{"as_of":"2026-08-10T07:20:00Z","caps":{"database_statements":6,"inbound":100,"outbound":100},"context_digest":"sha256:dd1cc7892558a5c008ee55f4b5610d9f05acbc031ef236553374187b9dbe7fb1","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":11,"lane":"standing_notices","note":"One-hop event checks from named stored sources.","records_observed":11,"source":"scholarly_work_events, retraction_status_cache","source_observed_at":"2026-08-10T06:31:04.303077+00:00","state":"measured"},{"denominator":11,"lane":"inbound_itemization","note":"Pith citing papers itemized under the disclosed page cap.","records_observed":11,"source":"paper_references, paper_reference_links","source_observed_at":"2026-08-09T05:46:29.252899Z","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":"2026-05-23T23:43:38.580590Z","state":"measured"}],"external_citation_measurements":[],"inbound":[{"citation":{"cited_paper":{"arxiv_id":"2312.08588","last_updated":"2025-03-06T23:37:06Z","snapshot_observed_at":"2026-08-09T09:06:23.714069Z","submitted_at":"2023-12-14T01:19:38Z","title":"Black Hole Spectroscopy for Precessing Binary Black Hole Coalescences","version":3},"cited_work":{"arxiv_id":"2312.08588","doi":null,"metadata_source":"arxiv_reference","pith_arxiv_id":"2312.08588","snapshot_observed_at":"2026-06-05T21:23:00.469572Z","title":"Zhu et al., arXiv preprint arXiv:2312.08588 (2023)","venue":null,"work_id":"f3a48962-9c46-4c5b-b9ee-171ab257d9ee","year":2023},"citing_paper":{"arxiv_id":"2407.18319","last_updated":"2026-05-15T21:01:12Z","snapshot_observed_at":"2026-08-03T01:10:17.314668Z","submitted_at":"2024-07-25T18:19:06Z","title":"Gravitational wave surrogate model for spinning, intermediate mass ratio binaries based on perturbation theory and numerical relativity","version":2},"reference_index":112,"source":"pdf_text","source_observed_at":"2026-05-23T23:38:37.094812Z"},"links":{"cited_paper":"/paper/2312.08588","citing_paper":"/paper/2407.18319"},"observation_digest":"sha256:3ab49416a19e782ac3f8b084eff07337c6897405eb90430515bf64fd57fdd9c0","observation_id":"5975ff51-0890-4058-8c90-f30e72d17c6a","resolution":{"observed_at":"2026-05-23T23:43:38.583371Z","resolver_source":"arxiv_id","status":"verified_exact"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-10T06:31:04.303077+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-10T06:31:04.303077+00:00","source":"crossref"},{"observed_at":"2026-08-10T06:30:57.382061+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":{"arxiv_id":"2312.08588","last_updated":"2025-03-06T23:37:06Z","snapshot_observed_at":"2026-08-09T09:06:23.714069Z","submitted_at":"2023-12-14T01:19:38Z","title":"Black Hole Spectroscopy for Precessing Binary Black Hole Coalescences","version":3},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2312.08588","snapshot_observed_at":"2026-08-09T05:46:29.252899Z","title":"2023 (Preprint 2312.08588)","venue":null,"work_id":null,"year":2023},"citing_paper":{"arxiv_id":"2502.03155","last_updated":"2025-02-05T13:24:49Z","snapshot_observed_at":"2026-08-09T09:06:19.876298Z","submitted_at":"2025-02-05T13:24:49Z","title":"Multimode ringdown modelling with $\\texttt{qnmfits}$ and $\\texttt{KerrRingdown}$","version":1},"reference_index":18,"source":"pdf_text","source_observed_at":"2026-08-09T05:46:29.252899Z"},"links":{"cited_paper":"/paper/2312.08588","citing_paper":"/paper/2502.03155"},"observation_digest":"sha256:ef19b89e9504c916db440c7c8a6e80ce07ecadc662185a6a3cc7138342b9bcb2","observation_id":"a71477e6-1596-4c43-a9fa-07d919303898","resolution":{"observed_at":"2026-08-09T05:46:29.252899Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2312.08588","last_updated":"2025-03-06T23:37:06Z","snapshot_observed_at":"2026-08-09T09:06:23.714069Z","submitted_at":"2023-12-14T01:19:38Z","title":"Black Hole Spectroscopy for Precessing Binary Black Hole Coalescences","version":3},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2312.08588","snapshot_observed_at":"2026-08-07T14:34:52.841974Z","title":null,"venue":null,"work_id":null,"year":2023},"citing_paper":{"arxiv_id":"2505.18560","last_updated":"2025-08-11T02:18:53Z","snapshot_observed_at":"2026-08-09T20:18:43.098549Z","submitted_at":"2025-05-24T07:00:31Z","title":"Statistical