{"as_of":"2026-08-10T20:45:00Z","caps":{"database_statements":6,"inbound":100,"outbound":100},"context_digest":"sha256:7e1964a078f139d9fa2697c815326467d3007311021873f2ae7bd943956402db","coverage":[{"denominator":101,"lane":"reference_resolution","note":"Typed states for the displayed outbound observations.","records_observed":100,"source":"paper_references, paper_reference_links","source_observed_at":"2026-08-08T23:12:26.303970Z","state":"measured"},{"denominator":135,"lane":"standing_notices","note":"One-hop event checks from named stored sources.","records_observed":135,"source":"scholarly_work_events, retraction_status_cache","source_observed_at":"2026-08-10T06:31:04.303077+00:00","state":"measured"},{"denominator":35,"lane":"inbound_itemization","note":"Pith citing papers itemized under the disclosed page cap.","records_observed":35,"source":"paper_references, paper_reference_links","source_observed_at":"2026-08-08T21:04:17.779578Z","state":"measured"},{"denominator":1,"lane":"external_citation_measurements","note":"A source-named dated measurement, never combined with another source.","records_observed":0,"source":"arxiv_reference","source_observed_at":"2026-07-04T05:19:36.214969Z","state":"measured"}],"external_citation_measurements":[],"inbound":[{"citation":{"cited_paper":{"arxiv_id":"2502.04212","last_updated":"2025-07-17T16:27:03Z","snapshot_observed_at":"2026-08-09T04:53:21.314754Z","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},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2502.04212","snapshot_observed_at":"2026-08-08T21:04:17.779578Z","title":"Huang, R.-G","venue":null,"work_id":null,"year":2024},"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":71,"source":"pdf_text","source_observed_at":"2026-08-08T21:04:17.779578Z"},"links":{"cited_paper":"/paper/2502.04212","citing_paper":"/paper/2502.04929"},"observation_digest":"sha256:0288b02e3f34d0dc7a80d541a728a6a598ad5a13bedfa609267cdeef4712fade","observation_id":"445a4a87-624c-46ce-9d68-77ce54cf518b","resolution":{"observed_at":"2026-08-08T21:04:17.779578Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2502.04212","last_updated":"2025-07-17T16:27:03Z","snapshot_observed_at":"2026-08-09T04:53:21.314754Z","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},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2502.04212","snapshot_observed_at":"2026-08-07T18:51:44.283531Z","title":"The DESI 2024 hint for dynamical dark energy is biased by low-redshift supernovae,","venue":null,"work_id":null,"year":2025},"citing_paper":{"arxiv_id":"2502.10264","last_updated":"2025-04-10T17:38:46Z","snapshot_observed_at":"2026-08-09T09:16:02.090706Z","submitted_at":"2025-02-14T16:17:23Z","title":"An overview of what current data can (and cannot yet) say about evolving dark energy","version":2},"reference_index":268,"source":"pdf_text","source_observed_at":"2026-08-07T18:51:44.283531Z"},"links":{"cited_paper":"/paper/2502.04212","citing_paper":"/paper/2502.10264"},"observation_digest":"sha256:1df269dc421ee34b668c4377efd91b3b2b8569d29ee9d7f2723b92a16909fe3d","observation_id":"f8852ea6-447a-411d-b9d5-3091da5e01d8","resolution":{"observed_at":"2026-08-07T18:51:44.283531Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2502.04212","last_updated":"2025-07-17T16:27:03Z","snapshot_observed_at":"2026-08-09T04:53:21.314754Z","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},"cited_work":{"arxiv_id":"2502.04212","doi":null,"metadata_source":"arxiv_reference","pith_arxiv_id":"2502.04212","snapshot_observed_at":"2026-07-04T05:19:36.214969Z","title":"Huang, R.-G","venue":null,"work_id":"4652291e-dffc-4ca9-bd26-bf0f3d92d3f9","year":2025},"citing_paper":{"arxiv_id":"2505.24732","last_updated":"2026-04-11T09:17:44Z","snapshot_observed_at":"2026-07-06T02:11:23.670680Z","submitted_at":"2025-05-30T15:54:16Z","title":"The Quintom theory of dark energy after DESI DR2","version":3},"reference_index":29,"source":"pdf_text","source_observed_at":"2026-05-19T13:08:20.192767Z"},"links":{"cited_paper":"/paper/2502.04212","citing_paper":"/paper/2505.24732"},"observation_digest":"sha256:3a591b882a61a24a7dc572107e07462a6c36df312ae3ba68d25772606391a069","observation_id":"d8202962-1d19-413f-b05a-100d7248950f","resolution":{"observed_at":"2026-05-19T13:12:19.267389Z","resolver_source":"arxiv_id","status":"verified_exact"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-10T06:31:04.303077+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-10T06:31:04.303077+00:00","source":"crossref"},{"observed_at":"2026-08-10T06:30:57.382061+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":{"arxiv_id":"2502.04212","last_updated":"2025-07-17T16:27:03Z","snapshot_observed_at":"2026-08-09T04:53:21.314754Z","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},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2502.04212","snapshot_observed_at":"2026-08-07T04:41:33.543751Z","title":"The DESI DR1/DR2 evidence for dynamical dark energy is biased by low-redshift supernovae,","venue":null,"work_id":null,"year":null},"citing_paper":{"arxiv_id":"2506.10075","last_updated":"2025-06-11T18:00:21Z","snapshot_observed_at":"2026-08-07T08:21:59.745367Z","submitted_at":"2025-06-11T18:00:21Z","title":"Topological defects as effective dynamical dark energy","version":1},"reference_index":6,"source":"pdf_text","source_observed_at":"2026-08-07T04:41:33.543751Z"},"links":{"cited_paper":"/paper/2502.04212","citing_paper":"/paper/2506.10075"},"observation_digest":"sha256:3ef22af93bc7316068626b10c53852446a5b1f6b297baea3ab54a86583855d3e","observation_id":"2e0fb7c9-5a6f-4d64-9be1-ad9a7b613bd2","resolution":{"observed_at":"2026-08-07T04:41:33.543751Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2502.04212","last_updated":"2025-07-17T16:27:03Z","snapshot_observed_at":"2026-08-09T04:53:21.314754Z","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},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2502.04212","snapshot_observed_at":"2026-08-06T18:36:59.471286Z","title":"Huang, R.-G","venue":null,"work_id":null,"year":2025},"citing_paper":{"arxiv_id":"2507.07798","last_updated":"2025-07-10T14:26:06Z","snapshot_observed_at":"2026-08-10T05:27:39.960371Z","submitted_at":"2025-07-10T14:26:06Z","title":"Exploring non-cold dark matter in a scenario of dynamical dark energy with DESI DR2 data","version":1},"reference_index":37,"source":"pdf_text","source_observed_at":"2026-08-06T18:36:59.471286Z"},"links":{"cited_paper":"/paper/2502.04212","citing_paper":"/paper/2507.07798"},"observation_digest":"sha256:f197829caacb2daadd8f6012ebe4a55a9bb11f3f302f6e46afa25374d3e9b046","observation_id":"c0f2a26b-8d2f-4cdb-b18a-51856afce11f","resolution":{"observed_at":"2026-08-06T18:36:59.471286Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2502.04212","last_updated":"2025-07-17T16:27:03Z","snapshot_observed_at":"2026-08-09T04:53:21.314754Z","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},"cited_work":{"arxiv_id":"2502.04212","doi":null,"metadata_source":"arxiv_reference","pith_arxiv_id":"2502.04212","snapshot_observed_at":"2026-07-04T05:19:36.214969Z","title":"Huang, R.-G","venue":null,"work_id":"4652291e-dffc-4ca9-bd26-bf0f3d92d3f9","year":2025},"citing_paper":{"arxiv_id":"2507.09981","last_updated":"2026-05-06T01:55:59Z","snapshot_observed_at":"2026-08-02T08:54:19.882729Z","submitted_at":"2025-07-14T06:55:37Z","title":"New Insights into Dark Energy from DESI DR2 with CMB and SNIa","version":2},"reference_index":36,"source":"pdf_text","source_observed_at":"2026-05-19T05:19:08.520262Z"},"links":{"cited_paper":"/paper/2502.04212","citing_paper":"/paper/2507.09981"},"observation_digest":"sha256:a07e053d9c70c70e0f77469b9822a3ee2e74e6554308b956fbfec9bdc945866a","observation_id":"9237c92e-8240-4eee-b615-256af3013964","resolution":{"observed_at":"2026-05-19T05:22:06.323883Z","resolver_source":"arxiv_id","status":"verified_exact"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-10T06:31:04.303077+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-10T06:31:04.303077+00:00","source":"crossref"},{"observed_at":"2026-08-10T06:30:57.382061+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":{"arxiv_id":"2502.04212","last_updated":"2025-07-17T16:27:03Z","snapshot_observed_at":"2026-08-09T04:53:21.314754Z","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},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2502.04212","snapshot_observed_at":"2026-08-06T15:12:33.689414Z","title":"Huang, R.-G","venue":null,"work_id":null,"year":2025},"citing_paper":{"arxiv_id":"2507.16589","last_updated":"2026-06-23T13:43:52Z","snapshot_observed_at":"2026-08-08T06:56:16.966820Z","submitted_at":"2025-07-22T13:45:38Z","title":"Cosmological preference for a positive neutrino mass at 2.7$\\sigma$: A joint analysis of DESI DR2, DESY5, and DESY1 data","version":3},"reference_index":25,"source":"pdf_text","source_observed_at":"2026-08-06T15:12:33.689414Z"},"links":{"cited_paper":"/paper/2502.04212","citing_paper":"/paper/2507.16589"},"observation_digest":"sha256:d7b21c7d8448959e687e2e24c466f8205e0fdd6c6db197b1598437c139eb21cc","observation_id":"2ecadffc-23f3-46db-9b93-7bff9b840ab6","resolution":{"observed_at":"2026-08-06T15:12:33.689414Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2502.04212","last_updated":"2025-07-17T16:27:03Z","snapshot_observed_at":"2026-08-09T04:53:21.314754Z","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},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2502.04212","snapshot_observed_at":"2026-08-06T11:39:53.276298Z","title":"Huang, R","venue":null,"work_id":null,"year":null},"citing_paper":{"arxiv_id":"2507.22575","last_updated":"2025-08-08T08:31:23Z","snapshot_observed_at":"2026-08-08T13:30:49.505565Z","submitted_at":"2025-07-30T11:02:24Z","title":"Revisiting cosmic acceleration with DESI BAO","version":2},"reference_index":78,"source":"pdf_text","source_observed_at":"2026-08-06T11:39:53.276298Z"},"links":{"cited_paper":"/paper/2502.04212","citing_paper":"/paper/2507.22575"},"observation_digest":"sha256:bb6495252333efdc5e444fad18c85966616ba3cb76f4145a72fde945567efd59","observation_id":"57744f48-8d3c-447b-9136-4ae245300e17","resolution":{"observed_at":"2026-08-06T11:39:53.276298Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2502.04212","last_updated":"2025-07-17T16:27:03Z","snapshot_observed_at":"2026-08-09T04:53:21.314754Z","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},"cited_work":{"arxiv_id":"2502.04212","doi":null,"metadata_source":"arxiv_reference","pith_arxiv_id":"2502.04212","snapshot_observed_at":"2026-07-04T05:19:36.214969Z","title":"Huang, R.-G","venue":null,"work_id":"4652291e-dffc-4ca9-bd26-bf0f3d92d3f9","year":2025},"citing_paper":{"arxiv_id":"2509.09202","last_updated":"2026-04-12T17:53:51Z","snapshot_observed_at":"2026-07-06T22:28:38.311664Z","submitted_at":"2025-09-11T07:18:09Z","title":"Interacting $k$-essence field with non-pressureless Dark Matter: Cosmological Dynamics and Observational Constraints","version":2},"reference_index":40,"source":"pdf_text","source_observed_at":"2026-05-18T18:14:18.793821Z"},"links":{"cited_paper":"/paper/2502.04212","citing_paper":"/paper/2509.09202"},"observation_digest":"sha256:e0e3107ff1fa4edca0159079cfe498ab07bddbd49399c531eef6adb85c436910","observation_id":"2fd1c9f4-b2be-4eec-956c-f1f2641b148f","resolution":{"observed_at":"2026-05-18T18:16:43.651730Z","resolver_source":"arxiv_id","status":"verified_exact"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-10T06:31:04.303077+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-10T06:31:04.303077+00:00","source":"crossref"},{"observed_at":"2026-08-10T06:30:57.382061+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":{"arxiv_id":"2502.04212","last_updated":"2025-07-17T16:27:03Z","snapshot_observed_at":"2026-08-09T04:53:21.314754Z","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},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2502.04212","snapshot_observed_at":"2026-08-04T13:43:12.226732Z","title":"Huang, R.-G","venue":null,"work_id":null,"year":2025},"citing_paper":{"arxiv_id":"2509.25812","last_updated":"2026-07-24T17:00:01Z","snapshot_observed_at":"2026-08-06T01:07:38.127403Z","submitted_at":"2025-09-30T05:41:44Z","title":"Updated observational constraints on $\\phi$CDM dynamical dark energy cosmological models","version":3},"reference_index":29,"source":"pdf_text","source_observed_at":"2026-08-04T13:43:12.226732Z"},"links":{"cited_paper":"/paper/2502.04212","citing_paper":"/paper/2509.25812"},"observation_digest":"sha256:2bb4c26720ed009f8e8635cf3c9f51d2847ef445aff571c71106d6b166731f66","observation_id":"44e4e4e1-c973-4dae-8fa7-91ad1f8ce86c","resolution":{"observed_at":"2026-08-04T13:43:12.226732Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2502.04212","last_updated":"2025-07-17T16:27:03Z","snapshot_observed_at":"2026-08-09T04:53:21.314754Z","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},"cited_work":{"arxiv_id":"2502.04212","doi":null,"metadata_source":"arxiv_reference","pith_arxiv_id":"2502.04212","snapshot_observed_at":"2026-07-04T05:19:36.214969Z","title":"Huang, R.-G","venue":null,"work_id":"4652291e-dffc-4ca9-bd26-bf0f3d92d3f9","year":2025},"citing_paper":{"arxiv_id":"2510.04179","last_updated":"2026-06-10T06:51:56Z","snapshot_observed_at":"2026-08-05T23:09:35.681983Z","submitted_at":"2025-10-05T12:41:23Z","title":"Crosschecking Cosmic Distances from DESI BAO and DES SNe","version":3},"reference_index":55,"source":"pdf_text","source_observed_at":"2026-05-18T10:32:00.438157Z"},"links":{"cited_paper":"/paper/2502.04212","citing_paper":"/paper/2510.04179"},"observation_digest":"sha256:aba1617cc1fba72e38cce04658f31d2dd92c9d70105906fb327f20797da346fb","observation_id":"70c35886-05bb-46c5-8639-dec1c1d7f3bb","resolution":{"observed_at":"2026-05-18T10:32:33.733026Z","resolver_source":"arxiv_id","status":"verified_exact"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-10T06:31:04.303077+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-10T06:31:04.303077+00:00","source":"crossref"},{"observed_at":"2026-08-10T06:30:57.382061+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":{"arxiv_id":"2502.04212","last_updated":"2025-07-17T16:27:03Z","snapshot_observed_at":"2026-08-09T04:53:21.314754Z","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},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2502.04212","snapshot_observed_at":"2026-08-04T11:34:12.869859Z","title":"Huang, R.-G","venue":null,"work_id":null,"year":2025},"citing_paper":{"arxiv_id":"2510.04179","last_updated":"2026-06-10T06:51:56Z","snapshot_observed_at":"2026-08-05T23:09:35.681983Z","submitted_at":"2025-10-05T12:41:23Z","title":"Crosschecking Cosmic Distances from DESI BAO and DES SNe","version":4},"reference_index":55,"source":"pdf_text","source_observed_at":"2026-08-04T11:34:12.869859Z"},"links":{"cited_paper":"/paper/2502.04212","citing_paper":"/paper/2510.04179"},"observation_digest":"sha256:05c678b26d1475ed9d9f63b761dcb94232b9c431c297fe9ae04907a8e5a20439","observation_id":"0c231518-0685-4b6a-9ad7-231e805d03eb","resolution":{"observed_at":"2026-08-04T11:34:12.869859Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2502.04212","last_updated":"2025-07-17T16:27:03Z","snapshot_observed_at":"2026-08-09T04:53:21.314754Z","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},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2502.04212","snapshot_observed_at":"2026-08-04T09:59:22.769194Z","title":"Huang, R.-G","venue":null,"work_id":null,"year":2025},"citing_paper":{"arxiv_id":"2510.12627","last_updated":"2026-06-20T07:00:45Z","snapshot_observed_at":"2026-08-07T12:03:55.381688Z","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":125,"source":"pdf_text","source_observed_at":"2026-08-04T09:59:22.769194Z"},"links":{"cited_paper":"/paper/2502.04212","citing_paper":"/paper/2510.12627"},"observation_digest":"sha256:401d1fe99d6e53d246720f939bb31d950e10507a1ec612dfd56e7563de18a8a3","observation_id":"b0265588-bbdf-4def-baaf-96333d6a9fa1","resolution":{"observed_at":"2026-08-04T09:59:22.769194Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2502.04212","last_updated":"2025-07-17T16:27:03Z","snapshot_observed_at":"2026-08-09T04:53:21.314754Z","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},"cited_work":{"arxiv_id":"2502.04212","doi":null,"metadata_source":"arxiv_reference","pith_arxiv_id":"2502.04212","snapshot_observed_at":"2026-07-04T05:19:36.214969Z","title":"Huang, R.-G","venue":null,"work_id":"4652291e-dffc-4ca9-bd26-bf0f3d92d3f9","year":2025},"citing_paper":{"arxiv_id":"2510.14888","last_updated":"2026-04-08T20:26:41Z","snapshot_observed_at":"2026-08-08T04:42:19.696993Z","submitted_at":"2025-10-16T17:07:57Z","title":"Modeling nonlinear scales for dynamical dark energy cosmologies with COLA","version":2},"reference_index":69,"source":"pdf_text","source_observed_at":"2026-05-18T06:13:13.345307Z"},"links":{"cited_paper":"/paper/2502.04212","citing_paper":"/paper/2510.14888"},"observation_digest":"sha256:68ea0888f0e9b5cabc386bca060d027949144367064dd00ba213d284161291fc","observation_id":"856f41ef-ed6c-488d-b64d-6ab76b783046","resolution":{"observed_at":"2026-05-18T06:15:58.557461Z","resolver_source":"arxiv_id","status":"verified_exact"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-10T06:31:04.303077+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-10T06:31:04.303077+00:00","source":"crossref"},{"observed_at":"2026-08-10T06:30:57.382061+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":{"arxiv_id":"2502.04212","last_updated":"2025-07-17T16:27:03Z","snapshot_observed_at":"2026-08-09T04:53:21.314754Z","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},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2502.04212","snapshot_observed_at":"2026-08-04T07:19:40.270534Z","title":"Huang, R.