{"as_of":"2026-08-09T03:55:00Z","caps":{"database_statements":6,"inbound":100,"outbound":100},"context_digest":"sha256:497b387861f156a1d713278d497185f39aac0058534619f2640cfb692328a585","coverage":[{"denominator":50,"lane":"reference_resolution","note":"Typed states for the displayed outbound observations.","records_observed":50,"source":"paper_references, paper_reference_links","source_observed_at":"2026-08-06T23:21:56.064746Z","state":"measured"},{"denominator":50,"lane":"standing_notices","note":"One-hop event checks from named stored sources.","records_observed":50,"source":"scholarly_work_events, retraction_status_cache","source_observed_at":"2026-08-08T06:32:00.761636+00:00","state":"measured"},{"denominator":0,"lane":"inbound_itemization","note":"Pith citing papers itemized under the disclosed page cap.","records_observed":0,"source":"paper_references, paper_reference_links","source_observed_at":null,"state":"measured"},{"denominator":1,"lane":"external_citation_measurements","note":"A source-named dated measurement, never combined with another source.","records_observed":0,"source":"cited_works","source_observed_at":null,"state":"measured"}],"external_citation_measurements":[],"inbound":[],"links":{"evidence":"/evidence","html":"/paper/2506.18445/citation-record","integrity":"/paper/2506.18445/integrity","json":"/paper/2506.18445/citation-record.json","paper":"/paper/2506.18445"},"outbound":[{"citation":{"cited_paper":{"arxiv_id":"astro-ph/0207347","last_updated":"2002-11-20T20:31:52Z","snapshot_observed_at":"2026-07-07T00:27:27.276456Z","submitted_at":"2002-07-16T21:40:00Z","title":"The Cosmological Constant and Dark Energy","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"astro-ph/0207347","snapshot_observed_at":"2026-08-06T23:21:48.744746Z","title":null,"venue":null,"work_id":null,"year":2003},"citing_paper":{"arxiv_id":"2506.18445","last_updated":"2025-06-23T09:30:19Z","snapshot_observed_at":"2026-08-08T19:03:41.502084Z","submitted_at":"2025-06-23T09:30:19Z","title":"Comparison of $R_h=ct$ and $\\Lambda$CDM using DESI DR1 measurements","version":1},"reference_index":1,"source":"pdf_text","source_observed_at":"2026-08-06T23:21:48.744746Z"},"links":{"cited_paper":"/paper/astro-ph/0207347","citing_paper":"/paper/2506.18445"},"observation_digest":"sha256:c5eaa5c15ac71700befd4cf88d4050c9d08b5c816422759a5d18bcb4f4de4359","observation_id":"b37383a5-89af-416c-abdc-3eb5bc9893f2","resolution":{"observed_at":"2026-08-06T23:21:48.744746Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"1807.06209","last_updated":"2021-08-09T10:43:18Z","snapshot_observed_at":"2026-07-06T02:11:23.670680Z","submitted_at":"2018-07-17T04:05:07Z","title":"Planck 2018 results. VI. Cosmological parameters","version":4},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"1807.06209","snapshot_observed_at":"2026-08-06T23:21:48.954952Z","title":"Aghanim, Y","venue":null,"work_id":null,"year":2020},"citing_paper":{"arxiv_id":"2506.18445","last_updated":"2025-06-23T09:30:19Z","snapshot_observed_at":"2026-08-08T19:03:41.502084Z","submitted_at":"2025-06-23T09:30:19Z","title":"Comparison of $R_h=ct$ and $\\Lambda$CDM using DESI DR1 measurements","version":1},"reference_index":2,"source":"pdf_text","source_observed_at":"2026-08-06T23:21:48.954952Z"},"links":{"cited_paper":"/paper/1807.06209","citing_paper":"/paper/2506.18445"},"observation_digest":"sha256:6e72199ee40841ceba51c1f3a2600bbdd58ef18164e8edcef0cdeb70254cd2e2","observation_id":"6d1d8ba5-ead2-44d0-9dd0-9ba912dfe703","resolution":{"observed_at":"2026-08-06T23:21:48.954952Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2109.01161","last_updated":"2021-10-29T17:53:26Z","snapshot_observed_at":"2026-07-06T11:43:50.717280Z","submitted_at":"2021-09-02T18:09:34Z","title":"A buyer's guide to the Hubble Constant","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2109.01161","snapshot_observed_at":"2026-08-06T23:21:49.255173Z","title":null,"venue":null,"work_id":null,"year":2021},"citing_paper":{"arxiv_id":"2506.18445","last_updated":"2025-06-23T09:30:19Z","snapshot_observed_at":"2026-08-08T19:03:41.502084Z","submitted_at":"2025-06-23T09:30:19Z","title":"Comparison of $R_h=ct$ and $\\Lambda$CDM using DESI DR1 measurements","version":1},"reference_index":3,"source":"pdf_text","source_observed_at":"2026-08-06T23:21:49.255173Z"},"links":{"cited_paper":"/paper/2109.01161","citing_paper":"/paper/2506.18445"},"observation_digest":"sha256:b523a61c48e51b379c885480af493901f63c270d34d5dd18b4bb4b9daed3d3d5","observation_id":"424a99b7-56d9-467d-b7c5-71dfefac933b","resolution":{"observed_at":"2026-08-06T23:21:49.255173Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2103.01183","last_updated":"2021-06-05T10:18:21Z","snapshot_observed_at":"2026-07-06T02:11:23.670680Z","submitted_at":"2021-03-01T18:27:48Z","title":"In the Realm of the Hubble tension $-$ a Review of Solutions","version":3},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2103.01183","snapshot_observed_at":"2026-08-06T23:21:49.414879Z","title":"Di Valentino, O","venue":null,"work_id":null,"year":2021},"citing_paper":{"arxiv_id":"2506.18445","last_updated":"2025-06-23T09:30:19Z","snapshot_observed_at":"2026-08-08T19:03:41.502084Z","submitted_at":"2025-06-23T09:30:19Z","title":"Comparison of $R_h=ct$ and $\\Lambda$CDM using DESI DR1 measurements","version":1},"reference_index":4,"source":"pdf_text","source_observed_at":"2026-08-06T23:21:49.414879Z"},"links":{"cited_paper":"/paper/2103.01183","citing_paper":"/paper/2506.18445"},"observation_digest":"sha256:4738514f99686f2d05d759af3211d03fbc5232da8da9d0636e8c573fbb216641","observation_id":"17adbb92-e127-47fe-8bdf-ed659cb25076","resolution":{"observed_at":"2026-08-06T23:21:49.414879Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"1907.10625","last_updated":"2019-07-24T18:00:09Z","snapshot_observed_at":"2026-07-06T08:09:59.842324Z","submitted_at":"2019-07-24T18:00:09Z","title":"Tensions between the Early and the Late Universe","version":1},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"1907.10625","snapshot_observed_at":"2026-08-06T23:21:49.514746Z","title":"Verde, T","venue":null,"work_id":null,"year":2019},"citing_paper":{"arxiv_id":"2506.18445","last_updated":"2025-06-23T09:30:19Z","snapshot_observed_at":"2026-08-08T19:03:41.502084Z","submitted_at":"2025-06-23T09:30:19Z","title":"Comparison of $R_h=ct$ and $\\Lambda$CDM using DESI DR1 measurements","version":1},"reference_index":5,"source":"pdf_text","source_observed_at":"2026-08-06T23:21:49.514746Z"},"links":{"cited_paper":"/paper/1907.10625","citing_paper":"/paper/2506.18445"},"observation_digest":"sha256:6b4646ecd382d931bce5750260fe5bb6063493252a86e198a68752a874e6e5c6","observation_id":"7e6a69c7-c5bb-4312-9f51-62db39f5610d","resolution":{"observed_at":"2026-08-06T23:21:49.514746Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"1701.01789","last_updated":"2017-01-10T06:47:38Z","snapshot_observed_at":"2026-08-09T01:11:37.477571Z","submitted_at":"2017-01-07T03:56:06Z","title":"Median statistics estimates of Hubble and Newton's Constant","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"1701.01789","snapshot_observed_at":"2026-08-06T23:21:49.614740Z","title":"Bethapudi and S","venue":null,"work_id":null,"year":2017},"citing_paper":{"arxiv_id":"2506.18445","last_updated":"2025-06-23T09:30:19Z","snapshot_observed_at":"2026-08-08T19:03:41.502084Z","submitted_at":"2025-06-23T09:30:19Z","title":"Comparison of $R_h=ct$ and $\\Lambda$CDM using DESI DR1 measurements","version":1},"reference_index":6,"source":"pdf_text","source_observed_at":"2026-08-06T23:21:49.614740Z"},"links":{"cited_paper":"/paper/1701.01789","citing_paper":"/paper/2506.18445"},"observation_digest":"sha256:f0e9b3f376df8f8966141e10f1987dbdce6e9ac97387403eafde366bf02a7793","observation_id":"d5be682e-6aac-4504-9e6e-85f5de5e18b1","resolution":{"observed_at":"2026-08-06T23:21:49.614740Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2311.07552","last_updated":"2023-12-26T19:18:30Z","snapshot_observed_at":"2026-07-06T16:46:57.403995Z","submitted_at":"2023-11-13T18:42:03Z","title":"The Unsettled Number: Hubble's