{"as_of":"2026-08-21T06:58:00Z","caps":{"database_statements":6,"inbound":100,"outbound":100},"context_digest":"sha256:a4a733b89e18f847624c4b1740d3ea3c6eceab394866aecd51b73fdf9a00aaef","coverage":[{"denominator":78,"lane":"reference_resolution","note":"Typed states for the displayed outbound observations.","records_observed":78,"source":"paper_references, paper_reference_links","source_observed_at":"2026-08-04T00:32:31.443709Z","state":"measured"},{"denominator":78,"lane":"standing_notices","note":"One-hop event checks from named stored sources.","records_observed":78,"source":"scholarly_work_events, retraction_status_cache","source_observed_at":"2026-08-21T06:32:19.484+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/2511.00789/citation-record","integrity":"/paper/2511.00789/integrity","json":"/paper/2511.00789/citation-record.json","paper":"/paper/2511.00789"},"outbound":[{"citation":{"cited_paper":{"arxiv_id":"1807.06209","last_updated":"2021-08-09T10:43:18Z","snapshot_observed_at":"2026-08-15T17:00:11.410484Z","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":"2026-08-04T00:32:24.266554Z","title":"Aghanim, Y","venue":null,"work_id":null,"year":2018},"citing_paper":{"arxiv_id":"2511.00789","last_updated":"2026-06-04T04:14:37Z","snapshot_observed_at":"2026-08-15T06:24:02.254376Z","submitted_at":"2025-11-02T04:00:48Z","title":"A cosmographic analysis using DESI-DR2 and strong lensing: II. Distance Ratio measurements","version":2},"reference_index":1,"source":"pdf_text","source_observed_at":"2026-08-04T00:32:24.266554Z"},"links":{"cited_paper":"/paper/1807.06209","citing_paper":"/paper/2511.00789"},"observation_digest":"sha256:93d11fb02528beb09d7b06b8828a1d804ba09c1a1835900c57b74a7ea257e18c","observation_id":"76eac845-7016-4d70-a2d4-501f843c92e7","resolution":{"observed_at":"2026-08-04T00:32:24.266554Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2112.04510","last_updated":"2022-07-18T20:33:57Z","snapshot_observed_at":"2026-07-06T12:16:41.817858Z","submitted_at":"2021-12-08T19:00:02Z","title":"A Comprehensive Measurement of the Local Value of the Hubble Constant with 1 km/s/Mpc Uncertainty from the Hubble Space Telescope and the SH0ES Team","version":3},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2112.04510","snapshot_observed_at":"2026-08-04T00:32:24.407337Z","title":"Riess, W","venue":null,"work_id":null,"year":2022},"citing_paper":{"arxiv_id":"2511.00789","last_updated":"2026-06-04T04:14:37Z","snapshot_observed_at":"2026-08-15T06:24:02.254376Z","submitted_at":"2025-11-02T04:00:48Z","title":"A cosmographic analysis using DESI-DR2 and strong lensing: II. Distance Ratio measurements","version":2},"reference_index":2,"source":"pdf_text","source_observed_at":"2026-08-04T00:32:24.407337Z"},"links":{"cited_paper":"/paper/2112.04510","citing_paper":"/paper/2511.00789"},"observation_digest":"sha256:f153368a3bbe76455fc1b4f33908b9e2385454308a292d25fa92dbae7613d4d8","observation_id":"3696c52d-3d46-42e9-9387-a8252a0d6757","resolution":{"observed_at":"2026-08-04T00:32:24.407337Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"1911.02087","last_updated":"2019-11-05T21:14:06Z","snapshot_observed_at":"2026-07-31T14:26:34.353301Z","submitted_at":"2019-11-05T21:14:06Z","title":"Planck evidence for a closed Universe and a possible crisis for cosmology","version":1},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"1911.02087","snapshot_observed_at":"2026-08-04T00:32:24.515121Z","title":"Di Valentino, A","venue":null,"work_id":null,"year":2020},"citing_paper":{"arxiv_id":"2511.00789","last_updated":"2026-06-04T04:14:37Z","snapshot_observed_at":"2026-08-15T06:24:02.254376Z","submitted_at":"2025-11-02T04:00:48Z","title":"A cosmographic analysis using DESI-DR2 and strong lensing: II. Distance Ratio measurements","version":2},"reference_index":3,"source":"pdf_text","source_observed_at":"2026-08-04T00:32:24.515121Z"},"links":{"cited_paper":"/paper/1911.02087","citing_paper":"/paper/2511.00789"},"observation_digest":"sha256:a506d520fb85395f24da8dac4be06a952dc5181d7e2376e30fe5f3d6010ab9f2","observation_id":"8b401011-e86e-4879-969c-8ece706dde57","resolution":{"observed_at":"2026-08-04T00:32:24.515121Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"1908.09139","last_updated":"2019-08-24T13:56:59Z","snapshot_observed_at":"2026-08-15T11:58:31.212016Z","submitted_at":"2019-08-24T13:56:59Z","title":"Curvature tension: evidence for a closed universe","version":1},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"1908.09139","snapshot_observed_at":"2026-08-04T00:32:24.654297Z","title":"Handley,Curvature tension: Evidence for a closed universe,Phys","venue":null,"work_id":null,"year":2021},"citing_paper":{"arxiv_id":"2511.00789","last_updated":"2026-06-04T04:14:37Z","snapshot_observed_at":"2026-08-15T06:24:02.254376Z","submitted_at":"2025-11-02T04:00:48Z","title":"A cosmographic analysis using DESI-DR2 and strong lensing: II. Distance Ratio measurements","version":2},"reference_index":4,"source":"pdf_text","source_observed_at":"2026-08-04T00:32:24.654297Z"},"links":{"cited_paper":"/paper/1908.09139","citing_paper":"/paper/2511.00789"},"observation_digest":"sha256:7d6fb32a801e2849e63e29acf96dd22f92fb8d8af0dc4925f7fc28dfda4912f9","observation_id":"9461ef3a-e079-447b-8282-a05b7ba59480","resolution":{"observed_at":"2026-08-04T00:32:24.654297Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":null,"snapshot_observed_at":"2026-08-04T00:32:24.767981Z","title":"Weinberg,The cosmological constant problem,Reviews of Modern Physics61(1989) 1","venue":null,"work_id":null,"year":1989},"citing_paper":{"arxiv_id":"2511.00789","last_updated":"2026-06-04T04:14:37Z","snapshot_observed_at":"2026-08-15T06:24:02.254376Z","submitted_at":"2025-11-02T04:00:48Z","title":"A cosmographic analysis using DESI-DR2 and strong lensing: II. Distance Ratio measurements","version":2},"reference_index":5,"source":"pdf_text","source_observed_at":"2026-08-04T00:32:24.767981Z"},"links":{"citing_paper":"/paper/2511.00789"},"observation_digest":"sha256:dbdc020a4e17d4c23fc6128a7f63ccb46ea18c155b500ce08411b50d92b7b821","observation_id":"8625db5f-b775-4c0a-910f-091ea6036f7e","resolution":{"observed_at":"2026-08-04T00:32:24.767981Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"astro-ph/9807002","last_updated":"1998-10-21T23:30:11Z","snapshot_observed_at":"2026-08-18T02:33:38.872236Z","submitted_at":"1998-07-01T00:38:31Z","title":"Quintessence, Cosmic Coincidence, and the Cosmological Constant","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"astro-ph/9807002","snapshot_observed_at":"2026-08-04T00:32:24.873314Z","title":"Zlatev, L","venue":null,"work_id":null,"year":1999},"citing_paper":{"arxiv_id":"2511.00789","last_updated":"2026-06-04T04:14:37Z","snapshot_observed_at":"2026-08-15T06:24:02.254376Z","submitted_at":"2025-11-02T04:00:48Z","title":"A cosmographic analysis using DESI-DR2 and strong lensing: II. Distance Ratio measurements","version":2},"reference_index":6,"source":"pdf_text","source_observed_at":"2026-08-04T00:32:24.873314Z"},"links":{"cited_paper":"/paper/astro-ph/9807002","citing_paper":"/paper/2511.00789"},"observation_digest":"sha256:2cce9e9c5211abf18af985d72cf0d9b3db02e75e770d3cec1f7d2971687cb2fc","observation_id":"72bdc439-82e2-4009-8bf5-44501833bdce","resolution":{"observed_at":"2026-08-04T00:32:24.873314Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"astro-ph/0005265","last_updated":"2000-05-12T03:24:49Z","snapshot_observed_at":"2026-07-06T02:11:23.670680Z","submitted_at":"2000-05-12T03:24:49Z","title":"The Cosmological Constant Problems (Talk given at Dark Matter 2000, February, 2000)","version":1},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"astro-ph/0005265","snapshot_observed_at":"2026-08-04T00:32:24.981306Z","title":"Weinberg,The Cosmological Constant Problems (Talk given at Dark Matter 2000, February, 2000),arXiv e-prints(2000) astro [astro-ph/0005265]","venue":null,"work_id":null,"year":2000},"citing_paper":{"arxiv_id":"2511.00789","last_updated":"2026-06-04T04:14:37Z","snapshot_observed_at":"2026-08-15T06:24:02.254376Z","submitted_at":"2025-11-02T04:00:48Z","title":"A cosmographic analysis using DESI-DR2 and strong lensing: II. Distance Ratio measurements","version":2},"reference_index":7,"source":"pdf_text","source_observed_at":"2026-08-04T00:32:24.981306Z"},"links":{"cited_paper":"/paper/astro-ph/0005265","citing_paper":"/paper/2511.00789"},"observation_digest":"sha256:62c4aa840bc49060aff3f28945c47631dbc29283e4064ae5b929c65597994335","observation_id":"77958dfa-6cd6-439f-8055-645b3b6ab6a4","resolution":{"observed_at":"2026-08-04T00:32:24.981306Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"1412.4976","last_updated":"2015-09-09T13:06:00Z","snapshot_observed_at":"2026-08-15T03:05:16.587688Z","submitted_at":"2014-12-16T12:35:02Z","title":"New test of the FLRW metric using the distance sum rule","version":3},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"1412.4976","snapshot_observed_at":"2026-08-04T00:32:25.086503Z","title":"R¨ as¨ anen, K","venue":null,"work_id":null,"year":2015},"citing_paper":{"arxiv_id":"2511.00789","last_updated":"2026-06-04T04:14:37Z","snapshot_observed_at":"2026-08-15T06:24:02.254376Z","submitted_at":"2025-11-02T04:00:48Z","title":"A cosmographic analysis using DESI-DR2 and strong lensing: II. Distance Ratio measurements","version":2},"reference_index":8,"source":"pdf_text","source_observed_at":"2026-08-04T00:32:25.086503Z"},"links":{"cited_paper":"/paper/1412.4976","citing_paper":"/paper/2511.00789"},"observation_digest":"sha256:88c8d88ad8cbc939fec913b43cfc682de0d7ba36482d16815080b5c0e2539643","observation_id":"8de9bda1-e7f7-4290-8da4-e4618529b9c0","resolution":{"observed_at":"2026-08-04T00:32:25.086503Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"1905.09781","last_updated":"2019-12-02T18:17:16Z","snapshot_observed_at":"2026-08-18T20:22:45.085483Z","submitted_at":"2019-05-23T17:12:01Z","title":"Model-independent determination of $H_0$ and $\\Omega_{K0}$ from strong lensing and type Ia supernovae","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"1905.09781","snapshot_observed_at":"2026-08-04T00:32:25.164561Z","title":"Collett, F","venue":null,"work_id":null,"year":2019},"citing_paper":{"arxiv_id":"2511.00789","last_updated":"2026-06-04T04:14:37Z","snapshot_observed_at":"2026-08-15T06:24:02.254376Z","submitted_at":"2025-11-02T04:00:48Z","title":"A cosmographic analysis using DESI-DR2 and strong lensing: II. Distance Ratio measurements","version":2},"reference_index":9,"source":"pdf_text","source_observed_at":"2026-08-04T00:32:25.164561Z"},"links":{"cited_paper":"/paper/1905.09781","citing_paper":"/paper/2511.00789"},"observation_digest":"sha256:acbb2d8e2c18daaff844e80400ccd843f9c589b7e9a5ab2a7a591da17ce4135b","observation_id":"71b1950e-1eed-4387-9f65-60edd9168118","resolution":{"observed_at":"2026-08-04T00:32:25.164561Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2302.13887","last_updated":"2023-02-27T15:33:07Z","snapshot_observed_at":"2026-08-18T20:25:56.354184Z","submitted_at":"2023-02-27T15:33:07Z","title":"Model-Independent Determination of $H_0$ and $\\Omega_{K,0}$ using Time-Delay Galaxy Lenses and Gamma-Ray Bursts","version":1},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2302.13887","snapshot_observed_at":"2026-08-04T00:32:25.240814Z","title":"Du, J.