{"as_of":"2026-08-21T12:00:00Z","caps":{"database_statements":6,"inbound":100,"outbound":100},"context_digest":"sha256:c901f2afa6de56d197294e9344224fc04a47c79646fc89d009bb7b9b040a145c","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":12,"lane":"standing_notices","note":"One-hop event checks from named stored sources.","records_observed":12,"source":"scholarly_work_events, retraction_status_cache","source_observed_at":"2026-08-21T06:32:19.484+00:00","state":"measured"},{"denominator":12,"lane":"inbound_itemization","note":"Pith citing papers itemized under the disclosed page cap.","records_observed":12,"source":"paper_references, paper_reference_links","source_observed_at":"2026-08-15T14:34:47.671383Z","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":"2026-05-19T09:35:12.681908Z","state":"measured"}],"external_citation_measurements":[],"inbound":[{"citation":{"cited_paper":{"arxiv_id":"2012.09554","last_updated":"2021-06-08T16:23:29Z","snapshot_observed_at":"2026-08-16T18:57:48.189869Z","submitted_at":"2020-12-17T13:06:58Z","title":"Assessing tension metrics with Dark Energy Survey and Planck data","version":2},"cited_work":{"arxiv_id":"2012.09554","doi":null,"metadata_source":"arxiv_reference","pith_arxiv_id":"2012.09554","snapshot_observed_at":"2026-06-05T21:23:00.469572Z","title":"Lemos, P","venue":null,"work_id":"3d7c53ce-8beb-4a9a-8986-8d16a848f7cb","year":2020},"citing_paper":{"arxiv_id":"2105.13549","last_updated":"2022-03-21T13:57:33Z","snapshot_observed_at":"2026-08-14T23:39:27.638377Z","submitted_at":"2021-05-28T01:58:58Z","title":"Dark Energy Survey Year 3 Results: Cosmological Constraints from Galaxy Clustering and Weak Lensing","version":3},"reference_index":134,"source":"pdf_text","source_observed_at":"2026-05-19T09:35:12.156800Z"},"links":{"cited_paper":"/paper/2012.09554","citing_paper":"/paper/2105.13549"},"observation_digest":"sha256:78c5bedc64c0461c8393411532ee3caab3e926ce15e9a65e88c7f47f41e2e94e","observation_id":"4aba44b3-86e4-49bb-ae0e-73646cd4eda7","resolution":{"observed_at":"2026-05-19T09:35:12.686079Z","resolver_source":"arxiv_id","status":"verified_exact"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-21T06:32:19.484+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-21T06:32:19.484+00:00","source":"crossref"},{"observed_at":"2026-08-21T06:32:16.066871+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":{"arxiv_id":"2012.09554","last_updated":"2021-06-08T16:23:29Z","snapshot_observed_at":"2026-08-16T18:57:48.189869Z","submitted_at":"2020-12-17T13:06:58Z","title":"Assessing tension metrics with Dark Energy Survey and Planck data","version":2},"cited_work":{"arxiv_id":"2012.09554","doi":null,"metadata_source":"arxiv_reference","pith_arxiv_id":"2012.09554","snapshot_observed_at":"2026-06-05T21:23:00.469572Z","title":"Lemos, P","venue":null,"work_id":"3d7c53ce-8beb-4a9a-8986-8d16a848f7cb","year":2020},"citing_paper":{"arxiv_id":"2404.03002","last_updated":"2024-11-04T16:43:36Z","snapshot_observed_at":"2026-08-18T15:21:57.876983Z","submitted_at":"2024-04-03T18:41:51Z","title":"DESI 2024 VI: Cosmological Constraints from the Measurements of Baryon Acoustic