{"as_of":"2026-08-07T03:30:00Z","caps":{"database_statements":6,"inbound":100,"outbound":100},"context_digest":"sha256:af6c1c3d4f1df6e6fca75b0679e697a5d917267d006e27943686f18d446b9634","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":"2026-08-06T06:34:29.942622+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":"2026-08-07T00:54:40.924500Z","state":"measured"},{"denominator":1,"lane":"external_citation_measurements","note":"A source-named dated measurement, never combined with another source.","records_observed":0,"source":"pith","source_observed_at":"2026-06-30T13:54:44.667611Z","state":"measured"}],"external_citation_measurements":[],"inbound":[{"citation":{"cited_paper":{"arxiv_id":"1312.4611","last_updated":"2014-06-28T23:41:11Z","snapshot_observed_at":"2026-07-06T03:31:04.362874Z","submitted_at":"2013-12-17T02:21:04Z","title":"The clustering of galaxies in the SDSS-III Baryon Oscillation Spectroscopic Survey: Testing gravity with redshift-space distortions using the power spectrum multipoles","version":2},"cited_work":{"arxiv_id":"1312.4611","doi":null,"metadata_source":"pith","pith_arxiv_id":"1312.4611","snapshot_observed_at":"2026-06-30T13:54:44.667611Z","title":"The clustering of galaxies in the SDSS-III Baryon Oscillation Spectroscopic Survey: Testing gravity with redshift-space distortions using the power spectrum multipoles","venue":"astro-ph.CO","work_id":"d0a57a07-f9e3-4fe4-9291-fe5e87f45b75","year":2013},"citing_paper":{"arxiv_id":"1611.00036","last_updated":"2016-12-13T15:55:51Z","snapshot_observed_at":"2026-07-29T15:27:21.480241Z","submitted_at":"2016-10-31T20:47:42Z","title":"The DESI Experiment Part I: Science,Targeting, and Survey Design","version":2},"reference_index":86,"source":"pdf_text","source_observed_at":"2026-05-12T23:40:20.792511Z"},"links":{"cited_paper":"/paper/1312.4611","citing_paper":"/paper/1611.00036"},"observation_digest":"sha256:0897a1dc4da516070ab548f73d316bd401fb6397b44581ca7ea6b71f58dba5dd","observation_id":"bdc63fcd-d14f-43d8-8a85-d8897a5cc723","resolution":{"observed_at":"2026-05-12T23:40:21.617064Z","resolver_source":"arxiv_id","status":"verified_exact"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-06T06:34:29.942622+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-06T06:34:29.942622+00:00","source":"crossref"},{"observed_at":"2026-08-06T06:34:23.284952+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":{"arxiv_id":"1312.4611","last_updated":"2014-06-28T23:41:11Z","snapshot_observed_at":"2026-07-06T03:31:04.362874Z","submitted_at":"2013-12-17T02:21:04Z","title":"The clustering of galaxies in the SDSS-III Baryon Oscillation Spectroscopic Survey: Testing gravity with redshift-space distortions using the power spectrum multipoles","version":2},"cited_work":{"arxiv_id":"1312.4611","doi":null,"metadata_source":"pith","pith_arxiv_id":"1312.4611","snapshot_observed_at":"2026-06-30T13:54:44.667611Z","title":"The clustering of galaxies in the SDSS-III Baryon Oscillation Spectroscopic Survey: Testing gravity with redshift-space distortions using the power spectrum