identification of ringdown modes with rational filters","version":2},"reference_index":56,"source":"pdf_text","source_observed_at":"2026-08-07T14:34:52.841974Z"},"links":{"cited_paper":"/paper/2312.08588","citing_paper":"/paper/2505.18560"},"observation_digest":"sha256:6301aee5e2e10ff246c40093ebe3b9bc8615be24f931e0be3a0d6e38650384a2","observation_id":"4ef95fc7-60da-4891-949e-e89cdca9845a","resolution":{"observed_at":"2026-08-07T14:34:52.841974Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2312.08588","last_updated":"2025-03-06T23:37:06Z","snapshot_observed_at":"2026-08-09T09:06:23.714069Z","submitted_at":"2023-12-14T01:19:38Z","title":"Black Hole Spectroscopy for Precessing Binary Black Hole Coalescences","version":3},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2312.08588","snapshot_observed_at":"2026-08-06T18:15:44.974727Z","title":"Black hole spectroscopy for precessing binary black hole coalescences,","venue":null,"work_id":null,"year":2025},"citing_paper":{"arxiv_id":"2507.08789","last_updated":"2025-08-11T03:04:31Z","snapshot_observed_at":"2026-08-09T06:54:59.862771Z","submitted_at":"2025-07-11T17:51:40Z","title":"Potential science with GW250114 -- the loudest binary black hole merger detected to date","version":2},"reference_index":29,"source":"pdf_text","source_observed_at":"2026-08-06T18:15:44.974727Z"},"links":{"cited_paper":"/paper/2312.08588","citing_paper":"/paper/2507.08789"},"observation_digest":"sha256:5aa8c08a63e556f08f4dfd0f17b3b119852256e33de95ff1fa2df4830c699469","observation_id":"bd3c2df2-244d-4773-b8f0-adea76a84ef7","resolution":{"observed_at":"2026-08-06T18:15:44.974727Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2312.08588","last_updated":"2025-03-06T23:37:06Z","snapshot_observed_at":"2026-08-09T09:06:23.714069Z","submitted_at":"2023-12-14T01:19:38Z","title":"Black Hole Spectroscopy for Precessing Binary Black Hole Coalescences","version":3},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2312.08588","snapshot_observed_at":"2026-08-05T12:06:00.799860Z","title":"Zhu et al","venue":null,"work_id":null,"year":2025},"citing_paper":{"arxiv_id":"2509.02047","last_updated":"2025-09-02T07:44:14Z","snapshot_observed_at":"2026-08-08T01:29:37.575195Z","submitted_at":"2025-09-02T07:44:14Z","title":"Detection of a Higher Harmonic Quasi-normal Mode in the Ringdown Signal of GW231123","version":1},"reference_index":36,"source":"pdf_text","source_observed_at":"2026-08-05T12:06:00.799860Z"},"links":{"cited_paper":"/paper/2312.08588","citing_paper":"/paper/2509.02047"},"observation_digest":"sha256:e3bf3cd0aaed66942485b8884cac1b25d266b4a7a4762226bdecf27239ba8c12","observation_id":"a8a955f8-06c0-48be-b484-ef3c801448bd","resolution":{"observed_at":"2026-08-05T12:06:00.799860Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2312.08588","last_updated":"2025-03-06T23:37:06Z","snapshot_observed_at":"2026-08-09T09:06:23.714069Z","submitted_at":"2023-12-14T01:19:38Z","title":"Black Hole Spectroscopy for Precessing Binary Black Hole Coalescences","version":3},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2312.08588","snapshot_observed_at":"2026-08-04T09:43:29.371588Z","title":"Zhuet al., PRD111, 064052 (2025), arXiv:2312.08588 [gr-qc]","venue":null,"work_id":null,"year":2025},"citing_paper":{"arxiv_id":"2510.13954","last_updated":"2026-06-24T11:08:04Z","snapshot_observed_at":"2026-08-08T07:07:31.166521Z","submitted_at":"2025-10-15T18:00:03Z","title":"Quasinormal mode content of binary black hole ringdowns","version":2},"reference_index":14,"source":"pdf_text","source_observed_at":"2026-08-04T09:43:29.371588Z"},"links":{"cited_paper":"/paper/2312.08588","citing_paper":"/paper/2510.13954"},"observation_digest":"sha256:95f47de704e4417e1b5521ef035691513727d421457563d826821bbf0dd9db04","observation_id":"ffc87d45-5a81-4363-99a9-8136d9faf566","resolution":{"observed_at":"2026-08-04T09:43:29.371588Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2312.08588","last_updated":"2025-03-06T23:37:06Z","snapshot_observed_at":"2026-08-09T09:06:23.714069Z","submitted_at":"2023-12-14T01:19:38Z","title":"Black