{"as_of":"2026-08-07T23:54:00Z","caps":{"database_statements":6,"inbound":100,"outbound":100},"context_digest":"sha256:8fbecfa98d901b93f579d2e397e972433673d1efc7be40634ebfe6ee1f82b76c","coverage":[{"denominator":80,"lane":"reference_resolution","note":"Typed states for the displayed outbound observations.","records_observed":80,"source":"paper_references, paper_reference_links","source_observed_at":"2026-08-07T12:22:21.787388Z","state":"measured"},{"denominator":81,"lane":"standing_notices","note":"One-hop event checks from named stored sources.","records_observed":81,"source":"scholarly_work_events, retraction_status_cache","source_observed_at":"2026-08-07T06:34:17.273281+00:00","state":"measured"},{"denominator":1,"lane":"inbound_itemization","note":"Pith citing papers itemized under the disclosed page cap.","records_observed":1,"source":"paper_references, paper_reference_links","source_observed_at":"2026-08-01T11:25:06.226043Z","state":"measured"},{"denominator":1,"lane":"external_citation_measurements","note":"A source-named dated measurement, never combined with another source.","records_observed":0,"source":"cited_works","source_observed_at":null,"state":"measured"}],"external_citation_measurements":[],"inbound":[{"citation":{"cited_paper":{"arxiv_id":"2505.24743","last_updated":"2025-06-11T17:49:24Z","snapshot_observed_at":"2026-08-07T12:12:18.402918Z","submitted_at":"2025-05-30T16:01:50Z","title":"What solves the Hubble tension in phenomenological dark energy models at background level?","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2505.24743","snapshot_observed_at":"2026-08-01T11:25:06.226043Z","title":null,"venue":null,"work_id":null,"year":2025},"citing_paper":{"arxiv_id":"2607.19915","last_updated":"2026-07-22T08:45:43Z","snapshot_observed_at":"2026-08-07T04:48:41.686709Z","submitted_at":"2026-07-22T08:45:43Z","title":"QCD CP-violation scenario for a revised cosmological dynamics: analysis of the binned Pantheon Sample of Super Novae Ia","version":1},"reference_index":18,"source":"pdf_text","source_observed_at":"2026-08-01T11:25:06.226043Z"},"links":{"cited_paper":"/paper/2505.24743","citing_paper":"/paper/2607.19915"},"observation_digest":"sha256:23f7981a325b74d5d1b2dba173c1021480c828f5c3e22ddd50a012d3de879629","observation_id":"1efe3b65-95a2-4cc8-9579-1a394e1498a8","resolution":{"observed_at":"2026-08-01T11:25:06.226043Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}}],"links":{"evidence":"/evidence","html":"/paper/2505.24743/citation-record","integrity":"/paper/2505.24743/integrity","json":"/paper/2505.24743/citation-record.json","paper":"/paper/2505.24743"},"outbound":[{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":"raw_reference","pith_arxiv_id":null,"snapshot_observed_at":"2026-08-07T12:22:32.788049Z","title":null,"venue":null,"work_id":"b73b92dd-2da0-45b7-acc3-9aa8263154dd","year":null},"citing_paper":{"arxiv_id":"2505.24743","last_updated":"2025-06-11T17:49:24Z","snapshot_observed_at":"2026-08-07T12:12:18.402918Z","submitted_at":"2025-05-30T16:01:50Z","title":"What solves the Hubble tension in phenomenological dark energy models at background level?","version":2},"reference_index":1,"source":"pdf_text","source_observed_at":"2026-08-07T12:22:14.380694Z"},"links":{"citing_paper":"/paper/2505.24743"},"observation_digest":"sha256:ce3458ff2870d07e4e095a98bc329fc96c2ea59adf08d72f82b847ebd5f290e6","observation_id":"aad686e4-7993-457f-91be-981ec59e1197","resolution":{"observed_at":"2026-08-07T12:22:32.880940Z","resolver_source":"raw_fallback","status":"unresolved"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-07T06:34:17.273281+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-07T06:34:17.273281+00:00","source":"crossref"},{"observed_at":"2026-08-07T06:34:11.927384+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":"raw_reference","pith_arxiv_id":null,"snapshot_observed_at":"2026-08-07T12:22:32.590206Z","title":"In our case, once specific values are chosen for the additional free parameters, all models effectively possess the same free parameters as ΛCDM","venue":null,"work_id":"698e4645-f231-4df2-bf45-0f19f8cfdae7","year":null},"citing_paper":{"arxiv_id":"2505.24743","last_updated":"2025-06-11T17:49:24Z","snapshot_observed_at":"2026-08-07T12:12:18.402918Z","submitted_at":"2025-05-30T16:01:50Z","title":"What solves the Hubble tension in phenomenological dark energy models at background level?","version":2},"reference_index":2,"source":"pdf_text","source_observed_at":"2026-08-07T12:22:14.452522Z"},"links":{"citing_paper":"/paper/2505.24743"},"observation_digest":"sha256:2b2f961dad98739997ba9b896c3b069d5dc75606d1abe19d4e43b1b10dd62fa9","observation_id":"1a26ac65-cbf6-4054-9706-20f725bdeb5a","resolution":{"observed_at":"2026-08-07T12:22:32.658264Z","resolver_source":"raw_fallback","status":"verified_fuzzy"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-07T06:34:17.273281+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-07T06:34:17.273281+00:00","source":"crossref"},{"observed_at":"2026-08-07T06:34:11.927384+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":"raw_reference","pith_arxiv_id":null,"snapshot_observed_at":"2026-08-07T12:22:33.160927Z","title":"Ly 𝛼-QSO+","venue":null,"work_id":"5170d7ae-bbb8-478a-a0dc-7416e834c314","year":2013},"citing_paper":{"arxiv_id":"2505.24743","last_updated":"2025-06-11T17:49:24Z","snapshot_observed_at":"2026-08-07T12:12:18.402918Z","submitted_at":"2025-05-30T16:01:50Z","title":"What solves the Hubble tension in phenomenological dark energy models at background level?","version":2},"reference_index":3,"source":"pdf_text","source_observed_at":"2026-08-07T12:22:14.254368Z"},"links":{"citing_paper":"/paper/2505.24743"},"observation_digest":"sha256:c5c2139d1bbf9102627bbc1505205e99be93b78233cf60f21573240e00ed6406","observation_id":"08f832f4-9c24-4360-b6fa-54c26bcf8855","resolution":{"observed_at":"2026-08-07T12:22:33.258073Z","resolver_source":"raw_fallback","status":"verified_fuzzy"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-07T06:34:17.273281+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-07T06:34:17.273281+00:00","source":"crossref"},{"observed_at":"2026-08-07T06:34:11.927384+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":{"arxiv_id":"2408.06153","last_updated":"2025-03-17T18:25:04Z","snapshot_observed_at":"2026-07-06T18:59:38.952273Z","submitted_at":"2024-08-12T13:48:33Z","title":"Status Report on the Chicago-Carnegie Hubble Program (CCHP): Measurement of the Hubble Constant Using the Hubble and James Webb Space Telescopes","version":3},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2408.06153","snapshot_observed_at":"2026-08-07T12:22:14.848650Z","title":null,"venue":null,"work_id":null,"year":2025},"citing_paper":{"arxiv_id":"2505.24743","last_updated":"2025-06-11T17:49:24Z","snapshot_observed_at":"2026-08-07T12:12:18.402918Z","submitted_at":"2025-05-30T16:01:50Z","title":"What solves the Hubble tension in phenomenological dark energy models at background level?","version":2},"reference_index":4,"source":"pdf_text","source_observed_at":"2026-08-07T12:22:14.848650Z"},"links":{"cited_paper":"/paper/2408.06153","citing_paper":"/paper/2505.24743"},"observation_digest":"sha256:1e1fb954d680a8db2939071173284168a8f66929aa32fb0e5690f5b966b9fdb5","observation_id":"f94a6db3-f024-412a-9b69-7927a2fe6c0b","resolution":{"observed_at":"2026-08-07T12:22:14.848650Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":"raw_reference","pith_arxiv_id":null,"snapshot_observed_at":"2026-08-07T12:22:32.380165Z","title":"Instead, we use 𝜎𝑢 ifA𝑒 is less than the reference value and𝜎𝑙 otherwise","venue":null,"work_id":"201f503a-ad7b-4892-863d-7c4ad9736488","year":null},"citing_paper":{"arxiv_id":"2505.24743","last_updated":"2025-06-11T17:49:24Z","snapshot_observed_at":"2026-08-07T12:12:18.402918Z","submitted_at":"2025-05-30T16:01:50Z","title":"What solves the Hubble tension in phenomenological dark energy models at background level?","version":2},"reference_index":5,"source":"pdf_text","source_observed_at":"2026-08-07T12:22:14.524068Z"},"links":{"citing_paper":"/paper/2505.24743"},"observation_digest":"sha256:2a144f979ec74e987fc2402e3d38aecf6bfe0fd980ed10f423f3302c989c9acc","observation_id":"1803a4ff-5a89-489b-83bc-7a985bc7cd1b","resolution":{"observed_at":"2026-08-07T12:22:32.466390Z","resolver_source":"raw_fallback","status":"verified_fuzzy"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-07T06:34:17.273281+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-07T06:34:17.273281+00:00","source":"crossref"},{"observed_at":"2026-08-07T06:34:11.927384+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":"raw_reference","pith_arxiv_id":null,"snapshot_observed_at":"2026-08-07T12:22:32.158585Z","title":"Python modules used","venue":null,"work_id":"ec151a72-6d84-4894-a396-cd89fb83cf20","year":1974},"citing_paper":{"arxiv_id":"2505.24743","last_updated":"2025-06-11T17:49:24Z","snapshot_observed_at":"2026-08-07T12:12:18.402918Z","submitted_at":"2025-05-30T16:01:50Z","title":"What solves the Hubble tension in phenomenological dark energy models at background