{"as_of":"2026-08-17T06:14:00Z","caps":{"database_statements":6,"inbound":100,"outbound":100},"context_digest":"sha256:2407003f3167f64a7b2c9c30408e2967b6818f312195f7b8c37c309c812d2c32","coverage":[{"denominator":36,"lane":"reference_resolution","note":"Typed states for the displayed outbound observations.","records_observed":36,"source":"paper_references, paper_reference_links","source_observed_at":"2026-08-07T14:30:38.020409Z","state":"measured"},{"denominator":55,"lane":"standing_notices","note":"One-hop event checks from named stored sources.","records_observed":55,"source":"scholarly_work_events, retraction_status_cache","source_observed_at":"2026-08-16T06:30:59.297886+00:00","state":"measured"},{"denominator":19,"lane":"inbound_itemization","note":"Pith citing papers itemized under the disclosed page cap.","records_observed":19,"source":"paper_references, paper_reference_links","source_observed_at":"2026-08-16T05:27:54.594572Z","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":"2026-07-10T18:27:31.461114Z","state":"measured"}],"external_citation_measurements":[],"inbound":[{"citation":{"cited_paper":{"arxiv_id":"2505.18937","last_updated":"2025-07-06T08:35:15Z","snapshot_observed_at":"2026-08-17T00:57:47.634789Z","submitted_at":"2025-05-25T02:09:41Z","title":"Examining Quintessence Models with DESI Data","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2505.18937","snapshot_observed_at":"2026-08-16T05:27:54.594572Z","title":"Bayat and M","venue":null,"work_id":null,"year":2025},"citing_paper":{"arxiv_id":"2504.20664","last_updated":"2025-08-15T13:21:18Z","snapshot_observed_at":"2026-08-16T10:58:29.999626Z","submitted_at":"2025-04-29T11:38:28Z","title":"Challenging $\\Lambda$CDM: 5$\\sigma$ Evidence for a Dynamical Dark Energy Late-Time Transition","version":2},"reference_index":131,"source":"pdf_text","source_observed_at":"2026-08-16T05:27:54.594572Z"},"links":{"cited_paper":"/paper/2505.18937","citing_paper":"/paper/2504.20664"},"observation_digest":"sha256:fcb355c8aae8acfd2ff8cd6d3fc25bd0dcaccf208da75b002d3b5c5ab795c50d","observation_id":"816c7b25-f457-480e-be20-ef79f3003eb4","resolution":{"observed_at":"2026-08-16T05:27:54.594572Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2505.18937","last_updated":"2025-07-06T08:35:15Z","snapshot_observed_at":"2026-08-17T00:57:47.634789Z","submitted_at":"2025-05-25T02:09:41Z","title":"Examining Quintessence Models with DESI Data","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2505.18937","snapshot_observed_at":"2026-08-07T11:24:25.139702Z","title":"Bayat and M","venue":null,"work_id":null,"year":2025},"citing_paper":{"arxiv_id":"2506.03019","last_updated":"2025-06-03T15:56:26Z","snapshot_observed_at":"2026-08-14T01:48:45.084629Z","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":95,"source":"pdf_text","source_observed_at":"2026-08-07T11:24:25.139702Z"},"links":{"cited_paper":"/paper/2505.18937","citing_paper":"/paper/2506.03019"},"observation_digest":"sha256:c69d967964460c1c3eb3c4021fc0c18bc2d1f5043cd06baafbc10b4cff5a27e7","observation_id":"9342193c-056a-4594-8ab9-2e245ef8f4c4","resolution":{"observed_at":"2026-08-07T11:24:25.139702Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2505.18937","last_updated":"2025-07-06T08:35:15Z","snapshot_observed_at":"2026-08-17T00:57:47.634789Z","submitted_at":"2025-05-25T02:09:41Z","title":"Examining Quintessence Models with DESI Data","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2505.18937","snapshot_observed_at":"2026-08-07T04:41:33.632820Z","title":"Examining Quintessence Models with DESI Data,","venue":null,"work_id":null,"year":null},"citing_paper":{"arxiv_id":"2506.10075","last_updated":"2025-06-11T18:00:21Z","snapshot_observed_at":"2026-08-14T04:44:20.112426Z","submitted_at":"2025-06-11T18:00:21Z","title":"Topological defects as effective dynamical dark energy","version":1},"reference_index":30,"source":"pdf_text","source_observed_at":"2026-08-07T04:41:33.632820Z"},"links":{"cited_paper":"/paper/2505.18937","citing_paper":"/paper/2506.10075"},"observation_digest":"sha256:86326b6ff46293ae7e42c914cc413da1eed7dc5818ac302a2a00423386228d77","observation_id":"fb9536bd-5283-4017-8c5b-6472cdd48878","resolution":{"observed_at":"2026-08-07T04:41:33.632820Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2505.18937","last_updated":"2025-07-06T08:35:15Z","snapshot_observed_at":"2026-08-17T00:57:47.634789Z","submitted_at":"2025-05-25T02:09:41Z","title":"Examining Quintessence Models with DESI Data","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2505.18937","snapshot_observed_at":"2026-08-07T00:43:09.868849Z","title":"Examining Quintessence Models with DESI Data,","venue":null,"work_id":null,"year":null},"citing_paper":{"arxiv_id":"2506.13047","last_updated":"2025-06-16T02:31:33Z","snapshot_observed_at":"2026-08-16T05:28:11.928870Z","submitted_at":"2025-06-16T02:31:33Z","title":"Simple quintessence models in light of DESI-BAO observations","version":1},"reference_index":47,"source":"pdf_text","source_observed_at":"2026-08-07T00:43:09.868849Z"},"links":{"cited_paper":"/paper/2505.18937","citing_paper":"/paper/2506.13047"},"observation_digest":"sha256:2e8feb98ecede7bee21b740abcdfe7551e180218c6657dbe0a74f2d41c895876","observation_id":"2d2be372-597f-45f3-8ba4-bae294293b1c","resolution":{"observed_at":"2026-08-07T00:43:09.868849Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2505.18937","last_updated":"2025-07-06T08:35:15Z","snapshot_observed_at":"2026-08-17T00:57:47.634789Z","submitted_at":"2025-05-25T02:09:41Z","title":"Examining Quintessence Models with DESI Data","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2505.18937","snapshot_observed_at":"2026-08-06T23:52:21.974313Z","title":"Bayat and M.P","venue":null,"work_id":null,"year":2025},"citing_paper":{"arxiv_id":"2506.16223","last_updated":"2025-06-19T11:28:24Z","snapshot_observed_at":"2026-08-14T20:58:14.280025Z","submitted_at":"2025-06-19T11:28:24Z","title":"Observational Constraints on Scalar Field--Matter Interaction in Weyl Integrable Spacetime","version":1},"reference_index":25,"source":"pdf_text","source_observed_at":"2026-08-06T23:52:21.974313Z"},"links":{"cited_paper":"/paper/2505.18937","citing_paper":"/paper/2506.16223"},"observation_digest":"sha256:50493f2808136f7c849397efa5eaacb0dc87c469d2e448aec62df14532408d57","observation_id":"0712744d-c893-4568-99f3-e20a909dc2b9","resolution":{"observed_at":"2026-08-06T23:52:21.974313Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2505.18937","last_updated":"2025-07-06T08:35:15Z","snapshot_observed_at":"2026-08-17T00:57:47.634789Z","submitted_at":"2025-05-25T02:09:41Z","title":"Examining Quintessence Models with DESI Data","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2505.18937","snapshot_observed_at":"2026-08-06T19:22:36.088310Z","title":"Bayat and M","venue":null,"work_id":null,"year":2025},"citing_paper":{"arxiv_id":"2507.05975","last_updated":"2025-07-08T13:29:42Z","snapshot_observed_at":"2026-08-15T08:18:58.508792Z","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":72,"source":"pdf_text","source_observed_at":"2026-08-06T19:22:36.088310Z"},"links":{"cited_paper":"/paper/2505.18937","citing_paper":"/paper/2507.05975"},"observation_digest":"sha256:efed6e0a0886e1ff548a27ba54f1fc5e9fbb5f08a764e3d799467999dbc9647d","observation_id":"746b1877-76d3-4046-9c58-cd9f5d84a5f6","resolution":{"observed_at":"2026-08-06T19:22:36.088310Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2505.18937","last_updated":"2025-07-06T08:35:15Z","snapshot_observed_at":"2026-08-17T00:57:47.634789Z","submitted_at":"2025-05-25T02:09:41Z","title":"Examining Quintessence Models with DESI