{"as_of":"2026-08-18T21:15:00Z","caps":{"database_statements":6,"inbound":100,"outbound":100},"context_digest":"sha256:5ad72c989ec0e358c9f95b71578d6f18f062c3c36bf238676414e487fbaaf6a5","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":"2026-08-18T06:34:40.430872+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":"2026-08-16T10:56:15.826689Z","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":1,"observed_at":"2026-08-05T02:28:24.338817Z","source":"arxiv_reference"}],"inbound":[{"citation":{"cited_paper":{"arxiv_id":"2410.05166","last_updated":"2024-10-07T16:23:57Z","snapshot_observed_at":"2026-08-16T13:11:50.621663Z","submitted_at":"2024-10-07T16:23:57Z","title":"Radiation Transport Simulations of Quasi-Periodic Eruptions from Star-Disk Collisions","version":1},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2410.05166","snapshot_observed_at":"2026-08-12T11:42:42.085608Z","title":null,"venue":null,"work_id":null,"year":null},"citing_paper":{"arxiv_id":"2411.18046","last_updated":"2025-04-21T08:41:27Z","snapshot_observed_at":"2026-08-18T16:07:44.593089Z","submitted_at":"2024-11-27T04:31:22Z","title":"Secular evolution of quasi-periodic eruptions","version":3},"reference_index":13,"source":"pdf_text","source_observed_at":"2026-08-12T11:42:42.085608Z"},"links":{"cited_paper":"/paper/2410.05166","citing_paper":"/paper/2411.18046"},"observation_digest":"sha256:eb7d492f4b18a18beea15c1d9984e988b39cb2de274c4ca67befc067131e8fc9","observation_id":"e987d93e-3fd1-4594-9137-e96a6bd6d883","resolution":{"observed_at":"2026-08-12T11:42:42.085608Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2410.05166","last_updated":"2024-10-07T16:23:57Z","snapshot_observed_at":"2026-08-16T13:11:50.621663Z","submitted_at":"2024-10-07T16:23:57Z","title":"Radiation Transport Simulations of Quasi-Periodic Eruptions from Star-Disk Collisions","version":1},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2410.05166","snapshot_observed_at":"2026-08-10T21:59:57.024275Z","title":null,"venue":null,"work_id":null,"year":2024},"citing_paper":{"arxiv_id":"2501.03333","last_updated":"2025-04-28T18:00:23Z","snapshot_observed_at":"2026-08-16T08:25:01.249052Z","submitted_at":"2025-01-06T19:01:43Z","title":"The properties of GSN 069 accretion disk from a joint X-ray and UV spectral analysis: stress-testing quasi-periodic eruption models","version":2},"reference_index":101,"source":"arxiv_source","source_observed_at":"2026-08-10T21:59:57.024275Z"},"links":{"cited_paper":"/paper/2410.05166","citing_paper":"/paper/2501.03333"},"observation_digest":"sha256:c387ab3496307148b5a85e687100230dae263ee2e1dde295ac766f5fe551e1f1","observation_id":"97332b6e-84da-4e60-ac73-7577521f695c","resolution":{"observed_at":"2026-08-10T21:59:57.024275Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2410.05166","last_updated":"2024-10-07T16:23:57Z","snapshot_observed_at":"2026-08-16T13:11:50.621663Z","submitted_at":"2024-10-07T16:23:57Z","title":"Radiation Transport Simulations of Quasi-Periodic Eruptions from Star-Disk Collisions","version":1},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2410.05166","snapshot_observed_at":"2026-08-10T22:03:00.768167Z","title":null,"venue":null,"work_id":null,"year":2024},"citing_paper":{"arxiv_id":"2501.03335","last_updated":"2025-01-23T14:17:08Z","snapshot_observed_at":"2026-08-13T09:13:06.858486Z","submitted_at":"2025-01-06T19:01:47Z","title":"Time-resolved Hubble Space Telescope UV observations of an X-ray quasi-periodic eruption