{"as_of":"2026-08-13T11:32:00Z","caps":{"database_statements":6,"inbound":100,"outbound":100},"context_digest":"sha256:110ca54baa01e2814c8bc2a41442654f859c551f82c50c99190a58ac0ed55a0f","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":"2026-08-13T06:32:02.005865+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":"2026-08-13T09:34:27.936588Z","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":"2026-08-13T09:34:11.410088Z","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":"sha256:9ed86fa4d52f5c48098cd5daf07d328114957a5e0de676c4a5fcc949c10c51f3","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":"2026-08-13T09:34:27.936588Z","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":"2026-08-07T18:33:21.469015Z","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":"sha256:59495b03443ac1a05401032a8f0d5dd7e0d9501a613a44f667f347021865e1b7","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":"2026-08-13T09:34:27.936588Z","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":"2026-08-11T01:19:49.482282Z","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:f9ee538948d345187a4a3aa41dd030c40ed340c5265063e160c261d3d08973f3","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 2026-08-13T06:32:02.005865+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-13T06:32:02.005865+00:00","source":"crossref"},{"observed_at":"2026-08-13T06:31:53.387327+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":{"arxiv_id":"2411.09147","last_updated":"2025-03-27T07:52:56Z","snapshot_observed_at":"2026-08-13T09:34:27.936588Z","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":"2026-08-11T01:19:49.482282Z","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":"sha256:3ce6794f7b09175ddd5d467d0d34c7fe92ee44df9b4b05de2e9f9a59d122ab22","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 2026-08-13T06:32:02.005865+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-13T06:32:02.005865+00:00","source":"crossref"},{"observed_at":"2026-08-13T06:31:53.387327+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":{"arxiv_id":"2411.09147","last_updated":"2025-03-27T07:52:56Z","snapshot_observed_at":"2026-08-13T09:34:27.936588Z","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":"2026-08-11T01:19:49.482282Z","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":"sha256:713c0e86cf65943872f457deacdd3f801656454af9b1a3c0d820a7a50139172c","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 2026-08-13T06:32:02.005865+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-13T06:32:02.005865+00:00","source":"crossref"},{"observed_at":"2026-08-13T06:31:53.387327+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":"2026-08-11T09:09:15.127132Z","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":"2026-08-13T09:34:27.936588Z","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":"sha256:619ba545fc4b0ba5e1be4085e362ca567cdcd42b1b1a31ca6a46242ed138dde0","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":"2026-08-05T11:59:29.671184Z","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":"2026-08-13T09:34:27.936588Z","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":"sha256:95827111efa17782d42fa75b925ec208d1a57189476d466c3adc82d5b15b7d49","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":"2026-08-06T11:30:25.358997Z","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":"2026-08-13T09:34:27.936588Z","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":"sha256:3bd892eb5155ae58349293b237b53d454736da32a1592d7fffe0248287954fdb","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":"2026-07-06T02:05:54.432258Z","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":"2026-08-13T09:34:27.936588Z","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:f55927d782461db0b539bf6e16f5c8e2bcb5d067f1417ba073919e48d7c30ef6","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 2026-08-13T06:32:02.005865+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-13T06:32:02.005865+00:00","source":"crossref"},{"observed_at":"2026-08-13T06:31:53.387327+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":{"arxiv_id":"1703.09722","last_updated":"2018-04-11T11:52:26Z","snapshot_observed_at":"2026-07-06T02:11:23.670680Z","submitted_at":"2017-03-28T18:00:17Z","title":"Science with the space-based interferometer LISA. V: Extreme mass-ratio inspirals","version":2},"cited_work":{"arxiv_id":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":"2026-08-13T09:34:27.936588Z","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:a7cb5a5470130b74de44e30f39a5a197b54c69b6b3b092b00f4a8be97a4354bb","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":"2026-08-02T20:50:24.339978Z","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":"2026-08-13T09:34:27.936588Z","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:af886524173c41399dd414099994b92806d41c9374e39ef42749b04f698fd56d","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":"2026-08-13T09:34:27.936588Z","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":"sha256:11066f67b1fc1e543bca94603fa4fca0ccf52be4b89e4eafcdb63fd2ebbe7604","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":"2026-08-13T09:34:27.936588Z","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":"sha256:587bad6e8b274201221b5ebf24532982fc89649a17155846befde66d049e3fd9","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":"2026-08-13T09:34:27.936588Z","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":"sha256:9ba46cfd5342680bc477e4ece4d9129f86fbf6efb98806a285d9b831b21c168f","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":"2026-08-10T10:20:37.277758Z","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":"2026-08-13T09:34:27.936588Z","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:be534218695459ba9be91299a41ad3c113e778c2284a4b00580b2d1cc2b0f139","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":"2026-08-13T09:34:27.936588Z","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:ca6de1240e890d942afc314195123b22653b2e5034863f80101e2c249cd92e63","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 