{"as_of":"2026-08-21T04:59:00Z","caps":{"database_statements":6,"inbound":100,"outbound":100},"context_digest":"sha256:55330f42cce905347ee6a50838658cdb69b0a3156020ccec16bbfe18c0e18bf8","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":67,"lane":"standing_notices","note":"One-hop event checks from named stored sources.","records_observed":67,"source":"scholarly_work_events, retraction_status_cache","source_observed_at":"2026-08-20T06:33:59.587034+00:00","state":"measured"},{"denominator":67,"lane":"inbound_itemization","note":"Pith citing papers itemized under the disclosed page cap.","records_observed":67,"source":"paper_references, paper_reference_links","source_observed_at":"2026-08-16T11:53:56.129167Z","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":"2026-07-09T13:46:17.479123Z","state":"measured"}],"external_citation_measurements":[],"inbound":[{"citation":{"cited_paper":{"arxiv_id":"2404.15232","last_updated":"2024-12-19T16:25:49Z","snapshot_observed_at":"2026-08-16T13:58:27.312344Z","submitted_at":"2024-04-23T17:05:14Z","title":"Interacting Dark Energy after DESI Baryon Acoustic Oscillation measurements","version":2},"cited_work":{"arxiv_id":"2404.15232","doi":null,"metadata_source":"pith","pith_arxiv_id":"2404.15232","snapshot_observed_at":"2026-07-09T13:46:17.479123Z","title":"Giar` e, M","venue":"astro-ph.CO","work_id":"5be9e1ba-8076-41a9-b994-919073086747","year":2024},"citing_paper":{"arxiv_id":"2402.07716","last_updated":"2026-04-28T16:55:09Z","snapshot_observed_at":"2026-07-06T02:11:23.670680Z","submitted_at":"2024-02-12T15:29:10Z","title":"$\\Lambda_{\\rm s}$CDM cosmology from a type-II minimally modified gravity","version":3},"reference_index":137,"source":"pdf_text","source_observed_at":"2026-05-24T03:50:50.435997Z"},"links":{"cited_paper":"/paper/2404.15232","citing_paper":"/paper/2402.07716"},"observation_digest":"sha256:cd574c52a77273c1fd42d4e81e2cae8d7b4994210e882157452725f1e076f4f9","observation_id":"4d25b231-2b9d-4c25-b27e-fad1add89644","resolution":{"observed_at":"2026-05-24T03:53:54.441637Z","resolver_source":"arxiv_id","status":"verified_exact"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-20T06:33:59.587034+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-20T06:33:59.587034+00:00","source":"crossref"},{"observed_at":"2026-08-20T06:33:54.927442+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":{"arxiv_id":"2404.15232","last_updated":"2024-12-19T16:25:49Z","snapshot_observed_at":"2026-08-16T13:58:27.312344Z","submitted_at":"2024-04-23T17:05:14Z","title":"Interacting Dark Energy after DESI Baryon Acoustic Oscillation measurements","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2404.15232","snapshot_observed_at":"2026-08-12T15:32:30.564091Z","title":"Interacting Dark Energy after DESI Baryon Acoustic Oscillation measurements,","venue":null,"work_id":null,"year":2024},"citing_paper":{"arxiv_id":"2411.14189","last_updated":"2024-11-21T14:58:40Z","snapshot_observed_at":"2026-08-14T16:11:56.146618Z","submitted_at":"2024-11-21T14:58:40Z","title":"Reevaluating $H_0$ Tension with Non-Planck CMB and DESI BAO Joint Analysis","version":1},"reference_index":21,"source":"pdf_text","source_observed_at":"2026-08-12T15:32:30.564091Z"},"links":{"cited_paper":"/paper/2404.15232","citing_paper":"/paper/2411.14189"},"observation_digest":"sha256:dfab2880ca81690e3a4f5e56af09bb18a9b631a2a56e6a29d5f4283081194790","observation_id":"7fed6e95-d5c9-4619-a316-ac6a9c0ae3ff","resolution":{"observed_at":"2026-08-12T15:32:30.564091Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2404.15232","last_updated":"2024-12-19T16:25:49Z","snapshot_observed_at":"2026-08-16T13:58:27.312344Z","submitted_at":"2024-04-23T17:05:14Z","title":"Interacting Dark Energy after DESI Baryon Acoustic Oscillation measurements","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2404.15232","snapshot_observed_at":"2026-08-12T13:51:30.398043Z","title":"Giarè, M.A","venue":null,"work_id":null,"year":null},"citing_paper":{"arxiv_id":"2411.15892","last_updated":"2025-03-08T21:28:55Z","snapshot_observed_at":"2026-08-19T05:44:12.305320Z","submitted_at":"2024-11-24T16:02:11Z","title":"General parametrization for energy density of quintessence field","version":2},"reference_index":15,"source":"pdf_text","source_observed_at":"2026-08-12T13:51:30.398043Z"},"links":{"cited_paper":"/paper/2404.15232","citing_paper":"/paper/2411.15892"},"observation_digest":"sha256:ad929a29eddd259e21cfc4d5c518c53e180619066ea49f27ae3545ca37d95461","observation_id":"0895ca74-f2dd-409c-83be-040742e07c61","resolution":{"observed_at":"2026-08-12T13:51:30.398043Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2404.15232","last_updated":"2024-12-19T16:25:49Z","snapshot_observed_at":"2026-08-16T13:58:27.312344Z","submitted_at":"2024-04-23T17:05:14Z","title":"Interacting Dark Energy after DESI Baryon Acoustic Oscillation measurements","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2404.15232","snapshot_observed_at":"2026-08-12T11:29:07.801749Z","title":"Giar` e, M","venue":null,"work_id":null,"year":2024},"citing_paper":{"arxiv_id":"2411.18300","last_updated":"2025-07-10T15:45:02Z","snapshot_observed_at":"2026-08-20T17:26:15.055500Z","submitted_at":"2024-11-27T12:47:00Z","title":"Interacting phantom dark energy: new accelerating scaling attractors","version":2},"reference_index":99,"source":"pdf_text","source_observed_at":"2026-08-12T11:29:07.801749Z"},"links":{"cited_paper":"/paper/2404.15232","citing_paper":"/paper/2411.18300"},"observation_digest":"sha256:d88c92379055e3907bc0c2bd0c5541bab83454228861c19447e36d40d31feaea","observation_id":"0f7892e2-7912-4693-8980-cb97daa23086","resolution":{"observed_at":"2026-08-12T11:29:07.801749Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2404.15232","last_updated":"2024-12-19T16:25:49Z","snapshot_observed_at":"2026-08-16T13:58:27.312344Z","submitted_at":"2024-04-23T17:05:14Z","title":"Interacting Dark Energy after DESI Baryon Acoustic Oscillation measurements","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2404.15232","snapshot_observed_at":"2026-08-12T10:22:40.398627Z","title":"Sabogal, Rafael C","venue":null,"work_id":null,"year":2024},"citing_paper":{"arxiv_id":"2411.19362","last_updated":"2025-08-20T17:11:12Z","snapshot_observed_at":"2026-08-17T04:57:14.460052Z","submitted_at":"2024-11-28T20:18:13Z","title":"A preference for dynamical phantom dark energy using one-parameter model with Planck, DESI DR1 BAO and SN data","version":2},"reference_index":39,"source":"pdf_text","source_observed_at":"2026-08-12T10:22:40.398627Z"},"links":{"cited_paper":"/paper/2404.15232","citing_paper":"/paper/2411.19362"},"observation_digest":"sha256:6c165936e7adf4ac74a8fc3b8d3b23ec4bcb70046a4497cdf02d8a5e831f40ab","observation_id":"d3a32705-cf95-4337-b643-36894cbc82f2","resolution":{"observed_at":"2026-08-12T10:22:40.398627Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2404.15232","last_updated":"2024-12-19T16:25:49Z","snapshot_observed_at":"2026-08-16T13:58:27.312344Z","submitted_at":"2024-04-23T17:05:14Z","title":"Interacting Dark Energy after DESI Baryon Acoustic Oscillation measurements","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2404.15232","snapshot_observed_at":"2026-08-11T13:41:23.820821Z","title":"Giar `e, M","venue":null,"work_id":null,"year":2024},"citing_paper":{"arxiv_id":"2412.12905","last_updated":"2025-01-25T08:30:04Z","snapshot_observed_at":"2026-08-17T16:16:24.002443Z","submitted_at":"2024-12-17T13:31:15Z","title":"DESI and SNe: Dynamical Dark Energy, $\\Omega_m$ Tension or Systematics?","version":2},"reference_index":70,"source":"pdf_text","source_observed_at":"2026-08-11T13:41:23.820821Z"},"links":{"cited_paper":"/paper/2404.15232","citing_paper":"/paper/2412.12905"},"observation_digest":"sha256:1b1228615ed53cb77a51226f9a5050ab49c9a2ccf8d63c2842f9bbb7c0b8d981","observation_id":"e558c932-1e8f-4f76-8e9f-f796da7e45a9","resolution":{"observed_at":"2026-08-11T13:41:23.820821Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2404.15232","last_updated":"2024-12-19T16:25:49Z","snapshot_observed_at":"2026-08-16T13:58:27.312344Z","submitted_at":"2024-04-23T17:05:14Z","title":"Interacting Dark Energy after DESI Baryon Acoustic Oscillation measurements","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2404.15232","snapshot_observed_at":"2026-08-11T13:36:50.257771Z","title":"L., Madore, B","venue":null,"work_id":null,"year":2020},"citing_paper":{"arxiv_id":"2412.13045","last_updated":"2024-12-17T16:10:28Z","snapshot_observed_at":"2026-08-17T21:52:41.868349Z","submitted_at":"2024-12-17T16:10:28Z","title":"Newest measurements of Hubble constant from DESI 2024 BAO observations","version":1},"reference_index":17,"source":"pdf_text","source_observed_at":"2026-08-11T13:36:50.257771Z"},"links":{"cited_paper":"/paper/2404.15232","citing_paper":"/paper/2412.13045"},"observation_digest":"sha256:d6ccd3d00003bc2e5bb835ca3bd80994071f878d43c09183deaefa75d510e9c9","observation_id":"5ebfb583-0a98-41c9-b7d8-bfd438cb0ddb","resolution":{"observed_at":"2026-08-11T13:36:50.257771Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2404.15232","last_updated":"2024-12-19T16:25:49Z","snapshot_observed_at":"2026-08-16T13:58:27.312344Z","submitted_at":"2024-04-23T17:05:14Z","title":"Interacting Dark Energy after DESI Baryon Acoustic Oscillation measurements","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2404.15232","snapshot_observed_at":"2026-08-11T12:34:38.215553Z","title":"Giar` e, M","venue":null,"work_id":null,"year":2024},"citing_paper":{"arxiv_id":"2412.14139","last_updated":"2024-12-18T18:37:30Z","snapshot_observed_at":"2026-08-17T16:13:00.025774Z","submitted_at":"2024-12-18T18:37:30Z","title":"Alleviating cosmological tensions with a hybrid dark sector","version":1},"reference_index":36,"source":"pdf_text","source_observed_at":"2026-08-11T12:34:38.215553Z"},"links":{"cited_paper":"/paper/2404.15232","citing_paper":"/paper/2412.14139"},"observation_digest":"sha256:ff2a7a71b6833beed8035829ddb6a0a260764a08c554314ed8a2f3757cdfa241","observation_id":"cde4490a-37f3-4a03-b20f-69ccb7cbdcfc","resolution":{"observed_at":"2026-08-11T12:34:38.215553Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2404.15232","last_updated":"2024-12-19T16:25:49Z","snapshot_observed_at":"2026-08-16T13:58:27.312344Z","submitted_at":"2024-04-23T17:05:14Z","title":"Interacting Dark Energy after DESI Baryon Acoustic Oscillation measurements","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2404.15232","snapshot_observed_at":"2026-08-11T12:25:17.494856Z","title":"Giar` e, M","venue":null,"work_id":null,"year":2024},"citing_paper":{"arxiv_id":"2412.14290","last_updated":"2024-12-18T19:31:08Z","snapshot_observed_at":"2026-08-18T19:21:58.010798Z","submitted_at":"2024-12-18T19:31:08Z","title":"Impact