{"as_of":"2026-08-18T13:22:00Z","caps":{"database_statements":6,"inbound":100,"outbound":100},"context_digest":"sha256:882458d3781e839c40aea5e064e4efb386090610c2b4ce452e37a292d205ed6e","coverage":[{"denominator":51,"lane":"reference_resolution","note":"Typed states for the displayed outbound observations.","records_observed":51,"source":"paper_references, paper_reference_links","source_observed_at":"2026-08-12T21:08:18.352538Z","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":"2026-08-18T06:34:40.430872+00:00","state":"measured"},{"denominator":5,"lane":"inbound_itemization","note":"Pith citing papers itemized under the disclosed page cap.","records_observed":5,"source":"paper_references, paper_reference_links","source_observed_at":"2026-08-12T20:28:15.018325Z","state":"measured"},{"denominator":1,"lane":"external_citation_measurements","note":"A source-named dated measurement, never combined with another source.","records_observed":0,"source":"arxiv_reference","source_observed_at":"2026-07-01T13:35:45.732062Z","state":"measured"}],"external_citation_measurements":[],"inbound":[{"citation":{"cited_paper":{"arxiv_id":"2411.09147","last_updated":"2025-03-27T07:52:56Z","snapshot_observed_at":"2026-08-16T08:34:44.313485Z","submitted_at":"2024-11-14T02:57:25Z","title":"Post-Newtonian templates for phase evolution of spherical extreme mass ratio inspirals","version":3},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2411.09147","snapshot_observed_at":"2026-08-12T20:28:15.018325Z","title":null,"venue":null,"work_id":null,"year":2024},"citing_paper":{"arxiv_id":"2411.09700","last_updated":"2025-03-31T21:04:49Z","snapshot_observed_at":"2026-08-17T00:47:37.991874Z","submitted_at":"2024-11-14T18:59:35Z","title":"Post-Newtonian expansion of gravitational energy and angular momentum fluxes: inclined spherical orbits about a Kerr black hole","version":2},"reference_index":62,"source":"pdf_text","source_observed_at":"2026-08-12T20:28:15.018325Z"},"links":{"cited_paper":"/paper/2411.09147","citing_paper":"/paper/2411.09700"},"observation_digest":"sha256:0d9221caa78071658d9b33bd336cbf7052f34d50eefc3cd0558d67c31dc8dc37","observation_id":"a5b494ff-aa8b-4075-b9dd-bdc02481ed92","resolution":{"observed_at":"2026-08-12T20:28:15.018325Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2411.09147","last_updated":"2025-03-27T07:52:56Z","snapshot_observed_at":"2026-08-16T08:34:44.313485Z","submitted_at":"2024-11-14T02:57:25Z","title":"Post-Newtonian templates for phase evolution of spherical extreme mass ratio inspirals","version":3},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2411.09147","snapshot_observed_at":"2026-08-03T02:31:00.550181Z","title":null,"venue":null,"work_id":null,"year":2025},"citing_paper":{"arxiv_id":"2603.27941","last_updated":"2026-03-30T01:34:12Z","snapshot_observed_at":"2026-08-17T20:11:24.293089Z","submitted_at":"2026-03-30T01:34:12Z","title":"Secular evolution of orbital parameters for general bound orbits in Kerr spacetime","version":1},"reference_index":77,"source":"pdf_text","source_observed_at":"2026-08-03T02:31:00.550181Z"},"links":{"cited_paper":"/paper/2411.09147","citing_paper":"/paper/2603.27941"},"observation_digest":"sha256:e275c275de5fabf6325ab389d0c2cad57f79232705331ced2cba749b79eaa43a","observation_id":"287055cf-a023-493b-92a6-b4e3d2fadc7e","resolution":{"observed_at":"2026-08-03T02:31:00.550181Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2411.09147","last_updated":"2025-03-27T07:52:56Z","snapshot_observed_at":"2026-08-16T08:34:44.313485Z","submitted_at":"2024-11-14T02:57:25Z","title":"Post-Newtonian templates for phase evolution of spherical extreme mass ratio inspirals","version":3},"cited_work":{"arxiv_id":"2411.09147","doi":null,"metadata_source":"arxiv_reference","pith_arxiv_id":"2411.09147","snapshot_observed_at":"2026-07-01T13:35:45.732062Z","title":null,"venue":null,"work_id":"84a1a53a-71b5-450d-8df2-249ee812954c","year":2025},"citing_paper":{"arxiv_id":"2605.09250","last_updated":"2026-06-25T02:39:11Z","snapshot_observed_at":"2026-08-14T23:51:10.108139Z","submitted_at":"2026-05-10T01:28:01Z","title":"Efficient and Stable Computation of Gravitational-Wave Fluxes from Generic Kerr Orbits via a Unified HeunC Framework","version":1},"reference_index":76,"source":"pdf_text","source_observed_at":"2026-05-12T03:04:27.279604Z"},"links":{"cited_paper":"/paper/2411.09147","citing_paper":"/paper/2605.09250"},"observation_digest":"sha256:6bd3df891304baa68ddb0ac945ec0fbb0e8cf6a51aec044ed00331da3eaf6d82","observation_id":"d5a95f2e-3342-4e8a-8f4a-2921488d315a","resolution":{"observed_at":"2026-05-12T03:06:19.372922Z","resolver_source":"arxiv_id","status":"verified_exact"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-18T06:34:40.430872+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-18T06:34:40.430872+00:00","source":"crossref"},{"observed_at":"2026-08-18T06:34:34.496301+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":{"arxiv_id":"2411.09147","last_updated":"2025-03-27T07:52:56Z","snapshot_observed_at":"2026-08-16T08:34:44.313485Z","submitted_at":"2024-11-14T02:57:25Z","title":"Post-Newtonian templates for phase evolution of spherical extreme mass ratio inspirals","version":3},"cited_work":{"arxiv_id":"2411.09147","doi":null,"metadata_source":"arxiv_reference","pith_arxiv_id":"2411.09147","snapshot_observed_at":"2026-07-01T13:35:45.732062Z","title":null,"venue":null,"work_id":"84a1a53a-71b5-450d-8df2-249ee812954c","year":2025},"citing_paper":{"arxiv_id":"2605.09250","last_updated":"2026-06-25T02:39:11Z","snapshot_observed_at":"2026-08-14T23:51:10.108139Z","submitted_at":"2026-05-10T01:28:01Z","title":"Efficient and Stable Computation of Gravitational-Wave Fluxes from Generic Kerr Orbits via a Unified HeunC Framework","version":2},"reference_index":76,"source":"pdf_text","source_observed_at":"2026-05-13T07:47:14.054826Z"},"links":{"cited_paper":"/paper/2411.09147","citing_paper":"/paper/2605.09250"},"observation_digest":"sha256:74d9d4be21353987da0ac4c11331fb380e2b3b94bce340cb8f34c48bc28434c2","observation_id":"71d556e1-b50e-4e1e-8563-a3ff5fc49cd9","resolution":{"observed_at":"2026-05-13T07:47:32.613387Z","resolver_source":"arxiv_id","status":"verified_exact"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-18T06:34:40.430872+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-18T06:34:40.430872+00:00","source":"crossref"},{"observed_at":"2026-08-18T06:34:34.496301+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":{"arxiv_id":"2411.09147","last_updated":"2025-03-27T07:52:56Z","snapshot_observed_at":"2026-08-16T08:34:44.313485Z","submitted_at":"2024-11-14T02:57:25Z","title":"Post-Newtonian templates for phase evolution of spherical extreme mass ratio inspirals","version":3},"cited_work":{"arxiv_id":"2411.09147","doi":null,"metadata_source":"arxiv_reference","pith_arxiv_id":"2411.09147","snapshot_observed_at":"2026-07-01T13:35:45.732062Z","title":null,"venue":null,"work_id":"84a1a53a-71b5-450d-8df2-249ee812954c","year":2025},"citing_paper":{"arxiv_id":"2605.09250","last_updated":"2026-06-25T02:39:11Z","snapshot_observed_at":"2026-08-14T23:51:10.108139Z","submitted_at":"2026-05-10T01:28:01Z","title":"Efficient and Stable Computation of Gravitational-Wave Fluxes from Generic Kerr Orbits via a Unified HeunC Framework","version":3},"reference_index":76,"source":"pdf_text","source_observed_at":"2026-06-30T23:08:26.953490Z"},"links":{"cited_paper":"/paper/2411.09147","citing_paper":"/paper/2605.09250"},"observation_digest":"sha256:aac3fbe8697abab59fa7cefa18467a21bfede05ffc6df240cb359b06629cd6cd","observation_id":"62e0961f-b4bb-4784-9bbc-68030475b420","resolution":{"observed_at":"2026-07-01T13:35:45.733406Z","resolver_source":"arxiv_id","status":"verified_exact"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-18T06:34:40.430872+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-18T06:34:40.430872+00:00","source":"crossref"},{"observed_at":"2026-08-18T06:34:34.496301+00:00","source":"retraction_watch"}],"state":"measured"}}],"links":{"evidence":"/evidence","html":"/paper/2411.09147/citation-record","integrity":"/paper/2411.09147/integrity","json":"/paper/2411.09147/citation-record.json","paper":"/paper/2411.09147"},"outbound":[{"citation":{"cited_paper":{"arxiv_id":"1702.00786","last_updated":"2017-02-23T05:33:01Z","snapshot_observed_at":"2026-08-17T04:50:23.618217Z","submitted_at":"2017-02-02T07:06:53Z","title":"Laser Interferometer Space Antenna","version":3},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"1702.00786","snapshot_observed_at":"2026-08-12T21:08:18.096167Z","title":"Amaro-Seoane