{"as_of":"2026-08-23T06:56:00Z","caps":{"database_statements":6,"inbound":100,"outbound":100},"context_digest":"sha256:3e61f59921570140f027137488abba7285c81fe25004043509c6d81feda50aa3","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":13,"lane":"standing_notices","note":"One-hop event checks from named stored sources.","records_observed":13,"source":"scholarly_work_events, retraction_status_cache","source_observed_at":"2026-08-23T06:30:58.430688+00:00","state":"measured"},{"denominator":13,"lane":"inbound_itemization","note":"Pith citing papers itemized under the disclosed page cap.","records_observed":13,"source":"paper_references, paper_reference_links","source_observed_at":"2026-08-16T01:06:27.397769Z","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":"2026-07-02T14:57:04.118144Z","state":"measured"}],"external_citation_measurements":[],"inbound":[{"citation":{"cited_paper":{"arxiv_id":"1902.04029","last_updated":"2019-11-23T12:20:25Z","snapshot_observed_at":"2026-08-14T17:17:58.396509Z","submitted_at":"2019-02-11T18:11:13Z","title":"Quantifying tensions in cosmological parameters: Interpreting the DES evidence ratio","version":5},"cited_work":{"arxiv_id":"1902.04029","doi":null,"metadata_source":"arxiv_reference","pith_arxiv_id":"1902.04029","snapshot_observed_at":"2026-07-02T14:57:04.118144Z","title":"Handley and P","venue":null,"work_id":"4c47107e-900f-4b84-8036-6b72053ac13d","year":2019},"citing_paper":{"arxiv_id":"1907.10946","last_updated":"2019-07-25T10:18:12Z","snapshot_observed_at":"2026-08-03T05:47:08.666465Z","submitted_at":"2019-07-25T10:18:12Z","title":"Constraining Dark Energy Perturbations: the Role of Early Dark Energy","version":1},"reference_index":37,"source":"pdf_text","source_observed_at":"2026-05-24T16:08:46.516373Z"},"links":{"cited_paper":"/paper/1902.04029","citing_paper":"/paper/1907.10946"},"observation_digest":"sha256:f6238eac4db1056bb5c1172f8c3d6c51bf45ca723b18dca167b0fa75ad863ec4","observation_id":"52ef4490-db96-4ddb-a6df-3a08b28e4920","resolution":{"observed_at":"2026-05-24T16:09:39.690126Z","resolver_source":"arxiv_id","status":"verified_exact"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-23T06:30:58.430688+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-23T06:30:58.430688+00:00","source":"crossref"},{"observed_at":"2026-08-23T06:30:53.778098+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":{"arxiv_id":"1902.04029","last_updated":"2019-11-23T12:20:25Z","snapshot_observed_at":"2026-08-14T17:17:58.396509Z","submitted_at":"2019-02-11T18:11:13Z","title":"Quantifying tensions in cosmological parameters: Interpreting the DES evidence ratio","version":5},"cited_work":{"arxiv_id":"1902.04029","doi":null,"metadata_source":"arxiv_reference","pith_arxiv_id":"1902.04029","snapshot_observed_at":"2026-07-02T14:57:04.118144Z","title":"Handley and P","venue":null,"work_id":"4c47107e-900f-4b84-8036-6b72053ac13d","year":2019},"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":149,"source":"pdf_text","source_observed_at":"2026-05-17T06:00:49.044220Z"},"links":{"cited_paper":"/paper/1902.04029","citing_paper":"/paper/2411.12021"},"observation_digest":"sha256:d56e9a0af1d944874ee563bd7d9c520a9a926f8f6a48ae57c6c0c9a5c9d3e2bb","observation_id":"95f10b0f-5b57-428e-8ea8-b38506a31559","resolution":{"observed_at":"2026-05-17T06:00:49.938088Z","resolver_source":"arxiv_id","status":"verified_exact"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-23T06:30:58.430688+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-23T06:30:58.430688+00:00","source":"crossref"},{"observed_at":"2026-08-23T06:30:53.778098+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":{"arxiv_id":"1902.04029","last_updated":"2019-11-23T12:20:25Z","snapshot_observed_at":"2026-08-14T17:17:58.396509Z","submitted_at":"2019-02-11T18:11:13Z","title":"Quantifying