Data","version":2},"cited_work":{"arxiv_id":"2505.18937","doi":null,"metadata_source":"pith","pith_arxiv_id":"2505.18937","snapshot_observed_at":"2026-07-10T18:27:31.461114Z","title":"Bayat and M","venue":"astro-ph.CO","work_id":"ab8ace84-c871-447d-9c59-c98465d3946c","year":2025},"citing_paper":{"arxiv_id":"2509.13302","last_updated":"2025-10-09T17:57:59Z","snapshot_observed_at":"2026-08-11T11:22:48.808825Z","submitted_at":"2025-09-16T17:55:24Z","title":"Comparing Minimal and Non-Minimal Quintessence Models to 2025 DESI Data","version":2},"reference_index":52,"source":"pdf_text","source_observed_at":"2026-05-18T15:46:46.916264Z"},"links":{"cited_paper":"/paper/2505.18937","citing_paper":"/paper/2509.13302"},"observation_digest":"sha256:288cf8662fd0bbf2d691d03bf780f1178fecf80ebc144d41fea22b575d83d1fe","observation_id":"7d571dcf-9b60-46cc-aaaf-67fcff32419b","resolution":{"observed_at":"2026-05-18T15:51:35.130120Z","resolver_source":"arxiv_id","status":"verified_exact"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-16T06:30:59.297886+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-16T06:30:59.297886+00:00","source":"crossref"},{"observed_at":"2026-08-16T06:30:54.164669+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":{"arxiv_id":"2505.18937","last_updated":"2025-07-06T08:35:15Z","snapshot_observed_at":"2026-08-17T00:57:47.634789Z","submitted_at":"2025-05-25T02:09:41Z","title":"Examining Quintessence Models with DESI Data","version":2},"cited_work":{"arxiv_id":"2505.18937","doi":null,"metadata_source":"pith","pith_arxiv_id":"2505.18937","snapshot_observed_at":"2026-07-10T18:27:31.461114Z","title":"Bayat and M","venue":"astro-ph.CO","work_id":"ab8ace84-c871-447d-9c59-c98465d3946c","year":2025},"citing_paper":{"arxiv_id":"2601.02077","last_updated":"2026-04-04T13:29:01Z","snapshot_observed_at":"2026-08-14T19:15:34.404775Z","submitted_at":"2026-01-05T12:58:36Z","title":"Joint Constraints on Neutrinos and Dynamical Dark Energy in Minimally Modified Gravity","version":2},"reference_index":39,"source":"pdf_text","source_observed_at":"2026-05-16T18:00:59.984076Z"},"links":{"cited_paper":"/paper/2505.18937","citing_paper":"/paper/2601.02077"},"observation_digest":"sha256:935aec56e5422ef0b087761498fdcdaaefcc08c305da6a93620b0636b2b140da","observation_id":"e2bd3461-a2c8-450b-a91a-fe0307771030","resolution":{"observed_at":"2026-05-16T18:01:09.074819Z","resolver_source":"arxiv_id","status":"verified_exact"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-16T06:30:59.297886+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-16T06:30:59.297886+00:00","source":"crossref"},{"observed_at":"2026-08-16T06:30:54.164669+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":{"arxiv_id":"2505.18937","last_updated":"2025-07-06T08:35:15Z","snapshot_observed_at":"2026-08-17T00:57:47.634789Z","submitted_at":"2025-05-25T02:09:41Z","title":"Examining Quintessence Models with DESI Data","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2505.18937","snapshot_observed_at":"2026-08-03T07:07:15.715247Z","title":"Bayat and M","venue":null,"work_id":null,"year":2025},"citing_paper":{"arxiv_id":"2601.21274","last_updated":"2026-05-30T03:19:05Z","snapshot_observed_at":"2026-08-16T13:55:44.781511Z","submitted_at":"2026-01-29T05:11:07Z","title":"Realizing the phantom-divide crossing with vector and scalar fields","version":2},"reference_index":36,"source":"pdf_text","source_observed_at":"2026-08-03T07:07:15.715247Z"},"links":{"cited_paper":"/paper/2505.18937","citing_paper":"/paper/2601.21274"},"observation_digest":"sha256:4539207f57c4cb07023076bf888e0f1a8a1dcc5766680ae810ca681fd99534b8","observation_id":"52caac23-d457-42b0-8a97-d9956d873da2","resolution":{"observed_at":"2026-08-03T07:07:15.715247Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2505.18937","last_updated":"2025-07-06T08:35:15Z","snapshot_observed_at":"2026-08-17T00:57:47.634789Z","submitted_at":"2025-05-25T02:09:41Z","title":"Examining Quintessence Models with DESI Data","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2505.18937","snapshot_observed_at":"2026-08-03T01:24:41.294199Z","title":"Bayat and M","venue":null,"work_id":null,"year":null},"citing_paper":{"arxiv_id":"2602.10223","last_updated":"2026-07-07T12:26:33Z","snapshot_observed_at":"2026-08-06T12:12:02.801292Z","submitted_at":"2026-02-10T19:14:42Z","title":"Accelerated expansion of the universe purely driven by scalar field fluctuations","version":2},"reference_index":10,"source":"pdf_text","source_observed_at":"2026-08-03T01:24:41.294199Z"},"links":{"cited_paper":"/paper/2505.18937","citing_paper":"/paper/2602.10223"},"observation_digest":"sha256:713534fd23df214fb313f3aec05c3a672955978126e770ae0a2d4288db2d46ef","observation_id":"827ab1a7-aa4f-4b1a-9479-fadee1e5e3df","resolution":{"observed_at":"2026-08-03T01:24:41.294199Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2505.18937","last_updated":"2025-07-06T08:35:15Z","snapshot_observed_at":"2026-08-17T00:57:47.634789Z","submitted_at":"2025-05-25T02:09:41Z","title":"Examining Quintessence Models with DESI Data","version":2},"cited_work":{"arxiv_id":"2505.18937","doi":null,"metadata_source":"pith","pith_arxiv_id":"2505.18937","snapshot_observed_at":"2026-07-10T18:27:31.461114Z","title":"Bayat and M","venue":"astro-ph.CO","work_id":"ab8ace84-c871-447d-9c59-c98465d3946c","year":2025},"citing_paper":{"arxiv_id":"2602.19118","last_updated":"2026-05-13T02:13:18Z","snapshot_observed_at":"2026-08-13T19:26:32.221828Z","submitted_at":"2026-02-22T10:25:36Z","title":"Exponential Quintessence Model: Analytical Quantification of the Fine-Tuning Problem in Dark Energy","version":2},"reference_index":38,"source":"pdf_text","source_observed_at":"2026-05-15T21:07:09.123537Z"},"links":{"cited_paper":"/paper/2505.18937","citing_paper":"/paper/2602.19118"},"observation_digest":"sha256:9e0c127eaf99ed78b4609bf00d9ca7370ab3d10f36aaf1ff2914e527eaeb0f09","observation_id":"753cb559-ecc1-44a3-868e-f6fe28829b1a","resolution":{"observed_at":"2026-05-15T21:10:18.798978Z","resolver_source":"arxiv_id","status":"verified_exact"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-16T06:30:59.297886+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-16T06:30:59.297886+00:00","source":"crossref"},{"observed_at":"2026-08-16T06:30:54.164669+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":{"arxiv_id":"2505.18937","last_updated":"2025-07-06T08:35:15Z","snapshot_observed_at":"2026-08-17T00:57:47.634789Z","submitted_at":"2025-05-25T02:09:41Z","title":"Examining Quintessence Models with DESI Data","version":2},"cited_work":{"arxiv_id":"2505.18937","doi":null,"metadata_source":"pith","pith_arxiv_id":"2505.18937","snapshot_observed_at":"2026-07-10T18:27:31.461114Z","title":"Bayat and M","venue":"astro-ph.CO","work_id":"ab8ace84-c871-447d-9c59-c98465d3946c","year":2025},"citing_paper":{"arxiv_id":"2603.25797","last_updated":"2026-04-09T08:47:22Z","snapshot_observed_at":"2026-08-11T06:06:49.688965Z","submitted_at":"2026-03-26T18:05:41Z","title":"Dark energy from string theory: an introductory review","version":2},"reference_index":179,"source":"pdf_text","source_observed_at":"2026-05-15T00:16:01.150874Z"},"links":{"cited_paper":"/paper/2505.18937","citing_paper":"/paper/2603.25797"},"observation_digest":"sha256:b6502a752c18877b6e30f8c32c427cc338e277a6809c37ba6d07a5029106a8de","observation_id":"fdf0fec9-00b0-4bf3-8f33-d95820670cc8","resolution":{"observed_at":"2026-05-15T00:18:22.134397Z","resolver_source":"arxiv_id","status":"verified_exact"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-16T06:30:59.297886+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-16T06:30:59.297886+00:00","source":"crossref"},{"observed_at":"2026-08-16T06:30:54.164669+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":{"arxiv_id":"2505.18937","last_updated":"2025-07-06T08:35:15Z","snapshot_observed_at":"2026-08-17T00:57:47.634789Z","submitted_at":"2025-05-25T02:09:41Z","title":"Examining