{"as_of":"2026-08-20T04:22:00Z","caps":{"database_statements":6,"inbound":100,"outbound":100},"context_digest":"sha256:6dc02cd8e1dcfa0b6d2509aa775c09296d358fe27c73a926687ff8793908f159","coverage":[{"denominator":131,"lane":"reference_resolution","note":"Typed states for the displayed outbound observations.","records_observed":100,"source":"paper_references, paper_reference_links","source_observed_at":"2026-08-11T13:41:23.944879Z","state":"measured"},{"denominator":144,"lane":"standing_notices","note":"One-hop event checks from named stored sources.","records_observed":144,"source":"scholarly_work_events, retraction_status_cache","source_observed_at":"2026-08-19T06:32:44.657259+00:00","state":"measured"},{"denominator":44,"lane":"inbound_itemization","note":"Pith citing papers itemized under the disclosed page cap.","records_observed":44,"source":"paper_references, paper_reference_links","source_observed_at":"2026-08-16T01:06:27.564754Z","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":"2026-07-08T15:55:05.017633Z","state":"measured"}],"external_citation_measurements":[],"inbound":[{"citation":{"cited_paper":{"arxiv_id":"2412.12905","last_updated":"2025-01-25T08:30:04Z","snapshot_observed_at":"2026-08-17T16:16:24.002443Z","submitted_at":"2024-12-17T13:31:15Z","title":"DESI and SNe: Dynamical Dark Energy, $\\Omega_m$ Tension or Systematics?","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2412.12905","snapshot_observed_at":"2026-08-11T13:41:23.555260Z","title":"Ωm tension","venue":null,"work_id":null,"year":2025},"citing_paper":{"arxiv_id":"2412.12905","last_updated":"2025-01-25T08:30:04Z","snapshot_observed_at":"2026-08-17T16:16:24.002443Z","submitted_at":"2024-12-17T13:31:15Z","title":"DESI and SNe: Dynamical Dark Energy, $\\Omega_m$ Tension or Systematics?","version":2},"reference_index":53,"source":"pdf_text","source_observed_at":"2026-08-11T13:41:23.555260Z"},"links":{"cited_paper":"/paper/2412.12905","citing_paper":"/paper/2412.12905"},"observation_digest":"sha256:a943d0e097a0bf6bee6bdc2df3c8d421b560645e556d28f4d79b5013758e0d5d","observation_id":"8b020e06-ff4b-4439-aaa9-c581490fbb20","resolution":{"observed_at":"2026-08-11T13:41:23.555260Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2412.12905","last_updated":"2025-01-25T08:30:04Z","snapshot_observed_at":"2026-08-17T16:16:24.002443Z","submitted_at":"2024-12-17T13:31:15Z","title":"DESI and SNe: Dynamical Dark Energy, $\\Omega_m$ Tension or Systematics?","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2412.12905","snapshot_observed_at":"2026-08-11T00:53:46.931889Z","title":null,"venue":null,"work_id":null,"year":2024},"citing_paper":{"arxiv_id":"2412.19240","last_updated":"2025-04-23T01:47:03Z","snapshot_observed_at":"2026-08-18T09:53:59.913284Z","submitted_at":"2024-12-26T14:51:09Z","title":"Effect of Peak Absolute Magnitude of Type Ia Supernovae and Sound Horizon Values on Hubble Tension using DESI results","version":2},"reference_index":23,"source":"pdf_text","source_observed_at":"2026-08-11T00:53:46.931889Z"},"links":{"cited_paper":"/paper/2412.12905","citing_paper":"/paper/2412.19240"},"observation_digest":"sha256:3298f1eeb55e318c4950ef19ff986520b08f4673ced507f322441d8a3e12b2ee","observation_id":"72a97d19-eda2-4da7-80e2-93e37c657bf1","resolution":{"observed_at":"2026-08-11T00:53:46.931889Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2412.12905","last_updated":"2025-01-25T08:30:04Z","snapshot_observed_at":"2026-08-17T16:16:24.002443Z","submitted_at":"2024-12-17T13:31:15Z","title":"DESI and SNe: Dynamical Dark Energy, $\\Omega_m$ Tension or Systematics?","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2412.12905","snapshot_observed_at":"2026-08-10T20:19:23.973969Z","title":null,"venue":null,"work_id":null,"year":2024},"citing_paper":{"arxiv_id":"2501.08915","last_updated":"2025-01-15T16:22:11Z","snapshot_observed_at":"2026-08-18T07:58:36.259456Z","submitted_at":"2025-01-15T16:22:11Z","title":"The case for a low dark matter density in dynamical dark energy model from local probes","version":1},"reference_index":39,"source":"pdf_text","source_observed_at":"2026-08-10T20:19:23.973969Z"},"links":{"cited_paper":"/paper/2412.12905","citing_paper":"/paper/2501.08915"},"observation_digest":"sha256:15bc2d3584869002585048313709adc65e09863f28b8456d14966a495e682f0a","observation_id":"9af6bd66-3091-4952-bb36-cf195d650600","resolution":{"observed_at":"2026-08-10T20:19:23.973969Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2412.12905","last_updated":"2025-01-25T08:30:04Z","snapshot_observed_at":"2026-08-17T16:16:24.002443Z","submitted_at":"2024-12-17T13:31:15Z","title":"DESI and SNe: Dynamical Dark Energy, $\\Omega_m$ Tension or Systematics?","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2412.12905","snapshot_observed_at":"2026-08-10T14:34:39.619924Z","title":null,"venue":null,"work_id":null,"year":2024},"citing_paper":{"arxiv_id":"2501.15233","last_updated":"2025-01-25T14:36:55Z","snapshot_observed_at":"2026-08-16T09:11:32.506343Z","submitted_at":"2025-01-25T14:36:55Z","title":"Cosmic distance duality after DESI 2024 data release and dark energy evolution","version":1},"reference_index":25,"source":"pdf_text","source_observed_at":"2026-08-10T14:34:39.619924Z"},"links":{"cited_paper":"/paper/2412.12905","citing_paper":"/paper/2501.15233"},"observation_digest":"sha256:e0165524b45f834112f8ce1f0e99de256b4b6d1c1cb753732cf167f64420c225","observation_id":"5f3cbf0b-8440-4417-8273-f3aba6fa0d17","resolution":{"observed_at":"2026-08-10T14:34:39.619924Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2412.12905","last_updated":"2025-01-25T08:30:04Z","snapshot_observed_at":"2026-08-17T16:16:24.002443Z","submitted_at":"2024-12-17T13:31:15Z","title":"DESI and SNe: Dynamical Dark Energy, $\\Omega_m$ Tension or Systematics?","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2412.12905","snapshot_observed_at":"2026-08-10T14:29:27.592156Z","title":null,"venue":null,"work_id":null,"year":2024},"citing_paper":{"arxiv_id":"2501.15298","last_updated":"2025-04-12T08:58:51Z","snapshot_observed_at":"2026-08-14T12:45:12.698388Z","submitted_at":"2025-01-25T18:30:04Z","title":"Scalar-Tensor Gravity and DESI 2024 BAO data","version":2},"reference_index":49,"source":"pdf_text","source_observed_at":"2026-08-10T14:29:27.592156Z"},"links":{"cited_paper":"/paper/2412.12905","citing_paper":"/paper/2501.15298"},"observation_digest":"sha256:88c67efc1ca4bda3d585fb40f7216c592dc788ec3f89d0feab75c3ab0d52e7cf","observation_id":"38003a1c-7e93-438f-91bc-142cfc61135f","resolution":{"observed_at":"2026-08-10T14:29:27.592156Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2412.12905","last_updated":"2025-01-25T08:30:04Z","snapshot_observed_at":"2026-08-17T16:16:24.002443Z","submitted_at":"2024-12-17T13:31:15Z","title":"DESI and SNe: Dynamical Dark Energy, $\\Omega_m$ Tension or Systematics?","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2412.12905","snapshot_observed_at":"2026-08-09T14:46:06.550296Z","title":"Colgáin and M.M","venue":null,"work_id":null,"year":null},"citing_paper":{"arxiv_id":"2502.01722","last_updated":"2025-06-30T13:35:52Z","snapshot_observed_at":"2026-08-14T08:36:58.524440Z","submitted_at":"2025-02-03T19:00:00Z","title":"Tuning the cosmic instrument: robust cosmology through combined probes","version":4},"reference_index":24,"source":"pdf_text","source_observed_at":"2026-08-09T14:46:06.550296Z"},"links":{"cited_paper":"/paper/2412.12905","citing_paper":"/paper/2502.01722"},"observation_digest":"sha256:db93cccdf5ebcca29eeb1b53c21f061b1afe3350a45d9e66d3731c3d96128aa0","observation_id":"50bd8e14-3d94-4b74-91d0-574444d146e8","resolution":{"observed_at":"2026-08-09T14:46:06.550296Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2412.12905","last_updated":"2025-01-25T08:30:04Z","snapshot_observed_at":"2026-08-17T16:16:24.002443Z","submitted_at":"2024-12-17T13:31:15Z","title":"DESI and SNe: Dynamical Dark Energy, $\\Omega_m$ Tension or Systematics?","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2412.12905","snapshot_observed_at":"2026-08-08T23:12:26.188946Z","title":"DESI and SNe: Dynamical Dark Energy, Ω m Tension or System- atics?","venue":null,"work_id":null,"year":2024},"citing_paper":{"arxiv_id":"2502.04212","last_updated":"2025-07-17T16:27:03Z","snapshot_observed_at":"2026-08-18T11:01:42.213182Z","submitted_at":"2025-02-06T16:51:39Z","title":"The DESI DR1/DR2 evidence for dynamical dark energy is biased by low-redshift supernovae","version":5},"reference_index":68,"source":"pdf_text","source_observed_at":"2026-08-08T23:12:26.188946Z"},"links":{"cited_paper":"/paper/2412.12905","citing_paper":"/paper/2502.04212"},"observation_digest":"sha256:a958140a1486791241fc0e14b7b3c21d0c071386bbf50a0309f00f3662b261b0","observation_id":"47743180-6287-4f9f-a974-c6603a39bb86","resolution":{"observed_at":"2026-08-08T23:12:26.188946Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2412.12905","last_updated":"2025-01-25T08:30:04Z","snapshot_observed_at":"2026-08-17T16:16:24.002443Z","submitted_at":"2024-12-17T13:31:15Z","title":"DESI and SNe: Dynamical Dark Energy, $\\Omega_m$ Tension or Systematics?","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2412.12905","snapshot_observed_at":"2026-08-08T22:04:59.451872Z","title":null,"venue":null,"work_id":null,"year":2024},"citing_paper":{"arxiv_id":"2502.04641","last_updated":"2025-02-18T07:50:34Z","snapshot_observed_at":"2026-08-13T19:16:09.824806Z","submitted_at":"2025-02-07T03:58:52Z","title":"Dark energy and lensing anomaly in Planck CMB data","version":2},"reference_index":35,"source":"pdf_text","source_observed_at":"2026-08-08T22:04:59.451872Z"},"links":{"cited_paper":"/paper/2412.12905","citing_paper":"/paper/2502.04641"},"observation_digest":"sha256:fed6250e94e4a555688045498d912899f4f39cf33248f53cccef33dd32d59f7c","observation_id":"28ad7101-f891-4310-b8e8-ffb65d5c015b","resolution":{"observed_at":"2026-08-08T22:04:59.451872Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2412.12905","last_updated":"2025-01-25T08:30:04Z","snapshot_observed_at":"2026-08-17T16:16:24.002443Z","submitted_at":"2024-12-17T13:31:15Z","title":"DESI and SNe: Dynamical Dark Energy, $\\Omega_m$ Tension or Systematics?","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2412.12905","snapshot_observed_at":"2026-08-08T21:04:17.705968Z","title":"Colgáin and M.M","venue":null,"work_id":null,"year":null},"citing_paper":{"arxiv_id":"2502.04929","last_updated":"2025-05-14T14:57:09Z","snapshot_observed_at":"2026-08-08T20:55:05.610325Z","submitted_at":"2025-02-07T13:49:14Z","title":"Robustness of dark energy phenomenology across different parameterizations","version":3},"reference_index":50,"source":"pdf_text","source_observed_at":"2026-08-08T21:04:17.705968Z"},"links":{"cited_paper":"/paper/2412.12905","citing_paper":"/paper/2502.04929"},"observation_digest":"sha256:b2edd7980459965e0111bd97ef506f1a4f665e9d5cdf27fd5c53daae6f4ab559","observation_id":"83665ba1-751d-4e0b-8f14-57482ab2743b","resolution":{"observed_at":"2026-08-08T21:04:17.705968Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2412.12905","last_updated":"2025-01-25T08:30:04Z","snapshot_observed_at":"2026-08-17T16:16:24.002443Z","submitted_at":"2024-12-17T13:31:15Z","title":"DESI and SNe: Dynamical Dark Energy, $\\Omega_m$ Tension or Systematics?","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2412.12905","snapshot_observed_at":"2026-08-08T17:56:51.936732Z","title":null,"venue":null,"work_id":null,"year":2024},"citing_paper":{"arxiv_id":"2502.05823","last_updated":"2025-03-08T06:00:58Z","snapshot_observed_at":"2026-08-13T08:47:30.152710Z","submitted_at":"2025-02-09T09:12:55Z","title":"Little ado about everything II: an `emergent' dark energy from structure formation to rule cosmic tensions","version":2},"reference_index":27,"source":"pdf_text","source_observed_at":"2026-08-08T17:56:51.936732Z"},"links":{"cited_paper":"/paper/2412.12905","citing_paper":"/paper/2502.05823"},"observation_digest":"sha256:906b357dc49f9517aea6250a7a05aa3887c015b35c510b0fa86cfb104e74f863","observation_id":"d3bd8737-908e-4ffc-84ed-b91778b78e6e","resolution":{"observed_at":"2026-08-08T17:56:51.936732Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2412.12905","last_updated":"2025-01-25T08:30:04Z","snapshot_observed_at":"2026-08-17T16:16:24.002443Z","submitted_at":"2024-12-17T13:31:15Z","title":"DESI and SNe: Dynamical Dark Energy, $\\Omega_m$ Tension or Systematics?","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2412.12905","snapshot_observed_at":"2026-08-16T01:06:27.564754Z","title":null,"venue":null,"work_id":null,"year":2024},"citing_paper":{"arxiv_id":"2505.02207","last_updated":"2025-05-06T20:39:31Z","snapshot_observed_at":"2026-08-17T11:47:20.831905Z","submitted_at":"2025-05-04T18:06:04Z","title":"On the tension between DESI DR2 BAO and CMB","version":2},"reference_index":65,"source":"pdf_text","source_observed_at":"2026-08-16T01:06:27.564754Z"},"links":{"cited_paper":"/paper/2412.12905","citing_paper":"/paper/2505.02207"},"observation_digest":"sha256:9f33d3f5bea162b56c0bb288da42134fc71ff9b1de409418e8fbc5c82ab4c21e","observation_id":"0036e1ca-c4d1-40e4-93f3-37bf1663fdf7","resolution":{"observed_at":"2026-08-16T01:06:27.564754Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2412.12905","last_updated":"2025-01-25T08:30:04Z","snapshot_observed_at":"2026-08-17T16:16:24.002443Z","submitted_at":"2024-12-17T13:31:15Z","title":"DESI and SNe: Dynamical Dark Energy, $\\Omega_m$ Tension or Systematics?","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2412.12905","snapshot_observed_at":"2026-08-15T22:00:18.119696Z","title":null,"venue":null,"work_id":null,"year":2024},"citing_paper":{"arxiv_id":"2505.08467","last_updated":"2025-07-28T14:02:47Z","snapshot_observed_at":"2026-08-18T13:57:54.104246Z","submitted_at":"2025-05-13T11:50:01Z","title":"The matter with(in) CPL","version":3},"reference_index":18,"source":"arxiv_source","source_observed_at":"2026-08-15T22:00:18.119696Z"},"links":{"cited_paper":"/paper/2412.12905","citing_paper":"/paper/2505.08467"},"observation_digest":"sha256:ad39b5006a19044ddfdfc68599d68dded9bc1af6fa18804c89043e13507381ea","observation_id":"72b703df-f824-4778-b910-8960bb73a018","resolution":{"observed_at":"2026-08-15T22:00:18.119696Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2412.12905","last_updated":"2025-01-25T08:30:04Z","snapshot_observed_at":"2026-08-17T16:16:24.002443Z","submitted_at":"2024-12-17T13:31:15Z","title":"DESI and SNe: Dynamical Dark Energy, $\\Omega_m$ Tension or Systematics?","version":2},"cited_work":{"arxiv_id":"2412.12905","doi":null,"metadata_source":"pith","pith_arxiv_id":"2412.12905","snapshot_observed_at":"2026-07-08T15:55:05.017633Z","title":"DESI and SNe: Dynamical Dark Energy, Ω m Tension or System- atics?","venue":"astro-ph.CO","work_id":"9bc5da8e-a5f2-4c58-be0d-9dbcbe1c8f87","year":2024},"citing_paper":{"arxiv_id":"2505.24732","last_updated":"2026-04-11T09:17:44Z","snapshot_observed_at":"2026-08-15T11:15:56.688737Z","submitted_at":"2025-05-30T15:54:16Z","title":"The Quintom theory of dark energy after DESI DR2","version":3},"reference_index":111,"source":"pdf_text","source_observed_at":"2026-05-19T13:08:20.192767Z"},"links":{"cited_paper":"/paper/2412.12905","citing_paper":"/paper/2505.24732"},"observation_digest":"sha256:e7f0d759496abf3d520c91b3cac2e719c4e813e7e9b7e00a23502f7fa699ed46","observation_id":"9f3af7a7-aa82-4dc6-868e-ea1495d64f8e","resolution":{"observed_at":"2026-05-19T13:12:18.750206Z","resolver_source":"arxiv_id","status":"verified_exact"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-19T06:32:44.657259+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-19T06:32:44.657259+00:00","source":"crossref"},{"observed_at":"2026-08-19T06:32:39.956319+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":{"arxiv_id":"2412.12905","last_updated":"2025-01-25T08:30:04Z","snapshot_observed_at":"2026-08-17T16:16:24.002443Z","submitted_at":"2024-12-17T13:31:15Z","title":"DESI and SNe: Dynamical Dark Energy, $\\Omega_m$ Tension or Systematics?","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2412.12905","snapshot_observed_at":"2026-08-07T10:52:56.353704Z","title":null,"venue":null,"work_id":null,"year":null},"citing_paper":{"arxiv_id":"2506.04306","last_updated":"2025-06-04T17:51:05Z","snapshot_observed_at":"2026-08-13T10:19:27.378849Z","submitted_at":"2025-06-04T17:51:05Z","title":"Can the universe experience an AdS landscape since matter-radiation equality?","version":1},"reference_index":52,"source":"pdf_text","source_observed_at":"2026-08-07T10:52:56.353704Z"},"links":{"cited_paper":"/paper/2412.12905","citing_paper":"/paper/2506.04306"},"observation_digest":"sha256:c984a3221c0de3ceb8e85024b55e71c27112b1d5121a746704f903c077dbcad6","observation_id":"6440c24a-ece6-4113-8c50-99950e84c2d9","resolution":{"observed_at":"2026-08-07T10:52:56.353704Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2412.12905","last_updated":"2025-01-25T08:30:04Z","snapshot_observed_at":"2026-08-17T16:16:24.002443Z","submitted_at":"2024-12-17T13:31:15Z","title":"DESI and SNe: Dynamical Dark Energy, $\\Omega_m$ Tension or Systematics?","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2412.12905","snapshot_observed_at":"2026-08-07T10:50:52.110174Z","title":"\\'O ., & Sheikh-Jabbari, M","venue":null,"work_id":null,"year":2024},"citing_paper":{"arxiv_id":"2506.04333","last_updated":"2025-08-10T17:39:23Z","snapshot_observed_at":"2026-08-12T07:24:06.460547Z","submitted_at":"2025-06-04T18:00:10Z","title":"Uncalibrated Cosmic Standards as a Robust Test on Late-Time Cosmological Models","version":3},"reference_index":20,"source":"arxiv_source","source_observed_at":"2026-08-07T10:50:52.110174Z"},"links":{"cited_paper":"/paper/2412.12905","citing_paper":"/paper/2506.04333"},"observation_digest":"sha256:26910ca54dd7388ca26f206fa1c1f4d679c6374593632b180398fab90ce535cb","observation_id":"dcf8f4d6-d429-4d38-ba43-1ca11b478f93","resolution":{"observed_at":"2026-08-07T10:50:52.110174Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2412.12905","last_updated":"2025-01-25T08:30:04Z","snapshot_observed_at":"2026-08-17T16:16:24.002443Z","submitted_at":"2024-12-17T13:31:15Z","title":"DESI and SNe: Dynamical Dark Energy, $\\Omega_m$ Tension or Systematics?","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2412.12905","snapshot_observed_at":"2026-08-06T21:34:26.662248Z","title":null,"venue":null,"work_id":null,"year":null},"citing_paper":{"arxiv_id":"2507.00115","last_updated":"2025-08-24T22:45:00Z","snapshot_observed_at":"2026-08-16T10:03:01.817270Z","submitted_at":"2025-06-30T18:00:00Z","title":"Quantum stress-energy at timelike boundaries: testing a new beyond-$\\Lambda$CDM parameter with cosmological data","version":3},"reference_index":15,"source":"pdf_text","source_observed_at":"2026-08-06T21:34:26.662248Z"},"links":{"cited_paper":"/paper/2412.12905","citing_paper":"/paper/2507.00115"},"observation_digest":"sha256:3e86bd40281c6dc2ad4434e2ddcc97bc3c455596a1ac6900601729ccad2707f8","observation_id":"199f838b-4681-4a66-ad47-d892e4787fd3","resolution":{"observed_at":"2026-08-06T21:34:26.662248Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2412.12905","last_updated":"2025-01-25T08:30:04Z","snapshot_observed_at":"2026-08-17T16:16:24.002443Z","submitted_at":"2024-12-17T13:31:15Z","title":"DESI and SNe: Dynamical Dark Energy, $\\Omega_m$ Tension or Systematics?","version":2},"cited_work":{"arxiv_id":"2412.12905","doi":null,"metadata_source":"pith","pith_arxiv_id":"2412.12905","snapshot_observed_at":"2026-07-08T15:55:05.017633Z","title":"DESI and SNe: Dynamical Dark Energy, Ω m Tension or System- atics?","venue":"astro-ph.CO","work_id":"9bc5da8e-a5f2-4c58-be0d-9dbcbe1c8f87","year":2024},"citing_paper":{"arxiv_id":"2507.09981","last_updated":"2026-05-06T01:55:59Z","snapshot_observed_at":"2026-08-15T02:07:33.193429Z","submitted_at":"2025-07-14T06:55:37Z","title":"New Insights into Dark Energy from DESI DR2 with CMB and