et al","venue":null,"work_id":null,"year":2017},"citing_paper":{"arxiv_id":"2411.09147","last_updated":"2025-03-27T07:52:56Z","snapshot_observed_at":"2026-08-16T08:34:44.313485Z","submitted_at":"2024-11-14T02:57:25Z","title":"Post-Newtonian templates for phase evolution of spherical extreme mass ratio inspirals","version":3},"reference_index":1,"source":"pdf_text","source_observed_at":"2026-08-12T21:08:18.096167Z"},"links":{"cited_paper":"/paper/1702.00786","citing_paper":"/paper/2411.09147"},"observation_digest":"sha256:6dea11fed3817e1dae5029473d49a107357d53e4f37c6f117588ec1a174a09d1","observation_id":"1406b477-5fe6-404b-a3b2-f5f49ed97967","resolution":{"observed_at":"2026-08-12T21:08:18.096167Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"1512.02076","last_updated":"2015-12-07T14:57:50Z","snapshot_observed_at":"2026-08-14T22:19:42.208890Z","submitted_at":"2015-12-07T14:57:50Z","title":"TianQin: a space-borne gravitational wave detector","version":1},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"1512.02076","snapshot_observed_at":"2026-08-12T21:08:18.101638Z","title":"Luo et al","venue":null,"work_id":null,"year":2016},"citing_paper":{"arxiv_id":"2411.09147","last_updated":"2025-03-27T07:52:56Z","snapshot_observed_at":"2026-08-16T08:34:44.313485Z","submitted_at":"2024-11-14T02:57:25Z","title":"Post-Newtonian templates for phase evolution of spherical extreme mass ratio inspirals","version":3},"reference_index":2,"source":"pdf_text","source_observed_at":"2026-08-12T21:08:18.101638Z"},"links":{"cited_paper":"/paper/1512.02076","citing_paper":"/paper/2411.09147"},"observation_digest":"sha256:695e67246c78e348ba4e372886c361def3c4945b5eeb703074f9966d0be90203","observation_id":"9e0d4f88-6a3d-4946-a5c3-3285ec3d924e","resolution":{"observed_at":"2026-08-12T21:08:18.101638Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"1807.09495","last_updated":"2020-06-04T08:56:43Z","snapshot_observed_at":"2026-08-15T09:42:06.539001Z","submitted_at":"2018-07-25T09:11:17Z","title":"Taiji Program: Gravitational-Wave Sources","version":3},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"1807.09495","snapshot_observed_at":"2026-08-12T21:08:18.107349Z","title":"Ruan, Z.-K","venue":null,"work_id":null,"year":2020},"citing_paper":{"arxiv_id":"2411.09147","last_updated":"2025-03-27T07:52:56Z","snapshot_observed_at":"2026-08-16T08:34:44.313485Z","submitted_at":"2024-11-14T02:57:25Z","title":"Post-Newtonian templates for phase evolution of spherical extreme mass ratio inspirals","version":3},"reference_index":3,"source":"pdf_text","source_observed_at":"2026-08-12T21:08:18.107349Z"},"links":{"cited_paper":"/paper/1807.09495","citing_paper":"/paper/2411.09147"},"observation_digest":"sha256:dd733134a1ae2d6addc2360c5079282be32dc200424a42f285ad4948a7830628","observation_id":"9252e3ca-4380-42a9-baf2-149b9e3bf564","resolution":{"observed_at":"2026-08-12T21:08:18.107349Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"1003.5553","last_updated":"2010-03-29T14:31:22Z","snapshot_observed_at":"2026-08-17T11:24:21.534800Z","submitted_at":"2010-03-29T14:31:22Z","title":"Gravitational Waves Notes, Issue #2 : \"A probe of spacetime and astrophysics: EMRIs\"","version":1},"cited_work":{"arxiv_id":"1003.5553","doi":null,"metadata_source":"pith","pith_arxiv_id":"1003.5553","snapshot_observed_at":"2026-08-12T21:08:19.033580Z","title":"Gravitational Waves Notes, Issue #2 : \"A probe of spacetime and astrophysics: EMRIs\"","venue":"astro-ph.CO","work_id":"71107833-21e4-4c3d-9ab5-486e9f65f9ac","year":2010},"citing_paper":{"arxiv_id":"2411.09147","last_updated":"2025-03-27T07:52:56Z","snapshot_observed_at":"2026-08-16T08:34:44.313485Z","submitted_at":"2024-11-14T02:57:25Z","title":"Post-Newtonian templates for phase evolution of spherical extreme mass ratio inspirals","version":3},"reference_index":4,"source":"pdf_text","source_observed_at":"2026-08-12T21:08:18.112421Z"},"links":{"cited_paper":"/paper/1003.5553","citing_paper":"/paper/2411.09147"},"observation_digest":"sha256:767d5a064087da1406b9a71af179ee87a83e5708c1f62291f6d88af716cd0aba","observation_id":"d33c4838-639d-412c-a3b2-1c9554cbba3d","resolution":{"observed_at":"2026-08-12T21:08:19.038395Z","resolver_source":"local_arxiv","status":"verified_exact"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-18T06:34:40.430872+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-18T06:34:40.430872+00:00","source":"crossref"},{"observed_at":"2026-08-18T06:34:34.496301+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":{"arxiv_id":"1703.09722","last_updated":"2018-04-11T11:52:26Z","snapshot_observed_at":"2026-08-14T21:09:32.929806Z","submitted_at":"2017-03-28T18:00:17Z","title":"Science with the space-based interferometer LISA. V: Extreme mass-ratio inspirals","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"1703.09722","snapshot_observed_at":"2026-08-12T21:08:18.118355Z","title":"Babak, J","venue":null,"work_id":null,"year":2017},"citing_paper":{"arxiv_id":"2411.09147","last_updated":"2025-03-27T07:52:56Z","snapshot_observed_at":"2026-08-16T08:34:44.313485Z","submitted_at":"2024-11-14T02:57:25Z","title":"Post-Newtonian templates for phase evolution of spherical extreme mass ratio inspirals","version":3},"reference_index":5,"source":"pdf_text","source_observed_at":"2026-08-12T21:08:18.118355Z"},"links":{"cited_paper":"/paper/1703.09722","citing_paper":"/paper/2411.09147"},"observation_digest":"sha256:2c4982c83632816dc7c9ed214ef740b49b0f4c1e4fddffbb6279623b5c732b08","observation_id":"7bfdf446-9494-45bf-911b-284eecf935e9","resolution":{"observed_at":"2026-08-12T21:08:18.118355Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"1903.03686","last_updated":"2019-03-08T22:35:28Z","snapshot_observed_at":"2026-08-15T11:14:51.686103Z","submitted_at":"2019-03-08T22:35:28Z","title":"The unique potential of extreme mass-ratio inspirals for gravitational-wave astronomy","version":1},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"1903.03686","snapshot_observed_at":"2026-08-12T21:08:18.123443Z","title":"Berry, S","venue":null,"work_id":null,"year":2019},"citing_paper":{"arxiv_id":"2411.09147","last_updated":"2025-03-27T07:52:56Z","snapshot_observed_at":"2026-08-16T08:34:44.313485Z","submitted_at":"2024-11-14T02:57:25Z","title":"Post-Newtonian templates for phase evolution of spherical extreme mass ratio inspirals","version":3},"reference_index":6,"source":"pdf_text","source_observed_at":"2026-08-12T21:08:18.123443Z"},"links":{"cited_paper":"/paper/1903.03686","citing_paper":"/paper/2411.09147"},"observation_digest":"sha256:e8f4211cfdaa88b2e4379dd172aab2f3b58d972a2342486499c113b30b0be844","observation_id":"99b982f5-b50b-4697-a4d9-7e2fe325f449","resolution":{"observed_at":"2026-08-12T21:08:18.123443Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":null,"snapshot_observed_at":"2026-08-12T21:08:18.129537Z","title":"Newman and R","venue":null,"work_id":null,"year":1962},"citing_paper":{"arxiv_id":"2411.09147","last_updated":"2025-03-27T07:52:56Z","snapshot_observed_at":"2026-08-16T08:34:44.313485Z","submitted_at":"2024-11-14T02:57:25Z","title":"Post-Newtonian templates for phase evolution of spherical extreme mass ratio inspirals","version":3},"reference_index":7,"source":"pdf_text","source_observed_at":"2026-08-12T21:08:18.129537Z"},"links":{"citing_paper":"/paper/2411.09147"},"observation_digest":"sha256:89cbf8fba6030499985a30671e4d87d9143cafb746c9bda084c02048e67e56cd","observation_id":"729cf1aa-f2bc-4285-b159-761579342a0a","resolution":{"observed_at":"2026-08-12T21:08:18.129537Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":null,"snapshot_observed_at":"2026-08-12T21:08:18.133710Z","title":null,"venue":null,"work_id":null,"year":1972},"citing_paper":{"arxiv_id":"2411.09147","last_updated":"2025-03-27T07:52:56Z","snapshot_observed_at":"2026-08-16T08:34:44.313485Z","submitted_at":"2024-11-14T02:57:25Z","title":"Post-Newtonian templates for phase evolution of spherical extreme mass ratio inspirals","version":3},"reference_index":8,"source":"pdf_text","source_observed_at":"2026-08-12T21:08:18.133710Z"},"links":{"citing_paper":"/paper/2411.09147"},"observation_digest":"sha256:df6e877142129103feaabf94bf99ccee904f1e31715ded4ddc47c1032528f947","observation_id":"bca1009f-2fc6-46a5-95e6-7d5179f0a55d","resolution":{"observed_at":"2026-08-12T21:08:18.133710Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":null,"snapshot_observed_at":"2026-08-12T21:08:18.137801Z","title":null,"venue":null,"work_id":null,"year":1973},"citing_paper":{"arxiv_id":"2411.09147","last_updated":"2025-03-27T07:52:56Z","snapshot_observed_at":"2026-08-16T08:34:44.313485Z","submitted_at":"2024-11-14T02:57:25Z","title":"Post-Newtonian