{"as_of":"2026-07-13T08:57:00Z","caps":{"database_statements":6,"inbound":100,"outbound":100},"context_digest":"sha256:16b906b785b33c76a3530cc72b2a4aa85585decc02da735254523499ab1d112b","coverage":[{"denominator":52,"lane":"reference_resolution","note":"Typed states for the displayed outbound observations.","records_observed":52,"source":"paper_references, paper_reference_links","source_observed_at":"2026-05-23T23:17:55.191990Z","state":"measured"},{"denominator":56,"lane":"standing_notices","note":"One-hop event checks from named stored sources.","records_observed":56,"source":"scholarly_work_events, retraction_status_cache","source_observed_at":"2026-07-13T06:30:06.624239+00:00","state":"measured"},{"denominator":4,"lane":"inbound_itemization","note":"Pith citing papers itemized under the disclosed page cap.","records_observed":4,"source":"paper_references, paper_reference_links","source_observed_at":"2026-06-30T08:47:20.958239Z","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":"2026-07-04T18:50:05.413142Z","state":"measured"}],"external_citation_measurements":[],"inbound":[{"citation":{"cited_paper":{"arxiv_id":"2407.00366","last_updated":"2025-12-17T10:16:02Z","snapshot_observed_at":"2026-07-06T02:11:23.670680Z","submitted_at":"2024-06-29T08:31:38Z","title":"Comparison of 4.5PN and 2SF gravitational energy fluxes from quasicircular compact binaries","version":2},"cited_work":{"arxiv_id":"2407.00366","doi":null,"metadata_source":"pith","pith_arxiv_id":"2407.00366","snapshot_observed_at":"2026-07-04T18:50:05.413142Z","title":"Comparison of 4.5PN and 2SF gravitational energy fluxes from quasicircular compact binaries","venue":"gr-qc","work_id":"6c9286ca-3900-4267-b4a1-90557933b14d","year":2024},"citing_paper":{"arxiv_id":"2510.16113","last_updated":"2026-04-26T06:30:13Z","snapshot_observed_at":"2026-07-06T02:11:23.670680Z","submitted_at":"2025-10-17T18:00:38Z","title":"Post-adiabatic self-force waveforms: slowly spinning primary and precessing secondary","version":2},"reference_index":37,"source":"pdf_text","source_observed_at":"2026-05-18T05:52:48.547252Z"},"links":{"cited_paper":"/paper/2407.00366","citing_paper":"/paper/2510.16113"},"observation_digest":"sha256:6b53279549d75f262eb2de23335a1c43ede672a275e8fd53f8168193d5f69d1f","observation_id":"801f249b-ec16-4ed4-97f5-a15eb257a4dd","resolution":{"observed_at":"2026-05-18T05:55:57.147248Z","resolver_source":"local_arxiv","status":"verified_exact"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-07-13T06:30:06.624239+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-07-13T06:30:06.624239+00:00","source":"crossref"},{"observed_at":"2026-07-13T06:30:01.874667+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":{"arxiv_id":"2407.00366","last_updated":"2025-12-17T10:16:02Z","snapshot_observed_at":"2026-07-06T02:11:23.670680Z","submitted_at":"2024-06-29T08:31:38Z","title":"Comparison of 4.5PN and 2SF gravitational energy fluxes from quasicircular compact binaries","version":2},"cited_work":{"arxiv_id":"2407.00366","doi":null,"metadata_source":"pith","pith_arxiv_id":"2407.00366","snapshot_observed_at":"2026-07-04T18:50:05.413142Z","title":"Comparison of 4.5PN and 2SF gravitational energy fluxes from quasicircular compact binaries","venue":"gr-qc","work_id":"6c9286ca-3900-4267-b4a1-90557933b14d","year":2024},"citing_paper":{"arxiv_id":"2606.24816","last_updated":"2026-06-23T17:02:02Z","snapshot_observed_at":"2026-07-06T02:11:23.670680Z","submitted_at":"2026-06-23T17:02:02Z","title":"The Bondi--Sachs gauge, BMS frames, and memory in black hole perturbation theory","version":1},"reference_index":85,"source":"pdf_text","source_observed_at":"2026-06-25T22:19:51.278679Z"},"links":{"cited_paper":"/paper/2407.00366","citing_paper":"/paper/2606.24816"},"observation_digest":"sha256:1aceb0f15615fca350d0a51c645ff556662b96ef957f26b444d0f2e9540cd38e","observation_id":"8ab29d9f-3af9-4254-b243-ed43073a61a5","resolution":{"observed_at":"2026-07-04T18:50:05.414310Z","resolver_source":"local_arxiv","status":"verified_exact"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-07-13T06:30:06.624239+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-07-13T06:30:06.624239+00:00","source":"crossref"},{"observed_at":"2026-07-13T06:30:01.874667+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":{"arxiv_id":"2407.00366","last_updated":"2025-12-17T10:16:02Z","snapshot_observed_at":"2026-07-06T02:11:23.670680Z","submitted_at":"2024-06-29T08:31:38Z","title":"Comparison of 4.5PN and 2SF gravitational energy fluxes from quasicircular compact binaries","version":2},"cited_work":{"arxiv_id":"2407.00366","doi":null,"metadata_source":"pith","pith_arxiv_id":"2407.00366","snapshot_observed_at":"2026-07-04T18:50:05.413142Z","title":"Comparison of 4.5PN and 2SF gravitational energy fluxes from quasicircular compact binaries","venue":"gr-qc","work_id":"6c9286ca-3900-4267-b4a1-90557933b14d","year":2024},"citing_paper":{"arxiv_id":"2606.27429","last_updated":"2026-06-25T18:00:07Z","snapshot_observed_at":"2026-07-07T00:01:39.205208Z","submitted_at":"2026-06-25T18:00:07Z","title":"Massive scalar fields in eccentric regime: Detectability and constraints from LISA observations of extreme mass-ratio inspirals","version":1},"reference_index":58,"source":"pdf_text","source_observed_at":"2026-06-29T01:52:24.227372Z"},"links":{"cited_paper":"/paper/2407.00366","citing_paper":"/paper/2606.27429"},"observation_digest":"sha256:cddc01af79b73eb165e0edad1616fe89011882ff69e07ed289029767c53d12eb","observation_id":"21cfb20e-4b8b-4de8-9ded-174bf09d0f9a","resolution":{"observed_at":"2026-07-01T18:35:58.932892Z","resolver_source":"local_arxiv","status":"verified_exact"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-07-13T06:30:06.624239+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-07-13T06:30:06.624239+00:00","source":"crossref"},{"observed_at":"2026-07-13T06:30:01.874667+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":{"arxiv_id":"2407.00366","last_updated":"2025-12-17T10:16:02Z","snapshot_observed_at":"2026-07-06T02:11:23.670680Z","submitted_at":"2024-06-29T08:31:38Z","title":"Comparison of 4.5PN and 2SF gravitational energy fluxes from quasicircular compact binaries","version":2},"cited_work":{"arxiv_id":"2407.00366","doi":null,"metadata_source":"pith","pith_arxiv_id":"2407.00366","snapshot_observed_at":"2026-07-04T18:50:05.413142Z","title":"Comparison of 4.5PN and 2SF gravitational energy fluxes from quasicircular compact binaries","venue":"gr-qc","work_id":"6c9286ca-3900-4267-b4a1-90557933b14d","year":2024},"citing_paper":{"arxiv_id":"2606.28937","last_updated":"2026-06-27T14:17:05Z","snapshot_observed_at":"2026-07-06T02:11:23.670680Z","submitted_at":"2026-06-27T14:17:05Z","title":"Quadrupole and quadratic-in-spin effects in quasicircular, spinning, asymmetric binaries","version":1},"reference_index":170,"source":"pdf_text","source_observed_at":"2026-06-30T08:47:20.958239Z"},"links":{"cited_paper":"/paper/2407.00366","citing_paper":"/paper/2606.28937"},"observation_digest":"sha256:87af3c8c8fefac5fd57606b0d4eac685f40d5a651440fdd463d3d575cf40b04d","observation_id":"7bde275c-dc2f-462f-974f-508220c1b67e","resolution":{"observed_at":"2026-06-30T08:54:30.024486Z","resolver_source":"local_arxiv","status":"verified_exact"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-07-13T06:30:06.624239+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-07-13T06:30:06.624239+00:00","source":"crossref"},{"observed_at":"2026-07-13T06:30:01.874667+00:00","source":"retraction_watch"}],"state":"measured"}}],"links":{"evidence":"/evidence","html":"/paper/2407.00366/citation-record","integrity":"/paper/2407.00366/integrity","json":"/paper/2407.00366/citation-record.json","paper":"/paper/2407.00366"},"outbound":[{"citation":{"cited_paper":{"arxiv_id":"1912.10055","last_updated":"2019-12-20T19:00:16Z","snapshot_observed_at":"2026-07-06T08:46:07.030878Z","submitted_at":"2019-12-20T19:00:16Z","title":"Ready for what lies ahead? -- Gravitational waveform accuracy requirements for future ground based detectors","version":1},"cited_work":{"arxiv_id":"1912.10055","doi":null,"metadata_source":"arxiv_reference","pith_arxiv_id":"1912.10055","snapshot_observed_at":"2026-07-04T18:50:05.392953Z","title":"P¨ urrer and C.-J","venue":null,"work_id":"c554b94c-6642-4922-a027-6a0c975066b0","year":2020},"citing_paper":{"arxiv_id":"2407.00366","last_updated":"2025-12-17T10:16:02Z","snapshot_observed_at":"2026-07-06T02:11:23.670680Z","submitted_at":"2024-06-29T08:31:38Z","title":"Comparison of 4.5PN and 2SF gravitational energy fluxes from quasicircular compact binaries","version":2},"reference_index":1,"source":"pdf_text","source_observed_at":"2026-05-23T23:17:55.191990Z"},"links":{"cited_paper":"/paper/1912.10055","citing_paper":"/paper/2407.00366"},"observation_digest":"sha256:32ed6421f9b293e19f084a74ce169cde06bd075ce8d8ba7f6c1e197df15af290","observation_id":"24e89aa5-ef81-47a5-9d1d-2b6e70bcd244","resolution":{"observed_at":"2026-05-23T23:18:35.973754Z","resolver_source":"arxiv_id","status":"verified_exact"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-07-13T06:30:06.624239+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-07-13T06:30:06.624239+00:00","source":"crossref"},{"observed_at":"2026-07-13T06:30:01.874667+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":"2404.05811","doi":null,"metadata_source":"arxiv_reference","pith_arxiv_id":null,"snapshot_observed_at":"2026-07-04T18:50:05.451295Z","title":"Dhani, S","venue":null,"work_id":"65101c84-92a2-45d6-8144-5377f12bd8bd","year":2025},"citing_paper":{"arxiv_id":"2407.00366","last_updated":"2025-12-17T10:16:02Z","snapshot_observed_at":"2026-07-06T02:11:23.670680Z","submitted_at":"2024-06-29T08:31:38Z","title":"Comparison of 4.5PN and 2SF gravitational energy fluxes from quasicircular compact binaries","version":2},"reference_index":2,"source":"pdf_text","source_observed_at":"2026-05-23T23:17:55.191990Z"},"links":{"citing_paper":"/paper/2407.00366"},"observation_digest":"sha256:70abf779dac1b5b831bafa91610cde73af0e6a20cac71f86254c1f1ef6916dd9","observation_id":"0f531bae-1bec-41bd-9de0-c2d5e9540544","resolution":{"observed_at":"2026-05-23T23:18:35.850500Z","resolver_source":"arxiv_id","status":"verified_exact"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-07-13T06:30:06.624239+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-07-13T06:30:06.624239+00:00","source":"crossref"},{"observed_at":"2026-07-13T06:30:01.874667+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":{"arxiv_id":"2311.01300","last_updated":"2026-05-01T11:22:19Z","snapshot_observed_at":"2026-07-06T02:11:23.670680Z","submitted_at":"2023-11-02T15:15:33Z","title":"Waveform