multipoles","venue":"astro-ph.CO","work_id":"d0a57a07-f9e3-4fe4-9291-fe5e87f45b75","year":2013},"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":32,"source":"pdf_text","source_observed_at":"2026-05-17T06:00:49.044220Z"},"links":{"cited_paper":"/paper/1312.4611","citing_paper":"/paper/2411.12021"},"observation_digest":"sha256:34c6901746518c7bdfeabec4517e2e0738f58e4f8de065fc80e2bba6a52be362","observation_id":"1b86f16e-7fb6-4b8c-9abd-79923e0fb1ae","resolution":{"observed_at":"2026-05-17T06:00:49.408433Z","resolver_source":"local_arxiv","status":"verified_exact"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-06T06:34:29.942622+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-06T06:34:29.942622+00:00","source":"crossref"},{"observed_at":"2026-08-06T06:34:23.284952+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":{"arxiv_id":"1312.4611","last_updated":"2014-06-28T23:41:11Z","snapshot_observed_at":"2026-07-06T03:31:04.362874Z","submitted_at":"2013-12-17T02:21:04Z","title":"The clustering of galaxies in the SDSS-III Baryon Oscillation Spectroscopic Survey: Testing gravity with redshift-space distortions using the power spectrum multipoles","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"1312.4611","snapshot_observed_at":"2026-08-07T00:54:40.924500Z","title":"Beutler, S","venue":null,"work_id":null,"year":2014},"citing_paper":{"arxiv_id":"2506.12709","last_updated":"2025-07-01T13:57:37Z","snapshot_observed_at":"2026-08-07T02:56:57.904130Z","submitted_at":"2025-06-15T03:43:47Z","title":"Constraints on Dark Energy Models Using Late Universe Probes","version":3},"reference_index":28,"source":"pdf_text","source_observed_at":"2026-08-07T00:54:40.924500Z"},"links":{"cited_paper":"/paper/1312.4611","citing_paper":"/paper/2506.12709"},"observation_digest":"sha256:60318727adab67d876f09dfd682be63cb191e2bb43870f81b5497016b79568a4","observation_id":"bdc76919-f158-48c4-a232-667f92fe9372","resolution":{"observed_at":"2026-08-07T00:54:40.924500Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"1312.4611","last_updated":"2014-06-28T23:41:11Z","snapshot_observed_at":"2026-07-06T03:31:04.362874Z","submitted_at":"2013-12-17T02:21:04Z","title":"The clustering of galaxies in the SDSS-III Baryon Oscillation Spectroscopic Survey: Testing gravity with redshift-space distortions using the power spectrum multipoles","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"1312.4611","snapshot_observed_at":"2026-08-03T22:43:44.124108Z","title":"Beutler, S","venue":null,"work_id":null,"year":2014},"citing_paper":{"arxiv_id":"2511.09466","last_updated":"2026-06-18T18:40:30Z","snapshot_observed_at":"2026-08-03T22:43:34.889399Z","submitted_at":"2025-11-12T16:33:34Z","title":"Unbiased analysis of primordial non-Gaussianity: the multipoles of the full relativistic power spectrum","version":3},"reference_index":53,"source":"pdf_text","source_observed_at":"2026-08-03T22:43:44.124108Z"},"links":{"cited_paper":"/paper/1312.4611","citing_paper":"/paper/2511.09466"},"observation_digest":"sha256:f698686bc862f91ef34c1ad312373067368ea7963d5758811e32287ad9392a16","observation_id":"fd75874f-b6fa-4635-9aa5-183693cdccaa","resolution":{"observed_at":"2026-08-03T22:43:44.124108Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"1312.4611","last_updated":"2014-06-28T23:41:11Z","snapshot_observed_at":"2026-07-06T03:31:04.362874Z","submitted_at":"2013-12-17T02:21:04Z","title":"The clustering of galaxies in the SDSS-III Baryon Oscillation Spectroscopic Survey: Testing gravity with redshift-space distortions using the power spectrum multipoles","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"1312.4611","snapshot_observed_at":"2026-08-04T06:23:29.160007Z","title":"Beutler, S","venue":null,"work_id":null,"year":2014},"citing_paper":{"arxiv_id":"2601.19438","last_updated":"2026-08-03T17:50:09Z","snapshot_observed_at":"2026-08-06T23:37:33.205003Z","submitted_at":"2026-01-27T10:18:40Z","title":"Large-scale Modeling of the Observed Power Spectrum