tensions in cosmological parameters: Interpreting the DES evidence ratio","version":5},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"1902.04029","snapshot_observed_at":"2026-08-10T22:01:00.032038Z","title":"Handley and P","venue":null,"work_id":null,"year":2019},"citing_paper":{"arxiv_id":"2501.03480","last_updated":"2025-07-02T14:03:15Z","snapshot_observed_at":"2026-08-12T17:48:55.146084Z","submitted_at":"2025-01-07T02:51:33Z","title":"Is excess smoothing of Planck CMB ansiotropy data partially responsible for evidence for dark energy dynamics in other $w(z)$CDM parametrizations?","version":2},"reference_index":91,"source":"pdf_text","source_observed_at":"2026-08-10T22:01:00.032038Z"},"links":{"cited_paper":"/paper/1902.04029","citing_paper":"/paper/2501.03480"},"observation_digest":"sha256:764a182fba31a54643d23a724a6bdb7ac9a3a75bbc946272b0a802ed7af0f3ff","observation_id":"b5ac13d4-de45-4953-a756-34d075432ef2","resolution":{"observed_at":"2026-08-10T22:01:00.032038Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"1902.04029","last_updated":"2019-11-23T12:20:25Z","snapshot_observed_at":"2026-08-14T17:17:58.396509Z","submitted_at":"2019-02-11T18:11:13Z","title":"Quantifying tensions in cosmological parameters: Interpreting the DES evidence ratio","version":5},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"1902.04029","snapshot_observed_at":"2026-08-16T01:06:27.397769Z","title":"Handley and P","venue":null,"work_id":null,"year":2019},"citing_paper":{"arxiv_id":"2505.02207","last_updated":"2025-05-06T20:39:31Z","snapshot_observed_at":"2026-08-17T11:47:20.831905Z","submitted_at":"2025-05-04T18:06:04Z","title":"On the tension between DESI DR2 BAO and CMB","version":2},"reference_index":27,"source":"pdf_text","source_observed_at":"2026-08-16T01:06:27.397769Z"},"links":{"cited_paper":"/paper/1902.04029","citing_paper":"/paper/2505.02207"},"observation_digest":"sha256:af49099654f095c7b135744779cee81e674cda392d256688ab76b5c25840c867","observation_id":"a659257d-bf00-41bd-908b-43140b2810f1","resolution":{"observed_at":"2026-08-16T01:06:27.397769Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"1902.04029","last_updated":"2019-11-23T12:20:25Z","snapshot_observed_at":"2026-08-14T17:17:58.396509Z","submitted_at":"2019-02-11T18:11:13Z","title":"Quantifying tensions in cosmological parameters: Interpreting the DES evidence ratio","version":5},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"1902.04029","snapshot_observed_at":"2026-08-06T13:22:38.630456Z","title":"Handley and P","venue":null,"work_id":null,"year":2019},"citing_paper":{"arxiv_id":"2507.20991","last_updated":"2025-07-28T16:50:33Z","snapshot_observed_at":"2026-08-16T12:12:29.559886Z","submitted_at":"2025-07-28T16:50:33Z","title":"Debiasing inference in large-scale structure with non-flat volume measures","version":1},"reference_index":29,"source":"pdf_text","source_observed_at":"2026-08-06T13:22:38.630456Z"},"links":{"cited_paper":"/paper/1902.04029","citing_paper":"/paper/2507.20991"},"observation_digest":"sha256:c3caa567cb6a4d99819709dc4ad349429a80ed1624116419b647d0360f75f161","observation_id":"7fae9b19-9d5f-492e-92d5-55e52ec9b9c2","resolution":{"observed_at":"2026-08-06T13:22:38.630456Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"1902.04029","last_updated":"2019-11-23T12:20:25Z","snapshot_observed_at":"2026-08-14T17:17:58.396509Z","submitted_at":"2019-02-11T18:11:13Z","title":"Quantifying tensions in cosmological