2026-08-13T06:32:02.005865+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-13T06:32:02.005865+00:00","source":"crossref"},{"observed_at":"2026-08-13T06:31:53.387327+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":"2026-08-13T09:34:27.936588Z","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:cc698a6e0df8f5c987afa7e93d306dc8e0f98bba73898e1b34607cbb5941de27","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":"2026-07-06T01:31:43.159471Z","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":"2026-08-13T09:34:27.936588Z","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":"sha256:251c0640b4a6b12f3329e8a8817a032ac667c2dc7fd92c7c7d6f54b857236360","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 2026-08-13T06:32:02.005865+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-13T06:32:02.005865+00:00","source":"crossref"},{"observed_at":"2026-08-13T06:31:53.387327+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":{"arxiv_id":"0904.3810","last_updated":"2009-05-20T11:26:59Z","snapshot_observed_at":"2026-07-06T01:53:55.408125Z","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":"2026-08-13T09:34:27.936588Z","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:edad4539528a646ae0d8c483c11cec986f4224321916b227aa8299b8598eb602","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":"2026-08-13T09:34:27.936588Z","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":"sha256:4170f1578f64e0fae66bfc8c49a86423c2754b86e6ce67aa5add8066d23faa20","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":"2026-07-07T03:28:23.418344Z","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":"2026-08-13T09:34:27.936588Z","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":"sha256:75456f5052f7a3c27aab74ad4bc7c62bfff57dbe495270b1baee47f58f9a1b51","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":"2026-08-13T09:34:27.936588Z","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:bb4ab6806acdc2934ffaf15e341fba71d48a451ebc00f767f53272080a535fda","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":"2026-08-13T09:34:27.936588Z","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":"sha256:44958ef7a6f3a109d6b7a5c15b9969d64cec65828846bf3ecb8a3a780c235296","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":"2026-07-07T03:23:45.063198Z","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":"2026-08-13T09:34:27.936588Z","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":"sha256:5aa3035d9641785ab0791b28e63f85101c826941b45345c1bd8793d226e7dbd9","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":"2026-08-10T08:54:09.125820Z","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":"2026-08-13T09:34:27.936588Z","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:beb6a99e48107b896c054f9dd1fe625f8dedc3698505183ae3bfa6cf4700398d","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":"2026-08-09T11:03:26.998913Z","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":"2026-08-13T09:34:27.936588Z","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:fcdad4574a61871323655081ab05902e8e3fcba18b46aa8e812ebaaf5bf120e1","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":"2026-08-09T00:21:39.566923Z","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":"2026-08-13T09:34:27.936588Z","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":"sha256:36829942818314e53ac3ccbeb299cad3490606ffc91b1e49ae0360ffc39f8681","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":"2026-08-13T03:19:46.623577Z","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":"2026-08-13T09:34:27.936588Z","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":"sha256:4465ce84deb7bdd2439182badb1b1f3c4cfecd4aeeba54f134145f8ab3daafea","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":"2026-08-13T09:34:27.936588Z","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:fdeba0b8e110f383c72f88487e48fb1dcdf6a6408fa15946ea9f0ff0988046fe","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":"2026-08-13T11:12:25.600104Z","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":"2026-08-13T09:34:27.936588Z","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:c8def4b52031d01055c1ab9221f73604f475731df567231e2cd5aab191553e14","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":"2026-08-13T02:18:46.388810Z","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":"2026-08-13T09:34:27.936588Z","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":"sha256:5d4139a71cb3c5bd425138e5131699606d3eee9ee95ba25a6d41de6eee5005f4","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":"2026-08-12T18:48:46.893620Z","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":"2026-08-13T09:34:27.936588Z","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:b388fb1b46faf755cb2058ffa1efe74ff2e45e7240a5bea5fbc473df742d3b61","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":"2026-08-11T10:42:53.701150Z","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":"2026-08-13T09:34:27.936588Z","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":"sha256:6d8d782ef857bd234b3ebb57161e0137cd7fa85d4ebde229915c739707674278","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":"2026-08-13T10:50:55.844913Z","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":"2026-08-13T09:34:27.936588Z","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:c596569e4e97b48659ebd9333fe13aac4fea8594dc513997d71e99cacb7879db","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":"2026-08-13T09:34:27.936588Z","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:ed7c9786925771b6515b941d11f74394b0dfc69b954ad3e2a9f5e1929044f2ab","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":"2026-08-13T09:34:27.936588Z","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":"sha256:09d41cd91f01294761760c8bb0a5f176f533be40411672d32cd0fef97b4f0cf0","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 