{"as_of":"2026-08-18T18:46:00Z","caps":{"database_statements":6,"inbound":100,"outbound":100},"context_digest":"sha256:de562426a6ddd59ab9bc859685758bcd94c5ababf1cee23e3a9cf6fdf6729409","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":7,"lane":"standing_notices","note":"One-hop event checks from named stored sources.","records_observed":7,"source":"scholarly_work_events, retraction_status_cache","source_observed_at":"2026-08-18T06:34:40.430872+00:00","state":"measured"},{"denominator":7,"lane":"inbound_itemization","note":"Pith citing papers itemized under the disclosed page cap.","records_observed":7,"source":"paper_references, paper_reference_links","source_observed_at":"2026-08-15T19:52:21.019016Z","state":"measured"},{"denominator":1,"lane":"external_citation_measurements","note":"A source-named dated measurement, never combined with another source.","records_observed":0,"source":"arxiv_reference","source_observed_at":"2026-07-10T06:15:00.866473Z","state":"measured"}],"external_citation_measurements":[],"inbound":[{"citation":{"cited_paper":{"arxiv_id":"2405.12146","last_updated":"2025-07-12T14:55:39Z","snapshot_observed_at":"2026-08-18T14:47:42.368556Z","submitted_at":"2024-05-20T16:16:59Z","title":"Cosmic Ray Diffusion in the Turbulent Interstellar Medium: Effects of Mirror Diffusion and Pitch Angle Scattering","version":3},"cited_work":{"arxiv_id":"2405.12146","doi":"10.48550/arxiv.2405.12146","metadata_source":"arxiv_reference","pith_arxiv_id":"2405.12146","snapshot_observed_at":"2026-07-10T06:15:00.866473Z","title":"M., Xu , S., & Lazarian , A","venue":null,"work_id":"afebd50a-5da5-416f-9de9-b62a6b0e00ae","year":2024},"citing_paper":{"arxiv_id":"2410.13071","last_updated":"2026-05-19T03:38:04Z","snapshot_observed_at":"2026-08-15T09:02:44.767393Z","submitted_at":"2024-10-16T21:59:33Z","title":"Particle Acceleration Time due to Turbulent-Induced Magnetic Reconnection","version":3},"reference_index":7,"source":"arxiv_source","source_observed_at":"2026-05-23T18:48:55.194260Z"},"links":{"cited_paper":"/paper/2405.12146","citing_paper":"/paper/2410.13071"},"observation_digest":"sha256:b350ad5e9a7619bc54476e254079809ac3c9d771199f72c3b74ba994ace78fd0","observation_id":"9e1503f2-922c-4aa8-85ab-4581c365211c","resolution":{"observed_at":"2026-05-23T18:53:21.532917Z","resolver_source":"arxiv_id","status":"verified_exact"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-18T06:34:40.430872+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-18T06:34:40.430872+00:00","source":"crossref"},{"observed_at":"2026-08-18T06:34:34.496301+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":{"arxiv_id":"2405.12146","last_updated":"2025-07-12T14:55:39Z","snapshot_observed_at":"2026-08-18T14:47:42.368556Z","submitted_at":"2024-05-20T16:16:59Z","title":"Cosmic Ray Diffusion in the Turbulent Interstellar Medium: Effects of Mirror Diffusion and Pitch Angle Scattering","version":3},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2405.12146","snapshot_observed_at":"2026-08-11T13:40:33.559891Z","title":"M., Xu, S., & Lazarian, A","venue":null,"work_id":null,"year":2024},"citing_paper":{"arxiv_id":"2412.12923","last_updated":"2025-02-10T16:34:13Z","snapshot_observed_at":"2026-08-18T04:38:39.745396Z","submitted_at":"2024-12-17T13:55:19Z","title":"Generation of cosmic ray trajectories by a Diffusion Model trained on test particles in 3D magnetohydrodynamic turbulence","version":2},"reference_index":6,"source":"arxiv_source","source_observed_at":"2026-08-11T13:40:33.559891Z"},"links":{"cited_paper":"/paper/2405.12146","citing_paper":"/paper/2412.12923"},"observation_digest":"sha256:8a45d005a253ccbee4efea54562e4b42d3fcb4f739fc73dc51d9ed27ff317dd3","observation_id":"215b6999-3d5d-43ed-83f4-0ccbfecff9a0","resolution":{"observed_at":"2026-08-11T13:40:33.559891Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2405.12146","last_updated":"2025-07-12T14:55:39Z","snapshot_observed_at":"2026-08-18T14:47:42.368556Z","submitted_at":"2024-05-20T16:16:59Z","title":"Cosmic