parameters: Interpreting the DES evidence ratio","version":5},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"1902.04029","snapshot_observed_at":"2026-08-04T13:43:12.350764Z","title":"Handley and P","venue":null,"work_id":null,"year":2019},"citing_paper":{"arxiv_id":"2509.25812","last_updated":"2026-07-24T17:00:01Z","snapshot_observed_at":"2026-08-06T01:07:38.127403Z","submitted_at":"2025-09-30T05:41:44Z","title":"Updated observational constraints on $\\phi$CDM dynamical dark energy cosmological models","version":3},"reference_index":78,"source":"pdf_text","source_observed_at":"2026-08-04T13:43:12.350764Z"},"links":{"cited_paper":"/paper/1902.04029","citing_paper":"/paper/2509.25812"},"observation_digest":"sha256:42fa9e0430e28629f7d4fd51846f12ce2efe863aadb36530e38c82e89c6cdfdd","observation_id":"86507e60-e432-484b-8f4c-58d4efec1d58","resolution":{"observed_at":"2026-08-04T13:43:12.350764Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"1902.04029","last_updated":"2019-11-23T12:20:25Z","snapshot_observed_at":"2026-08-14T17:17:58.396509Z","submitted_at":"2019-02-11T18:11:13Z","title":"Quantifying tensions in cosmological parameters: Interpreting the DES evidence ratio","version":5},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"1902.04029","snapshot_observed_at":"2026-08-03T23:41:00.474366Z","title":"Handley and P","venue":null,"work_id":null,"year":2019},"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":8,"source":"pdf_text","source_observed_at":"2026-08-03T23:41:00.474366Z"},"links":{"cited_paper":"/paper/1902.04029","citing_paper":"/paper/2511.04661"},"observation_digest":"sha256:87498303f34fb9f97978ca404341dfdcc1c4cfb1bee54799d55eb20231032657","observation_id":"7dc31a25-11a2-404a-8850-9cacc5dccd20","resolution":{"observed_at":"2026-08-03T23:41:00.474366Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"1902.04029","last_updated":"2019-11-23T12:20:25Z","snapshot_observed_at":"2026-08-14T17:17:58.396509Z","submitted_at":"2019-02-11T18:11:13Z","title":"Quantifying tensions in cosmological parameters: Interpreting the DES evidence ratio","version":5},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"1902.04029","snapshot_observed_at":"2026-08-03T18:51:47.098949Z","title":"Handley and P","venue":null,"work_id":null,"year":2019},"citing_paper":{"arxiv_id":"2512.04130","last_updated":"2026-07-26T05:14:02Z","snapshot_observed_at":"2026-08-09T18:20:38.058807Z","submitted_at":"2025-12-03T06:33:55Z","title":"Controlled Tension Forecasting: Quantifying Cross-Probe Biases in $\\omega_0\\omega_a$CDM","version":2},"reference_index":88,"source":"pdf_text","source_observed_at":"2026-08-03T18:51:47.098949Z"},"links":{"cited_paper":"/paper/1902.04029","citing_paper":"/paper/2512.04130"},"observation_digest":"sha256:69c909b14caa03b7bbb53fd2a4fc81a06eefc3814a50c2d0a5ad2f0038a60ad8","observation_id":"cced95be-4749-4e0f-b454-220f0541a4ce","resolution":{"observed_at":"2026-08-03T18:51:47.098949Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"1902.04029","last_updated":"2019-11-23T12:20:25Z","snapshot_observed_at":"2026-08-14T17:17:58.396509Z","submitted_at":"2019-02-11T18:11:13Z","title":"Quantifying tensions in cosmological parameters: Interpreting the DES evidence ratio","version":5},"cited_work":{"arxiv_id":"1902.04029","doi":null,"metadata_source":"arxiv_reference","pith_arxiv_id":"1902.04029","snapshot_observed_at":"2026-07-02T14:57:04.118144Z","title":"Handley and P","venue":null,"work_id":"4c47107e-900f-4b84-8036-6b72053ac13d","year":2019},"citing_paper":{"arxiv_id":"2603.05472","last_updated":"2026-05-15T16:45:14Z","snapshot_observed_at":"2026-08-14T08:04:08.566813Z","submitted_at":"2026-03-05T18:43:27Z","title":"The