SNIa","version":2},"reference_index":47,"source":"pdf_text","source_observed_at":"2026-05-19T05:19:08.520262Z"},"links":{"cited_paper":"/paper/2412.12905","citing_paper":"/paper/2507.09981"},"observation_digest":"sha256:b632320ebffb3ef3a3858594ec751422baab40c725b73cbddde1846de3efcfb1","observation_id":"122e1715-1dab-46bd-8458-9bf4c58d908c","resolution":{"observed_at":"2026-05-19T05:22:06.259094Z","resolver_source":"arxiv_id","status":"verified_exact"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-19T06:32:44.657259+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-19T06:32:44.657259+00:00","source":"crossref"},{"observed_at":"2026-08-19T06:32:39.956319+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":{"arxiv_id":"2412.12905","last_updated":"2025-01-25T08:30:04Z","snapshot_observed_at":"2026-08-17T16:16:24.002443Z","submitted_at":"2024-12-17T13:31:15Z","title":"DESI and SNe: Dynamical Dark Energy, $\\Omega_m$ Tension or Systematics?","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2412.12905","snapshot_observed_at":"2026-08-06T11:39:53.234165Z","title":null,"venue":null,"work_id":null,"year":null},"citing_paper":{"arxiv_id":"2507.22575","last_updated":"2025-08-08T08:31:23Z","snapshot_observed_at":"2026-08-14T18:19:20.163160Z","submitted_at":"2025-07-30T11:02:24Z","title":"Revisiting cosmic acceleration with DESI BAO","version":2},"reference_index":68,"source":"pdf_text","source_observed_at":"2026-08-06T11:39:53.234165Z"},"links":{"cited_paper":"/paper/2412.12905","citing_paper":"/paper/2507.22575"},"observation_digest":"sha256:5bce180d4df4b2e1ed9915ff145629e3e668ee78ac60b7400b4cbced3a07b281","observation_id":"9a320c14-c6bc-4cc0-a34d-90bf61eb52d9","resolution":{"observed_at":"2026-08-06T11:39:53.234165Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2412.12905","last_updated":"2025-01-25T08:30:04Z","snapshot_observed_at":"2026-08-17T16:16:24.002443Z","submitted_at":"2024-12-17T13:31:15Z","title":"DESI and SNe: Dynamical Dark Energy, $\\Omega_m$ Tension or Systematics?","version":2},"cited_work":{"arxiv_id":"2412.12905","doi":null,"metadata_source":"pith","pith_arxiv_id":"2412.12905","snapshot_observed_at":"2026-07-08T15:55:05.017633Z","title":"DESI and SNe: Dynamical Dark Energy, Ω m Tension or System- atics?","venue":"astro-ph.CO","work_id":"9bc5da8e-a5f2-4c58-be0d-9dbcbe1c8f87","year":2024},"citing_paper":{"arxiv_id":"2508.01759","last_updated":"2026-04-28T15:04:32Z","snapshot_observed_at":"2026-07-06T22:07:02.782730Z","submitted_at":"2025-08-03T14:00:54Z","title":"Resolving the Planck-DESI tension by nonminimally coupled quintessence","version":5},"reference_index":22,"source":"pdf_text","source_observed_at":"2026-05-19T01:35:36.430109Z"},"links":{"cited_paper":"/paper/2412.12905","citing_paper":"/paper/2508.01759"},"observation_digest":"sha256:8e5ae290464e58069249d997b8899e155d88d7071accb431347a0f48824051a6","observation_id":"fd5d076d-1a8e-41e9-afa5-535a68345bca","resolution":{"observed_at":"2026-05-19T01:36:57.984521Z","resolver_source":"arxiv_id","status":"verified_exact"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-19T06:32:44.657259+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-19T06:32:44.657259+00:00","source":"crossref"},{"observed_at":"2026-08-19T06:32:39.956319+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":{"arxiv_id":"2412.12905","last_updated":"2025-01-25T08:30:04Z","snapshot_observed_at":"2026-08-17T16:16:24.002443Z","submitted_at":"2024-12-17T13:31:15Z","title":"DESI and SNe: Dynamical Dark Energy, $\\Omega_m$ Tension or Systematics?","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2412.12905","snapshot_observed_at":"2026-08-05T23:25:36.592233Z","title":"\\'O ., Sheikh-Jabbari M","venue":null,"work_id":null,"year":2024},"citing_paper":{"arxiv_id":"2508.05389","last_updated":"2025-08-07T13:39:07Z","snapshot_observed_at":"2026-08-19T05:44:40.901702Z","submitted_at":"2025-08-07T13:39:07Z","title":"Constraints on transition redshift utilizing the latest H(z) measurements and comments on the Hubble tension","version":1},"reference_index":39,"source":"arxiv_source","source_observed_at":"2026-08-05T23:25:36.592233Z"},"links":{"cited_paper":"/paper/2412.12905","citing_paper":"/paper/2508.05389"},"observation_digest":"sha256:7deb1defe3d3137195a8a1dd4d1086bcf4a90584f418d1ce829d09968e82dd31","observation_id":"1d46001f-521b-4551-9832-7efba630134c","resolution":{"observed_at":"2026-08-05T23:25:36.592233Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2412.12905","last_updated":"2025-01-25T08:30:04Z","snapshot_observed_at":"2026-08-17T16:16:24.002443Z","submitted_at":"2024-12-17T13:31:15Z","title":"DESI and SNe: Dynamical Dark Energy, $\\Omega_m$ Tension or Systematics?","version":2},"cited_work":{"arxiv_id":"2412.12905","doi":null,"metadata_source":"pith","pith_arxiv_id":"2412.12905","snapshot_observed_at":"2026-07-08T15:55:05.017633Z","title":"DESI and SNe: Dynamical Dark Energy, Ω m Tension or System- atics?","venue":"astro-ph.CO","work_id":"9bc5da8e-a5f2-4c58-be0d-9dbcbe1c8f87","year":2024},"citing_paper":{"arxiv_id":"2510.03779","last_updated":"2026-02-17T10:47:14Z","snapshot_observed_at":"2026-08-20T02:01:23.133869Z","submitted_at":"2025-10-04T11:08:41Z","title":"Beyond CPL: Evidence for dynamical dark energy in three-parameter models","version":3},"reference_index":47,"source":"pdf_text","source_observed_at":"2026-05-18T10:45:16.985887Z"},"links":{"cited_paper":"/paper/2412.12905","citing_paper":"/paper/2510.03779"},"observation_digest":"sha256:f688b3bd3b53b24181668baf5affabc67a327490c84d900be41f6df04378984c","observation_id":"ffa7031c-815d-482f-8412-e9e6d5f9e703","resolution":{"observed_at":"2026-05-18T10:46:16.666674Z","resolver_source":"arxiv_id","status":"verified_exact"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-19T06:32:44.657259+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-19T06:32:44.657259+00:00","source":"crossref"},{"observed_at":"2026-08-19T06:32:39.956319+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":{"arxiv_id":"2412.12905","last_updated":"2025-01-25T08:30:04Z","snapshot_observed_at":"2026-08-17T16:16:24.002443Z","submitted_at":"2024-12-17T13:31:15Z","title":"DESI and SNe: Dynamical Dark Energy, $\\Omega_m$ Tension or Systematics?","version":2},"cited_work":{"arxiv_id":"2412.12905","doi":null,"metadata_source":"pith","pith_arxiv_id":"2412.12905","snapshot_observed_at":"2026-07-08T15:55:05.017633Z","title":"DESI and SNe: Dynamical Dark Energy, Ω m Tension or System- atics?","venue":"astro-ph.CO","work_id":"9bc5da8e-a5f2-4c58-be0d-9dbcbe1c8f87","year":2024},"citing_paper":{"arxiv_id":"2510.04179","last_updated":"2026-06-10T06:51:56Z","snapshot_observed_at":"2026-08-13T04:13:29.572534Z","submitted_at":"2025-10-05T12:41:23Z","title":"Crosschecking Cosmic Distances from DESI BAO and DES SNe","version":3},"reference_index":19,"source":"pdf_text","source_observed_at":"2026-05-18T10:32:00.438157Z"},"links":{"cited_paper":"/paper/2412.12905","citing_paper":"/paper/2510.04179"},"observation_digest":"sha256:7ddbae0fef2b5105f354beff6b042fbd3d94c558046978e47e4728e6f7d52007","observation_id":"410db800-809c-4c19-ab80-350d64582361","resolution":{"observed_at":"2026-05-18T10:32:33.857388Z","resolver_source":"arxiv_id","status":"verified_exact"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-19T06:32:44.657259+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-19T06:32:44.657259+00:00","source":"crossref"},{"observed_at":"2026-08-19T06:32:39.956319+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":{"arxiv_id":"2412.12905","last_updated":"2025-01-25T08:30:04Z","snapshot_observed_at":"2026-08-17T16:16:24.002443Z","submitted_at":"2024-12-17T13:31:15Z","title":"DESI and SNe: Dynamical Dark Energy, $\\Omega_m$ Tension or Systematics?","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2412.12905","snapshot_observed_at":"2026-08-04T11:34:09.414604Z","title":"´O Colg ´ain and M","venue":null,"work_id":null,"year":2025},"citing_paper":{"arxiv_id":"2510.04179","last_updated":"2026-06-10T06:51:56Z","snapshot_observed_at":"2026-08-13T04:13:29.572534Z","submitted_at":"2025-10-05T12:41:23Z","title":"Crosschecking Cosmic Distances from DESI BAO and DES SNe","version":4},"reference_index":19,"source":"pdf_text","source_observed_at":"2026-08-04T11:34:09.414604Z"},"links":{"cited_paper":"/paper/2412.12905","citing_paper":"/paper/2510.04179"},"observation_digest":"sha256:7f7c8a58e3c5ee01473ccc1102a01d451f0c65b88714e4debe34229add38b372","observation_id":"4fc247fa-9fdf-4fa9-845b-01bd6507f3a4","resolution":{"observed_at":"2026-08-04T11:34:09.414604Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2412.12905","last_updated":"2025-01-25T08:30:04Z","snapshot_observed_at":"2026-08-17T16:16:24.002443Z","submitted_at":"2024-12-17T13:31:15Z","title":"DESI and SNe: Dynamical Dark Energy, $\\Omega_m$ Tension or Systematics?","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2412.12905","snapshot_observed_at":"2026-08-04T09:59:21.190629Z","title":null,"venue":null,"work_id":null,"year":2024},"citing_paper":{"arxiv_id":"2510.12627","last_updated":"2026-06-20T07:00:45Z","snapshot_observed_at":"2026-08-19T21:41:40.945785Z","submitted_at":"2025-10-14T15:24:50Z","title":"Alleviating the $H_0$ tension through the interacting dark energy model from quantum gravitational field theory in light of DESI DR2","version":2},"reference_index":112,"source":"pdf_text","source_observed_at":"2026-08-04T09:59:21.190629Z"},"links":{"cited_paper":"/paper/2412.12905","citing_paper":"/paper/2510.12627"},"observation_digest":"sha256:c876fd303838eb03ad561b897f8bf1e31747e44bd8b51e230d477e5f7113f644","observation_id":"1d7d9152-e2ee-4b50-bbed-5cf4908110fb","resolution":{"observed_at":"2026-08-04T09:59:21.190629Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2412.12905","last_updated":"2025-01-25T08:30:04Z","snapshot_observed_at":"2026-08-17T16:16:24.002443Z","submitted_at":"2024-12-17T13:31:15Z","title":"DESI and SNe: Dynamical Dark Energy, $\\Omega_m$ Tension or Systematics?","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2412.12905","snapshot_observed_at":"2026-08-04T08:18:50.581465Z","title":null,"venue":null,"work_id":null,"year":2024},"citing_paper":{"arxiv_id":"2510.21627","last_updated":"2026-07-14T13:09:37Z","snapshot_observed_at":"2026-08-20T02:00:07.202577Z","submitted_at":"2025-10-24T16:32:10Z","title":"DESI constraints on two-field quintessence with exponential potentials","version":2},"reference_index":56,"source":"pdf_text","source_observed_at":"2026-08-04T08:18:50.581465Z"},"links":{"cited_paper":"/paper/2412.12905","citing_paper":"/paper/2510.21627"},"observation_digest":"sha256:4918f8936ee853d52d1a97c57a304881e7e9a215f9d38e4231ae1ebc3b7f47f8","observation_id":"960b6dd7-e0ce-4210-a6a7-2d4bb0514029","resolution":{"observed_at":"2026-08-04T08:18:50.581465Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2412.12905","last_updated":"2025-01-25T08:30:04Z","snapshot_observed_at":"2026-08-17T16:16:24.002443Z","submitted_at":"2024-12-17T13:31:15Z","title":"DESI and SNe: Dynamical Dark Energy, $\\Omega_m$ Tension or Systematics?","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2412.12905","snapshot_observed_at":"2026-08-03T18:51:46.262584Z","title":null,"venue":null,"work_id":null,"year":2025},"citing_paper":{"arxiv_id":"2512.04130","last_updated":"2026-07-26T05:14:02Z","snapshot_observed_at":"2026-08-09T18:20:38.058807Z","submitted_at":"2025-12-03T06:33:55Z","title":"Controlled Tension Forecasting: Quantifying Cross-Probe Biases in $\\omega_0\\omega_a$CDM","version":2},"reference_index":79,"source":"pdf_text","source_observed_at":"2026-08-03T18:51:46.262584Z"},"links":{"cited_paper":"/paper/2412.12905","citing_paper":"/paper/2512.04130"},"observation_digest":"sha256:3674834fa9799f88d91ad980b9dcbc612a2bb09caf2331c59cd8d5ca3f30b117","observation_id":"1f7274ea-cdd9-47ee-ace7-de4d3b057dfb","resolution":{"observed_at":"2026-08-03T18:51:46.262584Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2412.12905","last_updated":"2025-01-25T08:30:04Z","snapshot_observed_at":"2026-08-17T16:16:24.002443Z","submitted_at":"2024-12-17T13:31:15Z","title":"DESI and SNe: Dynamical Dark Energy, $\\Omega_m$ Tension or Systematics?","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2412.12905","snapshot_observed_at":"2026-08-03T14:40:55.433543Z","title":null,"venue":null,"work_id":null,"year":2025},"citing_paper":{"arxiv_id":"2512.19888","last_updated":"2026-06-18T12:16:03Z","snapshot_observed_at":"2026-08-17T17:44:10.961719Z","submitted_at":"2025-12-22T21:27:32Z","title":"Observational constraints on early time non-phantom behaviour of dynamical dark energy","version":2},"reference_index":47,"source":"pdf_text","source_observed_at":"2026-08-03T14:40:55.433543Z"},"links":{"cited_paper":"/paper/2412.12905","citing_paper":"/paper/2512.19888"},"observation_digest":"sha256:cdd9b6bf38006cf8b88bc0cfc3f3f8fa0ec31e41ade983cefb814727da4c5c1d","observation_id":"80dbbca6-24a9-41ec-a019-6ec4cc6bf6da","resolution":{"observed_at":"2026-08-03T14:40:55.433543Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2412.12905","last_updated":"2025-01-25T08:30:04Z","snapshot_observed_at":"2026-08-17T16:16:24.002443Z","submitted_at":"2024-12-17T13:31:15Z","title":"DESI and SNe: Dynamical Dark Energy, $\\Omega_m$ Tension or Systematics?","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2412.12905","snapshot_observed_at":"2026-08-03T11:11:48.995267Z","title":null,"venue":null,"work_id":null,"year":2025},"citing_paper":{"arxiv_id":"2601.07361","last_updated":"2026-07-15T07:08:06Z","snapshot_observed_at":"2026-08-19T06:05:14.523776Z","submitted_at":"2026-01-12T09:36:30Z","title":"Robust Preference for Dark Sector Interactions","version":2},"reference_index":150,"source":"pdf_text","source_observed_at":"2026-08-03T11:11:48.995267Z"},"links":{"cited_paper":"/paper/2412.12905","citing_paper":"/paper/2601.07361"},"observation_digest":"sha256:d0a437ffff7e7c8c56357134db1903e4639d38b33c89faab52531ab825c91ce2","observation_id":"2b51538f-5cdf-440f-9e35-039b5547cdd7","resolution":{"observed_at":"2026-08-03T11:11:48.995267Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2412.12905","last_updated":"2025-01-25T08:30:04Z","snapshot_observed_at":"2026-08-17T16:16:24.002443Z","submitted_at":"2024-12-17T13:31:15Z","title":"DESI and SNe: Dynamical Dark Energy, $\\Omega_m$ Tension or Systematics?","version":2},"cited_work":{"arxiv_id":"2412.12905","doi":null,"metadata_source":"pith","pith_arxiv_id":"2412.12905","snapshot_observed_at":"2026-07-08T15:55:05.017633Z","title":"DESI and SNe: Dynamical Dark Energy, Ω m Tension or System- atics?","venue":"astro-ph.CO","work_id":"9bc5da8e-a5f2-4c58-be0d-9dbcbe1c8f87","year":2024},"citing_paper":{"arxiv_id":"2602.11093","last_updated":"2026-04-18T16:30:32Z","snapshot_observed_at":"2026-08-08T00:16:50.248213Z","submitted_at":"2026-02-11T18:01:44Z","title":"New constraints on cosmic anisotropy from galaxy clusters using an improved dipole fitting method","version":2},"reference_index":34,"source":"pdf_text","source_observed_at":"2026-05-16T02:22:49.920780Z"},"links":{"cited_paper":"/paper/2412.12905","citing_paper":"/paper/2602.11093"},"observation_digest":"sha256:71b6b3258c197e8adedb35d482af3d2a2109a923538c23248acb95e99173052b","observation_id":"8b7928cb-d6c1-4d12-9b1d-667b96bccc1c","resolution":{"observed_at":"2026-05-16T02:27:10.063580Z","resolver_source":"arxiv_id","status":"verified_exact"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-19T06:32:44.657259+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-19T06:32:44.657259+00:00","source":"crossref"},{"observed_at":"2026-08-19T06:32:39.956319+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":{"arxiv_id":"2412.12905","last_updated":"2025-01-25T08:30:04Z","snapshot_observed_at":"2026-08-17T16:16:24.002443Z","submitted_at":"2024-12-17T13:31:15Z","title":"DESI and SNe: Dynamical Dark Energy, $\\Omega_m$ Tension or Systematics?","version":2},"cited_work":{"arxiv_id":"2412.12905","doi":null,"metadata_source":"pith","pith_arxiv_id":"2412.12905","snapshot_observed_at":"2026-07-08T15:55:05.017633Z","title":"DESI and SNe: Dynamical Dark Energy, Ω m Tension or System- atics?","venue":"astro-ph.CO","work_id":"9bc5da8e-a5f2-4c58-be0d-9dbcbe1c8f87","year":2024},"citing_paper":{"arxiv_id":"2604.03167","last_updated":"2026-04-03T16:44:30Z","snapshot_observed_at":"2026-08-19T14:01:49.571363Z","submitted_at":"2026-04-03T16:44:30Z","title":"Mapping the redshift drift at various redshifts through cosmography","version":1},"reference_index":32,"source":"pdf_text","source_observed_at":"2026-05-13T18:35:55.346976Z"},"links":{"cited_paper":"/paper/2412.12905","citing_paper":"/paper/2604.03167"},"observation_digest":"sha256:24a4a867cfbd21bc7c153f8eb70322f08ec4c36fe72c52fea22e4ce4fcf02173","observation_id":"0f0f6064-6fc8-4b5d-8189-e6d0d3f27f3f","resolution":{"observed_at":"2026-05-13T18:38:07.456074Z","resolver_source":"arxiv_id","status":"verified_exact"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-19T06:32:44.657259+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-19T06:32:44.657259+00:00","source":"crossref"},{"observed_at":"2026-08-19T06:32:39.956319+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":{"arxiv_id":"2412.12905","last_updated":"2025-01-25T08:30:04Z","snapshot_observed_at":"2026-08-17T16:16:24.002443Z","submitted_at":"2024-12-17T13:31:15Z","title":"DESI and SNe: Dynamical Dark Energy, $\\Omega_m$ Tension or Systematics?","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2412.12905","snapshot_observed_at":"2026-08-02T14:29:23.253844Z","title":null,"venue":null,"work_id":null,"year":2025},"citing_paper":{"arxiv_id":"2605.10476","last_updated":"2026-07-21T12:07:55Z","snapshot_observed_at":"2026-08-11T08:05:13.599295Z","submitted_at":"2026-05-11T12:38:17Z","title":"Breaking Free from the Swampland of Impossible Universes through the DESI Portal","version":4},"reference_index":84,"source":"pdf_text","source_observed_at":"2026-08-02T14:29:23.253844Z"},"links":{"cited_paper":"/paper/2412.12905","citing_paper":"/paper/2605.10476"},"observation_digest":"sha256:6b898807e24598636ce0d244e959f89d31af45e4195cbf2dfc1f48694e50facb","observation_id":"ed036ebe-61b0-451a-a137-ab1ce39e26ca","resolution":{"observed_at":"2026-08-02T14:29:23.253844Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2412.12905","last_updated":"2025-01-25T08:30:04Z","snapshot_observed_at":"2026-08-17T16:16:24.002443Z","submitted_at":"2024-12-17T13:31:15Z","title":"DESI and SNe: Dynamical Dark Energy, $\\Omega_m$ Tension or Systematics?","version":2},"cited_work":{"arxiv_id":"2412.12905","doi":null,"metadata_source":"pith","pith_arxiv_id":"2412.12905","snapshot_observed_at":"2026-07-08T15:55:05.017633Z","title":"DESI and SNe: Dynamical Dark Energy, Ω m Tension or System- atics?","venue":"astro-ph.CO","work_id":"9bc5da8e-a5f2-4c58-be0d-9dbcbe1c8f87","year":2024},"citing_paper":{"arxiv_id":"2606.01360","last_updated":"2026-07-18T02:00:49Z","snapshot_observed_at":"2026-08-12T22:06:47.187155Z","submitted_at":"2026-05-31T17:31:59Z","title":"A short review on Quintom dark energy theory","version":1},"reference_index":41,"source":"pdf_text","source_observed_at":"2026-06-28T16:17:39.285285Z"},"links":{"cited_paper":"/paper/2412.12905","citing_paper":"/paper/2606.01360"},"observation_digest":"sha256:e75eb95e80e59d37ec57d196e0d780d9f0dccd78fc607279845cae1b88ec5bae","observation_id":"ad9e7e72-a52b-4509-adce-fce27fa8e5f9","resolution":{"observed_at":"2026-07-01T21:46:15.850126Z","resolver_source":"arxiv_id","status":"verified_exact"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-19T06:32:44.657259+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-19T06:32:44.657259+00:00","source":"crossref"},{"observed_at":"2026-08-19T06:32:39.956319+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":{"arxiv_id":"2412.12905","last_updated":"2025-01-25T08:30:04Z","snapshot_observed_at":"2026-08-17T16:16:24.002443Z","submitted_at":"2024-12-17T13:31:15Z","title":"DESI and SNe: Dynamical Dark Energy, $\\Omega_m$ Tension or Systematics?","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2412.12905","snapshot_observed_at":"2026-08-02T12:40:02.711551Z","title":null,"venue":null,"work_id":null,"year":2025},"citing_paper":{"arxiv_id":"2606.01360","last_updated":"2026-07-18T02:00:49Z","snapshot_observed_at":"2026-08-12T22:06:47.187155Z","submitted_at":"2026-05-31T17:31:59Z","title":"A short review on Quintom dark energy