-G","venue":null,"work_id":null,"year":2025},"citing_paper":{"arxiv_id":"2510.26355","last_updated":"2026-07-07T01:20:38Z","snapshot_observed_at":"2026-08-07T08:46:25.463224Z","submitted_at":"2025-10-30T11:06:11Z","title":"Model-independent late-universe measurements of $H_0$ and $\\Omega_K$ with the parametrization based on cosmic age-improved inverse distance ladder","version":2},"reference_index":95,"source":"pdf_text","source_observed_at":"2026-08-04T07:19:40.270534Z"},"links":{"cited_paper":"/paper/2502.04212","citing_paper":"/paper/2510.26355"},"observation_digest":"sha256:72c07025966e29fbf5786b448224b5e3893ce48e194591192c2f40df42fce763","observation_id":"0967bca4-967c-4872-b138-ffefed32722f","resolution":{"observed_at":"2026-08-04T07:19:40.270534Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2502.04212","last_updated":"2025-07-17T16:27:03Z","snapshot_observed_at":"2026-08-09T04:53:21.314754Z","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},"cited_work":{"arxiv_id":"2502.04212","doi":null,"metadata_source":"arxiv_reference","pith_arxiv_id":"2502.04212","snapshot_observed_at":"2026-07-04T05:19:36.214969Z","title":"Huang, R.-G","venue":null,"work_id":"4652291e-dffc-4ca9-bd26-bf0f3d92d3f9","year":2025},"citing_paper":{"arxiv_id":"2511.09467","last_updated":"2026-03-30T07:50:13Z","snapshot_observed_at":"2026-08-03T06:16:33.350640Z","submitted_at":"2025-11-12T16:39:04Z","title":"Revisiting the Hubble tension problem in the framework of holographic dark energy","version":2},"reference_index":54,"source":"pdf_text","source_observed_at":"2026-05-17T22:17:32.138764Z"},"links":{"cited_paper":"/paper/2502.04212","citing_paper":"/paper/2511.09467"},"observation_digest":"sha256:e14a1ea005ae665d4024efb49b416a2a31c7e38c08bf2fa3805d72d718d37bd1","observation_id":"07740211-d852-464b-b784-4b1159124992","resolution":{"observed_at":"2026-05-17T22:20:23.798078Z","resolver_source":"arxiv_id","status":"verified_exact"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-10T06:31:04.303077+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-10T06:31:04.303077+00:00","source":"crossref"},{"observed_at":"2026-08-10T06:30:57.382061+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":{"arxiv_id":"2502.04212","last_updated":"2025-07-17T16:27:03Z","snapshot_observed_at":"2026-08-09T04:53:21.314754Z","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},"cited_work":{"arxiv_id":"2502.04212","doi":null,"metadata_source":"arxiv_reference","pith_arxiv_id":"2502.04212","snapshot_observed_at":"2026-07-04T05:19:36.214969Z","title":"Huang, R.-G","venue":null,"work_id":"4652291e-dffc-4ca9-bd26-bf0f3d92d3f9","year":2025},"citing_paper":{"arxiv_id":"2511.20757","last_updated":"2026-04-14T17:58:15Z","snapshot_observed_at":"2026-07-06T22:36:59.311174Z","submitted_at":"2025-11-25T19:00:04Z","title":"Reanalyzing DESI DR1: 2. Constraints on Dark Energy, Spatial Curvature, and Neutrino Masses","version":2},"reference_index":27,"source":"pdf_text","source_observed_at":"2026-05-17T04:15:18.730245Z"},"links":{"cited_paper":"/paper/2502.04212","citing_paper":"/paper/2511.20757"},"observation_digest":"sha256:6ece082101f4550ebd37120d8451b8b18db2ee4d37ff4474e878b59b5a6ce1d7","observation_id":"d960720e-ca59-49b6-b511-2e203f5a6581","resolution":{"observed_at":"2026-05-17T04:19:00.920329Z","resolver_source":"arxiv_id","status":"verified_exact"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-10T06:31:04.303077+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-10T06:31:04.303077+00:00","source":"crossref"},{"observed_at":"2026-08-10T06:30:57.382061+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":{"arxiv_id":"2502.04212","last_updated":"2025-07-17T16:27:03Z","snapshot_observed_at":"2026-08-09T04:53:21.314754Z","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},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2502.04212","snapshot_observed_at":"2026-08-03T20:12:23.338390Z","title":"Huang, R.-G","venue":null,"work_id":null,"year":2024},"citing_paper":{"arxiv_id":"2511.21071","last_updated":"2026-06-27T14:06:53Z","snapshot_observed_at":"2026-08-08T22:41:12.425390Z","submitted_at":"2025-11-26T05:26:01Z","title":"Cosmological tensions in Proca-Nuevo theory","version":2},"reference_index":17,"source":"pdf_text","source_observed_at":"2026-08-03T20:12:23.338390Z"},"links":{"cited_paper":"/paper/2502.04212","citing_paper":"/paper/2511.21071"},"observation_digest":"sha256:2acde0c91387833aeac921cea416445e8256dbda87d9b6f21cd1a4a02ace4e6f","observation_id":"b8466c79-980e-434b-abf6-38ca6c56517c","resolution":{"observed_at":"2026-08-03T20:12:23.338390Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2502.04212","last_updated":"2025-07-17T16:27:03Z","snapshot_observed_at":"2026-08-09T04:53:21.314754Z","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},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2502.04212","snapshot_observed_at":"2026-08-03T18:51:46.766290Z","title":"Huang, R","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":85,"source":"pdf_text","source_observed_at":"2026-08-03T18:51:46.766290Z"},"links":{"cited_paper":"/paper/2502.04212","citing_paper":"/paper/2512.04130"},"observation_digest":"sha256:c182d6f6904d75dd9783e4bbff358c4be6dd24ad261b074e1840798318915d98","observation_id":"1c1afff0-988e-44c2-85a1-9196a484301e","resolution":{"observed_at":"2026-08-03T18:51:46.766290Z","resolver_source":null,"status":"malformed_identifier"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2502.04212","last_updated":"2025-07-17T16:27:03Z","snapshot_observed_at":"2026-08-09T04:53:21.314754Z","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},"cited_work":{"arxiv_id":"2502.04212","doi":null,"metadata_source":"arxiv_reference","pith_arxiv_id":"2502.04212","snapshot_observed_at":"2026-07-04T05:19:36.214969Z","title":"Huang, R.-G","venue":null,"work_id":"4652291e-dffc-4ca9-bd26-bf0f3d92d3f9","year":2025},"citing_paper":{"arxiv_id":"2602.03110","last_updated":"2026-04-28T09:37:14Z","snapshot_observed_at":"2026-08-09T16:54:12.160048Z","submitted_at":"2026-02-03T05:11:50Z","title":"Evidence for deviation in gravitational light deflection from general relativity at cosmological scales with KiDS-Legacy and CMB lensing","version":2},"reference_index":68,"source":"pdf_text","source_observed_at":"2026-05-16T08:17:34.164338Z"},"links":{"cited_paper":"/paper/2502.04212","citing_paper":"/paper/2602.03110"},"observation_digest":"sha256:ac50b167bffd0d7702c1be395c72598d2e0234e5f62cd78ec17ead024c7c6d87","observation_id":"c9605df0-0871-4f7e-8ebc-2e8f7f1e764c","resolution":{"observed_at":"2026-05-16T08:17:35.788628Z","resolver_source":"arxiv_id","status":"verified_exact"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-10T06:31:04.303077+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-10T06:31:04.303077+00:00","source":"crossref"},{"observed_at":"2026-08-10T06:30:57.382061+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":{"arxiv_id":"2502.04212","last_updated":"2025-07-17T16:27:03Z","snapshot_observed_at":"2026-08-09T04:53:21.314754Z","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},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2502.04212","snapshot_observed_at":"2026-08-02T22:16:52.733530Z","title":"Huang, R.-G","venue":null,"work_id":null,"year":2025},"citing_paper":{"arxiv_id":"2602.17644","last_updated":"2026-07-21T14:05:04Z","snapshot_observed_at":"2026-08-06T06:36:14.515098Z","submitted_at":"2026-02-19T18:54:23Z","title":"Cosmic voids evolution in modified gravity via hydrodynamics","version":2},"reference_index":28,"source":"pdf_text","source_observed_at":"2026-08-02T22:16:52.733530Z"},"links":{"cited_paper":"/paper/2502.04212","citing_paper":"/paper/2602.17644"},"observation_digest":"sha256:0b88580b42854c22bfe29ad8fd9ef016a441920069c367edbf328f49ea0d7b73","observation_id":"cca71284-e26b-46a6-ac69-2809d4fdbadf","resolution":{"observed_at":"2026-08-02T22:16:52.733530Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2502.04212","last_updated":"2025-07-17T16:27:03Z","snapshot_observed_at":"2026-08-09T04:53:21.314754Z","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},"cited_work":{"arxiv_id":"2502.04212","doi":null,"metadata_source":"arxiv_reference","pith_arxiv_id":"2502.04212","snapshot_observed_at":"2026-07-04T05:19:36.214969Z","title":"Huang, R.-G","venue":null,"work_id":"4652291e-dffc-4ca9-bd26-bf0f3d92d3f9","year":2025},"citing_paper":{"arxiv_id":"2603.10787","last_updated":"2026-03-11T14:00:06Z","snapshot_observed_at":"2026-07-06T22:48:39.649787Z","submitted_at":"2026-03-11T14:00:06Z","title":"Measuring neutrino mass in light of ACT DR6 and DESI DR2","version":1},"reference_index":41,"source":"pdf_text","source_observed_at":"2026-05-15T13:14:03.491513Z"},"links":{"cited_paper":"/paper/2502.04212","citing_paper":"/paper/2603.10787"},"observation_digest":"sha256:8aca73e4c8ccbf41a6177b18ed202630c917c92cd75a53ce01383884d05dc5cc","observation_id":"1f838d2f-4f71-4bf2-aa64-6fd87870a24e","resolution":{"observed_at":"2026-05-15T13:15:50.405465Z","resolver_source":"arxiv_id","status":"verified_exact"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-10T06:31:04.303077+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-10T06:31:04.303077+00:00","source":"crossref"},{"observed_at":"2026-08-10T06:30:57.382061+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":{"arxiv_id":"2502.04212","last_updated":"2025-07-17T16:27:03Z","snapshot_observed_at":"2026-08-09T04:53:21.314754Z","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},"cited_work":{"arxiv_id":"2502.04212","doi":null,"metadata_source":"arxiv_reference","pith_arxiv_id":"2502.04212","snapshot_observed_at":"2026-07-04T05:19:36.214969Z","title":"Huang, R.-G","venue":null,"work_id":"4652291e-dffc-4ca9-bd26-bf0f3d92d3f9","year":2025},"citing_paper":{"arxiv_id":"2604.02204","last_updated":"2026-04-09T15:37:40Z","snapshot_observed_at":"2026-07-06T02:11:23.670680Z","submitted_at":"2026-04-02T15:57:57Z","title":"Non-minimally coupled quintessence with sign-switching interaction","version":2},"reference_index":27,"source":"pdf_text","source_observed_at":"2026-05-13T20:44:54.743879Z"},"links":{"cited_paper":"/paper/2502.04212","citing_paper":"/paper/2604.02204"},"observation_digest":"sha256:79ff7ba9ad91311975936a68c7cfa4c9c2e3625bdf6def39416457bf19d684a3","observation_id":"b9d9cb6c-f512-48c7-8389-9759e346b147","resolution":{"observed_at":"2026-05-13T20:48:15.306591Z","resolver_source":"arxiv_id","status":"metadata_mismatch"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-10T06:31:04.303077+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-10T06:31:04.303077+00:00","source":"crossref"},{"observed_at":"2026-08-10T06:30:57.382061+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":{"arxiv_id":"2502.04212","last_updated":"2025-07-17T16:27:03Z","snapshot_observed_at":"2026-08-09T04:53:21.314754Z","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},"cited_work":{"arxiv_id":"2502.04212","doi":null,"metadata_source":"arxiv_reference","pith_arxiv_id":"2502.04212","snapshot_observed_at":"2026-07-04T05:19:36.214969Z","title":"Huang, R.-G","venue":null,"work_id":"4652291e-dffc-4ca9-bd26-bf0f3d92d3f9","year":2025},"citing_paper":{"arxiv_id":"2604.11883","last_updated":"2026-04-13T18:00:02Z","snapshot_observed_at":"2026-07-06T02:11:23.670680Z","submitted_at":"2026-04-13T18:00:02Z","title":"Model-Independent Analysis of Type Ia Supernova Datasets and Implications for Dark Energy","version":1},"reference_index":40,"source":"pdf_text","source_observed_at":"2026-05-10T16:10:57.497230Z"},"links":{"cited_paper":"/paper/2502.04212","citing_paper":"/paper/2604.11883"},"observation_digest":"sha256:6bc19747a1baba6cd666d996750acb838e862caab204a8dec5929dd680041cfb","observation_id":"46102c81-fa72-42dc-a04a-bf238462f462","resolution":{"observed_at":"2026-05-11T09:11:06.200278Z","resolver_source":"arxiv_id","status":"verified_exact"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-10T06:31:04.303077+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-10T06:31:04.303077+00:00","source":"crossref"},{"observed_at":"2026-08-10T06:30:57.382061+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":{"arxiv_id":"2502.04212","last_updated":"2025-07-17T16:27:03Z","snapshot_observed_at":"2026-08-09T04:53:21.314754Z","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},"cited_work":{"arxiv_id":"2502.04212","doi":null,"metadata_source":"arxiv_reference","pith_arxiv_id":"2502.04212","snapshot_observed_at":"2026-07-04T05:19:36.214969Z","title":"Huang, R.-G","venue":null,"work_id":"4652291e-dffc-4ca9-bd26-bf0f3d92d3f9","year":2025},"citing_paper":{"arxiv_id":"2604.28013","last_updated":"2026-04-30T15:31:57Z","snapshot_observed_at":"2026-07-06T23:13:20.516759Z","submitted_at":"2026-04-30T15:31:57Z","title":"Cosmological intercept tension","version":1},"reference_index":33,"source":"pdf_text","source_observed_at":"2026-05-07T05:59:51.789689Z"},"links":{"cited_paper":"/paper/2502.04212","citing_paper":"/paper/2604.28013"},"observation_digest":"sha256:9c8f7acebc4e149b8db87f1c2162ba4c15dbfcebe1e408d8d5d6649d6ef18051","observation_id":"82a26c30-b283-4057-a80e-49647563d71a","resolution":{"observed_at":"2026-05-12T10:26:30.655901Z","resolver_source":"arxiv_id","status":"verified_exact"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-10T06:31:04.303077+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-10T06:31:04.303077+00:00","source":"crossref"},{"observed_at":"2026-08-10T06:30:57.382061+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":{"arxiv_id":"2502.04212","last_updated":"2025-07-17T16:27:03Z","snapshot_observed_at":"2026-08-09T04:53:21.314754Z","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},"cited_work":{"arxiv_id":"2502.04212","doi":null,"metadata_source":"arxiv_reference","pith_arxiv_id":"2502.04212","snapshot_observed_at":"2026-07-04T05:19:36.214969Z","title":"Huang, R.-G","venue":null,"work_id":"4652291e-dffc-4ca9-bd26-bf0f3d92d3f9","year":2025},"citing_paper":{"arxiv_id":"2606.01360","last_updated":"2026-07-18T02:00:49Z","snapshot_observed_at":"2026-08-10T03:45:11.694932Z","submitted_at":"2026-05-31T17:31:59Z","title":"A short review on Quintom dark energy theory","version":1},"reference_index":47,"source":"pdf_text","source_observed_at":"2026-06-28T16:17:39.285285Z"},"links":{"cited_paper":"/paper/2502.04212","citing_paper":"/paper/2606.01360"},"observation_digest":"sha256:605214b6a1e8ded7d75a05406a019431ac2f09a6469670c23071bc3b9c3d8d22","observation_id":"1171d055-7083-4366-a3ae-4790764b665a","resolution":{"observed_at":"2026-07-01T21:46:16.136804Z","resolver_source":"arxiv_id","status":"verified_exact"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-10T06:31:04.303077+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-10T06:31:04.303077+00:00","source":"crossref"},{"observed_at":"2026-08-10T06:30:57.382061+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":{"arxiv_id":"2502.04212","last_updated":"2025-07-17T16:27:03Z","snapshot_observed_at":"2026-08-09T04:53:21.314754Z","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},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2502.04212","snapshot_observed_at":"2026-08-02T12:40:03.192153Z","title":"Huang, R.-G","venue":null,"work_id":null,"year":2025},"citing_paper":{"arxiv_id":"2606.01360","last_updated":"2026-07-18T02:00:49Z","snapshot_observed_at":"2026-08-10T03:45:11.694932Z","submitted_at":"2026-05-31T17:31:59Z","title":"A short review on Quintom dark energy theory","version":2},"reference_index":47,"source":"pdf_text","source_observed_at":"2026-08-02T12:40:03.192153Z"},"links":{"cited_paper":"/paper/2502.04212","citing_paper":"/paper/2606.01360"},"observation_digest":"sha256:c86ca6f9aa85dafab80bc5c02d97f63fbfe8a0a2d1442bcef8aebbd43f9c4c7c","observation_id":"0638205c-2a92-4b46-8bd0-101d90042369","resolution":{"observed_at":"2026-08-02T12:40:03.192153Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2502.04212","last_updated":"2025-07-17T16:27:03Z","snapshot_observed_at":"2026-08-09T04:53:21.314754Z","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},"cited_work":{"arxiv_id":"2502.04212","doi":null,"metadata_source":"arxiv_reference","pith_arxiv_id":"2502.04212","snapshot_observed_at":"2026-07-04T05:19:36.214969Z","title":"Huang, R.-G","venue":null,"work_id":"4652291e-dffc-4ca9-bd26-bf0f3d92d3f9","year":2025},"citing_paper":{"arxiv_id":"2606.05005","last_updated":"2026-06-03T15:26:36Z","snapshot_observed_at":"2026-07-06T23:45:02.342193Z","submitted_at":"2026-06-03T15:26:36Z","title":"Neutrino mass constraints in interacting dark energy models after DESI DR2","version":1},"reference_index":74,"source":"pdf_text","source_observed_at":"2026-06-28T04:52:33.342231Z"},"links":{"cited_paper":"/paper/2502.04212","citing_paper":"/paper/2606.05005"},"observation_digest":"sha256:c0f677194b59bae077137e18ecce51ee0cd1bdd848ed50517c01ab6b88959f10","observation_id":"ea20f16a-b098-4b00-8fc9-6af32b8d99c3","resolution":{"observed_at":"2026-07-02T10:56:52.301532Z","resolver_source":"arxiv_id","status":"verified_exact"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-10T06:31:04.303077+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-10T06:31:04.303077+00:00","source":"crossref"},{"observed_at":"2026-08-10T06:30:57.382061+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":{"arxiv_id":"2502.04212","last_updated":"2025-07-17T16:27:03Z","snapshot_observed_at":"2026-08-09T04:53:21.314754Z","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},"cited_work":{"arxiv_id":"2502.04212","doi":null,"metadata_source":"arxiv_reference","pith_arxiv_id":"2502.04212","snapshot_observed_at":"2026-07-04T05:19:36.214969Z","title":"Huang, R.-G","venue":null,"work_id":"4652291e-dffc-4ca9-bd26-bf0f3d92d3f9","year":2025},"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":55,"source":"pdf_text","source_observed_at":"2026-06-27T06:23:50.957273Z"},"links":{"cited_paper":"/paper/2502.04212","citing_paper":"/paper/2606.12822"},"observation_digest":"sha256:fa9961a5888929252f2651f105cc60923fd57a31d3e5d549a8a192d9dcc780fd","observation_id":"4bfbb58f-64d4-48d7-838d-8e4ca29eea10","resolution":{"observed_at":"2026-07-03T15:38:33.955667Z","resolver_source":"arxiv_id","status":"verified_exact"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-10T06:31:04.303077+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-10T06:31:04.303077+00:00","source":"crossref"},{"observed_at":"2026-08-10T06:30:57.382061+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":{"arxiv_id":"2502.04212","last_updated":"2025-07-17T16:27:03Z","snapshot_observed_at":"2026-08-09T04:53:21.314754Z","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},"cited_work":{"arxiv_id":"2502.04212","doi":null,"metadata_source":"arxiv_reference","pith_arxiv_id":"2502.04212","snapshot_observed_at":"2026-07-04T05:19:36.214969Z","title":"Huang, R.