{"as_of":"2026-08-13T09:47:00Z","caps":{"database_statements":6,"inbound":100,"outbound":100},"context_digest":"sha256:c41230b70a04d906194434a1533b4812e2ad68162f82c60c640858b39039738c","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":4,"lane":"standing_notices","note":"One-hop event checks from named stored sources.","records_observed":4,"source":"scholarly_work_events, retraction_status_cache","source_observed_at":"2026-08-13T06:32:02.005865+00:00","state":"measured"},{"denominator":4,"lane":"inbound_itemization","note":"Pith citing papers itemized under the disclosed page cap.","records_observed":4,"source":"paper_references, paper_reference_links","source_observed_at":"2026-08-11T21:31:38.615074Z","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":"2026-07-04T15:29:55.177999Z","state":"measured"}],"external_citation_measurements":[],"inbound":[{"citation":{"cited_paper":{"arxiv_id":"2312.08934","last_updated":"2024-07-19T09:49:38Z","snapshot_observed_at":"2026-08-13T05:02:29.646041Z","submitted_at":"2023-12-14T13:40:47Z","title":"Accurate field-level weak lensing inference for precision cosmology","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2312.08934","snapshot_observed_at":"2026-08-11T21:31:38.615074Z","title":null,"venue":null,"work_id":null,"year":2024},"citing_paper":{"arxiv_id":"2412.04443","last_updated":"2025-07-16T23:44:34Z","snapshot_observed_at":"2026-08-13T09:31:39.995727Z","submitted_at":"2024-12-05T18:57:00Z","title":"Diagnosing Systematic Effects Using the Inferred Initial Power Spectrum","version":2},"reference_index":128,"source":"pdf_text","source_observed_at":"2026-08-11T21:31:38.615074Z"},"links":{"cited_paper":"/paper/2312.08934","citing_paper":"/paper/2412.04443"},"observation_digest":"sha256:6f89fee99ea83b0051db0eb7493e69af139f1ccdb1eab9d6052806ec0bd2cca2","observation_id":"6476e220-217d-4c06-840c-5865ff2511b7","resolution":{"observed_at":"2026-08-11T21:31:38.615074Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2312.08934","last_updated":"2024-07-19T09:49:38Z","snapshot_observed_at":"2026-08-13T05:02:29.646041Z","submitted_at":"2023-12-14T13:40:47Z","title":"Accurate field-level weak lensing inference for precision cosmology","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2312.08934","snapshot_observed_at":"2026-08-08T23:21:44.966503Z","title":null,"venue":null,"work_id":null,"year":2024},"citing_paper":{"arxiv_id":"2502.04158","last_updated":"2025-02-06T15:44:05Z","snapshot_observed_at":"2026-08-12T14:44:28.073030Z","submitted_at":"2025-02-06T15:44:05Z","title":"Diffusion-based mass map reconstruction from weak lensing data","version":1},"reference_index":28,"source":"pdf_text","source_observed_at":"2026-08-08T23:21:44.966503Z"},"links":{"cited_paper":"/paper/2312.08934","citing_paper":"/paper/2502.04158"},"observation_digest":"sha256:cedaad60ba63d20ee4e004749bae0f2aafc06fa834b75730042e41a5f2e48e2d","observation_id":"4e6c0b20-79f1-4acc-b74e-4ad80b984c89","resolution":{"observed_at":"2026-08-08T23:21:44.966503Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2312.08934","last_updated":"2024-07-19T09:49:38Z","snapshot_observed_at":"2026-08-13T05:02:29.646041Z","submitted_at":"2023-12-14T13:40:47Z","title":"Accurate field-level weak lensing inference for precision cosmology","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2312.08934","snapshot_observed_at":"2026-08-04T11:25:25.757543Z","title":null,"venue":null,"work_id":null,"year":2024},"citing_paper":{"arxiv_id":"2510.05206","last_updated":"2025-10-06T18:00:05Z","snapshot_observed_at":"2026-08-09T15:07:13.979046Z","submitted_at":"2025-10-06T18:00:05Z","title":"DISCO-DJ II: a differentiable particle-mesh code for cosmology","version":1},"reference_index":9,"source":"pdf_text","source_observed_at":"2026-08-04T11:25:25.757543Z"},"links":{"cited_paper":"/paper/2312.08934","citing_paper":"/paper/2510.05206"},"observation_digest":"sha256:ae78605d388bff0b5b39d9c27d3d85620a23730c7f55fb8490f960fa89fd1250","observation_id":"7b9b9c69-c1f3-4170-8e63-28c9ca52dcf0","resolution":{"observed_at":"2026-08-04T11:25:25.757543Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2312.08934","last_updated":"2024-07-19T09:49:38Z","snapshot_observed_at":"2026-08-13T05:02:29.646041Z","submitted_at":"2023-12-14T13:40:47Z","title":"Accurate field-level weak lensing inference for precision cosmology","version":2},"cited_work":{"arxiv_id":"2312.08934","doi":null,"metadata_source":"arxiv_reference","pith_arxiv_id":"2312.08934","snapshot_observed_at":"2026-07-04T15:29:55.177999Z","title":null,"venue":null,"work_id":"7c287742-54af-4e2c-8ea6-d30a52331263","year":2024},"citing_paper":{"arxiv_id":"2606.26234","last_updated":"2026-06-24T18:00:02Z","snapshot_observed_at":"2026-08-06T10:28:45.654237Z","submitted_at":"2026-06-24T18:00:02Z","title":"Lyman-Alpha Forest and its Cross-Correlation with High-Redshift Galaxies in Effective Field Theory at the Field Level","version":1},"reference_index":197,"source":"pdf_text","source_observed_at":"2026-06-26T01:38:09.398349Z"},"links":{"cited_paper":"/paper/2312.08934","citing_paper":"/paper/2606.26234"},"observation_digest":"sha256:2a43222c8f7be60bb8349665638a3cc6474ac6365688f3123fb85a35d7ebc0d8","observation_id":"39b849a4-6c02-44f7-bf97-8bade8de4957","resolution":{"observed_at":"2026-07-04T15:29:55.179756Z","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"}}],"links":{"evidence":"/evidence","html":"/paper/2312.08934/citation-record","integrity":"/paper/2312.08934/integrity","json":"/paper/2312.08934/citation-record.json","paper":"/paper/2312.08934"},"outbound":[],"paper":{"arxiv_id":"2312.08934","last_updated":"2024-07-19T09:49:38Z","latest_version":2,"primary_category":"astro-ph.CO","snapshot_observed_at":"2026-08-13T05:02:29.646041Z","submitted_at":"2023-12-14T13:40:47Z","title":"Accurate field-level weak lensing inference for precision cosmology"},"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 4 inbound Pith citation observations for arXiv:2312.08934."}