{"as_of":"2026-08-13T05:49:00Z","caps":{"database_statements":6,"inbound":100,"outbound":100},"context_digest":"sha256:09c904e86aa8f0d06d125a516f62c875f82272dd1e0c80d92bccfa539912036a","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":32,"lane":"standing_notices","note":"One-hop event checks from named stored sources.","records_observed":32,"source":"scholarly_work_events, retraction_status_cache","source_observed_at":"2026-08-12T06:34:41.77262+00:00","state":"measured"},{"denominator":32,"lane":"inbound_itemization","note":"Pith citing papers itemized under the disclosed page cap.","records_observed":32,"source":"paper_references, paper_reference_links","source_observed_at":"2026-08-11T19:40:50.825329Z","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":"2026-07-08T15:55:05.042750Z","state":"measured"}],"external_citation_measurements":[],"inbound":[{"citation":{"cited_paper":{"arxiv_id":"2411.08639","last_updated":"2025-05-04T13:39:59Z","snapshot_observed_at":"2026-08-12T21:27:31.566500Z","submitted_at":"2024-11-13T14:29:02Z","title":"Revisiting holographic dark energy after DESI 2024","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2411.08639","snapshot_observed_at":"2026-08-11T19:40:50.825329Z","title":"Revisiting holographic dark energy after DESI 2024.arXiv 2024, arXiv:2411.08639v1","venue":null,"work_id":null,"year":2024},"citing_paper":{"arxiv_id":"2412.06873","last_updated":"2025-03-06T12:14:11Z","snapshot_observed_at":"2026-08-12T09:39:55.857865Z","submitted_at":"2024-12-09T14:12:34Z","title":"Revisiting holographic dark energy from the perspective of multi-messenger gravitational wave astronomy: future joint observations with short gamma-ray bursts","version":2},"reference_index":31,"source":"pdf_text","source_observed_at":"2026-08-11T19:40:50.825329Z"},"links":{"cited_paper":"/paper/2411.08639","citing_paper":"/paper/2412.06873"},"observation_digest":"sha256:09f6b1feede7064898cb8945b4e7d16e51dd427b72cca16244090b21cd2ac1b5","observation_id":"ad447a3c-5acd-446b-81cf-50443fd21d92","resolution":{"observed_at":"2026-08-11T19:40:50.825329Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2411.08639","last_updated":"2025-05-04T13:39:59Z","snapshot_observed_at":"2026-08-12T21:27:31.566500Z","submitted_at":"2024-11-13T14:29:02Z","title":"Revisiting holographic dark energy after DESI 2024","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2411.08639","snapshot_observed_at":"2026-08-11T17:28:35.321627Z","title":"Li, Y.-H","venue":null,"work_id":null,"year":2024},"citing_paper":{"arxiv_id":"2412.09064","last_updated":"2025-06-24T01:24:27Z","snapshot_observed_at":"2026-08-12T15:08:50.818044Z","submitted_at":"2024-12-12T08:51:54Z","title":"A comprehensive numerical study on four categories of holographic dark energy models","version":3},"reference_index":108,"source":"pdf_text","source_observed_at":"2026-08-11T17:28:35.321627Z"},"links":{"cited_paper":"/paper/2411.08639","citing_paper":"/paper/2412.09064"},"observation_digest":"sha256:14a73b76aacae7fd8d2bbb28135951fe28f1cd660c630a706c9c1b36121c5643","observation_id":"9243e175-ff4b-4013-aca4-3ed199677385","resolution":{"observed_at":"2026-08-11T17:28:35.321627Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2411.08639","last_updated":"2025-05-04T13:39:59Z","snapshot_observed_at":"2026-08-12T21:27:31.566500Z","submitted_at":"2024-11-13T14:29:02Z","title":"Revisiting holographic dark energy after DESI 2024","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2411.08639","snapshot_observed_at":"2026-08-11T13:41:23.863131Z","title":"Li, Y .-H","venue":null,"work_id":null,"year":2024},"citing_paper":{"arxiv_id":"2412.12905","last_updated":"2025-01-25T08:30:04Z","snapshot_observed_at":"2026-08-11T13:34:44.390307Z","submitted_at":"2024-12-17T13:31:15Z","title":"DESI and SNe: Dynamical Dark Energy, $\\Omega_m$ Tension or Systematics?","version":2},"reference_index":81,"source":"pdf_text","source_observed_at":"2026-08-11T13:41:23.863131Z"},"links":{"cited_paper":"/paper/2411.08639","citing_paper":"/paper/2412.12905"},"observation_digest":"sha256:f066b82ec84fef7447fe2dc5e6c4f8308c26ca0464e8f0a3ac99442d70f6c48f","observation_id":"4dcf575c-8f15-4206-a70a-b4685909d701","resolution":{"observed_at":"2026-08-11T13:41:23.863131Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2411.08639","last_updated":"2025-05-04T13:39:59Z","snapshot_observed_at":"2026-08-12T21:27:31.566500Z","submitted_at":"2024-11-13T14:29:02Z","title":"Revisiting holographic dark energy after DESI 2024","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2411.08639","snapshot_observed_at":"2026-08-10T22:00:59.874362Z","title":"Li, Y.