{"as_of":"2026-08-17T20:10:00Z","caps":{"database_statements":6,"inbound":100,"outbound":100},"context_digest":"sha256:276573d972f96515e856efe7f9f3d8bde400b9048ee5855af07084a266919c1e","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":4,"lane":"standing_notices","note":"One-hop event checks from named stored sources.","records_observed":4,"source":"scholarly_work_events, retraction_status_cache","source_observed_at":"2026-08-17T06:30:58.91139+00:00","state":"measured"},{"denominator":4,"lane":"inbound_itemization","note":"Pith citing papers itemized under the disclosed page cap.","records_observed":4,"source":"paper_references, paper_reference_links","source_observed_at":"2026-08-16T11:38:47.373448Z","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":"2026-05-19T01:36:58.086294Z","state":"measured"}],"external_citation_measurements":[],"inbound":[{"citation":{"cited_paper":{"arxiv_id":"1412.6501","last_updated":"2014-12-19T19:49:17Z","snapshot_observed_at":"2026-08-14T23:06:43.278738Z","submitted_at":"2014-12-19T19:49:17Z","title":"Confirmation of a Star Formation Bias in Type Ia Supernova Distances and its Effect on Measurement of the Hubble Constant","version":1},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"1412.6501","snapshot_observed_at":"2026-08-14T12:34:56.806158Z","title":"Rigault et al","venue":null,"work_id":null,"year":2015},"citing_paper":{"arxiv_id":"1908.06995","last_updated":"2019-08-19T18:00:08Z","snapshot_observed_at":"2026-08-17T06:03:23.038237Z","submitted_at":"2019-08-19T18:00:08Z","title":"Oscillating scalar fields and the Hubble tension: a resolution with novel signatures","version":1},"reference_index":27,"source":"pdf_text","source_observed_at":"2026-08-14T12:34:56.806158Z"},"links":{"cited_paper":"/paper/1412.6501","citing_paper":"/paper/1908.06995"},"observation_digest":"sha256:8347b34eb8709482dc11dbb758441c0a2fd9d2be97262d31f29c1ca311ff289a","observation_id":"5d61c654-eda0-4334-b0ad-d40a7a54a673","resolution":{"observed_at":"2026-08-14T12:34:56.806158Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"1412.6501","last_updated":"2014-12-19T19:49:17Z","snapshot_observed_at":"2026-08-14T23:06:43.278738Z","submitted_at":"2014-12-19T19:49:17Z","title":"Confirmation of a Star Formation Bias in Type Ia Supernova Distances and its Effect on Measurement of the Hubble Constant","version":1},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"1412.6501","snapshot_observed_at":"2026-08-09T11:42:48.595509Z","title":"Rigault, G","venue":null,"work_id":null,"year":2015},"citing_paper":{"arxiv_id":"2502.02638","last_updated":"2025-06-03T17:12:21Z","snapshot_observed_at":"2026-08-12T15:12:46.310398Z","submitted_at":"2025-02-04T19:00:01Z","title":"An Alcock-Paczynski Test on Reionization Bubbles for Cosmology","version":2},"reference_index":12,"source":"pdf_text","source_observed_at":"2026-08-09T11:42:48.595509Z"},"links":{"cited_paper":"/paper/1412.6501","citing_paper":"/paper/2502.02638"},"observation_digest":"sha256:14764b075235e87730fb5ffa68fb405d0487dba0a23685b8ebfd90df928fed6e","observation_id":"70f01e94-25ac-4e22-9768-ec3fa6a4df83","resolution":{"observed_at":"2026-08-09T11:42:48.595509Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"1412.6501","last_updated":"2014-12-19T19:49:17Z","snapshot_observed_at":"2026-08-14T23:06:43.278738Z","submitted_at":"2014-12-19T19:49:17Z","title":"Confirmation of a Star Formation Bias in Type Ia Supernova Distances and its