{"as_of":"2026-08-09T10:31:00Z","caps":{"database_statements":6,"inbound":100,"outbound":100},"context_digest":"sha256:a9091e74f7173f75b00b762dd2c263902e3170fa99bd765722cd249ea710e5b1","coverage":[{"denominator":0,"lane":"reference_resolution","note":"Typed states for the displayed outbound observations.","records_observed":0,"source":"paper_references, paper_reference_links","source_observed_at":null,"state":"measured"},{"denominator":12,"lane":"standing_notices","note":"One-hop event checks from named stored sources.","records_observed":12,"source":"scholarly_work_events, retraction_status_cache","source_observed_at":"2026-08-09T06:31:02.800959+00:00","state":"measured"},{"denominator":12,"lane":"inbound_itemization","note":"Pith citing papers itemized under the disclosed page cap.","records_observed":12,"source":"paper_references, paper_reference_links","source_observed_at":"2026-08-07T00:15:12.580018Z","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":"2026-07-04T06:59:38.023178Z","state":"measured"}],"external_citation_measurements":[],"inbound":[{"citation":{"cited_paper":{"arxiv_id":"2404.00090","last_updated":"2024-05-15T17:16:59Z","snapshot_observed_at":"2026-07-06T17:53:15.011246Z","submitted_at":"2024-03-29T18:00:01Z","title":"Systematic bias from waveform modeling for binary black hole populations in next-generation gravitational wave detectors","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2404.00090","snapshot_observed_at":"2026-08-06T18:34:53.138515Z","title":"Kapil, L","venue":null,"work_id":null,"year":2024},"citing_paper":{"arxiv_id":"2507.08081","last_updated":"2025-07-10T18:00:03Z","snapshot_observed_at":"2026-08-07T18:16:31.003795Z","submitted_at":"2025-07-10T18:00:03Z","title":"Post-adiabatic dynamics and waveform generation in self-force theory: an invariant pseudo-Hamiltonian framework","version":1},"reference_index":19,"source":"pdf_text","source_observed_at":"2026-08-06T18:34:53.138515Z"},"links":{"cited_paper":"/paper/2404.00090","citing_paper":"/paper/2507.08081"},"observation_digest":"sha256:a788f91653e7308b1ef215bfbfb7839374a53f177149d05740a447531fff7371","observation_id":"af483181-2426-43f3-8500-c3904566091e","resolution":{"observed_at":"2026-08-06T18:34:53.138515Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2404.00090","last_updated":"2024-05-15T17:16:59Z","snapshot_observed_at":"2026-07-06T17:53:15.011246Z","submitted_at":"2024-03-29T18:00:01Z","title":"Systematic bias from waveform modeling for binary black hole populations in next-generation gravitational wave detectors","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2404.00090","snapshot_observed_at":"2026-08-06T17:20:16.627466Z","title":"Kapil, L","venue":null,"work_id":null,"year":2024},"citing_paper":{"arxiv_id":"2507.11278","last_updated":"2025-07-16T09:32:35Z","snapshot_observed_at":"2026-08-09T04:49:33.009548Z","submitted_at":"2025-07-15T12:55:00Z","title":"The fault in our sirens: Hierarchical diagnosis of waveform systematics in Hubble-Lema\\^itre constant measurements","version":2},"reference_index":34,"source":"pdf_text","source_observed_at":"2026-08-06T17:20:16.627466Z"},"links":{"cited_paper":"/paper/2404.00090","citing_paper":"/paper/2507.11278"},"observation_digest":"sha256:b8de953eaefb15f47996370619c686a0fe5e17128d665df6595c85373e0a8e13","observation_id":"544ec542-b897-41d9-9c82-ba7e01e0281e","resolution":{"observed_at":"2026-08-06T17:20:16.627466Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2404.00090","last_updated":"2024-05-15T17:16:59Z","snapshot_observed_at":"2026-07-06T17:53:15.011246Z","submitted_at":"2024-03-29T18:00:01Z","title":"Systematic