{"as_of":"2026-08-07T17:34:00Z","caps":{"database_statements":6,"inbound":100,"outbound":100},"context_digest":"sha256:868439af68cf577e93b29adb5c3006a832e2aa4cc4d91e7eebdb5bb94de872ae","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":"2026-08-07T06:34:17.273281+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":"2026-08-06T13:05:39.890853Z","state":"measured"},{"denominator":1,"lane":"external_citation_measurements","note":"A source-named dated measurement, never combined with another source.","records_observed":0,"source":"cited_works","source_observed_at":null,"state":"measured"}],"external_citation_measurements":[],"inbound":[{"citation":{"cited_paper":{"arxiv_id":"2202.07967","last_updated":"2022-08-18T11:52:13Z","snapshot_observed_at":"2026-07-06T12:38:19.702992Z","submitted_at":"2022-02-16T10:20:24Z","title":"Magnetic support for neutrino-driven explosion of 3D non-rotating core-collapse supernova models","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2202.07967","snapshot_observed_at":"2026-08-04T19:19:16.611362Z","title":"MNRAS516(2), 1752–1767 (2022) https://doi.org/10.1093/mnras/ stac2335 arXiv:2202.07967 [astro-ph.HE]","venue":null,"work_id":null,"year":2022},"citing_paper":{"arxiv_id":"2509.09419","last_updated":"2025-09-11T13:01:45Z","snapshot_observed_at":"2026-08-07T17:10:25.407213Z","submitted_at":"2025-09-11T13:01:45Z","title":"Impact of rotation on the accretion of entropy perturbations in collapsing massive stars","version":1},"reference_index":47,"source":"pdf_text","source_observed_at":"2026-08-04T19:19:16.611362Z"},"links":{"cited_paper":"/paper/2202.07967","citing_paper":"/paper/2509.09419"},"observation_digest":"sha256:7b2e0b5e8202d43a4a51753ec452868a7e6c166281167c3c7e115008b1c9eddf","observation_id":"e90770db-46b3-4f42-93cd-28c1fd143de2","resolution":{"observed_at":"2026-08-04T19:19:16.611362Z","resolver_source":null,"status":"malformed_identifier"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2202.07967","last_updated":"2022-08-18T11:52:13Z","snapshot_observed_at":"2026-07-06T12:38:19.702992Z","submitted_at":"2022-02-16T10:20:24Z","title":"Magnetic support for neutrino-driven explosion of 3D non-rotating core-collapse supernova models","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2202.07967","snapshot_observed_at":"2026-08-06T13:05:39.890853Z","title":", keywords =","venue":null,"work_id":null,"year":null},"citing_paper":{"arxiv_id":"2608.04954","last_updated":"2026-08-05T15:24:33Z","snapshot_observed_at":"2026-08-07T17:26:52.883714Z","submitted_at":"2026-08-05T15:24:33Z","title":"3D simulations of a complete convective silicon shell burning phase","version":1},"reference_index":241,"source":"arxiv_source","source_observed_at":"2026-08-06T13:05:39.890853Z"},"links":{"cited_paper":"/paper/2202.07967","citing_paper":"/paper/2608.04954"},"observation_digest":"sha256:bff99fe63a203db9e150aa5f92662cb5989a85f69b8452ac82bd51d7e39aad69","observation_id":"f617fad6-dc28-4f0e-a220-47745428dfb1","resolution":{"observed_at":"2026-08-06T13:05:39.890853Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}}],"links":{"evidence":"/evidence","html":"/paper/2202.07967/citation-record","integrity":"/paper/2202.07967/integrity","json":"/paper/2202.07967/citation-record.json","paper":"/paper/2202.07967"},"outbound":[],"paper":{"arxiv_id":"2202.07967","last_updated":"2022-08-18T11:52:13Z","latest_version":2,"primary_category":"astro-ph.HE","snapshot_observed_at":"2026-07-06T12:38:19.702992Z","submitted_at":"2022-02-16T10:20:24Z","title":"Magnetic support for neutrino-driven explosion of 3D non-rotating core-collapse supernova models"},"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":"2026-08-07T06:34:17.273281+00:00","source":"crossref"},{"observed_at":"2026-08-07T06:34:11.927384+00:00","source":"retraction_watch"}],"thesis":"As of 7 August 2026, this Paper Citation Record lists 0 of 0 outbound references and 2 inbound Pith citation observations for arXiv:2202.07967."}