{"as_of":"2026-08-06T07:11:00Z","caps":{"database_statements":6,"inbound":100,"outbound":100},"context_digest":"sha256:8edd3e06f4304fe0f7bd919358b6a12b0e50dee6cc6d049de2d38d13e94ac389","coverage":[{"denominator":0,"lane":"reference_resolution","note":"Typed states for the displayed outbound observations.","records_observed":0,"source":"paper_references, paper_reference_links","source_observed_at":null,"state":"measured"},{"denominator":30,"lane":"standing_notices","note":"One-hop event checks from named stored sources.","records_observed":30,"source":"scholarly_work_events, retraction_status_cache","source_observed_at":"2026-08-06T06:34:29.942622+00:00","state":"measured"},{"denominator":30,"lane":"inbound_itemization","note":"Pith citing papers itemized under the disclosed page cap.","records_observed":30,"source":"paper_references, paper_reference_links","source_observed_at":"2026-08-04T18:59:22.713386Z","state":"measured"},{"denominator":1,"lane":"external_citation_measurements","note":"A source-named dated measurement, never combined with another source.","records_observed":0,"source":"pith","source_observed_at":"2026-07-10T06:15:00.866473Z","state":"measured"}],"external_citation_measurements":[],"inbound":[{"citation":{"cited_paper":{"arxiv_id":"2405.13588","last_updated":"2024-05-30T08:22:06Z","snapshot_observed_at":"2026-08-02T10:45:27.974737Z","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":"2405.13588","doi":"10.48550/arxiv.2405.13588","metadata_source":"pith","pith_arxiv_id":"2405.13588","snapshot_observed_at":"2026-07-10T06:15:00.866473Z","title":"Lodha et al","venue":"astro-ph.CO","work_id":"17865e79-0745-4fb6-935d-c7022e823f6b","year":2024},"citing_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},"reference_index":226,"source":"pdf_text","source_observed_at":"2026-05-12T02:13:10.766505Z"},"links":{"cited_paper":"/paper/2405.13588","citing_paper":"/paper/2404.03002"},"observation_digest":"sha256:6bd8c60745e786358eaa70cd6fedce63622c46963ca15673ab02b9c3dad85078","observation_id":"8b230288-884e-46b0-9e9c-5fcec8dbce30","resolution":{"observed_at":"2026-05-12T02:13:10.963275Z","resolver_source":"arxiv_id","status":"verified_exact"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-06T06:34:29.942622+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-06T06:34:29.942622+00:00","source":"crossref"},{"observed_at":"2026-08-06T06:34:23.284952+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":{"arxiv_id":"2405.13588","last_updated":"2024-05-30T08:22:06Z","snapshot_observed_at":"2026-08-02T10:45:27.974737Z","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":"2405.13588","doi":"10.48550/arxiv.2405.13588","metadata_source":"pith","pith_arxiv_id":"2405.13588","snapshot_observed_at":"2026-07-10T06:15:00.866473Z","title":"Lodha et al","venue":"astro-ph.CO","work_id":"17865e79-0745-4fb6-935d-c7022e823f6b","year":2024},"citing_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},"reference_index":43,"source":"pdf_text","source_observed_at":"2026-05-18T16:14:18.379876Z"},"links":{"cited_paper":"/paper/2405.13588","citing_paper":"/paper/2409.13022"},"observation_digest":"sha256:fec134dc2896a647e3912b91c1e326f5bdb4f128dc78bf008f020d1a9751cd17","observation_id":"84bd8a1c-fc87-4ffc-ad02-2a4bfbf00db2","resolution":{"observed_at":"2026-05-18T16:14:18.542799Z","resolver_source":"arxiv_id","status":"metadata_mismatch"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-06T06:34:29.942622+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-06T06:34:29.942622+00:00","source":"crossref"},{"observed_at":"2026-08-06T06:34:23.284952+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":{"arxiv_id":"2405.13588","last_updated":"2024-05-30T08:22:06Z","snapshot_observed_at":"2026-08-02T10:45:27.974737Z","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":"2405.13588","doi":"10.48550/arxiv.2405.13588","metadata_source":"pith","pith_arxiv_id":"2405.13588","snapshot_observed_at":"2026-07-10T06:15:00.866473Z","title":"Lodha et al","venue":"astro-ph.CO","work_id":"17865e79-0745-4fb6-935d-c7022e823f6b","year":2024},"citing_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},"reference_index":164,"source":"pdf_text","source_observed_at":"2026-05-15T21:36:41.223414Z"},"links":{"cited_paper":"/paper/2405.13588","citing_paper":"/paper/2411.12022"},"observation_digest":"sha256:3b3d257c5862b779a4dd63907b04afc9ea1de9d2b91f78ac05e6ea0c621753a2","observation_id":"a43b0e79-9398-43fe-8d60-5bd871a4be08","resolution":{"observed_at":"2026-05-15T21:36:42.493806Z","resolver_source":"arxiv_id","status":"verified_exact"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-06T06:34:29.942622+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-06T06:34:29.942622+00:00","source":"crossref"},{"observed_at":"2026-08-06T06:34:23.284952+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":{"arxiv_id":"2405.13588","last_updated":"2024-05-30T08:22:06Z","snapshot_observed_at":"2026-08-02T10:45:27.974737Z","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":"2405.13588","doi":"10.48550/arxiv.2405.13588","metadata_source":"pith","pith_arxiv_id":"2405.13588","snapshot_observed_at":"2026-07-10T06:15:00.866473Z","title":"Lodha