{"as_of":"2026-08-09T09:48:00Z","caps":{"database_statements":6,"inbound":100,"outbound":100},"context_digest":"sha256:9e056eac333e40f905fb2f9df532a61ae768f8f4f977e2fa52a9f353e52854a8","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":23,"lane":"standing_notices","note":"One-hop event checks from named stored sources.","records_observed":23,"source":"scholarly_work_events, retraction_status_cache","source_observed_at":"2026-08-09T06:31:02.800959+00:00","state":"measured"},{"denominator":23,"lane":"inbound_itemization","note":"Pith citing papers itemized under the disclosed page cap.","records_observed":23,"source":"paper_references, paper_reference_links","source_observed_at":"2026-08-07T14:27:09.863743Z","state":"measured"},{"denominator":1,"lane":"external_citation_measurements","note":"A source-named dated measurement, never combined with another source.","records_observed":1,"source":"arxiv_reference","source_observed_at":"2026-08-05T02:28:24.338817Z","state":"measured"}],"external_citation_measurements":[{"count":0,"observed_at":"2026-08-05T02:28:24.338817Z","source":"arxiv_reference"}],"inbound":[{"citation":{"cited_paper":{"arxiv_id":"2503.17342","last_updated":"2025-07-31T19:49:36Z","snapshot_observed_at":"2026-08-07T16:45:52.592701Z","submitted_at":"2025-03-21T17:45:04Z","title":"Comparison of dynamical dark energy with {\\Lambda}CDM in light of DESI DR2","version":3},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2503.17342","snapshot_observed_at":"2026-08-07T14:27:09.863743Z","title":"Comparison of dynamical dark energy with ΛCDM in light of DESI DR2,","venue":null,"work_id":null,"year":2025},"citing_paper":{"arxiv_id":"2505.18900","last_updated":"2025-05-27T18:05:09Z","snapshot_observed_at":"2026-08-07T16:20:24.033303Z","submitted_at":"2025-05-24T23:16:41Z","title":"Dynamical Dark Energy at Late Time $\\Lambda$CDM","version":2},"reference_index":5,"source":"pdf_text","source_observed_at":"2026-08-07T14:27:09.863743Z"},"links":{"cited_paper":"/paper/2503.17342","citing_paper":"/paper/2505.18900"},"observation_digest":"sha256:2715be41324e5da98867379d3ac9a1334ec159ce73abb14b52479ecd7ca592aa","observation_id":"1e2779be-2b9c-4337-bea1-61a26cc58735","resolution":{"observed_at":"2026-08-07T14:27:09.863743Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2503.17342","last_updated":"2025-07-31T19:49:36Z","snapshot_observed_at":"2026-08-07T16:45:52.592701Z","submitted_at":"2025-03-21T17:45:04Z","title":"Comparison of dynamical dark energy with {\\Lambda}CDM in light of DESI DR2","version":3},"cited_work":{"arxiv_id":"2503.17342","doi":"10.48550/arxiv.2503.17342","metadata_source":"arxiv_reference","pith_arxiv_id":"2503.17342","snapshot_observed_at":"2026-08-05T02:28:24.338817Z","title":"N., Handley W","venue":"ArXiv.org","work_id":"2ff50020-e4d6-4952-9337-705b42da7b2d","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":32,"source":"pdf_text","source_observed_at":"2026-05-19T13:08:20.192767Z"},"links":{"cited_paper":"/paper/2503.17342","citing_paper":"/paper/2505.24732"},"observation_digest":"sha256:39b4958475f8283813fc5100d96cb7de17555d262c4e47427fd726de3f86f603","observation_id":"fb84cbd0-3c73-4b01-9e31-c013e1bd40dc","resolution":{"observed_at":"2026-05-19T13:12:19.132886Z","resolver_source":"arxiv_id","status":"verified_exact"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-09T06:31:02.800959+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-09T06:31:02.800959+00:00","source":"crossref"},{"observed_at":"2026-08-09T06:30:57.326959+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":{"arxiv_id":"2503.17342","last_updated":"2025-07-31T19:49:36Z","snapshot_observed_at":"2026-08-07T16:45:52.592701Z","submitted_at":"2025-03-21T17:45:04Z","title":"Comparison of dynamical dark energy with {\\Lambda}CDM in light of DESI DR2","version":3},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2503.17342","snapshot_observed_at":"2026-08-07T11:24:21.941307Z","title":null,"venue":null,"work_id":null,"year":2025},"citing_paper":{"arxiv_id":"2506.03019","last_updated":"2025-06-03T15:56:26Z","snapshot_observed_at":"2026-08-09T03:21:02.776928Z","submitted_at":"2025-06-03T15:56:26Z","title":"Constraints