_id":"2839673e-162a-4238-9478-ed15ef0e2a0b","year":1970},"citing_paper":{"arxiv_id":"2509.09986","last_updated":"2026-04-08T06:08:20Z","snapshot_observed_at":"2026-07-06T22:29:06.119014Z","submitted_at":"2025-09-12T06:00:19Z","title":"Plunge spectra as discriminators of black hole mimickers","version":3},"reference_index":66,"source":"pdf_text","source_observed_at":"2026-05-18T18:16:19.200462Z"},"links":{"citing_paper":"/paper/2509.09986"},"observation_digest":"sha256:6d6e8ec93097f124f2914aabf7d5b1dea071db08799b13a30cf5307012e087f0","observation_id":"6907f0d6-82aa-438e-9884-27321c253012","resolution":{"observed_at":"2026-05-18T18:16:43.956005Z","resolver_source":"raw_fallback","status":"unresolved"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-04T06:34:03.388597+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-04T06:34:03.388597+00:00","source":"crossref"},{"observed_at":"2026-08-04T06:33:57.428241+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":"raw_reference","pith_arxiv_id":null,"snapshot_observed_at":"2026-06-05T21:23:00.469572Z","title":null,"venue":null,"work_id":"e787ce0f-2d8d-48f1-a7e5-694b5743512e","year":1970},"citing_paper":{"arxiv_id":"2509.09986","last_updated":"2026-04-08T06:08:20Z","snapshot_observed_at":"2026-07-06T22:29:06.119014Z","submitted_at":"2025-09-12T06:00:19Z","title":"Plunge spectra as discriminators of black hole mimickers","version":3},"reference_index":67,"source":"pdf_text","source_observed_at":"2026-05-18T18:16:19.200462Z"},"links":{"citing_paper":"/paper/2509.09986"},"observation_digest":"sha256:0d41338437910094e22319dff80ec421b9a66c1eff8a2aafd7c1b303af839248","observation_id":"623be1cb-8df2-43d8-8064-432d0e3a9ad0","resolution":{"observed_at":"2026-05-18T18:16:43.950167Z","resolver_source":"raw_fallback","status":"unresolved"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-04T06:34:03.388597+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-04T06:34:03.388597+00:00","source":"crossref"},{"observed_at":"2026-08-04T06:33:57.428241+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":"raw_reference","pith_arxiv_id":null,"snapshot_observed_at":"2026-06-05T21:23:00.469572Z","title":"Davis, R","venue":null,"work_id":"e17bd551-0e0b-47ea-9ae7-e2072bf63300","year":1971},"citing_paper":{"arxiv_id":"2509.09986","last_updated":"2026-04-08T06:08:20Z","snapshot_observed_at":"2026-07-06T22:29:06.119014Z","submitted_at":"2025-09-12T06:00:19Z","title":"Plunge spectra as discriminators of black hole mimickers","version":3},"reference_index":68,"source":"pdf_text","source_observed_at":"2026-05-18T18:16:19.200462Z"},"links":{"citing_paper":"/paper/2509.09986"},"observation_digest":"sha256:96a97196e1518254b7a9827dccd6ddadeb0fbfceadf1589c4f1f4b9dfcb0f826","observation_id":"65199320-0c14-4925-9176-265e89ca13d4","resolution":{"observed_at":"2026-05-18T18:16:43.941707Z","resolver_source":"raw_fallback","status":"verified_fuzzy"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-04T06:34:03.388597+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-04T06:34:03.388597+00:00","source":"crossref"},{"observed_at":"2026-08-04T06:33:57.428241+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":"raw_reference","pith_arxiv_id":null,"snapshot_observed_at":"2026-06-05T21:23:00.469572Z","title":"Tashiro and H","venue":null,"work_id":"7351ff6e-303f-4f2e-b5fc-818fb48f0b2a","year":1981},"citing_paper":{"arxiv_id":"2509.09986","last_updated":"2026-04-08T06:08:20Z","snapshot_observed_at":"2026-07-06T22:29:06.119014Z","submitted_at":"2025-09-12T06:00:19Z","title":"Plunge spectra as discriminators of black hole