et al","venue":"astro-ph.CO","work_id":"17865e79-0745-4fb6-935d-c7022e823f6b","year":2024},"citing_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},"reference_index":152,"source":"pdf_text","source_observed_at":"2026-05-11T09:56:01.601036Z"},"links":{"cited_paper":"/paper/2405.13588","citing_paper":"/paper/2503.14738"},"observation_digest":"sha256:a2296f011358631a2b07c4780b5dabec9b692c62e35f45b6c786529709f93df7","observation_id":"b05ab066-544b-4873-809c-bb3b63a9c952","resolution":{"observed_at":"2026-05-11T09:56:03.590915Z","resolver_source":"arxiv_id","status":"verified_exact"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-06T06:34:29.942622+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-06T06:34:29.942622+00:00","source":"crossref"},{"observed_at":"2026-08-06T06:34:23.284952+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":{"arxiv_id":"2405.13588","last_updated":"2024-05-30T08:22:06Z","snapshot_observed_at":"2026-08-02T10:45:27.974737Z","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":"2405.13588","doi":"10.48550/arxiv.2405.13588","metadata_source":"pith","pith_arxiv_id":"2405.13588","snapshot_observed_at":"2026-07-10T06:15:00.866473Z","title":"Lodha et al","venue":"astro-ph.CO","work_id":"17865e79-0745-4fb6-935d-c7022e823f6b","year":2024},"citing_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},"reference_index":45,"source":"pdf_text","source_observed_at":"2026-05-14T21:04:02.994288Z"},"links":{"cited_paper":"/paper/2405.13588","citing_paper":"/paper/2503.14743"},"observation_digest":"sha256:2e8b58484205352b86c7e83370c0ef688332ad35f8d3af29f794b4a471e525b2","observation_id":"5e8536f2-785f-4709-bb14-d1190ddc414c","resolution":{"observed_at":"2026-05-14T21:04:03.526722Z","resolver_source":"arxiv_id","status":"verified_exact"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-06T06:34:29.942622+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-06T06:34:29.942622+00:00","source":"crossref"},{"observed_at":"2026-08-06T06:34:23.284952+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":{"arxiv_id":"2405.13588","last_updated":"2024-05-30T08:22:06Z","snapshot_observed_at":"2026-08-02T10:45:27.974737Z","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":"2405.13588","doi":"10.48550/arxiv.2405.13588","metadata_source":"pith","pith_arxiv_id":"2405.13588","snapshot_observed_at":"2026-07-10T06:15:00.866473Z","title":"Lodha et al","venue":"astro-ph.CO","work_id":"17865e79-0745-4fb6-935d-c7022e823f6b","year":2024},"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":15,"source":"pdf_text","source_observed_at":"2026-05-19T13:08:20.192767Z"},"links":{"cited_paper":"/paper/2405.13588","citing_paper":"/paper/2505.24732"},"observation_digest":"sha256:a5c44a710e96cfc4d5fc477d6a024c9d0cd9b401f02c44c8cb7f1048448187e7","observation_id":"c264a0a5-2166-4c0c-bcfe-3355da38436a","resolution":{"observed_at":"2026-05-19T13:12:18.975480Z","resolver_source":"arxiv_id","status":"metadata_mismatch"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-06T06:34:29.942622+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-06T06:34:29.942622+00:00","source":"crossref"},{"observed_at":"2026-08-06T06:34:23.284952+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":{"arxiv_id":"2405.13588","last_updated":"2024-05-30T08:22:06Z","snapshot_observed_at":"2026-08-02T10:45:27.974737Z","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":"2405.13588","doi":"10.48550/arxiv.2405.13588","metadata_source":"pith","pith_arxiv_id":"2405.13588","snapshot_observed_at":"2026-07-10T06:15:00.866473Z","title":"Lodha et al","venue":"astro-ph.CO","work_id":"17865e79-0745-4fb6-935d-c7022e823f6b","year":2024},"citing_paper":{"arxiv_id":"2507.02037","last_updated":"2026-05-05T11:02:42Z","snapshot_observed_at":"2026-07-06T02:11:23.670680Z","submitted_at":"2025-07-02T18:00:00Z","title":"An M-theory dS maximum from Casimir energies on Riemann-flat manifolds","version":3},"reference_index":60,"source":"pdf_text","source_observed_at":"2026-05-19T05:46:16.920455Z"},"links":{"cited_paper":"/paper/2405.13588","citing_paper":"/paper/2507.02037"},"observation_digest":"sha256:291385ecdb00ab473eef78429b2e9e392786ae5724bc5cace92b573cd08ea916","observation_id":"16b5deb0-b8fd-4eb9-a81f-d5e6f6905798","resolution":{"observed_at":"2026-05-19T05:47:07.591111Z","resolver_source":"arxiv_id","status":"metadata_mismatch"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-06T06:34:29.942622+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-06T06:34:29.942622+00:00","source":"crossref"},{"observed_at":"2026-08-06T06:34:23.284952+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":{"arxiv_id":"2405.13588","last_updated":"2024-05-30T08:22:06Z","snapshot_observed_at":"2026-08-02T10:45:27.974737Z","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":"2405.13588","doi":"10.48550/arxiv.2405.13588","metadata_source":"pith","pith_arxiv_id":"2405.13588","snapshot_observed_at":"2026-07-10T06:15:00.866473Z","title":"Lodha