{"as_of":"2026-08-05T20:45:00Z","caps":{"database_statements":6,"inbound":100,"outbound":100},"context_digest":"sha256:c62de206463338512a564a448a0089495c6b00abefd99f32c6c4b289eae9f966","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":"2026-06-26T19:28:46.080115Z","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":"2026-07-04T02:39:25.249417Z","state":"measured"}],"external_citation_measurements":[],"inbound":[{"citation":{"cited_paper":{"arxiv_id":"2410.10616","last_updated":"2024-10-14T15:20:36Z","snapshot_observed_at":"2026-07-06T19:33:08.264958Z","submitted_at":"2024-10-14T15:20:36Z","title":"Field-level cosmological model selection: field-level simulation-based inference for Stage IV cosmic shear can distinguish dynamical dark energy","version":1},"cited_work":{"arxiv_id":"2410.10616","doi":null,"metadata_source":"arxiv_reference","pith_arxiv_id":"2410.10616","snapshot_observed_at":"2026-07-04T02:39:25.249417Z","title":"arXiv preprint arXiv:2410.10616 , year=","venue":null,"work_id":"2291ca45-e95c-4396-8812-1c0d5c38b7ee","year":2024},"citing_paper":{"arxiv_id":"2511.03636","last_updated":"2026-04-11T11:40:44Z","snapshot_observed_at":"2026-07-06T22:34:58.108904Z","submitted_at":"2025-11-05T16:54:17Z","title":"Quantifying Weighted Morphological Content of Large-Scale Structures via Simulation-Based Inference","version":2},"reference_index":73,"source":"pdf_text","source_observed_at":"2026-05-18T01:11:20.309084Z"},"links":{"cited_paper":"/paper/2410.10616","citing_paper":"/paper/2511.03636"},"observation_digest":"sha256:67a36a4a3f23bed975ea86066dd3fd8cf95b37dc5a9e8521d3669b419c3965d1","observation_id":"c380fa3f-a3f8-4102-8a8c-f715a256a48e","resolution":{"observed_at":"2026-05-18T01:12:15.338028Z","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":"2410.10616","last_updated":"2024-10-14T15:20:36Z","snapshot_observed_at":"2026-07-06T19:33:08.264958Z","submitted_at":"2024-10-14T15:20:36Z","title":"Field-level cosmological model selection: field-level simulation-based inference for Stage IV cosmic shear can distinguish dynamical dark energy","version":1},"cited_work":{"arxiv_id":"2410.10616","doi":null,"metadata_source":"arxiv_reference","pith_arxiv_id":"2410.10616","snapshot_observed_at":"2026-07-04T02:39:25.249417Z","title":"arXiv preprint arXiv:2410.10616 , year=","venue":null,"work_id":"2291ca45-e95c-4396-8812-1c0d5c38b7ee","year":2024},"citing_paper":{"arxiv_id":"2606.19518","last_updated":"2026-06-17T19:07:03Z","snapshot_observed_at":"2026-07-06T23:54:46.974663Z","submitted_at":"2026-06-17T19:07:03Z","title":"Increasing the sensitivity of full-shape galaxy clustering measurements in configuration-space with three-point statistics","version":1},"reference_index":52,"source":"arxiv_source","source_observed_at":"2026-06-26T19:28:46.080115Z"},"links":{"cited_paper":"/paper/2410.10616","citing_paper":"/paper/2606.19518"},"observation_digest":"sha256:973abd5dc512bd7a06a2ffbacc46c89267ae219a9b892e73d87794b538589fb0","observation_id":"885cc131-a7bd-47f9-a282-7e399390fcc3","resolution":{"observed_at":"2026-07-04T02:39:25.251043Z","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"}}],"links":{"evidence":"/evidence","html":"/paper/2410.10616/citation-record","integrity":"/paper/2410.10616/integrity","json":"/paper/2410.10616/citation-record.json","paper":"/paper/2410.10616"},"outbound":[],"paper":{"arxiv_id":"2410.10616","last_updated":"2024-10-14T15:20:36Z","latest_version":1,"primary_category":"astro-ph.CO","snapshot_observed_at":"2026-07-06T19:33:08.264958Z","submitted_at":"2024-10-14T15:20:36Z","title":"Field-level cosmological model selection: field-level simulation-based inference for Stage IV cosmic shear can distinguish dynamical dark energy"},"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:2410.10616."}