source","version":2},"reference_index":78,"source":"arxiv_source","source_observed_at":"2026-08-10T22:03:00.768167Z"},"links":{"cited_paper":"/paper/2410.05166","citing_paper":"/paper/2501.03335"},"observation_digest":"sha256:8445b584dd26fbf803be541306d1a19e11cb47189be4572d78d0ad7856979e9e","observation_id":"f2b00a19-34c1-4304-ae81-fac5baafbf74","resolution":{"observed_at":"2026-08-10T22:03:00.768167Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2410.05166","last_updated":"2024-10-07T16:23:57Z","snapshot_observed_at":"2026-08-16T13:11:50.621663Z","submitted_at":"2024-10-07T16:23:57Z","title":"Radiation Transport Simulations of Quasi-Periodic Eruptions from Star-Disk Collisions","version":1},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2410.05166","snapshot_observed_at":"2026-08-16T10:56:15.826689Z","title":null,"venue":null,"work_id":null,"year":2024},"citing_paper":{"arxiv_id":"2504.17016","last_updated":"2025-04-23T18:04:05Z","snapshot_observed_at":"2026-08-16T22:55:29.254839Z","submitted_at":"2025-04-23T18:04:05Z","title":"Black hole-accretion disk collision in general relativity: Axisymmetric simulations","version":1},"reference_index":9,"source":"pdf_text","source_observed_at":"2026-08-16T10:56:15.826689Z"},"links":{"cited_paper":"/paper/2410.05166","citing_paper":"/paper/2504.17016"},"observation_digest":"sha256:e0a14c0821bca3042753a05d4f298626f73f4a875993b75576b54bed1f1cd1ad","observation_id":"7d269e07-5284-44ef-a90f-96fa9b74e7e6","resolution":{"observed_at":"2026-08-16T10:56:15.826689Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2410.05166","last_updated":"2024-10-07T16:23:57Z","snapshot_observed_at":"2026-08-16T13:11:50.621663Z","submitted_at":"2024-10-07T16:23:57Z","title":"Radiation Transport Simulations of Quasi-Periodic Eruptions from Star-Disk Collisions","version":1},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2410.05166","snapshot_observed_at":"2026-08-16T05:12:44.810361Z","title":"D., 2024, @doi [arXiv e-prints] 10.48550/arXiv.2410.05166 , https://ui.adsabs.harvard.edu/abs/2024arXiv241005166V p","venue":null,"work_id":null,"year":2024},"citing_paper":{"arxiv_id":"2504.21456","last_updated":"2025-04-30T09:23:21Z","snapshot_observed_at":"2026-08-16T05:00:42.880794Z","submitted_at":"2025-04-30T09:23:21Z","title":"Collisions with tidal disruption event disks: implications for quasi-periodic X-ray eruptions","version":1},"reference_index":30,"source":"arxiv_source","source_observed_at":"2026-08-16T05:12:44.810361Z"},"links":{"cited_paper":"/paper/2410.05166","citing_paper":"/paper/2504.21456"},"observation_digest":"sha256:89eb1c251769eb959725da42ed80e10e76e3673dd567e57a180b0ecb440d868e","observation_id":"d3c4772c-b7a3-4176-81fc-1ae77bf8c8f4","resolution":{"observed_at":"2026-08-16T05:12:44.810361Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2410.05166","last_updated":"2024-10-07T16:23:57Z","snapshot_observed_at":"2026-08-16T13:11:50.621663Z","submitted_at":"2024-10-07T16:23:57Z","title":"Radiation Transport Simulations of Quasi-Periodic Eruptions from Star-Disk Collisions","version":1},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2410.05166","snapshot_observed_at":"2026-08-15T19:15:57.482622Z","title":null,"venue":null,"work_id":null,"year":2024},"citing_paper":{"arxiv_id":"2506.17138","last_updated":"2025-07-08T14:25:19Z","snapshot_observed_at":"2026-08-18T16:08:13.961933Z","submitted_at":"2025-06-20T16:38:25Z","title":"SRG/eROSITA No. 5: Discovery of quasi-periodic eruptions every ~3.7 days from a galaxy at z>0.1","version":2},"reference_index":87,"source":"pdf_text","source_observed_at":"2026-08-15T19:15:57.482622Z"},"links":{"cited_paper":"/paper/2410.05166","citing_paper":"/paper/2506.17138"},"observation_digest":"sha256:2ea1904a567b999ca54424d9480763cbad5c2bfd0f77bd0ff7cd5443242b9ecc","observation_id":"24b50466-788d-4f5a-ba59-8ac44d0b3ab6","resolution":{"observed_at":"2026-08-15T19:15:57.482622Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2410.05166","last_updated":"2024-10-07T16:23:57Z","snapshot_observed_at":"2026-08-16T13:11:50.621663Z","submitted_at":"2024-10-07T16:23:57Z","title":"Radiation