{"as_of":"2026-08-19T08:13:00Z","caps":{"database_statements":6,"inbound":100,"outbound":100},"context_digest":"sha256:d564e78ad7c07b8f8492757dcef1d23df38e340049ffe2047cc34e134a72f973","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":2,"lane":"standing_notices","note":"One-hop event checks from named stored sources.","records_observed":2,"source":"scholarly_work_events, retraction_status_cache","source_observed_at":"2026-08-19T06:32:44.657259+00:00","state":"measured"},{"denominator":2,"lane":"inbound_itemization","note":"Pith citing papers itemized under the disclosed page cap.","records_observed":2,"source":"paper_references, paper_reference_links","source_observed_at":"2026-08-11T23:11:26.492484Z","state":"measured"},{"denominator":1,"lane":"external_citation_measurements","note":"A source-named dated measurement, never combined with another source.","records_observed":1,"source":"arxiv_reference","source_observed_at":"2026-08-05T02:28:24.338817Z","state":"measured"}],"external_citation_measurements":[{"count":0,"observed_at":"2026-08-05T02:28:24.338817Z","source":"arxiv_reference"}],"inbound":[{"citation":{"cited_paper":{"arxiv_id":"2406.03646","last_updated":"2024-08-06T19:50:02Z","snapshot_observed_at":"2026-08-19T01:04:25.650087Z","submitted_at":"2024-06-05T22:49:41Z","title":"CLASSY X: Highlighting Differences Between Partial Covering and Semi-Analytic Modeling in the Estimate of Galactic Outflow Properties","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2406.03646","snapshot_observed_at":"2026-08-11T23:11:26.492484Z","title":null,"venue":null,"work_id":null,"year":2024},"citing_paper":{"arxiv_id":"2412.02794","last_updated":"2024-12-03T19:53:33Z","snapshot_observed_at":"2026-08-15T02:41:02.470665Z","submitted_at":"2024-12-03T19:53:33Z","title":"A Simulated Galaxy Laboratory: Exploring the Observational Effects on UV Spectral Absorption Line Measurements","version":1},"reference_index":38,"source":"arxiv_source","source_observed_at":"2026-08-11T23:11:26.492484Z"},"links":{"cited_paper":"/paper/2406.03646","citing_paper":"/paper/2412.02794"},"observation_digest":"sha256:806cfd743b5ce4f77f07c3115b01af6b0e0dd4383f48163cddc973788a30c17e","observation_id":"a3b472b3-723f-4134-8e9d-a743058cb33b","resolution":{"observed_at":"2026-08-11T23:11:26.492484Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2406.03646","last_updated":"2024-08-06T19:50:02Z","snapshot_observed_at":"2026-08-19T01:04:25.650087Z","submitted_at":"2024-06-05T22:49:41Z","title":"CLASSY X: Highlighting Differences Between Partial Covering and Semi-Analytic Modeling in the Estimate of Galactic Outflow Properties","version":2},"cited_work":{"arxiv_id":"2406.03646","doi":"10.48550/arxiv.2406.03646","metadata_source":"arxiv_reference","pith_arxiv_id":"2406.03646","snapshot_observed_at":"2026-08-05T02:28:24.338817Z","title":"arXiv e-prints , keywords =","venue":"arXiv (Cornell University)","work_id":"f752c989-6a18-42e1-8498-5b35d6d768a4","year":null},"citing_paper":{"arxiv_id":"2605.01105","last_updated":"2026-05-01T21:20:47Z","snapshot_observed_at":"2026-07-06T23:14:24.758147Z","submitted_at":"2026-05-01T21:20:47Z","title":"Resolving the Unresolved Galactic Winds in Multi-phase Models. I. Methodology and Application","version":1},"reference_index":165,"source":"arxiv_source","source_observed_at":"2026-05-09T18:21:15.208343Z"},"links":{"cited_paper":"/paper/2406.03646","citing_paper":"/paper/2605.01105"},"observation_digest":"sha256:899490bfa11e845cb3d5ba217fcb47fd008397f66c42bd6d87990582b0ad7feb","observation_id":"247dfafc-9cb8-48df-9854-971179bb29e9","resolution":{"observed_at":"2026-05-09T20:01:37.365616Z","resolver_source":"arxiv_id","status":"verified_exact"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-19T06:32:44.657259+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-19T06:32:44.657259+00:00","source":"crossref"},{"observed_at":"2026-08-19T06:32:39.956319+00:00","source":"retraction_watch"}],"state":"measured"}}],"links":{"evidence":"/evidence","html":"/paper/2406.03646/citation-record","integrity":"/paper/2406.03646/integrity","json":"/paper/2406.03646/citation-record.json","paper":"/paper/2406.03646"},"outbound":[],"paper":{"arxiv_id":"2406.03646","last_updated":"2024-08-06T19:50:02Z","latest_version":2,"primary_category":"astro-ph.GA","snapshot_observed_at":"2026-08-19T01:04:25.650087Z","submitted_at":"2024-06-05T22:49:41Z","title":"CLASSY X: Highlighting Differences Between Partial Covering and Semi-Analytic Modeling in the Estimate of Galactic Outflow Properties"},"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":"2026-08-19T06:32:44.657259+00:00","source":"crossref"},{"observed_at":"2026-08-19T06:32:39.956319+00:00","source":"retraction_watch"}],"thesis":"As of 19 August 2026, this Paper Citation Record lists 0 of 0 outbound references and 2 inbound Pith citation observations for arXiv:2406.03646."}