et al","venue":"astro-ph.CO","work_id":"17865e79-0745-4fb6-935d-c7022e823f6b","year":2024},"citing_paper":{"arxiv_id":"2509.02539","last_updated":"2026-04-17T18:00:05Z","snapshot_observed_at":"2026-07-06T22:22:26.392981Z","submitted_at":"2025-09-02T17:41:58Z","title":"Extending the Dynamical Systems Toolkit: Coupled Fields in Multiscalar Dark Energy","version":3},"reference_index":4,"source":"pdf_text","source_observed_at":"2026-05-18T19:39:43.620270Z"},"links":{"cited_paper":"/paper/2405.13588","citing_paper":"/paper/2509.02539"},"observation_digest":"sha256:0fce28264a70fbb23d3ac109e72293c269cb28323eff0d3e58495d2e2bd6098f","observation_id":"1d4cc017-1491-429e-9afd-b8a15eddfdfd","resolution":{"observed_at":"2026-05-18T19:41:48.579162Z","resolver_source":"arxiv_id","status":"metadata_mismatch"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-06T06:34:29.942622+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-06T06:34:29.942622+00:00","source":"crossref"},{"observed_at":"2026-08-06T06:34:23.284952+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":{"arxiv_id":"2405.13588","last_updated":"2024-05-30T08:22:06Z","snapshot_observed_at":"2026-08-02T10:45:27.974737Z","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":"2026-08-04T18:59:22.713386Z","title":"Lodha, A","venue":null,"work_id":null,"year":2024},"citing_paper":{"arxiv_id":"2509.09562","last_updated":"2025-09-11T15:52:46Z","snapshot_observed_at":"2026-08-05T15:28:40.413746Z","submitted_at":"2025-09-11T15:52:46Z","title":"The simple way to measure evolving dark energy without prior-volume effects","version":1},"reference_index":82,"source":"pdf_text","source_observed_at":"2026-08-04T18:59:22.713386Z"},"links":{"cited_paper":"/paper/2405.13588","citing_paper":"/paper/2509.09562"},"observation_digest":"sha256:114adff9a4f29fcf9e0c1df2e7ad41c27d4b9c118ae81f846079f443689db94e","observation_id":"b042687c-be67-42a9-b7be-767847d535a7","resolution":{"observed_at":"2026-08-04T18:59:22.713386Z","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":"2026-08-02T10:45:27.974737Z","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":"2405.13588","doi":"10.48550/arxiv.2405.13588","metadata_source":"pith","pith_arxiv_id":"2405.13588","snapshot_observed_at":"2026-07-10T06:15:00.866473Z","title":"Lodha et al","venue":"astro-ph.CO","work_id":"17865e79-0745-4fb6-935d-c7022e823f6b","year":2024},"citing_paper":{"arxiv_id":"2510.03779","last_updated":"2026-02-17T10:47:14Z","snapshot_observed_at":"2026-08-02T18:47:17.528052Z","submitted_at":"2025-10-04T11:08:41Z","title":"Beyond CPL: Evidence for dynamical dark energy in three-parameter models","version":3},"reference_index":14,"source":"pdf_text","source_observed_at":"2026-05-18T10:45:16.985887Z"},"links":{"cited_paper":"/paper/2405.13588","citing_paper":"/paper/2510.03779"},"observation_digest":"sha256:8812403f8b7fff6fdc64a90ba009d136df836593bddfdcd6ee222de9f6046ac8","observation_id":"6e4b39ff-0e51-4b53-bd76-08c8c6513846","resolution":{"observed_at":"2026-05-18T10:46:16.415161Z","resolver_source":"arxiv_id","status":"verified_exact"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-06T06:34:29.942622+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-06T06:34:29.942622+00:00","source":"crossref"},{"observed_at":"2026-08-06T06:34:23.284952+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":{"arxiv_id":"2405.13588","last_updated":"2024-05-30T08:22:06Z","snapshot_observed_at":"2026-08-02T10:45:27.974737Z","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":"2405.13588","doi":"10.48550/arxiv.2405.13588","metadata_source":"pith","pith_arxiv_id":"2405.13588","snapshot_observed_at":"2026-07-10T06:15:00.866473Z","title":"Lodha et al","venue":"astro-ph.CO","work_id":"17865e79-0745-4fb6-935d-c7022e823f6b","year":2024},"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":24,"source":"pdf_text","source_observed_at":"2026-05-17T22:17:32.138764Z"},"links":{"cited_paper":"/paper/2405.13588","citing_paper":"/paper/2511.09467"},"observation_digest":"sha256:176fb075cdfa54f5fa050c0e4444254d8b8455032b1ef5e3b751c9a0625da91d","observation_id":"6647a0eb-8c78-46eb-b6ab-2a7032f31c03","resolution":{"observed_at":"2026-05-17T22:20:23.442049Z","resolver_source":"arxiv_id","status":"verified_exact"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-06T06:34:29.942622+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-06T06:34:29.942622+00:00","source":"crossref"},{"observed_at":"2026-08-06T06:34:23.284952+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":{"arxiv_id":"2405.13588","last_updated":"2024-05-30T08:22:06Z","snapshot_observed_at":"2026-08-02T10:45:27.974737Z","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":"2026-08-03T14:40:55.350993Z","title":"Lodhaet al.