on Barrow and Tsallis Holographic Dark Energy from DESI DR2 BAO data","version":1},"reference_index":58,"source":"pdf_text","source_observed_at":"2026-08-07T11:24:21.941307Z"},"links":{"cited_paper":"/paper/2503.17342","citing_paper":"/paper/2506.03019"},"observation_digest":"sha256:369cff388e804c08eafe4f5647baf08a5da9c809bbe20e586808b7247d4cf013","observation_id":"fb0c0512-5413-41f3-954c-28a61f6ba3b4","resolution":{"observed_at":"2026-08-07T11:24:21.941307Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2503.17342","last_updated":"2025-07-31T19:49:36Z","snapshot_observed_at":"2026-08-07T16:45:52.592701Z","submitted_at":"2025-03-21T17:45:04Z","title":"Comparison of dynamical dark energy with {\\Lambda}CDM in light of DESI DR2","version":3},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2503.17342","snapshot_observed_at":"2026-08-07T04:41:33.551299Z","title":"Comparison of dynamical dark energy with ΛCDM in light of DESI DR2,","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":8,"source":"pdf_text","source_observed_at":"2026-08-07T04:41:33.551299Z"},"links":{"cited_paper":"/paper/2503.17342","citing_paper":"/paper/2506.10075"},"observation_digest":"sha256:5266123d799c6025a62100e1d2b851847176f76c63a09a0292a88e753f183637","observation_id":"a384f8b5-d218-427b-828c-fcf9295ccccf","resolution":{"observed_at":"2026-08-07T04:41:33.551299Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2503.17342","last_updated":"2025-07-31T19:49:36Z","snapshot_observed_at":"2026-08-07T16:45:52.592701Z","submitted_at":"2025-03-21T17:45:04Z","title":"Comparison of dynamical dark energy with {\\Lambda}CDM in light of DESI DR2","version":3},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2503.17342","snapshot_observed_at":"2026-08-06T23:52:23.753649Z","title":null,"venue":null,"work_id":null,"year":2025},"citing_paper":{"arxiv_id":"2506.16223","last_updated":"2025-06-19T11:28:24Z","snapshot_observed_at":"2026-08-09T03:21:14.676120Z","submitted_at":"2025-06-19T11:28:24Z","title":"Observational Constraints on Scalar Field--Matter Interaction in Weyl Integrable Spacetime","version":1},"reference_index":75,"source":"pdf_text","source_observed_at":"2026-08-06T23:52:23.753649Z"},"links":{"cited_paper":"/paper/2503.17342","citing_paper":"/paper/2506.16223"},"observation_digest":"sha256:a96227b2782ab875551854a50dd7a5d97de6cfd5ff42f6d6b801c9af5c71047a","observation_id":"0d3f9f30-cedf-4744-84bc-c868fdb7df0e","resolution":{"observed_at":"2026-08-06T23:52:23.753649Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2503.17342","last_updated":"2025-07-31T19:49:36Z","snapshot_observed_at":"2026-08-07T16:45:52.592701Z","submitted_at":"2025-03-21T17:45:04Z","title":"Comparison of dynamical dark energy with {\\Lambda}CDM in light of DESI DR2","version":3},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2503.17342","snapshot_observed_at":"2026-08-06T19:22:35.931673Z","title":null,"venue":null,"work_id":null,"year":2025},"citing_paper":{"arxiv_id":"2507.05975","last_updated":"2025-07-08T13:29:42Z","snapshot_observed_at":"2026-08-07T23:01:05.582113Z","submitted_at":"2025-07-08T13:29:42Z","title":"Constraint on Symmetric Teleparallel Gravity with Different Dark energy Parametrizations from DESI DR2 BAO Data","version":1},"reference_index":35,"source":"pdf_text","source_observed_at":"2026-08-06T19:22:35.931673Z"},"links":{"cited_paper":"/paper/2503.17342","citing_paper":"/paper/2507.05975"},"observation_digest":"sha256:0bf6b89e6a2bff2f8c80c3b9f85353dcd51f1be487a55c99fc4674c47c08d4c3","observation_id":"424bebc7-80be-49f5-9824-446abaec7696","resolution":{"observed_at":"2026-08-06T19:22:35.931673Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2503.17342","last_updated":"2025-07-31T19:49:36Z","snapshot_observed_at":"2026-08-07T16:45:52.592701Z","submitted_at":"2025-03-21T17:45:04Z","title":"Comparison of