{"as_of":"2026-08-15T08:41:00Z","caps":{"database_statements":6,"inbound":100,"outbound":100},"context_digest":"sha256:346e57edbed06a5bc4a6e0a70fc9ad5818cb65d72eb643d3cb4fa1a5e3f4c319","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":6,"lane":"standing_notices","note":"One-hop event checks from named stored sources.","records_observed":6,"source":"scholarly_work_events, retraction_status_cache","source_observed_at":"2026-08-15T06:32:42.880941+00:00","state":"measured"},{"denominator":6,"lane":"inbound_itemization","note":"Pith citing papers itemized under the disclosed page cap.","records_observed":6,"source":"paper_references, paper_reference_links","source_observed_at":"2026-08-14T14:40:46.872936Z","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":"2026-08-14T10:35:40.747342Z","state":"measured"}],"external_citation_measurements":[],"inbound":[{"citation":{"cited_paper":{"arxiv_id":"1905.12496","last_updated":"2019-07-31T17:06:38Z","snapshot_observed_at":"2026-08-14T17:48:59.524747Z","submitted_at":"2019-05-29T14:30:18Z","title":"The Hubble Constant determined through an inverse distance ladder including quasar time delays and Type Ia supernovae","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"1905.12496","snapshot_observed_at":"2026-08-14T14:40:46.872936Z","title":"H., Komatsu E., 2019, arXiv:1905.12496","venue":null,"work_id":null,"year":2019},"citing_paper":{"arxiv_id":"1908.02892","last_updated":"2019-08-08T00:56:02Z","snapshot_observed_at":"2026-08-15T06:20:59.681299Z","submitted_at":"2019-08-08T00:56:02Z","title":"Measuring the distances to quasars at high redshifts with strong lensing","version":1},"reference_index":53,"source":"arxiv_source","source_observed_at":"2026-08-14T14:40:46.872936Z"},"links":{"cited_paper":"/paper/1905.12496","citing_paper":"/paper/1908.02892"},"observation_digest":"sha256:69d3e812b3bacefc6775e2b589598aaf80bf9b1c4a736f2075b61c79161e7678","observation_id":"09f07f62-d4b3-4ccf-af8c-2558f03e9215","resolution":{"observed_at":"2026-08-14T14:40:46.872936Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"1905.12496","last_updated":"2019-07-31T17:06:38Z","snapshot_observed_at":"2026-08-14T17:48:59.524747Z","submitted_at":"2019-05-29T14:30:18Z","title":"The Hubble Constant determined through an inverse distance ladder including quasar time delays and Type Ia supernovae","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"1905.12496","snapshot_observed_at":"2026-08-14T13:02:33.771776Z","title":"The Hubble Constant de- termined through an inverse distance ladder includ- ing quasar time delays and Type Ia supernovae,","venue":null,"work_id":null,"year":1905},"citing_paper":{"arxiv_id":"1908.06100","last_updated":"2019-08-16T18:00:01Z","snapshot_observed_at":"2026-08-15T08:28:43.374570Z","submitted_at":"2019-08-16T18:00:01Z","title":"Gravitational waves, CMB polarization, and the Hubble tension","version":1},"reference_index":16,"source":"pdf_text","source_observed_at":"2026-08-14T13:02:33.771776Z"},"links":{"cited_paper":"/paper/1905.12496","citing_paper":"/paper/1908.06100"},"observation_digest":"sha256:e7cf639cae050bf90e1d1c9e1fe4b14582060e412b4d69db1dd639d1d56510a0","observation_id":"d774dced-0ceb-4913-b315-5c03f89c1568","resolution":{"observed_at":"2026-08-14T13:02:33.771776Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"1905.12496","last_updated":"2019-07-31T17:06:38Z","snapshot_observed_at":"2026-08-14T17:48:59.524747Z","submitted_at":"2019-05-29T14:30:18Z","title":"The Hubble Constant determined through an inverse distance ladder including quasar time delays and Type Ia supernovae","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"1905.12496","snapshot_observed_at":"2026-08-14T12:34:56.825836Z","title":"Taubenberger, S","venue":null,"work_id":null,"year":2019},"citing_paper":{"arxiv_id":"1908.06995","last_updated":"2019-08-19T18:00:08Z","snapshot_observed_at":"2026-08-14T13:36:29.463344Z","submitted_at":"2019-08-19T18:00:08Z","title":"Oscillating scalar fields and the Hubble tension: a resolution with novel signatures","version":1},"reference_index":32,"source":"pdf_text","source_observed_at":"2026-08-14T12:34:56.825836Z"},"links":{"cited_paper":"/paper/1905.12496","citing_paper":"/paper/1908.06995"},"observation_digest":"sha256:22f3d5a29cc11f1ea70b029e517e58e208b46f422e9b8bb9be165f137ef6b766","observation_id":"416878ba-2cac-488d-b0f9-1614191bf4de","resolution":{"observed_at":"2026-08-14T12:34:56.825836Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"1905.12496","last_updated":"2019-07-31T17:06:38Z","snapshot_observed_at":"2026-08-14T17:48:59.524747Z","submitted_at":"2019-05-29T14:30:18Z","title":"The Hubble Constant determined through an inverse distance ladder including quasar time delays and Type Ia