(DESI), Phys","venue":null,"work_id":null,"year":2025},"citing_paper":{"arxiv_id":"2512.19888","last_updated":"2026-06-18T12:16:03Z","snapshot_observed_at":"2026-08-03T14:40:50.762025Z","submitted_at":"2025-12-22T21:27:32Z","title":"Observational constraints on early time non-phantom behaviour of dynamical dark energy","version":2},"reference_index":15,"source":"pdf_text","source_observed_at":"2026-08-03T14:40:55.350993Z"},"links":{"cited_paper":"/paper/2405.13588","citing_paper":"/paper/2512.19888"},"observation_digest":"sha256:220cfbe7a7f2ec7fe11422b90d2cbd10e88383ace722fb031e1cbce23db2ee1c","observation_id":"3e3a7d97-a329-47fd-8123-b00427ff0283","resolution":{"observed_at":"2026-08-03T14:40:55.350993Z","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":"2026-08-02T10:45:27.974737Z","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":"2026-08-03T11:11:48.667957Z","title":"Lodhaet al.(DESI), Phys","venue":null,"work_id":null,"year":2025},"citing_paper":{"arxiv_id":"2601.07361","last_updated":"2026-07-15T07:08:06Z","snapshot_observed_at":"2026-08-03T11:11:44.974779Z","submitted_at":"2026-01-12T09:36:30Z","title":"Robust Preference for Dark Sector Interactions","version":2},"reference_index":15,"source":"pdf_text","source_observed_at":"2026-08-03T11:11:48.667957Z"},"links":{"cited_paper":"/paper/2405.13588","citing_paper":"/paper/2601.07361"},"observation_digest":"sha256:44625574f81f14bc2525a53731ae4b05355c4400bca91b823505f89bad629053","observation_id":"3c1dd8b5-0ed1-4bfd-bc4c-3a829f52fc90","resolution":{"observed_at":"2026-08-03T11:11:48.667957Z","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":"2026-08-02T10:45:27.974737Z","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":"2026-07-15T14:51:12.413085Z","title":"Lodhaet al.(DESI), DESI 2024: Constraints on physics-focused aspects of dark energy using DESI DR1 BAO data, Phys","venue":null,"work_id":null,"year":2024},"citing_paper":{"arxiv_id":"2603.05049","last_updated":"2026-07-07T11:57:15Z","snapshot_observed_at":"2026-08-06T05:09:03.953635Z","submitted_at":"2026-03-05T10:59:03Z","title":"Sound Mode and Scale-Dependent Growth in Two-Fluid Dynamical Dark Energy","version":2},"reference_index":79,"source":"pdf_text","source_observed_at":"2026-07-15T14:51:12.413085Z"},"links":{"cited_paper":"/paper/2405.13588","citing_paper":"/paper/2603.05049"},"observation_digest":"sha256:d56df1bf549b8154a87ca93c6ebac941138dab76f6f99783c1cd154a8ddb9fb3","observation_id":"0fae7818-47da-4403-a6fa-1d71db72bfd6","resolution":{"observed_at":"2026-07-15T14:51:12.413085Z","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":"2026-08-02T10:45:27.974737Z","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":"2405.13588","doi":"10.48550/arxiv.2405.13588","metadata_source":"pith","pith_arxiv_id":"2405.13588","snapshot_observed_at":"2026-07-10T06:15:00.866473Z","title":"Lodha et al","venue":"astro-ph.CO","work_id":"17865e79-0745-4fb6-935d-c7022e823f6b","year":2024},"citing_paper":{"arxiv_id":"2603.21125","last_updated":"2026-03-22T08:46:57Z","snapshot_observed_at":"2026-07-06T22:50:01.539214Z","submitted_at":"2026-03-22T08:46:57Z","title":"Model-Independent Reconstruction of Quintessence Potential and Kinetic Energy from DESI DR2 and Pantheon+ Supernovae","version":1},"reference_index":17,"source":"pdf_text","source_observed_at":"2026-05-15T01:30:47.614992Z"},"links":{"cited_paper":"/paper/2405.13588","citing_paper":"/paper/2603.21125"},"observation_digest":"sha256:ae3f121d6939ba694c64f197857c1509ccddd4919930a0f0373f12b3d8c08430","observation_id":"9e7dc5c0-aab8-4816-92c4-c1722fbef756","resolution":{"observed_at":"2026-05-15T01:33:27.342561Z","resolver_source":"arxiv_id","status":"verified_exact"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-06T06:34:29.942622+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-06T06:34:29.942622+00:00","source":"crossref"},{"observed_at":"2026-08-06T06:34:23.284952+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":{"arxiv_id":"2405.13588","last_updated":"2024-05-30T08:22:06Z","snapshot_observed_at":"2026-08-02T10:45:27.974737Z","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":"2405.13588","doi":"10.48550/arxiv.2405.13588","metadata_source":"pith","pith_arxiv_id":"2405.13588","snapshot_observed_at":"2026-07-10T06:15:00.866473Z","title":"Lodha et al","venue":"astro-ph.CO","work_id":"17865e79-0745-4fb6-935d-c7022e823f6b","year":2024},"citing_paper":{"arxiv_id":"2605.10102","last_updated":"2026-05-11T07:18:09Z","snapshot_observed_at":"2026-07-06T02:11:23.670680Z","submitted_at":"2026-05-11T07:18:09Z","title":"From Large Telescopes to the MUltiplexed Survey