templates for phase evolution of spherical extreme mass ratio inspirals","version":3},"reference_index":9,"source":"pdf_text","source_observed_at":"2026-08-12T21:08:18.137801Z"},"links":{"citing_paper":"/paper/2411.09147"},"observation_digest":"sha256:d7d9afea8a32489aac34f8b078ccc29994dc08d0434a6ecaf5966c9accaa0856","observation_id":"95ab105c-55c3-415a-8357-6768fe87a85d","resolution":{"observed_at":"2026-08-12T21:08:18.137801Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"1805.10385","last_updated":"2018-11-19T12:44:05Z","snapshot_observed_at":"2026-08-14T19:10:55.410662Z","submitted_at":"2018-05-25T22:48:11Z","title":"Self-force and radiation reaction in general relativity","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"1805.10385","snapshot_observed_at":"2026-08-12T21:08:18.143705Z","title":"Barack and A","venue":null,"work_id":null,"year":2019},"citing_paper":{"arxiv_id":"2411.09147","last_updated":"2025-03-27T07:52:56Z","snapshot_observed_at":"2026-08-16T08:34:44.313485Z","submitted_at":"2024-11-14T02:57:25Z","title":"Post-Newtonian templates for phase evolution of spherical extreme mass ratio inspirals","version":3},"reference_index":10,"source":"pdf_text","source_observed_at":"2026-08-12T21:08:18.143705Z"},"links":{"cited_paper":"/paper/1805.10385","citing_paper":"/paper/2411.09147"},"observation_digest":"sha256:45b71cc1bd4ac50e52fbfce6e463b642800518555b8f055a62f9b7fff7d66a13","observation_id":"1892d8d3-261d-46e3-810d-178d11daead4","resolution":{"observed_at":"2026-08-12T21:08:18.143705Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":"raw_reference","pith_arxiv_id":null,"snapshot_observed_at":"2026-08-12T21:08:19.099317Z","title":"Pound and B","venue":null,"work_id":"eb4b23ee-4fdb-4d6b-97ef-10ca0321df46","year":2022},"citing_paper":{"arxiv_id":"2411.09147","last_updated":"2025-03-27T07:52:56Z","snapshot_observed_at":"2026-08-16T08:34:44.313485Z","submitted_at":"2024-11-14T02:57:25Z","title":"Post-Newtonian templates for phase evolution of spherical extreme mass ratio inspirals","version":3},"reference_index":11,"source":"pdf_text","source_observed_at":"2026-08-12T21:08:18.148554Z"},"links":{"citing_paper":"/paper/2411.09147"},"observation_digest":"sha256:c64e1ed35fb4eca08581e1d392234c85cf9ee5b0330b8accfa535bcf3716e8bc","observation_id":"5a087cea-fdaf-4662-95fc-b394ec4b0d91","resolution":{"observed_at":"2026-08-12T21:08:19.103269Z","resolver_source":"raw_fallback","status":"verified_fuzzy"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-18T06:34:40.430872+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-18T06:34:40.430872+00:00","source":"crossref"},{"observed_at":"2026-08-18T06:34:34.496301+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":{"arxiv_id":"gr-qc/0509101","last_updated":"2006-01-19T23:19:18Z","snapshot_observed_at":"2026-08-07T22:17:31.177486Z","submitted_at":"2005-09-26T21:53:09Z","title":"Gravitational wave snapshots of generic extreme mass ratio inspirals","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"gr-qc/0509101","snapshot_observed_at":"2026-08-12T21:08:18.152846Z","title":"Drasco and S","venue":null,"work_id":null,"year":2006},"citing_paper":{"arxiv_id":"2411.09147","last_updated":"2025-03-27T07:52:56Z","snapshot_observed_at":"2026-08-16T08:34:44.313485Z","submitted_at":"2024-11-14T02:57:25Z","title":"Post-Newtonian templates for phase evolution of spherical extreme mass ratio inspirals","version":3},"reference_index":12,"source":"pdf_text","source_observed_at":"2026-08-12T21:08:18.152846Z"},"links":{"cited_paper":"/paper/gr-qc/0509101","citing_paper":"/paper/2411.09147"},"observation_digest":"sha256:d0a779b13419a4c4ddba14175496fbcaed00085e24f323bdf33657d00b5f04ef","observation_id":"77d4d564-f33d-4288-8a43-c71132f27f0a","resolution":{"observed_at":"2026-08-12T21:08:18.152846Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"0711.4644","last_updated":"2009-05-08T04:51:14Z","snapshot_observed_at":"2026-08-15T10:26:45.491812Z","submitted_at":"2007-11-29T02:48:55Z","title":"Verifying black hole orbits with gravitational spectroscopy","version":2},"cited_work":{"arxiv_id":"0711.4644","doi":null,"metadata_source":"pith","pith_arxiv_id":"0711.4644","snapshot_observed_at":"2026-08-12T21:08:18.955508Z","title":"Verifying black hole orbits with gravitational spectroscopy","venue":"gr-qc","work_id":"ce9d67d8-79cf-4a42-8645-d50eccf83996","year":2007},"citing_paper":{"arxiv_id":"2411.09147","last_updated":"2025-03-27T07:52:56Z","snapshot_observed_at":"2026-08-16T08:34:44.313485Z","submitted_at":"2024-11-14T02:57:25Z","title":"Post-Newtonian templates for phase evolution of spherical extreme mass ratio inspirals","version":3},"reference_index":13,"source":"pdf_text","source_observed_at":"2026-08-12T21:08:18.158773Z"},"links":{"cited_paper":"/paper/0711.4644","citing_paper":"/paper/2411.09147"},"observation_digest":"sha256:5a225f9229c00dfc1bf097ad39318505f15f6cbc278a2264235814ad21ce6302","observation_id":"8a42eb79-da4f-469d-9bad-3987513e2886","resolution":{"observed_at":"2026-08-12T21:08:18.961703Z","resolver_source":"local_arxiv","status":"verified_exact"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-18T06:34:40.430872+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-18T06:34:40.430872+00:00","source":"crossref"},{"observed_at":"2026-08-18T06:34:34.496301+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":{"arxiv_id":"0904.3810","last_updated":"2009-05-20T11:26:59Z","snapshot_observed_at":"2026-08-15T05:49:52.794516Z","submitted_at":"2009-04-24T07:27:26Z","title":"An Efficient Numerical Method for Computing Gravitational Waves Induced by a Particle Moving on Eccentric Inclined Orbits around a Kerr Black Hole","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"0904.3810","snapshot_observed_at":"2026-08-12T21:08:18.163959Z","title":"Fujita, W","venue":null,"work_id":null,"year":2009},"citing_paper":{"arxiv_id":"2411.09147","last_updated":"2025-03-27T07:52:56Z","snapshot_observed_at":"2026-08-16T08:34:44.313485Z","submitted_at":"2024-11-14T02:57:25Z","title":"Post-Newtonian templates for phase evolution of spherical extreme mass ratio inspirals","version":3},"reference_index":14,"source":"pdf_text","source_observed_at":"2026-08-12T21:08:18.163959Z"},"links":{"cited_paper":"/paper/0904.3810","citing_paper":"/paper/2411.09147"},"observation_digest":"sha256:9cff2add054e0c92f9dc647eac56b242c7d6b7853307fffa830292cf74c02655","observation_id":"747479e3-1074-473d-bf9d-aaa5113d3228","resolution":{"observed_at":"2026-08-12T21:08:18.163959Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2008.13554","last_updated":"2020-09-09T11:44:46Z","snapshot_observed_at":"2026-08-08T16:15:42.401454Z","submitted_at":"2020-08-31T12:39:01Z","title":"Extreme mass ratio inspirals on the equatorial plane in the adiabatic order","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2008.13554","snapshot_observed_at":"2026-08-12T21:08:18.169503Z","title":"Fujita and M","venue":null,"work_id":null,"year":2020},"citing_paper":{"arxiv_id":"2411.09147","last_updated":"2025-03-27T07:52:56Z","snapshot_observed_at":"2026-08-16T08:34:44.313485Z","submitted_at":"2024-11-14T02:57:25Z","title":"Post-Newtonian templates for phase evolution of spherical extreme mass ratio inspirals","version":3},"reference_index":15,"source":"pdf_text","source_observed_at":"2026-08-12T21:08:18.169503Z"},"links":{"cited_paper":"/paper/2008.13554","citing_paper":"/paper/2411.09147"},"observation_digest":"sha256:1e6031bb4d2e11b3b7dd8b876f287f37091bd283ac0249fe519778561eb6ba08","observation_id":"495e0cf3-a3d5-4820-b277-e4925162c9db","resolution":{"observed_at":"2026-08-12T21:08:18.169503Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"gr-qc/9712057","last_updated":"1997-12-12T09:46:08Z","snapshot_observed_at":"2026-08-14T20:10:53.581348Z","submitted_at":"1997-12-12T09:46:08Z","title":"Black Hole Perturbation","version":1},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"gr-qc/9712057","snapshot_observed_at":"2026-08-12T21:08:18.173731Z","title":null,"venue":null,"work_id":null,"year":1997},"citing_paper":{"arxiv_id":"2411.09147","last_updated":"2025-03-27T07:52:56Z","snapshot_observed_at":"2026-08-16T08:34:44.313485Z","submitted_at":"2024-11-14T02:57:25Z","title":"Post-Newtonian templates for phase evolution of spherical extreme mass ratio