{"as_of":"2026-08-04T18:01:00Z","caps":{"database_statements":6,"inbound":100,"outbound":100},"context_digest":"sha256:94c296e95c7828f15eaac691cd599e2bcfa09072592a463fd01c443993cb7d08","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":8,"lane":"standing_notices","note":"One-hop event checks from named stored sources.","records_observed":8,"source":"scholarly_work_events, retraction_status_cache","source_observed_at":"2026-08-04T06:34:03.388597+00:00","state":"measured"},{"denominator":8,"lane":"inbound_itemization","note":"Pith citing papers itemized under the disclosed page cap.","records_observed":8,"source":"paper_references, paper_reference_links","source_observed_at":"2026-08-03T08:42:00.263097Z","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":"2026-07-01T12:25:44.409378Z","state":"measured"}],"external_citation_measurements":[],"inbound":[{"citation":{"cited_paper":{"arxiv_id":"2210.17044","last_updated":"2023-02-06T19:59:21Z","snapshot_observed_at":"2026-08-04T14:30:40.736961Z","submitted_at":"2022-10-31T03:46:16Z","title":"Cosmological constraints from the power spectrum of eBOSS quasars","version":2},"cited_work":{"arxiv_id":"2210.17044","doi":null,"metadata_source":"arxiv_reference","pith_arxiv_id":"2210.17044","snapshot_observed_at":"2026-07-01T12:25:44.409378Z","title":"Chudaykin and M.M","venue":null,"work_id":"0f7f34c9-d659-4e09-8ce4-e9239c8489b6","year":2022},"citing_paper":{"arxiv_id":"2411.12021","last_updated":"2025-11-24T12:55:36Z","snapshot_observed_at":"2026-07-06T02:11:23.670680Z","submitted_at":"2024-11-18T20:03:34Z","title":"DESI 2024 V: Full-Shape Galaxy Clustering from Galaxies and Quasars","version":5},"reference_index":131,"source":"pdf_text","source_observed_at":"2026-05-17T06:00:49.044220Z"},"links":{"cited_paper":"/paper/2210.17044","citing_paper":"/paper/2411.12021"},"observation_digest":"sha256:4fcaf94efdd3d7201f5d19edd969b143d9b4709b47907e0f9c8ad2edb78a408f","observation_id":"d7dcbd41-1ebb-4f4a-8f50-4ba6d730055e","resolution":{"observed_at":"2026-05-17T06:00:49.862016Z","resolver_source":"arxiv_id","status":"verified_exact"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-04T06:34:03.388597+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-04T06:34:03.388597+00:00","source":"crossref"},{"observed_at":"2026-08-04T06:33:57.428241+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":{"arxiv_id":"2210.17044","last_updated":"2023-02-06T19:59:21Z","snapshot_observed_at":"2026-08-04T14:30:40.736961Z","submitted_at":"2022-10-31T03:46:16Z","title":"Cosmological constraints from the power spectrum of eBOSS quasars","version":2},"cited_work":{"arxiv_id":"2210.17044","doi":null,"metadata_source":"arxiv_reference","pith_arxiv_id":"2210.17044","snapshot_observed_at":"2026-07-01T12:25:44.409378Z","title":"Chudaykin and M.M","venue":null,"work_id":"0f7f34c9-d659-4e09-8ce4-e9239c8489b6","year":2022},"citing_paper":{"arxiv_id":"2411.12022","last_updated":"2024-11-21T16:47:10Z","snapshot_observed_at":"2026-07-06T19:52:15.853216Z","submitted_at":"2024-11-18T20:03:35Z","title":"DESI 2024 VII: Cosmological Constraints from the Full-Shape Modeling of Clustering Measurements","version":2},"reference_index":43,"source":"pdf_text","source_observed_at":"2026-05-15T21:36:41.223414Z"},"links":{"cited_paper":"/paper/2210.17044","citing_paper":"/paper/2411.12022"},"observation_digest":"sha256:adfcb9923d3bc7bbd0016e78593706b64b5d67f0769ff5b81b70355906255046","observation_id":"83d36b35-4272-4e03-87a3-5733e81555b3","resolution":{"observed_at":"2026-05-15T21:36:41.864026Z","resolver_source":"arxiv_id","status":"verified_exact"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-04T06:34:03.388597+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-04T06:34:03.388597+00:00","source":"crossref"},{"observed_at":"2026-08-04T06:33:57.428241+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":{"arxiv_id":"2210.17044","last_updated":"2023-02-06T19:59:21Z","snapshot_observed_at":"2026-08-04T14:30:40.736961Z","submitted_at":"2022-10-31T03:46:16Z","title":"Cosmological constraints