Transport Simulations of Quasi-Periodic Eruptions from Star-Disk Collisions","version":1},"cited_work":{"arxiv_id":"2410.05166","doi":"10.48550/arxiv.2410.05166","metadata_source":"arxiv_reference","pith_arxiv_id":"2410.05166","snapshot_observed_at":"2026-08-05T02:28:24.338817Z","title":"arXiv e-prints , keywords =","venue":"arXiv (Cornell University)","work_id":"c4c6b960-33df-42de-8666-103469f3d2e8","year":null},"citing_paper":{"arxiv_id":"2607.00921","last_updated":"2026-07-01T13:24:29Z","snapshot_observed_at":"2026-08-12T14:47:37.425581Z","submitted_at":"2026-07-01T13:24:29Z","title":"Spatially resolved optical and mid-infrared spectroscopy of SDSS1335+0728: implications for the origin of the Ansky event","version":1},"reference_index":93,"source":"arxiv_source","source_observed_at":"2026-07-02T08:56:40.113509Z"},"links":{"cited_paper":"/paper/2410.05166","citing_paper":"/paper/2607.00921"},"observation_digest":"sha256:99937605df73c763f555ef878aa33024381b1184ef039b700a9dc4ffe2863326","observation_id":"24e40c0d-e47a-4741-9f6e-cf6d932552aa","resolution":{"observed_at":"2026-07-02T08:56:48.743194Z","resolver_source":"arxiv_id","status":"verified_exact"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-18T06:34:40.430872+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-18T06:34:40.430872+00:00","source":"crossref"},{"observed_at":"2026-08-18T06:34:34.496301+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":{"arxiv_id":"2410.05166","last_updated":"2024-10-07T16:23:57Z","snapshot_observed_at":"2026-08-16T13:11:50.621663Z","submitted_at":"2024-10-07T16:23:57Z","title":"Radiation Transport Simulations of Quasi-Periodic Eruptions from Star-Disk Collisions","version":1},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2410.05166","snapshot_observed_at":"2026-08-01T23:27:53.582896Z","title":"arXiv e-prints , keywords =","venue":null,"work_id":null,"year":null},"citing_paper":{"arxiv_id":"2607.15438","last_updated":"2026-07-16T20:16:43Z","snapshot_observed_at":"2026-08-15T18:28:12.676771Z","submitted_at":"2026-07-16T20:16:43Z","title":"Triple radio flares from tidal disruption events: jet-wind collisions and the discovery of a third radio flare from AT2020vwl","version":1},"reference_index":187,"source":"arxiv_source","source_observed_at":"2026-08-01T23:27:53.582896Z"},"links":{"cited_paper":"/paper/2410.05166","citing_paper":"/paper/2607.15438"},"observation_digest":"sha256:49d10fa5e9897fb0d3d979759ba8c79f8faac25a2719cc4171bbb20b5eec31cb","observation_id":"ba91dcb2-f739-4629-a3b2-d33075cea7ea","resolution":{"observed_at":"2026-08-01T23:27:53.582896Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}}],"links":{"evidence":"/evidence","html":"/paper/2410.05166/citation-record","integrity":"/paper/2410.05166/integrity","json":"/paper/2410.05166/citation-record.json","paper":"/paper/2410.05166"},"outbound":[],"paper":{"arxiv_id":"2410.05166","last_updated":"2024-10-07T16:23:57Z","latest_version":1,"primary_category":"astro-ph.HE","snapshot_observed_at":"2026-08-16T13:11:50.621663Z","submitted_at":"2024-10-07T16:23:57Z","title":"Radiation Transport Simulations of Quasi-Periodic Eruptions from Star-Disk Collisions"},"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":"2026-08-18T06:34:40.430872+00:00","source":"crossref"},{"observed_at":"2026-08-18T06:34:34.496301+00:00","source":"retraction_watch"}],"thesis":"As of 18 August 2026, this Paper Citation Record lists 0 of 0 outbound references and 8 inbound Pith citation observations for arXiv:2410.05166."}