dynamical dark energy with {\\Lambda}CDM in light of DESI DR2","version":3},"cited_work":{"arxiv_id":"2503.17342","doi":"10.48550/arxiv.2503.17342","metadata_source":"arxiv_reference","pith_arxiv_id":"2503.17342","snapshot_observed_at":"2026-08-05T02:28:24.338817Z","title":"N., Handley W","venue":"ArXiv.org","work_id":"2ff50020-e4d6-4952-9337-705b42da7b2d","year":2025},"citing_paper":{"arxiv_id":"2509.13220","last_updated":"2026-07-29T15:33:01Z","snapshot_observed_at":"2026-08-05T20:45:32.210951Z","submitted_at":"2025-09-16T16:27:46Z","title":"Dynamic or Systematic? Bayesian model selection between dark energy and supernova biases","version":2},"reference_index":46,"source":"arxiv_source","source_observed_at":"2026-05-18T16:07:03.405932Z"},"links":{"cited_paper":"/paper/2503.17342","citing_paper":"/paper/2509.13220"},"observation_digest":"sha256:7d12d57d2e391a96e4a407fa1d3d421209eaf271cb0012d973687e17d7a7c7c6","observation_id":"b1d2aac1-91a6-47ae-98c0-fece7f958790","resolution":{"observed_at":"2026-05-18T16:11:35.341448Z","resolver_source":"arxiv_id","status":"verified_exact"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-09T06:31:02.800959+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-09T06:31:02.800959+00:00","source":"crossref"},{"observed_at":"2026-08-09T06:30:57.326959+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":{"arxiv_id":"2503.17342","last_updated":"2025-07-31T19:49:36Z","snapshot_observed_at":"2026-08-07T16:45:52.592701Z","submitted_at":"2025-03-21T17:45:04Z","title":"Comparison of dynamical dark energy with {\\Lambda}CDM in light of DESI DR2","version":3},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2503.17342","snapshot_observed_at":"2026-08-04T16:32:48.927519Z","title":"N., Handley W","venue":null,"work_id":null,"year":null},"citing_paper":{"arxiv_id":"2509.13220","last_updated":"2026-07-29T15:33:01Z","snapshot_observed_at":"2026-08-05T20:45:32.210951Z","submitted_at":"2025-09-16T16:27:46Z","title":"Dynamic or Systematic? Bayesian model selection between dark energy and supernova biases","version":3},"reference_index":46,"source":"arxiv_source","source_observed_at":"2026-08-04T16:32:48.927519Z"},"links":{"cited_paper":"/paper/2503.17342","citing_paper":"/paper/2509.13220"},"observation_digest":"sha256:ccc05d48203b404456ecc25331b980cd8b3bbc74b34370cbb6adf2d5fb61656e","observation_id":"aa9d8605-fb0b-4ab2-9fe2-3208b8ba323d","resolution":{"observed_at":"2026-08-04T16:32:48.927519Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2503.17342","last_updated":"2025-07-31T19:49:36Z","snapshot_observed_at":"2026-08-07T16:45:52.592701Z","submitted_at":"2025-03-21T17:45:04Z","title":"Comparison of dynamical dark energy with {\\Lambda}CDM in light of DESI DR2","version":3},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2503.17342","snapshot_observed_at":"2026-08-04T09:19:38.388759Z","title":null,"venue":null,"work_id":null,"year":2025},"citing_paper":{"arxiv_id":"2510.16228","last_updated":"2025-10-17T21:36:56Z","snapshot_observed_at":"2026-08-08T22:55:33.999165Z","submitted_at":"2025-10-17T21:36:56Z","title":"Observational constraints on the modified cosmology inspired by string T-duality","version":1},"reference_index":45,"source":"pdf_text","source_observed_at":"2026-08-04T09:19:38.388759Z"},"links":{"cited_paper":"/paper/2503.17342","citing_paper":"/paper/2510.16228"},"observation_digest":"sha256:53af5427b499f6e04194ed6c999e787a12ab8fda454f80843a075f5ca82ac7ba","observation_id":"1910fa79-b15a-4dc9-a6d3-4e1ca63b8939","resolution":{"observed_at":"2026-08-04T09:19:38.388759Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2503.17342","last_updated":"2025-07-31T19:49:36Z","snapshot_observed_at":"2026-08-07T16:45:52.592701Z","submitted_at":"2025-03-21T17:45:04Z","title":"Comparison of dynamical dark energy with {\\Lambda}CDM in light of DESI DR2","version":3},"cited_work":{"arxiv_id":"2503.17342","doi":"10.48550/arxiv.2503.17342","metadata_source":"arxiv_reference","pith_arxiv_id":"2503.17342","snapshot_observed_at":"2026-08-05T02:28:24.338817Z","title":"N., Handley