of DESI BAO Data on Inflationary Parameters: stability against late-time new physics","version":1},"reference_index":46,"source":"pdf_text","source_observed_at":"2026-08-11T12:25:17.494856Z"},"links":{"cited_paper":"/paper/2404.15232","citing_paper":"/paper/2412.14290"},"observation_digest":"sha256:a7c7c9543a6f3bc3e9026ffeaf6a7490f3788b9e3021f37fadece1f78111e89f","observation_id":"a20f11fc-2f71-4b70-ac97-3af24602d177","resolution":{"observed_at":"2026-08-11T12:25:17.494856Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2404.15232","last_updated":"2024-12-19T16:25:49Z","snapshot_observed_at":"2026-08-16T13:58:27.312344Z","submitted_at":"2024-04-23T17:05:14Z","title":"Interacting Dark Energy after DESI Baryon Acoustic Oscillation measurements","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2404.15232","snapshot_observed_at":"2026-08-10T19:20:17.183204Z","title":"Giar` e, M","venue":null,"work_id":null,"year":2024},"citing_paper":{"arxiv_id":"2501.10323","last_updated":"2025-02-24T12:41:54Z","snapshot_observed_at":"2026-08-19T21:21:05.354025Z","submitted_at":"2025-01-17T17:52:49Z","title":"Sign Switching in Dark Sector Coupling Interactions as a Candidate for Resolving Cosmological Tensions","version":2},"reference_index":137,"source":"pdf_text","source_observed_at":"2026-08-10T19:20:17.183204Z"},"links":{"cited_paper":"/paper/2404.15232","citing_paper":"/paper/2501.10323"},"observation_digest":"sha256:aca5d2038fd566a5d15b9e176ef943a128af022fffef39a508f125aebba90c72","observation_id":"c5d2e94d-ae66-484d-aa51-7776e8400401","resolution":{"observed_at":"2026-08-10T19:20:17.183204Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2404.15232","last_updated":"2024-12-19T16:25:49Z","snapshot_observed_at":"2026-08-16T13:58:27.312344Z","submitted_at":"2024-04-23T17:05:14Z","title":"Interacting Dark Energy after DESI Baryon Acoustic Oscillation measurements","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2404.15232","snapshot_observed_at":"2026-08-10T14:29:27.452166Z","title":"Giar` e, M","venue":null,"work_id":null,"year":2024},"citing_paper":{"arxiv_id":"2501.15298","last_updated":"2025-04-12T08:58:51Z","snapshot_observed_at":"2026-08-14T12:45:12.698388Z","submitted_at":"2025-01-25T18:30:04Z","title":"Scalar-Tensor Gravity and DESI 2024 BAO data","version":2},"reference_index":25,"source":"pdf_text","source_observed_at":"2026-08-10T14:29:27.452166Z"},"links":{"cited_paper":"/paper/2404.15232","citing_paper":"/paper/2501.15298"},"observation_digest":"sha256:d517e8298ca0b54b991af5a71ffa721b8d1dd1b080f2686527a720aa54340e52","observation_id":"123a2d88-93e6-46fc-acee-76d1474a18f2","resolution":{"observed_at":"2026-08-10T14:29:27.452166Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2404.15232","last_updated":"2024-12-19T16:25:49Z","snapshot_observed_at":"2026-08-16T13:58:27.312344Z","submitted_at":"2024-04-23T17:05:14Z","title":"Interacting Dark Energy after DESI Baryon Acoustic Oscillation measurements","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2404.15232","snapshot_observed_at":"2026-08-08T23:12:26.069386Z","title":"Interacting Dark Energy after DESI Baryon Acoustic Oscillation Measurements,","venue":null,"work_id":null,"year":2024},"citing_paper":{"arxiv_id":"2502.04212","last_updated":"2025-07-17T16:27:03Z","snapshot_observed_at":"2026-08-18T11:01:42.213182Z","submitted_at":"2025-02-06T16:51:39Z","title":"The DESI DR1/DR2 evidence for dynamical dark energy is biased by low-redshift supernovae","version":5},"reference_index":35,"source":"pdf_text","source_observed_at":"2026-08-08T23:12:26.069386Z"},"links":{"cited_paper":"/paper/2404.15232","citing_paper":"/paper/2502.04212"},"observation_digest":"sha256:7ccee8e0bd1efee528e4ed8aff0d460a02822b15f982f7a191e1ac4e0f371091","observation_id":"8ac42b03-5561-4f83-b4b5-17e07998f0f0","resolution":{"observed_at":"2026-08-08T23:12:26.069386Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2404.15232","last_updated":"2024-12-19T16:25:49Z","snapshot_observed_at":"2026-08-16T13:58:27.312344Z","submitted_at":"2024-04-23T17:05:14Z","title":"Interacting Dark Energy after DESI Baryon Acoustic Oscillation measurements","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2404.15232","snapshot_observed_at":"2026-08-08T22:04:59.460838Z","title":"Giar` e, M","venue":null,"work_id":null,"year":2024},"citing_paper":{"arxiv_id":"2502.04641","last_updated":"2025-02-18T07:50:34Z","snapshot_observed_at":"2026-08-20T20:02:20.505719Z","submitted_at":"2025-02-07T03:58:52Z","title":"Dark energy and lensing anomaly in Planck CMB data","version":2},"reference_index":37,"source":"pdf_text","source_observed_at":"2026-08-08T22:04:59.460838Z"},"links":{"cited_paper":"/paper/2404.15232","citing_paper":"/paper/2502.04641"},"observation_digest":"sha256:1b9d66c9fe886cd90f90d9aaf0139ec92abfc623ee707498be29ad7186b62b3f","observation_id":"362dd013-d112-4da6-8eec-5249eb2bb7cb","resolution":{"observed_at":"2026-08-08T22:04:59.460838Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2404.15232","last_updated":"2024-12-19T16:25:49Z","snapshot_observed_at":"2026-08-16T13:58:27.312344Z","submitted_at":"2024-04-23T17:05:14Z","title":"Interacting Dark Energy after DESI Baryon Acoustic Oscillation measurements","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2404.15232","snapshot_observed_at":"2026-08-08T21:04:17.981748Z","title":"Giarè, M.A","venue":null,"work_id":null,"year":2024},"citing_paper":{"arxiv_id":"2502.04929","last_updated":"2025-05-14T14:57:09Z","snapshot_observed_at":"2026-08-08T20:55:05.610325Z","submitted_at":"2025-02-07T13:49:14Z","title":"Robustness of dark energy phenomenology across different parameterizations","version":3},"reference_index":129,"source":"pdf_text","source_observed_at":"2026-08-08T21:04:17.981748Z"},"links":{"cited_paper":"/paper/2404.15232","citing_paper":"/paper/2502.04929"},"observation_digest":"sha256:9e7f3d93f958ee083a5ed8eb5ba4dcca06237e4caec1590a34bddd6b538e00d7","observation_id":"fc3788b4-a960-44ed-9aa3-1abca5b43738","resolution":{"observed_at":"2026-08-08T21:04:17.981748Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2404.15232","last_updated":"2024-12-19T16:25:49Z","snapshot_observed_at":"2026-08-16T13:58:27.312344Z","submitted_at":"2024-04-23T17:05:14Z","title":"Interacting Dark Energy after DESI Baryon Acoustic Oscillation measurements","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2404.15232","snapshot_observed_at":"2026-08-08T12:50:18.002599Z","title":"title Interacting Dark Energy after DESI Baryon Acoustic Oscillation measurements 2404.15232","venue":null,"work_id":null,"year":2024},"citing_paper":{"arxiv_id":"2502.07437","last_updated":"2025-02-11T10:25:50Z","snapshot_observed_at":"2026-08-15T05:05:46.129855Z","submitted_at":"2025-02-11T10:25:50Z","title":"Modified theories of gravity at different curvature scales","version":1},"reference_index":231,"source":"arxiv_source","source_observed_at":"2026-08-08T12:50:18.002599Z"},"links":{"cited_paper":"/paper/2404.15232","citing_paper":"/paper/2502.07437"},"observation_digest":"sha256:869525d8181a55dedfd7c70f02976e9d5e9856ec02929de6272ce909402fcc4b","observation_id":"c4bd085a-e72f-49b3-9712-c05afb87a53c","resolution":{"observed_at":"2026-08-08T12:50:18.002599Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2404.15232","last_updated":"2024-12-19T16:25:49Z","snapshot_observed_at":"2026-08-16T13:58:27.312344Z","submitted_at":"2024-04-23T17:05:14Z","title":"Interacting Dark Energy after DESI Baryon Acoustic Oscillation measurements","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2404.15232","snapshot_observed_at":"2026-08-07T18:51:43.685319Z","title":"Interacting Dark Energy after DESI Baryon Acoustic Oscillation Measurements,","venue":null,"work_id":null,"year":2024},"citing_paper":{"arxiv_id":"2502.10264","last_updated":"2025-04-10T17:38:46Z","snapshot_observed_at":"2026-08-19T21:36:29.298768Z","submitted_at":"2025-02-14T16:17:23Z","title":"An overview of what current data can (and cannot yet) say about evolving dark energy","version":2},"reference_index":115,"source":"pdf_text","source_observed_at":"2026-08-07T18:51:43.685319Z"},"links":{"cited_paper":"/paper/2404.15232","citing_paper":"/paper/2502.10264"},"observation_digest":"sha256:da2243ad580da639dffee73890c8e0cb51fcbb4fe04f22808db02528f899b7fa","observation_id":"63b3be25-dfe2-4e88-aac5-a8dcc46322c9","resolution":{"observed_at":"2026-08-07T18:51:43.685319Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2404.15232","last_updated":"2024-12-19T16:25:49Z","snapshot_observed_at":"2026-08-16T13:58:27.312344Z","submitted_at":"2024-04-23T17:05:14Z","title":"Interacting Dark Energy after DESI Baryon Acoustic Oscillation measurements","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2404.15232","snapshot_observed_at":"2026-08-16T11:53:56.129167Z","title":"Interacting Dark Energy after DESI Baryon Acoustic Oscillation Measurements,","venue":null,"work_id":null,"year":2024},"citing_paper":{"arxiv_id":"2504.14419","last_updated":"2025-04-19T23:02:02Z","snapshot_observed_at":"2026-08-18T02:53:15.611835Z","submitted_at":"2025-04-19T23:02:02Z","title":"Evidence for non-cold dark matter from DESI DR2 measurements","version":1},"reference_index":103,"source":"pdf_text","source_observed_at":"2026-08-16T11:53:56.129167Z"},"links":{"cited_paper":"/paper/2404.15232","citing_paper":"/paper/2504.14419"},"observation_digest":"sha256:834c269949d5f4e59a05d2467d481bece41206e47659902f90a5c329d26e1315","observation_id":"32f0d96d-091d-49b4-b17a-3935f189ec2e","resolution":{"observed_at":"2026-08-16T11:53:56.129167Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2404.15232","last_updated":"2024-12-19T16:25:49Z","snapshot_observed_at":"2026-08-16T13:58:27.312344Z","submitted_at":"2024-04-23T17:05:14Z","title":"Interacting Dark Energy after DESI Baryon Acoustic Oscillation measurements","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2404.15232","snapshot_observed_at":"2026-08-15T23:39:45.623021Z","title":"Giarè, M","venue":null,"work_id":null,"year":2024},"citing_paper":{"arxiv_id":"2505.04336","last_updated":"2025-07-23T19:10:27Z","snapshot_observed_at":"2026-08-17T21:26:13.566598Z","submitted_at":"2025-05-07T11:33:48Z","title":"In search of an interaction in the dark sector through Gaussian Process and ANN approaches","version":2},"reference_index":44,"source":"pdf_text","source_observed_at":"2026-08-15T23:39:45.623021Z"},"links":{"cited_paper":"/paper/2404.15232","citing_paper":"/paper/2505.04336"},"observation_digest":"sha256:4efa414d4108a7d4116488ee38dd9a7db2f399fcb46d0d7b4ba8fb043cf5ffea","observation_id":"ea9e50a2-7316-46a0-8ea9-aca3b3261679","resolution":{"observed_at":"2026-08-15T23:39:45.623021Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2404.15232","last_updated":"2024-12-19T16:25:49Z","snapshot_observed_at":"2026-08-16T13:58:27.312344Z","submitted_at":"2024-04-23T17:05:14Z","title":"Interacting