Telescope (MUST)","version":1},"reference_index":147,"source":"arxiv_source","source_observed_at":"2026-05-12T03:45:17.616133Z"},"links":{"cited_paper":"/paper/2405.13588","citing_paper":"/paper/2605.10102"},"observation_digest":"sha256:2ed82ed98499151f7c05a2914658db9a402989c06005f8a7d99584ffe9392584","observation_id":"af2775e1-ad08-45bc-a1da-f6b98a6ec21e","resolution":{"observed_at":"2026-05-12T03:46:20.548478Z","resolver_source":"arxiv_id","status":"metadata_mismatch"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-06T06:34:29.942622+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-06T06:34:29.942622+00:00","source":"crossref"},{"observed_at":"2026-08-06T06:34:23.284952+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":{"arxiv_id":"2405.13588","last_updated":"2024-05-30T08:22:06Z","snapshot_observed_at":"2026-08-02T10:45:27.974737Z","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":"2405.13588","doi":"10.48550/arxiv.2405.13588","metadata_source":"pith","pith_arxiv_id":"2405.13588","snapshot_observed_at":"2026-07-10T06:15:00.866473Z","title":"Lodha et al","venue":"astro-ph.CO","work_id":"17865e79-0745-4fb6-935d-c7022e823f6b","year":2024},"citing_paper":{"arxiv_id":"2605.13546","last_updated":"2026-05-20T13:53:56Z","snapshot_observed_at":"2026-07-06T23:25:07.022065Z","submitted_at":"2026-05-13T13:54:57Z","title":"No evidence for phantom crossing: local goodness-of-fit improvements do not persist under global Bayesian model comparison","version":1},"reference_index":3,"source":"pdf_text","source_observed_at":"2026-05-14T19:09:24.620353Z"},"links":{"cited_paper":"/paper/2405.13588","citing_paper":"/paper/2605.13546"},"observation_digest":"sha256:baf58f4515c508283ef1fd74a52e6b660b1a4ff93b11b800c37ee75f5a62f2da","observation_id":"688e63f9-9d77-4a67-8037-dcfcaa6cd3c1","resolution":{"observed_at":"2026-05-14T19:12:51.364263Z","resolver_source":"arxiv_id","status":"verified_exact"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-06T06:34:29.942622+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-06T06:34:29.942622+00:00","source":"crossref"},{"observed_at":"2026-08-06T06:34:23.284952+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":{"arxiv_id":"2405.13588","last_updated":"2024-05-30T08:22:06Z","snapshot_observed_at":"2026-08-02T10:45:27.974737Z","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":"2405.13588","doi":"10.48550/arxiv.2405.13588","metadata_source":"pith","pith_arxiv_id":"2405.13588","snapshot_observed_at":"2026-07-10T06:15:00.866473Z","title":"Lodha et al","venue":"astro-ph.CO","work_id":"17865e79-0745-4fb6-935d-c7022e823f6b","year":2024},"citing_paper":{"arxiv_id":"2605.13546","last_updated":"2026-05-20T13:53:56Z","snapshot_observed_at":"2026-07-06T23:25:07.022065Z","submitted_at":"2026-05-13T13:54:57Z","title":"No evidence for phantom crossing: local goodness-of-fit improvements do not persist under global Bayesian model comparison","version":2},"reference_index":3,"source":"pdf_text","source_observed_at":"2026-05-21T08:18:49.500864Z"},"links":{"cited_paper":"/paper/2405.13588","citing_paper":"/paper/2605.13546"},"observation_digest":"sha256:6c9affdf1325e5a37732a1773129373d4689836f3ba584d1a870df6c188c8e35","observation_id":"f90efbc0-f57b-40eb-a2b4-c9fe41635760","resolution":{"observed_at":"2026-05-21T08:19:52.449553Z","resolver_source":"arxiv_id","status":"verified_exact"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-06T06:34:29.942622+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-06T06:34:29.942622+00:00","source":"crossref"},{"observed_at":"2026-08-06T06:34:23.284952+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":{"arxiv_id":"2405.13588","last_updated":"2024-05-30T08:22:06Z","snapshot_observed_at":"2026-08-02T10:45:27.974737Z","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":"2405.13588","doi":"10.48550/arxiv.2405.13588","metadata_source":"pith","pith_arxiv_id":"2405.13588","snapshot_observed_at":"2026-07-10T06:15:00.866473Z","title":"Lodha et al","venue":"astro-ph.CO","work_id":"17865e79-0745-4fb6-935d-c7022e823f6b","year":2024},"citing_paper":{"arxiv_id":"2605.21456","last_updated":"2026-05-20T17:46:56Z","snapshot_observed_at":"2026-07-06T23:31:56.199912Z","submitted_at":"2026-05-20T17:46:56Z","title":"Negative neutrino mass or negative dark energy?","version":1},"reference_index":122,"source":"pdf_text","source_observed_at":"2026-05-21T03:03:07.191130Z"},"links":{"cited_paper":"/paper/2405.13588","citing_paper":"/paper/2605.21456"},"observation_digest":"sha256:f4a2e5ce596ebc6167271aa8de8c98b5091e532ba7e6d57de1fae781c196e96e","observation_id":"d65cd57d-11db-42b6-b4a8-20a52fb54bb2","resolution":{"observed_at":"2026-05-21T03:03:55.656556Z","resolver_source":"arxiv_id","status":"metadata_mismatch"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-06T06:34:29.942622+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-06T06:34:29.942622+00:00","source":"crossref"},{"observed_at":"2026-08-06T06:34:23.284952+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":{"arxiv_id":"2405.13588","last_updated":"2024-05-30T08:22:06Z","snapshot_observed_at":"2026-08-02T10:45:27.974737Z","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":"2405.13588","doi":"10.48550/arxiv.2405.13588","metadata_source":"pith","pith_arxiv_id":"2405.13588","snapshot_observed_at":"2026-07-10T06:15:00.866473Z","title":"Lodha