-H","venue":null,"work_id":null,"year":2024},"citing_paper":{"arxiv_id":"2501.03480","last_updated":"2025-07-02T14:03:15Z","snapshot_observed_at":"2026-08-12T17:48:55.146084Z","submitted_at":"2025-01-07T02:51:33Z","title":"Is excess smoothing of Planck CMB ansiotropy data partially responsible for evidence for dark energy dynamics in other $w(z)$CDM parametrizations?","version":2},"reference_index":51,"source":"pdf_text","source_observed_at":"2026-08-10T22:00:59.874362Z"},"links":{"cited_paper":"/paper/2411.08639","citing_paper":"/paper/2501.03480"},"observation_digest":"sha256:608da4d90502a2d98cf6b7941d928c3c0a531a22a8a5677bf6e85fbd7e5c7f6f","observation_id":"33e5b1f7-5ab8-4774-8769-a9b681d288ad","resolution":{"observed_at":"2026-08-10T22:00:59.874362Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2411.08639","last_updated":"2025-05-04T13:39:59Z","snapshot_observed_at":"2026-08-12T21:27:31.566500Z","submitted_at":"2024-11-13T14:29:02Z","title":"Revisiting holographic dark energy after DESI 2024","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2411.08639","snapshot_observed_at":"2026-08-08T23:12:26.131843Z","title":"Revisiting holographic dark energy after DESI 2024,","venue":null,"work_id":null,"year":2025},"citing_paper":{"arxiv_id":"2502.04212","last_updated":"2025-07-17T16:27:03Z","snapshot_observed_at":"2026-08-09T04:53:21.314754Z","submitted_at":"2025-02-06T16:51:39Z","title":"The DESI DR1/DR2 evidence for dynamical dark energy is biased by low-redshift supernovae","version":5},"reference_index":52,"source":"pdf_text","source_observed_at":"2026-08-08T23:12:26.131843Z"},"links":{"cited_paper":"/paper/2411.08639","citing_paper":"/paper/2502.04212"},"observation_digest":"sha256:024246f3d9ded66ebfd7a9b99c62e3fc4356c533c362edf351239b3db64a8267","observation_id":"8b7fa834-9f64-4c0e-b2ab-aac483e2d638","resolution":{"observed_at":"2026-08-08T23:12:26.131843Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2411.08639","last_updated":"2025-05-04T13:39:59Z","snapshot_observed_at":"2026-08-12T21:27:31.566500Z","submitted_at":"2024-11-13T14:29:02Z","title":"Revisiting holographic dark energy after DESI 2024","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2411.08639","snapshot_observed_at":"2026-08-08T22:04:59.517428Z","title":"Li, Y.-H","venue":null,"work_id":null,"year":2024},"citing_paper":{"arxiv_id":"2502.04641","last_updated":"2025-02-18T07:50:34Z","snapshot_observed_at":"2026-08-12T23:36:23.357886Z","submitted_at":"2025-02-07T03:58:52Z","title":"Dark energy and lensing anomaly in Planck CMB data","version":2},"reference_index":51,"source":"pdf_text","source_observed_at":"2026-08-08T22:04:59.517428Z"},"links":{"cited_paper":"/paper/2411.08639","citing_paper":"/paper/2502.04641"},"observation_digest":"sha256:2d1dfd9e5f7f97e4c8972233b78895c9e8fe09d98d62b9507d4cdaf10fb4bbd7","observation_id":"d725cdde-3504-492b-8596-2d824371be28","resolution":{"observed_at":"2026-08-08T22:04:59.517428Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2411.08639","last_updated":"2025-05-04T13:39:59Z","snapshot_observed_at":"2026-08-12T21:27:31.566500Z","submitted_at":"2024-11-13T14:29:02Z","title":"Revisiting holographic dark energy after DESI 2024","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2411.08639","snapshot_observed_at":"2026-08-07T18:51:44.108743Z","title":"Revisit- ing holographic dark energy after DESI 2024,","venue":null,"work_id":null,"year":2024},"citing_paper":{"arxiv_id":"2502.10264","last_updated":"2025-04-10T17:38:46Z","snapshot_observed_at":"2026-08-09T09:16:02.090706Z","submitted_at":"2025-02-14T16:17:23Z","title":"An overview of what current data can (and cannot yet) say about evolving dark energy","version":2},"reference_index":223,"source":"pdf_text","source_observed_at":"2026-08-07T18:51:44.108743Z"},"links":{"cited_paper":"/paper/2411.08639","citing_paper":"/paper/2502.10264"},"observation_digest":"sha256:4551d74d65e5cba288e980118532e639403e4abdda4da15fd968080d0786a7ef","observation_id":"05601f15-1e6b-4a1c-92ed-8351c02aa5fc","resolution":{"observed_at":"2026-08-07T18:51:44.108743Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2411.08639","last_updated":"2025-05-04T13:39:59Z","snapshot_observed_at":"2026-08-12T21:27:31.566500Z","submitted_at":"2024-11-13T14:29:02Z","title":"Revisiting holographic dark energy after DESI 2024","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2411.08639","snapshot_observed_at":"2026-08-07T10:52:56.335341Z","title":null,"venue":null,"work_id":null,"year":null},"citing_paper":{"arxiv_id":"2506.04306","last_updated":"2025-06-04T17:51:05Z","snapshot_observed_at":"2026-08-07T14:10:01.304994Z","submitted_at":"2025-06-04T17:51:05Z","title":"Can the universe experience an AdS landscape since matter-radiation equality?","version":1},"reference_index":48,"source":"pdf_text","source_observed_at":"2026-08-07T10:52:56.335341Z"},"links":{"cited_paper":"/paper/2411.08639","citing_paper":"/paper/2506.04306"},"observation_digest":"sha256:860458bfb7a35aa6682d12c6a9f290830e2684338800a8e4708c5a70aab05977","observation_id":"c0fabfa2-a7ed-43e0-a17b-9b4ddf82644e","resolution":{"observed_at":"2026-08-07T10:52:56.335341Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2411.08639","last_updated":"2025-05-04T13:39:59Z","snapshot_observed_at":"2026-08-12T21:27:31.566500Z","submitted_at":"2024-11-13T14:29:02Z","title":"Revisiting holographic dark energy after DESI 2024","version":2},"cited_work":{"arxiv_id":"2411.08639","doi":null,"metadata_source":"pith","pith_arxiv_id":"2411.08639","snapshot_observed_at":"2026-07-08T15:55:05.042750Z","title":"Li, Y.