Dark Energy after DESI Baryon Acoustic Oscillation measurements","version":2},"cited_work":{"arxiv_id":"2404.15232","doi":null,"metadata_source":"pith","pith_arxiv_id":"2404.15232","snapshot_observed_at":"2026-07-09T13:46:17.479123Z","title":"Giar` e, M","venue":"astro-ph.CO","work_id":"5be9e1ba-8076-41a9-b994-919073086747","year":2024},"citing_paper":{"arxiv_id":"2505.24732","last_updated":"2026-04-11T09:17:44Z","snapshot_observed_at":"2026-08-15T11:15:56.688737Z","submitted_at":"2025-05-30T15:54:16Z","title":"The Quintom theory of dark energy after DESI DR2","version":3},"reference_index":101,"source":"pdf_text","source_observed_at":"2026-05-19T13:08:20.192767Z"},"links":{"cited_paper":"/paper/2404.15232","citing_paper":"/paper/2505.24732"},"observation_digest":"sha256:e927caab8b42bc080e7f0f0731c9653a722fcf3aacea1e37611f57af605c4f8a","observation_id":"2ebc9e21-554b-4185-bf14-0508fa77682b","resolution":{"observed_at":"2026-05-19T13:12:19.139647Z","resolver_source":"arxiv_id","status":"verified_exact"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-20T06:33:59.587034+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-20T06:33:59.587034+00:00","source":"crossref"},{"observed_at":"2026-08-20T06:33:54.927442+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":{"arxiv_id":"2404.15232","last_updated":"2024-12-19T16:25:49Z","snapshot_observed_at":"2026-08-16T13:58:27.312344Z","submitted_at":"2024-04-23T17:05:14Z","title":"Interacting Dark Energy after DESI Baryon Acoustic Oscillation measurements","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2404.15232","snapshot_observed_at":"2026-08-07T10:52:56.174156Z","title":"Giar` e, M","venue":null,"work_id":null,"year":null},"citing_paper":{"arxiv_id":"2506.04306","last_updated":"2025-06-04T17:51:05Z","snapshot_observed_at":"2026-08-13T10:19:27.378849Z","submitted_at":"2025-06-04T17:51:05Z","title":"Can the universe experience an AdS landscape since matter-radiation equality?","version":1},"reference_index":11,"source":"pdf_text","source_observed_at":"2026-08-07T10:52:56.174156Z"},"links":{"cited_paper":"/paper/2404.15232","citing_paper":"/paper/2506.04306"},"observation_digest":"sha256:2bc34667ba404a6805f76f8dd308ae0e872f393b96b292834f51c8acf7413758","observation_id":"bfe436a8-b94f-4bb3-97a6-17841581cb02","resolution":{"observed_at":"2026-08-07T10:52:56.174156Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2404.15232","last_updated":"2024-12-19T16:25:49Z","snapshot_observed_at":"2026-08-16T13:58:27.312344Z","submitted_at":"2024-04-23T17:05:14Z","title":"Interacting Dark Energy after DESI Baryon Acoustic Oscillation measurements","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2404.15232","snapshot_observed_at":"2026-08-06T18:14:16.137595Z","title":"Giar` e, M","venue":null,"work_id":null,"year":2024},"citing_paper":{"arxiv_id":"2507.09258","last_updated":"2025-07-12T11:35:53Z","snapshot_observed_at":"2026-08-13T11:10:19.237636Z","submitted_at":"2025-07-12T11:35:53Z","title":"Solving an Interacting Quintessence Model with a Sound Horizon Initial Condition and its Observational Constraints","version":1},"reference_index":87,"source":"pdf_text","source_observed_at":"2026-08-06T18:14:16.137595Z"},"links":{"cited_paper":"/paper/2404.15232","citing_paper":"/paper/2507.09258"},"observation_digest":"sha256:7ae1775b7da174c6c622df80739609a07d8177de27bc0cc0f86481ee7a67fb4c","observation_id":"26b9c956-a1ef-4d7e-8cf3-5e2644f9f1c6","resolution":{"observed_at":"2026-08-06T18:14:16.137595Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2404.15232","last_updated":"2024-12-19T16:25:49Z","snapshot_observed_at":"2026-08-16T13:58:27.312344Z","submitted_at":"2024-04-23T17:05:14Z","title":"Interacting Dark Energy after DESI Baryon Acoustic Oscillation measurements","version":2},"cited_work":{"arxiv_id":"2404.15232","doi":null,"metadata_source":"pith","pith_arxiv_id":"2404.15232","snapshot_observed_at":"2026-07-09T13:46:17.479123Z","title":"Giar` e, M","venue":"astro-ph.CO","work_id":"5be9e1ba-8076-41a9-b994-919073086747","year":2024},"citing_paper":{"arxiv_id":"2507.09981","last_updated":"2026-05-06T01:55:59Z","snapshot_observed_at":"2026-08-15T02:07:33.193429Z","submitted_at":"2025-07-14T06:55:37Z","title":"New Insights into Dark Energy from DESI DR2 with CMB and SNIa","version":2},"reference_index":24,"source":"pdf_text","source_observed_at":"2026-05-19T05:19:08.520262Z"},"links":{"cited_paper":"/paper/2404.15232","citing_paper":"/paper/2507.09981"},"observation_digest":"sha256:57859c2ce97a3c12a46178bb907b2ad5d2af05c1574c4e21f3e9d41e64d9d149","observation_id":"909b5787-d89a-43d9-8302-917e2c38d826","resolution":{"observed_at":"2026-05-19T05:22:05.887625Z","resolver_source":"arxiv_id","status":"verified_exact"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-20T06:33:59.587034+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-20T06:33:59.587034+00:00","source":"crossref"},{"observed_at":"2026-08-20T06:33:54.927442+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":{"arxiv_id":"2404.15232","last_updated":"2024-12-19T16:25:49Z","snapshot_observed_at":"2026-08-16T13:58:27.312344Z","submitted_at":"2024-04-23T17:05:14Z","title":"Interacting Dark Energy after DESI Baryon Acoustic Oscillation measurements","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2404.15232","snapshot_observed_at":"2026-08-06T15:36:19.609471Z","title":"Giar` e, M","venue":null,"work_id":null,"year":2024},"citing_paper":{"arxiv_id":"2507.15575","last_updated":"2026-06-05T08:18:06Z","snapshot_observed_at":"2026-08-16T23:20:25.270543Z","submitted_at":"2025-07-21T12:56:39Z","title":"Is Dark Energy an Effective Manifestation of Non-equilibrium Thermodynamics? -- Insights from DESI","version":2},"reference_index":49,"source":"pdf_text","source_observed_at":"2026-08-06T15:36:19.609471Z"},"links":{"cited_paper":"/paper/2404.15232","citing_paper":"/paper/2507.15575"},"observation_digest":"sha256:9bcc875bf7406b09969772db57e07104659267503d4c1c1430796e0f630a327b","observation_id":"1a0b614f-640b-496e-adca-55b650fc5241","resolution":{"observed_at":"2026-08-06T15:36:19.609471Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2404.15232","last_updated":"2024-12-19T16:25:49Z","snapshot_observed_at":"2026-08-16T13:58:27.312344Z","submitted_at":"2024-04-23T17:05:14Z","title":"Interacting Dark Energy after DESI Baryon Acoustic Oscillation measurements","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2404.15232","snapshot_observed_at":"2026-08-06T15:12:33.246910Z","title":"Giar` e, M","venue":null,"work_id":null,"year":2024},"citing_paper":{"arxiv_id":"2507.16589","last_updated":"2026-06-23T13:43:52Z","snapshot_observed_at":"2026-08-20T04:16:10.561421Z","submitted_at":"2025-07-22T13:45:38Z","title":"Cosmological preference for a positive neutrino mass at 2.7$\\sigma$: A joint analysis of DESI DR2, DESY5, and DESY1 data","version":3},"reference_index":19,"source":"pdf_text","source_observed_at":"2026-08-06T15:12:33.246910Z"},"links":{"cited_paper":"/paper/2404.15232","citing_paper":"/paper/2507.16589"},"observation_digest":"sha256:fb0d473a010ba5316adebc9640ecc3a297de736f16effdf4df54cf2500ba5220","observation_id":"b0253b05-b210-4bd8-86cf-13a8d823cece","resolution":{"observed_at":"2026-08-06T15:12:33.246910Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2404.15232","last_updated":"2024-12-19T16:25:49Z","snapshot_observed_at":"2026-08-16T13:58:27.312344Z","submitted_at":"2024-04-23T17:05:14Z","title":"Interacting Dark Energy after DESI Baryon Acoustic Oscillation measurements","version":2},"cited_work":{"arxiv_id":"2404.15232","doi":null,"metadata_source":"pith","pith_arxiv_id":"2404.15232","snapshot_observed_at":"2026-07-09T13:46:17.479123Z","title":"Giar` e, M","venue":"astro-ph.CO","work_id":"5be9e1ba-8076-41a9-b994-919073086747","year":2024},"citing_paper":{"arxiv_id":"2508.01759","last_updated":"2026-04-28T15:04:32Z","snapshot_observed_at":"2026-07-06T22:07:02.782730Z","submitted_at":"2025-08-03T14:00:54Z","title":"Resolving the Planck-DESI tension by nonminimally coupled quintessence","version":5},"reference_index":46,"source":"pdf_text","source_observed_at":"2026-05-19T01:35:36.430109Z"},"links":{"cited_paper":"/paper/2404.15232","citing_paper":"/paper/2508.01759"},"observation_digest":"sha256:6aec4bae7dde8e7f145b2c90321b3f181275d72616e945ec65dd1d72ac2b1eb2","observation_id":"8b74a1ac-a7d1-45e7-a643-49db0e0df199","resolution":{"observed_at":"2026-05-19T01:36:57.894275Z","resolver_source":"arxiv_id","status":"metadata_mismatch"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-20T06:33:59.587034+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-20T06:33:59.587034+00:00","source":"crossref"},{"observed_at":"2026-08-20T06:33:54.927442+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":{"arxiv_id":"2404.15232","last_updated":"2024-12-19T16:25:49Z","snapshot_observed_at":"2026-08-16T13:58:27.312344Z","submitted_at":"2024-04-23T17:05:14Z","title":"Interacting Dark Energy after DESI Baryon Acoustic Oscillation measurements","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2404.15232","snapshot_observed_at":"2026-08-06T05:29:01.892565Z","title":"Giarè, M","venue":null,"work_id":null,"year":2024},"citing_paper":{"arxiv_id":"2508.01876","last_updated":"2025-08-05T05:02:30Z","snapshot_observed_at":"2026-08-16T11:58:59.072774Z","submitted_at":"2025-08-03T18:18:17Z","title":"Averaging Dynamics of Scalar Field-Matter Interacting Models in Anisotropic Universes: The Locally Rotationally Symmetric Bianchi I Spacetime","version":2},"reference_index":77,"source":"pdf_text","source_observed_at":"2026-08-06T05:29:01.892565Z"},"links":{"cited_paper":"/paper/2404.15232","citing_paper":"/paper/2508.01876"},"observation_digest":"sha256:ab403c3a04b8f5dfb803e997f84dd45d6805f075e28c37ff9fcd260a3e454e96","observation_id":"c006d971-c973-4e23-8da8-16efbc43dd5a","resolution":{"observed_at":"2026-08-06T05:29:01.892565Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2404.15232","last_updated":"2024-12-19T16:25:49Z","snapshot_observed_at":"2026-08-16T13:58:27.312344Z","submitted_at":"2024-04-23T17:05:14Z","title":"Interacting Dark Energy after DESI Baryon Acoustic Oscillation measurements","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2404.15232","snapshot_observed_at":"2026-08-05T16:03:01.395296Z","title":"Giar` e, M","venue":null,"work_id":null,"year":2024},"citing_paper":{"arxiv_id":"2508.19109","last_updated":"2025-08-26T15:13:27Z","snapshot_observed_at":"2026-08-17T20:49:58.191765Z","submitted_at":"2025-08-26T15:13:27Z","title":"Dark Energy Is Not That Into You: Variable Couplings after DESI DR2 