Quintessence Models with DESI Data","version":2},"cited_work":{"arxiv_id":"2505.18937","doi":null,"metadata_source":"pith","pith_arxiv_id":"2505.18937","snapshot_observed_at":"2026-07-10T18:27:31.461114Z","title":"Bayat and M","venue":"astro-ph.CO","work_id":"ab8ace84-c871-447d-9c59-c98465d3946c","year":2025},"citing_paper":{"arxiv_id":"2604.08449","last_updated":"2026-04-17T13:38:47Z","snapshot_observed_at":"2026-08-11T13:45:12.764050Z","submitted_at":"2026-04-09T16:45:31Z","title":"Coupled Dark Energy and Dark Matter for DESI: An Effective Guide to the Phantom Divide","version":2},"reference_index":54,"source":"pdf_text","source_observed_at":"2026-05-10T17:12:43.883197Z"},"links":{"cited_paper":"/paper/2505.18937","citing_paper":"/paper/2604.08449"},"observation_digest":"sha256:0b7b4306d32a741b3abbcd9a80734043f8b87a7d3c12d620b04c2a651cc5f2a1","observation_id":"1f821367-3223-43bb-9ebc-67637620d62a","resolution":{"observed_at":"2026-05-11T07:21:00.188744Z","resolver_source":"arxiv_id","status":"metadata_mismatch"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-16T06:30:59.297886+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-16T06:30:59.297886+00:00","source":"crossref"},{"observed_at":"2026-08-16T06:30:54.164669+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":{"arxiv_id":"2505.18937","last_updated":"2025-07-06T08:35:15Z","snapshot_observed_at":"2026-08-17T00:57:47.634789Z","submitted_at":"2025-05-25T02:09:41Z","title":"Examining Quintessence Models with DESI Data","version":2},"cited_work":{"arxiv_id":"2505.18937","doi":null,"metadata_source":"pith","pith_arxiv_id":"2505.18937","snapshot_observed_at":"2026-07-10T18:27:31.461114Z","title":"Bayat and M","venue":"astro-ph.CO","work_id":"ab8ace84-c871-447d-9c59-c98465d3946c","year":2025},"citing_paper":{"arxiv_id":"2605.05122","last_updated":"2026-05-06T16:51:02Z","snapshot_observed_at":"2026-08-11T01:48:41.699582Z","submitted_at":"2026-05-06T16:51:02Z","title":"Exponential Quintessence: Analytic Relationship Between the Current Equation of State Parameter and the Potential Parameter","version":1},"reference_index":41,"source":"pdf_text","source_observed_at":"2026-05-08T16:52:03.209429Z"},"links":{"cited_paper":"/paper/2505.18937","citing_paper":"/paper/2605.05122"},"observation_digest":"sha256:579c020acadc1e21029c36722eee080d77e1ca33b84343fc0f461a8c10f51380","observation_id":"03143b51-5cbe-4f88-8c8c-d036022164c0","resolution":{"observed_at":"2026-05-11T18:01:05.109291Z","resolver_source":"arxiv_id","status":"verified_exact"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-16T06:30:59.297886+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-16T06:30:59.297886+00:00","source":"crossref"},{"observed_at":"2026-08-16T06:30:54.164669+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":{"arxiv_id":"2505.18937","last_updated":"2025-07-06T08:35:15Z","snapshot_observed_at":"2026-08-17T00:57:47.634789Z","submitted_at":"2025-05-25T02:09:41Z","title":"Examining Quintessence Models with DESI Data","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2505.18937","snapshot_observed_at":"2026-08-02T14:29:39.794130Z","title":"Bayat and M","venue":null,"work_id":null,"year":2025},"citing_paper":{"arxiv_id":"2605.10476","last_updated":"2026-07-21T12:07:55Z","snapshot_observed_at":"2026-08-11T08:05:13.599295Z","submitted_at":"2026-05-11T12:38:17Z","title":"Breaking Free from the Swampland of Impossible Universes through the DESI Portal","version":4},"reference_index":250,"source":"pdf_text","source_observed_at":"2026-08-02T14:29:39.794130Z"},"links":{"cited_paper":"/paper/2505.18937","citing_paper":"/paper/2605.10476"},"observation_digest":"sha256:688cffdf855c54354c953f5863e06fe514acee9a9dd279fd304df1f4c319ff6f","observation_id":"0ec6906e-9644-4d06-881d-0602f9d7f5ac","resolution":{"observed_at":"2026-08-02T14:29:39.794130Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2505.18937","last_updated":"2025-07-06T08:35:15Z","snapshot_observed_at":"2026-08-17T00:57:47.634789Z","submitted_at":"2025-05-25T02:09:41Z","title":"Examining Quintessence Models with DESI Data","version":2},"cited_work":{"arxiv_id":"2505.18937","doi":null,"metadata_source":"pith","pith_arxiv_id":"2505.18937","snapshot_observed_at":"2026-07-10T18:27:31.461114Z","title":"Bayat and M","venue":"astro-ph.CO","work_id":"ab8ace84-c871-447d-9c59-c98465d3946c","year":2025},"citing_paper":{"arxiv_id":"2605.20748","last_updated":"2026-05-20T05:49:49Z","snapshot_observed_at":"2026-08-16T03:09:37.920752Z","submitted_at":"2026-05-20T05:49:49Z","title":"Probing late-time deviations from $\\Lambda$CDM with a quadratic dark energy expansion","version":1},"reference_index":46,"source":"pdf_text","source_observed_at":"2026-05-21T02:43:57.001089Z"},"links":{"cited_paper":"/paper/2505.18937","citing_paper":"/paper/2605.20748"},"observation_digest":"sha256:b84827a76399d429b1023cc7a8c5c39953ba884b32deafb16a5375b3bad7c852","observation_id":"6a87f2d7-69c7-4d07-8d69-2845f3392af2","resolution":{"observed_at":"2026-05-21T02:44:25.208744Z","resolver_source":"arxiv_id","status":"verified_exact"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-16T06:30:59.297886+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-16T06:30:59.297886+00:00","source":"crossref"},{"observed_at":"2026-08-16T06:30:54.164669+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":{"arxiv_id":"2505.18937","last_updated":"2025-07-06T08:35:15Z","snapshot_observed_at":"2026-08-17T00:57:47.634789Z","submitted_at":"2025-05-25T02:09:41Z","title":"Examining Quintessence Models with DESI Data","version":2},"cited_work":{"arxiv_id":"2505.18937","doi":null,"metadata_source":"pith","pith_arxiv_id":"2505.18937","snapshot_observed_at":"2026-07-10T18:27:31.461114Z","title":"Bayat and M","venue":"astro-ph.CO","work_id":"ab8ace84-c871-447d-9c59-c98465d3946c","year":2025},"citing_paper":{"arxiv_id":"2607.07777","last_updated":"2026-07-08T17:38:46Z","snapshot_observed_at":"2026-08-05T11:19:33.253012Z","submitted_at":"2026-07-08T17:38:46Z","title":"The Status of Single Scalar Field Dark Energy","version":1},"reference_index":98,"source":"pdf_text","source_observed_at":"2026-07-10T18:19:17.740185Z"},"links":{"cited_paper":"/paper/2505.18937","citing_paper":"/paper/2607.07777"},"observation_digest":"sha256:a5a53846563f9d6031352f93c65959d2f197e4d3554d6dd97ea3acf3cd3baf91","observation_id":"bd20cbfa-fd51-4595-a790-16fe46c5f6a9","resolution":{"observed_at":"2026-07-10T18:27:31.462376Z","resolver_source":"local_arxiv","status":"verified_exact"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-16T06:30:59.297886+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-16T06:30:59.297886+00:00","source":"crossref"},{"observed_at":"2026-08-16T06:30:54.164669+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":{"arxiv_id":"2505.18937","last_updated":"2025-07-06T08:35:15Z","snapshot_observed_at":"2026-08-17T00:57:47.634789Z","submitted_at":"2025-05-25T02:09:41Z","title":"Examining Quintessence Models with DESI Data","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2505.18937","snapshot_observed_at":"2026-08-01T15:41:42.128075Z","title":"Bayat and M","venue":null,"work_id":null,"year":2025},"citing_paper":{"arxiv_id":"2607.26447","last_updated":"2026-07-29T03:52:12Z","snapshot_observed_at":"2026-08-09T00:15:56.534898Z","submitted_at":"2026-07-29T03:52:12Z","title":"Phantom-divide