from the power spectrum of eBOSS quasars","version":2},"cited_work":{"arxiv_id":"2210.17044","doi":null,"metadata_source":"arxiv_reference","pith_arxiv_id":"2210.17044","snapshot_observed_at":"2026-07-01T12:25:44.409378Z","title":"Chudaykin and M.M","venue":null,"work_id":"0f7f34c9-d659-4e09-8ce4-e9239c8489b6","year":2022},"citing_paper":{"arxiv_id":"2511.20757","last_updated":"2026-04-14T17:58:15Z","snapshot_observed_at":"2026-07-06T22:36:59.311174Z","submitted_at":"2025-11-25T19:00:04Z","title":"Reanalyzing DESI DR1: 2. Constraints on Dark Energy, Spatial Curvature, and Neutrino Masses","version":2},"reference_index":99,"source":"pdf_text","source_observed_at":"2026-05-17T04:15:18.730245Z"},"links":{"cited_paper":"/paper/2210.17044","citing_paper":"/paper/2511.20757"},"observation_digest":"sha256:f956b51350b5e9b6e058ab22c44ff14cfe40c59779f96a8e7fef5bfc41e37bf4","observation_id":"d3e1ed2f-9a83-4f44-9267-c3bf19a7c6a0","resolution":{"observed_at":"2026-05-17T04:19:01.260059Z","resolver_source":"arxiv_id","status":"verified_exact"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-04T06:34:03.388597+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-04T06:34:03.388597+00:00","source":"crossref"},{"observed_at":"2026-08-04T06:33:57.428241+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":{"arxiv_id":"2210.17044","last_updated":"2023-02-06T19:59:21Z","snapshot_observed_at":"2026-08-04T14:30:40.736961Z","submitted_at":"2022-10-31T03:46:16Z","title":"Cosmological constraints from the power spectrum of eBOSS quasars","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2210.17044","snapshot_observed_at":"2026-08-03T08:42:00.263097Z","title":"Chudaykin and M","venue":null,"work_id":null,"year":2022},"citing_paper":{"arxiv_id":"2601.16165","last_updated":"2026-07-22T13:53:51Z","snapshot_observed_at":"2026-08-04T08:50:16.397178Z","submitted_at":"2026-01-22T18:10:50Z","title":"Reanalyzing DESI DR1: 4. Percent-Level Cosmological Constraints from Combined Probes and Robust Evidence for the Normal Neutrino Mass Hierarchy","version":2},"reference_index":118,"source":"pdf_text","source_observed_at":"2026-08-03T08:42:00.263097Z"},"links":{"cited_paper":"/paper/2210.17044","citing_paper":"/paper/2601.16165"},"observation_digest":"sha256:787a6cb9c0db8abe25c3fb93cb0881572715f45c13645d74c5656620c5941dbb","observation_id":"f7b0f26a-bc8b-47a7-98dc-bb4d32daae60","resolution":{"observed_at":"2026-08-03T08:42:00.263097Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2210.17044","last_updated":"2023-02-06T19:59:21Z","snapshot_observed_at":"2026-08-04T14:30:40.736961Z","submitted_at":"2022-10-31T03:46:16Z","title":"Cosmological constraints from the power spectrum of eBOSS quasars","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2210.17044","snapshot_observed_at":"2026-08-02T22:01:24.118018Z","title":"Chudaykin and M","venue":null,"work_id":null,"year":2022},"citing_paper":{"arxiv_id":"2602.18554","last_updated":"2026-07-18T17:18:40Z","snapshot_observed_at":"2026-08-02T22:01:11.013300Z","submitted_at":"2026-02-20T19:00:00Z","title":"Reanalyzing DESI DR1: 5. Cosmological Constraints with Simulation-Based Priors","version":2},"reference_index":76,"source":"pdf_text","source_observed_at":"2026-08-02T22:01:24.118018Z"},"links":{"cited_paper":"/paper/2210.17044","citing_paper":"/paper/2602.18554"},"observation_digest":"sha256:afc20f0a3ac266764275ddc7765af22b701d687bad85750cbf5fdd11e99ec55e","observation_id":"94189d28-3d00-4244-96f0-2665c4c47ed8","resolution":{"observed_at":"2026-08-02T22:01:24.118018Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2210.17044","last_updated":"2023-02-06T19:59:21Z","snapshot_observed_at":"2026-08-04T14:30:40.736961Z","submitted_at":"2022-10-31T03:46:16Z","title":"Cosmological constraints from the power spectrum of eBOSS quasars","version":2},"cited_work":{"arxiv_id":"2210.17044","doi":null,"metadata_source":"arxiv_reference","pith_arxiv_id":"2210.17044","snapshot_observed_at":"2026-07-01T12:25:44.409378Z","title":"Chudaykin and