-H","venue":"astro-ph.CO","work_id":"51d54d56-8f5a-429d-bc95-c12c1201edf1","year":2024},"citing_paper":{"arxiv_id":"2507.01070","last_updated":"2025-08-04T07:24:35Z","snapshot_observed_at":"2026-08-08T03:11:50.344387Z","submitted_at":"2025-07-01T07:51:56Z","title":"Barrow holographic dark energy interacting model in the presence of radiation and matter","version":2},"reference_index":25,"source":"pdf_text","source_observed_at":"2026-05-19T07:03:29.207286Z"},"links":{"cited_paper":"/paper/2411.08639","citing_paper":"/paper/2507.01070"},"observation_digest":"sha256:fa533637d8ed2ed643b60e460b0c0c7bfd2513545f30c5ad8ae0f163bd014a4a","observation_id":"f14a923e-e0d7-47c8-9637-8a0456f15460","resolution":{"observed_at":"2026-05-19T07:07:07.847917Z","resolver_source":"arxiv_id","status":"verified_exact"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-12T06:34:41.77262+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-12T06:34:41.77262+00:00","source":"crossref"},{"observed_at":"2026-08-12T06:34:36.333875+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":{"arxiv_id":"2411.08639","last_updated":"2025-05-04T13:39:59Z","snapshot_observed_at":"2026-08-12T21:27:31.566500Z","submitted_at":"2024-11-13T14:29:02Z","title":"Revisiting holographic dark energy after DESI 2024","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2411.08639","snapshot_observed_at":"2026-08-06T18:36:59.456112Z","title":"Li, Y.-H","venue":null,"work_id":null,"year":2025},"citing_paper":{"arxiv_id":"2507.07798","last_updated":"2025-07-10T14:26:06Z","snapshot_observed_at":"2026-08-10T05:27:39.960371Z","submitted_at":"2025-07-10T14:26:06Z","title":"Exploring non-cold dark matter in a scenario of dynamical dark energy with DESI DR2 data","version":1},"reference_index":34,"source":"pdf_text","source_observed_at":"2026-08-06T18:36:59.456112Z"},"links":{"cited_paper":"/paper/2411.08639","citing_paper":"/paper/2507.07798"},"observation_digest":"sha256:fb4ed745ac2d4ded80ccbdaaf73d350a64cf1275e23ad6a2df0d2b4a0ccb1602","observation_id":"69fb7fa8-9650-4802-bbf4-1b2312973672","resolution":{"observed_at":"2026-08-06T18:36:59.456112Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2411.08639","last_updated":"2025-05-04T13:39:59Z","snapshot_observed_at":"2026-08-12T21:27:31.566500Z","submitted_at":"2024-11-13T14:29:02Z","title":"Revisiting holographic dark energy after DESI 2024","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2411.08639","snapshot_observed_at":"2026-08-06T15:12:33.619328Z","title":"Li, Y.-H","venue":null,"work_id":null,"year":2025},"citing_paper":{"arxiv_id":"2507.16589","last_updated":"2026-06-23T13:43:52Z","snapshot_observed_at":"2026-08-08T06:56:16.966820Z","submitted_at":"2025-07-22T13:45:38Z","title":"Cosmological preference for a positive neutrino mass at 2.7$\\sigma$: A joint analysis of DESI DR2, DESY5, and DESY1 data","version":3},"reference_index":24,"source":"pdf_text","source_observed_at":"2026-08-06T15:12:33.619328Z"},"links":{"cited_paper":"/paper/2411.08639","citing_paper":"/paper/2507.16589"},"observation_digest":"sha256:77edbd63d6b823b8a0047f5215995b096f25e12927ade3c1818c5864a18db4ff","observation_id":"f030daf4-ba3a-4928-a2f3-d119280002d7","resolution":{"observed_at":"2026-08-06T15:12:33.619328Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2411.08639","last_updated":"2025-05-04T13:39:59Z","snapshot_observed_at":"2026-08-12T21:27:31.566500Z","submitted_at":"2024-11-13T14:29:02Z","title":"Revisiting holographic dark energy after DESI 2024","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2411.08639","snapshot_observed_at":"2026-08-06T12:01:08.767689Z","title":"Li, Y.-H","venue":null,"work_id":null,"year":2024},"citing_paper":{"arxiv_id":"2507.22292","last_updated":"2026-07-13T23:28:39Z","snapshot_observed_at":"2026-08-10T10:18:35.082681Z","submitted_at":"2025-07-29T23:56:48Z","title":"How Holographic is the Dark Energy? A Spline Nodal reconstruction approach","version":2},"reference_index":66,"source":"pdf_text","source_observed_at":"2026-08-06T12:01:08.767689Z"},"links":{"cited_paper":"/paper/2411.08639","citing_paper":"/paper/2507.22292"},"observation_digest":"sha256:7c052faf6587692f66b59e140e58f56be8b9acea76a98f753d6a04311ce8f7dd","observation_id":"9be4c1cb-77c6-4d61-9ea3-062ffd456abf","resolution":{"observed_at":"2026-08-06T12:01:08.767689Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2411.08639","last_updated":"2025-05-04T13:39:59Z","snapshot_observed_at":"2026-08-12T21:27:31.566500Z","submitted_at":"2024-11-13T14:29:02Z","title":"Revisiting holographic dark energy after DESI 2024","version":2},"cited_work":{"arxiv_id":"2411.08639","doi":null,"metadata_source":"pith","pith_arxiv_id":"2411.08639","snapshot_observed_at":"2026-07-08T15:55:05.042750Z","title":"Li, Y.