crossing and suppressed structure growth in kinetically braided dark energy with momentum exchange","version":1},"reference_index":44,"source":"pdf_text","source_observed_at":"2026-08-01T15:41:42.128075Z"},"links":{"cited_paper":"/paper/2505.18937","citing_paper":"/paper/2607.26447"},"observation_digest":"sha256:2c0b6f399007379cc2844559118a7430c3ee31576d9c93b52d7fa268e091f2a1","observation_id":"b236bf66-c7c7-4865-b6d9-e397f6a84717","resolution":{"observed_at":"2026-08-01T15:41:42.128075Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2505.18937","last_updated":"2025-07-06T08:35:15Z","snapshot_observed_at":"2026-08-17T00:57:47.634789Z","submitted_at":"2025-05-25T02:09:41Z","title":"Examining Quintessence Models with DESI Data","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2505.18937","snapshot_observed_at":"2026-08-14T06:05:37.022992Z","title":"Bayat and M","venue":null,"work_id":null,"year":null},"citing_paper":{"arxiv_id":"2608.13488","last_updated":"2026-08-13T17:16:23Z","snapshot_observed_at":"2026-08-16T23:13:03.817631Z","submitted_at":"2026-08-13T17:16:23Z","title":"Higher-Order Analytical Expansion of Thawing Dark Energy with an Exponential Potential","version":1},"reference_index":56,"source":"pdf_text","source_observed_at":"2026-08-14T06:05:37.022992Z"},"links":{"cited_paper":"/paper/2505.18937","citing_paper":"/paper/2608.13488"},"observation_digest":"sha256:f39cf3c450527bd8c82d77de5f697cdaf7f2f0eae18237c59e46286a64315033","observation_id":"c1a4196c-55c9-42d0-91c2-e5aa5a3a512a","resolution":{"observed_at":"2026-08-14T06:05:37.022992Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}}],"links":{"evidence":"/evidence","html":"/paper/2505.18937/citation-record","integrity":"/paper/2505.18937/integrity","json":"/paper/2505.18937/citation-record.json","paper":"/paper/2505.18937"},"outbound":[{"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":"2026-08-07T14:30:34.877272Z","title":"DESI 2024 VI: cosmologi- cal constraints from the measurements of baryon acous- tic oscillations,","venue":null,"work_id":null,"year":2025},"citing_paper":{"arxiv_id":"2505.18937","last_updated":"2025-07-06T08:35:15Z","snapshot_observed_at":"2026-08-17T00:57:47.634789Z","submitted_at":"2025-05-25T02:09:41Z","title":"Examining Quintessence Models with DESI Data","version":2},"reference_index":1,"source":"pdf_text","source_observed_at":"2026-08-07T14:30:34.877272Z"},"links":{"cited_paper":"/paper/2404.03002","citing_paper":"/paper/2505.18937"},"observation_digest":"sha256:0640f1ac83e6599aa3fd20e1332724c2ee838d59451f46d5bc0e99cbe7c483eb","observation_id":"4e2c6818-7d42-42b9-bb36-fc2449256e92","resolution":{"observed_at":"2026-08-07T14:30:34.877272Z","resolver_source":null,"status":"malformed_identifier"},"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":"2026-08-16T23:26:44.283674Z","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":"2026-08-07T14:30:34.980058Z","title":"Assessing observational constraints on dark energy,","venue":null,"work_id":null,"year":2024},"citing_paper":{"arxiv_id":"2505.18937","last_updated":"2025-07-06T08:35:15Z","snapshot_observed_at":"2026-08-17T00:57:47.634789Z","submitted_at":"2025-05-25T02:09:41Z","title":"Examining Quintessence Models with DESI Data","version":2},"reference_index":2,"source":"pdf_text","source_observed_at":"2026-08-07T14:30:34.980058Z"},"links":{"cited_paper":"/paper/2405.03933","citing_paper":"/paper/2505.18937"},"observation_digest":"sha256:4a505b85d57760a8bc6a920d4fe6482461938adafd3f76013579311acf87d28a","observation_id":"060c7a18-00b3-42bf-b20d-e6d4859a3fd6","resolution":{"observed_at":"2026-08-07T14:30:34.980058Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2405.18747","last_updated":"2024-05-29T04:09:59Z","snapshot_observed_at":"2026-08-16T13:48:21.389151Z","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":"2026-08-07T14:30:35.093085Z","title":"DESI con- straints on exponential quintessence,","venue":null,"work_id":null,"year":2024},"citing_paper":{"arxiv_id":"2505.18937","last_updated":"2025-07-06T08:35:15Z","snapshot_observed_at":"2026-08-17T00:57:47.634789Z","submitted_at":"2025-05-25T02:09:41Z","title":"Examining Quintessence Models with DESI Data","version":2},"reference_index":3,"source":"pdf_text","source_observed_at":"2026-08-07T14:30:35.093085Z"},"links":{"cited_paper":"/paper/2405.18747","citing_paper":"/paper/2505.18937"},"observation_digest":"sha256:5dc6f39e8d30fc27f29442af80ff7cd2bb7099f0fdebb8258b9f6cddfb606543","observation_id":"77c7445a-86ed-4302-9635-714a0f3bb007","resolution":{"observed_at":"2026-08-07T14:30:35.093085Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2412.07418","last_updated":"2025-03-07T15:16:26Z","snapshot_observed_at":"2026-08-16T13:00:19.007103Z","submitted_at":"2024-12-10T11:12:24Z","title":"Kick it like DESI: PNGB quintessence with a dynamically generated initial velocity","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2412.07418","snapshot_observed_at":"2026-08-07T14:30:35.180092Z","title":"Kick it like DESI: PNGB quintessence with a dynamically generated initial velocity,","venue":null,"work_id":null,"year":2025},"citing_paper":{"arxiv_id":"2505.18937","last_updated":"2025-07-06T08:35:15Z","snapshot_observed_at":"2026-08-17T00:57:47.634789Z","submitted_at":"2025-05-25T02:09:41Z","title":"Examining Quintessence Models with DESI Data","version":2},"reference_index":4,"source":"pdf_text","source_observed_at":"2026-08-07T14:30:35.180092Z"},"links":{"cited_paper":"/paper/2412.07418","citing_paper":"/paper/2505.18937"},"observation_digest":"sha256:afac38eebd52d72bc6ea5be7748b97295a51c6ae51b9befada74f62e6c70fdab","observation_id":"a778d6b1-a552-4c72-b04b-609eb5d3d10b","resolution":{"observed_at":"2026-08-07T14:30:35.180092Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2503.19428","last_updated":"2025-06-03T14:07:36Z","snapshot_observed_at":"2026-08-16T12:47:04.732944Z","submitted_at":"2025-03-25T08:19:01Z","title":"S-dual Quintessence, the Swampland, and the DESI DR2 Results","version":3},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2503.19428","snapshot_observed_at":"2026-08-07T14:30:35.294826Z","title":"S-dual Quintessence, the Swampland, and the DESI DR2 Re- sults,","venue":null,"work_id":null,"year":null},"citing_paper":{"arxiv_id":"2505.18937","last_updated":"2025-07-06T08:35:15Z","snapshot_observed_at":"2026-08-17T00:57:47.634789Z","submitted_at":"2025-05-25T02:09:41Z","title":"Examining Quintessence Models with DESI Data","version":2},"reference_index":5,"source":"pdf_text","source_observed_at":"2026-08-07T14:30:35.294826Z"},"links":{"cited_paper":"/paper/2503.19428","citing_paper":"/paper/2505.18937"},"observation_digest":"sha256:1d1566cf9c132fa5bced735eb533688f8a3f9ac093410c4e533cb4ef30e9373d","observation_id":"ae71f570-4b05-4757-b83b-55f5dfb4749b","resolution":{"observed_at":"2026-08-07T14:30:35.294826Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2504.04226","last_updated":"2025-04-11T15:54:01Z","snapshot_observed_at":"2026-08-16T12:43:43.365387Z","submitted_at":"2025-04-05T16:26:51Z","title":"Has DESI detected exponential quintessence?","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2504.04226","snapshot_observed_at":"2026-08-07T14:30:35.372731Z","title":"Has DESI detected exponential quintessence?,","venue":null,"work_id":null,"year":null},"citing_paper":{"arxiv_id":"2505.18937","last_updated":"2025-07-06T08:35:15Z","snapshot_observed_at":"2026-08-17T00:57:47.634789Z","submitted_at":"2025-05-25T02:09:41Z","title":"Examining Quintessence Models with DESI