W","venue":"ArXiv.org","work_id":"2ff50020-e4d6-4952-9337-705b42da7b2d","year":2025},"citing_paper":{"arxiv_id":"2510.18741","last_updated":"2026-04-10T13:03:33Z","snapshot_observed_at":"2026-07-06T02:11:23.670680Z","submitted_at":"2025-10-21T15:46:25Z","title":"Nonlinear Matter Power Spectrum from relativistic $N$-body Simulations: $\\Lambda_{\\rm s}$CDM versus $\\Lambda$CDM","version":2},"reference_index":113,"source":"pdf_text","source_observed_at":"2026-05-18T04:46:14.832965Z"},"links":{"cited_paper":"/paper/2503.17342","citing_paper":"/paper/2510.18741"},"observation_digest":"sha256:fc0ef59e5bcf8d19b162bc59b1ba65e6cae86387dc0b3c8796b345ef4e8cb8a6","observation_id":"73b48932-d0bf-4899-89a1-0c92c7e03549","resolution":{"observed_at":"2026-05-18T04:50:55.540273Z","resolver_source":"arxiv_id","status":"verified_exact"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-09T06:31:02.800959+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-09T06:31:02.800959+00:00","source":"crossref"},{"observed_at":"2026-08-09T06:30:57.326959+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":{"arxiv_id":"2503.17342","last_updated":"2025-07-31T19:49:36Z","snapshot_observed_at":"2026-08-07T16:45:52.592701Z","submitted_at":"2025-03-21T17:45:04Z","title":"Comparison of dynamical dark energy with {\\Lambda}CDM in light of DESI DR2","version":3},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2503.17342","snapshot_observed_at":"2026-08-03T11:11:48.733078Z","title":null,"venue":null,"work_id":null,"year":2025},"citing_paper":{"arxiv_id":"2601.07361","last_updated":"2026-07-15T07:08:06Z","snapshot_observed_at":"2026-08-07T00:15:37.338897Z","submitted_at":"2026-01-12T09:36:30Z","title":"Robust Preference for Dark Sector Interactions","version":2},"reference_index":41,"source":"pdf_text","source_observed_at":"2026-08-03T11:11:48.733078Z"},"links":{"cited_paper":"/paper/2503.17342","citing_paper":"/paper/2601.07361"},"observation_digest":"sha256:6cc40f30eef5af6a45c9dc407aba9f0fa004bbc01d024f580810990a87a99300","observation_id":"6f161763-1a13-4f69-97f5-97643df7bc66","resolution":{"observed_at":"2026-08-03T11:11:48.733078Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2503.17342","last_updated":"2025-07-31T19:49:36Z","snapshot_observed_at":"2026-08-07T16:45:52.592701Z","submitted_at":"2025-03-21T17:45:04Z","title":"Comparison of dynamical dark energy with {\\Lambda}CDM in light of DESI DR2","version":3},"cited_work":{"arxiv_id":"2503.17342","doi":"10.48550/arxiv.2503.17342","metadata_source":"arxiv_reference","pith_arxiv_id":"2503.17342","snapshot_observed_at":"2026-08-05T02:28:24.338817Z","title":"N., Handley W","venue":"ArXiv.org","work_id":"2ff50020-e4d6-4952-9337-705b42da7b2d","year":2025},"citing_paper":{"arxiv_id":"2602.11936","last_updated":"2026-05-18T12:54:32Z","snapshot_observed_at":"2026-08-02T13:51:44.487752Z","submitted_at":"2026-02-12T13:35:54Z","title":"Probing Dynamical Dark Energy with Late-Time Data: Evidence, Tensions, and the Limits of the $w_0w_a$CDM Framework","version":3},"reference_index":182,"source":"pdf_text","source_observed_at":"2026-05-21T13:29:05.147292Z"},"links":{"cited_paper":"/paper/2503.17342","citing_paper":"/paper/2602.11936"},"observation_digest":"sha256:64d2e9eb62d8dd54d9ad00113a82af8cfb257c660fdc141ddb2354bb5f9faf8b","observation_id":"d4ac999d-ca9f-4fe0-9778-4ab5ba319858","resolution":{"observed_at":"2026-05-21T13:30:12.082325Z","resolver_source":"arxiv_id","status":"verified_exact"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-09T06:31:02.800959+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-09T06:31:02.800959+00:00","source":"crossref"},{"observed_at":"2026-08-09T06:30:57.326959+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":{"arxiv_id":"2503.17342","last_updated":"2025-07-31T19:49:36Z","snapshot_observed_at":"2026-08-07T16:45:52.592701Z","submitted_at":"2025-03-21T17:45:04Z","title":"Comparison of dynamical dark energy with {\\Lambda}CDM in light of