Bayesian view of DESI DR2 with unimpeded: Evidence and tension in a combined analysis with CMB and supernovae across cosmological models","version":2},"reference_index":19,"source":"pdf_text","source_observed_at":"2026-05-21T11:30:45.991122Z"},"links":{"cited_paper":"/paper/1902.04029","citing_paper":"/paper/2603.05472"},"observation_digest":"sha256:d53d61eb7e4bd34617b89f6454907ce7944b38f839ea534ff9303ff215a4e8ec","observation_id":"4cac7ea3-8324-45f9-838b-9a1b04665a80","resolution":{"observed_at":"2026-05-21T11:34:09.240572Z","resolver_source":"arxiv_id","status":"verified_exact"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-23T06:30:58.430688+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-23T06:30:58.430688+00:00","source":"crossref"},{"observed_at":"2026-08-23T06:30:53.778098+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":{"arxiv_id":"1902.04029","last_updated":"2019-11-23T12:20:25Z","snapshot_observed_at":"2026-08-14T17:17:58.396509Z","submitted_at":"2019-02-11T18:11:13Z","title":"Quantifying tensions in cosmological parameters: Interpreting the DES evidence ratio","version":5},"cited_work":{"arxiv_id":"1902.04029","doi":null,"metadata_source":"arxiv_reference","pith_arxiv_id":"1902.04029","snapshot_observed_at":"2026-07-02T14:57:04.118144Z","title":"Handley and P","venue":null,"work_id":"4c47107e-900f-4b84-8036-6b72053ac13d","year":2019},"citing_paper":{"arxiv_id":"2604.03756","last_updated":"2026-04-07T02:58:46Z","snapshot_observed_at":"2026-08-20T18:25:14.136901Z","submitted_at":"2026-04-04T15:05:07Z","title":"Is the $w_0w_a$CDM cosmological parameterization evidence for dark energy dynamics partially caused by the excess smoothing of Planck PR4 CMB anisotropy data?","version":2},"reference_index":88,"source":"pdf_text","source_observed_at":"2026-05-13T17:33:08.222231Z"},"links":{"cited_paper":"/paper/1902.04029","citing_paper":"/paper/2604.03756"},"observation_digest":"sha256:656754b90f74819d8f61a2d3e2ea91316f5c2a6c7403f5c793354d3b62fc83c2","observation_id":"859f2640-2b31-42f1-871c-1bbea4cda310","resolution":{"observed_at":"2026-05-13T17:38:03.163086Z","resolver_source":"arxiv_id","status":"verified_exact"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-23T06:30:58.430688+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-23T06:30:58.430688+00:00","source":"crossref"},{"observed_at":"2026-08-23T06:30:53.778098+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":{"arxiv_id":"1902.04029","last_updated":"2019-11-23T12:20:25Z","snapshot_observed_at":"2026-08-14T17:17:58.396509Z","submitted_at":"2019-02-11T18:11:13Z","title":"Quantifying tensions in cosmological parameters: Interpreting the DES evidence ratio","version":5},"cited_work":{"arxiv_id":"1902.04029","doi":null,"metadata_source":"arxiv_reference","pith_arxiv_id":"1902.04029","snapshot_observed_at":"2026-07-02T14:57:04.118144Z","title":"Handley and P","venue":null,"work_id":"4c47107e-900f-4b84-8036-6b72053ac13d","year":2019},"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":19,"source":"pdf_text","source_observed_at":"2026-05-10T15:10:48.528283Z"},"links":{"cited_paper":"/paper/1902.04029","citing_paper":"/paper/2604.11694"},"observation_digest":"sha256:9b0eb52de3401bc424a0e5a5e9f738b12bdf39e6b80a91f671c3196edc9dec89","observation_id":"eaae04d1-5fba-4832-b1d2-bef50814ee0b","resolution":{"observed_at":"2026-05-11T11:01:24.488356Z","resolver_source":"arxiv_id","status":"verified_exact"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-23T06:30:58.430688+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-23T06:30:58.430688+00:00","source":"crossref"},{"observed_at":"2026-08-23T06:30:53.778098+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":{"arxiv_id":"1902.04029","last_updated":"2019-11-23T12:20:25Z","snapshot_observed_at":"2026-08-14T17:17:58.396509Z","submitted_at":"2019-02-11T18:11:13Z","title":"Quantifying