Data","version":2},"reference_index":6,"source":"pdf_text","source_observed_at":"2026-08-07T14:30:35.372731Z"},"links":{"cited_paper":"/paper/2504.04226","citing_paper":"/paper/2505.18937"},"observation_digest":"sha256:49acdad9822fd7408983acae2f96b85bc0400523b0cbec6d5f6fd2aba8e7b6fb","observation_id":"089f76cf-8641-4633-9462-2aaf3dcc3856","resolution":{"observed_at":"2026-08-07T14:30:35.372731Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2504.15190","last_updated":"2025-06-12T09:40:00Z","snapshot_observed_at":"2026-08-16T23:56:56.917068Z","submitted_at":"2025-04-21T16:00:28Z","title":"Physical vs phantom dark energy after DESI: thawing quintessence in a curved background","version":3},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2504.15190","snapshot_observed_at":"2026-08-07T14:30:35.453275Z","title":"Physical vs phantom dark energy after DESI: thawing quintessence in a curved background,","venue":null,"work_id":null,"year":null},"citing_paper":{"arxiv_id":"2505.18937","last_updated":"2025-07-06T08:35:15Z","snapshot_observed_at":"2026-08-17T00:57:47.634789Z","submitted_at":"2025-05-25T02:09:41Z","title":"Examining Quintessence Models with DESI Data","version":2},"reference_index":7,"source":"pdf_text","source_observed_at":"2026-08-07T14:30:35.453275Z"},"links":{"cited_paper":"/paper/2504.15190","citing_paper":"/paper/2505.18937"},"observation_digest":"sha256:1d9575285ee3d0ef6dd5723615dfb8020fb2a73888a2270ecd01e295b41f8a32","observation_id":"85ddcbee-ea72-4bbe-9617-9864825f92bb","resolution":{"observed_at":"2026-08-07T14:30:35.453275Z","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":"2026-08-07T14:30:35.602677Z","title":"Thawing quintessence and transient cosmic acceleration in light of DESI,","venue":null,"work_id":null,"year":null},"citing_paper":{"arxiv_id":"2505.18937","last_updated":"2025-07-06T08:35:15Z","snapshot_observed_at":"2026-08-17T00:57:47.634789Z","submitted_at":"2025-05-25T02:09:41Z","title":"Examining Quintessence Models with DESI Data","version":2},"reference_index":8,"source":"pdf_text","source_observed_at":"2026-08-07T14:30:35.602677Z"},"links":{"citing_paper":"/paper/2505.18937"},"observation_digest":"sha256:3fe50a2b81d4138a9227b94557dee7e5fb7ab175ed87d0a957e9d21bd77f15cb","observation_id":"a15de1ba-5e2d-497c-9642-64c0ebdf24cd","resolution":{"observed_at":"2026-08-07T14:30:35.602677Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2404.08056","last_updated":"2024-11-08T14:34:18Z","snapshot_observed_at":"2026-08-16T14:01:37.304051Z","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":"2026-08-07T14:30:35.713553Z","title":"Interpreting DESI’s evi- dence for evolving dark energy,","venue":null,"work_id":null,"year":2024},"citing_paper":{"arxiv_id":"2505.18937","last_updated":"2025-07-06T08:35:15Z","snapshot_observed_at":"2026-08-17T00:57:47.634789Z","submitted_at":"2025-05-25T02:09:41Z","title":"Examining Quintessence Models with DESI Data","version":2},"reference_index":9,"source":"pdf_text","source_observed_at":"2026-08-07T14:30:35.713553Z"},"links":{"cited_paper":"/paper/2404.08056","citing_paper":"/paper/2505.18937"},"observation_digest":"sha256:d3b4a1e823511299bcff148aadf77623cb29c4464d44690b90a72a173ea861c5","observation_id":"1cb854d5-b7fd-46e1-9e07-5b515bda127a","resolution":{"observed_at":"2026-08-07T14:30:35.713553Z","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":"2026-08-16T13:53:40.637771Z","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":"2026-08-07T14:30:35.801004Z","title":"A new diagnostic for the null test of dy- namical dark energy in light of DESI 2024 and other BAO data,","venue":null,"work_id":null,"year":2024},"citing_paper":{"arxiv_id":"2505.18937","last_updated":"2025-07-06T08:35:15Z","snapshot_observed_at":"2026-08-17T00:57:47.634789Z","submitted_at":"2025-05-25T02:09:41Z","title":"Examining Quintessence Models with DESI Data","version":2},"reference_index":10,"source":"pdf_text","source_observed_at":"2026-08-07T14:30:35.801004Z"},"links":{"cited_paper":"/paper/2405.06618","citing_paper":"/paper/2505.18937"},"observation_digest":"sha256:ab9dd30f3f0a9cf6c6d305495304c51838a0a812c076c0eb337aab219bb8f01c","observation_id":"c0519a7a-23bd-4865-9937-455b3062e868","resolution":{"observed_at":"2026-08-07T14:30:35.801004Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2405.09323","last_updated":"2024-08-20T12:00:11Z","snapshot_observed_at":"2026-08-16T13:52:29.625077Z","submitted_at":"2024-05-15T13:24:39Z","title":"Exponential Quintessence: curved, steep and stringy?","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2405.09323","snapshot_observed_at":"2026-08-07T14:30:35.890558Z","title":"Exponential quintessence: curved, steep and stringy?,","venue":null,"work_id":null,"year":2024},"citing_paper":{"arxiv_id":"2505.18937","last_updated":"2025-07-06T08:35:15Z","snapshot_observed_at":"2026-08-17T00:57:47.634789Z","submitted_at":"2025-05-25T02:09:41Z","title":"Examining Quintessence Models with DESI Data","version":2},"reference_index":11,"source":"pdf_text","source_observed_at":"2026-08-07T14:30:35.890558Z"},"links":{"cited_paper":"/paper/2405.09323","citing_paper":"/paper/2505.18937"},"observation_digest":"sha256:5f4b6e26acadf3362b9298f60194ec095bfa166e560d85d797b35da750987dd4","observation_id":"9307c0a5-ecc0-4f54-9686-ef1c18f3f3dc","resolution":{"observed_at":"2026-08-07T14:30:35.890558Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2406.00634","last_updated":"2025-05-15T05:24:24Z","snapshot_observed_at":"2026-08-16T13:47:03.794700Z","submitted_at":"2024-06-02T06:40:05Z","title":"Dynamical dark energy in the light of DESI 2024 data","version":3},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2406.00634","snapshot_observed_at":"2026-08-07T14:30:35.926364Z","title":"Dynamical dark energy in the light of DESI 2024 data,","venue":null,"work_id":null,"year":2025},"citing_paper":{"arxiv_id":"2505.18937","last_updated":"2025-07-06T08:35:15Z","snapshot_observed_at":"2026-08-17T00:57:47.634789Z","submitted_at":"2025-05-25T02:09:41Z","title":"Examining Quintessence Models with DESI Data","version":2},"reference_index":12,"source":"pdf_text","source_observed_at":"2026-08-07T14:30:35.926364Z"},"links":{"cited_paper":"/paper/2406.00634","citing_paper":"/paper/2505.18937"},"observation_digest":"sha256:a1ae171cc7e2551232b182e3b528bd63a79314bee1ba943107d27024281c0585","observation_id":"6332865e-e8fc-42be-8933-ea72c2f5d648","resolution":{"observed_at":"2026-08-07T14:30:35.926364Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2406.08459","last_updated":"2024-11-15T13:55:27Z","snapshot_observed_at":"2026-08-16T13:43:37.968289Z","submitted_at":"2024-06-12T17:50:47Z","title":"Consistent Theories for the DESI dark energy fit","version":3},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2406.08459","snapshot_observed_at":"2026-08-07T14:30:35.994598Z","title":"Consistent theories for the DESI dark energy fit,","venue":null,"work_id":null,"year":2024},"citing_paper":{"arxiv_id":"2505.18937","last_updated":"2025-07-06T08:35:15Z","snapshot_observed_at":"2026-08-17T00:57:47.634789Z","submitted_at":"2025-05-25T02:09:41Z","title":"Examining Quintessence Models with DESI Data","version":2},"reference_index":13,"source":"pdf_text","source_observed_at":"2026-08-07T14:30:35.994598Z"},"links":{"cited_paper":"/paper/2406.08459","citing_paper":"/paper/2505.18937"},"observation_digest":"sha256:e4b5199dbbb09e991d342aca5834082e325448226e0f0198a0a70187359bddf5","observation_id":"38b2ee09-67d0-4296-8da6-494e8f7859ab","resolution":{"observed_at":"2026-08-07T14:30:35.994598Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2407.14378","last_updated":"2025-05-05T12:03:47Z","snapshot_observed_at":"2026-08-16T13:32:41.150132Z","submitted_at":"2024-07-19T15:06:16Z","title":"New