{"as_of":"2026-08-13T20:41:00Z","caps":{"database_statements":6,"inbound":100,"outbound":100},"context_digest":"sha256:a18ecf8d69f42a2bb3478e4eebe8ec15d59ec4168363eba1f57d4a7450545e79","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":7,"lane":"standing_notices","note":"One-hop event checks from named stored sources.","records_observed":7,"source":"scholarly_work_events, retraction_status_cache","source_observed_at":"2026-08-13T06:32:02.005865+00:00","state":"measured"},{"denominator":7,"lane":"inbound_itemization","note":"Pith citing papers itemized under the disclosed page cap.","records_observed":7,"source":"paper_references, paper_reference_links","source_observed_at":"2026-08-11T11:42:50.480887Z","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":"2026-05-22T10:41:25.621467Z","state":"measured"}],"external_citation_measurements":[],"inbound":[{"citation":{"cited_paper":{"arxiv_id":"2301.07215","last_updated":"2023-02-12T20:21:47Z","snapshot_observed_at":"2026-08-13T13:02:52.554148Z","submitted_at":"2023-01-17T22:39:38Z","title":"Remnant black hole properties from numerical-relativity-informed perturbation theory and implications for waveform modelling","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2301.07215","snapshot_observed_at":"2026-08-11T11:42:50.480887Z","title":"Phys Rev D 108(6):064048","venue":null,"work_id":null,"year":2023},"citing_paper":{"arxiv_id":"2412.15046","last_updated":"2024-12-19T16:52:43Z","snapshot_observed_at":"2026-08-13T19:18:50.501882Z","submitted_at":"2024-12-19T16:52:43Z","title":"Applications of machine learning in gravitational wave research with current interferometric detectors","version":1},"reference_index":213,"source":"arxiv_source","source_observed_at":"2026-08-11T11:42:50.480887Z"},"links":{"cited_paper":"/paper/2301.07215","citing_paper":"/paper/2412.15046"},"observation_digest":"sha256:209fca9003f3ffa47f43b62fcbbd4520bcdb7cc6c4a450c874b08d235da38eaa","observation_id":"e21bbeba-1e7f-47a8-8014-5cee99b4444a","resolution":{"observed_at":"2026-08-11T11:42:50.480887Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2301.07215","last_updated":"2023-02-12T20:21:47Z","snapshot_observed_at":"2026-08-13T13:02:52.554148Z","submitted_at":"2023-01-17T22:39:38Z","title":"Remnant black hole properties from numerical-relativity-informed perturbation theory and implications for waveform modelling","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2301.07215","snapshot_observed_at":"2026-08-10T22:05:21.878537Z","title":"Remnant black hole properties from numerical-relativity-informed pertur- bation theory and implications for waveform modeling,","venue":null,"work_id":null,"year":2023},"citing_paper":{"arxiv_id":"2501.02974","last_updated":"2025-05-14T05:01:12Z","snapshot_observed_at":"2026-08-11T01:25:26.436694Z","submitted_at":"2025-01-06T12:34:52Z","title":"Surrogate modeling of gravitational waves microlensed by spherically symmetric potentials","version":3},"reference_index":77,"source":"pdf_text","source_observed_at":"2026-08-10T22:05:21.878537Z"},"links":{"cited_paper":"/paper/2301.07215","citing_paper":"/paper/2501.02974"},"observation_digest":"sha256:d67ed22568ee86e9403fdd1a03ef56b32c5c6cac1fa96f64f7877049b3583951","observation_id":"679c343a-0386-4b16-893b-bee0d8d716b1","resolution":{"observed_at":"2026-08-10T22:05:21.878537Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2301.07215","last_updated":"2023-02-12T20:21:47Z","snapshot_observed_at":"2026-08-13T13:02:52.554148Z","submitted_at":"2023-01-17T22:39:38Z","title":"Remnant black hole properties from numerical-relativity-informed perturbation theory and implications for waveform