BAO","version":1},"reference_index":102,"source":"pdf_text","source_observed_at":"2026-08-05T16:03:01.395296Z"},"links":{"cited_paper":"/paper/2404.15232","citing_paper":"/paper/2508.19109"},"observation_digest":"sha256:6351422a44e6b19a411166ecb5b290ae86231270e26cea0b4c0564808c1d0905","observation_id":"2a8d81b2-bb3c-4659-9170-0f145c615cc9","resolution":{"observed_at":"2026-08-05T16:03:01.395296Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2404.15232","last_updated":"2024-12-19T16:25:49Z","snapshot_observed_at":"2026-08-16T13:58:27.312344Z","submitted_at":"2024-04-23T17:05:14Z","title":"Interacting Dark Energy after DESI Baryon Acoustic Oscillation measurements","version":2},"cited_work":{"arxiv_id":"2404.15232","doi":null,"metadata_source":"pith","pith_arxiv_id":"2404.15232","snapshot_observed_at":"2026-07-09T13:46:17.479123Z","title":"Giar` e, M","venue":"astro-ph.CO","work_id":"5be9e1ba-8076-41a9-b994-919073086747","year":2024},"citing_paper":{"arxiv_id":"2510.03779","last_updated":"2026-02-17T10:47:14Z","snapshot_observed_at":"2026-08-20T02:01:23.133869Z","submitted_at":"2025-10-04T11:08:41Z","title":"Beyond CPL: Evidence for dynamical dark energy in three-parameter models","version":3},"reference_index":15,"source":"pdf_text","source_observed_at":"2026-05-18T10:45:16.985887Z"},"links":{"cited_paper":"/paper/2404.15232","citing_paper":"/paper/2510.03779"},"observation_digest":"sha256:116cb51081233acb9db33f9f33824f58dcb82abcb84f90f71d7b5fcbf8d9d175","observation_id":"b9d03c01-ffc0-46d6-a9f7-876b74acc389","resolution":{"observed_at":"2026-05-18T10:46:16.813816Z","resolver_source":"arxiv_id","status":"verified_exact"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-20T06:33:59.587034+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-20T06:33:59.587034+00:00","source":"crossref"},{"observed_at":"2026-08-20T06:33:54.927442+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":{"arxiv_id":"2404.15232","last_updated":"2024-12-19T16:25:49Z","snapshot_observed_at":"2026-08-16T13:58:27.312344Z","submitted_at":"2024-04-23T17:05:14Z","title":"Interacting Dark Energy after DESI Baryon Acoustic Oscillation measurements","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2404.15232","snapshot_observed_at":"2026-08-04T09:59:29.682637Z","title":"Giar` e, M","venue":null,"work_id":null,"year":2024},"citing_paper":{"arxiv_id":"2510.12627","last_updated":"2026-06-20T07:00:45Z","snapshot_observed_at":"2026-08-19T21:41:40.945785Z","submitted_at":"2025-10-14T15:24:50Z","title":"Alleviating the $H_0$ tension through the interacting dark energy model from quantum gravitational field theory in light of DESI DR2","version":2},"reference_index":174,"source":"pdf_text","source_observed_at":"2026-08-04T09:59:29.682637Z"},"links":{"cited_paper":"/paper/2404.15232","citing_paper":"/paper/2510.12627"},"observation_digest":"sha256:76b2d774bf4f4e5a4bc519998561e6cf27c45cbfe73051c5262b79d3e494cabf","observation_id":"917893a8-5b30-4ee2-a84d-878423ee4257","resolution":{"observed_at":"2026-08-04T09:59:29.682637Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2404.15232","last_updated":"2024-12-19T16:25:49Z","snapshot_observed_at":"2026-08-16T13:58:27.312344Z","submitted_at":"2024-04-23T17:05:14Z","title":"Interacting Dark Energy after DESI Baryon Acoustic Oscillation measurements","version":2},"cited_work":{"arxiv_id":"2404.15232","doi":null,"metadata_source":"pith","pith_arxiv_id":"2404.15232","snapshot_observed_at":"2026-07-09T13:46:17.479123Z","title":"Giar` e, M","venue":"astro-ph.CO","work_id":"5be9e1ba-8076-41a9-b994-919073086747","year":2024},"citing_paper":{"arxiv_id":"2510.18741","last_updated":"2026-04-10T13:03:33Z","snapshot_observed_at":"2026-08-13T23:09:37.713842Z","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":87,"source":"pdf_text","source_observed_at":"2026-05-18T04:46:14.832965Z"},"links":{"cited_paper":"/paper/2404.15232","citing_paper":"/paper/2510.18741"},"observation_digest":"sha256:f999942f33268f9fde3417b53590238666b8fe2192e575a75585900050c24b53","observation_id":"61eef0a9-cf10-455c-bcd7-81e4872f2920","resolution":{"observed_at":"2026-05-18T04:50:55.452708Z","resolver_source":"arxiv_id","status":"verified_exact"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-20T06:33:59.587034+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-20T06:33:59.587034+00:00","source":"crossref"},{"observed_at":"2026-08-20T06:33:54.927442+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":{"arxiv_id":"2404.15232","last_updated":"2024-12-19T16:25:49Z","snapshot_observed_at":"2026-08-16T13:58:27.312344Z","submitted_at":"2024-04-23T17:05:14Z","title":"Interacting Dark Energy after DESI Baryon Acoustic Oscillation measurements","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2404.15232","snapshot_observed_at":"2026-08-04T07:19:40.213745Z","title":"Giar` e, M","venue":null,"work_id":null,"year":2024},"citing_paper":{"arxiv_id":"2510.26355","last_updated":"2026-07-07T01:20:38Z","snapshot_observed_at":"2026-08-21T04:24:30.119012Z","submitted_at":"2025-10-30T11:06:11Z","title":"Model-independent late-universe measurements of $H_0$ and $\\Omega_K$ with the parametrization based on cosmic age-improved inverse distance ladder","version":2},"reference_index":88,"source":"pdf_text","source_observed_at":"2026-08-04T07:19:40.213745Z"},"links":{"cited_paper":"/paper/2404.15232","citing_paper":"/paper/2510.26355"},"observation_digest":"sha256:743a54394075585a2a2dae893a3cece8bd17e8ef70792e63d535c6902a39f07a","observation_id":"06644300-3ce4-49d1-8041-9d87e9f304d8","resolution":{"observed_at":"2026-08-04T07:19:40.213745Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2404.15232","last_updated":"2024-12-19T16:25:49Z","snapshot_observed_at":"2026-08-16T13:58:27.312344Z","submitted_at":"2024-04-23T17:05:14Z","title":"Interacting Dark Energy after DESI Baryon Acoustic Oscillation measurements","version":2},"cited_work":{"arxiv_id":"2404.15232","doi":null,"metadata_source":"pith","pith_arxiv_id":"2404.15232","snapshot_observed_at":"2026-07-09T13:46:17.479123Z","title":"Giar` e, M","venue":"astro-ph.CO","work_id":"5be9e1ba-8076-41a9-b994-919073086747","year":2024},"citing_paper":{"arxiv_id":"2511.09467","last_updated":"2026-03-30T07:50:13Z","snapshot_observed_at":"2026-08-15T23:25:25.692634Z","submitted_at":"2025-11-12T16:39:04Z","title":"Revisiting the Hubble tension problem in the framework of holographic dark energy","version":2},"reference_index":30,"source":"pdf_text","source_observed_at":"2026-05-17T22:17:32.138764Z"},"links":{"cited_paper":"/paper/2404.15232","citing_paper":"/paper/2511.09467"},"observation_digest":"sha256:a595bbc752eb4e3e66e72b9fb81e2f4ecd08d9731e76cb45a0b92b09e1c79f9c","observation_id":"f1b1ffee-1182-48ff-af3b-b2f418aaaf67","resolution":{"observed_at":"2026-05-17T22:20:23.274309Z","resolver_source":"arxiv_id","status":"verified_exact"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-20T06:33:59.587034+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-20T06:33:59.587034+00:00","source":"crossref"},{"observed_at":"2026-08-20T06:33:54.927442+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":{"arxiv_id":"2404.15232","last_updated":"2024-12-19T16:25:49Z","snapshot_observed_at":"2026-08-16T13:58:27.312344Z","submitted_at":"2024-04-23T17:05:14Z","title":"Interacting Dark Energy after DESI Baryon Acoustic Oscillation measurements","version":2},"cited_work":{"arxiv_id":"2404.15232","doi":null,"metadata_source":"pith","pith_arxiv_id":"2404.15232","snapshot_observed_at":"2026-07-09T13:46:17.479123Z","title":"Giar` e, M","venue":"astro-ph.CO","work_id":"5be9e1ba-8076-41a9-b994-919073086747","year":2024},"citing_paper":{"arxiv_id":"2512.10530","last_updated":"2026-04-09T12:39:52Z","snapshot_observed_at":"2026-08-19T21:06:45.239013Z","submitted_at":"2025-12-11T11:02:39Z","title":"Cosmological and lunar laser ranging constraints on evolving dark energy in a nonminimally coupled curvature-matter gravity model","version":2},"reference_index":14,"source":"pdf_text","source_observed_at":"2026-05-16T23:27:57.096438Z"},"links":{"cited_paper":"/paper/2404.15232","citing_paper":"/paper/2512.10530"},"observation_digest":"sha256:ca36e8b4c3d2c34a4f45ee4b6ff47b5f4a8d8af6b63ed5dc284890ace1278c93","observation_id":"ffe45f4f-a65a-4250-b9ef-2d7e82c3703f","resolution":{"observed_at":"2026-05-16T23:28:40.643692Z","resolver_source":"arxiv_id","status":"verified_exact"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-20T06:33:59.587034+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-20T06:33:59.587034+00:00","source":"crossref"},{"observed_at":"2026-08-20T06:33:54.927442+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":{"arxiv_id":"2404.15232","last_updated":"2024-12-19T16:25:49Z","snapshot_observed_at":"2026-08-16T13:58:27.312344Z","submitted_at":"2024-04-23T17:05:14Z","title":"Interacting Dark Energy after DESI Baryon Acoustic Oscillation measurements","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2404.15232","snapshot_observed_at":"2026-08-03T14:40:55.353779Z","title":"Giar` e, M","venue":null,"work_id":null,"year":2024},"citing_paper":{"arxiv_id":"2512.19888","last_updated":"2026-06-18T12:16:03Z","snapshot_observed_at":"2026-08-17T17:44:10.961719Z","submitted_at":"2025-12-22T21:27:32Z","title":"Observational constraints on early time non-phantom behaviour of dynamical dark energy","version":2},"reference_index":16,"source":"pdf_text","source_observed_at":"2026-08-03T14:40:55.353779Z"},"links":{"cited_paper":"/paper/2404.15232","citing_paper":"/paper/2512.19888"},"observation_digest":"sha256:24dc5f8d1333c211599c4674f824442e59fdba87c06e288bf87acbd1afd709e8","observation_id":"28bf4d10-4a1d-4c5d-88aa-3ae7925f5c53","resolution":{"observed_at":"2026-08-03T14:40:55.353779Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2404.15232","last_updated":"2024-12-19T16:25:49Z","snapshot_observed_at":"2026-08-16T13:58:27.312344Z","submitted_at":"2024-04-23T17:05:14Z","title":"Interacting Dark Energy after DESI Baryon Acoustic Oscillation measurements","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2404.15232","snapshot_observed_at":"2026-08-03T11:11:48.901893Z","title":"Giarè, M","venue":null,"work_id":null,"year":2024},"citing_paper":{"arxiv_id":"2601.07361","last_updated":"2026-07-15T07:08:06Z","snapshot_observed_at":"2026-08-19T06:05:14.523776Z","submitted_at":"2026-01-12T09:36:30Z","title":"Robust Preference for Dark Sector Interactions","version":2},"reference_index":111,"source":"pdf_text","source_observed_at":"2026-08-03T11:11:48.901893Z"},"links":{"cited_paper":"/paper/2404.15232","citing_paper":"/paper/2601.07361"},"observation_digest":"sha256:02a995deb07a41a2bf82d52b747705649a099b7402b41081ca49995c84ad86d8","observation_id":"51cb5864-f29c-48e2-87be-db66058644f8","resolution":{"observed_at":"2026-08-03T11:11:48.901893Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2404.15232","last_updated":"2024-12-19T16:25:49Z","snapshot_observed_at":"2026-08-16T13:58:27.312344Z","submitted_at":"2024-04-23T17:05:14Z","title":"Interacting