Ray Diffusion in the Turbulent Interstellar Medium: Effects of Mirror Diffusion and Pitch Angle Scattering","version":3},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2405.12146","snapshot_observed_at":"2026-08-10T21:29:05.538559Z","title":"M., Xu , S., & Lazarian , A","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":4,"source":"arxiv_source","source_observed_at":"2026-08-10T21:29:05.538559Z"},"links":{"cited_paper":"/paper/2405.12146","citing_paper":"/paper/2501.04986"},"observation_digest":"sha256:1396b5e044bcbed4616e9891ad0c14e4be256719e973f0f2bc3185a3d85fa0d8","observation_id":"b87019ca-fd14-4e5e-bb33-b8e5ff1161b8","resolution":{"observed_at":"2026-08-10T21:29:05.538559Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2405.12146","last_updated":"2025-07-12T14:55:39Z","snapshot_observed_at":"2026-08-18T14:47:42.368556Z","submitted_at":"2024-05-20T16:16:59Z","title":"Cosmic Ray Diffusion in the Turbulent Interstellar Medium: Effects of Mirror Diffusion and Pitch Angle Scattering","version":3},"cited_work":{"arxiv_id":"2405.12146","doi":"10.48550/arxiv.2405.12146","metadata_source":"arxiv_reference","pith_arxiv_id":"2405.12146","snapshot_observed_at":"2026-07-10T06:15:00.866473Z","title":"M., Xu , S., & Lazarian , A","venue":null,"work_id":"afebd50a-5da5-416f-9de9-b62a6b0e00ae","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":43,"source":"pdf_text","source_observed_at":"2026-05-19T10:45:37.848326Z"},"links":{"cited_paper":"/paper/2405.12146","citing_paper":"/paper/2506.04212"},"observation_digest":"sha256:1ad43defad0d1139a06fd8307082f6886f851e9cf37294443150596548a6ff92","observation_id":"a7f4e342-52d6-4010-9299-39bb7ec65a58","resolution":{"observed_at":"2026-05-09T02:33:42.991285Z","resolver_source":"arxiv_id","status":"verified_exact"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-18T06:34:40.430872+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-18T06:34:40.430872+00:00","source":"crossref"},{"observed_at":"2026-08-18T06:34:34.496301+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":{"arxiv_id":"2405.12146","last_updated":"2025-07-12T14:55:39Z","snapshot_observed_at":"2026-08-18T14:47:42.368556Z","submitted_at":"2024-05-20T16:16:59Z","title":"Cosmic Ray Diffusion in the Turbulent Interstellar Medium: Effects of Mirror Diffusion and Pitch Angle Scattering","version":3},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2405.12146","snapshot_observed_at":"2026-08-15T19:52:21.019016Z","title":"M., Xu, S., & Lazarian, A","venue":null,"work_id":null,"year":2024},"citing_paper":{"arxiv_id":"2506.15031","last_updated":"2025-06-22T22:44:12Z","snapshot_observed_at":"2026-08-18T00:44:58.192864Z","submitted_at":"2025-06-18T00:17:43Z","title":"Studying the diffusion mechanism of cosmic-ray particles","version":2},"reference_index":4,"source":"pdf_text","source_observed_at":"2026-08-15T19:52:21.019016Z"},"links":{"cited_paper":"/paper/2405.12146","citing_paper":"/paper/2506.15031"},"observation_digest":"sha256:2a77d004eba39e349acd5604e9d5803f72161a8342eb81498f209fba89d479e0","observation_id":"ffb4438e-a89b-4837-a3c1-b7015e043657","resolution":{"observed_at":"2026-08-15T19:52:21.019016Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2405.12146","last_updated":"2025-07-12T14:55:39Z","snapshot_observed_at":"2026-08-18T14:47:42.368556Z","submitted_at":"2024-05-20T16:16:59Z","title":"Cosmic Ray Diffusion in the Turbulent Interstellar Medium: Effects of Mirror Diffusion and Pitch Angle