{"as_of":"2026-08-08T16:48:00Z","caps":{"database_statements":6,"inbound":100,"outbound":100},"context_digest":"sha256:5580c46b17aa3c8d0a95bffaeafe714299e9c565e70aed457c3f4a634ba4e330","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":9,"lane":"standing_notices","note":"One-hop event checks from named stored sources.","records_observed":9,"source":"scholarly_work_events, retraction_status_cache","source_observed_at":"2026-08-08T06:32:00.761636+00:00","state":"measured"},{"denominator":9,"lane":"inbound_itemization","note":"Pith citing papers itemized under the disclosed page cap.","records_observed":9,"source":"paper_references, paper_reference_links","source_observed_at":"2026-08-06T21:30:54.812184Z","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":"2026-07-04T05:19:35.819577Z","state":"measured"}],"external_citation_measurements":[],"inbound":[{"citation":{"cited_paper":{"arxiv_id":"2002.04035","last_updated":"2020-05-13T19:13:00Z","snapshot_observed_at":"2026-08-04T17:00:41.192234Z","submitted_at":"2020-02-10T19:00:00Z","title":"Combining Full-Shape and BAO Analyses of Galaxy Power Spectra: A 1.6% CMB-independent constraint on H0","version":3},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2002.04035","snapshot_observed_at":"2026-08-06T21:30:54.812184Z","title":null,"venue":null,"work_id":null,"year":2020},"citing_paper":{"arxiv_id":"2507.00118","last_updated":"2025-06-30T18:00:01Z","snapshot_observed_at":"2026-08-07T11:10:22.278337Z","submitted_at":"2025-06-30T18:00:01Z","title":"Constraining Dynamical Dark Energy from Galaxy Clustering with Simulation-Based Priors","version":1},"reference_index":81,"source":"pdf_text","source_observed_at":"2026-08-06T21:30:54.812184Z"},"links":{"cited_paper":"/paper/2002.04035","citing_paper":"/paper/2507.00118"},"observation_digest":"sha256:883d669f84e3e45d22abe573024c320804f560d1372cb1405aec16068be90b5c","observation_id":"aea6ea0a-5e8f-44c1-9603-e1d8b2fb390c","resolution":{"observed_at":"2026-08-06T21:30:54.812184Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2002.04035","last_updated":"2020-05-13T19:13:00Z","snapshot_observed_at":"2026-08-04T17:00:41.192234Z","submitted_at":"2020-02-10T19:00:00Z","title":"Combining Full-Shape and BAO Analyses of Galaxy Power Spectra: A 1.6% CMB-independent constraint on H0","version":3},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2002.04035","snapshot_observed_at":"2026-08-06T19:34:08.384290Z","title":null,"venue":null,"work_id":null,"year":2002},"citing_paper":{"arxiv_id":"2507.05378","last_updated":"2025-07-07T18:04:52Z","snapshot_observed_at":"2026-08-08T13:16:58.105496Z","submitted_at":"2025-07-07T18:04:52Z","title":"Equivalence of the field-level inference and conventional analyses on large scales","version":1},"reference_index":62,"source":"pdf_text","source_observed_at":"2026-08-06T19:34:08.384290Z"},"links":{"cited_paper":"/paper/2002.04035","citing_paper":"/paper/2507.05378"},"observation_digest":"sha256:842aa6baf7ead080255f0102d71b33679599f3539c97e10a012087ce749c2c7a","observation_id":"a4f62fc5-a3df-43ef-8086-d5d08b33d567","resolution":{"observed_at":"2026-08-06T19:34:08.384290Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2002.04035","last_updated":"2020-05-13T19:13:00Z","snapshot_observed_at":"2026-08-04T17:00:41.192234Z","submitted_at":"2020-02-10T19:00:00Z","title":"Combining Full-Shape and BAO Analyses of Galaxy Power Spectra: A 1.6% CMB-independent constraint on H0","version":3},"cited_work":{"arxiv_id":"2002.04035","doi":null,"metadata_source":"arxiv_reference","pith_arxiv_id":"2002.04035","snapshot_observed_at":"2026-07-04T05:19:35.819577Z","title":null,"venue":null,"work_id":"b339fa2a-3a93-405f-8bfc-8c33ff2c5754","year":2005},"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":128,"source":"pdf_text","source_observed_at":"2026-05-17T04:15:18.730245Z"},"links":{"cited_paper":"/paper/2002.04035","citing_paper":"/paper/2511.20757"},"observation_digest":"sha256:47bab3a586be7e9cbd4c4ec030c3eeef8027ddaab4b762a979095285954501c0","observation_id":"6f2b9448-d181-4246-a22f-7103bdbd1882","resolution":{"observed_at":"2026-05-17T04:19:00.932178Z","resolver_source":"arxiv_id","status":"verified_exact"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-08T06:32:00.761636+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-08T06:32:00.761636+00:00","source":"crossref"},{"observed_at":"2026-08-08T06:31:55.24221+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":{"arxiv_id":"2002.04035","last_updated":"2020-05-13T19:13:00Z","snapshot_observed_at":"2026-08-04T17:00:41.192234Z","submitted_at":"2020-02-10T19:00:00Z","title":"Combining