bias from waveform modeling for binary black hole populations in next-generation gravitational wave detectors","version":2},"cited_work":{"arxiv_id":"2404.00090","doi":null,"metadata_source":"arxiv_reference","pith_arxiv_id":"2404.00090","snapshot_observed_at":"2026-07-04T06:59:38.023178Z","title":"Kapil, L","venue":null,"work_id":"eb79e04e-4531-4bea-8ce4-8066a822651c","year":2024},"citing_paper":{"arxiv_id":"2510.11793","last_updated":"2026-05-13T10:10:18Z","snapshot_observed_at":"2026-08-01T10:09:57.706869Z","submitted_at":"2025-10-13T18:00:08Z","title":"Black hole mergers beyond general relativity: a self-force approach","version":2},"reference_index":27,"source":"pdf_text","source_observed_at":"2026-05-18T07:14:28.658616Z"},"links":{"cited_paper":"/paper/2404.00090","citing_paper":"/paper/2510.11793"},"observation_digest":"sha256:bdc57e0d617f8fd87960a23fb3dd74e4943b8d1fe75666f5076be54ce83678b3","observation_id":"2a4662be-a00d-4fbc-befe-569a987e20f2","resolution":{"observed_at":"2026-05-18T07:16:02.529131Z","resolver_source":"arxiv_id","status":"verified_exact"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-09T06:31:02.800959+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-09T06:31:02.800959+00:00","source":"crossref"},{"observed_at":"2026-08-09T06:30:57.326959+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":{"arxiv_id":"2404.00090","last_updated":"2024-05-15T17:16:59Z","snapshot_observed_at":"2026-07-06T17:53:15.011246Z","submitted_at":"2024-03-29T18:00:01Z","title":"Systematic bias from waveform modeling for binary black hole populations in next-generation gravitational wave detectors","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2404.00090","snapshot_observed_at":"2026-08-02T22:22:55.248157Z","title":"Kapil, L","venue":null,"work_id":null,"year":2024},"citing_paper":{"arxiv_id":"2602.17524","last_updated":"2026-06-26T14:54:58Z","snapshot_observed_at":"2026-08-07T00:53:00.353437Z","submitted_at":"2026-02-19T16:36:52Z","title":"Inspiral tests of general relativity and waveform geometry","version":2},"reference_index":73,"source":"pdf_text","source_observed_at":"2026-08-02T22:22:55.248157Z"},"links":{"cited_paper":"/paper/2404.00090","citing_paper":"/paper/2602.17524"},"observation_digest":"sha256:d17a7fcbbe7b6c2d3e233f7171f9db23db64659902e2743c9ed34da464528415","observation_id":"1d1c1266-2eae-436d-9171-c773bd1eb857","resolution":{"observed_at":"2026-08-02T22:22:55.248157Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2404.00090","last_updated":"2024-05-15T17:16:59Z","snapshot_observed_at":"2026-07-06T17:53:15.011246Z","submitted_at":"2024-03-29T18:00:01Z","title":"Systematic bias from waveform modeling for binary black hole populations in next-generation gravitational wave detectors","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2404.00090","snapshot_observed_at":"2026-07-14T00:11:25.155489Z","title":"Kapil, L","venue":null,"work_id":null,"year":2024},"citing_paper":{"arxiv_id":"2603.15765","last_updated":"2026-06-09T22:46:52Z","snapshot_observed_at":"2026-07-14T00:11:19.516003Z","submitted_at":"2026-03-16T18:00:45Z","title":"Impact of numerical-relativity waveform calibration on parametrized post-Einsteinian