-J","venue":null,"work_id":null,"year":2023},"citing_paper":{"arxiv_id":"2511.00789","last_updated":"2026-06-04T04:14:37Z","snapshot_observed_at":"2026-08-15T06:24:02.254376Z","submitted_at":"2025-11-02T04:00:48Z","title":"A cosmographic analysis using DESI-DR2 and strong lensing: II. Distance Ratio measurements","version":2},"reference_index":10,"source":"pdf_text","source_observed_at":"2026-08-04T00:32:25.240814Z"},"links":{"cited_paper":"/paper/2302.13887","citing_paper":"/paper/2511.00789"},"observation_digest":"sha256:0fbb2b9d19d978d38bccc6d661ec64181d5c1380fa15f86d6c20d7b0b3a002dd","observation_id":"09235172-a661-4972-b9e1-8f03ec45a9ec","resolution":{"observed_at":"2026-08-04T00:32:25.240814Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"1904.01744","last_updated":"2019-04-03T02:22:17Z","snapshot_observed_at":"2026-08-18T20:29:20.217364Z","submitted_at":"2019-04-03T02:22:17Z","title":"Constraints on cosmic curvature with lensing time delays and gravitational waves","version":1},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"1904.01744","snapshot_observed_at":"2026-08-04T00:32:25.338862Z","title":"Liao,Constraints on cosmic curvature with lensing time delays and gravitational waves, Phys","venue":null,"work_id":null,"year":2019},"citing_paper":{"arxiv_id":"2511.00789","last_updated":"2026-06-04T04:14:37Z","snapshot_observed_at":"2026-08-15T06:24:02.254376Z","submitted_at":"2025-11-02T04:00:48Z","title":"A cosmographic analysis using DESI-DR2 and strong lensing: II. Distance Ratio measurements","version":2},"reference_index":11,"source":"pdf_text","source_observed_at":"2026-08-04T00:32:25.338862Z"},"links":{"cited_paper":"/paper/1904.01744","citing_paper":"/paper/2511.00789"},"observation_digest":"sha256:1460628650a1c0cf36fb93eb08632f5dd7b885f07b8461462fa91ed267008742","observation_id":"db1a1e29-e9df-4e5a-944e-b9e6950a9063","resolution":{"observed_at":"2026-08-04T00:32:25.338862Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"1003.5567","last_updated":"2010-03-29T15:24:14Z","snapshot_observed_at":"2026-08-15T05:23:01.986484Z","submitted_at":"2010-03-29T15:24:14Z","title":"Strong Lensing by Galaxies","version":1},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"1003.5567","snapshot_observed_at":"2026-08-04T00:32:25.451358Z","title":"Treu,Strong Lensing by Galaxies,Ann","venue":null,"work_id":null,"year":2010},"citing_paper":{"arxiv_id":"2511.00789","last_updated":"2026-06-04T04:14:37Z","snapshot_observed_at":"2026-08-15T06:24:02.254376Z","submitted_at":"2025-11-02T04:00:48Z","title":"A cosmographic analysis using DESI-DR2 and strong lensing: II. Distance Ratio measurements","version":2},"reference_index":12,"source":"pdf_text","source_observed_at":"2026-08-04T00:32:25.451358Z"},"links":{"cited_paper":"/paper/1003.5567","citing_paper":"/paper/2511.00789"},"observation_digest":"sha256:c58c5d0d022690b197ee52e2686e8fc4d19b06f563be2ad6e12cf3065817093d","observation_id":"a26cea31-fed8-4905-98d8-d5a29c21f3d4","resolution":{"observed_at":"2026-08-04T00:32:25.451358Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":null,"snapshot_observed_at":"2026-08-04T00:32:25.523569Z","title":"Refsdal,On the possibility of determining Hubble’s parameter and the masses of galaxies from the gravitational lens effect,Mon","venue":null,"work_id":null,"year":1964},"citing_paper":{"arxiv_id":"2511.00789","last_updated":"2026-06-04T04:14:37Z","snapshot_observed_at":"2026-08-15T06:24:02.254376Z","submitted_at":"2025-11-02T04:00:48Z","title":"A cosmographic analysis using DESI-DR2 and strong lensing: II. Distance Ratio measurements","version":2},"reference_index":13,"source":"pdf_text","source_observed_at":"2026-08-04T00:32:25.523569Z"},"links":{"citing_paper":"/paper/2511.00789"},"observation_digest":"sha256:bc282d842b50bbc7efe1a6b2a72fe7a4d76808e9f1e7ce5eccfc1ca5284018a1","observation_id":"629107aa-733d-4752-8ab9-ac8c786c80d8","resolution":{"observed_at":"2026-08-04T00:32:25.523569Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2210.10833","last_updated":"2024-05-06T16:16:29Z","snapshot_observed_at":"2026-08-18T20:21:59.430920Z","submitted_at":"2022-10-19T18:53:31Z","title":"Time-Delay Cosmography: Measuring the Hubble Constant and other cosmological parameters with strong gravitational lensing","version":4},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2210.10833","snapshot_observed_at":"2026-08-04T00:32:25.579515Z","title":"Birrer, M","venue":null,"work_id":null,"year":2024},"citing_paper":{"arxiv_id":"2511.00789","last_updated":"2026-06-04T04:14:37Z","snapshot_observed_at":"2026-08-15T06:24:02.254376Z","submitted_at":"2025-11-02T04:00:48Z","title":"A cosmographic analysis using DESI-DR2 and strong lensing: II. Distance Ratio measurements","version":2},"reference_index":14,"source":"pdf_text","source_observed_at":"2026-08-04T00:32:25.579515Z"},"links":{"cited_paper":"/paper/2210.10833","citing_paper":"/paper/2511.00789"},"observation_digest":"sha256:985a944349a42057861114f0d5514b710e3ed3775bf7cb7dd99e89ba3ba08161","observation_id":"37485474-22a2-4fc5-b330-4f7c985850dd","resolution":{"observed_at":"2026-08-04T00:32:25.579515Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"astro-ph/0202342","last_updated":"2002-04-10T03:06:59Z","snapshot_observed_at":"2026-07-07T00:25:08.568215Z","submitted_at":"2002-02-18T23:59:14Z","title":"The internal structure and formation of early-type galaxies: the gravitational--lens system MG2016+112 at z=1.004","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"astro-ph/0202342","snapshot_observed_at":"2026-08-04T00:32:25.738745Z","title":"Treu and L.V.E","venue":null,"work_id":null,"year":2016},"citing_paper":{"arxiv_id":"2511.00789","last_updated":"2026-06-04T04:14:37Z","snapshot_observed_at":"2026-08-15T06:24:02.254376Z","submitted_at":"2025-11-02T04:00:48Z","title":"A cosmographic analysis using DESI-DR2 and strong lensing: II. Distance Ratio measurements","version":2},"reference_index":15,"source":"pdf_text","source_observed_at":"2026-08-04T00:32:25.738745Z"},"links":{"cited_paper":"/paper/astro-ph/0202342","citing_paper":"/paper/2511.00789"},"observation_digest":"sha256:00963b43ffb5ebe753813e8b494147a3bed0e753cfd03c49db8dfd3beeee12a0","observation_id":"cfc6e03b-2dc6-44ee-9bbf-aad9625f3e2c","resolution":{"observed_at":"2026-08-04T00:32:25.738745Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"astro-ph/0205281","last_updated":"2002-10-02T21:21:39Z","snapshot_observed_at":"2026-07-07T00:26:30.195508Z","submitted_at":"2002-05-16T23:07:00Z","title":"The Structure and Dynamics of Luminous and Dark Matter in the Early-Type Lens Galaxy of 0047-281 at z=0.485","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"astro-ph/0205281","snapshot_observed_at":"2026-08-04T00:32:25.847876Z","title":"Koopmans and T","venue":null,"work_id":null,"year":2003},"citing_paper":{"arxiv_id":"2511.00789","last_updated":"2026-06-04T04:14:37Z","snapshot_observed_at":"2026-08-15T06:24:02.254376Z","submitted_at":"2025-11-02T04:00:48Z","title":"A cosmographic analysis using DESI-DR2 and strong lensing: II. Distance Ratio measurements","version":2},"reference_index":16,"source":"pdf_text","source_observed_at":"2026-08-04T00:32:25.847876Z"},"links":{"cited_paper":"/paper/astro-ph/0205281","citing_paper":"/paper/2511.00789"},"observation_digest":"sha256:b1cb1248bf276364a22f95f122b85ab3ac846e51046f28a205067fef6d45eb4e","observation_id":"37418a64-a67f-412a-a54e-bab79604d27a","resolution":{"observed_at":"2026-08-04T00:32:25.847876Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"astro-ph/0601628","last_updated":"2006-03-24T14:36:56Z","snapshot_observed_at":"2026-07-07T00:57:58.115447Z","submitted_at":"2006-01-26T23:49:52Z","title":"The Sloan Lens ACS Survey. III - The Structure and Formation of Early-type Galaxies and their Evolution since z~1","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"astro-ph/0601628","snapshot_observed_at":"2026-08-04T00:32:25.929142Z","title":"Koopmans, T","venue":null,"work_id":null,"year":2006},"citing_paper":{"arxiv_id":"2511.00789","last_updated":"2026-06-04T04:14:37Z","snapshot_observed_at":"2026-08-15T06:24:02.254376Z","submitted_at":"2025-11-02T04:00:48Z","title":"A cosmographic analysis using DESI-DR2 and strong lensing: II. Distance Ratio measurements","version":2},"reference_index":17,"source":"pdf_text","source_observed_at":"2026-08-04T00:32:25.929142Z"},"links":{"cited_paper":"/paper/astro-ph/0601628","citing_paper":"/paper/2511.00789"},"observation_digest":"sha256:42224838c537a3e7bf58b46fd5b7f8fb43c20d03ac33a329473b1d6321c5fed6","observation_id":"6a5d9b4e-844c-4f07-a90c-d6447dc86401","resolution":{"observed_at":"2026-08-04T00:32:25.929142Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":null,"snapshot_observed_at":"2026-08-04T00:32:26.038681Z","title":"Cao, Z.-H","venue":null,"work_id":null,"year":2011},"citing_paper":{"arxiv_id":"2511.00789","last_updated":"2026-06-04T04:14:37Z","snapshot_observed_at":"2026-08-15T06:24:02.254376Z","submitted_at":"2025-11-02T04:00:48Z","title":"A cosmographic analysis using DESI-DR2 and strong lensing: II. Distance Ratio measurements","version":2},"reference_index":18,"source":"pdf_text","source_observed_at":"2026-08-04T00:32:26.038681Z"},"links":{"citing_paper":"/paper/2511.00789"},"observation_digest":"sha256:015caaccc58d37fb007581ec55ff84f09ead7958d04408896f4d40171320c339","observation_id":"caa3c597-d8dc-4677-935c-d382b105a9a2","resolution":{"observed_at":"2026-08-04T00:32:26.038681Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"1105.0946","last_updated":"2011-05-04T21:16:50Z","snapshot_observed_at":"2026-08-18T23:30:09.844493Z","submitted_at":"2011-05-04T21:16:50Z","title":"Cosmic Equation of state from Strong Gravitational Lensing Systems","version":1},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"1105.0946","snapshot_observed_at":"2026-08-04T00:32:26.214122Z","title":"Biesiada, A","venue":null,"work_id":null,"year":2010},"citing_paper":{"arxiv_id":"2511.00789","last_updated":"2026-06-04T04:14:37Z","snapshot_observed_at":"2026-08-15T06:24:02.254376Z","submitted_at":"2025-11-02T04:00:48Z","title":"A cosmographic analysis using DESI-DR2 and strong lensing: II. Distance Ratio measurements","version":2},"reference_index":19,"source":"pdf_text","source_observed_at":"2026-08-04T00:32:26.214122Z"},"links":{"cited_paper":"/paper/1105.0946","citing_paper":"/paper/2511.00789"},"observation_digest":"sha256:9ede0b5946bbdd351da913a9ad013e98753d0ae77fab5cd44e2750f55c50c0e5","observation_id":"9035655b-806a-4426-b46b-ce11f8e2704b","resolution":{"observed_at":"2026-08-04T00:32:26.214122Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2201.12553","last_updated":"2022-09-28T03:17:48Z","snapshot_observed_at":"2026-08-16T17:25:02.760078Z","submitted_at":"2022-01-29T10:42:04Z","title":"Cosmological model-independent measurement of cosmic curvature using distance sum rule with the help of gravitational waves","version":3},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2201.12553","snapshot_observed_at":"2026-08-04T00:32:26.324859Z","title":"Wang, J.