-H","venue":"astro-ph.CO","work_id":"51d54d56-8f5a-429d-bc95-c12c1201edf1","year":2024},"citing_paper":{"arxiv_id":"2510.03779","last_updated":"2026-02-17T10:47:14Z","snapshot_observed_at":"2026-08-11T15:12:03.651068Z","submitted_at":"2025-10-04T11:08:41Z","title":"Beyond CPL: Evidence for dynamical dark energy in three-parameter models","version":3},"reference_index":54,"source":"pdf_text","source_observed_at":"2026-05-18T10:45:16.985887Z"},"links":{"cited_paper":"/paper/2411.08639","citing_paper":"/paper/2510.03779"},"observation_digest":"sha256:d519540e749e549e5734dce3111cbf6d98c1db26974e0d591d1bc0c49a6c83e2","observation_id":"566e281e-8bc2-4e42-a830-7b987c877862","resolution":{"observed_at":"2026-05-18T10:46:16.642731Z","resolver_source":"arxiv_id","status":"verified_exact"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-12T06:34:41.77262+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-12T06:34:41.77262+00:00","source":"crossref"},{"observed_at":"2026-08-12T06:34:36.333875+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":{"arxiv_id":"2411.08639","last_updated":"2025-05-04T13:39:59Z","snapshot_observed_at":"2026-08-12T21:27:31.566500Z","submitted_at":"2024-11-13T14:29:02Z","title":"Revisiting holographic dark energy after DESI 2024","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2411.08639","snapshot_observed_at":"2026-08-04T09:59:17.046982Z","title":"Li, Y.-H","venue":null,"work_id":null,"year":2025},"citing_paper":{"arxiv_id":"2510.12627","last_updated":"2026-06-20T07:00:45Z","snapshot_observed_at":"2026-08-12T13:22:12.009948Z","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":69,"source":"pdf_text","source_observed_at":"2026-08-04T09:59:17.046982Z"},"links":{"cited_paper":"/paper/2411.08639","citing_paper":"/paper/2510.12627"},"observation_digest":"sha256:371a30dbe654c18dc061d64954dfa7ba9cba189df5fea11523d72a6646793c51","observation_id":"653bfe8c-9c52-4fc8-8832-1071e4f75588","resolution":{"observed_at":"2026-08-04T09:59:17.046982Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2411.08639","last_updated":"2025-05-04T13:39:59Z","snapshot_observed_at":"2026-08-12T21:27:31.566500Z","submitted_at":"2024-11-13T14:29:02Z","title":"Revisiting holographic dark energy after DESI 2024","version":2},"cited_work":{"arxiv_id":"2411.08639","doi":null,"metadata_source":"pith","pith_arxiv_id":"2411.08639","snapshot_observed_at":"2026-07-08T15:55:05.042750Z","title":"Li, Y.-H","venue":"astro-ph.CO","work_id":"51d54d56-8f5a-429d-bc95-c12c1201edf1","year":2024},"citing_paper":{"arxiv_id":"2510.21521","last_updated":"2026-03-24T13:25:09Z","snapshot_observed_at":"2026-07-06T02:11:23.670680Z","submitted_at":"2025-10-24T14:43:09Z","title":"Synergy between CSST and third-generation gravitational-wave detectors: Inferring cosmological parameters using cross-correlation of dark sirens and galaxies","version":2},"reference_index":20,"source":"pdf_text","source_observed_at":"2026-05-18T04:48:55.126852Z"},"links":{"cited_paper":"/paper/2411.08639","citing_paper":"/paper/2510.21521"},"observation_digest":"sha256:2dd8030cd2848eea551e91808356f824807f59528d20c87048c5bfb3e825775b","observation_id":"f9bb374e-65d4-465f-81de-6c261a54f9f4","resolution":{"observed_at":"2026-05-18T04:50:53.823771Z","resolver_source":"arxiv_id","status":"verified_exact"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-12T06:34:41.77262+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-12T06:34:41.77262+00:00","source":"crossref"},{"observed_at":"2026-08-12T06:34:36.333875+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":{"arxiv_id":"2411.08639","last_updated":"2025-05-04T13:39:59Z","snapshot_observed_at":"2026-08-12T21:27:31.566500Z","submitted_at":"2024-11-13T14:29:02Z","title":"Revisiting holographic dark energy after DESI 2024","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2411.08639","snapshot_observed_at":"2026-08-04T07:19:40.260989Z","title":"Li, Y.-H","venue":null,"work_id":null,"year":2025},"citing_paper":{"arxiv_id":"2510.26355","last_updated":"2026-07-07T01:20:38Z","snapshot_observed_at":"2026-08-12T22:27:53.420894Z","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":94,"source":"pdf_text","source_observed_at":"2026-08-04T07:19:40.260989Z"},"links":{"cited_paper":"/paper/2411.08639","citing_paper":"/paper/2510.26355"},"observation_digest":"sha256:4d2692a0469f420b5de7eb03ad82fc7430e599f86ccb61e4c93a244cd2648464","observation_id":"868f3853-4f67-4959-b834-0654d50a120d","resolution":{"observed_at":"2026-08-04T07:19:40.260989Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2411.08639","last_updated":"2025-05-04T13:39:59Z","snapshot_observed_at":"2026-08-12T21:27:31.566500Z","submitted_at":"2024-11-13T14:29:02Z","title":"Revisiting holographic dark energy after DESI 2024","version":2},"cited_work":{"arxiv_id":"2411.08639","doi":null,"metadata_source":"pith","pith_arxiv_id":"2411.08639","snapshot_observed_at":"2026-07-08T15:55:05.042750Z","title":"Li, Y.