Dark Energy after DESI Baryon Acoustic Oscillation measurements","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2404.15232","snapshot_observed_at":"2026-08-03T07:07:23.639144Z","title":"Giar` e, M","venue":null,"work_id":null,"year":2024},"citing_paper":{"arxiv_id":"2601.21356","last_updated":"2026-07-16T19:48:47Z","snapshot_observed_at":"2026-08-20T09:37:00.194183Z","submitted_at":"2026-01-29T07:32:33Z","title":"Is Phantom Divide Crossing in General Relativity Completely Impossible? Shortcomings in canonical and minimally coupled scalar field and Possible Solutions in $k$-essence Models","version":2},"reference_index":12,"source":"pdf_text","source_observed_at":"2026-08-03T07:07:23.639144Z"},"links":{"cited_paper":"/paper/2404.15232","citing_paper":"/paper/2601.21356"},"observation_digest":"sha256:80e05ac0dff62a5b2db85f8ff901971c5ebb49e45877ccb405136c5452798d4a","observation_id":"8a008a6d-0675-4147-bc75-54c6615eead8","resolution":{"observed_at":"2026-08-03T07:07:23.639144Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2404.15232","last_updated":"2024-12-19T16:25:49Z","snapshot_observed_at":"2026-08-16T13:58:27.312344Z","submitted_at":"2024-04-23T17:05:14Z","title":"Interacting Dark Energy after DESI Baryon Acoustic Oscillation measurements","version":2},"cited_work":{"arxiv_id":"2404.15232","doi":null,"metadata_source":"pith","pith_arxiv_id":"2404.15232","snapshot_observed_at":"2026-07-09T13:46:17.479123Z","title":"Giar` e, M","venue":"astro-ph.CO","work_id":"5be9e1ba-8076-41a9-b994-919073086747","year":2024},"citing_paper":{"arxiv_id":"2602.03110","last_updated":"2026-04-28T09:37:14Z","snapshot_observed_at":"2026-08-17T20:59:00.323360Z","submitted_at":"2026-02-03T05:11:50Z","title":"Evidence for deviation in gravitational light deflection from general relativity at cosmological scales with KiDS-Legacy and CMB lensing","version":2},"reference_index":51,"source":"pdf_text","source_observed_at":"2026-05-16T08:17:34.164338Z"},"links":{"cited_paper":"/paper/2404.15232","citing_paper":"/paper/2602.03110"},"observation_digest":"sha256:dda815a84d8c62a5f116ffcb04d96638bf8903e8b772c022d9bcaffbeb2d963a","observation_id":"a4aca092-3d46-4518-aad2-de8bfd1ce15e","resolution":{"observed_at":"2026-05-16T08:17:35.585631Z","resolver_source":"arxiv_id","status":"verified_exact"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-20T06:33:59.587034+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-20T06:33:59.587034+00:00","source":"crossref"},{"observed_at":"2026-08-20T06:33:54.927442+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":{"arxiv_id":"2404.15232","last_updated":"2024-12-19T16:25:49Z","snapshot_observed_at":"2026-08-16T13:58:27.312344Z","submitted_at":"2024-04-23T17:05:14Z","title":"Interacting Dark Energy after DESI Baryon Acoustic Oscillation measurements","version":2},"cited_work":{"arxiv_id":"2404.15232","doi":null,"metadata_source":"pith","pith_arxiv_id":"2404.15232","snapshot_observed_at":"2026-07-09T13:46:17.479123Z","title":"Giar` e, M","venue":"astro-ph.CO","work_id":"5be9e1ba-8076-41a9-b994-919073086747","year":2024},"citing_paper":{"arxiv_id":"2602.11936","last_updated":"2026-08-10T08:18:00Z","snapshot_observed_at":"2026-08-13T23:37:48.189492Z","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":66,"source":"pdf_text","source_observed_at":"2026-05-21T13:29:05.147292Z"},"links":{"cited_paper":"/paper/2404.15232","citing_paper":"/paper/2602.11936"},"observation_digest":"sha256:2de9a9bddb83de6a8555e6787182b7cfab1170dbb62fbdb9eb9f1d3054920ec3","observation_id":"1e5a3a71-c37c-43be-a0c6-d8437c81fdbd","resolution":{"observed_at":"2026-05-21T13:30:11.971971Z","resolver_source":"arxiv_id","status":"verified_exact"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-20T06:33:59.587034+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-20T06:33:59.587034+00:00","source":"crossref"},{"observed_at":"2026-08-20T06:33:54.927442+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":{"arxiv_id":"2404.15232","last_updated":"2024-12-19T16:25:49Z","snapshot_observed_at":"2026-08-16T13:58:27.312344Z","submitted_at":"2024-04-23T17:05:14Z","title":"Interacting Dark Energy after DESI Baryon Acoustic Oscillation measurements","version":2},"cited_work":{"arxiv_id":"2404.15232","doi":null,"metadata_source":"pith","pith_arxiv_id":"2404.15232","snapshot_observed_at":"2026-07-09T13:46:17.479123Z","title":"Giar` e, M","venue":"astro-ph.CO","work_id":"5be9e1ba-8076-41a9-b994-919073086747","year":2024},"citing_paper":{"arxiv_id":"2603.10787","last_updated":"2026-03-11T14:00:06Z","snapshot_observed_at":"2026-08-11T15:40:03.224454Z","submitted_at":"2026-03-11T14:00:06Z","title":"Measuring neutrino mass in light of ACT DR6 and DESI DR2","version":1},"reference_index":39,"source":"pdf_text","source_observed_at":"2026-05-15T13:14:03.491513Z"},"links":{"cited_paper":"/paper/2404.15232","citing_paper":"/paper/2603.10787"},"observation_digest":"sha256:87159094307614631e5418a954c01f30dae19c363259fccc03a8fca241872b49","observation_id":"f1be76f0-2814-4feb-abb0-240807c71cbd","resolution":{"observed_at":"2026-05-15T13:15:50.458129Z","resolver_source":"arxiv_id","status":"verified_exact"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-20T06:33:59.587034+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-20T06:33:59.587034+00:00","source":"crossref"},{"observed_at":"2026-08-20T06:33:54.927442+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":{"arxiv_id":"2404.15232","last_updated":"2024-12-19T16:25:49Z","snapshot_observed_at":"2026-08-16T13:58:27.312344Z","submitted_at":"2024-04-23T17:05:14Z","title":"Interacting Dark Energy after DESI Baryon Acoustic Oscillation measurements","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2404.15232","snapshot_observed_at":"2026-07-15T12:01:04.317365Z","title":"Giar` e, M","venue":null,"work_id":null,"year":2024},"citing_paper":{"arxiv_id":"2603.14693","last_updated":"2026-07-14T04:50:03Z","snapshot_observed_at":"2026-08-15T18:05:37.165382Z","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":75,"source":"pdf_text","source_observed_at":"2026-07-15T12:01:04.317365Z"},"links":{"cited_paper":"/paper/2404.15232","citing_paper":"/paper/2603.14693"},"observation_digest":"sha256:0a7b87c8625a4a69d9455454e3534dc8874c0d822cc6834fffb6ec813943f8bd","observation_id":"de1a06ba-0cdf-4f04-ad00-5178dccb7b67","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":"2404.15232","last_updated":"2024-12-19T16:25:49Z","snapshot_observed_at":"2026-08-16T13:58:27.312344Z","submitted_at":"2024-04-23T17:05:14Z","title":"Interacting Dark Energy after DESI Baryon Acoustic Oscillation measurements","version":2},"cited_work":{"arxiv_id":"2404.15232","doi":null,"metadata_source":"pith","pith_arxiv_id":"2404.15232","snapshot_observed_at":"2026-07-09T13:46:17.479123Z","title":"Giar` e, M","venue":"astro-ph.CO","work_id":"5be9e1ba-8076-41a9-b994-919073086747","year":2024},"citing_paper":{"arxiv_id":"2603.21125","last_updated":"2026-03-22T08:46:57Z","snapshot_observed_at":"2026-08-20T23:25:02.076346Z","submitted_at":"2026-03-22T08:46:57Z","title":"Model-Independent Reconstruction of Quintessence Potential and Kinetic Energy from DESI DR2 and Pantheon+ Supernovae","version":1},"reference_index":36,"source":"pdf_text","source_observed_at":"2026-05-15T01:30:47.614992Z"},"links":{"cited_paper":"/paper/2404.15232","citing_paper":"/paper/2603.21125"},"observation_digest":"sha256:d3548f43fba0fee0d6d5279ce549131bad1535e7c2c86bb05efc9cbe4b67d795","observation_id":"1fbe5e60-81c0-4c37-a8bc-9a0d174e9ea2","resolution":{"observed_at":"2026-05-15T01:33:27.453207Z","resolver_source":"arxiv_id","status":"verified_exact"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-20T06:33:59.587034+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-20T06:33:59.587034+00:00","source":"crossref"},{"observed_at":"2026-08-20T06:33:54.927442+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":{"arxiv_id":"2404.15232","last_updated":"2024-12-19T16:25:49Z","snapshot_observed_at":"2026-08-16T13:58:27.312344Z","submitted_at":"2024-04-23T17:05:14Z","title":"Interacting Dark Energy after DESI Baryon Acoustic Oscillation measurements","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2404.15232","snapshot_observed_at":"2026-08-03T02:32:25.256541Z","title":"Giar` e, M","venue":null,"work_id":null,"year":2024},"citing_paper":{"arxiv_id":"2603.24685","last_updated":"2026-07-31T11:04:39Z","snapshot_observed_at":"2026-08-14T16:36:02.923591Z","submitted_at":"2026-03-25T18:04:12Z","title":"UV-complete and stable Quintom Dark Energy models in the light of DESI DR2","version":3},"reference_index":15,"source":"pdf_text","source_observed_at":"2026-08-03T02:32:25.256541Z"},"links":{"cited_paper":"/paper/2404.15232","citing_paper":"/paper/2603.24685"},"observation_digest":"sha256:c31792dd57d8861b5fc7acc3a86da40ed4af611f02c74abae0a77568d2415336","observation_id":"e04192f8-5876-4656-a6f8-9c9c51251049","resolution":{"observed_at":"2026-08-03T02:32:25.256541Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2404.15232","last_updated":"2024-12-19T16:25:49Z","snapshot_observed_at":"2026-08-16T13:58:27.312344Z","submitted_at":"2024-04-23T17:05:14Z","title":"Interacting Dark Energy after DESI Baryon Acoustic Oscillation measurements","version":2},"cited_work":{"arxiv_id":"2404.15232","doi":null,"metadata_source":"pith","pith_arxiv_id":"2404.15232","snapshot_observed_at":"2026-07-09T13:46:17.479123Z","title":"Giar` e, M","venue":"astro-ph.CO","work_id":"5be9e1ba-8076-41a9-b994-919073086747","year":2024},"citing_paper":{"arxiv_id":"2604.13535","last_updated":"2026-04-15T06:29:12Z","snapshot_observed_at":"2026-08-18T05:23:44.122534Z","submitted_at":"2026-04-15T06:29:12Z","title":"Double the axions, half the tension: multi-field early dark energy eases the Hubble tension","version":1},"reference_index":68,"source":"pdf_text","source_observed_at":"2026-05-10T12:56:21.466420Z"},"links":{"cited_paper":"/paper/2404.15232","citing_paper":"/paper/2604.13535"},"observation_digest":"sha256:f27a904e0b0c6a79a67eb92e40bc3c9161f0c57f3405b78df84ea9da6cc6c9e9","observation_id":"007cebce-67d8-40fb-87a8-08d2c73efdf5","resolution":{"observed_at":"2026-05-11T11:41:01.854398Z","resolver_source":"arxiv_id","status":"verified_exact"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-20T06:33:59.587034+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-20T06:33:59.587034+00:00","source":"crossref"},{"observed_at":"2026-08-20T06:33:54.927442+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":{"arxiv_id":"2404.15232","last_updated":"2024-12-19T16:25:49Z","snapshot_observed_at":"2026-08-16T13:58:27.312344Z","submitted_at":"2024-04-23T17:05:14Z","title":"Interacting