{"as_of":"2026-08-08T02:51:00Z","caps":{"database_statements":6,"inbound":100,"outbound":100},"context_digest":"sha256:bd9631904f9c366707e9fa32fc37a4e8ee12159077a73ec8762d407fd3e5ecb6","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":"2026-08-07T06:34:17.273281+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":"2026-08-02T06:10:08.339253Z","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":"2410.21722","last_updated":"2024-10-29T04:22:04Z","snapshot_observed_at":"2026-08-06T09:15:12.956892Z","submitted_at":"2024-10-29T04:22:04Z","title":"On the Significance of Covariance for Constraining Theoretical Models From Galaxy Observables","version":1},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2410.21722","snapshot_observed_at":"2026-08-02T06:10:08.339253Z","title":", keywords =","venue":null,"work_id":null,"year":null},"citing_paper":{"arxiv_id":"2607.13151","last_updated":"2026-07-14T18:01:38Z","snapshot_observed_at":"2026-08-06T10:10:01.626872Z","submitted_at":"2026-07-14T18:01:38Z","title":"Evaluating the flexibility of the MillenniumTNG galaxy formation model with multi-zoom re-simulations","version":1},"reference_index":1,"source":"arxiv_source","source_observed_at":"2026-08-02T06:10:08.339253Z"},"links":{"cited_paper":"/paper/2410.21722","citing_paper":"/paper/2607.13151"},"observation_digest":"sha256:8152bd3fb7d57d40399d903fc4fdcc1e9783252c413c44f0768b646c754acd0d","observation_id":"0a5231a9-fb71-4832-8682-4c5b85a7bf58","resolution":{"observed_at":"2026-08-02T06:10:08.339253Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}}],"links":{"evidence":"/evidence","html":"/paper/2410.21722/citation-record","integrity":"/paper/2410.21722/integrity","json":"/paper/2410.21722/citation-record.json","paper":"/paper/2410.21722"},"outbound":[],"paper":{"arxiv_id":"2410.21722","last_updated":"2024-10-29T04:22:04Z","latest_version":1,"primary_category":"astro-ph.CO","snapshot_observed_at":"2026-08-06T09:15:12.956892Z","submitted_at":"2024-10-29T04:22:04Z","title":"On the Significance of Covariance for Constraining Theoretical Models From Galaxy Observables"},"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":"2026-08-07T06:34:17.273281+00:00","source":"crossref"},{"observed_at":"2026-08-07T06:34:11.927384+00:00","source":"retraction_watch"}],"thesis":"As of 8 August 2026, this Paper Citation Record lists 0 of 0 outbound references and 1 inbound Pith citation observation for arXiv:2410.21722."}