modelling","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2301.07215","snapshot_observed_at":"2026-08-03T22:13:48.346507Z","title":"Remnant black hole properties from numerical-relativity-informed pertur- bation theory and implications for waveform modeling,","venue":null,"work_id":null,"year":2023},"citing_paper":{"arxiv_id":"2511.11536","last_updated":"2026-06-18T20:28:43Z","snapshot_observed_at":"2026-08-13T05:37:39.870344Z","submitted_at":"2025-11-14T18:13:37Z","title":"Accurate models for recoil velocity distribution in black hole mergers with comparable to extreme mass-ratios and their astrophysical implications","version":2},"reference_index":28,"source":"pdf_text","source_observed_at":"2026-08-03T22:13:48.346507Z"},"links":{"cited_paper":"/paper/2301.07215","citing_paper":"/paper/2511.11536"},"observation_digest":"sha256:2c220f853829ed749c99e7ec1013ed55c55af9d4b003cca3676f6f71d61034ea","observation_id":"d13fbd62-4a8c-4e6f-8345-bdb40c01e09a","resolution":{"observed_at":"2026-08-03T22:13:48.346507Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2301.07215","last_updated":"2023-02-12T20:21:47Z","snapshot_observed_at":"2026-08-13T13:02:52.554148Z","submitted_at":"2023-01-17T22:39:38Z","title":"Remnant black hole properties from numerical-relativity-informed perturbation theory and implications for waveform modelling","version":2},"cited_work":{"arxiv_id":"2301.07215","doi":null,"metadata_source":"arxiv_reference","pith_arxiv_id":"2301.07215","snapshot_observed_at":"2026-06-05T21:23:00.469572Z","title":"Remnant black hole properties from numerical-relativity- informed perturbation theory and implications for wave- form modeling","venue":null,"work_id":"25a44292-b5da-4a7d-86eb-5542300f05b7","year":2023},"citing_paper":{"arxiv_id":"2604.04546","last_updated":"2026-06-18T20:56:44Z","snapshot_observed_at":"2026-08-13T15:01:24.307741Z","submitted_at":"2026-04-06T09:13:33Z","title":"Recoil kicks from binary black hole mergers in GWTC catalogs: implications for retention and hierarchical mergers","version":1},"reference_index":29,"source":"pdf_text","source_observed_at":"2026-05-10T20:05:50.776920Z"},"links":{"cited_paper":"/paper/2301.07215","citing_paper":"/paper/2604.04546"},"observation_digest":"sha256:bc2b6a2055be6839c5f642db4f71329cdbedd4119674155c003a22cb04a360a1","observation_id":"8cac23ed-745c-4b3d-b733-1117d5943c89","resolution":{"observed_at":"2026-05-10T22:15:49.414341Z","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":"2301.07215","last_updated":"2023-02-12T20:21:47Z","snapshot_observed_at":"2026-08-13T13:02:52.554148Z","submitted_at":"2023-01-17T22:39:38Z","title":"Remnant black hole properties from numerical-relativity-informed perturbation theory and implications for waveform modelling","version":2},"cited_work":{"arxiv_id":"2301.07215","doi":null,"metadata_source":"arxiv_reference","pith_arxiv_id":"2301.07215","snapshot_observed_at":"2026-06-05T21:23:00.469572Z","title":"Remnant black hole properties from numerical-relativity- informed perturbation theory and implications for wave- form modeling","venue":null,"work_id":"25a44292-b5da-4a7d-86eb-5542300f05b7","year":2023},"citing_paper":{"arxiv_id":"2605.00124","last_updated":"2026-05-20T21:35:50Z","snapshot_observed_at":"2026-07-06T23:13:38.354733Z","submitted_at":"2026-04-30T18:25:52Z","title":"Merger remnant and eccentricity dynamics surrogates for eccentric nonspinning black hole