{"as_of":"2026-08-10T02:53:00Z","caps":{"database_statements":6,"inbound":100,"outbound":100},"context_digest":"sha256:2c72a54444e759ab83ec8e507dda1921d696e3bf07c70249bab88f4f3c9a8737","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":5,"lane":"standing_notices","note":"One-hop event checks from named stored sources.","records_observed":5,"source":"scholarly_work_events, retraction_status_cache","source_observed_at":"2026-08-09T06:31:02.800959+00:00","state":"measured"},{"denominator":5,"lane":"inbound_itemization","note":"Pith citing papers itemized under the disclosed page cap.","records_observed":5,"source":"paper_references, paper_reference_links","source_observed_at":"2026-08-03T06:36:29.175530Z","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":"2026-07-01T13:25:45.798696Z","state":"measured"}],"external_citation_measurements":[],"inbound":[{"citation":{"cited_paper":{"arxiv_id":"2206.14399","last_updated":"2023-08-10T08:41:40Z","snapshot_observed_at":"2026-07-06T13:25:47.414878Z","submitted_at":"2022-06-29T04:42:03Z","title":"SgrA$^{*}$ spin and mass estimates through the detection of an extremely large mass-ratio inspiral","version":2},"cited_work":{"arxiv_id":"2206.14399","doi":null,"metadata_source":"arxiv_reference","pith_arxiv_id":"2206.14399","snapshot_observed_at":"2026-07-01T13:25:45.798696Z","title":"Vazquez-Aceves, Y","venue":null,"work_id":"c54c82da-be1f-4b00-9f21-00138b5f3e2a","year":2023},"citing_paper":{"arxiv_id":"2311.01300","last_updated":"2026-05-01T11:22:19Z","snapshot_observed_at":"2026-07-06T02:11:23.670680Z","submitted_at":"2023-11-02T15:15:33Z","title":"Waveform Modelling for the Laser Interferometer Space Antenna","version":3},"reference_index":74,"source":"pdf_text","source_observed_at":"2026-05-24T05:21:16.199631Z"},"links":{"cited_paper":"/paper/2206.14399","citing_paper":"/paper/2311.01300"},"observation_digest":"sha256:27857d66a8190bbc913c025135907cf3e8053229b254313328aae5f824a51d69","observation_id":"c9d655cc-e143-44b5-927c-fe9040aea14c","resolution":{"observed_at":"2026-05-24T05:23:56.941858Z","resolver_source":"arxiv_id","status":"verified_exact"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-09T06:31:02.800959+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-09T06:31:02.800959+00:00","source":"crossref"},{"observed_at":"2026-08-09T06:30:57.326959+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":{"arxiv_id":"2206.14399","last_updated":"2023-08-10T08:41:40Z","snapshot_observed_at":"2026-07-06T13:25:47.414878Z","submitted_at":"2022-06-29T04:42:03Z","title":"SgrA$^{*}$ spin and mass estimates through the detection of an extremely large mass-ratio inspiral","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2206.14399","snapshot_observed_at":"2026-08-03T06:36:29.175530Z","title":"Vazquez-Aceves, Y","venue":null,"work_id":null,"year":2023},"citing_paper":{"arxiv_id":"2601.22464","last_updated":"2026-07-27T02:13:36Z","snapshot_observed_at":"2026-08-05T06:05:50.516736Z","submitted_at":"2026-01-30T02:22:22Z","title":"Constructing a gravitational wave analysis pipeline for extremely large mass ratio inspirals","version":2},"reference_index":9,"source":"pdf_text","source_observed_at":"2026-08-03T06:36:29.175530Z"},"links":{"cited_paper":"/paper/2206.14399","citing_paper":"/paper/2601.22464"},"observation_digest":"sha256:7cc45d7e4db562282e80b710e1ae5d424a7bb45b59af3516cf51f1017e49f701","observation_id":"e6356ad8-2d84-43f2-b755-7187a8d2ce4e","resolution":{"observed_at":"2026-08-03T06:36:29.175530Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2206.14399","last_updated":"2023-08-10T08:41:40Z","snapshot_observed_at":"2026-07-06T13:25:47.414878Z","submitted_at":"2022-06-29T04:42:03Z","title":"SgrA$^{*}$ spin and mass estimates through the detection of an extremely large mass-ratio inspiral","version":2},"cited_work":{"arxiv_id":"2206.14399","doi":null,"metadata_source":"arxiv_reference","pith_arxiv_id":"2206.14399","snapshot_observed_at":"2026-07-01T13:25:45.798696Z","title":"Vazquez-Aceves, Y","venue":null,"work_id":"c54c82da-be1f-4b00-9f21-00138b5f3e2a","year":2023},"citing_paper":{"arxiv_id":"2605.05362","last_updated":"2026-06-04T15:01:39Z","snapshot_observed_at":"2026-07-06T02:11:23.670680Z","submitted_at":"2026-05-06T18:40:43Z","title":"Constraining Lorentz symmetry breaking in bumblebee gravity with extreme mass-ratio