inspirals","version":3},"reference_index":16,"source":"pdf_text","source_observed_at":"2026-08-12T21:08:18.173731Z"},"links":{"cited_paper":"/paper/gr-qc/9712057","citing_paper":"/paper/2411.09147"},"observation_digest":"sha256:53879a91a72f65898275a64859205d81e6df739a16ad2a5023a680f6d69882a2","observation_id":"a4ccac19-c818-4c87-9136-554c72cb2807","resolution":{"observed_at":"2026-08-12T21:08:18.173731Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"gr-qc/0306120","last_updated":"2003-06-27T08:31:03Z","snapshot_observed_at":"2026-07-07T03:17:59.913247Z","submitted_at":"2003-06-27T08:31:03Z","title":"Analytic black hole perturbation approach to gravitational radiation","version":1},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"gr-qc/0306120","snapshot_observed_at":"2026-08-12T21:08:18.178043Z","title":"Sasaki and H","venue":null,"work_id":null,"year":2003},"citing_paper":{"arxiv_id":"2411.09147","last_updated":"2025-03-27T07:52:56Z","snapshot_observed_at":"2026-08-16T08:34:44.313485Z","submitted_at":"2024-11-14T02:57:25Z","title":"Post-Newtonian templates for phase evolution of spherical extreme mass ratio inspirals","version":3},"reference_index":17,"source":"pdf_text","source_observed_at":"2026-08-12T21:08:18.178043Z"},"links":{"cited_paper":"/paper/gr-qc/0306120","citing_paper":"/paper/2411.09147"},"observation_digest":"sha256:8be900f716d2802684a715e87a3c3655d88fed5c1acbf950bbf994cdffd7ca0f","observation_id":"4089afe0-b568-4832-adfe-089f7c22efeb","resolution":{"observed_at":"2026-08-12T21:08:18.178043Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"gr-qc/0511151","last_updated":"2005-11-29T08:48:26Z","snapshot_observed_at":"2026-07-07T03:21:48.708813Z","submitted_at":"2005-11-29T08:48:26Z","title":"The adiabatic evolution of orbital parameters in the Kerr spacetime","version":1},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"gr-qc/0511151","snapshot_observed_at":"2026-08-12T21:08:18.182418Z","title":null,"venue":null,"work_id":null,"year":2006},"citing_paper":{"arxiv_id":"2411.09147","last_updated":"2025-03-27T07:52:56Z","snapshot_observed_at":"2026-08-16T08:34:44.313485Z","submitted_at":"2024-11-14T02:57:25Z","title":"Post-Newtonian templates for phase evolution of spherical extreme mass ratio inspirals","version":3},"reference_index":18,"source":"pdf_text","source_observed_at":"2026-08-12T21:08:18.182418Z"},"links":{"cited_paper":"/paper/gr-qc/0511151","citing_paper":"/paper/2411.09147"},"observation_digest":"sha256:f21fd5845ce4f1e6cdae6ea56e3b9307b17698003d317c49ef52ee86e73d358d","observation_id":"e5adf186-b83c-4ee5-a694-1fcc75007409","resolution":{"observed_at":"2026-08-12T21:08:18.182418Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"gr-qc/0702054","last_updated":"2007-05-31T11:13:35Z","snapshot_observed_at":"2026-08-15T10:48:14.825867Z","submitted_at":"2007-02-09T01:33:24Z","title":"Adiabatic Evolution of three 'Constants' of Motion for Greatly Inclined Orbits in Kerr spacetime","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"gr-qc/0702054","snapshot_observed_at":"2026-08-12T21:08:18.186399Z","title":null,"venue":null,"work_id":null,"year":2007},"citing_paper":{"arxiv_id":"2411.09147","last_updated":"2025-03-27T07:52:56Z","snapshot_observed_at":"2026-08-16T08:34:44.313485Z","submitted_at":"2024-11-14T02:57:25Z","title":"Post-Newtonian templates for phase evolution of spherical extreme mass ratio inspirals","version":3},"reference_index":19,"source":"pdf_text","source_observed_at":"2026-08-12T21:08:18.186399Z"},"links":{"cited_paper":"/paper/gr-qc/0702054","citing_paper":"/paper/2411.09147"},"observation_digest":"sha256:7c940a4c29f8a1d58b668c9e23205067d07dfac5b94a9fb622a4d18c79297ba6","observation_id":"77472fa5-5238-48df-93f2-a2eaa55e1c77","resolution":{"observed_at":"2026-08-12T21:08:18.186399Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"1505.01600","last_updated":"2015-07-13T13:34:11Z","snapshot_observed_at":"2026-08-14T22:49:32.751610Z","submitted_at":"2015-05-07T06:22:20Z","title":"Calculation of radiation reaction effect on orbital parameters in Kerr spacetime","version":3},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"1505.01600","snapshot_observed_at":"2026-08-12T21:08:18.190503Z","title":"Sago and R","venue":null,"work_id":null,"year":2015},"citing_paper":{"arxiv_id":"2411.09147","last_updated":"2025-03-27T07:52:56Z","snapshot_observed_at":"2026-08-16T08:34:44.313485Z","submitted_at":"2024-11-14T02:57:25Z","title":"Post-Newtonian templates for phase evolution of spherical extreme mass ratio inspirals","version":3},"reference_index":20,"source":"pdf_text","source_observed_at":"2026-08-12T21:08:18.190503Z"},"links":{"cited_paper":"/paper/1505.01600","citing_paper":"/paper/2411.09147"},"observation_digest":"sha256:a5bdf2cac18d25e94834117bc43161c3fa90ef03bcc27880c93dacc4e667cfb1","observation_id":"39826f4d-a5a5-44b1-817f-6aae343e0ed2","resolution":{"observed_at":"2026-08-12T21:08:18.190503Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"1211.5535","last_updated":"2012-11-23T16:04:44Z","snapshot_observed_at":"2026-08-15T00:38:22.600035Z","submitted_at":"2012-11-23T16:04:44Z","title":"Gravitational Waves from a Particle in Circular Orbits around a Schwarzschild Black Hole to the 22nd Post-Newtonian Order","version":1},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"1211.5535","snapshot_observed_at":"2026-08-12T21:08:18.195019Z","title":"Fujita, Prog","venue":null,"work_id":null,"year":2012},"citing_paper":{"arxiv_id":"2411.09147","last_updated":"2025-03-27T07:52:56Z","snapshot_observed_at":"2026-08-16T08:34:44.313485Z","submitted_at":"2024-11-14T02:57:25Z","title":"Post-Newtonian templates for phase evolution of spherical extreme mass ratio inspirals","version":3},"reference_index":21,"source":"pdf_text","source_observed_at":"2026-08-12T21:08:18.195019Z"},"links":{"cited_paper":"/paper/1211.5535","citing_paper":"/paper/2411.09147"},"observation_digest":"sha256:a978693439051e0a0557a51629258745858a21e7e2596d4fe6aa76c11ba92664","observation_id":"1f83a069-46e8-43bf-b362-886e21af7b4a","resolution":{"observed_at":"2026-08-12T21:08:18.195019Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"1412.5689","last_updated":"2015-03-26T07:42:17Z","snapshot_observed_at":"2026-08-14T23:07:03.909295Z","submitted_at":"2014-12-18T00:30:03Z","title":"Gravitational Waves from a Particle in Circular Orbits around a Rotating Black Hole to the 11th Post-Newtonian Order","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"1412.5689","snapshot_observed_at":"2026-08-12T21:08:18.199307Z","title":"Fujita, PTEP 2015, 033E01 (2015), arXiv:1412.5689 [gr-qc]","venue":null,"work_id":null,"year":2015},"citing_paper":{"arxiv_id":"2411.09147","last_updated":"2025-03-27T07:52:56Z","snapshot_observed_at":"2026-08-16T08:34:44.313485Z","submitted_at":"2024-11-14T02:57:25Z","title":"Post-Newtonian templates for phase evolution of spherical extreme mass ratio inspirals","version":3},"reference_index":22,"source":"pdf_text","source_observed_at":"2026-08-12T21:08:18.199307Z"},"links":{"cited_paper":"/paper/1412.5689","citing_paper":"/paper/2411.09147"},"observation_digest":"sha256:b94a736fc181d8e203b65de7281228a94cf79e8e23c2f80485fb7cde2b2f1228","observation_id":"1be6f980-102c-4122-a44c-c3b807cccd88","resolution":{"observed_at":"2026-08-12T21:08:18.199307Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2008.10622","last_updated":"2020-08-24T18:00:22Z","snapshot_observed_at":"2026-08-15T17:56:26.922193Z","submitted_at":"2020-08-24T18:00:22Z","title":"Analytic post-Newtonian expansion of the energy and angular momentum radiated to infinity by eccentric-orbit non-spinning extreme-mass-ratio inspirals to 19PN","version":1},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2008.10622","snapshot_observed_at":"2026-08-12T21:08:18.204299Z","title":"Munna, Phys","venue":null,"work_id":null,"year":2020},"citing_paper":{"arxiv_id":"2411.09147","last_updated":"2025-03-27T07:52:56Z","snapshot_observed_at":"2026-08-16T08:34:44.313485Z","submitted_at":"2024-11-14T02:57:25Z","title":"Post-Newtonian templates for phase evolution of spherical extreme mass ratio inspirals","version":3},"reference_index":23,"source":"pdf_text","source_observed_at":"2026-08-12T21:08:18.204299Z"},"links":{"cited_paper":"/paper/2008.10622","citing_paper":"/paper/2411.09147"},"observation_digest":"sha256:1a8d92e30ecc99f5ed2d7f513dfa08c93e6f637c232cf69e4b829919208ca2e4","observation_id":"2eda6ae2-66e2-4e01-9a9e-3227cff3b8f8","resolution":{"observed_at":"2026-08-12T21:08:18.204299Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2005.03044","last_updated":"2020-05-06T18:00:13Z","snapshot_observed_at":"2026-08-09T19:49:52.940778Z","submitted_at":"2020-05-06T18:00:13Z","title":"Determination