{"as_of":"2026-08-11T19:34:00Z","caps":{"database_statements":6,"inbound":100,"outbound":100},"context_digest":"sha256:de5d9024f57e81a6ecfa4658d26aeed9c9d4d873e4231b523d581f64e1e68a14","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":"2026-08-11T06:34:44.6726+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":"2026-08-10T17:19:39.906396Z","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":"2101.07637","last_updated":"2021-01-19T14:27:53Z","snapshot_observed_at":"2026-07-06T10:33:46.608549Z","submitted_at":"2021-01-19T14:27:53Z","title":"The properties of clusters, and the orientation of magnetic fields relative to filaments, in magnetohydrodynamic simulations of colliding clouds","version":1},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2101.07637","snapshot_observed_at":"2026-08-10T17:19:39.906396Z","title":", keywords =","venue":null,"work_id":null,"year":null},"citing_paper":{"arxiv_id":"2608.06978","last_updated":"2026-08-07T08:55:46Z","snapshot_observed_at":"2026-08-11T19:10:42.431914Z","submitted_at":"2026-08-07T08:55:46Z","title":"Smoothed particle magnetohydrodynamics for simulations of galaxy and cosmic structure formation","version":1},"reference_index":83,"source":"arxiv_source","source_observed_at":"2026-08-10T17:19:39.906396Z"},"links":{"cited_paper":"/paper/2101.07637","citing_paper":"/paper/2608.06978"},"observation_digest":"sha256:85472a2099567f15981224f3ef16c41db6799c9e0f2fc1fcde01b4ec98b35e0f","observation_id":"d4b6dd48-dd84-451d-af34-2fb23b0c7d01","resolution":{"observed_at":"2026-08-10T17:19:39.906396Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}}],"links":{"evidence":"/evidence","html":"/paper/2101.07637/citation-record","integrity":"/paper/2101.07637/integrity","json":"/paper/2101.07637/citation-record.json","paper":"/paper/2101.07637"},"outbound":[],"paper":{"arxiv_id":"2101.07637","last_updated":"2021-01-19T14:27:53Z","latest_version":1,"primary_category":"astro-ph.GA","snapshot_observed_at":"2026-07-06T10:33:46.608549Z","submitted_at":"2021-01-19T14:27:53Z","title":"The properties of clusters, and the orientation of magnetic fields relative to filaments, in magnetohydrodynamic simulations of colliding clouds"},"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":"2026-08-11T06:34:44.6726+00:00","source":"crossref"},{"observed_at":"2026-08-11T06:34:36.301508+00:00","source":"retraction_watch"}],"thesis":"As of 11 August 2026, this Paper Citation Record lists 0 of 0 outbound references and 1 inbound Pith citation observation for arXiv:2101.07637."}