{"as_of":"2026-08-06T13:47:00Z","caps":{"database_statements":6,"inbound":100,"outbound":100},"context_digest":"sha256:9ee91d238184b12ad615e8efb3ef416d9c78d513695486f25a914ab9b328e236","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":"2026-08-06T06:34:29.942622+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":"2026-08-03T20:12:23.757789Z","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":"2026-05-16T18:01:09.133304Z","state":"measured"}],"external_citation_measurements":[],"inbound":[{"citation":{"cited_paper":{"arxiv_id":"1912.04880","last_updated":"2019-12-10T18:40:14Z","snapshot_observed_at":"2026-08-04T16:02:18.701984Z","submitted_at":"2019-12-10T18:40:14Z","title":"Quantifying concordance of correlated cosmological data sets","version":1},"cited_work":{"arxiv_id":"1912.04880","doi":null,"metadata_source":"arxiv_reference","pith_arxiv_id":"1912.04880","snapshot_observed_at":"2026-06-05T21:23:00.469572Z","title":"Raveri, G","venue":null,"work_id":"7ead8c65-1553-43e9-8909-7abab70685c6","year":2020},"citing_paper":{"arxiv_id":"2503.14744","last_updated":"2025-10-07T13:00:34Z","snapshot_observed_at":"2026-07-06T20:55:04.493800Z","submitted_at":"2025-03-18T21:14:18Z","title":"Constraints on Neutrino Physics from DESI DR2 BAO and DR1 Full Shape","version":3},"reference_index":205,"source":"pdf_text","source_observed_at":"2026-05-16T17:46:22.581000Z"},"links":{"cited_paper":"/paper/1912.04880","citing_paper":"/paper/2503.14744"},"observation_digest":"sha256:1f6753941830c08a7659a1747d394007cdaa01134203b341e57fc75c91e74042","observation_id":"5fe2d0c8-0bbc-47b3-bd91-7cb5b3311b9c","resolution":{"observed_at":"2026-05-16T17:46:22.747596Z","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":"1912.04880","last_updated":"2019-12-10T18:40:14Z","snapshot_observed_at":"2026-08-04T16:02:18.701984Z","submitted_at":"2019-12-10T18:40:14Z","title":"Quantifying concordance of correlated cosmological data sets","version":1},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"1912.04880","snapshot_observed_at":"2026-08-03T20:12:23.757789Z","title":"Raveri, G","venue":null,"work_id":null,"year":2020},"citing_paper":{"arxiv_id":"2511.21071","last_updated":"2026-06-27T14:06:53Z","snapshot_observed_at":"2026-08-03T23:12:51.843963Z","submitted_at":"2025-11-26T05:26:01Z","title":"Cosmological tensions in Proca-Nuevo theory","version":2},"reference_index":119,"source":"pdf_text","source_observed_at":"2026-08-03T20:12:23.757789Z"},"links":{"cited_paper":"/paper/1912.04880","citing_paper":"/paper/2511.21071"},"observation_digest":"sha256:69d769e9df0951a9d03ac7ac5a322ee19223e1a9c650fc623942adc9ba868667","observation_id":"2af17ac2-2250-42e5-a2d3-413f84b1078f","resolution":{"observed_at":"2026-08-03T20:12:23.757789Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"1912.04880","last_updated":"2019-12-10T18:40:14Z","snapshot_observed_at":"2026-08-04T16:02:18.701984Z","submitted_at":"2019-12-10T18:40:14Z","title":"Quantifying concordance of correlated cosmological data sets","version":1},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"1912.04880","snapshot_observed_at":"2026-08-03T17:24:59.354541Z","title":"Raveri, G","venue":null,"work_id":null,"year":2020},"citing_paper":{"arxiv_id":"2512.09991","last_updated":"2026-06-01T10:52:35Z","snapshot_observed_at":"2026-08-03T17:24:26.448316Z","submitted_at":"2025-12-10T19:00:02Z","title":"Observational constraints on 3-forms dark energy","version":2},"reference_index":89,"source":"pdf_text","source_observed_at":"2026-08-03T17:24:59.354541Z"},"links":{"cited_paper":"/paper/1912.04880","citing_paper":"/paper/2512.09991"},"observation_digest":"sha256:49c9c2d8f4652d0d43a5e2b6a0bec0771a1e5051474e697769341c56edddc531","observation_id":"89811542-ffee-48fa-a686-62c9732a3d4a","resolution":{"observed_at":"2026-08-03T17:24:59.354541Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"1912.04880","last_updated":"2019-12-10T18:40:14Z","snapshot_observed_at":"2026-08-04T16:02:18.701984Z","submitted_at":"2019-12-10T18:40:14Z","title":"Quantifying