{"as_of":"2026-08-14T09:15:00Z","caps":{"database_statements":6,"inbound":100,"outbound":100},"context_digest":"sha256:8b2e6823ed4214652102bc9e66b2f6327aa1bc86caae2fedd69aa475c6e6bafd","coverage":[{"denominator":54,"lane":"reference_resolution","note":"Typed states for the displayed outbound observations.","records_observed":54,"source":"paper_references, paper_reference_links","source_observed_at":"2026-08-12T21:36:14.239144Z","state":"measured"},{"denominator":55,"lane":"standing_notices","note":"One-hop event checks from named stored sources.","records_observed":55,"source":"scholarly_work_events, retraction_status_cache","source_observed_at":"2026-08-14T06:32:32.682623+00:00","state":"measured"},{"denominator":1,"lane":"inbound_itemization","note":"Pith citing papers itemized under the disclosed page cap.","records_observed":1,"source":"paper_references, paper_reference_links","source_observed_at":"2026-08-12T15:36:37.523333Z","state":"measured"},{"denominator":1,"lane":"external_citation_measurements","note":"A source-named dated measurement, never combined with another source.","records_observed":0,"source":"pith","source_observed_at":"2026-08-12T18:16:22.223912Z","state":"measured"}],"external_citation_measurements":[],"inbound":[{"citation":{"cited_paper":{"arxiv_id":"2411.08498","last_updated":"2024-12-27T06:29:18Z","snapshot_observed_at":"2026-08-13T02:19:47.582623Z","submitted_at":"2024-11-13T10:32:37Z","title":"A dark energy parameterization independent constraint of the spatial curvature $\\Omega_K$","version":2},"cited_work":{"arxiv_id":"2411.08498","doi":"10.48550/arxiv.2411.08498","metadata_source":"pith","pith_arxiv_id":"2411.08498","snapshot_observed_at":"2026-08-12T18:16:22.223912Z","title":"A dark energy parameterization independent constraint of the spatial curvature $\\Omega_K$","venue":"astro-ph.CO","work_id":"06859dcc-3216-443a-8d1a-397db4b650f4","year":2024},"citing_paper":{"arxiv_id":"2411.14154","last_updated":"2024-11-21T14:18:26Z","snapshot_observed_at":"2026-08-13T02:19:15.914453Z","submitted_at":"2024-11-21T14:18:26Z","title":"Determination of cosmic curvature independent of the sound horizon and $H_0$ using BOSS/eBOSS and DESI DR1 BAO observations","version":1},"reference_index":75,"source":"pdf_text","source_observed_at":"2026-08-12T15:36:37.523333Z"},"links":{"cited_paper":"/paper/2411.08498","citing_paper":"/paper/2411.14154"},"observation_digest":"sha256:737560242f8ac1b04b32e6c9ce3e495cf24e0136a6f3df77c917bec2dc319b82","observation_id":"84e8172d-5e4e-4fe5-a62d-ac9f97facf83","resolution":{"observed_at":"2026-08-12T15:36:37.554172Z","resolver_source":"local_arxiv","status":"verified_exact"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-14T06:32:32.682623+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-14T06:32:32.682623+00:00","source":"crossref"},{"observed_at":"2026-08-14T06:32:18.44784+00:00","source":"retraction_watch"}],"state":"measured"}}],"links":{"evidence":"/evidence","html":"/paper/2411.08498/citation-record","integrity":"/paper/2411.08498/integrity","json":"/paper/2411.08498/citation-record.json","paper":"/paper/2411.08498"},"outbound":[{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":"raw_reference","pith_arxiv_id":null,"snapshot_observed_at":"2026-08-12T21:36:15.176384Z","title":"Guth, Inflationary universe: A possible solution to the horizon and flatness problems , Physical Review D 23 (1981) 347","venue":null,"work_id":"4b14c3c8-480e-47d9-bc8d-a9dda8888c64","year":1981},"citing_paper":{"arxiv_id":"2411.08498","last_updated":"2024-12-27T06:29:18Z","snapshot_observed_at":"2026-08-13T02:19:47.582623Z","submitted_at":"2024-11-13T10:32:37Z","title":"A dark energy parameterization independent constraint of the spatial curvature $\\Omega_K$","version":2},"reference_index":1,"source":"pdf_text","source_observed_at":"2026-08-12T21:36:13.986094Z"},"links":{"citing_paper":"/paper/2411.08498"},"observation_digest":"sha256:be3cbb0013d21c56464cbdcbd388262440cdc557983d290fc8103bd5583879c7","observation_id":"35d8188e-804d-404a-a15d-094586ec12e6","resolution":{"observed_at":"2026-08-12T21:36:15.181725Z","resolver_source":"raw_fallback","status":"verified_fuzzy"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-14T06:32:32.682623+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-14T06:32:32.682623+00:00","source":"crossref"},{"observed_at":"2026-08-14T06:32:18.44784+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":null,"snapshot_observed_at":"2026-08-12T21:36:13.991935Z","title":"Linde, A new inflationary universe scenario: A possible solution of the horizon, flatness, homogeneity, isotropy and primordial monopole problems , Physics Letters B 108 (1982) 389","venue":null,"work_id":null,"year":1982},"citing_paper":{"arxiv_id":"2411.08498","last_updated":"2024-12-27T06:29:18Z","snapshot_observed_at":"2026-08-13T02:19:47.582623Z","submitted_at":"2024-11-13T10:32:37Z","title":"A dark energy parameterization independent constraint of the spatial curvature $\\Omega_K$","version":2},"reference_index":2,"source":"pdf_text","source_observed_at":"2026-08-12T21:36:13.991935Z"},"links":{"citing_paper":"/paper/2411.08498"},"observation_digest":"sha256:07937635c213e704289461b09f379b39a9fd982151e95bddee1d899900dd3eac","observation_id":"9698247c-845c-4f92-b7df-12847b582594","resolution":{"observed_at":"2026-08-12T21:36:13.991935Z","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":"raw_reference","pith_arxiv_id":null,"snapshot_observed_at":"2026-08-12T21:36:15.149107Z","title":"Netterfield, P.A.R","venue":null,"work_id":"c31cf5da-96f9-4119-b507-0b17a34612e0","year":2002},"citing_paper":{"arxiv_id":"2411.08498","last_updated":"2024-12-27T06:29:18Z","snapshot_observed_at":"2026-08-13T02:19:47.582623Z","submitted_at":"2024-11-13T10:32:37Z","title":"A dark energy parameterization independent constraint of the spatial curvature $\\Omega_K$","version":2},"reference_index":3,"source":"pdf_text","source_observed_at":"2026-08-12T21:36:13.997404Z"},"links":{"citing_paper":"/paper/2411.08498"},"observation_digest":"sha256:fc2f29573f70c534e1c6fcf87a6e22cc8c7f87d7c9f7789ff2217bab8fbe8679","observation_id":"2f708809-da08-4b8d-8188-4e3cdfbcbb88","resolution":{"observed_at":"2026-08-12T21:36:15.153762Z","resolver_source":"raw_fallback","status":"verified_fuzzy"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-14T06:32:32.682623+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-14T06:32:32.682623+00:00","source":"crossref"},{"observed_at":"2026-08-14T06:32:18.44784+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":"raw_reference","pith_arxiv_id":null,"snapshot_observed_at":"2026-08-12T21:36:15.133591Z","title":"Hanany, P","venue":null,"work_id":"d51f4fce-7677-4881-ba9e-0f3d7937ed21","year":2000},"citing_paper":{"arxiv_id":"2411.08498","last_updated":"2024-12-27T06:29:18Z","snapshot_observed_at":"2026-08-13T02:19:47.582623Z","submitted_at":"2024-11-13T10:32:37Z","title":"A dark energy parameterization independent constraint of the spatial curvature $\\Omega_K$","version":2},"reference_index":4,"source":"pdf_text","source_observed_at":"2026-08-12T21:36:14.001934Z"},"links":{"citing_paper":"/paper/2411.08498"},"observation_digest":"sha256:402cb389c26916f9af205a1771fdcfe5a77f2c2b7063e78ec4cf1034d23cc9ad","observation_id":"9e4bae18-efad-4853-b214-6320908b4491","resolution":{"observed_at":"2026-08-12T21:36:15.138321Z","resolver_source":"raw_fallback","status":"verified_fuzzy"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-14T06:32:32.682623+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-14T06:32:32.682623+00:00","source":"crossref"},{"observed_at":"2026-08-14T06:32:18.44784+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":"raw_reference","pith_arxiv_id":null,"snapshot_observed_at":"2026-08-12T21:36:15.116785Z","title":"de Bernardis, P.A.R","venue":null,"work_id":"2f86a6d2-e081-4277-abb9-721cc9f203e2","year":2000},"citing_paper":{"arxiv_id":"2411.08498","last_updated":"2024-12-27T06:29:18Z","snapshot_observed_at":"2026-08-13T02:19:47.582623Z","submitted_at":"2024-11-13T10:32:37Z","title":"A dark energy parameterization independent constraint of the spatial curvature $\\Omega_K$","version":2},"reference_index":5,"source":"pdf_text","source_observed_at":"2026-08-12T21:36:14.006377Z"},"links":{"citing_paper":"/paper/2411.08498"},"observation_digest":"sha256:260a09b66d59b1b9f0174c560f6f49bbdc41d6bf9d57c479bfe7ac234d92d344","observation_id":"9ac70e2b-6aee-45a7-9e50-f276bdf3b15b","resolution":{"observed_at":"2026-08-12T21:36:15.122422Z","resolver_source":"raw_fallback","status":"verified_fuzzy"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-14T06:32:32.682623+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-14T06:32:32.682623+00:00","source":"crossref"},{"observed_at":"2026-08-14T06:32:18.44784+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":{"arxiv_id":"astro-ph/0005124","last_updated":"2001-09-04T14:52:06Z","snapshot_observed_at":"2026-08-14T03:15:42.844736Z","submitted_at":"2000-05-08T22:25:27Z","title":"Constraints on Cosmological Parameters from MAXIMA-1","version":3},"cited_work":{"arxiv_id":"astro-ph/0005124","doi":null,"metadata_source":"pith","pith_arxiv_id":"astro-ph/0005124","snapshot_observed_at":"2026-08-12T21:36:15.038681Z","title":"Constraints on Cosmological Parameters from MAXIMA-1","venue":"astro-ph","work_id":"1d9b0321-c3b3-4460-ab15-215fe3cf4130","year":2000},"citing_paper":{"arxiv_id":"2411.08498","last_updated":"2024-12-27T06:29:18Z","snapshot_observed_at":"2026-08-13T02:19:47.582623Z","submitted_at":"2024-11-13T10:32:37Z","title":"A dark energy parameterization independent constraint of the spatial curvature $\\Omega_K$","version":2},"reference_index":6,"source":"pdf_text","source_observed_at":"2026-08-12T21:36:14.011164Z"},"links":{"cited_paper":"/paper/astro-ph/0005124","citing_paper":"/paper/2411.08498"},"observation_digest":"sha256:403013fbf52b136f4a31378c551f0b387a5e30c19063df7df2195c8c0b234c58","observation_id":"4dad0ea5-d660-4324-9b7f-845d2d01908f","resolution":{"observed_at":"2026-08-12T21:36:15.044271Z","resolver_source":"local_arxiv","status":"verified_exact"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-14T06:32:32.682623+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-14T06:32:32.682623+00:00","source":"crossref"},{"observed_at":"2026-08-14T06:32:18.44784+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":"raw_reference","pith_arxiv_id":null,"snapshot_observed_at":"2026-08-12T21:36:15.100618Z","title":"Jaffe, P.A.R","venue":null,"work_id":"a7406e27-f1e5-44ca-80fc-09cba6da4376","year":2001},"citing_paper":{"arxiv_id":"2411.08498","last_updated":"2024-12-27T06:29:18Z","snapshot_observed_at":"2026-08-13T02:19:47.582623Z","submitted_at":"2024-11-13T10:32:37Z","title":"A dark energy parameterization independent constraint of the spatial curvature $\\Omega_K$","version":2},"reference_index":7,"source":"pdf_text","source_observed_at":"2026-08-12T21:36:14.016978Z"},"links":{"citing_paper":"/paper/2411.08498"},"observation_digest":"sha256:03cbe087d5702094abd296c5fb463c7dd289c09ce3439d4c86bbf43550acb96f","observation_id":"46de2ae8-6cea-4754-aa0f-1c42f5860c1d","resolution":{"observed_at":"2026-08-12T21:36:15.105771Z","resolver_source":"raw_fallback","status":"verified_fuzzy"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-14T06:32:32.682623+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-14T06:32:32.682623+00:00","source":"crossref"},{"observed_at":"2026-08-14T06:32:18.44784+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":{"arxiv_id":"2007.08991","last_updated":"2024-07-09T09:56:49Z","snapshot_observed_at":"2026-08-13T11:53:26.094346Z","submitted_at":"2020-07-17T14:09:48Z","title":"The Completed SDSS-IV extended Baryon Oscillation Spectroscopic Survey: Cosmological Implications from two Decades of Spectroscopic Surveys at the Apache Point observatory","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2007.08991","snapshot_observed_at":"2026-08-12T21:36:14.022051Z","title":null,"venue":null,"work_id":null,"year":2021},"citing_paper":{"arxiv_id":"2411.08498","last_updated":"2024-12-27T06:29:18Z","snapshot_observed_at":"2026-08-13T02:19:47.582623Z","submitted_at":"2024-11-13T10:32:37Z","title":"A dark energy parameterization independent constraint of the spatial curvature $\\Omega_K$","version":2},"reference_index":8,"source":"pdf_text","source_observed_at":"2026-08-12T21:36:14.022051Z"},"links":{"cited_paper":"/paper/2007.08991","citing_paper":"/paper/2411.08498"},"observation_digest":"sha256:be2e91e4185c21e1e65898abcabbe9f649f4e3324923134d60e28580453f3734","observation_id":"65387610-487b-4641-bda2-ac2345f5fc60","resolution":{"observed_at":"2026-08-12T21:36:14.022051Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"1807.06209","last_updated":"2021-08-09T10:43:18Z","snapshot_observed_at":"2026-07-06T02:11:23.670680Z","submitted_at":"2018-07-17T04:05:07Z","title":"Planck 2018 results. VI. Cosmological parameters","version":4},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"1807.06209","snapshot_observed_at":"2026-08-12T21:36:14.027532Z","title":"Aghanim, Y","venue":null,"work_id":null,"year":2020},"citing_paper":{"arxiv_id":"2411.08498","last_updated":"2024-12-27T06:29:18Z","snapshot_observed_at":"2026-08-13T02:19:47.582623Z","submitted_at":"2024-11-13T10:32:37Z","title":"A dark energy parameterization independent constraint of the spatial curvature $\\Omega_K$","version":2},"reference_index":9,"source":"pdf_text","source_observed_at":"2026-08-12T21:36:14.027532Z"},"links":{"cited_paper":"/paper/1807.06209","citing_paper":"/paper/2411.08498"},"observation_digest":"sha256:63482ba1d3fd61b4d35a31fb813ac0364544c4202df812e0d207a2992d424598","observation_id":"8d0483b5-6238-427e-8fa1-048e900993c3","resolution":{"observed_at":"2026-08-12T21:36:14.027532Z","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":"raw_reference","pith_arxiv_id":null,"snapshot_observed_at":"2026-08-12T21:36:15.083960Z","title":"Anselmi, M.F","venue":null,"work_id":"2c3c83d1-d580-4cd7-987c-03e4aa46e6ae","year":2023},"citing_paper":{"arxiv_id":"2411.08498","last_updated":"2024-12-27T06:29:18Z","snapshot_observed_at":"2026-08-13T02:19:47.582623Z","submitted_at":"2024-11-13T10:32:37Z","title":"A dark energy parameterization independent constraint of the spatial curvature $\\Omega_K$","version":2},"reference_index":10,"source":"pdf_text","source_observed_at":"2026-08-12T21:36:14.032019Z"},"links":{"citing_paper":"/paper/2411.08498"},"observation_digest":"sha256:433e40e9d0bfdeeff90de06b3787193243830b9c3a5727d0bf7df3ccae7d948d","observation_id":"bda0a1f5-a291-49cc-a76e-da43f83b7691","resolution":{"observed_at":"2026-08-12T21:36:15.089244Z","resolver_source":"raw_fallback","status":"verified_fuzzy"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-14T06:32:32.682623+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-14T06:32:32.682623+00:00","source":"crossref"},{"observed_at":"2026-08-14T06:32:18.44784+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":{"arxiv_id":"astro-ph/9702100","last_updated":"1997-08-27T08:28:13Z","snapshot_observed_at":"2026-07-07T01:15:55.239042Z","submitted_at":"1997-02-12T04:19:10Z","title":"Forecasting Cosmic Parameter Errors from Microwave Background Anisotropy Experiments","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"astro-ph/9702100","snapshot_observed_at":"2026-08-12T21:36:14.036857Z","title":null,"venue":null,"work_id":null,"year":1997},"citing_paper":{"arxiv_id":"2411.08498","last_updated":"2024-12-27T06:29:18Z","snapshot_observed_at":"2026-08-13T02:19:47.582623Z","submitted_at":"2024-11-13T10:32:37Z","title":"A dark energy parameterization independent constraint of the spatial curvature $\\Omega_K$","version":2},"reference_index":11,"source":"pdf_text","source_observed_at":"2026-08-12T21:36:14.036857Z"},"links":{"cited_paper":"/paper/astro-ph/9702100","citing_paper":"/paper/2411.08498"},"observation_digest":"sha256:891be1181533595d4a54ad374dfbf4f3995afe67eadfc55347fcf0620fed93e6","observation_id":"b237b818-c7b1-4bef-8c5c-3c8fab786895","resolution":{"observed_at":"2026-08-12T21:36:14.036857Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"astro-ph/9702157","last_updated":"1997-09-11T22:32:13Z","snapshot_observed_at":"2026-07-07T01:15:55.239042Z","submitted_at":"1997-02-19T00:23:59Z","title":"Microwave Background Constraints on Cosmological