level?","version":2},"reference_index":6,"source":"pdf_text","source_observed_at":"2026-08-07T12:22:14.589598Z"},"links":{"citing_paper":"/paper/2505.24743"},"observation_digest":"sha256:558dbc4780c23a431b519f38aab234bdfd0c8bceed9bcd69ff3cb92c62c86e04","observation_id":"cea9a2a6-6f06-41e3-828c-7bb2c24ae66d","resolution":{"observed_at":"2026-08-07T12:22:32.268120Z","resolver_source":"raw_fallback","status":"verified_fuzzy"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-07T06:34:17.273281+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-07T06:34:17.273281+00:00","source":"crossref"},{"observed_at":"2026-08-07T06:34:11.927384+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":{"arxiv_id":"2504.01669","last_updated":"2025-08-04T13:56:55Z","snapshot_observed_at":"2026-08-01T19:48:28.599955Z","submitted_at":"2025-04-02T12:17:19Z","title":"The CosmoVerse White Paper: Addressing observational tensions in cosmology with systematics and fundamental physics","version":3},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2504.01669","snapshot_observed_at":"2026-08-07T12:22:14.657481Z","title":"Di Valentino, J","venue":null,"work_id":null,"year":2025},"citing_paper":{"arxiv_id":"2505.24743","last_updated":"2025-06-11T17:49:24Z","snapshot_observed_at":"2026-08-07T12:12:18.402918Z","submitted_at":"2025-05-30T16:01:50Z","title":"What solves the Hubble tension in phenomenological dark energy models at background level?","version":2},"reference_index":7,"source":"pdf_text","source_observed_at":"2026-08-07T12:22:14.657481Z"},"links":{"cited_paper":"/paper/2504.01669","citing_paper":"/paper/2505.24743"},"observation_digest":"sha256:8c7e8bafcfa5142b7674a30ff23aa159a74314d1e199590914c4354ca09e4d94","observation_id":"a2a0f18f-08c7-4be3-934c-20d63412f28b","resolution":{"observed_at":"2026-08-07T12:22:14.657481Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":"raw_reference","pith_arxiv_id":null,"snapshot_observed_at":"2026-08-07T12:22:31.936853Z","title":null,"venue":null,"work_id":"3703027b-04c7-4be2-ad79-1105c8c88928","year":2022},"citing_paper":{"arxiv_id":"2505.24743","last_updated":"2025-06-11T17:49:24Z","snapshot_observed_at":"2026-08-07T12:12:18.402918Z","submitted_at":"2025-05-30T16:01:50Z","title":"What solves the Hubble tension in phenomenological dark energy models at background level?","version":2},"reference_index":8,"source":"pdf_text","source_observed_at":"2026-08-07T12:22:14.729190Z"},"links":{"citing_paper":"/paper/2505.24743"},"observation_digest":"sha256:1f5199cdf238c6b83d527823917d0d87a9d8674a04dfafe2abc7d378fd43d487","observation_id":"fa85277d-ed32-4b1e-8da2-1209f1dbfb76","resolution":{"observed_at":"2026-08-07T12:22:32.040520Z","resolver_source":"raw_fallback","status":"unresolved"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-07T06:34:17.273281+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-07T06:34:17.273281+00:00","source":"crossref"},{"observed_at":"2026-08-07T06:34:11.927384+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":"raw_reference","pith_arxiv_id":null,"snapshot_observed_at":"2026-08-07T12:22:31.742535Z","title":"Aghanim et al., A&A 641, A6 (2020)","venue":null,"work_id":"d4a4e103-1915-45d9-bc03-69937c8ba69f","year":2020},"citing_paper":{"arxiv_id":"2505.24743","last_updated":"2025-06-11T17:49:24Z","snapshot_observed_at":"2026-08-07T12:12:18.402918Z","submitted_at":"2025-05-30T16:01:50Z","title":"What solves the Hubble tension in phenomenological dark energy models at background level?","version":2},"reference_index":9,"source":"pdf_text","source_observed_at":"2026-08-07T12:22:14.805911Z"},"links":{"citing_paper":"/paper/2505.24743"},"observation_digest":"sha256:64b0b5af3e35ab688b0c6dd3226f6e7214081c9358b4ad68996beb2a0102eea6","observation_id":"045b162f-603e-4c13-b67d-1e5146df96ba","resolution":{"observed_at":"2026-08-07T12:22:31.822182Z","resolver_source":"raw_fallback","status":"verified_fuzzy"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-07T06:34:17.273281+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-07T06:34:17.273281+00:00","source":"crossref"},{"observed_at":"2026-08-07T06:34:11.927384+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":"raw_reference","pith_arxiv_id":null,"snapshot_observed_at":"2026-08-07T12:22:30.946238Z","title":"von Marttens, L","venue":null,"work_id":"4ee959f1-9789-4a22-8b2c-8455d6d55b62","year":2020},"citing_paper":{"arxiv_id":"2505.24743","last_updated":"2025-06-11T17:49:24Z","snapshot_observed_at":"2026-08-07T12:12:18.402918Z","submitted_at":"2025-05-30T16:01:50Z","title":"What solves the Hubble tension in phenomenological dark energy models at background level?","version":2},"reference_index":10,"source":"pdf_text","source_observed_at":"2026-08-07T12:22:15.267561Z"},"links":{"citing_paper":"/paper/2505.24743"},"observation_digest":"sha256:06326840f8268a05cd6eff824b260a0abc1ffba5e24cd4030646a454f45f7b03","observation_id":"d866c886-8aba-4685-9630-cca2e9bb7da4","resolution":{"observed_at":"2026-08-07T12:22:31.004838Z","resolver_source":"raw_fallback","status":"verified_fuzzy"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-07T06:34:17.273281+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-07T06:34:17.273281+00:00","source":"crossref"},{"observed_at":"2026-08-07T06:34:11.927384+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":"raw_reference","pith_arxiv_id":null,"snapshot_observed_at":"2026-08-07T12:22:31.546744Z","title":"Li et al., The Astrophysical Journal 976, 177 (2024)","venue":null,"work_id":"a67ed1d6-74ac-4e8d-9995-e3fe8bc57ae4","year":2024},"citing_paper":{"arxiv_id":"2505.24743","last_updated":"2025-06-11T17:49:24Z","snapshot_observed_at":"2026-08-07T12:12:18.402918Z","submitted_at":"2025-05-30T16:01:50Z","title":"What solves the Hubble tension in phenomenological dark energy models at background level?","version":2},"reference_index":11,"source":"pdf_text","source_observed_at":"2026-08-07T12:22:14.926311Z"},"links":{"citing_paper":"/paper/2505.24743"},"observation_digest":"sha256:e93d4f096f51bdb4ba59db726c4f22b53d856f8a1ed1c51cdf41ac9055d1c3fb","observation_id":"c56c976a-ac4c-4399-bdca-e8bd342c72ba","resolution":{"observed_at":"2026-08-07T12:22:31.632850Z","resolver_source":"raw_fallback","status":"verified_fuzzy"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-07T06:34:17.273281+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-07T06:34:17.273281+00:00","source":"crossref"},{"observed_at":"2026-08-07T06:34:11.927384+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":{"arxiv_id":"2503.14738","last_updated":"2025-10-09T16:45:28Z","snapshot_observed_at":"2026-07-06T02:11:23.670680Z","submitted_at":"2025-03-18T21:14:12Z","title":"DESI DR2 Results II: Measurements of Baryon Acoustic Oscillations and Cosmological Constraints","version":3},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2503.14738","snapshot_observed_at":"2026-08-07T12:22:14.986835Z","title":", (2025), arXiv:2503.14738 [astro- ph.CO]","venue":null,"work_id":null,"year":2025},"citing_paper":{"arxiv_id":"2505.24743","last_updated":"2025-06-11T17:49:24Z","snapshot_observed_at":"2026-08-07T12:12:18.402918Z","submitted_at":"2025-05-30T16:01:50Z","title":"What solves the Hubble tension in phenomenological dark energy models at background level?","version":2},"reference_index":12,"source":"pdf_text","source_observed_at":"2026-08-07T12:22:14.986835Z"},"links":{"cited_paper":"/paper/2503.14738","citing_paper":"/paper/2505.24743"},"observation_digest":"sha256:1608901ef9ba22ebfda0c998b11e3a7c5dfc1c0fcde3c8dded6dfca055cdb10b","observation_id":"5298c10b-8418-4507-899e-f723b34d2508","resolution":{"observed_at":"2026-08-07T12:22:14.986835Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":{"arxiv_id":"2504.20664","last_updated":"2025-08-15T13:21:18Z","snapshot_observed_at":"2026-08-07T15:58:15.798058Z","submitted_at":"2025-04-29T11:38:28Z","title":"Challenging $\\Lambda$CDM: 5$\\sigma$ Evidence for a Dynamical Dark Energy Late-Time Transition","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2504.20664","snapshot_observed_at":"2026-08-07T12:22:15.063343Z","title":"Scherer, M","venue":null,"work_id":null,"year":2025},"citing_paper":{"arxiv_id":"2505.24743","last_updated":"2025-06-11T17:49:24Z","snapshot_observed_at":"2026-08-07T12:12:18.402918Z","submitted_at":"2025-05-30T16:01:50Z","title":"What solves the Hubble tension in phenomenological dark energy models at background level?","version":2},"reference_index":13,"source":"pdf_text","source_observed_at":"2026-08-07T12:22:15.063343Z"},"links":{"cited_paper":"/paper/2504.20664","citing_paper":"/paper/2505.24743"},"observation_digest":"sha256:0a7aa13f0f48e1aa79ae344e3447a5b5b9083182ccd9656b1ae1bb9de0ecaf3b","observation_id":"af9ad887-5449-4ccb-9ebd-391960df3e3d","resolution":{"observed_at":"2026-08-07T12:22:15.063343Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":"raw_reference","pith_arxiv_id":null,"snapshot_observed_at":"2026-08-07T12:22:31.378937Z","title":"Li and A","venue":null,"work_id":"5f50c5ab-74b6-4a76-8c54-25658c074a60","year":2019},"citing_paper":{"arxiv_id":"2505.24743","last_updated":"2025-06-11T17:49:24Z","snapshot_observed_at":"2026-08-07T12:12:18.402918Z","submitted_at":"2025-05-30T16:01:50Z","title":"What solves the Hubble tension in phenomenological dark energy models at background level?","version":2},"reference_index":14,"source":"pdf_text","source_observed_at":"2026-08-07T12:22:15.151092Z"},"links":{"citing_paper":"/paper/2505.24743"},"observation_digest":"sha256:6d8ef68b0aae9476965670e95bc19a7ec2d93db3c99d9404f31a5235e9eb7736","observation_id":"485ed9bc-c152-41ac-8644-39835bf1f6ae","resolution":{"observed_at":"2026-08-07T12:22:31.477962Z","resolver_source":"raw_fallback","status":"verified_fuzzy"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-07T06:34:17.273281+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-07T06:34:17.273281+00:00","source":"crossref"},{"observed_at":"2026-08-07T06:34:11.927384+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":"raw_reference","pith_arxiv_id":null,"snapshot_observed_at":"2026-08-07T12:22:31.103106Z","title":"Granda