Oscillations","version":3},"reference_index":201,"source":"pdf_text","source_observed_at":"2026-05-12T02:13:10.766505Z"},"links":{"cited_paper":"/paper/2012.09554","citing_paper":"/paper/2404.03002"},"observation_digest":"sha256:bffc8329810087ebe1e52784607d49f5ed358541347b493bc1b8a89e8424c81c","observation_id":"70eb1e50-77b4-44cc-b72b-9f3687a6380f","resolution":{"observed_at":"2026-05-12T02:16:16.179267Z","resolver_source":"arxiv_id","status":"verified_exact"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-21T06:32:19.484+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-21T06:32:19.484+00:00","source":"crossref"},{"observed_at":"2026-08-21T06:32:16.066871+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":{"arxiv_id":"2012.09554","last_updated":"2021-06-08T16:23:29Z","snapshot_observed_at":"2026-08-16T18:57:48.189869Z","submitted_at":"2020-12-17T13:06:58Z","title":"Assessing tension metrics with Dark Energy Survey and Planck data","version":2},"cited_work":{"arxiv_id":"2012.09554","doi":null,"metadata_source":"arxiv_reference","pith_arxiv_id":"2012.09554","snapshot_observed_at":"2026-06-05T21:23:00.469572Z","title":"Lemos, P","venue":null,"work_id":"3d7c53ce-8beb-4a9a-8986-8d16a848f7cb","year":2020},"citing_paper":{"arxiv_id":"2411.12021","last_updated":"2025-11-24T12:55:36Z","snapshot_observed_at":"2026-08-21T11:43:52.818576Z","submitted_at":"2024-11-18T20:03:34Z","title":"DESI 2024 V: Full-Shape Galaxy Clustering from Galaxies and Quasars","version":5},"reference_index":150,"source":"pdf_text","source_observed_at":"2026-05-17T06:00:49.044220Z"},"links":{"cited_paper":"/paper/2012.09554","citing_paper":"/paper/2411.12021"},"observation_digest":"sha256:b2429f5f5b6a9e53102de26290d71f3f96a79ca813bd62fc769ffec5be1b6bdb","observation_id":"283d6455-6da2-4144-bb25-610eec2ddece","resolution":{"observed_at":"2026-05-17T06:00:49.942510Z","resolver_source":"arxiv_id","status":"verified_exact"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-21T06:32:19.484+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-21T06:32:19.484+00:00","source":"crossref"},{"observed_at":"2026-08-21T06:32:16.066871+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":{"arxiv_id":"2012.09554","last_updated":"2021-06-08T16:23:29Z","snapshot_observed_at":"2026-08-16T18:57:48.189869Z","submitted_at":"2020-12-17T13:06:58Z","title":"Assessing tension metrics with Dark Energy Survey and Planck data","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2012.09554","snapshot_observed_at":"2026-08-08T14:22:01.494914Z","title":"Lemos, M","venue":null,"work_id":null,"year":2021},"citing_paper":{"arxiv_id":"2502.06929","last_updated":"2025-07-29T21:28:38Z","snapshot_observed_at":"2026-08-18T14:06:23.428437Z","submitted_at":"2025-02-10T19:00:00Z","title":"Scalar field dark energy models: Current and forecast constraints","version":2},"reference_index":68,"source":"pdf_text","source_observed_at":"2026-08-08T14:22:01.494914Z"},"links":{"cited_paper":"/paper/2012.09554","citing_paper":"/paper/2502.06929"},"observation_digest":"sha256:72357ef5a41361bb3f5a75372ec8c13ab471de24391af9583e9fd057aa0b57b8","observation_id":"ac7f672f-2432-4c9d-a918-682392581c45","resolution":{"observed_at":"2026-08-08T14:22:01.494914Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2012.09554","last_updated":"2021-06-08T16:23:29Z","snapshot_observed_at":"2026-08-16T18:57:48.189869Z","submitted_at":"2020-12-17T13:06:58Z","title":"Assessing tension metrics with Dark Energy Survey and Planck data","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2012.09554","snapshot_observed_at":"2026-08-03T23:41:00.517571Z","title":"Lemos, M","venue":null,"work_id":null,"year":2021},"citing_paper":{"arxiv_id":"2511.04661","last_updated":"2026-06-10T16:49:52Z","snapshot_observed_at":"2026-08-12T19:40:05.915235Z","submitted_at":"2025-11-06T18:48:39Z","title":"unimpeded: A Public Grid of Nested Sampling Chains for Cosmological Model Comparison and Tension Analysis","version":3},"reference_index":28,"source":"pdf_text","source_observed_at":"2026-08-03T23:41:00.517571Z"},"links":{"cited_paper":"/paper/2012.09554","citing_paper":"/paper/2511.04661"},"observation_digest":"sha256:4d1afd5784b7a59b682f6803126dfe9ce4af98341aae491ed7d4a38b6067afb9","observation_id":"89e206e9-1c83-478b-a93c-34b488e02b57","resolution":{"observed_at":"2026-08-03T23:41:00.517571Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2012.09554","last_updated":"2021-06-08T16:23:29Z","snapshot_observed_at":"2026-08-16T18:57:48.189869Z","submitted_at":"2020-12-17T13:06:58Z","title":"Assessing tension metrics with Dark Energy Survey and Planck data","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2012.09554","snapshot_observed_at":"2026-08-03T20:12:23.754797Z","title":"Watanabe,A widely applicable bayesian information criterion,J","venue":null,"work_id":null,"year":2013},"citing_paper":{"arxiv_id":"2511.21071","last_updated":"2026-06-27T14:06:53Z","snapshot_observed_at":"2026-08-20T03:46:28.459146Z","submitted_at":"2025-11-26T05:26:01Z","title":"Cosmological tensions in Proca-Nuevo theory","version":2},"reference_index":117,"source":"pdf_text","source_observed_at":"2026-08-03T20:12:23.754797Z"},"links":{"cited_paper":"/paper/2012.09554","citing_paper":"/paper/2511.21071"},"observation_digest":"sha256:9d7e6a919d9f8ead3a023092e68ff66d5584f1bfeffcf38a623b259f5f479300","observation_id":"6e424605-1be2-4012-a74c-cdf386d6cab6","resolution":{"observed_at":"2026-08-03T20:12:23.754797Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2012.09554","last_updated":"2021-06-08T16:23:29Z","snapshot_observed_at":"2026-08-16T18:57:48.189869Z","submitted_at":"2020-12-17T13:06:58Z","title":"Assessing tension metrics with Dark Energy Survey and Planck data","version":2},"cited_work":{"arxiv_id":"2012.09554","doi":null,"metadata_source":"arxiv_reference","pith_arxiv_id":"2012.09554","snapshot_observed_at":"2026-06-05T21:23:00.469572Z","title":"Lemos, P","venue":null,"work_id":"3d7c53ce-8beb-4a9a-8986-8d16a848f7cb","year":2020},"citing_paper":{"arxiv_id":"2601.02077","last_updated":"2026-04-04T13:29:01Z","snapshot_observed_at":"2026-08-14T19:15:34.404775Z","submitted_at":"2026-01-05T12:58:36Z","title":"Joint Constraints on Neutrinos and Dynamical Dark Energy in Minimally Modified Gravity","version":2},"reference_index":121,"source":"pdf_text","source_observed_at":"2026-05-16T18:00:59.984076Z"},"links":{"cited_paper":"/paper/2012.09554","citing_paper":"/paper/2601.02077"},"observation_digest":"sha256:6fc0ac6185b9fd5944138e1b0a80f5500f240be7006b0381e041716b77d167b8","observation_id":"ce1a2fbb-9388-433a-a5f9-7087569c3bcd","resolution":{"observed_at":"2026-05-16T18:01:09.053435Z","resolver_source":"arxiv_id","status":"verified_exact"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-21T06:32:19.484+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-21T06:32:19.484+00:00","source":"crossref"},{"observed_at":"2026-08-21T06:32:16.066871+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":{"arxiv_id":"2012.09554","last_updated":"2021-06-08T16:23:29Z","snapshot_observed_at":"2026-08-16T18:57:48.189869Z","submitted_at":"2020-12-17T13:06:58Z","title":"Assessing tension metrics with Dark Energy Survey and Planck