Parameters","version":3},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"astro-ph/9702157","snapshot_observed_at":"2026-08-12T21:36:14.042025Z","title":"Zaldarriaga, D.N","venue":null,"work_id":null,"year":1997},"citing_paper":{"arxiv_id":"2411.08498","last_updated":"2024-12-27T06:29:18Z","snapshot_observed_at":"2026-08-13T02:19:47.582623Z","submitted_at":"2024-11-13T10:32:37Z","title":"A dark energy parameterization independent constraint of the spatial curvature $\\Omega_K$","version":2},"reference_index":12,"source":"pdf_text","source_observed_at":"2026-08-12T21:36:14.042025Z"},"links":{"cited_paper":"/paper/astro-ph/9702157","citing_paper":"/paper/2411.08498"},"observation_digest":"sha256:fcfb744a85d08c9dba0f81968e5667220bdad3fdfa66ab6dba2fbc1e795be037","observation_id":"a211ff56-d731-4591-b55d-8ee8eb9454ce","resolution":{"observed_at":"2026-08-12T21:36:14.042025Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"1502.01589","last_updated":"2016-06-17T14:55:14Z","snapshot_observed_at":"2026-08-04T11:38:00.035477Z","submitted_at":"2015-02-05T15:08:33Z","title":"Planck 2015 results. XIII. Cosmological parameters","version":3},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"1502.01589","snapshot_observed_at":"2026-08-12T21:36:14.047112Z","title":null,"venue":null,"work_id":null,"year":2016},"citing_paper":{"arxiv_id":"2411.08498","last_updated":"2024-12-27T06:29:18Z","snapshot_observed_at":"2026-08-13T02:19:47.582623Z","submitted_at":"2024-11-13T10:32:37Z","title":"A dark energy parameterization independent constraint of the spatial curvature $\\Omega_K$","version":2},"reference_index":13,"source":"pdf_text","source_observed_at":"2026-08-12T21:36:14.047112Z"},"links":{"cited_paper":"/paper/1502.01589","citing_paper":"/paper/2411.08498"},"observation_digest":"sha256:620a4f8fdc57b2de7bef2ab565ae05f1c8a28a7db05149d1d8cda4e4b0a08c36","observation_id":"8c38421f-4e28-42c3-b24b-bccd09cd41e8","resolution":{"observed_at":"2026-08-12T21:36:14.047112Z","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":"2026-08-08T17:19:33.489680Z","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":"2026-08-12T21:36:14.052266Z","title":"Handley, Curvature tension: Evidence for a closed universe , Physical Review D 103 (2021) L041301 [1908.09139]","venue":null,"work_id":null,"year":2021},"citing_paper":{"arxiv_id":"2411.08498","last_updated":"2024-12-27T06:29:18Z","snapshot_observed_at":"2026-08-13T02:19:47.582623Z","submitted_at":"2024-11-13T10:32:37Z","title":"A dark energy parameterization independent constraint of the spatial curvature $\\Omega_K$","version":2},"reference_index":14,"source":"pdf_text","source_observed_at":"2026-08-12T21:36:14.052266Z"},"links":{"cited_paper":"/paper/1908.09139","citing_paper":"/paper/2411.08498"},"observation_digest":"sha256:27a0e55f014e2594efd0df765e2fc9141db0c9710f67f79f260652a6dd7bdf54","observation_id":"f4f119ec-45d6-4838-a780-9cbf5087762a","resolution":{"observed_at":"2026-08-12T21:36:14.052266Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2010.02230","last_updated":"2021-06-23T09:20:52Z","snapshot_observed_at":"2026-08-10T10:04:14.882294Z","submitted_at":"2020-10-05T18:00:03Z","title":"The galaxy power spectrum take on spatial curvature and cosmic concordance","version":3},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2010.02230","snapshot_observed_at":"2026-08-12T21:36:14.057494Z","title":"Vagnozzi, E","venue":null,"work_id":null,"year":2021},"citing_paper":{"arxiv_id":"2411.08498","last_updated":"2024-12-27T06:29:18Z","snapshot_observed_at":"2026-08-13T02:19:47.582623Z","submitted_at":"2024-11-13T10:32:37Z","title":"A dark energy parameterization independent constraint of the spatial curvature $\\Omega_K$","version":2},"reference_index":15,"source":"pdf_text","source_observed_at":"2026-08-12T21:36:14.057494Z"},"links":{"cited_paper":"/paper/2010.02230","citing_paper":"/paper/2411.08498"},"observation_digest":"sha256:3a1ba43957f147164fc94e28b330f63518ea2c723e6ea1087d400019b9b28fcb","observation_id":"7c054a54-7aea-4f11-a186-5035b69d07a7","resolution":{"observed_at":"2026-08-12T21:36:14.057494Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2011.11645","last_updated":"2020-12-16T16:55:42Z","snapshot_observed_at":"2026-08-09T19:52:26.183573Z","submitted_at":"2020-11-23T19:00:01Z","title":"Eppur \\`e piatto? The cosmic chronometer take on spatial curvature and cosmic concordance","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2011.11645","snapshot_observed_at":"2026-08-12T21:36:14.062612Z","title":"Vagnozzi, A","venue":null,"work_id":null,"year":2021},"citing_paper":{"arxiv_id":"2411.08498","last_updated":"2024-12-27T06:29:18Z","snapshot_observed_at":"2026-08-13T02:19:47.582623Z","submitted_at":"2024-11-13T10:32:37Z","title":"A dark energy parameterization independent constraint of the spatial curvature $\\Omega_K$","version":2},"reference_index":16,"source":"pdf_text","source_observed_at":"2026-08-12T21:36:14.062612Z"},"links":{"cited_paper":"/paper/2011.11645","citing_paper":"/paper/2411.08498"},"observation_digest":"sha256:3e3640c5683550ef9ef8df6d4144d238e0156588b68dc5ac949c8ff7c13c5052","observation_id":"0230875e-aa34-4d7b-9c3a-4772218bbfe4","resolution":{"observed_at":"2026-08-12T21:36:14.062612Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2104.02485","last_updated":"2021-04-06T13:10:32Z","snapshot_observed_at":"2026-08-13T19:44:53.624425Z","submitted_at":"2021-04-06T13:10:32Z","title":"Non-parametric spatial curvature inference using late-universe cosmological probes","version":1},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2104.02485","snapshot_observed_at":"2026-08-12T21:36:14.067495Z","title":"Dhawan, J","venue":null,"work_id":null,"year":2021},"citing_paper":{"arxiv_id":"2411.08498","last_updated":"2024-12-27T06:29:18Z","snapshot_observed_at":"2026-08-13T02:19:47.582623Z","submitted_at":"2024-11-13T10:32:37Z","title":"A dark energy parameterization independent constraint of the spatial curvature $\\Omega_K$","version":2},"reference_index":17,"source":"pdf_text","source_observed_at":"2026-08-12T21:36:14.067495Z"},"links":{"cited_paper":"/paper/2104.02485","citing_paper":"/paper/2411.08498"},"observation_digest":"sha256:2327ac28507f129b5cfa4f257cf59ce8e252adbe03c59789cfb669ffcad714bf","observation_id":"72839643-ee17-4baf-a60c-a9c7ee4b97e3","resolution":{"observed_at":"2026-08-12T21:36:14.067495Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"1903.07603","last_updated":"2019-03-27T15:38:08Z","snapshot_observed_at":"2026-08-03T04:46:01.318400Z","submitted_at":"2019-03-18T17:50:59Z","title":"Large Magellanic Cloud Cepheid Standards Provide a 1% Foundation for the Determination of the Hubble Constant and Stronger Evidence for Physics Beyond LambdaCDM","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"1903.07603","snapshot_observed_at":"2026-08-12T21:36:14.072497Z","title":"Riess, S","venue":null,"work_id":null,"year":2019},"citing_paper":{"arxiv_id":"2411.08498","last_updated":"2024-12-27T06:29:18Z","snapshot_observed_at":"2026-08-13T02:19:47.582623Z","submitted_at":"2024-11-13T10:32:37Z","title":"A dark energy parameterization independent constraint of the spatial curvature $\\Omega_K$","version":2},"reference_index":18,"source":"pdf_text","source_observed_at":"2026-08-12T21:36:14.072497Z"},"links":{"cited_paper":"/paper/1903.07603","citing_paper":"/paper/2411.08498"},"observation_digest":"sha256:57c0ab5378c518893ab11307cfba85ca031c3014292320da97d392664fb96b74","observation_id":"821e6484-9ec5-454f-9c36-7b57126b24ea","resolution":{"observed_at":"2026-08-12T21:36:14.072497Z","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":"2026-08-12T21:36:14.077824Z","title":"Riess, W","venue":null,"work_id":null,"year":2022},"citing_paper":{"arxiv_id":"2411.08498","last_updated":"2024-12-27T06:29:18Z","snapshot_observed_at":"2026-08-13T02:19:47.582623Z","submitted_at":"2024-11-13T10:32:37Z","title":"A dark energy parameterization independent constraint of the spatial curvature $\\Omega_K$","version":2},"reference_index":19,"source":"pdf_text","source_observed_at":"2026-08-12T21:36:14.077824Z"},"links":{"cited_paper":"/paper/2112.04510","citing_paper":"/paper/2411.08498"},"observation_digest":"sha256:d042c79fe5c77ffa8cf69014e51011ecbe4dc646af57c538ad9e3d76f9eb69e8","observation_id":"aba656b8-379b-46a5-9c4e-16af8d12f657","resolution":{"observed_at":"2026-08-12T21:36:14.077824Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"0712.3457","last_updated":"2008-03-17T20:01:52Z","snapshot_observed_at":"2026-08-08T01:16:57.412483Z","submitted_at":"2007-12-20T15:22:16Z","title":"A