Modelling for the Laser Interferometer Space Antenna","version":3},"cited_work":{"arxiv_id":"2311.01300","doi":"10.1093/mnras/stad412","metadata_source":"pith","pith_arxiv_id":"2311.01300","snapshot_observed_at":"2026-07-11T11:50:26.030339Z","title":"Waveform Modelling for the Laser Interferometer Space Antenna","venue":"gr-qc","work_id":"2fcc1ea4-a549-4476-aa65-921ab7bab52b","year":2023},"citing_paper":{"arxiv_id":"2407.00366","last_updated":"2025-12-17T10:16:02Z","snapshot_observed_at":"2026-07-06T02:11:23.670680Z","submitted_at":"2024-06-29T08:31:38Z","title":"Comparison of 4.5PN and 2SF gravitational energy fluxes from quasicircular compact binaries","version":2},"reference_index":3,"source":"pdf_text","source_observed_at":"2026-05-23T23:17:55.191990Z"},"links":{"cited_paper":"/paper/2311.01300","citing_paper":"/paper/2407.00366"},"observation_digest":"sha256:eb8fd029e17b7516aa507650756a4c4f01ee7fd84a23e08907219a2559658f9a","observation_id":"de30d55f-1e79-4baf-8805-6ca791bcad95","resolution":{"observed_at":"2026-05-23T23:18:35.888741Z","resolver_source":"local_arxiv","status":"verified_exact"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-07-13T06:30:06.624239+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-07-13T06:30:06.624239+00:00","source":"crossref"},{"observed_at":"2026-07-13T06:30:01.874667+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":"Pound, B","venue":null,"work_id":"c5f6a5a3-2f26-41c3-beca-49f088ac8c61","year":2020},"citing_paper":{"arxiv_id":"2407.00366","last_updated":"2025-12-17T10:16:02Z","snapshot_observed_at":"2026-07-06T02:11:23.670680Z","submitted_at":"2024-06-29T08:31:38Z","title":"Comparison of 4.5PN and 2SF gravitational energy fluxes from quasicircular compact binaries","version":2},"reference_index":4,"source":"pdf_text","source_observed_at":"2026-05-23T23:17:55.191990Z"},"links":{"citing_paper":"/paper/2407.00366"},"observation_digest":"sha256:fe305d431c57b6a7b8536632ea958b1c126d688d335caf41a4d0051977e88b28","observation_id":"ee6f8aa0-53c2-4726-8370-f0db93bb8dfa","resolution":{"observed_at":"2026-05-23T23:18:36.302718Z","resolver_source":"raw_fallback","status":"verified_fuzzy"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-07-13T06:30:06.624239+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-07-13T06:30:06.624239+00:00","source":"crossref"},{"observed_at":"2026-07-13T06:30:01.874667+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":{"arxiv_id":"2107.01298","last_updated":"2021-10-09T21:35:14Z","snapshot_observed_at":"2026-07-06T11:25:35.527703Z","submitted_at":"2021-07-02T23:08:31Z","title":"Gravitational-wave energy flux for compact binaries through second order in the mass ratio","version":2},"cited_work":{"arxiv_id":"2107.01298","doi":null,"metadata_source":"arxiv_reference","pith_arxiv_id":"2107.01298","snapshot_observed_at":"2026-07-04T18:50:05.316238Z","title":"Warburton, A","venue":null,"work_id":"7ba33353-40d7-4470-91de-2962181fbd73","year":2021},"citing_paper":{"arxiv_id":"2407.00366","last_updated":"2025-12-17T10:16:02Z","snapshot_observed_at":"2026-07-06T02:11:23.670680Z","submitted_at":"2024-06-29T08:31:38Z","title":"Comparison of 4.5PN and 2SF gravitational energy fluxes from quasicircular compact binaries","version":2},"reference_index":5,"source":"pdf_text","source_observed_at":"2026-05-23T23:17:55.191990Z"},"links":{"cited_paper":"/paper/2107.01298","citing_paper":"/paper/2407.00366"},"observation_digest":"sha256:005781399911c39ab337909d3f1264cdbd3ad3f96ed4e7c7540eca69972cbeb0","observation_id":"0c39f4d4-bda7-464e-b4e3-4e0262e2908d","resolution":{"observed_at":"2026-05-23T23:18:35.924622Z","resolver_source":"arxiv_id","status":"verified_exact"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-07-13T06:30:06.624239+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-07-13T06:30:06.624239+00:00","source":"crossref"},{"observed_at":"2026-07-13T06:30:01.874667+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":{"arxiv_id":"2112.12265","last_updated":"2023-03-29T15:24:30Z","snapshot_observed_at":"2026-07-06T12:21:45.521326Z","submitted_at":"2021-12-22T23:09:31Z","title":"Gravitational waveforms for compact binaries from second-order self-force theory","version":2},"cited_work":{"arxiv_id":"2112.12265","doi":null,"metadata_source":"arxiv_reference","pith_arxiv_id":"2112.12265","snapshot_observed_at":"2026-07-04T18:50:05.255776Z","title":"Wardell, A","venue":null,"work_id":"e358e2a1-cfbd-463e-b5b2-dbde61100e0f","year":2023},"citing_paper":{"arxiv_id":"2407.00366","last_updated":"2025-12-17T10:16:02Z","snapshot_observed_at":"2026-07-06T02:11:23.670680Z","submitted_at":"2024-06-29T08:31:38Z","title":"Comparison of 4.5PN and 2SF gravitational energy fluxes from quasicircular compact binaries","version":2},"reference_index":6,"source":"pdf_text","source_observed_at":"2026-05-23T23:17:55.191990Z"},"links":{"cited_paper":"/paper/2112.12265","citing_paper":"/paper/2407.00366"},"observation_digest":"sha256:bb6d3964bfb8520769b5d1de29cade6f28e6426da77693bd9183a179516a6021","observation_id":"3e2c6d84-3058-4e08-9104-96325badb6b5","resolution":{"observed_at":"2026-05-23T23:18:35.943118Z","resolver_source":"arxiv_id","status":"verified_exact"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-07-13T06:30:06.624239+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-07-13T06:30:06.624239+00:00","source":"crossref"},{"observed_at":"2026-07-13T06:30:01.874667+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":{"arxiv_id":"1401.4548","last_updated":"2014-03-28T16:27:21Z","snapshot_observed_at":"2026-07-06T03:33:40.618501Z","submitted_at":"2014-01-18T15:39:20Z","title":"Nonlocal-in-time action for the fourth post-Newtonian conservative dynamics of two-body systems","version":2},"cited_work":{"arxiv_id":"1401.4548","doi":null,"metadata_source":"pith","pith_arxiv_id":"1401.4548","snapshot_observed_at":"2026-06-30T20:15:04.659120Z","title":"Nonlocal-in-time action for the fourth post-Newtonian conservative dynamics of two-body systems","venue":"gr-qc","work_id":"e304c9b7-2e4a-4101-911f-7c658c374943","year":2014},"citing_paper":{"arxiv_id":"2407.00366","last_updated":"2025-12-17T10:16:02Z","snapshot_observed_at":"2026-07-06T02:11:23.670680Z","submitted_at":"2024-06-29T08:31:38Z","title":"Comparison of 4.5PN and 2SF gravitational energy fluxes from quasicircular compact binaries","version":2},"reference_index":7,"source":"pdf_text","source_observed_at":"2026-05-23T23:17:55.191990Z"},"links":{"cited_paper":"/paper/1401.4548","citing_paper":"/paper/2407.00366"},"observation_digest":"sha256:58a8a871265d297f31c0162a3aee5b084c4c5bdf1e6b20742fedbaea4b7151fe","observation_id":"74ec24fb-0f19-4e9f-aa9a-c0688cadfd81","resolution":{"observed_at":"2026-05-23T23:18:35.936862Z","resolver_source":"local_arxiv","status":"verified_exact"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-07-13T06:30:06.624239+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-07-13T06:30:06.624239+00:00","source":"crossref"},{"observed_at":"2026-07-13T06:30:01.874667+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":{"arxiv_id":"1601.01283","last_updated":"2016-04-27T08:04:28Z","snapshot_observed_at":"2026-07-06T04:42:04.003177Z","submitted_at":"2016-01-06T19:27:55Z","title":"Conservative dynamics of two-body systems at the fourth post-Newtonian approximation of general relativity","version":2},"cited_work":{"arxiv_id":"1601.01283","doi":null,"metadata_source":"pith","pith_arxiv_id":"1601.01283","snapshot_observed_at":"2026-06-05T21:23:00.469572Z","title":"Conservative dynamics of two-body systems at the fourth post-Newtonian approximation of general relativity","venue":"gr-qc","work_id":"488c6221-7e91-4bc0-ac0c-dfa9ecff942f","year":2016},"citing_paper":{"arxiv_id":"2407.00366","last_updated":"2025-12-17T10:16:02Z","snapshot_observed_at":"2026-07-06T02:11:23.670680Z","submitted_at":"2024-06-29T08:31:38Z","title":"Comparison of 4.5PN and 2SF gravitational energy fluxes from quasicircular compact binaries","version":2},"reference_index":8,"source":"pdf_text","source_observed_at":"2026-05-23T23:17:55.191990Z"},"links":{"cited_paper":"/paper/1601.01283","citing_paper":"/paper/2407.00366"},"observation_digest":"sha256:5600615e39fdeb202f2a008f9a7b3a45b3f855d5a1dc3f9ac456177b3069bb3b","observation_id":"a8c8071b-94b7-4029-a853-0c758a1d604d","resolution":{"observed_at":"2026-05-23T23:18:35.856183Z","resolver_source":"local_arxiv","status":"verified_exact"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-07-13T06:30:06.624239+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-07-13T06:30:06.624239+00:00","source":"crossref"},{"observed_at":"2026-07-13T06:30:01.874667+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":{"arxiv_id":"1706.08480","last_updated":"2018-01-08T14:11:09Z","snapshot_observed_at":"2026-07-06T05:48:30.254634Z","submitted_at":"2017-06-26T17:01:45Z","title":"Dimensional regularization of the IR divergences in the Fokker action of point-particle binaries at the fourth post-Newtonian order","version":4},"cited_work":{"arxiv_id":"1706.08480","doi":null,"metadata_source":"pith","pith_arxiv_id":"1706.08480","snapshot_observed_at":"2026-06-05T21:23:00.469572Z","title":"Dimensional regularization of the IR divergences in the Fokker action of point-particle binaries at the fourth post-Newtonian order","venue":"gr-qc","work_id":"d7759d28-5549-48a4-b163-764623eee780","year":2017},"citing_paper":{"arxiv_id":"2407.00366","last_updated":"2025-12-17T10:16:02Z","snapshot_observed_at":"2026-07-06T02:11:23.670680Z","submitted_at":"2024-06-29T08:31:38Z","title":"Comparison of 4.5PN and 2SF gravitational energy fluxes from quasicircular compact binaries","version":2},"reference_index":9,"source":"pdf_text","source_observed_at":"2026-05-23T23:17:55.191990Z"},"links":{"cited_paper":"/paper/1706.08480","citing_paper":"/paper/2407.00366"},"observation_digest":"sha256:d96f2fa7bcf8793c091ee1a95d6f54a99a0720f89d51c4e626adaf58a722d79b","observation_id":"0049434a-d75c-4257-b850-4195973312d6","resolution":{"observed_at":"2026-05-23T23:18:36.061289Z","resolver_source":"local_arxiv","status":"verified_exact"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-07-13T06:30:06.624239+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-07-13T06:30:06.624239+00:00","source":"crossref"},{"observed_at":"2026-07-13T06:30:01.874667+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":{"arxiv_id":"1707.09289","last_updated":"2018-03-09T15:56:56Z","snapshot_observed_at":"2026-07-06T05:53:10.980136Z","submitted_at":"2017-07-28T15:46:55Z","title":"Ambiguity-Free