-Z","venue":null,"work_id":null,"year":2022},"citing_paper":{"arxiv_id":"2511.00789","last_updated":"2026-06-04T04:14:37Z","snapshot_observed_at":"2026-08-15T06:24:02.254376Z","submitted_at":"2025-11-02T04:00:48Z","title":"A cosmographic analysis using DESI-DR2 and strong lensing: II. Distance Ratio measurements","version":2},"reference_index":20,"source":"pdf_text","source_observed_at":"2026-08-04T00:32:26.324859Z"},"links":{"cited_paper":"/paper/2201.12553","citing_paper":"/paper/2511.00789"},"observation_digest":"sha256:78ad6e7cc1a5a3d2e4819527e7cd235161bb234a56b015358d613a5696caa4ab","observation_id":"c5cf7246-419d-4bad-9aa5-158712f1d503","resolution":{"observed_at":"2026-08-04T00:32:26.324859Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"1611.07196","last_updated":"2017-03-16T12:03:50Z","snapshot_observed_at":"2026-08-14T21:29:15.425001Z","submitted_at":"2016-11-22T08:41:47Z","title":"Constraining cosmic curvature by using age of galaxies and gravitational lenses","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"1611.07196","snapshot_observed_at":"2026-08-04T00:32:26.439083Z","title":null,"venue":null,"work_id":null,"year":2017},"citing_paper":{"arxiv_id":"2511.00789","last_updated":"2026-06-04T04:14:37Z","snapshot_observed_at":"2026-08-15T06:24:02.254376Z","submitted_at":"2025-11-02T04:00:48Z","title":"A cosmographic analysis using DESI-DR2 and strong lensing: II. Distance Ratio measurements","version":2},"reference_index":21,"source":"pdf_text","source_observed_at":"2026-08-04T00:32:26.439083Z"},"links":{"cited_paper":"/paper/1611.07196","citing_paper":"/paper/2511.00789"},"observation_digest":"sha256:732a092cd99242ccacef3be5c9685dfa0ffaecddd7b7d5c0b31cbe260a15dc52","observation_id":"2783afe4-532d-4d9f-940c-5ccde989dd65","resolution":{"observed_at":"2026-08-04T00:32:26.439083Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"1509.07649","last_updated":"2015-09-25T09:30:35Z","snapshot_observed_at":"2026-08-18T20:24:05.474736Z","submitted_at":"2015-09-25T09:30:35Z","title":"Cosmology with Strong Lensing Systems","version":1},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"1509.07649","snapshot_observed_at":"2026-08-04T00:32:26.531190Z","title":null,"venue":null,"work_id":null,"year":2015},"citing_paper":{"arxiv_id":"2511.00789","last_updated":"2026-06-04T04:14:37Z","snapshot_observed_at":"2026-08-15T06:24:02.254376Z","submitted_at":"2025-11-02T04:00:48Z","title":"A cosmographic analysis using DESI-DR2 and strong lensing: II. Distance Ratio measurements","version":2},"reference_index":22,"source":"pdf_text","source_observed_at":"2026-08-04T00:32:26.531190Z"},"links":{"cited_paper":"/paper/1509.07649","citing_paper":"/paper/2511.00789"},"observation_digest":"sha256:64ce05891d6500c21bb355e91f47e667e83e63a46553d4686ec653734039e6b2","observation_id":"1e62776c-943c-465b-a332-b5df17b78e25","resolution":{"observed_at":"2026-08-04T00:32:26.531190Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"1510.03494","last_updated":"2015-12-11T04:34:58Z","snapshot_observed_at":"2026-08-14T22:28:11.916286Z","submitted_at":"2015-10-13T00:51:40Z","title":"Comparison of cosmological models using standard rulers and candles","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"1510.03494","snapshot_observed_at":"2026-08-04T00:32:26.642932Z","title":null,"venue":null,"work_id":null,"year":2016},"citing_paper":{"arxiv_id":"2511.00789","last_updated":"2026-06-04T04:14:37Z","snapshot_observed_at":"2026-08-15T06:24:02.254376Z","submitted_at":"2025-11-02T04:00:48Z","title":"A cosmographic analysis using DESI-DR2 and strong lensing: II. Distance Ratio measurements","version":2},"reference_index":23,"source":"pdf_text","source_observed_at":"2026-08-04T00:32:26.642932Z"},"links":{"cited_paper":"/paper/1510.03494","citing_paper":"/paper/2511.00789"},"observation_digest":"sha256:77ae7e40297938552b84ecd0083a035c6e8de0fd34469af25a2eaf154fb442a4","observation_id":"fd593516-d1f1-4295-bbee-8c85994104aa","resolution":{"observed_at":"2026-08-04T00:32:26.642932Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"1604.05625","last_updated":"2016-04-19T15:23:16Z","snapshot_observed_at":"2026-08-18T20:21:55.669128Z","submitted_at":"2016-04-19T15:23:16Z","title":"Limits on the power-law mass and luminosity density profiles of elliptical galaxies from gravitational lensing systems","version":1},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"1604.05625","snapshot_observed_at":"2026-08-04T00:32:26.746241Z","title":null,"venue":null,"work_id":null,"year":2016},"citing_paper":{"arxiv_id":"2511.00789","last_updated":"2026-06-04T04:14:37Z","snapshot_observed_at":"2026-08-15T06:24:02.254376Z","submitted_at":"2025-11-02T04:00:48Z","title":"A cosmographic analysis using DESI-DR2 and strong lensing: II. Distance Ratio measurements","version":2},"reference_index":24,"source":"pdf_text","source_observed_at":"2026-08-04T00:32:26.746241Z"},"links":{"cited_paper":"/paper/1604.05625","citing_paper":"/paper/2511.00789"},"observation_digest":"sha256:d1e7797438151f68df01e4de5534e11cdcde7f9babec61dcf6c2de5c49a97910","observation_id":"ccc23037-d4c1-4f61-9fc7-e00ac1181d31","resolution":{"observed_at":"2026-08-04T00:32:26.746241Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"1704.07614","last_updated":"2017-05-14T15:20:54Z","snapshot_observed_at":"2026-08-14T21:04:55.088676Z","submitted_at":"2017-04-25T10:21:00Z","title":"No evidence for the evolution of mass density power-law index $\\gamma$ from strong gravitational lensing observation","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"1704.07614","snapshot_observed_at":"2026-08-04T00:32:26.859406Z","title":"Cui, H.-L","venue":null,"work_id":null,"year":2017},"citing_paper":{"arxiv_id":"2511.00789","last_updated":"2026-06-04T04:14:37Z","snapshot_observed_at":"2026-08-15T06:24:02.254376Z","submitted_at":"2025-11-02T04:00:48Z","title":"A cosmographic analysis using DESI-DR2 and strong lensing: II. Distance Ratio measurements","version":2},"reference_index":25,"source":"pdf_text","source_observed_at":"2026-08-04T00:32:26.859406Z"},"links":{"cited_paper":"/paper/1704.07614","citing_paper":"/paper/2511.00789"},"observation_digest":"sha256:e9ef38e0e17bf7f495dd1f817b58c5323ec268528785617422f648634d4e98a4","observation_id":"05b1112e-48c7-4291-8c0b-6f0fa29a005e","resolution":{"observed_at":"2026-08-04T00:32:26.859406Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"1809.09845","last_updated":"2019-07-12T08:06:22Z","snapshot_observed_at":"2026-08-18T20:22:47.285249Z","submitted_at":"2018-09-26T08:27:34Z","title":"Assessing the effect of lens mass model in cosmological application with updated galaxy-scale strong gravitational lensing sample","version":5},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"1809.09845","snapshot_observed_at":"2026-08-04T00:32:26.977062Z","title":null,"venue":null,"work_id":null,"year":2019},"citing_paper":{"arxiv_id":"2511.00789","last_updated":"2026-06-04T04:14:37Z","snapshot_observed_at":"2026-08-15T06:24:02.254376Z","submitted_at":"2025-11-02T04:00:48Z","title":"A cosmographic analysis using DESI-DR2 and strong lensing: II. Distance Ratio measurements","version":2},"reference_index":26,"source":"pdf_text","source_observed_at":"2026-08-04T00:32:26.977062Z"},"links":{"cited_paper":"/paper/1809.09845","citing_paper":"/paper/2511.00789"},"observation_digest":"sha256:8e2edd0249d96d85a6a2a77ad55e80e329057736af21012a453e5ededee3223a","observation_id":"ddb3a9a1-7488-4f12-b479-9077071e6840","resolution":{"observed_at":"2026-08-04T00:32:26.977062Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"1611.04731","last_updated":"2017-01-12T02:12:05Z","snapshot_observed_at":"2026-08-14T21:30:24.264352Z","submitted_at":"2016-11-15T08:11:21Z","title":"Revisiting Studies of the Statistical Property of a Strong Gravitational Lens System and Model-independent Constraint on the Curvature of the Universe","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"1611.04731","snapshot_observed_at":"2026-08-04T00:32:27.090630Z","title":null,"venue":null,"work_id":null,"year":2017},"citing_paper":{"arxiv_id":"2511.00789","last_updated":"2026-06-04T04:14:37Z","snapshot_observed_at":"2026-08-15T06:24:02.254376Z","submitted_at":"2025-11-02T04:00:48Z","title":"A cosmographic analysis using DESI-DR2 and strong lensing: II. Distance Ratio measurements","version":2},"reference_index":27,"source":"pdf_text","source_observed_at":"2026-08-04T00:32:27.090630Z"},"links":{"cited_paper":"/paper/1611.04731","citing_paper":"/paper/2511.00789"},"observation_digest":"sha256:900743d6275c5973cfaafe59c75dd26677551055017abe07e84de1ce14dec34a","observation_id":"55c479c0-abdb-4b56-945c-c43d545775d1","resolution":{"observed_at":"2026-08-04T00:32:27.090630Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2307.09271","last_updated":"2023-07-18T14:03:30Z","snapshot_observed_at":"2026-08-16T15:15:20.263711Z","submitted_at":"2023-07-18T14:03:30Z","title":"Cosmology from Large Populations of Galaxy-Galaxy Strong Gravitational Lenses","version":1},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2307.09271","snapshot_observed_at":"2026-08-04T00:32:27.211665Z","title":null,"venue":null,"work_id":null,"year":2024},"citing_paper":{"arxiv_id":"2511.00789","last_updated":"2026-06-04T04:14:37Z","snapshot_observed_at":"2026-08-15T06:24:02.254376Z","submitted_at":"2025-11-02T04:00:48Z","title":"A cosmographic analysis using DESI-DR2 and strong lensing: II. Distance Ratio measurements","version":2},"reference_index":28,"source":"pdf_text","source_observed_at":"2026-08-04T00:32:27.211665Z"},"links":{"cited_paper":"/paper/2307.09271","citing_paper":"/paper/2511.00789"},"observation_digest":"sha256:e2c43806cb4439bc98b301cf401a5ec64bcd2debcb04cbd55f96c2deecf60725","observation_id":"45b883ed-3207-4f46-9ad2-878024c231ff","resolution":{"observed_at":"2026-08-04T00:32:27.211665Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2309.11915","last_updated":"2023-10-27T08:27:41Z","snapshot_observed_at":"2026-08-20T01:35:29.064424Z","submitted_at":"2023-09-21T09:26:56Z","title":"Probing a scale dependent gravitational slip with galaxy strong lensing systems","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2309.11915","snapshot_observed_at":"2026-08-04T00:32:27.338242Z","title":"Guerrini and E","venue":null,"work_id":null,"year":2024},"citing_paper":{"arxiv_id":"2511.00789","last_updated":"2026-06-04T04:14:37Z","snapshot_observed_at":"2026-08-15T06:24:02.254376Z","submitted_at":"2025-11-02T04:00:48Z","title":"A cosmographic analysis using DESI-DR2 and strong lensing: II. Distance Ratio