Tension","version":4},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2311.07552","snapshot_observed_at":"2026-08-06T23:21:49.734819Z","title":null,"venue":null,"work_id":null,"year":2023},"citing_paper":{"arxiv_id":"2506.18445","last_updated":"2025-06-23T09:30:19Z","snapshot_observed_at":"2026-08-08T19:03:41.502084Z","submitted_at":"2025-06-23T09:30:19Z","title":"Comparison of $R_h=ct$ and $\\Lambda$CDM using DESI DR1 measurements","version":1},"reference_index":7,"source":"pdf_text","source_observed_at":"2026-08-06T23:21:49.734819Z"},"links":{"cited_paper":"/paper/2311.07552","citing_paper":"/paper/2506.18445"},"observation_digest":"sha256:b418e222115901c82eabf8382ed895d505d209e5c0ef47eca640abe5faf82313","observation_id":"3f016262-604f-4531-8dc2-22fa8dbb10db","resolution":{"observed_at":"2026-08-06T23:21:49.734819Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2203.06142","last_updated":"2022-04-24T16:57:09Z","snapshot_observed_at":"2026-07-06T02:11:23.670680Z","submitted_at":"2022-03-11T18:13:52Z","title":"Cosmology Intertwined: A Review of the Particle Physics, Astrophysics, and Cosmology Associated with the Cosmological Tensions and Anomalies","version":3},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2203.06142","snapshot_observed_at":"2026-08-06T23:21:49.864771Z","title":"Abdalla, G","venue":null,"work_id":null,"year":2022},"citing_paper":{"arxiv_id":"2506.18445","last_updated":"2025-06-23T09:30:19Z","snapshot_observed_at":"2026-08-08T19:03:41.502084Z","submitted_at":"2025-06-23T09:30:19Z","title":"Comparison of $R_h=ct$ and $\\Lambda$CDM using DESI DR1 measurements","version":1},"reference_index":8,"source":"pdf_text","source_observed_at":"2026-08-06T23:21:49.864771Z"},"links":{"cited_paper":"/paper/2203.06142","citing_paper":"/paper/2506.18445"},"observation_digest":"sha256:c063c47ffcc31feee7fb13a377eec721521986f7702c8f7994c0b9a219669bd7","observation_id":"334a1d47-1046-4afa-9a79-99b68bd36fa8","resolution":{"observed_at":"2026-08-06T23:21:49.864771Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"1703.02389","last_updated":"2017-03-11T17:55:08Z","snapshot_observed_at":"2026-07-06T05:32:43.095957Z","submitted_at":"2017-03-07T14:13:49Z","title":"Cosmology and Convention","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"1703.02389","snapshot_observed_at":"2026-08-06T23:21:49.939088Z","title":"Merritt, Studies in the History and Philosophy of Modern Physics57, 41 (2017), 1703.02389","venue":null,"work_id":null,"year":2017},"citing_paper":{"arxiv_id":"2506.18445","last_updated":"2025-06-23T09:30:19Z","snapshot_observed_at":"2026-08-08T19:03:41.502084Z","submitted_at":"2025-06-23T09:30:19Z","title":"Comparison of $R_h=ct$ and $\\Lambda$CDM using DESI DR1 measurements","version":1},"reference_index":9,"source":"pdf_text","source_observed_at":"2026-08-06T23:21:49.939088Z"},"links":{"cited_paper":"/paper/1703.02389","citing_paper":"/paper/2506.18445"},"observation_digest":"sha256:2dde2ab02a2ff885916326c553e979de3c3cd6914552dbdc6611152d207d2310","observation_id":"0c59fe9b-5411-4fb4-ad58-0e665a557e90","resolution":{"observed_at":"2026-08-06T23:21:49.939088Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"1912.01132","last_updated":"2019-12-03T00:15:19Z","snapshot_observed_at":"2026-08-07T02:53:48.766450Z","submitted_at":"2019-12-03T00:15:19Z","title":"Big-Bang Nucleosynthesis After Planck","version":1},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"1912.01132","snapshot_observed_at":"2026-08-06T23:21:50.064815Z","title":null,"venue":null,"work_id":null,"year":2020},"citing_paper":{"arxiv_id":"2506.18445","last_updated":"2025-06-23T09:30:19Z","snapshot_observed_at":"2026-08-08T19:03:41.502084Z","submitted_at":"2025-06-23T09:30:19Z","title":"Comparison of $R_h=ct$ and $\\Lambda$CDM using DESI DR1 measurements","version":1},"reference_index":10,"source":"pdf_text","source_observed_at":"2026-08-06T23:21:50.064815Z"},"links":{"cited_paper":"/paper/1912.01132","citing_paper":"/paper/2506.18445"},"observation_digest":"sha256:e4f9ac03cec6da4715d26173626e4eb30de7d1c1cf45363d9e088f2aad54f563","observation_id":"72ba1598-354f-4e52-a7b7-49592359a53f","resolution":{"observed_at":"2026-08-06T23:21:50.064815Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2208.01611","last_updated":"2023-02-20T17:56:39Z","snapshot_observed_at":"2026-07-06T13:38:01.856971Z","submitted_at":"2022-08-02T17:40:40Z","title":"Stress Testing $\\Lambda$CDM with High-redshift Galaxy Candidates","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2208.01611","snapshot_observed_at":"2026-08-06T23:21:50.153407Z","title":"Boylan-Kolchin, Nature Astronomy7, 731 (2023), 2208.01611","venue":null,"work_id":null,"year":2023},"citing_paper":{"arxiv_id":"2506.18445","last_updated":"2025-06-23T09:30:19Z","snapshot_observed_at":"2026-08-08T19:03:41.502084Z","submitted_at":"2025-06-23T09:30:19Z","title":"Comparison of $R_h=ct$ and $\\Lambda$CDM using DESI DR1 measurements","version":1},"reference_index":11,"source":"pdf_text","source_observed_at":"2026-08-06T23:21:50.153407Z"},"links":{"cited_paper":"/paper/2208.01611","citing_paper":"/paper/2506.18445"},"observation_digest":"sha256:6867d91d4617a4fc4bf2bc1c0b971666501573c09b4d702efa5a845b35b6edbe","observation_id":"58a802d0-5fee-4f0a-a13c-574387650f3a","resolution":{"observed_at":"2026-08-06T23:21:50.153407Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2105.05208","last_updated":"2022-04-06T12:16:37Z","snapshot_observed_at":"2026-08-04T21:52:15.150186Z","submitted_at":"2021-05-11T17:17:34Z","title":"Challenges for $\\Lambda$CDM: An update","version":3},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2105.05208","snapshot_observed_at":"2026-08-06T23:21:50.234741Z","title":"Perivolaropoulos and F","venue":null,"work_id":null,"year":2022},"citing_paper":{"arxiv_id":"2506.18445","last_updated":"2025-06-23T09:30:19Z","snapshot_observed_at":"2026-08-08T19:03:41.502084Z","submitted_at":"2025-06-23T09:30:19Z","title":"Comparison of $R_h=ct$ and $\\Lambda$CDM using DESI DR1 measurements","version":1},"reference_index":12,"source":"pdf_text","source_observed_at":"2026-08-06T23:21:50.234741Z"},"links":{"cited_paper":"/paper/2105.05208","citing_paper":"/paper/2506.18445"},"observation_digest":"sha256:5e1ceb7fe767d6033d53565b6dc64eab09de6f73ed607ad651fae90899e64df7","observation_id":"7c9d95b1-2798-4386-9600-a4d5c1d5bd8e","resolution":{"observed_at":"2026-08-06T23:21:50.234741Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2208.05018","last_updated":"2022-08-09T19:47:54Z","snapshot_observed_at":"2026-07-06T13:40:23.993017Z","submitted_at":"2022-08-09T19:47:54Z","title":"Anomalies in Physical Cosmology","version":1},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2208.05018","snapshot_observed_at":"2026-08-06T23:21:50.364895Z","title":null,"venue":null,"work_id":null,"year":2022},"citing_paper":{"arxiv_id":"2506.18445","last_updated":"2025-06-23T09:30:19Z","snapshot_observed_at":"2026-08-08T19:03:41.502084Z","submitted_at":"2025-06-23T09:30:19Z","title":"Comparison of $R_h=ct$ and $\\Lambda$CDM using DESI DR1 measurements","version":1},"reference_index":13,"source":"pdf_text","source_observed_at":"2026-08-06T23:21:50.364895Z"},"links":{"cited_paper":"/paper/2208.05018","citing_paper":"/paper/2506.18445"},"observation_digest":"sha256:e05bd85736c77d542cb458dc879e30f246021a831ab36a4c974e10602f4ac7f8","observation_id":"731db38b-6416-45d7-9b15-8795aaafdd9a","resolution":{"observed_at":"2026-08-06T23:21:50.364895Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2110.06936","last_updated":"2022-07-06T16:21:47Z","snapshot_observed_at":"2026-08-07T19:10:35.614990Z","submitted_at":"2021-10-13T18:00:01Z","title":"From galactic bars to the Hubble tension: weighing up the astrophysical evidence for Milgromian gravity","version":9},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2110.06936","snapshot_observed_at":"2026-08-06T23:21:50.475006Z","title":"Banik and H","venue":null,"work_id":null,"year":2022},"citing_paper":{"arxiv_id":"2506.18445","last_updated":"2025-06-23T09:30:19Z","snapshot_observed_at":"2026-08-08T19:03:41.502084Z","submitted_at":"2025-06-23T09:30:19Z","title":"Comparison of $R_h=ct$ and $\\Lambda$CDM using DESI DR1 