{"as_of":"2026-08-16T06:02:00Z","caps":{"database_statements":6,"inbound":100,"outbound":100},"context_digest":"sha256:64cea50284fe384aeaaee9a2be92639cc96a3d42af6d8946f96281408c0bf3de","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":6,"lane":"standing_notices","note":"One-hop event checks from named stored sources.","records_observed":6,"source":"scholarly_work_events, retraction_status_cache","source_observed_at":"2026-08-15T06:32:42.880941+00:00","state":"measured"},{"denominator":6,"lane":"inbound_itemization","note":"Pith citing papers itemized under the disclosed page cap.","records_observed":6,"source":"paper_references, paper_reference_links","source_observed_at":"2026-08-15T16:30:11.450740Z","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":"2026-05-19T02:52:00.046332Z","state":"measured"}],"external_citation_measurements":[],"inbound":[{"citation":{"cited_paper":{"arxiv_id":"1702.00872","last_updated":"2020-11-09T14:59:02Z","snapshot_observed_at":"2026-08-14T21:18:17.686253Z","submitted_at":"2017-02-02T23:48:41Z","title":"Post-Newtonian Quasicircular Initial Orbits for Numerical Relativity","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"1702.00872","snapshot_observed_at":"2026-08-14T13:50:47.400181Z","title":"Healy, C","venue":null,"work_id":null,"year":2017},"citing_paper":{"arxiv_id":"1908.04382","last_updated":"2019-08-12T21:03:11Z","snapshot_observed_at":"2026-08-15T06:58:37.857302Z","submitted_at":"2019-08-12T21:03:11Z","title":"Kicking gravitational wave detectors with recoiling black holes","version":1},"reference_index":72,"source":"pdf_text","source_observed_at":"2026-08-14T13:50:47.400181Z"},"links":{"cited_paper":"/paper/1702.00872","citing_paper":"/paper/1908.04382"},"observation_digest":"sha256:a9c7a78045ee405cb10110ea0d50ec66012f47d1a34f2831d6d1723190c26042","observation_id":"6597514c-738a-49f7-a939-f1d3bc771a1b","resolution":{"observed_at":"2026-08-14T13:50:47.400181Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"1702.00872","last_updated":"2020-11-09T14:59:02Z","snapshot_observed_at":"2026-08-14T21:18:17.686253Z","submitted_at":"2017-02-02T23:48:41Z","title":"Post-Newtonian Quasicircular Initial Orbits for Numerical Relativity","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"1702.00872","snapshot_observed_at":"2026-08-09T11:24:09.281122Z","title":"Post-Newtonian Quasicircular Initial Orbits for Nu- merical Relativity,","venue":null,"work_id":null,"year":2017},"citing_paper":{"arxiv_id":"2502.02739","last_updated":"2026-06-18T21:58:44Z","snapshot_observed_at":"2026-08-09T15:01:16.647086Z","submitted_at":"2025-02-04T21:57:30Z","title":"Post-Newtonian theory-inspired framework for characterizing eccentricity in gravitational waveforms","version":2},"reference_index":4,"source":"pdf_text","source_observed_at":"2026-08-09T11:24:09.281122Z"},"links":{"cited_paper":"/paper/1702.00872","citing_paper":"/paper/2502.02739"},"observation_digest":"sha256:b58d6b9af942460a91df1b43a3a7c2f8798744a687202bb128b72bcbc838d811","observation_id":"62be2990-011f-4524-8dd8-abf6a33ab161","resolution":{"observed_at":"2026-08-09T11:24:09.281122Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"1702.00872","last_updated":"2020-11-09T14:59:02Z","snapshot_observed_at":"2026-08-14T21:18:17.686253Z","submitted_at":"2017-02-02T23:48:41Z","title":"Post-Newtonian Quasicircular Initial Orbits for Numerical Relativity","version":2},"cited_work":{"arxiv_id":"1702.00872","doi":null,"metadata_source":"arxiv_reference","pith_arxiv_id":"1702.00872","snapshot_observed_at":"2026-06-05T21:23:00.469572Z","title":"Healy, C","venue":null,"work_id":"56199af3-a5da-4d2a-9a3e-76383d6270c7","year":2017},"citing_paper":{"arxiv_id":"2507.22862","last_updated":"2026-05-01T13:55:06Z","snapshot_observed_at":"2026-07-06T22:05:17.795002Z","submitted_at":"2025-07-30T17:38:27Z","title":"Parameter Estimation with Targeted Eccentric Numerical-Relativity Simulations for GW200208_22 and GW190620","version":2},"reference_index":90,"source":"pdf_text","source_observed_at":"2026-05-19T02:51:11.710911Z"},"links":{"cited_paper":"/paper/1702.00872","citing_paper":"/paper/2507.22862"},"observation_digest":"sha256:f18fcee41f06866292ed589ed01f019e7f3592ba5d533a17270c44a14630fa1c","observation_id":"076486c8-c419-460a-8e84-30e5137851d1","resolution":{"observed_at":"2026-05-19T02:52:00.049397Z","resolver_source":"arxiv_id","status":"verified_exact"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-15T06:32:42.880941+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-15T06:32:42.880941+00:00","source":"crossref"},{"observed_at":"2026-08-15T06:32:39.529945+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":{"arxiv_id":"1702.00872","last_updated":"2020-11-09T14:59:02Z","snapshot_observed_at":"2026-08-14T21:18:17.686253Z","submitted_at":"2017-02-02T23:48:41Z","title":"Post-Newtonian