theory","version":2},"reference_index":41,"source":"pdf_text","source_observed_at":"2026-08-02T12:40:02.711551Z"},"links":{"cited_paper":"/paper/2412.12905","citing_paper":"/paper/2606.01360"},"observation_digest":"sha256:293fc0e46164124c04907ad5d27132884313e919ab783fabe8b27f35316f17af","observation_id":"1f509e89-c6a5-447e-9448-22c1330908e7","resolution":{"observed_at":"2026-08-02T12:40:02.711551Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2412.12905","last_updated":"2025-01-25T08:30:04Z","snapshot_observed_at":"2026-08-17T16:16:24.002443Z","submitted_at":"2024-12-17T13:31:15Z","title":"DESI and SNe: Dynamical Dark Energy, $\\Omega_m$ Tension or Systematics?","version":2},"cited_work":{"arxiv_id":"2412.12905","doi":null,"metadata_source":"pith","pith_arxiv_id":"2412.12905","snapshot_observed_at":"2026-07-08T15:55:05.017633Z","title":"DESI and SNe: Dynamical Dark Energy, Ω m Tension or System- atics?","venue":"astro-ph.CO","work_id":"9bc5da8e-a5f2-4c58-be0d-9dbcbe1c8f87","year":2024},"citing_paper":{"arxiv_id":"2606.12822","last_updated":"2026-06-11T02:35:35Z","snapshot_observed_at":"2026-07-06T23:51:40.528967Z","submitted_at":"2026-06-11T02:35:35Z","title":"Geometric obstruction to resolving the Hubble tension: orthogonality of scale and shape in distance measurements","version":1},"reference_index":58,"source":"pdf_text","source_observed_at":"2026-06-27T06:23:50.957273Z"},"links":{"cited_paper":"/paper/2412.12905","citing_paper":"/paper/2606.12822"},"observation_digest":"sha256:977b4a128551a8f50044c331f11e9f94f44dc34c63f5ae4ada8509bbfa9bdd15","observation_id":"1b97afb1-7395-4693-be8c-e4ed53511c94","resolution":{"observed_at":"2026-07-03T15:38:34.040238Z","resolver_source":"arxiv_id","status":"verified_exact"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-19T06:32:44.657259+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-19T06:32:44.657259+00:00","source":"crossref"},{"observed_at":"2026-08-19T06:32:39.956319+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":{"arxiv_id":"2412.12905","last_updated":"2025-01-25T08:30:04Z","snapshot_observed_at":"2026-08-17T16:16:24.002443Z","submitted_at":"2024-12-17T13:31:15Z","title":"DESI and SNe: Dynamical Dark Energy, $\\Omega_m$ Tension or Systematics?","version":2},"cited_work":{"arxiv_id":"2412.12905","doi":null,"metadata_source":"pith","pith_arxiv_id":"2412.12905","snapshot_observed_at":"2026-07-08T15:55:05.017633Z","title":"DESI and SNe: Dynamical Dark Energy, Ω m Tension or System- atics?","venue":"astro-ph.CO","work_id":"9bc5da8e-a5f2-4c58-be0d-9dbcbe1c8f87","year":2024},"citing_paper":{"arxiv_id":"2606.19090","last_updated":"2026-06-17T13:58:39Z","snapshot_observed_at":"2026-07-06T23:54:27.624372Z","submitted_at":"2026-06-17T13:58:39Z","title":"Resolving the Hubble Tension in the Early Dark Energy Framework with JWST and DESI Data","version":1},"reference_index":133,"source":"pdf_text","source_observed_at":"2026-06-26T19:48:32.340111Z"},"links":{"cited_paper":"/paper/2412.12905","citing_paper":"/paper/2606.19090"},"observation_digest":"sha256:c15d4cfd275fe87fce0f6206d61bf6bfa6dfab000396fff231f3495fecc5ac12","observation_id":"ca645464-17f8-43d8-8fbc-1346abd31363","resolution":{"observed_at":"2026-07-04T02:19:23.617817Z","resolver_source":"arxiv_id","status":"verified_exact"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-19T06:32:44.657259+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-19T06:32:44.657259+00:00","source":"crossref"},{"observed_at":"2026-08-19T06:32:39.956319+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":{"arxiv_id":"2412.12905","last_updated":"2025-01-25T08:30:04Z","snapshot_observed_at":"2026-08-17T16:16:24.002443Z","submitted_at":"2024-12-17T13:31:15Z","title":"DESI and SNe: Dynamical Dark Energy, $\\Omega_m$ Tension or Systematics?","version":2},"cited_work":{"arxiv_id":"2412.12905","doi":null,"metadata_source":"pith","pith_arxiv_id":"2412.12905","snapshot_observed_at":"2026-07-08T15:55:05.017633Z","title":"DESI and SNe: Dynamical Dark Energy, Ω m Tension or System- atics?","venue":"astro-ph.CO","work_id":"9bc5da8e-a5f2-4c58-be0d-9dbcbe1c8f87","year":2024},"citing_paper":{"arxiv_id":"2607.01226","last_updated":"2026-08-10T20:43:51Z","snapshot_observed_at":"2026-08-18T00:17:05.378129Z","submitted_at":"2026-07-01T17:57:32Z","title":"Intertwined Constraints in Extended Cosmologies: Dark Energy, Curvature, Neutrinos, and Inflation","version":1},"reference_index":268,"source":"pdf_text","source_observed_at":"2026-07-02T06:14:20.101706Z"},"links":{"cited_paper":"/paper/2412.12905","citing_paper":"/paper/2607.01226"},"observation_digest":"sha256:dc2ec2c63616409665490663bfd5fe44d45aa6ba60fe3373a3c0e8ecb427a6e7","observation_id":"68042e03-fbd0-43b4-81de-d51a0cc6a7f6","resolution":{"observed_at":"2026-07-02T06:16:43.190898Z","resolver_source":"arxiv_id","status":"verified_exact"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-19T06:32:44.657259+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-19T06:32:44.657259+00:00","source":"crossref"},{"observed_at":"2026-08-19T06:32:39.956319+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":{"arxiv_id":"2412.12905","last_updated":"2025-01-25T08:30:04Z","snapshot_observed_at":"2026-08-17T16:16:24.002443Z","submitted_at":"2024-12-17T13:31:15Z","title":"DESI and SNe: Dynamical Dark Energy, $\\Omega_m$ Tension or Systematics?","version":2},"cited_work":{"arxiv_id":"2412.12905","doi":null,"metadata_source":"pith","pith_arxiv_id":"2412.12905","snapshot_observed_at":"2026-07-08T15:55:05.017633Z","title":"DESI and SNe: Dynamical Dark Energy, Ω m Tension or System- atics?","venue":"astro-ph.CO","work_id":"9bc5da8e-a5f2-4c58-be0d-9dbcbe1c8f87","year":2024},"citing_paper":{"arxiv_id":"2607.06147","last_updated":"2026-07-07T11:15:39Z","snapshot_observed_at":"2026-08-07T05:12:27.762181Z","submitted_at":"2026-07-07T11:15:39Z","title":"Imprint of swampland-inspired coupled early dark energy","version":1},"reference_index":53,"source":"pdf_text","source_observed_at":"2026-07-08T15:47:53.145943Z"},"links":{"cited_paper":"/paper/2412.12905","citing_paper":"/paper/2607.06147"},"observation_digest":"sha256:9b9906eba153ba09447831693f9324ef1f32ed62dcbbf5f52532821d6406527f","observation_id":"a3b60f7a-85b8-4118-b307-3374bbf79db4","resolution":{"observed_at":"2026-07-08T15:55:05.018866Z","resolver_source":"local_arxiv","status":"verified_exact"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-19T06:32:44.657259+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-19T06:32:44.657259+00:00","source":"crossref"},{"observed_at":"2026-08-19T06:32:39.956319+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":{"arxiv_id":"2412.12905","last_updated":"2025-01-25T08:30:04Z","snapshot_observed_at":"2026-08-17T16:16:24.002443Z","submitted_at":"2024-12-17T13:31:15Z","title":"DESI and SNe: Dynamical Dark Energy, $\\Omega_m$ Tension or Systematics?","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2412.12905","snapshot_observed_at":"2026-08-02T03:36:03.719306Z","title":null,"venue":null,"work_id":null,"year":2025},"citing_paper":{"arxiv_id":"2607.13857","last_updated":"2026-07-15T14:02:52Z","snapshot_observed_at":"2026-08-18T10:37:50.336246Z","submitted_at":"2026-07-15T14:02:52Z","title":"Evaporating cosmologically coupled black holes","version":1},"reference_index":257,"source":"pdf_text","source_observed_at":"2026-08-02T03:36:03.719306Z"},"links":{"cited_paper":"/paper/2412.12905","citing_paper":"/paper/2607.13857"},"observation_digest":"sha256:005957a285c62a6fb033289dea7d3f8fa61e1258717dcceb463c9000db973eb4","observation_id":"948cf7cd-c83e-4538-abe4-fc8448d4ca92","resolution":{"observed_at":"2026-08-02T03:36:03.719306Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2412.12905","last_updated":"2025-01-25T08:30:04Z","snapshot_observed_at":"2026-08-17T16:16:24.002443Z","submitted_at":"2024-12-17T13:31:15Z","title":"DESI and SNe: Dynamical Dark Energy, $\\Omega_m$ Tension or Systematics?","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2412.12905","snapshot_observed_at":"2026-08-01T08:09:03.729947Z","title":null,"venue":null,"work_id":null,"year":2025},"citing_paper":{"arxiv_id":"2607.21244","last_updated":"2026-07-23T12:08:39Z","snapshot_observed_at":"2026-08-18T04:16:34.790019Z","submitted_at":"2026-07-23T12:08:39Z","title":"Hubble tension: the shape wall","version":1},"reference_index":297,"source":"pdf_text","source_observed_at":"2026-08-01T08:09:03.729947Z"},"links":{"cited_paper":"/paper/2412.12905","citing_paper":"/paper/2607.21244"},"observation_digest":"sha256:ddf7ebbf90ea6c072f966ee4a9a6d455553ea77d5c3ab431363a2fb758bfe0a2","observation_id":"7cde0bcd-25e4-4488-9227-69babe230479","resolution":{"observed_at":"2026-08-01T08:09:03.729947Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2412.12905","last_updated":"2025-01-25T08:30:04Z","snapshot_observed_at":"2026-08-17T16:16:24.002443Z","submitted_at":"2024-12-17T13:31:15Z","title":"DESI and SNe: Dynamical Dark Energy, $\\Omega_m$ Tension or Systematics?","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2412.12905","snapshot_observed_at":"2026-07-31T11:14:46.860699Z","title":"and Sheikh-Jabbari, M","venue":null,"work_id":null,"year":2025},"citing_paper":{"arxiv_id":"2607.28326","last_updated":"2026-07-30T14:57:39Z","snapshot_observed_at":"2026-08-17T14:41:15.492160Z","submitted_at":"2026-07-30T14:57:39Z","title":"Growth, geometry, and early-universe split of the matter density parameter $\\Omega_{\\rm m}$","version":1},"reference_index":49,"source":"arxiv_source","source_observed_at":"2026-07-31T11:14:46.860699Z"},"links":{"cited_paper":"/paper/2412.12905","citing_paper":"/paper/2607.28326"},"observation_digest":"sha256:0585ba67008a4ff85f3c3fa56bdaad80f7c49386691225836d4890d33bf52d00","observation_id":"cd3ea272-4f26-44cf-ab7a-e6ae3a55f1b9","resolution":{"observed_at":"2026-07-31T11:14:46.860699Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2412.12905","last_updated":"2025-01-25T08:30:04Z","snapshot_observed_at":"2026-08-17T16:16:24.002443Z","submitted_at":"2024-12-17T13:31:15Z","title":"DESI and SNe: Dynamical Dark Energy, $\\Omega_m$ Tension or Systematics?","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2412.12905","snapshot_observed_at":"2026-08-03T17:20:49.356567Z","title":"Ó Colgáin and M.M","venue":null,"work_id":null,"year":2025},"citing_paper":{"arxiv_id":"2607.28918","last_updated":"2026-08-19T02:07:22Z","snapshot_observed_at":"2026-08-20T03:20:54.419500Z","submitted_at":"2026-07-31T00:34:31Z","title":"A Sequentially-Valid Reanalysis of DESI's Dynamical Dark Energy Signal","version":1},"reference_index":18,"source":"pdf_text","source_observed_at":"2026-08-03T17:20:49.356567Z"},"links":{"cited_paper":"/paper/2412.12905","citing_paper":"/paper/2607.28918"},"observation_digest":"sha256:da924a9b2a158a17d072312d0112ef4a32d3018b8d38f8d17b06c6cb31c69e9a","observation_id":"ea65fd28-5167-4c6c-94e1-e0a177ddb26c","resolution":{"observed_at":"2026-08-03T17:20:49.356567Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2412.12905","last_updated":"2025-01-25T08:30:04Z","snapshot_observed_at":"2026-08-17T16:16:24.002443Z","submitted_at":"2024-12-17T13:31:15Z","title":"DESI and SNe: Dynamical Dark Energy, $\\Omega_m$ Tension or Systematics?","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2412.12905","snapshot_observed_at":"2026-08-06T00:32:11.190153Z","title":null,"venue":null,"work_id":null,"year":2025},"citing_paper":{"arxiv_id":"2608.01215","last_updated":"2026-08-02T13:02:59Z","snapshot_observed_at":"2026-08-13T11:46:41.598479Z","submitted_at":"2026-08-02T13:02:59Z","title":"Do we really need alternatives to the $\\omega_0\\omega_a$CDM parameterization after the DESI DR2?","version":1},"reference_index":69,"source":"pdf_text","source_observed_at":"2026-08-06T00:32:11.190153Z"},"links":{"cited_paper":"/paper/2412.12905","citing_paper":"/paper/2608.01215"},"observation_digest":"sha256:1f7e065aadd03812d7ebb2c4c2094ba9481b8495b7b65711021ab26758e197bc","observation_id":"d92f815b-229a-48f9-a494-01171dbc2c9f","resolution":{"observed_at":"2026-08-06T00:32:11.190153Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2412.12905","last_updated":"2025-01-25T08:30:04Z","snapshot_observed_at":"2026-08-17T16:16:24.002443Z","submitted_at":"2024-12-17T13:31:15Z","title":"DESI and SNe: Dynamical Dark Energy, $\\Omega_m$ Tension or Systematics?","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2412.12905","snapshot_observed_at":"2026-08-08T19:17:22.472790Z","title":null,"venue":null,"work_id":null,"year":2024},"citing_paper":{"arxiv_id":"2608.04353","last_updated":"2026-08-05T01:54:49Z","snapshot_observed_at":"2026-08-19T10:57:51.211946Z","submitted_at":"2026-08-05T01:54:49Z","title":"Revisiting the equation of state of dark energy from DESI BAO with SNe Ia and CMB","version":1},"reference_index":33,"source":"pdf_text","source_observed_at":"2026-08-08T19:17:22.472790Z"},"links":{"cited_paper":"/paper/2412.12905","citing_paper":"/paper/2608.04353"},"observation_digest":"sha256:90fa2f75d50695ba1546f393c020b89343ec891f99affb9ee89df1120ef67314","observation_id":"9947ecac-7951-4d33-ad32-8fe6bffd5686","resolution":{"observed_at":"2026-08-08T19:17:22.472790Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2412.12905","last_updated":"2025-01-25T08:30:04Z","snapshot_observed_at":"2026-08-17T16:16:24.002443Z","submitted_at":"2024-12-17T13:31:15Z","title":"DESI and SNe: Dynamical Dark Energy, $\\Omega_m$ Tension or Systematics?","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2412.12905","snapshot_observed_at":"2026-08-15T14:42:16.880292Z","title":null,"venue":null,"work_id":null,"year":2025},"citing_paper":{"arxiv_id":"2608.04922","last_updated":"2026-08-05T14:51:13Z","snapshot_observed_at":"2026-08-19T11:16:25.476467Z","submitted_at":"2026-08-05T14:51:13Z","title":"Evolution of matter perturbations in the context of cosmic slowing down","version":1},"reference_index":34,"source":"pdf_text","source_observed_at":"2026-08-15T14:42:16.880292Z"},"links":{"cited_paper":"/paper/2412.12905","citing_paper":"/paper/2608.04922"},"observation_digest":"sha256:891aa5fb30176624a6a05cfafebd409328be159a6ab94c7e3a044755f5b5b387","observation_id":"d19cd7a2-5172-4b5e-b04f-dc77ebf8c355","resolution":{"observed_at":"2026-08-15T14:42:16.880292Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}}],"links":{"evidence":"/evidence","html":"/paper/2412.12905/citation-record","integrity":"/paper/2412.12905/integrity","json":"/paper/2412.12905/citation-record.json","paper":"/paper/2412.12905"},"outbound":[{"citation":{"cited_paper":{"arxiv_id":"2103.01183","last_updated":"2021-06-05T10:18:21Z","snapshot_observed_at":"2026-08-16T02:36:16.088814Z","submitted_at":"2021-03-01T18:27:48Z","title":"In the Realm of the Hubble tension $-$ a Review of Solutions","version":3},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2103.01183","snapshot_observed_at":"2026-08-11T13:41:23.565712Z","title":"Di Valentino, O","venue":null,"work_id":null,"year":2021},"citing_paper":{"arxiv_id":"2412.12905","last_updated":"2025-01-25T08:30:04Z","snapshot_observed_at":"2026-08-17T16:16:24.002443Z","submitted_at":"2024-12-17T13:31:15Z","title":"DESI and SNe: Dynamical Dark Energy, $\\Omega_m$ Tension or Systematics?","version":2},"reference_index":1,"source":"pdf_text","source_observed_at":"2026-08-11T13:41:23.565712Z"},"links":{"cited_paper":"/paper/2103.01183","citing_paper":"/paper/2412.12905"},"observation_digest":"sha256:d88a1b51ea61317dd020f098669b6bb5a637df8f098cece6b546ac90a97b0dbf","observation_id":"97007a7f-e3a3-4c5f-9bba-bccb9375ece3","resolution":{"observed_at":"2026-08-11T13:41:23.565712Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2105.05208","last_updated":"2022-04-06T12:16:37Z","snapshot_observed_at":"2026-08-04T21:52:15.150186Z","submitted_at":"2021-05-11T17:17:34Z","title":"Challenges for $\\Lambda$CDM: An update","version":3},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2105.05208","snapshot_observed_at":"2026-08-11T13:41:23.570089Z","title":"Perivolaropoulos and F","venue":null,"work_id":null,"year":2022},"citing_paper":{"arxiv_id":"2412.12905","last_updated":"2025-01-25T08:30:04Z","snapshot_observed_at":"2026-08-17T16:16:24.002443Z","submitted_at":"2024-12-17T13:31:15Z","title":"DESI and SNe: Dynamical Dark Energy, $\\Omega_m$ Tension or Systematics?","version":2},"reference_index":2,"source":"pdf_text","source_observed_at":"2026-08-11T13:41:23.570089Z"},"links":{"cited_paper":"/paper/2105.05208","citing_paper":"/paper/2412.12905"},"observation_digest":"sha256:d29d54f2455d2fb7cbfad1fcf3810b9a9164efdff95d4fd560a99af3bb880726","observation_id":"0a010786-948f-4086-a367-a916cb28619a","resolution":{"observed_at":"2026-08-11T13:41:23.570089Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2203.06142","last_updated":"2022-04-24T16:57:09Z","snapshot_observed_at":"2026-08-18T00:05:15.748844Z","submitted_at":"2022-03-11T18:13:52Z","title":"Cosmology Intertwined: A Review of the Particle Physics, Astrophysics, and Cosmology Associated with the Cosmological Tensions and Anomalies","version":3},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2203.06142","snapshot_observed_at":"2026-08-11T13:41:23.574349Z","title":"Abdalla et al","venue":null,"work_id":null,"year":2022},"citing_paper":{"arxiv_id":"2412.12905","last_updated":"2025-01-25T08:30:04Z","snapshot_observed_at":"2026-08-17T16:16:24.002443Z","submitted_at":"2024-12-17T13:31:15Z","title":"DESI and SNe: Dynamical Dark Energy, $\\Omega_m$ Tension or Systematics?","version":2},"reference_index":3,"source":"pdf_text","source_observed_at":"2026-08-11T13:41:23.574349Z"},"links":{"cited_paper":"/paper/2203.06142","citing_paper":"/paper/2412.12905"},"observation_digest":"sha256:ec4d997b1b88a659579d4c837a90a659023e1f8055fdeaf2b66be6464b4b1d99","observation_id":"bff04e44-7a25-4fb6-9020-c3e606d2daca","resolution":{"observed_at":"2026-08-11T13:41:23.574349Z","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":"2026-08-15T17:00:11.410484Z","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":"2026-08-11T13:41:23.578354Z","title":"Aghanim et al","venue":null,"work_id":null,"year":2020},"citing_paper":{"arxiv_id":"2412.12905","last_updated":"2025-01-25T08:30:04Z","snapshot_observed_at":"2026-08-17T16:16:24.002443Z","submitted_at":"2024-12-17T13:31:15Z","title":"DESI and SNe: Dynamical Dark Energy, $\\Omega_m$ Tension or Systematics?","version":2},"reference_index":4,"source":"pdf_text","source_observed_at":"2026-08-11T13:41:23.578354Z"},"links":{"cited_paper":"/paper/1807.06209","citing_paper":"/paper/2412.12905"},"observation_digest":"sha256:22180d28918afa3c18a2522873ecd3763765939b72b8cf74fa387a82e127e2c2","observation_id":"e6f053eb-cf06-4ca7-8b4c-75864590d0d5","resolution":{"observed_at":"2026-08-11T13:41:23.578354Z","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":"2026-08-11T13:41:23.582812Z","title":null,"venue":null,"work_id":null,"year":2022},"citing_paper":{"arxiv_id":"2412.12905","last_updated":"2025-01-25T08:30:04Z","snapshot_observed_at":"2026-08-17T16:16:24.002443Z","submitted_at":"2024-12-17T13:31:15Z","title":"DESI and SNe: Dynamical Dark Energy, $\\Omega_m$ Tension or Systematics?","version":2},"reference_index":5,"source":"pdf_text","source_observed_at":"2026-08-11T13:41:23.582812Z"},"links":{"cited_paper":"/paper/2112.04510","citing_paper":"/paper/2412.12905"},"observation_digest":"sha256:5f4ab55ad03f00e88ba7ecc10cc5f2fbf4f25f28332848fc8575648bbaa0565f","observation_id":"fadfeda2-d95c-4683-a955-d7a6a0ab06b7","resolution":{"observed_at":"2026-08-11T13:41:23.582812Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2106.15656","last_updated":"2021-06-29T18:09:57Z","snapshot_observed_at":"2026-08-16T18:13:32.550098Z","submitted_at":"2021-06-29T18:09:57Z","title":"Measurements of the Hubble Constant: Tensions in Perspective","version":1},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2106.15656","snapshot_observed_at":"2026-08-11T13:41:23.586771Z","title":null,"venue":null,"work_id":null,"year":2021},"citing_paper":{"arxiv_id":"2412.12905","last_updated":"2025-01-25T08:30:04Z","snapshot_observed_at":"2026-08-17T16:16:24.002443Z","submitted_at":"2024-12-17T13:31:15Z","title":"DESI and SNe: Dynamical Dark Energy, $\\Omega_m$ Tension or Systematics?","version":2},"reference_index":6,"source":"pdf_text","source_observed_at":"2026-08-11T13:41:23.586771Z"},"links":{"cited_paper":"/paper/2106.15656","citing_paper":"/paper/2412.12905"},"observation_digest":"sha256:7dc2236e7c1d7cdfb6e0f41a3ea9c7b635ab73538db277e64d0b49372665ba1e","observation_id":"049f476a-cffa-41b0-9142-4b16ba803675","resolution":{"observed_at":"2026-08-11T13:41:23.586771Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2001.09213","last_updated":"2020-02-18T20:10:10Z","snapshot_observed_at":"2026-08-15T01:47:20.280445Z","submitted_at":"2020-01-24T22:18:18Z","title":"The