et al","venue":"astro-ph.CO","work_id":"17865e79-0745-4fb6-935d-c7022e823f6b","year":2024},"citing_paper":{"arxiv_id":"2606.01360","last_updated":"2026-07-18T02:00:49Z","snapshot_observed_at":"2026-08-02T12:39:56.892030Z","submitted_at":"2026-05-31T17:31:59Z","title":"A short review on Quintom dark energy theory","version":1},"reference_index":15,"source":"pdf_text","source_observed_at":"2026-06-28T16:17:39.285285Z"},"links":{"cited_paper":"/paper/2405.13588","citing_paper":"/paper/2606.01360"},"observation_digest":"sha256:b54b60ac78bacc7c8469282a45be5d2601a2dec10730b1f78281d87206bea082","observation_id":"701139c0-8d57-4eea-8095-e01c4f8195fd","resolution":{"observed_at":"2026-07-01T21:46:16.103482Z","resolver_source":"arxiv_id","status":"metadata_mismatch"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-06T06:34:29.942622+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-06T06:34:29.942622+00:00","source":"crossref"},{"observed_at":"2026-08-06T06:34:23.284952+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":{"arxiv_id":"2405.13588","last_updated":"2024-05-30T08:22:06Z","snapshot_observed_at":"2026-08-02T10:45:27.974737Z","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":"2026-08-02T12:40:00.359241Z","title":"Lodha, et al., DESI 2024: Constraints on physics-focused aspects of dark energy using DESI DR1 BAO data, Phys","venue":null,"work_id":null,"year":2024},"citing_paper":{"arxiv_id":"2606.01360","last_updated":"2026-07-18T02:00:49Z","snapshot_observed_at":"2026-08-02T12:39:56.892030Z","submitted_at":"2026-05-31T17:31:59Z","title":"A short review on Quintom dark energy theory","version":2},"reference_index":15,"source":"pdf_text","source_observed_at":"2026-08-02T12:40:00.359241Z"},"links":{"cited_paper":"/paper/2405.13588","citing_paper":"/paper/2606.01360"},"observation_digest":"sha256:281e0e96dfa28a8044a98f4567285270f7f00d47389422891ee0caa4e064517c","observation_id":"f14beb1f-947b-41f1-afc4-2558253b5c90","resolution":{"observed_at":"2026-08-02T12:40:00.359241Z","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":"2026-08-02T10:45:27.974737Z","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":"2405.13588","doi":"10.48550/arxiv.2405.13588","metadata_source":"pith","pith_arxiv_id":"2405.13588","snapshot_observed_at":"2026-07-10T06:15:00.866473Z","title":"Lodha et al","venue":"astro-ph.CO","work_id":"17865e79-0745-4fb6-935d-c7022e823f6b","year":2024},"citing_paper":{"arxiv_id":"2606.04830","last_updated":"2026-07-09T16:06:41Z","snapshot_observed_at":"2026-07-12T23:18:43.613366Z","submitted_at":"2026-06-03T12:53:52Z","title":"Cosmic variance or galaxy bias? Disentangling finite-volume and galaxy formation effects in cosmological analysis","version":1},"reference_index":9,"source":"pdf_text","source_observed_at":"2026-06-28T05:03:06.464090Z"},"links":{"cited_paper":"/paper/2405.13588","citing_paper":"/paper/2606.04830"},"observation_digest":"sha256:89b8d9d79a47e8853519724c5a4e303a48f90f02cac40c1250f83aa9ead9944a","observation_id":"0fd80be8-5b6b-40f5-ba9e-554308af2412","resolution":{"observed_at":"2026-07-02T10:26:52.074058Z","resolver_source":"arxiv_id","status":"verified_exact"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-06T06:34:29.942622+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-06T06:34:29.942622+00:00","source":"crossref"},{"observed_at":"2026-08-06T06:34:23.284952+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":{"arxiv_id":"2405.13588","last_updated":"2024-05-30T08:22:06Z","snapshot_observed_at":"2026-08-02T10:45:27.974737Z","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":"2026-07-12T15:09:49.195956Z","title":"Lodha, A","venue":null,"work_id":null,"year":2024},"citing_paper":{"arxiv_id":"2606.04830","last_updated":"2026-07-09T16:06:41Z","snapshot_observed_at":"2026-07-12T23:18:43.613366Z","submitted_at":"2026-06-03T12:53:52Z","title":"Cosmic variance or galaxy bias? Disentangling finite-volume and galaxy formation effects in cosmological analysis","version":2},"reference_index":9,"source":"pdf_text","source_observed_at":"2026-07-12T15:09:49.195956Z"},"links":{"cited_paper":"/paper/2405.13588","citing_paper":"/paper/2606.04830"},"observation_digest":"sha256:9e3d8932e572f803a5222e70eb2e3e79eb38e7a5f80a165bea6e75d3ab2d81b8","observation_id":"cf0194ba-e697-44ad-b6af-56683bcd6e91","resolution":{"observed_at":"2026-07-12T15:09:49.195956Z","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":"2026-08-02T10:45:27.974737Z","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":"2405.13588","doi":"10.48550/arxiv.2405.13588","metadata_source":"pith","pith_arxiv_id":"2405.13588","snapshot_observed_at":"2026-07-10T06:15:00.866473Z","title":"Lodha