Full-Shape and BAO Analyses of Galaxy Power Spectra: A 1.6% CMB-independent constraint on H0","version":3},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2002.04035","snapshot_observed_at":"2026-08-03T08:42:08.386170Z","title":null,"venue":null,"work_id":null,"year":2020},"citing_paper":{"arxiv_id":"2601.16165","last_updated":"2026-07-22T13:53:51Z","snapshot_observed_at":"2026-08-08T14:24:16.036685Z","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":189,"source":"pdf_text","source_observed_at":"2026-08-03T08:42:08.386170Z"},"links":{"cited_paper":"/paper/2002.04035","citing_paper":"/paper/2601.16165"},"observation_digest":"sha256:a68c353501ae7c5127a58bad74f2a1b4c211c7476404622dd45c6f2046bd65aa","observation_id":"90e61533-6e1a-4399-9969-b8cac095737e","resolution":{"observed_at":"2026-08-03T08:42:08.386170Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2002.04035","last_updated":"2020-05-13T19:13:00Z","snapshot_observed_at":"2026-08-04T17:00:41.192234Z","submitted_at":"2020-02-10T19:00:00Z","title":"Combining Full-Shape and BAO Analyses of Galaxy Power Spectra: A 1.6% CMB-independent constraint on H0","version":3},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2002.04035","snapshot_observed_at":"2026-08-02T22:01:20.417119Z","title":null,"venue":null,"work_id":null,"year":2020},"citing_paper":{"arxiv_id":"2602.18554","last_updated":"2026-07-18T17:18:40Z","snapshot_observed_at":"2026-08-07T15:21:25.685152Z","submitted_at":"2026-02-20T19:00:00Z","title":"Reanalyzing DESI DR1: 5. Cosmological Constraints with Simulation-Based Priors","version":2},"reference_index":29,"source":"pdf_text","source_observed_at":"2026-08-02T22:01:20.417119Z"},"links":{"cited_paper":"/paper/2002.04035","citing_paper":"/paper/2602.18554"},"observation_digest":"sha256:8cdde404c286f6dd03bb1840b3d0c46078184bed47c7734ce88e1f35545f6024","observation_id":"e2cde145-d2b0-47a2-8fca-a316cbb1b049","resolution":{"observed_at":"2026-08-02T22:01:20.417119Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2002.04035","last_updated":"2020-05-13T19:13:00Z","snapshot_observed_at":"2026-08-04T17:00:41.192234Z","submitted_at":"2020-02-10T19:00:00Z","title":"Combining Full-Shape and BAO Analyses of Galaxy Power Spectra: A 1.6% CMB-independent constraint on H0","version":3},"cited_work":{"arxiv_id":"2002.04035","doi":null,"metadata_source":"arxiv_reference","pith_arxiv_id":"2002.04035","snapshot_observed_at":"2026-07-04T05:19:35.819577Z","title":null,"venue":null,"work_id":"b339fa2a-3a93-405f-8bfc-8c33ff2c5754","year":2005},"citing_paper":{"arxiv_id":"2604.11694","last_updated":"2026-04-13T16:33:23Z","snapshot_observed_at":"2026-07-06T23:00:03.762376Z","submitted_at":"2026-04-13T16:33:23Z","title":"Cosmological inference with halo clustering reconstructed from the redshift-space galaxy distribution","version":1},"reference_index":11,"source":"pdf_text","source_observed_at":"2026-05-10T15:10:48.528283Z"},"links":{"cited_paper":"/paper/2002.04035","citing_paper":"/paper/2604.11694"},"observation_digest":"sha256:4d50374bec6ad55bfb5ce48bf8eb8acbc51f9867cc28becc511f16df3bf3a7a1","observation_id":"ca233d6d-cdfc-4c8e-b74f-713c149aa3f3","resolution":{"observed_at":"2026-05-11T11:06:00.874076Z","resolver_source":"arxiv_id","status":"verified_exact"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-08T06:32:00.761636+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-08T06:32:00.761636+00:00","source":"crossref"},{"observed_at":"2026-08-08T06:31:55.24221+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":{"arxiv_id":"2002.04035","last_updated":"2020-05-13T19:13:00Z","snapshot_observed_at":"2026-08-04T17:00:41.192234Z","submitted_at":"2020-02-10T19:00:00Z","title":"Combining Full-Shape and BAO Analyses of Galaxy Power Spectra: A 1.6% CMB-independent constraint on