simple and accurate quintessence approximations","version":3},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2407.14378","snapshot_observed_at":"2026-08-07T14:30:36.074783Z","title":"New simple and accurate quintessence approximations,","venue":null,"work_id":null,"year":2025},"citing_paper":{"arxiv_id":"2505.18937","last_updated":"2025-07-06T08:35:15Z","snapshot_observed_at":"2026-08-17T00:57:47.634789Z","submitted_at":"2025-05-25T02:09:41Z","title":"Examining Quintessence Models with DESI Data","version":2},"reference_index":14,"source":"pdf_text","source_observed_at":"2026-08-07T14:30:36.074783Z"},"links":{"cited_paper":"/paper/2407.14378","citing_paper":"/paper/2505.18937"},"observation_digest":"sha256:7731d9cf271a16c25c5548211b425306ecebcbbace47486572f18e836228f9df","observation_id":"b07decbf-bd7f-44c5-8772-1720b40f93ef","resolution":{"observed_at":"2026-08-07T14:30:36.074783Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2407.16689","last_updated":"2024-09-24T15:26:01Z","snapshot_observed_at":"2026-08-16T13:31:40.342702Z","submitted_at":"2024-07-23T17:54:39Z","title":"Robust Preference for Dynamical Dark Energy in DESI BAO and SN Measurements","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2407.16689","snapshot_observed_at":"2026-08-07T14:30:36.123147Z","title":"Robust preference for Dy- namical Dark Energy in DESI BAO and SN mea- surements,","venue":null,"work_id":null,"year":2024},"citing_paper":{"arxiv_id":"2505.18937","last_updated":"2025-07-06T08:35:15Z","snapshot_observed_at":"2026-08-17T00:57:47.634789Z","submitted_at":"2025-05-25T02:09:41Z","title":"Examining Quintessence Models with DESI Data","version":2},"reference_index":15,"source":"pdf_text","source_observed_at":"2026-08-07T14:30:36.123147Z"},"links":{"cited_paper":"/paper/2407.16689","citing_paper":"/paper/2505.18937"},"observation_digest":"sha256:5b75efee0678dfa0199a01700804a629e976eb361d84794f8ad878d6ee31592f","observation_id":"9243c9a7-5475-479a-a5fa-7c103135ebeb","resolution":{"observed_at":"2026-08-07T14:30:36.123147Z","resolver_source":null,"status":"malformed_identifier"},"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":"2026-08-16T13:22:37.112596Z","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":"2026-08-07T14:30:36.160280Z","title":"Scant evidence for thawing quintessence,","venue":null,"work_id":null,"year":2024},"citing_paper":{"arxiv_id":"2505.18937","last_updated":"2025-07-06T08:35:15Z","snapshot_observed_at":"2026-08-17T00:57:47.634789Z","submitted_at":"2025-05-25T02:09:41Z","title":"Examining Quintessence Models with DESI Data","version":2},"reference_index":16,"source":"pdf_text","source_observed_at":"2026-08-07T14:30:36.160280Z"},"links":{"cited_paper":"/paper/2408.17318","citing_paper":"/paper/2505.18937"},"observation_digest":"sha256:7b60ce42136a9182aa8b4449eb1a13af5ee6501c2412e8bfd6e0b0212aef4867","observation_id":"b4613d46-4ccd-497d-a424-8c685d4053b8","resolution":{"observed_at":"2026-08-07T14:30:36.160280Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2410.17182","last_updated":"2025-05-23T10:31:48Z","snapshot_observed_at":"2026-08-16T13:06:54.538308Z","submitted_at":"2024-10-22T16:59:06Z","title":"Quintessence: an analytical study, with theoretical and observational applications","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2410.17182","snapshot_observed_at":"2026-08-07T14:30:36.187919Z","title":"Quintessence: an analytical study, with theoretical and observational applications,","venue":null,"work_id":null,"year":null},"citing_paper":{"arxiv_id":"2505.18937","last_updated":"2025-07-06T08:35:15Z","snapshot_observed_at":"2026-08-17T00:57:47.634789Z","submitted_at":"2025-05-25T02:09:41Z","title":"Examining Quintessence Models with DESI Data","version":2},"reference_index":17,"source":"pdf_text","source_observed_at":"2026-08-07T14:30:36.187919Z"},"links":{"cited_paper":"/paper/2410.17182","citing_paper":"/paper/2505.18937"},"observation_digest":"sha256:d6cbae8330fdc19d8658f57540bfd0cdaf6d92c3e6768fc88a5d5ef1b339127b","observation_id":"86d9603a-ec32-496c-8c2e-0e805bb58158","resolution":{"observed_at":"2026-08-07T14:30:36.187919Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2411.13637","last_updated":"2025-05-30T21:49:57Z","snapshot_observed_at":"2026-08-15T02:51:48.572798Z","submitted_at":"2024-11-20T19:00:00Z","title":"Do Observations Prefer Thawing Quintessence?","version":4},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2411.13637","snapshot_observed_at":"2026-08-07T14:30:36.268653Z","title":"Do Observations Prefer Thawing Quintessence?,","venue":null,"work_id":null,"year":null},"citing_paper":{"arxiv_id":"2505.18937","last_updated":"2025-07-06T08:35:15Z","snapshot_observed_at":"2026-08-17T00:57:47.634789Z","submitted_at":"2025-05-25T02:09:41Z","title":"Examining Quintessence Models with DESI Data","version":2},"reference_index":18,"source":"pdf_text","source_observed_at":"2026-08-07T14:30:36.268653Z"},"links":{"cited_paper":"/paper/2411.13637","citing_paper":"/paper/2505.18937"},"observation_digest":"sha256:9f10ff7d0139325248332f86019811808cb89918732f690ff2afe1b43958e1ac","observation_id":"69359bfa-a2e3-4eb0-83eb-08f6f3118b23","resolution":{"observed_at":"2026-08-07T14:30:36.268653Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2411.16046","last_updated":"2024-11-25T02:19:48Z","snapshot_observed_at":"2026-08-14T03:17:26.016710Z","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":"2026-08-07T14:30:36.340461Z","title":"On the Evidence of Dynamical Dark Energy,","venue":null,"work_id":null,"year":2025},"citing_paper":{"arxiv_id":"2505.18937","last_updated":"2025-07-06T08:35:15Z","snapshot_observed_at":"2026-08-17T00:57:47.634789Z","submitted_at":"2025-05-25T02:09:41Z","title":"Examining Quintessence Models with DESI Data","version":2},"reference_index":19,"source":"pdf_text","source_observed_at":"2026-08-07T14:30:36.340461Z"},"links":{"cited_paper":"/paper/2411.16046","citing_paper":"/paper/2505.18937"},"observation_digest":"sha256:f29d67c8f26b1ecd23aae86fa21044deda8751f0beaca30eb94a5a5211a83ee2","observation_id":"01d81f5f-2021-4c66-a69b-1b8c2b24e92b","resolution":{"observed_at":"2026-08-07T14:30:36.340461Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2502.06929","last_updated":"2025-07-29T21:28:38Z","snapshot_observed_at":"2026-08-09T04:36:44.066827Z","submitted_at":"2025-02-10T19:00:00Z","title":"Scalar field dark energy models: Current and forecast constraints","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2502.06929","snapshot_observed_at":"2026-08-07T14:30:36.483516Z","title":"Evolving dark energy models: Current and forecast constraints,","venue":null,"work_id":null,"year":null},"citing_paper":{"arxiv_id":"2505.18937","last_updated":"2025-07-06T08:35:15Z","snapshot_observed_at":"2026-08-17T00:57:47.634789Z","submitted_at":"2025-05-25T02:09:41Z","title":"Examining Quintessence Models with DESI Data","version":2},"reference_index":20,"source":"pdf_text","source_observed_at":"2026-08-07T14:30:36.483516Z"},"links":{"cited_paper":"/paper/2502.06929","citing_paper":"/paper/2505.18937"},"observation_digest":"sha256:3b92e744d92856b84750fae105a2d01b2fa5df5e01fb35f141449b44fb6e203b","observation_id":"bc1a6e5e-e797-4db3-b833-73822786abd3","resolution":{"observed_at":"2026-08-07T14:30:36.483516Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_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},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2502.10264","snapshot_observed_at":"2026-08-07T14:30:36.600462Z","title":"An overview of what current data can (and cannot yet) say about evolving dark