{"as_of":"2026-08-14T01:05:00Z","caps":{"database_statements":6,"inbound":100,"outbound":100},"context_digest":"sha256:a62983ea012105147feb28744f1352fe895679126e78e6261d1d6a6f085daa0f","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":5,"lane":"standing_notices","note":"One-hop event checks from named stored sources.","records_observed":5,"source":"scholarly_work_events, retraction_status_cache","source_observed_at":"2026-08-13T06:32:02.005865+00:00","state":"measured"},{"denominator":5,"lane":"inbound_itemization","note":"Pith citing papers itemized under the disclosed page cap.","records_observed":5,"source":"paper_references, paper_reference_links","source_observed_at":"2026-08-12T12:45:53.108317Z","state":"measured"},{"denominator":1,"lane":"external_citation_measurements","note":"A source-named dated measurement, never combined with another source.","records_observed":1,"source":"pith","source_observed_at":"2026-08-05T02:28:24.338817Z","state":"measured"}],"external_citation_measurements":[{"count":33,"observed_at":"2026-08-05T02:28:24.338817Z","source":"pith"}],"inbound":[{"citation":{"cited_paper":{"arxiv_id":"2004.09515","last_updated":"2020-05-29T19:32:42Z","snapshot_observed_at":"2026-08-03T16:07:23.787577Z","submitted_at":"2020-04-20T18:00:00Z","title":"The Effective Halo Model: Creating a Physical and Accurate Model of the Matter Power Spectrum and Cluster Counts","version":3},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2004.09515","snapshot_observed_at":"2026-08-12T12:45:53.108317Z","title":"Philcox, D.N","venue":null,"work_id":null,"year":2020},"citing_paper":{"arxiv_id":"2411.16948","last_updated":"2025-03-03T20:37:30Z","snapshot_observed_at":"2026-08-12T12:40:20.053112Z","submitted_at":"2024-11-25T21:40:31Z","title":"Super sample covariance and the volume scaling of galaxy survey covariance matrices","version":2},"reference_index":60,"source":"pdf_text","source_observed_at":"2026-08-12T12:45:53.108317Z"},"links":{"cited_paper":"/paper/2004.09515","citing_paper":"/paper/2411.16948"},"observation_digest":"sha256:a7651cf7d61bd64283da76bfc6ac85efbcd2d186b85123263b8202bbcfe680c3","observation_id":"cf911cc3-ff8a-4bc9-b378-25b54463144e","resolution":{"observed_at":"2026-08-12T12:45:53.108317Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2004.09515","last_updated":"2020-05-29T19:32:42Z","snapshot_observed_at":"2026-08-03T16:07:23.787577Z","submitted_at":"2020-04-20T18:00:00Z","title":"The Effective Halo Model: Creating a Physical and Accurate Model of the Matter Power Spectrum and Cluster Counts","version":3},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2004.09515","snapshot_observed_at":"2026-08-12T12:42:56.850412Z","title":null,"venue":null,"work_id":null,"year":2020},"citing_paper":{"arxiv_id":"2411.17094","last_updated":"2025-09-10T14:55:29Z","snapshot_observed_at":"2026-08-13T02:07:30.394596Z","submitted_at":"2024-11-26T04:12:04Z","title":"Analytical modeling of the one-dimensional power spectrum of 21-cm forest based on a halo model method","version":2},"reference_index":41,"source":"pdf_text","source_observed_at":"2026-08-12T12:42:56.850412Z"},"links":{"cited_paper":"/paper/2004.09515","citing_paper":"/paper/2411.17094"},"observation_digest":"sha256:b29022c0d21c293d3b10bc98246698ae20a8e9fd9fd65601f976272bc9bb952f","observation_id":"cffb6c6a-400f-4541-8bdd-bdab9d756a45","resolution":{"observed_at":"2026-08-12T12:42:56.850412Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2004.09515","last_updated":"2020-05-29T19:32:42Z","snapshot_observed_at":"2026-08-03T16:07:23.787577Z","submitted_at":"2020-04-20T18:00:00Z","title":"The Effective Halo Model: Creating a Physical and Accurate Model of the Matter Power Spectrum and Cluster Counts","version":3},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2004.09515","snapshot_observed_at":"2026-08-10T22:48:21.782243Z","title":null,"venue":null,"work_id":null,"year":2020},"citing_paper":{"arxiv_id":"2501.00769","last_updated":"2025-02-26T10:16:34Z","snapshot_observed_at":"2026-08-13T15:53:10.659193Z","submitted_at":"2025-01-01T08:15:33Z","title":"Prospects