H0","version":3},"cited_work":{"arxiv_id":"2002.04035","doi":null,"metadata_source":"arxiv_reference","pith_arxiv_id":"2002.04035","snapshot_observed_at":"2026-07-04T05:19:35.819577Z","title":null,"venue":null,"work_id":"b339fa2a-3a93-405f-8bfc-8c33ff2c5754","year":2005},"citing_paper":{"arxiv_id":"2606.20434","last_updated":"2026-07-14T16:58:56Z","snapshot_observed_at":"2026-07-17T23:19:04.117001Z","submitted_at":"2026-06-18T16:12:11Z","title":"The Hubble tension: A decade review","version":1},"reference_index":130,"source":"pdf_text","source_observed_at":"2026-06-26T16:04:43.230344Z"},"links":{"cited_paper":"/paper/2002.04035","citing_paper":"/paper/2606.20434"},"observation_digest":"sha256:8d8b523f28ee9e7aff255475ccf12930cf2d0bf1304aeceee4f7e60303d493c0","observation_id":"69da8271-ebe5-407d-a36c-31125a0e6976","resolution":{"observed_at":"2026-07-04T05:19:35.821172Z","resolver_source":"arxiv_id","status":"verified_exact"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-08T06:32:00.761636+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-08T06:32:00.761636+00:00","source":"crossref"},{"observed_at":"2026-08-08T06:31:55.24221+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":{"arxiv_id":"2002.04035","last_updated":"2020-05-13T19:13:00Z","snapshot_observed_at":"2026-08-04T17:00:41.192234Z","submitted_at":"2020-02-10T19:00:00Z","title":"Combining Full-Shape and BAO Analyses of Galaxy Power Spectra: A 1.6% CMB-independent constraint on H0","version":3},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2002.04035","snapshot_observed_at":"2026-07-15T10:41:50.733215Z","title":null,"venue":null,"work_id":null,"year":2005},"citing_paper":{"arxiv_id":"2606.20434","last_updated":"2026-07-14T16:58:56Z","snapshot_observed_at":"2026-07-17T23:19:04.117001Z","submitted_at":"2026-06-18T16:12:11Z","title":"The Hubble tension: A decade review","version":2},"reference_index":130,"source":"pdf_text","source_observed_at":"2026-07-15T10:41:50.733215Z"},"links":{"cited_paper":"/paper/2002.04035","citing_paper":"/paper/2606.20434"},"observation_digest":"sha256:112dfc50744b84e0af65ae2fe2a2d4a416d6ad5d59a6c0c3e55e6a9cbdcbd09b","observation_id":"73b30330-17c4-480c-9f52-b7aff2910d48","resolution":{"observed_at":"2026-07-15T10:41:50.733215Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2002.04035","last_updated":"2020-05-13T19:13:00Z","snapshot_observed_at":"2026-08-04T17:00:41.192234Z","submitted_at":"2020-02-10T19:00:00Z","title":"Combining Full-Shape and BAO Analyses of Galaxy Power Spectra: A 1.6% CMB-independent constraint on H0","version":3},"cited_work":{"arxiv_id":"2002.04035","doi":null,"metadata_source":"arxiv_reference","pith_arxiv_id":"2002.04035","snapshot_observed_at":"2026-07-04T05:19:35.819577Z","title":null,"venue":null,"work_id":"b339fa2a-3a93-405f-8bfc-8c33ff2c5754","year":2005},"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":21,"source":"pdf_text","source_observed_at":"2026-07-01T02:01:27.807230Z"},"links":{"cited_paper":"/paper/2002.04035","citing_paper":"/paper/2606.30713"},"observation_digest":"sha256:df88c4bec4a19547fb6e9dc8da1f3776b0454d2c6f4d135355daab948755066b","observation_id":"47ba3292-8e78-476b-8941-875ef5c5877e","resolution":{"observed_at":"2026-07-01T12:25:44.408084Z","resolver_source":"arxiv_id","status":"verified_exact"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-08T06:32:00.761636+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-08T06:32:00.761636+00:00","source":"crossref"},{"observed_at":"2026-08-08T06:31:55.24221+00:00","source":"retraction_watch"}],"state":"measured"}}],"links":{"evidence":"/evidence","html":"/paper/2002.04035/citation-record","integrity":"/paper/2002.04035/integrity","json":"/paper/2002.04035/citation-record.json","paper":"/paper/2002.04035"},"outbound":[],"paper":{"arxiv_id":"2002.04035","last_updated":"2020-05-13T19:13:00Z","latest_version":3,"primary_category":"astro-ph.CO","snapshot_observed_at":"2026-08-04T17:00:41.192234Z","submitted_at":"2020-02-10T19:00:00Z","title":"Combining Full-Shape and BAO Analyses of Galaxy Power Spectra: A 1.6% CMB-independent constraint on H0"},"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":"2026-08-08T06:32:00.761636+00:00","source":"crossref"},{"observed_at":"2026-08-08T06:31:55.24221+00:00","source":"retraction_watch"}],"thesis":"As of 8 August 2026, this Paper Citation Record lists 0 of 0 outbound references and 9 inbound Pith citation observations for arXiv:2002.04035."}