DESI DR2","version":3},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2503.17342","snapshot_observed_at":"2026-07-15T12:01:04.317365Z","title":null,"venue":null,"work_id":null,"year":2025},"citing_paper":{"arxiv_id":"2603.14693","last_updated":"2026-07-14T04:50:03Z","snapshot_observed_at":"2026-08-06T08:35:01.524662Z","submitted_at":"2026-03-16T01:02:08Z","title":"Background-level reconstruction of scalar-field potentials from dark-energy histories and comparison with analytic potential families","version":2},"reference_index":207,"source":"pdf_text","source_observed_at":"2026-07-15T12:01:04.317365Z"},"links":{"cited_paper":"/paper/2503.17342","citing_paper":"/paper/2603.14693"},"observation_digest":"sha256:743790b3cbd81c1dcd3868730a438c7c6b6c66d506cff0af2f0b5d3fcdf30d56","observation_id":"9b17a453-0a6c-414b-b782-5eeff7e3a8d7","resolution":{"observed_at":"2026-07-15T12:01:04.317365Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2503.17342","last_updated":"2025-07-31T19:49:36Z","snapshot_observed_at":"2026-08-07T16:45:52.592701Z","submitted_at":"2025-03-21T17:45:04Z","title":"Comparison of dynamical dark energy with {\\Lambda}CDM in light of DESI DR2","version":3},"cited_work":{"arxiv_id":"2503.17342","doi":"10.48550/arxiv.2503.17342","metadata_source":"arxiv_reference","pith_arxiv_id":"2503.17342","snapshot_observed_at":"2026-08-05T02:28:24.338817Z","title":"N., Handley W","venue":"ArXiv.org","work_id":"2ff50020-e4d6-4952-9337-705b42da7b2d","year":2025},"citing_paper":{"arxiv_id":"2604.02433","last_updated":"2026-04-02T18:03:36Z","snapshot_observed_at":"2026-07-06T02:11:23.670680Z","submitted_at":"2026-04-02T18:03:36Z","title":"Cosmology-Independent Constraints on the Etherington Relation and SNeIa Absolute Magnitude Evolution from DESI-DR2","version":1},"reference_index":53,"source":"pdf_text","source_observed_at":"2026-05-13T20:20:26.803979Z"},"links":{"cited_paper":"/paper/2503.17342","citing_paper":"/paper/2604.02433"},"observation_digest":"sha256:e4d209c0a3df9dedb6aa8b8b410a80dcb44f1ce8e0a338dafa68a845b1271022","observation_id":"e7f4772e-e8ce-4660-9999-977f0041b610","resolution":{"observed_at":"2026-05-13T20:23:13.690322Z","resolver_source":"arxiv_id","status":"verified_exact"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-09T06:31:02.800959+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-09T06:31:02.800959+00:00","source":"crossref"},{"observed_at":"2026-08-09T06:30:57.326959+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":{"arxiv_id":"2503.17342","last_updated":"2025-07-31T19:49:36Z","snapshot_observed_at":"2026-08-07T16:45:52.592701Z","submitted_at":"2025-03-21T17:45:04Z","title":"Comparison of dynamical dark energy with {\\Lambda}CDM in light of DESI DR2","version":3},"cited_work":{"arxiv_id":"2503.17342","doi":"10.48550/arxiv.2503.17342","metadata_source":"arxiv_reference","pith_arxiv_id":"2503.17342","snapshot_observed_at":"2026-08-05T02:28:24.338817Z","title":"N., Handley W","venue":"ArXiv.org","work_id":"2ff50020-e4d6-4952-9337-705b42da7b2d","year":2025},"citing_paper":{"arxiv_id":"2604.22450","last_updated":"2026-04-24T11:08:31Z","snapshot_observed_at":"2026-08-02T12:41:46.299268Z","submitted_at":"2026-04-24T11:08:31Z","title":"Exploring Cosmic Evolution in R\\'enyi Entropic Cosmology with Constraints from DESI DR2 BAO and GW Data","version":1},"reference_index":45,"source":"pdf_text","source_observed_at":"2026-05-08T10:32:58.967506Z"},"links":{"cited_paper":"/paper/2503.17342","citing_paper":"/paper/2604.22450"},"observation_digest":"sha256:9babf7cbf067a6df25121a521005936a38895fcd49882989e94a382404b90b5b","observation_id":"499b337f-2d56-4b4b-8749-e20050e83bf2","resolution":{"observed_at":"2026-05-11T20:01:09.811572Z","resolver_source":"arxiv_id","status":"verified_exact"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-09T06:31:02.800959+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-09T06:31:02.800959+00:00","source":"crossref"},{"observed_at":"2026-08-09T06:30:57.326959+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":{"arxiv_id":"2503.17342","last_updated":"2025-07-31T19:49:36Z","snapshot_observed_at":"2026-08-07T16:45:52.592701Z","submitted_at":"2025-03-21T17:45:04Z","title":"Comparison