Scattering","version":3},"cited_work":{"arxiv_id":"2405.12146","doi":"10.48550/arxiv.2405.12146","metadata_source":"arxiv_reference","pith_arxiv_id":"2405.12146","snapshot_observed_at":"2026-07-10T06:15:00.866473Z","title":"M., Xu , S., & Lazarian , A","venue":null,"work_id":"afebd50a-5da5-416f-9de9-b62a6b0e00ae","year":2024},"citing_paper":{"arxiv_id":"2508.13667","last_updated":"2026-01-30T10:45:06Z","snapshot_observed_at":"2026-08-13T09:43:26.814298Z","submitted_at":"2025-08-19T09:15:39Z","title":"PHECT: A lightweight computation tool for pulsar halo emission","version":2},"reference_index":47,"source":"pdf_text","source_observed_at":"2026-05-18T23:02:15.483780Z"},"links":{"cited_paper":"/paper/2405.12146","citing_paper":"/paper/2508.13667"},"observation_digest":"sha256:887b480f8b13ebef1d4be1ccc958a298075fdb02b39139678633a5f4fac823a3","observation_id":"87518850-f9af-4d15-aeeb-1130a9fd52f7","resolution":{"observed_at":"2026-05-18T23:02:52.384779Z","resolver_source":"arxiv_id","status":"verified_exact"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-18T06:34:40.430872+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-18T06:34:40.430872+00:00","source":"crossref"},{"observed_at":"2026-08-18T06:34:34.496301+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":{"arxiv_id":"2405.12146","last_updated":"2025-07-12T14:55:39Z","snapshot_observed_at":"2026-08-18T14:47:42.368556Z","submitted_at":"2024-05-20T16:16:59Z","title":"Cosmic Ray Diffusion in the Turbulent Interstellar Medium: Effects of Mirror Diffusion and Pitch Angle Scattering","version":3},"cited_work":{"arxiv_id":"2405.12146","doi":"10.48550/arxiv.2405.12146","metadata_source":"arxiv_reference","pith_arxiv_id":"2405.12146","snapshot_observed_at":"2026-07-10T06:15:00.866473Z","title":"M., Xu , S., & Lazarian , A","venue":null,"work_id":"afebd50a-5da5-416f-9de9-b62a6b0e00ae","year":2024},"citing_paper":{"arxiv_id":"2509.07104","last_updated":"2026-04-29T05:52:37Z","snapshot_observed_at":"2026-08-05T05:28:12.451340Z","submitted_at":"2025-09-08T18:00:40Z","title":"Cosmic Rays on Galaxy Scales: Progress and Pitfalls for CR-MHD Dynamical Models","version":2},"reference_index":16,"source":"arxiv_source","source_observed_at":"2026-05-18T17:40:44.882670Z"},"links":{"cited_paper":"/paper/2405.12146","citing_paper":"/paper/2509.07104"},"observation_digest":"sha256:4a884ddd8ff3fb4229298f99c8f9c911147130a86d10e9d19c2bbad529e3b22c","observation_id":"add018bb-8c2b-4ce7-b00a-0a2e869e03ce","resolution":{"observed_at":"2026-05-18T17:41:41.734165Z","resolver_source":"arxiv_id","status":"metadata_mismatch"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-18T06:34:40.430872+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-18T06:34:40.430872+00:00","source":"crossref"},{"observed_at":"2026-08-18T06:34:34.496301+00:00","source":"retraction_watch"}],"state":"measured"}}],"links":{"evidence":"/evidence","html":"/paper/2405.12146/citation-record","integrity":"/paper/2405.12146/integrity","json":"/paper/2405.12146/citation-record.json","paper":"/paper/2405.12146"},"outbound":[],"paper":{"arxiv_id":"2405.12146","last_updated":"2025-07-12T14:55:39Z","latest_version":3,"primary_category":"astro-ph.HE","snapshot_observed_at":"2026-08-18T14:47:42.368556Z","submitted_at":"2024-05-20T16:16:59Z","title":"Cosmic Ray Diffusion in the Turbulent Interstellar Medium: Effects of Mirror Diffusion and Pitch Angle Scattering"},"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":"2026-08-18T06:34:40.430872+00:00","source":"crossref"},{"observed_at":"2026-08-18T06:34:34.496301+00:00","source":"retraction_watch"}],"thesis":"As of 18 August 2026, this Paper Citation Record lists 0 of 0 outbound references and 7 inbound Pith citation observations for arXiv:2405.12146."}