of new coefficients in the angular momentum and energy fluxes at infinity to 9PN for eccentric Schwarzschild extreme-mass-ratio inspirals using mode-by-mode fitting","version":1},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2005.03044","snapshot_observed_at":"2026-08-12T21:08:18.208978Z","title":"Munna, C","venue":null,"work_id":null,"year":2020},"citing_paper":{"arxiv_id":"2411.09147","last_updated":"2025-03-27T07:52:56Z","snapshot_observed_at":"2026-08-16T08:34:44.313485Z","submitted_at":"2024-11-14T02:57:25Z","title":"Post-Newtonian templates for phase evolution of spherical extreme mass ratio inspirals","version":3},"reference_index":24,"source":"pdf_text","source_observed_at":"2026-08-12T21:08:18.208978Z"},"links":{"cited_paper":"/paper/2005.03044","citing_paper":"/paper/2411.09147"},"observation_digest":"sha256:2c5d73ea93197b9d82f6bc27d4ac8a071f05829baff963073ef23dbf1d26ac16","observation_id":"72c24cdc-80b9-49a0-8436-9e99df043b36","resolution":{"observed_at":"2026-08-12T21:08:18.208978Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2306.12481","last_updated":"2023-06-21T18:00:04Z","snapshot_observed_at":"2026-08-16T15:22:08.914762Z","submitted_at":"2023-06-21T18:00:04Z","title":"Tidal heating and torquing of the primary black hole in eccentric-orbit, non-spinning extreme-mass-ratio inspirals to 22PN order","version":1},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2306.12481","snapshot_observed_at":"2026-08-12T21:08:18.213623Z","title":"Munna, C","venue":null,"work_id":null,"year":2023},"citing_paper":{"arxiv_id":"2411.09147","last_updated":"2025-03-27T07:52:56Z","snapshot_observed_at":"2026-08-16T08:34:44.313485Z","submitted_at":"2024-11-14T02:57:25Z","title":"Post-Newtonian templates for phase evolution of spherical extreme mass ratio inspirals","version":3},"reference_index":25,"source":"pdf_text","source_observed_at":"2026-08-12T21:08:18.213623Z"},"links":{"cited_paper":"/paper/2306.12481","citing_paper":"/paper/2411.09147"},"observation_digest":"sha256:0c3908db7055ac5ef04bd0dadb79726ea942652d51ee9c93b4bdeb6ae890eb10","observation_id":"ca9ff800-2260-4907-bf31-e99436259745","resolution":{"observed_at":"2026-08-12T21:08:18.213623Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"1503.02334","last_updated":"2021-05-05T10:04:25Z","snapshot_observed_at":"2026-08-16T00:19:24.990720Z","submitted_at":"2015-03-08T22:16:44Z","title":"Analytical high-order post-Newtonian expansions for extreme mass ratio binaries","version":3},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"1503.02334","snapshot_observed_at":"2026-08-12T21:08:18.218645Z","title":"Kavanagh, A","venue":null,"work_id":null,"year":2015},"citing_paper":{"arxiv_id":"2411.09147","last_updated":"2025-03-27T07:52:56Z","snapshot_observed_at":"2026-08-16T08:34:44.313485Z","submitted_at":"2024-11-14T02:57:25Z","title":"Post-Newtonian templates for phase evolution of spherical extreme mass ratio inspirals","version":3},"reference_index":26,"source":"pdf_text","source_observed_at":"2026-08-12T21:08:18.218645Z"},"links":{"cited_paper":"/paper/1503.02334","citing_paper":"/paper/2411.09147"},"observation_digest":"sha256:23a09670aac1d383acfdbf95deda8f9f7254cdd6cf8d72b57094157262f26b7d","observation_id":"737e136b-9eb6-400c-a5d9-52086b2d4797","resolution":{"observed_at":"2026-08-12T21:08:18.218645Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"1601.03394","last_updated":"2021-05-05T10:42:34Z","snapshot_observed_at":"2026-08-14T22:14:44.563309Z","submitted_at":"2016-01-13T21:00:00Z","title":"Analytical high-order post-Newtonian expansions for spinning extreme mass ratio binaries","version":4},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"1601.03394","snapshot_observed_at":"2026-08-12T21:08:18.225810Z","title":"Kavanagh, A","venue":null,"work_id":null,"year":2016},"citing_paper":{"arxiv_id":"2411.09147","last_updated":"2025-03-27T07:52:56Z","snapshot_observed_at":"2026-08-16T08:34:44.313485Z","submitted_at":"2024-11-14T02:57:25Z","title":"Post-Newtonian templates for phase evolution of spherical extreme mass ratio inspirals","version":3},"reference_index":27,"source":"pdf_text","source_observed_at":"2026-08-12T21:08:18.225810Z"},"links":{"cited_paper":"/paper/1601.03394","citing_paper":"/paper/2411.09147"},"observation_digest":"sha256:a3a4de6ff6700a9b7f33b1c05461e0c57d03dfa6a0367a26fd862ad064536161","observation_id":"8a0a713c-1aad-4cd7-8763-5eac80ae4be1","resolution":{"observed_at":"2026-08-12T21:08:18.225810Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2203.13832","last_updated":"2022-03-25T18:00:27Z","snapshot_observed_at":"2026-08-16T17:11:44.191239Z","submitted_at":"2022-03-25T18:00:27Z","title":"High-order post-Newtonian expansion of the redshift invariant for eccentric-orbit non-spinning extreme-mass-ratio inspirals","version":1},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2203.13832","snapshot_observed_at":"2026-08-12T21:08:18.231603Z","title":"Munna and C","venue":null,"work_id":null,"year":2022},"citing_paper":{"arxiv_id":"2411.09147","last_updated":"2025-03-27T07:52:56Z","snapshot_observed_at":"2026-08-16T08:34:44.313485Z","submitted_at":"2024-11-14T02:57:25Z","title":"Post-Newtonian templates for phase evolution of spherical extreme mass ratio inspirals","version":3},"reference_index":28,"source":"pdf_text","source_observed_at":"2026-08-12T21:08:18.231603Z"},"links":{"cited_paper":"/paper/2203.13832","citing_paper":"/paper/2411.09147"},"observation_digest":"sha256:2fd2a2eaaa6e7b3c9556dbdb6735cce4ced4af5c89ee7e0b7aa452d1b19aad76","observation_id":"b0b80c0d-f231-4b67-a87c-dcfc2b323eee","resolution":{"observed_at":"2026-08-12T21:08:18.231603Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2307.11158","last_updated":"2023-07-20T18:00:04Z","snapshot_observed_at":"2026-08-16T15:14:33.006130Z","submitted_at":"2023-07-20T18:00:04Z","title":"High-order post-Newtonian expansion of the generalized redshift invariant for eccentric-orbit, equatorial extreme-mass-ratio inspirals with a spinning primary","version":1},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2307.11158","snapshot_observed_at":"2026-08-12T21:08:18.236145Z","title":"Munna, Phys","venue":null,"work_id":null,"year":2023},"citing_paper":{"arxiv_id":"2411.09147","last_updated":"2025-03-27T07:52:56Z","snapshot_observed_at":"2026-08-16T08:34:44.313485Z","submitted_at":"2024-11-14T02:57:25Z","title":"Post-Newtonian templates for phase evolution of spherical extreme mass ratio inspirals","version":3},"reference_index":29,"source":"pdf_text","source_observed_at":"2026-08-12T21:08:18.236145Z"},"links":{"cited_paper":"/paper/2307.11158","citing_paper":"/paper/2411.09147"},"observation_digest":"sha256:b096a6e3726cb02f3fa715d149c86884acc17682a19084596f8237024ff8a2be","observation_id":"c213eb2a-8814-4774-bfa8-3e192d206300","resolution":{"observed_at":"2026-08-12T21:08:18.236145Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"gr-qc/9409054","last_updated":"1994-09-27T10:26:08Z","snapshot_observed_at":"2026-07-07T03:24:55.788627Z","submitted_at":"1994-09-27T10:26:08Z","title":"Gravitational Waves from a Particle Orbiting Around a Rotating Black Holes: Post-Newtonian Expansion","version":1},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"gr-qc/9409054","snapshot_observed_at":"2026-08-12T21:08:18.241194Z","title":"Shibata, M","venue":null,"work_id":null,"year":1995},"citing_paper":{"arxiv_id":"2411.09147","last_updated":"2025-03-27T07:52:56Z","snapshot_observed_at":"2026-08-16T08:34:44.313485Z","submitted_at":"2024-11-14T02:57:25Z","title":"Post-Newtonian templates for phase evolution of spherical extreme mass ratio inspirals","version":3},"reference_index":30,"source":"pdf_text","source_observed_at":"2026-08-12T21:08:18.241194Z"},"links":{"cited_paper":"/paper/gr-qc/9409054","citing_paper":"/paper/2411.09147"},"observation_digest":"sha256:e375de1b2e5b545867ea5c994047a105fca6cecb05e7b06c47fc1be1398b37f6","observation_id":"d753f9c4-8b9f-40e3-9492-d6aea52a30cb","resolution":{"observed_at":"2026-08-12T21:08:18.241194Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":"raw_reference","pith_arxiv_id":null,"snapshot_observed_at":"2026-08-12T21:08:19.086007Z","title":null,"venue":null,"work_id":"d18d42f6-d15b-44bc-9eac-7c43088b06e5","year":null},"citing_paper":{"arxiv_id":"2411.09147","last_updated":"2025-03-27T07:52:56Z","snapshot_observed_at":"2026-08-16T08:34:44.313485Z","submitted_at":"2024-11-14T02:57:25Z","title":"Post-Newtonian