-H","venue":"astro-ph.CO","work_id":"51d54d56-8f5a-429d-bc95-c12c1201edf1","year":2024},"citing_paper":{"arxiv_id":"2511.09467","last_updated":"2026-03-30T07:50:13Z","snapshot_observed_at":"2026-08-11T14:45:58.475436Z","submitted_at":"2025-11-12T16:39:04Z","title":"Revisiting the Hubble tension problem in the framework of holographic dark energy","version":2},"reference_index":98,"source":"pdf_text","source_observed_at":"2026-05-17T22:17:32.138764Z"},"links":{"cited_paper":"/paper/2411.08639","citing_paper":"/paper/2511.09467"},"observation_digest":"sha256:5ac9ffa7f5aff1ab1c00a98b904191860a990c9ea970e4335331986963a0ff75","observation_id":"fae009f2-d90b-4952-9ce8-779970b38ba5","resolution":{"observed_at":"2026-05-17T22:20:23.559747Z","resolver_source":"arxiv_id","status":"verified_exact"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-12T06:34:41.77262+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-12T06:34:41.77262+00:00","source":"crossref"},{"observed_at":"2026-08-12T06:34:36.333875+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":{"arxiv_id":"2411.08639","last_updated":"2025-05-04T13:39:59Z","snapshot_observed_at":"2026-08-12T21:27:31.566500Z","submitted_at":"2024-11-13T14:29:02Z","title":"Revisiting holographic dark energy after DESI 2024","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2411.08639","snapshot_observed_at":"2026-08-03T14:40:55.447820Z","title":"Li, Y.-H","venue":null,"work_id":null,"year":2025},"citing_paper":{"arxiv_id":"2512.19888","last_updated":"2026-06-18T12:16:03Z","snapshot_observed_at":"2026-08-07T04:04:01.596809Z","submitted_at":"2025-12-22T21:27:32Z","title":"Observational constraints on early time non-phantom behaviour of dynamical dark energy","version":2},"reference_index":53,"source":"pdf_text","source_observed_at":"2026-08-03T14:40:55.447820Z"},"links":{"cited_paper":"/paper/2411.08639","citing_paper":"/paper/2512.19888"},"observation_digest":"sha256:033c451798b9dea92b9416674997c1571a6ff2a524153a4fd4326d7dc9e5df42","observation_id":"fd53ccf2-8951-45ce-9735-0ba22c1aecd7","resolution":{"observed_at":"2026-08-03T14:40:55.447820Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2411.08639","last_updated":"2025-05-04T13:39:59Z","snapshot_observed_at":"2026-08-12T21:27:31.566500Z","submitted_at":"2024-11-13T14:29:02Z","title":"Revisiting holographic dark energy after DESI 2024","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2411.08639","snapshot_observed_at":"2026-08-03T11:11:48.686695Z","title":"Li, Y.-H","venue":null,"work_id":null,"year":2025},"citing_paper":{"arxiv_id":"2601.07361","last_updated":"2026-07-15T07:08:06Z","snapshot_observed_at":"2026-08-13T05:33:14.828344Z","submitted_at":"2026-01-12T09:36:30Z","title":"Robust Preference for Dark Sector Interactions","version":2},"reference_index":22,"source":"pdf_text","source_observed_at":"2026-08-03T11:11:48.686695Z"},"links":{"cited_paper":"/paper/2411.08639","citing_paper":"/paper/2601.07361"},"observation_digest":"sha256:a0c11323b24faa416218c58395e6786ce41503a5529510357a701ac096bdc809","observation_id":"90ccf01e-248f-4adf-aa30-6424f0dd6a2b","resolution":{"observed_at":"2026-08-03T11:11:48.686695Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2411.08639","last_updated":"2025-05-04T13:39:59Z","snapshot_observed_at":"2026-08-12T21:27:31.566500Z","submitted_at":"2024-11-13T14:29:02Z","title":"Revisiting holographic dark energy after DESI 2024","version":2},"cited_work":{"arxiv_id":"2411.08639","doi":null,"metadata_source":"pith","pith_arxiv_id":"2411.08639","snapshot_observed_at":"2026-07-08T15:55:05.042750Z","title":"Li, Y.-H","venue":"astro-ph.CO","work_id":"51d54d56-8f5a-429d-bc95-c12c1201edf1","year":2024},"citing_paper":{"arxiv_id":"2602.03110","last_updated":"2026-04-28T09:37:14Z","snapshot_observed_at":"2026-08-09T16:54:12.160048Z","submitted_at":"2026-02-03T05:11:50Z","title":"Evidence for deviation in gravitational light deflection from general relativity at cosmological scales with KiDS-Legacy and CMB lensing","version":2},"reference_index":58,"source":"pdf_text","source_observed_at":"2026-05-16T08:17:34.164338Z"},"links":{"cited_paper":"/paper/2411.08639","citing_paper":"/paper/2602.03110"},"observation_digest":"sha256:f5f84bad5ac52ee54e980856161c1bbf3ca0666a9100d3f3be23455030f6c8da","observation_id":"94fb8cc2-da09-4766-b33e-1ebfb0624ac6","resolution":{"observed_at":"2026-05-16T08:17:35.630881Z","resolver_source":"arxiv_id","status":"verified_exact"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-12T06:34:41.77262+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-12T06:34:41.77262+00:00","source":"crossref"},{"observed_at":"2026-08-12T06:34:36.333875+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":{"arxiv_id":"2411.08639","last_updated":"2025-05-04T13:39:59Z","snapshot_observed_at":"2026-08-12T21:27:31.566500Z","submitted_at":"2024-11-13T14:29:02Z","title":"Revisiting holographic dark energy after DESI 2024","version":2},"cited_work":{"arxiv_id":"2411.08639","doi":null,"metadata_source":"pith","pith_arxiv_id":"2411.08639","snapshot_observed_at":"2026-07-08T15:55:05.042750Z","title":"Li, Y.-H","venue":"astro-ph.CO","work_id":"51d54d56-8f5a-429d-bc95-c12c1201edf1","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":125,"source":"pdf_text","source_observed_at":"2026-05-15T13:14:03.491513Z"},"links":{"cited_paper":"/paper/2411.08639","citing_paper":"/paper/2603.10787"},"observation_digest":"sha256:6c71dc155d7a115cdd111bb8a168505a4b776c47bea91f924c8dfa2af25fdf49","observation_id":"d3d6f401-674c-45a6-9287-8c7b5c93465f","resolution":{"observed_at":"2026-05-15T13:15:49.943931Z","resolver_source":"arxiv_id","status":"verified_exact"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-12T06:34:41.77262+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-12T06:34:41.77262+00:00","source":"crossref"},{"observed_at":"2026-08-12T06:34:36.333875+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":{"arxiv_id":"2411.08639","last_updated":"2025-05-04T13:39:59Z","snapshot_observed_at":"2026-08-12T21:27:31.566500Z","submitted_at":"2024-11-13T14:29:02Z","title":"Revisiting holographic dark energy after DESI 2024","version":2},"cited_work":{"arxiv_id":"2411.08639","doi":null,"metadata_source":"pith","pith_arxiv_id":"2411.08639","snapshot_observed_at":"2026-07-08T15:55:05.042750Z","title":"Li, Y.