and A","venue":null,"work_id":"c3f6228a-7655-49f9-b022-fe5d01f6524e","year":2008},"citing_paper":{"arxiv_id":"2505.24743","last_updated":"2025-06-11T17:49:24Z","snapshot_observed_at":"2026-08-07T12:12:18.402918Z","submitted_at":"2025-05-30T16:01:50Z","title":"What solves the Hubble tension in phenomenological dark energy models at background level?","version":2},"reference_index":15,"source":"pdf_text","source_observed_at":"2026-08-07T12:22:15.208480Z"},"links":{"citing_paper":"/paper/2505.24743"},"observation_digest":"sha256:94aa94d9104012725f89d7f081d224465f070f2070294ca8289a8e213463e901","observation_id":"932354c9-bb42-4e42-a25f-1c4acb62048c","resolution":{"observed_at":"2026-08-07T12:22:31.242478Z","resolver_source":"raw_fallback","status":"verified_fuzzy"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-07T06:34:17.273281+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-07T06:34:17.273281+00:00","source":"crossref"},{"observed_at":"2026-08-07T06:34:11.927384+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":"raw_reference","pith_arxiv_id":null,"snapshot_observed_at":"2026-08-07T12:22:30.358700Z","title":"Li and A","venue":null,"work_id":"7fb905e1-ac1e-415b-a806-15091efbf123","year":2020},"citing_paper":{"arxiv_id":"2505.24743","last_updated":"2025-06-11T17:49:24Z","snapshot_observed_at":"2026-08-07T12:12:18.402918Z","submitted_at":"2025-05-30T16:01:50Z","title":"What solves the Hubble tension in phenomenological dark energy models at background level?","version":2},"reference_index":16,"source":"pdf_text","source_observed_at":"2026-08-07T12:22:15.828453Z"},"links":{"citing_paper":"/paper/2505.24743"},"observation_digest":"sha256:221e9dbe944b79e7a22ca62daa698b216e914dfc5064e2983998b8d57184f560","observation_id":"abf84bae-894d-430e-94d4-7a9e9359bd37","resolution":{"observed_at":"2026-08-07T12:22:30.431237Z","resolver_source":"raw_fallback","status":"verified_fuzzy"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-07T06:34:17.273281+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-07T06:34:17.273281+00:00","source":"crossref"},{"observed_at":"2026-08-07T06:34:11.927384+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":null,"snapshot_observed_at":"2026-08-07T12:22:15.366949Z","title":"Weinberg, Rev","venue":null,"work_id":null,"year":1989},"citing_paper":{"arxiv_id":"2505.24743","last_updated":"2025-06-11T17:49:24Z","snapshot_observed_at":"2026-08-07T12:12:18.402918Z","submitted_at":"2025-05-30T16:01:50Z","title":"What solves the Hubble tension in phenomenological dark energy models at background level?","version":2},"reference_index":17,"source":"pdf_text","source_observed_at":"2026-08-07T12:22:15.366949Z"},"links":{"citing_paper":"/paper/2505.24743"},"observation_digest":"sha256:5e2caab7abb5f18ff314d52bf1528e4235230ba808c49e50f00fd57f36938595","observation_id":"3cf118f9-6f68-4971-9376-23c115c528cd","resolution":{"observed_at":"2026-08-07T12:22:15.366949Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":null,"snapshot_observed_at":"2026-08-07T12:22:15.386051Z","title":null,"venue":null,"work_id":null,"year":2003},"citing_paper":{"arxiv_id":"2505.24743","last_updated":"2025-06-11T17:49:24Z","snapshot_observed_at":"2026-08-07T12:12:18.402918Z","submitted_at":"2025-05-30T16:01:50Z","title":"What solves the Hubble tension in phenomenological dark energy models at background level?","version":2},"reference_index":18,"source":"pdf_text","source_observed_at":"2026-08-07T12:22:15.386051Z"},"links":{"citing_paper":"/paper/2505.24743"},"observation_digest":"sha256:8f87367a1e8d17bb980985d8aa025ea36d048ba0b3e0122ef5ba2d02d2021071","observation_id":"189d82da-4699-4271-8444-3a0c5d4a07cf","resolution":{"observed_at":"2026-08-07T12:22:15.386051Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":"raw_reference","pith_arxiv_id":null,"snapshot_observed_at":"2026-08-07T12:22:30.779153Z","title":null,"venue":null,"work_id":"891cb566-7db4-47a9-975f-0e8f006c440e","year":2024},"citing_paper":{"arxiv_id":"2505.24743","last_updated":"2025-06-11T17:49:24Z","snapshot_observed_at":"2026-08-07T12:12:18.402918Z","submitted_at":"2025-05-30T16:01:50Z","title":"What solves the Hubble tension in phenomenological dark energy models at background level?","version":2},"reference_index":19,"source":"pdf_text","source_observed_at":"2026-08-07T12:22:15.442582Z"},"links":{"citing_paper":"/paper/2505.24743"},"observation_digest":"sha256:aab96e15a12b7f8ed0c808a23886381622c3b86ff3c8274ec022f4ffd861ed3e","observation_id":"087fa812-1c39-4166-a071-5877f0724647","resolution":{"observed_at":"2026-08-07T12:22:30.860819Z","resolver_source":"raw_fallback","status":"unresolved"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-07T06:34:17.273281+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-07T06:34:17.273281+00:00","source":"crossref"},{"observed_at":"2026-08-07T06:34:11.927384+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":{"arxiv_id":"2503.14739","last_updated":"2025-06-30T00:11:58Z","snapshot_observed_at":"2026-07-30T08:44:56.946347Z","submitted_at":"2025-03-18T21:14:13Z","title":"DESI DR2 Results I: Baryon Acoustic Oscillations from the Lyman Alpha Forest","version":3},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2503.14739","snapshot_observed_at":"2026-08-07T12:22:15.578771Z","title":null,"venue":null,"work_id":null,"year":2025},"citing_paper":{"arxiv_id":"2505.24743","last_updated":"2025-06-11T17:49:24Z","snapshot_observed_at":"2026-08-07T12:12:18.402918Z","submitted_at":"2025-05-30T16:01:50Z","title":"What solves the Hubble tension in phenomenological dark energy models at background level?","version":2},"reference_index":20,"source":"pdf_text","source_observed_at":"2026-08-07T12:22:15.578771Z"},"links":{"cited_paper":"/paper/2503.14739","citing_paper":"/paper/2505.24743"},"observation_digest":"sha256:cdbfba2fd5a20302afa99ef8c405dc2ff202d15b9da35e61f77a82328b2968d3","observation_id":"32d7b831-b805-404f-a3d6-5b47a644da5d","resolution":{"observed_at":"2026-08-07T12:22:15.578771Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":"raw_reference","pith_arxiv_id":null,"snapshot_observed_at":"2026-08-07T12:22:30.548333Z","title":"Vagnozzi, Phys","venue":null,"work_id":"68630f10-2e6b-43e6-8c51-8cbd8f10031f","year":2020},"citing_paper":{"arxiv_id":"2505.24743","last_updated":"2025-06-11T17:49:24Z","snapshot_observed_at":"2026-08-07T12:12:18.402918Z","submitted_at":"2025-05-30T16:01:50Z","title":"What solves the Hubble tension in phenomenological dark energy models at background level?","version":2},"reference_index":21,"source":"pdf_text","source_observed_at":"2026-08-07T12:22:15.680732Z"},"links":{"citing_paper":"/paper/2505.24743"},"observation_digest":"sha256:a6d18660164f0b2667fc73baec413b02d73c970d42dbb1163717ce1e853ea297","observation_id":"2f10d27f-1021-4ba5-b297-a0ed7efbb6d2","resolution":{"observed_at":"2026-08-07T12:22:30.674175Z","resolver_source":"raw_fallback","status":"verified_fuzzy"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-07T06:34:17.273281+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-07T06:34:17.273281+00:00","source":"crossref"},{"observed_at":"2026-08-07T06:34:11.927384+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":"raw_reference","pith_arxiv_id":null,"snapshot_observed_at":"2026-08-07T12:22:29.655657Z","title":"Tamayo, E","venue":null,"work_id":"dccb548f-caad-465d-9762-1b78fdf3715d","year":2025},"citing_paper":{"arxiv_id":"2505.24743","last_updated":"2025-06-11T17:49:24Z","snapshot_observed_at":"2026-08-07T12:12:18.402918Z","submitted_at":"2025-05-30T16:01:50Z","title":"What solves the Hubble tension in phenomenological dark energy models at background level?","version":2},"reference_index":22,"source":"pdf_text","source_observed_at":"2026-08-07T12:22:16.630165Z"},"links":{"citing_paper":"/paper/2505.24743"},"observation_digest":"sha256:74a6e19365e4aa5bf00a8a451e74ac1144f95d9c8f2c0af7ee1a288f2398749b","observation_id":"ebd45bf6-9312-45df-9be7-b4b592cbcf35","resolution":{"observed_at":"2026-08-07T12:22:29.729935Z","resolver_source":"raw_fallback","status":"verified_fuzzy"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-07T06:34:17.273281+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-07T06:34:17.273281+00:00","source":"crossref"},{"observed_at":"2026-08-07T06:34:11.927384+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":"raw_reference","pith_arxiv_id":null,"snapshot_observed_at":"2026-08-07T12:22:30.195660Z","title":null,"venue":null,"work_id":"2b27d126-ed77-425c-90dd-96f8b41d2ef2","year":2021},"citing_paper":{"arxiv_id":"2505.24743","last_updated":"2025-06-11T17:49:24Z","snapshot_observed_at":"2026-08-07T12:12:18.402918Z","submitted_at":"2025-05-30T16:01:50Z","title":"What solves the Hubble tension in phenomenological dark energy models at background level?","version":2},"reference_index":23,"source":"pdf_text","source_observed_at":"2026-08-07T12:22:15.951774Z"},"links":{"citing_paper":"/paper/2505.24743"},"observation_digest":"sha256:2766b59850603b624b610f100857f2ef34404c0ae125e0266c22b843b6267210","observation_id":"12ed84ab-c6c1-4f0f-b534-5e0ccdd9d59e","resolution":{"observed_at":"2026-08-07T12:22:30.265154Z","resolver_source":"raw_fallback","status":"unresolved"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-07T06:34:17.273281+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-07T06:34:17.273281+00:00","source":"crossref"},{"observed_at":"2026-08-07T06:34:11.927384+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":{"arxiv_id":"2310.05594","last_updated":"2023-10-09T10:28:41Z","snapshot_observed_at":"2026-08-06T03:47:54.976164Z","submitted_at":"2023-10-09T10:28:41Z","title":"Observational