{"as_of":"2026-08-19T12:05:00Z","caps":{"database_statements":6,"inbound":100,"outbound":100},"context_digest":"sha256:da16b0fb942323fe56388e1d4a658038a6f721c05c67f2a3e70b1dd9bfe69a6a","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":"2026-08-19T06:32:44.657259+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":"2026-08-09T14:46:06.868607Z","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":"2026-07-03T06:27:41.790915Z","state":"measured"}],"external_citation_measurements":[],"inbound":[{"citation":{"cited_paper":{"arxiv_id":"1909.05869","last_updated":"2019-09-12T18:00:02Z","snapshot_observed_at":"2026-08-13T14:43:59.763133Z","submitted_at":"2019-09-12T18:00:02Z","title":"Data compression in cosmology: A compressed likelihood for Planck data","version":1},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"1909.05869","snapshot_observed_at":"2026-08-09T14:46:06.868607Z","title":"Prince and J","venue":null,"work_id":null,"year":2019},"citing_paper":{"arxiv_id":"2502.01722","last_updated":"2025-06-30T13:35:52Z","snapshot_observed_at":"2026-08-14T08:36:58.524440Z","submitted_at":"2025-02-03T19:00:00Z","title":"Tuning the cosmic instrument: robust cosmology through combined probes","version":4},"reference_index":122,"source":"pdf_text","source_observed_at":"2026-08-09T14:46:06.868607Z"},"links":{"cited_paper":"/paper/1909.05869","citing_paper":"/paper/2502.01722"},"observation_digest":"sha256:f825163a1967af6da6367d976bd4e3eba727ac8455bcbfda5ecefcf40c97ea8c","observation_id":"b242d157-3265-424c-abe7-cbd3943bf3ce","resolution":{"observed_at":"2026-08-09T14:46:06.868607Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"1909.05869","last_updated":"2019-09-12T18:00:02Z","snapshot_observed_at":"2026-08-13T14:43:59.763133Z","submitted_at":"2019-09-12T18:00:02Z","title":"Data compression in cosmology: A compressed likelihood for Planck data","version":1},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"1909.05869","snapshot_observed_at":"2026-08-07T20:33:58.185066Z","title":"Prince and J","venue":null,"work_id":null,"year":2019},"citing_paper":{"arxiv_id":"2502.09810","last_updated":"2025-03-28T12:50:30Z","snapshot_observed_at":"2026-08-09T21:41:06.451790Z","submitted_at":"2025-02-13T23:02:39Z","title":"$\\Lambda$CDM and early dark energy in latent space: a data-driven parametrization of the CMB temperature power spectrum","version":2},"reference_index":56,"source":"pdf_text","source_observed_at":"2026-08-07T20:33:58.185066Z"},"links":{"cited_paper":"/paper/1909.05869","citing_paper":"/paper/2502.09810"},"observation_digest":"sha256:2b4fa199f6a899a40c917844be35199931793c7860f5eb9e80b7f037a5ae1715","observation_id":"15590f7a-a5de-4263-8953-94e52e418232","resolution":{"observed_at":"2026-08-07T20:33:58.185066Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"1909.05869","last_updated":"2019-09-12T18:00:02Z","snapshot_observed_at":"2026-08-13T14:43:59.763133Z","submitted_at":"2019-09-12T18:00:02Z","title":"Data compression in cosmology: A compressed likelihood for Planck data","version":1},"cited_work":{"arxiv_id":"1909.05869","doi":null,"metadata_source":"arxiv_reference","pith_arxiv_id":"1909.05869","snapshot_observed_at":"2026-07-03T06:27:41.790915Z","title":"Prince and J","venue":null,"work_id":"b28a2f2c-f448-4953-9783-f6892aca8bdb","year":2019},"citing_paper":{"arxiv_id":"2607.02498","last_updated":"2026-07-09T17:52:11Z","snapshot_observed_at":"2026-08-16T05:38:15.177963Z","submitted_at":"2026-07-02T17:57:15Z","title":"Alleviating prior dependencies for DESI DR1 clustering fits through