-H","venue":"astro-ph.CO","work_id":"51d54d56-8f5a-429d-bc95-c12c1201edf1","year":2024},"citing_paper":{"arxiv_id":"2603.21125","last_updated":"2026-03-22T08:46:57Z","snapshot_observed_at":"2026-08-11T04:11:48.474892Z","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":34,"source":"pdf_text","source_observed_at":"2026-05-15T01:30:47.614992Z"},"links":{"cited_paper":"/paper/2411.08639","citing_paper":"/paper/2603.21125"},"observation_digest":"sha256:1abeb6d0c760bdee4809c6f97ba01d8b5d1353684916f7f38dc82a1a15508b34","observation_id":"e1a39c2d-1073-475b-ba91-9a8d281d0578","resolution":{"observed_at":"2026-05-15T01:33:27.438902Z","resolver_source":"arxiv_id","status":"verified_exact"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-12T06:34:41.77262+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-12T06:34:41.77262+00:00","source":"crossref"},{"observed_at":"2026-08-12T06:34:36.333875+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":{"arxiv_id":"2411.08639","last_updated":"2025-05-04T13:39:59Z","snapshot_observed_at":"2026-08-12T21:27:31.566500Z","submitted_at":"2024-11-13T14:29:02Z","title":"Revisiting holographic dark energy after DESI 2024","version":2},"cited_work":{"arxiv_id":"2411.08639","doi":null,"metadata_source":"pith","pith_arxiv_id":"2411.08639","snapshot_observed_at":"2026-07-08T15:55:05.042750Z","title":"Li, Y.-H","venue":"astro-ph.CO","work_id":"51d54d56-8f5a-429d-bc95-c12c1201edf1","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":56,"source":"pdf_text","source_observed_at":"2026-05-08T05:38:44.860590Z"},"links":{"cited_paper":"/paper/2411.08639","citing_paper":"/paper/2604.23492"},"observation_digest":"sha256:7211963eed0417edb4e74ef50edad8f3a58d1cea2aec2faa1c4a0726d3b1ed2e","observation_id":"ac40267f-9caf-494e-b499-e499418dd0cd","resolution":{"observed_at":"2026-05-11T21:26:15.816807Z","resolver_source":"arxiv_id","status":"metadata_mismatch"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-12T06:34:41.77262+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-12T06:34:41.77262+00:00","source":"crossref"},{"observed_at":"2026-08-12T06:34:36.333875+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":{"arxiv_id":"2411.08639","last_updated":"2025-05-04T13:39:59Z","snapshot_observed_at":"2026-08-12T21:27:31.566500Z","submitted_at":"2024-11-13T14:29:02Z","title":"Revisiting holographic dark energy after DESI 2024","version":2},"cited_work":{"arxiv_id":"2411.08639","doi":null,"metadata_source":"pith","pith_arxiv_id":"2411.08639","snapshot_observed_at":"2026-07-08T15:55:05.042750Z","title":"Li, Y.-H","venue":"astro-ph.CO","work_id":"51d54d56-8f5a-429d-bc95-c12c1201edf1","year":2024},"citing_paper":{"arxiv_id":"2605.21310","last_updated":"2026-05-20T15:37:58Z","snapshot_observed_at":"2026-08-02T18:34:09.495996Z","submitted_at":"2026-05-20T15:37:58Z","title":"Contrastive self-supervised convolutional autoencoder for core-collapse supernova gravitational-wave detection","version":1},"reference_index":50,"source":"pdf_text","source_observed_at":"2026-05-21T03:33:53.198336Z"},"links":{"cited_paper":"/paper/2411.08639","citing_paper":"/paper/2605.21310"},"observation_digest":"sha256:d2b38163fa1e61c5853c55db0d0502db6d05ac0f51068b4298b9ac4863e3d0db","observation_id":"f0f49c5b-6e2f-4708-82d6-0a206422d943","resolution":{"observed_at":"2026-05-21T03:33:56.368474Z","resolver_source":"arxiv_id","status":"verified_exact"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-12T06:34:41.77262+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-12T06:34:41.77262+00:00","source":"crossref"},{"observed_at":"2026-08-12T06:34:36.333875+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":{"arxiv_id":"2411.08639","last_updated":"2025-05-04T13:39:59Z","snapshot_observed_at":"2026-08-12T21:27:31.566500Z","submitted_at":"2024-11-13T14:29:02Z","title":"Revisiting holographic dark energy after DESI 2024","version":2},"cited_work":{"arxiv_id":"2411.08639","doi":null,"metadata_source":"pith","pith_arxiv_id":"2411.08639","snapshot_observed_at":"2026-07-08T15:55:05.042750Z","title":"Li, Y.