general test of the Copernican Principle","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"0712.3457","snapshot_observed_at":"2026-08-12T21:36:14.082205Z","title":"Clarkson, B","venue":null,"work_id":null,"year":2008},"citing_paper":{"arxiv_id":"2411.08498","last_updated":"2024-12-27T06:29:18Z","snapshot_observed_at":"2026-08-13T02:19:47.582623Z","submitted_at":"2024-11-13T10:32:37Z","title":"A dark energy parameterization independent constraint of the spatial curvature $\\Omega_K$","version":2},"reference_index":20,"source":"pdf_text","source_observed_at":"2026-08-12T21:36:14.082205Z"},"links":{"cited_paper":"/paper/0712.3457","citing_paper":"/paper/2411.08498"},"observation_digest":"sha256:df0e7175b6fdc19007536412ab622e9270802ac9354b615fc1edfff6ca74409e","observation_id":"747d9ebd-1f09-4ee7-8abd-3cbfecb73b27","resolution":{"observed_at":"2026-08-12T21:36:14.082205Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"1205.2422","last_updated":"2012-12-20T05:57:28Z","snapshot_observed_at":"2026-08-11T12:36:14.041294Z","submitted_at":"2012-05-11T03:05:41Z","title":"Spatial curvature and cosmological tests of general relativity","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"1205.2422","snapshot_observed_at":"2026-08-12T21:36:14.086944Z","title":"Dossett and M","venue":null,"work_id":null,"year":2012},"citing_paper":{"arxiv_id":"2411.08498","last_updated":"2024-12-27T06:29:18Z","snapshot_observed_at":"2026-08-13T02:19:47.582623Z","submitted_at":"2024-11-13T10:32:37Z","title":"A dark energy parameterization independent constraint of the spatial curvature $\\Omega_K$","version":2},"reference_index":21,"source":"pdf_text","source_observed_at":"2026-08-12T21:36:14.086944Z"},"links":{"cited_paper":"/paper/1205.2422","citing_paper":"/paper/2411.08498"},"observation_digest":"sha256:25f7be1ef73a56d362d9a6c6f22cef4b197b34e86b5e3a03339208c1dd1de4be","observation_id":"cc8e74a5-ce81-40c0-9743-9f0e250b1e24","resolution":{"observed_at":"2026-08-12T21:36:14.086944Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"0710.1887","last_updated":"2007-10-10T00:00:19Z","snapshot_observed_at":"2026-08-06T03:41:35.929199Z","submitted_at":"2007-10-10T00:00:19Z","title":"The Hubble series: Convergence properties and redshift variables","version":1},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"0710.1887","snapshot_observed_at":"2026-08-12T21:36:14.091833Z","title":"Catto¨ en and M","venue":null,"work_id":null,"year":2007},"citing_paper":{"arxiv_id":"2411.08498","last_updated":"2024-12-27T06:29:18Z","snapshot_observed_at":"2026-08-13T02:19:47.582623Z","submitted_at":"2024-11-13T10:32:37Z","title":"A dark energy parameterization independent constraint of the spatial curvature $\\Omega_K$","version":2},"reference_index":22,"source":"pdf_text","source_observed_at":"2026-08-12T21:36:14.091833Z"},"links":{"cited_paper":"/paper/0710.1887","citing_paper":"/paper/2411.08498"},"observation_digest":"sha256:2147efab747311beaaeaca47eb6ff54130e981703bec9f58366e3a0ae4bcb152","observation_id":"f1d86f3f-c1ac-48bf-9611-fc487e15365d","resolution":{"observed_at":"2026-08-12T21:36:14.091833Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"1204.1109","last_updated":"2012-07-10T06:58:13Z","snapshot_observed_at":"2026-08-06T01:08:19.238553Z","submitted_at":"2012-04-05T02:08:47Z","title":"Crossing Statistic: Reconstructing the Expansion History of the Universe","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"1204.1109","snapshot_observed_at":"2026-08-12T21:36:14.096818Z","title":"Shafieloo, Crossing statistic: reconstructing the expansion history of the universe , Journal of Cosmology and Astroparticle Physics 2012 (2012) 002 [ 1204.1109]","venue":null,"work_id":null,"year":2012},"citing_paper":{"arxiv_id":"2411.08498","last_updated":"2024-12-27T06:29:18Z","snapshot_observed_at":"2026-08-13T02:19:47.582623Z","submitted_at":"2024-11-13T10:32:37Z","title":"A dark energy parameterization independent constraint of the spatial curvature $\\Omega_K$","version":2},"reference_index":23,"source":"pdf_text","source_observed_at":"2026-08-12T21:36:14.096818Z"},"links":{"cited_paper":"/paper/1204.1109","citing_paper":"/paper/2411.08498"},"observation_digest":"sha256:91ad44370518dfdad73571b11711b915e10064f547a1e7d15475f07fae81e943","observation_id":"60fb3073-d937-47c2-972a-f022c2f428c1","resolution":{"observed_at":"2026-08-12T21:36:14.096818Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"1301.4044","last_updated":"2013-01-17T11:04:46Z","snapshot_observed_at":"2026-08-12T17:24:13.358523Z","submitted_at":"2013-01-17T11:04:46Z","title":"Constraints from Cosmography in various parameterizations","version":1},"cited_work":{"arxiv_id":"1301.4044","doi":null,"metadata_source":"pith","pith_arxiv_id":"1301.4044","snapshot_observed_at":"2026-08-12T21:36:14.780023Z","title":"Constraints from Cosmography in various parameterizations","venue":"astro-ph.CO","work_id":"4a61b8c6-9052-4a33-a948-c6503a9a46f2","year":2013},"citing_paper":{"arxiv_id":"2411.08498","last_updated":"2024-12-27T06:29:18Z","snapshot_observed_at":"2026-08-13T02:19:47.582623Z","submitted_at":"2024-11-13T10:32:37Z","title":"A dark energy parameterization independent constraint of the spatial curvature $\\Omega_K$","version":2},"reference_index":24,"source":"pdf_text","source_observed_at":"2026-08-12T21:36:14.102279Z"},"links":{"cited_paper":"/paper/1301.4044","citing_paper":"/paper/2411.08498"},"observation_digest":"sha256:d84ba2daca105703e5b3de250f130d026c9bdc2a1b06b9e4522aeeb218d81115","observation_id":"2f6a502f-0282-4dc8-8abf-3ff185a5eccb","resolution":{"observed_at":"2026-08-12T21:36:14.785672Z","resolver_source":"local_arxiv","status":"verified_exact"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-14T06:32:32.682623+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-14T06:32:32.682623+00:00","source":"crossref"},{"observed_at":"2026-08-14T06:32:18.44784+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":{"arxiv_id":"2003.09341","last_updated":"2020-03-25T17:04:30Z","snapshot_observed_at":"2026-08-12T22:18:36.002404Z","submitted_at":"2020-03-20T15:50:03Z","title":"High-redshift cosmography: auxiliary variables versus Pad\\'e polynomials","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2003.09341","snapshot_observed_at":"2026-08-12T21:36:14.106760Z","title":"Capozziello, R","venue":null,"work_id":null,"year":2020},"citing_paper":{"arxiv_id":"2411.08498","last_updated":"2024-12-27T06:29:18Z","snapshot_observed_at":"2026-08-13T02:19:47.582623Z","submitted_at":"2024-11-13T10:32:37Z","title":"A dark energy parameterization independent constraint of the spatial curvature $\\Omega_K$","version":2},"reference_index":25,"source":"pdf_text","source_observed_at":"2026-08-12T21:36:14.106760Z"},"links":{"cited_paper":"/paper/2003.09341","citing_paper":"/paper/2411.08498"},"observation_digest":"sha256:0adb06d12bb0a0abe36d349ba432d6d954daef3eaeae551ec9040c0f0ef4dc76","observation_id":"91b68153-0ac6-4219-9fac-a44687ba2546","resolution":{"observed_at":"2026-08-12T21:36:14.106760Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"1903.11433","last_updated":"2019-11-24T11:43:34Z","snapshot_observed_at":"2026-07-06T07:42:00.255729Z","submitted_at":"2019-03-27T14:03:03Z","title":"General Cosmography Model with Spatial Curvature","version":3},"cited_work":{"arxiv_id":"1903.11433","doi":null,"metadata_source":"pith","pith_arxiv_id":"1903.11433","snapshot_observed_at":"2026-08-12T21:36:14.740039Z","title":"General Cosmography Model with Spatial Curvature","venue":"astro-ph.CO","work_id":"b57e1a90-349e-49f4-8465-3d633c94f37c","year":2019},"citing_paper":{"arxiv_id":"2411.08498","last_updated":"2024-12-27T06:29:18Z","snapshot_observed_at":"2026-08-13T02:19:47.582623Z","submitted_at":"2024-11-13T10:32:37Z","title":"A dark energy parameterization independent constraint of the spatial curvature $\\Omega_K$","version":2},"reference_index":26,"source":"pdf_text","source_observed_at":"2026-08-12T21:36:14.111642Z"},"links":{"cited_paper":"/paper/1903.11433","citing_paper":"/paper/2411.08498"},"observation_digest":"sha256:18d0d44914656f3f1a8e018a4f0c9d07f99e05af470a21b22ba31d1503a14509","observation_id":"b80956d6-6585-435f-8d80-57c32fba66ed","resolution":{"observed_at":"2026-08-12T21:36:14.747625Z","resolver_source":"local_arxiv","status":"verified_exact"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-14T06:32:32.682623+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-14T06:32:32.682623+00:00","source":"crossref"},{"observed_at":"2026-08-14T06:32:18.44784+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":{"arxiv_id":"2310.16512","last_updated":"2023-11-23T12:39:17Z","snapshot_observed_at":"2026-08-13T05:40:49.569774Z","submitted_at":"2023-10-25T10:02:48Z","title":"Joint Constraints on the Hubble Constant, Spatial Curvature, and Sound Horizon from the Late-time Universe with Cosmography","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2310.16512","snapshot_observed_at":"2026-08-12T21:36:14.116164Z","title":"Zhang, T","venue":null,"work_id":null,"year":2023},"citing_paper":{"arxiv_id":"2411.08498","last_updated":"2024-12-27T06:29:18Z","snapshot_observed_at":"2026-08-13T02:19:47.582623Z","submitted_at":"2024-11-13T10:32:37Z","title":"A dark energy parameterization independent constraint of the spatial curvature $\\Omega_K$","version":2},"reference_index":27,"source":"pdf_text","source_observed_at":"2026-08-12T21:36:14.116164Z"},"links":{"cited_paper":"/paper/2310.16512","citing_paper":"/paper/2411.08498"},"observation_digest":"sha256:03af4ff818f0d2d8d7662a3a10ed2602352ebb5ad23b9663c8a96a6f514686e8","observation_id":"5b299f60-b4e8-4e09-ac24-494693f6f53f","resolution":{"observed_at":"2026-08-12T21:36:14.116164Z","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":"2026-08-12T21:36:14.121127Z","title":"Scolnic, D","venue":null,"work_id":null,"year":2022},"citing_paper":{"arxiv_id":"2411.08498","last_updated":"2024-12-27T06:29:18Z","snapshot_observed_at":"2026-08-13T02:19:47.582623Z","submitted_at":"2024-11-13T10:32:37Z","title":"A dark energy parameterization independent constraint of the spatial curvature $\\Omega_K$","version":2},"reference_index":28,"source":"pdf_text","source_observed_at":"2026-08-12T21:36:14.121127Z"},"links":{"cited_paper":"/paper/2112.03863","citing_paper":"/paper/2411.08498"},"observation_digest":"sha256:318fdcc2ea9d061b268314d49f0b63ba9f9ea7e4a242c5b20d984fdd56a41ea1","observation_id":"cf124b76-3b87-4927-bc5c-8d2ef15c27bc","resolution":{"observed_at":"2026-08-12T21:36:14.121127Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"astro-ph/0302560","last_updated":"2003-02-27T17:34:27Z","snapshot_observed_at":"2026-07-07T00:31:35.668551Z","submitted_at":"2003-02-27T17:34:27Z","title":"Constraints on the equation of state of dark energy and the Hubble constant from stellar ages and the CMB","version":1},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"astro-ph/0302560","snapshot_observed_at":"2026-08-12T21:36:14.126142Z","title":"Jimenez, L","venue":null,"work_id":null,"year":2003},"citing_paper":{"arxiv_id":"2411.08498","last_updated":"2024-12-27T06:29:18Z","snapshot_observed_at":"2026-08-13T02:19:47.582623Z","submitted_at":"2024-11-13T10:32:37Z","title":"A dark energy parameterization independent constraint of the spatial curvature $\\Omega_K$","version":2},"reference_index":29,"source":"pdf_text","source_observed_at":"2026-08-12T21:36:14.126142Z"},"links":{"cited_paper":"/paper/astro-ph/0302560","citing_paper":"/paper/2411.08498"},"observation_digest":"sha256:4e712b2a1b8170c989b5d5f7d33a954175573c72381c0d1eae74d0cc99105c64","observation_id":"214ec6be-b905-413a-9cc6-0f1443360bd7","resolution":{"observed_at":"2026-08-12T21:36:14.126142Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"astro-ph/0412269","last_updated":"2004-12-13T10:50:48Z","snapshot_observed_at":"2026-07-07T00:46:54.442173Z","submitted_at":"2004-12-13T10:50:48Z","title":"Constraints on the redshift dependence of the dark energy potential","version":1},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"astro-ph/0412269","snapshot_observed_at":"2026-08-12T21:36:14.130728Z","title":"Simon, L","venue":null,"work_id":null,"year":2005},"citing_paper":{"arxiv_id":"2411.08498","last_updated":"2024-12-27T06:29:18Z","snapshot_observed_at":"2026-08-13T02:19:47.582623Z","submitted_at":"2024-11-13T10:32:37Z","title":"A dark energy parameterization independent constraint of the spatial curvature $\\Omega_K$","version":2},"reference_index":30,"source":"pdf_text","source_observed_at":"2026-08-12T21:36:14.130728Z"},"links":{"cited_paper":"/paper/astro-ph/0412269","citing_paper":"/paper/2411.08498"},"observation_digest":"sha256:a1a1d23ef756e90531f3d5c6b93d21ed4380de6f781fb7a8bac204f70c1f4e92","observation_id":"e49951a4-53d5-4412-96e8-ee6066fc75bf","resolution":{"observed_at":"2026-08-12T21:36:14.130728Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"0907.3149","last_updated":"2009-07-18T16:00:52Z","snapshot_observed_at":"2026-07-06T01:58:45.004946Z","submitted_at":"2009-07-18T16:00:52Z","title":"Cosmic Chronometers: Constraining the Equation of State of Dark Energy. I: H(z) Measurements","version":1},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"0907.3149","snapshot_observed_at":"2026-08-12T21:36:14.135181Z","title":"Stern, R","venue":null,"work_id":null,"year":2010},"citing_paper":{"arxiv_id":"2411.08498","last_updated":"2024-12-27T06:29:18Z","snapshot_observed_at":"2026-08-13T02:19:47.582623Z","submitted_at":"2024-11-13T10:32:37Z","title":"A dark energy parameterization independent constraint of the spatial curvature $\\Omega_K$","version":2},"reference_index":31,"source":"pdf_text","source_observed_at":"2026-08-12T21:36:14.135181Z"},"links":{"cited_paper":"/paper/0907.3149","citing_paper":"/paper/2411.08498"},"observation_digest":"sha256:5ed08c2f315c57fe8baa89e5051a9243042938c3798f09d9da19fc487e5f3cc4","observation_id":"65ec5ff0-7bed-4f51-b350-8d3df28c67e9","resolution":{"observed_at":"2026-08-12T21:36:14.135181Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"1201.6658","last_updated":"2013-02-05T15:07:12Z","snapshot_observed_at":"2026-07-06T02:42:05.078758Z","submitted_at":"2012-01-31T19:42:22Z","title":"New constraints on cosmological parameters and neutrino properties using the expansion rate of the Universe to z~1.75","version":3},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"1201.6658","snapshot_observed_at":"2026-08-12T21:36:14.139685Z","title":"Moresco, L","venue":null,"work_id":null,"year":2012},"citing_paper":{"arxiv_id":"2411.08498","last_updated":"2024-12-27T06:29:18Z","snapshot_observed_at":"2026-08-13T02:19:47.582623Z","submitted_at":"2024-11-13T10:32:37Z","title":"A dark energy parameterization independent constraint of the spatial curvature $\\Omega_K$","version":2},"reference_index":32,"source":"pdf_text","source_observed_at":"2026-08-12T21:36:14.139685Z"},"links":{"cited_paper":"/paper/1201.6658","citing_paper":"/paper/2411.08498"},"observation_digest":"sha256:b03bcd7e42a8c77adafaf8d6b2c46dd5ee4447ccb5a1b6b863760d1423c16282","observation_id":"3711042b-dd4f-4954-a380-e55f3389aad0","resolution":{"observed_at":"2026-08-12T21:36:14.139685Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"1207.4541","last_updated":"2014-05-22T10:50:07Z","snapshot_observed_at":"2026-08-03T16:10:14.051758Z","submitted_at":"2012-07-19T03:27:26Z","title":"Four New Observational $H(z)$ Data From Luminous Red Galaxies of Sloan Digital Sky Survey Data Release Seven","version":3},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"1207.4541","snapshot_observed_at":"2026-08-12T21:36:14.143840Z","title":"Zhang, H","venue":null,"work_id":null,"year":2014},"citing_paper":{"arxiv_id":"2411.08498","last_updated":"2024-12-27T06:29:18Z","snapshot_observed_at":"2026-08-13T02:19:47.582623Z","submitted_at":"2024-11-13T10:32:37Z","title":"A dark energy parameterization independent constraint of the spatial curvature $\\Omega_K$","version":2},"reference_index":33,"source":"pdf_text","source_observed_at":"2026-08-12T21:36:14.143840Z"},"links":{"cited_paper":"/paper/1207.4541","citing_paper":"/paper/2411.08498"},"observation_digest":"sha256:887fe2d179245ef042eeb7d06942b64b0c24cf593c962e70d9c71eeccc6c8c5f","observation_id":"231ecfec-eb49-453c-bdf0-f8d1dcf73b68","resolution":{"observed_at":"2026-08-12T21:36:14.143840Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"1503.01116","last_updated":"2015-03-03T21:00:11Z","snapshot_observed_at":"2026-08-10T09:05:25.588256Z","submitted_at":"2015-03-03T21:00:11Z","title":"Raising the bar: new constraints on the Hubble parameter with cosmic chronometers at z$\\sim$2","version":1},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"1503.01116","snapshot_observed_at":"2026-08-12T21:36:14.148265Z","title":"Moresco, Raising the bar: new constraints on the Hubble parameter with cosmic chronometers at z ˜2., Monthly Notices of the Royal Astronomical Society 450 (2015) L16 [1503.01116]","venue":null,"work_id":null,"year":2015},"citing_paper":{"arxiv_id":"2411.08498","last_updated":"2024-12-27T06:29:18Z","snapshot_observed_at":"2026-08-13T02:19:47.582623Z","submitted_at":"2024-11-13T10:32:37Z","title":"A dark energy parameterization independent constraint of the spatial curvature $\\Omega_K$","version":2},"reference_index":34,"source":"pdf_text","source_observed_at":"2026-08-12T21:36:14.148265Z"},"links":{"cited_paper":"/paper/1503.01116","citing_paper":"/paper/2411.08498"},"observation_digest":"sha256:377674174d20b6f75f78d492e47625638f5486d49e7da66aca5f73f8d34a65a6","observation_id":"ac57bfbb-6b64-40da-bdb0-f3c4792e18a0","resolution":{"observed_at":"2026-08-12T21:36:14.148265Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"1601.01701","last_updated":"2016-05-02T10:21:27Z","snapshot_observed_at":"2026-07-06T04:42:11.317805Z","submitted_at":"2016-01-07T21:10:24Z","title":"A 6% measurement of the Hubble parameter at $z\\sim0.45$: direct evidence of the epoch of cosmic re-acceleration","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"1601.01701","snapshot_observed_at":"2026-08-12T21:36:14.152790Z","title":"Moresco, L","venue":null,"work_id":null,"year":2016},"citing_paper":{"arxiv_id":"2411.08498","last_updated":"2024-12-27T06:29:18Z","snapshot_observed_at":"2026-08-13T02:19:47.582623Z","submitted_at":"2024-11-13T10:32:37Z","title":"A dark energy parameterization independent constraint of the spatial curvature $\\Omega_K$","version":2},"reference_index":35,"source":"pdf_text","source_observed_at":"2026-08-12T21:36:14.152790Z"},"links":{"cited_paper":"/paper/1601.01701","citing_paper":"/paper/2411.08498"},"observation_digest":"sha256:294cba462604af0f4f6eb4eb6f845c42b7dea2fa8c1eae620193fd4b0e41fe43","observation_id":"bd1d0488-7c60-47ac-a019-1e5e8ea3db5e","resolution":{"observed_at":"2026-08-12T21:36:14.152790Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"1702.00418","last_updated":"2017-11-21T06:34:22Z","snapshot_observed_at":"2026-07-06T05:28:26.411134Z","submitted_at":"2017-02-01T19:12:47Z","title":"Age-dating Luminous Red Galaxies observed with the Southern African Large Telescope","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"1702.00418","snapshot_observed_at":"2026-08-12T21:36:14.157172Z","title":"Ratsimbazafy, S.I","venue":null,"work_id":null,"year":2017},"citing_paper":{"arxiv_id":"2411.08498","last_updated":"2024-12-27T06:29:18Z","snapshot_observed_at":"2026-08-13T02:19:47.582623Z","submitted_at":"2024-11-13T10:32:37Z","title":"A dark energy parameterization independent constraint of the spatial curvature $\\Omega_K$","version":2},"reference_index":36,"source":"pdf_text","source_observed_at":"2026-08-12T21:36:14.157172Z"},"links":{"cited_paper":"/paper/1702.00418","citing_paper":"/paper/2411.08498"},"observation_digest":"sha256:f7373c4f07a2344316ad3754f9e66938ba9a888fee40991e5a8bc292b0816cdd","observation_id":"482fd3f7-ebd4-4002-91ae-68dcea57eacc","resolution":{"observed_at":"2026-08-12T21:36:14.157172Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2110.04304","last_updated":"2022-03-22T18:05:13Z","snapshot_observed_at":"2026-08-13T17:57:02.099234Z","submitted_at":"2021-10-08T18:00:00Z","title":"Toward a Better Understanding of Cosmic Chronometers: A new measurement of H(z) at z~0.7","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2110.04304","snapshot_observed_at":"2026-08-12T21:36:14.161612Z","title":"Borghi, M","venue":null,"work_id":null,"year":2022},"citing_paper":{"arxiv_id":"2411.08498","last_updated":"2024-12-27T06:29:18Z","snapshot_observed_at":"2026-08-13T02:19:47.582623Z","submitted_at":"2024-11-13T10:32:37Z","title":"A dark energy parameterization independent constraint of the spatial curvature $\\Omega_K$","version":2},"reference_index":37,"source":"pdf_text","source_observed_at":"2026-08-12T21:36:14.161612Z"},"links":{"cited_paper":"/paper/2110.04304","citing_paper":"/paper/2411.08498"},"observation_digest":"sha256:8a2c787e5dee7bda109eaffe5d17efa0761d6d3177301ebdbcf6c870aa223dd2","observation_id":"b3aa81d3-8dac-4259-b4a7-c221b300da5d","resolution":{"observed_at":"2026-08-12T21:36:14.161612Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2205.05701","last_updated":"2023-04-07T14:42:08Z","snapshot_observed_at":"2026-08-13T15:45:36.031783Z","submitted_at":"2022-05-11T18:00:04Z","title":"New Observational $H(z)$ Data from Full-Spectrum Fitting of Cosmic Chronometers in the LEGA-C Survey","version":3},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2205.05701","snapshot_observed_at":"2026-08-12T21:36:14.165903Z","title":null,"venue":null,"work_id":null,"year":2023},"citing_paper":{"arxiv_id":"2411.08498","last_updated":"2024-12-27T06:29:18Z","snapshot_observed_at":"2026-08-13T02:19:47.582623Z","submitted_at":"2024-11-13T10:32:37Z","title":"A dark energy parameterization independent constraint of the spatial curvature $\\Omega_K$","version":2},"reference_index":38,"source":"pdf_text","source_observed_at":"2026-08-12T21:36:14.165903Z"},"links":{"cited_paper":"/paper/2205.05701","citing_paper":"/paper/2411.08498"},"observation_digest":"sha256:50a27c747ec300172ffd1155be59c7e5c052bf21feea4221b67fc0342670a5da","observation_id":"4bae8c81-0e1b-433d-81d1-caad791920a0","resolution":{"observed_at":"2026-08-12T21:36:14.165903Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2404.03000","last_updated":"2024-04-03T18:41:49Z","snapshot_observed_at":"2026-08-13T21:13:25.845998Z","submitted_at":"2024-04-03T18:41:49Z","title":"DESI 2024 III: Baryon Acoustic Oscillations from Galaxies and Quasars","version":1},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2404.03000","snapshot_observed_at":"2026-08-12T21:36:14.170015Z","title":"Adame, J","venue":null,"work_id":null,"year":2024},"citing_paper":{"arxiv_id":"2411.08498","last_updated":"2024-12-27T06:29:18Z","snapshot_observed_at":"2026-08-13T02:19:47.582623Z","submitted_at":"2024-11-13T10:32:37Z","title":"A dark energy parameterization independent constraint of the spatial curvature $\\Omega_K$","version":2},"reference_index":39,"source":"pdf_text","source_observed_at":"2026-08-12T21:36:14.170015Z"},"links":{"cited_paper":"/paper/2404.03000","citing_paper":"/paper/2411.08498"},"observation_digest":"sha256:33cef2bf38e244c69f575f0db76c4ea55fbd66f210c38f1c233b8e832f55ebe8","observation_id":"2b845f8a-54f2-406c-a1e1-2b5dcb6ee11c","resolution":{"observed_at":"2026-08-12T21:36:14.170015Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2404.03001","last_updated":"2024-09-27T07:18:27Z","snapshot_observed_at":"2026-08-13T04:43:24.265866Z","submitted_at":"2024-04-03T18:41:50Z","title":"DESI 2024 IV: Baryon Acoustic Oscillations from the Lyman Alpha Forest","version":4},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2404.03001","snapshot_observed_at":"2026-08-12T21:36:14.174538Z","title":"Adame, J","venue":null,"work_id":null,"year":2024},"citing_paper":{"arxiv_id":"2411.08498","last_updated":"2024-12-27T06:29:18Z","snapshot_observed_at":"2026-08-13T02:19:47.582623Z","submitted_at":"2024-11-13T10:32:37Z","title":"A dark energy parameterization independent constraint of the spatial curvature $\\Omega_K$","version":2},"reference_index":40,"source":"pdf_text","source_observed_at":"2026-08-12T21:36:14.174538Z"},"links":{"cited_paper":"/paper/2404.03001","citing_paper":"/paper/2411.08498"},"observation_digest":"sha256:8929665878fbeff0ebb8ee0b92560ceee2dee48c6c6d85b619edf2a0ddaf0ddd","observation_id":"08c70b38-286c-4967-bf8d-14a0f5787691","resolution":{"observed_at":"2026-08-12T21:36:14.174538Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2404.03002","last_updated":"2024-11-04T16:43:36Z","snapshot_observed_at":"2026-07-06T17:55:21.083912Z","submitted_at":"2024-04-03T18:41:51Z","title":"DESI 