of dynamical dark energy with {\\Lambda}CDM in light of DESI DR2","version":3},"cited_work":{"arxiv_id":"2503.17342","doi":"10.48550/arxiv.2503.17342","metadata_source":"arxiv_reference","pith_arxiv_id":"2503.17342","snapshot_observed_at":"2026-08-05T02:28:24.338817Z","title":"N., Handley W","venue":"ArXiv.org","work_id":"2ff50020-e4d6-4952-9337-705b42da7b2d","year":2025},"citing_paper":{"arxiv_id":"2604.23793","last_updated":"2026-04-26T16:35:30Z","snapshot_observed_at":"2026-07-06T23:09:58.193241Z","submitted_at":"2026-04-26T16:35:30Z","title":"From Big Bang Nucleosynthesis to Late-Time Acceleration in $f(Q,L_m)$ Gravity","version":1},"reference_index":63,"source":"pdf_text","source_observed_at":"2026-05-08T05:42:53.721029Z"},"links":{"cited_paper":"/paper/2503.17342","citing_paper":"/paper/2604.23793"},"observation_digest":"sha256:6dbae308d4d455effeb3dc584172186033e776d68d81e93338493480dc51d688","observation_id":"e9518f62-43c1-4eac-8970-aa3b11e8a23c","resolution":{"observed_at":"2026-05-11T21:26:12.900156Z","resolver_source":"arxiv_id","status":"verified_exact"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-09T06:31:02.800959+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-09T06:31:02.800959+00:00","source":"crossref"},{"observed_at":"2026-08-09T06:30:57.326959+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":{"arxiv_id":"2503.17342","last_updated":"2025-07-31T19:49:36Z","snapshot_observed_at":"2026-08-07T16:45:52.592701Z","submitted_at":"2025-03-21T17:45:04Z","title":"Comparison of dynamical dark energy with {\\Lambda}CDM in light of DESI DR2","version":3},"cited_work":{"arxiv_id":"2503.17342","doi":"10.48550/arxiv.2503.17342","metadata_source":"arxiv_reference","pith_arxiv_id":"2503.17342","snapshot_observed_at":"2026-08-05T02:28:24.338817Z","title":"N., Handley W","venue":"ArXiv.org","work_id":"2ff50020-e4d6-4952-9337-705b42da7b2d","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":46,"source":"pdf_text","source_observed_at":"2026-06-28T04:52:33.342231Z"},"links":{"cited_paper":"/paper/2503.17342","citing_paper":"/paper/2606.05005"},"observation_digest":"sha256:318ea7cf18ed7df7f2de9a9ab1cffaaa0d5c82939a94b7097a4a008b6d056166","observation_id":"f6e7bd65-05cf-4c47-8278-6394b402785b","resolution":{"observed_at":"2026-07-02T10:56:52.458456Z","resolver_source":"arxiv_id","status":"verified_exact"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-09T06:31:02.800959+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-09T06:31:02.800959+00:00","source":"crossref"},{"observed_at":"2026-08-09T06:30:57.326959+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":{"arxiv_id":"2503.17342","last_updated":"2025-07-31T19:49:36Z","snapshot_observed_at":"2026-08-07T16:45:52.592701Z","submitted_at":"2025-03-21T17:45:04Z","title":"Comparison of dynamical dark energy with {\\Lambda}CDM in light of DESI DR2","version":3},"cited_work":{"arxiv_id":"2503.17342","doi":"10.48550/arxiv.2503.17342","metadata_source":"arxiv_reference","pith_arxiv_id":"2503.17342","snapshot_observed_at":"2026-08-05T02:28:24.338817Z","title":"N., Handley W","venue":"ArXiv.org","work_id":"2ff50020-e4d6-4952-9337-705b42da7b2d","year":2025},"citing_paper":{"arxiv_id":"2606.05853","last_updated":"2026-06-04T08:27:25Z","snapshot_observed_at":"2026-08-01T21:34:07.002669Z","submitted_at":"2026-06-04T08:27:25Z","title":"Reconstructing dark energy with fewer