measurements","version":1},"reference_index":14,"source":"pdf_text","source_observed_at":"2026-08-06T23:21:50.475006Z"},"links":{"cited_paper":"/paper/2110.06936","citing_paper":"/paper/2506.18445"},"observation_digest":"sha256:5dfc630988fa6457ccb6f5d037876a2c9f592b57cfcf547acb03899355121ea8","observation_id":"d71b4448-0e3a-4dd8-950e-364433352bc6","resolution":{"observed_at":"2026-08-06T23:21:50.475006Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"0711.4181","last_updated":"2007-11-27T05:28:46Z","snapshot_observed_at":"2026-08-04T06:34:15.826514Z","submitted_at":"2007-11-27T05:28:46Z","title":"The Cosmic Horizon","version":1},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"0711.4181","snapshot_observed_at":"2026-08-06T23:21:50.625080Z","title":"Melia, Mon","venue":null,"work_id":null,"year":2007},"citing_paper":{"arxiv_id":"2506.18445","last_updated":"2025-06-23T09:30:19Z","snapshot_observed_at":"2026-08-08T19:03:41.502084Z","submitted_at":"2025-06-23T09:30:19Z","title":"Comparison of $R_h=ct$ and $\\Lambda$CDM using DESI DR1 measurements","version":1},"reference_index":15,"source":"pdf_text","source_observed_at":"2026-08-06T23:21:50.625080Z"},"links":{"cited_paper":"/paper/0711.4181","citing_paper":"/paper/2506.18445"},"observation_digest":"sha256:3ede2300fef7956d1e35ebb79bc7057b2a04b917bdf716dc58d78c7e7767109d","observation_id":"3ef24ee3-4e8c-4738-8e82-3743d24c098d","resolution":{"observed_at":"2026-08-06T23:21:50.625080Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"1109.5189","last_updated":"2011-09-23T20:10:59Z","snapshot_observed_at":"2026-07-06T02:34:32.759448Z","submitted_at":"2011-09-23T20:10:59Z","title":"The R_h = ct Universe","version":1},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"1109.5189","snapshot_observed_at":"2026-08-06T23:21:50.859271Z","title":"Melia and A","venue":null,"work_id":null,"year":2012},"citing_paper":{"arxiv_id":"2506.18445","last_updated":"2025-06-23T09:30:19Z","snapshot_observed_at":"2026-08-08T19:03:41.502084Z","submitted_at":"2025-06-23T09:30:19Z","title":"Comparison of $R_h=ct$ and $\\Lambda$CDM using DESI DR1 measurements","version":1},"reference_index":16,"source":"pdf_text","source_observed_at":"2026-08-06T23:21:50.859271Z"},"links":{"cited_paper":"/paper/1109.5189","citing_paper":"/paper/2506.18445"},"observation_digest":"sha256:ac69a5e8bc7f8b4183d4013a83a447d21a77a970a16774575615657e6a192392","observation_id":"b51ee76f-8fd4-49fc-aed8-329d9bf74d36","resolution":{"observed_at":"2026-08-06T23:21:50.859271Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"1205.2713","last_updated":"2012-05-11T20:32:11Z","snapshot_observed_at":"2026-07-06T02:47:59.547815Z","submitted_at":"2012-05-11T20:32:11Z","title":"The Cosmic Spacetime","version":1},"cited_work":{"arxiv_id":"1205.2713","doi":null,"metadata_source":"pith","pith_arxiv_id":"1205.2713","snapshot_observed_at":"2026-08-06T23:22:03.045271Z","title":"The Cosmic Spacetime","venue":"physics.pop-ph","work_id":"167bc648-75eb-4773-88c5-d05c89cb3cc8","year":2012},"citing_paper":{"arxiv_id":"2506.18445","last_updated":"2025-06-23T09:30:19Z","snapshot_observed_at":"2026-08-08T19:03:41.502084Z","submitted_at":"2025-06-23T09:30:19Z","title":"Comparison of $R_h=ct$ and $\\Lambda$CDM using DESI DR1 measurements","version":1},"reference_index":17,"source":"pdf_text","source_observed_at":"2026-08-06T23:21:51.294793Z"},"links":{"cited_paper":"/paper/1205.2713","citing_paper":"/paper/2506.18445"},"observation_digest":"sha256:11f0b74d9d3b9432552ad0dfd80c67bb8b421289451ab2e53ccd974de227c44a","observation_id":"31caca5b-8020-44c3-9e87-981fefb95426","resolution":{"observed_at":"2026-08-06T23:22:03.220666Z","resolver_source":"local_arxiv","status":"metadata_mismatch"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-08T06:32:00.761636+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-08T06:32:00.761636+00:00","source":"crossref"},{"observed_at":"2026-08-08T06:31:55.24221+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":{"arxiv_id":"1304.1802","last_updated":"2013-04-05T18:46:50Z","snapshot_observed_at":"2026-07-06T03:10:29.622191Z","submitted_at":"2013-04-05T18:46:50Z","title":"Cosmic Chronometers in the R_h=ct Universe","version":1},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"1304.1802","snapshot_observed_at":"2026-08-06T23:21:51.424810Z","title":"Melia and R","venue":null,"work_id":null,"year":2013},"citing_paper":{"arxiv_id":"2506.18445","last_updated":"2025-06-23T09:30:19Z","snapshot_observed_at":"2026-08-08T19:03:41.502084Z","submitted_at":"2025-06-23T09:30:19Z","title":"Comparison of $R_h=ct$ and $\\Lambda$CDM using DESI DR1 measurements","version":1},"reference_index":18,"source":"pdf_text","source_observed_at":"2026-08-06T23:21:51.424810Z"},"links":{"cited_paper":"/paper/1304.1802","citing_paper":"/paper/2506.18445"},"observation_digest":"sha256:0388cafeb25766de5f48deebaaf466bad2b6d0f61515e76f3d0368d1f51a6f24","observation_id":"6a6eb40f-fd91-4c73-b091-e3876c2df47d","resolution":{"observed_at":"2026-08-06T23:21:51.424810Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"1802.02255","last_updated":"2018-02-15T21:31:53Z","snapshot_observed_at":"2026-07-06T06:22:08.261855Z","submitted_at":"2018-02-06T23:09:31Z","title":"Model Selection Using Cosmic Chronometers with Gaussian Processes","version":2},"cited_work":{"arxiv_id":"1802.02255","doi":null,"metadata_source":"pith","pith_arxiv_id":"1802.02255","snapshot_observed_at":"2026-08-06T23:22:02.826868Z","title":"Model Selection Using Cosmic Chronometers with Gaussian Processes","venue":"astro-ph.CO","work_id":"02aef616-aa55-4571-aa73-7e8eb435b6cc","year":2018},"citing_paper":{"arxiv_id":"2506.18445","last_updated":"2025-06-23T09:30:19Z","snapshot_observed_at":"2026-08-08T19:03:41.502084Z","submitted_at":"2025-06-23T09:30:19Z","title":"Comparison of $R_h=ct$ and $\\Lambda$CDM using DESI DR1 measurements","version":1},"reference_index":19,"source":"pdf_text","source_observed_at":"2026-08-06T23:21:51.525063Z"},"links":{"cited_paper":"/paper/1802.02255","citing_paper":"/paper/2506.18445"},"observation_digest":"sha256:cc867e4de6e8a7887e6f3cf91398e06621fffc3239582a9355347f469d784fbc","observation_id":"f0e8af30-27fd-41d1-8e69-94d5a33d1fb3","resolution":{"observed_at":"2026-08-06T23:22:02.945683Z","resolver_source":"local_arxiv","status":"verified_exact"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-08T06:32:00.761636+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-08T06:32:00.761636+00:00","source":"crossref"},{"observed_at":"2026-08-08T06:31:55.24221+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":{"arxiv_id":"1910.14024","last_updated":"2019-10-30T02:44:57Z","snapshot_observed_at":"2026-08-08T18:37:58.249769Z","submitted_at":"2019-10-30T02:44:57Z","title":"Testing the $R_{\\rm h}=ct$ Universe Jointly with the Redshift-dependent Expansion rate and Angular-diameter and Luminosity Distances","version":1},"cited_work":{"arxiv_id":"1910.14024","doi":null,"metadata_source":"pith","pith_arxiv_id":"1910.14024","snapshot_observed_at":"2026-08-06T23:22:02.645586Z","title":"Testing the $R_{\\rm h}=ct$ Universe Jointly with the Redshift-dependent Expansion rate and Angular-diameter and Luminosity Distances","venue":"astro-ph.CO","work_id":"9e3d6e21-b3a6-46e9-bc48-543e2cb4e095","year":2019},"citing_paper":{"arxiv_id":"2506.18445","last_updated":"2025-06-23T09:30:19Z","snapshot_observed_at":"2026-08-08T19:03:41.502084Z","submitted_at":"2025-06-23T09:30:19Z","title":"Comparison of $R_h=ct$ and $\\Lambda$CDM using DESI DR1 measurements","version":1},"reference_index":20,"source":"pdf_text","source_observed_at":"2026-08-06T23:21:51.735094Z"},"links":{"cited_paper":"/paper/1910.14024","citing_paper":"/paper/2506.18445"},"observation_digest":"sha256:d9f45332ea435a058a15ec96adc6ad7ce4e93d91ca597363f5ab675f8896daca","observation_id":"37758357-6f55-4e78-9d49-edd5c81d5287","resolution":{"observed_at":"2026-08-06T23:22:02.704875Z","resolver_source":"local_arxiv","status":"verified_exact"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-08T06:32:00.761636+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-08T06:32:00.761636+00:00","source":"crossref"},{"observed_at":"2026-08-08T06:31:55.24221+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":{"arxiv_id":"1907.13127","last_updated":"2019-07-30T14:35:55Z","snapshot_observed_at":"2026-07-06T08:11:17.778786Z","submitted_at":"2019-07-30T14:35:55Z","title":"Cosmological