Megamaser Cosmology Project. XIII. Combined Hubble constant constraints","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2001.09213","snapshot_observed_at":"2026-08-11T13:41:23.590602Z","title":null,"venue":null,"work_id":null,"year":2020},"citing_paper":{"arxiv_id":"2412.12905","last_updated":"2025-01-25T08:30:04Z","snapshot_observed_at":"2026-08-17T16:16:24.002443Z","submitted_at":"2024-12-17T13:31:15Z","title":"DESI and SNe: Dynamical Dark Energy, $\\Omega_m$ Tension or Systematics?","version":2},"reference_index":7,"source":"pdf_text","source_observed_at":"2026-08-11T13:41:23.590602Z"},"links":{"cited_paper":"/paper/2001.09213","citing_paper":"/paper/2412.12905"},"observation_digest":"sha256:0a1e1644dd4495eb6ef594c21c22daeb0c25d3592158647dae6fe3b746d3ef64","observation_id":"c02e93ac-ecf5-4c28-b726-1782ede1dfb7","resolution":{"observed_at":"2026-08-11T13:41:23.590602Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2101.02221","last_updated":"2021-02-26T19:08:05Z","snapshot_observed_at":"2026-08-16T18:53:52.573198Z","submitted_at":"2021-01-06T19:00:06Z","title":"The Hubble Constant from Infrared Surface Brightness Fluctuation Distances","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2101.02221","snapshot_observed_at":"2026-08-11T13:41:23.594906Z","title":null,"venue":null,"work_id":null,"year":2021},"citing_paper":{"arxiv_id":"2412.12905","last_updated":"2025-01-25T08:30:04Z","snapshot_observed_at":"2026-08-17T16:16:24.002443Z","submitted_at":"2024-12-17T13:31:15Z","title":"DESI and SNe: Dynamical Dark Energy, $\\Omega_m$ Tension or Systematics?","version":2},"reference_index":8,"source":"pdf_text","source_observed_at":"2026-08-11T13:41:23.594906Z"},"links":{"cited_paper":"/paper/2101.02221","citing_paper":"/paper/2412.12905"},"observation_digest":"sha256:160f438dc530e44e472a510f65f127e059b905e66f4b120b583d10616c46a3d1","observation_id":"60e0bbd9-04f6-453e-b5f4-ace2b72820e4","resolution":{"observed_at":"2026-08-11T13:41:23.594906Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2004.14499","last_updated":"2020-05-21T07:07:07Z","snapshot_observed_at":"2026-08-14T16:46:08.334447Z","submitted_at":"2020-04-29T22:11:11Z","title":"Cosmicflows 4: The Calibration of Optical and Infrared Tully-Fisher Relations","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2004.14499","snapshot_observed_at":"2026-08-11T13:41:23.598825Z","title":"Kourkchi, R","venue":null,"work_id":null,"year":2020},"citing_paper":{"arxiv_id":"2412.12905","last_updated":"2025-01-25T08:30:04Z","snapshot_observed_at":"2026-08-17T16:16:24.002443Z","submitted_at":"2024-12-17T13:31:15Z","title":"DESI and SNe: Dynamical Dark Energy, $\\Omega_m$ Tension or Systematics?","version":2},"reference_index":9,"source":"pdf_text","source_observed_at":"2026-08-11T13:41:23.598825Z"},"links":{"cited_paper":"/paper/2004.14499","citing_paper":"/paper/2412.12905"},"observation_digest":"sha256:aefb6523555f9828910c88a025cfff2314a2fd525fe316f283a242eaed83eb82","observation_id":"99718dc6-d2ae-4fd9-add1-9ed0599e7585","resolution":{"observed_at":"2026-08-11T13:41:23.598825Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"1303.1808","last_updated":"2013-03-07T20:42:16Z","snapshot_observed_at":"2026-08-15T00:26:11.778691Z","submitted_at":"2013-03-07T20:42:16Z","title":"CFHTLenS tomographic weak lensing cosmological parameter constraints: Mitigating the impact of intrinsic galaxy alignments","version":1},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"1303.1808","snapshot_observed_at":"2026-08-11T13:41:23.602725Z","title":"Heymans et al","venue":null,"work_id":null,"year":2013},"citing_paper":{"arxiv_id":"2412.12905","last_updated":"2025-01-25T08:30:04Z","snapshot_observed_at":"2026-08-17T16:16:24.002443Z","submitted_at":"2024-12-17T13:31:15Z","title":"DESI and SNe: Dynamical Dark Energy, $\\Omega_m$ Tension or Systematics?","version":2},"reference_index":10,"source":"pdf_text","source_observed_at":"2026-08-11T13:41:23.602725Z"},"links":{"cited_paper":"/paper/1303.1808","citing_paper":"/paper/2412.12905"},"observation_digest":"sha256:64eeb85001a3e8dfc4aa206cb1ae0a4e4e8ae55b54120b291edbaac208840967","observation_id":"3269fa9f-4e40-4fa5-b2f3-ea792de19068","resolution":{"observed_at":"2026-08-11T13:41:23.602725Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"1601.05786","last_updated":"2016-11-19T04:08:52Z","snapshot_observed_at":"2026-08-14T22:13:38.457952Z","submitted_at":"2016-01-21T20:57:10Z","title":"CFHTLenS revisited: assessing concordance with Planck including astrophysical systematics","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"1601.05786","snapshot_observed_at":"2026-08-11T13:41:23.607059Z","title":"Joudaki et al","venue":null,"work_id":null,"year":2017},"citing_paper":{"arxiv_id":"2412.12905","last_updated":"2025-01-25T08:30:04Z","snapshot_observed_at":"2026-08-17T16:16:24.002443Z","submitted_at":"2024-12-17T13:31:15Z","title":"DESI and SNe: Dynamical Dark Energy, $\\Omega_m$ Tension or Systematics?","version":2},"reference_index":11,"source":"pdf_text","source_observed_at":"2026-08-11T13:41:23.607059Z"},"links":{"cited_paper":"/paper/1601.05786","citing_paper":"/paper/2412.12905"},"observation_digest":"sha256:bb6c433ff357dd52cbcab27a2fae8b7f3aaa3c98e2ce1a650c21f51910fadf48","observation_id":"536dc58f-bd0e-4850-b39e-8f58628aaa3a","resolution":{"observed_at":"2026-08-11T13:41:23.607059Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"1708.01538","last_updated":"2018-04-30T14:41:56Z","snapshot_observed_at":"2026-08-15T00:59:44.277888Z","submitted_at":"2017-08-04T14:52:35Z","title":"Dark Energy Survey Year 1 Results: Cosmological Constraints from Cosmic Shear","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"1708.01538","snapshot_observed_at":"2026-08-11T13:41:23.611663Z","title":null,"venue":null,"work_id":null,"year":2018},"citing_paper":{"arxiv_id":"2412.12905","last_updated":"2025-01-25T08:30:04Z","snapshot_observed_at":"2026-08-17T16:16:24.002443Z","submitted_at":"2024-12-17T13:31:15Z","title":"DESI and SNe: Dynamical Dark Energy, $\\Omega_m$ Tension or Systematics?","version":2},"reference_index":12,"source":"pdf_text","source_observed_at":"2026-08-11T13:41:23.611663Z"},"links":{"cited_paper":"/paper/1708.01538","citing_paper":"/paper/2412.12905"},"observation_digest":"sha256:b356489d490269b0bcf296adf698eb17ffb4ac9c886b941bb0c08e89b2ff2eca","observation_id":"7238fd11-1e43-4721-9650-61b5f556dbc7","resolution":{"observed_at":"2026-08-11T13:41:23.611663Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"1809.09148","last_updated":"2019-01-27T01:32:21Z","snapshot_observed_at":"2026-08-20T03:44:34.256618Z","submitted_at":"2018-09-24T18:22:04Z","title":"Cosmology from cosmic shear power spectra with Subaru Hyper Suprime-Cam first-year data","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"1809.09148","snapshot_observed_at":"2026-08-11T13:41:23.615610Z","title":"Hikage et al","venue":null,"work_id":null,"year":2019},"citing_paper":{"arxiv_id":"2412.12905","last_updated":"2025-01-25T08:30:04Z","snapshot_observed_at":"2026-08-17T16:16:24.002443Z","submitted_at":"2024-12-17T13:31:15Z","title":"DESI and SNe: Dynamical Dark Energy, $\\Omega_m$ Tension or Systematics?","version":2},"reference_index":13,"source":"pdf_text","source_observed_at":"2026-08-11T13:41:23.615610Z"},"links":{"cited_paper":"/paper/1809.09148","citing_paper":"/paper/2412.12905"},"observation_digest":"sha256:13a5cb9f651a756e04fbb84933aa138b5dde054011fdd1b9bcd1fa14b881a566","observation_id":"c8916fde-5524-475f-8ae1-38234d6dc48d","resolution":{"observed_at":"2026-08-11T13:41:23.615610Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2007.15633","last_updated":"2020-10-13T16:23:19Z","snapshot_observed_at":"2026-08-18T07:43:05.270334Z","submitted_at":"2020-07-30T17:54:56Z","title":"KiDS-1000 Cosmology: Cosmic shear constraints and comparison between two point statistics","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2007.15633","snapshot_observed_at":"2026-08-11T13:41:23.619419Z","title":"Asgari et al","venue":null,"work_id":null,"year":2021},"citing_paper":{"arxiv_id":"2412.12905","last_updated":"2025-01-25T08:30:04Z","snapshot_observed_at":"2026-08-17T16:16:24.002443Z","submitted_at":"2024-12-17T13:31:15Z","title":"DESI and SNe: Dynamical Dark Energy, $\\Omega_m$ Tension or Systematics?","version":2},"reference_index":14,"source":"pdf_text","source_observed_at":"2026-08-11T13:41:23.619419Z"},"links":{"cited_paper":"/paper/2007.15633","citing_paper":"/paper/2412.12905"},"observation_digest":"sha256:34eb9b8a6f8186fb6ee511b080444dc611e49254459017a686e385b8103a3742","observation_id":"5aa4dcd4-df7c-4bef-a338-2c2efd5c4c20","resolution":{"observed_at":"2026-08-11T13:41:23.619419Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2105.13549","last_updated":"2022-03-21T13:57:33Z","snapshot_observed_at":"2026-08-14T23:39:27.638377Z","submitted_at":"2021-05-28T01:58:58Z","title":"Dark Energy Survey Year 3 Results: Cosmological Constraints from Galaxy Clustering and Weak Lensing","version":3},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2105.13549","snapshot_observed_at":"2026-08-11T13:41:23.623372Z","title":null,"venue":null,"work_id":null,"year":2022},"citing_paper":{"arxiv_id":"2412.12905","last_updated":"2025-01-25T08:30:04Z","snapshot_observed_at":"2026-08-17T16:16:24.002443Z","submitted_at":"2024-12-17T13:31:15Z","title":"DESI and SNe: Dynamical Dark Energy, $\\Omega_m$ Tension or Systematics?","version":2},"reference_index":15,"source":"pdf_text","source_observed_at":"2026-08-11T13:41:23.623372Z"},"links":{"cited_paper":"/paper/2105.13549","citing_paper":"/paper/2412.12905"},"observation_digest":"sha256:dd6d28c2658b1c062821bbc78c745b9c63bd3aecbf35de5737f4f0abfa098298","observation_id":"6602d4a5-5565-49ac-bbc4-b569de3383e2","resolution":{"observed_at":"2026-08-11T13:41:23.623372Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"1907.04869","last_updated":"2019-11-06T02:34:45Z","snapshot_observed_at":"2026-08-18T20:27:14.996643Z","submitted_at":"2019-07-10T18:00:07Z","title":"H0LiCOW XIII. A 2.4% measurement of $H_{0}$ from lensed quasars: $5.3\\sigma$ tension between early and late-Universe probes","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"1907.04869","snapshot_observed_at":"2026-08-11T13:41:23.627487Z","title":null,"venue":null,"work_id":null,"year":2020},"citing_paper":{"arxiv_id":"2412.12905","last_updated":"2025-01-25T08:30:04Z","snapshot_observed_at":"2026-08-17T16:16:24.002443Z","submitted_at":"2024-12-17T13:31:15Z","title":"DESI and SNe: Dynamical Dark Energy, $\\Omega_m$ Tension or Systematics?","version":2},"reference_index":16,"source":"pdf_text","source_observed_at":"2026-08-11T13:41:23.627487Z"},"links":{"cited_paper":"/paper/1907.04869","citing_paper":"/paper/2412.12905"},"observation_digest":"sha256:a719b567bd71adcd48bb96a5bf877be403b8fe562fa63377ca62dd05604b0f66","observation_id":"331e37a2-de33-4f88-8df7-c7f3e317f158","resolution":{"observed_at":"2026-08-11T13:41:23.627487Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"1912.08027","last_updated":"2020-07-22T09:28:58Z","snapshot_observed_at":"2026-08-18T20:27:17.194651Z","submitted_at":"2019-12-17T14:15:19Z","title":"TDCOSMO. I. An exploration of systematic uncertainties in the inference of $H_0$ from time-delay cosmography","version":3},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"1912.08027","snapshot_observed_at":"2026-08-11T13:41:23.631216Z","title":"Millon et al","venue":null,"work_id":null,"year":2020},"citing_paper":{"arxiv_id":"2412.12905","last_updated":"2025-01-25T08:30:04Z","snapshot_observed_at":"2026-08-17T16:16:24.002443Z","submitted_at":"2024-12-17T13:31:15Z","title":"DESI and SNe: Dynamical Dark Energy, $\\Omega_m$ Tension or Systematics?","version":2},"reference_index":17,"source":"pdf_text","source_observed_at":"2026-08-11T13:41:23.631216Z"},"links":{"cited_paper":"/paper/1912.08027","citing_paper":"/paper/2412.12905"},"observation_digest":"sha256:90e9cbcd187af598423465f58349e8b5b67f071a3f1f7525c0c169b696a6fcba","observation_id":"d00ff5fb-1cd2-43b3-a65f-62e3a7e4040d","resolution":{"observed_at":"2026-08-11T13:41:23.631216Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2002.06044","last_updated":"2020-10-22T01:05:32Z","snapshot_observed_at":"2026-08-12T04:59:29.138588Z","submitted_at":"2020-02-14T14:15:26Z","title":"Is there an early Universe solution to Hubble tension?","version":3},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2002.06044","snapshot_observed_at":"2026-08-11T13:41:23.635044Z","title":"Krishnan, E","venue":null,"work_id":null,"year":2020},"citing_paper":{"arxiv_id":"2412.12905","last_updated":"2025-01-25T08:30:04Z","snapshot_observed_at":"2026-08-17T16:16:24.002443Z","submitted_at":"2024-12-17T13:31:15Z","title":"DESI and SNe: Dynamical Dark Energy, $\\Omega_m$ Tension or Systematics?","version":2},"reference_index":18,"source":"pdf_text","source_observed_at":"2026-08-11T13:41:23.635044Z"},"links":{"cited_paper":"/paper/2002.06044","citing_paper":"/paper/2412.12905"},"observation_digest":"sha256:5a067231eccf27db7bac1b17e12e613ea6cf9180d8ac5c96cf87988007a560c5","observation_id":"6d91820b-5af5-499c-829d-de411f4d7c09","resolution":{"observed_at":"2026-08-11T13:41:23.635044Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2011.02858","last_updated":"2021-05-12T14:44:16Z","snapshot_observed_at":"2026-08-16T19:08:11.630017Z","submitted_at":"2020-11-04T11:21:03Z","title":"Running Hubble Tension and a H0 Diagnostic","version":3},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2011.02858","snapshot_observed_at":"2026-08-11T13:41:23.642186Z","title":"Krishnan, E","venue":null,"work_id":null,"year":2021},"citing_paper":{"arxiv_id":"2412.12905","last_updated":"2025-01-25T08:30:04Z","snapshot_observed_at":"2026-08-17T16:16:24.002443Z","submitted_at":"2024-12-17T13:31:15Z","title":"DESI and SNe: Dynamical Dark Energy, $\\Omega_m$ Tension or Systematics?","version":2},"reference_index":19,"source":"pdf_text","source_observed_at":"2026-08-11T13:41:23.642186Z"},"links":{"cited_paper":"/paper/2011.02858","citing_paper":"/paper/2412.12905"},"observation_digest":"sha256:bab1d2165c180fb2b4e47c59717bace858330704029d04b119cf422916cb2655","observation_id":"b6b0f4ca-8e4f-40bf-9173-861069b5d539","resolution":{"observed_at":"2026-08-11T13:41:23.642186Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2103.02117","last_updated":"2021-05-20T20:48:20Z","snapshot_observed_at":"2026-08-17T16:05:34.468431Z","submitted_at":"2021-03-03T01:22:00Z","title":"On the Hubble constant tension in the SNe Ia Pantheon sample","version":4},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2103.02117","snapshot_observed_at":"2026-08-11T13:41:23.647752Z","title":null,"venue":null,"work_id":null,"year":2021},"citing_paper":{"arxiv_id":"2412.12905","last_updated":"2025-01-25T08:30:04Z","snapshot_observed_at":"2026-08-17T16:16:24.002443Z","submitted_at":"2024-12-17T13:31:15Z","title":"DESI and SNe: Dynamical Dark Energy, $\\Omega_m$ Tension or Systematics?","version":2},"reference_index":20,"source":"pdf_text","source_observed_at":"2026-08-11T13:41:23.647752Z"},"links":{"cited_paper":"/paper/2103.02117","citing_paper":"/paper/2412.12905"},"observation_digest":"sha256:420355b462fd939f4271bb10c0aae5ec890e8a98b7360416446c9fbbb9c8def2","observation_id":"a705abd6-a3cc-49c1-ba16-cda1fa153461","resolution":{"observed_at":"2026-08-11T13:41:23.647752Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2201.09848","last_updated":"2022-01-29T19:35:40Z","snapshot_observed_at":"2026-08-19T20:56:28.673255Z","submitted_at":"2022-01-24T18:12:00Z","title":"On the evolution of the Hubble constant with the SNe Ia Pantheon Sample and Baryon Acoustic Oscillations: a feasibility study for GRB-cosmology in 2030","version":3},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2201.09848","snapshot_observed_at":"2026-08-11T13:41:23.651476Z","title":null,"venue":null,"work_id":null,"year":2022},"citing_paper":{"arxiv_id":"2412.12905","last_updated":"2025-01-25T08:30:04Z","snapshot_observed_at":"2026-08-17T16:16:24.002443Z","submitted_at":"2024-12-17T13:31:15Z","title":"DESI and SNe: Dynamical Dark Energy, $\\Omega_m$ Tension or Systematics?","version":2},"reference_index":21,"source":"pdf_text","source_observed_at":"2026-08-11T13:41:23.651476Z"},"links":{"cited_paper":"/paper/2201.09848","citing_paper":"/paper/2412.12905"},"observation_digest":"sha256:d279bf279384b644a68594bba7e485d5951c76e1f48afead111de4f06a17ff9c","observation_id":"d7c2db04-91b9-4368-a13c-837a563e65de","resolution":{"observed_at":"2026-08-11T13:41:23.651476Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2203.13037","last_updated":"2022-09-23T10:57:55Z","snapshot_observed_at":"2026-08-16T17:12:05.758274Z","submitted_at":"2022-03-24T12:32:13Z","title":"Revealing the late-time transition of $H_{0}$: relieve the Hubble crisis","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2203.13037","snapshot_observed_at":"2026-08-11T13:41:23.655284Z","title":"Hu and F","venue":null,"work_id":null,"year":2022},"citing_paper":{"arxiv_id":"2412.12905","last_updated":"2025-01-25T08:30:04Z","snapshot_observed_at":"2026-08-17T16:16:24.002443Z","submitted_at":"2024-12-17T13:31:15Z","title":"DESI and SNe: Dynamical Dark Energy, $\\Omega_m$ Tension or Systematics?","version":2},"reference_index":22,"source":"pdf_text","source_observed_at":"2026-08-11T13:41:23.655284Z"},"links":{"cited_paper":"/paper/2203.13037","citing_paper":"/paper/2412.12905"},"observation_digest":"sha256:e30375d86a943a253fe23d8aaaf7947100c17f1f11d765b6671c7b8dc5922823","observation_id":"605b3b10-5c5d-4fb6-9874-8ff852b9034f","resolution":{"observed_at":"2026-08-11T13:41:23.655284Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2203.10558","last_updated":"2022-08-08T13:32:14Z","snapshot_observed_at":"2026-08-16T17:13:12.624742Z","submitted_at":"2022-03-20T14:12:45Z","title":"Revealing Intrinsic Flat $\\Lambda$CDM Biases with Standardizable Candles","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2203.10558","snapshot_observed_at":"2026-08-11T13:41:23.658951Z","title":"´O Colg ´ain, M","venue":null,"work_id":null,"year":2022},"citing_paper":{"arxiv_id":"2412.12905","last_updated":"2025-01-25T08:30:04Z","snapshot_observed_at":"2026-08-17T16:16:24.002443Z","submitted_at":"2024-12-17T13:31:15Z","title":"DESI and SNe: Dynamical Dark Energy, $\\Omega_m$ Tension or Systematics?","version":2},"reference_index":23,"source":"pdf_text","source_observed_at":"2026-08-11T13:41:23.658951Z"},"links":{"cited_paper":"/paper/2203.10558","citing_paper":"/paper/2412.12905"},"observation_digest":"sha256:b0a305e55aa45ac3d3d8516da3a67afc659cb2f724d46d7182fd0ab524e9350e","observation_id":"48dbd911-d0a8-4b02-a77d-aed7c66ef382","resolution":{"observed_at":"2026-08-11T13:41:23.658951Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2206.11447","last_updated":"2024-03-16T14:09:54Z","snapshot_observed_at":"2026-08-17T11:06:51.778933Z","submitted_at":"2022-06-23T01:40:10Z","title":"Putting Flat $\\Lambda$CDM In The (Redshift) Bin","version":3},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2206.11447","snapshot_observed_at":"2026-08-11T13:41:23.663237Z","title":"´O Colg´ain, M","venue":null,"work_id":null,"year":2024},"citing_paper":{"arxiv_id":"2412.12905","last_updated":"2025-01-25T08:30:04Z","snapshot_observed_at":"2026-08-17T16:16:24.002443Z","submitted_at":"2024-12-17T13:31:15Z","title":"DESI and SNe: Dynamical Dark Energy, $\\Omega_m$ Tension or Systematics?","version":2},"reference_index":24,"source":"pdf_text","source_observed_at":"2026-08-11T13:41:23.663237Z"},"links":{"cited_paper":"/paper/2206.11447","citing_paper":"/paper/2412.12905"},"observation_digest":"sha256:c649daffbadfb8d2ea650a7fcdf99051664c8a1861074ad0d6ba4f2ee10ac087","observation_id":"2d090643-657c-4933-9268-ab97db89d01c","resolution":{"observed_at":"2026-08-11T13:41:23.663237Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2212.00238","last_updated":"2023-04-14T11:46:36Z","snapshot_observed_at":"2026-08-16T16:11:53.167768Z","submitted_at":"2022-12-01T03:05:24Z","title":"Evidence of a decreasing trend for the Hubble