Dark Energy after DESI Baryon Acoustic Oscillation measurements","version":2},"cited_work":{"arxiv_id":"2404.15232","doi":null,"metadata_source":"pith","pith_arxiv_id":"2404.15232","snapshot_observed_at":"2026-07-09T13:46:17.479123Z","title":"Giar` e, M","venue":"astro-ph.CO","work_id":"5be9e1ba-8076-41a9-b994-919073086747","year":2024},"citing_paper":{"arxiv_id":"2604.21770","last_updated":"2026-06-05T08:25:09Z","snapshot_observed_at":"2026-08-16T19:22:03.201436Z","submitted_at":"2026-04-23T15:28:34Z","title":"Accelerating scaling solutions from dark matter particle creation","version":1},"reference_index":91,"source":"pdf_text","source_observed_at":"2026-05-09T21:25:37.448155Z"},"links":{"cited_paper":"/paper/2404.15232","citing_paper":"/paper/2604.21770"},"observation_digest":"sha256:e1c020d334e232bce7c6d1b5726e8a2a7e869176ff1c9cb2a83c5dd194253b74","observation_id":"ce635795-f3cb-48d2-940b-1e820da0c4fb","resolution":{"observed_at":"2026-05-11T14:36:07.943313Z","resolver_source":"arxiv_id","status":"malformed_identifier"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-20T06:33:59.587034+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-20T06:33:59.587034+00:00","source":"crossref"},{"observed_at":"2026-08-20T06:33:54.927442+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":{"arxiv_id":"2404.15232","last_updated":"2024-12-19T16:25:49Z","snapshot_observed_at":"2026-08-16T13:58:27.312344Z","submitted_at":"2024-04-23T17:05:14Z","title":"Interacting Dark Energy after DESI Baryon Acoustic Oscillation measurements","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2404.15232","snapshot_observed_at":"2026-07-12T18:37:05.978670Z","title":"Giar\\`e, M","venue":null,"work_id":null,"year":2024},"citing_paper":{"arxiv_id":"2604.21770","last_updated":"2026-06-05T08:25:09Z","snapshot_observed_at":"2026-08-16T19:22:03.201436Z","submitted_at":"2026-04-23T15:28:34Z","title":"Accelerating scaling solutions from dark matter particle creation","version":2},"reference_index":85,"source":"arxiv_source","source_observed_at":"2026-07-12T18:37:05.978670Z"},"links":{"cited_paper":"/paper/2404.15232","citing_paper":"/paper/2604.21770"},"observation_digest":"sha256:0a53fd811371d4d8d32b91929386944e244757fd7228a3c8a2c5d89d9f952b1c","observation_id":"f2b61a5d-a08d-4e3a-a7ec-06939644b9f7","resolution":{"observed_at":"2026-07-12T18:37:05.978670Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2404.15232","last_updated":"2024-12-19T16:25:49Z","snapshot_observed_at":"2026-08-16T13:58:27.312344Z","submitted_at":"2024-04-23T17:05:14Z","title":"Interacting Dark Energy after DESI Baryon Acoustic Oscillation measurements","version":2},"cited_work":{"arxiv_id":"2404.15232","doi":null,"metadata_source":"pith","pith_arxiv_id":"2404.15232","snapshot_observed_at":"2026-07-09T13:46:17.479123Z","title":"Giar` e, M","venue":"astro-ph.CO","work_id":"5be9e1ba-8076-41a9-b994-919073086747","year":2024},"citing_paper":{"arxiv_id":"2604.23492","last_updated":"2026-04-26T01:51:22Z","snapshot_observed_at":"2026-08-08T06:56:09.579935Z","submitted_at":"2026-04-26T01:51:22Z","title":"The open-Universe signal: A model artifact rather than genuine curvature","version":1},"reference_index":26,"source":"pdf_text","source_observed_at":"2026-05-08T05:38:44.860590Z"},"links":{"cited_paper":"/paper/2404.15232","citing_paper":"/paper/2604.23492"},"observation_digest":"sha256:00dbbe9c87952a2a61b82de9fa3847a4be0bc88c8c74832d818bd22f455c30ee","observation_id":"1371249a-1844-4687-8df5-0981a224454d","resolution":{"observed_at":"2026-05-11T21:26:15.833121Z","resolver_source":"arxiv_id","status":"metadata_mismatch"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-20T06:33:59.587034+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-20T06:33:59.587034+00:00","source":"crossref"},{"observed_at":"2026-08-20T06:33:54.927442+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":{"arxiv_id":"2404.15232","last_updated":"2024-12-19T16:25:49Z","snapshot_observed_at":"2026-08-16T13:58:27.312344Z","submitted_at":"2024-04-23T17:05:14Z","title":"Interacting Dark Energy after DESI Baryon Acoustic Oscillation measurements","version":2},"cited_work":{"arxiv_id":"2404.15232","doi":null,"metadata_source":"pith","pith_arxiv_id":"2404.15232","snapshot_observed_at":"2026-07-09T13:46:17.479123Z","title":"Giar` e, M","venue":"astro-ph.CO","work_id":"5be9e1ba-8076-41a9-b994-919073086747","year":2024},"citing_paper":{"arxiv_id":"2604.25813","last_updated":"2026-04-28T16:22:13Z","snapshot_observed_at":"2026-08-17T10:50:37.056286Z","submitted_at":"2026-04-28T16:22:13Z","title":"Geometric Constraints on the Pre-Recombination Expansion History from the Hubble Tension","version":1},"reference_index":50,"source":"pdf_text","source_observed_at":"2026-05-07T14:55:55.250283Z"},"links":{"cited_paper":"/paper/2404.15232","citing_paper":"/paper/2604.25813"},"observation_digest":"sha256:4c06f22b4ffe6262c96bef393f23899fa6aa5e77b7969f33bb84400212772748","observation_id":"abd2ece5-b9af-4674-9c30-cd87fe4400d5","resolution":{"observed_at":"2026-05-12T00:36:16.242914Z","resolver_source":"arxiv_id","status":"verified_exact"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-20T06:33:59.587034+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-20T06:33:59.587034+00:00","source":"crossref"},{"observed_at":"2026-08-20T06:33:54.927442+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":{"arxiv_id":"2404.15232","last_updated":"2024-12-19T16:25:49Z","snapshot_observed_at":"2026-08-16T13:58:27.312344Z","submitted_at":"2024-04-23T17:05:14Z","title":"Interacting Dark Energy after DESI Baryon Acoustic Oscillation measurements","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2404.15232","snapshot_observed_at":"2026-08-02T14:29:44.062348Z","title":"Giar` e, M","venue":null,"work_id":null,"year":2024},"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":297,"source":"pdf_text","source_observed_at":"2026-08-02T14:29:44.062348Z"},"links":{"cited_paper":"/paper/2404.15232","citing_paper":"/paper/2605.10476"},"observation_digest":"sha256:439209f0f3b7f999c27b088637b0a7a675eb9a0743dc3fe4fe64f58f846cbe52","observation_id":"8ca5013d-ce8e-4efd-b78e-36772f31e1f2","resolution":{"observed_at":"2026-08-02T14:29:44.062348Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2404.15232","last_updated":"2024-12-19T16:25:49Z","snapshot_observed_at":"2026-08-16T13:58:27.312344Z","submitted_at":"2024-04-23T17:05:14Z","title":"Interacting Dark Energy after DESI Baryon Acoustic Oscillation measurements","version":2},"cited_work":{"arxiv_id":"2404.15232","doi":null,"metadata_source":"pith","pith_arxiv_id":"2404.15232","snapshot_observed_at":"2026-07-09T13:46:17.479123Z","title":"Giar` e, M","venue":"astro-ph.CO","work_id":"5be9e1ba-8076-41a9-b994-919073086747","year":2024},"citing_paper":{"arxiv_id":"2605.22348","last_updated":"2026-05-21T11:34:03Z","snapshot_observed_at":"2026-08-13T15:26:56.399802Z","submitted_at":"2026-05-21T11:34:03Z","title":"Dark Energy in Ghost-free non-local Gravity","version":1},"reference_index":32,"source":"pdf_text","source_observed_at":"2026-05-22T05:24:23.654862Z"},"links":{"cited_paper":"/paper/2404.15232","citing_paper":"/paper/2605.22348"},"observation_digest":"sha256:f3d2c39038d52ad89fc97ee4c27f4fe0befea9ff2fe1f90d1b481f8b09f1ba72","observation_id":"60d49e16-41b0-4613-a3f8-39c0f52603ca","resolution":{"observed_at":"2026-05-22T05:24:37.997900Z","resolver_source":"arxiv_id","status":"verified_exact"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-20T06:33:59.587034+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-20T06:33:59.587034+00:00","source":"crossref"},{"observed_at":"2026-08-20T06:33:54.927442+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":{"arxiv_id":"2404.15232","last_updated":"2024-12-19T16:25:49Z","snapshot_observed_at":"2026-08-16T13:58:27.312344Z","submitted_at":"2024-04-23T17:05:14Z","title":"Interacting Dark Energy after DESI Baryon Acoustic Oscillation measurements","version":2},"cited_work":{"arxiv_id":"2404.15232","doi":null,"metadata_source":"pith","pith_arxiv_id":"2404.15232","snapshot_observed_at":"2026-07-09T13:46:17.479123Z","title":"Giar` e, M","venue":"astro-ph.CO","work_id":"5be9e1ba-8076-41a9-b994-919073086747","year":2024},"citing_paper":{"arxiv_id":"2605.26116","last_updated":"2026-05-25T17:59:53Z","snapshot_observed_at":"2026-07-06T23:36:01.564747Z","submitted_at":"2026-05-25T17:59:53Z","title":"Unifying Early and Late Dark Energy: Dynamical Requirements and Obstructions","version":1},"reference_index":146,"source":"pdf_text","source_observed_at":"2026-06-29T20:17:08.107860Z"},"links":{"cited_paper":"/paper/2404.15232","citing_paper":"/paper/2605.26116"},"observation_digest":"sha256:f50f5c102f906e39f88eaf38c1833e7cfb10cda472b773ae893bc60ecd13c57a","observation_id":"94feebc8-e4ec-4271-a1ba-846fde556935","resolution":{"observed_at":"2026-07-01T16:45:51.197724Z","resolver_source":"arxiv_id","status":"verified_exact"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-20T06:33:59.587034+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-20T06:33:59.587034+00:00","source":"crossref"},{"observed_at":"2026-08-20T06:33:54.927442+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":{"arxiv_id":"2404.15232","last_updated":"2024-12-19T16:25:49Z","snapshot_observed_at":"2026-08-16T13:58:27.312344Z","submitted_at":"2024-04-23T17:05:14Z","title":"Interacting Dark Energy after DESI Baryon Acoustic Oscillation measurements","version":2},"cited_work":{"arxiv_id":"2404.15232","doi":null,"metadata_source":"pith","pith_arxiv_id":"2404.15232","snapshot_observed_at":"2026-07-09T13:46:17.479123Z","title":"Giar` e, M","venue":"astro-ph.CO","work_id":"5be9e1ba-8076-41a9-b994-919073086747","year":2024},"citing_paper":{"arxiv_id":"2606.01360","last_updated":"2026-07-18T02:00:49Z","snapshot_observed_at":"2026-08-12T22:06:47.187155Z","submitted_at":"2026-05-31T17:31:59Z","title":"A short review on Quintom dark energy theory","version":1},"reference_index":24,"source":"pdf_text","source_observed_at":"2026-06-28T16:17:39.285285Z"},"links":{"cited_paper":"/paper/2404.15232","citing_paper":"/paper/2606.01360"},"observation_digest":"sha256:bf7a937cf9b8f4d4669506ddaf6eb83e5fc7fd3b18d75366912ad938261c108f","observation_id":"63971910-0fec-4137-a77a-4cb215c6761b","resolution":{"observed_at":"2026-07-01T21:46:15.956582Z","resolver_source":"arxiv_id","status":"verified_exact"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-20T06:33:59.587034+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-20T06:33:59.587034+00:00","source":"crossref"},{"observed_at":"2026-08-20T06:33:54.927442+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":{"arxiv_id":"2404.15232","last_updated":"2024-12-19T16:25:49Z","snapshot_observed_at":"2026-08-16T13:58:27.312344Z","submitted_at":"2024-04-23T17:05:14Z","title":"Interacting