measurements","version":2},"reference_index":29,"source":"pdf_text","source_observed_at":"2026-08-04T00:32:27.338242Z"},"links":{"cited_paper":"/paper/2309.11915","citing_paper":"/paper/2511.00789"},"observation_digest":"sha256:772c9b59af458c134ad742f2702b59dd4ab3d5dc73542bb4803a8e06749efa3c","observation_id":"b4e1b76f-18d2-4ab3-a260-fa4aea42306b","resolution":{"observed_at":"2026-08-04T00:32:27.338242Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":null,"snapshot_observed_at":"2026-08-04T00:32:27.471538Z","title":"Weinberg,Gravitation and Cosmology: Principles and Applications of the General Theory of Relativity(1972)","venue":null,"work_id":null,"year":1972},"citing_paper":{"arxiv_id":"2511.00789","last_updated":"2026-06-04T04:14:37Z","snapshot_observed_at":"2026-08-15T06:24:02.254376Z","submitted_at":"2025-11-02T04:00:48Z","title":"A cosmographic analysis using DESI-DR2 and strong lensing: II. Distance Ratio measurements","version":2},"reference_index":30,"source":"pdf_text","source_observed_at":"2026-08-04T00:32:27.471538Z"},"links":{"citing_paper":"/paper/2511.00789"},"observation_digest":"sha256:f119798aa5026b141070b37ca0b3aecd6ab53439448d1368f761cc1fd7b623fb","observation_id":"78a0bd23-2b11-4b8b-81af-1aaa1425a0b2","resolution":{"observed_at":"2026-08-04T00:32:27.471538Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"1501.01619","last_updated":"2015-01-07T20:48:01Z","snapshot_observed_at":"2026-08-14T23:04:54.161875Z","submitted_at":"2015-01-07T20:48:01Z","title":"Energy conditions in the epoch of galaxy formation","version":1},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"1501.01619","snapshot_observed_at":"2026-08-04T00:32:27.519334Z","title":"Visser,Energy conditions in the epoch of galaxy formation.,Science276(1997) 88 [1501.01619]","venue":null,"work_id":null,"year":1997},"citing_paper":{"arxiv_id":"2511.00789","last_updated":"2026-06-04T04:14:37Z","snapshot_observed_at":"2026-08-15T06:24:02.254376Z","submitted_at":"2025-11-02T04:00:48Z","title":"A cosmographic analysis using DESI-DR2 and strong lensing: II. Distance Ratio measurements","version":2},"reference_index":31,"source":"pdf_text","source_observed_at":"2026-08-04T00:32:27.519334Z"},"links":{"cited_paper":"/paper/1501.01619","citing_paper":"/paper/2511.00789"},"observation_digest":"sha256:83057605aeb84e764bddc8a6e9447f56546083660da058bfb12c0ed74e7ab837","observation_id":"0e0a3ccc-0e01-46de-8883-4e0f5f0d27cd","resolution":{"observed_at":"2026-08-04T00:32:27.519334Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":null,"snapshot_observed_at":"2026-08-04T00:32:27.669135Z","title":"Visser,Cosmography: Cosmology without the Einstein equations,General Relativity and Gravitation37(2005) 1541","venue":null,"work_id":null,"year":2005},"citing_paper":{"arxiv_id":"2511.00789","last_updated":"2026-06-04T04:14:37Z","snapshot_observed_at":"2026-08-15T06:24:02.254376Z","submitted_at":"2025-11-02T04:00:48Z","title":"A cosmographic analysis using DESI-DR2 and strong lensing: II. Distance Ratio measurements","version":2},"reference_index":32,"source":"pdf_text","source_observed_at":"2026-08-04T00:32:27.669135Z"},"links":{"citing_paper":"/paper/2511.00789"},"observation_digest":"sha256:5154a642462b9a192ce5570f60ace41b46edbcccdf71568c4c0b3e14e819c679","observation_id":"64e65fb9-1267-47a7-adba-7f329f8c22bf","resolution":{"observed_at":"2026-08-04T00:32:27.669135Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"astro-ph/0403003","last_updated":"2004-02-27T21:01:51Z","snapshot_observed_at":"2026-08-04T22:51:09.947223Z","submitted_at":"2004-02-27T21:01:51Z","title":"Expansion, Geometry, and Gravity","version":1},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"astro-ph/0403003","snapshot_observed_at":"2026-08-04T00:32:27.705295Z","title":"Caldwell and M","venue":null,"work_id":null,"year":2004},"citing_paper":{"arxiv_id":"2511.00789","last_updated":"2026-06-04T04:14:37Z","snapshot_observed_at":"2026-08-15T06:24:02.254376Z","submitted_at":"2025-11-02T04:00:48Z","title":"A cosmographic analysis using DESI-DR2 and strong lensing: II. Distance Ratio measurements","version":2},"reference_index":33,"source":"pdf_text","source_observed_at":"2026-08-04T00:32:27.705295Z"},"links":{"cited_paper":"/paper/astro-ph/0403003","citing_paper":"/paper/2511.00789"},"observation_digest":"sha256:96d326abaccb00827eefa2ce45e38e2068e7acd6acebd4e39795c0f380998d72","observation_id":"719d0899-091c-4421-a68a-cb8f83f33829","resolution":{"observed_at":"2026-08-04T00:32:27.705295Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"astro-ph/0402512","last_updated":"2004-03-31T22:17:42Z","snapshot_observed_at":"2026-08-16T20:43:26.414902Z","submitted_at":"2004-02-23T16:46:43Z","title":"Type Ia Supernova Discoveries at z>1 From the Hubble Space Telescope: Evidence for Past Deceleration and Constraints on Dark Energy Evolution","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"astro-ph/0402512","snapshot_observed_at":"2026-08-04T00:32:27.772777Z","title":"Riess, L.-G","venue":null,"work_id":null,"year":2004},"citing_paper":{"arxiv_id":"2511.00789","last_updated":"2026-06-04T04:14:37Z","snapshot_observed_at":"2026-08-15T06:24:02.254376Z","submitted_at":"2025-11-02T04:00:48Z","title":"A cosmographic analysis using DESI-DR2 and strong lensing: II. Distance Ratio measurements","version":2},"reference_index":34,"source":"pdf_text","source_observed_at":"2026-08-04T00:32:27.772777Z"},"links":{"cited_paper":"/paper/astro-ph/0402512","citing_paper":"/paper/2511.00789"},"observation_digest":"sha256:473895f2d1ed4f1568491f881588cba50aa930f1bbb0414032899b36e87d51da","observation_id":"3b4d86ea-f434-45d0-ab11-bfdb2fcde27d","resolution":{"observed_at":"2026-08-04T00:32:27.772777Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"gr-qc/0009008","last_updated":"2000-09-25T18:37:17Z","snapshot_observed_at":"2026-07-07T03:13:00.877347Z","submitted_at":"2000-09-04T15:09:00Z","title":"Accelerating Universes with Scaling Dark Matter","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"gr-qc/0009008","snapshot_observed_at":"2026-08-04T00:32:27.816881Z","title":"Chevallier and D","venue":null,"work_id":null,"year":2001},"citing_paper":{"arxiv_id":"2511.00789","last_updated":"2026-06-04T04:14:37Z","snapshot_observed_at":"2026-08-15T06:24:02.254376Z","submitted_at":"2025-11-02T04:00:48Z","title":"A cosmographic analysis using DESI-DR2 and strong lensing: II. Distance Ratio measurements","version":2},"reference_index":35,"source":"pdf_text","source_observed_at":"2026-08-04T00:32:27.816881Z"},"links":{"cited_paper":"/paper/gr-qc/0009008","citing_paper":"/paper/2511.00789"},"observation_digest":"sha256:adfb51d6a6b6a77c3ec2c9a351194f176f22d9dfe9001c6ac124801413279b47","observation_id":"85de14bb-b04f-4926-add5-ec5d650176ee","resolution":{"observed_at":"2026-08-04T00:32:27.816881Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"astro-ph/0208512","last_updated":"2002-08-28T23:21:10Z","snapshot_observed_at":"2026-07-07T00:28:09.066072Z","submitted_at":"2002-08-28T23:21:10Z","title":"Exploring the Expansion History of the Universe","version":1},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"astro-ph/0208512","snapshot_observed_at":"2026-08-04T00:32:27.903278Z","title":"Linder,Exploring the Expansion History of the Universe,Phys","venue":null,"work_id":null,"year":2003},"citing_paper":{"arxiv_id":"2511.00789","last_updated":"2026-06-04T04:14:37Z","snapshot_observed_at":"2026-08-15T06:24:02.254376Z","submitted_at":"2025-11-02T04:00:48Z","title":"A cosmographic analysis using DESI-DR2 and strong lensing: II. Distance Ratio measurements","version":2},"reference_index":36,"source":"pdf_text","source_observed_at":"2026-08-04T00:32:27.903278Z"},"links":{"cited_paper":"/paper/astro-ph/0208512","citing_paper":"/paper/2511.00789"},"observation_digest":"sha256:27a1e75b3444e32ac273f5efaec0971595b6060160a810968bb2206f2a3ddb29","observation_id":"3208b5a0-1abd-4dd3-82f9-b97dcb76e704","resolution":{"observed_at":"2026-08-04T00:32:27.903278Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"1309.3215","last_updated":"2013-09-12T16:50:40Z","snapshot_observed_at":"2026-08-15T00:03:24.029226Z","submitted_at":"2013-09-12T16:50:40Z","title":"Cosmographic analysis of the equation of state of the universe through Pad\\'e approximations","version":1},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"1309.3215","snapshot_observed_at":"2026-08-04T00:32:27.970768Z","title":"Gruber and O","venue":null,"work_id":null,"year":2014},"citing_paper":{"arxiv_id":"2511.00789","last_updated":"2026-06-04T04:14:37Z","snapshot_observed_at":"2026-08-15T06:24:02.254376Z","submitted_at":"2025-11-02T04:00:48Z","title":"A cosmographic analysis using DESI-DR2 and strong lensing: II. Distance Ratio measurements","version":2},"reference_index":37,"source":"pdf_text","source_observed_at":"2026-08-04T00:32:27.970768Z"},"links":{"cited_paper":"/paper/1309.3215","citing_paper":"/paper/2511.00789"},"observation_digest":"sha256:a3396a603149d70605e5eb4d26b17040dd4445a2badfc3d033c172a68ebafc6a","observation_id":"fa3d7ccd-9312-4658-a3c4-00a22e6a47c7","resolution":{"observed_at":"2026-08-04T00:32:27.970768Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"1202.4808","last_updated":"2012-05-13T15:14:28Z","snapshot_observed_at":"2026-08-15T04:18:31.509988Z","submitted_at":"2012-02-22T02:25:10Z","title":"Crossing Statistic: Bayesian interpretation, model selection and resolving dark energy parametrization problem","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"1202.4808","snapshot_observed_at":"2026-08-04T00:32:28.042741Z","title":"Shafieloo,Crossing statistic: Bayesian interpretation, model selection and resolving dark energy parametrization problem,J","venue":null,"work_id":null,"year":2012},"citing_paper":{"arxiv_id":"2511.00789","last_updated":"2026-06-04T04:14:37Z","snapshot_observed_at":"2026-08-15T06:24:02.254376Z","submitted_at":"2025-11-02T04:00:48Z","title":"A cosmographic analysis using DESI-DR2 and strong lensing: II. Distance Ratio measurements","version":2},"reference_index":38,"source":"pdf_text","source_observed_at":"2026-08-04T00:32:28.042741Z"},"links":{"cited_paper":"/paper/1202.4808","citing_paper":"/paper/2511.00789"},"observation_digest":"sha256:f3ae4fa6a917b5cbba6719dc6e75709d79c17cb85a42c2d627aa68ac6248b416","observation_id":"87772108-b174-470c-b808-1d8375113dd0","resolution":{"observed_at":"2026-08-04T00:32:28.042741Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":null,"snapshot_observed_at":"2026-08-04T00:32:28.098231Z","title":"Blandford and R","venue":null,"work_id":null,"year":1992},"citing_paper":{"arxiv_id":"2511.00789","last_updated":"2026-06-04T04:14:37Z","snapshot_observed_at":"2026-08-15T06:24:02.254376Z","submitted_at":"2025-11-02T04:00:48Z","title":"A cosmographic analysis using DESI-DR2 and strong lensing: II. Distance Ratio