Completion of the Equations of Motion of Compact Binary Systems at the Fourth Post-Newtonian Order","version":2},"cited_work":{"arxiv_id":"1707.09289","doi":null,"metadata_source":"pith","pith_arxiv_id":"1707.09289","snapshot_observed_at":"2026-06-05T21:23:00.469572Z","title":"Ambiguity-Free Completion of the Equations of Motion of Compact Binary Systems at the Fourth Post-Newtonian Order","venue":"gr-qc","work_id":"ad3ba3fb-1d6f-4619-b188-c4f46b4689d6","year":2017},"citing_paper":{"arxiv_id":"2407.00366","last_updated":"2025-12-17T10:16:02Z","snapshot_observed_at":"2026-07-06T02:11:23.670680Z","submitted_at":"2024-06-29T08:31:38Z","title":"Comparison of 4.5PN and 2SF gravitational energy fluxes from quasicircular compact binaries","version":2},"reference_index":10,"source":"pdf_text","source_observed_at":"2026-05-23T23:17:55.191990Z"},"links":{"cited_paper":"/paper/1707.09289","citing_paper":"/paper/2407.00366"},"observation_digest":"sha256:bb8982a0ef2f01e76da0ae0c36b5fd43b160be2245a3f77b0b5cda14b5cbde64","observation_id":"cf6eb63f-d664-4d6d-bb56-0e76b2d7ee46","resolution":{"observed_at":"2026-05-23T23:18:35.997992Z","resolver_source":"local_arxiv","status":"verified_exact"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-07-13T06:30:06.624239+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-07-13T06:30:06.624239+00:00","source":"crossref"},{"observed_at":"2026-07-13T06:30:01.874667+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":{"arxiv_id":"1903.05113","last_updated":"2019-08-02T19:44:25Z","snapshot_observed_at":"2026-07-06T07:38:46.983735Z","submitted_at":"2019-03-12T18:03:36Z","title":"Conservative dynamics of binary systems to fourth Post-Newtonian order in the EFT approach I: Regularized Lagrangian","version":2},"cited_work":{"arxiv_id":"1903.05113","doi":null,"metadata_source":"arxiv_reference","pith_arxiv_id":"1903.05113","snapshot_observed_at":"2026-07-03T07:27:44.567889Z","title":"Foffa and R","venue":null,"work_id":"f7ecb611-628f-4e96-afc3-c55f9a3586f4","year":2019},"citing_paper":{"arxiv_id":"2407.00366","last_updated":"2025-12-17T10:16:02Z","snapshot_observed_at":"2026-07-06T02:11:23.670680Z","submitted_at":"2024-06-29T08:31:38Z","title":"Comparison of 4.5PN and 2SF gravitational energy fluxes from quasicircular compact binaries","version":2},"reference_index":11,"source":"pdf_text","source_observed_at":"2026-05-23T23:17:55.191990Z"},"links":{"cited_paper":"/paper/1903.05113","citing_paper":"/paper/2407.00366"},"observation_digest":"sha256:9d74eb04081872934a3c1d92f3ffaad35238bf7eee4c4e1f4a1ef1e11f8ab89b","observation_id":"72ac8112-2201-457e-b2fe-284590b296a1","resolution":{"observed_at":"2026-05-23T23:18:35.863011Z","resolver_source":"arxiv_id","status":"verified_exact"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-07-13T06:30:06.624239+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-07-13T06:30:06.624239+00:00","source":"crossref"},{"observed_at":"2026-07-13T06:30:01.874667+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":{"arxiv_id":"1903.05118","last_updated":"2019-07-30T08:14:00Z","snapshot_observed_at":"2026-07-06T07:38:46.983735Z","submitted_at":"2019-03-12T18:05:43Z","title":"Conservative dynamics of binary systems to fourth Post-Newtonian order in the EFT approach II: Renormalized Lagrangian","version":2},"cited_work":{"arxiv_id":"1903.05118","doi":null,"metadata_source":"arxiv_reference","pith_arxiv_id":"1903.05118","snapshot_observed_at":"2026-07-03T07:27:44.661464Z","title":"Foffa, R","venue":null,"work_id":"05b20f8f-4ddb-40c6-8b01-a99c3c98613b","year":2019},"citing_paper":{"arxiv_id":"2407.00366","last_updated":"2025-12-17T10:16:02Z","snapshot_observed_at":"2026-07-06T02:11:23.670680Z","submitted_at":"2024-06-29T08:31:38Z","title":"Comparison of 4.5PN and 2SF gravitational energy fluxes from quasicircular compact binaries","version":2},"reference_index":12,"source":"pdf_text","source_observed_at":"2026-05-23T23:17:55.191990Z"},"links":{"cited_paper":"/paper/1903.05118","citing_paper":"/paper/2407.00366"},"observation_digest":"sha256:9b36e5475d0a0d4fe7592b9f9afacf0f56159ed86f7b7fd3247b6037cca6aa2f","observation_id":"e634bb5a-da75-4d24-b88b-9ced3f36d312","resolution":{"observed_at":"2026-05-23T23:18:35.931471Z","resolver_source":"arxiv_id","status":"verified_exact"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-07-13T06:30:06.624239+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-07-13T06:30:06.624239+00:00","source":"crossref"},{"observed_at":"2026-07-13T06:30:01.874667+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":{"arxiv_id":"2003.13672","last_updated":"2020-09-21T14:53:17Z","snapshot_observed_at":"2026-07-06T09:08:28.873280Z","submitted_at":"2020-03-30T17:55:13Z","title":"The mass quadrupole moment of compact binary systems at the fourth post-Newtonian order","version":2},"cited_work":{"arxiv_id":"2003.13672","doi":null,"metadata_source":"arxiv_reference","pith_arxiv_id":"2003.13672","snapshot_observed_at":"2026-06-05T21:23:00.469572Z","title":"Marchand, Q","venue":null,"work_id":"42cfc8b3-21ec-4c9b-a9c1-bd8556854671","year":2020},"citing_paper":{"arxiv_id":"2407.00366","last_updated":"2025-12-17T10:16:02Z","snapshot_observed_at":"2026-07-06T02:11:23.670680Z","submitted_at":"2024-06-29T08:31:38Z","title":"Comparison of 4.5PN and 2SF gravitational energy fluxes from quasicircular compact binaries","version":2},"reference_index":13,"source":"pdf_text","source_observed_at":"2026-05-23T23:17:55.191990Z"},"links":{"cited_paper":"/paper/2003.13672","citing_paper":"/paper/2407.00366"},"observation_digest":"sha256:2005d39b993cc9db7aa9b4a9e37eabd5f1f9f334d292085fbdc267595796e363","observation_id":"622e4b14-24d0-4ea8-bdf6-04abb5c81e8d","resolution":{"observed_at":"2026-05-23T23:18:35.949281Z","resolver_source":"arxiv_id","status":"verified_exact"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-07-13T06:30:06.624239+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-07-13T06:30:06.624239+00:00","source":"crossref"},{"observed_at":"2026-07-13T06:30:01.874667+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":{"arxiv_id":"1607.07601","last_updated":"2016-11-28T09:41:12Z","snapshot_observed_at":"2026-07-06T05:04:54.061681Z","submitted_at":"2016-07-26T09:19:09Z","title":"Gravitational-wave tail effects to quartic non-linear order","version":2},"cited_work":{"arxiv_id":"1607.07601","doi":null,"metadata_source":"pith","pith_arxiv_id":"1607.07601","snapshot_observed_at":"2026-07-03T15:28:34.641397Z","title":"Gravitational-wave tail effects to quartic non-linear order","venue":"gr-qc","work_id":"8d1f27a1-ebdc-40e6-a81e-d6354f407d4c","year":2016},"citing_paper":{"arxiv_id":"2407.00366","last_updated":"2025-12-17T10:16:02Z","snapshot_observed_at":"2026-07-06T02:11:23.670680Z","submitted_at":"2024-06-29T08:31:38Z","title":"Comparison of 4.5PN and 2SF gravitational energy fluxes from quasicircular compact binaries","version":2},"reference_index":14,"source":"pdf_text","source_observed_at":"2026-05-23T23:17:55.191990Z"},"links":{"cited_paper":"/paper/1607.07601","citing_paper":"/paper/2407.00366"},"observation_digest":"sha256:83a97db2ecdbdd07258eae16a19f43c9623bb330ef4032900399eed19f387779","observation_id":"6a706059-ca5d-4b31-b196-4272e95e982c","resolution":{"observed_at":"2026-05-23T23:18:36.084131Z","resolver_source":"local_arxiv","status":"verified_exact"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-07-13T06:30:06.624239+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-07-13T06:30:06.624239+00:00","source":"crossref"},{"observed_at":"2026-07-13T06:30:01.874667+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":{"arxiv_id":"2110.02240","last_updated":"2022-06-20T12:42:41Z","snapshot_observed_at":"2026-07-06T11:54:41.350035Z","submitted_at":"2021-10-05T18:00:13Z","title":"The Quadrupole Moment of Compact Binaries to the Fourth post-Newtonian Order: I. Non-Locality in Time and Infra-Red Divergencies","version":3},"cited_work":{"arxiv_id":"2110.02240","doi":null,"metadata_source":"arxiv_reference","pith_arxiv_id":"2110.02240","snapshot_observed_at":"2026-06-05T21:23:00.469572Z","title":"Larrouturou, Q","venue":null,"work_id":"c5792e23-9d98-4ff0-998d-e48ac9981f33","year":2022},"citing_paper":{"arxiv_id":"2407.00366","last_updated":"2025-12-17T10:16:02Z","snapshot_observed_at":"2026-07-06T02:11:23.670680Z","submitted_at":"2024-06-29T08:31:38Z","title":"Comparison of 4.5PN and 2SF gravitational energy fluxes from quasicircular compact binaries","version":2},"reference_index":15,"source":"pdf_text","source_observed_at":"2026-05-23T23:17:55.191990Z"},"links":{"cited_paper":"/paper/2110.02240","citing_paper":"/paper/2407.00366"},"observation_digest":"sha256:5891a2f2fc6cb57b9af4dcd0b4368d42419e7361df698f170c48567ef34b0fb5","observation_id":"d3466397-bc3c-4385-8865-5d9e01573e8d","resolution":{"observed_at":"2026-05-23T23:18:36.049392Z","resolver_source":"arxiv_id","status":"verified_exact"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-07-13T06:30:06.624239+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-07-13T06:30:06.624239+00:00","source":"crossref"},{"observed_at":"2026-07-13T06:30:01.874667+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":{"arxiv_id":"2110.02243","last_updated":"2022-06-20T12:45:17Z","snapshot_observed_at":"2026-07-06T11:54:41.350035Z","submitted_at":"2021-10-05T18:00:37Z","title":"The Quadrupole Moment of Compact Binaries to the Fourth post-Newtonian Order: II. Dimensional Regularization and Renormalization","version":3},"cited_work":{"arxiv_id":"2110.02243","doi":null,"metadata_source":"arxiv_reference","pith_arxiv_id":"2110.02243","snapshot_observed_at":"2026-06-05T21:23:00.469572Z","title":"Larrouturou, L","venue":null,"work_id":"6428eaa6-9596-41bb-89a7-913793b6de45","year":2022},"citing_paper":{"arxiv_id":"2407.00366","last_updated":"2025-12-17T10:16:02Z","snapshot_observed_at":"2026-07-06T02:11:23.670680Z","submitted_at":"2024-06-29T08:31:38Z","title":"Comparison of 4.5PN and 2SF gravitational energy fluxes from quasicircular compact