evidence for parametrized emergent dark energy models","version":1},"cited_work":{"arxiv_id":"2310.05594","doi":null,"metadata_source":"pith","pith_arxiv_id":"2310.05594","snapshot_observed_at":"2026-08-07T12:22:22.482931Z","title":"Observational evidence for parametrized emergent dark energy models","venue":"astro-ph.CO","work_id":"f570f582-1ec7-42e9-9ec2-8df46f5744af","year":2023},"citing_paper":{"arxiv_id":"2505.24743","last_updated":"2025-06-11T17:49:24Z","snapshot_observed_at":"2026-08-07T12:12:18.402918Z","submitted_at":"2025-05-30T16:01:50Z","title":"What solves the Hubble tension in phenomenological dark energy models at background level?","version":2},"reference_index":24,"source":"pdf_text","source_observed_at":"2026-08-07T12:22:16.083732Z"},"links":{"cited_paper":"/paper/2310.05594","citing_paper":"/paper/2505.24743"},"observation_digest":"sha256:cec57d58444b0f7bf337a7b5c96adf085e92ecfb2c81916854b7d2a8365d2532","observation_id":"5b18a661-6041-4612-820e-3cc8b2f06ca1","resolution":{"observed_at":"2026-08-07T12:22:22.610615Z","resolver_source":"local_arxiv","status":"verified_exact"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-07T06:34:17.273281+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-07T06:34:17.273281+00:00","source":"crossref"},{"observed_at":"2026-08-07T06:34:11.927384+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":"raw_reference","pith_arxiv_id":null,"snapshot_observed_at":"2026-08-07T12:22:30.013848Z","title":null,"venue":null,"work_id":"9767a5fd-e182-45c5-ab23-2d3686584949","year":2017},"citing_paper":{"arxiv_id":"2505.24743","last_updated":"2025-06-11T17:49:24Z","snapshot_observed_at":"2026-08-07T12:12:18.402918Z","submitted_at":"2025-05-30T16:01:50Z","title":"What solves the Hubble tension in phenomenological dark energy models at background level?","version":2},"reference_index":25,"source":"pdf_text","source_observed_at":"2026-08-07T12:22:16.248168Z"},"links":{"citing_paper":"/paper/2505.24743"},"observation_digest":"sha256:8d16453fbf6ccc8762cd61c10e4545f337d603d5fd6e54a1b6b672865d7a8983","observation_id":"408ef6b1-3cb3-4f28-bd4b-68af0f215904","resolution":{"observed_at":"2026-08-07T12:22:30.080696Z","resolver_source":"raw_fallback","status":"unresolved"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-07T06:34:17.273281+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-07T06:34:17.273281+00:00","source":"crossref"},{"observed_at":"2026-08-07T06:34:11.927384+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":"2501.18144","doi":null,"metadata_source":"raw_reference","pith_arxiv_id":null,"snapshot_observed_at":"2026-08-07T12:22:22.250726Z","title":null,"venue":null,"work_id":"94313dbd-453f-4a2a-ba18-6bfa1c0cb9d5","year":2025},"citing_paper":{"arxiv_id":"2505.24743","last_updated":"2025-06-11T17:49:24Z","snapshot_observed_at":"2026-08-07T12:12:18.402918Z","submitted_at":"2025-05-30T16:01:50Z","title":"What solves the Hubble tension in phenomenological dark energy models at background level?","version":2},"reference_index":26,"source":"pdf_text","source_observed_at":"2026-08-07T12:22:16.412983Z"},"links":{"citing_paper":"/paper/2505.24743"},"observation_digest":"sha256:f80b5a1304b56ad320304c4e2d02ddc062d3c5155d04cdd3371359c826d91291","observation_id":"cf3806ce-3d4c-40b6-acf2-a6ebbf5f6be8","resolution":{"observed_at":"2026-08-07T12:22:22.336508Z","resolver_source":"raw_fallback","status":"verified_exact"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-07T06:34:17.273281+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-07T06:34:17.273281+00:00","source":"crossref"},{"observed_at":"2026-08-07T06:34:11.927384+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":"raw_reference","pith_arxiv_id":null,"snapshot_observed_at":"2026-08-07T12:22:29.830073Z","title":null,"venue":null,"work_id":"b7e4cde6-6b68-4184-903e-37e8e1478b30","year":2024},"citing_paper":{"arxiv_id":"2505.24743","last_updated":"2025-06-11T17:49:24Z","snapshot_observed_at":"2026-08-07T12:12:18.402918Z","submitted_at":"2025-05-30T16:01:50Z","title":"What solves the Hubble tension in phenomenological dark energy models at background level?","version":2},"reference_index":27,"source":"pdf_text","source_observed_at":"2026-08-07T12:22:16.509467Z"},"links":{"citing_paper":"/paper/2505.24743"},"observation_digest":"sha256:f97e0b78607dbf9881478ba34125a5fb2b98f2a30c5986a393de25d65ab8467e","observation_id":"16aa4eeb-f59f-4cf0-8e28-e9505e08809c","resolution":{"observed_at":"2026-08-07T12:22:29.917428Z","resolver_source":"raw_fallback","status":"unresolved"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-07T06:34:17.273281+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-07T06:34:17.273281+00:00","source":"crossref"},{"observed_at":"2026-08-07T06:34:11.927384+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":"raw_reference","pith_arxiv_id":null,"snapshot_observed_at":"2026-08-07T12:22:29.003138Z","title":"Jimenez and A","venue":null,"work_id":"e736c791-4291-4648-a5a7-834154b5d378","year":2002},"citing_paper":{"arxiv_id":"2505.24743","last_updated":"2025-06-11T17:49:24Z","snapshot_observed_at":"2026-08-07T12:12:18.402918Z","submitted_at":"2025-05-30T16:01:50Z","title":"What solves the Hubble tension in phenomenological dark energy models at background level?","version":2},"reference_index":28,"source":"pdf_text","source_observed_at":"2026-08-07T12:22:17.364027Z"},"links":{"citing_paper":"/paper/2505.24743"},"observation_digest":"sha256:2d75a16dcd35395e0199b82d2049a910bce5b7967761c2b8ae77676066da00bd","observation_id":"32eed952-87ea-42b0-823a-f3a580f1c2d8","resolution":{"observed_at":"2026-08-07T12:22:29.086516Z","resolver_source":"raw_fallback","status":"verified_fuzzy"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-07T06:34:17.273281+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-07T06:34:17.273281+00:00","source":"crossref"},{"observed_at":"2026-08-07T06:34:11.927384+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":{"arxiv_id":"2503.21652","last_updated":"2025-09-08T07:08:45Z","snapshot_observed_at":"2026-08-07T16:32:22.960010Z","submitted_at":"2025-03-27T16:16:43Z","title":"Interacting Dark Sectors in light of DESI DR2","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2503.21652","snapshot_observed_at":"2026-08-07T12:22:16.756389Z","title":null,"venue":null,"work_id":null,"year":2025},"citing_paper":{"arxiv_id":"2505.24743","last_updated":"2025-06-11T17:49:24Z","snapshot_observed_at":"2026-08-07T12:12:18.402918Z","submitted_at":"2025-05-30T16:01:50Z","title":"What solves the Hubble tension in phenomenological dark energy models at background level?","version":2},"reference_index":29,"source":"pdf_text","source_observed_at":"2026-08-07T12:22:16.756389Z"},"links":{"cited_paper":"/paper/2503.21652","citing_paper":"/paper/2505.24743"},"observation_digest":"sha256:3f5e5ef69174c4d1059c33ebf5ccd24b6c1efe3961f0d57acc7101b368f09a9d","observation_id":"b603e1ca-c95d-4a9c-9a7c-ea7f55cf4274","resolution":{"observed_at":"2026-08-07T12:22:16.756389Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":"raw_reference","pith_arxiv_id":null,"snapshot_observed_at":"2026-08-07T12:22:29.488082Z","title":null,"venue":null,"work_id":"7b6eb88c-1e6f-4f1d-93f1-0be174ff0fe8","year":2024},"citing_paper":{"arxiv_id":"2505.24743","last_updated":"2025-06-11T17:49:24Z","snapshot_observed_at":"2026-08-07T12:12:18.402918Z","submitted_at":"2025-05-30T16:01:50Z","title":"What solves the Hubble tension in phenomenological dark energy models at background level?","version":2},"reference_index":30,"source":"pdf_text","source_observed_at":"2026-08-07T12:22:16.917953Z"},"links":{"citing_paper":"/paper/2505.24743"},"observation_digest":"sha256:c12ce00bc3b77af19590e3c111fbc7e615f736641d11279614df9ba502c0b651","observation_id":"4eae3d0d-dcce-43c0-8c76-78d5afc523eb","resolution":{"observed_at":"2026-08-07T12:22:29.540105Z","resolver_source":"raw_fallback","status":"unresolved"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-07T06:34:17.273281+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-07T06:34:17.273281+00:00","source":"crossref"},{"observed_at":"2026-08-07T06:34:11.927384+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":"raw_reference","pith_arxiv_id":null,"snapshot_observed_at":"2026-08-07T12:22:29.292896Z","title":null,"venue":null,"work_id":"68292a5a-3b72-44f8-b640-73d6614a6724","year":2018},"citing_paper":{"arxiv_id":"2505.24743","last_updated":"2025-06-11T17:49:24Z","snapshot_observed_at":"2026-08-07T12:12:18.402918Z","submitted_at":"2025-05-30T16:01:50Z","title":"What solves the Hubble tension in phenomenological dark energy models at background level?","version":2},"reference_index":31,"source":"pdf_text","source_observed_at":"2026-08-07T12:22:17.062409Z"},"links":{"citing_paper":"/paper/2505.24743"},"observation_digest":"sha256:fcfb4bd67b0a69f48ce0321f8c335e0fc61dcd5edf75d252905a408c2050a78e","observation_id":"4ec5d628-388f-465e-b25b-61139ebf125b","resolution":{"observed_at":"2026-08-07T12:22:29.387832Z","resolver_source":"raw_fallback","status":"unresolved"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-07T06:34:17.273281+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-07T06:34:17.273281+00:00","source":"crossref"},{"observed_at":"2026-08-07T06:34:11.927384+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":"raw_reference","pith_arxiv_id":null,"snapshot_observed_at":"2026-08-07T12:22:29.164364Z","title":"Di