2024 VI: Cosmological Constraints from the Measurements of Baryon Acoustic Oscillations","version":3},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2404.03002","snapshot_observed_at":"2026-08-12T21:36:14.178923Z","title":"Adame, J","venue":null,"work_id":null,"year":2024},"citing_paper":{"arxiv_id":"2411.08498","last_updated":"2024-12-27T06:29:18Z","snapshot_observed_at":"2026-08-13T02:19:47.582623Z","submitted_at":"2024-11-13T10:32:37Z","title":"A dark energy parameterization independent constraint of the spatial curvature $\\Omega_K$","version":2},"reference_index":41,"source":"pdf_text","source_observed_at":"2026-08-12T21:36:14.178923Z"},"links":{"cited_paper":"/paper/2404.03002","citing_paper":"/paper/2411.08498"},"observation_digest":"sha256:66133bea4ac3040e429bb2e3efab0ba849250dfde3a4c4985e0fe1a2196405dc","observation_id":"e3601184-e863-4384-b3e1-b71915fc7b6b","resolution":{"observed_at":"2026-08-12T21:36:14.178923Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"1607.03155","last_updated":"2016-07-11T20:29:52Z","snapshot_observed_at":"2026-08-12T15:10:46.393033Z","submitted_at":"2016-07-11T20:29:52Z","title":"The clustering of galaxies in the completed SDSS-III Baryon Oscillation Spectroscopic Survey: cosmological analysis of the DR12 galaxy sample","version":1},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"1607.03155","snapshot_observed_at":"2026-08-12T21:36:14.183124Z","title":null,"venue":null,"work_id":null,"year":2017},"citing_paper":{"arxiv_id":"2411.08498","last_updated":"2024-12-27T06:29:18Z","snapshot_observed_at":"2026-08-13T02:19:47.582623Z","submitted_at":"2024-11-13T10:32:37Z","title":"A dark energy parameterization independent constraint of the spatial curvature $\\Omega_K$","version":2},"reference_index":42,"source":"pdf_text","source_observed_at":"2026-08-12T21:36:14.183124Z"},"links":{"cited_paper":"/paper/1607.03155","citing_paper":"/paper/2411.08498"},"observation_digest":"sha256:8a9e27331d05e8c19c257d1d9df7987e5882d9a64b97d2e25ae2c9ad01d4fa8b","observation_id":"c4d9c684-a09a-418c-90f6-e4a523198d9b","resolution":{"observed_at":"2026-08-12T21:36:14.183124Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2007.08994","last_updated":"2020-12-21T15:51:28Z","snapshot_observed_at":"2026-08-10T15:40:43.860926Z","submitted_at":"2020-07-17T14:09:51Z","title":"The Completed SDSS-IV extended Baryon Oscillation Spectroscopic Survey: measurement of the BAO and growth rate of structure of the luminous red galaxy sample from the anisotropic power spectrum between redshifts 0.6 and 1.0","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2007.08994","snapshot_observed_at":"2026-08-12T21:36:14.187595Z","title":"Gil-Mar ´ ın, J.E","venue":null,"work_id":null,"year":2020},"citing_paper":{"arxiv_id":"2411.08498","last_updated":"2024-12-27T06:29:18Z","snapshot_observed_at":"2026-08-13T02:19:47.582623Z","submitted_at":"2024-11-13T10:32:37Z","title":"A dark energy parameterization independent constraint of the spatial curvature $\\Omega_K$","version":2},"reference_index":43,"source":"pdf_text","source_observed_at":"2026-08-12T21:36:14.187595Z"},"links":{"cited_paper":"/paper/2007.08994","citing_paper":"/paper/2411.08498"},"observation_digest":"sha256:2ea719d3543f86c282092cac81d249748464f5ba45658736612846b6d4044fab","observation_id":"0ea977a1-1853-4a3d-9751-fd31ea1e8f1b","resolution":{"observed_at":"2026-08-12T21:36:14.187595Z","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":"2026-08-12T21:36:14.191788Z","title":"Neveux, E","venue":null,"work_id":null,"year":2020},"citing_paper":{"arxiv_id":"2411.08498","last_updated":"2024-12-27T06:29:18Z","snapshot_observed_at":"2026-08-13T02:19:47.582623Z","submitted_at":"2024-11-13T10:32:37Z","title":"A dark energy parameterization independent constraint of the spatial curvature $\\Omega_K$","version":2},"reference_index":44,"source":"pdf_text","source_observed_at":"2026-08-12T21:36:14.191788Z"},"links":{"citing_paper":"/paper/2411.08498"},"observation_digest":"sha256:aa3ce9c404d6eb2999e3ea6de095f0dffd2eb90ea8bf79f68ac2d81f05436c29","observation_id":"8188eceb-d88b-4d68-8b43-6df2369d9ba9","resolution":{"observed_at":"2026-08-12T21:36:14.191788Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2007.08995","last_updated":"2020-10-05T21:33:59Z","snapshot_observed_at":"2026-08-06T11:49:33.064914Z","submitted_at":"2020-07-17T14:09:52Z","title":"The Completed SDSS-IV extended Baryon Oscillation Spectroscopic Survey: Baryon acoustic oscillations with Lyman-$\\alpha$ forests","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2007.08995","snapshot_observed_at":"2026-08-12T21:36:14.195894Z","title":"du Mas des Bourboux, J","venue":null,"work_id":null,"year":2020},"citing_paper":{"arxiv_id":"2411.08498","last_updated":"2024-12-27T06:29:18Z","snapshot_observed_at":"2026-08-13T02:19:47.582623Z","submitted_at":"2024-11-13T10:32:37Z","title":"A dark energy parameterization independent constraint of the spatial curvature $\\Omega_K$","version":2},"reference_index":45,"source":"pdf_text","source_observed_at":"2026-08-12T21:36:14.195894Z"},"links":{"cited_paper":"/paper/2007.08995","citing_paper":"/paper/2411.08498"},"observation_digest":"sha256:fa0e819cbcccd5e4919719bd095c2f05ae12bbf76706de2bfa5f573ebedf0f5a","observation_id":"ebb7d70e-c7f8-4205-b24e-02589914da91","resolution":{"observed_at":"2026-08-12T21:36:14.195894Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"1710.00845","last_updated":"2018-03-26T02:21:13Z","snapshot_observed_at":"2026-08-09T21:32:48.253157Z","submitted_at":"2017-10-02T18:03:12Z","title":"The Complete Light-curve Sample of Spectroscopically Confirmed Type Ia Supernovae from Pan-STARRS1 and Cosmological Constraints from The Combined Pantheon Sample","version":3},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"1710.00845","snapshot_observed_at":"2026-08-12T21:36:14.200353Z","title":"Scolnic, D.O","venue":null,"work_id":null,"year":2018},"citing_paper":{"arxiv_id":"2411.08498","last_updated":"2024-12-27T06:29:18Z","snapshot_observed_at":"2026-08-13T02:19:47.582623Z","submitted_at":"2024-11-13T10:32:37Z","title":"A dark energy parameterization independent constraint of the spatial curvature $\\Omega_K$","version":2},"reference_index":46,"source":"pdf_text","source_observed_at":"2026-08-12T21:36:14.200353Z"},"links":{"cited_paper":"/paper/1710.00845","citing_paper":"/paper/2411.08498"},"observation_digest":"sha256:625689e46e7baacb2b4306c17570f8990b8bf107d433821e21ad52a131d126ae","observation_id":"a8eab0bf-02ba-40b6-8bdd-4ce002d3bdaa","resolution":{"observed_at":"2026-08-12T21:36:14.200353Z","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":"2026-08-12T21:36:14.204783Z","title":"Foreman-Mackey, D.W","venue":null,"work_id":null,"year":2013},"citing_paper":{"arxiv_id":"2411.08498","last_updated":"2024-12-27T06:29:18Z","snapshot_observed_at":"2026-08-13T02:19:47.582623Z","submitted_at":"2024-11-13T10:32:37Z","title":"A dark energy parameterization independent constraint of the spatial curvature $\\Omega_K$","version":2},"reference_index":47,"source":"pdf_text","source_observed_at":"2026-08-12T21:36:14.204783Z"},"links":{"cited_paper":"/paper/1202.3665","citing_paper":"/paper/2411.08498"},"observation_digest":"sha256:065a6728c560c1d39c0bb7d3588f7657cb2da924d3e466bafef7a9cacbaba58b","observation_id":"919337fe-2de9-47eb-9c41-76dab1f9a5b8","resolution":{"observed_at":"2026-08-12T21:36:14.204783Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2306.06307","last_updated":"2024-01-13T00:50:36Z","snapshot_observed_at":"2026-08-13T11:19:54.790703Z","submitted_at":"2023-06-09T23:55:36Z","title":"Validation of the Scientific Program for the Dark Energy Spectroscopic Instrument","version":3},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2306.06307","snapshot_observed_at":"2026-08-12T21:36:14.209410Z","title":"Adame, J","venue":null,"work_id":null,"year":2024},"citing_paper":{"arxiv_id":"2411.08498","last_updated":"2024-12-27T06:29:18Z","snapshot_observed_at":"2026-08-13T02:19:47.582623Z","submitted_at":"2024-11-13T10:32:37Z","title":"A