{"as_of":"2026-08-11T19:53:00Z","caps":{"database_statements":6,"inbound":100,"outbound":100},"context_digest":"sha256:2f8b5162f2341a20d0718d1924c55a65ff63bbcc0fc0d15a17ca45d196eaf79e","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":8,"lane":"standing_notices","note":"One-hop event checks from named stored sources.","records_observed":8,"source":"scholarly_work_events, retraction_status_cache","source_observed_at":"2026-08-11T06:34:44.6726+00:00","state":"measured"},{"denominator":8,"lane":"inbound_itemization","note":"Pith citing papers itemized under the disclosed page cap.","records_observed":8,"source":"paper_references, paper_reference_links","source_observed_at":"2026-08-11T15:59:26.666306Z","state":"measured"},{"denominator":1,"lane":"external_citation_measurements","note":"A source-named dated measurement, never combined with another source.","records_observed":1,"source":"arxiv_reference","source_observed_at":"2026-08-05T02:28:24.338817Z","state":"measured"}],"external_citation_measurements":[{"count":3,"observed_at":"2026-08-05T02:28:24.338817Z","source":"arxiv_reference"}],"inbound":[{"citation":{"cited_paper":{"arxiv_id":"2311.08453","last_updated":"2024-09-08T10:14:41Z","snapshot_observed_at":"2026-08-11T09:09:24.732973Z","submitted_at":"2023-11-14T19:00:01Z","title":"Asteroseismic Modelling of Fast Rotators and its Opportunities for Astrophysics","version":4},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2311.08453","snapshot_observed_at":"2026-08-11T15:59:26.666306Z","title":"& Tkachenko , A","venue":null,"work_id":null,"year":2024},"citing_paper":{"arxiv_id":"2412.10508","last_updated":"2024-12-13T19:00:46Z","snapshot_observed_at":"2026-08-11T15:51:41.762605Z","submitted_at":"2024-12-13T19:00:46Z","title":"MOCKA -- A PLATO mock asteroseismic catalogue: Simulations for gravity-mode oscillators","version":1},"reference_index":7,"source":"arxiv_source","source_observed_at":"2026-08-11T15:59:26.666306Z"},"links":{"cited_paper":"/paper/2311.08453","citing_paper":"/paper/2412.10508"},"observation_digest":"sha256:b713d21f98b8faee0b22a54c6b5f6ee78d00c9195cf8cf39ff9157aaba323b89","observation_id":"e9368298-bc4c-428e-ad72-4c286168e656","resolution":{"observed_at":"2026-08-11T15:59:26.666306Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2311.08453","last_updated":"2024-09-08T10:14:41Z","snapshot_observed_at":"2026-08-11T09:09:24.732973Z","submitted_at":"2023-11-14T19:00:01Z","title":"Asteroseismic Modelling of Fast Rotators and its Opportunities for Astrophysics","version":4},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2311.08453","snapshot_observed_at":"2026-08-06T22:43:41.432308Z","title":"2023, arXiv e-prints, arXiv:2311.08453","venue":null,"work_id":null,"year":2023},"citing_paper":{"arxiv_id":"2506.20868","last_updated":"2025-06-25T22:38:06Z","snapshot_observed_at":"2026-08-10T12:10:40.083244Z","submitted_at":"2025-06-25T22:38:06Z","title":"Physics Of Eclipsing Binaries. IX. Spectroscopic module","version":1},"reference_index":6,"source":"arxiv_source","source_observed_at":"2026-08-06T22:43:41.432308Z"},"links":{"cited_paper":"/paper/2311.08453","citing_paper":"/paper/2506.20868"},"observation_digest":"sha256:4c08c658014db5a48ff539ae1fa7187f0f2e0c194a96e247f728f110d4018178","observation_id":"b30c8144-abbd-48dd-a295-25ffbd5b29b1","resolution":{"observed_at":"2026-08-06T22:43:41.432308Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2311.08453","last_updated":"2024-09-08T10:14:41Z","snapshot_observed_at":"2026-08-11T09:09:24.732973Z","submitted_at":"2023-11-14T19:00:01Z","title":"Asteroseismic Modelling of Fast Rotators and its Opportunities for