{"as_of":"2026-08-10T00:46:00Z","caps":{"database_statements":6,"inbound":100,"outbound":100},"context_digest":"sha256:549bea18d60e56827cdc9d82fcacbd79485736f57ea28c3a59d78f6192a2b172","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":"2026-08-09T06:31:02.800959+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":"2026-07-11T11:50:26.030339Z","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":"2026-07-10T22:17:38.556884Z","state":"measured"}],"external_citation_measurements":[],"inbound":[{"citation":{"cited_paper":{"arxiv_id":"2105.12132","last_updated":"2022-07-05T14:49:54Z","snapshot_observed_at":"2026-07-06T11:12:41.293659Z","submitted_at":"2021-05-25T18:00:00Z","title":"Simulating radio synchrotron emission in star-forming galaxies: small-scale magnetic dynamo and the origin of the far infrared-radio correlation","version":3},"cited_work":{"arxiv_id":"2105.12132","doi":null,"metadata_source":"pith","pith_arxiv_id":"2105.12132","snapshot_observed_at":"2026-07-10T22:17:38.556884Z","title":"Pfrommer and M","venue":"astro-ph.GA","work_id":"d5cba5be-c893-4c7f-9377-664be06c510d","year":2021},"citing_paper":{"arxiv_id":"2605.20318","last_updated":"2026-05-19T18:00:00Z","snapshot_observed_at":"2026-08-08T02:00:45.845756Z","submitted_at":"2026-05-19T18:00:00Z","title":"Guide-Field-mediated Multiscale Instabilities in Relativistic Reconnection","version":1},"reference_index":262,"source":"arxiv_source","source_observed_at":"2026-05-21T02:06:01.311344Z"},"links":{"cited_paper":"/paper/2105.12132","citing_paper":"/paper/2605.20318"},"observation_digest":"sha256:88d03a60344d4d349e1b80da66d062317c26a1ff4f8628faf76302004cc80fc0","observation_id":"30e290f7-eb37-49da-af19-97a973690fe3","resolution":{"observed_at":"2026-05-21T02:09:24.556082Z","resolver_source":"arxiv_id","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"}},{"citation":{"cited_paper":{"arxiv_id":"2105.12132","last_updated":"2022-07-05T14:49:54Z","snapshot_observed_at":"2026-07-06T11:12:41.293659Z","submitted_at":"2021-05-25T18:00:00Z","title":"Simulating radio synchrotron emission in star-forming galaxies: small-scale magnetic dynamo and the origin of the far infrared-radio correlation","version":3},"cited_work":{"arxiv_id":"2105.12132","doi":null,"metadata_source":"pith","pith_arxiv_id":"2105.12132","snapshot_observed_at":"2026-07-10T22:17:38.556884Z","title":"Pfrommer and M","venue":"astro-ph.GA","work_id":"d5cba5be-c893-4c7f-9377-664be06c510d","year":2021},"citing_paper":{"arxiv_id":"2607.06744","last_updated":"2026-07-07T19:19:58Z","snapshot_observed_at":"2026-07-11T23:18:32.741925Z","submitted_at":"2026-07-07T19:19:58Z","title":"CRexit observed: probing cosmic ray transport in the circumgalactic medium with absorption line spectra","version":1},"reference_index":79,"source":"arxiv_source","source_observed_at":"2026-07-11T11:50:26.030339Z"},"links":{"cited_paper":"/paper/2105.12132","citing_paper":"/paper/2607.06744"},"observation_digest":"sha256:a0c1764e894d651781b22e525d1d13b4b2042b916b5a0f6c51b2e24d345ca3b0","observation_id":"a0f702eb-8bbe-4331-8241-0d202e5d65ad","resolution":{"observed_at":"2026-07-10T22:17:38.571835Z","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/2105.12132/citation-record","integrity":"/paper/2105.12132/integrity","json":"/paper/2105.12132/citation-record.json","paper":"/paper/2105.12132"},"outbound":[],"paper":{"arxiv_id":"2105.12132","last_updated":"2022-07-05T14:49:54Z","latest_version":3,"primary_category":"astro-ph.GA","snapshot_observed_at":"2026-07-06T11:12:41.293659Z","submitted_at":"2021-05-25T18:00:00Z","title":"Simulating radio synchrotron emission in star-forming galaxies: small-scale magnetic dynamo and the origin of the far infrared-radio correlation"},"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 10 August 2026, this Paper Citation Record lists 0 of 0 outbound references and 2 inbound Pith citation observations for arXiv:2105.12132."}