{"as_of":"2026-08-10T23:15:00Z","caps":{"database_statements":6,"inbound":100,"outbound":100},"context_digest":"sha256:b81708a304bcf3230ccb66931d2af5e126b37c9b57cbaf2cd00521834d8b4a04","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":"2026-08-10T06:31:04.303077+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":"2026-08-01T12:43:57.521856Z","state":"measured"},{"denominator":1,"lane":"external_citation_measurements","note":"A source-named dated measurement, never combined with another source.","records_observed":0,"source":"cited_works","source_observed_at":null,"state":"measured"}],"external_citation_measurements":[],"inbound":[{"citation":{"cited_paper":{"arxiv_id":"2103.02946","last_updated":"2021-03-04T10:59:14Z","snapshot_observed_at":"2026-07-06T10:46:46.899067Z","submitted_at":"2021-03-04T10:59:14Z","title":"The less and the more IGM transmitted galaxies from z~2.7 to z~6 from VANDELS and VUDS","version":1},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2103.02946","snapshot_observed_at":"2026-08-01T12:43:57.521856Z","title":"and Pentericci, L","venue":null,"work_id":null,"year":2021},"citing_paper":{"arxiv_id":"2607.19472","last_updated":"2026-07-21T18:00:04Z","snapshot_observed_at":"2026-08-06T19:22:15.795870Z","submitted_at":"2026-07-21T18:00:04Z","title":"Cosmic CORALS: Timing the Universe with high-z star clusters","version":1},"reference_index":112,"source":"arxiv_source","source_observed_at":"2026-08-01T12:43:57.521856Z"},"links":{"cited_paper":"/paper/2103.02946","citing_paper":"/paper/2607.19472"},"observation_digest":"sha256:229916e879189e2ab23bddf191450058f4c2e2a073626704fab1eedaceb772ef","observation_id":"158907e7-0938-46d8-bb2a-35a320024485","resolution":{"observed_at":"2026-08-01T12:43:57.521856Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}}],"links":{"evidence":"/evidence","html":"/paper/2103.02946/citation-record","integrity":"/paper/2103.02946/integrity","json":"/paper/2103.02946/citation-record.json","paper":"/paper/2103.02946"},"outbound":[],"paper":{"arxiv_id":"2103.02946","last_updated":"2021-03-04T10:59:14Z","latest_version":1,"primary_category":"astro-ph.CO","snapshot_observed_at":"2026-07-06T10:46:46.899067Z","submitted_at":"2021-03-04T10:59:14Z","title":"The less and the more IGM transmitted galaxies from z~2.7 to z~6 from VANDELS and VUDS"},"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":"2026-08-10T06:31:04.303077+00:00","source":"crossref"},{"observed_at":"2026-08-10T06:30:57.382061+00:00","source":"retraction_watch"}],"thesis":"As of 10 August 2026, this Paper Citation Record lists 0 of 0 outbound references and 1 inbound Pith citation observation for arXiv:2103.02946."}