{"as_of":"2026-08-16T23:48:00Z","caps":{"database_statements":6,"inbound":100,"outbound":100},"context_digest":"sha256:8253e459edafa59559b4f5d889e3da3ef8dcfe867a3e55cbc09d772e609a8931","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":4,"lane":"standing_notices","note":"One-hop event checks from named stored sources.","records_observed":4,"source":"scholarly_work_events, retraction_status_cache","source_observed_at":"2026-08-16T06:30:59.297886+00:00","state":"measured"},{"denominator":4,"lane":"inbound_itemization","note":"Pith citing papers itemized under the disclosed page cap.","records_observed":4,"source":"paper_references, paper_reference_links","source_observed_at":"2026-08-15T22:28:12.909885Z","state":"measured"},{"denominator":1,"lane":"external_citation_measurements","note":"A source-named dated measurement, never combined with another source.","records_observed":0,"source":"pith","source_observed_at":"2026-08-08T00:10:27.609399Z","state":"measured"}],"external_citation_measurements":[],"inbound":[{"citation":{"cited_paper":{"arxiv_id":"2201.05512","last_updated":"2022-01-14T15:30:56Z","snapshot_observed_at":"2026-08-16T19:14:00.561608Z","submitted_at":"2022-01-14T15:30:56Z","title":"MOBSTER -- VI. The crucial influence of rotation on the radio magnetospheres of hot stars","version":1},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2201.05512","snapshot_observed_at":"2026-08-15T22:28:12.909885Z","title":"E., Owocki , S","venue":null,"work_id":null,"year":2022},"citing_paper":{"arxiv_id":"2505.07195","last_updated":"2025-05-12T02:59:34Z","snapshot_observed_at":"2026-08-15T22:20:31.157968Z","submitted_at":"2025-05-12T02:59:34Z","title":"Discovery of Main-sequence Radio Pulse emitters from widefield sky surveys","version":1},"reference_index":63,"source":"arxiv_source","source_observed_at":"2026-08-15T22:28:12.909885Z"},"links":{"cited_paper":"/paper/2201.05512","citing_paper":"/paper/2505.07195"},"observation_digest":"sha256:7fa5a123d837d6442b9e941fcc7cb0e97874a973cb2e7c72983b196f8469b5fc","observation_id":"3fb04716-95d3-49eb-ba92-13614a420935","resolution":{"observed_at":"2026-08-15T22:28:12.909885Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2201.05512","last_updated":"2022-01-14T15:30:56Z","snapshot_observed_at":"2026-08-16T19:14:00.561608Z","submitted_at":"2022-01-14T15:30:56Z","title":"MOBSTER -- VI. The crucial influence of rotation on the radio magnetospheres of hot stars","version":1},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2201.05512","snapshot_observed_at":"2026-08-15T21:44:08.868162Z","title":"E., Owocki , S","venue":null,"work_id":null,"year":2022},"citing_paper":{"arxiv_id":"2505.09148","last_updated":"2025-09-02T03:27:49Z","snapshot_observed_at":"2026-08-15T21:36:22.662063Z","submitted_at":"2025-05-14T05:10:03Z","title":"VAST-MeMeS: Characterising non-thermal radio emission from magnetic massive stars using the Australian SKA Pathfinder","version":2},"reference_index":86,"source":"arxiv_source","source_observed_at":"2026-08-15T21:44:08.868162Z"},"links":{"cited_paper":"/paper/2201.05512","citing_paper":"/paper/2505.09148"},"observation_digest":"sha256:d9a4ecd46d189fbd9315f56d13c80fc9710cb86a1262a7c87aefe033483ed70a","observation_id":"809a9135-a1f3-44dc-a6aa-0a0ea27709fb","resolution":{"observed_at":"2026-08-15T21:44:08.868162Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2201.05512","last_updated":"2022-01-14T15:30:56Z","snapshot_observed_at":"2026-08-16T19:14:00.561608Z","submitted_at":"2022-01-14T15:30:56Z","title":"MOBSTER -- VI. The crucial influence of rotation on the radio magnetospheres of hot stars","version":1},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2201.05512","snapshot_observed_at":"2026-08-15T15:19:16.439033Z","title":"The crucial influence of rotation on the radio magnetospheres of hot stars","venue":null,"work_id":null,"year":null},"citing_paper":{"arxiv_id":"2608.00968","last_updated":"2026-08-02T03:47:11Z","snapshot_observed_at":"2026-08-15T15:11:51.522640Z","submitted_at":"2026-08-02T03:47:11Z","title":"First monitoring campaign of a Main-sequence Radio Pulse emitter: the case of CU Vir","version":1},"reference_index":12,"source":"arxiv_source","source_observed_at":"2026-08-15T15:19:16.439033Z"},"links":{"cited_paper":"/paper/2201.05512","citing_paper":"/paper/2608.00968"},"observation_digest":"sha256:05c5bce9bab765288d3eb37854c104eb37123e292b77f4ee158a268014e1177a","observation_id":"9b04c4b3-7457-4c1b-9bcc-4c751d466638","resolution":{"observed_at":"2026-08-15T15:19:16.439033Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2201.05512","last_updated":"2022-01-14T15:30:56Z","snapshot_observed_at":"2026-08-16T19:14:00.561608Z","submitted_at":"2022-01-14T15:30:56Z","title":"MOBSTER -- VI. The crucial influence of rotation on the radio magnetospheres of hot stars","version":1},"cited_work":{"arxiv_id":"2201.05512","doi":null,"metadata_source":"pith","pith_arxiv_id":"2201.05512","snapshot_observed_at":"2026-08-08T00:10:27.609399Z","title":"MOBSTER -- VI. The crucial influence of rotation on the radio magnetospheres of hot stars","venue":"astro-ph.SR","work_id":"83a0b91d-4912-4c67-8eea-bbcf87edef09","year":2022},"citing_paper":{"arxiv_id":"2608.04250","last_updated":"2026-08-04T22:00:25Z","snapshot_observed_at":"2026-08-09T02:57:56.061355Z","submitted_at":"2026-08-04T22:00:25Z","title":"Searching for Habitable Exoplanets with Relative Astrometry (SHERA). I. The Case for Searching for Planets in Binary Star Systems","version":1},"reference_index":165,"source":"arxiv_source","source_observed_at":"2026-08-08T00:10:26.439699Z"},"links":{"cited_paper":"/paper/2201.05512","citing_paper":"/paper/2608.04250"},"observation_digest":"sha256:7caa9dd1ee1c10d5423463452f55a0c39bdc1714bbaca4aed0fc42783c3b9e9a","observation_id":"4e4d871b-4fd2-49d3-b53e-15e6286ad006","resolution":{"observed_at":"2026-08-08T00:10:27.614604Z","resolver_source":"local_arxiv","status":"verified_exact"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-16T06:30:59.297886+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-16T06:30:59.297886+00:00","source":"crossref"},{"observed_at":"2026-08-16T06:30:54.164669+00:00","source":"retraction_watch"}],"state":"measured"}}],"links":{"evidence":"/evidence","html":"/paper/2201.05512/citation-record","integrity":"/paper/2201.05512/integrity","json":"/paper/2201.05512/citation-record.json","paper":"/paper/2201.05512"},"outbound":[],"paper":{"arxiv_id":"2201.05512","last_updated":"2022-01-14T15:30:56Z","latest_version":1,"primary_category":"astro-ph.SR","snapshot_observed_at":"2026-08-16T19:14:00.561608Z","submitted_at":"2022-01-14T15:30:56Z","title":"MOBSTER -- VI. The crucial influence of rotation on the radio magnetospheres of hot stars"},"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":"2026-08-16T06:30:59.297886+00:00","source":"crossref"},{"observed_at":"2026-08-16T06:30:54.164669+00:00","source":"retraction_watch"}],"thesis":"As of 16 August 2026, this Paper Citation Record lists 0 of 0 outbound references and 4 inbound Pith citation observations for arXiv:2201.05512."}