Quasicircular Initial Orbits for Numerical Relativity","version":2},"cited_work":{"arxiv_id":"1702.00872","doi":null,"metadata_source":"arxiv_reference","pith_arxiv_id":"1702.00872","snapshot_observed_at":"2026-06-05T21:23:00.469572Z","title":"Healy, C","venue":null,"work_id":"56199af3-a5da-4d2a-9a3e-76383d6270c7","year":2017},"citing_paper":{"arxiv_id":"2508.21216","last_updated":"2026-04-14T18:55:26Z","snapshot_observed_at":"2026-08-14T14:21:11.574676Z","submitted_at":"2025-08-28T21:11:00Z","title":"Persistence of post-Newtonian amplitude structure in binary black hole mergers","version":2},"reference_index":54,"source":"pdf_text","source_observed_at":"2026-05-18T20:12:03.416788Z"},"links":{"cited_paper":"/paper/1702.00872","citing_paper":"/paper/2508.21216"},"observation_digest":"sha256:e57b434346049fd629ca2e37e16c0f8d559458dc2f3bbc2939c308ced277a676","observation_id":"59669975-5c56-4fdd-83f0-ef7a0448c96d","resolution":{"observed_at":"2026-05-18T20:12:50.478176Z","resolver_source":"arxiv_id","status":"verified_exact"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-15T06:32:42.880941+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-15T06:32:42.880941+00:00","source":"crossref"},{"observed_at":"2026-08-15T06:32:39.529945+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":{"arxiv_id":"1702.00872","last_updated":"2020-11-09T14:59:02Z","snapshot_observed_at":"2026-08-14T21:18:17.686253Z","submitted_at":"2017-02-02T23:48:41Z","title":"Post-Newtonian Quasicircular Initial Orbits for Numerical Relativity","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"1702.00872","snapshot_observed_at":"2026-08-15T16:30:11.450740Z","title":"Healy, C","venue":null,"work_id":null,"year":2017},"citing_paper":{"arxiv_id":"2509.05269","last_updated":"2025-09-05T17:24:50Z","snapshot_observed_at":"2026-08-16T00:35:14.301568Z","submitted_at":"2025-09-05T17:24:50Z","title":"First ICCUB Numerical Relativity Waveform Catalog of Eccentric Black Hole Binaries","version":1},"reference_index":36,"source":"pdf_text","source_observed_at":"2026-08-15T16:30:11.450740Z"},"links":{"cited_paper":"/paper/1702.00872","citing_paper":"/paper/2509.05269"},"observation_digest":"sha256:3b04a0b606ec7040f6b32a827ee3db50aa2c62ce2d5543982a87935d267ec5ef","observation_id":"be82c004-05ca-476a-9da0-140a4ab2d5a0","resolution":{"observed_at":"2026-08-15T16:30:11.450740Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"1702.00872","last_updated":"2020-11-09T14:59:02Z","snapshot_observed_at":"2026-08-14T21:18:17.686253Z","submitted_at":"2017-02-02T23:48:41Z","title":"Post-Newtonian Quasicircular Initial Orbits for Numerical Relativity","version":2},"cited_work":{"arxiv_id":"1702.00872","doi":null,"metadata_source":"arxiv_reference","pith_arxiv_id":"1702.00872","snapshot_observed_at":"2026-06-05T21:23:00.469572Z","title":"Healy, C","venue":null,"work_id":"56199af3-a5da-4d2a-9a3e-76383d6270c7","year":2017},"citing_paper":{"arxiv_id":"2604.17868","last_updated":"2026-04-20T06:28:06Z","snapshot_observed_at":"2026-08-14T00:41:43.153316Z","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":32,"source":"pdf_text","source_observed_at":"2026-05-10T04:38:37.066802Z"},"links":{"cited_paper":"/paper/1702.00872","citing_paper":"/paper/2604.17868"},"observation_digest":"sha256:e2a318d181e50f15c42feda8cc3f015f00d5b8bf44653d15e7f0536cc7dad8b2","observation_id":"d16755a5-453c-4e7f-ac78-739d4388547e","resolution":{"observed_at":"2026-05-10T12:10:22.387216Z","resolver_source":"arxiv_id","status":"metadata_mismatch"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-15T06:32:42.880941+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-15T06:32:42.880941+00:00","source":"crossref"},{"observed_at":"2026-08-15T06:32:39.529945+00:00","source":"retraction_watch"}],"state":"measured"}}],"links":{"evidence":"/evidence","html":"/paper/1702.00872/citation-record","integrity":"/paper/1702.00872/integrity","json":"/paper/1702.00872/citation-record.json","paper":"/paper/1702.00872"},"outbound":[],"paper":{"arxiv_id":"1702.00872","last_updated":"2020-11-09T14:59:02Z","latest_version":2,"primary_category":"gr-qc","snapshot_observed_at":"2026-08-14T21:18:17.686253Z","submitted_at":"2017-02-02T23:48:41Z","title":"Post-Newtonian Quasicircular Initial Orbits for Numerical Relativity"},"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":"2026-08-15T06:32:42.880941+00:00","source":"crossref"},{"observed_at":"2026-08-15T06:32:39.529945+00:00","source":"retraction_watch"}],"thesis":"As of 16 August 2026, this Paper Citation Record lists 0 of 0 outbound references and 6 inbound Pith citation observations for arXiv:1702.00872."}