{"as_of":"2026-08-12T21:06:00Z","caps":{"database_statements":6,"inbound":100,"outbound":100},"context_digest":"sha256:bd405e666d7453312653b3b55d3848ad4e57184f58677bdc4ade13764bff4bca","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":"2026-08-12T06:34:41.77262+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":"2026-08-12T12:56:44.825674Z","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":"2026-05-17T23:41:11.327412Z","state":"measured"}],"external_citation_measurements":[],"inbound":[{"citation":{"cited_paper":{"arxiv_id":"2208.01045","last_updated":"2022-08-01T18:00:01Z","snapshot_observed_at":"2026-08-12T13:04:03.754413Z","submitted_at":"2022-08-01T18:00:01Z","title":"Cluster Cepheids with High Precision Gaia Parallaxes, Low Zeropoint Uncertainties, and Hubble Space Telescope Photometry","version":1},"cited_work":{"arxiv_id":"2208.01045","doi":null,"metadata_source":"arxiv_reference","pith_arxiv_id":"2208.01045","snapshot_observed_at":"2026-06-05T21:23:00.469572Z","title":"Riess, Louise Breuval, Wenlong Yuan, Stefano Casertano, Lucas M","venue":null,"work_id":"cc1edf56-313f-40a0-ba1e-7586a417cbcf","year":2022},"citing_paper":{"arxiv_id":"2211.04492","last_updated":"2022-11-08T19:00:16Z","snapshot_observed_at":"2026-08-01T18:06:39.805867Z","submitted_at":"2022-11-08T19:00:16Z","title":"The Hubble Tension and Early Dark Energy","version":1},"reference_index":37,"source":"pdf_text","source_observed_at":"2026-05-17T23:41:11.040188Z"},"links":{"cited_paper":"/paper/2208.01045","citing_paper":"/paper/2211.04492"},"observation_digest":"sha256:73014481f2d33935899bbe737cf83fd64db9a34bd98366e161c91cee4650bc4f","observation_id":"f02d3ed3-26b6-42f3-aa3d-b1492516984e","resolution":{"observed_at":"2026-05-17T23:41:11.329696Z","resolver_source":"arxiv_id","status":"verified_exact"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-12T06:34:41.77262+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-12T06:34:41.77262+00:00","source":"crossref"},{"observed_at":"2026-08-12T06:34:36.333875+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":{"arxiv_id":"2208.01045","last_updated":"2022-08-01T18:00:01Z","snapshot_observed_at":"2026-08-12T13:04:03.754413Z","submitted_at":"2022-08-01T18:00:01Z","title":"Cluster Cepheids with High Precision Gaia Parallaxes, Low Zeropoint Uncertainties, and Hubble Space Telescope Photometry","version":1},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2208.01045","snapshot_observed_at":"2026-08-12T12:56:44.825674Z","title":null,"venue":null,"work_id":null,"year":2022},"citing_paper":{"arxiv_id":"2411.16678","last_updated":"2025-04-12T04:21:23Z","snapshot_observed_at":"2026-08-12T12:47:23.717721Z","submitted_at":"2024-11-25T18:59:23Z","title":"Modified recombination and the Hubble tension","version":2},"reference_index":7,"source":"pdf_text","source_observed_at":"2026-08-12T12:56:44.825674Z"},"links":{"cited_paper":"/paper/2208.01045","citing_paper":"/paper/2411.16678"},"observation_digest":"sha256:c59304ccfba3603eff4edb6ed0d20314b625e9d1858f410c6c71c806c5e097b9","observation_id":"c715b741-2cd5-409e-9a6c-ee619e2ac867","resolution":{"observed_at":"2026-08-12T12:56:44.825674Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2208.01045","last_updated":"2022-08-01T18:00:01Z","snapshot_observed_at":"2026-08-12T13:04:03.754413Z","submitted_at":"2022-08-01T18:00:01Z","title":"Cluster Cepheids with High Precision Gaia Parallaxes, Low Zeropoint Uncertainties, and Hubble Space Telescope Photometry","version":1},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2208.01045","snapshot_observed_at":"2026-08-11T12:50:11.722974Z","title":null,"venue":null,"work_id":null,"year":2022},"citing_paper":{"arxiv_id":"2412.13894","last_updated":"2025-04-23T12:33:02Z","snapshot_observed_at":"2026-08-12T07:34:04.991202Z","submitted_at":"2024-12-18T14:35:07Z","title":"Understanding