test using the Hubble diagram of high-z quasars","version":1},"cited_work":{"arxiv_id":"1907.13127","doi":null,"metadata_source":"pith","pith_arxiv_id":"1907.13127","snapshot_observed_at":"2026-08-06T23:22:02.381652Z","title":"Cosmological test using the Hubble diagram of high-z quasars","venue":"astro-ph.CO","work_id":"cb0798a7-6af2-44de-8dde-d27faf0016c3","year":2019},"citing_paper":{"arxiv_id":"2506.18445","last_updated":"2025-06-23T09:30:19Z","snapshot_observed_at":"2026-08-08T19:03:41.502084Z","submitted_at":"2025-06-23T09:30:19Z","title":"Comparison of $R_h=ct$ and $\\Lambda$CDM using DESI DR1 measurements","version":1},"reference_index":21,"source":"pdf_text","source_observed_at":"2026-08-06T23:21:51.894764Z"},"links":{"cited_paper":"/paper/1907.13127","citing_paper":"/paper/2506.18445"},"observation_digest":"sha256:4d7213ed90cabbd523626c30da473ea293278d3ae01094b96f417b08f1693788","observation_id":"559f1bff-79b1-4ef2-a7c4-9f47a5d7c8dd","resolution":{"observed_at":"2026-08-06T23:22:02.495008Z","resolver_source":"local_arxiv","status":"verified_exact"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-08T06:32:00.761636+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-08T06:32:00.761636+00:00","source":"crossref"},{"observed_at":"2026-08-08T06:31:55.24221+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":{"arxiv_id":"1601.04649","last_updated":"2016-01-18T18:37:32Z","snapshot_observed_at":"2026-08-06T03:16:11.310719Z","submitted_at":"2016-01-18T18:37:32Z","title":"Constancy of the Cluster Gas Mass Fraction in the R_h=ct Universe","version":1},"cited_work":{"arxiv_id":"1601.04649","doi":null,"metadata_source":"pith","pith_arxiv_id":"1601.04649","snapshot_observed_at":"2026-08-06T23:22:02.089547Z","title":"Constancy of the Cluster Gas Mass Fraction in the R_h=ct Universe","venue":"astro-ph.CO","work_id":"610a4480-b2e1-4351-8a5b-e50d9e646c05","year":2016},"citing_paper":{"arxiv_id":"2506.18445","last_updated":"2025-06-23T09:30:19Z","snapshot_observed_at":"2026-08-08T19:03:41.502084Z","submitted_at":"2025-06-23T09:30:19Z","title":"Comparison of $R_h=ct$ and $\\Lambda$CDM using DESI DR1 measurements","version":1},"reference_index":22,"source":"pdf_text","source_observed_at":"2026-08-06T23:21:51.984748Z"},"links":{"cited_paper":"/paper/1601.04649","citing_paper":"/paper/2506.18445"},"observation_digest":"sha256:83949451ebcdbd9420688339b6a72549893a46a4b551a243fe849cad6d037651","observation_id":"ff84c64f-bab5-4603-b540-2764cc89a547","resolution":{"observed_at":"2026-08-06T23:22:02.224966Z","resolver_source":"local_arxiv","status":"metadata_mismatch"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-08T06:32:00.761636+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-08T06:32:00.761636+00:00","source":"crossref"},{"observed_at":"2026-08-08T06:31:55.24221+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":{"arxiv_id":"1809.05094","last_updated":"2018-09-12T14:45:56Z","snapshot_observed_at":"2026-07-06T07:02:02.624968Z","submitted_at":"2018-09-12T14:45:56Z","title":"Cosmological Tests with the Joint Lightcurve Analysis","version":1},"cited_work":{"arxiv_id":"1809.05094","doi":null,"metadata_source":"pith","pith_arxiv_id":"1809.05094","snapshot_observed_at":"2026-08-06T23:22:01.838215Z","title":"Cosmological Tests with the Joint Lightcurve Analysis","venue":"astro-ph.CO","work_id":"9ccdc999-8d27-4fbd-a30d-ddd5e0e7a602","year":2018},"citing_paper":{"arxiv_id":"2506.18445","last_updated":"2025-06-23T09:30:19Z","snapshot_observed_at":"2026-08-08T19:03:41.502084Z","submitted_at":"2025-06-23T09:30:19Z","title":"Comparison of $R_h=ct$ and $\\Lambda$CDM using DESI DR1 measurements","version":1},"reference_index":23,"source":"pdf_text","source_observed_at":"2026-08-06T23:21:52.094837Z"},"links":{"cited_paper":"/paper/1809.05094","citing_paper":"/paper/2506.18445"},"observation_digest":"sha256:116a6d13202a6915bdfde5ba7600f56f0bbc97eaa02da25aa83bf08761c65f54","observation_id":"45c8edc3-6795-4cc2-8c14-1705f7d6263e","resolution":{"observed_at":"2026-08-06T23:22:01.909733Z","resolver_source":"local_arxiv","status":"verified_exact"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-08T06:32:00.761636+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-08T06:32:00.761636+00:00","source":"crossref"},{"observed_at":"2026-08-08T06:31:55.24221+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":{"arxiv_id":"1805.08640","last_updated":"2018-05-22T14:40:17Z","snapshot_observed_at":"2026-07-06T06:40:33.998972Z","submitted_at":"2018-05-22T14:40:17Z","title":"Model Selection with Strong-lensing Systems","version":1},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"1805.08640","snapshot_observed_at":"2026-08-06T23:21:52.320009Z","title":"Leaf and F","venue":null,"work_id":null,"year":2018},"citing_paper":{"arxiv_id":"2506.18445","last_updated":"2025-06-23T09:30:19Z","snapshot_observed_at":"2026-08-08T19:03:41.502084Z","submitted_at":"2025-06-23T09:30:19Z","title":"Comparison of $R_h=ct$ and $\\Lambda$CDM using DESI DR1 measurements","version":1},"reference_index":24,"source":"pdf_text","source_observed_at":"2026-08-06T23:21:52.320009Z"},"links":{"cited_paper":"/paper/1805.08640","citing_paper":"/paper/2506.18445"},"observation_digest":"sha256:be27f41dee125621382222514af7e9f4ae43df3117a736a898480cc6364e1506","observation_id":"ba262fbf-076a-461a-860e-d6e7762a70d7","resolution":{"observed_at":"2026-08-06T23:21:52.320009Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2212.06113","last_updated":"2022-12-12T18:38:41Z","snapshot_observed_at":"2026-08-05T13:54:33.088409Z","submitted_at":"2022-12-12T18:38:41Z","title":"Model selection using time-delay lenses","version":1},"cited_work":{"arxiv_id":"2212.06113","doi":null,"metadata_source":"pith","pith_arxiv_id":"2212.06113","snapshot_observed_at":"2026-08-06T23:22:01.514532Z","title":"Model selection using time-delay lenses","venue":"astro-ph.CO","work_id":"0ff751f1-36ed-429f-b824-d95aaccfc837","year":2022},"citing_paper":{"arxiv_id":"2506.18445","last_updated":"2025-06-23T09:30:19Z","snapshot_observed_at":"2026-08-08T19:03:41.502084Z","submitted_at":"2025-06-23T09:30:19Z","title":"Comparison of $R_h=ct$ and $\\Lambda$CDM using DESI DR1 measurements","version":1},"reference_index":25,"source":"pdf_text","source_observed_at":"2026-08-06T23:21:52.424747Z"},"links":{"cited_paper":"/paper/2212.06113","citing_paper":"/paper/2506.18445"},"observation_digest":"sha256:ef7f01143453f7c060f44ab56bae1ef68df42cd271c81429ce3c202dfc808777","observation_id":"930f1f24-8528-44cc-89da-7d93421c2a23","resolution":{"observed_at":"2026-08-06T23:22:01.632414Z","resolver_source":"local_arxiv","status":"verified_exact"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-08T06:32:00.761636+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-08T06:32:00.761636+00:00","source":"crossref"},{"observed_at":"2026-08-08T06:31:55.24221+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":{"arxiv_id":"2308.05918","last_updated":"2023-08-11T02:55:30Z","snapshot_observed_at":"2026-07-06T16:05:06.272859Z","submitted_at":"2023-08-11T02:55:30Z","title":"Investigating Cosmological Models and the Hubble Tension using Localized Fast Radio Bursts","version":1},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2308.05918","snapshot_observed_at":"2026-08-06T23:21:52.519719Z","title":"Wei and F","venue":null,"work_id":null,"year":2023},"citing_paper":{"arxiv_id":"2506.18445","last_updated":"2025-06-23T09:30:19Z","snapshot_observed_at":"2026-08-08T19:03:41.502084Z","submitted_at":"2025-06-23T09:30:19Z","title":"Comparison of $R_h=ct$ and $\\Lambda$CDM using DESI DR1 measurements","version":1},"reference_index":26,"source":"pdf_text","source_observed_at":"2026-08-06T23:21:52.519719Z"},"links":{"cited_paper":"/paper/2308.05918","citing_paper":"/paper/2506.18445"},"observation_digest":"sha256:55273725a9eb426623a748f8c658aacb69a7a19d4d25c2dd36e3c9c976c63f55","observation_id":"1a2cba3b-b6e4-4d34-84af-628856d1502e","resolution":{"observed_at":"2026-08-06T23:21:52.519719Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2412.02706","last_updated":"2024-11-24T20:53:07Z","snapshot_observed_at":"2026-08-06T15:15:59.568152Z","submitted_at":"2024-11-24T20:53:07Z","title":"The