binaries","version":2},"reference_index":16,"source":"pdf_text","source_observed_at":"2026-05-23T23:17:55.191990Z"},"links":{"cited_paper":"/paper/2110.02243","citing_paper":"/paper/2407.00366"},"observation_digest":"sha256:748864bd1d30af6733bcdc89f276b56014fd7309a23149799b7682a7ba623590","observation_id":"b017d3b5-662f-4f70-a046-4452ebb0db58","resolution":{"observed_at":"2026-05-23T23:18:35.992054Z","resolver_source":"arxiv_id","status":"verified_exact"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-07-13T06:30:06.624239+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-07-13T06:30:06.624239+00:00","source":"crossref"},{"observed_at":"2026-07-13T06:30:01.874667+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":"Trestini and L","venue":null,"work_id":"0727d461-4294-4595-99ec-6d010edd7784","year":2023},"citing_paper":{"arxiv_id":"2407.00366","last_updated":"2025-12-17T10:16:02Z","snapshot_observed_at":"2026-07-06T02:11:23.670680Z","submitted_at":"2024-06-29T08:31:38Z","title":"Comparison of 4.5PN and 2SF gravitational energy fluxes from quasicircular compact binaries","version":2},"reference_index":17,"source":"pdf_text","source_observed_at":"2026-05-23T23:17:55.191990Z"},"links":{"citing_paper":"/paper/2407.00366"},"observation_digest":"sha256:f3107a6509e70f5a13ddbd0cd72e777ab28fd9b42922c423d5e8ea9222c68b35","observation_id":"b680320b-2c6a-46e8-947b-356999036d9b","resolution":{"observed_at":"2026-05-23T23:18:36.279235Z","resolver_source":"raw_fallback","status":"verified_fuzzy"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-07-13T06:30:06.624239+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-07-13T06:30:06.624239+00:00","source":"crossref"},{"observed_at":"2026-07-13T06:30:01.874667+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":{"arxiv_id":"2304.11185","last_updated":"2023-09-30T10:43:34Z","snapshot_observed_at":"2026-07-06T15:18:34.225078Z","submitted_at":"2023-04-21T18:00:06Z","title":"Gravitational-Wave Phasing of Quasi-Circular Compact Binary Systems to the Fourth-and-a-Half post-Newtonian Order","version":4},"cited_work":{"arxiv_id":"2304.11185","doi":null,"metadata_source":"arxiv_reference","pith_arxiv_id":"2304.11185","snapshot_observed_at":"2026-07-03T15:28:34.535836Z","title":"Blanchet, G","venue":null,"work_id":"17d57aec-004e-431e-96db-50bc1654c4c9","year":2023},"citing_paper":{"arxiv_id":"2407.00366","last_updated":"2025-12-17T10:16:02Z","snapshot_observed_at":"2026-07-06T02:11:23.670680Z","submitted_at":"2024-06-29T08:31:38Z","title":"Comparison of 4.5PN and 2SF gravitational energy fluxes from quasicircular compact binaries","version":2},"reference_index":18,"source":"pdf_text","source_observed_at":"2026-05-23T23:17:55.191990Z"},"links":{"cited_paper":"/paper/2304.11185","citing_paper":"/paper/2407.00366"},"observation_digest":"sha256:a488e7ccaf40d789c3bc519561ef16e43ec3490100227be34fa03d0cd09442c8","observation_id":"4e247324-a27c-4533-9461-dbd561e6a59e","resolution":{"observed_at":"2026-05-23T23:18:35.980620Z","resolver_source":"arxiv_id","status":"verified_exact"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-07-13T06:30:06.624239+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-07-13T06:30:06.624239+00:00","source":"crossref"},{"observed_at":"2026-07-13T06:30:01.874667+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":{"arxiv_id":"2304.11186","last_updated":"2023-09-30T10:40:56Z","snapshot_observed_at":"2026-07-06T15:18:34.225078Z","submitted_at":"2023-04-21T18:00:08Z","title":"Gravitational Wave Flux and Quadrupole Modes from Quasi-Circular Non-Spinning Compact Binaries to the Fourth Post-Newtonian Order","version":4},"cited_work":{"arxiv_id":"2304.11186","doi":null,"metadata_source":"arxiv_reference","pith_arxiv_id":"2304.11186","snapshot_observed_at":"2026-07-03T15:28:34.555837Z","title":"Blanchet, G","venue":null,"work_id":"2c5e2c8d-e9b6-47b5-9b1a-65f9e09b6307","year":2023},"citing_paper":{"arxiv_id":"2407.00366","last_updated":"2025-12-17T10:16:02Z","snapshot_observed_at":"2026-07-06T02:11:23.670680Z","submitted_at":"2024-06-29T08:31:38Z","title":"Comparison of 4.5PN and 2SF gravitational energy fluxes from quasicircular compact binaries","version":2},"reference_index":19,"source":"pdf_text","source_observed_at":"2026-05-23T23:17:55.191990Z"},"links":{"cited_paper":"/paper/2304.11186","citing_paper":"/paper/2407.00366"},"observation_digest":"sha256:88e86226af9bc3a41f15ef30e54edc49c3454f80309a349a4b1e9f809119e6a5","observation_id":"988a0070-c00c-4c84-b6ba-3c05fac29cbe","resolution":{"observed_at":"2026-05-23T23:18:36.031379Z","resolver_source":"arxiv_id","status":"verified_exact"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-07-13T06:30:06.624239+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-07-13T06:30:06.624239+00:00","source":"crossref"},{"observed_at":"2026-07-13T06:30:01.874667+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":{"arxiv_id":"2304.13647","last_updated":"2023-05-03T20:22:18Z","snapshot_observed_at":"2026-07-06T15:20:21.679635Z","submitted_at":"2023-04-26T16:10:31Z","title":"Gravitational waves from compact binaries to the fourth post-Newtonian order","version":2},"cited_work":{"arxiv_id":"2304.13647","doi":null,"metadata_source":"arxiv_reference","pith_arxiv_id":"2304.13647","snapshot_observed_at":"2026-06-05T21:23:00.469572Z","title":"Blanchet, G","venue":null,"work_id":"df360f50-251a-4ff3-9271-0f6cbfc279d9","year":2023},"citing_paper":{"arxiv_id":"2407.00366","last_updated":"2025-12-17T10:16:02Z","snapshot_observed_at":"2026-07-06T02:11:23.670680Z","submitted_at":"2024-06-29T08:31:38Z","title":"Comparison of 4.5PN and 2SF gravitational energy fluxes from quasicircular compact binaries","version":2},"reference_index":20,"source":"pdf_text","source_observed_at":"2026-05-23T23:17:55.191990Z"},"links":{"cited_paper":"/paper/2304.13647","citing_paper":"/paper/2407.00366"},"observation_digest":"sha256:bbaa5eba5cdca5e249331ed23e39a6e834d09af1cf998d5afa8fed66adf8c316","observation_id":"3178d5a5-70bf-4ac7-9d56-f1544f4a3c14","resolution":{"observed_at":"2026-05-23T23:18:35.986284Z","resolver_source":"arxiv_id","status":"verified_exact"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-07-13T06:30:06.624239+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-07-13T06:30:06.624239+00:00","source":"crossref"},{"observed_at":"2026-07-13T06:30:01.874667+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":{"arxiv_id":"gr-qc/9405062","last_updated":"1994-05-26T01:47:37Z","snapshot_observed_at":"2026-07-07T03:24:45.763672Z","submitted_at":"1994-05-26T01:47:37Z","title":"Post-Newtonian expansion of gravitational waves from a particle in circular orbit around a Schwarzschild black hole","version":1},"cited_work":{"arxiv_id":"gr-qc/9405062","doi":null,"metadata_source":"pith","pith_arxiv_id":"gr-qc/9405062","snapshot_observed_at":"2026-07-02T19:27:19.052130Z","title":"Post-Newtonian expansion of gravitational waves from a particle in circular orbit around a Schwarzschild black hole","venue":"gr-qc","work_id":"192afaf9-072a-419a-a617-86857c155666","year":1994},"citing_paper":{"arxiv_id":"2407.00366","last_updated":"2025-12-17T10:16:02Z","snapshot_observed_at":"2026-07-06T02:11:23.670680Z","submitted_at":"2024-06-29T08:31:38Z","title":"Comparison of 4.5PN and 2SF gravitational energy fluxes from quasicircular compact binaries","version":2},"reference_index":21,"source":"pdf_text","source_observed_at":"2026-05-23T23:17:55.191990Z"},"links":{"cited_paper":"/paper/gr-qc/9405062","citing_paper":"/paper/2407.00366"},"observation_digest":"sha256:f0fe7c9cb3d5ba3c1dacd6c9667fc45a701f40702fefb2d0d654e973f717304f","observation_id":"d75a3436-daf5-48b9-b424-8759f11dd1c0","resolution":{"observed_at":"2026-05-23T23:18:35.875940Z","resolver_source":"local_arxiv","status":"verified_exact"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-07-13T06:30:06.624239+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-07-13T06:30:06.624239+00:00","source":"crossref"},{"observed_at":"2026-07-13T06:30:01.874667+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":{"arxiv_id":"gr-qc/9701050","last_updated":"1997-01-23T11:43:37Z","snapshot_observed_at":"2026-07-07T03:27:12.065931Z","submitted_at":"1997-01-23T11:43:37Z","title":"Gravitational Waves by a Particle in Circular Orbits around a Schwarzschild black hole -5.5 Post-Newtonian Formula-","version":1},"cited_work":{"arxiv_id":"gr-qc/9701050","doi":null,"metadata_source":"pith","pith_arxiv_id":"gr-qc/9701050","snapshot_observed_at":"2026-07-03T02:57:35.576439Z","title":"Gravitational Waves by a Particle in Circular Orbits around a Schwarzschild black hole -5.5 Post-Newtonian Formula-","venue":"gr-qc","work_id":"49dc14d8-7113-44dc-afd8-4f0de9b61924","year":1997},"citing_paper":{"arxiv_id":"2407.00366","last_updated":"2025-12-17T10:16:02Z","snapshot_observed_at":"2026-07-06T02:11:23.670680Z","submitted_at":"2024-06-29T08:31:38Z","title":"Comparison of 4.5PN and 2SF gravitational energy fluxes from quasicircular compact binaries","version":2},"reference_index":22,"source":"pdf_text","source_observed_at":"2026-05-23T23:17:55.191990Z"},"links":{"cited_paper":"/paper/gr-qc/9701050","citing_paper":"/paper/2407.00366"},"observation_digest":"sha256:c08cde424ac359808596ff01f9a4bba33f001108cd876b242e14afc5b64aa028","observation_id":"4d44db38-a5db-4c0d-8706-424a5a599b81","resolution":{"observed_at":"2026-05-23T23:18:35.869941Z","resolver_source":"local_arxiv","status":"verified_exact"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-07-13T06:30:06.624239+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-07-13T06:30:06.624239+00:00","source":"crossref"},{"observed_at":"2026-07-13T06:30:01.874667+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":"raw_reference","pith_arxiv_id":null,"snapshot_observed_at":"2026-06-05T21:23:00.469572Z","title":"Blanchet and T","venue":null,"work_id":"8cb0a2f7-f415-440a-8441-a5da05e2f715","year":1986},"citing_paper":{"arxiv_id":"2407.00366","last_updated":"2025-12-17T10:16:02Z","snapshot_observed_at":"2026-07-06T02:11:23.670680Z","submitted_at":"2024-06-29T08:31:38Z","title":"Comparison of 4.5PN and 2SF gravitational energy fluxes from quasicircular compact