measurements","version":2},"reference_index":39,"source":"pdf_text","source_observed_at":"2026-08-04T00:32:28.098231Z"},"links":{"citing_paper":"/paper/2511.00789"},"observation_digest":"sha256:654404ddcb720c0cb9797aadcf158c776becda85468c0b3cdd41e6954e0a7320","observation_id":"2ea37038-c05e-424d-ad5a-0699bd484e0c","resolution":{"observed_at":"2026-08-04T00:32:28.098231Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"astro-ph/9606001","last_updated":"1997-10-02T07:49:42Z","snapshot_observed_at":"2026-08-16T10:21:18.346027Z","submitted_at":"1996-06-03T06:45:37Z","title":"Lectures on Gravitational Lensing","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"astro-ph/9606001","snapshot_observed_at":"2026-08-04T00:32:28.178492Z","title":"Narayan and M","venue":null,"work_id":null,"year":1996},"citing_paper":{"arxiv_id":"2511.00789","last_updated":"2026-06-04T04:14:37Z","snapshot_observed_at":"2026-08-15T06:24:02.254376Z","submitted_at":"2025-11-02T04:00:48Z","title":"A cosmographic analysis using DESI-DR2 and strong lensing: II. Distance Ratio measurements","version":2},"reference_index":40,"source":"pdf_text","source_observed_at":"2026-08-04T00:32:28.178492Z"},"links":{"cited_paper":"/paper/astro-ph/9606001","citing_paper":"/paper/2511.00789"},"observation_digest":"sha256:eab95169aff61789ca2a3919465c7c229f5cdd66e419cd4b339cf691174e195e","observation_id":"6b1c01a5-5148-4eef-930d-e9ee1f0d0d21","resolution":{"observed_at":"2026-08-04T00:32:28.178492Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":null,"snapshot_observed_at":"2026-08-04T00:32:28.278472Z","title":"Jorgensen, M","venue":null,"work_id":null,"year":1995},"citing_paper":{"arxiv_id":"2511.00789","last_updated":"2026-06-04T04:14:37Z","snapshot_observed_at":"2026-08-15T06:24:02.254376Z","submitted_at":"2025-11-02T04:00:48Z","title":"A cosmographic analysis using DESI-DR2 and strong lensing: II. Distance Ratio measurements","version":2},"reference_index":41,"source":"pdf_text","source_observed_at":"2026-08-04T00:32:28.278472Z"},"links":{"citing_paper":"/paper/2511.00789"},"observation_digest":"sha256:2bb7f6c3421abb5e9f4f9984671e39891ea4ff2fc1b945b54f2d66ff50a0d1c3","observation_id":"b1375c32-c5f6-4402-a515-2e744f346837","resolution":{"observed_at":"2026-08-04T00:32:28.278472Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"astro-ph/0505042","last_updated":"2005-11-29T19:07:46Z","snapshot_observed_at":"2026-07-07T00:50:18.319159Z","submitted_at":"2005-05-03T17:03:25Z","title":"The SAURON project - IV. The mass-to-light ratio, the virial mass estimator and the fundamental plane of elliptical and lenticular galaxies","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"astro-ph/0505042","snapshot_observed_at":"2026-08-04T00:32:28.351619Z","title":"Cappellari, R","venue":null,"work_id":null,"year":2006},"citing_paper":{"arxiv_id":"2511.00789","last_updated":"2026-06-04T04:14:37Z","snapshot_observed_at":"2026-08-15T06:24:02.254376Z","submitted_at":"2025-11-02T04:00:48Z","title":"A cosmographic analysis using DESI-DR2 and strong lensing: II. Distance Ratio measurements","version":2},"reference_index":42,"source":"pdf_text","source_observed_at":"2026-08-04T00:32:28.351619Z"},"links":{"cited_paper":"/paper/astro-ph/0505042","citing_paper":"/paper/2511.00789"},"observation_digest":"sha256:b0b1227f8d12c132e76055c627885dcbebaa55b4e64778aa9e5d2cab792a9cc3","observation_id":"a7eeda31-a674-45d0-b3a2-f5d3cfbdd4a3","resolution":{"observed_at":"2026-08-04T00:32:28.351619Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"astro-ph/0201017","last_updated":"2002-03-01T23:49:35Z","snapshot_observed_at":"2026-08-15T12:14:53.314286Z","submitted_at":"2002-01-02T19:01:34Z","title":"The stellar velocity dispersion of the lens galaxy in MG2016+112 at z=1.004","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"astro-ph/0201017","snapshot_observed_at":"2026-08-04T00:32:28.421189Z","title":"Koopmans and T","venue":null,"work_id":null,"year":2016},"citing_paper":{"arxiv_id":"2511.00789","last_updated":"2026-06-04T04:14:37Z","snapshot_observed_at":"2026-08-15T06:24:02.254376Z","submitted_at":"2025-11-02T04:00:48Z","title":"A cosmographic analysis using DESI-DR2 and strong lensing: II. Distance Ratio measurements","version":2},"reference_index":43,"source":"pdf_text","source_observed_at":"2026-08-04T00:32:28.421189Z"},"links":{"cited_paper":"/paper/astro-ph/0201017","citing_paper":"/paper/2511.00789"},"observation_digest":"sha256:1700d70e68ce0b93566a51e2be1f50896ed6b92b2636563c95a48715e0362407","observation_id":"5b20dced-965f-418d-a731-ce9b31517cde","resolution":{"observed_at":"2026-08-04T00:32:28.421189Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"astro-ph/0401373","last_updated":"2004-05-01T18:46:33Z","snapshot_observed_at":"2026-07-07T00:39:50.327348Z","submitted_at":"2004-01-19T21:08:50Z","title":"Massive Dark-matter halos and Evolution of Early-type Galaxies to z=1","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"astro-ph/0401373","snapshot_observed_at":"2026-08-04T00:32:28.535807Z","title":"Treu and L.V.E","venue":null,"work_id":null,"year":2004},"citing_paper":{"arxiv_id":"2511.00789","last_updated":"2026-06-04T04:14:37Z","snapshot_observed_at":"2026-08-15T06:24:02.254376Z","submitted_at":"2025-11-02T04:00:48Z","title":"A cosmographic analysis using DESI-DR2 and strong lensing: II. Distance Ratio measurements","version":2},"reference_index":44,"source":"pdf_text","source_observed_at":"2026-08-04T00:32:28.535807Z"},"links":{"cited_paper":"/paper/astro-ph/0401373","citing_paper":"/paper/2511.00789"},"observation_digest":"sha256:cdcb89333017c44349c7795d9a18703b678f60e66ddef6020d841e364d85ed56","observation_id":"895215d2-ecf9-4ab8-bafc-04ad81ba064c","resolution":{"observed_at":"2026-08-04T00:32:28.535807Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"1008.3167","last_updated":"2010-08-18T20:05:28Z","snapshot_observed_at":"2026-08-15T05:11:10.081145Z","submitted_at":"2010-08-18T20:05:28Z","title":"The SL2S Galaxy-scale Lens Sample. II. Cosmic evolution of dark and luminous mass in early-type galaxies","version":1},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"1008.3167","snapshot_observed_at":"2026-08-04T00:32:28.624632Z","title":null,"venue":null,"work_id":null,"year":2011},"citing_paper":{"arxiv_id":"2511.00789","last_updated":"2026-06-04T04:14:37Z","snapshot_observed_at":"2026-08-15T06:24:02.254376Z","submitted_at":"2025-11-02T04:00:48Z","title":"A cosmographic analysis using DESI-DR2 and strong lensing: II. Distance Ratio measurements","version":2},"reference_index":45,"source":"pdf_text","source_observed_at":"2026-08-04T00:32:28.624632Z"},"links":{"cited_paper":"/paper/1008.3167","citing_paper":"/paper/2511.00789"},"observation_digest":"sha256:0ed2d52f7da597252d6126bfeac5af1ba7efd5bcefd6a067424280cc5f7f355f","observation_id":"08dd1474-6b0c-4e5f-89d3-3107c4aa0bd0","resolution":{"observed_at":"2026-08-04T00:32:28.624632Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"1307.4764","last_updated":"2013-07-17T20:00:07Z","snapshot_observed_at":"2026-08-15T00:09:59.481177Z","submitted_at":"2013-07-17T20:00:07Z","title":"The SL2S Galaxy-scale Lens Sample. III. Lens Models, Surface Photometry and Stellar Masses for the final sample","version":1},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"1307.4764","snapshot_observed_at":"2026-08-04T00:32:28.685375Z","title":"Sonnenfeld, R","venue":null,"work_id":null,"year":2013},"citing_paper":{"arxiv_id":"2511.00789","last_updated":"2026-06-04T04:14:37Z","snapshot_observed_at":"2026-08-15T06:24:02.254376Z","submitted_at":"2025-11-02T04:00:48Z","title":"A cosmographic analysis using DESI-DR2 and strong lensing: II. Distance Ratio measurements","version":2},"reference_index":46,"source":"pdf_text","source_observed_at":"2026-08-04T00:32:28.685375Z"},"links":{"cited_paper":"/paper/1307.4764","citing_paper":"/paper/2511.00789"},"observation_digest":"sha256:1cde02df6618f09b33f556079910d090486450dc4e8f15fb6ac7d27260bd06bf","observation_id":"771a7ddd-33aa-43c9-9a30-1593713568fd","resolution":{"observed_at":"2026-08-04T00:32:28.685375Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"1307.4759","last_updated":"2013-07-17T20:00:02Z","snapshot_observed_at":"2026-08-18T20:21:25.254779Z","submitted_at":"2013-07-17T20:00:02Z","title":"The SL2S Galaxy-scale Lens Sample. IV. The dependence of the total mass density profile of early-type galaxies on redshift, stellar mass, and size","version":1},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"1307.4759","snapshot_observed_at":"2026-08-04T00:32:28.766076Z","title":"Sonnenfeld, T","venue":null,"work_id":null,"year":2013},"citing_paper":{"arxiv_id":"2511.00789","last_updated":"2026-06-04T04:14:37Z","snapshot_observed_at":"2026-08-15T06:24:02.254376Z","submitted_at":"2025-11-02T04:00:48Z","title":"A cosmographic analysis using DESI-DR2 and strong lensing: II. Distance Ratio measurements","version":2},"reference_index":47,"source":"pdf_text","source_observed_at":"2026-08-04T00:32:28.766076Z"},"links":{"cited_paper":"/paper/1307.4759","citing_paper":"/paper/2511.00789"},"observation_digest":"sha256:c39661858318ff964604fe116b439bf1111e704e00b6b205237a9cc7ce16005e","observation_id":"dc65dad3-f943-4065-aebd-e96367ce732b","resolution":{"observed_at":"2026-08-04T00:32:28.766076Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"1410.1881","last_updated":"2014-12-19T16:02:11Z","snapshot_observed_at":"2026-08-14T23:16:36.423108Z","submitted_at":"2014-10-07T20:00:42Z","title":"The SL2S Galaxy-scale Lens Sample. V. Dark Matter Halos and Stellar IMF of Massive Early-type Galaxies out to Redshift 0.8","version":3},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"1410.1881","snapshot_observed_at":"2026-08-04T00:32:28.827008Z","title":"Sonnenfeld, T","venue":null,"work_id":null,"year":2015},"citing_paper":{"arxiv_id":"2511.00789","last_updated":"2026-06-04T04:14:37Z","snapshot_observed_at":"2026-08-15T06:24:02.254376Z","submitted_at":"2025-11-02T04:00:48Z","title":"A cosmographic analysis using DESI-DR2 and strong lensing: II. Distance Ratio measurements","version":2},"reference_index":48,"source":"pdf_text","source_observed_at":"2026-08-04T00:32:28.827008Z"},"links":{"cited_paper":"/paper/1410.1881","citing_paper":"/paper/2511.00789"},"observation_digest":"sha256:ef834b3d799b11ea7aeb3fa98c9a0d27bb5bba8178fbc9e2e3eb8c8d9ea50653","observation_id":"76797763-fc25-4583-bf24-895c690a1b43","resolution":{"observed_at":"2026-08-04T00:32:28.827008Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"0805.1931","last_updated":"2008-05-14T17:16:25Z","snapshot_observed_at":"2026-08-18T20:30:33.250087Z","submitted_at":"2008-05-14T17:16:25Z","title":"The Sloan Lens ACS Survey. V. The Full ACS Strong-Lens Sample","version":1},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"0805.1931","snapshot_observed_at":"2026-08-04T00:32:28.899597Z","title":"Bolton, S","venue":null,"work_id":null,"year":2008},"citing_paper":{"arxiv_id":"2511.00789","last_updated":"2026-06-04T04:14:37Z","snapshot_observed_at":"2026-08-15T06:24:02.254376Z","submitted_at":"2025-11-02T04:00:48Z","title":"A cosmographic analysis using DESI-DR2 and strong lensing: II. Distance Ratio