mimickers","version":3},"reference_index":69,"source":"pdf_text","source_observed_at":"2026-05-18T18:16:19.200462Z"},"links":{"citing_paper":"/paper/2509.09986"},"observation_digest":"sha256:990a81d615c071230af817de3d284b9042d2fc8aba028a803b02b015415ba21d","observation_id":"0ef16cab-9728-4e17-9812-a916a3a6427d","resolution":{"observed_at":"2026-05-18T18:16:43.944397Z","resolver_source":"raw_fallback","status":"verified_fuzzy"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-04T06:34:03.388597+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-04T06:34:03.388597+00:00","source":"crossref"},{"observed_at":"2026-08-04T06:33:57.428241+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":"raw_reference","pith_arxiv_id":null,"snapshot_observed_at":"2026-06-05T21:23:00.469572Z","title":"Shibata, T","venue":null,"work_id":"ce898d67-5648-4012-8b31-9f53b58c771a","year":1992},"citing_paper":{"arxiv_id":"2509.09986","last_updated":"2026-04-08T06:08:20Z","snapshot_observed_at":"2026-07-06T22:29:06.119014Z","submitted_at":"2025-09-12T06:00:19Z","title":"Plunge spectra as discriminators of black hole mimickers","version":3},"reference_index":70,"source":"pdf_text","source_observed_at":"2026-05-18T18:16:19.200462Z"},"links":{"citing_paper":"/paper/2509.09986"},"observation_digest":"sha256:04397c5f16c5b41b23909bfdbf3cb2a3a282408fbe58c1d82bb01229889eb644","observation_id":"6a124344-61e0-43c0-beea-9c79007c7a3e","resolution":{"observed_at":"2026-05-18T18:16:43.947594Z","resolver_source":"raw_fallback","status":"verified_fuzzy"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-04T06:34:03.388597+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-04T06:34:03.388597+00:00","source":"crossref"},{"observed_at":"2026-08-04T06:33:57.428241+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":{"arxiv_id":"gr-qc/0208060","last_updated":"2002-08-21T15:00:31Z","snapshot_observed_at":"2026-07-07T03:16:14.670986Z","submitted_at":"2002-08-21T15:00:31Z","title":"Gauge Problem in the Gravitational Self-Force I. Harmonic Gauge Approach in the Schwarzschild Background","version":1},"cited_work":{"arxiv_id":"gr-qc/0208060","doi":null,"metadata_source":"pith","pith_arxiv_id":"gr-qc/0208060","snapshot_observed_at":"2026-07-02T19:27:18.933107Z","title":"Gauge Problem in the Gravitational Self-Force I. Harmonic Gauge Approach in the Schwarzschild Background","venue":"gr-qc","work_id":"7c008d28-358e-444d-a8f5-eeaa6f0af0a1","year":2002},"citing_paper":{"arxiv_id":"2509.09986","last_updated":"2026-04-08T06:08:20Z","snapshot_observed_at":"2026-07-06T22:29:06.119014Z","submitted_at":"2025-09-12T06:00:19Z","title":"Plunge spectra as discriminators of black hole mimickers","version":3},"reference_index":71,"source":"pdf_text","source_observed_at":"2026-05-18T18:16:19.200462Z"},"links":{"cited_paper":"/paper/gr-qc/0208060","citing_paper":"/paper/2509.09986"},"observation_digest":"sha256:da0fb181feca269078554eaab1dab90f792958dbd0f608a6f8722f9a31c561ce","observation_id":"0d0a2257-392c-4dbf-91c6-7bec07434cad","resolution":{"observed_at":"2026-05-18T18:16:42.869886Z","resolver_source":"local_arxiv","status":"verified_exact"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-04T06:34:03.388597+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-04T06:34:03.388597+00:00","source":"crossref"},{"observed_at":"2026-08-04T06:33:57.428241+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":{"arxiv_id":"1003.0812","last_updated":"2010-05-19T06:11:45Z","snapshot_observed_at":"2026-07-06T02:08:33.599650Z","submitted_at":"2010-03-03T14:13:29Z","title":"Semianalytical estimates of scattering thresholds and gravitational radiation in ultrarelativistic black hole encounters","version":2},"cited_work":{"arxiv_id":"1003.0812","doi":null,"metadata_source":"pith","pith_arxiv_id":"1003.0812","snapshot_observed_at":"2026-07-03T03:27:35.843912Z","title":"Semianalytical estimates of scattering thresholds and gravitational