binaries","version":2},"reference_index":23,"source":"pdf_text","source_observed_at":"2026-05-23T23:17:55.191990Z"},"links":{"citing_paper":"/paper/2407.00366"},"observation_digest":"sha256:0c371e36235d2b1ae65fb63d22003b70b7a51acd9d1298e753a665729eb538a9","observation_id":"5e35c573-9880-42eb-b907-d09b0cbc0f73","resolution":{"observed_at":"2026-05-23T23:18:36.297702Z","resolver_source":"raw_fallback","status":"verified_fuzzy"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-07-13T06:30:06.624239+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-07-13T06:30:06.624239+00:00","source":"crossref"},{"observed_at":"2026-07-13T06:30:01.874667+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":"raw_reference","pith_arxiv_id":null,"snapshot_observed_at":"2026-06-05T21:23:00.469572Z","title":"Blanchet, Radiative gravitational fields in general rel- ativity","venue":null,"work_id":"402cfe31-a168-4a53-bd42-e1d70a30a7a5","year":1987},"citing_paper":{"arxiv_id":"2407.00366","last_updated":"2025-12-17T10:16:02Z","snapshot_observed_at":"2026-07-06T02:11:23.670680Z","submitted_at":"2024-06-29T08:31:38Z","title":"Comparison of 4.5PN and 2SF gravitational energy fluxes from quasicircular compact binaries","version":2},"reference_index":24,"source":"pdf_text","source_observed_at":"2026-05-23T23:17:55.191990Z"},"links":{"citing_paper":"/paper/2407.00366"},"observation_digest":"sha256:e630bc1c5430b18bd48a5f14d242992beea7f1d0c4897ab570495c758705c99d","observation_id":"4d1fea7c-5b18-451c-b671-2a5151892f3a","resolution":{"observed_at":"2026-05-23T23:18:36.292127Z","resolver_source":"raw_fallback","status":"verified_fuzzy"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-07-13T06:30:06.624239+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-07-13T06:30:06.624239+00:00","source":"crossref"},{"observed_at":"2026-07-13T06:30:01.874667+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":"raw_reference","pith_arxiv_id":null,"snapshot_observed_at":"2026-06-05T21:23:00.469572Z","title":"Blanchet and T","venue":null,"work_id":"500f4004-51be-4e9a-af06-f940a25b791a","year":1988},"citing_paper":{"arxiv_id":"2407.00366","last_updated":"2025-12-17T10:16:02Z","snapshot_observed_at":"2026-07-06T02:11:23.670680Z","submitted_at":"2024-06-29T08:31:38Z","title":"Comparison of 4.5PN and 2SF gravitational energy fluxes from quasicircular compact binaries","version":2},"reference_index":25,"source":"pdf_text","source_observed_at":"2026-05-23T23:17:55.191990Z"},"links":{"citing_paper":"/paper/2407.00366"},"observation_digest":"sha256:a1f1616976eab483c8c535f7e3e43943742612a1b4cf2fe398403a263dfd6c03","observation_id":"779b2023-fe95-4900-afd9-95aa665db1bc","resolution":{"observed_at":"2026-05-23T23:18:36.274778Z","resolver_source":"raw_fallback","status":"verified_fuzzy"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-07-13T06:30:06.624239+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-07-13T06:30:06.624239+00:00","source":"crossref"},{"observed_at":"2026-07-13T06:30:01.874667+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":"raw_reference","pith_arxiv_id":null,"snapshot_observed_at":"2026-06-05T21:23:00.469572Z","title":"Blanchet and T","venue":null,"work_id":"18b33487-9c7a-468a-a5c4-cad691f34df2","year":1992},"citing_paper":{"arxiv_id":"2407.00366","last_updated":"2025-12-17T10:16:02Z","snapshot_observed_at":"2026-07-06T02:11:23.670680Z","submitted_at":"2024-06-29T08:31:38Z","title":"Comparison of 4.5PN and 2SF gravitational energy fluxes from quasicircular compact binaries","version":2},"reference_index":26,"source":"pdf_text","source_observed_at":"2026-05-23T23:17:55.191990Z"},"links":{"citing_paper":"/paper/2407.00366"},"observation_digest":"sha256:589dc9e3c59a350ade5bb30d78faf032e05c85d1f65febe61f68e181aeac9225","observation_id":"7307fd74-44ec-475d-bf39-da7a401b64ea","resolution":{"observed_at":"2026-05-23T23:18:36.310846Z","resolver_source":"raw_fallback","status":"verified_fuzzy"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-07-13T06:30:06.624239+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-07-13T06:30:06.624239+00:00","source":"crossref"},{"observed_at":"2026-07-13T06:30:01.874667+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":"qc/9801101","doi":null,"metadata_source":"arxiv_reference","pith_arxiv_id":null,"snapshot_observed_at":"2026-06-05T21:23:00.469572Z","title":"Blanchet, On the multipole expansion of the gravi- tational field, Class","venue":null,"work_id":"c876321a-5a4a-49a3-a3d7-2e81f0496263","year":1971},"citing_paper":{"arxiv_id":"2407.00366","last_updated":"2025-12-17T10:16:02Z","snapshot_observed_at":"2026-07-06T02:11:23.670680Z","submitted_at":"2024-06-29T08:31:38Z","title":"Comparison of 4.5PN and 2SF gravitational energy fluxes from quasicircular compact binaries","version":2},"reference_index":27,"source":"pdf_text","source_observed_at":"2026-05-23T23:17:55.191990Z"},"links":{"citing_paper":"/paper/2407.00366"},"observation_digest":"sha256:ba5481dafe0c434f411d048333e8b4e415fc2bc1386d19981650f6cb8908fca0","observation_id":"1531113e-6125-49d1-a2d7-08e37cad588f","resolution":{"observed_at":"2026-05-23T23:18:35.955089Z","resolver_source":"arxiv_id","status":"verified_exact"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-07-13T06:30:06.624239+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-07-13T06:30:06.624239+00:00","source":"crossref"},{"observed_at":"2026-07-13T06:30:01.874667+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":"raw_reference","pith_arxiv_id":null,"snapshot_observed_at":"2026-06-05T21:23:00.469572Z","title":"Blanchet, G","venue":null,"work_id":"fa779351-a885-432c-887b-46fd266a99de","year":2022},"citing_paper":{"arxiv_id":"2407.00366","last_updated":"2025-12-17T10:16:02Z","snapshot_observed_at":"2026-07-06T02:11:23.670680Z","submitted_at":"2024-06-29T08:31:38Z","title":"Comparison of 4.5PN and 2SF gravitational energy fluxes from quasicircular compact binaries","version":2},"reference_index":28,"source":"pdf_text","source_observed_at":"2026-05-23T23:17:55.191990Z"},"links":{"citing_paper":"/paper/2407.00366"},"observation_digest":"sha256:2d1f5ada3815cdc4d332c9b964f87c578f286e88ce23cd7b5d4e4d427a15c9ac","observation_id":"048733f2-543f-49c9-8835-7895090c284c","resolution":{"observed_at":"2026-05-23T23:18:36.287617Z","resolver_source":"raw_fallback","status":"verified_fuzzy"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-07-13T06:30:06.624239+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-07-13T06:30:06.624239+00:00","source":"crossref"},{"observed_at":"2026-07-13T06:30:01.874667+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":{"arxiv_id":"0802.1249","last_updated":"2012-10-19T17:44:28Z","snapshot_observed_at":"2026-07-06T01:34:46.001237Z","submitted_at":"2008-02-09T07:12:40Z","title":"The third post-Newtonian gravitational wave polarisations and associated spherical harmonic modes for inspiralling compact binaries in quasi-circular orbits","version":3},"cited_work":{"arxiv_id":"0802.1249","doi":null,"metadata_source":"pith","pith_arxiv_id":"0802.1249","snapshot_observed_at":"2026-06-28T05:11:39.909681Z","title":"The third post-Newtonian gravitational wave polarisations and associated spherical harmonic modes for inspiralling compact binaries in quasi-circular orbits","venue":"gr-qc","work_id":"8743cd35-613a-4648-b205-6de85bd567bf","year":2008},"citing_paper":{"arxiv_id":"2407.00366","last_updated":"2025-12-17T10:16:02Z","snapshot_observed_at":"2026-07-06T02:11:23.670680Z","submitted_at":"2024-06-29T08:31:38Z","title":"Comparison of 4.5PN and 2SF gravitational energy fluxes from quasicircular compact binaries","version":2},"reference_index":29,"source":"pdf_text","source_observed_at":"2026-05-23T23:17:55.191990Z"},"links":{"cited_paper":"/paper/0802.1249","citing_paper":"/paper/2407.00366"},"observation_digest":"sha256:ed08d6eaced9bfa1a0461712e43bb2f7742f32bb9f501a0a2c07aae3a8d2a93f","observation_id":"b63ff224-e770-4dc3-95b0-878301d55115","resolution":{"observed_at":"2026-05-23T23:18:36.037595Z","resolver_source":"local_arxiv","status":"verified_exact"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-07-13T06:30:06.624239+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-07-13T06:30:06.624239+00:00","source":"crossref"},{"observed_at":"2026-07-13T06:30:01.874667+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":"2407.00366","last_updated":"2025-12-17T10:16:02Z","snapshot_observed_at":"2026-07-06T02:11:23.670680Z","submitted_at":"2024-06-29T08:31:38Z","title":"Comparison of 4.5PN and 2SF gravitational energy fluxes from quasicircular compact binaries","version":2},"reference_index":30,"source":"pdf_text","source_observed_at":"2026-05-23T23:17:55.191990Z"},"links":{"cited_paper":"/paper/gr-qc/9412027","citing_paper":"/paper/2407.00366"},"observation_digest":"sha256:f7d5a0c2d5f304e4047b4905c72976a1d417502b053d9ac3210b83e6686cbb69","observation_id":"0bb87a5f-62ab-4164-b3a7-7a89d6e350f1","resolution":{"observed_at":"2026-05-23T23:18:36.024127Z","resolver_source":"local_arxiv","status":"verified_exact"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-07-13T06:30:06.624239+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-07-13T06:30:06.624239+00:00","source":"crossref"},{"observed_at":"2026-07-13T06:30:01.874667+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":{"arxiv_id":"1409.3546","last_updated":"2015-02-04T20:41:39Z","snapshot_observed_at":"2026-07-06T03:54:16.458401Z","submitted_at":"2014-09-11T19:13:25Z","title":"Non-linear multipole interactions and gravitational-wave octupole modes for inspiralling compact binaries to third-and-a-half post-Newtonian order","version":2},"cited_work":{"arxiv_id":"1409.3546","doi":null,"metadata_source":"pith","pith_arxiv_id":"1409.3546","snapshot_observed_at":"2026-06-05T21:23:00.469572Z","title":"Non-linear multipole interactions and gravitational-wave octupole modes for inspiralling compact binaries to third-and-a-half post-Newtonian order","venue":"gr-qc","work_id":"f12eb12f-b5e0-4363-abd0-db4bf6750ad4","year":2014},"citing_paper":{"arxiv_id":"2407.00366","last_updated":"2025-12-17T10:16:02Z","snapshot_observed_at":"2026-07-06T02:11:23.670680Z","submitted_at":"2024-06-29T08:31:38Z","title":"Comparison of 4.5PN and 2SF gravitational energy fluxes from quasicircular compact binaries","version":2},"reference_index":31,"source":"pdf_text","source_observed_at":"2026-05-23T23:17:55.191990Z"},"links":{"cited_paper":"/paper/1409.3546","citing_paper":"/paper/2407.00366"},"observation_digest":"sha256:ec99b338cfacd39869838f4218fbc7f47c89305bec7c4ab8f5be61b9436c60dc","observation_id":"da536e87-ad7a-42cc-b205-85063d999ac4","resolution":{"observed_at":"2026-05-23T23:18:35.917955Z","resolver_source":"local_arxiv","status":"verified_exact"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-07-13T06:30:06.624239+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-07-13T06:30:06.624239+00:00","source":"crossref"},{"observed_at":"2026-07-13T06:30:01.874667+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":{"arxiv_id":"2105.10876","last_updated":"2021-06-14T15:26:38Z","snapshot_observed_at":"2026-07-06T11:11:58.263934Z","submitted_at":"2021-05-23T07:58:58Z","title":"The