measurements","version":2},"reference_index":49,"source":"pdf_text","source_observed_at":"2026-08-04T00:32:28.899597Z"},"links":{"cited_paper":"/paper/0805.1931","citing_paper":"/paper/2511.00789"},"observation_digest":"sha256:af519f26dfd217b1536b916088648b5d5cc8a14fdf81aa5dd8f61d40163ede6c","observation_id":"17f05b56-82ea-4ae8-8789-afce01df9391","resolution":{"observed_at":"2026-08-04T00:32:28.899597Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"0911.2471","last_updated":"2009-11-12T21:01:12Z","snapshot_observed_at":"2026-08-15T05:34:03.809000Z","submitted_at":"2009-11-12T21:01:12Z","title":"The Sloan Lens ACS Survey. IX. Colors, Lensing and Stellar Masses of Early-type Galaxies","version":1},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"0911.2471","snapshot_observed_at":"2026-08-04T00:32:28.986373Z","title":"Auger, T","venue":null,"work_id":null,"year":2009},"citing_paper":{"arxiv_id":"2511.00789","last_updated":"2026-06-04T04:14:37Z","snapshot_observed_at":"2026-08-15T06:24:02.254376Z","submitted_at":"2025-11-02T04:00:48Z","title":"A cosmographic analysis using DESI-DR2 and strong lensing: II. Distance Ratio measurements","version":2},"reference_index":50,"source":"pdf_text","source_observed_at":"2026-08-04T00:32:28.986373Z"},"links":{"cited_paper":"/paper/0911.2471","citing_paper":"/paper/2511.00789"},"observation_digest":"sha256:08168ea19ac8a765028e1e6d7850727dcff188379b6c94a52d4a5f694dc9f4ba","observation_id":"6b0b9f10-cbcc-4dcd-8f98-0898e106abcb","resolution":{"observed_at":"2026-08-04T00:32:28.986373Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"1007.2880","last_updated":"2010-07-16T21:54:39Z","snapshot_observed_at":"2026-08-18T20:21:26.183872Z","submitted_at":"2010-07-16T21:54:39Z","title":"The Sloan Lens ACS Survey. X. Stellar, Dynamical, and Total Mass Correlations of Massive Early-type Galaxies","version":1},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"1007.2880","snapshot_observed_at":"2026-08-04T00:32:29.045767Z","title":"Auger, T","venue":null,"work_id":null,"year":2010},"citing_paper":{"arxiv_id":"2511.00789","last_updated":"2026-06-04T04:14:37Z","snapshot_observed_at":"2026-08-15T06:24:02.254376Z","submitted_at":"2025-11-02T04:00:48Z","title":"A cosmographic analysis using DESI-DR2 and strong lensing: II. Distance Ratio measurements","version":2},"reference_index":51,"source":"pdf_text","source_observed_at":"2026-08-04T00:32:29.045767Z"},"links":{"cited_paper":"/paper/1007.2880","citing_paper":"/paper/2511.00789"},"observation_digest":"sha256:b7ec64b6f710f0faeba0f6c5e11f03aeeff677ed3aca5a33812f26b04f30aedd","observation_id":"27d1af74-7035-4cc3-a203-8dfba29ffdbb","resolution":{"observed_at":"2026-08-04T00:32:29.045767Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"1407.2240","last_updated":"2015-02-10T20:49:10Z","snapshot_observed_at":"2026-08-14T23:27:28.078464Z","submitted_at":"2014-07-08T19:59:09Z","title":"The Sloan Lens ACS Survey. XII. Extending Strong Lensing to Lower Masses","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"1407.2240","snapshot_observed_at":"2026-08-04T00:32:29.092923Z","title":"Shu, A.S","venue":null,"work_id":null,"year":2015},"citing_paper":{"arxiv_id":"2511.00789","last_updated":"2026-06-04T04:14:37Z","snapshot_observed_at":"2026-08-15T06:24:02.254376Z","submitted_at":"2025-11-02T04:00:48Z","title":"A cosmographic analysis using DESI-DR2 and strong lensing: II. Distance Ratio measurements","version":2},"reference_index":52,"source":"pdf_text","source_observed_at":"2026-08-04T00:32:29.092923Z"},"links":{"cited_paper":"/paper/1407.2240","citing_paper":"/paper/2511.00789"},"observation_digest":"sha256:de85f3c4cbd10d42ee1c163f923322c78d0f9975b338501a5bfc8baed45572c0","observation_id":"c576dab6-62b0-4dcb-b302-b13fb19d231f","resolution":{"observed_at":"2026-08-04T00:32:29.092923Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"1711.00072","last_updated":"2018-01-12T02:26:35Z","snapshot_observed_at":"2026-08-14T20:18:14.233020Z","submitted_at":"2017-10-31T19:44:14Z","title":"The Sloan Lens ACS Survey. XIII. Discovery of 40 New Galaxy-Scale Strong Lenses","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"1711.00072","snapshot_observed_at":"2026-08-04T00:32:29.226072Z","title":"Shu, J.R","venue":null,"work_id":null,"year":2017},"citing_paper":{"arxiv_id":"2511.00789","last_updated":"2026-06-04T04:14:37Z","snapshot_observed_at":"2026-08-15T06:24:02.254376Z","submitted_at":"2025-11-02T04:00:48Z","title":"A cosmographic analysis using DESI-DR2 and strong lensing: II. Distance Ratio measurements","version":2},"reference_index":53,"source":"pdf_text","source_observed_at":"2026-08-04T00:32:29.226072Z"},"links":{"cited_paper":"/paper/1711.00072","citing_paper":"/paper/2511.00789"},"observation_digest":"sha256:b390e87d6a7a2641f48172b36e427d589f9f9eb37eba275743fba7b4056548c2","observation_id":"030efc07-95da-43b6-af35-afc1ad367e7d","resolution":{"observed_at":"2026-08-04T00:32:29.226072Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"1112.3683","last_updated":"2011-12-15T22:10:36Z","snapshot_observed_at":"2026-08-15T04:25:26.019328Z","submitted_at":"2011-12-15T22:10:36Z","title":"The BOSS Emission-Line Lens Survey (BELLS). I. A large spectroscopically selected sample of Lens Galaxies at redshift ~ 0.5","version":1},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"1112.3683","snapshot_observed_at":"2026-08-04T00:32:29.339039Z","title":"Brownstein, A.S","venue":null,"work_id":null,"year":2012},"citing_paper":{"arxiv_id":"2511.00789","last_updated":"2026-06-04T04:14:37Z","snapshot_observed_at":"2026-08-15T06:24:02.254376Z","submitted_at":"2025-11-02T04:00:48Z","title":"A cosmographic analysis using DESI-DR2 and strong lensing: II. Distance Ratio measurements","version":2},"reference_index":54,"source":"pdf_text","source_observed_at":"2026-08-04T00:32:29.339039Z"},"links":{"cited_paper":"/paper/1112.3683","citing_paper":"/paper/2511.00789"},"observation_digest":"sha256:7fe8916fe591da62bd6cb36f6f39fe3958fdca78cd4e46a561938c43cad28e84","observation_id":"fe733985-ab91-4e1f-a036-047e831cc067","resolution":{"observed_at":"2026-08-04T00:32:29.339039Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"1604.01842","last_updated":"2016-07-25T05:44:01Z","snapshot_observed_at":"2026-08-18T01:08:48.195223Z","submitted_at":"2016-04-07T01:19:47Z","title":"The BOSS Emission-Line Lens Survey. III. : Strong Lensing of Ly$\\alpha$ Emitters by Individual Galaxies","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"1604.01842","snapshot_observed_at":"2026-08-04T00:32:29.441215Z","title":"Shu, A.S","venue":null,"work_id":null,"year":2016},"citing_paper":{"arxiv_id":"2511.00789","last_updated":"2026-06-04T04:14:37Z","snapshot_observed_at":"2026-08-15T06:24:02.254376Z","submitted_at":"2025-11-02T04:00:48Z","title":"A cosmographic analysis using DESI-DR2 and strong lensing: II. Distance Ratio measurements","version":2},"reference_index":55,"source":"pdf_text","source_observed_at":"2026-08-04T00:32:29.441215Z"},"links":{"cited_paper":"/paper/1604.01842","citing_paper":"/paper/2511.00789"},"observation_digest":"sha256:d1fd988f538ed90b1bb39ed1c303357da0c9986d83f0c6b75a727c1308ece978","observation_id":"c1f01878-e0d4-42d5-8ae8-140914245b5e","resolution":{"observed_at":"2026-08-04T00:32:29.441215Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"1608.08707","last_updated":"2016-12-27T06:54:42Z","snapshot_observed_at":"2026-08-14T21:42:03.322852Z","submitted_at":"2016-08-31T02:16:10Z","title":"The BOSS Emission-Line Lens Survey. IV. : Smooth Lens Models for the BELLS GALLERY Sample","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"1608.08707","snapshot_observed_at":"2026-08-04T00:32:29.553196Z","title":"Shu, A.S","venue":null,"work_id":null,"year":2016},"citing_paper":{"arxiv_id":"2511.00789","last_updated":"2026-06-04T04:14:37Z","snapshot_observed_at":"2026-08-15T06:24:02.254376Z","submitted_at":"2025-11-02T04:00:48Z","title":"A cosmographic analysis using DESI-DR2 and strong lensing: II. Distance Ratio measurements","version":2},"reference_index":56,"source":"pdf_text","source_observed_at":"2026-08-04T00:32:29.553196Z"},"links":{"cited_paper":"/paper/1608.08707","citing_paper":"/paper/2511.00789"},"observation_digest":"sha256:8c6974f8e695dccdcec3ac7b668a8447f155ff6c64cb0c877a3e5175df8e5031","observation_id":"397786c1-1ca1-44aa-8630-dd13c44ee7bc","resolution":{"observed_at":"2026-08-04T00:32:29.553196Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2503.14743","last_updated":"2025-04-03T13:50:59Z","snapshot_observed_at":"2026-08-14T18:00:34.965712Z","submitted_at":"2025-03-18T21:14:17Z","title":"Extended Dark Energy analysis using DESI DR2 BAO measurements","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2503.14743","snapshot_observed_at":"2026-08-04T00:32:29.636726Z","title":"Lodha et al.,Extended Dark Energy analysis using DESI DR2 BAO measurements,arXiv e-prints(2025) arXiv:2503.14743 [2503.14743]","venue":null,"work_id":null,"year":2025},"citing_paper":{"arxiv_id":"2511.00789","last_updated":"2026-06-04T04:14:37Z","snapshot_observed_at":"2026-08-15T06:24:02.254376Z","submitted_at":"2025-11-02T04:00:48Z","title":"A cosmographic analysis using DESI-DR2 and strong lensing: II. Distance Ratio measurements","version":2},"reference_index":57,"source":"pdf_text","source_observed_at":"2026-08-04T00:32:29.636726Z"},"links":{"cited_paper":"/paper/2503.14743","citing_paper":"/paper/2511.00789"},"observation_digest":"sha256:66965ed8454bb54da880b458b46646a2c39b8f0ec12c8714ce4f6638a279fab7","observation_id":"e46aa5e7-9724-44e4-9ad0-7fe61d7a9a63","resolution":{"observed_at":"2026-08-04T00:32:29.636726Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"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":"2026-08-04T00:32:29.699543Z","title":"Abdul Karim et al.,DESI DR2 Results II: Measurements of Baryon Acoustic Oscillations and Cosmological Constraints,arXiv e-prints(2025) arXiv:2503.14738 [2503.14738]","venue":null,"work_id":null,"year":2025},"citing_paper":{"arxiv_id":"2511.00789","last_updated":"2026-06-04T04:14:37Z","snapshot_observed_at":"2026-08-15T06:24:02.254376Z","submitted_at":"2025-11-02T04:00:48Z","title":"A cosmographic analysis using DESI-DR2 and strong lensing: II. Distance Ratio measurements","version":2},"reference_index":58,"source":"pdf_text","source_observed_at":"2026-08-04T00:32:29.699543Z"},"links":{"cited_paper":"/paper/2503.14738","citing_paper":"/paper/2511.00789"},"observation_digest":"sha256:ca7a57a3b84224a65561002ca8142668378955686e9b5a60e6597524f9263229","observation_id":"8699a596-17bd-4b71-9204-fad4e5cb66cf","resolution":{"observed_at":"2026-08-04T00:32:29.699543Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":null,"snapshot_observed_at":"2026-08-04T00:32:29.739096Z","title":"Bassett and R","venue":null,"work_id":null,"year":2010},"citing_paper":{"arxiv_id":"2511.00789","last_updated":"2026-06-04T04:14:37Z","snapshot_observed_at":"2026-08-15T06:24:02.254376Z","submitted_at":"2025-11-02T04:00:48Z","title":"A cosmographic analysis using DESI-DR2 and strong lensing: II. Distance