templates for phase evolution of spherical extreme mass ratio inspirals","version":3},"reference_index":31,"source":"pdf_text","source_observed_at":"2026-08-12T21:08:18.245736Z"},"links":{"citing_paper":"/paper/2411.09147"},"observation_digest":"sha256:325ac5cfc4f744db8579484dfe15860fc5915bb7533adba0c08bc5a5ab223426","observation_id":"bc38e6c4-416a-48e5-8c74-8ff26374e451","resolution":{"observed_at":"2026-08-12T21:08:19.090784Z","resolver_source":"raw_fallback","status":"unresolved"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-18T06:34:40.430872+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-18T06:34:40.430872+00:00","source":"crossref"},{"observed_at":"2026-08-18T06:34:34.496301+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":{"arxiv_id":"astro-ph/0703495","last_updated":"2007-07-14T13:40:14Z","snapshot_observed_at":"2026-08-15T10:44:26.940057Z","submitted_at":"2007-03-19T16:01:36Z","title":"Intermediate and Extreme Mass-Ratio Inspirals -- Astrophysics, Science Applications and Detection using LISA","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"astro-ph/0703495","snapshot_observed_at":"2026-08-12T21:08:18.252376Z","title":"Amaro-Seoane, J","venue":null,"work_id":null,"year":2007},"citing_paper":{"arxiv_id":"2411.09147","last_updated":"2025-03-27T07:52:56Z","snapshot_observed_at":"2026-08-16T08:34:44.313485Z","submitted_at":"2024-11-14T02:57:25Z","title":"Post-Newtonian templates for phase evolution of spherical extreme mass ratio inspirals","version":3},"reference_index":32,"source":"pdf_text","source_observed_at":"2026-08-12T21:08:18.252376Z"},"links":{"cited_paper":"/paper/astro-ph/0703495","citing_paper":"/paper/2411.09147"},"observation_digest":"sha256:ca2189ba3f2013cb52f48abaab751aab60313db2f139f32cad3079f084baa4cb","observation_id":"f88a527d-c871-48d5-9e73-040b33f1cb33","resolution":{"observed_at":"2026-08-12T21:08:18.252376Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"1410.0958","last_updated":"2014-10-03T20:00:01Z","snapshot_observed_at":"2026-08-14T23:17:02.317377Z","submitted_at":"2014-10-03T20:00:01Z","title":"Research Update on Extreme-Mass-Ratio Inspirals","version":1},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"1410.0958","snapshot_observed_at":"2026-08-12T21:08:18.257280Z","title":"Amaro-Seoane, J","venue":null,"work_id":null,"year":2015},"citing_paper":{"arxiv_id":"2411.09147","last_updated":"2025-03-27T07:52:56Z","snapshot_observed_at":"2026-08-16T08:34:44.313485Z","submitted_at":"2024-11-14T02:57:25Z","title":"Post-Newtonian templates for phase evolution of spherical extreme mass ratio inspirals","version":3},"reference_index":33,"source":"pdf_text","source_observed_at":"2026-08-12T21:08:18.257280Z"},"links":{"cited_paper":"/paper/1410.0958","citing_paper":"/paper/2411.09147"},"observation_digest":"sha256:e5db4ea7822d88b62ff82aa6990344992677df81801872804e265a4807d0d302","observation_id":"94f7875c-abfc-47fa-84ba-6399e072c2b7","resolution":{"observed_at":"2026-08-12T21:08:18.257280Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2411.09700","last_updated":"2025-03-31T21:04:49Z","snapshot_observed_at":"2026-08-17T00:47:37.991874Z","submitted_at":"2024-11-14T18:59:35Z","title":"Post-Newtonian expansion of gravitational energy and angular momentum fluxes: inclined spherical orbits about a Kerr black hole","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2411.09700","snapshot_observed_at":"2026-08-12T21:08:18.262035Z","title":null,"venue":null,"work_id":null,"year":2024},"citing_paper":{"arxiv_id":"2411.09147","last_updated":"2025-03-27T07:52:56Z","snapshot_observed_at":"2026-08-16T08:34:44.313485Z","submitted_at":"2024-11-14T02:57:25Z","title":"Post-Newtonian templates for phase evolution of spherical extreme mass ratio inspirals","version":3},"reference_index":34,"source":"pdf_text","source_observed_at":"2026-08-12T21:08:18.262035Z"},"links":{"cited_paper":"/paper/2411.09700","citing_paper":"/paper/2411.09147"},"observation_digest":"sha256:8627d28e2af7ae2d7675d1d818198309015d03b5ad2e53341a4e9115d45e5136","observation_id":"a35897fc-0207-419c-a919-653747ea6a75","resolution":{"observed_at":"2026-08-12T21:08:18.262035Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2305.10533","last_updated":"2024-06-04T08:43:29Z","snapshot_observed_at":"2026-08-16T15:32:13.097218Z","submitted_at":"2023-05-17T19:37:07Z","title":"Self-forced inspirals with spin-orbit precession","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2305.10533","snapshot_observed_at":"2026-08-12T21:08:18.268578Z","title":"Lynch, M","venue":null,"work_id":null,"year":2024},"citing_paper":{"arxiv_id":"2411.09147","last_updated":"2025-03-27T07:52:56Z","snapshot_observed_at":"2026-08-16T08:34:44.313485Z","submitted_at":"2024-11-14T02:57:25Z","title":"Post-Newtonian templates for phase evolution of spherical extreme mass ratio inspirals","version":3},"reference_index":35,"source":"pdf_text","source_observed_at":"2026-08-12T21:08:18.268578Z"},"links":{"cited_paper":"/paper/2305.10533","citing_paper":"/paper/2411.09147"},"observation_digest":"sha256:4856f09d8265d9a63bab840c7ffddfbe4d9c64af9003379a452f66fcf2be3f69","observation_id":"cc80397a-d23e-46f5-8fd8-ef68043be119","resolution":{"observed_at":"2026-08-12T21:08:18.268578Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"gr-qc/0010009","last_updated":"2005-06-17T05:36:56Z","snapshot_observed_at":"2026-08-03T08:38:51.308901Z","submitted_at":"2000-10-04T03:01:06Z","title":"A Comparison of search templates for gravitational waves from binary inspiral","version":4},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"gr-qc/0010009","snapshot_observed_at":"2026-08-12T21:08:18.273866Z","title":"Damour, B","venue":null,"work_id":null,"year":2001},"citing_paper":{"arxiv_id":"2411.09147","last_updated":"2025-03-27T07:52:56Z","snapshot_observed_at":"2026-08-16T08:34:44.313485Z","submitted_at":"2024-11-14T02:57:25Z","title":"Post-Newtonian templates for phase evolution of spherical extreme mass ratio inspirals","version":3},"reference_index":36,"source":"pdf_text","source_observed_at":"2026-08-12T21:08:18.273866Z"},"links":{"cited_paper":"/paper/gr-qc/0010009","citing_paper":"/paper/2411.09147"},"observation_digest":"sha256:2adcd80323cda5d8ccf46dd929cce8a5a746e5b1b2be6e5f72912aee9963631d","observation_id":"df05d248-066f-4a1c-8c46-1dc98afa45c3","resolution":{"observed_at":"2026-08-12T21:08:18.273866Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"0907.0700","last_updated":"2009-07-03T19:31:53Z","snapshot_observed_at":"2026-08-15T05:44:27.431525Z","submitted_at":"2009-07-03T19:31:53Z","title":"Comparison of post-Newtonian templates for compact binary inspiral signals in gravitational-wave detectors","version":1},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"0907.0700","snapshot_observed_at":"2026-08-12T21:08:18.278501Z","title":"Buonanno, B","venue":null,"work_id":null,"year":2009},"citing_paper":{"arxiv_id":"2411.09147","last_updated":"2025-03-27T07:52:56Z","snapshot_observed_at":"2026-08-16T08:34:44.313485Z","submitted_at":"2024-11-14T02:57:25Z","title":"Post-Newtonian templates for phase evolution of spherical extreme mass ratio inspirals","version":3},"reference_index":37,"source":"pdf_text","source_observed_at":"2026-08-12T21:08:18.278501Z"},"links":{"cited_paper":"/paper/0907.0700","citing_paper":"/paper/2411.09147"},"observation_digest":"sha256:0be27a574b55a291ea794f438f76a13dce37107962730f716e5818d4a4fedff9","observation_id":"462e55a0-711d-4993-a9a7-7c207c2dfdfd","resolution":{"observed_at":"2026-08-12T21:08:18.278501Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"1304.5675","last_updated":"2013-07-30T16:03:00Z","snapshot_observed_at":"2026-08-15T00:20:32.366754Z","submitted_at":"2013-04-20T23:04:47Z","title":"Comparison of post-Newtonian templates for extreme mass ratio inspirals","version":2},"cited_work":{"arxiv_id":"1304.5675","doi":null,"metadata_source":"pith","pith_arxiv_id":"1304.5675","snapshot_observed_at":"2026-08-12T21:08:18.635411Z","title":"Comparison of post-Newtonian templates for extreme mass ratio inspirals","venue":"gr-qc","work_id":"e251fd97-b0c1-4c34-b5c4-7cab0d8942df","year":2013},"citing_paper":{"arxiv_id":"2411.09147","last_updated":"2025-03-27T07:52:56Z","snapshot_observed_at":"2026-08-16T08:34:44.313485Z","submitted_at":"2024-11-14T02:57:25Z","title":"Post-Newtonian templates for phase evolution of spherical extreme mass ratio