-H","venue":"astro-ph.CO","work_id":"51d54d56-8f5a-429d-bc95-c12c1201edf1","year":2024},"citing_paper":{"arxiv_id":"2606.03634","last_updated":"2026-06-02T13:31:54Z","snapshot_observed_at":"2026-07-06T23:43:50.943530Z","submitted_at":"2026-06-02T13:31:54Z","title":"Model-independent H0 from GWTC-4 standard sirens and TDCOSMO 2025 strong lensing time delays","version":1},"reference_index":15,"source":"pdf_text","source_observed_at":"2026-06-28T08:37:43.649043Z"},"links":{"cited_paper":"/paper/2411.08639","citing_paper":"/paper/2606.03634"},"observation_digest":"sha256:d07281af3577dda47498dbf5ee47ca6b27061a076a405252418f19d642a0beaa","observation_id":"0f259ac1-ff1f-49e6-b594-7e395d0e7de5","resolution":{"observed_at":"2026-07-02T04:56:39.637187Z","resolver_source":"arxiv_id","status":"verified_exact"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-12T06:34:41.77262+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-12T06:34:41.77262+00:00","source":"crossref"},{"observed_at":"2026-08-12T06:34:36.333875+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":{"arxiv_id":"2411.08639","last_updated":"2025-05-04T13:39:59Z","snapshot_observed_at":"2026-08-12T21:27:31.566500Z","submitted_at":"2024-11-13T14:29:02Z","title":"Revisiting holographic dark energy after DESI 2024","version":2},"cited_work":{"arxiv_id":"2411.08639","doi":null,"metadata_source":"pith","pith_arxiv_id":"2411.08639","snapshot_observed_at":"2026-07-08T15:55:05.042750Z","title":"Li, Y.-H","venue":"astro-ph.CO","work_id":"51d54d56-8f5a-429d-bc95-c12c1201edf1","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":30,"source":"pdf_text","source_observed_at":"2026-06-28T04:52:33.342231Z"},"links":{"cited_paper":"/paper/2411.08639","citing_paper":"/paper/2606.05005"},"observation_digest":"sha256:a32a6b50f0846cdc2f56f4bcb8d464a6e857ec30b21feecc3f83b4e577892d22","observation_id":"846ff88d-9484-40ea-a9c0-c4bd41148b5b","resolution":{"observed_at":"2026-07-02T10:56:52.521603Z","resolver_source":"arxiv_id","status":"verified_exact"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-12T06:34:41.77262+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-12T06:34:41.77262+00:00","source":"crossref"},{"observed_at":"2026-08-12T06:34:36.333875+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":{"arxiv_id":"2411.08639","last_updated":"2025-05-04T13:39:59Z","snapshot_observed_at":"2026-08-12T21:27:31.566500Z","submitted_at":"2024-11-13T14:29:02Z","title":"Revisiting holographic dark energy after DESI 2024","version":2},"cited_work":{"arxiv_id":"2411.08639","doi":null,"metadata_source":"pith","pith_arxiv_id":"2411.08639","snapshot_observed_at":"2026-07-08T15:55:05.042750Z","title":"Li, Y.-H","venue":"astro-ph.CO","work_id":"51d54d56-8f5a-429d-bc95-c12c1201edf1","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":75,"source":"pdf_text","source_observed_at":"2026-06-26T19:48:32.340111Z"},"links":{"cited_paper":"/paper/2411.08639","citing_paper":"/paper/2606.19090"},"observation_digest":"sha256:4ded50497934fbae298ac1abac618f0995a8c8e2b037745fd932ad52c598f7f7","observation_id":"95d0f56e-cfee-4eff-bf89-b02c2613f4ce","resolution":{"observed_at":"2026-07-04T02:19:23.545115Z","resolver_source":"arxiv_id","status":"verified_exact"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-12T06:34:41.77262+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-12T06:34:41.77262+00:00","source":"crossref"},{"observed_at":"2026-08-12T06:34:36.333875+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":{"arxiv_id":"2411.08639","last_updated":"2025-05-04T13:39:59Z","snapshot_observed_at":"2026-08-12T21:27:31.566500Z","submitted_at":"2024-11-13T14:29:02Z","title":"Revisiting holographic dark energy after DESI 2024","version":2},"cited_work":{"arxiv_id":"2411.08639","doi":null,"metadata_source":"pith","pith_arxiv_id":"2411.08639","snapshot_observed_at":"2026-07-08T15:55:05.042750Z","title":"Li, Y.-H","venue":"astro-ph.CO","work_id":"51d54d56-8f5a-429d-bc95-c12c1201edf1","year":2024},"citing_paper":{"arxiv_id":"2606.28175","last_updated":"2026-06-26T15:10:43Z","snapshot_observed_at":"2026-08-12T19:26:46.349936Z","submitted_at":"2026-06-26T15:10:43Z","title":"HIcosmo: a differentiable JAX-based framework for cosmology inference","version":1},"reference_index":66,"source":"pdf_text","source_observed_at":"2026-06-29T02:41:34.484342Z"},"links":{"cited_paper":"/paper/2411.08639","citing_paper":"/paper/2606.28175"},"observation_digest":"sha256:508bbd4409934b6d2f240d0150e1b99f0655412f0af500d98a0a3b117bf5e999","observation_id":"13044591-f84f-4523-aa47-2b41fe8b86a3","resolution":{"observed_at":"2026-07-01T18:05:58.567518Z","resolver_source":"arxiv_id","status":"verified_exact"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-12T06:34:41.77262+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-12T06:34:41.77262+00:00","source":"crossref"},{"observed_at":"2026-08-12T06:34:36.333875+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":{"arxiv_id":"2411.08639","last_updated":"2025-05-04T13:39:59Z","snapshot_observed_at":"2026-08-12T21:27:31.566500Z","submitted_at":"2024-11-13T14:29:02Z","title":"Revisiting holographic dark energy after DESI 2024","version":2},"cited_work":{"arxiv_id":"2411.08639","doi":null,"metadata_source":"pith","pith_arxiv_id":"2411.08639","snapshot_observed_at":"2026-07-08T15:55:05.042750Z","title":"Li, Y.