2026-08-13T06:32:02.005865+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-13T06:32:02.005865+00:00","source":"crossref"},{"observed_at":"2026-08-13T06:31:53.387327+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":"2026-07-06T02:11:23.670680Z","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":"2026-08-13T09:34:27.936588Z","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:bc107232d6a222b69468fae1e68527f79f2be6c0477ee55080b319278348f1fc","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":"2026-07-06T03:56:22.766353Z","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":"2026-08-13T09:34:27.936588Z","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:a056d29e4a19177c1dc12555222c16124fbc4de3a8c7c57b7e4ffa4cd209ad42","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":"2026-08-13T09:34:11.410088Z","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":"2026-08-13T09:34:27.936588Z","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":"sha256:57a05988b5e21cc09f9c5bc203810e2ee8574da994240d60fed30943409d0d30","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":"2026-08-09T22:10:38.808050Z","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":"2026-08-13T09:34:27.936588Z","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":"sha256:9b8f70c0a515a4a650d91b6d26968d2ea30b66ca823cb2e0744debf0d4377b6b","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":"2026-08-13T09:34:27.936588Z","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:fe2cb4fef9b360d3ebaa464663dd6aa6448a75340913e7c180af0516c180c8e9","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":"2026-08-12T19:16:18.975117Z","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":"2026-08-13T09:34:27.936588Z","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:b57cc259cc12398fa23b7da21a9d25051555c2df0a9e1f3a4345825c7e7b572e","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":"2026-07-06T03:11:38.072107Z","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":"2026-08-13T09:34:27.936588Z","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:a9dbf25c4ba95adf237af3e2027d071e7059f096b131dd6f3f55699858f67d7c","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 2026-08-13T06:32:02.005865+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-13T06:32:02.005865+00:00","source":"crossref"},{"observed_at":"2026-08-13T06:31:53.387327+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":{"arxiv_id":"0710.0158","last_updated":"2008-02-21T21:22:09Z","snapshot_observed_at":"2026-08-12T19:16:25.714057Z","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":"2026-08-13T09:34:27.936588Z","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":"sha256:8ecdeffc9bac4106ecb8e42c965a37aea75f159a8795ea63b813cf628c9ba483","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":"2026-07-06T01:41:41.454496Z","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":"2026-08-13T09:34:27.936588Z","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:c39a0b2fb9cdef96aa0c43f0099ad0242bc876b32a809e88f047ccd607eea3fe","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 2026-08-13T06:32:02.005865+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-13T06:32:02.005865+00:00","source":"crossref"},{"observed_at":"2026-08-13T06:31:53.387327+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":"2026-08-13T09:34:27.936588Z","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:a710b3ad03cb15d6ca098cd9f4f6d1bd3d44ed224820d205e1917c18b07ab6a9","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":"2026-08-12T22:04:15.771387Z","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":"2026-08-13T09:34:27.936588Z","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:d1fe33fb0f15dd1b21396f5fbad63a24fbf66d7044b8bd585e667323c23e0b0d","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":"2026-07-06T11:18:53.721387Z","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":"2026-08-13T09:34:27.936588Z","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:daeb5ac1b1446b1a9df3482164bc6c359e81edcf7006207718a4d5372bca6e37","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":"2026-08-02T22:50:20.643289Z","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":"2026-08-13T09:34:27.936588Z","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":"sha256:564d58cafcbbcd2fb57e11d36ba38c6a8f3de74a6d8c6fbc5bdb622b50c24f6c","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":"2026-07-06T01:50:52.457111Z","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":"2026-08-13T09:34:27.936588Z","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:e815fb0eb2ad9d8de3b95a1db81d63fb81f1f4114a87cf2741017f706ae50a15","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":"2026-07-06T02:11:23.670680Z","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":"2026-08-13T09:34:27.936588Z","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":"sha256:3c0551fa9a56003e68afdab29675dea2bb4a296bbfdcdc83891a5e9111f0b5d8","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":"2026-08-10T13:39:08.330888Z","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":"2026-08-13T09:34:27.936588Z","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":"sha256:29085d860cdd85884a1f117b82150f6ee6ba45a45736c0e62b9b53105e54e6f5","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":"2026-08-07T20:37:30.926743Z","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":"2026-08-13T09:34:27.936588Z","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":"sha256:4979f28cf885ccf43403dec78c42dac2457f94d5b56115c0288c06a490ec92a3","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":"2026-07-06T01:31:39.105519Z","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":"2026-08-13T09:34:27.936588Z","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":"sha256:1dfbbd5c1be219e9eb0cd01eefaa84b19eab52073c44497d33ab2c908b2c7096","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":"2026-08-01T19:05:14.813040Z","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":"2026-08-13T09:34:27.936588Z","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:ffa3dbae02ccb4b1d328af565669eaccb8540b96a8ef7d5680c9fc8b6290b2ab","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":"2026-07-06T02:57:16.492138Z","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":"2026-08-13T09:34:27.936588Z","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":"sha256:800abde43291ac9b6a936eca8c5f18aa6c10bb326a667dbd958b60860e9cfef3","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 2026-08-13T06:32:02.005865+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-13T06:32:02.005865+00:00","source":"crossref"},{"observed_at":"2026-08-13T06:31:53.387327+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":"2026-08-13T09:34:27.936588Z","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":"2026-08-13T06:32:02.005865+00:00","source":"crossref"},{"observed_at":"2026-08-13T06:31:53.387327+00:00","source":"retraction_watch"}],"thesis":"As of 13 August 2026, this Paper Citation Record lists 51 of 51 outbound references and 5 inbound Pith citation observations for arXiv:2411.09147."}