Astrophysics","version":4},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2311.08453","snapshot_observed_at":"2026-08-06T20:22:25.320709Z","title":null,"venue":null,"work_id":null,"year":2024},"citing_paper":{"arxiv_id":"2507.03093","last_updated":"2025-07-03T18:05:40Z","snapshot_observed_at":"2026-08-08T13:57:38.124958Z","submitted_at":"2025-07-03T18:05:40Z","title":"From stellar light to astrophysical insight: automating variable star research with machine learning","version":1},"reference_index":5,"source":"arxiv_source","source_observed_at":"2026-08-06T20:22:25.320709Z"},"links":{"cited_paper":"/paper/2311.08453","citing_paper":"/paper/2507.03093"},"observation_digest":"sha256:e0d2f74e95f17b59cfece93d2a12ea9cbdd3d3a025be3f977d95e24a45526d1d","observation_id":"6f4659ea-18cd-4efd-8efc-f1ef4fd674fc","resolution":{"observed_at":"2026-08-06T20:22:25.320709Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2311.08453","last_updated":"2024-09-08T10:14:41Z","snapshot_observed_at":"2026-08-11T09:09:24.732973Z","submitted_at":"2023-11-14T19:00:01Z","title":"Asteroseismic Modelling of Fast Rotators and its Opportunities for Astrophysics","version":4},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2311.08453","snapshot_observed_at":"2026-08-06T20:11:46.309431Z","title":null,"venue":null,"work_id":null,"year":2024},"citing_paper":{"arxiv_id":"2507.03561","last_updated":"2026-05-31T13:36:53Z","snapshot_observed_at":"2026-08-06T20:04:34.189728Z","submitted_at":"2025-07-04T13:12:36Z","title":"Modelling $\\delta$ Scuti pulsations: A new grid of p, g, and f modes across pre-main-sequence to post-main-sequence evolution","version":5},"reference_index":3,"source":"arxiv_source","source_observed_at":"2026-08-06T20:11:46.309431Z"},"links":{"cited_paper":"/paper/2311.08453","citing_paper":"/paper/2507.03561"},"observation_digest":"sha256:05f9cbbecdcc8101afec7432880b41e44996ae7248816d79995e14488e9d10a3","observation_id":"da99b968-c83c-401a-accd-81feef4d03a1","resolution":{"observed_at":"2026-08-06T20:11:46.309431Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2311.08453","last_updated":"2024-09-08T10:14:41Z","snapshot_observed_at":"2026-08-11T09:09:24.732973Z","submitted_at":"2023-11-14T19:00:01Z","title":"Asteroseismic Modelling of Fast Rotators and its Opportunities for Astrophysics","version":4},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2311.08453","snapshot_observed_at":"2026-08-06T18:53:20.223364Z","title":"2023, arXiv e-prints, arXiv:2311.08453, doi: 10.48550/arXiv.2311.08453","venue":null,"work_id":null,"year":2023},"citing_paper":{"arxiv_id":"2507.06989","last_updated":"2025-07-09T16:13:26Z","snapshot_observed_at":"2026-08-08T02:41:26.932545Z","submitted_at":"2025-07-09T16:13:26Z","title":"Sloan Digital Sky Survey-V: Pioneering Panoptic Spectroscopy","version":1},"reference_index":4,"source":"pdf_text","source_observed_at":"2026-08-06T18:53:20.223364Z"},"links":{"cited_paper":"/paper/2311.08453","citing_paper":"/paper/2507.06989"},"observation_digest":"sha256:6017401ee5929b493be6cc12e8923023791f1aeaef17b070254e98da0da41741","observation_id":"6a72eec7-070a-4544-9bb2-af3d62b44f48","resolution":{"observed_at":"2026-08-06T18:53:20.223364Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2311.08453","last_updated":"2024-09-08T10:14:41Z","snapshot_observed_at":"2026-08-11T09:09:24.732973Z","submitted_at":"2023-11-14T19:00:01Z","title":"Asteroseismic Modelling of Fast Rotators and its Opportunities for Astrophysics","version":4},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2311.08453","snapshot_observed_at":"2026-08-03T20:37:51.141118Z","title":"A&A692, 1 (2024) https://doi.org/10.1051/0004-6361/202348575 arXiv:2311.08453 [astro-ph.SR]","venue":null,"work_id":null,"year":2024},"citing_paper":{"arxiv_id":"2511.19196","last_updated":"2026-06-10T08:46:59Z","snapshot_observed_at":"2026-08-05T20:39:39.326640Z","submitted_at":"2025-11-24T15:05:39Z","title":"Observing