Valentino, A","venue":null,"work_id":"88ad6aff-87d7-46bd-8fce-dad4e16376e6","year":2020},"citing_paper":{"arxiv_id":"2505.24743","last_updated":"2025-06-11T17:49:24Z","snapshot_observed_at":"2026-08-07T12:12:18.402918Z","submitted_at":"2025-05-30T16:01:50Z","title":"What solves the Hubble tension in phenomenological dark energy models at background level?","version":2},"reference_index":32,"source":"pdf_text","source_observed_at":"2026-08-07T12:22:17.153285Z"},"links":{"citing_paper":"/paper/2505.24743"},"observation_digest":"sha256:d16e45303a1250058542b7178b9aabdab7289ef490f44f4e641889df3298ea3b","observation_id":"d303ecd3-f95d-4f2a-89f3-a5c0a45f30e2","resolution":{"observed_at":"2026-08-07T12:22:29.234302Z","resolver_source":"raw_fallback","status":"verified_fuzzy"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-07T06:34:17.273281+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-07T06:34:17.273281+00:00","source":"crossref"},{"observed_at":"2026-08-07T06:34:11.927384+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":{"arxiv_id":"2503.23225","last_updated":"2025-06-11T18:36:13Z","snapshot_observed_at":"2026-08-07T16:28:07.594746Z","submitted_at":"2025-03-29T21:11:16Z","title":"New constraints on interacting dark energy from DESI DR2 BAO observations","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2503.23225","snapshot_observed_at":"2026-08-07T12:22:17.247293Z","title":"Silva, M","venue":null,"work_id":null,"year":2025},"citing_paper":{"arxiv_id":"2505.24743","last_updated":"2025-06-11T17:49:24Z","snapshot_observed_at":"2026-08-07T12:12:18.402918Z","submitted_at":"2025-05-30T16:01:50Z","title":"What solves the Hubble tension in phenomenological dark energy models at background level?","version":2},"reference_index":33,"source":"pdf_text","source_observed_at":"2026-08-07T12:22:17.247293Z"},"links":{"cited_paper":"/paper/2503.23225","citing_paper":"/paper/2505.24743"},"observation_digest":"sha256:d66d8afe8cd2238af7bb440d02b27ed950ade8629142f3678166326446533e5a","observation_id":"4a0279c1-9382-41ff-9b44-35b0fff9fef1","resolution":{"observed_at":"2026-08-07T12:22:17.247293Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":"raw_reference","pith_arxiv_id":null,"snapshot_observed_at":"2026-08-07T12:22:27.892907Z","title":null,"venue":null,"work_id":"c12d9b30-ecc1-4fc0-af09-9048857d4058","year":2017},"citing_paper":{"arxiv_id":"2505.24743","last_updated":"2025-06-11T17:49:24Z","snapshot_observed_at":"2026-08-07T12:12:18.402918Z","submitted_at":"2025-05-30T16:01:50Z","title":"What solves the Hubble tension in phenomenological dark energy models at background level?","version":2},"reference_index":34,"source":"pdf_text","source_observed_at":"2026-08-07T12:22:17.835472Z"},"links":{"citing_paper":"/paper/2505.24743"},"observation_digest":"sha256:291bccc0577cf1e3bccf189dcdadef2073506f8d6d89ea20575e2c8a49fc02db","observation_id":"05478d55-9566-4b14-b24c-5e746cea3a62","resolution":{"observed_at":"2026-08-07T12:22:28.025659Z","resolver_source":"raw_fallback","status":"unresolved"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-07T06:34:17.273281+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-07T06:34:17.273281+00:00","source":"crossref"},{"observed_at":"2026-08-07T06:34:11.927384+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":"raw_reference","pith_arxiv_id":null,"snapshot_observed_at":"2026-08-07T12:22:28.797832Z","title":"Stern, R","venue":null,"work_id":"bd3b8e2d-ca27-41a7-ac9f-509b58c578f4","year":2010},"citing_paper":{"arxiv_id":"2505.24743","last_updated":"2025-06-11T17:49:24Z","snapshot_observed_at":"2026-08-07T12:12:18.402918Z","submitted_at":"2025-05-30T16:01:50Z","title":"What solves the Hubble tension in phenomenological dark energy models at background level?","version":2},"reference_index":35,"source":"pdf_text","source_observed_at":"2026-08-07T12:22:17.405395Z"},"links":{"citing_paper":"/paper/2505.24743"},"observation_digest":"sha256:6c713968527343ca17b1d702dbb0e596c897f3378d9645fd86b6124ec00e6819","observation_id":"0dfb6b06-7ca3-46e7-8a71-d615463a676d","resolution":{"observed_at":"2026-08-07T12:22:28.889984Z","resolver_source":"raw_fallback","status":"verified_fuzzy"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-07T06:34:17.273281+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-07T06:34:17.273281+00:00","source":"crossref"},{"observed_at":"2026-08-07T06:34:11.927384+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":"raw_reference","pith_arxiv_id":null,"snapshot_observed_at":"2026-08-07T12:22:28.625643Z","title":"Moresco et al","venue":null,"work_id":"8fdf7153-0d0f-45f6-8422-ea8167fad60b","year":2016},"citing_paper":{"arxiv_id":"2505.24743","last_updated":"2025-06-11T17:49:24Z","snapshot_observed_at":"2026-08-07T12:12:18.402918Z","submitted_at":"2025-05-30T16:01:50Z","title":"What solves the Hubble tension in phenomenological dark energy models at background level?","version":2},"reference_index":36,"source":"pdf_text","source_observed_at":"2026-08-07T12:22:17.501929Z"},"links":{"citing_paper":"/paper/2505.24743"},"observation_digest":"sha256:ee88249008f464761ed2499880e8c6f2f231dd4a4d3a08d7dc28b0286c9286df","observation_id":"58bd1a11-b070-43c8-a689-5a7d10194f95","resolution":{"observed_at":"2026-08-07T12:22:28.715199Z","resolver_source":"raw_fallback","status":"verified_fuzzy"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-07T06:34:17.273281+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-07T06:34:17.273281+00:00","source":"crossref"},{"observed_at":"2026-08-07T06:34:11.927384+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":"raw_reference","pith_arxiv_id":null,"snapshot_observed_at":"2026-08-07T12:22:28.489671Z","title":null,"venue":null,"work_id":"b06c3d57-2501-4f9a-adcd-27a33a79d3f5","year":2014},"citing_paper":{"arxiv_id":"2505.24743","last_updated":"2025-06-11T17:49:24Z","snapshot_observed_at":"2026-08-07T12:12:18.402918Z","submitted_at":"2025-05-30T16:01:50Z","title":"What solves the Hubble tension in phenomenological dark energy models at background level?","version":2},"reference_index":37,"source":"pdf_text","source_observed_at":"2026-08-07T12:22:17.573684Z"},"links":{"citing_paper":"/paper/2505.24743"},"observation_digest":"sha256:ad11bc664676e2894ec1249e9e16bd0597e2d390f95d22b3a003abe06b518e57","observation_id":"07b75a2a-854a-41cd-9494-a65ca8d5481d","resolution":{"observed_at":"2026-08-07T12:22:28.542611Z","resolver_source":"raw_fallback","status":"unresolved"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-07T06:34:17.273281+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-07T06:34:17.273281+00:00","source":"crossref"},{"observed_at":"2026-08-07T06:34:11.927384+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":"raw_reference","pith_arxiv_id":null,"snapshot_observed_at":"2026-08-07T12:22:28.333406Z","title":"Moresco et al","venue":null,"work_id":"facc9582-75bc-4efa-b52b-3aca92ea28d6","year":2012},"citing_paper":{"arxiv_id":"2505.24743","last_updated":"2025-06-11T17:49:24Z","snapshot_observed_at":"2026-08-07T12:12:18.402918Z","submitted_at":"2025-05-30T16:01:50Z","title":"What solves the Hubble tension in phenomenological dark energy models at background level?","version":2},"reference_index":38,"source":"pdf_text","source_observed_at":"2026-08-07T12:22:17.661102Z"},"links":{"citing_paper":"/paper/2505.24743"},"observation_digest":"sha256:0749234099b41fe036b228e5d7a5e6dd91790e83ea248f4d250231819b1e7e63","observation_id":"a646ef39-85a5-4d3f-b740-7e55f115581e","resolution":{"observed_at":"2026-08-07T12:22:28.388141Z","resolver_source":"raw_fallback","status":"verified_fuzzy"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-07T06:34:17.273281+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-07T06:34:17.273281+00:00","source":"crossref"},{"observed_at":"2026-08-07T06:34:11.927384+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":"raw_reference","pith_arxiv_id":null,"snapshot_observed_at":"2026-08-07T12:22:28.136307Z","title":"Moresco, Monthly Notices of the Royal Astronomical Soci- ety: Letters 450, L16 (2015)","venue":null,"work_id":"e857c09c-dca7-4a3f-8695-0d52555cc125","year":2015},"citing_paper":{"arxiv_id":"2505.24743","last_updated":"2025-06-11T17:49:24Z","snapshot_observed_at":"2026-08-07T12:12:18.402918Z","submitted_at":"2025-05-30T16:01:50Z","title":"What solves the Hubble tension in phenomenological dark energy models at background level?","version":2},"reference_index":39,"source":"pdf_text","source_observed_at":"2026-08-07T12:22:17.761892Z"},"links":{"citing_paper":"/paper/2505.24743"},"observation_digest":"sha256:2df37032a6a3278e77b3637bb26b49a802441c71a8eaf3c44feb94e1584809bb","observation_id":"1e3b62e2-c9eb-4636-8bd3-300f70cf56e2","resolution":{"observed_at":"2026-08-07T12:22:28.234903Z","resolver_source":"raw_fallback","status":"verified_fuzzy"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-07T06:34:17.273281+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-07T06:34:17.273281+00:00","source":"crossref"},{"observed_at":"2026-08-07T06:34:11.927384+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":"raw_reference","pith_arxiv_id":null,"snapshot_observed_at":"2026-08-07T12:22:26.896951Z","title":"Chuang and