current-type quadrupole moment and gravitational-wave mode $(\\ell,m)=(2,1)$ of compact binary systems at the third post-Newtonian order","version":2},"cited_work":{"arxiv_id":"2105.10876","doi":null,"metadata_source":"arxiv_reference","pith_arxiv_id":"2105.10876","snapshot_observed_at":"2026-06-05T21:23:00.469572Z","title":"Henry, G","venue":null,"work_id":"cc44ed33-0acf-467a-bd37-dd88c9cff16c","year":2021},"citing_paper":{"arxiv_id":"2407.00366","last_updated":"2025-12-17T10:16:02Z","snapshot_observed_at":"2026-07-06T02:11:23.670680Z","submitted_at":"2024-06-29T08:31:38Z","title":"Comparison of 4.5PN and 2SF gravitational energy fluxes from quasicircular compact binaries","version":2},"reference_index":32,"source":"pdf_text","source_observed_at":"2026-05-23T23:17:55.191990Z"},"links":{"cited_paper":"/paper/2105.10876","citing_paper":"/paper/2407.00366"},"observation_digest":"sha256:afd0d485e1ebf829625232417436e55b9c8cd7543f5ab9fcafa8e0795a7338cd","observation_id":"530e3255-bff5-458d-b51e-52bdf1a33172","resolution":{"observed_at":"2026-05-23T23:18:36.004971Z","resolver_source":"arxiv_id","status":"verified_exact"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-07-13T06:30:06.624239+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-07-13T06:30:06.624239+00:00","source":"crossref"},{"observed_at":"2026-07-13T06:30:01.874667+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":"Wiseman, Coalescing binary-systems of compact ob- jects to (post)5/2-Newtonian order","venue":null,"work_id":"6df1b143-0483-4ed5-9bf0-bc760a18c0f3","year":1993},"citing_paper":{"arxiv_id":"2407.00366","last_updated":"2025-12-17T10:16:02Z","snapshot_observed_at":"2026-07-06T02:11:23.670680Z","submitted_at":"2024-06-29T08:31:38Z","title":"Comparison of 4.5PN and 2SF gravitational energy fluxes from quasicircular compact binaries","version":2},"reference_index":33,"source":"pdf_text","source_observed_at":"2026-05-23T23:17:55.191990Z"},"links":{"citing_paper":"/paper/2407.00366"},"observation_digest":"sha256:2c7b3323dbea136ed304aa7c2c151ee33818e8544585414fa6a4e672d64e65d8","observation_id":"54ee5514-fa9b-40b1-8fbb-181082cba873","resolution":{"observed_at":"2026-05-23T23:18:36.324785Z","resolver_source":"raw_fallback","status":"verified_fuzzy"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-07-13T06:30:06.624239+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-07-13T06:30:06.624239+00:00","source":"crossref"},{"observed_at":"2026-07-13T06:30:01.874667+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":"raw_reference","pith_arxiv_id":null,"snapshot_observed_at":"2026-06-05T21:23:00.469572Z","title":"Blanchet and G","venue":null,"work_id":"c7dd93d7-c69e-47f8-8f17-944e8c8802a8","year":1993},"citing_paper":{"arxiv_id":"2407.00366","last_updated":"2025-12-17T10:16:02Z","snapshot_observed_at":"2026-07-06T02:11:23.670680Z","submitted_at":"2024-06-29T08:31:38Z","title":"Comparison of 4.5PN and 2SF gravitational energy fluxes from quasicircular compact binaries","version":2},"reference_index":34,"source":"pdf_text","source_observed_at":"2026-05-23T23:17:55.191990Z"},"links":{"citing_paper":"/paper/2407.00366"},"observation_digest":"sha256:3952985c06c198a17fb906c8e1f70d10c017eab51d1135ec3f346bfbe82e7ef7","observation_id":"824ebd88-e4fc-4f23-a31c-5d18f28bff4d","resolution":{"observed_at":"2026-05-23T23:18:36.330413Z","resolver_source":"raw_fallback","status":"verified_fuzzy"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-07-13T06:30:06.624239+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-07-13T06:30:06.624239+00:00","source":"crossref"},{"observed_at":"2026-07-13T06:30:01.874667+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":{"arxiv_id":"gr-qc/9602024","last_updated":"1996-02-13T10:22:44Z","snapshot_observed_at":"2026-07-07T03:26:06.538559Z","submitted_at":"1996-02-13T10:22:44Z","title":"Gravitational waveforms from inspiralling compact binaries to second-post-Newtonian order","version":1},"cited_work":{"arxiv_id":"gr-qc/9602024","doi":null,"metadata_source":"pith","pith_arxiv_id":"gr-qc/9602024","snapshot_observed_at":"2026-06-26T23:10:14.234236Z","title":"Gravitational waveforms from inspiralling compact binaries to second-post-Newtonian order","venue":"gr-qc","work_id":"fc74a4d8-fe4b-4392-932b-d153bce50c4a","year":1996},"citing_paper":{"arxiv_id":"2407.00366","last_updated":"2025-12-17T10:16:02Z","snapshot_observed_at":"2026-07-06T02:11:23.670680Z","submitted_at":"2024-06-29T08:31:38Z","title":"Comparison of 4.5PN and 2SF gravitational energy fluxes from quasicircular compact binaries","version":2},"reference_index":35,"source":"pdf_text","source_observed_at":"2026-05-23T23:17:55.191990Z"},"links":{"cited_paper":"/paper/gr-qc/9602024","citing_paper":"/paper/2407.00366"},"observation_digest":"sha256:be26551d1c0936aa3cd2a2d2fd765387adde7e6173ea528cdc5927e3913600b7","observation_id":"a74c4456-ce16-43f3-ae01-0bafafe8b324","resolution":{"observed_at":"2026-05-23T23:18:36.055201Z","resolver_source":"local_arxiv","status":"verified_exact"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-07-13T06:30:06.624239+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-07-13T06:30:06.624239+00:00","source":"crossref"},{"observed_at":"2026-07-13T06:30:01.874667+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":{"arxiv_id":"2210.15602","last_updated":"2022-11-29T10:10:22Z","snapshot_observed_at":"2026-07-06T14:11:19.558533Z","submitted_at":"2022-10-27T16:40:55Z","title":"Complete gravitational-waveform amplitude modes for quasi-circular compact binaries to the 3.5PN order","version":2},"cited_work":{"arxiv_id":"2210.15602","doi":null,"metadata_source":"arxiv_reference","pith_arxiv_id":"2210.15602","snapshot_observed_at":"2026-07-02T09:26:51.186244Z","title":"Henry, Complete gravitational-waveform amplitude modes for quasicircular compact binaries to the 3.5PN or- der, Phys","venue":null,"work_id":"7e3ea998-f004-4ab5-9fc2-13f427579a76","year":2023},"citing_paper":{"arxiv_id":"2407.00366","last_updated":"2025-12-17T10:16:02Z","snapshot_observed_at":"2026-07-06T02:11:23.670680Z","submitted_at":"2024-06-29T08:31:38Z","title":"Comparison of 4.5PN and 2SF gravitational energy fluxes from quasicircular compact binaries","version":2},"reference_index":36,"source":"pdf_text","source_observed_at":"2026-05-23T23:17:55.191990Z"},"links":{"cited_paper":"/paper/2210.15602","citing_paper":"/paper/2407.00366"},"observation_digest":"sha256:271706b2230ab7c9326d3c9c20c76345102640e005af3fcac0681967e2dcdf6b","observation_id":"ed9b06db-e196-4d25-a529-85a6558890de","resolution":{"observed_at":"2026-05-23T23:18:36.012403Z","resolver_source":"arxiv_id","status":"verified_exact"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-07-13T06:30:06.624239+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-07-13T06:30:06.624239+00:00","source":"crossref"},{"observed_at":"2026-07-13T06:30:01.874667+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":{"arxiv_id":"2006.11263","last_updated":"2021-02-24T23:58:55Z","snapshot_observed_at":"2026-07-06T09:30:50.462029Z","submitted_at":"2020-06-19T17:51:08Z","title":"Two-timescale evolution of extreme-mass-ratio inspirals: waveform generation scheme for quasicircular orbits in Schwarzschild spacetime","version":3},"cited_work":{"arxiv_id":"2006.11263","doi":null,"metadata_source":"arxiv_reference","pith_arxiv_id":"2006.11263","snapshot_observed_at":"2026-07-04T18:50:05.351720Z","title":"Miller and A","venue":null,"work_id":"32c5b3ee-1234-4ea9-83ad-10d0aa3d661c","year":2021},"citing_paper":{"arxiv_id":"2407.00366","last_updated":"2025-12-17T10:16:02Z","snapshot_observed_at":"2026-07-06T02:11:23.670680Z","submitted_at":"2024-06-29T08:31:38Z","title":"Comparison of 4.5PN and 2SF gravitational energy fluxes from quasicircular compact binaries","version":2},"reference_index":37,"source":"pdf_text","source_observed_at":"2026-05-23T23:17:55.191990Z"},"links":{"cited_paper":"/paper/2006.11263","citing_paper":"/paper/2407.00366"},"observation_digest":"sha256:165ab44f9467bfd1a901f28852a869a7e16f27cdde48350b0b4dbc5c1eaddf05","observation_id":"cbd6dc14-1a4b-43a3-a3e3-4dc6c9068c0e","resolution":{"observed_at":"2026-05-23T23:18:35.842771Z","resolver_source":"arxiv_id","status":"verified_exact"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-07-13T06:30:06.624239+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-07-13T06:30:06.624239+00:00","source":"crossref"},{"observed_at":"2026-07-13T06:30:01.874667+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":{"arxiv_id":"2401.00455","last_updated":"2024-10-26T18:56:05Z","snapshot_observed_at":"2026-07-06T17:10:21.098136Z","submitted_at":"2023-12-31T11:15:41Z","title":"Worldtube puncture scheme for first- and second-order self-force calculations in the Fourier domain","version":2},"cited_work":{"arxiv_id":"2401.00455","doi":null,"metadata_source":"arxiv_reference","pith_arxiv_id":"2401.00455","snapshot_observed_at":"2026-07-04T18:50:05.424948Z","title":"Miller, B","venue":null,"work_id":"9aa0d0d3-36f4-4d3f-a742-d6b0b8a36bbe","year":2024},"citing_paper":{"arxiv_id":"2407.00366","last_updated":"2025-12-17T10:16:02Z","snapshot_observed_at":"2026-07-06T02:11:23.670680Z","submitted_at":"2024-06-29T08:31:38Z","title":"Comparison of 4.5PN and 2SF gravitational energy fluxes from quasicircular compact binaries","version":2},"reference_index":38,"source":"pdf_text","source_observed_at":"2026-05-23T23:17:55.191990Z"},"links":{"cited_paper":"/paper/2401.00455","citing_paper":"/paper/2407.00366"},"observation_digest":"sha256:e191aeae70c0e4b763cdb74b1c3f95f647868a12f9845d04c79ebf1a7721ab8f","observation_id":"0b8edc22-332f-4344-935f-7445b157e900","resolution":{"observed_at":"2026-05-23T23:18:35.961443Z","resolver_source":"arxiv_id","status":"verified_exact"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-07-13T06:30:06.624239+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-07-13T06:30:06.624239+00:00","source":"crossref"},{"observed_at":"2026-07-13T06:30:01.874667+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":{"arxiv_id":"0805.3337","last_updated":"2008-06-17T21:34:36Z","snapshot_observed_at":"2026-07-06T01:39:39.170355Z","submitted_at":"2008-05-21T19:48:20Z","title":"Two