energy,","venue":null,"work_id":null,"year":2025},"citing_paper":{"arxiv_id":"2505.18937","last_updated":"2025-07-06T08:35:15Z","snapshot_observed_at":"2026-08-17T00:57:47.634789Z","submitted_at":"2025-05-25T02:09:41Z","title":"Examining Quintessence Models with DESI Data","version":2},"reference_index":21,"source":"pdf_text","source_observed_at":"2026-08-07T14:30:36.600462Z"},"links":{"cited_paper":"/paper/2502.10264","citing_paper":"/paper/2505.18937"},"observation_digest":"sha256:234f330ebdfcee2999926ca17995d01e5d2729c8a96d3fd138dcff04286af46d","observation_id":"ccaffa88-dd34-4747-8448-263741739a14","resolution":{"observed_at":"2026-08-07T14:30:36.600462Z","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":"2026-08-07T14:30:36.758507Z","title":"DESI results: Hint towards coupled dark matter and dark energy,","venue":null,"work_id":null,"year":null},"citing_paper":{"arxiv_id":"2505.18937","last_updated":"2025-07-06T08:35:15Z","snapshot_observed_at":"2026-08-17T00:57:47.634789Z","submitted_at":"2025-05-25T02:09:41Z","title":"Examining Quintessence Models with DESI Data","version":2},"reference_index":22,"source":"pdf_text","source_observed_at":"2026-08-07T14:30:36.758507Z"},"links":{"citing_paper":"/paper/2505.18937"},"observation_digest":"sha256:6791c3d0bd7ff3c3404bc284da71fa1874f0d5919e9719c43703a6d09710b73c","observation_id":"6942c1c6-536c-4788-82a7-b924e080a2f9","resolution":{"observed_at":"2026-08-07T14:30:36.758507Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2503.19955","last_updated":"2025-06-29T01:33:24Z","snapshot_observed_at":"2026-08-16T12:46:53.041595Z","submitted_at":"2025-03-25T18:00:00Z","title":"How Much NEC Breaking Can the Universe Endure?","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2503.19955","snapshot_observed_at":"2026-08-07T14:30:36.869398Z","title":"How Much NEC Breaking Can the Universe En- dure?,","venue":null,"work_id":null,"year":null},"citing_paper":{"arxiv_id":"2505.18937","last_updated":"2025-07-06T08:35:15Z","snapshot_observed_at":"2026-08-17T00:57:47.634789Z","submitted_at":"2025-05-25T02:09:41Z","title":"Examining Quintessence Models with DESI Data","version":2},"reference_index":23,"source":"pdf_text","source_observed_at":"2026-08-07T14:30:36.869398Z"},"links":{"cited_paper":"/paper/2503.19955","citing_paper":"/paper/2505.18937"},"observation_digest":"sha256:9925ac408df28d446c55b89deebe713522dd8d43f79d9e95bcc5fdfaecde8058","observation_id":"ba1c752c-e054-4ab1-b855-d4d4a5cf3ae2","resolution":{"observed_at":"2026-08-07T14:30:36.869398Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2504.02028","last_updated":"2025-06-25T19:25:18Z","snapshot_observed_at":"2026-08-16T12:44:30.002542Z","submitted_at":"2025-04-02T18:00:00Z","title":"Optimal parameterizations for observational constraints on thawing dark energy","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2504.02028","snapshot_observed_at":"2026-08-07T14:30:36.968298Z","title":"Op- timal parameterizations for observational constraints on thawing dark energy,","venue":null,"work_id":null,"year":null},"citing_paper":{"arxiv_id":"2505.18937","last_updated":"2025-07-06T08:35:15Z","snapshot_observed_at":"2026-08-17T00:57:47.634789Z","submitted_at":"2025-05-25T02:09:41Z","title":"Examining Quintessence Models with DESI Data","version":2},"reference_index":24,"source":"pdf_text","source_observed_at":"2026-08-07T14:30:36.968298Z"},"links":{"cited_paper":"/paper/2504.02028","citing_paper":"/paper/2505.18937"},"observation_digest":"sha256:aa3f4ed60e9c31444c362e58d2f0e2862830ab86ea23ba19488efd4fb18c3a48","observation_id":"f2f2dc9b-efda-4c00-a789-95f414f9b268","resolution":{"observed_at":"2026-08-07T14:30:36.968298Z","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":"2026-08-07T14:30:37.075303Z","title":"Testing Quintessence Axion Dark Energy with Recent Cosmo- logical Results,","venue":null,"work_id":null,"year":null},"citing_paper":{"arxiv_id":"2505.18937","last_updated":"2025-07-06T08:35:15Z","snapshot_observed_at":"2026-08-17T00:57:47.634789Z","submitted_at":"2025-05-25T02:09:41Z","title":"Examining Quintessence Models with DESI Data","version":2},"reference_index":25,"source":"pdf_text","source_observed_at":"2026-08-07T14:30:37.075303Z"},"links":{"citing_paper":"/paper/2505.18937"},"observation_digest":"sha256:58c190ddcee31798d81c79fec8bb567993dbfe1e8c759831467bd30b4e33ebd9","observation_id":"bacd2fee-66e2-4a84-aedc-7fbef60c1019","resolution":{"observed_at":"2026-08-07T14:30:37.075303Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2505.08467","last_updated":"2025-07-28T14:02:47Z","snapshot_observed_at":"2026-08-16T02:59:28.712016Z","submitted_at":"2025-05-13T11:50:01Z","title":"The matter with(in) CPL","version":3},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2505.08467","snapshot_observed_at":"2026-08-07T14:30:37.235920Z","title":"The matter with(in) CPL,","venue":null,"work_id":null,"year":null},"citing_paper":{"arxiv_id":"2505.18937","last_updated":"2025-07-06T08:35:15Z","snapshot_observed_at":"2026-08-17T00:57:47.634789Z","submitted_at":"2025-05-25T02:09:41Z","title":"Examining Quintessence Models with DESI Data","version":2},"reference_index":26,"source":"pdf_text","source_observed_at":"2026-08-07T14:30:37.235920Z"},"links":{"cited_paper":"/paper/2505.08467","citing_paper":"/paper/2505.18937"},"observation_digest":"sha256:ebc9b069356359ea995a7933110cdad5283407b0013145a2e88fe463449b49f2","observation_id":"17ffa91f-2a60-485e-bc70-fe419bf7fe2f","resolution":{"observed_at":"2026-08-07T14:30:37.235920Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2505.10410","last_updated":"2025-07-10T10:02:08Z","snapshot_observed_at":"2026-08-15T23:37:49.060886Z","submitted_at":"2025-05-15T15:31:18Z","title":"Phantom matters","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2505.10410","snapshot_observed_at":"2026-08-07T14:30:37.350456Z","title":"Phantom matters,","venue":null,"work_id":null,"year":null},"citing_paper":{"arxiv_id":"2505.18937","last_updated":"2025-07-06T08:35:15Z","snapshot_observed_at":"2026-08-17T00:57:47.634789Z","submitted_at":"2025-05-25T02:09:41Z","title":"Examining Quintessence Models with DESI Data","version":2},"reference_index":27,"source":"pdf_text","source_observed_at":"2026-08-07T14:30:37.350456Z"},"links":{"cited_paper":"/paper/2505.10410","citing_paper":"/paper/2505.18937"},"observation_digest":"sha256:de9263b429f8a2eff00676e0ead506e24d72aa99e1de3b5f5467d6542b828a77","observation_id":"c7ac82bf-48f5-4538-80cb-537ae1cee2af","resolution":{"observed_at":"2026-08-07T14:30:37.350456Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_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},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2502.04929","snapshot_observed_at":"2026-08-07T14:30:37.452029Z","title":"Robustness of dark energy phenomenology across different parameterizations,","venue":null,"work_id":null,"year":2025},"citing_paper":{"arxiv_id":"2505.18937","last_updated":"2025-07-06T08:35:15Z","snapshot_observed_at":"2026-08-17T00:57:47.634789Z","submitted_at":"2025-05-25T02:09:41Z","title":"Examining Quintessence Models with DESI Data","version":2},"reference_index":28,"source":"pdf_text","source_observed_at":"2026-08-07T14:30:37.452029Z"},"links":{"cited_paper":"/paper/2502.04929","citing_paper":"/paper/2505.18937"},"observation_digest":"sha256:64be5b44e7ad26abdf1036ceabc148d64295d3f5988548b1b91802436512f17c","observation_id":"a0b519c6-e073-4d43-86e7-96ae5658bc09","resolution":{"observed_at":"2026-08-07T14:30:37.452029Z","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":"2026-08-16T13:15:27.455064Z","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":"2026-08-07T14:30:37.533728Z","title":"Match- ing