supernovae","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"1905.12496","snapshot_observed_at":"2026-08-14T11:06:35.467418Z","title":"The Hubble Constant determined through an inverse distance ladder including quasar time delays and Type Ia supernovae,","venue":null,"work_id":null,"year":2019},"citing_paper":{"arxiv_id":"1908.09843","last_updated":"2021-01-10T05:49:45Z","snapshot_observed_at":"2026-08-15T06:23:54.389541Z","submitted_at":"2019-08-26T18:00:03Z","title":"Dark Neutrino interactions phase out the Hubble tension","version":2},"reference_index":62,"source":"pdf_text","source_observed_at":"2026-08-14T11:06:35.467418Z"},"links":{"cited_paper":"/paper/1905.12496","citing_paper":"/paper/1908.09843"},"observation_digest":"sha256:b489ba6da58083dde88d70aafc457aeaacca364689c28b11eb1ad6b13d6b1ede","observation_id":"d006316f-5c3d-40df-ae1e-628113f386d8","resolution":{"observed_at":"2026-08-14T11:06:35.467418Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"1905.12496","last_updated":"2019-07-31T17:06:38Z","snapshot_observed_at":"2026-08-14T17:48:59.524747Z","submitted_at":"2019-05-29T14:30:18Z","title":"The Hubble Constant determined through an inverse distance ladder including quasar time delays and Type Ia supernovae","version":2},"cited_work":{"arxiv_id":"1905.12496","doi":null,"metadata_source":"pith","pith_arxiv_id":"1905.12496","snapshot_observed_at":"2026-08-14T10:35:40.747342Z","title":"The Hubble Constant determined through an inverse distance ladder including quasar time delays and Type Ia supernovae","venue":"astro-ph.CO","work_id":"214cfc11-be2b-485c-b4c1-c89f19fbf42f","year":2019},"citing_paper":{"arxiv_id":"1908.10883","last_updated":"2019-12-03T17:02:47Z","snapshot_observed_at":"2026-08-14T21:44:41.148873Z","submitted_at":"2019-08-28T18:01:02Z","title":"Hubble Space Telescope Observations of Mira Variables in the Type Ia Supernova Host NGC 1559: An Alternative Candle to Measure the Hubble Constant","version":2},"reference_index":43,"source":"pdf_text","source_observed_at":"2026-08-14T10:35:40.629651Z"},"links":{"cited_paper":"/paper/1905.12496","citing_paper":"/paper/1908.10883"},"observation_digest":"sha256:48457a87ce2c6a621387466f2f1ed11b3e5979cdd190828b9f33a8b46187b0c9","observation_id":"d7edd418-c520-48a5-99d7-e8ab139649d7","resolution":{"observed_at":"2026-08-14T10:35:40.751208Z","resolver_source":"local_arxiv","status":"metadata_mismatch"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-15T06:32:42.880941+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-15T06:32:42.880941+00:00","source":"crossref"},{"observed_at":"2026-08-15T06:32:39.529945+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":{"arxiv_id":"1905.12496","last_updated":"2019-07-31T17:06:38Z","snapshot_observed_at":"2026-08-14T17:48:59.524747Z","submitted_at":"2019-05-29T14:30:18Z","title":"The Hubble Constant determined through an inverse distance ladder including quasar time delays and Type Ia supernovae","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"1905.12496","snapshot_observed_at":"2026-08-04T07:19:40.034813Z","title":"Taubenberger, S","venue":null,"work_id":null,"year":2019},"citing_paper":{"arxiv_id":"2510.26355","last_updated":"2026-07-07T01:20:38Z","snapshot_observed_at":"2026-08-12T22:27:53.420894Z","submitted_at":"2025-10-30T11:06:11Z","title":"Model-independent late-universe measurements of $H_0$ and $\\Omega_K$ with the parametrization based on cosmic age-improved inverse distance ladder","version":2},"reference_index":70,"source":"pdf_text","source_observed_at":"2026-08-04T07:19:40.034813Z"},"links":{"cited_paper":"/paper/1905.12496","citing_paper":"/paper/2510.26355"},"observation_digest":"sha256:1cb3dca2f75cb8c9117b4a645c0f171406f0e9ed6a78b274ac146bdaefeac8bf","observation_id":"239889a8-f311-4874-abf5-838db4750679","resolution":{"observed_at":"2026-08-04T07:19:40.034813Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}}],"links":{"evidence":"/evidence","html":"/paper/1905.12496/citation-record","integrity":"/paper/1905.12496/integrity","json":"/paper/1905.12496/citation-record.json","paper":"/paper/1905.12496"},"outbound":[],"paper":{"arxiv_id":"1905.12496","last_updated":"2019-07-31T17:06:38Z","latest_version":2,"primary_category":"astro-ph.CO","snapshot_observed_at":"2026-08-14T17:48:59.524747Z","submitted_at":"2019-05-29T14:30:18Z","title":"The Hubble Constant determined through an inverse distance ladder including quasar time delays and Type Ia supernovae"},"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":"2026-08-15T06:32:42.880941+00:00","source":"crossref"},{"observed_at":"2026-08-15T06:32:39.529945+00:00","source":"retraction_watch"}],"thesis":"As of 15 August 2026, this Paper Citation Record lists 0 of 0 outbound references and 6 inbound Pith citation observations for arXiv:1905.12496."}