-H","venue":"astro-ph.CO","work_id":"51d54d56-8f5a-429d-bc95-c12c1201edf1","year":2024},"citing_paper":{"arxiv_id":"2607.01226","last_updated":"2026-08-10T20:43:51Z","snapshot_observed_at":"2026-08-13T05:20:39.720521Z","submitted_at":"2026-07-01T17:57:32Z","title":"Intertwined Constraints in Extended Cosmologies: Dark Energy, Curvature, Neutrinos, and Inflation","version":1},"reference_index":130,"source":"pdf_text","source_observed_at":"2026-07-02T06:14:20.101706Z"},"links":{"cited_paper":"/paper/2411.08639","citing_paper":"/paper/2607.01226"},"observation_digest":"sha256:cefab220ab8ec6e3e2e6ac22b4d0a3cdde59ddde29605b99a81ffc751113eddb","observation_id":"e52bb9be-0490-432e-9531-28b9bcef1a20","resolution":{"observed_at":"2026-07-02T06:16:43.230077Z","resolver_source":"arxiv_id","status":"verified_exact"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-12T06:34:41.77262+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-12T06:34:41.77262+00:00","source":"crossref"},{"observed_at":"2026-08-12T06:34:36.333875+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":{"arxiv_id":"2411.08639","last_updated":"2025-05-04T13:39:59Z","snapshot_observed_at":"2026-08-12T21:27:31.566500Z","submitted_at":"2024-11-13T14:29:02Z","title":"Revisiting holographic dark energy after DESI 2024","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2411.08639","snapshot_observed_at":"2026-07-12T04:18:55.037825Z","title":"Li, Y.-H","venue":null,"work_id":null,"year":2025},"citing_paper":{"arxiv_id":"2607.03183","last_updated":"2026-07-03T10:38:35Z","snapshot_observed_at":"2026-08-09T00:31:45.734870Z","submitted_at":"2026-07-03T10:38:35Z","title":"Neutrino mass constraints in the Schwarzschild-de Sitter black-hole dark energy model with ACT DR6 and DESI DR2 data","version":1},"reference_index":95,"source":"pdf_text","source_observed_at":"2026-07-12T04:18:55.037825Z"},"links":{"cited_paper":"/paper/2411.08639","citing_paper":"/paper/2607.03183"},"observation_digest":"sha256:6aa367a3d6a384aadd827b2d3ec21eac799070032c84c2cf402e16579629dc01","observation_id":"867f059f-6c89-4d73-b410-32337e597ef5","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":"2411.08639","last_updated":"2025-05-04T13:39:59Z","snapshot_observed_at":"2026-08-12T21:27:31.566500Z","submitted_at":"2024-11-13T14:29:02Z","title":"Revisiting holographic dark energy after DESI 2024","version":2},"cited_work":{"arxiv_id":"2411.08639","doi":null,"metadata_source":"pith","pith_arxiv_id":"2411.08639","snapshot_observed_at":"2026-07-08T15:55:05.042750Z","title":"Li, Y.-H","venue":"astro-ph.CO","work_id":"51d54d56-8f5a-429d-bc95-c12c1201edf1","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":49,"source":"pdf_text","source_observed_at":"2026-07-08T15:47:53.145943Z"},"links":{"cited_paper":"/paper/2411.08639","citing_paper":"/paper/2607.06147"},"observation_digest":"sha256:296ff38f327f64129af079ca6775eed0289935bbcd474e24fa24f7315bac14d9","observation_id":"0ee9bd43-0e8b-45b7-85d9-d0784e923994","resolution":{"observed_at":"2026-07-08T15:55:05.044512Z","resolver_source":"local_arxiv","status":"verified_exact"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-12T06:34:41.77262+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-12T06:34:41.77262+00:00","source":"crossref"},{"observed_at":"2026-08-12T06:34:36.333875+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":{"arxiv_id":"2411.08639","last_updated":"2025-05-04T13:39:59Z","snapshot_observed_at":"2026-08-12T21:27:31.566500Z","submitted_at":"2024-11-13T14:29:02Z","title":"Revisiting holographic dark energy after DESI 2024","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2411.08639","snapshot_observed_at":"2026-07-31T04:44:10.229849Z","title":"Revisiting holographic dark energy after DESI 2024.Euro- pean Physical Journal C, 85:608, 2025","venue":null,"work_id":null,"year":2024},"citing_paper":{"arxiv_id":"2607.26089","last_updated":"2026-07-27T18:20:37Z","snapshot_observed_at":"2026-08-10T17:59:09.101164Z","submitted_at":"2026-07-27T18:20:37Z","title":"Phantom-Divide Crossing in Barrow-Tsallis Holographic Dark Energy with a Scale-Dependent Barrow Exponent","version":1},"reference_index":30,"source":"pdf_text","source_observed_at":"2026-07-31T04:44:10.229849Z"},"links":{"cited_paper":"/paper/2411.08639","citing_paper":"/paper/2607.26089"},"observation_digest":"sha256:4af14f0e19d9e8f55199eb8e8a14117de0b2d656bf3de697e3ea1bd217774fce","observation_id":"92420f23-ddf4-4a24-9b39-5b8dea8a54d6","resolution":{"observed_at":"2026-07-31T04:44:10.229849Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}}],"links":{"evidence":"/evidence","html":"/paper/2411.08639/citation-record","integrity":"/paper/2411.08639/integrity","json":"/paper/2411.08639/citation-record.json","paper":"/paper/2411.08639"},"outbound":[],"paper":{"arxiv_id":"2411.08639","last_updated":"2025-05-04T13:39:59Z","latest_version":2,"primary_category":"astro-ph.CO","snapshot_observed_at":"2026-08-12T21:27:31.566500Z","submitted_at":"2024-11-13T14:29:02Z","title":"Revisiting holographic dark energy after DESI 2024"},"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":"2026-08-12T06:34:41.77262+00:00","source":"crossref"},{"observed_at":"2026-08-12T06:34:36.333875+00:00","source":"retraction_watch"}],"thesis":"As of 13 August 2026, this Paper Citation Record lists 0 of 0 outbound references and 32 inbound Pith citation observations for arXiv:2411.08639."}