-G","venue":null,"work_id":"4652291e-dffc-4ca9-bd26-bf0f3d92d3f9","year":2025},"citing_paper":{"arxiv_id":"2606.20434","last_updated":"2026-07-14T16:58:56Z","snapshot_observed_at":"2026-07-17T23:19:04.117001Z","submitted_at":"2026-06-18T16:12:11Z","title":"The Hubble tension: A decade review","version":1},"reference_index":116,"source":"pdf_text","source_observed_at":"2026-06-26T16:04:43.230344Z"},"links":{"cited_paper":"/paper/2502.04212","citing_paper":"/paper/2606.20434"},"observation_digest":"sha256:5cb37b8fdedda65bc25f0bea0e523914e211580dcfa093b2b5ba8b4efcebe99c","observation_id":"3fad8716-c098-4783-a93e-c337925a4a8b","resolution":{"observed_at":"2026-07-04T05:19:36.216372Z","resolver_source":"arxiv_id","status":"verified_exact"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-10T06:31:04.303077+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-10T06:31:04.303077+00:00","source":"crossref"},{"observed_at":"2026-08-10T06:30:57.382061+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":{"arxiv_id":"2502.04212","last_updated":"2025-07-17T16:27:03Z","snapshot_observed_at":"2026-08-09T04:53:21.314754Z","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},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2502.04212","snapshot_observed_at":"2026-07-15T10:41:50.733215Z","title":"Huang, R.-G","venue":null,"work_id":null,"year":2025},"citing_paper":{"arxiv_id":"2606.20434","last_updated":"2026-07-14T16:58:56Z","snapshot_observed_at":"2026-07-17T23:19:04.117001Z","submitted_at":"2026-06-18T16:12:11Z","title":"The Hubble tension: A decade review","version":2},"reference_index":116,"source":"pdf_text","source_observed_at":"2026-07-15T10:41:50.733215Z"},"links":{"cited_paper":"/paper/2502.04212","citing_paper":"/paper/2606.20434"},"observation_digest":"sha256:0ddbf43e21f66faaf6bc1dacaccfb9a39a466babfffbda2a539bb76f0ff3de37","observation_id":"6cb54a05-9714-42fa-8d31-f688a3a4ade2","resolution":{"observed_at":"2026-07-15T10:41:50.733215Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2502.04212","last_updated":"2025-07-17T16:27:03Z","snapshot_observed_at":"2026-08-09T04:53:21.314754Z","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},"cited_work":{"arxiv_id":"2502.04212","doi":null,"metadata_source":"arxiv_reference","pith_arxiv_id":"2502.04212","snapshot_observed_at":"2026-07-04T05:19:36.214969Z","title":"Huang, R.-G","venue":null,"work_id":"4652291e-dffc-4ca9-bd26-bf0f3d92d3f9","year":2025},"citing_paper":{"arxiv_id":"2607.01226","last_updated":"2026-07-01T17:57:32Z","snapshot_observed_at":"2026-08-09T06:10:45.071570Z","submitted_at":"2026-07-01T17:57:32Z","title":"Intertwined Constraints in Extended Cosmologies: Dark Energy, Curvature, Neutrinos, and Inflation","version":1},"reference_index":202,"source":"pdf_text","source_observed_at":"2026-07-02T06:14:20.101706Z"},"links":{"cited_paper":"/paper/2502.04212","citing_paper":"/paper/2607.01226"},"observation_digest":"sha256:7bf9f28511808b668fccb7f938791bc9d015eaccf6e79d95fea87978849e6be9","observation_id":"110b0434-add3-43d6-b9d7-98f73fea4e13","resolution":{"observed_at":"2026-07-02T06:16:43.426365Z","resolver_source":"arxiv_id","status":"verified_exact"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-10T06:31:04.303077+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-10T06:31:04.303077+00:00","source":"crossref"},{"observed_at":"2026-08-10T06:30:57.382061+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":{"arxiv_id":"2502.04212","last_updated":"2025-07-17T16:27:03Z","snapshot_observed_at":"2026-08-09T04:53:21.314754Z","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},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2502.04212","snapshot_observed_at":"2026-07-12T04:18:55.037825Z","title":"Huang, R.-G","venue":null,"work_id":null,"year":2025},"citing_paper":{"arxiv_id":"2607.03183","last_updated":"2026-07-03T10:38:35Z","snapshot_observed_at":"2026-08-09T00:31:45.734870Z","submitted_at":"2026-07-03T10:38:35Z","title":"Neutrino mass constraints in the Schwarzschild-de Sitter black-hole dark energy model with ACT DR6 and DESI DR2 data","version":1},"reference_index":105,"source":"pdf_text","source_observed_at":"2026-07-12T04:18:55.037825Z"},"links":{"cited_paper":"/paper/2502.04212","citing_paper":"/paper/2607.03183"},"observation_digest":"sha256:55a1ae8fd021d0f63f74b1e8a108bbdae05b7a78b37b04704d5ef062cfcac2cf","observation_id":"f1f262c4-2a5a-4680-9795-3234fcf92244","resolution":{"observed_at":"2026-07-12T04:18:55.037825Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2502.04212","last_updated":"2025-07-17T16:27:03Z","snapshot_observed_at":"2026-08-09T04:53:21.314754Z","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},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2502.04212","snapshot_observed_at":"2026-08-01T07:20:07.676060Z","title":"The DESI DR1/DR2 evidence for dy- namical dark energy is biased by low-redshift supernovae,","venue":null,"work_id":null,"year":2025},"citing_paper":{"arxiv_id":"2607.21497","last_updated":"2026-07-23T16:45:10Z","snapshot_observed_at":"2026-08-09T21:28:10.481411Z","submitted_at":"2026-07-23T16:45:10Z","title":"Hubble tension: a short review of theoretical explanations","version":1},"reference_index":69,"source":"pdf_text","source_observed_at":"2026-08-01T07:20:07.676060Z"},"links":{"cited_paper":"/paper/2502.04212","citing_paper":"/paper/2607.21497"},"observation_digest":"sha256:1573fcb51d3d6243e71b76045bd4fb6e9350787492d062e330afc4875c1c8e96","observation_id":"63e8dbb4-99bc-409b-88e4-1884362ef377","resolution":{"observed_at":"2026-08-01T07:20:07.676060Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2502.04212","last_updated":"2025-07-17T16:27:03Z","snapshot_observed_at":"2026-08-09T04:53:21.314754Z","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},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2502.04212","snapshot_observed_at":"2026-08-08T19:17:22.415775Z","title":"Huang, R.G","venue":null,"work_id":null,"year":2025},"citing_paper":{"arxiv_id":"2608.04353","last_updated":"2026-08-05T01:54:49Z","snapshot_observed_at":"2026-08-09T04:13:26.478945Z","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":19,"source":"pdf_text","source_observed_at":"2026-08-08T19:17:22.415775Z"},"links":{"cited_paper":"/paper/2502.04212","citing_paper":"/paper/2608.04353"},"observation_digest":"sha256:4051ed8411f5c1157f3e056c59ca7d934ea61c4793a13686e939ba3e001a1794","observation_id":"22d4d46d-e0b8-40a1-b223-7ff67a005150","resolution":{"observed_at":"2026-08-08T19:17:22.415775Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}}],"links":{"evidence":"/evidence","html":"/paper/2502.04212/citation-record","integrity":"/paper/2502.04212/integrity","json":"/paper/2502.04212/citation-record.json","paper":"/paper/2502.04212"},"outbound":[{"citation":{"cited_paper":{"arxiv_id":"astro-ph/9805201","last_updated":"1998-05-15T03:59:02Z","snapshot_observed_at":"2026-08-04T06:34:53.046342Z","submitted_at":"1998-05-15T03:59:02Z","title":"Observational Evidence from Supernovae for an Accelerating Universe and a Cosmological Constant","version":1},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"astro-ph/9805201","snapshot_observed_at":"2026-08-08T23:12:25.940113Z","title":"Ob- servational evidence from supernovae for an accelerating universe and a cosmological constant,","venue":null,"work_id":null,"year":1998},"citing_paper":{"arxiv_id":"2502.04212","last_updated":"2025-07-17T16:27:03Z","snapshot_observed_at":"2026-08-09T04:53:21.314754Z","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":1,"source":"pdf_text","source_observed_at":"2026-08-08T23:12:25.940113Z"},"links":{"cited_paper":"/paper/astro-ph/9805201","citing_paper":"/paper/2502.04212"},"observation_digest":"sha256:fed5d3ae1e652e8d00a4cc10ffddac98d3d4de0868018dc6de3de69bde78b800","observation_id":"e71ad952-d21d-470f-8233-5ff29a784a09","resolution":{"observed_at":"2026-08-08T23:12:25.940113Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"astro-ph/0501171","last_updated":"2005-01-10T21:25:29Z","snapshot_observed_at":"2026-07-07T00:47:26.027972Z","submitted_at":"2005-01-10T21:25:29Z","title":"Detection of the Baryon Acoustic Peak in the Large-Scale Correlation Function of SDSS Luminous Red Galaxies","version":1},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"astro-ph/0501171","snapshot_observed_at":"2026-08-08T23:12:25.944703Z","title":"Detection of the Baryon Acoustic Peak in the Large-Scale Correlation Function of SDSS Luminous Red Galaxies,","venue":null,"work_id":null,"year":2005},"citing_paper":{"arxiv_id":"2502.04212","last_updated":"2025-07-17T16:27:03Z","snapshot_observed_at":"2026-08-09T04:53:21.314754Z","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":2,"source":"pdf_text","source_observed_at":"2026-08-08T23:12:25.944703Z"},"links":{"cited_paper":"/paper/astro-ph/0501171","citing_paper":"/paper/2502.04212"},"observation_digest":"sha256:fe5e8180e140371cab985a1316d09f726054de55e1e900ecacfb0db18144d332","observation_id":"4ae55b58-6e85-48f8-bd70-297188a132bb","resolution":{"observed_at":"2026-08-08T23:12:25.944703Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"1907.08605","last_updated":"2019-09-25T03:43:45Z","snapshot_observed_at":"2026-08-08T08:46:15.022189Z","submitted_at":"2019-07-19T17:55:28Z","title":"A Detection of CMB-Cluster Lensing using Polarization Data from SPTpol","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"1907.08605","snapshot_observed_at":"2026-08-08T23:12:25.948642Z","title":"Detection of CMB- Cluster Lensing using Polarization Data from SPTpol,","venue":null,"work_id":null,"year":2019},"citing_paper":{"arxiv_id":"2502.04212","last_updated":"2025-07-17T16:27:03Z","snapshot_observed_at":"2026-08-09T04:53:21.314754Z","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":3,"source":"pdf_text","source_observed_at":"2026-08-08T23:12:25.948642Z"},"links":{"cited_paper":"/paper/1907.08605","citing_paper":"/paper/2502.04212"},"observation_digest":"sha256:549a3479bd56ef5e3a1623edbed9fd2753c79afef2cf5ad70dab2fac2deaf6cd","observation_id":"285368d6-fdc8-4972-a5c9-c98e9f041340","resolution":{"observed_at":"2026-08-08T23:12:25.948642Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"1807.06209","last_updated":"2021-08-09T10:43:18Z","snapshot_observed_at":"2026-07-06T02:11:23.670680Z","submitted_at":"2018-07-17T04:05:07Z","title":"Planck 2018 results. VI. Cosmological parameters","version":4},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"1807.06209","snapshot_observed_at":"2026-08-08T23:12:25.952271Z","title":"Planck 2018 results. VI. Cosmological parameters,","venue":null,"work_id":null,"year":2020},"citing_paper":{"arxiv_id":"2502.04212","last_updated":"2025-07-17T16:27:03Z","snapshot_observed_at":"2026-08-09T04:53:21.314754Z","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":4,"source":"pdf_text","source_observed_at":"2026-08-08T23:12:25.952271Z"},"links":{"cited_paper":"/paper/1807.06209","citing_paper":"/paper/2502.04212"},"observation_digest":"sha256:da2915a571aeb4a022a78239e27f5cf62ef198248d74546a60dc95e27da5a3ec","observation_id":"c91d6c7f-1141-49ab-ba76-8af55a78519f","resolution":{"observed_at":"2026-08-08T23:12:25.952271Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2007.08991","last_updated":"2024-07-09T09:56:49Z","snapshot_observed_at":"2026-07-06T02:11:23.670680Z","submitted_at":"2020-07-17T14:09:48Z","title":"The Completed SDSS-IV extended Baryon Oscillation Spectroscopic Survey: Cosmological Implications from two Decades of Spectroscopic Surveys at the Apache Point observatory","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2007.08991","snapshot_observed_at":"2026-08-08T23:12:25.956110Z","title":"Completed SDSS-IV ex- tended Baryon Oscillation Spectroscopic Survey: Cos- mological implications from two decades of spectro- scopic surveys at the Apache Point Observatory,","venue":null,"work_id":null,"year":2021},"citing_paper":{"arxiv_id":"2502.04212","last_updated":"2025-07-17T16:27:03Z","snapshot_observed_at":"2026-08-09T04:53:21.314754Z","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":5,"source":"pdf_text","source_observed_at":"2026-08-08T23:12:25.956110Z"},"links":{"cited_paper":"/paper/2007.08991","citing_paper":"/paper/2502.04212"},"observation_digest":"sha256:668d30aa710a04cf328f82d671accf6f5006c97a0bf28a6c95f9f870deb50ff5","observation_id":"5e865e6d-a5f3-4342-b844-ec5aa68515e9","resolution":{"observed_at":"2026-08-08T23:12:25.956110Z","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":"2026-08-02T14:00:01.779912Z","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":"2026-08-08T23:12:25.960154Z","title":"Dark Energy Survey Year 3 results: Cosmological constraints from galaxy clustering and weak lensing,","venue":null,"work_id":null,"year":2022},"citing_paper":{"arxiv_id":"2502.04212","last_updated":"2025-07-17T16:27:03Z","snapshot_observed_at":"2026-08-09T04:53:21.314754Z","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":6,"source":"pdf_text","source_observed_at":"2026-08-08T23:12:25.960154Z"},"links":{"cited_paper":"/paper/2105.13549","citing_paper":"/paper/2502.04212"},"observation_digest":"sha256:03f40307a48fad69c3c04f5f49927cb988b15f590b8457bb52425f96a5b50b0c","observation_id":"6e596033-01eb-46d9-b8a1-ba52b405e2fe","resolution":{"observed_at":"2026-08-08T23:12:25.960154Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2304.05203","last_updated":"2024-08-12T18:43:42Z","snapshot_observed_at":"2026-07-06T15:14:24.794122Z","submitted_at":"2023-04-11T13:13:14Z","title":"The Atacama Cosmology Telescope: DR6 Gravitational Lensing Map and Cosmological Parameters","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2304.05203","snapshot_observed_at":"2026-08-08T23:12:25.964740Z","title":"The Atacama Cosmology Telescope: DR6 Gravitational Lensing Map and Cosmological Parameters,","venue":null,"work_id":null,"year":2024},"citing_paper":{"arxiv_id":"2502.04212","last_updated":"2025-07-17T16:27:03Z","snapshot_observed_at":"2026-08-09T04:53:21.314754Z","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":7,"source":"pdf_text","source_observed_at":"2026-08-08T23:12:25.964740Z"},"links":{"cited_paper":"/paper/2304.05203","citing_paper":"/paper/2502.04212"},"observation_digest":"sha256:ba7184e883581ccb3097e82885ac542fd2771d07b2bb6ce3f5556c219c564ae2","observation_id":"30e3c253-0b78-4ece-ad26-9ac7dde6e756","resolution":{"observed_at":"2026-08-08T23:12:25.964740Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"astro-ph/9601067","last_updated":"1996-01-12T02:21:46Z","snapshot_observed_at":"2026-07-07T01:12:36.776963Z","submitted_at":"1996-01-12T02:21:46Z","title":"4-Year COBE DMR Cosmic Microwave Background Observations: Maps and Basic Results","version":1},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"astro-ph/9601067","snapshot_observed_at":"2026-08-08T23:12:25.968222Z","title":"Four year COBE DMR cosmic microwave background obser- vations: Maps and basic results,","venue":null,"work_id":null,"year":1996},"citing_paper":{"arxiv_id":"2502.04212","last_updated":"2025-07-17T16:27:03Z","snapshot_observed_at":"2026-08-09T04:53:21.314754Z","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":8,"source":"pdf_text","source_observed_at":"2026-08-08T23:12:25.968222Z"},"links":{"cited_paper":"/paper/astro-ph/9601067","citing_paper":"/paper/2502.04212"},"observation_digest":"sha256:abd08e3fdd2dd7dbdf767a368a39122df65f485037ffc4e156a87edc16046fc3","observation_id":"8a505817-a1a8-4343-a580-fd058d06b50c","resolution":{"observed_at":"2026-08-08T23:12:25.968222Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"1212.5226","last_updated":"2013-06-04T19:07:35Z","snapshot_observed_at":"2026-07-06T03:02:33.289120Z","submitted_at":"2012-12-20T20:24:52Z","title":"Nine-Year Wilkinson Microwave Anisotropy Probe (WMAP) Observations: Cosmological Parameter Results","version":3},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"1212.5226","snapshot_observed_at":"2026-08-08T23:12:25.971712Z","title":"Nine-Year Wilkinson Microwave Anisotropy Probe (WMAP) Observations: Cosmological Parameter Results,","venue":null,"work_id":null,"year":2013},"citing_paper":{"arxiv_id":"2502.04212","last_updated":"2025-07-17T16:27:03Z","snapshot_observed_at":"2026-08-09T04:53:21.314754Z","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":9,"source":"pdf_text","source_observed_at":"2026-08-08T23:12:25.971712Z"},"links":{"cited_paper":"/paper/1212.5226","citing_paper":"/paper/2502.04212"},"observation_digest":"sha256:e68b6e5f1b556df2cb3c8eb7f818aa318d3be0362d5b112ffdd333c172c10851","observation_id":"d4c56530-e84e-4f7c-b160-a204a96d7fdb","resolution":{"observed_at":"2026-08-08T23:12:25.971712Z","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":"2026-08-08T23:12:25.975312Z","title":"Chal- lenges for ΛCDM: An update,","venue":null,"work_id":null,"year":2022},"citing_paper":{"arxiv_id":"2502.04212","last_updated":"2025-07-17T16:27:03Z","snapshot_observed_at":"2026-08-09T04:53:21.314754Z","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":10,"source":"pdf_text","source_observed_at":"2026-08-08T23:12:25.975312Z"},"links":{"cited_paper":"/paper/2105.05208","citing_paper":"/paper/2502.04212"},"observation_digest":"sha256:b083b032ca669c8349aa90aece5170415eb1cac2ef91ebf1f82b485f8b938abe","observation_id":"8024d9ac-a7e5-4457-b06e-9509eadb4091","resolution":{"observed_at":"2026-08-08T23:12:25.975312Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"1607.05617","last_updated":"2016-10-20T11:40:06Z","snapshot_observed_at":"2026-07-06T05:04:09.690126Z","submitted_at":"2016-07-19T14:55:13Z","title":"The trouble with $H_0$","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"1607.05617","snapshot_observed_at":"2026-08-08T23:12:25.979033Z","title":"The trouble with H0,","venue":null,"work_id":null,"year":2016},"citing_paper":{"arxiv_id":"2502.04212","last_updated":"2025-07-17T16:27:03Z","snapshot_observed_at":"2026-08-09T04:53:21.314754Z","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":11,"source":"pdf_text","source_observed_at":"2026-08-08T23:12:25.979033Z"},"links":{"cited_paper":"/paper/1607.05617","citing_paper":"/paper/2502.04212"},"observation_digest":"sha256:3f9e668ccd5ccc2614e20600eeb3db5c2309f0c8c62754774f15d8b56c547cc2","observation_id":"030372b4-44c6-4e61-a98f-6be57eef2c67","resolution":{"observed_at":"2026-08-08T23:12:25.979033Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"1907.10625","last_updated":"2019-07-24T18:00:09Z","snapshot_observed_at":"2026-07-06T08:09:59.842324Z","submitted_at":"2019-07-24T18:00:09Z","title":"Tensions between the Early and the Late Universe","version":1},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"1907.10625","snapshot_observed_at":"2026-08-08T23:12:25.982550Z","title":"Tensions between the Early and the Late Universe,","venue":null,"work_id":null,"year":2019},"citing_paper":{"arxiv_id":"2502.04212","last_updated":"2025-07-17T16:27:03Z","snapshot_observed_at":"2026-08-09T04:53:21.314754Z","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":12,"source":"pdf_text","source_observed_at":"2026-08-08T23:12:25.982550Z"},"links":{"cited_paper":"/paper/1907.10625","citing_paper":"/paper/2502.04212"},"observation_digest":"sha256:5d55a2425203f25884e4f548f2ba69f14f4ba1071cf1c4c8cf518c6efa5beb09","observation_id":"7e8e2de9-0e5f-431d-bb9d-0da9ba25293e","resolution":{"observed_at":"2026-08-08T23:12:25.982550Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"1908.03663","last_updated":"2019-09-16T21:35:34Z","snapshot_observed_at":"2026-07-06T08:13:29.049283Z","submitted_at":"2019-08-10T01:40:10Z","title":"The Hubble Hunter's Guide","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"1908.03663","snapshot_observed_at":"2026-08-08T23:12:25.986019Z","title":"Hubble constant hunter’s guide,","venue":null,"work_id":null,"year":2020},"citing_paper":{"arxiv_id":"2502.04212","last_updated":"2025-07-17T16:27:03Z","snapshot_observed_at":"2026-08-09T04:53:21.314754Z","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":13,"source":"pdf_text","source_observed_at":"2026-08-08T23:12:25.986019Z"},"links":{"cited_paper":"/paper/1908.03663","citing_paper":"/paper/2502.04212"},"observation_digest":"sha256:3f8d78b3bb5426f882e22b489d396753020b16e42db169e4cd71b18dc2dbf300","observation_id":"a42b0b2e-be4b-4af5-b3a4-8b29863614a1","resolution":{"observed_at":"2026-08-08T23:12:25.986019Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2001.03624","last_updated":"2020-01-10T19:00:06Z","snapshot_observed_at":"2026-08-07T08:40:54.490186Z","submitted_at":"2020-01-10T19:00:06Z","title":"The Expansion of the Universe is Faster than Expected","version":1},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2001.03624","snapshot_observed_at":"2026-08-08T23:12:25.989700Z","title":"The Expansion of the Universe is Faster than Expected,","venue":null,"work_id":null,"year":2019},"citing_paper":{"arxiv_id":"2502.04212","last_updated":"2025-07-17T16:27:03Z","snapshot_observed_at":"2026-08-09T04:53:21.314754Z","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":14,"source":"pdf_text","source_observed_at":"2026-08-08T23:12:25.989700Z"},"links":{"cited_paper":"/paper/2001.03624","citing_paper":"/paper/2502.04212"},"observation_digest":"sha256:e45f5cd10cff1730987360946eb768206967b1de01a87b9e42a40b611062f990","observation_id":"5ba8a8f7-db16-4d05-a5dd-ce2bee06e784","resolution":{"observed_at":"2026-08-08T23:12:25.989700Z","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":"2026-08-09T16:24:49.177784Z","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":"2026-08-08T23:12:25.993350Z","title":"Measurements of the Hubble Constant: Tensions in Perspective,","venue":null,"work_id":null,"year":2021},"citing_paper":{"arxiv_id":"2502.04212","last_updated":"2025-07-17T16:27:03Z","snapshot_observed_at":"2026-08-09T04:53:21.314754Z","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":15,"source":"pdf_text","source_observed_at":"2026-08-08T23:12:25.993350Z"},"links":{"cited_paper":"/paper/2106.15656","citing_paper":"/paper/2502.04212"},"observation_digest":"sha256:b6ddc74f27cabd9e155db1aaf93533bee21d4270bcc2abe3062dae8be32e03fb","observation_id":"4bdd5133-eef2-428f-a834-b5282015d324","resolution":{"observed_at":"2026-08-08T23:12:25.993350Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2008.11285","last_updated":"2020-10-13T11:11:55Z","snapshot_observed_at":"2026-08-10T13:14:09.209280Z","submitted_at":"2020-08-25T21:41:42Z","title":"Cosmology Intertwined III: $f \\sigma_8$ and $S_8$","version":4},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2008.11285","snapshot_observed_at":"2026-08-08T23:12:25.996766Z","title":"Cosmology intertwined III: f σ8 and S8,","venue":null,"work_id":null,"year":2021},"citing_paper":{"arxiv_id":"2502.04212","last_updated":"2025-07-17T16:27:03Z","snapshot_observed_at":"2026-08-09T04:53:21.314754Z","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":16,"source":"pdf_text","source_observed_at":"2026-08-08T23:12:25.996766Z"},"links":{"cited_paper":"/paper/2008.11285","citing_paper":"/paper/2502.04212"},"observation_digest":"sha256:1097f694ccabb8b4df97800cbe6c3b565939fc2e07fd37349a505060d68a34a5","observation_id":"f2cf4fa8-1a1e-4fcb-b3ec-b228e8b88d3e","resolution":{"observed_at":"2026-08-08T23:12:25.996766Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2203.06142","last_updated":"2022-04-24T16:57:09Z","snapshot_observed_at":"2026-07-06T02:11:23.670680Z","submitted_at":"2022-03-11T18:13:52Z","title":"Cosmology Intertwined: A Review of the Particle Physics, Astrophysics, and Cosmology Associated with the Cosmological Tensions and Anomalies","version":3},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2203.06142","snapshot_observed_at":"2026-08-08T23:12:26.001256Z","title":"Cosmology intertwined: A review of the particle physics, astrophysics, and cosmology as- sociated with the cosmological tensions and anomalies,","venue":null,"work_id":null,"year":2022},"citing_paper":{"arxiv_id":"2502.04212","last_updated":"2025-07-17T16:27:03Z","snapshot_observed_at":"2026-08-09T04:53:21.314754Z","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":17,"source":"pdf_text","source_observed_at":"2026-08-08T23:12:26.001256Z"},"links":{"cited_paper":"/paper/2203.06142","citing_paper":"/paper/2502.04212"},"observation_digest":"sha256:13dd5a56e126c11fabc90b110d29dae49d24195eb303b07a538ece07c0795808","observation_id":"73744bb9-bf08-4f5c-84fa-6cfb89d8054e","resolution":{"observed_at":"2026-08-08T23:12:26.001256Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2302.01331","last_updated":"2023-08-07T16:54:18Z","snapshot_observed_at":"2026-08-10T07:50:48.576559Z","submitted_at":"2023-02-02T18:59:19Z","title":"Evidence for suppression of structure growth in the concordance cosmological model","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2302.01331","snapshot_observed_at":"2026-08-08T23:12:26.004652Z","title":"Evidence for Suppression of Structure Growth in the Concordance Cosmological Model,","venue":null,"work_id":null,"year":2023},"citing_paper":{"arxiv_id":"2502.04212","last_updated":"2025-07-17T16:27:03Z","snapshot_observed_at":"2026-08-09T04:53:21.314754Z","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":18,"source":"pdf_text","source_observed_at":"2026-08-08T23:12:26.004652Z"},"links":{"cited_paper":"/paper/2302.01331","citing_paper":"/paper/2502.04212"},"observation_digest":"sha256:56b2b954d5f7d6aff11ac2fbe109fbe7b6fb0758efedf9086c30f8f9a5595eec","observation_id":"01d3ee5d-3dfa-4c84-933a-f62892adb5f5","resolution":{"observed_at":"2026-08-08T23:12:26.004652Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2209.14732","last_updated":"2023-04-12T15:40:21Z","snapshot_observed_at":"2026-07-06T13:57:43.546448Z","submitted_at":"2022-09-29T12:52:56Z","title":"First detection of the Hubble variation correlation and its scale dependence","version":3},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2209.14732","snapshot_observed_at":"2026-08-08T23:12:26.007985Z","title":"First de- tection of the Hubble variation correlation and its scale dependence,","venue":null,"work_id":null,"year":2022},"citing_paper":{"arxiv_id":"2502.04212","last_updated":"2025-07-17T16:27:03Z","snapshot_observed_at":"2026-08-09T04:53:21.314754Z","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":19,"source":"pdf_text","source_observed_at":"2026-08-08T23:12:26.007985Z"},"links":{"cited_paper":"/paper/2209.14732","citing_paper":"/paper/2502.04212"},"observation_digest":"sha256:9d280f615a8dcecd689aa40ff768346f1266919f8475ec59e42ffdb04f1991a0","observation_id":"08444cd1-6712-499b-9337-9f29f79476bb","resolution":{"observed_at":"2026-08-08T23:12:26.007985Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"astro-ph/0510346","last_updated":"2005-10-12T13:33:59Z","snapshot_observed_at":"2026-08-07T10:52:21.666534Z","submitted_at":"2005-10-12T13:33:59Z","title":"The Dark Energy Survey","version":1},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"astro-ph/0510346","snapshot_observed_at":"2026-08-08T23:12:26.011456Z","title":"The Dark Energy Survey,","venue":null,"work_id":null,"year":2005},"citing_paper":{"arxiv_id":"2502.04212","last_updated":"2025-07-17T16:27:03Z","snapshot_observed_at":"2026-08-09T04:53:21.314754Z","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":20,"source":"pdf_text","source_observed_at":"2026-08-08T23:12:26.011456Z"},"links":{"cited_paper":"/paper/astro-ph/0510346","citing_paper":"/paper/2502.04212"},"observation_digest":"sha256:c5a659996d7f63111b514d523fecd0d4ed3df31648adb2f9e64403a5d9c20008","observation_id":"d6862c3b-1eb2-43aa-ba25-3f67325fa260","resolution":{"observed_at":"2026-08-08T23:12:26.011456Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"1111.1969","last_updated":"2012-07-12T19:50:22Z","snapshot_observed_at":"2026-08-05T21:02:44.551429Z","submitted_at":"2011-11-08T16:49:05Z","title":"Supernova Simulations and Strategies For the Dark Energy Survey","version":4},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"1111.1969","snapshot_observed_at":"2026-08-08T23:12:26.015812Z","title":"Supernova Simulations and Strategies For the Dark Energy Survey,","venue":null,"work_id":null,"year":2012},"citing_paper":{"arxiv_id":"2502.04212","last_updated":"2025-07-17T16:27:03Z","snapshot_observed_at":"2026-08-09T04:53:21.314754Z","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":21,"source":"pdf_text","source_observed_at":"2026-08-08T23:12:26.015812Z"},"links":{"cited_paper":"/paper/1111.1969","citing_paper":"/paper/2502.04212"},"observation_digest":"sha256:443632350ffc74dbd830f7207295f0c8de995c3a714109647cfb085407e28a92","observation_id":"8195ff67-385e-4598-829b-c9b5c0414cfe","resolution":{"observed_at":"2026-08-08T23:12:26.015812Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"1601.00329","last_updated":"2016-08-19T15:43:52Z","snapshot_observed_at":"2026-08-03T02:40:21.221368Z","submitted_at":"2016-01-03T19:33:10Z","title":"The Dark Energy Survey: more than dark energy - an overview","version":3},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"1601.00329","snapshot_observed_at":"2026-08-08T23:12:26.019208Z","title":"The Dark Energy Survey: more than dark energy – an overview,","venue":null,"work_id":null,"year":2016},"citing_paper":{"arxiv_id":"2502.04212","last_updated":"2025-07-17T16:27:03Z","snapshot_observed_at":"2026-08-09T04:53:21.314754Z","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":22,"source":"pdf_text","source_observed_at":"2026-08-08T23:12:26.019208Z"},"links":{"cited_paper":"/paper/1601.00329","citing_paper":"/paper/2502.04212"},"observation_digest":"sha256:e3676b73cf56f7a3fe721380894a4a9263ab73efe84f033923ca1c6b0f866e3c","observation_id":"3fb30bbd-0462-42c7-95b7-327468e53869","resolution":{"observed_at":"2026-08-08T23:12:26.019208Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2404.03002","last_updated":"2024-11-04T16:43:36Z","snapshot_observed_at":"2026-07-06T17:55:21.083912Z","submitted_at":"2024-04-03T18:41:51Z","title":"DESI 2024 VI: Cosmological Constraints from the Measurements of Baryon Acoustic Oscillations","version":3},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2404.03002","snapshot_observed_at":"2026-08-08T23:12:26.023011Z","title":"DESI 2024 VI: cosmological constraints from the measurements of baryon acoustic oscillations,","venue":null,"work_id":null,"year":2025},"citing_paper":{"arxiv_id":"2502.04212","last_updated":"2025-07-17T16:27:03Z","snapshot_observed_at":"2026-08-09T04:53:21.314754Z","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":23,"source":"pdf_text","source_observed_at":"2026-08-08T23:12:26.023011Z"},"links":{"cited_paper":"/paper/2404.03002","citing_paper":"/paper/2502.04212"},"observation_digest":"sha256:efa0c7146d178a5aa2499270b366866e91f3f4bcc620878f90f26b7644d9aac2","observation_id":"432ffecb-396e-418f-848d-0a1ce1f76e11","resolution":{"observed_at":"2026-08-08T23:12:26.023011Z","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":"2026-08-09T18:42:58.809582Z","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":"2026-08-08T23:12:26.026689Z","title":"DESI 2024 III: baryon acoustic oscillations from galaxies and quasars,","venue":null,"work_id":null,"year":2025},"citing_paper":{"arxiv_id":"2502.04212","last_updated":"2025-07-17T16:27:03Z","snapshot_observed_at":"2026-08-09T04:53:21.314754Z","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":24,"source":"pdf_text","source_observed_at":"2026-08-08T23:12:26.026689Z"},"links":{"cited_paper":"/paper/2404.03000","citing_paper":"/paper/2502.04212"},"observation_digest":"sha256:717099d9faf0f1eba95b512c6fa10af0f39493f2f5ab44ea8a71006e899b5513","observation_id":"a9664840-026c-4f1d-86c3-aad15ea44cb8","resolution":{"observed_at":"2026-08-08T23:12:26.026689Z","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":"2026-08-09T21:48:39.628348Z","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":"2026-08-08T23:12:26.030728Z","title":"DESI 2024 IV: Baryon Acoustic Oscillations from the Lyman alpha forest,","venue":null,"work_id":null,"year":2025},"citing_paper":{"arxiv_id":"2502.04212","last_updated":"2025-07-17T16:27:03Z","snapshot_observed_at":"2026-08-09T04:53:21.314754Z","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":25,"source":"pdf_text","source_observed_at":"2026-08-08T23:12:26.030728Z"},"links":{"cited_paper":"/paper/2404.03001","citing_paper":"/paper/2502.04212"},"observation_digest":"sha256:d3681de1d422b11c43b92db9e7cf2e1a1eeec29ffddebec240d9b50ed9d3908a","observation_id":"3e6c1f2e-e373-4589-936a-8367f6416889","resolution":{"observed_at":"2026-08-08T23:12:26.030728Z","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":"2026-07-06T17:12:06.715778Z","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":"2026-08-08T23:12:26.034033Z","title":"The Dark Energy Sur- vey: Cosmology Results with ∼1500 New High-redshift Type Ia Supernovae Using the Full 5 yr Data Set,","venue":null,"work_id":null,"year":2024},"citing_paper":{"arxiv_id":"2502.04212","last_updated":"2025-07-17T16:27:03Z","snapshot_observed_at":"2026-08-09T04:53:21.314754Z","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":26,"source":"pdf_text","source_observed_at":"2026-08-08T23:12:26.034033Z"},"links":{"cited_paper":"/paper/2401.02929","citing_paper":"/paper/2502.04212"},"observation_digest":"sha256:d99dfd7ce82e65748fc509a1b2856919f304c5c58ee62ae3a36bbaa457b0bf6a","observation_id":"f2f5dfdc-f60b-401f-ab6b-fb6ae7fe1aef","resolution":{"observed_at":"2026-08-08T23:12:26.034033Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2401.02945","last_updated":"2024-01-22T19:12:21Z","snapshot_observed_at":"2026-08-08T05:27:42.569443Z","submitted_at":"2024-01-05T18:34:07Z","title":"The Dark Energy Survey Supernova Program: Cosmological Analysis and Systematic Uncertainties","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2401.02945","snapshot_observed_at":"2026-08-08T23:12:26.037594Z","title":"The Dark Energy Survey Supernova Program: Cosmological Analysis and Sys- tematic Uncertainties,","venue":null,"work_id":null,"year":2024},"citing_paper":{"arxiv_id":"2502.04212","last_updated":"2025-07-17T16:27:03Z","snapshot_observed_at":"2026-08-09T04:53:21.314754Z","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":27,"source":"pdf_text","source_observed_at":"2026-08-08T23:12:26.037594Z"},"links":{"cited_paper":"/paper/2401.02945","citing_paper":"/paper/2502.04212"},"observation_digest":"sha256:38b94c9d436fbb1c94d9cd3784fa4fd76e4e0334d64b448efa0ef1387b953ead","observation_id":"b7f687b2-dbc2-4ef7-9dac-94eeb9dce537","resolution":{"observed_at":"2026-08-08T23:12:26.037594Z","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":"2026-07-06T19:52:15.853216Z","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":"2026-08-08T23:12:26.040912Z","title":"DESI 2024 VII: cos- mological constraints from the full-shape modeling of clustering measurements,","venue":null,"work_id":null,"year":2025},"citing_paper":{"arxiv_id":"2502.04212","last_updated":"2025-07-17T16:27:03Z","snapshot_observed_at":"2026-08-09T04:53:21.314754Z","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":28,"source":"pdf_text","source_observed_at":"2026-08-08T23:12:26.040912Z"},"links":{"cited_paper":"/paper/2411.12022","citing_paper":"/paper/2502.04212"},"observation_digest":"sha256:ff2ce070fc59dcefddb44b5abd02936f7278137fb94467b8d4f7d575d280eaa2","observation_id":"8e4a4771-4237-4c66-98ca-c06fd3a0d96e","resolution":{"observed_at":"2026-08-08T23:12:26.040912Z","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":"2026-08-06T17:07:41.767936Z","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":"2026-08-08T23:12:26.044202Z","title":"Using non-DESI data to confirm and strengthen the DESI 2024 spatially flat w0waCDM cosmological parametrization