Multipoles","version":2},"reference_index":95,"source":"pdf_text","source_observed_at":"2026-08-04T06:23:29.160007Z"},"links":{"cited_paper":"/paper/1312.4611","citing_paper":"/paper/2601.19438"},"observation_digest":"sha256:c705da7c909d0a7631c75d87e432763e893d02c720f5ed1a8246f8b581bb0cc6","observation_id":"3e781ccb-47c1-4276-a7c1-f0b200f0dfbe","resolution":{"observed_at":"2026-08-04T06:23:29.160007Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"1312.4611","last_updated":"2014-06-28T23:41:11Z","snapshot_observed_at":"2026-07-06T03:31:04.362874Z","submitted_at":"2013-12-17T02:21:04Z","title":"The clustering of galaxies in the SDSS-III Baryon Oscillation Spectroscopic Survey: Testing gravity with redshift-space distortions using the power spectrum multipoles","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"1312.4611","snapshot_observed_at":"2026-08-02T21:01:59.395472Z","title":"Beutleret al.(BOSS), Mon","venue":null,"work_id":null,"year":2014},"citing_paper":{"arxiv_id":"2602.21733","last_updated":"2026-06-28T15:46:45Z","snapshot_observed_at":"2026-08-03T16:14:32.333490Z","submitted_at":"2026-02-25T09:43:05Z","title":"A sound horizon independent measurement of $H_0$ from BOSS, DESI and DES Y3","version":2},"reference_index":71,"source":"pdf_text","source_observed_at":"2026-08-02T21:01:59.395472Z"},"links":{"cited_paper":"/paper/1312.4611","citing_paper":"/paper/2602.21733"},"observation_digest":"sha256:89d6559d13c91ae556682e8463fb76f8bab9549201cec8b3d02ca5e37e3f21c1","observation_id":"7b9454a7-49a4-4db8-aef4-c24321e833af","resolution":{"observed_at":"2026-08-02T21:01:59.395472Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"1312.4611","last_updated":"2014-06-28T23:41:11Z","snapshot_observed_at":"2026-07-06T03:31:04.362874Z","submitted_at":"2013-12-17T02:21:04Z","title":"The clustering of galaxies in the SDSS-III Baryon Oscillation Spectroscopic Survey: Testing gravity with redshift-space distortions using the power spectrum multipoles","version":2},"cited_work":{"arxiv_id":"1312.4611","doi":null,"metadata_source":"pith","pith_arxiv_id":"1312.4611","snapshot_observed_at":"2026-06-30T13:54:44.667611Z","title":"The clustering of galaxies in the SDSS-III Baryon Oscillation Spectroscopic Survey: Testing gravity with redshift-space distortions using the power spectrum multipoles","venue":"astro-ph.CO","work_id":"d0a57a07-f9e3-4fe4-9291-fe5e87f45b75","year":2013},"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":78,"source":"pdf_text","source_observed_at":"2026-05-10T10:45:17.266279Z"},"links":{"cited_paper":"/paper/1312.4611","citing_paper":"/paper/2604.14504"},"observation_digest":"sha256:2d4f6a1b2d1d9172e114a1cb88dbe95e8f052ad5230bad5c24524b8d165bdb6d","observation_id":"5cf19380-269b-4b7b-8b68-8598b442bba7","resolution":{"observed_at":"2026-05-10T10:49:57.203121Z","resolver_source":"arxiv_id","status":"verified_exact"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-06T06:34:29.942622+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-06T06:34:29.942622+00:00","source":"crossref"},{"observed_at":"2026-08-06T06:34:23.284952+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":{"arxiv_id":"1312.4611","last_updated":"2014-06-28T23:41:11Z","snapshot_observed_at":"2026-07-06T03:31:04.362874Z","submitted_at":"2013-12-17T02:21:04Z","title":"The clustering of galaxies in the SDSS-III Baryon Oscillation Spectroscopic Survey: Testing gravity with redshift-space distortions using the power spectrum