inspirals","version":3},"reference_index":38,"source":"pdf_text","source_observed_at":"2026-08-12T21:08:18.284122Z"},"links":{"cited_paper":"/paper/1304.5675","citing_paper":"/paper/2411.09147"},"observation_digest":"sha256:3a3cd21be9f32b36f02b6c296fd1e3387769917c721ae93347b5c25b512c6eb9","observation_id":"71378598-d321-4fc7-80d9-af594bdba01b","resolution":{"observed_at":"2026-08-12T21:08:18.640906Z","resolver_source":"local_arxiv","status":"verified_exact"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-18T06:34:40.430872+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-18T06:34:40.430872+00:00","source":"crossref"},{"observed_at":"2026-08-18T06:34:34.496301+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":{"arxiv_id":"0710.0158","last_updated":"2008-02-21T21:22:09Z","snapshot_observed_at":"2026-08-15T10:31:14.303639Z","submitted_at":"2007-09-30T17:28:58Z","title":"High-accuracy comparison of numerical relativity simulations with post-Newtonian expansions","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"0710.0158","snapshot_observed_at":"2026-08-12T21:08:18.290015Z","title":"Boyle, D","venue":null,"work_id":null,"year":2007},"citing_paper":{"arxiv_id":"2411.09147","last_updated":"2025-03-27T07:52:56Z","snapshot_observed_at":"2026-08-16T08:34:44.313485Z","submitted_at":"2024-11-14T02:57:25Z","title":"Post-Newtonian templates for phase evolution of spherical extreme mass ratio inspirals","version":3},"reference_index":39,"source":"pdf_text","source_observed_at":"2026-08-12T21:08:18.290015Z"},"links":{"cited_paper":"/paper/0710.0158","citing_paper":"/paper/2411.09147"},"observation_digest":"sha256:6ca64b9114bbc994d7e2723fecf57e50ca4a072ddd94b08236544f8c4a2ad348","observation_id":"5a81cbfe-23b4-40d2-b472-401ead6897ff","resolution":{"observed_at":"2026-08-12T21:08:18.290015Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"0805.2390","last_updated":"2008-05-30T18:22:13Z","snapshot_observed_at":"2026-08-15T10:15:18.916165Z","submitted_at":"2008-05-15T19:49:12Z","title":"Ineffectiveness of Pad\\'e resummation techniques in post-Newtonian approximations","version":3},"cited_work":{"arxiv_id":"0805.2390","doi":null,"metadata_source":"pith","pith_arxiv_id":"0805.2390","snapshot_observed_at":"2026-08-12T21:08:18.600575Z","title":"Ineffectiveness of Pad\\'e resummation techniques in post-Newtonian approximations","venue":"gr-qc","work_id":"8e6652e9-80ad-4f15-b6df-5aea1834909f","year":2008},"citing_paper":{"arxiv_id":"2411.09147","last_updated":"2025-03-27T07:52:56Z","snapshot_observed_at":"2026-08-16T08:34:44.313485Z","submitted_at":"2024-11-14T02:57:25Z","title":"Post-Newtonian templates for phase evolution of spherical extreme mass ratio inspirals","version":3},"reference_index":40,"source":"pdf_text","source_observed_at":"2026-08-12T21:08:18.296173Z"},"links":{"cited_paper":"/paper/0805.2390","citing_paper":"/paper/2411.09147"},"observation_digest":"sha256:b1b8bc07e07c900b10f8e8fb97d30d7f9db8f225e6f805115a4a2893118086a4","observation_id":"31b7fb85-3485-4879-9599-bf7d63610c2d","resolution":{"observed_at":"2026-08-12T21:08:18.605150Z","resolver_source":"local_arxiv","status":"verified_exact"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-18T06:34:40.430872+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-18T06:34:40.430872+00:00","source":"crossref"},{"observed_at":"2026-08-18T06:34:34.496301+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":{"arxiv_id":"gr-qc/9710129","last_updated":"1997-10-30T18:14:35Z","snapshot_observed_at":"2026-08-06T21:15:39.586108Z","submitted_at":"1997-10-30T18:14:35Z","title":"Measuring gravitational waves from binary black hole coalescences: II. the waves' information and its extraction, with and without templates","version":1},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"gr-qc/9710129","snapshot_observed_at":"2026-08-12T21:08:18.301198Z","title":null,"venue":null,"work_id":null,"year":1998},"citing_paper":{"arxiv_id":"2411.09147","last_updated":"2025-03-27T07:52:56Z","snapshot_observed_at":"2026-08-16T08:34:44.313485Z","submitted_at":"2024-11-14T02:57:25Z","title":"Post-Newtonian templates for phase evolution of spherical extreme mass ratio inspirals","version":3},"reference_index":41,"source":"pdf_text","source_observed_at":"2026-08-12T21:08:18.301198Z"},"links":{"cited_paper":"/paper/gr-qc/9710129","citing_paper":"/paper/2411.09147"},"observation_digest":"sha256:f4e4cee9120a61e946041c3afbf12554f2926c9a5d2cca83f7a50bd217c16d57","observation_id":"cc406892-12ba-4983-943b-ae3ead476e3d","resolution":{"observed_at":"2026-08-12T21:08:18.301198Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"0809.3844","last_updated":"2008-11-05T17:07:03Z","snapshot_observed_at":"2026-08-15T10:06:18.907979Z","submitted_at":"2008-09-23T03:35:04Z","title":"Model Waveform Accuracy Standards for Gravitational Wave Data Analysis","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"0809.3844","snapshot_observed_at":"2026-08-12T21:08:18.305889Z","title":"Lindblom, B","venue":null,"work_id":null,"year":2008},"citing_paper":{"arxiv_id":"2411.09147","last_updated":"2025-03-27T07:52:56Z","snapshot_observed_at":"2026-08-16T08:34:44.313485Z","submitted_at":"2024-11-14T02:57:25Z","title":"Post-Newtonian templates for phase evolution of spherical extreme mass ratio inspirals","version":3},"reference_index":42,"source":"pdf_text","source_observed_at":"2026-08-12T21:08:18.305889Z"},"links":{"cited_paper":"/paper/0809.3844","citing_paper":"/paper/2411.09147"},"observation_digest":"sha256:855a984a15571ed76d7176a876a8cbcb754b16257affe35a3c39d208ff29e177","observation_id":"de89cca9-5254-464d-b062-f40f948eaa76","resolution":{"observed_at":"2026-08-12T21:08:18.305889Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2106.07195","last_updated":"2021-11-10T17:08:16Z","snapshot_observed_at":"2026-08-17T01:47:44.716541Z","submitted_at":"2021-06-14T06:58:02Z","title":"Extreme mass-ratio inspirals around a spinning horizonless compact object","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2106.07195","snapshot_observed_at":"2026-08-12T21:08:18.310609Z","title":"Maggio, M","venue":null,"work_id":null,"year":2021},"citing_paper":{"arxiv_id":"2411.09147","last_updated":"2025-03-27T07:52:56Z","snapshot_observed_at":"2026-08-16T08:34:44.313485Z","submitted_at":"2024-11-14T02:57:25Z","title":"Post-Newtonian templates for phase evolution of spherical extreme mass ratio inspirals","version":3},"reference_index":43,"source":"pdf_text","source_observed_at":"2026-08-12T21:08:18.310609Z"},"links":{"cited_paper":"/paper/2106.07195","citing_paper":"/paper/2411.09147"},"observation_digest":"sha256:534a3b461c559fd4f35fffbc039bb481078e85c57a03dcd37b5fd0cb84e9d3ae","observation_id":"0f077490-8e3a-45b2-91b9-00ef266729de","resolution":{"observed_at":"2026-08-12T21:08:18.310609Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"gr-qc/9708034","last_updated":"1997-08-18T08:52:17Z","snapshot_observed_at":"2026-08-18T12:08:30.514751Z","submitted_at":"1997-08-18T08:52:17Z","title":"Improved filters for gravitational waves from inspiralling compact binaries","version":1},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"gr-qc/9708034","snapshot_observed_at":"2026-08-12T21:08:18.315394Z","title":"Damour, B","venue":null,"work_id":null,"year":1998},"citing_paper":{"arxiv_id":"2411.09147","last_updated":"2025-03-27T07:52:56Z","snapshot_observed_at":"2026-08-16T08:34:44.313485Z","submitted_at":"2024-11-14T02:57:25Z","title":"Post-Newtonian templates for phase evolution of spherical extreme mass ratio inspirals","version":3},"reference_index":44,"source":"pdf_text","source_observed_at":"2026-08-12T21:08:18.315394Z"},"links":{"cited_paper":"/paper/gr-qc/9708034","citing_paper":"/paper/2411.09147"},"observation_digest":"sha256:3d40f6944f2a964ddba8342b194c3908ba8f14d29794d027b953fb063976c878","observation_id":"50146948-8125-4164-9e6b-fe6dbe2a4010","resolution":{"observed_at":"2026-08-12T21:08:18.315394Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"0811.2069","last_updated":"2009-03-11T13:55:12Z","snapshot_observed_at":"2026-08-15T10:02:08.006230Z","submitted_at":"2008-11-13T11:33:11Z","title":"Improved resummation of post-Newtonian multipolar waveforms from circularized compact binaries","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"0811.2069","snapshot_observed_at":"2026-08-12T21:08:18.320634Z","title":"Damour, B","venue":null,"work_id":null,"year":2009},"citing_paper":{"arxiv_id":"2411.09147","last_updated":"2025-03-27T07:52:56Z","snapshot_observed_at":"2026-08-16T08:34:44.313485Z","submitted_at":"2024-11-14T02:57:25Z","title":"Post-Newtonian templates for phase evolution of spherical extreme mass