radiation in ultrarelativistic black hole encounters","venue":"gr-qc","work_id":"3ec48350-ee76-4f17-9712-f30b214c8950","year":2010},"citing_paper":{"arxiv_id":"2509.09986","last_updated":"2026-04-08T06:08:20Z","snapshot_observed_at":"2026-07-06T22:29:06.119014Z","submitted_at":"2025-09-12T06:00:19Z","title":"Plunge spectra as discriminators of black hole mimickers","version":3},"reference_index":72,"source":"pdf_text","source_observed_at":"2026-05-18T18:16:19.200462Z"},"links":{"cited_paper":"/paper/1003.0812","citing_paper":"/paper/2509.09986"},"observation_digest":"sha256:4a772fb4759db468b9e66e8f4aa76e8b09948935bb6c9f2f257532de270f86ba","observation_id":"43ed0b11-755e-415b-a37e-e66af702a2af","resolution":{"observed_at":"2026-05-18T18:16:42.817920Z","resolver_source":"local_arxiv","status":"verified_exact"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-04T06:34:03.388597+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-04T06:34:03.388597+00:00","source":"crossref"},{"observed_at":"2026-08-04T06:33:57.428241+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":{"arxiv_id":"2308.14823","last_updated":"2024-01-25T13:00:46Z","snapshot_observed_at":"2026-07-06T16:11:27.419669Z","submitted_at":"2023-08-28T18:20:50Z","title":"Gravitational radiation from a particle plunging into a Schwarzschild black hole: frequency-domain and semirelativistic analyses","version":2},"cited_work":{"arxiv_id":"2308.14823","doi":null,"metadata_source":"arxiv_reference","pith_arxiv_id":"2308.14823","snapshot_observed_at":"2026-06-05T21:23:00.469572Z","title":null,"venue":null,"work_id":"246fbe4e-1ae4-4e11-a2c7-6458e184dcd3","year":2024},"citing_paper":{"arxiv_id":"2509.09986","last_updated":"2026-04-08T06:08:20Z","snapshot_observed_at":"2026-07-06T22:29:06.119014Z","submitted_at":"2025-09-12T06:00:19Z","title":"Plunge spectra as discriminators of black hole mimickers","version":3},"reference_index":73,"source":"pdf_text","source_observed_at":"2026-05-18T18:16:19.200462Z"},"links":{"cited_paper":"/paper/2308.14823","citing_paper":"/paper/2509.09986"},"observation_digest":"sha256:2876ed9306bde0b962883126a73ee08b49d8c8b0d5e6ea17b5750b69cb2cafd5","observation_id":"a3f81e3f-b405-4b01-9218-98f750b6abe6","resolution":{"observed_at":"2026-05-18T18:16:42.842120Z","resolver_source":"arxiv_id","status":"verified_exact"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-04T06:34:03.388597+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-04T06:34:03.388597+00:00","source":"crossref"},{"observed_at":"2026-08-04T06:33:57.428241+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":{"arxiv_id":"1003.2939","last_updated":"2010-03-15T15:11:19Z","snapshot_observed_at":"2026-07-06T02:04:37.545541Z","submitted_at":"2010-03-15T15:11:19Z","title":"A tapering window for time-domain templates and simulated signals in the detection of gravitational waves from coalescing compact binaries","version":1},"cited_work":{"arxiv_id":"1003.2939","doi":null,"metadata_source":"pith","pith_arxiv_id":"1003.2939","snapshot_observed_at":"2026-07-03T03:07:35.648626Z","title":"A tapering window for time-domain templates and simulated signals in the detection of gravitational waves from coalescing compact binaries","venue":"gr-qc","work_id":"dd6fbbbe-d1ae-40bb-bec4-87dd5e1c1d01","year":2010},"citing_paper":{"arxiv_id":"2509.09986","last_updated":"2026-04-08T06:08:20Z","snapshot_observed_at":"2026-07-06T22:29:06.119014Z","submitted_at":"2025-09-12T06:00:19Z","title":"Plunge spectra as discriminators of black hole