tests","version":2},"reference_index":47,"source":"pdf_text","source_observed_at":"2026-07-14T00:11:25.155489Z"},"links":{"cited_paper":"/paper/2404.00090","citing_paper":"/paper/2603.15765"},"observation_digest":"sha256:ef5f38a5880825ce5fc0e199aedf70f0e1a731788a67fa36f3d34b6e9eec920e","observation_id":"77598a83-dd4b-447d-a265-fe4a038b62e6","resolution":{"observed_at":"2026-07-14T00:11:25.155489Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2404.00090","last_updated":"2024-05-15T17:16:59Z","snapshot_observed_at":"2026-07-06T17:53:15.011246Z","submitted_at":"2024-03-29T18:00:01Z","title":"Systematic bias from waveform modeling for binary black hole populations in next-generation gravitational wave detectors","version":2},"cited_work":{"arxiv_id":"2404.00090","doi":null,"metadata_source":"arxiv_reference","pith_arxiv_id":"2404.00090","snapshot_observed_at":"2026-07-04T06:59:38.023178Z","title":"Kapil, L","venue":null,"work_id":"eb79e04e-4531-4bea-8ce4-8066a822651c","year":2024},"citing_paper":{"arxiv_id":"2604.21990","last_updated":"2026-05-28T19:22:04Z","snapshot_observed_at":"2026-08-02T01:26:33.523001Z","submitted_at":"2026-04-23T18:17:29Z","title":"A New Spin on Dissipative Tides: First-Post-Newtonian Effects in Compact Binary Inspirals","version":1},"reference_index":82,"source":"pdf_text","source_observed_at":"2026-05-09T20:51:27.972685Z"},"links":{"cited_paper":"/paper/2404.00090","citing_paper":"/paper/2604.21990"},"observation_digest":"sha256:3821b2b173da82a8a1db61a96a09d61f8b7dd46313bdf6ac7daaf4b89839928b","observation_id":"0b78c26f-06cf-4569-a1b3-71b4a1d175fe","resolution":{"observed_at":"2026-05-11T14:56:06.412678Z","resolver_source":"arxiv_id","status":"verified_exact"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-09T06:31:02.800959+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-09T06:31:02.800959+00:00","source":"crossref"},{"observed_at":"2026-08-09T06:30:57.326959+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":{"arxiv_id":"2404.00090","last_updated":"2024-05-15T17:16:59Z","snapshot_observed_at":"2026-07-06T17:53:15.011246Z","submitted_at":"2024-03-29T18:00:01Z","title":"Systematic bias from waveform modeling for binary black hole populations in next-generation gravitational wave detectors","version":2},"cited_work":{"arxiv_id":"2404.00090","doi":null,"metadata_source":"arxiv_reference","pith_arxiv_id":"2404.00090","snapshot_observed_at":"2026-07-04T06:59:38.023178Z","title":"Kapil, L","venue":null,"work_id":"eb79e04e-4531-4bea-8ce4-8066a822651c","year":2024},"citing_paper":{"arxiv_id":"2606.21076","last_updated":"2026-06-19T03:55:04Z","snapshot_observed_at":"2026-08-06T13:48:15.917788Z","submitted_at":"2026-06-19T03:55:04Z","title":"Population-level correlations in Bayesian statistics: an illustrative model for gravitational-wave astronomy","version":1},"reference_index":30,"source":"pdf_text","source_observed_at":"2026-06-26T13:59:14.326070Z"},"links":{"cited_paper":"/paper/2404.00090","citing_paper":"/paper/2606.21076"},"observation_digest":"sha256:a3257c9e503a431b655f7944b45f563bcdbdc435e2f0f52bc3b9b05f24028cc0","observation_id":"1ab9d1b1-813e-4ad9-a0f7-a560733c2973","resolution":{"observed_at":"2026-07-04T06:59:38.024443Z","resolver_source":"arxiv_id","status":"verified_exact"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-09T06:31:02.800959+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-09T06:31:02.800959+00:00","source":"crossref"},{"observed_at":"2026-08-09T06:30:57.326959+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":{"arxiv_id":"2404.00090","last_updated":"2024-05-15T17:16:59Z","snapshot_observed_at":"2026-07-06T17:53:15.011246Z","submitted_at":"2024-03-29T18:00:01Z","title":"Systematic bias from waveform modeling for binary black hole populations