binaries","version":1},"reference_index":32,"source":"pdf_text","source_observed_at":"2026-05-09T20:41:09.388195Z"},"links":{"cited_paper":"/paper/2301.07215","citing_paper":"/paper/2605.00124"},"observation_digest":"sha256:5c2cfd9e982b3618fc9540f180563b71bdcd7804d176469a27a3302f52d80b1f","observation_id":"312ec02c-c845-4581-9f7e-62612dba51bc","resolution":{"observed_at":"2026-05-11T15:01:08.760355Z","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":"2301.07215","last_updated":"2023-02-12T20:21:47Z","snapshot_observed_at":"2026-08-13T13:02:52.554148Z","submitted_at":"2023-01-17T22:39:38Z","title":"Remnant black hole properties from numerical-relativity-informed perturbation theory and implications for waveform modelling","version":2},"cited_work":{"arxiv_id":"2301.07215","doi":null,"metadata_source":"arxiv_reference","pith_arxiv_id":"2301.07215","snapshot_observed_at":"2026-06-05T21:23:00.469572Z","title":"Remnant black hole properties from numerical-relativity- informed perturbation theory and implications for wave- form modeling","venue":null,"work_id":"25a44292-b5da-4a7d-86eb-5542300f05b7","year":2023},"citing_paper":{"arxiv_id":"2605.00124","last_updated":"2026-05-20T21:35:50Z","snapshot_observed_at":"2026-07-06T23:13:38.354733Z","submitted_at":"2026-04-30T18:25:52Z","title":"Merger remnant and eccentricity dynamics surrogates for eccentric nonspinning black hole binaries","version":2},"reference_index":32,"source":"pdf_text","source_observed_at":"2026-05-22T10:37:23.693585Z"},"links":{"cited_paper":"/paper/2301.07215","citing_paper":"/paper/2605.00124"},"observation_digest":"sha256:ddff447977f26f1e419c7b6be73c0badbf2f86b9debe34584a817abc5f0d917d","observation_id":"ce1e3695-b551-462c-bf1a-6d34957aac68","resolution":{"observed_at":"2026-05-22T10:41:25.623974Z","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":"2301.07215","last_updated":"2023-02-12T20:21:47Z","snapshot_observed_at":"2026-08-13T13:02:52.554148Z","submitted_at":"2023-01-17T22:39:38Z","title":"Remnant black hole properties from numerical-relativity-informed perturbation theory and implications for waveform modelling","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2301.07215","snapshot_observed_at":"2026-08-06T00:42:32.481704Z","title":"Remnant black hole properties from numerical-relativity-informed per- turbation theory and implications for waveform modeling,","venue":null,"work_id":null,"year":2023},"citing_paper":{"arxiv_id":"2608.00934","last_updated":"2026-08-02T02:19:55Z","snapshot_observed_at":"2026-08-06T23:25:13.079313Z","submitted_at":"2026-08-02T02:19:55Z","title":"Unified remnant models for aligned-spin, precessing, and eccentric binary black hole mergers","version":1},"reference_index":30,"source":"pdf_text","source_observed_at":"2026-08-06T00:42:32.481704Z"},"links":{"cited_paper":"/paper/2301.07215","citing_paper":"/paper/2608.00934"},"observation_digest":"sha256:6e109eba3f895fc7be57fc039760c151f6dca9dc855a8f683779136e59e5e126","observation_id":"b801c02d-daba-4772-b3d3-16da5274f3dd","resolution":{"observed_at":"2026-08-06T00:42:32.481704Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}}],"links":{"evidence":"/evidence","html":"/paper/2301.07215/citation-record","integrity":"/paper/2301.07215/integrity","json":"/paper/2301.07215/citation-record.json","paper":"/paper/2301.07215"},"outbound":[],"paper":{"arxiv_id":"2301.07215","last_updated":"2023-02-12T20:21:47Z","latest_version":2,"primary_category":"gr-qc","snapshot_observed_at":"2026-08-13T13:02:52.554148Z","submitted_at":"2023-01-17T22:39:38Z","title":"Remnant black hole properties from numerical-relativity-informed perturbation theory and implications for waveform modelling"},"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":"2026-08-13T06:32:02.005865+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 0 of 0 outbound references and 7 inbound Pith citation observations for arXiv:2301.07215."}