cosmic timeline implied by the highest redshift quasars","version":1},"cited_work":{"arxiv_id":"2412.02706","doi":null,"metadata_source":"pith","pith_arxiv_id":"2412.02706","snapshot_observed_at":"2026-08-06T23:22:01.209503Z","title":"The cosmic timeline implied by the highest redshift quasars","venue":"astro-ph.CO","work_id":"b2413d66-5700-4e92-8aa9-fac90ca4d029","year":2024},"citing_paper":{"arxiv_id":"2506.18445","last_updated":"2025-06-23T09:30:19Z","snapshot_observed_at":"2026-08-08T19:03:41.502084Z","submitted_at":"2025-06-23T09:30:19Z","title":"Comparison of $R_h=ct$ and $\\Lambda$CDM using DESI DR1 measurements","version":1},"reference_index":27,"source":"pdf_text","source_observed_at":"2026-08-06T23:21:52.634880Z"},"links":{"cited_paper":"/paper/2412.02706","citing_paper":"/paper/2506.18445"},"observation_digest":"sha256:43719e07a3a329bbdd36624a7ded682ec8e786ee732bb999646dca9afbe86594","observation_id":"bb110615-dea3-4b27-94f9-7d523ce5fc06","resolution":{"observed_at":"2026-08-06T23:22:01.292232Z","resolver_source":"local_arxiv","status":"metadata_mismatch"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-08T06:32:00.761636+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-08T06:32:00.761636+00:00","source":"crossref"},{"observed_at":"2026-08-08T06:31:55.24221+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":{"arxiv_id":"2503.09607","last_updated":"2025-02-24T17:51:39Z","snapshot_observed_at":"2026-08-07T17:52:32.678311Z","submitted_at":"2025-02-24T17:51:39Z","title":"The lens mass in the Einstein ring JWST-ER1","version":1},"cited_work":{"arxiv_id":"2503.09607","doi":null,"metadata_source":"pith","pith_arxiv_id":"2503.09607","snapshot_observed_at":"2026-08-06T23:22:00.966870Z","title":"The lens mass in the Einstein ring JWST-ER1","venue":"astro-ph.CO","work_id":"a8919a79-a42c-4321-a99d-6a4bc97b2049","year":2025},"citing_paper":{"arxiv_id":"2506.18445","last_updated":"2025-06-23T09:30:19Z","snapshot_observed_at":"2026-08-08T19:03:41.502084Z","submitted_at":"2025-06-23T09:30:19Z","title":"Comparison of $R_h=ct$ and $\\Lambda$CDM using DESI DR1 measurements","version":1},"reference_index":28,"source":"pdf_text","source_observed_at":"2026-08-06T23:21:52.813627Z"},"links":{"cited_paper":"/paper/2503.09607","citing_paper":"/paper/2506.18445"},"observation_digest":"sha256:26fdfb962ae6a07fe01a159ec2204418ac80f9bd92e2a9452d6a052c4ac4165a","observation_id":"27151a16-75c4-4ec6-bdbf-580b550ff061","resolution":{"observed_at":"2026-08-06T23:22:01.103700Z","resolver_source":"local_arxiv","status":"metadata_mismatch"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-08T06:32:00.761636+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-08T06:32:00.761636+00:00","source":"crossref"},{"observed_at":"2026-08-08T06:31:55.24221+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":{"arxiv_id":"1502.05416","last_updated":"2015-07-08T21:47:13Z","snapshot_observed_at":"2026-07-06T04:09:39.172428Z","submitted_at":"2015-02-18T21:06:55Z","title":"Robust model comparison disfavors power law cosmology","version":2},"cited_work":{"arxiv_id":"1502.05416","doi":null,"metadata_source":"pith","pith_arxiv_id":"1502.05416","snapshot_observed_at":"2026-08-06T23:22:00.664742Z","title":"Robust model comparison disfavors power law cosmology","venue":"astro-ph.CO","work_id":"dd7b5a80-7fa9-4394-a316-e212a06bb36c","year":2015},"citing_paper":{"arxiv_id":"2506.18445","last_updated":"2025-06-23T09:30:19Z","snapshot_observed_at":"2026-08-08T19:03:41.502084Z","submitted_at":"2025-06-23T09:30:19Z","title":"Comparison of $R_h=ct$ and $\\Lambda$CDM using DESI DR1 measurements","version":1},"reference_index":29,"source":"pdf_text","source_observed_at":"2026-08-06T23:21:52.934868Z"},"links":{"cited_paper":"/paper/1502.05416","citing_paper":"/paper/2506.18445"},"observation_digest":"sha256:e3ceea529acd4c13f8a6e7ebab4988693c5cc78b450330d26a553fd9395184de","observation_id":"6c0fb9a4-250d-4a2d-b6b3-3946af9bdd8c","resolution":{"observed_at":"2026-08-06T23:22:00.784788Z","resolver_source":"local_arxiv","status":"verified_exact"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-08T06:32:00.761636+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-08T06:32:00.761636+00:00","source":"crossref"},{"observed_at":"2026-08-08T06:31:55.24221+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":{"arxiv_id":"1206.5130","last_updated":"2012-08-20T11:24:48Z","snapshot_observed_at":"2026-08-06T20:39:36.857729Z","submitted_at":"2012-06-22T12:41:04Z","title":"We do not live in the R_h = c t universe","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"1206.5130","snapshot_observed_at":"2026-08-06T23:21:53.106257Z","title":"Bilicki and M","venue":null,"work_id":null,"year":2012},"citing_paper":{"arxiv_id":"2506.18445","last_updated":"2025-06-23T09:30:19Z","snapshot_observed_at":"2026-08-08T19:03:41.502084Z","submitted_at":"2025-06-23T09:30:19Z","title":"Comparison of $R_h=ct$ and $\\Lambda$CDM using DESI DR1 measurements","version":1},"reference_index":30,"source":"pdf_text","source_observed_at":"2026-08-06T23:21:53.106257Z"},"links":{"cited_paper":"/paper/1206.5130","citing_paper":"/paper/2506.18445"},"observation_digest":"sha256:2317104ef5276cc5683e47f84148f94b80c1ca842a3b6e4592fd224175e358ce","observation_id":"7946f751-fae5-4087-919f-c6e4602fa48b","resolution":{"observed_at":"2026-08-06T23:21:53.106257Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"1604.07460","last_updated":"2016-04-25T22:16:30Z","snapshot_observed_at":"2026-07-06T04:54:03.876286Z","submitted_at":"2016-04-25T22:16:30Z","title":"Primordial Nucleosynthesis in the Rh = ct cosmology: Pouring cold water on the Simmering Universe","version":1},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"1604.07460","snapshot_observed_at":"2026-08-06T23:21:53.207067Z","title":null,"venue":null,"work_id":null,"year":2016},"citing_paper":{"arxiv_id":"2506.18445","last_updated":"2025-06-23T09:30:19Z","snapshot_observed_at":"2026-08-08T19:03:41.502084Z","submitted_at":"2025-06-23T09:30:19Z","title":"Comparison of $R_h=ct$ and $\\Lambda$CDM using DESI DR1 measurements","version":1},"reference_index":31,"source":"pdf_text","source_observed_at":"2026-08-06T23:21:53.207067Z"},"links":{"cited_paper":"/paper/1604.07460","citing_paper":"/paper/2506.18445"},"observation_digest":"sha256:d2400a81b46380b0f289f71a48611bc7f177a0f6d16600f91939f9698908e8c7","observation_id":"ab1a1c3b-ed9b-4c2e-9dc4-4b596ad41254","resolution":{"observed_at":"2026-08-06T23:21:53.207067Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"1702.08244","last_updated":"2017-02-27T11:41:07Z","snapshot_observed_at":"2026-07-06T05:31:32.333303Z","submitted_at":"2017-02-27T11:41:07Z","title":"Strong evidence for an accelerating universe","version":1},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"1702.08244","snapshot_observed_at":"2026-08-06T23:21:53.324822Z","title":null,"venue":null,"work_id":null,"year":2017},"citing_paper":{"arxiv_id":"2506.18445","last_updated":"2025-06-23T09:30:19Z","snapshot_observed_at":"2026-08-08T19:03:41.502084Z","submitted_at":"2025-06-23T09:30:19Z","title":"Comparison of $R_h=ct$ and $\\Lambda$CDM using DESI DR1 measurements","version":1},"reference_index":32,"source":"pdf_text","source_observed_at":"2026-08-06T23:21:53.324822Z"},"links":{"cited_paper":"/paper/1702.08244","citing_paper":"/paper/2506.18445"},"observation_digest":"sha256:cc415b55184fa0ce997689fe3d64d85bf444d3ba6047d6f2d9a87f39cad8c273","observation_id":"c6b9b5fb-212b-4774-8e8e-9f5a58fbe531","resolution":{"observed_at":"2026-08-06T23:21:53.324822Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"1711.05025","last_updated":"2018-08-01T09:40:58Z","snapshot_observed_at":"2026-07-06T06:09:23.301436Z","submitted_at":"2017-11-14T09:44:45Z","title":"Local probes strongly favor $\\Lambda$CDM against power-law and $R_h=ct$ universe","version":2},"cited_work":{"arxiv_id":"1711.05025","doi":null,"metadata_source":"pith","pith_arxiv_id":"1711.05025","snapshot_observed_at":"2026-08-06T23:22:00.019970Z","title":"Local