{"as_of":"2026-08-18T05:14:00Z","caps":{"database_statements":6,"inbound":100,"outbound":100},"context_digest":"sha256:58564738f75b60fec405956c23e74eddadc8f6d698b3694a4a699a7af4a3d1d9","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":"2026-08-10T17:56:50.972628Z","state":"measured"},{"denominator":1,"lane":"external_citation_measurements","note":"A source-named dated measurement, never combined with another source.","records_observed":0,"source":"pith","source_observed_at":"2026-08-10T14:51:56.681165Z","state":"measured"}],"external_citation_measurements":[],"inbound":[{"citation":{"cited_paper":{"arxiv_id":"2211.10785","last_updated":"2023-01-28T15:24:00Z","snapshot_observed_at":"2026-08-16T16:14:51.574436Z","submitted_at":"2022-11-19T19:54:20Z","title":"A bias-free cosmological analysis with quasars alleviating $H_0$ tension","version":3},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2211.10785","snapshot_observed_at":"2026-08-10T17:56:50.972628Z","title":"The Astrophysical Journals 264, 46","venue":null,"work_id":null,"year":null},"citing_paper":{"arxiv_id":"2501.11772","last_updated":"2025-06-04T15:38:07Z","snapshot_observed_at":"2026-08-16T19:07:20.514901Z","submitted_at":"2025-01-20T22:31:05Z","title":"A New Master Supernovae Ia sample and the investigation of the $H_0$ tension","version":5},"reference_index":17,"source":"pdf_text","source_observed_at":"2026-08-10T17:56:50.972628Z"},"links":{"cited_paper":"/paper/2211.10785","citing_paper":"/paper/2501.11772"},"observation_digest":"sha256:8e5a487242d971e46285110403e9583fbecd63bae1f50f14739ed16a548574af","observation_id":"13924bc3-a93d-4cfc-b93b-177c6249cc13","resolution":{"observed_at":"2026-08-10T17:56:50.972628Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2211.10785","last_updated":"2023-01-28T15:24:00Z","snapshot_observed_at":"2026-08-16T16:14:51.574436Z","submitted_at":"2022-11-19T19:54:20Z","title":"A bias-free cosmological analysis with quasars alleviating $H_0$ tension","version":3},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2211.10785","snapshot_observed_at":"2026-08-10T16:31:22.140633Z","title":"ABias-freeCosmologicalAnalysiswithQuasarsAlleviating H 0 Tension","venue":null,"work_id":null,"year":2023},"citing_paper":{"arxiv_id":"2501.13102","last_updated":"2025-01-22T18:57:36Z","snapshot_observed_at":"2026-08-17T14:34:26.561925Z","submitted_at":"2025-01-22T18:57:36Z","title":"The Machine Learning to reconstruct GRB lightcurves","version":1},"reference_index":20,"source":"pdf_text","source_observed_at":"2026-08-10T16:31:22.140633Z"},"links":{"cited_paper":"/paper/2211.10785","citing_paper":"/paper/2501.13102"},"observation_digest":"sha256:e659a09f2400179951e888be1b3c1a1929c9e092e25cd26db6ade9c3625c4813","observation_id":"5a395034-1665-43e8-8725-e81ca265e92b","resolution":{"observed_at":"2026-08-10T16:31:22.140633Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2211.10785","last_updated":"2023-01-28T15:24:00Z","snapshot_observed_at":"2026-08-16T16:14:51.574436Z","submitted_at":"2022-11-19T19:54:20Z","title":"A bias-free cosmological analysis with quasars alleviating $H_0$ tension","version":3},"cited_work":{"arxiv_id":"2211.10785","doi":null,"metadata_source":"pith","pith_arxiv_id":"2211.10785","snapshot_observed_at":"2026-08-10T14:51:56.681165Z","title":"A bias-free cosmological analysis with quasars alleviating $H_0$ tension","venue":"astro-ph.CO","work_id":"22842f28-ce73-4e73-b22e-bf474fba58dc","year":2022},"citing_paper":{"arxiv_id":"2501.14944","last_updated":"2025-01-24T22:08:02Z","snapshot_observed_at":"2026-08-15T04:39:41.443704Z","submitted_at":"2025-01-24T22:08:02Z","title":"Supernovae Ia, high-redshift probes, and the Hubble tension: current status and future perspectives","version":1},"reference_index":16,"source":"pdf_text","source_observed_at":"2026-08-10T14:51:56.080208Z"},"links":{"cited_paper":"/paper/2211.10785","citing_paper":"/paper/2501.14944"},"observation_digest":"sha256:87937dbe9ceba0164bcee8b2f4d185f8b9f407cf210273838e860e4e9f6577d0","observation_id":"61b51bb2-58ee-467a-8782-28d5f693808d","resolution":{"observed_at":"2026-08-10T14:51:56.685151Z","resolver_source":"local_arxiv","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"}},{"citation":{"cited_paper":{"arxiv_id":"2211.10785","last_updated":"2023-01-28T15:24:00Z","snapshot_observed_at":"2026-08-16T16:14:51.574436Z","submitted_at":"2022-11-19T19:54:20Z","title":"A bias-free cosmological analysis with quasars alleviating $H_0$ tension","version":3},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2211.10785","snapshot_observed_at":"2026-07-14T16:44:02.461654Z","title":null,"venue":null,"work_id":null,"year":2023},"citing_paper":{"arxiv_id":"2607.09732","last_updated":"2026-07-02T07:56:02Z","snapshot_observed_at":"2026-08-15T03:20:30.109454Z","submitted_at":"2026-07-02T07:56:02Z","title":"Late-time cosmological constraints on three holographic dark energy models with DESI DR2 BAO and Type Ia supernovae","version":1},"reference_index":21,"source":"pdf_text","source_observed_at":"2026-07-14T16:44:02.461654Z"},"links":{"cited_paper":"/paper/2211.10785","citing_paper":"/paper/2607.09732"},"observation_digest":"sha256:0ae77ea174cd27f90a6f3f3505e5ad7c9fca5065449fef6ae8f3e6d095c46feb","observation_id":"9366eeda-9907-4591-8830-65c8fdbe19d2","resolution":{"observed_at":"2026-07-14T16:44:02.461654Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}}],"links":{"evidence":"/evidence","html":"/paper/2211.10785/citation-record","integrity":"/paper/2211.10785/integrity","json":"/paper/2211.10785/citation-record.json","paper":"/paper/2211.10785"},"outbound":[],"paper":{"arxiv_id":"2211.10785","last_updated":"2023-01-28T15:24:00Z","latest_version":3,"primary_category":"astro-ph.CO","snapshot_observed_at":"2026-08-16T16:14:51.574436Z","submitted_at":"2022-11-19T19:54:20Z","title":"A bias-free cosmological analysis with quasars alleviating $H_0$ tension"},"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 18 August 2026, this Paper Citation Record lists 0 of 0 outbound references and 4 inbound Pith citation observations for arXiv:2211.10785."}