{"as_of":"2026-08-11T09:10:00Z","caps":{"database_statements":6,"inbound":100,"outbound":100},"context_digest":"sha256:516eb3b6e1311c8b3a5120aa732008e145fa0749b652ad403dddea488bf93ed9","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":3,"lane":"standing_notices","note":"One-hop event checks from named stored sources.","records_observed":3,"source":"scholarly_work_events, retraction_status_cache","source_observed_at":"2026-08-11T06:34:44.6726+00:00","state":"measured"},{"denominator":3,"lane":"inbound_itemization","note":"Pith citing papers itemized under the disclosed page cap.","records_observed":3,"source":"paper_references, paper_reference_links","source_observed_at":"2026-08-10T13:27:10.573765Z","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":"2026-07-03T22:39:01.823443Z","state":"measured"}],"external_citation_measurements":[],"inbound":[{"citation":{"cited_paper":{"arxiv_id":"2110.09254","last_updated":"2021-11-05T12:29:11Z","snapshot_observed_at":"2026-07-06T11:59:04.643339Z","submitted_at":"2021-09-28T11:38:30Z","title":"An accurate analytical fit to the gravitational-wave inspiral duration for eccentric binaries","version":3},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2110.09254","snapshot_observed_at":"2026-08-10T13:27:10.573765Z","title":"An Accurate Analytical Fit to the Gravitational-wave Inspiral Duration for Eccentric Bina- ries,","venue":null,"work_id":null,"year":2021},"citing_paper":{"arxiv_id":"2501.16422","last_updated":"2025-03-26T13:39:24Z","snapshot_observed_at":"2026-08-11T02:35:26.695721Z","submitted_at":"2025-01-27T19:00:01Z","title":"Gravitational wave inference of star cluster properties from intermediate-mass black hole mergers","version":2},"reference_index":85,"source":"pdf_text","source_observed_at":"2026-08-10T13:27:10.573765Z"},"links":{"cited_paper":"/paper/2110.09254","citing_paper":"/paper/2501.16422"},"observation_digest":"sha256:fb9fe96e2f549064c9e9a5a5e80a705e75e24451ec5ecccb3f7b53e88af9c1a0","observation_id":"aaf788b7-d6e1-4c61-9ffe-d3fa90a5f9ad","resolution":{"observed_at":"2026-08-10T13:27:10.573765Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2110.09254","last_updated":"2021-11-05T12:29:11Z","snapshot_observed_at":"2026-07-06T11:59:04.643339Z","submitted_at":"2021-09-28T11:38:30Z","title":"An accurate analytical fit to the gravitational-wave inspiral duration for eccentric binaries","version":3},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2110.09254","snapshot_observed_at":"2026-08-03T14:34:34.561929Z","title":"An Accurate Analytical Fit to the Gravitational-wave Inspiral Duration for Eccentric Binaries.Research Notes of the American Astronomical Society5, 223 (2021)","venue":null,"work_id":null,"year":2021},"citing_paper":{"arxiv_id":"2512.20054","last_updated":"2026-07-20T11:38:48Z","snapshot_observed_at":"2026-08-04T23:37:26.854248Z","submitted_at":"2025-12-23T05:04:02Z","title":"Stable mass transfer in massive binaries leading to merging black holes","version":2},"reference_index":117,"source":"pdf_text","source_observed_at":"2026-08-03T14:34:34.561929Z"},"links":{"cited_paper":"/paper/2110.09254","citing_paper":"/paper/2512.20054"},"observation_digest":"sha256:f4a816c57a0431b14786013e9fa6b5802c8a426150d083d03388ed9520d17a15","observation_id":"ad7f9c47-54c4-4866-bf16-d8f9743a9e43","resolution":{"observed_at":"2026-08-03T14:34:34.561929Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2110.09254","last_updated":"2021-11-05T12:29:11Z","snapshot_observed_at":"2026-07-06T11:59:04.643339Z","submitted_at":"2021-09-28T11:38:30Z","title":"An accurate analytical fit to the gravitational-wave inspiral duration for eccentric binaries","version":3},"cited_work":{"arxiv_id":"2110.09254","doi":null,"metadata_source":"arxiv_reference","pith_arxiv_id":"2110.09254","snapshot_observed_at":"2026-07-03T22:39:01.823443Z","title":"Mandel, Res","venue":null,"work_id":"ae6272e9-93ca-4de7-b5f8-4b92d4388d46","year":2021},"citing_paper":{"arxiv_id":"2606.18341","last_updated":"2026-06-16T18:00:01Z","snapshot_observed_at":"2026-08-06T05:42:45.715105Z","submitted_at":"2026-06-16T18:00:01Z","title":"Orbital evolution of asymmetric binaries within accreting environments","version":1},"reference_index":51,"source":"pdf_text","source_observed_at":"2026-06-26T23:24:01.303227Z"},"links":{"cited_paper":"/paper/2110.09254","citing_paper":"/paper/2606.18341"},"observation_digest":"sha256:b2175fcfeaf6875f903ef51e6e6eba87808ac6fedbcf85eea30cba979909c913","observation_id":"5b20b6d6-cdc1-497c-bc2f-ce974fbb602a","resolution":{"observed_at":"2026-07-03T22:39:01.824656Z","resolver_source":"arxiv_id","status":"verified_exact"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-11T06:34:44.6726+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-11T06:34:44.6726+00:00","source":"crossref"},{"observed_at":"2026-08-11T06:34:36.301508+00:00","source":"retraction_watch"}],"state":"measured"}}],"links":{"evidence":"/evidence","html":"/paper/2110.09254/citation-record","integrity":"/paper/2110.09254/integrity","json":"/paper/2110.09254/citation-record.json","paper":"/paper/2110.09254"},"outbound":[],"paper":{"arxiv_id":"2110.09254","last_updated":"2021-11-05T12:29:11Z","latest_version":3,"primary_category":"astro-ph.HE","snapshot_observed_at":"2026-07-06T11:59:04.643339Z","submitted_at":"2021-09-28T11:38:30Z","title":"An accurate analytical fit to the gravitational-wave inspiral duration for eccentric binaries"},"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":"2026-08-11T06:34:44.6726+00:00","source":"crossref"},{"observed_at":"2026-08-11T06:34:36.301508+00:00","source":"retraction_watch"}],"thesis":"As of 11 August 2026, this Paper Citation Record lists 0 of 0 outbound references and 3 inbound Pith citation observations for arXiv:2110.09254."}