{"as_of":"2026-08-13T23:27:00Z","caps":{"database_statements":6,"inbound":100,"outbound":100},"context_digest":"sha256:da354fb6482b22bcb23762dd5088ea541b2aa84ab6187f8254451494cb3c98e1","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":"2026-08-13T06:32:02.005865+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":"2026-08-12T20:25:19.837322Z","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":"2026-08-12T20:25:20.798248Z","state":"measured"}],"external_citation_measurements":[],"inbound":[{"citation":{"cited_paper":{"arxiv_id":"1111.4492","last_updated":"2012-02-20T12:06:19Z","snapshot_observed_at":"2026-07-06T02:37:50.966961Z","submitted_at":"2011-11-18T21:25:42Z","title":"Type-Ia supernova rates and the progenitor problem, a review","version":2},"cited_work":{"arxiv_id":"1111.4492","doi":null,"metadata_source":"pith","pith_arxiv_id":"1111.4492","snapshot_observed_at":"2026-08-12T20:25:20.798248Z","title":"Type-Ia supernova rates and the progenitor problem, a review","venue":"astro-ph.CO","work_id":"20509f62-967d-4e17-911c-3151cd343df4","year":2011},"citing_paper":{"arxiv_id":"2411.09740","last_updated":"2025-06-05T13:48:28Z","snapshot_observed_at":"2026-08-12T20:19:13.177167Z","submitted_at":"2024-11-14T19:00:02Z","title":"Type Ia supernovae","version":2},"reference_index":66,"source":"arxiv_source","source_observed_at":"2026-08-12T20:25:19.837322Z"},"links":{"cited_paper":"/paper/1111.4492","citing_paper":"/paper/2411.09740"},"observation_digest":"sha256:05884b935ac7c81d54a9e0e14af8291bf6f18e90915decf2c6b7803a38009fd2","observation_id":"8d724026-3bf2-44e2-8414-27734a4817d0","resolution":{"observed_at":"2026-08-12T20:25:20.802677Z","resolver_source":"local_arxiv","status":"verified_exact"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-13T06:32:02.005865+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-13T06:32:02.005865+00:00","source":"crossref"},{"observed_at":"2026-08-13T06:31:53.387327+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":{"arxiv_id":"1111.4492","last_updated":"2012-02-20T12:06:19Z","snapshot_observed_at":"2026-07-06T02:37:50.966961Z","submitted_at":"2011-11-18T21:25:42Z","title":"Type-Ia supernova rates and the progenitor problem, a review","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"1111.4492","snapshot_observed_at":"2026-07-11T06:21:15.541076Z","title":"2012 , month = jan, pages =","venue":null,"work_id":null,"year":2012},"citing_paper":{"arxiv_id":"2607.05524","last_updated":"2026-07-06T18:02:19Z","snapshot_observed_at":"2026-08-06T20:15:42.740123Z","submitted_at":"2026-07-06T18:02:19Z","title":"Survival is not Enough: Dust Sputtering, Growth, and H$_2$ Formation in Galactic Winds","version":1},"reference_index":186,"source":"arxiv_source","source_observed_at":"2026-07-11T06:21:15.541076Z"},"links":{"cited_paper":"/paper/1111.4492","citing_paper":"/paper/2607.05524"},"observation_digest":"sha256:acd6c46a3aaeecaa2bff8c7a9c879a67304c2337ee7339ee0a1a965a508154b4","observation_id":"dea5fce4-b992-454c-99e8-1ce7f78ebb4c","resolution":{"observed_at":"2026-07-11T06:21:15.541076Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"1111.4492","last_updated":"2012-02-20T12:06:19Z","snapshot_observed_at":"2026-07-06T02:37:50.966961Z","submitted_at":"2011-11-18T21:25:42Z","title":"Type-Ia supernova rates and the progenitor problem, a review","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"1111.4492","snapshot_observed_at":"2026-08-02T03:50:10.209860Z","title":", keywords =","venue":null,"work_id":null,"year":null},"citing_paper":{"arxiv_id":"2607.13786","last_updated":"2026-07-15T12:41:44Z","snapshot_observed_at":"2026-08-12T16:58:10.679092Z","submitted_at":"2026-07-15T12:41:44Z","title":"RABBITS IV: Stellar feedback and SMBH merging time-scales in the sub-Milky Way mass regime","version":1},"reference_index":93,"source":"arxiv_source","source_observed_at":"2026-08-02T03:50:10.209860Z"},"links":{"cited_paper":"/paper/1111.4492","citing_paper":"/paper/2607.13786"},"observation_digest":"sha256:5cae7333c00ea2184172d47493b04388c18f6c844fee88d7bf233b081d8310af","observation_id":"d3dcf243-84b6-4076-a61e-d48dbfe4e5de","resolution":{"observed_at":"2026-08-02T03:50:10.209860Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}}],"links":{"evidence":"/evidence","html":"/paper/1111.4492/citation-record","integrity":"/paper/1111.4492/integrity","json":"/paper/1111.4492/citation-record.json","paper":"/paper/1111.4492"},"outbound":[],"paper":{"arxiv_id":"1111.4492","last_updated":"2012-02-20T12:06:19Z","latest_version":2,"primary_category":"astro-ph.CO","snapshot_observed_at":"2026-07-06T02:37:50.966961Z","submitted_at":"2011-11-18T21:25:42Z","title":"Type-Ia supernova rates and the progenitor problem, a review"},"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":"2026-08-13T06:32:02.005865+00:00","source":"crossref"},{"observed_at":"2026-08-13T06:31:53.387327+00:00","source":"retraction_watch"}],"thesis":"As of 13 August 2026, this Paper Citation Record lists 0 of 0 outbound references and 3 inbound Pith citation observations for arXiv:1111.4492."}