et al","venue":"astro-ph.CO","work_id":"17865e79-0745-4fb6-935d-c7022e823f6b","year":2024},"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":26,"source":"pdf_text","source_observed_at":"2026-06-28T04:52:33.342231Z"},"links":{"cited_paper":"/paper/2405.13588","citing_paper":"/paper/2606.05005"},"observation_digest":"sha256:e41c3e4889c15c09779cd6ec7f94e3d31cb14619e23d0fe5591ffdb9552b88d6","observation_id":"577af7fc-0625-414f-a5e2-7c1edc3661d4","resolution":{"observed_at":"2026-07-02T10:56:52.352603Z","resolver_source":"arxiv_id","status":"verified_exact"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-06T06:34:29.942622+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-06T06:34:29.942622+00:00","source":"crossref"},{"observed_at":"2026-08-06T06:34:23.284952+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":{"arxiv_id":"2405.13588","last_updated":"2024-05-30T08:22:06Z","snapshot_observed_at":"2026-08-02T10:45:27.974737Z","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":"2405.13588","doi":"10.48550/arxiv.2405.13588","metadata_source":"pith","pith_arxiv_id":"2405.13588","snapshot_observed_at":"2026-07-10T06:15:00.866473Z","title":"Lodha et al","venue":"astro-ph.CO","work_id":"17865e79-0745-4fb6-935d-c7022e823f6b","year":2024},"citing_paper":{"arxiv_id":"2606.26237","last_updated":"2026-06-24T18:00:03Z","snapshot_observed_at":"2026-07-07T00:00:36.766142Z","submitted_at":"2026-06-24T18:00:03Z","title":"First full-shape joint analysis of the two- and three-point correlation functions on real data: $\\Lambda$CDM cosmological constraints from BOSS DR12","version":1},"reference_index":168,"source":"arxiv_source","source_observed_at":"2026-06-26T01:35:05.451125Z"},"links":{"cited_paper":"/paper/2405.13588","citing_paper":"/paper/2606.26237"},"observation_digest":"sha256:79eb2eeba937e7a7df82891edbb868440440570656d69e24fcd1a259224d3203","observation_id":"375fdf7d-1ed9-4bc8-80da-94ebb4cffa98","resolution":{"observed_at":"2026-06-26T01:38:51.741879Z","resolver_source":"arxiv_id","status":"metadata_mismatch"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-06T06:34:29.942622+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-06T06:34:29.942622+00:00","source":"crossref"},{"observed_at":"2026-08-06T06:34:23.284952+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":{"arxiv_id":"2405.13588","last_updated":"2024-05-30T08:22:06Z","snapshot_observed_at":"2026-08-02T10:45:27.974737Z","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":"2405.13588","doi":"10.48550/arxiv.2405.13588","metadata_source":"pith","pith_arxiv_id":"2405.13588","snapshot_observed_at":"2026-07-10T06:15:00.866473Z","title":"Lodha et al","venue":"astro-ph.CO","work_id":"17865e79-0745-4fb6-935d-c7022e823f6b","year":2024},"citing_paper":{"arxiv_id":"2606.28488","last_updated":"2026-06-26T18:00:01Z","snapshot_observed_at":"2026-07-07T00:02:33.644076Z","submitted_at":"2026-06-26T18:00:01Z","title":"Dark energy from neutrino interactions in Unimodular Gravity","version":1},"reference_index":13,"source":"pdf_text","source_observed_at":"2026-06-30T01:30:46.593605Z"},"links":{"cited_paper":"/paper/2405.13588","citing_paper":"/paper/2606.28488"},"observation_digest":"sha256:6592514f5f72af88379f112d44fc10ff63cc42aa1d3503c07fb9d8cc98956efd","observation_id":"fe6934c3-9c45-4148-a648-1f64b68777f6","resolution":{"observed_at":"2026-07-01T15:25:48.259025Z","resolver_source":"arxiv_id","status":"verified_exact"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-06T06:34:29.942622+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-06T06:34:29.942622+00:00","source":"crossref"},{"observed_at":"2026-08-06T06:34:23.284952+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":{"arxiv_id":"2405.13588","last_updated":"2024-05-30T08:22:06Z","snapshot_observed_at":"2026-08-02T10:45:27.974737Z","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":"2405.13588","doi":"10.48550/arxiv.2405.13588","metadata_source":"pith","pith_arxiv_id":"2405.13588","snapshot_observed_at":"2026-07-10T06:15:00.866473Z","title":"Lodha et al","venue":"astro-ph.CO","work_id":"17865e79-0745-4fb6-935d-c7022e823f6b","year":2024},"citing_paper":{"arxiv_id":"2606.31324","last_updated":"2026-06-30T08:27:42Z","snapshot_observed_at":"2026-07-06T02:11:23.670680Z","submitted_at":"2026-06-30T08:27:42Z","title":"Cosmological Viability of Exponential Infrared $f(T)$ Gravity","version":1},"reference_index":69,"source":"pdf_text","source_observed_at":"2026-07-01T04:39:56.556632Z"},"links":{"cited_paper":"/paper/2405.13588","citing_paper":"/paper/2606.31324"},"observation_digest":"sha256:ae2f384d2da38094dd22e55d393bf3800af5db9fa0a0bd5136c9148e7f021bf4","observation_id":"3eb9481e-8d48-4495-b941-a3f3d1986242","resolution":{"observed_at":"2026-07-01T11:15:42.475901Z","resolver_source":"arxiv_id","status":"verified_exact"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-06T06:34:29.942622+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-06T06:34:29.942622+00:00","source":"crossref"},{"observed_at":"2026-08-06T06:34:23.284952+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":{"arxiv_id":"2405.13588","last_updated":"2024-05-30T08:22:06Z","snapshot_observed_at":"2026-08-02T10:45:27.974737Z","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":"2405.13588","doi":"10.48550/arxiv.2405.13588","metadata_source":"pith","pith_arxiv_id":"2405.13588","snapshot_observed_at":"2026-07-10T06:15:00.866473Z","title":"Lodha et al","venue":"astro-ph.CO","work_id":"17865e79-0745-4fb6-935d-c7022e823f6b","year":2024},"citing_paper":{"arxiv_id":"2607.07348","last_updated":"2026-07-08T12:38:37Z","snapshot_observed_at":"2026-07-30T01:35:48.257568Z","submitted_at":"2026-07-08T12:38:37Z","title":"Present Day Cosmic Acceleration from SDSS and DESI BAO: A Call for Finer Tomography of the DESI Bright Galaxy Survey","version":1},"reference_index":10,"source":"pdf_text","source_observed_at":"2026-07-09T13:44:49.684186Z"},"links":{"cited_paper":"/paper/2405.13588","citing_paper":"/paper/2607.07348"},"observation_digest":"sha256:08dd9bc24460359511a62e675b9e274c9771bb8808bca0933bb5268e1fd8a706","observation_id":"454c60b9-d8f5-4c23-ab97-611324fdd7a4","resolution":{"observed_at":"2026-07-09T13:46:17.572898Z","resolver_source":"local_arxiv","status":"verified_exact"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-06T06:34:29.942622+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-06T06:34:29.942622+00:00","source":"crossref"},{"observed_at":"2026-08-06T06:34:23.284952+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":{"arxiv_id":"2405.13588","last_updated":"2024-05-30T08:22:06Z","snapshot_observed_at":"2026-08-02T10:45:27.974737Z","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":"2026-08-01T01:25:44.066013Z","title":"Lodha et al","venue":null,"work_id":null,"year":2025},"citing_paper":{"arxiv_id":"2607.25841","last_updated":"2026-07-28T15:18:43Z","snapshot_observed_at":"2026-08-05T16:17:43.357001Z","submitted_at":"2026-07-28T15:18:43Z","title":"General Relativistic Entropic Acceleration at the perturbation level: a CLASS implementation and first Boltzmann-code constraints","version":1},"reference_index":61,"source":"pdf_text","source_observed_at":"2026-08-01T01:25:44.066013Z"},"links":{"cited_paper":"/paper/2405.13588","citing_paper":"/paper/2607.25841"},"observation_digest":"sha256:68f6671f1186d0365bbf63c488a0712519144185929f0f3a452f36c3ab030cec","observation_id":"30c3560f-e1b4-413f-8a2a-e8e51772b3d2","resolution":{"observed_at":"2026-08-01T01:25:44.066013Z","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":"2026-08-02T10:45:27.974737Z","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":"2026-08-03T04:36:13.596130Z","title":", keywords =","venue":null,"work_id":null,"year":2024},"citing_paper":{"arxiv_id":"2607.29562","last_updated":"2026-07-31T15:52:41Z","snapshot_observed_at":"2026-08-05T23:15:54.698890Z","submitted_at":"2026-07-31T15:52:41Z","title":"Late Time Dynamical Dark Energy and the CMB-Distance Ladder Tension","version":1},"reference_index":11,"source":"arxiv_source","source_observed_at":"2026-08-03T04:36:13.596130Z"},"links":{"cited_paper":"/paper/2405.13588","citing_paper":"/paper/2607.29562"},"observation_digest":"sha256:95ce8b94380d59bf8a74129ed0276913a24063790598d309773ac782d02261e2","observation_id":"bfa4a8b1-6273-45ab-bd63-bfabaf57a825","resolution":{"observed_at":"2026-08-03T04:36:13.596130Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}}],"links":{"evidence":"/evidence","html":"/paper/2405.13588/citation-record","integrity":"/paper/2405.13588/integrity","json":"/paper/2405.13588/citation-record.json","paper":"/paper/2405.13588"},"outbound":[],"paper":{"arxiv_id":"2405.13588","last_updated":"2024-05-30T08:22:06Z","latest_version":2,"primary_category":"astro-ph.CO","snapshot_observed_at":"2026-08-02T10:45:27.974737Z","submitted_at":"2024-05-22T12:35:37Z","title":"DESI 2024: Constraints on Physics-Focused Aspects of Dark Energy using DESI DR1 BAO Data"},"reference_resolution":{"displayed":0,"state_counts":{"malformed_identifier":0,"metadata_mismatch":0,"parse_uncertain":0,"unresolved":0,"verified_exact":0,"verified_fuzzy":0},"total_outbound_references":0},"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":"2026-08-06T06:34:29.942622+00:00","source":"crossref"},{"observed_at":"2026-08-06T06:34:23.284952+00:00","source":"retraction_watch"}],"thesis":"As of 6 August 2026, this Paper Citation Record lists 0 of 0 outbound references and 30 inbound Pith citation observations for arXiv:2405.13588."}