Hole Spectroscopy for Precessing Binary Black Hole Coalescences","version":3},"cited_work":{"arxiv_id":"2312.08588","doi":null,"metadata_source":"arxiv_reference","pith_arxiv_id":"2312.08588","snapshot_observed_at":"2026-06-05T21:23:00.469572Z","title":"Zhu et al., arXiv preprint arXiv:2312.08588 (2023)","venue":null,"work_id":"f3a48962-9c46-4c5b-b9ee-171ab257d9ee","year":2023},"citing_paper":{"arxiv_id":"2601.04276","last_updated":"2026-05-12T15:16:18Z","snapshot_observed_at":"2026-07-06T22:41:01.254450Z","submitted_at":"2026-01-07T12:25:02Z","title":"Search for Precessing Binary Black Holes in Advanced LIGO's Third Observing Run using Harmonic Decomposition","version":2},"reference_index":23,"source":"pdf_text","source_observed_at":"2026-05-16T16:35:21.153235Z"},"links":{"cited_paper":"/paper/2312.08588","citing_paper":"/paper/2601.04276"},"observation_digest":"sha256:4a26c281810afac84519834bd2e0a4b6c6dcc31e3357ade9b286c0b7e2b012c3","observation_id":"fd2c4b60-904a-4a38-9b43-653d8fcb102e","resolution":{"observed_at":"2026-05-16T16:38:06.303204Z","resolver_source":"arxiv_id","status":"metadata_mismatch"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-10T06:31:04.303077+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-10T06:31:04.303077+00:00","source":"crossref"},{"observed_at":"2026-08-10T06:30:57.382061+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":{"arxiv_id":"2312.08588","last_updated":"2025-03-06T23:37:06Z","snapshot_observed_at":"2026-08-09T09:06:23.714069Z","submitted_at":"2023-12-14T01:19:38Z","title":"Black Hole Spectroscopy for Precessing Binary Black Hole Coalescences","version":3},"cited_work":{"arxiv_id":"2312.08588","doi":null,"metadata_source":"arxiv_reference","pith_arxiv_id":"2312.08588","snapshot_observed_at":"2026-06-05T21:23:00.469572Z","title":"Zhu et al., arXiv preprint arXiv:2312.08588 (2023)","venue":null,"work_id":"f3a48962-9c46-4c5b-b9ee-171ab257d9ee","year":2023},"citing_paper":{"arxiv_id":"2604.15431","last_updated":"2026-04-16T18:00:02Z","snapshot_observed_at":"2026-08-02T05:54:54.327009Z","submitted_at":"2026-04-16T18:00:02Z","title":"Highly eccentric non-spinning binary black hole mergers: quadrupolar post-merger waveforms","version":1},"reference_index":192,"source":"pdf_text","source_observed_at":"2026-05-10T10:16:15.923894Z"},"links":{"cited_paper":"/paper/2312.08588","citing_paper":"/paper/2604.15431"},"observation_digest":"sha256:060ab8334d00d91d40a79a12e7f23f779ab28a2fd520069a39cc6abdae2f7506","observation_id":"28b75aee-e6a6-4aaf-91f3-8e9468ec9192","resolution":{"observed_at":"2026-05-10T10:19:20.973090Z","resolver_source":"arxiv_id","status":"verified_exact"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-10T06:31:04.303077+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-10T06:31:04.303077+00:00","source":"crossref"},{"observed_at":"2026-08-10T06:30:57.382061+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":{"arxiv_id":"2312.08588","last_updated":"2025-03-06T23:37:06Z","snapshot_observed_at":"2026-08-09T09:06:23.714069Z","submitted_at":"2023-12-14T01:19:38Z","title":"Black Hole Spectroscopy for Precessing Binary Black Hole Coalescences","version":3},"cited_work":{"arxiv_id":"2312.08588","doi":null,"metadata_source":"arxiv_reference","pith_arxiv_id":"2312.08588","snapshot_observed_at":"2026-06-05T21:23:00.469572Z","title":"Zhu et al., arXiv preprint arXiv:2312.08588 (2023)","venue":null,"work_id":"f3a48962-9c46-4c5b-b9ee-171ab257d9ee","year":2023},"citing_paper":{"arxiv_id":"2605.03576","last_updated":"2026-05-05T09:45:08Z","snapshot_observed_at":"2026-07-06T23:16:30.147006Z","submitted_at":"2026-05-05T09:45:08Z","title":"Ringdown Analysis of GW250114 with Orthonormal