{"as_of":"2026-08-11T20:42:00Z","caps":{"database_statements":6,"inbound":100,"outbound":100},"context_digest":"sha256:0d2268664784c93cde255c7f2b91f3199b40f4a6bf59d46b9e8bfec7dc9a1cd0","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":"2026-08-11T06:34:44.6726+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":"2026-08-11T00:08:01.298175Z","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":"2026-05-19T13:12:18.913970Z","state":"measured"}],"external_citation_measurements":[],"inbound":[{"citation":{"cited_paper":{"arxiv_id":"1307.4350","last_updated":"2013-10-07T21:21:02Z","snapshot_observed_at":"2026-07-06T03:18:21.944740Z","submitted_at":"2013-07-16T17:28:30Z","title":"Effective Field Theory of Cosmological Perturbations","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"1307.4350","snapshot_observed_at":"2026-08-11T00:08:01.298175Z","title":"Piazza and F","venue":null,"work_id":null,"year":2013},"citing_paper":{"arxiv_id":"2412.19782","last_updated":"2025-01-21T19:00:10Z","snapshot_observed_at":"2026-08-11T09:42:41.294222Z","submitted_at":"2024-12-27T18:25:17Z","title":"Cosmological perturbations meet Wheeler DeWitt","version":2},"reference_index":6,"source":"pdf_text","source_observed_at":"2026-08-11T00:08:01.298175Z"},"links":{"cited_paper":"/paper/1307.4350","citing_paper":"/paper/2412.19782"},"observation_digest":"sha256:fd8f2405fa23a94087e497db24520090e9a835d06b654012e91aaacd4642ec2c","observation_id":"6c4fe30f-5c80-4d85-9bd6-dc25185498e4","resolution":{"observed_at":"2026-08-11T00:08:01.298175Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"1307.4350","last_updated":"2013-10-07T21:21:02Z","snapshot_observed_at":"2026-07-06T03:18:21.944740Z","submitted_at":"2013-07-16T17:28:30Z","title":"Effective Field Theory of Cosmological Perturbations","version":2},"cited_work":{"arxiv_id":"1307.4350","doi":null,"metadata_source":"pith","pith_arxiv_id":"1307.4350","snapshot_observed_at":"2026-06-05T21:23:00.469572Z","title":"Effective Field Theory of Cosmological Perturbations","venue":"hep-th","work_id":"f1246e13-ce74-4b5d-a669-a29a7895aeac","year":2013},"citing_paper":{"arxiv_id":"2505.24732","last_updated":"2026-04-11T09:17:44Z","snapshot_observed_at":"2026-07-06T02:11:23.670680Z","submitted_at":"2025-05-30T15:54:16Z","title":"The Quintom theory of dark energy after DESI DR2","version":3},"reference_index":198,"source":"pdf_text","source_observed_at":"2026-05-19T13:08:20.192767Z"},"links":{"cited_paper":"/paper/1307.4350","citing_paper":"/paper/2505.24732"},"observation_digest":"sha256:9ed8e488930dad01f0518b744fc33aae71f226013ddf9fb6ec67a2cc5140061f","observation_id":"d8ef9525-cad5-4696-902b-c687a4638f4e","resolution":{"observed_at":"2026-05-19T13:12:18.915742Z","resolver_source":"local_arxiv","status":"verified_exact"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-11T06:34:44.6726+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-11T06:34:44.6726+00:00","source":"crossref"},{"observed_at":"2026-08-11T06:34:36.301508+00:00","source":"retraction_watch"}],"state":"measured"}}],"links":{"evidence":"/evidence","html":"/paper/1307.4350/citation-record","integrity":"/paper/1307.4350/integrity","json":"/paper/1307.4350/citation-record.json","paper":"/paper/1307.4350"},"outbound":[],"paper":{"arxiv_id":"1307.4350","last_updated":"2013-10-07T21:21:02Z","latest_version":2,"primary_category":"hep-th","snapshot_observed_at":"2026-07-06T03:18:21.944740Z","submitted_at":"2013-07-16T17:28:30Z","title":"Effective Field Theory of Cosmological Perturbations"},"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":"2026-08-11T06:34:44.6726+00:00","source":"crossref"},{"observed_at":"2026-08-11T06:34:36.301508+00:00","source":"retraction_watch"}],"thesis":"As of 11 August 2026, this Paper Citation Record lists 0 of 0 outbound references and 2 inbound Pith citation observations for arXiv:1307.4350."}