Dark Energy after DESI Baryon Acoustic Oscillation measurements","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2404.15232","snapshot_observed_at":"2026-08-02T12:40:01.093221Z","title":"Giarè, M","venue":null,"work_id":null,"year":2024},"citing_paper":{"arxiv_id":"2606.01360","last_updated":"2026-07-18T02:00:49Z","snapshot_observed_at":"2026-08-12T22:06:47.187155Z","submitted_at":"2026-05-31T17:31:59Z","title":"A short review on Quintom dark energy theory","version":2},"reference_index":24,"source":"pdf_text","source_observed_at":"2026-08-02T12:40:01.093221Z"},"links":{"cited_paper":"/paper/2404.15232","citing_paper":"/paper/2606.01360"},"observation_digest":"sha256:5d3bb3a5e6b76dc1d903de4916eab314527e0bae9dc1a9a1b9f005a1324cd65f","observation_id":"02d96286-70ef-4812-b164-fabfb6cc187c","resolution":{"observed_at":"2026-08-02T12:40:01.093221Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2404.15232","last_updated":"2024-12-19T16:25:49Z","snapshot_observed_at":"2026-08-16T13:58:27.312344Z","submitted_at":"2024-04-23T17:05:14Z","title":"Interacting Dark Energy after DESI Baryon Acoustic Oscillation measurements","version":2},"cited_work":{"arxiv_id":"2404.15232","doi":null,"metadata_source":"pith","pith_arxiv_id":"2404.15232","snapshot_observed_at":"2026-07-09T13:46:17.479123Z","title":"Giar` e, M","venue":"astro-ph.CO","work_id":"5be9e1ba-8076-41a9-b994-919073086747","year":2024},"citing_paper":{"arxiv_id":"2606.05005","last_updated":"2026-06-03T15:26:36Z","snapshot_observed_at":"2026-07-06T23:45:02.342193Z","submitted_at":"2026-06-03T15:26:36Z","title":"Neutrino mass constraints in interacting dark energy models after DESI DR2","version":1},"reference_index":151,"source":"pdf_text","source_observed_at":"2026-06-28T04:52:33.342231Z"},"links":{"cited_paper":"/paper/2404.15232","citing_paper":"/paper/2606.05005"},"observation_digest":"sha256:66cd3285a650d709c2f92003b317f595ca8a204a336a0244a39cfb2bfa31e2ec","observation_id":"0030bb84-fd26-45a7-80ca-51c592f4b886","resolution":{"observed_at":"2026-07-02T10:56:52.425874Z","resolver_source":"arxiv_id","status":"verified_exact"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-20T06:33:59.587034+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-20T06:33:59.587034+00:00","source":"crossref"},{"observed_at":"2026-08-20T06:33:54.927442+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":{"arxiv_id":"2404.15232","last_updated":"2024-12-19T16:25:49Z","snapshot_observed_at":"2026-08-16T13:58:27.312344Z","submitted_at":"2024-04-23T17:05:14Z","title":"Interacting Dark Energy after DESI Baryon Acoustic Oscillation measurements","version":2},"cited_work":{"arxiv_id":"2404.15232","doi":null,"metadata_source":"pith","pith_arxiv_id":"2404.15232","snapshot_observed_at":"2026-07-09T13:46:17.479123Z","title":"Giar` e, M","venue":"astro-ph.CO","work_id":"5be9e1ba-8076-41a9-b994-919073086747","year":2024},"citing_paper":{"arxiv_id":"2606.05539","last_updated":"2026-06-04T00:48:50Z","snapshot_observed_at":"2026-08-05T03:20:41.105304Z","submitted_at":"2026-06-04T00:48:50Z","title":"Dissipative Cosmology and the Nature of Dark Energy: Insights from Bulk Viscosity with DESI DR2 observations","version":1},"reference_index":68,"source":"pdf_text","source_observed_at":"2026-06-28T00:31:52.323240Z"},"links":{"cited_paper":"/paper/2404.15232","citing_paper":"/paper/2606.05539"},"observation_digest":"sha256:17966ea8052a0c3fd6282368c5696198bbe71ea3ba5aa3208ff3408fc7c295e3","observation_id":"dc7d1628-25e1-41c2-b84f-034889a04716","resolution":{"observed_at":"2026-07-02T14:17:03.631815Z","resolver_source":"arxiv_id","status":"verified_exact"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-20T06:33:59.587034+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-20T06:33:59.587034+00:00","source":"crossref"},{"observed_at":"2026-08-20T06:33:54.927442+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":{"arxiv_id":"2404.15232","last_updated":"2024-12-19T16:25:49Z","snapshot_observed_at":"2026-08-16T13:58:27.312344Z","submitted_at":"2024-04-23T17:05:14Z","title":"Interacting Dark Energy after DESI Baryon Acoustic Oscillation measurements","version":2},"cited_work":{"arxiv_id":"2404.15232","doi":null,"metadata_source":"pith","pith_arxiv_id":"2404.15232","snapshot_observed_at":"2026-07-09T13:46:17.479123Z","title":"Giar` e, M","venue":"astro-ph.CO","work_id":"5be9e1ba-8076-41a9-b994-919073086747","year":2024},"citing_paper":{"arxiv_id":"2606.09427","last_updated":"2026-07-28T09:24:20Z","snapshot_observed_at":"2026-08-16T22:07:17.720606Z","submitted_at":"2026-06-08T12:40:15Z","title":"Modifying $\\Lambda$CDM dynamics via out-of-equilibrium axions: reconciling SH0ES and DESI $H_0$ values","version":1},"reference_index":61,"source":"pdf_text","source_observed_at":"2026-06-27T15:53:35.003495Z"},"links":{"cited_paper":"/paper/2404.15232","citing_paper":"/paper/2606.09427"},"observation_digest":"sha256:8b62e753faf1b73f84a8c80af68999452616d225b77427686ef95e373443e960","observation_id":"2feaebf2-f0d7-4a6d-9508-7342f3281ef2","resolution":{"observed_at":"2026-07-03T02:27:35.312828Z","resolver_source":"arxiv_id","status":"metadata_mismatch"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-20T06:33:59.587034+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-20T06:33:59.587034+00:00","source":"crossref"},{"observed_at":"2026-08-20T06:33:54.927442+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":{"arxiv_id":"2404.15232","last_updated":"2024-12-19T16:25:49Z","snapshot_observed_at":"2026-08-16T13:58:27.312344Z","submitted_at":"2024-04-23T17:05:14Z","title":"Interacting Dark Energy after DESI Baryon Acoustic Oscillation measurements","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2404.15232","snapshot_observed_at":"2026-08-02T12:05:39.495259Z","title":"Sabogal, Rafael C","venue":null,"work_id":null,"year":2024},"citing_paper":{"arxiv_id":"2606.09427","last_updated":"2026-07-28T09:24:20Z","snapshot_observed_at":"2026-08-16T22:07:17.720606Z","submitted_at":"2026-06-08T12:40:15Z","title":"Modifying $\\Lambda$CDM dynamics via out-of-equilibrium axions: reconciling SH0ES and DESI $H_0$ values","version":2},"reference_index":61,"source":"pdf_text","source_observed_at":"2026-08-02T12:05:39.495259Z"},"links":{"cited_paper":"/paper/2404.15232","citing_paper":"/paper/2606.09427"},"observation_digest":"sha256:69409c57e4f46e1668ced0ef34ff811ab15255908bf22a1d214bbc37f6b00c08","observation_id":"7e3d21ea-b57b-46c5-93f8-230b9853a0d9","resolution":{"observed_at":"2026-08-02T12:05:39.495259Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2404.15232","last_updated":"2024-12-19T16:25:49Z","snapshot_observed_at":"2026-08-16T13:58:27.312344Z","submitted_at":"2024-04-23T17:05:14Z","title":"Interacting Dark Energy after DESI Baryon Acoustic Oscillation measurements","version":2},"cited_work":{"arxiv_id":"2404.15232","doi":null,"metadata_source":"pith","pith_arxiv_id":"2404.15232","snapshot_observed_at":"2026-07-09T13:46:17.479123Z","title":"Giar` e, M","venue":"astro-ph.CO","work_id":"5be9e1ba-8076-41a9-b994-919073086747","year":2024},"citing_paper":{"arxiv_id":"2606.19090","last_updated":"2026-06-17T13:58:39Z","snapshot_observed_at":"2026-07-06T23:54:27.624372Z","submitted_at":"2026-06-17T13:58:39Z","title":"Resolving the Hubble Tension in the Early Dark Energy Framework with JWST and DESI Data","version":1},"reference_index":52,"source":"pdf_text","source_observed_at":"2026-06-26T19:48:32.340111Z"},"links":{"cited_paper":"/paper/2404.15232","citing_paper":"/paper/2606.19090"},"observation_digest":"sha256:8bda412c071f1f22845b681713ecbde40bb53e999a0d1fafcbc8d66baa798a22","observation_id":"95acd21b-e667-41e9-907e-fc9e692e9452","resolution":{"observed_at":"2026-07-04T02:19:23.735673Z","resolver_source":"arxiv_id","status":"verified_exact"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-20T06:33:59.587034+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-20T06:33:59.587034+00:00","source":"crossref"},{"observed_at":"2026-08-20T06:33:54.927442+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":{"arxiv_id":"2404.15232","last_updated":"2024-12-19T16:25:49Z","snapshot_observed_at":"2026-08-16T13:58:27.312344Z","submitted_at":"2024-04-23T17:05:14Z","title":"Interacting Dark Energy after DESI Baryon Acoustic Oscillation measurements","version":2},"cited_work":{"arxiv_id":"2404.15232","doi":null,"metadata_source":"pith","pith_arxiv_id":"2404.15232","snapshot_observed_at":"2026-07-09T13:46:17.479123Z","title":"Giar` e, M","venue":"astro-ph.CO","work_id":"5be9e1ba-8076-41a9-b994-919073086747","year":2024},"citing_paper":{"arxiv_id":"2606.31362","last_updated":"2026-06-30T08:57:18Z","snapshot_observed_at":"2026-08-09T03:11:42.668077Z","submitted_at":"2026-06-30T08:57:18Z","title":"Running into tension: primordial black holes from ultra-slow-roll inflation, spectral running, and the Hubble tension","version":1},"reference_index":215,"source":"pdf_text","source_observed_at":"2026-07-01T04:31:47.886338Z"},"links":{"cited_paper":"/paper/2404.15232","citing_paper":"/paper/2606.31362"},"observation_digest":"sha256:d621683c537fd2355b3c91545929d79dd39948b834d8c3a57386003b847afc32","observation_id":"412f5266-af22-4ffc-86bf-e85dcf61a409","resolution":{"observed_at":"2026-07-01T11:25:45.477465Z","resolver_source":"arxiv_id","status":"verified_exact"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-20T06:33:59.587034+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-20T06:33:59.587034+00:00","source":"crossref"},{"observed_at":"2026-08-20T06:33:54.927442+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":{"arxiv_id":"2404.15232","last_updated":"2024-12-19T16:25:49Z","snapshot_observed_at":"2026-08-16T13:58:27.312344Z","submitted_at":"2024-04-23T17:05:14Z","title":"Interacting Dark Energy after DESI Baryon Acoustic Oscillation measurements","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2404.15232","snapshot_observed_at":"2026-07-12T04:18:55.037825Z","title":"Giar` e, M","venue":null,"work_id":null,"year":2024},"citing_paper":{"arxiv_id":"2607.03183","last_updated":"2026-07-03T10:38:35Z","snapshot_observed_at":"2026-08-18T07:54:15.383379Z","submitted_at":"2026-07-03T10:38:35Z","title":"Neutrino mass constraints in the Schwarzschild-de Sitter black-hole dark energy model with ACT DR6 and DESI DR2 