{"as_of":"2026-07-23T12:25:00Z","caps":{"database_statements":6,"inbound":100,"outbound":100},"context_digest":"sha256:96e8df964a067b6d86eaba57bb9cfe53054c2304b54e205d502ef162391e78a9","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":6,"lane":"standing_notices","note":"One-hop event checks from named stored sources.","records_observed":6,"source":"scholarly_work_events, retraction_status_cache","source_observed_at":"2026-07-23T06:31:01.910684+00:00","state":"measured"},{"denominator":6,"lane":"inbound_itemization","note":"Pith citing papers itemized under the disclosed page cap.","records_observed":6,"source":"paper_references, paper_reference_links","source_observed_at":"2026-07-14T18:39:20.634979Z","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":"2026-06-29T14:53:32.130982Z","state":"measured"}],"external_citation_measurements":[],"inbound":[{"citation":{"cited_paper":{"arxiv_id":"1810.05051","last_updated":"2021-06-11T12:21:53Z","snapshot_observed_at":"2026-07-06T07:07:29.511056Z","submitted_at":"2018-10-11T14:42:27Z","title":"Interpreting measurements of the anisotropic galaxy power spectrum","version":4},"cited_work":{"arxiv_id":"1810.05051","doi":null,"metadata_source":"arxiv_reference","pith_arxiv_id":"1810.05051","snapshot_observed_at":"2026-06-29T14:53:32.130982Z","title":"Beutler, E","venue":null,"work_id":"d3d3310c-c8f5-4d37-8794-1092b1a9c76c","year":2019},"citing_paper":{"arxiv_id":"2604.14504","last_updated":"2026-04-16T00:37:23Z","snapshot_observed_at":"2026-07-06T23:02:18.425249Z","submitted_at":"2026-04-16T00:37:23Z","title":"Forecasting neutrino mass constraints from the Nancy Grace Roman Space Telescope","version":1},"reference_index":77,"source":"pdf_text","source_observed_at":"2026-05-10T10:45:17.266279Z"},"links":{"cited_paper":"/paper/1810.05051","citing_paper":"/paper/2604.14504"},"observation_digest":"sha256:dd2cfa4090d6a48bab5ac63963f2ea28c23f9417a3b0cd4eeb60f367a2430e82","observation_id":"86e2d1be-6f3f-4bed-8b30-ef83fa3837a9","resolution":{"observed_at":"2026-05-10T10:49:57.163816Z","resolver_source":"arxiv_id","status":"verified_exact"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-07-23T06:31:01.910684+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-07-23T06:31:01.910684+00:00","source":"crossref"},{"observed_at":"2026-07-23T06:30:56.940895+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":{"arxiv_id":"1810.05051","last_updated":"2021-06-11T12:21:53Z","snapshot_observed_at":"2026-07-06T07:07:29.511056Z","submitted_at":"2018-10-11T14:42:27Z","title":"Interpreting measurements of the anisotropic galaxy power spectrum","version":4},"cited_work":{"arxiv_id":"1810.05051","doi":null,"metadata_source":"arxiv_reference","pith_arxiv_id":"1810.05051","snapshot_observed_at":"2026-06-29T14:53:32.130982Z","title":"Beutler, E","venue":null,"work_id":"d3d3310c-c8f5-4d37-8794-1092b1a9c76c","year":2019},"citing_paper":{"arxiv_id":"2605.18615","last_updated":"2026-05-18T16:25:02Z","snapshot_observed_at":"2026-07-06T23:29:29.105126Z","submitted_at":"2026-05-18T16:25:02Z","title":"Primordial power spectrum reconstructions from BOSS + eBOSS","version":1},"reference_index":83,"source":"pdf_text","source_observed_at":"2026-05-20T09:11:43.311993Z"},"links":{"cited_paper":"/paper/1810.05051","citing_paper":"/paper/2605.18615"},"observation_digest":"sha256:23c2c8a4bdfe30e5138c1d74b1f556151ca6eef64dd9f77395c405b3c17d68b9","observation_id":"6c426b1d-5f05-488a-a67f-84bc106bfa34","resolution":{"observed_at":"2026-05-20T09:13:09.912547Z","resolver_source":"arxiv_id","status":"verified_exact"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-07-23T06:31:01.910684+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-07-23T06:31:01.910684+00:00","source":"crossref"},{"observed_at":"2026-07-23T06:30:56.940895+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":{"arxiv_id":"1810.05051","last_updated":"2021-06-11T12:21:53Z","snapshot_observed_at":"2026-07-06T07:07:29.511056Z","submitted_at":"2018-10-11T14:42:27Z","title":"Interpreting measurements of the anisotropic galaxy power spectrum","version":4},"cited_work":{"arxiv_id":"1810.05051","doi":null,"metadata_source":"arxiv_reference","pith_arxiv_id":"1810.05051","snapshot_observed_at":"2026-06-29T14:53:32.130982Z","title":"Beutler, E","venue":null,"work_id":"d3d3310c-c8f5-4d37-8794-1092b1a9c76c","year":2019},"citing_paper":{"arxiv_id":"2605.29806","last_updated":"2026-07-10T19:56:27Z","snapshot_observed_at":"2026-07-16T23:17:52.463321Z","submitted_at":"2026-05-28T11:52:14Z","title":"The observer power spectrum for lightcone statistics, integrated relativistic observables and wide angle