acoustic scale observations: the one-sided fight against $\\Lambda$","version":3},"reference_index":23,"source":"pdf_text","source_observed_at":"2026-08-11T12:50:11.722974Z"},"links":{"cited_paper":"/paper/2208.01045","citing_paper":"/paper/2412.13894"},"observation_digest":"sha256:216d0fd225a48db98cfb2295188987029f3f326c94fb95f85067ab876a172804","observation_id":"08fb2605-3de8-446f-9a43-b357e4bd9de3","resolution":{"observed_at":"2026-08-11T12:50:11.722974Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2208.01045","last_updated":"2022-08-01T18:00:01Z","snapshot_observed_at":"2026-08-12T13:04:03.754413Z","submitted_at":"2022-08-01T18:00:01Z","title":"Cluster Cepheids with High Precision Gaia Parallaxes, Low Zeropoint Uncertainties, and Hubble Space Telescope Photometry","version":1},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2208.01045","snapshot_observed_at":"2026-08-02T03:06:04.233612Z","title":", keywords =","venue":null,"work_id":null,"year":null},"citing_paper":{"arxiv_id":"2607.14007","last_updated":"2026-07-15T16:37:06Z","snapshot_observed_at":"2026-08-09T17:58:29.385586Z","submitted_at":"2026-07-15T16:37:06Z","title":"The potential broader complex linked to the key Cepheid SV Vul","version":1},"reference_index":65,"source":"arxiv_source","source_observed_at":"2026-08-02T03:06:04.233612Z"},"links":{"cited_paper":"/paper/2208.01045","citing_paper":"/paper/2607.14007"},"observation_digest":"sha256:9805a12074506d740c2e162d0ae915bf81851abc530b340022c4c83b12e08cfa","observation_id":"c22b1cae-90a5-439e-8d2a-3bf37029a9bb","resolution":{"observed_at":"2026-08-02T03:06:04.233612Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2208.01045","last_updated":"2022-08-01T18:00:01Z","snapshot_observed_at":"2026-08-12T13:04:03.754413Z","submitted_at":"2022-08-01T18:00:01Z","title":"Cluster Cepheids with High Precision Gaia Parallaxes, Low Zeropoint Uncertainties, and Hubble Space Telescope Photometry","version":1},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2208.01045","snapshot_observed_at":"2026-08-01T07:20:07.563108Z","title":"Cluster Cepheids with High Precision Gaia Parallaxes, Low Zero- point Uncertainties, and Hubble Space Telescope Photometry,","venue":null,"work_id":null,"year":2022},"citing_paper":{"arxiv_id":"2607.21497","last_updated":"2026-07-23T16:45:10Z","snapshot_observed_at":"2026-08-09T21:28:10.481411Z","submitted_at":"2026-07-23T16:45:10Z","title":"Hubble tension: a short review of theoretical explanations","version":1},"reference_index":35,"source":"pdf_text","source_observed_at":"2026-08-01T07:20:07.563108Z"},"links":{"cited_paper":"/paper/2208.01045","citing_paper":"/paper/2607.21497"},"observation_digest":"sha256:9310cb8aab23e1cc6d49453ab73701ff2b9cba0397db05b6cfaf9e1900cf2ca4","observation_id":"1b058cd0-ecfe-4406-80a1-c305aaaebd3d","resolution":{"observed_at":"2026-08-01T07:20:07.563108Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}}],"links":{"evidence":"/evidence","html":"/paper/2208.01045/citation-record","integrity":"/paper/2208.01045/integrity","json":"/paper/2208.01045/citation-record.json","paper":"/paper/2208.01045"},"outbound":[],"paper":{"arxiv_id":"2208.01045","last_updated":"2022-08-01T18:00:01Z","latest_version":1,"primary_category":"astro-ph.CO","snapshot_observed_at":"2026-08-12T13:04:03.754413Z","submitted_at":"2022-08-01T18:00:01Z","title":"Cluster Cepheids with High Precision Gaia Parallaxes, Low Zeropoint Uncertainties, and Hubble Space Telescope Photometry"},"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":"2026-08-12T06:34:41.77262+00:00","source":"crossref"},{"observed_at":"2026-08-12T06:34:36.333875+00:00","source":"retraction_watch"}],"thesis":"As of 12 August 2026, this Paper Citation Record lists 0 of 0 outbound references and 5 inbound Pith citation observations for arXiv:2208.01045."}