{"as_of":"2026-08-19T21:22:00Z","caps":{"database_statements":6,"inbound":100,"outbound":100},"context_digest":"sha256:473f036b8b9a2de7d01cbe921a8647d1a9ad64b625f98bf7a5825662f0d9fe79","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":3,"lane":"standing_notices","note":"One-hop event checks from named stored sources.","records_observed":3,"source":"scholarly_work_events, retraction_status_cache","source_observed_at":"2026-08-19T06:32:44.657259+00:00","state":"measured"},{"denominator":3,"lane":"inbound_itemization","note":"Pith citing papers itemized under the disclosed page cap.","records_observed":3,"source":"paper_references, paper_reference_links","source_observed_at":"2026-08-10T21:29:05.925755Z","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":"2406.03542","last_updated":"2024-09-12T17:25:45Z","snapshot_observed_at":"2026-08-16T20:15:16.374483Z","submitted_at":"2024-06-05T18:00:03Z","title":"Cosmic ray diffusion in magnetic fields amplified by nonlinear turbulent dynamo","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2406.03542","snapshot_observed_at":"2026-08-10T21:29:05.925755Z","title":"& Xu , S","venue":null,"work_id":null,"year":2024},"citing_paper":{"arxiv_id":"2501.04986","last_updated":"2025-01-09T06:00:16Z","snapshot_observed_at":"2026-08-18T17:45:02.149859Z","submitted_at":"2025-01-09T06:00:16Z","title":"Anisotropic diffusion of high-energy cosmic rays in magnetohydrodynamic turbulence","version":1},"reference_index":86,"source":"arxiv_source","source_observed_at":"2026-08-10T21:29:05.925755Z"},"links":{"cited_paper":"/paper/2406.03542","citing_paper":"/paper/2501.04986"},"observation_digest":"sha256:c4c5fa73e744891819c8137c84799f6e30d92731343d346933f441f4fadb06e1","observation_id":"a1e22e89-76b9-4f4d-b32a-b8c28ee340d3","resolution":{"observed_at":"2026-08-10T21:29:05.925755Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2406.03542","last_updated":"2024-09-12T17:25:45Z","snapshot_observed_at":"2026-08-16T20:15:16.374483Z","submitted_at":"2024-06-05T18:00:03Z","title":"Cosmic ray diffusion in magnetic fields amplified by nonlinear turbulent dynamo","version":2},"cited_work":{"arxiv_id":"2406.03542","doi":"10.48550/arxiv.2406.03542","metadata_source":"arxiv_reference","pith_arxiv_id":"2406.03542","snapshot_observed_at":"2026-08-05T02:28:24.338817Z","title":"Zhang and S","venue":"arXiv (Cornell University)","work_id":"299af811-5d2c-46c0-b53a-defd384d4549","year":2024},"citing_paper":{"arxiv_id":"2506.04212","last_updated":"2026-05-06T18:45:15Z","snapshot_observed_at":"2026-08-17T12:05:10.395227Z","submitted_at":"2025-06-04T17:56:48Z","title":"Studying the mirror acceleration via kinetic simulations of relativistic plasma turbulence","version":2},"reference_index":42,"source":"pdf_text","source_observed_at":"2026-05-19T10:45:37.848326Z"},"links":{"cited_paper":"/paper/2406.03542","citing_paper":"/paper/2506.04212"},"observation_digest":"sha256:21c8a0b40c7cc316b25c29fe001c8801887babf2491439891206704a3c72ae3e","observation_id":"059f3c49-cf25-46f5-9225-4613742c36ea","resolution":{"observed_at":"2026-05-09T02:33:42.986026Z","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"}},{"citation":{"cited_paper":{"arxiv_id":"2406.03542","last_updated":"2024-09-12T17:25:45Z","snapshot_observed_at":"2026-08-16T20:15:16.374483Z","submitted_at":"2024-06-05T18:00:03Z","title":"Cosmic ray diffusion in magnetic fields amplified by nonlinear turbulent dynamo","version":2},"cited_work":{"arxiv_id":"2406.03542","doi":"10.48550/arxiv.2406.03542","metadata_source":"arxiv_reference","pith_arxiv_id":"2406.03542","snapshot_observed_at":"2026-08-05T02:28:24.338817Z","title":"Zhang and S","venue":"arXiv (Cornell University)","work_id":"299af811-5d2c-46c0-b53a-defd384d4549","year":2024},"citing_paper":{"arxiv_id":"2606.07741","last_updated":"2026-06-05T18:00:02Z","snapshot_observed_at":"2026-07-06T23:47:19.773490Z","submitted_at":"2026-06-05T18:00:02Z","title":"Clumps in a Cocoon: Geometry and Mixing Set the Universal X-ray to H$\\alpha$ Surface Brightness Ratio","version":1},"reference_index":103,"source":"arxiv_source","source_observed_at":"2026-06-27T21:13:45.849333Z"},"links":{"cited_paper":"/paper/2406.03542","citing_paper":"/paper/2606.07741"},"observation_digest":"sha256:2c5303095d14d5714954c982d05fdd2a4171932f76b3b61a6dc0a52f98569cc0","observation_id":"1a22587d-4a3e-4190-890d-705a00b32f72","resolution":{"observed_at":"2026-06-27T22:01:21.588925Z","resolver_source":"arxiv_id","status":"metadata_mismatch"},"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/2406.03542/citation-record","integrity":"/paper/2406.03542/integrity","json":"/paper/2406.03542/citation-record.json","paper":"/paper/2406.03542"},"outbound":[],"paper":{"arxiv_id":"2406.03542","last_updated":"2024-09-12T17:25:45Z","latest_version":2,"primary_category":"astro-ph.HE","snapshot_observed_at":"2026-08-16T20:15:16.374483Z","submitted_at":"2024-06-05T18:00:03Z","title":"Cosmic ray diffusion in magnetic fields amplified by nonlinear turbulent dynamo"},"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 3 inbound Pith citation observations for arXiv:2406.03542."}