in next-generation gravitational wave detectors","version":2},"cited_work":{"arxiv_id":"2404.00090","doi":null,"metadata_source":"arxiv_reference","pith_arxiv_id":"2404.00090","snapshot_observed_at":"2026-07-04T06:59:38.023178Z","title":"Kapil, L","venue":null,"work_id":"eb79e04e-4531-4bea-8ce4-8066a822651c","year":2024},"citing_paper":{"arxiv_id":"2606.28161","last_updated":"2026-07-07T07:15:18Z","snapshot_observed_at":"2026-07-12T11:31:57.318013Z","submitted_at":"2026-06-26T14:57:17Z","title":"Finite Coherence in Gravitational Waves from Tidally Excited Axion Clouds","version":1},"reference_index":19,"source":"pdf_text","source_observed_at":"2026-06-29T03:20:11.303696Z"},"links":{"cited_paper":"/paper/2404.00090","citing_paper":"/paper/2606.28161"},"observation_digest":"sha256:80a852247b68d349423b2290cc0130a3074d6c9d53fe9887cc2722e0e1843aa6","observation_id":"b3df2e89-9fc8-47c1-898b-bdd22610f52b","resolution":{"observed_at":"2026-07-01T17:45:51.434567Z","resolver_source":"arxiv_id","status":"verified_exact"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-09T06:31:02.800959+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-09T06:31:02.800959+00:00","source":"crossref"},{"observed_at":"2026-08-09T06:30:57.326959+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":{"arxiv_id":"2404.00090","last_updated":"2024-05-15T17:16:59Z","snapshot_observed_at":"2026-07-06T17:53:15.011246Z","submitted_at":"2024-03-29T18:00:01Z","title":"Systematic bias from waveform modeling for binary black hole populations in next-generation gravitational wave detectors","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2404.00090","snapshot_observed_at":"2026-07-12T11:32:03.126331Z","title":"Kapil, L","venue":null,"work_id":null,"year":2024},"citing_paper":{"arxiv_id":"2606.28161","last_updated":"2026-07-07T07:15:18Z","snapshot_observed_at":"2026-07-12T11:31:57.318013Z","submitted_at":"2026-06-26T14:57:17Z","title":"Finite Coherence in Gravitational Waves from Tidally Excited Axion Clouds","version":2},"reference_index":19,"source":"pdf_text","source_observed_at":"2026-07-12T11:32:03.126331Z"},"links":{"cited_paper":"/paper/2404.00090","citing_paper":"/paper/2606.28161"},"observation_digest":"sha256:1649fcc7abfbcfa729152ecfccf1b6d45301cfe175c49680189c704072ad6f96","observation_id":"3ee0d15a-45bf-4a9b-8e58-79a73a6db503","resolution":{"observed_at":"2026-07-12T11:32:03.126331Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2404.00090","last_updated":"2024-05-15T17:16:59Z","snapshot_observed_at":"2026-07-06T17:53:15.011246Z","submitted_at":"2024-03-29T18:00:01Z","title":"Systematic bias from waveform modeling for binary black hole populations in next-generation gravitational wave detectors","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2404.00090","snapshot_observed_at":"2026-07-31T04:58:16.754087Z","title":"Kapil, L","venue":null,"work_id":null,"year":2024},"citing_paper":{"arxiv_id":"2607.24960","last_updated":"2026-07-27T18:08:33Z","snapshot_observed_at":"2026-08-07T04:14:42.676396Z","submitted_at":"2026-07-27T18:08:33Z","title":"Fast, accurate, and differentiable: a neural-network surrogate for NRSur7dq4 precessing binary black hole waveforms","version":1},"reference_index":39,"source":"pdf_text","source_observed_at":"2026-07-31T04:58:16.754087Z"},"links":{"cited_paper":"/paper/2404.00090","citing_paper":"/paper/2607.24960"},"observation_digest":"sha256:57e3e96a849c1eaa7da142b898946cc3441212acd162a9a7df2dee9c34784b34","observation_id":"50cf7fc4-30b8-40ec-95cd-035efa081d91","resolution":{"observed_at":"2026-07-31T04:58:16.754087Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2404.00090","last_updated":"2024-05-15T17:16:59Z","snapshot_observed_at":"2026-07-06T17:53:15.011246Z","submitted_at":"2024-03-29T18:00:01Z","title":"Systematic