Y","venue":null,"work_id":"a6f1c290-aa26-49fa-b574-b9dd38cdbe3e","year":2013},"citing_paper":{"arxiv_id":"2505.24743","last_updated":"2025-06-11T17:49:24Z","snapshot_observed_at":"2026-08-07T12:12:18.402918Z","submitted_at":"2025-05-30T16:01:50Z","title":"What solves the Hubble tension in phenomenological dark energy models at background level?","version":2},"reference_index":40,"source":"pdf_text","source_observed_at":"2026-08-07T12:22:18.358725Z"},"links":{"citing_paper":"/paper/2505.24743"},"observation_digest":"sha256:abfc1748ba1897b72e9e21c9d58d249194f199642196157a8412ed1c40c54edf","observation_id":"91004b6e-e7fc-4939-89a7-04901ddb15a9","resolution":{"observed_at":"2026-08-07T12:22:26.961844Z","resolver_source":"raw_fallback","status":"verified_fuzzy"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-07T06:34:17.273281+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-07T06:34:17.273281+00:00","source":"crossref"},{"observed_at":"2026-08-07T06:34:11.927384+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":"raw_reference","pith_arxiv_id":null,"snapshot_observed_at":"2026-08-07T12:22:27.719015Z","title":"Alam et al","venue":null,"work_id":"84a93bc3-d944-4953-9e4d-21d09f0a82f1","year":2017},"citing_paper":{"arxiv_id":"2505.24743","last_updated":"2025-06-11T17:49:24Z","snapshot_observed_at":"2026-08-07T12:12:18.402918Z","submitted_at":"2025-05-30T16:01:50Z","title":"What solves the Hubble tension in phenomenological dark energy models at background level?","version":2},"reference_index":41,"source":"pdf_text","source_observed_at":"2026-08-07T12:22:17.879288Z"},"links":{"citing_paper":"/paper/2505.24743"},"observation_digest":"sha256:347cfca6191cfa5feb6a50f1f57b8253fa270f1cc6461560e6c2147825e59f45","observation_id":"4230d422-6533-4dc8-95b7-1a4ad384d2a1","resolution":{"observed_at":"2026-08-07T12:22:27.820834Z","resolver_source":"raw_fallback","status":"verified_fuzzy"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-07T06:34:17.273281+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-07T06:34:17.273281+00:00","source":"crossref"},{"observed_at":"2026-08-07T06:34:11.927384+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":"raw_reference","pith_arxiv_id":null,"snapshot_observed_at":"2026-08-07T12:22:27.543617Z","title":"Anderson et al., Monthly Notices of the Royal Astronomical Society 441, 24 (2014)","venue":null,"work_id":"f7229c6f-aa81-48e1-84e0-32a37f94942e","year":2014},"citing_paper":{"arxiv_id":"2505.24743","last_updated":"2025-06-11T17:49:24Z","snapshot_observed_at":"2026-08-07T12:12:18.402918Z","submitted_at":"2025-05-30T16:01:50Z","title":"What solves the Hubble tension in phenomenological dark energy models at background level?","version":2},"reference_index":42,"source":"pdf_text","source_observed_at":"2026-08-07T12:22:17.951356Z"},"links":{"citing_paper":"/paper/2505.24743"},"observation_digest":"sha256:450f8d1e3b7b190fc01d26a19249c7b36f14ca979554c93d7034a57039968865","observation_id":"56c49e77-3ffc-41ad-bd1e-48e9ebdf2959","resolution":{"observed_at":"2026-08-07T12:22:27.617473Z","resolver_source":"raw_fallback","status":"verified_fuzzy"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-07T06:34:17.273281+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-07T06:34:17.273281+00:00","source":"crossref"},{"observed_at":"2026-08-07T06:34:11.927384+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":"raw_reference","pith_arxiv_id":null,"snapshot_observed_at":"2026-08-07T12:22:27.360187Z","title":"Blake et al","venue":null,"work_id":"4b77957f-2a3e-4d97-b475-4635b5a93be6","year":2012},"citing_paper":{"arxiv_id":"2505.24743","last_updated":"2025-06-11T17:49:24Z","snapshot_observed_at":"2026-08-07T12:12:18.402918Z","submitted_at":"2025-05-30T16:01:50Z","title":"What solves the Hubble tension in phenomenological dark energy models at background level?","version":2},"reference_index":43,"source":"pdf_text","source_observed_at":"2026-08-07T12:22:18.045041Z"},"links":{"citing_paper":"/paper/2505.24743"},"observation_digest":"sha256:f0ed31eeef1cb07be03d94bc654b98d2785d8bb20451f4bcb0b5b75d63607c76","observation_id":"b0a5c652-45b4-4681-86fb-1573f5adea66","resolution":{"observed_at":"2026-08-07T12:22:27.447076Z","resolver_source":"raw_fallback","status":"verified_fuzzy"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-07T06:34:17.273281+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-07T06:34:17.273281+00:00","source":"crossref"},{"observed_at":"2026-08-07T06:34:11.927384+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":"raw_reference","pith_arxiv_id":null,"snapshot_observed_at":"2026-08-07T12:22:27.196541Z","title":"Wang et al","venue":null,"work_id":"b491ab49-5b54-4e96-a7e3-62185eb294b4","year":2017},"citing_paper":{"arxiv_id":"2505.24743","last_updated":"2025-06-11T17:49:24Z","snapshot_observed_at":"2026-08-07T12:12:18.402918Z","submitted_at":"2025-05-30T16:01:50Z","title":"What solves the Hubble tension in phenomenological dark energy models at background level?","version":2},"reference_index":44,"source":"pdf_text","source_observed_at":"2026-08-07T12:22:18.125817Z"},"links":{"citing_paper":"/paper/2505.24743"},"observation_digest":"sha256:1770a306ca2a78bd5e8e1ff568e71aee4184e01313dabc7a7f4e5cbf62dea0f5","observation_id":"eeb00fed-2ac7-4cb9-bad0-7c28547c2897","resolution":{"observed_at":"2026-08-07T12:22:27.256693Z","resolver_source":"raw_fallback","status":"verified_fuzzy"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-07T06:34:17.273281+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-07T06:34:17.273281+00:00","source":"crossref"},{"observed_at":"2026-08-07T06:34:11.927384+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":"raw_reference","pith_arxiv_id":null,"snapshot_observed_at":"2026-08-07T12:22:27.052846Z","title":null,"venue":null,"work_id":"2ada6b52-168d-467f-a25e-ca741f34ddd3","year":2014},"citing_paper":{"arxiv_id":"2505.24743","last_updated":"2025-06-11T17:49:24Z","snapshot_observed_at":"2026-08-07T12:12:18.402918Z","submitted_at":"2025-05-30T16:01:50Z","title":"What solves the Hubble tension in phenomenological dark energy models at background level?","version":2},"reference_index":45,"source":"pdf_text","source_observed_at":"2026-08-07T12:22:18.228865Z"},"links":{"citing_paper":"/paper/2505.24743"},"observation_digest":"sha256:461b7a0ab9bde4ed1fd66fe088a7fcb4fb1000a69e4d44655cd1ad99a53624df","observation_id":"45b72609-ac8f-4b35-a654-15f8d309fdcb","resolution":{"observed_at":"2026-08-07T12:22:27.121512Z","resolver_source":"raw_fallback","status":"unresolved"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-07T06:34:17.273281+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-07T06:34:17.273281+00:00","source":"crossref"},{"observed_at":"2026-08-07T06:34:11.927384+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":"raw_reference","pith_arxiv_id":null,"snapshot_observed_at":"2026-08-07T12:22:25.912942Z","title":"Alam et al., Phys","venue":null,"work_id":"99859e0e-ed35-4e23-af70-e1ae248a6448","year":2021},"citing_paper":{"arxiv_id":"2505.24743","last_updated":"2025-06-11T17:49:24Z","snapshot_observed_at":"2026-08-07T12:12:18.402918Z","submitted_at":"2025-05-30T16:01:50Z","title":"What solves the Hubble tension in phenomenological dark energy models at background level?","version":2},"reference_index":46,"source":"pdf_text","source_observed_at":"2026-08-07T12:22:18.820974Z"},"links":{"citing_paper":"/paper/2505.24743"},"observation_digest":"sha256:b1fe6d9d202423315131988aea86ac7d9a3cb4af4db8731e7c4f68ebb76c67d7","observation_id":"98b1f451-12c2-4840-b7ce-79a793bb9dee","resolution":{"observed_at":"2026-08-07T12:22:25.980120Z","resolver_source":"raw_fallback","status":"verified_fuzzy"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-07T06:34:17.273281+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-07T06:34:17.273281+00:00","source":"crossref"},{"observed_at":"2026-08-07T06:34:11.927384+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":"raw_reference","pith_arxiv_id":null,"snapshot_observed_at":"2026-08-07T12:22:26.713391Z","title":"Gaztanaga, A","venue":null,"work_id":"2d6523e5-f458-475e-ae20-f270f043bf4d","year":2009},"citing_paper":{"arxiv_id":"2505.24743","last_updated":"2025-06-11T17:49:24Z","snapshot_observed_at":"2026-08-07T12:12:18.402918Z","submitted_at":"2025-05-30T16:01:50Z","title":"What solves the Hubble tension in phenomenological dark energy models at background level?","version":2},"reference_index":47,"source":"pdf_text","source_observed_at":"2026-08-07T12:22:18.456261Z"},"links":{"citing_paper":"/paper/2505.24743"},"observation_digest":"sha256:d87b3d21f6bcbb6a0224433d9cd2babf74c752ee1e6ec431fa38ff452f52ccb6","observation_id":"5d39ed47-eebb-4136-89f1-56daa42c2569","resolution":{"observed_at":"2026-08-07T12:22:26.783986Z","resolver_source":"raw_fallback","status":"verified_fuzzy"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-07T06:34:17.273281+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-07T06:34:17.273281+00:00","source":"crossref"},{"observed_at":"2026-08-07T06:34:11.927384+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":"raw_reference","pith_arxiv_id":null,"snapshot_observed_at":"2026-08-07T12:22:26.559985Z","title":null,"venue":null,"work_id":"5a83ec13-f56f-4062-bf53-d998e550223e","year":2013},"citing_paper":{"arxiv_id":"2505.24743","last_updated":"2025-06-11T17:49:24Z","snapshot_observed_at":"2026-08-07T12:12:18.402918Z","submitted_at":"2025-05-30T16:01:50Z","title":"What solves the Hubble tension in phenomenological dark energy models at background