result,","venue":null,"work_id":null,"year":2024},"citing_paper":{"arxiv_id":"2502.04212","last_updated":"2025-07-17T16:27:03Z","snapshot_observed_at":"2026-08-09T04:53:21.314754Z","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":29,"source":"pdf_text","source_observed_at":"2026-08-08T23:12:26.044202Z"},"links":{"cited_paper":"/paper/2405.00502","citing_paper":"/paper/2502.04212"},"observation_digest":"sha256:61ee35454cec0cff3214ca537dfb93f4c8750042bd1a23096baae263913d33fc","observation_id":"2011c885-27a4-4422-899f-a41ac0dd650f","resolution":{"observed_at":"2026-08-08T23:12:26.044202Z","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":"2026-08-04T17:15:38.237315Z","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":"2026-08-08T23:12:26.048335Z","title":"Quintessential interpretation of the evolving dark energy in light of DESI observations,","venue":null,"work_id":null,"year":2024},"citing_paper":{"arxiv_id":"2502.04212","last_updated":"2025-07-17T16:27:03Z","snapshot_observed_at":"2026-08-09T04:53:21.314754Z","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":30,"source":"pdf_text","source_observed_at":"2026-08-08T23:12:26.048335Z"},"links":{"cited_paper":"/paper/2404.05722","citing_paper":"/paper/2502.04212"},"observation_digest":"sha256:429a52490f036968408b21635e4ee28f1b4416cb292d357aa99f3fc36531986c","observation_id":"926e3e81-b428-4e2b-8be3-cd8f0302bad9","resolution":{"observed_at":"2026-08-08T23:12:26.048335Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2404.14341","last_updated":"2024-11-18T22:02:37Z","snapshot_observed_at":"2026-08-07T20:22:25.786928Z","submitted_at":"2024-04-22T16:58:05Z","title":"Quantifying Scalar Field Dynamics with DESI 2024 Y1 BAO measurements","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2404.14341","snapshot_observed_at":"2026-08-08T23:12:26.053046Z","title":"Quantifying scalar field dynamics with DESI 2024 Y1 BAO measurements,","venue":null,"work_id":null,"year":2024},"citing_paper":{"arxiv_id":"2502.04212","last_updated":"2025-07-17T16:27:03Z","snapshot_observed_at":"2026-08-09T04:53:21.314754Z","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":31,"source":"pdf_text","source_observed_at":"2026-08-08T23:12:26.053046Z"},"links":{"cited_paper":"/paper/2404.14341","citing_paper":"/paper/2502.04212"},"observation_digest":"sha256:6fe2628fe12c2d3bd0985974924e7d5af818f3f036d6620433d0284fe1bf3aa8","observation_id":"154d47eb-d211-419e-b5e4-a81d0e957335","resolution":{"observed_at":"2026-08-08T23:12:26.053046Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2405.03933","last_updated":"2026-04-18T21:47:09Z","snapshot_observed_at":"2026-07-30T11:26:22.264591Z","submitted_at":"2024-05-07T01:42:30Z","title":"Assessing observational constraints on dark energy","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2405.03933","snapshot_observed_at":"2026-08-08T23:12:26.057673Z","title":"Assessing ob- servational constraints on dark energy,","venue":null,"work_id":null,"year":2024},"citing_paper":{"arxiv_id":"2502.04212","last_updated":"2025-07-17T16:27:03Z","snapshot_observed_at":"2026-08-09T04:53:21.314754Z","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":32,"source":"pdf_text","source_observed_at":"2026-08-08T23:12:26.057673Z"},"links":{"cited_paper":"/paper/2405.03933","citing_paper":"/paper/2502.04212"},"observation_digest":"sha256:701b937501225afc99e39e3eb37785c19ec6b0bd3399e066dc62a9b0603294a9","observation_id":"223d4a1c-6055-4ddb-8392-ae6837160e07","resolution":{"observed_at":"2026-08-08T23:12:26.057673Z","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":"2026-07-06T18:21:44.232687Z","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":"2026-08-08T23:12:26.061628Z","title":"DESI constraints on exponential quintessence,","venue":null,"work_id":null,"year":2024},"citing_paper":{"arxiv_id":"2502.04212","last_updated":"2025-07-17T16:27:03Z","snapshot_observed_at":"2026-08-09T04:53:21.314754Z","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":33,"source":"pdf_text","source_observed_at":"2026-08-08T23:12:26.061628Z"},"links":{"cited_paper":"/paper/2405.18747","citing_paper":"/paper/2502.04212"},"observation_digest":"sha256:e92bcb9da204b8178ce4bef8b539f22d61de9379a8987f91bf16c09e822a5c39","observation_id":"3c03681f-77fd-445a-a8bb-66d55ec86559","resolution":{"observed_at":"2026-08-08T23:12:26.061628Z","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":"2026-08-03T12:26:25.264043Z","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":"2026-08-08T23:12:26.065180Z","title":"Cosmological constraints on curved 9 quintessence,","venue":null,"work_id":null,"year":2024},"citing_paper":{"arxiv_id":"2502.04212","last_updated":"2025-07-17T16:27:03Z","snapshot_observed_at":"2026-08-09T04:53:21.314754Z","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":34,"source":"pdf_text","source_observed_at":"2026-08-08T23:12:26.065180Z"},"links":{"cited_paper":"/paper/2405.17396","citing_paper":"/paper/2502.04212"},"observation_digest":"sha256:905181a8e0d613e9ce045eed1b80f048dec573152e8a6bf1fa2e18f83784a34a","observation_id":"592a8230-53c5-4c74-b0f0-682665c79f0d","resolution":{"observed_at":"2026-08-08T23:12:26.065180Z","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":"2026-08-07T16:10:37.036129Z","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":"2026-08-08T23:12:26.069386Z","title":"Interacting Dark Energy after DESI Baryon Acoustic Oscillation Measurements,","venue":null,"work_id":null,"year":2024},"citing_paper":{"arxiv_id":"2502.04212","last_updated":"2025-07-17T16:27:03Z","snapshot_observed_at":"2026-08-09T04:53:21.314754Z","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":35,"source":"pdf_text","source_observed_at":"2026-08-08T23:12:26.069386Z"},"links":{"cited_paper":"/paper/2404.15232","citing_paper":"/paper/2502.04212"},"observation_digest":"sha256:f89a35ef7fa6f57cf2d302a1cbb5de4821079ae43d10f9d628cdd5d91b53f134","observation_id":"8ac42b03-5561-4f83-b4b5-17e07998f0f0","resolution":{"observed_at":"2026-08-08T23:12:26.069386Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2404.15220","last_updated":"2025-03-11T17:56:44Z","snapshot_observed_at":"2026-08-09T01:15:51.432162Z","submitted_at":"2024-04-23T16:52:14Z","title":"Reduced Hubble Tension in Dark Radiation Models after DESI 2024","version":3},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2404.15220","snapshot_observed_at":"2026-08-08T23:12:26.072994Z","title":"Reduced Hubble tension in dark radia- tion models after DESI 2024,","venue":null,"work_id":null,"year":2025},"citing_paper":{"arxiv_id":"2502.04212","last_updated":"2025-07-17T16:27:03Z","snapshot_observed_at":"2026-08-09T04:53:21.314754Z","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":36,"source":"pdf_text","source_observed_at":"2026-08-08T23:12:26.072994Z"},"links":{"cited_paper":"/paper/2404.15220","citing_paper":"/paper/2502.04212"},"observation_digest":"sha256:a3935e3dae6cf4accaed0a34733c732a5350c51a6d865da1a97a0d218ffb84e8","observation_id":"0e7f1f29-85bd-4587-86c4-e33d659ecf8b","resolution":{"observed_at":"2026-08-08T23:12:26.072994Z","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":"2026-08-10T14:43:56.060028Z","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":"2026-08-08T23:12:26.076923Z","title":"DESI dark energy time evolution is recovered by cosmologically coupled black holes,","venue":null,"work_id":null,"year":2024},"citing_paper":{"arxiv_id":"2502.04212","last_updated":"2025-07-17T16:27:03Z","snapshot_observed_at":"2026-08-09T04:53:21.314754Z","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":37,"source":"pdf_text","source_observed_at":"2026-08-08T23:12:26.076923Z"},"links":{"cited_paper":"/paper/2405.12282","citing_paper":"/paper/2502.04212"},"observation_digest":"sha256:7648b28223083b411556c57ee1c9f0e62b2d2123b042b7b9a4f5a23a0d26f5dd","observation_id":"cc0f30f1-7025-4d9c-9331-c972960e7de6","resolution":{"observed_at":"2026-08-08T23:12:26.076923Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2404.19437","last_updated":"2024-07-19T14:51:47Z","snapshot_observed_at":"2026-08-10T15:35:24.318701Z","submitted_at":"2024-04-30T10:35:04Z","title":"Quintom cosmology and modified gravity after DESI 2024","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2404.19437","snapshot_observed_at":"2026-08-08T23:12:26.080815Z","title":"Quintom cosmology and modified gravity after DESI 2024,","venue":null,"work_id":null,"year":2024},"citing_paper":{"arxiv_id":"2502.04212","last_updated":"2025-07-17T16:27:03Z","snapshot_observed_at":"2026-08-09T04:53:21.314754Z","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":38,"source":"pdf_text","source_observed_at":"2026-08-08T23:12:26.080815Z"},"links":{"cited_paper":"/paper/2404.19437","citing_paper":"/paper/2502.04212"},"observation_digest":"sha256:434cd70e823fca2447f42780b3869d3a5c91f16c2655cb14a0f69e312da5b33d","observation_id":"55590b40-163a-467a-b458-f530dd270243","resolution":{"observed_at":"2026-08-08T23:12:26.080815Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2405.00608","last_updated":"2024-05-14T19:37:41Z","snapshot_observed_at":"2026-07-06T18:08:17.557905Z","submitted_at":"2024-05-01T16:28:59Z","title":"$f(T)$ gravity after DESI Baryon Acoustic Oscillation and DES Supernovae 2024 data","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2405.00608","snapshot_observed_at":"2026-08-08T23:12:26.084527Z","title":"f(T) gravity after DESI Baryon acoustic oscillation and DES supernovae 2024 data,","venue":null,"work_id":null,"year":2024},"citing_paper":{"arxiv_id":"2502.04212","last_updated":"2025-07-17T16:27:03Z","snapshot_observed_at":"2026-08-09T04:53:21.314754Z","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":39,"source":"pdf_text","source_observed_at":"2026-08-08T23:12:26.084527Z"},"links":{"cited_paper":"/paper/2405.00608","citing_paper":"/paper/2502.04212"},"observation_digest":"sha256:ab6a17493f2259475778d30da469fce91b0adc873adfe5fb44362e3459c709f0","observation_id":"0eab95e8-1900-4606-87eb-8dcf9e4aef75","resolution":{"observed_at":"2026-08-08T23:12:26.084527Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2404.06444","last_updated":"2024-04-09T16:47:13Z","snapshot_observed_at":"2026-08-08T09:16:49.910983Z","submitted_at":"2024-04-09T16:47:13Z","title":"Cosmic Clues: DESI, Dark Energy, and the Cosmological Constant Problem","version":1},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2404.06444","snapshot_observed_at":"2026-08-08T23:12:26.087965Z","title":"Cosmic clues: DESI, dark energy, and the cosmological constant problem,","venue":null,"work_id":null,"year":2024},"citing_paper":{"arxiv_id":"2502.04212","last_updated":"2025-07-17T16:27:03Z","snapshot_observed_at":"2026-08-09T04:53:21.314754Z","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":40,"source":"pdf_text","source_observed_at":"2026-08-08T23:12:26.087965Z"},"links":{"cited_paper":"/paper/2404.06444","citing_paper":"/paper/2502.04212"},"observation_digest":"sha256:13a53d7d733fe9d87c76a29fa9292947fd207eeb8f80544a4c3ea25319854393","observation_id":"055c1961-4b7e-4b56-9f3b-57f2c3d1bf86","resolution":{"observed_at":"2026-08-08T23:12:26.087965Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2404.06303","last_updated":"2024-04-15T14:36:13Z","snapshot_observed_at":"2026-07-06T17:57:44.174936Z","submitted_at":"2024-04-09T13:34:15Z","title":"Dynamical dark energy in light of cosmic distance measurements I: a demonstration using simulated datasets","version":3},"cited_work":{"arxiv_id":"2404.06303","doi":null,"metadata_source":"pith","pith_arxiv_id":"2404.06303","snapshot_observed_at":"2026-08-08T23:12:27.359479Z","title":"Dynamical dark energy in light of cosmic distance measurements I: a demonstration using simulated datasets","venue":"astro-ph.CO","work_id":"8fa2fb19-68a1-4de3-bc95-442d270c25ec","year":2024},"citing_paper":{"arxiv_id":"2502.04212","last_updated":"2025-07-17T16:27:03Z","snapshot_observed_at":"2026-08-09T04:53:21.314754Z","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":41,"source":"pdf_text","source_observed_at":"2026-08-08T23:12:26.091508Z"},"links":{"cited_paper":"/paper/2404.06303","citing_paper":"/paper/2502.04212"},"observation_digest":"sha256:3b1677575086d78094ec146d57afdde47c15d1d65a0c0cb22fa7d14f1401a531","observation_id":"b437240b-3a69-4717-8d34-7b8784841649","resolution":{"observed_at":"2026-08-08T23:12:27.363153Z","resolver_source":"local_arxiv","status":"verified_exact"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-10T06:31:04.303077+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-10T06:31:04.303077+00:00","source":"crossref"},{"observed_at":"2026-08-10T06:30:57.382061+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":{"arxiv_id":"2404.06310","last_updated":"2024-04-15T14:37:45Z","snapshot_observed_at":"2026-07-06T17:57:48.153936Z","submitted_at":"2024-04-09T13:42:42Z","title":"Dynamical dark energy in light of cosmic distance measurements II: a study using current observations","version":3},"cited_work":{"arxiv_id":"2404.06310","doi":null,"metadata_source":"pith","pith_arxiv_id":"2404.06310","snapshot_observed_at":"2026-08-08T23:12:27.343097Z","title":"Dynamical dark energy in light of cosmic distance measurements II: a study using current observations","venue":"astro-ph.CO","work_id":"92c63034-7995-4b41-b26f-0958e025cf56","year":2024},"citing_paper":{"arxiv_id":"2502.04212","last_updated":"2025-07-17T16:27:03Z","snapshot_observed_at":"2026-08-09T04:53:21.314754Z","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":42,"source":"pdf_text","source_observed_at":"2026-08-08T23:12:26.094882Z"},"links":{"cited_paper":"/paper/2404.06310","citing_paper":"/paper/2502.04212"},"observation_digest":"sha256:22f77780257e8293e9ec7a01ee11d7a9f16eaac9c0a8f602dce603b7a4aa2987","observation_id":"5ce85100-35ac-45a5-8a37-4d0dc385282b","resolution":{"observed_at":"2026-08-08T23:12:27.348889Z","resolver_source":"local_arxiv","status":"verified_exact"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-10T06:31:04.303077+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-10T06:31:04.303077+00:00","source":"crossref"},{"observed_at":"2026-08-10T06:30:57.382061+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":{"arxiv_id":"2404.08056","last_updated":"2024-11-08T14:34:18Z","snapshot_observed_at":"2026-08-06T12:14:01.037607Z","submitted_at":"2024-04-11T18:00:21Z","title":"Interpreting DESI's evidence for evolving dark energy","version":3},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2404.08056","snapshot_observed_at":"2026-08-08T23:12:26.098176Z","title":"Interpreting DESI’s evidence for evolving dark energy,","venue":null,"work_id":null,"year":2024},"citing_paper":{"arxiv_id":"2502.04212","last_updated":"2025-07-17T16:27:03Z","snapshot_observed_at":"2026-08-09T04:53:21.314754Z","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":43,"source":"pdf_text","source_observed_at":"2026-08-08T23:12:26.098176Z"},"links":{"cited_paper":"/paper/2404.08056","citing_paper":"/paper/2502.04212"},"observation_digest":"sha256:4830be172ef74198c885612ac5ee5c671319a76f49d659058b18de99a2ab7b4a","observation_id":"a80af285-7250-4bf0-b6db-fa113cf80bac","resolution":{"observed_at":"2026-08-08T23:12:26.098176Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2404.08633","last_updated":"2025-07-28T08:54:28Z","snapshot_observed_at":"2026-08-07T10:52:13.461540Z","submitted_at":"2024-04-12T17:51:07Z","title":"Does DESI 2024 Confirm $\\Lambda$CDM?","version":3},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2404.08633","snapshot_observed_at":"2026-08-08T23:12:26.102448Z","title":"Does DESI 2024 Con- firm ΛCDM?","venue":null,"work_id":null,"year":2024},"citing_paper":{"arxiv_id":"2502.04212","last_updated":"2025-07-17T16:27:03Z","snapshot_observed_at":"2026-08-09T04:53:21.314754Z","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":44,"source":"pdf_text","source_observed_at":"2026-08-08T23:12:26.102448Z"},"links":{"cited_paper":"/paper/2404.08633","citing_paper":"/paper/2502.04212"},"observation_digest":"sha256:3bbb60df2ca0c2bb65eeae28b06d15ab1587780fbf826b088773faf015b4f3bd","observation_id":"fdf1ab36-a759-4897-80f7-9c8bd1c166ef","resolution":{"observed_at":"2026-08-08T23:12:26.102448Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2404.12068","last_updated":"2024-04-18T10:39:44Z","snapshot_observed_at":"2026-08-04T14:53:24.592982Z","submitted_at":"2024-04-18T10:39:44Z","title":"Does dark energy really revive using DESI 2024 data?","version":1},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2404.12068","snapshot_observed_at":"2026-08-08T23:12:26.106013Z","title":"Does dark energy really revive using DESI 2024 data?","venue":null,"work_id":null,"year":2025},"citing_paper":{"arxiv_id":"2502.04212","last_updated":"2025-07-17T16:27:03Z","snapshot_observed_at":"2026-08-09T04:53:21.314754Z","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":45,"source":"pdf_text","source_observed_at":"2026-08-08T23:12:26.106013Z"},"links":{"cited_paper":"/paper/2404.12068","citing_paper":"/paper/2502.04212"},"observation_digest":"sha256:7f3ffb282890036bdcf1f5bd39daafee1a8649b35ee71ac785a39bfe817b3b3f","observation_id":"3b144e72-d954-43bd-b94b-2772bfaf0a9b","resolution":{"observed_at":"2026-08-08T23:12:26.106013Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2405.13588","last_updated":"2024-05-30T08:22:06Z","snapshot_observed_at":"2026-08-09T11:32:15.266630Z","submitted_at":"2024-05-22T12:35:37Z","title":"DESI 2024: Constraints on Physics-Focused Aspects of Dark Energy using DESI DR1 BAO Data","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2405.13588","snapshot_observed_at":"2026-08-08T23:12:26.109599Z","title":"DESI 2024: Constraints on physics-focused aspects of dark energy using DESI DR1 BAO