probes strongly favor $\\Lambda$CDM against power-law and $R_h=ct$ universe","venue":"astro-ph.CO","work_id":"b805defb-8898-418c-914a-8017bf5daf35","year":2017},"citing_paper":{"arxiv_id":"2506.18445","last_updated":"2025-06-23T09:30:19Z","snapshot_observed_at":"2026-08-08T19:03:41.502084Z","submitted_at":"2025-06-23T09:30:19Z","title":"Comparison of $R_h=ct$ and $\\Lambda$CDM using DESI DR1 measurements","version":1},"reference_index":33,"source":"pdf_text","source_observed_at":"2026-08-06T23:21:53.457318Z"},"links":{"cited_paper":"/paper/1711.05025","citing_paper":"/paper/2506.18445"},"observation_digest":"sha256:1fc70f324124f11ef6d450fb5ed8a40a3b782147e2d1d3ff1b2ce29f27a63aaa","observation_id":"618032b8-8913-4db9-afe7-37959672e6d9","resolution":{"observed_at":"2026-08-06T23:22:00.156185Z","resolver_source":"local_arxiv","status":"verified_exact"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-08T06:32:00.761636+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-08T06:32:00.761636+00:00","source":"crossref"},{"observed_at":"2026-08-08T06:31:55.24221+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":{"arxiv_id":"1804.06606","last_updated":"2018-04-18T08:54:54Z","snapshot_observed_at":"2026-07-06T06:34:04.456625Z","submitted_at":"2018-04-18T08:54:54Z","title":"Testing the Distance-Duality Relation in the $R_h=ct$ Universe","version":1},"cited_work":{"arxiv_id":"1804.06606","doi":null,"metadata_source":"pith","pith_arxiv_id":"1804.06606","snapshot_observed_at":"2026-08-06T23:21:59.679231Z","title":"Testing the Distance-Duality Relation in the $R_h=ct$ Universe","venue":"astro-ph.CO","work_id":"2cbbad78-c38b-4d56-ac78-9d765a92b5d8","year":2018},"citing_paper":{"arxiv_id":"2506.18445","last_updated":"2025-06-23T09:30:19Z","snapshot_observed_at":"2026-08-08T19:03:41.502084Z","submitted_at":"2025-06-23T09:30:19Z","title":"Comparison of $R_h=ct$ and $\\Lambda$CDM using DESI DR1 measurements","version":1},"reference_index":34,"source":"pdf_text","source_observed_at":"2026-08-06T23:21:53.584742Z"},"links":{"cited_paper":"/paper/1804.06606","citing_paper":"/paper/2506.18445"},"observation_digest":"sha256:d7efc061ecab3437fcee140c935b4e073a36002c6522df6ada0f4409160dc2da","observation_id":"2f4233dd-8da0-40f5-ae18-4f442e256a2f","resolution":{"observed_at":"2026-08-06T23:21:59.784745Z","resolver_source":"local_arxiv","status":"verified_exact"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-08T06:32:00.761636+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-08T06:32:00.761636+00:00","source":"crossref"},{"observed_at":"2026-08-08T06:31:55.24221+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":{"arxiv_id":"1901.09144","last_updated":"2019-01-26T02:27:45Z","snapshot_observed_at":"2026-07-06T07:29:09.345877Z","submitted_at":"2019-01-26T02:27:45Z","title":"Probing cosmic acceleration by strong gravitational lensing systems","version":1},"cited_work":{"arxiv_id":"1901.09144","doi":null,"metadata_source":"pith","pith_arxiv_id":"1901.09144","snapshot_observed_at":"2026-08-06T23:21:59.353022Z","title":"Probing cosmic acceleration by strong gravitational lensing systems","venue":"astro-ph.CO","work_id":"3a595aa1-7765-4bbe-ba8a-ce32aae2a922","year":2019},"citing_paper":{"arxiv_id":"2506.18445","last_updated":"2025-06-23T09:30:19Z","snapshot_observed_at":"2026-08-08T19:03:41.502084Z","submitted_at":"2025-06-23T09:30:19Z","title":"Comparison of $R_h=ct$ and $\\Lambda$CDM using DESI DR1 measurements","version":1},"reference_index":35,"source":"pdf_text","source_observed_at":"2026-08-06T23:21:53.664746Z"},"links":{"cited_paper":"/paper/1901.09144","citing_paper":"/paper/2506.18445"},"observation_digest":"sha256:5d91e86ac7ac180de94284e412c623351c77615f71c866f3b98a586ebf408a68","observation_id":"8abb651b-8035-43aa-8faf-db5d30e2b014","resolution":{"observed_at":"2026-08-06T23:21:59.434747Z","resolver_source":"local_arxiv","status":"verified_exact"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-08T06:32:00.761636+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-08T06:32:00.761636+00:00","source":"crossref"},{"observed_at":"2026-08-08T06:31:55.24221+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":"raw_reference","pith_arxiv_id":null,"snapshot_observed_at":"2026-08-06T23:22:03.679234Z","title":"Fujii, Research Notes of the American Astronomical Society4, 72 (2020)","venue":null,"work_id":"b88e41b9-fc05-4bd8-9ff0-dda0a217b398","year":2020},"citing_paper":{"arxiv_id":"2506.18445","last_updated":"2025-06-23T09:30:19Z","snapshot_observed_at":"2026-08-08T19:03:41.502084Z","submitted_at":"2025-06-23T09:30:19Z","title":"Comparison of $R_h=ct$ and $\\Lambda$CDM using DESI DR1 measurements","version":1},"reference_index":36,"source":"pdf_text","source_observed_at":"2026-08-06T23:21:53.790049Z"},"links":{"citing_paper":"/paper/2506.18445"},"observation_digest":"sha256:5f8618ccd88d06e6abab07585ee31792b4271e2f4edfc90c0bc70f0ccac8cfe0","observation_id":"6f3a129b-4b4a-4084-ba63-eba75c7deac4","resolution":{"observed_at":"2026-08-06T23:22:03.797242Z","resolver_source":"raw_fallback","status":"verified_fuzzy"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-08T06:32:00.761636+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-08T06:32:00.761636+00:00","source":"crossref"},{"observed_at":"2026-08-08T06:31:55.24221+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":{"arxiv_id":"2003.00494","last_updated":"2020-07-25T18:55:31Z","snapshot_observed_at":"2026-08-03T22:32:32.438928Z","submitted_at":"2020-03-01T14:27:09Z","title":"Model Comparison of $\\Lambda$CDM vs $R_h=ct$ using Cosmic Chronometers","version":2},"cited_work":{"arxiv_id":"2003.00494","doi":null,"metadata_source":"pith","pith_arxiv_id":"2003.00494","snapshot_observed_at":"2026-08-06T23:21:58.993486Z","title":"Model Comparison of $\\Lambda$CDM vs $R_h=ct$ using Cosmic Chronometers","venue":"astro-ph.CO","work_id":"be56f670-0705-423d-9153-24faec34daee","year":2020},"citing_paper":{"arxiv_id":"2506.18445","last_updated":"2025-06-23T09:30:19Z","snapshot_observed_at":"2026-08-08T19:03:41.502084Z","submitted_at":"2025-06-23T09:30:19Z","title":"Comparison of $R_h=ct$ and $\\Lambda$CDM using DESI DR1 measurements","version":1},"reference_index":37,"source":"pdf_text","source_observed_at":"2026-08-06T23:21:53.905172Z"},"links":{"cited_paper":"/paper/2003.00494","citing_paper":"/paper/2506.18445"},"observation_digest":"sha256:d6a8785016b354ace351326c216fd2a51a90c792803f0bd7be686c92876dfab0","observation_id":"9d5cda04-8247-4e77-93de-384ad06bd900","resolution":{"observed_at":"2026-08-06T23:21:59.151828Z","resolver_source":"local_arxiv","status":"verified_exact"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-08T06:32:00.761636+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-08T06:32:00.761636+00:00","source":"crossref"},{"observed_at":"2026-08-08T06:31:55.24221+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":{"arxiv_id":"2401.11138","last_updated":"2024-06-06T07:37:36Z","snapshot_observed_at":"2026-08-06T13:41:01.873748Z","submitted_at":"2024-01-20T06:26:16Z","title":"Comparison of $\\Lambda$CDM and $R_h = ct$ with updated galaxy cluster $f_{gas}$ measurements using Bayesian inference","version":2},"cited_work":{"arxiv_id":"2401.11138","doi":null,"metadata_source":"pith","pith_arxiv_id":"2401.11138","snapshot_observed_at":"2026-08-06T23:21:58.628544Z","title":"Comparison of $\\Lambda$CDM and $R_h = ct$ with updated galaxy cluster $f_{gas}$ measurements using Bayesian inference","venue":"astro-ph.CO","work_id":"7baf6020-2da5-44bd-8fa9-478fc2f0aa78","year":2024},"citing_paper":{"arxiv_id":"2506.18445","last_updated":"2025-06-23T09:30:19Z","snapshot_observed_at":"2026-08-08T19:03:41.502084Z","submitted_at":"2025-06-23T09:30:19Z","title":"Comparison of $R_h=ct$ and $\\Lambda$CDM using DESI DR1 