M.M","venue":null,"work_id":"0f7f34c9-d659-4e09-8ce4-e9239c8489b6","year":2022},"citing_paper":{"arxiv_id":"2606.30713","last_updated":"2026-06-29T18:00:00Z","snapshot_observed_at":"2026-07-07T00:04:29.879877Z","submitted_at":"2026-06-29T18:00:00Z","title":"Galaxy Power Spectrum at Two-Loop Order: Implications for Weak Lensing Surveys and New Physics","version":1},"reference_index":24,"source":"pdf_text","source_observed_at":"2026-07-01T02:01:27.807230Z"},"links":{"cited_paper":"/paper/2210.17044","citing_paper":"/paper/2606.30713"},"observation_digest":"sha256:35ba456485bbf1a3def3d8ef1c885e3389c184c8db47dd05e0d7148352151a75","observation_id":"97a7f4e8-4af0-467d-b6fe-b6272a051a23","resolution":{"observed_at":"2026-07-01T12:25:44.410699Z","resolver_source":"arxiv_id","status":"verified_exact"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-04T06:34:03.388597+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-04T06:34:03.388597+00:00","source":"crossref"},{"observed_at":"2026-08-04T06:33:57.428241+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":{"arxiv_id":"2210.17044","last_updated":"2023-02-06T19:59:21Z","snapshot_observed_at":"2026-08-04T14:30:40.736961Z","submitted_at":"2022-10-31T03:46:16Z","title":"Cosmological constraints from the power spectrum of eBOSS quasars","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2210.17044","snapshot_observed_at":"2026-07-31T11:32:41.311604Z","title":"Chudaykin and M.M","venue":null,"work_id":null,"year":null},"citing_paper":{"arxiv_id":"2607.28314","last_updated":"2026-07-30T14:48:56Z","snapshot_observed_at":"2026-08-03T00:09:47.125997Z","submitted_at":"2026-07-30T14:48:56Z","title":"GGI Lectures on Large-Scale Structure Perturbation Theory (Effective Field Theory)","version":1},"reference_index":87,"source":"pdf_text","source_observed_at":"2026-07-31T11:32:41.311604Z"},"links":{"cited_paper":"/paper/2210.17044","citing_paper":"/paper/2607.28314"},"observation_digest":"sha256:8d57f1d4e7482dfb2c4b6d5a54b78a881de977e06a2ad3d4b76128aae79e0eab","observation_id":"39fb4122-0efe-4df4-86e8-a0ce6ff7bef8","resolution":{"observed_at":"2026-07-31T11:32:41.311604Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2210.17044","last_updated":"2023-02-06T19:59:21Z","snapshot_observed_at":"2026-08-04T14:30:40.736961Z","submitted_at":"2022-10-31T03:46:16Z","title":"Cosmological constraints from the power spectrum of eBOSS quasars","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2210.17044","snapshot_observed_at":"2026-07-31T07:10:45.678421Z","title":"Chudaykin and M.M","venue":null,"work_id":null,"year":2023},"citing_paper":{"arxiv_id":"2607.28445","last_updated":"2026-07-30T16:16:22Z","snapshot_observed_at":"2026-08-03T00:12:07.213417Z","submitted_at":"2026-07-30T16:16:22Z","title":"Inflation, Open Universes, and Dark Energy","version":1},"reference_index":44,"source":"pdf_text","source_observed_at":"2026-07-31T07:10:45.678421Z"},"links":{"cited_paper":"/paper/2210.17044","citing_paper":"/paper/2607.28445"},"observation_digest":"sha256:75bbafc0723e41557f86b8dd17434bab4447107dc442680615b2ea44bcb80199","observation_id":"498d9e40-fe09-43eb-8370-a742a72ae3f1","resolution":{"observed_at":"2026-07-31T07:10:45.678421Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}}],"links":{"evidence":"/evidence","html":"/paper/2210.17044/citation-record","integrity":"/paper/2210.17044/integrity","json":"/paper/2210.17044/citation-record.json","paper":"/paper/2210.17044"},"outbound":[],"paper":{"arxiv_id":"2210.17044","last_updated":"2023-02-06T19:59:21Z","latest_version":2,"primary_category":"astro-ph.CO","snapshot_observed_at":"2026-08-04T14:30:40.736961Z","submitted_at":"2022-10-31T03:46:16Z","title":"Cosmological constraints from the power spectrum of eBOSS quasars"},"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":"2026-08-04T06:34:03.388597+00:00","source":"crossref"},{"observed_at":"2026-08-04T06:33:57.428241+00:00","source":"retraction_watch"}],"thesis":"As of 4 August 2026, this Paper Citation Record lists 0 of 0 outbound references and 8 inbound Pith citation observations for arXiv:2210.17044."}