bias from waveform modeling for binary black hole populations in next-generation gravitational wave detectors","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2404.00090","snapshot_observed_at":"2026-08-04T21:28:07.250880Z","title":"Kapil, L","venue":null,"work_id":null,"year":2024},"citing_paper":{"arxiv_id":"2608.01774","last_updated":"2026-08-05T10:22:12Z","snapshot_observed_at":"2026-08-08T23:10:43.781147Z","submitted_at":"2026-08-03T06:47:21Z","title":"High-Post-Newtonian-Order Dynamics Induced by Tail-of-Tail Interactions: The Non-Geodesic Terms","version":1},"reference_index":34,"source":"pdf_text","source_observed_at":"2026-08-04T21:28:07.250880Z"},"links":{"cited_paper":"/paper/2404.00090","citing_paper":"/paper/2608.01774"},"observation_digest":"sha256:4bf197f0872765d0db073c2598cbb8f5696f1a482b6d8a2c078b4d6bb7f08a70","observation_id":"5ec2b69d-afb3-4759-bd27-338bd83bc403","resolution":{"observed_at":"2026-08-04T21:28:07.250880Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2404.00090","last_updated":"2024-05-15T17:16:59Z","snapshot_observed_at":"2026-07-06T17:53:15.011246Z","submitted_at":"2024-03-29T18:00:01Z","title":"Systematic bias from waveform modeling for binary black hole populations in next-generation gravitational wave detectors","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2404.00090","snapshot_observed_at":"2026-08-07T00:15:12.580018Z","title":"Kapil, L","venue":null,"work_id":null,"year":2024},"citing_paper":{"arxiv_id":"2608.01774","last_updated":"2026-08-05T10:22:12Z","snapshot_observed_at":"2026-08-08T23:10:43.781147Z","submitted_at":"2026-08-03T06:47:21Z","title":"High-Post-Newtonian-Order Dynamics Induced by Tail-of-Tail Interactions: The Non-Geodesic Terms","version":2},"reference_index":34,"source":"pdf_text","source_observed_at":"2026-08-07T00:15:12.580018Z"},"links":{"cited_paper":"/paper/2404.00090","citing_paper":"/paper/2608.01774"},"observation_digest":"sha256:f06e5958f8e05a7aca42281ba093480915e3fff5d4073989de9b8a22da9490c7","observation_id":"4ffa62e6-ae9b-4910-9026-0b4b3d1f73be","resolution":{"observed_at":"2026-08-07T00:15:12.580018Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}}],"links":{"evidence":"/evidence","html":"/paper/2404.00090/citation-record","integrity":"/paper/2404.00090/integrity","json":"/paper/2404.00090/citation-record.json","paper":"/paper/2404.00090"},"outbound":[],"paper":{"arxiv_id":"2404.00090","last_updated":"2024-05-15T17:16:59Z","latest_version":2,"primary_category":"gr-qc","snapshot_observed_at":"2026-07-06T17:53:15.011246Z","submitted_at":"2024-03-29T18:00:01Z","title":"Systematic bias from waveform modeling for binary black hole populations in next-generation gravitational wave detectors"},"reference_resolution":{"displayed":0,"state_counts":{"malformed_identifier":0,"metadata_mismatch":0,"parse_uncertain":0,"unresolved":0,"verified_exact":0,"verified_fuzzy":0},"total_outbound_references":0},"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":"2026-08-09T06:31:02.800959+00:00","source":"crossref"},{"observed_at":"2026-08-09T06:30:57.326959+00:00","source":"retraction_watch"}],"thesis":"As of 9 August 2026, this Paper Citation Record lists 0 of 0 outbound references and 12 inbound Pith citation observations for arXiv:2404.00090."}