measurements","version":1},"reference_index":38,"source":"pdf_text","source_observed_at":"2026-08-06T23:21:54.024747Z"},"links":{"cited_paper":"/paper/2401.11138","citing_paper":"/paper/2506.18445"},"observation_digest":"sha256:38e1e1ae87a18e1003d466b2dfc0e4be2d7a38b796bb79065cac250f4084a9f2","observation_id":"caf4eb92-bc94-4da8-a5e7-75597bce36e5","resolution":{"observed_at":"2026-08-06T23:21:58.776015Z","resolver_source":"local_arxiv","status":"verified_exact"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-08T06:32:00.761636+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-08T06:32:00.761636+00:00","source":"crossref"},{"observed_at":"2026-08-08T06:31:55.24221+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":{"arxiv_id":"1503.05052","last_updated":"2016-10-25T02:34:38Z","snapshot_observed_at":"2026-07-06T04:12:16.293283Z","submitted_at":"2015-03-16T18:24:58Z","title":"Alcock-Paczynski Test with Model-independent BAO Data","version":3},"cited_work":{"arxiv_id":"1503.05052","doi":null,"metadata_source":"pith","pith_arxiv_id":"1503.05052","snapshot_observed_at":"2026-08-06T23:21:58.182603Z","title":"Alcock-Paczynski Test with Model-independent BAO Data","venue":"astro-ph.CO","work_id":"3b36980f-79dd-4838-beb7-761d3d9ae31b","year":2015},"citing_paper":{"arxiv_id":"2506.18445","last_updated":"2025-06-23T09:30:19Z","snapshot_observed_at":"2026-08-08T19:03:41.502084Z","submitted_at":"2025-06-23T09:30:19Z","title":"Comparison of $R_h=ct$ and $\\Lambda$CDM using DESI DR1 measurements","version":1},"reference_index":39,"source":"pdf_text","source_observed_at":"2026-08-06T23:21:54.194751Z"},"links":{"cited_paper":"/paper/1503.05052","citing_paper":"/paper/2506.18445"},"observation_digest":"sha256:6ed1cdc9cb2a18fc2883f8177da305ccb6c7e4549c65b02d2d2560dc95dc6393","observation_id":"db400a57-c75e-46d6-beba-55e010938aed","resolution":{"observed_at":"2026-08-06T23:21:58.384746Z","resolver_source":"local_arxiv","status":"verified_exact"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-08T06:32:00.761636+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-08T06:32:00.761636+00:00","source":"crossref"},{"observed_at":"2026-08-08T06:31:55.24221+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":{"arxiv_id":"2008.12628","last_updated":"2020-08-28T12:43:32Z","snapshot_observed_at":"2026-08-04T12:43:27.577560Z","submitted_at":"2020-08-28T12:43:32Z","title":"Assessing Cosmic Acceleration with the Alcock-Paczynski Effect in the SDSS-IV Quasar Catalog","version":1},"cited_work":{"arxiv_id":"2008.12628","doi":null,"metadata_source":"pith","pith_arxiv_id":"2008.12628","snapshot_observed_at":"2026-08-06T23:21:57.727949Z","title":"Assessing Cosmic Acceleration with the Alcock-Paczynski Effect in the SDSS-IV Quasar Catalog","venue":"astro-ph.CO","work_id":"980c40d1-7370-46f9-9294-a104b825663d","year":2020},"citing_paper":{"arxiv_id":"2506.18445","last_updated":"2025-06-23T09:30:19Z","snapshot_observed_at":"2026-08-08T19:03:41.502084Z","submitted_at":"2025-06-23T09:30:19Z","title":"Comparison of $R_h=ct$ and $\\Lambda$CDM using DESI DR1 measurements","version":1},"reference_index":40,"source":"pdf_text","source_observed_at":"2026-08-06T23:21:54.415107Z"},"links":{"cited_paper":"/paper/2008.12628","citing_paper":"/paper/2506.18445"},"observation_digest":"sha256:8df3a72d0c90509f56527c5f978a7eafe2457850310a5fce6f4707a0383c569d","observation_id":"d1164e4f-d5d2-478f-9407-87446a41e9e8","resolution":{"observed_at":"2026-08-06T23:21:57.864816Z","resolver_source":"local_arxiv","status":"verified_exact"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-08T06:32:00.761636+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-08T06:32:00.761636+00:00","source":"crossref"},{"observed_at":"2026-08-08T06:31:55.24221+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":{"arxiv_id":"2204.02186","last_updated":"2022-04-06T12:32:33Z","snapshot_observed_at":"2026-08-07T18:11:28.646457Z","submitted_at":"2022-04-01T12:42:55Z","title":"Model Selection using Baryon Acoustic Oscillations in the Final SDSS-IV Release","version":2},"cited_work":{"arxiv_id":"2204.02186","doi":null,"metadata_source":"pith","pith_arxiv_id":"2204.02186","snapshot_observed_at":"2026-08-06T23:21:57.404756Z","title":"Model Selection using Baryon Acoustic Oscillations in the Final SDSS-IV Release","venue":"astro-ph.CO","work_id":"fd3c31eb-505c-426c-ba21-7bfaeb458750","year":2022},"citing_paper":{"arxiv_id":"2506.18445","last_updated":"2025-06-23T09:30:19Z","snapshot_observed_at":"2026-08-08T19:03:41.502084Z","submitted_at":"2025-06-23T09:30:19Z","title":"Comparison of $R_h=ct$ and $\\Lambda$CDM using DESI DR1 measurements","version":1},"reference_index":41,"source":"pdf_text","source_observed_at":"2026-08-06T23:21:54.554751Z"},"links":{"cited_paper":"/paper/2204.02186","citing_paper":"/paper/2506.18445"},"observation_digest":"sha256:1b5b1507a7a63b72e2f0b2e3610f876b294bdceebf183861c41bd4951bb00759","observation_id":"fc14c68a-6d98-43bd-a038-3848e95a39f1","resolution":{"observed_at":"2026-08-06T23:21:57.545473Z","resolver_source":"local_arxiv","status":"verified_exact"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-08T06:32:00.761636+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-08T06:32:00.761636+00:00","source":"crossref"},{"observed_at":"2026-08-08T06:31:55.24221+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":{"arxiv_id":"2309.00662","last_updated":"2023-09-01T13:35:56Z","snapshot_observed_at":"2026-08-04T16:35:36.648116Z","submitted_at":"2023-09-01T13:35:56Z","title":"Model Selection with Baryonic Acoustic Oscillations in the Lyman-alpha Forest","version":1},"cited_work":{"arxiv_id":"2309.00662","doi":null,"metadata_source":"pith","pith_arxiv_id":"2309.00662","snapshot_observed_at":"2026-08-06T23:21:56.774761Z","title":"Model Selection with Baryonic Acoustic Oscillations in the Lyman-alpha Forest","venue":"astro-ph.CO","work_id":"158570b3-e478-44ab-af53-86b448f67dda","year":2023},"citing_paper":{"arxiv_id":"2506.18445","last_updated":"2025-06-23T09:30:19Z","snapshot_observed_at":"2026-08-08T19:03:41.502084Z","submitted_at":"2025-06-23T09:30:19Z","title":"Comparison of $R_h=ct$ and $\\Lambda$CDM using DESI DR1 measurements","version":1},"reference_index":42,"source":"pdf_text","source_observed_at":"2026-08-06T23:21:54.924820Z"},"links":{"cited_paper":"/paper/2309.00662","citing_paper":"/paper/2506.18445"},"observation_digest":"sha256:45188cbd3eb1e145063ffe8b626862df1b98fe0d76c07547e92d4110a2105b60","observation_id":"bb6e72df-5d65-47a4-be2f-45f3108bb8d5","resolution":{"observed_at":"2026-08-06T23:21:57.164748Z","resolver_source":"local_arxiv","status":"metadata_mismatch"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-08T06:32:00.761636+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-08T06:32:00.761636+00:00","source":"crossref"},{"observed_at":"2026-08-08T06:31:55.24221+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":{"arxiv_id":"2503.14738","last_updated":"2025-10-09T16:45:28Z","snapshot_observed_at":"2026-07-06T02:11:23.670680Z","submitted_at":"2025-03-18T21:14:12Z","title":"DESI DR2 Results II: Measurements of Baryon Acoustic Oscillations and Cosmological Constraints","version":3},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2503.14738","snapshot_observed_at":"2026-08-06T23:21:55.144833Z","title":"Abdul-Karim, J","venue":null,"work_id":null,"year":2025},"citing_paper":{"arxiv_id":"2506.18445","last_updated":"2025-06-23T09:30:19Z","snapshot_observed_at":"2026-08-08T19:03:41.502084Z","submitted_at":"2025-06-23T09:30:19Z","title":"Comparison of $R_h=ct$ and $\\Lambda$CDM using DESI DR1 measurements","version":1},"reference_index":43,"source":"pdf_text","source_observed_at":"2026-08-06T23:21:55.144833Z"},"links":{"cited_paper":"/paper/2503.14738","citing_paper":"/paper/2506.18445"},"observation_digest":"sha256:5f10fb6311f29a3b1f44154d85e523c2e413a717c571a30f488d408d415b0f75","observation_id":"0facfce0-94f1-4597-bb28-e50c99bb775d","resolution":{"observed_at":"2026-08-06T23:21:55.144833Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2404.03002","last_updated":"2024-11-04T16:43:36Z","snapshot_observed_at":"2026-07-06T17:55:21.083912Z","submitted_at":"2024-04-03T18:41:51Z","title":"DESI 2024 VI: Cosmological Constraints from the Measurements of Baryon Acoustic