data","version":2},"cited_work":{"arxiv_id":"2012.09554","doi":null,"metadata_source":"arxiv_reference","pith_arxiv_id":"2012.09554","snapshot_observed_at":"2026-06-05T21:23:00.469572Z","title":"Lemos, P","venue":null,"work_id":"3d7c53ce-8beb-4a9a-8986-8d16a848f7cb","year":2020},"citing_paper":{"arxiv_id":"2602.03110","last_updated":"2026-04-28T09:37:14Z","snapshot_observed_at":"2026-08-17T20:59:00.323360Z","submitted_at":"2026-02-03T05:11:50Z","title":"Evidence for deviation in gravitational light deflection from general relativity at cosmological scales with KiDS-Legacy and CMB lensing","version":2},"reference_index":37,"source":"pdf_text","source_observed_at":"2026-05-16T08:17:34.164338Z"},"links":{"cited_paper":"/paper/2012.09554","citing_paper":"/paper/2602.03110"},"observation_digest":"sha256:f46ae52262543bf92db179893777d9f5ffb08391a2b7a614e449062e45c55789","observation_id":"bb2f0da1-34c5-49aa-96b4-a7a7f8cfc269","resolution":{"observed_at":"2026-05-16T08:17:35.679601Z","resolver_source":"arxiv_id","status":"verified_exact"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-21T06:32:19.484+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-21T06:32:19.484+00:00","source":"crossref"},{"observed_at":"2026-08-21T06:32:16.066871+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":{"arxiv_id":"2012.09554","last_updated":"2021-06-08T16:23:29Z","snapshot_observed_at":"2026-08-16T18:57:48.189869Z","submitted_at":"2020-12-17T13:06:58Z","title":"Assessing tension metrics with Dark Energy Survey and Planck data","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2012.09554","snapshot_observed_at":"2026-08-02T18:35:56.164241Z","title":"Lemoset al.(DES), Mon","venue":null,"work_id":null,"year":2021},"citing_paper":{"arxiv_id":"2603.09270","last_updated":"2026-07-22T07:14:15Z","snapshot_observed_at":"2026-08-14T16:32:53.753165Z","submitted_at":"2026-03-10T06:56:54Z","title":"Statistical consistency of sign-switching vacuum energy with cosmological observations","version":2},"reference_index":85,"source":"pdf_text","source_observed_at":"2026-08-02T18:35:56.164241Z"},"links":{"cited_paper":"/paper/2012.09554","citing_paper":"/paper/2603.09270"},"observation_digest":"sha256:8790e74aef595b1d1f2c3de34f671e47620a040a282e93af2d4fd250eac6c76d","observation_id":"407ac327-2835-4501-a301-707e30843d9b","resolution":{"observed_at":"2026-08-02T18:35:56.164241Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2012.09554","last_updated":"2021-06-08T16:23:29Z","snapshot_observed_at":"2026-08-16T18:57:48.189869Z","submitted_at":"2020-12-17T13:06:58Z","title":"Assessing tension metrics with Dark Energy Survey and Planck data","version":2},"cited_work":{"arxiv_id":"2012.09554","doi":null,"metadata_source":"arxiv_reference","pith_arxiv_id":"2012.09554","snapshot_observed_at":"2026-06-05T21:23:00.469572Z","title":"Lemos, P","venue":null,"work_id":"3d7c53ce-8beb-4a9a-8986-8d16a848f7cb","year":2020},"citing_paper":{"arxiv_id":"2604.11694","last_updated":"2026-04-13T16:33:23Z","snapshot_observed_at":"2026-08-14T14:06:33.818816Z","submitted_at":"2026-04-13T16:33:23Z","title":"Cosmological inference with halo clustering reconstructed from the redshift-space galaxy