{"as_of":"2026-08-05T17:05:00Z","caps":{"database_statements":6,"inbound":100,"outbound":100},"context_digest":"sha256:963d41b19741a60c7c96069d587d2c09ba5220cbc984a5270b38a40c73ff56cc","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":"2026-08-05T06:32:48.257954+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":"2026-08-01T16:40:19.420040Z","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":"2026-06-30T23:25:07.721770Z","state":"measured"}],"external_citation_measurements":[],"inbound":[{"citation":{"cited_paper":{"arxiv_id":"2211.12457","last_updated":"2023-08-08T14:28:59Z","snapshot_observed_at":"2026-08-01T16:02:11.745318Z","submitted_at":"2022-11-22T18:14:28Z","title":"Euclid: Modelling massive neutrinos in cosmology -- a code comparison","version":2},"cited_work":{"arxiv_id":"2211.12457","doi":null,"metadata_source":"arxiv_reference","pith_arxiv_id":"2211.12457","snapshot_observed_at":"2026-06-30T23:25:07.721770Z","title":"Euclid: Modelling massive neutrinos in cosmology – a code comparison,","venue":null,"work_id":"06b32904-74e7-44da-b525-d7ef9e0c78c2","year":2023},"citing_paper":{"arxiv_id":"2605.05114","last_updated":"2026-06-03T14:56:40Z","snapshot_observed_at":"2026-07-06T23:17:48.161262Z","submitted_at":"2026-05-06T16:45:33Z","title":"Effective Field Theory of Large Scale Structure and Newtonian Motion Gauges","version":2},"reference_index":58,"source":"pdf_text","source_observed_at":"2026-06-30T23:23:06.869558Z"},"links":{"cited_paper":"/paper/2211.12457","citing_paper":"/paper/2605.05114"},"observation_digest":"sha256:c1f4beec3ae1b2cf87dce0b95b9867494d179ae791cdbeae70aff110d6cc4f5d","observation_id":"b32e9425-fe29-44bd-8893-5f09d6e9f239","resolution":{"observed_at":"2026-06-30T23:25:07.723495Z","resolver_source":"arxiv_id","status":"verified_exact"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-05T06:32:48.257954+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-05T06:32:48.257954+00:00","source":"crossref"},{"observed_at":"2026-08-05T06:32:44.755628+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":{"arxiv_id":"2211.12457","last_updated":"2023-08-08T14:28:59Z","snapshot_observed_at":"2026-08-01T16:02:11.745318Z","submitted_at":"2022-11-22T18:14:28Z","title":"Euclid: Modelling massive neutrinos in cosmology -- a code comparison","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2211.12457","snapshot_observed_at":"2026-08-01T16:40:19.420040Z","title":"and others","venue":null,"work_id":null,"year":2023},"citing_paper":{"arxiv_id":"2607.17929","last_updated":"2026-07-20T13:27:31Z","snapshot_observed_at":"2026-08-01T16:40:18.383675Z","submitted_at":"2026-07-20T13:27:31Z","title":"gevolution 2.0: GPU-accelerated relativistic N-body simulations for cosmology","version":1},"reference_index":10,"source":"arxiv_source","source_observed_at":"2026-08-01T16:40:19.420040Z"},"links":{"cited_paper":"/paper/2211.12457","citing_paper":"/paper/2607.17929"},"observation_digest":"sha256:95df974f35c692f66888b0dad3e4a23971e1cb0c77008c87099a31bbc93c9164","observation_id":"e5f5e2e6-0554-462e-bab6-abf26cf5cb37","resolution":{"observed_at":"2026-08-01T16:40:19.420040Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}}],"links":{"evidence":"/evidence","html":"/paper/2211.12457/citation-record","integrity":"/paper/2211.12457/integrity","json":"/paper/2211.12457/citation-record.json","paper":"/paper/2211.12457"},"outbound":[],"paper":{"arxiv_id":"2211.12457","last_updated":"2023-08-08T14:28:59Z","latest_version":2,"primary_category":"astro-ph.CO","snapshot_observed_at":"2026-08-01T16:02:11.745318Z","submitted_at":"2022-11-22T18:14:28Z","title":"Euclid: Modelling massive neutrinos in cosmology -- a code comparison"},"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":"2026-08-05T06:32:48.257954+00:00","source":"crossref"},{"observed_at":"2026-08-05T06:32:44.755628+00:00","source":"retraction_watch"}],"thesis":"As of 5 August 2026, this Paper Citation Record lists 0 of 0 outbound references and 2 inbound Pith citation observations for arXiv:2211.12457."}