data,","venue":null,"work_id":null,"year":2025},"citing_paper":{"arxiv_id":"2502.04212","last_updated":"2025-07-17T16:27:03Z","snapshot_observed_at":"2026-08-09T04:53:21.314754Z","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":46,"source":"pdf_text","source_observed_at":"2026-08-08T23:12:26.109599Z"},"links":{"cited_paper":"/paper/2405.13588","citing_paper":"/paper/2502.04212"},"observation_digest":"sha256:2122a8917ca183a03de5bfac4bb8955132d6a1506a9d40c27e17134fbff6cfe1","observation_id":"98213401-6107-4104-9bf1-d317f7a4ff5b","resolution":{"observed_at":"2026-08-08T23:12:26.109599Z","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":"2026-08-10T05:08:15.169086Z","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":"2026-08-08T23:12:26.114074Z","title":"DESI 2024: reconstructing dark energy using crossing statistics with DESI DR1 BAO data,","venue":null,"work_id":null,"year":2024},"citing_paper":{"arxiv_id":"2502.04212","last_updated":"2025-07-17T16:27:03Z","snapshot_observed_at":"2026-08-09T04:53:21.314754Z","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":47,"source":"pdf_text","source_observed_at":"2026-08-08T23:12:26.114074Z"},"links":{"cited_paper":"/paper/2405.04216","citing_paper":"/paper/2502.04212"},"observation_digest":"sha256:e2e14302f9dcbcad2398ee5c3efe37515d2efbc0c862b5b38b2b9dd329a59a56","observation_id":"26f4dc72-df1f-4efa-856a-6128cd4d7a27","resolution":{"observed_at":"2026-08-08T23:12:26.114074Z","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":"2026-07-06T17:58:21.138881Z","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":"2026-08-08T23:12:26.117649Z","title":"Model- independent cosmographic constraints from DESI 2024,","venue":null,"work_id":null,"year":2024},"citing_paper":{"arxiv_id":"2502.04212","last_updated":"2025-07-17T16:27:03Z","snapshot_observed_at":"2026-08-09T04:53:21.314754Z","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":48,"source":"pdf_text","source_observed_at":"2026-08-08T23:12:26.117649Z"},"links":{"cited_paper":"/paper/2404.07070","citing_paper":"/paper/2502.04212"},"observation_digest":"sha256:5aee2592f31105aebf69396ba598c0a4b691dfe130c474f20a6ab561fbdc6ab4","observation_id":"f39f5104-71c9-4f80-992e-ff2181df8ddd","resolution":{"observed_at":"2026-08-08T23:12:26.117649Z","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":"2026-08-08T23:12:26.121553Z","title":"Model- independent cosmological inference post DESI DR1 BAO measurements,","venue":null,"work_id":null,"year":2024},"citing_paper":{"arxiv_id":"2502.04212","last_updated":"2025-07-17T16:27:03Z","snapshot_observed_at":"2026-08-09T04:53:21.314754Z","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":49,"source":"pdf_text","source_observed_at":"2026-08-08T23:12:26.121553Z"},"links":{"citing_paper":"/paper/2502.04212"},"observation_digest":"sha256:d39197b20e8d64e778ab8ceaa850b5fff3a34074d9b57e5cacb1d17761dd2c21","observation_id":"6d18bf14-3da8-4ffe-9fbc-ddcd5ec0521d","resolution":{"observed_at":"2026-08-08T23:12:26.121553Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2405.06618","last_updated":"2025-03-04T11:04:35Z","snapshot_observed_at":"2026-08-08T08:16:37.208573Z","submitted_at":"2024-05-10T17:29:06Z","title":"A new diagnostic for the null test of dynamical dark energy in light of DESI 2024 and other BAO data","version":3},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2405.06618","snapshot_observed_at":"2026-08-08T23:12:26.124757Z","title":"A new diagnostic for the null test of dynamical dark energy in light of DESI 2024 and other BAO data,","venue":null,"work_id":null,"year":2024},"citing_paper":{"arxiv_id":"2502.04212","last_updated":"2025-07-17T16:27:03Z","snapshot_observed_at":"2026-08-09T04:53:21.314754Z","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":50,"source":"pdf_text","source_observed_at":"2026-08-08T23:12:26.124757Z"},"links":{"cited_paper":"/paper/2405.06618","citing_paper":"/paper/2502.04212"},"observation_digest":"sha256:65aba8d1963fd067036f62988568d88ee727eb55e7ba80e65aa6e41466931316","observation_id":"e2061418-17e9-4473-833a-0bbadc40a159","resolution":{"observed_at":"2026-08-08T23:12:26.124757Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2406.05048","last_updated":"2024-09-13T00:31:49Z","snapshot_observed_at":"2026-08-02T07:44:18.385582Z","submitted_at":"2024-06-07T16:18:59Z","title":"The Dark Energy Survey Supernova Program: Investigating Beyond-$\\Lambda$CDM","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2406.05048","snapshot_observed_at":"2026-08-08T23:12:26.128273Z","title":"The dark energy sur- vey supernova program: investigating beyond-ΛCDM,","venue":null,"work_id":null,"year":2024},"citing_paper":{"arxiv_id":"2502.04212","last_updated":"2025-07-17T16:27:03Z","snapshot_observed_at":"2026-08-09T04:53:21.314754Z","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":51,"source":"pdf_text","source_observed_at":"2026-08-08T23:12:26.128273Z"},"links":{"cited_paper":"/paper/2406.05048","citing_paper":"/paper/2502.04212"},"observation_digest":"sha256:982c09762f97d3292706b8c83e12039e51fe7f52624a94cc7468a5f52db807aa","observation_id":"5bf2625e-8ca3-4401-8635-7f1e58243be7","resolution":{"observed_at":"2026-08-08T23:12:26.128273Z","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":"2026-08-06T06:47:38.734085Z","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":"2026-08-08T23:12:26.131843Z","title":"Revisiting holographic dark energy after DESI 2024,","venue":null,"work_id":null,"year":2025},"citing_paper":{"arxiv_id":"2502.04212","last_updated":"2025-07-17T16:27:03Z","snapshot_observed_at":"2026-08-09T04:53:21.314754Z","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":52,"source":"pdf_text","source_observed_at":"2026-08-08T23:12:26.131843Z"},"links":{"cited_paper":"/paper/2411.08639","citing_paper":"/paper/2502.04212"},"observation_digest":"sha256:2899bb23fc2ede5e38d2865453ddf93360c8678ae975997bd43701a98dfa8719","observation_id":"8b7fa834-9f64-4c0e-b2ab-aac483e2d638","resolution":{"observed_at":"2026-08-08T23:12:26.131843Z","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":"2026-07-06T19:56:17.117739Z","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":"2026-08-08T23:12:26.135286Z","title":"On the Evidence of Dynamical Dark Energy,","venue":null,"work_id":null,"year":2025},"citing_paper":{"arxiv_id":"2502.04212","last_updated":"2025-07-17T16:27:03Z","snapshot_observed_at":"2026-08-09T04:53:21.314754Z","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":53,"source":"pdf_text","source_observed_at":"2026-08-08T23:12:26.135286Z"},"links":{"cited_paper":"/paper/2411.16046","citing_paper":"/paper/2502.04212"},"observation_digest":"sha256:0a2c01a472bd6d4be6f77c0551fe03ffa03f26cfa1c7d2cfcc2adc4963ea87f9","observation_id":"c960f933-572b-427e-bd98-0adb62a9e29f","resolution":{"observed_at":"2026-08-08T23:12:26.135286Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2411.19362","last_updated":"2025-08-20T17:11:12Z","snapshot_observed_at":"2026-07-06T19:58:39.778401Z","submitted_at":"2024-11-28T20:18:13Z","title":"A preference for dynamical phantom dark energy using one-parameter model with Planck, DESI DR1 BAO and SN data","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2411.19362","snapshot_observed_at":"2026-08-08T23:12:26.138825Z","title":"A preference for dynamical phan- tom dark energy using one-parameter model with Planck, DESI DR1 BAO and SN data,","venue":null,"work_id":null,"year":2024},"citing_paper":{"arxiv_id":"2502.04212","last_updated":"2025-07-17T16:27:03Z","snapshot_observed_at":"2026-08-09T04:53:21.314754Z","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":54,"source":"pdf_text","source_observed_at":"2026-08-08T23:12:26.138825Z"},"links":{"cited_paper":"/paper/2411.19362","citing_paper":"/paper/2502.04212"},"observation_digest":"sha256:0b57d6ed3294033390030b9f9790b05d0a3ee9d3fe72749075341639d4dae279","observation_id":"c324ca3c-4d0a-4e69-bee9-6d053801514c","resolution":{"observed_at":"2026-08-08T23:12:26.138825Z","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":"2026-08-08T23:12:26.143211Z","title":"Prob- ing the sign-changeable interaction between dark energy and dark matter with DESI baryon acoustic oscillations and DES supernovae data,","venue":null,"work_id":null,"year":2025},"citing_paper":{"arxiv_id":"2502.04212","last_updated":"2025-07-17T16:27:03Z","snapshot_observed_at":"2026-08-09T04:53:21.314754Z","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":55,"source":"pdf_text","source_observed_at":"2026-08-08T23:12:26.143211Z"},"links":{"citing_paper":"/paper/2502.04212"},"observation_digest":"sha256:ffd2eb90719e1a29aa8eb2e2e32cd63890f85a0f6567b17054c5f68ab57ca6ae","observation_id":"045d8f2a-1d28-4512-b686-f4ea3be5b3b4","resolution":{"observed_at":"2026-08-08T23:12:26.143211Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"1607.03155","last_updated":"2016-07-11T20:29:52Z","snapshot_observed_at":"2026-07-06T05:03:11.934242Z","submitted_at":"2016-07-11T20:29:52Z","title":"The clustering of galaxies in the completed SDSS-III Baryon Oscillation Spectroscopic Survey: cosmological analysis of the DR12 galaxy sample","version":1},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"1607.03155","snapshot_observed_at":"2026-08-08T23:12:26.146533Z","title":"The clustering of galaxies in the completed SDSS-III Baryon Oscillation Spectro- scopic Survey: cosmological analysis of the DR12 galaxy sample,","venue":null,"work_id":null,"year":2017},"citing_paper":{"arxiv_id":"2502.04212","last_updated":"2025-07-17T16:27:03Z","snapshot_observed_at":"2026-08-09T04:53:21.314754Z","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":56,"source":"pdf_text","source_observed_at":"2026-08-08T23:12:26.146533Z"},"links":{"cited_paper":"/paper/1607.03155","citing_paper":"/paper/2502.04212"},"observation_digest":"sha256:9620dd241bb98d91b19cffc439148362827e4b673a6078673269c2b36e312ade","observation_id":"69a12525-686c-4e59-9537-0b4318265e3b","resolution":{"observed_at":"2026-08-08T23:12:26.146533Z","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":"2026-08-08T23:12:26.149898Z","title":"A Comprehensive Measure- ment of the Local Value of the Hubble Constant with 1 km/s/Mpc Uncertainty from the Hubble Space Tele- scope and the SH0ES Team,","venue":null,"work_id":null,"year":2022},"citing_paper":{"arxiv_id":"2502.04212","last_updated":"2025-07-17T16:27:03Z","snapshot_observed_at":"2026-08-09T04:53:21.314754Z","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":57,"source":"pdf_text","source_observed_at":"2026-08-08T23:12:26.149898Z"},"links":{"cited_paper":"/paper/2112.04510","citing_paper":"/paper/2502.04212"},"observation_digest":"sha256:f69d738ab4dcb187e732d2d08ced766f50e365a2f2a5ad64c88243361dbff06c","observation_id":"33ca6360-e4c4-4211-9344-41152a6cce72","resolution":{"observed_at":"2026-08-08T23:12:26.149898Z","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":"2026-08-08T23:12:26.153714Z","title":"The Pantheon+ Analysis: Cos- mological Constraints,","venue":null,"work_id":null,"year":2022},"citing_paper":{"arxiv_id":"2502.04212","last_updated":"2025-07-17T16:27:03Z","snapshot_observed_at":"2026-08-09T04:53:21.314754Z","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":58,"source":"pdf_text","source_observed_at":"2026-08-08T23:12:26.153714Z"},"links":{"cited_paper":"/paper/2202.04077","citing_paper":"/paper/2502.04212"},"observation_digest":"sha256:307f571bbf658f9620eb00228afaaba6c603573fd5359ec51833975a6df30796","observation_id":"e1a31702-4702-4524-b52d-873b6e61b826","resolution":{"observed_at":"2026-08-08T23:12:26.153714Z","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":"2026-08-08T23:12:26.157389Z","title":"The Pantheon+ Analysis: The Full Data Set and Light-curve Release,","venue":null,"work_id":null,"year":2022},"citing_paper":{"arxiv_id":"2502.04212","last_updated":"2025-07-17T16:27:03Z","snapshot_observed_at":"2026-08-09T04:53:21.314754Z","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":59,"source":"pdf_text","source_observed_at":"2026-08-08T23:12:26.157389Z"},"links":{"cited_paper":"/paper/2112.03863","citing_paper":"/paper/2502.04212"},"observation_digest":"sha256:8019f102fc236e388c2b594c410edc7c10ebf8d54df24e701069819683f4e0da","observation_id":"bef6d92d-7ee7-4665-bfcc-8bf29d9272e2","resolution":{"observed_at":"2026-08-08T23:12:26.157389Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2112.03864","last_updated":"2022-11-14T21:29:39Z","snapshot_observed_at":"2026-07-06T12:16:15.735863Z","submitted_at":"2021-12-07T17:57:24Z","title":"The Pantheon+ Analysis: SuperCal-Fragilistic Cross Calibration, Retrained SALT2 Light Curve Model, and Calibration Systematic Uncertainty","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2112.03864","snapshot_observed_at":"2026-08-08T23:12:26.160864Z","title":"The Pantheon+ Analysis: SuperCal-fragilistic Cross Calibration, Retrained SALT2 Light-curve Model, and Calibration System- atic Uncertainty,","venue":null,"work_id":null,"year":2022},"citing_paper":{"arxiv_id":"2502.04212","last_updated":"2025-07-17T16:27:03Z","snapshot_observed_at":"2026-08-09T04:53:21.314754Z","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":60,"source":"pdf_text","source_observed_at":"2026-08-08T23:12:26.160864Z"},"links":{"cited_paper":"/paper/2112.03864","citing_paper":"/paper/2502.04212"},"observation_digest":"sha256:6c13ff78229f14c2c413d9cb9827a40999f876cfce037c6e06f5563949128bee","observation_id":"7495864c-6667-4f78-8e66-8d1702f6d3da","resolution":{"observed_at":"2026-08-08T23:12:26.160864Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2110.03487","last_updated":"2022-01-13T19:34:14Z","snapshot_observed_at":"2026-07-06T11:55:24.902179Z","submitted_at":"2021-10-07T14:14:05Z","title":"The Pantheon+ Analysis: Evaluating Peculiar Velocity Corrections in Cosmological Analyses with Nearby Type Ia Supernovae","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2110.03487","snapshot_observed_at":"2026-08-08T23:12:26.164118Z","title":"The Pantheon+ Analysis: Evaluating Peculiar Velocity Corrections in Cosmolog- ical Analyses with Nearby Type Ia Supernovae,","venue":null,"work_id":null,"year":2022},"citing_paper":{"arxiv_id":"2502.04212","last_updated":"2025-07-17T16:27:03Z","snapshot_observed_at":"2026-08-09T04:53:21.314754Z","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":61,"source":"pdf_text","source_observed_at":"2026-08-08T23:12:26.164118Z"},"links":{"cited_paper":"/paper/2110.03487","citing_paper":"/paper/2502.04212"},"observation_digest":"sha256:619c98a56b623b48cfe25226c70850b4c83fcb0cf94739334dddac86abf5f02c","observation_id":"8c2db4c9-acf8-4a68-860c-77383b2e57fd","resolution":{"observed_at":"2026-08-08T23:12:26.164118Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2112.01471","last_updated":"2022-10-11T10:05:42Z","snapshot_observed_at":"2026-07-06T12:14:46.481396Z","submitted_at":"2021-12-02T18:15:50Z","title":"The Pantheon+ Analysis: Improving the Redshifts and Peculiar Velocities of Type Ia Supernovae Used in Cosmological Analyses","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2112.01471","snapshot_observed_at":"2026-08-08T23:12:26.167642Z","title":"The Pantheon+ analysis: Im- proving the redshifts and peculiar velocities of Type Ia supernovae used in cosmological analyses,","venue":null,"work_id":null,"year":2022},"citing_paper":{"arxiv_id":"2502.04212","last_updated":"2025-07-17T16:27:03Z","snapshot_observed_at":"2026-08-09T04:53:21.314754Z","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":62,"source":"pdf_text","source_observed_at":"2026-08-08T23:12:26.167642Z"},"links":{"cited_paper":"/paper/2112.01471","citing_paper":"/paper/2502.04212"},"observation_digest":"sha256:2dcaef706299c6b356ec1b81c0b41b7f907a08eb9f6bbd43f02882f21a24fa2a","observation_id":"df43478c-0739-4490-af3e-9a7059b90903","resolution":{"observed_at":"2026-08-08T23:12:26.167642Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2112.04456","last_updated":"2022-12-05T15:40:08Z","snapshot_observed_at":"2026-08-04T03:22:16.395529Z","submitted_at":"2021-12-08T18:31:33Z","title":"The Pantheon+ Analysis: Forward-Modeling the Dust and Intrinsic Colour Distributions of Type Ia Supernovae, and Quantifying their Impact on Cosmological Inferences","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2112.04456","snapshot_observed_at":"2026-08-08T23:12:26.171295Z","title":"The Pantheon+ Analysis: Forward 10 Modeling the Dust and Intrinsic Color Distributions of Type Ia Supernovae, and Quantifying Their Impact on Cosmological Inferences,","venue":null,"work_id":null,"year":2023},"citing_paper":{"arxiv_id":"2502.04212","last_updated":"2025-07-17T16:27:03Z","snapshot_observed_at":"2026-08-09T04:53:21.314754Z","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":63,"source":"pdf_text","source_observed_at":"2026-08-08T23:12:26.171295Z"},"links":{"cited_paper":"/paper/2112.04456","citing_paper":"/paper/2502.04212"},"observation_digest":"sha256:e444acbb5e668208e5713f005758af877f57637bc8a80847f01e0049918968b2","observation_id":"54b4c831-fd23-4bd6-ab30-1202d3e8878f","resolution":{"observed_at":"2026-08-08T23:12:26.171295Z","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":"2026-07-06T19:35:21.868885Z","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":"2026-08-08T23:12:26.174471Z","title":"Is the w0waCDM cosmological parameteriza- tion evidence for dark energy dynamics partially caused by the excess smoothing of Planck CMB anisotropy data?","venue":null,"work_id":null,"year":2024},"citing_paper":{"arxiv_id":"2502.04212","last_updated":"2025-07-17T16:27:03Z","snapshot_observed_at":"2026-08-09T04:53:21.314754Z","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":64,"source":"pdf_text","source_observed_at":"2026-08-08T23:12:26.174471Z"},"links":{"cited_paper":"/paper/2410.13627","citing_paper":"/paper/2502.04212"},"observation_digest":"sha256:b7358669a982fd7552566d3f7085734aeca08b8b06cf5b67266caa7a8a9617e7","observation_id":"fb5de902-a962-48a7-9d73-a899d93b99df","resolution":{"observed_at":"2026-08-08T23:12:26.174471Z","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":"2026-08-06T19:18:03.475201Z","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":"2026-08-08T23:12:26.177828Z","title":"Is excess smoothing of Planck CMB ansiotropy data partially responsible for evidence for dark energy dynam- ics in other w(z)CDM