constant","version":3},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2212.00238","snapshot_observed_at":"2026-08-11T13:41:23.667015Z","title":null,"venue":null,"work_id":null,"year":2023},"citing_paper":{"arxiv_id":"2412.12905","last_updated":"2025-01-25T08:30:04Z","snapshot_observed_at":"2026-08-17T16:16:24.002443Z","submitted_at":"2024-12-17T13:31:15Z","title":"DESI and SNe: Dynamical Dark Energy, $\\Omega_m$ Tension or Systematics?","version":2},"reference_index":25,"source":"pdf_text","source_observed_at":"2026-08-11T13:41:23.667015Z"},"links":{"cited_paper":"/paper/2212.00238","citing_paper":"/paper/2412.12905"},"observation_digest":"sha256:2c890cbf1b0cec54b50f1bb261f347ffb93b42328694f1d69a63ec33c7782c38","observation_id":"497fdefc-4816-4ddd-8996-9df1f6372639","resolution":{"observed_at":"2026-08-11T13:41:23.667015Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2406.02019","last_updated":"2025-01-15T10:57:02Z","snapshot_observed_at":"2026-08-16T13:46:25.637968Z","submitted_at":"2024-06-04T06:58:58Z","title":"Uncorrelated estimations of $H_0$ redshift evolution from DESI baryon acoustic oscillation observations","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2406.02019","snapshot_observed_at":"2026-08-11T13:41:23.670763Z","title":null,"venue":null,"work_id":null,"year":2024},"citing_paper":{"arxiv_id":"2412.12905","last_updated":"2025-01-25T08:30:04Z","snapshot_observed_at":"2026-08-17T16:16:24.002443Z","submitted_at":"2024-12-17T13:31:15Z","title":"DESI and SNe: Dynamical Dark Energy, $\\Omega_m$ Tension or Systematics?","version":2},"reference_index":26,"source":"pdf_text","source_observed_at":"2026-08-11T13:41:23.670763Z"},"links":{"cited_paper":"/paper/2406.02019","citing_paper":"/paper/2412.12905"},"observation_digest":"sha256:e1052c5cff2cf376b957dda8bfbdbf66b30c3b9adc0c4f73f3f04440733dcaec","observation_id":"45d8451e-cf7c-4503-be59-c841858cd103","resolution":{"observed_at":"2026-08-11T13:41:23.670763Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"1811.02590","last_updated":"2018-11-06T19:00:49Z","snapshot_observed_at":"2026-08-19T20:46:40.246878Z","submitted_at":"2018-11-06T19:00:49Z","title":"Cosmological constraints from the Hubble diagram of quasars at high redshifts","version":1},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"1811.02590","snapshot_observed_at":"2026-08-11T13:41:23.674333Z","title":"Risaliti and E","venue":null,"work_id":null,"year":2019},"citing_paper":{"arxiv_id":"2412.12905","last_updated":"2025-01-25T08:30:04Z","snapshot_observed_at":"2026-08-17T16:16:24.002443Z","submitted_at":"2024-12-17T13:31:15Z","title":"DESI and SNe: Dynamical Dark Energy, $\\Omega_m$ Tension or Systematics?","version":2},"reference_index":27,"source":"pdf_text","source_observed_at":"2026-08-11T13:41:23.674333Z"},"links":{"cited_paper":"/paper/1811.02590","citing_paper":"/paper/2412.12905"},"observation_digest":"sha256:2fb4250b39b0d8409b5292253cb1885d56337955361c6cf18c940af237ca990e","observation_id":"a1737a49-b12f-41a4-9107-571a99bd3dba","resolution":{"observed_at":"2026-08-11T13:41:23.674333Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2008.08586","last_updated":"2020-08-19T18:00:01Z","snapshot_observed_at":"2026-08-18T22:25:44.838097Z","submitted_at":"2020-08-19T18:00:01Z","title":"Quasars as standard candles III. Validation of a new sample for cosmological studies","version":1},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2008.08586","snapshot_observed_at":"2026-08-11T13:41:23.678186Z","title":"Lusso et al","venue":null,"work_id":null,"year":2020},"citing_paper":{"arxiv_id":"2412.12905","last_updated":"2025-01-25T08:30:04Z","snapshot_observed_at":"2026-08-17T16:16:24.002443Z","submitted_at":"2024-12-17T13:31:15Z","title":"DESI and SNe: Dynamical Dark Energy, $\\Omega_m$ Tension or Systematics?","version":2},"reference_index":28,"source":"pdf_text","source_observed_at":"2026-08-11T13:41:23.678186Z"},"links":{"cited_paper":"/paper/2008.08586","citing_paper":"/paper/2412.12905"},"observation_digest":"sha256:c6df069f1d6458e8dc1b5dab582f04bdf68a3c0ade31c0fda1e9c9d143279981","observation_id":"a2e74529-f9d5-48f7-a2ae-a03a59c8a12c","resolution":{"observed_at":"2026-08-11T13:41:23.678186Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2212.04118","last_updated":"2022-12-08T07:28:03Z","snapshot_observed_at":"2026-08-16T16:10:07.715750Z","submitted_at":"2022-12-08T07:28:03Z","title":"Can high-redshift Hubble diagrams rule out the standard model of cosmology in the context of cosmographic method?","version":1},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2212.04118","snapshot_observed_at":"2026-08-11T13:41:23.681692Z","title":"Pourojaghi, N","venue":null,"work_id":null,"year":2022},"citing_paper":{"arxiv_id":"2412.12905","last_updated":"2025-01-25T08:30:04Z","snapshot_observed_at":"2026-08-17T16:16:24.002443Z","submitted_at":"2024-12-17T13:31:15Z","title":"DESI and SNe: Dynamical Dark Energy, $\\Omega_m$ Tension or Systematics?","version":2},"reference_index":29,"source":"pdf_text","source_observed_at":"2026-08-11T13:41:23.681692Z"},"links":{"cited_paper":"/paper/2212.04118","citing_paper":"/paper/2412.12905"},"observation_digest":"sha256:2c071927087676d51390ebf5f006ca190bc13f11e95749cc39188125745b3d72","observation_id":"47cc54ea-e78b-4f3d-b783-a532f40aa394","resolution":{"observed_at":"2026-08-11T13:41:23.681692Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2301.10740","last_updated":"2023-04-18T19:23:21Z","snapshot_observed_at":"2026-08-16T16:00:09.948974Z","submitted_at":"2023-01-25T18:03:52Z","title":"Testing $\\Lambda$CDM cosmology in a binned universe: anomalies in the deceleration parameter","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2301.10740","snapshot_observed_at":"2026-08-11T13:41:23.685615Z","title":"Past ´en and V","venue":null,"work_id":null,"year":2023},"citing_paper":{"arxiv_id":"2412.12905","last_updated":"2025-01-25T08:30:04Z","snapshot_observed_at":"2026-08-17T16:16:24.002443Z","submitted_at":"2024-12-17T13:31:15Z","title":"DESI and SNe: Dynamical Dark Energy, $\\Omega_m$ Tension or Systematics?","version":2},"reference_index":30,"source":"pdf_text","source_observed_at":"2026-08-11T13:41:23.685615Z"},"links":{"cited_paper":"/paper/2301.10740","citing_paper":"/paper/2412.12905"},"observation_digest":"sha256:e151978f99eabb57d6a63463743ff3ea2596cff5de801d2492a058bb104b0dab","observation_id":"2248d2c2-b981-4b40-9b29-5e84ef9505d8","resolution":{"observed_at":"2026-08-11T13:41:23.685615Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2401.14170","last_updated":"2024-10-23T12:27:52Z","snapshot_observed_at":"2026-08-16T14:24:33.882105Z","submitted_at":"2024-01-25T13:28:20Z","title":"No-go guide for the Hubble tension: late-time or local-scale new physics","version":3},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2401.14170","snapshot_observed_at":"2026-08-11T13:41:23.689464Z","title":"Huang, S.-J","venue":null,"work_id":null,"year":2025},"citing_paper":{"arxiv_id":"2412.12905","last_updated":"2025-01-25T08:30:04Z","snapshot_observed_at":"2026-08-17T16:16:24.002443Z","submitted_at":"2024-12-17T13:31:15Z","title":"DESI and SNe: Dynamical Dark Energy, $\\Omega_m$ Tension or Systematics?","version":2},"reference_index":31,"source":"pdf_text","source_observed_at":"2026-08-11T13:41:23.689464Z"},"links":{"cited_paper":"/paper/2401.14170","citing_paper":"/paper/2412.12905"},"observation_digest":"sha256:dc5ff38105f372c35c48b4dd3fad348d0844264e5d8b29926df779b358fb8d4e","observation_id":"56eb58d6-4843-4588-8274-7f73b114d6f6","resolution":{"observed_at":"2026-08-11T13:41:23.689464Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2405.19953","last_updated":"2025-05-30T15:38:15Z","snapshot_observed_at":"2026-08-16T13:47:48.369247Z","submitted_at":"2024-05-30T11:18:17Z","title":"Do high redshift QSOs and GRBs corroborate JWST?","version":3},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2405.19953","snapshot_observed_at":"2026-08-11T13:41:23.693241Z","title":"´O Colg ´ain, M","venue":null,"work_id":null,"year":2024},"citing_paper":{"arxiv_id":"2412.12905","last_updated":"2025-01-25T08:30:04Z","snapshot_observed_at":"2026-08-17T16:16:24.002443Z","submitted_at":"2024-12-17T13:31:15Z","title":"DESI and SNe: Dynamical Dark Energy, $\\Omega_m$ Tension or Systematics?","version":2},"reference_index":32,"source":"pdf_text","source_observed_at":"2026-08-11T13:41:23.693241Z"},"links":{"cited_paper":"/paper/2405.19953","citing_paper":"/paper/2412.12905"},"observation_digest":"sha256:f686d00a4e6fe185ed183392a11c35541d3dcca5054c9ae1666f86cbbdee0d45","observation_id":"e26268e6-0616-45ec-9d1b-72757382205b","resolution":{"observed_at":"2026-08-11T13:41:23.693241Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2410.06053","last_updated":"2025-03-05T13:28:04Z","snapshot_observed_at":"2026-08-19T00:44:57.640248Z","submitted_at":"2024-10-08T13:55:27Z","title":"Narrowing down the Hubble tension to the first two rungs of distance ladders","version":3},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2410.06053","snapshot_observed_at":"2026-08-11T13:41:23.697699Z","title":"Huang, R.-G","venue":null,"work_id":null,"year":2024},"citing_paper":{"arxiv_id":"2412.12905","last_updated":"2025-01-25T08:30:04Z","snapshot_observed_at":"2026-08-17T16:16:24.002443Z","submitted_at":"2024-12-17T13:31:15Z","title":"DESI and SNe: Dynamical Dark Energy, $\\Omega_m$ Tension or Systematics?","version":2},"reference_index":33,"source":"pdf_text","source_observed_at":"2026-08-11T13:41:23.697699Z"},"links":{"cited_paper":"/paper/2410.06053","citing_paper":"/paper/2412.12905"},"observation_digest":"sha256:6c35ef25d3a0dde1a133b0740d487b0cc00d70bde954b6991caae92d293f2d96","observation_id":"c888a2ef-dd5f-4e6d-b081-1a5d1edabb25","resolution":{"observed_at":"2026-08-11T13:41:23.697699Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2111.09898","last_updated":"2022-01-18T17:06:45Z","snapshot_observed_at":"2026-08-16T17:40:49.848522Z","submitted_at":"2021-11-18T19:00:09Z","title":"Cosmological constraints from the tomographic cross-correlation of DESI Luminous Red Galaxies and Planck CMB lensing","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2111.09898","snapshot_observed_at":"2026-08-11T13:41:23.701523Z","title":"White et al","venue":null,"work_id":null,"year":2022},"citing_paper":{"arxiv_id":"2412.12905","last_updated":"2025-01-25T08:30:04Z","snapshot_observed_at":"2026-08-17T16:16:24.002443Z","submitted_at":"2024-12-17T13:31:15Z","title":"DESI and SNe: Dynamical Dark Energy, $\\Omega_m$ Tension or Systematics?","version":2},"reference_index":34,"source":"pdf_text","source_observed_at":"2026-08-11T13:41:23.701523Z"},"links":{"cited_paper":"/paper/2111.09898","citing_paper":"/paper/2412.12905"},"observation_digest":"sha256:c853c45433c42b0726485f8239a1f0091911e67b00ae2784158ccab7fea5725c","observation_id":"3c1b6491-11f8-4884-aead-8065246d51d4","resolution":{"observed_at":"2026-08-11T13:41:23.701523Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2105.12108","last_updated":"2021-09-09T09:23:46Z","snapshot_observed_at":"2026-08-20T02:03:56.569953Z","submitted_at":"2021-05-25T17:44:50Z","title":"The growth of density perturbations in the last $\\sim$10 billion years from tomographic large-scale structure data","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2105.12108","snapshot_observed_at":"2026-08-11T13:41:23.705201Z","title":"Garc ´ıa-Garc´ıa, J","venue":null,"work_id":null,"year":2021},"citing_paper":{"arxiv_id":"2412.12905","last_updated":"2025-01-25T08:30:04Z","snapshot_observed_at":"2026-08-17T16:16:24.002443Z","submitted_at":"2024-12-17T13:31:15Z","title":"DESI and SNe: Dynamical Dark Energy, $\\Omega_m$ Tension or Systematics?","version":2},"reference_index":35,"source":"pdf_text","source_observed_at":"2026-08-11T13:41:23.705201Z"},"links":{"cited_paper":"/paper/2105.12108","citing_paper":"/paper/2412.12905"},"observation_digest":"sha256:42b3b88d7ee27612b909380cf61e8acc351abc02e7bdc1e5ab6f3ba2f87a9eee","observation_id":"e263c487-26b7-4151-b9a1-8e3138c83695","resolution":{"observed_at":"2026-08-11T13:41:23.705201Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2202.00974","last_updated":"2022-06-28T08:55:51Z","snapshot_observed_at":"2026-08-16T17:24:09.809288Z","submitted_at":"2022-02-02T11:38:01Z","title":"Weighing Cosmic Structures with Clusters of Galaxies and the Intergalactic Medium","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2202.00974","snapshot_observed_at":"2026-08-11T13:41:23.708856Z","title":"Esposito, V","venue":null,"work_id":null,"year":2022},"citing_paper":{"arxiv_id":"2412.12905","last_updated":"2025-01-25T08:30:04Z","snapshot_observed_at":"2026-08-17T16:16:24.002443Z","submitted_at":"2024-12-17T13:31:15Z","title":"DESI and SNe: Dynamical Dark Energy, $\\Omega_m$ Tension or Systematics?","version":2},"reference_index":36,"source":"pdf_text","source_observed_at":"2026-08-11T13:41:23.708856Z"},"links":{"cited_paper":"/paper/2202.00974","citing_paper":"/paper/2412.12905"},"observation_digest":"sha256:5be859215c73c3a3d277354d9a7f66ae773cac890e51c53cb3f60bee27157d79","observation_id":"e1ca4d36-e867-4e4a-95cc-b767cb4f77f8","resolution":{"observed_at":"2026-08-11T13:41:23.708856Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"1811.07812","last_updated":"2019-01-29T14:31:24Z","snapshot_observed_at":"2026-08-16T18:40:37.090848Z","submitted_at":"2018-11-19T17:16:34Z","title":"More out of less: an excess integrated Sachs-Wolfe signal from supervoids mapped out by the Dark Energy Survey","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"1811.07812","snapshot_observed_at":"2026-08-11T13:41:23.712636Z","title":"Kov ´acs et al","venue":null,"work_id":null,"year":2019},"citing_paper":{"arxiv_id":"2412.12905","last_updated":"2025-01-25T08:30:04Z","snapshot_observed_at":"2026-08-17T16:16:24.002443Z","submitted_at":"2024-12-17T13:31:15Z","title":"DESI and SNe: Dynamical Dark Energy, $\\Omega_m$ Tension or Systematics?","version":2},"reference_index":37,"source":"pdf_text","source_observed_at":"2026-08-11T13:41:23.712636Z"},"links":{"cited_paper":"/paper/1811.07812","citing_paper":"/paper/2412.12905"},"observation_digest":"sha256:8ee53d4aec148e31c97d28f0d21f595f292a1a548ee60999bc859bcab0e56597","observation_id":"3dfe817d-b739-4222-a6be-e65b1522f9e2","resolution":{"observed_at":"2026-08-11T13:41:23.712636Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2107.13038","last_updated":"2022-04-18T17:57:52Z","snapshot_observed_at":"2026-08-19T19:18:13.384750Z","submitted_at":"2021-07-27T18:41:34Z","title":"Evidence for a high-z ISW signal from supervoids in the distribution of eBOSS quasars","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2107.13038","snapshot_observed_at":"2026-08-11T13:41:23.717007Z","title":"Kov ´acs, R","venue":null,"work_id":null,"year":2022},"citing_paper":{"arxiv_id":"2412.12905","last_updated":"2025-01-25T08:30:04Z","snapshot_observed_at":"2026-08-17T16:16:24.002443Z","submitted_at":"2024-12-17T13:31:15Z","title":"DESI and SNe: Dynamical Dark Energy, $\\Omega_m$ Tension or Systematics?","version":2},"reference_index":38,"source":"pdf_text","source_observed_at":"2026-08-11T13:41:23.717007Z"},"links":{"cited_paper":"/paper/2107.13038","citing_paper":"/paper/2412.12905"},"observation_digest":"sha256:62e2db086170dd7003f8e181629402910da87a719b8354d30d9032e5b7febb9d","observation_id":"4cd94edd-6549-4dc0-99ad-fd7a0ff39f0a","resolution":{"observed_at":"2026-08-11T13:41:23.717007Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2303.06928","last_updated":"2023-11-01T18:21:45Z","snapshot_observed_at":"2026-08-16T15:48:46.662964Z","submitted_at":"2023-03-13T08:46:15Z","title":"$S_8$ increases with effective redshift in $\\Lambda$CDM cosmology","version":3},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2303.06928","snapshot_observed_at":"2026-08-11T13:41:23.721183Z","title":null,"venue":null,"work_id":null,"year":2023},"citing_paper":{"arxiv_id":"2412.12905","last_updated":"2025-01-25T08:30:04Z","snapshot_observed_at":"2026-08-17T16:16:24.002443Z","submitted_at":"2024-12-17T13:31:15Z","title":"DESI and SNe: Dynamical Dark Energy, $\\Omega_m$ Tension or Systematics?","version":2},"reference_index":39,"source":"pdf_text","source_observed_at":"2026-08-11T13:41:23.721183Z"},"links":{"cited_paper":"/paper/2303.06928","citing_paper":"/paper/2412.12905"},"observation_digest":"sha256:59221b1b4e47e7c3e4521bddb5420e7329ec0c2a2e055e5ff465ccb122fc65a1","observation_id":"591d8bb0-b357-4c77-9e6b-04224461f597","resolution":{"observed_at":"2026-08-11T13:41:23.721183Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2410.23134","last_updated":"2024-12-02T13:56:40Z","snapshot_observed_at":"2026-08-19T05:25:12.168903Z","submitted_at":"2024-10-30T15:46:52Z","title":"Further support for $S_8$ increasing with effective redshift","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2410.23134","snapshot_observed_at":"2026-08-11T13:41:23.725031Z","title":"Akarsu, E","venue":null,"work_id":null,"year":2024},"citing_paper":{"arxiv_id":"2412.12905","last_updated":"2025-01-25T08:30:04Z","snapshot_observed_at":"2026-08-17T16:16:24.002443Z","submitted_at":"2024-12-17T13:31:15Z","title":"DESI and SNe: Dynamical Dark Energy, $\\Omega_m$ Tension or Systematics?","version":2},"reference_index":40,"source":"pdf_text","source_observed_at":"2026-08-11T13:41:23.725031Z"},"links":{"cited_paper":"/paper/2410.23134","citing_paper":"/paper/2412.12905"},"observation_digest":"sha256:2fdc539f6e9cd3de0ca86d6705194e8db597080e4da5eec18bd0e922d0ff37a9","observation_id":"09feb980-43c0-47f0-9c7a-a4c2d93b8f15","resolution":{"observed_at":"2026-08-11T13:41:23.725031Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2410.09499","last_updated":"2024-10-12T11:27:32Z","snapshot_observed_at":"2026-08-18T06:53:59.292461Z","submitted_at":"2024-10-12T11:27:32Z","title":"The SRG/eROSITA All-Sky Survey : Constraints on the structure growth from cluster number counts","version":1},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2410.09499","snapshot_observed_at":"2026-08-11T13:41:23.728656Z","title":"Artis, E","venue":null,"work_id":null,"year":2024},"citing_paper":{"arxiv_id":"2412.12905","last_updated":"2025-01-25T08:30:04Z","snapshot_observed_at":"2026-08-17T16:16:24.002443Z","submitted_at":"2024-12-17T13:31:15Z","title":"DESI and SNe: Dynamical Dark Energy, $\\Omega_m$ Tension or Systematics?","version":2},"reference_index":41,"source":"pdf_text","source_observed_at":"2026-08-11T13:41:23.728656Z"},"links":{"cited_paper":"/paper/2410.09499","citing_paper":"/paper/2412.12905"},"observation_digest":"sha256:89d98aaaf8ebfd4c11de111088c96b2077889c013438c0cf584e07f16512e722","observation_id":"71fa556b-214c-4219-9294-618140d17e9e","resolution":{"observed_at":"2026-08-11T13:41:23.728656Z","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":"2026-08-11T13:41:23.546991Z","title":null,"venue":null,"work_id":null,"year":2024},"citing_paper":{"arxiv_id":"2412.12905","last_updated":"2025-01-25T08:30:04Z","snapshot_observed_at":"2026-08-17T16:16:24.002443Z","submitted_at":"2024-12-17T13:31:15Z","title":"DESI and SNe: Dynamical Dark Energy, $\\Omega_m$ Tension or Systematics?","version":2},"reference_index":42,"source":"pdf_text","source_observed_at":"2026-08-11T13:41:23.546991Z"},"links":{"citing_paper":"/paper/2412.12905"},"observation_digest":"sha256:e957cccad1ee5abe25b15ba54c1cd2142d1070f807f6f9e28a223317500aca62","observation_id":"97641485-a9c0-47b1-8826-41ee81cd666f","resolution":{"observed_at":"2026-08-11T13:41:23.546991Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2411.12022","last_updated":"2024-11-21T16:47:10Z","snapshot_observed_at":"2026-08-19T23:10:43.518700Z","submitted_at":"2024-11-18T20:03:35Z","title":"DESI 2024 VII: Cosmological Constraints from the Full-Shape Modeling of Clustering Measurements","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2411.12022","snapshot_observed_at":"2026-08-11T13:41:23.735625Z","title":null,"venue":null,"work_id":null,"year":2024},"citing_paper":{"arxiv_id":"2412.12905","last_updated":"2025-01-25T08:30:04Z","snapshot_observed_at":"2026-08-17T16:16:24.002443Z","submitted_at":"2024-12-17T13:31:15Z","title":"DESI and SNe: Dynamical Dark Energy, $\\Omega_m$ Tension or