multipoles","version":2},"cited_work":{"arxiv_id":"1312.4611","doi":null,"metadata_source":"pith","pith_arxiv_id":"1312.4611","snapshot_observed_at":"2026-06-30T13:54:44.667611Z","title":"The clustering of galaxies in the SDSS-III Baryon Oscillation Spectroscopic Survey: Testing gravity with redshift-space distortions using the power spectrum multipoles","venue":"astro-ph.CO","work_id":"d0a57a07-f9e3-4fe4-9291-fe5e87f45b75","year":2013},"citing_paper":{"arxiv_id":"2606.29735","last_updated":"2026-06-29T03:19:33Z","snapshot_observed_at":"2026-08-03T19:18:06.305787Z","submitted_at":"2026-06-29T03:19:33Z","title":"Modeling survey-window and integral-constraint effects on PNG in the galaxy power spectrum with light-cone mocks","version":1},"reference_index":29,"source":"pdf_text","source_observed_at":"2026-06-30T05:41:24.565390Z"},"links":{"cited_paper":"/paper/1312.4611","citing_paper":"/paper/2606.29735"},"observation_digest":"sha256:d7eec5164b0440b7d5b04f9f35c44aed2e392a139d92024698e1cae9b35d0a45","observation_id":"ca184c79-ea6b-4c92-b608-985472e14a92","resolution":{"observed_at":"2026-06-30T13:54:44.668874Z","resolver_source":"local_arxiv","status":"verified_exact"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-06T06:34:29.942622+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-06T06:34:29.942622+00:00","source":"crossref"},{"observed_at":"2026-08-06T06:34:23.284952+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":{"arxiv_id":"1312.4611","last_updated":"2014-06-28T23:41:11Z","snapshot_observed_at":"2026-07-06T03:31:04.362874Z","submitted_at":"2013-12-17T02:21:04Z","title":"The clustering of galaxies in the SDSS-III Baryon Oscillation Spectroscopic Survey: Testing gravity with redshift-space distortions using the power spectrum multipoles","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"1312.4611","snapshot_observed_at":"2026-08-01T15:38:05.578284Z","title":"Beutler, S","venue":null,"work_id":null,"year":2014},"citing_paper":{"arxiv_id":"2607.18384","last_updated":"2026-07-20T18:00:02Z","snapshot_observed_at":"2026-08-01T15:37:56.916125Z","submitted_at":"2026-07-20T18:00:02Z","title":"Bispectrum BAO and the baryon-dark matter relative velocity","version":1},"reference_index":62,"source":"pdf_text","source_observed_at":"2026-08-01T15:38:05.578284Z"},"links":{"cited_paper":"/paper/1312.4611","citing_paper":"/paper/2607.18384"},"observation_digest":"sha256:1c28aaab07c9a1f71a72a3649021d05c5625a96cd83a56f502b3d3de1fb3b7c4","observation_id":"14af6ddf-f4d2-444e-adb9-33405b06616d","resolution":{"observed_at":"2026-08-01T15:38:05.578284Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}}],"links":{"evidence":"/evidence","html":"/paper/1312.4611/citation-record","integrity":"/paper/1312.4611/integrity","json":"/paper/1312.4611/citation-record.json","paper":"/paper/1312.4611"},"outbound":[],"paper":{"arxiv_id":"1312.4611","last_updated":"2014-06-28T23:41:11Z","latest_version":2,"primary_category":"astro-ph.CO","snapshot_observed_at":"2026-07-06T03:31:04.362874Z","submitted_at":"2013-12-17T02:21:04Z","title":"The clustering of galaxies in the SDSS-III Baryon Oscillation Spectroscopic Survey: Testing gravity with redshift-space distortions using the power spectrum multipoles"},"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":"2026-08-06T06:34:29.942622+00:00","source":"crossref"},{"observed_at":"2026-08-06T06:34:23.284952+00:00","source":"retraction_watch"}],"thesis":"As of 7 August 2026, this Paper Citation Record lists 0 of 0 outbound references and 9 inbound Pith citation observations for arXiv:1312.4611."}