Effect on Measurement of the Hubble Constant","version":1},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"1412.6501","snapshot_observed_at":"2026-08-16T11:38:47.373448Z","title":"Rigault et al","venue":null,"work_id":null,"year":2015},"citing_paper":{"arxiv_id":"2504.15127","last_updated":"2025-07-12T01:39:19Z","snapshot_observed_at":"2026-08-16T18:33:40.770191Z","submitted_at":"2025-04-21T14:22:41Z","title":"Reconstructing the redshift evolution of Type Ia supernovae absolute magnitude","version":2},"reference_index":19,"source":"pdf_text","source_observed_at":"2026-08-16T11:38:47.373448Z"},"links":{"cited_paper":"/paper/1412.6501","citing_paper":"/paper/2504.15127"},"observation_digest":"sha256:11fe584aaf7a981f70a4be7451fe22e25cddb1ac3b8b7afcbcfb33e89480380f","observation_id":"559cc501-945a-4420-9a33-134ddede335d","resolution":{"observed_at":"2026-08-16T11:38:47.373448Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"1412.6501","last_updated":"2014-12-19T19:49:17Z","snapshot_observed_at":"2026-08-14T23:06:43.278738Z","submitted_at":"2014-12-19T19:49:17Z","title":"Confirmation of a Star Formation Bias in Type Ia Supernova Distances and its Effect on Measurement of the Hubble Constant","version":1},"cited_work":{"arxiv_id":"1412.6501","doi":null,"metadata_source":"arxiv_reference","pith_arxiv_id":"1412.6501","snapshot_observed_at":"2026-06-05T21:23:00.469572Z","title":"Confirmation of a Star Formation Bias in Type Ia Supernova Distances and its Effect on Measurement of the Hubble Constant","venue":null,"work_id":"d1d5f475-22a2-42db-bc39-71fceb1ab134","year":2015},"citing_paper":{"arxiv_id":"2508.01759","last_updated":"2026-04-28T15:04:32Z","snapshot_observed_at":"2026-07-06T22:07:02.782730Z","submitted_at":"2025-08-03T14:00:54Z","title":"Resolving the Planck-DESI tension by nonminimally coupled quintessence","version":5},"reference_index":84,"source":"pdf_text","source_observed_at":"2026-05-19T01:35:36.430109Z"},"links":{"cited_paper":"/paper/1412.6501","citing_paper":"/paper/2508.01759"},"observation_digest":"sha256:5853b97ea82e30ae1dc207ea862ea4b1f83051d29664ffd2052ac8ccf903fb10","observation_id":"de61ff83-c1e9-4a55-8c41-7e88aaf20173","resolution":{"observed_at":"2026-05-19T01:36:58.089330Z","resolver_source":"arxiv_id","status":"verified_exact"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-17T06:30:58.91139+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-17T06:30:58.91139+00:00","source":"crossref"},{"observed_at":"2026-08-17T06:30:54.323127+00:00","source":"retraction_watch"}],"state":"measured"}}],"links":{"evidence":"/evidence","html":"/paper/1412.6501/citation-record","integrity":"/paper/1412.6501/integrity","json":"/paper/1412.6501/citation-record.json","paper":"/paper/1412.6501"},"outbound":[],"paper":{"arxiv_id":"1412.6501","last_updated":"2014-12-19T19:49:17Z","latest_version":1,"primary_category":"astro-ph.CO","snapshot_observed_at":"2026-08-14T23:06:43.278738Z","submitted_at":"2014-12-19T19:49:17Z","title":"Confirmation of a Star Formation Bias in Type Ia Supernova Distances and its Effect on Measurement of the Hubble Constant"},"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":"2026-08-17T06:30:58.91139+00:00","source":"crossref"},{"observed_at":"2026-08-17T06:30:54.323127+00:00","source":"retraction_watch"}],"thesis":"As of 17 August 2026, this Paper Citation Record lists 0 of 0 outbound references and 4 inbound Pith citation observations for arXiv:1412.6501."}