{"as_of":"2026-08-17T23:38:00Z","caps":{"database_statements":6,"inbound":100,"outbound":100},"context_digest":"sha256:1009b2b459e1064870732e5811e092815263625fe39bfd4ab263798e0ba50547","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":10,"lane":"standing_notices","note":"One-hop event checks from named stored sources.","records_observed":10,"source":"scholarly_work_events, retraction_status_cache","source_observed_at":"2026-08-17T06:30:58.91139+00:00","state":"measured"},{"denominator":10,"lane":"inbound_itemization","note":"Pith citing papers itemized under the disclosed page cap.","records_observed":10,"source":"paper_references, paper_reference_links","source_observed_at":"2026-08-16T12:40:19.761856Z","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":"2026-06-29T11:03:19.205500Z","state":"measured"}],"external_citation_measurements":[],"inbound":[{"citation":{"cited_paper":{"arxiv_id":"2101.11033","last_updated":"2021-06-08T12:28:57Z","snapshot_observed_at":"2026-08-17T18:50:31.173570Z","submitted_at":"2021-01-26T19:04:07Z","title":"Adding eccentricity to quasicircular binary-black-hole waveform models","version":2},"cited_work":{"arxiv_id":"2101.11033","doi":null,"metadata_source":"arxiv_reference","pith_arxiv_id":"2101.11033","snapshot_observed_at":"2026-06-29T11:03:19.205500Z","title":"Setyawati and F","venue":null,"work_id":"491dae92-70e5-4df1-b634-d24cc5b8b978","year":2021},"citing_paper":{"arxiv_id":"2404.14286","last_updated":"2026-05-05T08:23:34Z","snapshot_observed_at":"2026-08-08T10:26:27.851868Z","submitted_at":"2024-04-22T15:37:08Z","title":"Evidence for eccentricity in the population of binary black holes observed by LIGO-Virgo-KAGRA","version":3},"reference_index":170,"source":"pdf_text","source_observed_at":"2026-05-24T01:34:53.946159Z"},"links":{"cited_paper":"/paper/2101.11033","citing_paper":"/paper/2404.14286"},"observation_digest":"sha256:282538940c077d0fa07bbf8efcaeff382596299d153b55a7336e67eb6d1ee20e","observation_id":"a6f55151-88ce-4bdb-a12c-611574625844","resolution":{"observed_at":"2026-05-24T01:35:56.084725Z","resolver_source":"arxiv_id","status":"verified_exact"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-17T06:30:58.91139+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-17T06:30:58.91139+00:00","source":"crossref"},{"observed_at":"2026-08-17T06:30:54.323127+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":{"arxiv_id":"2101.11033","last_updated":"2021-06-08T12:28:57Z","snapshot_observed_at":"2026-08-17T18:50:31.173570Z","submitted_at":"2021-01-26T19:04:07Z","title":"Adding eccentricity to quasicircular binary-black-hole waveform models","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2101.11033","snapshot_observed_at":"2026-08-11T19:45:10.365921Z","title":"Setyawati and F","venue":null,"work_id":null,"year":2021},"citing_paper":{"arxiv_id":"2412.06433","last_updated":"2025-02-04T11:05:33Z","snapshot_observed_at":"2026-08-14T19:24:37.229129Z","submitted_at":"2024-12-09T12:21:00Z","title":"A geometric template bank for the detection of spinning low-mass compact binaries with moderate orbital eccentricity","version":3},"reference_index":153,"source":"pdf_text","source_observed_at":"2026-08-11T19:45:10.365921Z"},"links":{"cited_paper":"/paper/2101.11033","citing_paper":"/paper/2412.06433"},"observation_digest":"sha256:399ff075507184681d190d8c4e517ec96640ae6db4c8976adad520564c9bb551","observation_id":"8d48e77f-e7d7-4a6e-ba45-c689692768ee","resolution":{"observed_at":"2026-08-11T19:45:10.365921Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2101.11033","last_updated":"2021-06-08T12:28:57Z","snapshot_observed_at":"2026-08-17T18:50:31.173570Z","submitted_at":"2021-01-26T19:04:07Z","title":"Adding