Ratio measurements","version":2},"reference_index":59,"source":"pdf_text","source_observed_at":"2026-08-04T00:32:29.739096Z"},"links":{"citing_paper":"/paper/2511.00789"},"observation_digest":"sha256:89a991337873bd9c4963ad193a4a1700ebc6d206dc31080cc60f1f986fb5de44","observation_id":"6a14ea47-2422-48fe-8904-cb07727ed40a","resolution":{"observed_at":"2026-08-04T00:32:29.739096Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"astro-ph/9709112","last_updated":"1997-09-12T00:10:17Z","snapshot_observed_at":"2026-07-07T01:18:17.177186Z","submitted_at":"1997-09-12T00:10:17Z","title":"Baryonic Features in the Matter Transfer Function","version":1},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"astro-ph/9709112","snapshot_observed_at":"2026-08-04T00:32:29.796454Z","title":"Eisenstein and W","venue":null,"work_id":null,"year":1998},"citing_paper":{"arxiv_id":"2511.00789","last_updated":"2026-06-04T04:14:37Z","snapshot_observed_at":"2026-08-15T06:24:02.254376Z","submitted_at":"2025-11-02T04:00:48Z","title":"A cosmographic analysis using DESI-DR2 and strong lensing: II. Distance Ratio measurements","version":2},"reference_index":60,"source":"pdf_text","source_observed_at":"2026-08-04T00:32:29.796454Z"},"links":{"cited_paper":"/paper/astro-ph/9709112","citing_paper":"/paper/2511.00789"},"observation_digest":"sha256:ca3a963156930c63613c983a531ec00e239b3696173f3c22137f4b2176eab561","observation_id":"3a6382e8-ca5b-48bd-89c0-1e421ae1631a","resolution":{"observed_at":"2026-08-04T00:32:29.796454Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":null,"snapshot_observed_at":"2026-08-04T00:32:29.845070Z","title":"Sunyaev and Y.B","venue":null,"work_id":null,"year":1972},"citing_paper":{"arxiv_id":"2511.00789","last_updated":"2026-06-04T04:14:37Z","snapshot_observed_at":"2026-08-15T06:24:02.254376Z","submitted_at":"2025-11-02T04:00:48Z","title":"A cosmographic analysis using DESI-DR2 and strong lensing: II. Distance Ratio measurements","version":2},"reference_index":61,"source":"pdf_text","source_observed_at":"2026-08-04T00:32:29.845070Z"},"links":{"citing_paper":"/paper/2511.00789"},"observation_digest":"sha256:2af9c0e60e00f3266b11cadd8d79ba337658e0fad4da3ac7707e79afe2c4378e","observation_id":"4218f402-d682-4e80-9db8-5cb9a103e8ba","resolution":{"observed_at":"2026-08-04T00:32:29.845070Z","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":"2026-08-18T15:21:57.876983Z","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":"2026-08-04T00:32:29.890655Z","title":"Adame et al.,DESI 2024 VI: cosmological constraints from the measurements of baryon acoustic oscillations,J","venue":null,"work_id":null,"year":2024},"citing_paper":{"arxiv_id":"2511.00789","last_updated":"2026-06-04T04:14:37Z","snapshot_observed_at":"2026-08-15T06:24:02.254376Z","submitted_at":"2025-11-02T04:00:48Z","title":"A cosmographic analysis using DESI-DR2 and strong lensing: II. Distance Ratio measurements","version":2},"reference_index":62,"source":"pdf_text","source_observed_at":"2026-08-04T00:32:29.890655Z"},"links":{"cited_paper":"/paper/2404.03002","citing_paper":"/paper/2511.00789"},"observation_digest":"sha256:65dfecc2085e9310457528184b6cbd013a22d040f0fcd78948ac3db1b7e995d4","observation_id":"be9d5c60-eeca-4dd9-8e61-37b70e6fd648","resolution":{"observed_at":"2026-08-04T00:32:29.890655Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2112.03863","last_updated":"2022-02-07T19:00:01Z","snapshot_observed_at":"2026-07-06T12:16:15.735863Z","submitted_at":"2021-12-07T17:57:21Z","title":"The Pantheon+ Analysis: The Full Dataset and Light-Curve Release","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2112.03863","snapshot_observed_at":"2026-08-04T00:32:29.943819Z","title":"Scolnic, D","venue":null,"work_id":null,"year":2022},"citing_paper":{"arxiv_id":"2511.00789","last_updated":"2026-06-04T04:14:37Z","snapshot_observed_at":"2026-08-15T06:24:02.254376Z","submitted_at":"2025-11-02T04:00:48Z","title":"A cosmographic analysis using DESI-DR2 and strong lensing: II. Distance Ratio measurements","version":2},"reference_index":63,"source":"pdf_text","source_observed_at":"2026-08-04T00:32:29.943819Z"},"links":{"cited_paper":"/paper/2112.03863","citing_paper":"/paper/2511.00789"},"observation_digest":"sha256:e9c04c4d8a61f3945ebe1546fb3d48f46dbbf638d1200b9d9a4fae8881d1b16a","observation_id":"a160df9a-ab5c-4186-8c3e-873cae287818","resolution":{"observed_at":"2026-08-04T00:32:29.943819Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2311.12098","last_updated":"2025-06-20T17:34:15Z","snapshot_observed_at":"2026-08-20T01:14:42.272285Z","submitted_at":"2023-11-20T19:00:01Z","title":"Union Through UNITY: Cosmology with 2,000 SNe Using a Unified Bayesian Framework","version":4},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2311.12098","snapshot_observed_at":"2026-08-04T00:32:30.006668Z","title":"Rubin, G","venue":null,"work_id":null,"year":2000},"citing_paper":{"arxiv_id":"2511.00789","last_updated":"2026-06-04T04:14:37Z","snapshot_observed_at":"2026-08-15T06:24:02.254376Z","submitted_at":"2025-11-02T04:00:48Z","title":"A cosmographic analysis using DESI-DR2 and strong lensing: II. Distance Ratio measurements","version":2},"reference_index":64,"source":"pdf_text","source_observed_at":"2026-08-04T00:32:30.006668Z"},"links":{"cited_paper":"/paper/2311.12098","citing_paper":"/paper/2511.00789"},"observation_digest":"sha256:8fbe74bf32c2b9a3c20a8a6a2b2abbaaa44cd386b0c1b48f9220fe1f1bea31e6","observation_id":"e5da371d-fff1-4e01-919e-291a454b5935","resolution":{"observed_at":"2026-08-04T00:32:30.006668Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2401.02929","last_updated":"2025-07-20T07:40:37Z","snapshot_observed_at":"2026-08-19T08:23:29.124703Z","submitted_at":"2024-01-05T18:14:39Z","title":"The Dark Energy Survey: Cosmology Results With ~1500 New High-redshift Type Ia Supernovae Using The Full 5-year Dataset","version":4},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2401.02929","snapshot_observed_at":"2026-08-04T00:32:30.040430Z","title":"Abbott, M","venue":null,"work_id":null,"year":2024},"citing_paper":{"arxiv_id":"2511.00789","last_updated":"2026-06-04T04:14:37Z","snapshot_observed_at":"2026-08-15T06:24:02.254376Z","submitted_at":"2025-11-02T04:00:48Z","title":"A cosmographic analysis using DESI-DR2 and strong lensing: II. Distance Ratio measurements","version":2},"reference_index":65,"source":"pdf_text","source_observed_at":"2026-08-04T00:32:30.040430Z"},"links":{"cited_paper":"/paper/2401.02929","citing_paper":"/paper/2511.00789"},"observation_digest":"sha256:94c78cbb61e23dec93ff4b9b07dd74fa2b5987bf1b976fdec05cf9ead6131d2c","observation_id":"e224ec53-4ddb-48a7-8516-18e745e6fce3","resolution":{"observed_at":"2026-08-04T00:32:30.040430Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"1811.02377","last_updated":"2019-06-01T16:07:38Z","snapshot_observed_at":"2026-08-14T18:03:23.720965Z","submitted_at":"2018-11-06T14:42:52Z","title":"First Cosmology Results Using Type Ia Supernovae From the Dark Energy Survey: Analysis, Systematic Uncertainties, and Validation","version":5},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"1811.02377","snapshot_observed_at":"2026-08-04T00:32:30.118903Z","title":"Brout, D","venue":null,"work_id":null,"year":2019},"citing_paper":{"arxiv_id":"2511.00789","last_updated":"2026-06-04T04:14:37Z","snapshot_observed_at":"2026-08-15T06:24:02.254376Z","submitted_at":"2025-11-02T04:00:48Z","title":"A cosmographic analysis using DESI-DR2 and strong lensing: II. Distance Ratio measurements","version":2},"reference_index":66,"source":"pdf_text","source_observed_at":"2026-08-04T00:32:30.118903Z"},"links":{"cited_paper":"/paper/1811.02377","citing_paper":"/paper/2511.00789"},"observation_digest":"sha256:5b8d6524261b0dd46a6f0f8fa624de757a080b76d990fde638d8320e3da8aac5","observation_id":"c7501ddb-1ba8-4889-b739-c1b937c1166d","resolution":{"observed_at":"2026-08-04T00:32:30.118903Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2004.10206","last_updated":"2020-11-24T12:56:09Z","snapshot_observed_at":"2026-08-08T23:31:45.425506Z","submitted_at":"2020-04-21T18:00:01Z","title":"It's Dust: Solving the Mysteries of the Intrinsic Scatter and Host-Galaxy Dependence of Standardized Type Ia Supernova Brightnesses","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2004.10206","snapshot_observed_at":"2026-08-04T00:32:30.174367Z","title":"Brout and D","venue":null,"work_id":null,"year":2021},"citing_paper":{"arxiv_id":"2511.00789","last_updated":"2026-06-04T04:14:37Z","snapshot_observed_at":"2026-08-15T06:24:02.254376Z","submitted_at":"2025-11-02T04:00:48Z","title":"A cosmographic analysis using DESI-DR2 and strong lensing: II. Distance Ratio measurements","version":2},"reference_index":67,"source":"pdf_text","source_observed_at":"2026-08-04T00:32:30.174367Z"},"links":{"cited_paper":"/paper/2004.10206","citing_paper":"/paper/2511.00789"},"observation_digest":"sha256:b4df36b818267d86885a1dc161e0fb93100aebd045056db56dad38b0367b6a62","observation_id":"03e059fa-112c-40e4-842d-728fa745376d","resolution":{"observed_at":"2026-08-04T00:32:30.174367Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2102.01776","last_updated":"2021-02-02T22:01:19Z","snapshot_observed_at":"2026-08-16T18:48:10.240738Z","submitted_at":"2021-02-02T22:01:19Z","title":"Improved Treatment of Host-Galaxy Correlations in Cosmological Analyses With Type Ia Supernovae","version":1},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2102.01776","snapshot_observed_at":"2026-08-04T00:32:30.231835Z","title":"Popovic, D","venue":null,"work_id":null,"year":2021},"citing_paper":{"arxiv_id":"2511.00789","last_updated":"2026-06-04T04:14:37Z","snapshot_observed_at":"2026-08-15T06:24:02.254376Z","submitted_at":"2025-11-02T04:00:48Z","title":"A cosmographic analysis using DESI-DR2 and strong lensing: II. Distance Ratio measurements","version":2},"reference_index":68,"source":"pdf_text","source_observed_at":"2026-08-04T00:32:30.231835Z"},"links":{"cited_paper":"/paper/2102.01776","citing_paper":"/paper/2511.00789"},"observation_digest":"sha256:0b70e43f0a852cbae55940581f60ec25b5342caf90c5a1cbccbbb4692baac300","observation_id":"9f0f1693-dc8e-403e-a00f-a8a4e72df282","resolution":{"observed_at":"2026-08-04T00:32:30.231835Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2112.04456","last_updated":"2022-12-05T15:40:08Z","snapshot_observed_at":"2026-08-16T17:36:06.924847Z","submitted_at":"2021-12-08T18:31:33Z","title":"The Pantheon+ Analysis: Forward-Modeling the Dust and Intrinsic Colour Distributions of Type Ia Supernovae, and Quantifying their Impact on Cosmological Inferences","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2112.04456","snapshot_observed_at":"2026-08-04T00:32:30.298274Z","title":"Popovic, D","venue":null,"work_id":null,"year":2023},"citing_paper":{"arxiv_id":"2511.00789","last_updated":"2026-06-04T04:14:37Z","snapshot_observed_at":"2026-08-15T06:24:02.254376Z","submitted_at":"2025-11-02T04:00:48Z","title":"A cosmographic analysis using DESI-DR2 and