parametrizations?","venue":null,"work_id":null,"year":2025},"citing_paper":{"arxiv_id":"2502.04212","last_updated":"2025-07-17T16:27:03Z","snapshot_observed_at":"2026-08-09T04:53:21.314754Z","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":65,"source":"pdf_text","source_observed_at":"2026-08-08T23:12:26.177828Z"},"links":{"cited_paper":"/paper/2501.03480","citing_paper":"/paper/2502.04212"},"observation_digest":"sha256:61ec8c76c6e2f7a85314f30d56fddd0dc6fa95f75aa3b46dc9b0c31030b25730","observation_id":"fcf69485-f640-48c0-af2f-dad6b6c81b9b","resolution":{"observed_at":"2026-08-08T23:12:26.177828Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2407.04385","last_updated":"2024-07-12T10:45:03Z","snapshot_observed_at":"2026-07-06T18:41:53.152987Z","submitted_at":"2024-07-05T09:43:53Z","title":"Impact of LRG1 and LRG2 in DESI 2024 BAO data on dark energy evolution","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2407.04385","snapshot_observed_at":"2026-08-08T23:12:26.182115Z","title":"Impact of LRG1 and LRG2 in DESI 2024 BAO data on dark energy evolution,","venue":null,"work_id":null,"year":2024},"citing_paper":{"arxiv_id":"2502.04212","last_updated":"2025-07-17T16:27:03Z","snapshot_observed_at":"2026-08-09T04:53:21.314754Z","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":66,"source":"pdf_text","source_observed_at":"2026-08-08T23:12:26.182115Z"},"links":{"cited_paper":"/paper/2407.04385","citing_paper":"/paper/2502.04212"},"observation_digest":"sha256:21368ce1e00d643c15714e32edebc2435823cf38ae31c6e8ac7cb35e8ff88346","observation_id":"f5c072c8-009a-45d1-b7a4-3a21122f67f7","resolution":{"observed_at":"2026-08-08T23:12:26.182115Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2406.06389","last_updated":"2025-02-27T16:54:15Z","snapshot_observed_at":"2026-08-10T04:12:14.868399Z","submitted_at":"2024-06-10T15:45:15Z","title":"Implications of DES 5YR SNe Dataset for $\\Lambda$CDM","version":3},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2406.06389","snapshot_observed_at":"2026-08-08T23:12:26.185625Z","title":"Implications of DES 5YR SNe Dataset for ΛCDM,","venue":null,"work_id":null,"year":2025},"citing_paper":{"arxiv_id":"2502.04212","last_updated":"2025-07-17T16:27:03Z","snapshot_observed_at":"2026-08-09T04:53:21.314754Z","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":67,"source":"pdf_text","source_observed_at":"2026-08-08T23:12:26.185625Z"},"links":{"cited_paper":"/paper/2406.06389","citing_paper":"/paper/2502.04212"},"observation_digest":"sha256:9487b81eb6ebddb18e206ac919b10a9a9f87c9571736c296c85f744678213634","observation_id":"d744406d-ae2a-4104-a175-b643d8834c27","resolution":{"observed_at":"2026-08-08T23:12:26.185625Z","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":"2026-08-07T05:02:21.520500Z","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":"2026-08-09T04:53:21.314754Z","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":"sha256:5f8f4f286719dc3ae22d915ba58fd8c1714501b29ae697b265535795164669e2","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":"2405.02168","last_updated":"2024-05-30T15:32:11Z","snapshot_observed_at":"2026-07-06T18:09:25.715693Z","submitted_at":"2024-05-03T15:17:15Z","title":"The role of LRG1 and LRG2's monopole in inferring the DESI 2024 BAO cosmology","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2405.02168","snapshot_observed_at":"2026-08-08T23:12:26.192436Z","title":"The role of LRG1 and LRG2’s monopole in infer- ring the DESI 2024 BAO cosmology,","venue":null,"work_id":null,"year":2024},"citing_paper":{"arxiv_id":"2502.04212","last_updated":"2025-07-17T16:27:03Z","snapshot_observed_at":"2026-08-09T04:53:21.314754Z","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":69,"source":"pdf_text","source_observed_at":"2026-08-08T23:12:26.192436Z"},"links":{"cited_paper":"/paper/2405.02168","citing_paper":"/paper/2502.04212"},"observation_digest":"sha256:6e215801ff106808b296100b084492234eadb71db4de2df682d9ea7f787facca","observation_id":"6afef57e-f725-46d9-8c40-24de84292f62","resolution":{"observed_at":"2026-08-08T23:12:26.192436Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2405.03983","last_updated":"2025-02-20T09:04:47Z","snapshot_observed_at":"2026-07-06T18:10:45.376531Z","submitted_at":"2024-05-07T03:47:26Z","title":"Key drivers of the preference for dynamic dark energy","version":4},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2405.03983","snapshot_observed_at":"2026-08-08T23:12:26.195708Z","title":"Key drivers of the preference for dy- namic dark energy,","venue":null,"work_id":null,"year":2024},"citing_paper":{"arxiv_id":"2502.04212","last_updated":"2025-07-17T16:27:03Z","snapshot_observed_at":"2026-08-09T04:53:21.314754Z","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":70,"source":"pdf_text","source_observed_at":"2026-08-08T23:12:26.195708Z"},"links":{"cited_paper":"/paper/2405.03983","citing_paper":"/paper/2502.04212"},"observation_digest":"sha256:3dfb7b77ebd98826730a6e4e862253d6a129fae3a31454f43e5971d929943a03","observation_id":"d019e1fb-6651-4ded-9756-9f46efe8e655","resolution":{"observed_at":"2026-08-08T23:12:26.195708Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2409.18668","last_updated":"2024-09-27T11:53:38Z","snapshot_observed_at":"2026-07-06T19:23:19.829130Z","submitted_at":"2024-09-27T11:53:38Z","title":"The axis of systematic bias in SN~Ia cosmology and implications for DESI 2024 results","version":1},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2409.18668","snapshot_observed_at":"2026-08-08T23:12:26.200474Z","title":"The axis of systematic bias in SN˜Ia cosmology and implications for DESI 2024 results,","venue":null,"work_id":null,"year":2025},"citing_paper":{"arxiv_id":"2502.04212","last_updated":"2025-07-17T16:27:03Z","snapshot_observed_at":"2026-08-09T04:53:21.314754Z","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":71,"source":"pdf_text","source_observed_at":"2026-08-08T23:12:26.200474Z"},"links":{"cited_paper":"/paper/2409.18668","citing_paper":"/paper/2502.04212"},"observation_digest":"sha256:ba2c7bb257a9b1acace267de5aaedbf248562854396ac237e01d174c790acef7","observation_id":"eda1940b-0d86-456e-b419-ad192dec3127","resolution":{"observed_at":"2026-08-08T23:12:26.200474Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2409.13022","last_updated":"2024-11-17T16:25:29Z","snapshot_observed_at":"2026-07-06T02:11:23.670680Z","submitted_at":"2024-09-19T18:00:26Z","title":"Updated Cosmological Constraints in Extended Parameter Space with Planck PR4, DESI Baryon Acoustic Oscillations, and Supernovae: Dynamical Dark Energy, Neutrino Masses, Lensing Anomaly, and the Hubble Tension","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2409.13022","snapshot_observed_at":"2026-08-08T23:12:26.204461Z","title":null,"venue":null,"work_id":null,"year":2024},"citing_paper":{"arxiv_id":"2502.04212","last_updated":"2025-07-17T16:27:03Z","snapshot_observed_at":"2026-08-09T04:53:21.314754Z","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":72,"source":"pdf_text","source_observed_at":"2026-08-08T23:12:26.204461Z"},"links":{"cited_paper":"/paper/2409.13022","citing_paper":"/paper/2502.04212"},"observation_digest":"sha256:0d3eb8d6ea4f714059fb399c9e32018611f0fe981c04082e52bd3d43c8ab7d41","observation_id":"7cb046ed-2b47-4f7d-a314-91ef0bb69f03","resolution":{"observed_at":"2026-08-08T23:12:26.204461Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2406.07533","last_updated":"2025-02-25T19:56:20Z","snapshot_observed_at":"2026-08-06T15:27:47.254399Z","submitted_at":"2024-06-11T17:56:31Z","title":"Interpreting DESI 2024 BAO: late-time dynamical dark energy or a local effect?","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2406.07533","snapshot_observed_at":"2026-08-08T23:12:26.207929Z","title":"Interpreting DESI 2024 BAO: Late-time dy- namical dark energy or a local effect?","venue":null,"work_id":null,"year":2025},"citing_paper":{"arxiv_id":"2502.04212","last_updated":"2025-07-17T16:27:03Z","snapshot_observed_at":"2026-08-09T04:53:21.314754Z","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":73,"source":"pdf_text","source_observed_at":"2026-08-08T23:12:26.207929Z"},"links":{"cited_paper":"/paper/2406.07533","citing_paper":"/paper/2502.04212"},"observation_digest":"sha256:8b0b281b4eff8e473a625c029eeae14fdce75def42a26c15467719a4cca893ec","observation_id":"d2963e63-707e-4452-b46a-aaac97e8f49c","resolution":{"observed_at":"2026-08-08T23:12:26.207929Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2408.07175","last_updated":"2025-02-03T16:49:31Z","snapshot_observed_at":"2026-08-04T21:49:49.398185Z","submitted_at":"2024-08-13T19:37:46Z","title":"Evolving Dark Energy or Supernovae Systematics?","version":3},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2408.07175","snapshot_observed_at":"2026-08-08T23:12:26.211635Z","title":"Evolving dark energy or supernovae systematics?","venue":null,"work_id":null,"year":2025},"citing_paper":{"arxiv_id":"2502.04212","last_updated":"2025-07-17T16:27:03Z","snapshot_observed_at":"2026-08-09T04:53:21.314754Z","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":74,"source":"pdf_text","source_observed_at":"2026-08-08T23:12:26.211635Z"},"links":{"cited_paper":"/paper/2408.07175","citing_paper":"/paper/2502.04212"},"observation_digest":"sha256:dc6a486039a3c250c506c5fab55ad8e6a84aa13a0725b236bbd3299f35be6a11","observation_id":"e67c6e41-4f42-4546-9619-66c363dfec58","resolution":{"observed_at":"2026-08-08T23:12:26.211635Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2411.11685","last_updated":"2024-11-18T16:10:16Z","snapshot_observed_at":"2026-08-03T06:19:50.797140Z","submitted_at":"2024-11-18T16:10:16Z","title":"BAO vs. SN evidence for evolving dark energy","version":1},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2411.11685","snapshot_observed_at":"2026-08-08T23:12:26.215685Z","title":"BAO vs. SN evidence for evolving dark energy,","venue":null,"work_id":null,"year":2025},"citing_paper":{"arxiv_id":"2502.04212","last_updated":"2025-07-17T16:27:03Z","snapshot_observed_at":"2026-08-09T04:53:21.314754Z","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":75,"source":"pdf_text","source_observed_at":"2026-08-08T23:12:26.215685Z"},"links":{"cited_paper":"/paper/2411.11685","citing_paper":"/paper/2502.04212"},"observation_digest":"sha256:b3c8d2c595c64981fc8d21e38eb68d2a85266b975152fc83fe81540de285d6cb","observation_id":"6d53f37c-1098-438b-8a61-babcd83cfe17","resolution":{"observed_at":"2026-08-08T23:12:26.215685Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2501.14366","last_updated":"2025-01-24T09:59:06Z","snapshot_observed_at":"2026-08-10T15:11:30.869399Z","submitted_at":"2025-01-24T09:59:06Z","title":"Uncovering the bias in the evidence for dynamical dark energy through minimal and generalized modeling approaches","version":1},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2501.14366","snapshot_observed_at":"2026-08-08T23:12:26.219182Z","title":"Uncovering the bias in the evidence for dy- namical dark energy through minimal and generalized modeling approaches,","venue":null,"work_id":null,"year":2025},"citing_paper":{"arxiv_id":"2502.04212","last_updated":"2025-07-17T16:27:03Z","snapshot_observed_at":"2026-08-09T04:53:21.314754Z","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":76,"source":"pdf_text","source_observed_at":"2026-08-08T23:12:26.219182Z"},"links":{"cited_paper":"/paper/2501.14366","citing_paper":"/paper/2502.04212"},"observation_digest":"sha256:3878c21ec07840f793f012027fc53c7b9ec211e70caedc18fc1c45ec8cecd915","observation_id":"a9ab532e-1f08-4006-a218-2d96d653e0bc","resolution":{"observed_at":"2026-08-08T23:12:26.219182Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2501.06664","last_updated":"2025-01-11T23:32:58Z","snapshot_observed_at":"2026-07-06T20:19:50.997046Z","submitted_at":"2025-01-11T23:32:58Z","title":"Comparing the DES-SN5YR and Pantheon+ SN cosmology analyses: Investigation based on \"Evolving Dark Energy or Supernovae systematics?\"","version":1},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2501.06664","snapshot_observed_at":"2026-08-08T23:12:26.222665Z","title":"Comparing the DES-SN5YR and Pantheon+ SN cosmology analyses: Investigation based on","venue":null,"work_id":null,"year":2025},"citing_paper":{"arxiv_id":"2502.04212","last_updated":"2025-07-17T16:27:03Z","snapshot_observed_at":"2026-08-09T04:53:21.314754Z","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":77,"source":"pdf_text","source_observed_at":"2026-08-08T23:12:26.222665Z"},"links":{"cited_paper":"/paper/2501.06664","citing_paper":"/paper/2502.04212"},"observation_digest":"sha256:aa33cfbbf9483a9b018c1fbb6db4d6e17d54ced7b2486da07a06f3d21875835c","observation_id":"4e88a307-f0c8-4936-9937-e79ba91e3aaf","resolution":{"observed_at":"2026-08-08T23:12:26.222665Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"1709.05146","last_updated":"2017-11-07T19:50:49Z","snapshot_observed_at":"2026-07-06T05:59:49.044637Z","submitted_at":"2017-09-15T10:44:39Z","title":"The Carnegie Supernova Project I: Third Photometry Data Release of Low-Redshift Type Ia Supernovae and Other White Dwarf Explosions","version":3},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"1709.05146","snapshot_observed_at":"2026-08-08T23:12:26.225928Z","title":"The Carnegie Supernova Project I: Third Photometry Data Release of Low- Redshift Type Ia Supernovae and Other White Dwarf Explosions,","venue":null,"work_id":null,"year":2017},"citing_paper":{"arxiv_id":"2502.04212","last_updated":"2025-07-17T16:27:03Z","snapshot_observed_at":"2026-08-09T04:53:21.314754Z","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":78,"source":"pdf_text","source_observed_at":"2026-08-08T23:12:26.225928Z"},"links":{"cited_paper":"/paper/1709.05146","citing_paper":"/paper/2502.04212"},"observation_digest":"sha256:e56d196586d1adbfffc1b3ebc880f4fa3e7bf20f0212475ef4f86cc4d3561228","observation_id":"b49a0f5d-a5e1-4263-80da-a173413c127d","resolution":{"observed_at":"2026-08-08T23:12:26.225928Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"0901.4787","last_updated":"2009-06-14T14:05:10Z","snapshot_observed_at":"2026-07-06T01:50:53.158645Z","submitted_at":"2009-01-30T00:07:27Z","title":"CfA3: 185 Type Ia Supernova Light Curves from the CfA","version":5},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"0901.4787","snapshot_observed_at":"2026-08-08T23:12:26.229494Z","title":"CfA3: 185 Type Ia Su- pernova Light Curves from the CfA,","venue":null,"work_id":null,"year":2009},"citing_paper":{"arxiv_id":"2502.04212","last_updated":"2025-07-17T16:27:03Z","snapshot_observed_at":"2026-08-09T04:53:21.314754Z","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":79,"source":"pdf_text","source_observed_at":"2026-08-08T23:12:26.229494Z"},"links":{"cited_paper":"/paper/0901.4787","citing_paper":"/paper/2502.04212"},"observation_digest":"sha256:adb9a566360ce7aa5832fd827b90c2ec972a3a968743e82d73f64215f283aebf","observation_id":"73fefc38-bdf8-4b0d-b72e-4756c85e1637","resolution":{"observed_at":"2026-08-08T23:12:26.229494Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"1205.4493","last_updated":"2012-05-21T05:49:01Z","snapshot_observed_at":"2026-07-06T02:48:27.195790Z","submitted_at":"2012-05-21T05:49:01Z","title":"CfA4: Light Curves for 94 Type Ia Supernovae","version":1},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"1205.4493","snapshot_observed_at":"2026-08-08T23:12:26.232789Z","title":"CfA4: Light Curves for 94 Type Ia Supernovae,","venue":null,"work_id":null,"year":2012},"citing_paper":{"arxiv_id":"2502.04212","last_updated":"2025-07-17T16:27:03Z","snapshot_observed_at":"2026-08-09T04:53:21.314754Z","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":80,"source":"pdf_text","source_observed_at":"2026-08-08T23:12:26.232789Z"},"links":{"cited_paper":"/paper/1205.4493","citing_paper":"/paper/2502.04212"},"observation_digest":"sha256:6dd8534cadac085860e87712161a07a0ca9b0f7fa33bf9b4059e72a1384864dc","observation_id":"545b53dc-0050-4ae1-adf4-8d3ac09bea1a","resolution":{"observed_at":"2026-08-08T23:12:26.232789Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"1711.02474","last_updated":"2017-11-06T18:59:59Z","snapshot_observed_at":"2026-08-02T06:55:45.489670Z","submitted_at":"2017-11-06T18:59:59Z","title":"The Foundation Supernova Survey: Motivation, Design, Implementation, and First Data Release","version":1},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"1711.02474","snapshot_observed_at":"2026-08-08T23:12:26.236682Z","title":"The Foundation Supernova Sur- vey: Motivation, Design, Implementation, and First Data Release,","venue":null,"work_id":null,"year":2018},"citing_paper":{"arxiv_id":"2502.04212","last_updated":"2025-07-17T16:27:03Z","snapshot_observed_at":"2026-08-09T04:53:21.314754Z","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":81,"source":"pdf_text","source_observed_at":"2026-08-08T23:12:26.236682Z"},"links":{"cited_paper":"/paper/1711.02474","citing_paper":"/paper/2502.04212"},"observation_digest":"sha256:20aba78f5f35f1c8bd78b238de8d154fc0e1e96cea748d580504c8ae5be1acd2","observation_id":"e8aa698e-0e32-4089-bd06-c73d4b57f56e","resolution":{"observed_at":"2026-08-08T23:12:26.236682Z","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":"2026-08-09T04:23:25.022919Z","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":"2026-08-08T23:12:26.240232Z","title":"No- go guide for the Hubble tension: Late-time or local- scale new physics,","venue":null,"work_id":null,"year":2025},"citing_paper":{"arxiv_id":"2502.04212","last_updated":"2025-07-17T16:27:03Z","snapshot_observed_at":"2026-08-09T04:53:21.314754Z","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":82,"source":"pdf_text","source_observed_at":"2026-08-08T23:12:26.240232Z"},"links":{"cited_paper":"/paper/2401.14170","citing_paper":"/paper/2502.04212"},"observation_digest":"sha256:2330bb757208227d9b790d70f5b9251919f39d6a84585411e38225a4510983c1","observation_id":"e0bdb775-b6cb-41a0-b924-daa4e06470aa","resolution":{"observed_at":"2026-08-08T23:12:26.240232Z","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":"2026-08-04T05:31:17.968660Z","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":"2026-08-08T23:12:26.243555Z","title":"Narrowing down the