eccentricity to quasicircular binary-black-hole waveform models","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2101.11033","snapshot_observed_at":"2026-08-11T13:49:13.398699Z","title":"Setyawati and F","venue":null,"work_id":null,"year":2021},"citing_paper":{"arxiv_id":"2412.12823","last_updated":"2025-08-21T18:54:24Z","snapshot_observed_at":"2026-08-15T10:23:33.327006Z","submitted_at":"2024-12-17T11:42:40Z","title":"Accurate waveforms for eccentric, aligned-spin binary black holes: The multipolar effective-one-body model SEOBNRv5EHM","version":2},"reference_index":195,"source":"pdf_text","source_observed_at":"2026-08-11T13:49:13.398699Z"},"links":{"cited_paper":"/paper/2101.11033","citing_paper":"/paper/2412.12823"},"observation_digest":"sha256:8c9419768dddc24f0a49f5c717a90120501d6c779d82eda51558d7cb766efd33","observation_id":"39dae480-27d2-4d65-b6a7-0103ca22d41b","resolution":{"observed_at":"2026-08-11T13:49:13.398699Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2101.11033","last_updated":"2021-06-08T12:28:57Z","snapshot_observed_at":"2026-08-17T18:50:31.173570Z","submitted_at":"2021-01-26T19:04:07Z","title":"Adding eccentricity to quasicircular binary-black-hole waveform models","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2101.11033","snapshot_observed_at":"2026-08-11T13:46:55.081196Z","title":"Setyawati and F","venue":null,"work_id":null,"year":2021},"citing_paper":{"arxiv_id":"2412.12831","last_updated":"2025-08-21T18:40:59Z","snapshot_observed_at":"2026-08-15T09:37:12.331902Z","submitted_at":"2024-12-17T11:52:16Z","title":"Third post-Newtonian dynamics for eccentric orbits and aligned spins in the effective-one-body waveform model SEOBNRv5EHM","version":2},"reference_index":175,"source":"pdf_text","source_observed_at":"2026-08-11T13:46:55.081196Z"},"links":{"cited_paper":"/paper/2101.11033","citing_paper":"/paper/2412.12831"},"observation_digest":"sha256:bc79fb79e09d8bfbea2562c4a7a8fb41b2ad4720fff7327b6441f11984b24cf5","observation_id":"116e3ca0-868f-4b4e-a0be-07b51fde10f7","resolution":{"observed_at":"2026-08-11T13:46:55.081196Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2101.11033","last_updated":"2021-06-08T12:28:57Z","snapshot_observed_at":"2026-08-17T18:50:31.173570Z","submitted_at":"2021-01-26T19:04:07Z","title":"Adding eccentricity to quasicircular binary-black-hole waveform models","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2101.11033","snapshot_observed_at":"2026-08-09T11:24:09.492552Z","title":"Adding eccentricity to quasicircular binary-black-hole waveform models,","venue":null,"work_id":null,"year":2021},"citing_paper":{"arxiv_id":"2502.02739","last_updated":"2026-06-18T21:58:44Z","snapshot_observed_at":"2026-08-17T12:36:13.463991Z","submitted_at":"2025-02-04T21:57:30Z","title":"Post-Newtonian theory-inspired framework for characterizing eccentricity in gravitational waveforms","version":2},"reference_index":41,"source":"pdf_text","source_observed_at":"2026-08-09T11:24:09.492552Z"},"links":{"cited_paper":"/paper/2101.11033","citing_paper":"/paper/2502.02739"},"observation_digest":"sha256:2f52b1427a79eb9384d917d73732b0b4b0d64dcfc9d1b3e2a4736e34f89cf477","observation_id":"fc2e7d41-1240-4202-8700-674378e72807","resolution":{"observed_at":"2026-08-09T11:24:09.492552Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2101.11033","last_updated":"2021-06-08T12:28:57Z","snapshot_observed_at":"2026-08-17T18:50:31.173570Z","submitted_at":"2021-01-26T19:04:07Z","title":"Adding eccentricity to quasicircular