assumptions","version":1},"reference_index":135,"source":"pdf_text","source_observed_at":"2026-06-28T00:07:32.911711Z"},"links":{"cited_paper":"/paper/2503.17342","citing_paper":"/paper/2606.05853"},"observation_digest":"sha256:3f4d5ac38edf604bceaac5b663bdedcb9d9fee5bb8141b3a788b28b1953e7ab1","observation_id":"5b6ec8c6-ec2d-4e2c-b163-7543eec97362","resolution":{"observed_at":"2026-07-02T14:57:04.109049Z","resolver_source":"arxiv_id","status":"verified_exact"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-09T06:31:02.800959+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-09T06:31:02.800959+00:00","source":"crossref"},{"observed_at":"2026-08-09T06:30:57.326959+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":{"arxiv_id":"2503.17342","last_updated":"2025-07-31T19:49:36Z","snapshot_observed_at":"2026-08-07T16:45:52.592701Z","submitted_at":"2025-03-21T17:45:04Z","title":"Comparison of dynamical dark energy with {\\Lambda}CDM in light of DESI DR2","version":3},"cited_work":{"arxiv_id":"2503.17342","doi":"10.48550/arxiv.2503.17342","metadata_source":"arxiv_reference","pith_arxiv_id":"2503.17342","snapshot_observed_at":"2026-08-05T02:28:24.338817Z","title":"N., Handley W","venue":"ArXiv.org","work_id":"2ff50020-e4d6-4952-9337-705b42da7b2d","year":2025},"citing_paper":{"arxiv_id":"2606.17951","last_updated":"2026-06-16T14:04:36Z","snapshot_observed_at":"2026-07-06T23:53:25.839293Z","submitted_at":"2026-06-16T14:04:36Z","title":"Data-Driven Discovery of a Simple Phantom-Crossing Dark Energy Parametrization","version":1},"reference_index":30,"source":"pdf_text","source_observed_at":"2026-06-26T23:43:53.400685Z"},"links":{"cited_paper":"/paper/2503.17342","citing_paper":"/paper/2606.17951"},"observation_digest":"sha256:a0a309b72cd8f235407f19942939ffe13809434c98405892ed910692b81f909c","observation_id":"d1c6b3c4-9b1d-4e23-be74-ea579eaeaf74","resolution":{"observed_at":"2026-07-03T22:08:59.672823Z","resolver_source":"arxiv_id","status":"metadata_mismatch"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-09T06:31:02.800959+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-09T06:31:02.800959+00:00","source":"crossref"},{"observed_at":"2026-08-09T06:30:57.326959+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":{"arxiv_id":"2503.17342","last_updated":"2025-07-31T19:49:36Z","snapshot_observed_at":"2026-08-07T16:45:52.592701Z","submitted_at":"2025-03-21T17:45:04Z","title":"Comparison of dynamical dark energy with {\\Lambda}CDM in light of DESI DR2","version":3},"cited_work":{"arxiv_id":"2503.17342","doi":"10.48550/arxiv.2503.17342","metadata_source":"arxiv_reference","pith_arxiv_id":"2503.17342","snapshot_observed_at":"2026-08-05T02:28:24.338817Z","title":"N., Handley W","venue":"ArXiv.org","work_id":"2ff50020-e4d6-4952-9337-705b42da7b2d","year":2025},"citing_paper":{"arxiv_id":"2606.21826","last_updated":"2026-07-16T15:49:18Z","snapshot_observed_at":"2026-08-02T10:41:21.508983Z","submitted_at":"2026-06-20T01:29:51Z","title":"Dark Energy in the DESI Era: A Brief Review of Evidence, Beyond-$\\Lambda$CDM Interpretations, and Tensions","version":1},"reference_index":66,"source":"arxiv_source","source_observed_at":"2026-06-26T12:13:10.332722Z"},"links":{"cited_paper":"/paper/2503.17342","citing_paper":"/paper/2606.21826"},"observation_digest":"sha256:873a15a5050b328566b835a1028ee8cb85d614b31283d3e7d608bf8bef577780","observation_id":"a071db14-59d8-4304-9f7a-103e8ad036c9","resolution":{"observed_at":"2026-07-04T08:09:40.945726Z","resolver_source":"arxiv_id","status":"verified_exact"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-09T06:31:02.800959+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-09T06:31:02.800959+00:00","source":"crossref"},{"observed_at":"2026-08-09T06:30:57.326959+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":{"arxiv_id":"2503.17342","last_updated":"2025-07-31T19:49:36Z","snapshot_observed_at":"2026-08-07T16:45:52.592701Z","submitted_at":"2025-03-21T17:45:04Z","title":"Comparison of dynamical dark energy with {\\Lambda}CDM in light of DESI DR2","version":3},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2503.17342","snapshot_observed_at":"2026-08-02T10:41:46.414505Z","title":"N., Handley, W","venue":null,"work_id":null,"year":2025},"citing_paper":{"arxiv_id":"2606.21826","last_updated":"2026-07-16T15:49:18Z","snapshot_observed_at":"2026-08-02T10:41:21.508983Z","submitted_at":"2026-06-20T01:29:51Z","title":"Dark Energy in the