Systematics?","version":2},"reference_index":43,"source":"pdf_text","source_observed_at":"2026-08-11T13:41:23.735625Z"},"links":{"cited_paper":"/paper/2411.12022","citing_paper":"/paper/2412.12905"},"observation_digest":"sha256:3ef5adab45561f3519d65ad08826c2d9db8abdf8f67cdea5fab66029b94ac68e","observation_id":"6ab71e68-a859-48a4-a1dd-8692a72384ff","resolution":{"observed_at":"2026-08-11T13:41:23.735625Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2411.12021","last_updated":"2025-11-24T12:55:36Z","snapshot_observed_at":"2026-08-11T03:34:16.822999Z","submitted_at":"2024-11-18T20:03:34Z","title":"DESI 2024 V: Full-Shape Galaxy Clustering from Galaxies and Quasars","version":5},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2411.12021","snapshot_observed_at":"2026-08-11T13:41:23.739073Z","title":null,"venue":null,"work_id":null,"year":2024},"citing_paper":{"arxiv_id":"2412.12905","last_updated":"2025-01-25T08:30:04Z","snapshot_observed_at":"2026-08-17T16:16:24.002443Z","submitted_at":"2024-12-17T13:31:15Z","title":"DESI and SNe: Dynamical Dark Energy, $\\Omega_m$ Tension or Systematics?","version":2},"reference_index":44,"source":"pdf_text","source_observed_at":"2026-08-11T13:41:23.739073Z"},"links":{"cited_paper":"/paper/2411.12021","citing_paper":"/paper/2412.12905"},"observation_digest":"sha256:2322a66e1425a8072baa2ac2f01cc912965ed78ac2d0663f372a7bd7dc423327","observation_id":"60cfa6d7-2e23-42e7-8c25-d42b490607b9","resolution":{"observed_at":"2026-08-11T13:41:23.739073Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2312.06434","last_updated":"2025-07-11T15:52:08Z","snapshot_observed_at":"2026-08-17T18:40:33.344184Z","submitted_at":"2023-12-11T14:59:25Z","title":"Measurement of the Weyl potential evolution from the first three years of Dark Energy Survey data","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2312.06434","snapshot_observed_at":"2026-08-11T13:41:23.743415Z","title":"Tutusaus, C","venue":null,"work_id":null,"year":2023},"citing_paper":{"arxiv_id":"2412.12905","last_updated":"2025-01-25T08:30:04Z","snapshot_observed_at":"2026-08-17T16:16:24.002443Z","submitted_at":"2024-12-17T13:31:15Z","title":"DESI and SNe: Dynamical Dark Energy, $\\Omega_m$ Tension or Systematics?","version":2},"reference_index":45,"source":"pdf_text","source_observed_at":"2026-08-11T13:41:23.743415Z"},"links":{"cited_paper":"/paper/2312.06434","citing_paper":"/paper/2412.12905"},"observation_digest":"sha256:1f6f59cf0e7fdde834ad55e3a3706c649783788a8260451fc695c297e63e3271","observation_id":"bf996a66-ab16-4308-ac02-c4ca98d6b156","resolution":{"observed_at":"2026-08-11T13:41:23.743415Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2410.10808","last_updated":"2024-10-14T17:59:25Z","snapshot_observed_at":"2026-08-16T13:09:29.189838Z","submitted_at":"2024-10-14T17:59:25Z","title":"The Atacama Cosmology Telescope DR6 and DESI: Structure growth measurements from the cross-correlation of DESI Legacy Imaging galaxies and CMB lensing from ACT DR6 and Planck PR4","version":1},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2410.10808","snapshot_observed_at":"2026-08-11T13:41:23.732161Z","title":null,"venue":null,"work_id":null,"year":2024},"citing_paper":{"arxiv_id":"2412.12905","last_updated":"2025-01-25T08:30:04Z","snapshot_observed_at":"2026-08-17T16:16:24.002443Z","submitted_at":"2024-12-17T13:31:15Z","title":"DESI and SNe: Dynamical Dark Energy, $\\Omega_m$ Tension or Systematics?","version":2},"reference_index":46,"source":"pdf_text","source_observed_at":"2026-08-11T13:41:23.732161Z"},"links":{"cited_paper":"/paper/2410.10808","citing_paper":"/paper/2412.12905"},"observation_digest":"sha256:8f61eb291036793cd08a195f8a109902db58a369341a19a2310b2974b370e9b8","observation_id":"0c6d107a-371a-439f-827e-3e48b3b920ba","resolution":{"observed_at":"2026-08-11T13:41:23.732161Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2407.04607","last_updated":"2025-06-20T18:26:36Z","snapshot_observed_at":"2026-08-16T13:36:45.389909Z","submitted_at":"2024-07-05T15:53:25Z","title":"Cosmological constraints from the cross-correlation of DESI Luminous Red Galaxies with CMB lensing from Planck PR4 and ACT DR6","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2407.04607","snapshot_observed_at":"2026-08-11T13:41:23.751096Z","title":"Sailer et al","venue":null,"work_id":null,"year":2024},"citing_paper":{"arxiv_id":"2412.12905","last_updated":"2025-01-25T08:30:04Z","snapshot_observed_at":"2026-08-17T16:16:24.002443Z","submitted_at":"2024-12-17T13:31:15Z","title":"DESI and SNe: Dynamical Dark Energy, $\\Omega_m$ Tension or Systematics?","version":2},"reference_index":47,"source":"pdf_text","source_observed_at":"2026-08-11T13:41:23.751096Z"},"links":{"cited_paper":"/paper/2407.04607","citing_paper":"/paper/2412.12905"},"observation_digest":"sha256:deb786f7e018c45f79dc6331c224bed295570b77b406443bc2093d359d7f085c","observation_id":"3d02fdc0-2fbc-4b0b-b29c-6738c098858e","resolution":{"observed_at":"2026-08-11T13:41:23.751096Z","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":"2412.13973","doi":null,"metadata_source":"raw_reference","pith_arxiv_id":null,"snapshot_observed_at":"2026-08-11T13:41:25.263594Z","title":"Mukherjee and A","venue":null,"work_id":"fe721718-7b88-436f-b06f-607bbdd815ec","year":2024},"citing_paper":{"arxiv_id":"2412.12905","last_updated":"2025-01-25T08:30:04Z","snapshot_observed_at":"2026-08-17T16:16:24.002443Z","submitted_at":"2024-12-17T13:31:15Z","title":"DESI and SNe: Dynamical Dark Energy, $\\Omega_m$ Tension or Systematics?","version":2},"reference_index":48,"source":"pdf_text","source_observed_at":"2026-08-11T13:41:23.755107Z"},"links":{"citing_paper":"/paper/2412.12905"},"observation_digest":"sha256:888293cb3701f2b6191e00290fbcf564e78bd9cf7b039cbb585e63787a28dc46","observation_id":"85e8ed6a-5443-46c7-98f8-bf2e96e55bc6","resolution":{"observed_at":"2026-08-11T13:41:25.269135Z","resolver_source":"raw_fallback","status":"verified_exact"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-19T06:32:44.657259+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-19T06:32:44.657259+00:00","source":"crossref"},{"observed_at":"2026-08-19T06:32:39.956319+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":{"arxiv_id":"2402.04767","last_updated":"2024-07-22T12:19:28Z","snapshot_observed_at":"2026-08-16T14:20:39.653392Z","submitted_at":"2024-02-07T11:36:11Z","title":"$\\Lambda$CDM Tensions: Localising Missing Physics through Consistency Checks","version":3},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2402.04767","snapshot_observed_at":"2026-08-11T13:41:23.758572Z","title":"Akarsu, E","venue":null,"work_id":null,"year":2024},"citing_paper":{"arxiv_id":"2412.12905","last_updated":"2025-01-25T08:30:04Z","snapshot_observed_at":"2026-08-17T16:16:24.002443Z","submitted_at":"2024-12-17T13:31:15Z","title":"DESI and SNe: Dynamical Dark Energy, $\\Omega_m$ Tension or Systematics?","version":2},"reference_index":49,"source":"pdf_text","source_observed_at":"2026-08-11T13:41:23.758572Z"},"links":{"cited_paper":"/paper/2402.04767","citing_paper":"/paper/2412.12905"},"observation_digest":"sha256:08def8babb9dd431f508a75e5385bb8c1bd0492aaf0611d022fc78de188063ab","observation_id":"2016212f-7095-4aaa-9256-63a7a4cb76fd","resolution":{"observed_at":"2026-08-11T13:41:23.758572Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2406.10931","last_updated":"2024-06-16T13:24:55Z","snapshot_observed_at":"2026-08-16T13:42:34.115531Z","submitted_at":"2024-06-16T13:24:55Z","title":"A test for the redshift dependence of $\\sigma_8$ using $f\\sigma_8$ measurements","version":1},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2406.10931","snapshot_observed_at":"2026-08-11T13:41:23.747394Z","title":"Manna and S","venue":null,"work_id":null,"year":2024},"citing_paper":{"arxiv_id":"2412.12905","last_updated":"2025-01-25T08:30:04Z","snapshot_observed_at":"2026-08-17T16:16:24.002443Z","submitted_at":"2024-12-17T13:31:15Z","title":"DESI and SNe: Dynamical Dark Energy, $\\Omega_m$ Tension or Systematics?","version":2},"reference_index":50,"source":"pdf_text","source_observed_at":"2026-08-11T13:41:23.747394Z"},"links":{"cited_paper":"/paper/2406.10931","citing_paper":"/paper/2412.12905"},"observation_digest":"sha256:260422e82bc94038794d79387b78631c45fd7cca2d22e4ee1d7fb0bee27e392c","observation_id":"577586c7-ace0-4fea-8b5d-c45cd0612e81","resolution":{"observed_at":"2026-08-11T13:41:23.747394Z","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":"2026-08-18T05:33:20.406006Z","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":"2026-08-11T13:41:23.765774Z","title":null,"venue":null,"work_id":null,"year":2024},"citing_paper":{"arxiv_id":"2412.12905","last_updated":"2025-01-25T08:30:04Z","snapshot_observed_at":"2026-08-17T16:16:24.002443Z","submitted_at":"2024-12-17T13:31:15Z","title":"DESI and SNe: Dynamical Dark Energy, $\\Omega_m$ Tension or Systematics?","version":2},"reference_index":51,"source":"pdf_text","source_observed_at":"2026-08-11T13:41:23.765774Z"},"links":{"cited_paper":"/paper/2404.03000","citing_paper":"/paper/2412.12905"},"observation_digest":"sha256:161df1488f4d1a550e5bd824e1c2d5b611ee22c070156f226561e4590efef892","observation_id":"117a56f7-c4cb-49e4-bc6a-5c9336b1bb72","resolution":{"observed_at":"2026-08-11T13:41:23.765774Z","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":"2026-08-18T05:33:20.223461Z","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":"2026-08-11T13:41:23.769410Z","title":null,"venue":null,"work_id":null,"year":2024},"citing_paper":{"arxiv_id":"2412.12905","last_updated":"2025-01-25T08:30:04Z","snapshot_observed_at":"2026-08-17T16:16:24.002443Z","submitted_at":"2024-12-17T13:31:15Z","title":"DESI and SNe: Dynamical Dark Energy, $\\Omega_m$ Tension or Systematics?","version":2},"reference_index":52,"source":"pdf_text","source_observed_at":"2026-08-11T13:41:23.769410Z"},"links":{"cited_paper":"/paper/2404.03001","citing_paper":"/paper/2412.12905"},"observation_digest":"sha256:9f6a0a6da64999fe7c8baa14d35129ca4641f360c8dd21a78461addde3cd06bb","observation_id":"7eb74515-d1d2-44be-9caa-71537b861a67","resolution":{"observed_at":"2026-08-11T13:41:23.769410Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2412.12905","last_updated":"2025-01-25T08:30:04Z","snapshot_observed_at":"2026-08-17T16:16:24.002443Z","submitted_at":"2024-12-17T13:31:15Z","title":"DESI and SNe: Dynamical Dark Energy, $\\Omega_m$ Tension or Systematics?","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2412.12905","snapshot_observed_at":"2026-08-11T13:41:23.555260Z","title":"Ωm tension","venue":null,"work_id":null,"year":2025},"citing_paper":{"arxiv_id":"2412.12905","last_updated":"2025-01-25T08:30:04Z","snapshot_observed_at":"2026-08-17T16:16:24.002443Z","submitted_at":"2024-12-17T13:31:15Z","title":"DESI and SNe: Dynamical Dark Energy, $\\Omega_m$ Tension or Systematics?","version":2},"reference_index":53,"source":"pdf_text","source_observed_at":"2026-08-11T13:41:23.555260Z"},"links":{"cited_paper":"/paper/2412.12905","citing_paper":"/paper/2412.12905"},"observation_digest":"sha256:a943d0e097a0bf6bee6bdc2df3c8d421b560645e556d28f4d79b5013758e0d5d","observation_id":"8b020e06-ff4b-4439-aaa9-c581490fbb20","resolution":{"observed_at":"2026-08-11T13:41:23.555260Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2308.16628","last_updated":"2023-08-31T10:49:29Z","snapshot_observed_at":"2026-08-20T01:26:30.772412Z","submitted_at":"2023-08-31T10:49:29Z","title":"Seven hints that early-time new physics alone is not sufficient to solve the Hubble tension","version":1},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2308.16628","snapshot_observed_at":"2026-08-11T13:41:23.762185Z","title":"Vagnozzi, Universe 9, 393 (2023), arXiv:2308.16628 [astro-ph.CO]","venue":null,"work_id":null,"year":2023},"citing_paper":{"arxiv_id":"2412.12905","last_updated":"2025-01-25T08:30:04Z","snapshot_observed_at":"2026-08-17T16:16:24.002443Z","submitted_at":"2024-12-17T13:31:15Z","title":"DESI and SNe: Dynamical Dark Energy, $\\Omega_m$ Tension or Systematics?","version":2},"reference_index":54,"source":"pdf_text","source_observed_at":"2026-08-11T13:41:23.762185Z"},"links":{"cited_paper":"/paper/2308.16628","citing_paper":"/paper/2412.12905"},"observation_digest":"sha256:81db4858bc9dab7376fbd451494024c09651cb7a01c3a4dbbaa78c263dc61a77","observation_id":"d77141c4-02c6-43e4-8a4d-955a9596315b","resolution":{"observed_at":"2026-08-11T13:41:23.762185Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2202.04077","last_updated":"2022-11-14T21:28:25Z","snapshot_observed_at":"2026-08-01T22:04:41.273741Z","submitted_at":"2022-02-08T19:00:00Z","title":"The Pantheon+ Analysis: Cosmological Constraints","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2202.04077","snapshot_observed_at":"2026-08-11T13:41:23.780751Z","title":"Brout et al","venue":null,"work_id":null,"year":2022},"citing_paper":{"arxiv_id":"2412.12905","last_updated":"2025-01-25T08:30:04Z","snapshot_observed_at":"2026-08-17T16:16:24.002443Z","submitted_at":"2024-12-17T13:31:15Z","title":"DESI and SNe: Dynamical Dark Energy, $\\Omega_m$ Tension or Systematics?","version":2},"reference_index":55,"source":"pdf_text","source_observed_at":"2026-08-11T13:41:23.780751Z"},"links":{"cited_paper":"/paper/2202.04077","citing_paper":"/paper/2412.12905"},"observation_digest":"sha256:c3f34650fc47f0015f3bd17de7bf925233d0a2a7e9d18ed5152bac0c03cefc91","observation_id":"c0c7e13b-5ae8-475b-95ab-c2d1fa59f7ef","resolution":{"observed_at":"2026-08-11T13:41:23.780751Z","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":"2026-08-11T13:41:23.551233Z","title":"It has been claimed in","venue":null,"work_id":null,"year":null},"citing_paper":{"arxiv_id":"2412.12905","last_updated":"2025-01-25T08:30:04Z","snapshot_observed_at":"2026-08-17T16:16:24.002443Z","submitted_at":"2024-12-17T13:31:15Z","title":"DESI and SNe: Dynamical Dark Energy, $\\Omega_m$ Tension or Systematics?","version":2},"reference_index":56,"source":"pdf_text","source_observed_at":"2026-08-11T13:41:23.551233Z"},"links":{"citing_paper":"/paper/2412.12905"},"observation_digest":"sha256:8c6b6cde0f1e607302eff5a626d6fe6854136440ced79edc14a4adcd2e9a0b83","observation_id":"c03ca6e0-e658-4948-a5da-a012ff84072e","resolution":{"observed_at":"2026-08-11T13:41:23.551233Z","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":"2026-08-11T13:41:23.773266Z","title":null,"venue":null,"work_id":null,"year":2024},"citing_paper":{"arxiv_id":"2412.12905","last_updated":"2025-01-25T08:30:04Z","snapshot_observed_at":"2026-08-17T16:16:24.002443Z","submitted_at":"2024-12-17T13:31:15Z","title":"DESI and SNe: Dynamical Dark Energy, $\\Omega_m$ Tension or Systematics?","version":2},"reference_index":57,"source":"pdf_text","source_observed_at":"2026-08-11T13:41:23.773266Z"},"links":{"cited_paper":"/paper/2404.03002","citing_paper":"/paper/2412.12905"},"observation_digest":"sha256:b71a42703acd2887c3680340f6ceb877346c1b74be082aa3187574539321fe49","observation_id":"4483a87d-b676-497a-8450-89729642acf0","resolution":{"observed_at":"2026-08-11T13:41:23.773266Z","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":"2026-08-11T13:41:23.776968Z","title":"Scolnic et al","venue":null,"work_id":null,"year":2022},"citing_paper":{"arxiv_id":"2412.12905","last_updated":"2025-01-25T08:30:04Z","snapshot_observed_at":"2026-08-17T16:16:24.002443Z","submitted_at":"2024-12-17T13:31:15Z","title":"DESI and SNe: Dynamical Dark Energy, $\\Omega_m$ Tension or Systematics?","version":2},"reference_index":58,"source":"pdf_text","source_observed_at":"2026-08-11T13:41:23.776968Z"},"links":{"cited_paper":"/paper/2112.03863","citing_paper":"/paper/2412.12905"},"observation_digest":"sha256:217ad926e1f2faa8d643ffc789b224afeeb45ecc36a863ad5b8da066af2262eb","observation_id":"c029d3c4-ac63-40b7-bacc-6af8c4e877c0","resolution":{"observed_at":"2026-08-11T13:41:23.776968Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2407.16689","last_updated":"2024-09-24T15:26:01Z","snapshot_observed_at":"2026-08-19T21:36:31.464620Z","submitted_at":"2024-07-23T17:54:39Z","title":"Robust Preference for Dynamical Dark Energy in DESI BAO and SN Measurements","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2407.16689","snapshot_observed_at":"2026-08-11T13:41:23.795365Z","title":"Giar `e, M","venue":null,"work_id":null,"year":2024},"citing_paper":{"arxiv_id":"2412.12905","last_updated":"2025-01-25T08:30:04Z","snapshot_observed_at":"2026-08-17T16:16:24.002443Z","submitted_at":"2024-12-17T13:31:15Z","title":"DESI and SNe: Dynamical Dark Energy, $\\Omega_m$ Tension or Systematics?","version":2},"reference_index":59,"source":"pdf_text","source_observed_at":"2026-08-11T13:41:23.795365Z"},"links":{"cited_paper":"/paper/2407.16689","citing_paper":"/paper/2412.12905"},"observation_digest":"sha256:52b2a686843cfd64d6ec35a0b18292583b70988457a398a859675dc3f5189a4b","observation_id":"9ca9f387-9b31-42eb-98a0-a38d87ebfa64","resolution":{"observed_at":"2026-08-11T13:41:23.795365Z","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":"2026-08-11T13:41:23.784584Z","title":"Rubin et al., (2023), arXiv:2311.12098 [astro-ph.CO]","venue":null,"work_id":null,"year":2023},"citing_paper":{"arxiv_id":"2412.12905","last_updated":"2025-01-25T08:30:04Z","snapshot_observed_at":"2026-08-17T16:16:24.002443Z","submitted_at":"2024-12-17T13:31:15Z","title":"DESI and SNe: Dynamical Dark Energy, $\\Omega_m$ Tension or Systematics?","version":2},"reference_index":60,"source":"pdf_text","source_observed_at":"2026-08-11T13:41:23.784584Z"},"links":{"cited_paper":"/paper/2311.12098","citing_paper":"/paper/2412.12905"},"observation_digest":"sha256:1acb29e4f2050bcbc92c9527e6082cbd59465646d77aba2349d3b10374691dae","observation_id":"96c9328c-6684-4c89-80f5-eef31c349924","resolution":{"observed_at":"2026-08-11T13:41:23.784584Z","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":"2026-08-11T13:41:23.788090Z","title":null,"venue":null,"work_id":null,"year":2024},"citing_paper":{"arxiv_id":"2412.12905","last_updated":"2025-01-25T08:30:04Z","snapshot_observed_at":"2026-08-17T16:16:24.002443Z","submitted_at":"2024-12-17T13:31:15Z","title":"DESI and SNe: Dynamical Dark Energy, $\\Omega_m$ Tension or Systematics?","version":2},"reference_index":61,"source":"pdf_text","source_observed_at":"2026-08-11T13:41:23.788090Z"},"links":{"cited_paper":"/paper/2401.02929","citing_paper":"/paper/2412.12905"},"observation_digest":"sha256:b9bda3899b9b0d5ac1b286971fff284ed1b06357b0cc876b26fbc5c15c53c7b8","observation_id":"5c3270a5-4e05-40b2-8b1c-b14d997a464a","resolution":{"observed_at":"2026-08-11T13:41:23.788090Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2406.05046","last_updated":"2024-06-07T16:18:57Z","snapshot_observed_at":"2026-08-16T13:45:05.846246Z","submitted_at":"2024-06-07T16:18:57Z","title":"The Dark Energy Survey Supernova Program: Light curves and 5-Year data release","version":1},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2406.05046","snapshot_observed_at":"2026-08-11T13:41:23.791643Z","title":null,"venue":null,"work_id":null,"year":2024},"citing_paper":{"arxiv_id":"2412.12905","last_updated":"2025-01-25T08:30:04Z","snapshot_observed_at":"2026-08-17T16:16:24.002443Z","submitted_at":"2024-12-17T13:31:15Z","title":"DESI and SNe: Dynamical Dark Energy, $\\Omega_m$ Tension or Systematics?","version":2},"reference_index":62,"source":"pdf_text","source_observed_at":"2026-08-11T13:41:23.791643Z"},"links":{"cited_paper":"/paper/2406.05046","citing_paper":"/paper/2412.12905"},"observation_digest":"sha256:1d0c7718d7f077212aecd977b4517b43d045325cd781bc322ced8c581be2b7c4","observation_id":"e3f48507-5e7d-437e-ac61-96cd13e33a83","resolution":{"observed_at":"2026-08-11T13:41:23.791643Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2501.03480","last_updated":"2025-07-02T14:03:15Z","snapshot_observed_at":"2026-08-12T17:48:55.146084Z","submitted_at":"2025-01-07T02:51:33Z","title":"Is excess smoothing of Planck CMB ansiotropy data partially responsible for evidence for dark energy dynamics in other $w(z)$CDM parametrizations?","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2501.03480","snapshot_observed_at":"2026-08-11T13:41:23.809697Z","title":"Park and B","venue":null,"work_id":null,"year":2025},"citing_paper":{"arxiv_id":"2412.12905","last_updated":"2025-01-25T08:30:04Z","snapshot_observed_at":"2026-08-17T16:16:24.002443Z","submitted_at":"2024-12-17T13:31:15Z","title":"DESI and SNe: Dynamical Dark Energy, $\\Omega_m$ Tension or Systematics?","version":2},"reference_index":63,"source":"pdf_text","source_observed_at":"2026-08-11T13:41:23.809697Z"},"links":{"cited_paper":"/paper/2501.03480","citing_paper":"/paper/2412.12905"},"observation_digest":"sha256:0a5ba5037dacfd08f04f7be656c101907f2b28e0f4f58a9d5c21449856e250c3","observation_id":"58e8055b-6feb-4129-87ec-12f8c679a719","resolution":{"observed_at":"2026-08-11T13:41:23.809697Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2404.18579","last_updated":"2024-06-20T10:41:20Z","snapshot_observed_at":"2026-08-19T19:12:41.418326Z","submitted_at":"2024-04-29T10:41:15Z","title":"Dark energy in light of recent DESI BAO and Hubble tension","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2404.18579","snapshot_observed_at":"2026-08-11T13:41:23.799009Z","title":"Wang and Y .