{"as_of":"2026-08-22T17:27:00Z","caps":{"database_statements":6,"inbound":100,"outbound":100},"context_digest":"sha256:2ed385b9151c24b8b6cef6140a8faf020a4231d4f3d06439d5735dcc7b4032dd","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":"2026-08-22T06:32:14.747728+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":"2026-08-02T02:26:39.830416Z","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":"2026-07-01T18:05:58.771037Z","state":"measured"}],"external_citation_measurements":[],"inbound":[{"citation":{"cited_paper":{"arxiv_id":"2007.04294","last_updated":"2020-07-08T17:45:43Z","snapshot_observed_at":"2026-08-09T21:39:37.231164Z","submitted_at":"2020-07-08T17:45:43Z","title":"The low rate of Galactic pevatrons","version":1},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2007.04294","snapshot_observed_at":"2026-07-13T16:13:27.782513Z","title":"2020, arXiv e-prints, arXiv:2007.04294","venue":null,"work_id":null,"year":2020},"citing_paper":{"arxiv_id":"2603.28701","last_updated":"2026-03-30T17:18:47Z","snapshot_observed_at":"2026-08-14T13:35:43.807136Z","submitted_at":"2026-03-30T17:18:47Z","title":"Can a single supernova remnant account for the gamma-ray emission of G106.3+2.7?","version":1},"reference_index":26,"source":"pdf_text","source_observed_at":"2026-07-13T16:13:27.782513Z"},"links":{"cited_paper":"/paper/2007.04294","citing_paper":"/paper/2603.28701"},"observation_digest":"sha256:0bec3d13ee8010893c5305a717c16fdec16ac76d81b52a330c2cfe24faa34f6b","observation_id":"d1da2c55-efa8-4fd6-a103-e43cff602023","resolution":{"observed_at":"2026-07-13T16:13:27.782513Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2007.04294","last_updated":"2020-07-08T17:45:43Z","snapshot_observed_at":"2026-08-09T21:39:37.231164Z","submitted_at":"2020-07-08T17:45:43Z","title":"The low rate of Galactic pevatrons","version":1},"cited_work":{"arxiv_id":"2007.04294","doi":null,"metadata_source":"arxiv_reference","pith_arxiv_id":"2007.04294","snapshot_observed_at":"2026-07-01T18:05:58.771037Z","title":"Cristofari, P","venue":null,"work_id":"44641593-10a9-4a76-a4e7-09f7014df9c4","year":2020},"citing_paper":{"arxiv_id":"2606.28141","last_updated":"2026-06-26T14:40:34Z","snapshot_observed_at":"2026-08-01T13:15:41.790977Z","submitted_at":"2026-06-26T14:40:34Z","title":"Transition from Diffusion to Drift-Dominated Cosmic Ray Transport and the Origin of the Knee","version":1},"reference_index":22,"source":"pdf_text","source_observed_at":"2026-06-29T02:38:04.107001Z"},"links":{"cited_paper":"/paper/2007.04294","citing_paper":"/paper/2606.28141"},"observation_digest":"sha256:31a8966591d80ebb015faf54e933af36c9a3c7062c457964597f0f71029968c9","observation_id":"a204f296-8fa9-4d54-b050-ec8455e93d40","resolution":{"observed_at":"2026-07-01T18:05:58.772302Z","resolver_source":"arxiv_id","status":"verified_exact"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-22T06:32:14.747728+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-22T06:32:14.747728+00:00","source":"crossref"},{"observed_at":"2026-08-22T06:32:06.552537+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":{"arxiv_id":"2007.04294","last_updated":"2020-07-08T17:45:43Z","snapshot_observed_at":"2026-08-09T21:39:37.231164Z","submitted_at":"2020-07-08T17:45:43Z","title":"The low rate of Galactic pevatrons","version":1},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2007.04294","snapshot_observed_at":"2026-08-02T02:26:39.830416Z","title":"2020 , month = dec, pages =","venue":null,"work_id":null,"year":2020},"citing_paper":{"arxiv_id":"2607.14363","last_updated":"2026-07-15T21:01:45Z","snapshot_observed_at":"2026-08-15T08:27:19.643357Z","submitted_at":"2026-07-15T21:01:45Z","title":"CRESCENDO II: Spectral cosmic rays with improved energy losses and realistic supernova seeding","version":1},"reference_index":55,"source":"arxiv_source","source_observed_at":"2026-08-02T02:26:39.830416Z"},"links":{"cited_paper":"/paper/2007.04294","citing_paper":"/paper/2607.14363"},"observation_digest":"sha256:cf164675b46a55b159bbe5167841d9d18a67e335a6f4bb0d0b590853efea57fb","observation_id":"6ffd4481-e436-4fc9-955c-e61bab6ac3d3","resolution":{"observed_at":"2026-08-02T02:26:39.830416Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}}],"links":{"evidence":"/evidence","html":"/paper/2007.04294/citation-record","integrity":"/paper/2007.04294/integrity","json":"/paper/2007.04294/citation-record.json","paper":"/paper/2007.04294"},"outbound":[],"paper":{"arxiv_id":"2007.04294","last_updated":"2020-07-08T17:45:43Z","latest_version":1,"primary_category":"astro-ph.HE","snapshot_observed_at":"2026-08-09T21:39:37.231164Z","submitted_at":"2020-07-08T17:45:43Z","title":"The low rate of Galactic pevatrons"},"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":"2026-08-22T06:32:14.747728+00:00","source":"crossref"},{"observed_at":"2026-08-22T06:32:06.552537+00:00","source":"retraction_watch"}],"thesis":"As of 22 August 2026, this Paper Citation Record lists 0 of 0 outbound references and 3 inbound Pith citation observations for arXiv:2007.04294."}