binary-black-hole waveform models","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2101.11033","snapshot_observed_at":"2026-08-16T12:37:52.029988Z","title":"Adding eccentricity to quasicircular binary-black-hole waveform models,","venue":null,"work_id":null,"year":2021},"citing_paper":{"arxiv_id":"2504.12420","last_updated":"2025-04-16T18:36:59Z","snapshot_observed_at":"2026-08-17T23:02:45.574461Z","submitted_at":"2025-04-16T18:36:59Z","title":"gwharmone: first data-driven surrogate for eccentric harmonics in binary black hole merger waveforms","version":1},"reference_index":47,"source":"pdf_text","source_observed_at":"2026-08-16T12:37:52.029988Z"},"links":{"cited_paper":"/paper/2101.11033","citing_paper":"/paper/2504.12420"},"observation_digest":"sha256:7a2d5d05aa10ae710e01b77310a14201a1e9383110ecb12035e87eb266891148","observation_id":"2f6d35f0-0f1a-47bd-8cef-a57650206ee5","resolution":{"observed_at":"2026-08-16T12:37:52.029988Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2101.11033","last_updated":"2021-06-08T12:28:57Z","snapshot_observed_at":"2026-08-17T18:50:31.173570Z","submitted_at":"2021-01-26T19:04:07Z","title":"Adding eccentricity to quasicircular binary-black-hole waveform models","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2101.11033","snapshot_observed_at":"2026-08-16T12:40:19.761856Z","title":"Adding eccentricity to quasicircular binary-black-hole waveform models,","venue":null,"work_id":null,"year":2021},"citing_paper":{"arxiv_id":"2504.12469","last_updated":"2026-06-18T21:54:14Z","snapshot_observed_at":"2026-08-17T23:02:42.801571Z","submitted_at":"2025-04-16T20:16:35Z","title":"Data-driven extraction, phenomenology and modeling of eccentric harmonics in binary black hole merger waveforms","version":2},"reference_index":59,"source":"pdf_text","source_observed_at":"2026-08-16T12:40:19.761856Z"},"links":{"cited_paper":"/paper/2101.11033","citing_paper":"/paper/2504.12469"},"observation_digest":"sha256:1b59da8f04d2c0958dcc0e0a5aac8d5f0e81ff25d9743f3cbadddb2ae172a238","observation_id":"2be8bb46-5985-4776-98e8-c43b0cd2f6df","resolution":{"observed_at":"2026-08-16T12:40:19.761856Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2101.11033","last_updated":"2021-06-08T12:28:57Z","snapshot_observed_at":"2026-08-17T18:50:31.173570Z","submitted_at":"2021-01-26T19:04:07Z","title":"Adding eccentricity to quasicircular binary-black-hole waveform models","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2101.11033","snapshot_observed_at":"2026-08-04T13:34:57.491129Z","title":"Setyawati and F","venue":null,"work_id":null,"year":2021},"citing_paper":{"arxiv_id":"2510.00116","last_updated":"2026-07-21T22:58:27Z","snapshot_observed_at":"2026-08-14T02:13:36.463953Z","submitted_at":"2025-09-30T18:00:25Z","title":"Chase Orbits, not Time: A Scalable Paradigm for Long-Duration Eccentric Gravitational-Wave Surrogates","version":3},"reference_index":72,"source":"pdf_text","source_observed_at":"2026-08-04T13:34:57.491129Z"},"links":{"cited_paper":"/paper/2101.11033","citing_paper":"/paper/2510.00116"},"observation_digest":"sha256:791a8ebdf9c953d6992013bc8409dd128e084a127d010844eb9375414bf5109b","observation_id":"19e56e2b-27e7-4d11-a506-b549ab13994b","resolution":{"observed_at":"2026-08-04T13:34:57.491129Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2101.11033","last_updated":"2021-06-08T12:28:57Z","snapshot_observed_at":"2026-08-17T18:50:31.173570Z","submitted_at":"2021-01-26T19:04:07Z","title":"Adding eccentricity to quasicircular binary-black-hole waveform