mimickers","version":3},"reference_index":74,"source":"pdf_text","source_observed_at":"2026-05-18T18:16:19.200462Z"},"links":{"cited_paper":"/paper/1003.2939","citing_paper":"/paper/2509.09986"},"observation_digest":"sha256:ce5ee19e2fad0e603bc57181581eb16e53a5fb7ca9f62c6a76b332d15d9b5375","observation_id":"8c68df04-d656-4d42-b812-c534b6c3aa68","resolution":{"observed_at":"2026-05-18T18:16:42.836239Z","resolver_source":"local_arxiv","status":"verified_exact"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-04T06:34:03.388597+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-04T06:34:03.388597+00:00","source":"crossref"},{"observed_at":"2026-08-04T06:33:57.428241+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":{"arxiv_id":"2405.06197","last_updated":"2024-05-10T02:24:01Z","snapshot_observed_at":"2026-07-06T18:12:26.233112Z","submitted_at":"2024-05-10T02:24:01Z","title":"Improved frequency spectra of gravitational waves with memory in a binary-black-hole simulation","version":1},"cited_work":{"arxiv_id":"2405.06197","doi":null,"metadata_source":"arxiv_reference","pith_arxiv_id":"2405.06197","snapshot_observed_at":"2026-06-29T13:13:28.315676Z","title":"Chenet al., Phys","venue":null,"work_id":"e4b3c986-676a-4aae-a862-909e7b161e1c","year":2024},"citing_paper":{"arxiv_id":"2509.09986","last_updated":"2026-04-08T06:08:20Z","snapshot_observed_at":"2026-07-06T22:29:06.119014Z","submitted_at":"2025-09-12T06:00:19Z","title":"Plunge spectra as discriminators of black hole mimickers","version":3},"reference_index":75,"source":"pdf_text","source_observed_at":"2026-05-18T18:16:19.200462Z"},"links":{"cited_paper":"/paper/2405.06197","citing_paper":"/paper/2509.09986"},"observation_digest":"sha256:9eece7a6ca83f9bafb186bd593445df8418b4eabd2d625e72e9a4347e602753e","observation_id":"401de294-66f4-43e8-941d-71092bb47990","resolution":{"observed_at":"2026-05-18T18:16:43.028067Z","resolver_source":"arxiv_id","status":"verified_exact"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-04T06:34:03.388597+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-04T06:34:03.388597+00:00","source":"crossref"},{"observed_at":"2026-08-04T06:33:57.428241+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":{"arxiv_id":"2501.16433","last_updated":"2026-05-13T15:28:20Z","snapshot_observed_at":"2026-08-02T14:23:16.098022Z","submitted_at":"2025-01-27T19:00:06Z","title":"Greybody factors, reflectionless scattering modes, and echoes of ultracompact horizonless objects","version":3},"cited_work":{"arxiv_id":"2501.16433","doi":null,"metadata_source":"pith","pith_arxiv_id":"2501.16433","snapshot_observed_at":"2026-06-05T21:23:00.469572Z","title":"Greybody factors, reflectionless scattering modes, and echoes of ultracompact horizonless objects","venue":"gr-qc","work_id":"a9606f0f-2f29-4920-88c5-42bda47748f2","year":2025},"citing_paper":{"arxiv_id":"2509.09986","last_updated":"2026-04-08T06:08:20Z","snapshot_observed_at":"2026-07-06T22:29:06.119014Z","submitted_at":"2025-09-12T06:00:19Z","title":"Plunge spectra as discriminators of black hole mimickers","version":3},"reference_index":76,"source":"pdf_text","source_observed_at":"2026-05-18T18:16:19.200462Z"},"links":{"cited_paper":"/paper/2501.16433","citing_paper":"/paper/2509.09986"},"observation_digest":"sha256:5626f0d6bcd847af76f5709d8a96e71149ee9110a726384b38dff44de210f8b3","observation_id":"2543b218-14aa-422c-88f4-997c4a8820f8","resolution":{"observed_at":"2026-05-18T18:16:43.022667Z","resolver_source":"local_arxiv","status":"verified_exact"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-04T06:34:03.388597+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-04T06:34:03.388597+00:00","source":"crossref"},{"observed_at":"2026-08-04T06:33:57.428241+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":{"arxiv_id":"2406.04525","last_updated":"2024-06-06T21:51:21Z","snapshot_observed_at":"2026-08-03T15:49:04.628205Z","submitted_at":"2024-06-06T21:51:21Z","title":"(In)stability of the black hole greybody factors and