distribution","version":1},"reference_index":20,"source":"pdf_text","source_observed_at":"2026-05-10T15:10:48.528283Z"},"links":{"cited_paper":"/paper/2012.09554","citing_paper":"/paper/2604.11694"},"observation_digest":"sha256:77a85d682679c6be7e94b74ba206962409d2110b9b259ce355ff8497831a9019","observation_id":"dacb15e3-c334-4ece-9165-ff7bf7b9150a","resolution":{"observed_at":"2026-05-11T11:01:25.135814Z","resolver_source":"arxiv_id","status":"verified_exact"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-21T06:32:19.484+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-21T06:32:19.484+00:00","source":"crossref"},{"observed_at":"2026-08-21T06:32:16.066871+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":{"arxiv_id":"2012.09554","last_updated":"2021-06-08T16:23:29Z","snapshot_observed_at":"2026-08-16T18:57:48.189869Z","submitted_at":"2020-12-17T13:06:58Z","title":"Assessing tension metrics with Dark Energy Survey and Planck data","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2012.09554","snapshot_observed_at":"2026-07-11T09:40:49.196932Z","title":"Watanabe,A widely applicable bayesian information criterion, 2012","venue":null,"work_id":null,"year":2012},"citing_paper":{"arxiv_id":"2607.05044","last_updated":"2026-07-06T13:21:04Z","snapshot_observed_at":"2026-08-15T13:09:12.340147Z","submitted_at":"2026-07-06T13:21:04Z","title":"Alleviating the Hubble Tension with Smooth Sign-Switching Dark Energy: Full CMB Constraints with DESI and PantheonPlus","version":1},"reference_index":188,"source":"pdf_text","source_observed_at":"2026-07-11T09:40:49.196932Z"},"links":{"cited_paper":"/paper/2012.09554","citing_paper":"/paper/2607.05044"},"observation_digest":"sha256:451e2ff1bebaae91899f3f07cb61af84803e3d51b94eaba2cad1d34b6bcfb7e8","observation_id":"34021f29-9b3c-4d5c-b267-ad424b6e4b3b","resolution":{"observed_at":"2026-07-11T09:40:49.196932Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2012.09554","last_updated":"2021-06-08T16:23:29Z","snapshot_observed_at":"2026-08-16T18:57:48.189869Z","submitted_at":"2020-12-17T13:06:58Z","title":"Assessing tension metrics with Dark Energy Survey and Planck data","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2012.09554","snapshot_observed_at":"2026-08-15T14:34:47.671383Z","title":", keywords =","venue":null,"work_id":null,"year":2012},"citing_paper":{"arxiv_id":"2608.07377","last_updated":"2026-08-07T16:20:30Z","snapshot_observed_at":"2026-08-19T08:43:18.922464Z","submitted_at":"2026-08-07T16:20:30Z","title":"KiDS-1000: Improved constraints on cosmology, intrinsic alignments and baryonic feedback from clipped cosmic shear","version":1},"reference_index":223,"source":"arxiv_source","source_observed_at":"2026-08-15T14:34:47.671383Z"},"links":{"cited_paper":"/paper/2012.09554","citing_paper":"/paper/2608.07377"},"observation_digest":"sha256:fb9952fe73d0d0c1aea0d127e2a9b29e6630d3733c8d1f5663d36d19e004ef72","observation_id":"654b328f-8c12-4a54-8851-c2278886c923","resolution":{"observed_at":"2026-08-15T14:34:47.671383Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}}],"links":{"evidence":"/evidence","html":"/paper/2012.09554/citation-record","integrity":"/paper/2012.09554/integrity","json":"/paper/2012.09554/citation-record.json","paper":"/paper/2012.09554"},"outbound":[],"paper":{"arxiv_id":"2012.09554","last_updated":"2021-06-08T16:23:29Z","latest_version":2,"primary_category":"astro-ph.CO","snapshot_observed_at":"2026-08-16T18:57:48.189869Z","submitted_at":"2020-12-17T13:06:58Z","title":"Assessing tension metrics with Dark Energy Survey and Planck data"},"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":"2026-08-21T06:32:19.484+00:00","source":"crossref"},{"observed_at":"2026-08-21T06:32:16.066871+00:00","source":"retraction_watch"}],"thesis":"As of 21 August 2026, this Paper Citation Record lists 0 of 0 outbound references and 12 inbound Pith citation observations for arXiv:2012.09554."}