current observational constraints with nonminimally coupled dark energy,","venue":null,"work_id":null,"year":2025},"citing_paper":{"arxiv_id":"2505.18937","last_updated":"2025-07-06T08:35:15Z","snapshot_observed_at":"2026-08-17T00:57:47.634789Z","submitted_at":"2025-05-25T02:09:41Z","title":"Examining Quintessence Models with DESI Data","version":2},"reference_index":29,"source":"pdf_text","source_observed_at":"2026-08-07T14:30:37.533728Z"},"links":{"cited_paper":"/paper/2409.17019","citing_paper":"/paper/2505.18937"},"observation_digest":"sha256:f5c2dc0d4016bcd0d67d65b8345c0c1a565c59ee0371de35b8e7f1194c6c2d13","observation_id":"a70476c8-8b78-443c-8bf0-9163e2b4dcda","resolution":{"observed_at":"2026-08-07T14:30:37.533728Z","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":"2026-08-07T14:30:37.607411Z","title":"Roy Choudhury and T","venue":null,"work_id":null,"year":2024},"citing_paper":{"arxiv_id":"2505.18937","last_updated":"2025-07-06T08:35:15Z","snapshot_observed_at":"2026-08-17T00:57:47.634789Z","submitted_at":"2025-05-25T02:09:41Z","title":"Examining Quintessence Models with DESI Data","version":2},"reference_index":30,"source":"pdf_text","source_observed_at":"2026-08-07T14:30:37.607411Z"},"links":{"cited_paper":"/paper/2409.13022","citing_paper":"/paper/2505.18937"},"observation_digest":"sha256:a43bdf87f559b6f57a7f3c3e6b975901ae80437f3e84ce6b47d172fac342e5b1","observation_id":"d9b66e80-3320-4ebe-842e-0af6fce73b7b","resolution":{"observed_at":"2026-08-07T14:30:37.607411Z","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":"2026-08-07T14:30:37.680350Z","title":null,"venue":null,"work_id":null,"year":null},"citing_paper":{"arxiv_id":"2505.18937","last_updated":"2025-07-06T08:35:15Z","snapshot_observed_at":"2026-08-17T00:57:47.634789Z","submitted_at":"2025-05-25T02:09:41Z","title":"Examining Quintessence Models with DESI Data","version":2},"reference_index":31,"source":"pdf_text","source_observed_at":"2026-08-07T14:30:37.680350Z"},"links":{"citing_paper":"/paper/2505.18937"},"observation_digest":"sha256:3efdf2ad1ca517b18e8c1377d9a4c9ccc0f62006acb892061fb0b911af84b015","observation_id":"13b0dc07-8e66-40d6-bb74-513ecccec118","resolution":{"observed_at":"2026-08-07T14:30:37.680350Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2504.20664","last_updated":"2025-08-15T13:21:18Z","snapshot_observed_at":"2026-08-16T10:58:29.999626Z","submitted_at":"2025-04-29T11:38:28Z","title":"Challenging $\\Lambda$CDM: 5$\\sigma$ Evidence for a Dynamical Dark Energy Late-Time Transition","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2504.20664","snapshot_observed_at":"2026-08-07T14:30:37.774331Z","title":"Challenging ΛCDM: 5σ Evidence for a Dynamical Dark Energy Late-Time Transition,","venue":null,"work_id":null,"year":null},"citing_paper":{"arxiv_id":"2505.18937","last_updated":"2025-07-06T08:35:15Z","snapshot_observed_at":"2026-08-17T00:57:47.634789Z","submitted_at":"2025-05-25T02:09:41Z","title":"Examining Quintessence Models with DESI Data","version":2},"reference_index":32,"source":"pdf_text","source_observed_at":"2026-08-07T14:30:37.774331Z"},"links":{"cited_paper":"/paper/2504.20664","citing_paper":"/paper/2505.18937"},"observation_digest":"sha256:23af9b4311458694fdfe4ccb5ca26852a3e0083939e792e1948fd14409a2871c","observation_id":"1ac92414-96b4-4bd7-b50c-f61f46bcea58","resolution":{"observed_at":"2026-08-07T14:30:37.774331Z","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":"2026-08-16T13:48:56.676752Z","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":"2026-08-07T14:30:37.846348Z","title":"Cos- mological constraints on curved quintessence,","venue":null,"work_id":null,"year":2024},"citing_paper":{"arxiv_id":"2505.18937","last_updated":"2025-07-06T08:35:15Z","snapshot_observed_at":"2026-08-17T00:57:47.634789Z","submitted_at":"2025-05-25T02:09:41Z","title":"Examining Quintessence Models with DESI Data","version":2},"reference_index":33,"source":"pdf_text","source_observed_at":"2026-08-07T14:30:37.846348Z"},"links":{"cited_paper":"/paper/2405.17396","citing_paper":"/paper/2505.18937"},"observation_digest":"sha256:c60a4b95c9af22c4fb60b47334efb237e8ba5144bc787f3f27c3484213e81c88","observation_id":"1a41dd36-c790-4e2a-8faf-c970d19f1bf0","resolution":{"observed_at":"2026-08-07T14:30:37.846348Z","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":"2026-08-07T14:30:37.896981Z","title":"Cos- mological tests of quintessence in quantum gravity,","venue":null,"work_id":null,"year":2025},"citing_paper":{"arxiv_id":"2505.18937","last_updated":"2025-07-06T08:35:15Z","snapshot_observed_at":"2026-08-17T00:57:47.634789Z","submitted_at":"2025-05-25T02:09:41Z","title":"Examining Quintessence Models with DESI Data","version":2},"reference_index":34,"source":"pdf_text","source_observed_at":"2026-08-07T14:30:37.896981Z"},"links":{"citing_paper":"/paper/2505.18937"},"observation_digest":"sha256:12893985f12b3397059ecb939b829362ae13881eb19a17b95dd7921ff1ef2192","observation_id":"069926ae-e5b9-4504-8c04-25c95ecd9f21","resolution":{"observed_at":"2026-08-07T14:30:37.896981Z","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":"2026-08-07T14:30:37.960408Z","title":"Pressure Parametrization of Dark En- ergy: First and Second-Order Constraints with Latest Cosmological Data,","venue":null,"work_id":null,"year":null},"citing_paper":{"arxiv_id":"2505.18937","last_updated":"2025-07-06T08:35:15Z","snapshot_observed_at":"2026-08-17T00:57:47.634789Z","submitted_at":"2025-05-25T02:09:41Z","title":"Examining Quintessence Models with DESI Data","version":2},"reference_index":35,"source":"pdf_text","source_observed_at":"2026-08-07T14:30:37.960408Z"},"links":{"citing_paper":"/paper/2505.18937"},"observation_digest":"sha256:285751acf09fb9a47ee90dce6ce7f6b3b6ad663a1ba4b5b6b0af5430f890b846","observation_id":"65404cbb-c113-459a-a82e-6682c695e67c","resolution":{"observed_at":"2026-08-07T14:30:37.960408Z","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":"2026-08-07T14:30:38.020409Z","title":"DESI DR2 Results II: Measurements of Baryon Acoustic Oscillations and Cosmological Constraints,","venue":null,"work_id":null,"year":null},"citing_paper":{"arxiv_id":"2505.18937","last_updated":"2025-07-06T08:35:15Z","snapshot_observed_at":"2026-08-17T00:57:47.634789Z","submitted_at":"2025-05-25T02:09:41Z","title":"Examining Quintessence Models with DESI Data","version":2},"reference_index":36,"source":"pdf_text","source_observed_at":"2026-08-07T14:30:38.020409Z"},"links":{"cited_paper":"/paper/2503.14738","citing_paper":"/paper/2505.18937"},"observation_digest":"sha256:52d987d1e274d09cc6de29d3b3bad84b642902044d5f75cacb91d71dcc7758f0","observation_id":"8c7f9c9b-36b4-477e-841c-3d317fbde7e8","resolution":{"observed_at":"2026-08-07T14:30:38.020409Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}}],"paper":{"arxiv_id":"2505.18937","last_updated":"2025-07-06T08:35:15Z","latest_version":2,"primary_category":"astro-ph.CO","snapshot_observed_at":"2026-08-17T00:57:47.634789Z","submitted_at":"2025-05-25T02:09:41Z","title":"Examining Quintessence Models with DESI Data"},"reference_resolution":{"displayed":36,"state_counts":{"malformed_identifier":2,"metadata_mismatch":0,"parse_uncertain":0,"unresolved":34,"verified_exact":0,"verified_fuzzy":0},"total_outbound_references":36},"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":"2026-08-16T06:30:59.297886+00:00","source":"crossref"},{"observed_at":"2026-08-16T06:30:54.164669+00:00","source":"retraction_watch"}],"thesis":"As of 17 August 2026, this Paper Citation Record lists 36 of 36 outbound references and 19 inbound Pith citation observations for arXiv:2505.18937."}