concordance of correlated cosmological data sets","version":1},"cited_work":{"arxiv_id":"1912.04880","doi":null,"metadata_source":"arxiv_reference","pith_arxiv_id":"1912.04880","snapshot_observed_at":"2026-06-05T21:23:00.469572Z","title":"Raveri, G","venue":null,"work_id":"7ead8c65-1553-43e9-8909-7abab70685c6","year":2020},"citing_paper":{"arxiv_id":"2601.02077","last_updated":"2026-04-04T13:29:01Z","snapshot_observed_at":"2026-08-02T21:22:34.193403Z","submitted_at":"2026-01-05T12:58:36Z","title":"Joint Constraints on Neutrinos and Dynamical Dark Energy in Minimally Modified Gravity","version":2},"reference_index":119,"source":"pdf_text","source_observed_at":"2026-05-16T18:00:59.984076Z"},"links":{"cited_paper":"/paper/1912.04880","citing_paper":"/paper/2601.02077"},"observation_digest":"sha256:2b5a8c1773d4e9cacbb39451b7799f50b1e178a6ffa08d49155b3194516649e9","observation_id":"cb11b356-3ff2-4933-bcfb-2f630e9812a7","resolution":{"observed_at":"2026-05-16T18:01:09.135636Z","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":"1912.04880","last_updated":"2019-12-10T18:40:14Z","snapshot_observed_at":"2026-08-04T16:02:18.701984Z","submitted_at":"2019-12-10T18:40:14Z","title":"Quantifying concordance of correlated cosmological data sets","version":1},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"1912.04880","snapshot_observed_at":"2026-08-02T18:35:56.295627Z","title":"Raveri, G","venue":null,"work_id":null,"year":2020},"citing_paper":{"arxiv_id":"2603.09270","last_updated":"2026-07-22T07:14:15Z","snapshot_observed_at":"2026-08-05T18:56:34.104744Z","submitted_at":"2026-03-10T06:56:54Z","title":"Statistical consistency of sign-switching vacuum energy with cosmological observations","version":2},"reference_index":87,"source":"pdf_text","source_observed_at":"2026-08-02T18:35:56.295627Z"},"links":{"cited_paper":"/paper/1912.04880","citing_paper":"/paper/2603.09270"},"observation_digest":"sha256:deca902ce1a9fc9686d69d8886e3441f803a4c05bc404069166a226f797a8c3c","observation_id":"2eb8a407-4f24-4356-b0da-2e8196c35df4","resolution":{"observed_at":"2026-08-02T18:35:56.295627Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"1912.04880","last_updated":"2019-12-10T18:40:14Z","snapshot_observed_at":"2026-08-04T16:02:18.701984Z","submitted_at":"2019-12-10T18:40:14Z","title":"Quantifying concordance of correlated cosmological data sets","version":1},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"1912.04880","snapshot_observed_at":"2026-07-11T09:40:49.196932Z","title":"Raveri, G","venue":null,"work_id":null,"year":2020},"citing_paper":{"arxiv_id":"2607.05044","last_updated":"2026-07-06T13:21:04Z","snapshot_observed_at":"2026-08-06T06:21:38.078437Z","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":189,"source":"pdf_text","source_observed_at":"2026-07-11T09:40:49.196932Z"},"links":{"cited_paper":"/paper/1912.04880","citing_paper":"/paper/2607.05044"},"observation_digest":"sha256:ee2d2b27a00f0cae815d9b8371286dce9107956462ce8ab93e16a9c9603c8972","observation_id":"0cecb8d2-6cd8-4adf-9e68-8736ed6dbfe2","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"}}],"links":{"evidence":"/evidence","html":"/paper/1912.04880/citation-record","integrity":"/paper/1912.04880/integrity","json":"/paper/1912.04880/citation-record.json","paper":"/paper/1912.04880"},"outbound":[],"paper":{"arxiv_id":"1912.04880","last_updated":"2019-12-10T18:40:14Z","latest_version":1,"primary_category":"astro-ph.CO","snapshot_observed_at":"2026-08-04T16:02:18.701984Z","submitted_at":"2019-12-10T18:40:14Z","title":"Quantifying concordance of correlated cosmological data sets"},"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 6 August 2026, this Paper Citation Record lists 0 of 0 outbound references and 6 inbound Pith citation observations for arXiv:1912.04880."}