bright pulsating white dwarfs with PLATO: A new window into the late stages of stellar evolution","version":2},"reference_index":86,"source":"pdf_text","source_observed_at":"2026-08-03T20:37:51.141118Z"},"links":{"cited_paper":"/paper/2311.08453","citing_paper":"/paper/2511.19196"},"observation_digest":"sha256:7337c08bc818cc955f8be051c11f51a59e92c931886a396652d8f0215162c3db","observation_id":"5976207d-0510-4c8d-8759-48ac9dc89562","resolution":{"observed_at":"2026-08-03T20:37:51.141118Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2311.08453","last_updated":"2024-09-08T10:14:41Z","snapshot_observed_at":"2026-08-11T09:09:24.732973Z","submitted_at":"2023-11-14T19:00:01Z","title":"Asteroseismic Modelling of Fast Rotators and its Opportunities for Astrophysics","version":4},"cited_work":{"arxiv_id":"2311.08453","doi":"10.48550/arxiv.2311.08453","metadata_source":"arxiv_reference","pith_arxiv_id":"2311.08453","snapshot_observed_at":"2026-08-05T02:28:24.338817Z","title":"arXiv e-prints , keywords =","venue":"arXiv (Cornell University)","work_id":"fc1d24cc-3d34-47f5-93de-bdb4bbaa2741","year":null},"citing_paper":{"arxiv_id":"2605.04801","last_updated":"2026-05-06T11:52:26Z","snapshot_observed_at":"2026-07-06T23:17:33.252539Z","submitted_at":"2026-05-06T11:52:26Z","title":"Contribution of interstellar objects to local dark matter density","version":1},"reference_index":227,"source":"arxiv_source","source_observed_at":"2026-05-08T17:16:18.868405Z"},"links":{"cited_paper":"/paper/2311.08453","citing_paper":"/paper/2605.04801"},"observation_digest":"sha256:5f1977696132473d15e69a5b619024d0fb16f59fdf4aea0272f44279b80c7745","observation_id":"7a3657b6-6e4b-4b1e-870b-42045fda9acc","resolution":{"observed_at":"2026-05-08T17:18:39.782829Z","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"}},{"citation":{"cited_paper":{"arxiv_id":"2311.08453","last_updated":"2024-09-08T10:14:41Z","snapshot_observed_at":"2026-08-11T09:09:24.732973Z","submitted_at":"2023-11-14T19:00:01Z","title":"Asteroseismic Modelling of Fast Rotators and its Opportunities for Astrophysics","version":4},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2311.08453","snapshot_observed_at":"2026-08-01T04:30:07.969241Z","title":", keywords =","venue":null,"work_id":null,"year":null},"citing_paper":{"arxiv_id":"2607.22814","last_updated":"2026-07-24T18:00:01Z","snapshot_observed_at":"2026-08-04T20:17:39.597855Z","submitted_at":"2026-07-24T18:00:01Z","title":"Charting the Galactic Underworld I: Comprehensive simulations of the kinematics, rates, and demographics of Milky Way black holes","version":1},"reference_index":111,"source":"arxiv_source","source_observed_at":"2026-08-01T04:30:07.969241Z"},"links":{"cited_paper":"/paper/2311.08453","citing_paper":"/paper/2607.22814"},"observation_digest":"sha256:022673120ad28997ce486c9cd8251a171c3e05836f3d3b635b1be7663f66222e","observation_id":"513eb49b-6fc7-4784-b17e-915ea031f243","resolution":{"observed_at":"2026-08-01T04:30:07.969241Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}}],"links":{"evidence":"/evidence","html":"/paper/2311.08453/citation-record","integrity":"/paper/2311.08453/integrity","json":"/paper/2311.08453/citation-record.json","paper":"/paper/2311.08453"},"outbound":[],"paper":{"arxiv_id":"2311.08453","last_updated":"2024-09-08T10:14:41Z","latest_version":4,"primary_category":"astro-ph.SR","snapshot_observed_at":"2026-08-11T09:09:24.732973Z","submitted_at":"2023-11-14T19:00:01Z","title":"Asteroseismic Modelling of Fast Rotators and its Opportunities for Astrophysics"},"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 8 inbound Pith citation observations for arXiv:2311.08453."}