DESI Era: A Brief Review of Evidence, Beyond-$\\Lambda$CDM Interpretations, and Tensions","version":2},"reference_index":240,"source":"arxiv_source","source_observed_at":"2026-08-02T10:41:46.414505Z"},"links":{"cited_paper":"/paper/2503.17342","citing_paper":"/paper/2606.21826"},"observation_digest":"sha256:0085ed3e1e3527bd5fa2d9b58622f50102940b7a9e5e0f165d00e55b1db6e5d8","observation_id":"2457eaf6-f490-4013-a9c5-662557d4007c","resolution":{"observed_at":"2026-08-02T10:41:46.414505Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2503.17342","last_updated":"2025-07-31T19:49:36Z","snapshot_observed_at":"2026-08-07T16:45:52.592701Z","submitted_at":"2025-03-21T17:45:04Z","title":"Comparison of dynamical dark energy with {\\Lambda}CDM in light of DESI DR2","version":3},"cited_work":{"arxiv_id":"2503.17342","doi":"10.48550/arxiv.2503.17342","metadata_source":"arxiv_reference","pith_arxiv_id":"2503.17342","snapshot_observed_at":"2026-08-05T02:28:24.338817Z","title":"N., Handley W","venue":"ArXiv.org","work_id":"2ff50020-e4d6-4952-9337-705b42da7b2d","year":2025},"citing_paper":{"arxiv_id":"2606.30785","last_updated":"2026-07-21T12:06:55Z","snapshot_observed_at":"2026-08-02T09:31:52.836096Z","submitted_at":"2026-06-29T18:12:29Z","title":"Numerical polology: towards next-generation model-building for cosmology","version":1},"reference_index":98,"source":"pdf_text","source_observed_at":"2026-07-01T01:53:27.058990Z"},"links":{"cited_paper":"/paper/2503.17342","citing_paper":"/paper/2606.30785"},"observation_digest":"sha256:8783ac1d98ae24084c3b2f89ce09f499e2b0a7213bc54b9fa638d11cd4f0d988","observation_id":"46e7cf38-5546-49ee-8cb8-6491ddd799ac","resolution":{"observed_at":"2026-07-01T12:35:44.650750Z","resolver_source":"arxiv_id","status":"verified_exact"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-09T06:31:02.800959+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-09T06:31:02.800959+00:00","source":"crossref"},{"observed_at":"2026-08-09T06:30:57.326959+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":{"arxiv_id":"2503.17342","last_updated":"2025-07-31T19:49:36Z","snapshot_observed_at":"2026-08-07T16:45:52.592701Z","submitted_at":"2025-03-21T17:45:04Z","title":"Comparison of dynamical dark energy with {\\Lambda}CDM in light of DESI DR2","version":3},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2503.17342","snapshot_observed_at":"2026-08-02T09:32:00.268857Z","title":null,"venue":null,"work_id":null,"year":2025},"citing_paper":{"arxiv_id":"2606.30785","last_updated":"2026-07-21T12:06:55Z","snapshot_observed_at":"2026-08-02T09:31:52.836096Z","submitted_at":"2026-06-29T18:12:29Z","title":"Numerical polology: towards next-generation model-building for cosmology","version":2},"reference_index":98,"source":"pdf_text","source_observed_at":"2026-08-02T09:32:00.268857Z"},"links":{"cited_paper":"/paper/2503.17342","citing_paper":"/paper/2606.30785"},"observation_digest":"sha256:d1f8a6aa4469044da34da3395cd0f54a7a207fa2f171240f7d1bb475a1d85207","observation_id":"ace9b02a-d01e-45ff-8382-ffa3094eb600","resolution":{"observed_at":"2026-08-02T09:32:00.268857Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}}],"links":{"evidence":"/evidence","html":"/paper/2503.17342/citation-record","integrity":"/paper/2503.17342/integrity","json":"/paper/2503.17342/citation-record.json","paper":"/paper/2503.17342"},"outbound":[],"paper":{"arxiv_id":"2503.17342","last_updated":"2025-07-31T19:49:36Z","latest_version":3,"primary_category":"astro-ph.CO","snapshot_observed_at":"2026-08-07T16:45:52.592701Z","submitted_at":"2025-03-21T17:45:04Z","title":"Comparison of dynamical dark energy with {\\Lambda}CDM in light of DESI DR2"},"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":"2026-08-09T06:31:02.800959+00:00","source":"crossref"},{"observed_at":"2026-08-09T06:30:57.326959+00:00","source":"retraction_watch"}],"thesis":"As of 9 August 2026, this Paper Citation Record lists 0 of 0 outbound references and 23 inbound Pith citation observations for arXiv:2503.17342."}