reparameterization","version":1},"reference_index":123,"source":"pdf_text","source_observed_at":"2026-07-03T06:27:31.520900Z"},"links":{"cited_paper":"/paper/1909.05869","citing_paper":"/paper/2607.02498"},"observation_digest":"sha256:59e2b4f888a1a98563998071f0afbc72bfd8d2a6a0a3c35f3e31ca82b74f4aff","observation_id":"ac6da1af-5022-4bd7-9824-a658e12e973a","resolution":{"observed_at":"2026-07-03T06:27:41.792266Z","resolver_source":"arxiv_id","status":"verified_exact"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-19T06:32:44.657259+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-19T06:32:44.657259+00:00","source":"crossref"},{"observed_at":"2026-08-19T06:32:39.956319+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":{"arxiv_id":"1909.05869","last_updated":"2019-09-12T18:00:02Z","snapshot_observed_at":"2026-08-13T14:43:59.763133Z","submitted_at":"2019-09-12T18:00:02Z","title":"Data compression in cosmology: A compressed likelihood for Planck data","version":1},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"1909.05869","snapshot_observed_at":"2026-07-12T08:00:27.085537Z","title":"Prince and J","venue":null,"work_id":null,"year":2019},"citing_paper":{"arxiv_id":"2607.02498","last_updated":"2026-07-09T17:52:11Z","snapshot_observed_at":"2026-08-16T05:38:15.177963Z","submitted_at":"2026-07-02T17:57:15Z","title":"Alleviating prior dependencies for DESI DR1 clustering fits through reparameterization","version":2},"reference_index":123,"source":"pdf_text","source_observed_at":"2026-07-12T08:00:27.085537Z"},"links":{"cited_paper":"/paper/1909.05869","citing_paper":"/paper/2607.02498"},"observation_digest":"sha256:3d5295cd5d449c3b51a5c3b9be17facc205455e53c41915acdd86266c5045e75","observation_id":"76afa781-3e7d-479a-a1a1-5b2a3cec5fa6","resolution":{"observed_at":"2026-07-12T08:00:27.085537Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"1909.05869","last_updated":"2019-09-12T18:00:02Z","snapshot_observed_at":"2026-08-13T14:43:59.763133Z","submitted_at":"2019-09-12T18:00:02Z","title":"Data compression in cosmology: A compressed likelihood for Planck data","version":1},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"1909.05869","snapshot_observed_at":"2026-08-03T00:39:01.029960Z","title":", keywords =","venue":null,"work_id":null,"year":1909},"citing_paper":{"arxiv_id":"2607.28725","last_updated":"2026-07-30T18:00:01Z","snapshot_observed_at":"2026-08-14T14:32:47.438741Z","submitted_at":"2026-07-30T18:00:01Z","title":"A Simulation Based Inference Approach to Modelling of Type Ia Supernova Populations","version":1},"reference_index":107,"source":"arxiv_source","source_observed_at":"2026-08-03T00:39:01.029960Z"},"links":{"cited_paper":"/paper/1909.05869","citing_paper":"/paper/2607.28725"},"observation_digest":"sha256:6918d2306d6c7a29077e47bdda8917035964877b578ef218c284c02e0ebef892","observation_id":"51067bd8-8a44-425a-b8a4-541d1feaaf2c","resolution":{"observed_at":"2026-08-03T00:39:01.029960Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}}],"links":{"evidence":"/evidence","html":"/paper/1909.05869/citation-record","integrity":"/paper/1909.05869/integrity","json":"/paper/1909.05869/citation-record.json","paper":"/paper/1909.05869"},"outbound":[],"paper":{"arxiv_id":"1909.05869","last_updated":"2019-09-12T18:00:02Z","latest_version":1,"primary_category":"astro-ph.CO","snapshot_observed_at":"2026-08-13T14:43:59.763133Z","submitted_at":"2019-09-12T18:00:02Z","title":"Data compression in cosmology: A compressed likelihood for 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":"2026-08-19T06:32:44.657259+00:00","source":"crossref"},{"observed_at":"2026-08-19T06:32:39.956319+00:00","source":"retraction_watch"}],"thesis":"As of 19 August 2026, this Paper Citation Record lists 0 of 0 outbound references and 5 inbound Pith citation observations for arXiv:1909.05869."}