timescale analysis of extreme mass ratio inspirals in Kerr. I. Orbital Motion","version":2},"cited_work":{"arxiv_id":"0805.3337","doi":null,"metadata_source":"pith","pith_arxiv_id":"0805.3337","snapshot_observed_at":"2026-07-04T18:50:05.295908Z","title":"Two timescale analysis of extreme mass ratio inspirals in Kerr. I. Orbital Motion","venue":"gr-qc","work_id":"a98ec226-74d7-45d5-9438-ec8d9b733d76","year":2008},"citing_paper":{"arxiv_id":"2407.00366","last_updated":"2025-12-17T10:16:02Z","snapshot_observed_at":"2026-07-06T02:11:23.670680Z","submitted_at":"2024-06-29T08:31:38Z","title":"Comparison of 4.5PN and 2SF gravitational energy fluxes from quasicircular compact binaries","version":2},"reference_index":39,"source":"pdf_text","source_observed_at":"2026-05-23T23:17:55.191990Z"},"links":{"cited_paper":"/paper/0805.3337","citing_paper":"/paper/2407.00366"},"observation_digest":"sha256:5d91dc865ac2dcff8ad559770a96bed8d666c9304f43200698c21206b75ab0fe","observation_id":"e93bfaac-e688-46a5-b6d1-bcbd7ceb0a9a","resolution":{"observed_at":"2026-05-23T23:18:35.911352Z","resolver_source":"local_arxiv","status":"verified_exact"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-07-13T06:30:06.624239+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-07-13T06:30:06.624239+00:00","source":"crossref"},{"observed_at":"2026-07-13T06:30:01.874667+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":{"arxiv_id":"2101.04592","last_updated":"2024-01-25T01:29:56Z","snapshot_observed_at":"2026-07-06T10:31:53.668699Z","submitted_at":"2021-01-12T16:44:53Z","title":"Black hole perturbation theory and gravitational self-force","version":4},"cited_work":{"arxiv_id":"2101.04592","doi":null,"metadata_source":"arxiv_reference","pith_arxiv_id":"2101.04592","snapshot_observed_at":"2026-07-04T18:50:05.339910Z","title":"Pound and B","venue":null,"work_id":"2fe7b0b1-3984-4582-9913-1772a358f756","year":2022},"citing_paper":{"arxiv_id":"2407.00366","last_updated":"2025-12-17T10:16:02Z","snapshot_observed_at":"2026-07-06T02:11:23.670680Z","submitted_at":"2024-06-29T08:31:38Z","title":"Comparison of 4.5PN and 2SF gravitational energy fluxes from quasicircular compact binaries","version":2},"reference_index":40,"source":"pdf_text","source_observed_at":"2026-05-23T23:17:55.191990Z"},"links":{"cited_paper":"/paper/2101.04592","citing_paper":"/paper/2407.00366"},"observation_digest":"sha256:c9c791efd5b31512843b232c9e17acd257eb0ec0d00021c160184efa93670b79","observation_id":"acb99bf1-f636-4059-b357-fd97f16cdbe0","resolution":{"observed_at":"2026-05-23T23:18:36.078602Z","resolver_source":"arxiv_id","status":"verified_exact"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-07-13T06:30:06.624239+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-07-13T06:30:06.624239+00:00","source":"crossref"},{"observed_at":"2026-07-13T06:30:01.874667+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":{"arxiv_id":"gr-qc/9910091","last_updated":"2001-01-05T22:22:39Z","snapshot_observed_at":"2026-07-07T03:31:16.559218Z","submitted_at":"1999-10-26T18:32:02Z","title":"The evolution of circular, non-equatorial orbits of Kerr black holes due to gravitational-wave emission","version":3},"cited_work":{"arxiv_id":"gr-qc/9910091","doi":null,"metadata_source":"pith","pith_arxiv_id":"gr-qc/9910091","snapshot_observed_at":"2026-07-04T11:09:47.064563Z","title":"The evolution of circular, non-equatorial orbits of Kerr black holes due to gravitational-wave emission","venue":"gr-qc","work_id":"98b95432-db34-481e-975d-f70560fed373","year":1999},"citing_paper":{"arxiv_id":"2407.00366","last_updated":"2025-12-17T10:16:02Z","snapshot_observed_at":"2026-07-06T02:11:23.670680Z","submitted_at":"2024-06-29T08:31:38Z","title":"Comparison of 4.5PN and 2SF gravitational energy fluxes from quasicircular compact binaries","version":2},"reference_index":41,"source":"pdf_text","source_observed_at":"2026-05-23T23:17:55.191990Z"},"links":{"cited_paper":"/paper/gr-qc/9910091","citing_paper":"/paper/2407.00366"},"observation_digest":"sha256:a8cb2941d09c6215dda941210b7e90049b3dbc275c9e68eff36154dea4ee1b42","observation_id":"a608dd3e-674c-4402-bf4e-1793d94d364c","resolution":{"observed_at":"2026-05-23T23:18:36.018231Z","resolver_source":"local_arxiv","status":"verified_exact"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-07-13T06:30:06.624239+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-07-13T06:30:06.624239+00:00","source":"crossref"},{"observed_at":"2026-07-13T06:30:01.874667+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":{"arxiv_id":"1609.01731","last_updated":"2018-01-17T01:38:42Z","snapshot_observed_at":"2026-07-06T05:09:50.551461Z","submitted_at":"2016-09-06T20:00:36Z","title":"Bondi-Sachs Formalism","version":3},"cited_work":{"arxiv_id":"1609.01731","doi":null,"metadata_source":"pith","pith_arxiv_id":"1609.01731","snapshot_observed_at":"2026-07-10T16:27:22.139973Z","title":"Bondi-Sachs Formalism","venue":"gr-qc","work_id":"86ced1fd-4879-4ebd-8b3a-7bd8bfb2831b","year":2016},"citing_paper":{"arxiv_id":"2407.00366","last_updated":"2025-12-17T10:16:02Z","snapshot_observed_at":"2026-07-06T02:11:23.670680Z","submitted_at":"2024-06-29T08:31:38Z","title":"Comparison of 4.5PN and 2SF gravitational energy fluxes from quasicircular compact binaries","version":2},"reference_index":42,"source":"pdf_text","source_observed_at":"2026-05-23T23:17:55.191990Z"},"links":{"cited_paper":"/paper/1609.01731","citing_paper":"/paper/2407.00366"},"observation_digest":"sha256:65280b666519a75f61b562a663ba25607214906e576aefb3d968c49dc79cb27c","observation_id":"79d41dfb-2bf3-4f3b-861e-69ac34616d28","resolution":{"observed_at":"2026-05-23T23:18:35.835907Z","resolver_source":"local_arxiv","status":"verified_exact"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-07-13T06:30:06.624239+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-07-13T06:30:06.624239+00:00","source":"crossref"},{"observed_at":"2026-07-13T06:30:01.874667+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":{"arxiv_id":"1510.05172","last_updated":"2015-10-17T22:05:18Z","snapshot_observed_at":"2026-07-06T04:33:26.852705Z","submitted_at":"2015-10-17T22:05:18Z","title":"Second-order perturbation theory: problems on large scales","version":1},"cited_work":{"arxiv_id":"1510.05172","doi":null,"metadata_source":"pith","pith_arxiv_id":"1510.05172","snapshot_observed_at":"2026-07-04T18:50:05.362806Z","title":"Second-order perturbation theory: problems on large scales","venue":"gr-qc","work_id":"8b736d34-6de1-454e-895b-4c5c93ea4ea6","year":2015},"citing_paper":{"arxiv_id":"2407.00366","last_updated":"2025-12-17T10:16:02Z","snapshot_observed_at":"2026-07-06T02:11:23.670680Z","submitted_at":"2024-06-29T08:31:38Z","title":"Comparison of 4.5PN and 2SF gravitational energy fluxes from quasicircular compact binaries","version":2},"reference_index":43,"source":"pdf_text","source_observed_at":"2026-05-23T23:17:55.191990Z"},"links":{"cited_paper":"/paper/1510.05172","citing_paper":"/paper/2407.00366"},"observation_digest":"sha256:7159d84625cdafa0e15607b2f2623b0b42e9a359ef1330648327bef9bbcc2339","observation_id":"9d8b83ce-3e6e-409a-8605-bda7a82a4659","resolution":{"observed_at":"2026-05-23T23:18:36.067126Z","resolver_source":"local_arxiv","status":"verified_exact"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-07-13T06:30:06.624239+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-07-13T06:30:06.624239+00:00","source":"crossref"},{"observed_at":"2026-07-13T06:30:01.874667+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":{"arxiv_id":"2208.01049","last_updated":"2022-11-02T11:15:30Z","snapshot_observed_at":"2026-07-06T13:37:39.596081Z","submitted_at":"2022-08-01T18:00:02Z","title":"Comparing second-order gravitational self-force, numerical relativity and effective one body waveforms from inspiralling, quasi-circular and nonspinning black hole binaries","version":2},"cited_work":{"arxiv_id":"2208.01049","doi":null,"metadata_source":"arxiv_reference","pith_arxiv_id":"2208.01049","snapshot_observed_at":"2026-07-02T10:06:51.850583Z","title":"Albertini, A","venue":null,"work_id":"eb1fdedb-eeae-46c0-a368-bde32784e18b","year":2022},"citing_paper":{"arxiv_id":"2407.00366","last_updated":"2025-12-17T10:16:02Z","snapshot_observed_at":"2026-07-06T02:11:23.670680Z","submitted_at":"2024-06-29T08:31:38Z","title":"Comparison of 4.5PN and 2SF gravitational energy fluxes from quasicircular compact binaries","version":2},"reference_index":44,"source":"pdf_text","source_observed_at":"2026-05-23T23:17:55.191990Z"},"links":{"cited_paper":"/paper/2208.01049","citing_paper":"/paper/2407.00366"},"observation_digest":"sha256:41201029c685b788903476f313d43f87e4598c3848411505abd51079b7c909ad","observation_id":"51daa0fc-5fe3-46a9-aa76-0982460168e0","resolution":{"observed_at":"2026-05-23T23:18:35.882436Z","resolver_source":"arxiv_id","status":"verified_exact"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-07-13T06:30:06.624239+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-07-13T06:30:06.624239+00:00","source":"crossref"},{"observed_at":"2026-07-13T06:30:01.874667+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":"Boyle, D","venue":null,"work_id":"ec0f8564-2b75-4ff4-ae2f-7f959e53b5a9","year":2019},"citing_paper":{"arxiv_id":"2407.00366","last_updated":"2025-12-17T10:16:02Z","snapshot_observed_at":"2026-07-06T02:11:23.670680Z","submitted_at":"2024-06-29T08:31:38Z","title":"Comparison of 4.5PN and 2SF gravitational energy fluxes from quasicircular compact binaries","version":2},"reference_index":45,"source":"pdf_text","source_observed_at":"2026-05-23T23:17:55.191990Z"},"links":{"citing_paper":"/paper/2407.00366"},"observation_digest":"sha256:321827bf7a1d114cd2f2eddb0b6fe54d23e763cc2f5654751fd55aab254217c4","observation_id":"0a30d2f0-7d3c-4c59-b131-b9159065b66d","resolution":{"observed_at":"2026-05-23T23:18:36.283234Z","resolver_source":"raw_fallback","status":"verified_fuzzy"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-07-13T06:30:06.624239+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-07-13T06:30:06.624239+00:00","source":"crossref"},{"observed_at":"2026-07-13T06:30:01.874667+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":"10.5281/zenodo.3301955","metadata_source":"doi_reference","pith_arxiv_id":null,"snapshot_observed_at":"2026-06-05T21:23:00.469572Z","title":null,"venue":null,"work_id":"7f6286c1-5dcd-458c-bed4-4be788385603","year":2019},"citing_paper":{"arxiv_id":"2407.00366","last_updated":"2025-12-17T10:16:02Z","snapshot_observed_at":"2026-07-06T02:11:23.670680Z","submitted_at":"2024-06-29T08:31:38Z","title":"Comparison