{"as_of":"2026-08-09T23:27:00Z","caps":{"database_statements":6,"inbound":100,"outbound":100},"context_digest":"sha256:7a1a3325dd27e8b643a80dbb282d13efcd0a25d6c4bbe3291f680e75b561e4ce","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":1,"lane":"standing_notices","note":"One-hop event checks from named stored sources.","records_observed":1,"source":"scholarly_work_events, retraction_status_cache","source_observed_at":"2026-08-09T06:31:02.800959+00:00","state":"measured"},{"denominator":1,"lane":"inbound_itemization","note":"Pith citing papers itemized under the disclosed page cap.","records_observed":1,"source":"paper_references, paper_reference_links","source_observed_at":"2026-08-09T04:43:23.417236Z","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":"2026-08-09T04:43:24.115903Z","state":"measured"}],"external_citation_measurements":[],"inbound":[{"citation":{"cited_paper":{"arxiv_id":"2203.10851","last_updated":"2022-05-03T19:18:54Z","snapshot_observed_at":"2026-07-06T12:50:08.081200Z","submitted_at":"2022-03-21T10:19:21Z","title":"The 21-cm signal from the Cosmic Dawn: metallicity dependence of high mass X-ray binaries","version":2},"cited_work":{"arxiv_id":"2203.10851","doi":null,"metadata_source":"pith","pith_arxiv_id":"2203.10851","snapshot_observed_at":"2026-08-09T04:43:24.115903Z","title":"The 21-cm signal from the Cosmic Dawn: metallicity dependence of high mass X-ray binaries","venue":"astro-ph.GA","work_id":"28e4f5fe-a335-4d8e-9d56-fcb472d6e8d2","year":2022},"citing_paper":{"arxiv_id":"2502.03525","last_updated":"2025-02-05T19:00:01Z","snapshot_observed_at":"2026-08-09T07:15:51.502045Z","submitted_at":"2025-02-05T19:00:01Z","title":"Closing in on Pop-III Stars: Constraints and Predictions Across the Spectrum","version":1},"reference_index":55,"source":"pdf_text","source_observed_at":"2026-08-09T04:43:23.417236Z"},"links":{"cited_paper":"/paper/2203.10851","citing_paper":"/paper/2502.03525"},"observation_digest":"sha256:ddd719eec634bc4eaea215eb575cca7c16d7f67e9aa1c18b473a92622a6cb1b2","observation_id":"5e68b51c-1373-434a-8e45-b0073a0d2bf8","resolution":{"observed_at":"2026-08-09T04:43:24.154511Z","resolver_source":"local_arxiv","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/2203.10851/citation-record","integrity":"/paper/2203.10851/integrity","json":"/paper/2203.10851/citation-record.json","paper":"/paper/2203.10851"},"outbound":[],"paper":{"arxiv_id":"2203.10851","last_updated":"2022-05-03T19:18:54Z","latest_version":2,"primary_category":"astro-ph.GA","snapshot_observed_at":"2026-07-06T12:50:08.081200Z","submitted_at":"2022-03-21T10:19:21Z","title":"The 21-cm signal from the Cosmic Dawn: metallicity dependence of high mass X-ray 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":"2026-08-09T06:31:02.800959+00:00","source":"crossref"},{"observed_at":"2026-08-09T06:30:57.326959+00:00","source":"retraction_watch"}],"thesis":"As of 9 August 2026, this Paper Citation Record lists 0 of 0 outbound references and 1 inbound Pith citation observation for arXiv:2203.10851."}