strong lensing: II. Distance Ratio measurements","version":2},"reference_index":69,"source":"pdf_text","source_observed_at":"2026-08-04T00:32:30.298274Z"},"links":{"cited_paper":"/paper/2112.04456","citing_paper":"/paper/2511.00789"},"observation_digest":"sha256:e643dc7b37ee6202d15811a9d28cbad4beccac9d55a08371aece27f865bee382","observation_id":"644ab4fb-e5f0-4bd8-a125-7b730e808cd6","resolution":{"observed_at":"2026-08-04T00:32:30.298274Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"0705.3647","last_updated":"2007-05-24T19:17:09Z","snapshot_observed_at":"2026-08-15T10:40:08.663543Z","submitted_at":"2007-05-24T19:17:09Z","title":"The Baryon Fractions and Mass-to-Light Ratios of Early-Type Galaxies","version":1},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"0705.3647","snapshot_observed_at":"2026-08-04T00:32:30.354029Z","title":"Jiang and C.S","venue":null,"work_id":null,"year":2007},"citing_paper":{"arxiv_id":"2511.00789","last_updated":"2026-06-04T04:14:37Z","snapshot_observed_at":"2026-08-15T06:24:02.254376Z","submitted_at":"2025-11-02T04:00:48Z","title":"A cosmographic analysis using DESI-DR2 and strong lensing: II. Distance Ratio measurements","version":2},"reference_index":70,"source":"pdf_text","source_observed_at":"2026-08-04T00:32:30.354029Z"},"links":{"cited_paper":"/paper/0705.3647","citing_paper":"/paper/2511.00789"},"observation_digest":"sha256:7d2f9a1eaec75dfad5f16b5eecd4f4013fb9c5781bcd4b1a3623b1b09c54d7bf","observation_id":"eb64660b-9464-4e49-81a9-ddf14b631786","resolution":{"observed_at":"2026-08-04T00:32:30.354029Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"0911.1249","last_updated":"2010-03-02T12:37:00Z","snapshot_observed_at":"2026-08-18T19:46:06.416617Z","submitted_at":"2009-11-06T14:02:59Z","title":"High-Redshift Cosmography","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"0911.1249","snapshot_observed_at":"2026-08-04T00:32:30.479764Z","title":"Vitagliano, J.-Q","venue":null,"work_id":null,"year":2010},"citing_paper":{"arxiv_id":"2511.00789","last_updated":"2026-06-04T04:14:37Z","snapshot_observed_at":"2026-08-15T06:24:02.254376Z","submitted_at":"2025-11-02T04:00:48Z","title":"A cosmographic analysis using DESI-DR2 and strong lensing: II. Distance Ratio measurements","version":2},"reference_index":72,"source":"pdf_text","source_observed_at":"2026-08-04T00:32:30.479764Z"},"links":{"cited_paper":"/paper/0911.1249","citing_paper":"/paper/2511.00789"},"observation_digest":"sha256:079c849a68ff7b486f0c51d157373133be3a06ed9468f1019218c5aedb42d03a","observation_id":"6dc9a0cb-9c30-47a7-85ea-37a140f67e9c","resolution":{"observed_at":"2026-08-04T00:32:30.479764Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2008.03092","last_updated":"2020-08-07T11:27:08Z","snapshot_observed_at":"2026-08-20T17:12:33.150053Z","submitted_at":"2020-08-07T11:27:08Z","title":"Cosmography approach to dark energy cosmologies: new constrains using the Hubble diagrams of supernovae, quasars and gamma-ray bursts","version":1},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2008.03092","snapshot_observed_at":"2026-08-04T00:32:30.647369Z","title":"Rezaei, S","venue":null,"work_id":null,"year":2020},"citing_paper":{"arxiv_id":"2511.00789","last_updated":"2026-06-04T04:14:37Z","snapshot_observed_at":"2026-08-15T06:24:02.254376Z","submitted_at":"2025-11-02T04:00:48Z","title":"A cosmographic analysis using DESI-DR2 and strong lensing: II. Distance Ratio measurements","version":2},"reference_index":73,"source":"pdf_text","source_observed_at":"2026-08-04T00:32:30.647369Z"},"links":{"cited_paper":"/paper/2008.03092","citing_paper":"/paper/2511.00789"},"observation_digest":"sha256:865b6f8c7809e0df4ca7c34c0c764865ff712b4fa9e9afc4abb5cf893d59ac46","observation_id":"544d94ad-fc7c-4755-9213-359564d764e9","resolution":{"observed_at":"2026-08-04T00:32:30.647369Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"1803.01990","last_updated":"2018-11-26T01:11:31Z","snapshot_observed_at":"2026-08-14T19:39:13.897438Z","submitted_at":"2018-03-06T02:31:10Z","title":"The distance sum rule from strong lensing systems and quasars - test of cosmic curvature and beyond","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"1803.01990","snapshot_observed_at":"2026-08-04T00:32:30.781921Z","title":null,"venue":null,"work_id":null,"year":2019},"citing_paper":{"arxiv_id":"2511.00789","last_updated":"2026-06-04T04:14:37Z","snapshot_observed_at":"2026-08-15T06:24:02.254376Z","submitted_at":"2025-11-02T04:00:48Z","title":"A cosmographic analysis using DESI-DR2 and strong lensing: II. Distance Ratio measurements","version":2},"reference_index":74,"source":"pdf_text","source_observed_at":"2026-08-04T00:32:30.781921Z"},"links":{"cited_paper":"/paper/1803.01990","citing_paper":"/paper/2511.00789"},"observation_digest":"sha256:b95904b6f53a5b764543f31c8702fa7e05b0ef17da7cc34c3f0d9d056eb6df0a","observation_id":"ad28c157-f3f0-4a2b-8ba6-4d4ed40e5615","resolution":{"observed_at":"2026-08-04T00:32:30.781921Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2002.06354","last_updated":"2021-02-10T07:07:49Z","snapshot_observed_at":"2026-08-11T19:09:08.066245Z","submitted_at":"2020-02-15T10:04:46Z","title":"Constraining Cosmological and Galaxy Parameters using Strong Gravitational Lensing Systems","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2002.06354","snapshot_observed_at":"2026-08-04T00:32:30.895334Z","title":"Kumar, D","venue":null,"work_id":null,"year":2021},"citing_paper":{"arxiv_id":"2511.00789","last_updated":"2026-06-04T04:14:37Z","snapshot_observed_at":"2026-08-15T06:24:02.254376Z","submitted_at":"2025-11-02T04:00:48Z","title":"A cosmographic analysis using DESI-DR2 and strong lensing: II. Distance Ratio measurements","version":2},"reference_index":75,"source":"pdf_text","source_observed_at":"2026-08-04T00:32:30.895334Z"},"links":{"cited_paper":"/paper/2002.06354","citing_paper":"/paper/2511.00789"},"observation_digest":"sha256:6313fbbe92c7dc9db5ee3018ad54b2b351f4a43bddac81fb50c1b517c77d8bfd","observation_id":"87acc882-0823-4cae-a84e-b27b0c85f919","resolution":{"observed_at":"2026-08-04T00:32:30.895334Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"1910.13970","last_updated":"2025-07-09T12:22:45Z","snapshot_observed_at":"2026-08-12T19:40:10.586390Z","submitted_at":"2019-10-30T16:38:10Z","title":"GetDist: a Python package for analysing Monte Carlo samples","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"1910.13970","snapshot_observed_at":"2026-08-04T00:32:31.040312Z","title":"Lewis,GetDist: a Python package for analysing Monte Carlo samples,arXiv e-prints(2019) arXiv:1910.13970 [1910.13970]","venue":null,"work_id":null,"year":2019},"citing_paper":{"arxiv_id":"2511.00789","last_updated":"2026-06-04T04:14:37Z","snapshot_observed_at":"2026-08-15T06:24:02.254376Z","submitted_at":"2025-11-02T04:00:48Z","title":"A cosmographic analysis using DESI-DR2 and strong lensing: II. Distance Ratio measurements","version":2},"reference_index":76,"source":"pdf_text","source_observed_at":"2026-08-04T00:32:31.040312Z"},"links":{"cited_paper":"/paper/1910.13970","citing_paper":"/paper/2511.00789"},"observation_digest":"sha256:a9f6c0ab698f44bc894a5855ef42962a6aba21c36b6072ac53ec26e6170c9c7c","observation_id":"f9f7febe-6871-445a-826e-311848939400","resolution":{"observed_at":"2026-08-04T00:32:31.040312Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":null,"snapshot_observed_at":"2026-08-04T00:32:31.135631Z","title":"Oliphant,A guide to numpy,Trelgol Publishing USA1(2006)","venue":null,"work_id":null,"year":2006},"citing_paper":{"arxiv_id":"2511.00789","last_updated":"2026-06-04T04:14:37Z","snapshot_observed_at":"2026-08-15T06:24:02.254376Z","submitted_at":"2025-11-02T04:00:48Z","title":"A cosmographic analysis using DESI-DR2 and strong lensing: II. Distance Ratio measurements","version":2},"reference_index":77,"source":"pdf_text","source_observed_at":"2026-08-04T00:32:31.135631Z"},"links":{"citing_paper":"/paper/2511.00789"},"observation_digest":"sha256:63285200b94ca87b81d5d333d8916f378b847da7ba4b78850e2baec0c3cfe48c","observation_id":"6aa20fc4-f375-43b9-b201-e7efae751172","resolution":{"observed_at":"2026-08-04T00:32:31.135631Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":null,"snapshot_observed_at":"2026-08-04T00:32:31.285157Z","title":"Hunter,Matplotlib: A 2d graphics environment,Comput","venue":null,"work_id":null,"year":2007},"citing_paper":{"arxiv_id":"2511.00789","last_updated":"2026-06-04T04:14:37Z","snapshot_observed_at":"2026-08-15T06:24:02.254376Z","submitted_at":"2025-11-02T04:00:48Z","title":"A cosmographic analysis using DESI-DR2 and strong lensing: II. Distance Ratio measurements","version":2},"reference_index":78,"source":"pdf_text","source_observed_at":"2026-08-04T00:32:31.285157Z"},"links":{"citing_paper":"/paper/2511.00789"},"observation_digest":"sha256:289a87de13d601f7e4990fd8de9164aec7e595f961203e7c92edc29d5d23f0b8","observation_id":"fb5b352e-1102-4b7a-b094-70db90603b84","resolution":{"observed_at":"2026-08-04T00:32:31.285157Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"1202.3665","last_updated":"2013-11-25T15:56:48Z","snapshot_observed_at":"2026-07-06T02:43:00.981478Z","submitted_at":"2012-02-16T20:41:19Z","title":"emcee: The MCMC Hammer","version":4},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"1202.3665","snapshot_observed_at":"2026-08-04T00:32:31.443709Z","title":"Foreman-Mackey, D.W","venue":null,"work_id":null,"year":2013},"citing_paper":{"arxiv_id":"2511.00789","last_updated":"2026-06-04T04:14:37Z","snapshot_observed_at":"2026-08-15T06:24:02.254376Z","submitted_at":"2025-11-02T04:00:48Z","title":"A cosmographic analysis using DESI-DR2 and strong lensing: II. Distance Ratio measurements","version":2},"reference_index":79,"source":"pdf_text","source_observed_at":"2026-08-04T00:32:31.443709Z"},"links":{"cited_paper":"/paper/1202.3665","citing_paper":"/paper/2511.00789"},"observation_digest":"sha256:53148f5f5766a19e5b2d8b673a23f386a0714cb1cc22e37e938109b7ab2bd202","observation_id":"b2a3bbe0-5ded-45c0-aacd-fb159a2f8ec7","resolution":{"observed_at":"2026-08-04T00:32:31.443709Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}}],"paper":{"arxiv_id":"2511.00789","last_updated":"2026-06-04T04:14:37Z","latest_version":2,"primary_category":"astro-ph.CO","snapshot_observed_at":"2026-08-15T06:24:02.254376Z","submitted_at":"2025-11-02T04:00:48Z","title":"A cosmographic analysis using DESI-DR2 and strong lensing: II. Distance Ratio measurements"},"reference_resolution":{"displayed":78,"state_counts":{"malformed_identifier":0,"metadata_mismatch":0,"parse_uncertain":0,"unresolved":78,"verified_exact":0,"verified_fuzzy":0},"total_outbound_references":78},"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":"2026-08-21T06:32:19.484+00:00","source":"crossref"},{"observed_at":"2026-08-21T06:32:16.066871+00:00","source":"retraction_watch"}],"thesis":"As of 21 August 2026, this Paper Citation Record lists 78 of 78 outbound references and 0 inbound Pith citation observations for arXiv:2511.00789."}