-S","venue":null,"work_id":null,"year":2024},"citing_paper":{"arxiv_id":"2412.12905","last_updated":"2025-01-25T08:30:04Z","snapshot_observed_at":"2026-08-17T16:16:24.002443Z","submitted_at":"2024-12-17T13:31:15Z","title":"DESI and SNe: Dynamical Dark Energy, $\\Omega_m$ Tension or Systematics?","version":2},"reference_index":64,"source":"pdf_text","source_observed_at":"2026-08-11T13:41:23.799009Z"},"links":{"cited_paper":"/paper/2404.18579","citing_paper":"/paper/2412.12905"},"observation_digest":"sha256:bd5bef724868061e7a232ec3bcad993de736c2071d3f342830dedb0516d2a837","observation_id":"58c3253d-5764-4dd6-9db5-08bf9e80f807","resolution":{"observed_at":"2026-08-11T13:41:23.799009Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2405.00502","last_updated":"2024-11-28T15:20:41Z","snapshot_observed_at":"2026-08-16T13:56:18.156078Z","submitted_at":"2024-05-01T13:20:37Z","title":"Using non-DESI data to confirm and strengthen the DESI 2024 spatially-flat $w_0w_a$CDM cosmological parameterization result","version":3},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2405.00502","snapshot_observed_at":"2026-08-11T13:41:23.802324Z","title":null,"venue":null,"work_id":null,"year":2024},"citing_paper":{"arxiv_id":"2412.12905","last_updated":"2025-01-25T08:30:04Z","snapshot_observed_at":"2026-08-17T16:16:24.002443Z","submitted_at":"2024-12-17T13:31:15Z","title":"DESI and SNe: Dynamical Dark Energy, $\\Omega_m$ Tension or Systematics?","version":2},"reference_index":65,"source":"pdf_text","source_observed_at":"2026-08-11T13:41:23.802324Z"},"links":{"cited_paper":"/paper/2405.00502","citing_paper":"/paper/2412.12905"},"observation_digest":"sha256:5c13a3377763a4bf45ef29e47bdc9ab3157999062a838d5a6456ecc8d5b512b6","observation_id":"58b5d1d5-657e-4cef-9fe7-7cbdba7a6663","resolution":{"observed_at":"2026-08-11T13:41:23.802324Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2410.13627","last_updated":"2025-09-12T16:30:40Z","snapshot_observed_at":"2026-08-16T13:12:35.757293Z","submitted_at":"2024-10-04T13:12:49Z","title":"Is the $w_0w_a$CDM cosmological parameterization evidence for dark energy dynamics partially caused by the excess smoothing of Planck CMB anisotropy data?","version":3},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2410.13627","snapshot_observed_at":"2026-08-11T13:41:23.806173Z","title":null,"venue":null,"work_id":null,"year":2024},"citing_paper":{"arxiv_id":"2412.12905","last_updated":"2025-01-25T08:30:04Z","snapshot_observed_at":"2026-08-17T16:16:24.002443Z","submitted_at":"2024-12-17T13:31:15Z","title":"DESI and SNe: Dynamical Dark Energy, $\\Omega_m$ Tension or Systematics?","version":2},"reference_index":66,"source":"pdf_text","source_observed_at":"2026-08-11T13:41:23.806173Z"},"links":{"cited_paper":"/paper/2410.13627","citing_paper":"/paper/2412.12905"},"observation_digest":"sha256:5860f195c3b47834a461dace0c14a7d5be93371c6ccd7f6d411919943103410e","observation_id":"025870a4-0be3-4176-95ea-ccf02e5cd0c2","resolution":{"observed_at":"2026-08-11T13:41:23.806173Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2405.17396","last_updated":"2024-05-30T14:24:05Z","snapshot_observed_at":"2026-08-20T01:22:21.850585Z","submitted_at":"2024-05-27T17:48:44Z","title":"Cosmological constraints on curved quintessence","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2405.17396","snapshot_observed_at":"2026-08-11T13:41:23.824066Z","title":"Bhattacharya, G","venue":null,"work_id":null,"year":2024},"citing_paper":{"arxiv_id":"2412.12905","last_updated":"2025-01-25T08:30:04Z","snapshot_observed_at":"2026-08-17T16:16:24.002443Z","submitted_at":"2024-12-17T13:31:15Z","title":"DESI and SNe: Dynamical Dark Energy, $\\Omega_m$ Tension or Systematics?","version":2},"reference_index":67,"source":"pdf_text","source_observed_at":"2026-08-11T13:41:23.824066Z"},"links":{"cited_paper":"/paper/2405.17396","citing_paper":"/paper/2412.12905"},"observation_digest":"sha256:426ec2a812c21127707c48ce202f9dd46ee79c2a5a274e93c0d66b3904bda539","observation_id":"00e13731-2719-43e5-8585-87859c71105a","resolution":{"observed_at":"2026-08-11T13:41:23.824066Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2411.16046","last_updated":"2024-11-25T02:19:48Z","snapshot_observed_at":"2026-08-17T13:30:10.472213Z","submitted_at":"2024-11-25T02:19:48Z","title":"On the evidence of dynamical dark energy","version":1},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2411.16046","snapshot_observed_at":"2026-08-11T13:41:23.813711Z","title":null,"venue":null,"work_id":null,"year":2024},"citing_paper":{"arxiv_id":"2412.12905","last_updated":"2025-01-25T08:30:04Z","snapshot_observed_at":"2026-08-17T16:16:24.002443Z","submitted_at":"2024-12-17T13:31:15Z","title":"DESI and SNe: Dynamical Dark Energy, $\\Omega_m$ Tension or Systematics?","version":2},"reference_index":68,"source":"pdf_text","source_observed_at":"2026-08-11T13:41:23.813711Z"},"links":{"cited_paper":"/paper/2411.16046","citing_paper":"/paper/2412.12905"},"observation_digest":"sha256:151d2c0263770f2bca04f1fe8f2e677f4c7a1f4b4099004dcf555ee7c0a66a27","observation_id":"77d1c566-b986-4360-8477-f21b4bcf8265","resolution":{"observed_at":"2026-08-11T13:41:23.813711Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2404.05722","last_updated":"2024-07-06T15:54:47Z","snapshot_observed_at":"2026-08-16T14:02:37.747395Z","submitted_at":"2024-04-08T17:58:02Z","title":"Quintessential interpretation of the evolving dark energy in light of DESI","version":4},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2404.05722","snapshot_observed_at":"2026-08-11T13:41:23.817183Z","title":"Tada and T","venue":null,"work_id":null,"year":2024},"citing_paper":{"arxiv_id":"2412.12905","last_updated":"2025-01-25T08:30:04Z","snapshot_observed_at":"2026-08-17T16:16:24.002443Z","submitted_at":"2024-12-17T13:31:15Z","title":"DESI and SNe: Dynamical Dark Energy, $\\Omega_m$ Tension or Systematics?","version":2},"reference_index":69,"source":"pdf_text","source_observed_at":"2026-08-11T13:41:23.817183Z"},"links":{"cited_paper":"/paper/2404.05722","citing_paper":"/paper/2412.12905"},"observation_digest":"sha256:9e0382231c8a29f1c4b85ab560fe52d7a649ec37c7421a2a1ca6ec9a4350f4e7","observation_id":"3064d1cb-e6c2-4cec-b54e-9a43ae4c2638","resolution":{"observed_at":"2026-08-11T13:41:23.817183Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2404.15232","last_updated":"2024-12-19T16:25:49Z","snapshot_observed_at":"2026-08-16T13:58:27.312344Z","submitted_at":"2024-04-23T17:05:14Z","title":"Interacting Dark Energy after DESI Baryon Acoustic Oscillation measurements","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2404.15232","snapshot_observed_at":"2026-08-11T13:41:23.820821Z","title":"Giar `e, M","venue":null,"work_id":null,"year":2024},"citing_paper":{"arxiv_id":"2412.12905","last_updated":"2025-01-25T08:30:04Z","snapshot_observed_at":"2026-08-17T16:16:24.002443Z","submitted_at":"2024-12-17T13:31:15Z","title":"DESI and SNe: Dynamical Dark Energy, $\\Omega_m$ Tension or Systematics?","version":2},"reference_index":70,"source":"pdf_text","source_observed_at":"2026-08-11T13:41:23.820821Z"},"links":{"cited_paper":"/paper/2404.15232","citing_paper":"/paper/2412.12905"},"observation_digest":"sha256:1b1228615ed53cb77a51226f9a5050ab49c9a2ccf8d63c2842f9bbb7c0b8d981","observation_id":"e558c932-1e8f-4f76-8e9f-f796da7e45a9","resolution":{"observed_at":"2026-08-11T13:41:23.820821Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2406.04408","last_updated":"2024-12-13T05:27:27Z","snapshot_observed_at":"2026-08-16T13:45:23.943153Z","submitted_at":"2024-06-06T18:00:08Z","title":"First Constraints on a Pixelated Universe in Light of DESI","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2406.04408","snapshot_observed_at":"2026-08-11T13:41:23.839657Z","title":null,"venue":null,"work_id":null,"year":2025},"citing_paper":{"arxiv_id":"2412.12905","last_updated":"2025-01-25T08:30:04Z","snapshot_observed_at":"2026-08-17T16:16:24.002443Z","submitted_at":"2024-12-17T13:31:15Z","title":"DESI and SNe: Dynamical Dark Energy, $\\Omega_m$ Tension or Systematics?","version":2},"reference_index":71,"source":"pdf_text","source_observed_at":"2026-08-11T13:41:23.839657Z"},"links":{"cited_paper":"/paper/2406.04408","citing_paper":"/paper/2412.12905"},"observation_digest":"sha256:96c4327cfeab1c7a547212758d998bdd34e53f0f952a30dbe8f9eac4b506c00a","observation_id":"43bf9113-af94-4d88-8bd1-cc747652fc31","resolution":{"observed_at":"2026-08-11T13:41:23.839657Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2405.18747","last_updated":"2024-05-29T04:09:59Z","snapshot_observed_at":"2026-08-18T10:37:43.489357Z","submitted_at":"2024-05-29T04:09:59Z","title":"DESI Constraints on Exponential Quintessence","version":1},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2405.18747","snapshot_observed_at":"2026-08-11T13:41:23.828317Z","title":null,"venue":null,"work_id":null,"year":2024},"citing_paper":{"arxiv_id":"2412.12905","last_updated":"2025-01-25T08:30:04Z","snapshot_observed_at":"2026-08-17T16:16:24.002443Z","submitted_at":"2024-12-17T13:31:15Z","title":"DESI and SNe: Dynamical Dark Energy, $\\Omega_m$ Tension or Systematics?","version":2},"reference_index":72,"source":"pdf_text","source_observed_at":"2026-08-11T13:41:23.828317Z"},"links":{"cited_paper":"/paper/2405.18747","citing_paper":"/paper/2412.12905"},"observation_digest":"sha256:670ccd33451a8ccd7e1e512948de4fcc03b922908e8974d0d0dd91edcb86b9be","observation_id":"18b57926-af53-42b7-88ec-af0443254327","resolution":{"observed_at":"2026-08-11T13:41:23.828317Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2405.20240","last_updated":"2024-05-30T16:44:03Z","snapshot_observed_at":"2026-08-17T21:28:42.806161Z","submitted_at":"2024-05-30T16:44:03Z","title":"Alleviating the $H_0$ and $\\sigma_8$ tensions in the interacting cubic covariant Galileon model","version":1},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2405.20240","snapshot_observed_at":"2026-08-11T13:41:23.832056Z","title":"zabat, Y","venue":null,"work_id":null,"year":2024},"citing_paper":{"arxiv_id":"2412.12905","last_updated":"2025-01-25T08:30:04Z","snapshot_observed_at":"2026-08-17T16:16:24.002443Z","submitted_at":"2024-12-17T13:31:15Z","title":"DESI and SNe: Dynamical Dark Energy, $\\Omega_m$ Tension or Systematics?","version":2},"reference_index":73,"source":"pdf_text","source_observed_at":"2026-08-11T13:41:23.832056Z"},"links":{"cited_paper":"/paper/2405.20240","citing_paper":"/paper/2412.12905"},"observation_digest":"sha256:9905278f028f6ea4c20061d3de9febe8196edc37ae5bc014cb1bb232b335fdaf","observation_id":"0de474c3-58c2-446d-91a7-c5d32a580edb","resolution":{"observed_at":"2026-08-11T13:41:23.832056Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2406.01691","last_updated":"2024-09-13T16:29:00Z","snapshot_observed_at":"2026-08-16T13:46:35.412075Z","submitted_at":"2024-06-03T18:00:03Z","title":"Solar chameleons: Novel channels","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2406.01691","snapshot_observed_at":"2026-08-11T13:41:23.835951Z","title":"O’Shea, A.-C","venue":null,"work_id":null,"year":2024},"citing_paper":{"arxiv_id":"2412.12905","last_updated":"2025-01-25T08:30:04Z","snapshot_observed_at":"2026-08-17T16:16:24.002443Z","submitted_at":"2024-12-17T13:31:15Z","title":"DESI and SNe: Dynamical Dark Energy, $\\Omega_m$ Tension or Systematics?","version":2},"reference_index":74,"source":"pdf_text","source_observed_at":"2026-08-11T13:41:23.835951Z"},"links":{"cited_paper":"/paper/2406.01691","citing_paper":"/paper/2412.12905"},"observation_digest":"sha256:87c5409e069e9e4c24bf372d67b9967d83471244b0a5006558b0d3c76f15cf2e","observation_id":"182786a9-97c9-4d06-97fd-9fe1648ef838","resolution":{"observed_at":"2026-08-11T13:41:23.835951Z","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":"2026-08-11T13:41:23.855360Z","title":"Bhattacharya, G","venue":null,"work_id":null,"year":2024},"citing_paper":{"arxiv_id":"2412.12905","last_updated":"2025-01-25T08:30:04Z","snapshot_observed_at":"2026-08-17T16:16:24.002443Z","submitted_at":"2024-12-17T13:31:15Z","title":"DESI and SNe: Dynamical Dark Energy, $\\Omega_m$ Tension or Systematics?","version":2},"reference_index":75,"source":"pdf_text","source_observed_at":"2026-08-11T13:41:23.855360Z"},"links":{"citing_paper":"/paper/2412.12905"},"observation_digest":"sha256:14764109e16b7852acb6a4faaa131696988b6be04b9abd0ee798f6ce9c8cdd6a","observation_id":"b2ac7592-3c35-40bc-9c8a-4fa9ea802a37","resolution":{"observed_at":"2026-08-11T13:41:23.855360Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2407.14934","last_updated":"2024-11-12T01:42:43Z","snapshot_observed_at":"2026-08-16T13:32:27.640690Z","submitted_at":"2024-07-20T16:52:17Z","title":"Constraints on Interacting Dark Energy Models from the DESI Baryon Acoustic Oscillation and DES Supernovae Data","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2407.14934","snapshot_observed_at":"2026-08-11T13:41:23.843762Z","title":"Li, P.-J","venue":null,"work_id":null,"year":2024},"citing_paper":{"arxiv_id":"2412.12905","last_updated":"2025-01-25T08:30:04Z","snapshot_observed_at":"2026-08-17T16:16:24.002443Z","submitted_at":"2024-12-17T13:31:15Z","title":"DESI and SNe: Dynamical Dark Energy, $\\Omega_m$ Tension or Systematics?","version":2},"reference_index":76,"source":"pdf_text","source_observed_at":"2026-08-11T13:41:23.843762Z"},"links":{"cited_paper":"/paper/2407.14934","citing_paper":"/paper/2412.12905"},"observation_digest":"sha256:fdc5c2ed0f743efb155ba51836c8d1910b3d71c80b5952e598317820219ab85b","observation_id":"bbc57f82-c53b-4c6b-a438-cf0cadc724be","resolution":{"observed_at":"2026-08-11T13:41:23.843762Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2407.15832","last_updated":"2025-05-11T17:25:00Z","snapshot_observed_at":"2026-08-19T20:21:31.046031Z","submitted_at":"2024-07-22T17:50:31Z","title":"Hints of Nonminimally Coupled Gravity in DESI 2024 Baryon Acoustic Oscillation Measurements","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2407.15832","snapshot_observed_at":"2026-08-11T13:41:23.847529Z","title":null,"venue":null,"work_id":null,"year":2024},"citing_paper":{"arxiv_id":"2412.12905","last_updated":"2025-01-25T08:30:04Z","snapshot_observed_at":"2026-08-17T16:16:24.002443Z","submitted_at":"2024-12-17T13:31:15Z","title":"DESI and SNe: Dynamical Dark Energy, $\\Omega_m$ Tension or Systematics?","version":2},"reference_index":77,"source":"pdf_text","source_observed_at":"2026-08-11T13:41:23.847529Z"},"links":{"cited_paper":"/paper/2407.15832","citing_paper":"/paper/2412.12905"},"observation_digest":"sha256:6c4c83850b5249688330c9ef5ba85f8af719755a08045df37faf650bce8ff573","observation_id":"bcb269d1-1e4b-43fd-a380-fff5c08262e3","resolution":{"observed_at":"2026-08-11T13:41:23.847529Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2409.17019","last_updated":"2025-02-07T15:18:24Z","snapshot_observed_at":"2026-08-19T23:11:26.495144Z","submitted_at":"2024-09-25T15:22:09Z","title":"Matching current observational constraints with nonminimally coupled dark energy","version":4},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2409.17019","snapshot_observed_at":"2026-08-11T13:41:23.851637Z","title":null,"venue":null,"work_id":null,"year":2024},"citing_paper":{"arxiv_id":"2412.12905","last_updated":"2025-01-25T08:30:04Z","snapshot_observed_at":"2026-08-17T16:16:24.002443Z","submitted_at":"2024-12-17T13:31:15Z","title":"DESI and SNe: Dynamical Dark Energy, $\\Omega_m$ Tension or Systematics?","version":2},"reference_index":78,"source":"pdf_text","source_observed_at":"2026-08-11T13:41:23.851637Z"},"links":{"cited_paper":"/paper/2409.17019","citing_paper":"/paper/2412.12905"},"observation_digest":"sha256:a750e8ba3017a0bc146e96897a29d1d2a3a189684353f6d09e038495bcb12aca","observation_id":"ed1a930f-3f3f-4db0-9839-7893a69e5d2a","resolution":{"observed_at":"2026-08-11T13:41:23.851637Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2408.04432","last_updated":"2024-12-09T05:27:29Z","snapshot_observed_at":"2026-08-20T02:42:29.546778Z","submitted_at":"2024-08-08T13:00:33Z","title":"Consistency tests between SDSS and DESI BAO measurements","version":3},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2408.04432","snapshot_observed_at":"2026-08-11T13:41:23.870703Z","title":"Ghosh and C","venue":null,"work_id":null,"year":2024},"citing_paper":{"arxiv_id":"2412.12905","last_updated":"2025-01-25T08:30:04Z","snapshot_observed_at":"2026-08-17T16:16:24.002443Z","submitted_at":"2024-12-17T13:31:15Z","title":"DESI and SNe: Dynamical Dark Energy, $\\Omega_m$ Tension or Systematics?","version":2},"reference_index":79,"source":"pdf_text","source_observed_at":"2026-08-11T13:41:23.870703Z"},"links":{"cited_paper":"/paper/2408.04432","citing_paper":"/paper/2412.12905"},"observation_digest":"sha256:66e7fbd566c3db423f7554dd739bd08c6cdfd4099fc76808960a01c53c9c94fc","observation_id":"ecc4a2b4-c358-418e-b33c-4b59fc8b6bee","resolution":{"observed_at":"2026-08-11T13:41:23.870703Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2411.11743","last_updated":"2024-12-05T18:12:07Z","snapshot_observed_at":"2026-08-19T13:35:07.058694Z","submitted_at":"2024-11-18T17:15:14Z","title":"Bridge the Cosmological Tensions with Thawing Gravity","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2411.11743","snapshot_observed_at":"2026-08-11T13:41:23.858998Z","title":"Ye, (2024), arXiv:2411.11743 [astro-ph.CO]","venue":null,"work_id":null,"year":2024},"citing_paper":{"arxiv_id":"2412.12905","last_updated":"2025-01-25T08:30:04Z","snapshot_observed_at":"2026-08-17T16:16:24.002443Z","submitted_at":"2024-12-17T13:31:15Z","title":"DESI and SNe: Dynamical Dark Energy, $\\Omega_m$ Tension or Systematics?","version":2},"reference_index":80,"source":"pdf_text","source_observed_at":"2026-08-11T13:41:23.858998Z"},"links":{"cited_paper":"/paper/2411.11743","citing_paper":"/paper/2412.12905"},"observation_digest":"sha256:37c8ab06c8a88fbf73fb91871598540689cf0feaae922261c58019524a863a7b","observation_id":"f5153e82-4dbb-4468-a43d-899d691429e5","resolution":{"observed_at":"2026-08-11T13:41:23.858998Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2411.08639","last_updated":"2025-05-04T13:39:59Z","snapshot_observed_at":"2026-08-16T13:00:42.795225Z","submitted_at":"2024-11-13T14:29:02Z","title":"Revisiting holographic dark energy after DESI 2024","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2411.08639","snapshot_observed_at":"2026-08-11T13:41:23.863131Z","title":"Li, Y .