Hub- ble tension to the first two rungs of distance ladders,","venue":null,"work_id":null,"year":2025},"citing_paper":{"arxiv_id":"2502.04212","last_updated":"2025-07-17T16:27:03Z","snapshot_observed_at":"2026-08-09T04:53:21.314754Z","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":83,"source":"pdf_text","source_observed_at":"2026-08-08T23:12:26.243555Z"},"links":{"cited_paper":"/paper/2410.06053","citing_paper":"/paper/2502.04212"},"observation_digest":"sha256:c34ba14a6cbf1a07d619c3721ba60fc9fd340ad5d7757f4257e68ca50369dad1","observation_id":"bf7686a6-d104-4552-a73f-d7c9ccc2ac32","resolution":{"observed_at":"2026-08-08T23:12:26.243555Z","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":"2026-07-06T02:11:23.670680Z","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":"2026-08-08T23:12:26.246879Z","title":"Union Through UNITY: Cosmol- ogy with 2,000 SNe Using a Unified Bayesian Frame- work,","venue":null,"work_id":null,"year":2023},"citing_paper":{"arxiv_id":"2502.04212","last_updated":"2025-07-17T16:27:03Z","snapshot_observed_at":"2026-08-09T04:53:21.314754Z","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":84,"source":"pdf_text","source_observed_at":"2026-08-08T23:12:26.246879Z"},"links":{"cited_paper":"/paper/2311.12098","citing_paper":"/paper/2502.04212"},"observation_digest":"sha256:298c2fe1229f26db5d1040902e456fa5878f76311265d78d5d922b368df13a7a","observation_id":"25bff443-1d8d-47f6-8fc9-916924cd8a7b","resolution":{"observed_at":"2026-08-08T23:12:26.246879Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"1210.7183","last_updated":"2012-10-31T15:31:08Z","snapshot_observed_at":"2026-07-06T02:58:31.428367Z","submitted_at":"2012-10-26T16:43:43Z","title":"Conservative Constraints on Early Cosmology: an illustration of the Monte Python cosmological parameter inference code","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"1210.7183","snapshot_observed_at":"2026-08-08T23:12:26.250134Z","title":"Conservative Constraints on Early Cosmology: an illustration of the Monte Python cos- mological parameter inference code,","venue":null,"work_id":null,"year":2013},"citing_paper":{"arxiv_id":"2502.04212","last_updated":"2025-07-17T16:27:03Z","snapshot_observed_at":"2026-08-09T04:53:21.314754Z","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":85,"source":"pdf_text","source_observed_at":"2026-08-08T23:12:26.250134Z"},"links":{"cited_paper":"/paper/1210.7183","citing_paper":"/paper/2502.04212"},"observation_digest":"sha256:666774d93b49a453978d4e549cf222fa9095f7ae0fa9477a03999fc9e908f55f","observation_id":"e7dcd73a-bd09-4aca-945d-54279a20e346","resolution":{"observed_at":"2026-08-08T23:12:26.250134Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2503.14738","last_updated":"2025-10-09T16:45:28Z","snapshot_observed_at":"2026-07-06T02:11:23.670680Z","submitted_at":"2025-03-18T21:14:12Z","title":"DESI DR2 Results II: Measurements of Baryon Acoustic Oscillations and Cosmological Constraints","version":3},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2503.14738","snapshot_observed_at":"2026-08-08T23:12:26.253494Z","title":"DESI DR2 Results II: Measurements of Baryon Acoustic Oscillations and Cosmological Constraints,","venue":null,"work_id":null,"year":2025},"citing_paper":{"arxiv_id":"2502.04212","last_updated":"2025-07-17T16:27:03Z","snapshot_observed_at":"2026-08-09T04:53:21.314754Z","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":86,"source":"pdf_text","source_observed_at":"2026-08-08T23:12:26.253494Z"},"links":{"cited_paper":"/paper/2503.14738","citing_paper":"/paper/2502.04212"},"observation_digest":"sha256:bb3b80a726c37de2ce6032bf633c4aed590d509606db869ff09b9e0d09fd1571","observation_id":"6da8b4f1-cbe6-465c-8119-bb2d359e5c6f","resolution":{"observed_at":"2026-08-08T23:12:26.253494Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2503.14739","last_updated":"2025-06-30T00:11:58Z","snapshot_observed_at":"2026-07-30T08:44:56.946347Z","submitted_at":"2025-03-18T21:14:13Z","title":"DESI DR2 Results I: Baryon Acoustic Oscillations from the Lyman Alpha Forest","version":3},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2503.14739","snapshot_observed_at":"2026-08-08T23:12:26.257397Z","title":"DESI DR2 Results I: Baryon Acoustic Oscillations from the Lyman Alpha Forest,","venue":null,"work_id":null,"year":2025},"citing_paper":{"arxiv_id":"2502.04212","last_updated":"2025-07-17T16:27:03Z","snapshot_observed_at":"2026-08-09T04:53:21.314754Z","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":87,"source":"pdf_text","source_observed_at":"2026-08-08T23:12:26.257397Z"},"links":{"cited_paper":"/paper/2503.14739","citing_paper":"/paper/2502.04212"},"observation_digest":"sha256:5c11878b91a1a4397f5b9638df079222f0613063b1560754575ae3cf8186d87a","observation_id":"00d72346-84d7-41ba-8fb7-7855918a25a0","resolution":{"observed_at":"2026-08-08T23:12:26.257397Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2503.14743","last_updated":"2025-04-03T13:50:59Z","snapshot_observed_at":"2026-07-06T20:55:04.493800Z","submitted_at":"2025-03-18T21:14:17Z","title":"Extended Dark Energy analysis using DESI DR2 BAO measurements","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2503.14743","snapshot_observed_at":"2026-08-08T23:12:26.260771Z","title":"Extended Dark Energy anal- ysis using DESI DR2 BAO measurements,","venue":null,"work_id":null,"year":2025},"citing_paper":{"arxiv_id":"2502.04212","last_updated":"2025-07-17T16:27:03Z","snapshot_observed_at":"2026-08-09T04:53:21.314754Z","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":88,"source":"pdf_text","source_observed_at":"2026-08-08T23:12:26.260771Z"},"links":{"cited_paper":"/paper/2503.14743","citing_paper":"/paper/2502.04212"},"observation_digest":"sha256:2f7c33dd79e22618f5dc95187fa0607576d98505e1dfeceff8c4eb6cd216dc79","observation_id":"e06a7b74-b793-48fa-80b0-e7f586f48065","resolution":{"observed_at":"2026-08-08T23:12:26.260771Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2503.14744","last_updated":"2025-10-07T13:00:34Z","snapshot_observed_at":"2026-07-06T20:55:04.493800Z","submitted_at":"2025-03-18T21:14:18Z","title":"Constraints on Neutrino Physics from DESI DR2 BAO and DR1 Full Shape","version":3},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2503.14744","snapshot_observed_at":"2026-08-08T23:12:26.264044Z","title":"Constraints on Neutrino Physics from DESI DR2 BAO and DR1 Full Shape,","venue":null,"work_id":null,"year":2025},"citing_paper":{"arxiv_id":"2502.04212","last_updated":"2025-07-17T16:27:03Z","snapshot_observed_at":"2026-08-09T04:53:21.314754Z","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":89,"source":"pdf_text","source_observed_at":"2026-08-08T23:12:26.264044Z"},"links":{"cited_paper":"/paper/2503.14744","citing_paper":"/paper/2502.04212"},"observation_digest":"sha256:d5e0c9dc0b18c1fab98e8cb8844fedbbb0961a22f40ca4b85ed21b72efede42f","observation_id":"31658183-1333-40c8-bd69-c0f4f65175fb","resolution":{"observed_at":"2026-08-08T23:12:26.264044Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"astro-ph/0410654","last_updated":"2004-10-27T10:10:01Z","snapshot_observed_at":"2026-08-04T11:44:16.401773Z","submitted_at":"2004-10-27T10:10:01Z","title":"Cosmological Evolution of a Quintom Model of Dark Energy","version":1},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"astro-ph/0410654","snapshot_observed_at":"2026-08-08T23:12:26.267568Z","title":"Cosmological evolution of a quin- tom model of dark energy,","venue":null,"work_id":null,"year":2005},"citing_paper":{"arxiv_id":"2502.04212","last_updated":"2025-07-17T16:27:03Z","snapshot_observed_at":"2026-08-09T04:53:21.314754Z","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":90,"source":"pdf_text","source_observed_at":"2026-08-08T23:12:26.267568Z"},"links":{"cited_paper":"/paper/astro-ph/0410654","citing_paper":"/paper/2502.04212"},"observation_digest":"sha256:63eb87774ceb73b26e07e777e1564e20d3d2145d8cbd46b2249348097bd487bd","observation_id":"778d34a8-fdef-4bb7-acf0-05b57afd88bd","resolution":{"observed_at":"2026-08-08T23:12:26.267568Z","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":"2026-08-08T23:12:26.271072Z","title":"Dark energy constraints from the cosmic age and super- nova,","venue":null,"work_id":null,"year":2005},"citing_paper":{"arxiv_id":"2502.04212","last_updated":"2025-07-17T16:27:03Z","snapshot_observed_at":"2026-08-09T04:53:21.314754Z","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":91,"source":"pdf_text","source_observed_at":"2026-08-08T23:12:26.271072Z"},"links":{"citing_paper":"/paper/2502.04212"},"observation_digest":"sha256:7ed4cf6c26e3ef0083235e42f700b0e820e3bcc673e0c10d0e3e06d416dafa43","observation_id":"922ca0ce-dd5a-476e-a51a-05ffdd623536","resolution":{"observed_at":"2026-08-08T23:12:26.271072Z","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":"2026-08-08T23:12:26.274678Z","title":"Oscillating quintom and the recurrent uni- verse,","venue":null,"work_id":null,"year":2006},"citing_paper":{"arxiv_id":"2502.04212","last_updated":"2025-07-17T16:27:03Z","snapshot_observed_at":"2026-08-09T04:53:21.314754Z","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":92,"source":"pdf_text","source_observed_at":"2026-08-08T23:12:26.274678Z"},"links":{"citing_paper":"/paper/2502.04212"},"observation_digest":"sha256:c6c412a36b729cf74bc951e2ec32a3489db5831efe17c8118a8d8c54d836ba81","observation_id":"cd5353a6-bed2-4220-8c3d-64ae928fc6f1","resolution":{"observed_at":"2026-08-08T23:12:26.274678Z","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":"2026-08-06T10:47:28.712447Z","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":"2026-08-08T23:12:26.277928Z","title":"Hints of Nonminimally Coupled Gravity in DESI 2024 Baryon Acoustic Oscillation Measurements,","venue":null,"work_id":null,"year":2025},"citing_paper":{"arxiv_id":"2502.04212","last_updated":"2025-07-17T16:27:03Z","snapshot_observed_at":"2026-08-09T04:53:21.314754Z","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":93,"source":"pdf_text","source_observed_at":"2026-08-08T23:12:26.277928Z"},"links":{"cited_paper":"/paper/2407.15832","citing_paper":"/paper/2502.04212"},"observation_digest":"sha256:414c7f977c8c453d2942dc925d8141fd2e6c6a7e253d3bc3cfc785c89320ccce","observation_id":"eb48835a-c879-4d61-a2de-d01e1d1a6b95","resolution":{"observed_at":"2026-08-08T23:12:26.277928Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2503.19898","last_updated":"2026-05-01T19:29:13Z","snapshot_observed_at":"2026-07-30T13:42:45.142853Z","submitted_at":"2025-03-25T17:56:31Z","title":"Non-minimally coupled gravity constraints from DESI DR2 data","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2503.19898","snapshot_observed_at":"2026-08-08T23:12:26.281783Z","title":"Non-minimally coupled gravity constraints from DESI DR2 data,","venue":null,"work_id":null,"year":2025},"citing_paper":{"arxiv_id":"2502.04212","last_updated":"2025-07-17T16:27:03Z","snapshot_observed_at":"2026-08-09T04:53:21.314754Z","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":94,"source":"pdf_text","source_observed_at":"2026-08-08T23:12:26.281783Z"},"links":{"cited_paper":"/paper/2503.19898","citing_paper":"/paper/2502.04212"},"observation_digest":"sha256:01b84b572d39beb5a5a6cd36d54c3fcad5e43af68591a7fb956a2edd14e20212","observation_id":"360298b9-928e-41d9-af38-ccf82f38805c","resolution":{"observed_at":"2026-08-08T23:12:26.281783Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2504.07679","last_updated":"2025-07-28T16:54:23Z","snapshot_observed_at":"2026-08-07T16:06:52.964745Z","submitted_at":"2025-04-10T12:07:47Z","title":"Assessing cosmological evidence for non-minimal coupling","version":3},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2504.07679","snapshot_observed_at":"2026-08-08T23:12:26.285596Z","title":"The Cosmologi- cal Evidence for Non-Minimal Coupling,","venue":null,"work_id":null,"year":2025},"citing_paper":{"arxiv_id":"2502.04212","last_updated":"2025-07-17T16:27:03Z","snapshot_observed_at":"2026-08-09T04:53:21.314754Z","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":95,"source":"pdf_text","source_observed_at":"2026-08-08T23:12:26.285596Z"},"links":{"cited_paper":"/paper/2504.07679","citing_paper":"/paper/2502.04212"},"observation_digest":"sha256:b03294f70b17fd4ecfd390ddb19435d9ba7af92bebf0bbb75674c5bf75d8394e","observation_id":"3c0eaaab-8e70-4812-8a02-983902c76949","resolution":{"observed_at":"2026-08-08T23:12:26.285596Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2406.13388","last_updated":"2024-11-18T18:51:19Z","snapshot_observed_at":"2026-07-06T18:33:32.806635Z","submitted_at":"2024-06-19T09:30:04Z","title":"Suppression without Thawing: Constraining Structure Formation and Dark Energy with Galaxy Clustering","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2406.13388","snapshot_observed_at":"2026-08-08T23:12:26.289395Z","title":"Suppression without Thawing: Con- straining Structure Formation and Dark Energy with Galaxy Clustering,","venue":null,"work_id":null,"year":2024},"citing_paper":{"arxiv_id":"2502.04212","last_updated":"2025-07-17T16:27:03Z","snapshot_observed_at":"2026-08-09T04:53:21.314754Z","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":96,"source":"pdf_text","source_observed_at":"2026-08-08T23:12:26.289395Z"},"links":{"cited_paper":"/paper/2406.13388","citing_paper":"/paper/2502.04212"},"observation_digest":"sha256:2062076e6afb7f7f86a093924e4eca95985da1d6891fb8eb084f8ec4b7cf05d5","observation_id":"8ba8679d-92ba-47af-b59b-172a76ac0572","resolution":{"observed_at":"2026-08-08T23:12:26.289395Z","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":"2026-08-09T14:54:56.148828Z","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":"2026-08-08T23:12:26.293360Z","title":"Matching current observational constraints with nonminimally coupled dark energy,","venue":null,"work_id":null,"year":2025},"citing_paper":{"arxiv_id":"2502.04212","last_updated":"2025-07-17T16:27:03Z","snapshot_observed_at":"2026-08-09T04:53:21.314754Z","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":97,"source":"pdf_text","source_observed_at":"2026-08-08T23:12:26.293360Z"},"links":{"cited_paper":"/paper/2409.17019","citing_paper":"/paper/2502.04212"},"observation_digest":"sha256:11c3e79d6efc1740b6ebfcd901d95bb9bf0b2a1ca1e18951a150770a1c43f499","observation_id":"163373ea-d6a7-457d-9970-037b778e4857","resolution":{"observed_at":"2026-08-08T23:12:26.293360Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2408.17318","last_updated":"2025-02-05T13:48:08Z","snapshot_observed_at":"2026-08-06T06:13:59.706902Z","submitted_at":"2024-08-30T14:26:37Z","title":"Scant evidence for thawing quintessence","version":3},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2408.17318","snapshot_observed_at":"2026-08-08T23:12:26.296866Z","title":"Scant evidence for thawing quintessence,","venue":null,"work_id":null,"year":2024},"citing_paper":{"arxiv_id":"2502.04212","last_updated":"2025-07-17T16:27:03Z","snapshot_observed_at":"2026-08-09T04:53:21.314754Z","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":98,"source":"pdf_text","source_observed_at":"2026-08-08T23:12:26.296866Z"},"links":{"cited_paper":"/paper/2408.17318","citing_paper":"/paper/2502.04212"},"observation_digest":"sha256:1545f17fd4b91a08d18a2c07850cb7fa01ae72f0389c81ad02a3f8fcf57d77e6","observation_id":"0c036bd8-6b5d-4000-b8e8-d00cc123f2b7","resolution":{"observed_at":"2026-08-08T23:12:26.296866Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2102.02020","last_updated":"2021-06-06T05:08:23Z","snapshot_observed_at":"2026-08-06T18:31:21.876384Z","submitted_at":"2021-02-03T11:44:08Z","title":"Chameleon dark energy can resolve the Hubble tension","version":4},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2102.02020","snapshot_observed_at":"2026-08-08T23:12:26.300453Z","title":"Chameleon dark energy can resolve the Hubble tension,","venue":null,"work_id":null,"year":2021},"citing_paper":{"arxiv_id":"2502.04212","last_updated":"2025-07-17T16:27:03Z","snapshot_observed_at":"2026-08-09T04:53:21.314754Z","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":99,"source":"pdf_text","source_observed_at":"2026-08-08T23:12:26.300453Z"},"links":{"cited_paper":"/paper/2102.02020","citing_paper":"/paper/2502.04212"},"observation_digest":"sha256:419fdcd0a47b74c470a467eab7a31b6ffcaecd6e0d8f7b31bc05aeb4bf76a8f9","observation_id":"f97ff44d-177c-4d74-82db-9faa7da4d4a2","resolution":{"observed_at":"2026-08-08T23:12:26.300453Z","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":"2026-08-08T23:12:26.303970Z","title":"DESI results: Hint towards coupled dark matter and dark energy,","venue":null,"work_id":null,"year":2025},"citing_paper":{"arxiv_id":"2502.04212","last_updated":"2025-07-17T16:27:03Z","snapshot_observed_at":"2026-08-09T04:53:21.314754Z","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":100,"source":"pdf_text","source_observed_at":"2026-08-08T23:12:26.303970Z"},"links":{"citing_paper":"/paper/2502.04212"},"observation_digest":"sha256:d3004ae91036e2555e4f68ae236df4571b3af62f8a35729892a167f480afa2a2","observation_id":"ef86fef6-7cec-454b-ba27-47257d199c9c","resolution":{"observed_at":"2026-08-08T23:12:26.303970Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}}],"paper":{"arxiv_id":"2502.04212","last_updated":"2025-07-17T16:27:03Z","latest_version":5,"primary_category":"astro-ph.CO","snapshot_observed_at":"2026-08-09T04:53:21.314754Z","submitted_at":"2025-02-06T16:51:39Z","title":"The DESI DR1/DR2 evidence for dynamical dark energy is biased by low-redshift supernovae"},"reference_resolution":{"displayed":100,"state_counts":{"malformed_identifier":0,"metadata_mismatch":0,"parse_uncertain":0,"unresolved":98,"verified_exact":2,"verified_fuzzy":0},"total_outbound_references":101},"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":"2026-08-10T06:31:04.303077+00:00","source":"crossref"},{"observed_at":"2026-08-10T06:30:57.382061+00:00","source":"retraction_watch"}],"thesis":"As of 10 August 2026, this Paper Citation Record lists 100 of 101 outbound references and 35 inbound Pith citation observations for arXiv:2502.04212."}