of 4.5PN and 2SF gravitational energy fluxes from quasicircular compact binaries","version":2},"reference_index":46,"source":"pdf_text","source_observed_at":"2026-05-23T23:17:55.191990Z"},"links":{"citing_paper":"/paper/2407.00366"},"observation_digest":"sha256:ae77c990ece72a7445973ec0db448f351c32bd8f77ececeb8dc2e12741a8ab66","observation_id":"097b2010-2b65-40f9-ae48-185b8511b6e6","resolution":{"observed_at":"2026-05-23T23:18:35.698854Z","resolver_source":"doi","status":"verified_exact"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-07-13T06:30:06.624239+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-07-13T06:30:06.624239+00:00","source":"crossref"},{"observed_at":"2026-07-13T06:30:01.874667+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":"10.5281/zenodo.3302023","metadata_source":"doi_reference","pith_arxiv_id":null,"snapshot_observed_at":"2026-06-05T21:23:00.469572Z","title":"Collaboration, Binary black-hole simulation sxs:bbh:1107, 10.5281/zenodo.3302023 (2019)","venue":null,"work_id":"f919d689-96f7-4971-85e1-69f0df0bcadf","year":2019},"citing_paper":{"arxiv_id":"2407.00366","last_updated":"2025-12-17T10:16:02Z","snapshot_observed_at":"2026-07-06T02:11:23.670680Z","submitted_at":"2024-06-29T08:31:38Z","title":"Comparison of 4.5PN and 2SF gravitational energy fluxes from quasicircular compact binaries","version":2},"reference_index":47,"source":"pdf_text","source_observed_at":"2026-05-23T23:17:55.191990Z"},"links":{"citing_paper":"/paper/2407.00366"},"observation_digest":"sha256:5aac8950826ed53edd97175c6ce0de06d8783fb11ca11b40b929e8ccfebfdc4d","observation_id":"33924776-f839-4c4c-bd60-cb59785c72ac","resolution":{"observed_at":"2026-05-23T23:18:35.714673Z","resolver_source":"doi","status":"verified_exact"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-07-13T06:30:06.624239+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-07-13T06:30:06.624239+00:00","source":"crossref"},{"observed_at":"2026-07-13T06:30:01.874667+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":{"arxiv_id":"1509.00862","last_updated":"2016-03-23T14:59:10Z","snapshot_observed_at":"2026-07-06T04:28:37.319146Z","submitted_at":"2015-09-02T20:08:40Z","title":"Transformations of asymptotic gravitational-wave data","version":3},"cited_work":{"arxiv_id":"1509.00862","doi":null,"metadata_source":"pith","pith_arxiv_id":"1509.00862","snapshot_observed_at":"2026-07-04T18:50:05.369240Z","title":"Transformations of asymptotic gravitational-wave data","venue":"gr-qc","work_id":"9f73ba68-8735-4f16-89d2-ca2a9145f95a","year":2015},"citing_paper":{"arxiv_id":"2407.00366","last_updated":"2025-12-17T10:16:02Z","snapshot_observed_at":"2026-07-06T02:11:23.670680Z","submitted_at":"2024-06-29T08:31:38Z","title":"Comparison of 4.5PN and 2SF gravitational energy fluxes from quasicircular compact binaries","version":2},"reference_index":48,"source":"pdf_text","source_observed_at":"2026-05-23T23:17:55.191990Z"},"links":{"cited_paper":"/paper/1509.00862","citing_paper":"/paper/2407.00366"},"observation_digest":"sha256:4eeb683ad4a93ae3c7b79e359434e151cfc74fa1376ce1752f50e9e7addbe406","observation_id":"66eed9bd-65aa-402d-9e5f-e3c23c2d5e29","resolution":{"observed_at":"2026-05-23T23:18:35.896846Z","resolver_source":"local_arxiv","status":"verified_exact"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-07-13T06:30:06.624239+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-07-13T06:30:06.624239+00:00","source":"crossref"},{"observed_at":"2026-07-13T06:30:01.874667+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":{"arxiv_id":"1104.5615","last_updated":"2012-08-27T15:40:01Z","snapshot_observed_at":"2026-07-06T02:27:00.560695Z","submitted_at":"2011-04-29T12:51:19Z","title":"Gravitational radiation for extreme mass ratio inspirals to the 14th post-Newtonian order","version":2},"cited_work":{"arxiv_id":"1104.5615","doi":null,"metadata_source":"pith","pith_arxiv_id":"1104.5615","snapshot_observed_at":"2026-06-05T21:23:00.469572Z","title":"Gravitational radiation for extreme mass ratio inspirals to the 14th post-Newtonian order","venue":"gr-qc","work_id":"1cc4c623-1a41-4517-85fd-f0966795edfd","year":2011},"citing_paper":{"arxiv_id":"2407.00366","last_updated":"2025-12-17T10:16:02Z","snapshot_observed_at":"2026-07-06T02:11:23.670680Z","submitted_at":"2024-06-29T08:31:38Z","title":"Comparison of 4.5PN and 2SF gravitational energy fluxes from quasicircular compact binaries","version":2},"reference_index":49,"source":"pdf_text","source_observed_at":"2026-05-23T23:17:55.191990Z"},"links":{"cited_paper":"/paper/1104.5615","citing_paper":"/paper/2407.00366"},"observation_digest":"sha256:0cd2a0ea6304527798f7504c07381bc7f2aa0056749e42a66a089c92e52e117e","observation_id":"33cb801e-692f-4a87-bde5-9dfe45699311","resolution":{"observed_at":"2026-05-23T23:18:35.903335Z","resolver_source":"local_arxiv","status":"verified_exact"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-07-13T06:30:06.624239+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-07-13T06:30:06.624239+00:00","source":"crossref"},{"observed_at":"2026-07-13T06:30:01.874667+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":"Fujita, Gravitational waves from a particle in circular orbits around a schwarzschild black hole to the 22nd post- Newtonian order, Prog","venue":null,"work_id":"c84b5d42-446e-4f79-9129-523df5bff71d","year":2012},"citing_paper":{"arxiv_id":"2407.00366","last_updated":"2025-12-17T10:16:02Z","snapshot_observed_at":"2026-07-06T02:11:23.670680Z","submitted_at":"2024-06-29T08:31:38Z","title":"Comparison of 4.5PN and 2SF gravitational energy fluxes from quasicircular compact binaries","version":2},"reference_index":50,"source":"pdf_text","source_observed_at":"2026-05-23T23:17:55.191990Z"},"links":{"citing_paper":"/paper/2407.00366"},"observation_digest":"sha256:bb60fc3c6929262f72e3f21a2c2b4dfce7981469a1608ac09ef1d6c7ae0638e0","observation_id":"f1bd08d2-f8c1-4bc6-8a7c-b315e94be523","resolution":{"observed_at":"2026-05-23T23:18:36.319123Z","resolver_source":"raw_fallback","status":"verified_fuzzy"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-07-13T06:30:06.624239+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-07-13T06:30:06.624239+00:00","source":"crossref"},{"observed_at":"2026-07-13T06:30:01.874667+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":{"arxiv_id":"2405.08868","last_updated":"2024-11-11T16:15:34Z","snapshot_observed_at":"2026-07-06T18:14:20.889736Z","submitted_at":"2024-05-14T18:00:02Z","title":"A Review of Gravitational Memory and BMS Frame Fixing in Numerical Relativity","version":2},"cited_work":{"arxiv_id":"2405.08868","doi":null,"metadata_source":"pith","pith_arxiv_id":"2405.08868","snapshot_observed_at":"2026-07-10T16:27:22.222393Z","title":"Mitman, M","venue":"gr-qc","work_id":"3bf36261-950e-47dd-afad-b522719f24a4","year":2024},"citing_paper":{"arxiv_id":"2407.00366","last_updated":"2025-12-17T10:16:02Z","snapshot_observed_at":"2026-07-06T02:11:23.670680Z","submitted_at":"2024-06-29T08:31:38Z","title":"Comparison of 4.5PN and 2SF gravitational energy fluxes from quasicircular compact binaries","version":2},"reference_index":51,"source":"pdf_text","source_observed_at":"2026-05-23T23:17:55.191990Z"},"links":{"cited_paper":"/paper/2405.08868","citing_paper":"/paper/2407.00366"},"observation_digest":"sha256:c9749c0db6d8411b5c2116ffa243e58b148a77741961f6b08caaa41242ff5372","observation_id":"a692857d-eccc-4374-a70c-3900e5e7322c","resolution":{"observed_at":"2026-05-23T23:18:36.072796Z","resolver_source":"arxiv_id","status":"verified_exact"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-07-13T06:30:06.624239+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-07-13T06:30:06.624239+00:00","source":"crossref"},{"observed_at":"2026-07-13T06:30:01.874667+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":{"arxiv_id":"gr-qc/0312010","last_updated":"2003-12-01T22:07:53Z","snapshot_observed_at":"2026-07-07T03:18:35.419334Z","submitted_at":"2003-12-01T22:07:53Z","title":"Low multipole contributions to the gravitational self-force","version":1},"cited_work":{"arxiv_id":"gr-qc/0312010","doi":null,"metadata_source":"pith","pith_arxiv_id":"gr-qc/0312010","snapshot_observed_at":"2026-07-04T18:50:05.347312Z","title":"Low multipole contributions to the gravitational self-force","venue":"gr-qc","work_id":"bf19e510-d01f-4624-93f6-cdbd55f5df27","year":2003},"citing_paper":{"arxiv_id":"2407.00366","last_updated":"2025-12-17T10:16:02Z","snapshot_observed_at":"2026-07-06T02:11:23.670680Z","submitted_at":"2024-06-29T08:31:38Z","title":"Comparison of 4.5PN and 2SF gravitational energy fluxes from quasicircular compact binaries","version":2},"reference_index":52,"source":"pdf_text","source_observed_at":"2026-05-23T23:17:55.191990Z"},"links":{"cited_paper":"/paper/gr-qc/0312010","citing_paper":"/paper/2407.00366"},"observation_digest":"sha256:63dcf3e92c1895d84e8505216a5b0f716dc3db4c70fc351d0beb2742d87094bd","observation_id":"d2a4ede7-8b1a-4cb6-a151-f37894b90090","resolution":{"observed_at":"2026-05-23T23:18:36.043721Z","resolver_source":"local_arxiv","status":"verified_exact"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-07-13T06:30:06.624239+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-07-13T06:30:06.624239+00:00","source":"crossref"},{"observed_at":"2026-07-13T06:30:01.874667+00:00","source":"retraction_watch"}],"state":"measured"}}],"paper":{"arxiv_id":"2407.00366","last_updated":"2025-12-17T10:16:02Z","latest_version":2,"primary_category":"gr-qc","snapshot_observed_at":"2026-07-06T02:11:23.670680Z","submitted_at":"2024-06-29T08:31:38Z","title":"Comparison of 4.5PN and 2SF gravitational energy fluxes from quasicircular compact binaries"},"reference_resolution":{"displayed":52,"state_counts":{"malformed_identifier":0,"metadata_mismatch":0,"parse_uncertain":0,"unresolved":0,"verified_exact":41,"verified_fuzzy":11},"total_outbound_references":52},"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":"2026-07-13T06:30:06.624239+00:00","source":"crossref"},{"observed_at":"2026-07-13T06:30:01.874667+00:00","source":"retraction_watch"}],"thesis":"As of 13 July 2026, this Paper Citation Record lists 52 of 52 outbound references and 4 inbound Pith citation observations for arXiv:2407.00366."}