-H","venue":null,"work_id":null,"year":2024},"citing_paper":{"arxiv_id":"2412.12905","last_updated":"2025-01-25T08:30:04Z","snapshot_observed_at":"2026-08-17T16:16:24.002443Z","submitted_at":"2024-12-17T13:31:15Z","title":"DESI and SNe: Dynamical Dark Energy, $\\Omega_m$ Tension or Systematics?","version":2},"reference_index":81,"source":"pdf_text","source_observed_at":"2026-08-11T13:41:23.863131Z"},"links":{"cited_paper":"/paper/2411.08639","citing_paper":"/paper/2412.12905"},"observation_digest":"sha256:d4e0c18a5a942bd33d42c3995125ebe8209569caceebe22ed50dd878f263cd71","observation_id":"4dcf575c-8f15-4206-a70a-b4685909d701","resolution":{"observed_at":"2026-08-11T13:41:23.863131Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2404.07070","last_updated":"2024-04-10T15:01:17Z","snapshot_observed_at":"2026-08-19T16:08:37.572915Z","submitted_at":"2024-04-10T15:01:17Z","title":"Model independent cosmographic constraints from DESI 2024","version":1},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2404.07070","snapshot_observed_at":"2026-08-11T13:41:23.867048Z","title":"Luongo and M","venue":null,"work_id":null,"year":2024},"citing_paper":{"arxiv_id":"2412.12905","last_updated":"2025-01-25T08:30:04Z","snapshot_observed_at":"2026-08-17T16:16:24.002443Z","submitted_at":"2024-12-17T13:31:15Z","title":"DESI and SNe: Dynamical Dark Energy, $\\Omega_m$ Tension or Systematics?","version":2},"reference_index":82,"source":"pdf_text","source_observed_at":"2026-08-11T13:41:23.867048Z"},"links":{"cited_paper":"/paper/2404.07070","citing_paper":"/paper/2412.12905"},"observation_digest":"sha256:9993de3113be798fa3398c182253aa0b094a1bc7489816c10418b7b2b09c2bdc","observation_id":"f08bfac3-8b49-4e78-aa65-93dda40dd5c4","resolution":{"observed_at":"2026-08-11T13:41:23.867048Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2407.17252","last_updated":"2025-01-29T16:54:33Z","snapshot_observed_at":"2026-08-19T23:26:22.652816Z","submitted_at":"2024-07-24T13:11:38Z","title":"Model-agnostic assessment of dark energy after DESI DR1 BAO","version":3},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2407.17252","snapshot_observed_at":"2026-08-11T13:41:23.884644Z","title":null,"venue":null,"work_id":null,"year":2024},"citing_paper":{"arxiv_id":"2412.12905","last_updated":"2025-01-25T08:30:04Z","snapshot_observed_at":"2026-08-17T16:16:24.002443Z","submitted_at":"2024-12-17T13:31:15Z","title":"DESI and SNe: Dynamical Dark Energy, $\\Omega_m$ Tension or Systematics?","version":2},"reference_index":83,"source":"pdf_text","source_observed_at":"2026-08-11T13:41:23.884644Z"},"links":{"cited_paper":"/paper/2407.17252","citing_paper":"/paper/2412.12905"},"observation_digest":"sha256:6f4eccfaea0b3f9492958d8cef26237a7cdee634e90defc42ce03abdc27936cd","observation_id":"4fe0ea4c-1998-4944-9336-3b3d390ef661","resolution":{"observed_at":"2026-08-11T13:41:23.884644Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2408.10704","last_updated":"2025-01-08T06:34:27Z","snapshot_observed_at":"2026-08-18T08:13:38.983801Z","submitted_at":"2024-08-20T09:59:06Z","title":"$\\Lambda$CDM model against cosmography: A possible deviation after DESI 2024","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2408.10704","snapshot_observed_at":"2026-08-11T13:41:23.874531Z","title":"Pourojaghi, M","venue":null,"work_id":null,"year":2024},"citing_paper":{"arxiv_id":"2412.12905","last_updated":"2025-01-25T08:30:04Z","snapshot_observed_at":"2026-08-17T16:16:24.002443Z","submitted_at":"2024-12-17T13:31:15Z","title":"DESI and SNe: Dynamical Dark Energy, $\\Omega_m$ Tension or Systematics?","version":2},"reference_index":84,"source":"pdf_text","source_observed_at":"2026-08-11T13:41:23.874531Z"},"links":{"cited_paper":"/paper/2408.10704","citing_paper":"/paper/2412.12905"},"observation_digest":"sha256:ea270c1f8910b099b9ee0391c881edf4842a3561a73bdd004a389ebca686e2d5","observation_id":"49175ee4-5c6c-424d-a9cf-2e671a098038","resolution":{"observed_at":"2026-08-11T13:41:23.874531Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2405.04216","last_updated":"2024-10-25T14:59:48Z","snapshot_observed_at":"2026-08-19T07:19:17.944458Z","submitted_at":"2024-05-07T11:29:39Z","title":"DESI 2024: Reconstructing Dark Energy using Crossing Statistics with DESI DR1 BAO data","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2405.04216","snapshot_observed_at":"2026-08-11T13:41:23.878059Z","title":"Calderon et al","venue":null,"work_id":null,"year":2024},"citing_paper":{"arxiv_id":"2412.12905","last_updated":"2025-01-25T08:30:04Z","snapshot_observed_at":"2026-08-17T16:16:24.002443Z","submitted_at":"2024-12-17T13:31:15Z","title":"DESI and SNe: Dynamical Dark Energy, $\\Omega_m$ Tension or Systematics?","version":2},"reference_index":85,"source":"pdf_text","source_observed_at":"2026-08-11T13:41:23.878059Z"},"links":{"cited_paper":"/paper/2405.04216","citing_paper":"/paper/2412.12905"},"observation_digest":"sha256:803661474a3eb553aa3c0974dfc911f0aa9d00384681860b3dfa9b91b176b162","observation_id":"b1995bde-8da8-40a8-be27-0ff8b6b211c6","resolution":{"observed_at":"2026-08-11T13:41:23.878059Z","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":"2026-08-11T13:41:23.881375Z","title":"Mukherjee and A","venue":null,"work_id":null,"year":2024},"citing_paper":{"arxiv_id":"2412.12905","last_updated":"2025-01-25T08:30:04Z","snapshot_observed_at":"2026-08-17T16:16:24.002443Z","submitted_at":"2024-12-17T13:31:15Z","title":"DESI and SNe: Dynamical Dark Energy, $\\Omega_m$ Tension or Systematics?","version":2},"reference_index":86,"source":"pdf_text","source_observed_at":"2026-08-11T13:41:23.881375Z"},"links":{"citing_paper":"/paper/2412.12905"},"observation_digest":"sha256:0f33563513e520e62418a5f0c13ee96d54f5dae4ce2943877b8187f756bb4b0a","observation_id":"d4102dfd-a0b3-4b7d-b99b-95738a368222","resolution":{"observed_at":"2026-08-11T13:41:23.881375Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2405.12282","last_updated":"2024-10-28T20:40:26Z","snapshot_observed_at":"2026-08-16T13:51:13.153153Z","submitted_at":"2024-05-20T18:00:02Z","title":"DESI Dark Energy Time Evolution is Recovered by Cosmologically Coupled Black Holes","version":3},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2405.12282","snapshot_observed_at":"2026-08-11T13:41:23.899374Z","title":null,"venue":null,"work_id":null,"year":2024},"citing_paper":{"arxiv_id":"2412.12905","last_updated":"2025-01-25T08:30:04Z","snapshot_observed_at":"2026-08-17T16:16:24.002443Z","submitted_at":"2024-12-17T13:31:15Z","title":"DESI and SNe: Dynamical Dark Energy, $\\Omega_m$ Tension or Systematics?","version":2},"reference_index":87,"source":"pdf_text","source_observed_at":"2026-08-11T13:41:23.899374Z"},"links":{"cited_paper":"/paper/2405.12282","citing_paper":"/paper/2412.12905"},"observation_digest":"sha256:74a0f1931d2dbf18d9d971810a356f44162b9caba6815e730c0d0e504cb7c81d","observation_id":"38041bc7-c060-423e-9dea-febffbd65751","resolution":{"observed_at":"2026-08-11T13:41:23.899374Z","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":"2026-08-16T13:28:31.887239Z","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":"2026-08-11T13:41:23.888259Z","title":"Jiang, D","venue":null,"work_id":null,"year":2024},"citing_paper":{"arxiv_id":"2412.12905","last_updated":"2025-01-25T08:30:04Z","snapshot_observed_at":"2026-08-17T16:16:24.002443Z","submitted_at":"2024-12-17T13:31:15Z","title":"DESI and SNe: Dynamical Dark Energy, $\\Omega_m$ Tension or Systematics?","version":2},"reference_index":88,"source":"pdf_text","source_observed_at":"2026-08-11T13:41:23.888259Z"},"links":{"cited_paper":"/paper/2408.02365","citing_paper":"/paper/2412.12905"},"observation_digest":"sha256:5421ea3271c57a9b0dbbda094585f774d2b3e9a72175dc2c94a16886e8595c5c","observation_id":"6173f116-e4dd-4fdf-9a3c-e9e23d39ccba","resolution":{"observed_at":"2026-08-11T13:41:23.888259Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2411.04901","last_updated":"2024-11-07T17:43:47Z","snapshot_observed_at":"2026-08-19T04:56:08.594901Z","submitted_at":"2024-11-07T17:43:47Z","title":"Dark energy reconstructions combining BAO data with galaxy clusters and intermediate redshift catalogs","version":1},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2411.04901","snapshot_observed_at":"2026-08-11T13:41:23.891708Z","title":"Luongo and M","venue":null,"work_id":null,"year":2025},"citing_paper":{"arxiv_id":"2412.12905","last_updated":"2025-01-25T08:30:04Z","snapshot_observed_at":"2026-08-17T16:16:24.002443Z","submitted_at":"2024-12-17T13:31:15Z","title":"DESI and SNe: Dynamical Dark Energy, $\\Omega_m$ Tension or Systematics?","version":2},"reference_index":89,"source":"pdf_text","source_observed_at":"2026-08-11T13:41:23.891708Z"},"links":{"cited_paper":"/paper/2411.04901","citing_paper":"/paper/2412.12905"},"observation_digest":"sha256:52bde5592261572485717fd52a34f3b0a8293915c240d85a3b57973a1ce1bedf","observation_id":"f4cbc8cb-31fb-40ac-ad9d-32a110b3792b","resolution":{"observed_at":"2026-08-11T13:41:23.891708Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2404.11680","last_updated":"2024-09-17T15:15:39Z","snapshot_observed_at":"2026-08-17T19:12:28.082301Z","submitted_at":"2024-04-17T18:20:26Z","title":"What if string theory has a de Sitter excited state?","version":3},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2404.11680","snapshot_observed_at":"2026-08-11T13:41:23.895560Z","title":"Chakravarty and K","venue":null,"work_id":null,"year":2024},"citing_paper":{"arxiv_id":"2412.12905","last_updated":"2025-01-25T08:30:04Z","snapshot_observed_at":"2026-08-17T16:16:24.002443Z","submitted_at":"2024-12-17T13:31:15Z","title":"DESI and SNe: Dynamical Dark Energy, $\\Omega_m$ Tension or Systematics?","version":2},"reference_index":90,"source":"pdf_text","source_observed_at":"2026-08-11T13:41:23.895560Z"},"links":{"cited_paper":"/paper/2404.11680","citing_paper":"/paper/2412.12905"},"observation_digest":"sha256:2db54689284679f73b047c743d0b28a8a245cfe7aed48345cf3d3f7afdbb2f15","observation_id":"a8f0429b-3eb0-4313-8a41-c525ee21a858","resolution":{"observed_at":"2026-08-11T13:41:23.895560Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2406.07493","last_updated":"2025-08-15T10:40:56Z","snapshot_observed_at":"2026-08-19T08:04:13.767514Z","submitted_at":"2024-06-11T17:30:09Z","title":"Model-Independent Test of Prerecombination New Physics: Measuring the Sound Horizon with Gravitational Wave Standard Sirens and the Baryon Acoustic Oscillation Angular Scale","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2406.07493","snapshot_observed_at":"2026-08-11T13:41:23.914900Z","title":"Giar `e, J","venue":null,"work_id":null,"year":2024},"citing_paper":{"arxiv_id":"2412.12905","last_updated":"2025-01-25T08:30:04Z","snapshot_observed_at":"2026-08-17T16:16:24.002443Z","submitted_at":"2024-12-17T13:31:15Z","title":"DESI and SNe: Dynamical Dark Energy, $\\Omega_m$ Tension or Systematics?","version":2},"reference_index":91,"source":"pdf_text","source_observed_at":"2026-08-11T13:41:23.914900Z"},"links":{"cited_paper":"/paper/2406.07493","citing_paper":"/paper/2412.12905"},"observation_digest":"sha256:1a49679147906032f66a64cb57688f3b8c27f2f89cf5b83e2a7eb213fd587bfa","observation_id":"1474548b-47a9-44bf-8755-339ec9d46ab5","resolution":{"observed_at":"2026-08-11T13:41:23.914900Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2405.12142","last_updated":"2024-09-12T15:01:40Z","snapshot_observed_at":"2026-08-18T20:28:51.180461Z","submitted_at":"2024-05-20T16:04:47Z","title":"Quantification of 2D vs 3D BAO tension using SNIa as a redshift interpolator and test of the Etherington relation","version":3},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2405.12142","snapshot_observed_at":"2026-08-11T13:41:23.903347Z","title":"Favale, A","venue":null,"work_id":null,"year":2024},"citing_paper":{"arxiv_id":"2412.12905","last_updated":"2025-01-25T08:30:04Z","snapshot_observed_at":"2026-08-17T16:16:24.002443Z","submitted_at":"2024-12-17T13:31:15Z","title":"DESI and SNe: Dynamical Dark Energy, $\\Omega_m$ Tension or Systematics?","version":2},"reference_index":92,"source":"pdf_text","source_observed_at":"2026-08-11T13:41:23.903347Z"},"links":{"cited_paper":"/paper/2405.12142","citing_paper":"/paper/2412.12905"},"observation_digest":"sha256:efca12c40de8c0bb8d6a0753d5334473d91c43baa1ba53503a9150e32074f016","observation_id":"677633a4-b942-453a-95c2-c41e45ca7cca","resolution":{"observed_at":"2026-08-11T13:41:23.903347Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2406.03395","last_updated":"2024-09-11T19:08:11Z","snapshot_observed_at":"2026-08-16T13:45:49.870618Z","submitted_at":"2024-06-05T15:46:54Z","title":"Can recent DESI BAO measurements accommodate a negative cosmological constant?","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2406.03395","snapshot_observed_at":"2026-08-11T13:41:23.907084Z","title":"Wang, Z.-Y","venue":null,"work_id":null,"year":2024},"citing_paper":{"arxiv_id":"2412.12905","last_updated":"2025-01-25T08:30:04Z","snapshot_observed_at":"2026-08-17T16:16:24.002443Z","submitted_at":"2024-12-17T13:31:15Z","title":"DESI and SNe: Dynamical Dark Energy, $\\Omega_m$ Tension or Systematics?","version":2},"reference_index":93,"source":"pdf_text","source_observed_at":"2026-08-11T13:41:23.907084Z"},"links":{"cited_paper":"/paper/2406.03395","citing_paper":"/paper/2412.12905"},"observation_digest":"sha256:20feb82ade0f03c451dbb9fd4a179e7d79c41fc551ceb22ec401e0d8b19c0dcb","observation_id":"1bd9be2e-2d9b-4b8d-a651-52c2d9ee6636","resolution":{"observed_at":"2026-08-11T13:41:23.907084Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2407.07878","last_updated":"2024-07-10T17:46:41Z","snapshot_observed_at":"2026-08-19T20:06:02.306347Z","submitted_at":"2024-07-10T17:46:41Z","title":"The Cosmological Preference for Negative Neutrino Mass","version":1},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2407.07878","snapshot_observed_at":"2026-08-11T13:41:23.911127Z","title":"Green and J","venue":null,"work_id":null,"year":2024},"citing_paper":{"arxiv_id":"2412.12905","last_updated":"2025-01-25T08:30:04Z","snapshot_observed_at":"2026-08-17T16:16:24.002443Z","submitted_at":"2024-12-17T13:31:15Z","title":"DESI and SNe: Dynamical Dark Energy, $\\Omega_m$ Tension or Systematics?","version":2},"reference_index":94,"source":"pdf_text","source_observed_at":"2026-08-11T13:41:23.911127Z"},"links":{"cited_paper":"/paper/2407.07878","citing_paper":"/paper/2412.12905"},"observation_digest":"sha256:add2bd07caad9b55bd16df861073e7ba4eaada71081473565b8994a519575f58","observation_id":"46d15963-9e4d-43ca-9a38-d58109b9e8c9","resolution":{"observed_at":"2026-08-11T13:41:23.911127Z","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":"2026-08-11T13:41:23.930347Z","title":null,"venue":null,"work_id":null,"year":2024},"citing_paper":{"arxiv_id":"2412.12905","last_updated":"2025-01-25T08:30:04Z","snapshot_observed_at":"2026-08-17T16:16:24.002443Z","submitted_at":"2024-12-17T13:31:15Z","title":"DESI and SNe: Dynamical Dark Energy, $\\Omega_m$ Tension or Systematics?","version":2},"reference_index":95,"source":"pdf_text","source_observed_at":"2026-08-11T13:41:23.930347Z"},"links":{"citing_paper":"/paper/2412.12905"},"observation_digest":"sha256:f3ffcf1cdfb3afedf859db3ed2159c7cb0fd59f6a4f653335a3a8ae58c8eb82e","observation_id":"387beaf4-d86b-49c1-b20d-295f03e15773","resolution":{"observed_at":"2026-08-11T13:41:23.930347Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2407.11263","last_updated":"2024-07-15T22:10:20Z","snapshot_observed_at":"2026-08-16T13:33:58.094801Z","submitted_at":"2024-07-15T22:10:20Z","title":"Impact of evolving dark energy on the search for primordial gravitational waves","version":1},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2407.11263","snapshot_observed_at":"2026-08-11T13:41:23.918911Z","title":null,"venue":null,"work_id":null,"year":2024},"citing_paper":{"arxiv_id":"2412.12905","last_updated":"2025-01-25T08:30:04Z","snapshot_observed_at":"2026-08-17T16:16:24.002443Z","submitted_at":"2024-12-17T13:31:15Z","title":"DESI and SNe: Dynamical Dark Energy, $\\Omega_m$ Tension or Systematics?","version":2},"reference_index":96,"source":"pdf_text","source_observed_at":"2026-08-11T13:41:23.918911Z"},"links":{"cited_paper":"/paper/2407.11263","citing_paper":"/paper/2412.12905"},"observation_digest":"sha256:e020fbb8c3c32778f812cec6cd36e328754f55fc35cb6dd66880bb9ecd0fa696","observation_id":"67f38f31-baaa-4e7a-9283-976208000060","resolution":{"observed_at":"2026-08-11T13:41:23.918911Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2407.18047","last_updated":"2025-01-07T13:04:09Z","snapshot_observed_at":"2026-08-17T08:10:09.534463Z","submitted_at":"2024-07-25T13:54:27Z","title":"Neutrino cosmology after DESI: tightest mass upper limits, preference for the normal ordering, and tension with terrestrial observations","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2407.18047","snapshot_observed_at":"2026-08-11T13:41:23.922720Z","title":"Jiang, W","venue":null,"work_id":null,"year":2024},"citing_paper":{"arxiv_id":"2412.12905","last_updated":"2025-01-25T08:30:04Z","snapshot_observed_at":"2026-08-17T16:16:24.002443Z","submitted_at":"2024-12-17T13:31:15Z","title":"DESI and SNe: Dynamical Dark Energy, $\\Omega_m$ Tension or Systematics?","version":2},"reference_index":97,"source":"pdf_text","source_observed_at":"2026-08-11T13:41:23.922720Z"},"links":{"cited_paper":"/paper/2407.18047","citing_paper":"/paper/2412.12905"},"observation_digest":"sha256:bb384ae9c142f491700032c20a8c42d38f5566d71f266692e77b1618fa1a8d13","observation_id":"78745fd0-72b6-4e5c-800e-8b9f3a3b78b4","resolution":{"observed_at":"2026-08-11T13:41:23.922720Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2408.02536","last_updated":"2024-08-05T15:08:52Z","snapshot_observed_at":"2026-08-19T16:06:45.316940Z","submitted_at":"2024-08-05T15:08:52Z","title":"Cosmological constraints from calibrated $E_p-E_{iso}$ gamma-ray burst correlation by using DESI 2024 data release","version":1},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2408.02536","snapshot_observed_at":"2026-08-11T13:41:23.926643Z","title":null,"venue":null,"work_id":null,"year":2024},"citing_paper":{"arxiv_id":"2412.12905","last_updated":"2025-01-25T08:30:04Z","snapshot_observed_at":"2026-08-17T16:16:24.002443Z","submitted_at":"2024-12-17T13:31:15Z","title":"DESI and SNe: Dynamical Dark Energy, $\\Omega_m$ Tension or Systematics?","version":2},"reference_index":98,"source":"pdf_text","source_observed_at":"2026-08-11T13:41:23.926643Z"},"links":{"cited_paper":"/paper/2408.02536","citing_paper":"/paper/2412.12905"},"observation_digest":"sha256:86b6bcdf232544889391c3e313f1b3c36ce407d69f7a789e5812fbd63c2a80ed","observation_id":"fb111aa7-a35a-4102-9e0c-a1f1a56b0289","resolution":{"observed_at":"2026-08-11T13:41:23.926643Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2411.14189","last_updated":"2024-11-21T14:58:40Z","snapshot_observed_at":"2026-08-14T16:11:56.146618Z","submitted_at":"2024-11-21T14:58:40Z","title":"Reevaluating $H_0$ Tension with Non-Planck CMB and DESI BAO Joint Analysis","version":1},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2411.14189","snapshot_observed_at":"2026-08-11T13:41:23.944879Z","title":null,"venue":null,"work_id":null,"year":2024},"citing_paper":{"arxiv_id":"2412.12905","last_updated":"2025-01-25T08:30:04Z","snapshot_observed_at":"2026-08-17T16:16:24.002443Z","submitted_at":"2024-12-17T13:31:15Z","title":"DESI and SNe: Dynamical Dark Energy, $\\Omega_m$ Tension or Systematics?","version":2},"reference_index":99,"source":"pdf_text","source_observed_at":"2026-08-11T13:41:23.944879Z"},"links":{"cited_paper":"/paper/2411.14189","citing_paper":"/paper/2412.12905"},"observation_digest":"sha256:4a728ca72bef85d1149e52fc4e7de49cb5431197ea546ac9938439decd4ba7e0","observation_id":"93c0fbf6-8e9f-428e-ad00-5cb799c3df26","resolution":{"observed_at":"2026-08-11T13:41:23.944879Z","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":"2026-08-11T13:41:23.934037Z","title":"Arjona and S","venue":null,"work_id":null,"year":2024},"citing_paper":{"arxiv_id":"2412.12905","last_updated":"2025-01-25T08:30:04Z","snapshot_observed_at":"2026-08-17T16:16:24.002443Z","submitted_at":"2024-12-17T13:31:15Z","title":"DESI and SNe: Dynamical Dark Energy, $\\Omega_m$ Tension or Systematics?","version":2},"reference_index":100,"source":"pdf_text","source_observed_at":"2026-08-11T13:41:23.934037Z"},"links":{"citing_paper":"/paper/2412.12905"},"observation_digest":"sha256:a9065f269f0523ddc0e0bb0ec09954a775d1e9b1d308b80ae76bf599c4628688","observation_id":"4c7a8531-d031-435a-852c-1ac6864686c6","resolution":{"observed_at":"2026-08-11T13:41:23.934037Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}}],"paper":{"arxiv_id":"2412.12905","last_updated":"2025-01-25T08:30:04Z","latest_version":2,"primary_category":"astro-ph.CO","snapshot_observed_at":"2026-08-17T16:16:24.002443Z","submitted_at":"2024-12-17T13:31:15Z","title":"DESI and SNe: Dynamical Dark Energy, $\\Omega_m$ Tension or Systematics?"},"reference_resolution":{"displayed":100,"state_counts":{"malformed_identifier":0,"metadata_mismatch":0,"parse_uncertain":0,"unresolved":99,"verified_exact":1,"verified_fuzzy":0},"total_outbound_references":131},"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":"2026-08-19T06:32:44.657259+00:00","source":"crossref"},{"observed_at":"2026-08-19T06:32:39.956319+00:00","source":"retraction_watch"}],"thesis":"As of 20 August 2026, this Paper Citation Record lists 100 of 131 outbound references and 44 inbound Pith citation observations for arXiv:2412.12905."}