level?","version":2},"reference_index":48,"source":"pdf_text","source_observed_at":"2026-08-07T12:22:18.525984Z"},"links":{"citing_paper":"/paper/2505.24743"},"observation_digest":"sha256:8d2a2cdf60d5eaa25363d6a10906185a5cf80ef4fdad96aba34994a3fd701321","observation_id":"0e67d4d0-947b-4be9-a1b9-a2c80fddce1f","resolution":{"observed_at":"2026-08-07T12:22:26.627866Z","resolver_source":"raw_fallback","status":"unresolved"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-07T06:34:17.273281+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-07T06:34:17.273281+00:00","source":"crossref"},{"observed_at":"2026-08-07T06:34:11.927384+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":"raw_reference","pith_arxiv_id":null,"snapshot_observed_at":"2026-08-07T12:22:26.372468Z","title":"Font-Ribera et al., Journal of Cosmology and Astroparticle Physics 2014, 027 (2014)","venue":null,"work_id":"f97d115f-7e2e-47e3-b376-df71cd221a15","year":2014},"citing_paper":{"arxiv_id":"2505.24743","last_updated":"2025-06-11T17:49:24Z","snapshot_observed_at":"2026-08-07T12:12:18.402918Z","submitted_at":"2025-05-30T16:01:50Z","title":"What solves the Hubble tension in phenomenological dark energy models at background level?","version":2},"reference_index":49,"source":"pdf_text","source_observed_at":"2026-08-07T12:22:18.587748Z"},"links":{"citing_paper":"/paper/2505.24743"},"observation_digest":"sha256:df625c84c1a429c0b4e747c81cfc9d1bba112444868fe711400b9bdcc478e8f3","observation_id":"b6cad08b-3214-4882-bf80-a57a1445c367","resolution":{"observed_at":"2026-08-07T12:22:26.444128Z","resolver_source":"raw_fallback","status":"verified_fuzzy"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-07T06:34:17.273281+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-07T06:34:17.273281+00:00","source":"crossref"},{"observed_at":"2026-08-07T06:34:11.927384+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":"raw_reference","pith_arxiv_id":null,"snapshot_observed_at":"2026-08-07T12:22:26.223649Z","title":null,"venue":null,"work_id":"41ddf028-52f0-4108-bfae-aa654ab9a50e","year":2015},"citing_paper":{"arxiv_id":"2505.24743","last_updated":"2025-06-11T17:49:24Z","snapshot_observed_at":"2026-08-07T12:12:18.402918Z","submitted_at":"2025-05-30T16:01:50Z","title":"What solves the Hubble tension in phenomenological dark energy models at background level?","version":2},"reference_index":50,"source":"pdf_text","source_observed_at":"2026-08-07T12:22:18.663193Z"},"links":{"citing_paper":"/paper/2505.24743"},"observation_digest":"sha256:603ba7a8269eb2cf62183e46a8258bde6ecd71f5ef3b72b0f11374d7219f5288","observation_id":"3ef80c64-3d43-4fcb-9d40-af3670e26a15","resolution":{"observed_at":"2026-08-07T12:22:26.287548Z","resolver_source":"raw_fallback","status":"unresolved"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-07T06:34:17.273281+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-07T06:34:17.273281+00:00","source":"crossref"},{"observed_at":"2026-08-07T06:34:11.927384+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":"raw_reference","pith_arxiv_id":null,"snapshot_observed_at":"2026-08-07T12:22:26.058782Z","title":"et al., A&A 603, A12 (2017)","venue":null,"work_id":"8e654ce4-6cea-44bb-9bc8-a52fda4260d7","year":2017},"citing_paper":{"arxiv_id":"2505.24743","last_updated":"2025-06-11T17:49:24Z","snapshot_observed_at":"2026-08-07T12:12:18.402918Z","submitted_at":"2025-05-30T16:01:50Z","title":"What solves the Hubble tension in phenomenological dark energy models at background level?","version":2},"reference_index":51,"source":"pdf_text","source_observed_at":"2026-08-07T12:22:18.745223Z"},"links":{"citing_paper":"/paper/2505.24743"},"observation_digest":"sha256:a532476969dacbcd921eb24f058fe8328ee6118b119366a46cc2cb4468982bf6","observation_id":"2878cd7e-f5db-424b-bd7e-92fc21f32b07","resolution":{"observed_at":"2026-08-07T12:22:26.126873Z","resolver_source":"raw_fallback","status":"verified_fuzzy"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-07T06:34:17.273281+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-07T06:34:17.273281+00:00","source":"crossref"},{"observed_at":"2026-08-07T06:34:11.927384+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":"raw_reference","pith_arxiv_id":null,"snapshot_observed_at":"2026-08-07T12:22:32.980639Z","title":"For similar reasons, we do not consider the DES compilation either [54]","venue":null,"work_id":"6ec1ef9c-422e-413d-bb52-97af321dc764","year":null},"citing_paper":{"arxiv_id":"2505.24743","last_updated":"2025-06-11T17:49:24Z","snapshot_observed_at":"2026-08-07T12:12:18.402918Z","submitted_at":"2025-05-30T16:01:50Z","title":"What solves the Hubble tension in phenomenological dark energy models at background level?","version":2},"reference_index":52,"source":"pdf_text","source_observed_at":"2026-08-07T12:22:14.309266Z"},"links":{"citing_paper":"/paper/2505.24743"},"observation_digest":"sha256:0f8630188b9485d34bcf4d334a6486abb77729bb5934882708a916fba23206fb","observation_id":"9ee80ef4-f362-4277-bc10-db8cebe39b0e","resolution":{"observed_at":"2026-08-07T12:22:33.085677Z","resolver_source":"raw_fallback","status":"verified_fuzzy"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-07T06:34:17.273281+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-07T06:34:17.273281+00:00","source":"crossref"},{"observed_at":"2026-08-07T06:34:11.927384+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":"raw_reference","pith_arxiv_id":null,"snapshot_observed_at":"2026-08-07T12:22:25.769618Z","title":"du Mas des Bourboux et al., The Astrophysical Journal 901, 153 (2020)","venue":null,"work_id":"1f97ec60-f364-48b3-97e0-40e80bb8e922","year":2020},"citing_paper":{"arxiv_id":"2505.24743","last_updated":"2025-06-11T17:49:24Z","snapshot_observed_at":"2026-08-07T12:12:18.402918Z","submitted_at":"2025-05-30T16:01:50Z","title":"What solves the Hubble tension in phenomenological dark energy models at background level?","version":2},"reference_index":53,"source":"pdf_text","source_observed_at":"2026-08-07T12:22:18.901218Z"},"links":{"citing_paper":"/paper/2505.24743"},"observation_digest":"sha256:559938cca7b11725d679805271acbdc53783471b72288113d74582e45d171f80","observation_id":"05bd76b5-44d5-43ef-b4f5-255836d2ff22","resolution":{"observed_at":"2026-08-07T12:22:25.833286Z","resolver_source":"raw_fallback","status":"verified_fuzzy"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-07T06:34:17.273281+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-07T06:34:17.273281+00:00","source":"crossref"},{"observed_at":"2026-08-07T06:34:11.927384+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":"raw_reference","pith_arxiv_id":null,"snapshot_observed_at":"2026-08-07T12:22:25.617062Z","title":"Adame et al","venue":null,"work_id":"c4484869-e575-43dc-a891-ecb07013b18b","year":2025},"citing_paper":{"arxiv_id":"2505.24743","last_updated":"2025-06-11T17:49:24Z","snapshot_observed_at":"2026-08-07T12:12:18.402918Z","submitted_at":"2025-05-30T16:01:50Z","title":"What solves the Hubble tension in phenomenological dark energy models at background level?","version":2},"reference_index":54,"source":"pdf_text","source_observed_at":"2026-08-07T12:22:18.984098Z"},"links":{"citing_paper":"/paper/2505.24743"},"observation_digest":"sha256:e52daa6e8fa4453235a8d22c55204b0696755dbca27c416fbcf9228b1ec7008c","observation_id":"d0e2a3c1-626a-4f2c-ae1a-6549a53c8a56","resolution":{"observed_at":"2026-08-07T12:22:25.698031Z","resolver_source":"raw_fallback","status":"verified_fuzzy"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-07T06:34:17.273281+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-07T06:34:17.273281+00:00","source":"crossref"},{"observed_at":"2026-08-07T06:34:11.927384+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":{"arxiv_id":"2504.07299","last_updated":"2025-05-04T15:00:56Z","snapshot_observed_at":"2026-08-07T16:07:02.612122Z","submitted_at":"2025-04-09T21:41:35Z","title":"Dynamical dark energy with AdS-dS transitions vs. Baryon Acoustic Oscillations at $z =$ 2.3-2.4","version":2},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2504.07299","snapshot_observed_at":"2026-08-07T12:22:19.023796Z","title":"Akarsu, M","venue":null,"work_id":null,"year":2025},"citing_paper":{"arxiv_id":"2505.24743","last_updated":"2025-06-11T17:49:24Z","snapshot_observed_at":"2026-08-07T12:12:18.402918Z","submitted_at":"2025-05-30T16:01:50Z","title":"What solves the Hubble tension in phenomenological dark energy models at background level?","version":2},"reference_index":55,"source":"pdf_text","source_observed_at":"2026-08-07T12:22:19.023796Z"},"links":{"cited_paper":"/paper/2504.07299","citing_paper":"/paper/2505.24743"},"observation_digest":"sha256:6667fcd56b49f17fb9a558eb1396e4cb70e45ae1f28c824b90ccff3c6408b184","observation_id":"358f6a88-fad2-4512-b32a-542be7115b29","resolution":{"observed_at":"2026-08-07T12:22:19.023796Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":"raw_reference","pith_arxiv_id":null,"snapshot_observed_at":"2026-08-07T12:22:25.440254Z","title":null,"venue":null,"work_id":"60e5f980-f8e3-4e8d-80d6-e05bf95b0b9e","year":1998},"citing_paper":{"arxiv_id":"2505.24743","last_updated":"2025-06-11T17:49:24Z","snapshot_observed_at":"2026-08-07T12:12:18.402918Z","submitted_at":"2025-05-30T16:01:50Z","title":"What solves the Hubble tension in phenomenological dark energy models at background