Modes","version":1},"reference_index":92,"source":"pdf_text","source_observed_at":"2026-05-07T04:06:51.511923Z"},"links":{"cited_paper":"/paper/2312.08588","citing_paper":"/paper/2605.03576"},"observation_digest":"sha256:60b508924b189a4a59172db654ec8b7e02a844857426d6d8692ae47d74b285b8","observation_id":"f94e9a73-3236-4172-88e5-834595dbcb54","resolution":{"observed_at":"2026-05-12T11:01:31.215674Z","resolver_source":"arxiv_id","status":"metadata_mismatch"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-10T06:31:04.303077+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-10T06:31:04.303077+00:00","source":"crossref"},{"observed_at":"2026-08-10T06:30:57.382061+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":{"arxiv_id":"2312.08588","last_updated":"2025-03-06T23:37:06Z","snapshot_observed_at":"2026-08-09T09:06:23.714069Z","submitted_at":"2023-12-14T01:19:38Z","title":"Black Hole Spectroscopy for Precessing Binary Black Hole Coalescences","version":3},"cited_work":{"arxiv_id":"2312.08588","doi":null,"metadata_source":"arxiv_reference","pith_arxiv_id":"2312.08588","snapshot_observed_at":"2026-06-05T21:23:00.469572Z","title":"Zhu et al., arXiv preprint arXiv:2312.08588 (2023)","venue":null,"work_id":"f3a48962-9c46-4c5b-b9ee-171ab257d9ee","year":2023},"citing_paper":{"arxiv_id":"2605.15271","last_updated":"2026-05-14T18:00:02Z","snapshot_observed_at":"2026-08-02T18:46:19.285847Z","submitted_at":"2026-05-14T18:00:02Z","title":"Polarization Analysis of Ringdown Signals","version":1},"reference_index":25,"source":"pdf_text","source_observed_at":"2026-05-19T15:39:06.963382Z"},"links":{"cited_paper":"/paper/2312.08588","citing_paper":"/paper/2605.15271"},"observation_digest":"sha256:f2ec3c82ef0cb1c2945ea32bfa6a57ec2d685ef262888b41b9280e0dd87e1939","observation_id":"59fcb697-ac7e-46fc-b5b6-66aa914c3282","resolution":{"observed_at":"2026-05-19T15:42:38.461438Z","resolver_source":"arxiv_id","status":"verified_exact"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-10T06:31:04.303077+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-10T06:31:04.303077+00:00","source":"crossref"},{"observed_at":"2026-08-10T06:30:57.382061+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":{"arxiv_id":"2312.08588","last_updated":"2025-03-06T23:37:06Z","snapshot_observed_at":"2026-08-09T09:06:23.714069Z","submitted_at":"2023-12-14T01:19:38Z","title":"Black Hole Spectroscopy for Precessing Binary Black Hole Coalescences","version":3},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2312.08588","snapshot_observed_at":"2026-08-07T22:32:29.168804Z","title":"Zhu et al","venue":null,"work_id":null,"year":2025},"citing_paper":{"arxiv_id":"2608.05846","last_updated":"2026-08-06T10:19:40Z","snapshot_observed_at":"2026-08-09T23:11:42.159527Z","submitted_at":"2026-08-06T10:19:40Z","title":"Prospects for characterizing Population III remnants with next-generation gravitational-wave observatories","version":1},"reference_index":75,"source":"pdf_text","source_observed_at":"2026-08-07T22:32:29.168804Z"},"links":{"cited_paper":"/paper/2312.08588","citing_paper":"/paper/2608.05846"},"observation_digest":"sha256:44aa15382553e2aa17a5866becbef7c7e57667ac753dda70ab912bf118f538c2","observation_id":"5e49782c-9b88-48d8-a959-f9cbb726da45","resolution":{"observed_at":"2026-08-07T22:32:29.168804Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}}],"links":{"evidence":"/evidence","html":"/paper/2312.08588/citation-record","integrity":"/paper/2312.08588/integrity","json":"/paper/2312.08588/citation-record.json","paper":"/paper/2312.08588"},"outbound":[],"paper":{"arxiv_id":"2312.08588","last_updated":"2025-03-06T23:37:06Z","latest_version":3,"primary_category":"gr-qc","snapshot_observed_at":"2026-08-09T09:06:23.714069Z","submitted_at":"2023-12-14T01:19:38Z","title":"Black Hole Spectroscopy for Precessing Binary Black Hole Coalescences"},"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":"2026-08-10T06:31:04.303077+00:00","source":"crossref"},{"observed_at":"2026-08-10T06:30:57.382061+00:00","source":"retraction_watch"}],"thesis":"As of 10 August 2026, this Paper Citation Record lists 0 of 0 outbound references and 11 inbound Pith citation observations for arXiv:2312.08588."}