for measuring neutrino mass with 21-cm forest","version":2},"reference_index":85,"source":"pdf_text","source_observed_at":"2026-08-10T22:48:21.782243Z"},"links":{"cited_paper":"/paper/2004.09515","citing_paper":"/paper/2501.00769"},"observation_digest":"sha256:1fd569b1b0627ae5da46eed3a70d0fd7c1fdb99d56e3b7cfb44afb7e7535b8ed","observation_id":"ae2acd40-d1ad-4233-adb2-681d56badf97","resolution":{"observed_at":"2026-08-10T22:48:21.782243Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2004.09515","last_updated":"2020-05-29T19:32:42Z","snapshot_observed_at":"2026-08-03T16:07:23.787577Z","submitted_at":"2020-04-20T18:00:00Z","title":"The Effective Halo Model: Creating a Physical and Accurate Model of the Matter Power Spectrum and Cluster Counts","version":3},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2004.09515","snapshot_observed_at":"2026-08-03T08:42:06.949176Z","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":"2026-08-12T12:58:30.592699Z","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":176,"source":"pdf_text","source_observed_at":"2026-08-03T08:42:06.949176Z"},"links":{"cited_paper":"/paper/2004.09515","citing_paper":"/paper/2601.16165"},"observation_digest":"sha256:611262d6bf63896a75aaa4771c682cf71ab38710da07d3899574967d79b5c0a9","observation_id":"4cf85a84-26b1-418c-a372-2d33ed137dd6","resolution":{"observed_at":"2026-08-03T08:42:06.949176Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2004.09515","last_updated":"2020-05-29T19:32:42Z","snapshot_observed_at":"2026-08-03T16:07:23.787577Z","submitted_at":"2020-04-20T18:00:00Z","title":"The Effective Halo Model: Creating a Physical and Accurate Model of the Matter Power Spectrum and Cluster Counts","version":3},"cited_work":{"arxiv_id":"2004.09515","doi":"10.1103/physrevd.101.123520","metadata_source":"pith","pith_arxiv_id":"2004.09515","snapshot_observed_at":"2026-08-05T02:49:54.815029Z","title":"The Effective Halo Model: Creating a Physical and Accurate Model of the Matter Power Spectrum and Cluster Counts","venue":"astro-ph.CO","work_id":"00f014a1-bf4a-43a7-a232-ee9e30df3fb9","year":2020},"citing_paper":{"arxiv_id":"2607.09571","last_updated":"2026-07-10T16:18:53Z","snapshot_observed_at":"2026-08-13T09:10:39.617123Z","submitted_at":"2026-07-10T16:18:53Z","title":"CHEFT: A Hybrid Effective Field Theory halo model","version":1},"reference_index":30,"source":"arxiv_source","source_observed_at":"2026-07-13T02:04:26.563148Z"},"links":{"cited_paper":"/paper/2004.09515","citing_paper":"/paper/2607.09571"},"observation_digest":"sha256:6a0ab3e88669c8dda391f3494ed9a91db84a53f80fd4a23f9706f4ed54eab5db","observation_id":"f2531a72-c0fd-4fc7-ad85-365ef29a5873","resolution":{"observed_at":"2026-07-13T02:09:16.000537Z","resolver_source":"local_arxiv","status":"metadata_mismatch"},"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":"2026-07-20T16:52:06.10019+00:00","source":"crossref_status_cache"},{"observed_at":"2026-07-20T16:52:06.10019+00:00","source":"openalex_status_cache"},{"observed_at":"2026-08-13T06:31:53.387327+00:00","source":"retraction_watch"}],"state":"measured"}}],"links":{"evidence":"/evidence","html":"/paper/2004.09515/citation-record","integrity":"/paper/2004.09515/integrity","json":"/paper/2004.09515/citation-record.json","paper":"/paper/2004.09515"},"outbound":[],"paper":{"arxiv_id":"2004.09515","last_updated":"2020-05-29T19:32:42Z","latest_version":3,"primary_category":"astro-ph.CO","snapshot_observed_at":"2026-08-03T16:07:23.787577Z","submitted_at":"2020-04-20T18:00:00Z","title":"The Effective Halo Model: Creating a Physical and Accurate Model of the Matter Power Spectrum and Cluster Counts"},"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 14 August 2026, this Paper Citation Record lists 0 of 0 outbound references and 5 inbound Pith citation observations for arXiv:2004.09515."}