tensions in cosmological parameters: Interpreting the DES evidence ratio","version":5},"cited_work":{"arxiv_id":"1902.04029","doi":null,"metadata_source":"arxiv_reference","pith_arxiv_id":"1902.04029","snapshot_observed_at":"2026-07-02T14:57:04.118144Z","title":"Handley and P","venue":null,"work_id":"4c47107e-900f-4b84-8036-6b72053ac13d","year":2019},"citing_paper":{"arxiv_id":"2606.05853","last_updated":"2026-06-04T08:27:25Z","snapshot_observed_at":"2026-08-01T21:34:07.002669Z","submitted_at":"2026-06-04T08:27:25Z","title":"Reconstructing dark energy with fewer assumptions","version":1},"reference_index":125,"source":"pdf_text","source_observed_at":"2026-06-28T00:07:32.911711Z"},"links":{"cited_paper":"/paper/1902.04029","citing_paper":"/paper/2606.05853"},"observation_digest":"sha256:5fd5e9028ce6ec1c529c8670dc0e71fa4b94a24dffd116cfa79732277e3a5da3","observation_id":"9c0ec042-9ed2-440d-b3f4-0be144cd8706","resolution":{"observed_at":"2026-07-02T14:57:04.119751Z","resolver_source":"arxiv_id","status":"verified_exact"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-23T06:30:58.430688+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-23T06:30:58.430688+00:00","source":"crossref"},{"observed_at":"2026-08-23T06:30:53.778098+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":{"arxiv_id":"1902.04029","last_updated":"2019-11-23T12:20:25Z","snapshot_observed_at":"2026-08-14T17:17:58.396509Z","submitted_at":"2019-02-11T18:11:13Z","title":"Quantifying tensions in cosmological parameters: Interpreting the DES evidence ratio","version":5},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"1902.04029","snapshot_observed_at":"2026-08-01T07:20:07.584501Z","title":"Quantifying tensions in cosmological parameters: Interpreting the DES evidence ratio,","venue":null,"work_id":null,"year":2019},"citing_paper":{"arxiv_id":"2607.21497","last_updated":"2026-08-14T16:46:31Z","snapshot_observed_at":"2026-08-19T23:10:52.542376Z","submitted_at":"2026-07-23T16:45:10Z","title":"Hubble tension: a short review of theoretical explanations","version":1},"reference_index":41,"source":"pdf_text","source_observed_at":"2026-08-01T07:20:07.584501Z"},"links":{"cited_paper":"/paper/1902.04029","citing_paper":"/paper/2607.21497"},"observation_digest":"sha256:053c2743e73644789ce578252d2f1590422ff1d25b8b2a5f5fab9bdf0efbe213","observation_id":"79b293e9-86b8-41f6-b592-4fe315812fc4","resolution":{"observed_at":"2026-08-01T07:20:07.584501Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}}],"links":{"evidence":"/evidence","html":"/paper/1902.04029/citation-record","integrity":"/paper/1902.04029/integrity","json":"/paper/1902.04029/citation-record.json","paper":"/paper/1902.04029"},"outbound":[],"paper":{"arxiv_id":"1902.04029","last_updated":"2019-11-23T12:20:25Z","latest_version":5,"primary_category":"astro-ph.CO","snapshot_observed_at":"2026-08-14T17:17:58.396509Z","submitted_at":"2019-02-11T18:11:13Z","title":"Quantifying tensions in cosmological parameters: Interpreting the DES evidence ratio"},"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":"2026-08-23T06:30:58.430688+00:00","source":"crossref"},{"observed_at":"2026-08-23T06:30:53.778098+00:00","source":"retraction_watch"}],"thesis":"As of 23 August 2026, this Paper Citation Record lists 0 of 0 outbound references and 13 inbound Pith citation observations for arXiv:1902.04029."}