{"as_of":"2026-08-14T00:11:00Z","caps":{"database_statements":6,"inbound":100,"outbound":100},"context_digest":"sha256:c5caaa99bc48aa58be99427586548080ed092c21b899c5f0a7007de27da0ef0c","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":"2026-08-13T06:32:02.005865+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":"2026-08-01T06:02:14.899670Z","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":"2026-07-03T18:28:48.543947Z","state":"measured"}],"external_citation_measurements":[],"inbound":[{"citation":{"cited_paper":{"arxiv_id":"2209.05594","last_updated":"2022-10-31T16:51:48Z","snapshot_observed_at":"2026-08-13T14:28:17.572277Z","submitted_at":"2022-09-12T20:20:48Z","title":"SALT3-NIR: Taking the Open-Source Type Ia Supernova Model to Longer Wavelengths for Next-Generation Cosmological Measurements","version":2},"cited_work":{"arxiv_id":"2209.05594","doi":null,"metadata_source":"arxiv_reference","pith_arxiv_id":"2209.05594","snapshot_observed_at":"2026-07-03T18:28:48.543947Z","title":null,"venue":null,"work_id":"59286dd1-bccb-4d09-9fac-8eac0944f1a4","year":2022},"citing_paper":{"arxiv_id":"2606.17142","last_updated":"2026-06-15T18:00:02Z","snapshot_observed_at":"2026-07-06T23:52:47.494791Z","submitted_at":"2026-06-15T18:00:02Z","title":"Hawai`i Supernova Flows: Bulk Flow Measurements using SNe Ia in the Optical and NIR","version":1},"reference_index":68,"source":"arxiv_source","source_observed_at":"2026-06-27T03:07:55.886816Z"},"links":{"cited_paper":"/paper/2209.05594","citing_paper":"/paper/2606.17142"},"observation_digest":"sha256:c4cc8ce3ed0b2684b085c2edaa9af0df947ae35dcba8218c07bb84534b32fa45","observation_id":"b4caaa06-b614-48a9-8892-7c734bec3a05","resolution":{"observed_at":"2026-07-03T18:28:48.545793Z","resolver_source":"arxiv_id","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":"2209.05594","last_updated":"2022-10-31T16:51:48Z","snapshot_observed_at":"2026-08-13T14:28:17.572277Z","submitted_at":"2022-09-12T20:20:48Z","title":"SALT3-NIR: Taking the Open-Source Type Ia Supernova Model to Longer Wavelengths for Next-Generation Cosmological Measurements","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2209.05594","snapshot_observed_at":"2026-08-01T06:02:14.899670Z","title":"arXiv , author =:2209.05594 , journal =","venue":null,"work_id":null,"year":null},"citing_paper":{"arxiv_id":"2607.22050","last_updated":"2026-08-04T09:11:55Z","snapshot_observed_at":"2026-08-08T13:19:27.261652Z","submitted_at":"2026-07-24T07:35:53Z","title":"ZTF SN Ia DR2 follow-up: early excess in Type Ia supernova light curves","version":1},"reference_index":245,"source":"arxiv_source","source_observed_at":"2026-08-01T06:02:14.899670Z"},"links":{"cited_paper":"/paper/2209.05594","citing_paper":"/paper/2607.22050"},"observation_digest":"sha256:77be99547517b131c97413526d75f2ecdc6b0341ea54e48fb3deb2d6cf4d8f35","observation_id":"0ee82d00-8b65-45be-affc-aa1f0d76bf9a","resolution":{"observed_at":"2026-08-01T06:02:14.899670Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}}],"links":{"evidence":"/evidence","html":"/paper/2209.05594/citation-record","integrity":"/paper/2209.05594/integrity","json":"/paper/2209.05594/citation-record.json","paper":"/paper/2209.05594"},"outbound":[],"paper":{"arxiv_id":"2209.05594","last_updated":"2022-10-31T16:51:48Z","latest_version":2,"primary_category":"astro-ph.CO","snapshot_observed_at":"2026-08-13T14:28:17.572277Z","submitted_at":"2022-09-12T20:20:48Z","title":"SALT3-NIR: Taking the Open-Source Type Ia Supernova Model to Longer Wavelengths for Next-Generation Cosmological Measurements"},"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 14 August 2026, this Paper Citation Record lists 0 of 0 outbound references and 2 inbound Pith citation observations for arXiv:2209.05594."}