inspirals","version":1},"reference_index":25,"source":"pdf_text","source_observed_at":"2026-05-08T16:15:50.585102Z"},"links":{"cited_paper":"/paper/2206.14399","citing_paper":"/paper/2605.05362"},"observation_digest":"sha256:2c3773e6dc24f1490fd517c693cd720e9518916793dbe4e3bfbf1a49f0d987e2","observation_id":"e15bacdc-3a31-47e7-acca-a7eb4a950164","resolution":{"observed_at":"2026-05-11T18:21:07.827489Z","resolver_source":"arxiv_id","status":"verified_exact"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-09T06:31:02.800959+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-09T06:31:02.800959+00:00","source":"crossref"},{"observed_at":"2026-08-09T06:30:57.326959+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":{"arxiv_id":"2206.14399","last_updated":"2023-08-10T08:41:40Z","snapshot_observed_at":"2026-07-06T13:25:47.414878Z","submitted_at":"2022-06-29T04:42:03Z","title":"SgrA$^{*}$ spin and mass estimates through the detection of an extremely large mass-ratio inspiral","version":2},"cited_work":{"arxiv_id":"2206.14399","doi":null,"metadata_source":"arxiv_reference","pith_arxiv_id":"2206.14399","snapshot_observed_at":"2026-07-01T13:25:45.798696Z","title":"Vazquez-Aceves, Y","venue":null,"work_id":"c54c82da-be1f-4b00-9f21-00138b5f3e2a","year":2023},"citing_paper":{"arxiv_id":"2605.05362","last_updated":"2026-06-04T15:01:39Z","snapshot_observed_at":"2026-07-06T02:11:23.670680Z","submitted_at":"2026-05-06T18:40:43Z","title":"Constraining Lorentz symmetry breaking in bumblebee gravity with extreme mass-ratio inspirals","version":2},"reference_index":25,"source":"pdf_text","source_observed_at":"2026-05-11T01:12:19.470529Z"},"links":{"cited_paper":"/paper/2206.14399","citing_paper":"/paper/2605.05362"},"observation_digest":"sha256:466ab50ef609bd97d66e2570bb8d2e420461bb1ea7ecff074fe706084c0f2515","observation_id":"1dd1de1d-992b-440b-b81a-bf7899b79f8e","resolution":{"observed_at":"2026-05-11T04:36:00.423974Z","resolver_source":"arxiv_id","status":"verified_exact"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-09T06:31:02.800959+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-09T06:31:02.800959+00:00","source":"crossref"},{"observed_at":"2026-08-09T06:30:57.326959+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":{"arxiv_id":"2206.14399","last_updated":"2023-08-10T08:41:40Z","snapshot_observed_at":"2026-07-06T13:25:47.414878Z","submitted_at":"2022-06-29T04:42:03Z","title":"SgrA$^{*}$ spin and mass estimates through the detection of an extremely large mass-ratio inspiral","version":2},"cited_work":{"arxiv_id":"2206.14399","doi":null,"metadata_source":"arxiv_reference","pith_arxiv_id":"2206.14399","snapshot_observed_at":"2026-07-01T13:25:45.798696Z","title":"Vazquez-Aceves, Y","venue":null,"work_id":"c54c82da-be1f-4b00-9f21-00138b5f3e2a","year":2023},"citing_paper":{"arxiv_id":"2605.05362","last_updated":"2026-06-04T15:01:39Z","snapshot_observed_at":"2026-07-06T02:11:23.670680Z","submitted_at":"2026-05-06T18:40:43Z","title":"Constraining Lorentz symmetry breaking in bumblebee gravity with extreme mass-ratio inspirals","version":3},"reference_index":26,"source":"pdf_text","source_observed_at":"2026-06-30T23:15:57.036633Z"},"links":{"cited_paper":"/paper/2206.14399","citing_paper":"/paper/2605.05362"},"observation_digest":"sha256:fc5bb5d192917bcfaa53dc08ea5d6d2b941cee2f68ac311966d43ccee38e3448","observation_id":"3e13f941-2759-4c0b-8364-1ec3ed9c901f","resolution":{"observed_at":"2026-07-01T13:25:45.800078Z","resolver_source":"arxiv_id","status":"verified_exact"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-09T06:31:02.800959+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-09T06:31:02.800959+00:00","source":"crossref"},{"observed_at":"2026-08-09T06:30:57.326959+00:00","source":"retraction_watch"}],"state":"measured"}}],"links":{"evidence":"/evidence","html":"/paper/2206.14399/citation-record","integrity":"/paper/2206.14399/integrity","json":"/paper/2206.14399/citation-record.json","paper":"/paper/2206.14399"},"outbound":[],"paper":{"arxiv_id":"2206.14399","last_updated":"2023-08-10T08:41:40Z","latest_version":2,"primary_category":"astro-ph.HE","snapshot_observed_at":"2026-07-06T13:25:47.414878Z","submitted_at":"2022-06-29T04:42:03Z","title":"SgrA$^{*}$ spin and mass estimates through the detection of an extremely large mass-ratio inspiral"},"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":"2026-08-09T06:31:02.800959+00:00","source":"crossref"},{"observed_at":"2026-08-09T06:30:57.326959+00:00","source":"retraction_watch"}],"thesis":"As of 10 August 2026, this Paper Citation Record lists 0 of 0 outbound references and 5 inbound Pith citation observations for arXiv:2206.14399."}