effects","version":1},"reference_index":23,"source":"pdf_text","source_observed_at":"2026-06-29T06:12:10.521465Z"},"links":{"cited_paper":"/paper/1810.05051","citing_paper":"/paper/2605.29806"},"observation_digest":"sha256:67437035ea5926d61784c61bef6a1b98e31c42223a252f2ec62b37376381fa8a","observation_id":"2bb6c65d-a341-45e8-83f7-d80e746d1c58","resolution":{"observed_at":"2026-06-29T14:53:32.132240Z","resolver_source":"arxiv_id","status":"verified_exact"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-07-23T06:31:01.910684+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-07-23T06:31:01.910684+00:00","source":"crossref"},{"observed_at":"2026-07-23T06:30:56.940895+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":{"arxiv_id":"1810.05051","last_updated":"2021-06-11T12:21:53Z","snapshot_observed_at":"2026-07-06T07:07:29.511056Z","submitted_at":"2018-10-11T14:42:27Z","title":"Interpreting measurements of the anisotropic galaxy power spectrum","version":4},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"1810.05051","snapshot_observed_at":"2026-07-14T18:39:20.634979Z","title":"Beutler, E","venue":null,"work_id":null,"year":2019},"citing_paper":{"arxiv_id":"2605.29806","last_updated":"2026-07-10T19:56:27Z","snapshot_observed_at":"2026-07-16T23:17:52.463321Z","submitted_at":"2026-05-28T11:52:14Z","title":"The observer power spectrum for lightcone statistics, integrated relativistic observables and wide angle effects","version":2},"reference_index":23,"source":"pdf_text","source_observed_at":"2026-07-14T18:39:20.634979Z"},"links":{"cited_paper":"/paper/1810.05051","citing_paper":"/paper/2605.29806"},"observation_digest":"sha256:68ab33fdccba426a3ac0b15d24b5ea911ad689ed50047eafaeb5a65681c66955","observation_id":"c7bcb2ca-2578-48b6-8429-a962643e9971","resolution":{"observed_at":"2026-07-14T18:39:20.634979Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"1810.05051","last_updated":"2021-06-11T12:21:53Z","snapshot_observed_at":"2026-07-06T07:07:29.511056Z","submitted_at":"2018-10-11T14:42:27Z","title":"Interpreting measurements of the anisotropic galaxy power spectrum","version":4},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"1810.05051","snapshot_observed_at":"2026-07-11T06:32:08.971654Z","title":"Beutler, E","venue":null,"work_id":null,"year":2019},"citing_paper":{"arxiv_id":"2607.05513","last_updated":"2026-07-06T18:00:07Z","snapshot_observed_at":"2026-07-11T06:32:07.089137Z","submitted_at":"2026-07-06T18:00:07Z","title":"Optimal and exact wide-angle power spectrum estimation","version":1},"reference_index":10,"source":"pdf_text","source_observed_at":"2026-07-11T06:32:08.971654Z"},"links":{"cited_paper":"/paper/1810.05051","citing_paper":"/paper/2607.05513"},"observation_digest":"sha256:166383c09ae9e1d8e6ddc8ec928ae1268b615b3a7c51e206947e1471d97c06e4","observation_id":"875ae883-82d8-4f75-8381-dbaeb33319c2","resolution":{"observed_at":"2026-07-11T06:32:08.971654Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"1810.05051","last_updated":"2021-06-11T12:21:53Z","snapshot_observed_at":"2026-07-06T07:07:29.511056Z","submitted_at":"2018-10-11T14:42:27Z","title":"Interpreting measurements of the anisotropic galaxy power spectrum","version":4},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"1810.05051","snapshot_observed_at":"2026-07-14T14:25:37.540627Z","title":"Journal of Cosmology and Astroparticle Physics , keywords =","venue":null,"work_id":null,"year":null},"citing_paper":{"arxiv_id":"2607.09943","last_updated":"2026-07-15T12:28:21Z","snapshot_observed_at":"2026-07-18T23:19:08.500785Z","submitted_at":"2026-07-10T19:49:34Z","title":"Assessing the large-scale angular clustering of UNIONS Lyman Break Galaxies via cross-correlations","version":1},"reference_index":67,"source":"arxiv_source","source_observed_at":"2026-07-14T14:25:37.540627Z"},"links":{"cited_paper":"/paper/1810.05051","citing_paper":"/paper/2607.09943"},"observation_digest":"sha256:8b3f9888d75b2f18f64e5ce132a77e8b4d7930ec167bd5efcfc7097314aff48e","observation_id":"51e3d0d7-059a-4d69-8579-bc555bbc1e1a","resolution":{"observed_at":"2026-07-14T14:25:37.540627Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}}],"links":{"evidence":"/evidence","html":"/paper/1810.05051/citation-record","integrity":"/paper/1810.05051/integrity","json":"/paper/1810.05051/citation-record.json","paper":"/paper/1810.05051"},"outbound":[],"paper":{"arxiv_id":"1810.05051","last_updated":"2021-06-11T12:21:53Z","latest_version":4,"primary_category":"astro-ph.CO","snapshot_observed_at":"2026-07-06T07:07:29.511056Z","submitted_at":"2018-10-11T14:42:27Z","title":"Interpreting measurements of the anisotropic galaxy power spectrum"},"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":"2026-07-23T06:31:01.910684+00:00","source":"crossref"},{"observed_at":"2026-07-23T06:30:56.940895+00:00","source":"retraction_watch"}],"thesis":"As of 23 July 2026, this Paper Citation Record lists 0 of 0 outbound references and 6 inbound Pith citation observations for arXiv:1810.05051."}