Oscillations","version":3},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2404.03002","snapshot_observed_at":"2026-08-06T23:21:55.404825Z","title":null,"venue":null,"work_id":null,"year":2025},"citing_paper":{"arxiv_id":"2506.18445","last_updated":"2025-06-23T09:30:19Z","snapshot_observed_at":"2026-08-08T19:03:41.502084Z","submitted_at":"2025-06-23T09:30:19Z","title":"Comparison of $R_h=ct$ and $\\Lambda$CDM using DESI DR1 measurements","version":1},"reference_index":44,"source":"pdf_text","source_observed_at":"2026-08-06T23:21:55.404825Z"},"links":{"cited_paper":"/paper/2404.03002","citing_paper":"/paper/2506.18445"},"observation_digest":"sha256:eda2d240cc486d5d8d6df652132bf8786df63ad61f3d95317d5d168e13fcdc04","observation_id":"f424a87f-a00a-4fda-956a-b6e014275fc5","resolution":{"observed_at":"2026-08-06T23:21:55.404825Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"1701.01467","last_updated":"2017-01-05T20:23:53Z","snapshot_observed_at":"2026-08-03T11:30:18.533693Z","submitted_at":"2017-01-05T20:23:53Z","title":"Bayesian Methods in Cosmology","version":1},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"1701.01467","snapshot_observed_at":"2026-08-06T23:21:55.538145Z","title":"Trotta, ArXiv e-prints (2017), 1701.01467","venue":null,"work_id":null,"year":2017},"citing_paper":{"arxiv_id":"2506.18445","last_updated":"2025-06-23T09:30:19Z","snapshot_observed_at":"2026-08-08T19:03:41.502084Z","submitted_at":"2025-06-23T09:30:19Z","title":"Comparison of $R_h=ct$ and $\\Lambda$CDM using DESI DR1 measurements","version":1},"reference_index":45,"source":"pdf_text","source_observed_at":"2026-08-06T23:21:55.538145Z"},"links":{"cited_paper":"/paper/1701.01467","citing_paper":"/paper/2506.18445"},"observation_digest":"sha256:b2080b71ef806080102394fdf63d230bcdaf3e1b1537b84fe59875d48f8b6d18","observation_id":"ac64b9d3-2020-48c6-8ce4-1296c443dfef","resolution":{"observed_at":"2026-08-06T23:21:55.538145Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"1901.07726","last_updated":"2019-05-10T11:51:42Z","snapshot_observed_at":"2026-07-06T07:28:25.420986Z","submitted_at":"2019-01-23T05:14:06Z","title":"On Model Selection in Cosmology","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"1901.07726","snapshot_observed_at":"2026-08-06T23:21:55.692758Z","title":"Kerscher and J","venue":null,"work_id":null,"year":2019},"citing_paper":{"arxiv_id":"2506.18445","last_updated":"2025-06-23T09:30:19Z","snapshot_observed_at":"2026-08-08T19:03:41.502084Z","submitted_at":"2025-06-23T09:30:19Z","title":"Comparison of $R_h=ct$ and $\\Lambda$CDM using DESI DR1 measurements","version":1},"reference_index":46,"source":"pdf_text","source_observed_at":"2026-08-06T23:21:55.692758Z"},"links":{"cited_paper":"/paper/1901.07726","citing_paper":"/paper/2506.18445"},"observation_digest":"sha256:e5551c5b690a570eb3d8d11b96fa44c36b1e9bd89705a425cf4bb714c6ed6a85","observation_id":"3b06b3dc-5a8d-4a0c-a312-19de5811b46f","resolution":{"observed_at":"2026-08-06T23:21:55.692758Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"1706.01629","last_updated":"2017-06-06T07:09:25Z","snapshot_observed_at":"2026-08-03T00:59:20.184774Z","submitted_at":"2017-06-06T07:09:25Z","title":"Markov Chain Monte Carlo Methods for Bayesian Data Analysis in Astronomy","version":1},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"1706.01629","snapshot_observed_at":"2026-08-06T23:21:55.744751Z","title":"Sharma, Ann","venue":null,"work_id":null,"year":2017},"citing_paper":{"arxiv_id":"2506.18445","last_updated":"2025-06-23T09:30:19Z","snapshot_observed_at":"2026-08-08T19:03:41.502084Z","submitted_at":"2025-06-23T09:30:19Z","title":"Comparison of $R_h=ct$ and $\\Lambda$CDM using DESI DR1 measurements","version":1},"reference_index":47,"source":"pdf_text","source_observed_at":"2026-08-06T23:21:55.744751Z"},"links":{"cited_paper":"/paper/1706.01629","citing_paper":"/paper/2506.18445"},"observation_digest":"sha256:e43db8680a335d683301303006727de3ef0f5d00cdaa9c490819bdb5f5b6cebd","observation_id":"0981913d-9082-47d4-8e3e-db4cb4b86c2d","resolution":{"observed_at":"2026-08-06T23:21:55.744751Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2003.10127","last_updated":"2020-06-07T15:09:50Z","snapshot_observed_at":"2026-08-07T14:33:46.168767Z","submitted_at":"2020-03-23T08:25:06Z","title":"Model Comparison tests of modified gravity from the E\\\"ot-Wash experiment","version":3},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2003.10127","snapshot_observed_at":"2026-08-06T23:21:55.854834Z","title":"Krishak and S","venue":null,"work_id":null,"year":2020},"citing_paper":{"arxiv_id":"2506.18445","last_updated":"2025-06-23T09:30:19Z","snapshot_observed_at":"2026-08-08T19:03:41.502084Z","submitted_at":"2025-06-23T09:30:19Z","title":"Comparison of $R_h=ct$ and $\\Lambda$CDM using DESI DR1 measurements","version":1},"reference_index":48,"source":"pdf_text","source_observed_at":"2026-08-06T23:21:55.854834Z"},"links":{"cited_paper":"/paper/2003.10127","citing_paper":"/paper/2506.18445"},"observation_digest":"sha256:2c4808f55c67edbdfa0f7f3b0bd15b6dbdff13ffc5c53369e2e305823e539ed7","observation_id":"9439b39d-41ff-410e-95cc-2967ec3cad54","resolution":{"observed_at":"2026-08-06T23:21:55.854834Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"1906.03035","last_updated":"2019-06-07T12:09:01Z","snapshot_observed_at":"2026-08-03T15:38:29.347987Z","submitted_at":"2019-06-07T12:09:01Z","title":"The Impact of the Fiducial Cosmology Assumption on BAO Cosmological Parameter Inference","version":1},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"1906.03035","snapshot_observed_at":"2026-08-06T23:21:55.956299Z","title":"Carter, F","venue":null,"work_id":null,"year":2020},"citing_paper":{"arxiv_id":"2506.18445","last_updated":"2025-06-23T09:30:19Z","snapshot_observed_at":"2026-08-08T19:03:41.502084Z","submitted_at":"2025-06-23T09:30:19Z","title":"Comparison of $R_h=ct$ and $\\Lambda$CDM using DESI DR1 measurements","version":1},"reference_index":49,"source":"pdf_text","source_observed_at":"2026-08-06T23:21:55.956299Z"},"links":{"cited_paper":"/paper/1906.03035","citing_paper":"/paper/2506.18445"},"observation_digest":"sha256:a0d06cf5524c3daa1c852fd78ccd4e4e9470332b59c68fc04be6ff9f01313d0a","observation_id":"419f73c3-8c09-4945-9b14-27aec8452a53","resolution":{"observed_at":"2026-08-06T23:21:55.956299Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"1904.02180","last_updated":"2019-04-03T18:04:57Z","snapshot_observed_at":"2026-07-06T07:43:43.696691Z","submitted_at":"2019-04-03T18:04:57Z","title":"dynesty: A Dynamic Nested Sampling Package for Estimating Bayesian Posteriors and Evidences","version":1},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"1904.02180","snapshot_observed_at":"2026-08-06T23:21:56.064746Z","title":null,"venue":null,"work_id":null,"year":2020},"citing_paper":{"arxiv_id":"2506.18445","last_updated":"2025-06-23T09:30:19Z","snapshot_observed_at":"2026-08-08T19:03:41.502084Z","submitted_at":"2025-06-23T09:30:19Z","title":"Comparison of $R_h=ct$ and $\\Lambda$CDM using DESI DR1 measurements","version":1},"reference_index":50,"source":"pdf_text","source_observed_at":"2026-08-06T23:21:56.064746Z"},"links":{"cited_paper":"/paper/1904.02180","citing_paper":"/paper/2506.18445"},"observation_digest":"sha256:5e619e07df0815d1ffab20be2e39e280abae84e353e8b7a2ec0f4eb4a0c5d0e6","observation_id":"37b85661-71b1-45ca-b346-61363e533d54","resolution":{"observed_at":"2026-08-06T23:21:56.064746Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}}],"paper":{"arxiv_id":"2506.18445","last_updated":"2025-06-23T09:30:19Z","latest_version":1,"primary_category":"astro-ph.CO","snapshot_observed_at":"2026-08-08T19:03:41.502084Z","submitted_at":"2025-06-23T09:30:19Z","title":"Comparison of $R_h=ct$ and $\\Lambda$CDM using DESI DR1 measurements"},"reference_resolution":{"displayed":50,"state_counts":{"malformed_identifier":0,"metadata_mismatch":5,"parse_uncertain":0,"unresolved":30,"verified_exact":14,"verified_fuzzy":1},"total_outbound_references":50},"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":"2026-08-08T06:32:00.761636+00:00","source":"crossref"},{"observed_at":"2026-08-08T06:31:55.24221+00:00","source":"retraction_watch"}],"thesis":"As of 9 August 2026, this Paper Citation Record lists 50 of 50 outbound references and 0 inbound Pith citation observations for arXiv:2506.18445."}