ringdowns against a small-bump correction","version":1},"cited_work":{"arxiv_id":"2406.04525","doi":null,"metadata_source":"arxiv_reference","pith_arxiv_id":"2406.04525","snapshot_observed_at":"2026-06-05T21:23:00.469572Z","title":"Oshita, K","venue":null,"work_id":"861f9756-914d-4c3b-a0c4-8d3c890c800e","year":2024},"citing_paper":{"arxiv_id":"2509.09986","last_updated":"2026-04-08T06:08:20Z","snapshot_observed_at":"2026-07-06T22:29:06.119014Z","submitted_at":"2025-09-12T06:00:19Z","title":"Plunge spectra as discriminators of black hole mimickers","version":3},"reference_index":77,"source":"pdf_text","source_observed_at":"2026-05-18T18:16:19.200462Z"},"links":{"cited_paper":"/paper/2406.04525","citing_paper":"/paper/2509.09986"},"observation_digest":"sha256:13e17f9ddf78ffc875a0e71c1f82fb891722c95eaa8fd9bf621d7accd772f269","observation_id":"6405467e-31a3-4f1b-959c-6aa6a6c3780c","resolution":{"observed_at":"2026-05-18T18:16:43.042667Z","resolver_source":"arxiv_id","status":"verified_exact"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-04T06:34:03.388597+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-04T06:34:03.388597+00:00","source":"crossref"},{"observed_at":"2026-08-04T06:33:57.428241+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":{"arxiv_id":"2406.01692","last_updated":"2024-11-14T15:12:57Z","snapshot_observed_at":"2026-07-06T18:24:43.282366Z","submitted_at":"2024-06-03T18:00:06Z","title":"Ringdown stability: greybody factors as stable gravitational-wave observables","version":3},"cited_work":{"arxiv_id":"2406.01692","doi":null,"metadata_source":"arxiv_reference","pith_arxiv_id":"2406.01692","snapshot_observed_at":"2026-07-03T15:38:33.726176Z","title":"Ringdown stability: greybody factors as stable gravitational-wave observables","venue":null,"work_id":"b22b75ed-1ce7-48e0-b2fe-5e0a10012a9a","year":2024},"citing_paper":{"arxiv_id":"2509.09986","last_updated":"2026-04-08T06:08:20Z","snapshot_observed_at":"2026-07-06T22:29:06.119014Z","submitted_at":"2025-09-12T06:00:19Z","title":"Plunge spectra as discriminators of black hole mimickers","version":3},"reference_index":78,"source":"pdf_text","source_observed_at":"2026-05-18T18:16:19.200462Z"},"links":{"cited_paper":"/paper/2406.01692","citing_paper":"/paper/2509.09986"},"observation_digest":"sha256:3f7475e78204a08b85d6753f440fb853c9b06e6f20f8dd1720465d0f9cf889d0","observation_id":"b8142ee7-90c7-4fb6-acab-27ff2bea9872","resolution":{"observed_at":"2026-05-18T18:16:43.017665Z","resolver_source":"arxiv_id","status":"verified_exact"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-04T06:34:03.388597+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-04T06:34:03.388597+00:00","source":"crossref"},{"observed_at":"2026-08-04T06:33:57.428241+00:00","source":"retraction_watch"}],"state":"measured"}}],"paper":{"arxiv_id":"2509.09986","last_updated":"2026-04-08T06:08:20Z","latest_version":3,"primary_category":"gr-qc","snapshot_observed_at":"2026-07-06T22:29:06.119014Z","submitted_at":"2025-09-12T06:00:19Z","title":"Plunge spectra as discriminators of black hole mimickers"},"reference_resolution":{"displayed":77,"state_counts":{"malformed_identifier":0,"metadata_mismatch":0,"parse_uncertain":0,"unresolved":10,"verified_exact":52,"verified_fuzzy":15},"total_outbound_references":77},"refusal":"A citation records a reference. It does not transfer a finding from one paper to another.","schema":"pith.paper-citation-record.v1","standing_sources":[{"observed_at":"2026-08-04T06:34:03.388597+00:00","source":"crossref"},{"observed_at":"2026-08-04T06:33:57.428241+00:00","source":"retraction_watch"}],"thesis":"As of 4 August 2026, this Paper Citation Record lists 77 of 77 outbound references and 2 inbound Pith citation observations for arXiv:2509.09986."}