data","version":1},"reference_index":94,"source":"pdf_text","source_observed_at":"2026-07-12T04:18:55.037825Z"},"links":{"cited_paper":"/paper/2404.15232","citing_paper":"/paper/2607.03183"},"observation_digest":"sha256:5084482762ef547e15edca840cced1be97e5264698f6cd921077b0d62069407f","observation_id":"763e0bbc-5f4c-4f83-85da-c6b73c76ef71","resolution":{"observed_at":"2026-07-12T04:18:55.037825Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2404.15232","last_updated":"2024-12-19T16:25:49Z","snapshot_observed_at":"2026-08-16T13:58:27.312344Z","submitted_at":"2024-04-23T17:05:14Z","title":"Interacting Dark Energy after DESI Baryon Acoustic Oscillation measurements","version":2},"cited_work":{"arxiv_id":"2404.15232","doi":null,"metadata_source":"pith","pith_arxiv_id":"2404.15232","snapshot_observed_at":"2026-07-09T13:46:17.479123Z","title":"Giar` e, M","venue":"astro-ph.CO","work_id":"5be9e1ba-8076-41a9-b994-919073086747","year":2024},"citing_paper":{"arxiv_id":"2607.06147","last_updated":"2026-07-07T11:15:39Z","snapshot_observed_at":"2026-08-07T05:12:27.762181Z","submitted_at":"2026-07-07T11:15:39Z","title":"Imprint of swampland-inspired coupled early dark energy","version":1},"reference_index":11,"source":"pdf_text","source_observed_at":"2026-07-08T15:47:53.145943Z"},"links":{"cited_paper":"/paper/2404.15232","citing_paper":"/paper/2607.06147"},"observation_digest":"sha256:e66a1e158494b83536ffdd9e72d1c647571bba4e732093d1ceb194cf616b113f","observation_id":"a896061b-68ac-460d-b7e5-5507edf1ce64","resolution":{"observed_at":"2026-07-08T15:55:04.963643Z","resolver_source":"local_arxiv","status":"verified_exact"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-20T06:33:59.587034+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-20T06:33:59.587034+00:00","source":"crossref"},{"observed_at":"2026-08-20T06:33:54.927442+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":{"arxiv_id":"2404.15232","last_updated":"2024-12-19T16:25:49Z","snapshot_observed_at":"2026-08-16T13:58:27.312344Z","submitted_at":"2024-04-23T17:05:14Z","title":"Interacting Dark Energy after DESI Baryon Acoustic Oscillation measurements","version":2},"cited_work":{"arxiv_id":"2404.15232","doi":null,"metadata_source":"pith","pith_arxiv_id":"2404.15232","snapshot_observed_at":"2026-07-09T13:46:17.479123Z","title":"Giar` e, M","venue":"astro-ph.CO","work_id":"5be9e1ba-8076-41a9-b994-919073086747","year":2024},"citing_paper":{"arxiv_id":"2607.07348","last_updated":"2026-07-08T12:38:37Z","snapshot_observed_at":"2026-08-18T22:51:54.826209Z","submitted_at":"2026-07-08T12:38:37Z","title":"Present Day Cosmic Acceleration from SDSS and DESI BAO: A Call for Finer Tomography of the DESI Bright Galaxy Survey","version":1},"reference_index":40,"source":"pdf_text","source_observed_at":"2026-07-09T13:44:49.684186Z"},"links":{"cited_paper":"/paper/2404.15232","citing_paper":"/paper/2607.07348"},"observation_digest":"sha256:185a2e0f8829efbdfd52efdd43cab0dce03c96f7cae010f3641fffc75ac26ec6","observation_id":"e98b5eb5-941a-43a9-90cc-07e9a3191eb9","resolution":{"observed_at":"2026-07-09T13:46:17.481323Z","resolver_source":"local_arxiv","status":"malformed_identifier"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-20T06:33:59.587034+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-20T06:33:59.587034+00:00","source":"crossref"},{"observed_at":"2026-08-20T06:33:54.927442+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":{"arxiv_id":"2404.15232","last_updated":"2024-12-19T16:25:49Z","snapshot_observed_at":"2026-08-16T13:58:27.312344Z","submitted_at":"2024-04-23T17:05:14Z","title":"Interacting Dark Energy after DESI Baryon Acoustic Oscillation measurements","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2404.15232","snapshot_observed_at":"2026-07-14T16:44:02.461654Z","title":"Giar` e, M","venue":null,"work_id":null,"year":2024},"citing_paper":{"arxiv_id":"2607.09732","last_updated":"2026-07-02T07:56:02Z","snapshot_observed_at":"2026-08-15T03:20:30.109454Z","submitted_at":"2026-07-02T07:56:02Z","title":"Late-time cosmological constraints on three holographic dark energy models with DESI DR2 BAO and Type Ia supernovae","version":1},"reference_index":33,"source":"pdf_text","source_observed_at":"2026-07-14T16:44:02.461654Z"},"links":{"cited_paper":"/paper/2404.15232","citing_paper":"/paper/2607.09732"},"observation_digest":"sha256:c69826c315d21637aab043471844815f9b561db85b44a63e4834f3cd8c19daaa","observation_id":"c82c0a0d-5e61-4e6f-9338-177f5cecac1e","resolution":{"observed_at":"2026-07-14T16:44:02.461654Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2404.15232","last_updated":"2024-12-19T16:25:49Z","snapshot_observed_at":"2026-08-16T13:58:27.312344Z","submitted_at":"2024-04-23T17:05:14Z","title":"Interacting Dark Energy after DESI Baryon Acoustic Oscillation measurements","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2404.15232","snapshot_observed_at":"2026-07-14T03:00:21.146194Z","title":"Giarè, M","venue":null,"work_id":null,"year":2024},"citing_paper":{"arxiv_id":"2607.11813","last_updated":"2026-07-13T17:09:56Z","snapshot_observed_at":"2026-08-20T23:47:45.102909Z","submitted_at":"2026-07-13T17:09:56Z","title":"Breaking the Dark Sector Degeneracy with Nonparametric Expansion--Growth Reconstruction","version":1},"reference_index":24,"source":"pdf_text","source_observed_at":"2026-07-14T03:00:21.146194Z"},"links":{"cited_paper":"/paper/2404.15232","citing_paper":"/paper/2607.11813"},"observation_digest":"sha256:9a60f3a6fb339d14ccdf6dbec4fc5cf72947046ab7dfb0ea4fbcae27bb52ce75","observation_id":"7f5fd74a-a52f-4515-a4be-cf318fd77473","resolution":{"observed_at":"2026-07-14T03:00:21.146194Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2404.15232","last_updated":"2024-12-19T16:25:49Z","snapshot_observed_at":"2026-08-16T13:58:27.312344Z","submitted_at":"2024-04-23T17:05:14Z","title":"Interacting Dark Energy after DESI Baryon Acoustic Oscillation measurements","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2404.15232","snapshot_observed_at":"2026-08-01T08:08:47.106381Z","title":"Giar` e, M","venue":null,"work_id":null,"year":2024},"citing_paper":{"arxiv_id":"2607.21244","last_updated":"2026-07-23T12:08:39Z","snapshot_observed_at":"2026-08-18T04:16:34.790019Z","submitted_at":"2026-07-23T12:08:39Z","title":"Hubble tension: the shape wall","version":1},"reference_index":141,"source":"pdf_text","source_observed_at":"2026-08-01T08:08:47.106381Z"},"links":{"cited_paper":"/paper/2404.15232","citing_paper":"/paper/2607.21244"},"observation_digest":"sha256:33c552b8e626dfead92c9244f67ade1545a6336a105290c9dc8bb67db62ef7a4","observation_id":"0ecc0348-0404-4908-b72f-958b10d7cf65","resolution":{"observed_at":"2026-08-01T08:08:47.106381Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2404.15232","last_updated":"2024-12-19T16:25:49Z","snapshot_observed_at":"2026-08-16T13:58:27.312344Z","submitted_at":"2024-04-23T17:05:14Z","title":"Interacting Dark Energy after DESI Baryon Acoustic Oscillation measurements","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2404.15232","snapshot_observed_at":"2026-08-01T07:20:08.240266Z","title":"Interacting Dark Energy after DESI Baryon Acoustic Oscillation Measurements,","venue":null,"work_id":null,"year":2024},"citing_paper":{"arxiv_id":"2607.21497","last_updated":"2026-08-14T16:46:31Z","snapshot_observed_at":"2026-08-19T23:10:52.542376Z","submitted_at":"2026-07-23T16:45:10Z","title":"Hubble tension: a short review of theoretical explanations","version":1},"reference_index":231,"source":"pdf_text","source_observed_at":"2026-08-01T07:20:08.240266Z"},"links":{"cited_paper":"/paper/2404.15232","citing_paper":"/paper/2607.21497"},"observation_digest":"sha256:f3295806fece32e1e57f449f939adce6f17cef9653d2fe20f0d743b10dda922f","observation_id":"378aef4a-9015-4ec1-8e4e-a5bd8b4201ec","resolution":{"observed_at":"2026-08-01T07:20:08.240266Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2404.15232","last_updated":"2024-12-19T16:25:49Z","snapshot_observed_at":"2026-08-16T13:58:27.312344Z","submitted_at":"2024-04-23T17:05:14Z","title":"Interacting Dark Energy after DESI Baryon Acoustic Oscillation measurements","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2404.15232","snapshot_observed_at":"2026-08-04T19:55:29.070461Z","title":"Giar` e, M","venue":null,"work_id":null,"year":2024},"citing_paper":{"arxiv_id":"2608.01844","last_updated":"2026-08-03T07:52:17Z","snapshot_observed_at":"2026-08-18T02:09:10.467296Z","submitted_at":"2026-08-03T07:52:17Z","title":"Revisiting Metastable Dark Energy in Light of DESI DR2 BAO and DESI DR1 Full-Shape Measurements","version":1},"reference_index":37,"source":"pdf_text","source_observed_at":"2026-08-04T19:55:29.070461Z"},"links":{"cited_paper":"/paper/2404.15232","citing_paper":"/paper/2608.01844"},"observation_digest":"sha256:eab51bfc4ee16a168b0da8b80c9021e3d8d33c35a23586491bfd60a480ef5f29","observation_id":"9416b0fc-7247-4a2e-bf54-e3f6d2e6bd47","resolution":{"observed_at":"2026-08-04T19:55:29.070461Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2404.15232","last_updated":"2024-12-19T16:25:49Z","snapshot_observed_at":"2026-08-16T13:58:27.312344Z","submitted_at":"2024-04-23T17:05:14Z","title":"Interacting Dark Energy after DESI Baryon Acoustic Oscillation measurements","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2404.15232","snapshot_observed_at":"2026-08-04T18:21:13.152445Z","title":"Giar` e, M","venue":null,"work_id":null,"year":2024},"citing_paper":{"arxiv_id":"2608.01919","last_updated":"2026-08-03T08:53:16Z","snapshot_observed_at":"2026-08-19T15:33:45.890004Z","submitted_at":"2026-08-03T08:53:16Z","title":"Boosting the optical depth to Thomson scattering with primordial black hole evaporation at high redshift","version":1},"reference_index":95,"source":"pdf_text","source_observed_at":"2026-08-04T18:21:13.152445Z"},"links":{"cited_paper":"/paper/2404.15232","citing_paper":"/paper/2608.01919"},"observation_digest":"sha256:afe8e1970e7c935655ce9e4c9242fc82c11af09ec7f155e964635a6f3acb9fb6","observation_id":"e55f62d4-35d0-40d7-a3ea-3bfcf699fc40","resolution":{"observed_at":"2026-08-04T18:21:13.152445Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}}],"links":{"evidence":"/evidence","html":"/paper/2404.15232/citation-record","integrity":"/paper/2404.15232/integrity","json":"/paper/2404.15232/citation-record.json","paper":"/paper/2404.15232"},"outbound":[],"paper":{"arxiv_id":"2404.15232","last_updated":"2024-12-19T16:25:49Z","latest_version":2,"primary_category":"astro-ph.CO","snapshot_observed_at":"2026-08-16T13:58:27.312344Z","submitted_at":"2024-04-23T17:05:14Z","title":"Interacting Dark Energy after DESI Baryon Acoustic Oscillation measurements"},"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":"2026-08-20T06:33:59.587034+00:00","source":"crossref"},{"observed_at":"2026-08-20T06:33:54.927442+00:00","source":"retraction_watch"}],"thesis":"As of 21 August 2026, this Paper Citation Record lists 0 of 0 outbound references and 67 inbound Pith citation observations for arXiv:2404.15232."}