dark energy parameterization independent constraint of the spatial curvature $\\Omega_K$","version":2},"reference_index":48,"source":"pdf_text","source_observed_at":"2026-08-12T21:36:14.209410Z"},"links":{"cited_paper":"/paper/2306.06307","citing_paper":"/paper/2411.08498"},"observation_digest":"sha256:96d27b6342531ace8a77b11d9a027f4e3656274987ffcf02b803fbe9be7704e1","observation_id":"39334341-aba8-469b-aac9-ea207e0c10d1","resolution":{"observed_at":"2026-08-12T21:36:14.209410Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2408.02365","last_updated":"2024-12-11T15:46:18Z","snapshot_observed_at":"2026-08-12T23:08:35.832684Z","submitted_at":"2024-08-05T10:22:31Z","title":"Nonparametric late-time expansion history reconstruction and implications for the Hubble tension in light of recent DESI and type Ia supernovae data","version":3},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2408.02365","snapshot_observed_at":"2026-08-12T21:36:14.213799Z","title":"Jiang, D","venue":null,"work_id":null,"year":2024},"citing_paper":{"arxiv_id":"2411.08498","last_updated":"2024-12-27T06:29:18Z","snapshot_observed_at":"2026-08-13T02:19:47.582623Z","submitted_at":"2024-11-13T10:32:37Z","title":"A dark energy parameterization independent constraint of the spatial curvature $\\Omega_K$","version":2},"reference_index":49,"source":"pdf_text","source_observed_at":"2026-08-12T21:36:14.213799Z"},"links":{"cited_paper":"/paper/2408.02365","citing_paper":"/paper/2411.08498"},"observation_digest":"sha256:38b26f080922bc6536f790775e305db1d1764d75fb78bbd672ba7b0c3a5bed6c","observation_id":"0da7ef72-bcef-4d44-852f-b770e0c09ee0","resolution":{"observed_at":"2026-08-12T21:36:14.213799Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2212.09804","last_updated":"2023-07-14T13:56:39Z","snapshot_observed_at":"2026-08-13T21:43:12.119728Z","submitted_at":"2022-12-19T19:17:18Z","title":"Constraining the spatial curvature with cosmic expansion history in a cosmological model with a non-standard sound horizon","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2212.09804","snapshot_observed_at":"2026-08-12T21:36:14.218151Z","title":"Stevens, H","venue":null,"work_id":null,"year":2023},"citing_paper":{"arxiv_id":"2411.08498","last_updated":"2024-12-27T06:29:18Z","snapshot_observed_at":"2026-08-13T02:19:47.582623Z","submitted_at":"2024-11-13T10:32:37Z","title":"A dark energy parameterization independent constraint of the spatial curvature $\\Omega_K$","version":2},"reference_index":50,"source":"pdf_text","source_observed_at":"2026-08-12T21:36:14.218151Z"},"links":{"cited_paper":"/paper/2212.09804","citing_paper":"/paper/2411.08498"},"observation_digest":"sha256:b71fb0b45731332834a01b95a3f50c94128511ca9fd46249626acc19bc9c2ca4","observation_id":"e022ccce-f840-40be-941c-a120e0a77f73","resolution":{"observed_at":"2026-08-12T21:36:14.218151Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2006.10256","last_updated":"2020-06-18T03:39:27Z","snapshot_observed_at":"2026-08-09T08:28:30.953789Z","submitted_at":"2020-06-18T03:39:27Z","title":"Array Programming with NumPy","version":1},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2006.10256","snapshot_observed_at":"2026-08-12T21:36:14.223748Z","title":"Harris, K.J","venue":null,"work_id":null,"year":2020},"citing_paper":{"arxiv_id":"2411.08498","last_updated":"2024-12-27T06:29:18Z","snapshot_observed_at":"2026-08-13T02:19:47.582623Z","submitted_at":"2024-11-13T10:32:37Z","title":"A dark energy parameterization independent constraint of the spatial curvature $\\Omega_K$","version":2},"reference_index":51,"source":"pdf_text","source_observed_at":"2026-08-12T21:36:14.223748Z"},"links":{"cited_paper":"/paper/2006.10256","citing_paper":"/paper/2411.08498"},"observation_digest":"sha256:6c1b5f077c04d6c5036ca30adab3e03faec609d50a0b87c5d8bbe1827e9c2709","observation_id":"ad0cb6a4-79d9-462f-912e-e4474cbb55d7","resolution":{"observed_at":"2026-08-12T21:36:14.223748Z","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":"2026-08-12T21:36:14.229411Z","title":"Hunter, Matplotlib: A 2D Graphics Environment , Computing in Science and Engineering 9 (2007) 90","venue":null,"work_id":null,"year":2007},"citing_paper":{"arxiv_id":"2411.08498","last_updated":"2024-12-27T06:29:18Z","snapshot_observed_at":"2026-08-13T02:19:47.582623Z","submitted_at":"2024-11-13T10:32:37Z","title":"A dark energy parameterization independent constraint of the spatial curvature $\\Omega_K$","version":2},"reference_index":52,"source":"pdf_text","source_observed_at":"2026-08-12T21:36:14.229411Z"},"links":{"citing_paper":"/paper/2411.08498"},"observation_digest":"sha256:a0d14029fda954ba07d820363951fba066765947e2285e42cbf669d9a8f16141","observation_id":"7ca80616-f583-4a00-8cb0-f8b17bd564ad","resolution":{"observed_at":"2026-08-12T21:36:14.229411Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"1907.10121","last_updated":"2019-07-23T20:31:36Z","snapshot_observed_at":"2026-08-04T12:48:10.448438Z","submitted_at":"2019-07-23T20:31:36Z","title":"SciPy 1.0--Fundamental Algorithms for Scientific Computing in Python","version":1},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"1907.10121","snapshot_observed_at":"2026-08-12T21:36:14.233936Z","title":"Virtanen, R","venue":null,"work_id":null,"year":2020},"citing_paper":{"arxiv_id":"2411.08498","last_updated":"2024-12-27T06:29:18Z","snapshot_observed_at":"2026-08-13T02:19:47.582623Z","submitted_at":"2024-11-13T10:32:37Z","title":"A dark energy parameterization independent constraint of the spatial curvature $\\Omega_K$","version":2},"reference_index":53,"source":"pdf_text","source_observed_at":"2026-08-12T21:36:14.233936Z"},"links":{"cited_paper":"/paper/1907.10121","citing_paper":"/paper/2411.08498"},"observation_digest":"sha256:bb9410c7006d41e01003e2bf5c111cfc90031c9ad65d83fe08371f1cc21b5e7b","observation_id":"9900a8a3-639a-46b6-a6b2-83df2020eebf","resolution":{"observed_at":"2026-08-12T21:36:14.233936Z","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":"raw_reference","pith_arxiv_id":null,"snapshot_observed_at":"2026-08-12T21:36:15.057088Z","title":"Foreman-Mackey, corner.py: Scatterplot matrices in Python , The Journal of Open Source Software 1 (2016) 24","venue":null,"work_id":"4d3090a1-9329-4a6f-80ce-696214a0ebfb","year":2016},"citing_paper":{"arxiv_id":"2411.08498","last_updated":"2024-12-27T06:29:18Z","snapshot_observed_at":"2026-08-13T02:19:47.582623Z","submitted_at":"2024-11-13T10:32:37Z","title":"A dark energy parameterization independent constraint of the spatial curvature $\\Omega_K$","version":2},"reference_index":54,"source":"pdf_text","source_observed_at":"2026-08-12T21:36:14.239144Z"},"links":{"citing_paper":"/paper/2411.08498"},"observation_digest":"sha256:ef8a71a5be1a1b3ba7caffc48ecddba86d87a96eb178d832f3eaa0726dd702e2","observation_id":"53dc907d-6dba-4288-8401-1ab8409945d9","resolution":{"observed_at":"2026-08-12T21:36:15.063032Z","resolver_source":"raw_fallback","status":"verified_fuzzy"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-14T06:32:32.682623+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-14T06:32:32.682623+00:00","source":"crossref"},{"observed_at":"2026-08-14T06:32:18.44784+00:00","source":"retraction_watch"}],"state":"measured"}}],"paper":{"arxiv_id":"2411.08498","last_updated":"2024-12-27T06:29:18Z","latest_version":2,"primary_category":"astro-ph.CO","snapshot_observed_at":"2026-08-13T02:19:47.582623Z","submitted_at":"2024-11-13T10:32:37Z","title":"A dark energy parameterization independent constraint of the spatial curvature $\\Omega_K$"},"reference_resolution":{"displayed":54,"state_counts":{"malformed_identifier":0,"metadata_mismatch":0,"parse_uncertain":0,"unresolved":44,"verified_exact":3,"verified_fuzzy":7},"total_outbound_references":54},"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":"2026-08-14T06:32:32.682623+00:00","source":"crossref"},{"observed_at":"2026-08-14T06:32:18.44784+00:00","source":"retraction_watch"}],"thesis":"As of 14 August 2026, this Paper Citation Record lists 54 of 54 outbound references and 1 inbound Pith citation observation for arXiv:2411.08498."}