ratio inspirals","version":3},"reference_index":45,"source":"pdf_text","source_observed_at":"2026-08-12T21:08:18.320634Z"},"links":{"cited_paper":"/paper/0811.2069","citing_paper":"/paper/2411.09147"},"observation_digest":"sha256:f9e80b2d4c44a283d1a17851a9cf87968385cc0b83b1546bddab713fd05ba758","observation_id":"d0dd51e7-6714-4254-9f2b-88ade230a061","resolution":{"observed_at":"2026-08-12T21:08:18.320634Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"1803.01944","last_updated":"2018-10-15T16:27:32Z","snapshot_observed_at":"2026-08-14T19:39:16.581930Z","submitted_at":"2018-03-05T21:56:12Z","title":"The construction and use of LISA sensitivity curves","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"1803.01944","snapshot_observed_at":"2026-08-12T21:08:18.324995Z","title":"Robson, N","venue":null,"work_id":null,"year":2019},"citing_paper":{"arxiv_id":"2411.09147","last_updated":"2025-03-27T07:52:56Z","snapshot_observed_at":"2026-08-16T08:34:44.313485Z","submitted_at":"2024-11-14T02:57:25Z","title":"Post-Newtonian templates for phase evolution of spherical extreme mass ratio inspirals","version":3},"reference_index":46,"source":"pdf_text","source_observed_at":"2026-08-12T21:08:18.324995Z"},"links":{"cited_paper":"/paper/1803.01944","citing_paper":"/paper/2411.09147"},"observation_digest":"sha256:e11e1c9a3ba333ce4f623eeaf7fb18b3afe9650a7e6f67ca6ac5cc706f3db2d0","observation_id":"3cc3a6c8-8511-476d-bd9a-0d80eb06ffe2","resolution":{"observed_at":"2026-08-12T21:08:18.324995Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2107.07258","last_updated":"2023-02-15T10:52:01Z","snapshot_observed_at":"2026-08-16T18:09:50.571296Z","submitted_at":"2021-07-15T11:29:01Z","title":"Probing horizon scale quantum effects with Love","version":3},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2107.07258","snapshot_observed_at":"2026-08-12T21:08:18.329171Z","title":"Datta, Class","venue":null,"work_id":null,"year":2022},"citing_paper":{"arxiv_id":"2411.09147","last_updated":"2025-03-27T07:52:56Z","snapshot_observed_at":"2026-08-16T08:34:44.313485Z","submitted_at":"2024-11-14T02:57:25Z","title":"Post-Newtonian templates for phase evolution of spherical extreme mass ratio inspirals","version":3},"reference_index":47,"source":"pdf_text","source_observed_at":"2026-08-12T21:08:18.329171Z"},"links":{"cited_paper":"/paper/2107.07258","citing_paper":"/paper/2411.09147"},"observation_digest":"sha256:49176037cf204b2bf181ca059d2c608b27b2265864b350b7946d26f0b8d72331","observation_id":"3ba55963-9977-493d-8a6f-03af585e1565","resolution":{"observed_at":"2026-08-12T21:08:18.329171Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"0705.2519","last_updated":"2007-07-26T15:33:55Z","snapshot_observed_at":"2026-08-17T15:55:39.723887Z","submitted_at":"2007-05-17T11:47:54Z","title":"Faithful Effective-One-Body waveforms of small-mass-ratio coalescing black-hole binaries","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"0705.2519","snapshot_observed_at":"2026-08-12T21:08:18.333973Z","title":"Damour and A","venue":null,"work_id":null,"year":2007},"citing_paper":{"arxiv_id":"2411.09147","last_updated":"2025-03-27T07:52:56Z","snapshot_observed_at":"2026-08-16T08:34:44.313485Z","submitted_at":"2024-11-14T02:57:25Z","title":"Post-Newtonian templates for phase evolution of spherical extreme mass ratio inspirals","version":3},"reference_index":48,"source":"pdf_text","source_observed_at":"2026-08-12T21:08:18.333973Z"},"links":{"cited_paper":"/paper/0705.2519","citing_paper":"/paper/2411.09147"},"observation_digest":"sha256:a0704e94a24792ec09e6bedb7a2740895791cbdc11c94fa29302c8e938fe3974","observation_id":"9180b938-0ce5-4cc8-9710-918844e2f857","resolution":{"observed_at":"2026-08-12T21:08:18.333973Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"0711.2628","last_updated":"2007-12-19T16:24:40Z","snapshot_observed_at":"2026-08-15T10:27:35.112108Z","submitted_at":"2007-11-16T15:00:01Z","title":"Comparing Effective-One-Body gravitational waveforms to accurate numerical data","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"0711.2628","snapshot_observed_at":"2026-08-12T21:08:18.338345Z","title":"Damour and A","venue":null,"work_id":null,"year":2008},"citing_paper":{"arxiv_id":"2411.09147","last_updated":"2025-03-27T07:52:56Z","snapshot_observed_at":"2026-08-16T08:34:44.313485Z","submitted_at":"2024-11-14T02:57:25Z","title":"Post-Newtonian templates for phase evolution of spherical extreme mass ratio inspirals","version":3},"reference_index":49,"source":"pdf_text","source_observed_at":"2026-08-12T21:08:18.338345Z"},"links":{"cited_paper":"/paper/0711.2628","citing_paper":"/paper/2411.09147"},"observation_digest":"sha256:82286cdb577747708b70408d918796d1bbf69c296cadb23a9e41a2a1f4f5a18b","observation_id":"4dae310a-93d7-45d4-ac7b-bafe330749b5","resolution":{"observed_at":"2026-08-12T21:08:18.338345Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"1006.0431","last_updated":"2013-05-09T03:35:10Z","snapshot_observed_at":"2026-08-15T05:17:30.621873Z","submitted_at":"2010-06-02T16:01:38Z","title":"Post-Newtonian factorized multipolar waveforms for spinning, non-precessing black-hole binaries","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"1006.0431","snapshot_observed_at":"2026-08-12T21:08:18.344431Z","title":null,"venue":null,"work_id":null,"year":2011},"citing_paper":{"arxiv_id":"2411.09147","last_updated":"2025-03-27T07:52:56Z","snapshot_observed_at":"2026-08-16T08:34:44.313485Z","submitted_at":"2024-11-14T02:57:25Z","title":"Post-Newtonian templates for phase evolution of spherical extreme mass ratio inspirals","version":3},"reference_index":50,"source":"pdf_text","source_observed_at":"2026-08-12T21:08:18.344431Z"},"links":{"cited_paper":"/paper/1006.0431","citing_paper":"/paper/2411.09147"},"observation_digest":"sha256:99d5241a5e91e93ad96d524f5ff580bc471155c151f9812103ef73654a6e6c2c","observation_id":"e50fc89b-de62-4847-a930-44692cde7e5b","resolution":{"observed_at":"2026-08-12T21:08:18.344431Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"1210.2569","last_updated":"2013-01-08T20:09:54Z","snapshot_observed_at":"2026-08-15T00:43:48.372980Z","submitted_at":"2012-10-09T11:39:16Z","title":"Impact of the second order self-forces on the dephasing of the gravitational waves from quasi-circular extreme mass-ratio inspirals","version":2},"cited_work":{"arxiv_id":"1210.2569","doi":null,"metadata_source":"pith","pith_arxiv_id":"1210.2569","snapshot_observed_at":"2026-08-12T21:08:18.404279Z","title":"Impact of the second order self-forces on the dephasing of the gravitational waves from quasi-circular extreme mass-ratio inspirals","venue":"gr-qc","work_id":"975f73ee-f39e-4af1-a246-94ceb6f48813","year":2012},"citing_paper":{"arxiv_id":"2411.09147","last_updated":"2025-03-27T07:52:56Z","snapshot_observed_at":"2026-08-16T08:34:44.313485Z","submitted_at":"2024-11-14T02:57:25Z","title":"Post-Newtonian templates for phase evolution of spherical extreme mass ratio inspirals","version":3},"reference_index":51,"source":"pdf_text","source_observed_at":"2026-08-12T21:08:18.352538Z"},"links":{"cited_paper":"/paper/1210.2569","citing_paper":"/paper/2411.09147"},"observation_digest":"sha256:8ff9b5f5f12478c74a154d00631b13a9ae652e6f9cd09d985b12d24846c252b5","observation_id":"c63670cf-9a2f-438b-934b-02dafdb516d2","resolution":{"observed_at":"2026-08-12T21:08:18.411400Z","resolver_source":"local_arxiv","status":"verified_exact"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-18T06:34:40.430872+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-18T06:34:40.430872+00:00","source":"crossref"},{"observed_at":"2026-08-18T06:34:34.496301+00:00","source":"retraction_watch"}],"state":"measured"}}],"paper":{"arxiv_id":"2411.09147","last_updated":"2025-03-27T07:52:56Z","latest_version":3,"primary_category":"gr-qc","snapshot_observed_at":"2026-08-16T08:34:44.313485Z","submitted_at":"2024-11-14T02:57:25Z","title":"Post-Newtonian templates for phase evolution of spherical extreme mass ratio inspirals"},"reference_resolution":{"displayed":51,"state_counts":{"malformed_identifier":0,"metadata_mismatch":0,"parse_uncertain":0,"unresolved":45,"verified_exact":5,"verified_fuzzy":1},"total_outbound_references":51},"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":"2026-08-18T06:34:40.430872+00:00","source":"crossref"},{"observed_at":"2026-08-18T06:34:34.496301+00:00","source":"retraction_watch"}],"thesis":"As of 18 August 2026, this Paper Citation Record lists 51 of 51 outbound references and 5 inbound Pith citation observations for arXiv:2411.09147."}