models","version":2},"cited_work":{"arxiv_id":"2101.11033","doi":null,"metadata_source":"arxiv_reference","pith_arxiv_id":"2101.11033","snapshot_observed_at":"2026-06-29T11:03:19.205500Z","title":"Setyawati and F","venue":null,"work_id":"491dae92-70e5-4df1-b634-d24cc5b8b978","year":2021},"citing_paper":{"arxiv_id":"2604.17868","last_updated":"2026-04-20T06:28:06Z","snapshot_observed_at":"2026-08-16T22:39:46.169646Z","submitted_at":"2026-04-20T06:28:06Z","title":"Including higher-order modes in a quadrupolar eccentric numerical relativity surrogate using universal eccentric modulation functions","version":1},"reference_index":71,"source":"pdf_text","source_observed_at":"2026-05-10T04:38:37.066802Z"},"links":{"cited_paper":"/paper/2101.11033","citing_paper":"/paper/2604.17868"},"observation_digest":"sha256:fea8eb15dc86f46d3125b4b8a88c3ca751ae518c432d8fc35195d08324beacc0","observation_id":"a8cbf8c0-c521-4080-a474-9b47f046d553","resolution":{"observed_at":"2026-05-10T12:10:22.511689Z","resolver_source":"arxiv_id","status":"metadata_mismatch"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-17T06:30:58.91139+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-17T06:30:58.91139+00:00","source":"crossref"},{"observed_at":"2026-08-17T06:30:54.323127+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":{"arxiv_id":"2101.11033","last_updated":"2021-06-08T12:28:57Z","snapshot_observed_at":"2026-08-17T18:50:31.173570Z","submitted_at":"2021-01-26T19:04:07Z","title":"Adding eccentricity to quasicircular binary-black-hole waveform models","version":2},"cited_work":{"arxiv_id":"2101.11033","doi":null,"metadata_source":"arxiv_reference","pith_arxiv_id":"2101.11033","snapshot_observed_at":"2026-06-29T11:03:19.205500Z","title":"Setyawati and F","venue":null,"work_id":"491dae92-70e5-4df1-b634-d24cc5b8b978","year":2021},"citing_paper":{"arxiv_id":"2605.28715","last_updated":"2026-05-27T16:38:09Z","snapshot_observed_at":"2026-08-17T11:57:09.898577Z","submitted_at":"2026-05-27T16:38:09Z","title":"Accurate waveforms for generic planar-orbit binary black holes: The multipolar effective-one-body model SEOBNRv6EHM","version":1},"reference_index":190,"source":"pdf_text","source_observed_at":"2026-06-29T10:39:57.468339Z"},"links":{"cited_paper":"/paper/2101.11033","citing_paper":"/paper/2605.28715"},"observation_digest":"sha256:bdefe67c7b9757a7320c36e027ab68436ec25e7f22f4e5d299a3bbd2e8b29638","observation_id":"acdd2968-a228-4698-baad-5743998b37dc","resolution":{"observed_at":"2026-06-29T11:03:19.207069Z","resolver_source":"arxiv_id","status":"verified_exact"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-17T06:30:58.91139+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-17T06:30:58.91139+00:00","source":"crossref"},{"observed_at":"2026-08-17T06:30:54.323127+00:00","source":"retraction_watch"}],"state":"measured"}}],"links":{"evidence":"/evidence","html":"/paper/2101.11033/citation-record","integrity":"/paper/2101.11033/integrity","json":"/paper/2101.11033/citation-record.json","paper":"/paper/2101.11033"},"outbound":[],"paper":{"arxiv_id":"2101.11033","last_updated":"2021-06-08T12:28:57Z","latest_version":2,"primary_category":"gr-qc","snapshot_observed_at":"2026-08-17T18:50:31.173570Z","submitted_at":"2021-01-26T19:04:07Z","title":"Adding eccentricity to quasicircular binary-black-hole waveform models"},"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":"2026-08-17T06:30:58.91139+00:00","source":"crossref"},{"observed_at":"2026-08-17T06:30:54.323127+00:00","source":"retraction_watch"}],"thesis":"As of 17 August 2026, this Paper Citation Record lists 0 of 0 outbound references and 10 inbound Pith citation observations for arXiv:2101.11033."}