level?","version":2},"reference_index":56,"source":"pdf_text","source_observed_at":"2026-08-07T12:22:19.118625Z"},"links":{"citing_paper":"/paper/2505.24743"},"observation_digest":"sha256:cd2eabf35137fe38d28a99a352e7f81ee45a5b06efffc4d36568debbf5ce7c98","observation_id":"2dd1297a-4e1f-4db2-ba22-64ca9570cfd5","resolution":{"observed_at":"2026-08-07T12:22:25.520158Z","resolver_source":"raw_fallback","status":"unresolved"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-07T06:34:17.273281+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-07T06:34:17.273281+00:00","source":"crossref"},{"observed_at":"2026-08-07T06:34:11.927384+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":"raw_reference","pith_arxiv_id":null,"snapshot_observed_at":"2026-08-07T12:22:25.281236Z","title":"Perlmutter et al","venue":null,"work_id":"fcdd23f3-cdaa-4de9-a4fc-36d7e817068e","year":1998},"citing_paper":{"arxiv_id":"2505.24743","last_updated":"2025-06-11T17:49:24Z","snapshot_observed_at":"2026-08-07T12:12:18.402918Z","submitted_at":"2025-05-30T16:01:50Z","title":"What solves the Hubble tension in phenomenological dark energy models at background level?","version":2},"reference_index":57,"source":"pdf_text","source_observed_at":"2026-08-07T12:22:19.223617Z"},"links":{"citing_paper":"/paper/2505.24743"},"observation_digest":"sha256:741118da6d406e786b5de9c5ae36cb748b02e39bdf2b20876aea6c5b0d97f0cc","observation_id":"c34b6522-9ef4-4d38-9300-714e884242a3","resolution":{"observed_at":"2026-08-07T12:22:25.361574Z","resolver_source":"raw_fallback","status":"verified_fuzzy"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-07T06:34:17.273281+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-07T06:34:17.273281+00:00","source":"crossref"},{"observed_at":"2026-08-07T06:34:11.927384+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":"raw_reference","pith_arxiv_id":null,"snapshot_observed_at":"2026-08-07T12:22:25.118375Z","title":"Suzuki et al., The Astrophysical Journal 746, 85 (2012)","venue":null,"work_id":"70c7deb7-1f80-44cd-ab95-7e5938380899","year":2012},"citing_paper":{"arxiv_id":"2505.24743","last_updated":"2025-06-11T17:49:24Z","snapshot_observed_at":"2026-08-07T12:12:18.402918Z","submitted_at":"2025-05-30T16:01:50Z","title":"What solves the Hubble tension in phenomenological dark energy models at background level?","version":2},"reference_index":58,"source":"pdf_text","source_observed_at":"2026-08-07T12:22:19.296212Z"},"links":{"citing_paper":"/paper/2505.24743"},"observation_digest":"sha256:b0faa507473d8b9be5bb1af5ab87c5d76b28e5e194b08602b5a326e04ee01743","observation_id":"5692660b-361e-4d36-a042-1828f6f97218","resolution":{"observed_at":"2026-08-07T12:22:25.207026Z","resolver_source":"raw_fallback","status":"verified_fuzzy"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-07T06:34:17.273281+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-07T06:34:17.273281+00:00","source":"crossref"},{"observed_at":"2026-08-07T06:34:11.927384+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":{"arxiv_id":"2311.12098","last_updated":"2025-06-20T17:34:15Z","snapshot_observed_at":"2026-07-06T02:11:23.670680Z","submitted_at":"2023-11-20T19:00:01Z","title":"Union Through UNITY: Cosmology with 2,000 SNe Using a Unified Bayesian Framework","version":4},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"2311.12098","snapshot_observed_at":"2026-08-07T12:22:19.374684Z","title":"Rubin, G","venue":null,"work_id":null,"year":2023},"citing_paper":{"arxiv_id":"2505.24743","last_updated":"2025-06-11T17:49:24Z","snapshot_observed_at":"2026-08-07T12:12:18.402918Z","submitted_at":"2025-05-30T16:01:50Z","title":"What solves the Hubble tension in phenomenological dark energy models at background level?","version":2},"reference_index":59,"source":"pdf_text","source_observed_at":"2026-08-07T12:22:19.374684Z"},"links":{"cited_paper":"/paper/2311.12098","citing_paper":"/paper/2505.24743"},"observation_digest":"sha256:b8d906a8d1e6ba2d4a07c2d566776a83b5d248f89a3174f912bfd6e423a019b6","observation_id":"843bca54-a140-48fa-bfb5-8fd1e809a6d3","resolution":{"observed_at":"2026-08-07T12:22:19.374684Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":"raw_reference","pith_arxiv_id":null,"snapshot_observed_at":"2026-08-07T12:22:24.933298Z","title":"Collaboration et al., The Astrophysical Journal Letters 973, L14 (2024)","venue":null,"work_id":"a2b0cc58-1d68-4bb9-93a7-423169731b8b","year":2024},"citing_paper":{"arxiv_id":"2505.24743","last_updated":"2025-06-11T17:49:24Z","snapshot_observed_at":"2026-08-07T12:12:18.402918Z","submitted_at":"2025-05-30T16:01:50Z","title":"What solves the Hubble tension in phenomenological dark energy models at background level?","version":2},"reference_index":60,"source":"pdf_text","source_observed_at":"2026-08-07T12:22:19.455975Z"},"links":{"citing_paper":"/paper/2505.24743"},"observation_digest":"sha256:512aeb19b56503da70d789e5f2c5704d13942cfc718d38919e930b3a6756ca97","observation_id":"c8344ed3-585e-416f-8a89-5d4221c45652","resolution":{"observed_at":"2026-08-07T12:22:25.013453Z","resolver_source":"raw_fallback","status":"verified_fuzzy"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-07T06:34:17.273281+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-07T06:34:17.273281+00:00","source":"crossref"},{"observed_at":"2026-08-07T06:34:11.927384+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":"raw_reference","pith_arxiv_id":null,"snapshot_observed_at":"2026-08-07T12:22:24.783639Z","title":null,"venue":null,"work_id":"5b1c19ae-964b-4a87-8832-e09ea00219f4","year":2021},"citing_paper":{"arxiv_id":"2505.24743","last_updated":"2025-06-11T17:49:24Z","snapshot_observed_at":"2026-08-07T12:12:18.402918Z","submitted_at":"2025-05-30T16:01:50Z","title":"What solves the Hubble tension in phenomenological dark energy models at background level?","version":2},"reference_index":61,"source":"pdf_text","source_observed_at":"2026-08-07T12:22:19.560346Z"},"links":{"citing_paper":"/paper/2505.24743"},"observation_digest":"sha256:fca6c8522ece70ff1ead6f61580767168d37fc85650ede69dae10d8b6c5cd6bd","observation_id":"142b89fa-99c1-44ee-8457-4f1444d53028","resolution":{"observed_at":"2026-08-07T12:22:24.850115Z","resolver_source":"raw_fallback","status":"unresolved"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-07T06:34:17.273281+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-07T06:34:17.273281+00:00","source":"crossref"},{"observed_at":"2026-08-07T06:34:11.927384+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":"raw_reference","pith_arxiv_id":null,"snapshot_observed_at":"2026-08-07T12:22:24.637407Z","title":"Code for anisotropies in the mi- crowave background (camb),","venue":null,"work_id":"6dc1615f-a17c-42da-b5cc-af724c4bccf8","year":null},"citing_paper":{"arxiv_id":"2505.24743","last_updated":"2025-06-11T17:49:24Z","snapshot_observed_at":"2026-08-07T12:12:18.402918Z","submitted_at":"2025-05-30T16:01:50Z","title":"What solves the Hubble tension in phenomenological dark energy models at background level?","version":2},"reference_index":62,"source":"pdf_text","source_observed_at":"2026-08-07T12:22:19.671749Z"},"links":{"citing_paper":"/paper/2505.24743"},"observation_digest":"sha256:65a3bb928ab086871e3b2856f4f0f942f2a35246ff736d6aaae2d50eb32b68b5","observation_id":"dc2f4d65-8e88-42c1-8c78-44676c6d23f9","resolution":{"observed_at":"2026-08-07T12:22:24.704044Z","resolver_source":"raw_fallback","status":"verified_fuzzy"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-07T06:34:17.273281+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-07T06:34:17.273281+00:00","source":"crossref"},{"observed_at":"2026-08-07T06:34:11.927384+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":"raw_reference","pith_arxiv_id":null,"snapshot_observed_at":"2026-08-07T12:22:24.459529Z","title":"Chen, Q.-G","venue":null,"work_id":"7f8e5879-602f-4cdd-a87d-e71dfb822b77","year":2019},"citing_paper":{"arxiv_id":"2505.24743","last_updated":"2025-06-11T17:49:24Z","snapshot_observed_at":"2026-08-07T12:12:18.402918Z","submitted_at":"2025-05-30T16:01:50Z","title":"What solves the Hubble tension in phenomenological dark energy models at background level?","version":2},"reference_index":63,"source":"pdf_text","source_observed_at":"2026-08-07T12:22:19.781685Z"},"links":{"citing_paper":"/paper/2505.24743"},"observation_digest":"sha256:5145b1a59f6ce5c2a103cad9db805d1ee53baa3e88f8cbffc86d8da80a36f44c","observation_id":"9340bb32-f4ff-43a0-8d6e-b5717ae91b19","resolution":{"observed_at":"2026-08-07T12:22:24.562277Z","resolver_source":"raw_fallback","status":"verified_fuzzy"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-07T06:34:17.273281+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-07T06:34:17.273281+00:00","source":"crossref"},{"observed_at":"2026-08-07T06:34:11.927384+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":null,"snapshot_observed_at":"2026-08-07T12:22:19.891892Z","title":"Akaike, IEEE Transactions on Automatic Control 19, 716 (1974)","venue":null,"work_id":null,"year":1974},"citing_paper":{"arxiv_id":"2505.24743","last_updated":"2025-06-11T17:49:24Z","snapshot_observed_at":"2026-08-07T12:12:18.402918Z","submitted_at":"2025-05-30T16:01:50Z","title":"What solves the Hubble tension in phenomenological dark energy models at background level?","version":2},"reference_index":64,"source":"pdf_text","source_observed_at":"2026-08-07T12:22:19.891892Z"},"links":{"citing_paper":"/paper/2505.24743"},"observation_digest":"sha256:448764935482ee57cf1cbf17ca3ab03f35a3203b01174a33f649957c62f63da7","observation_id":"5099504a-02f5-41a3-9f89-56d4c0544ab9","resolution":{"observed_at":"2026-08-07T12:22:19.891892Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":"raw_reference","pith_arxiv_id":null,"snapshot_observed_at":"2026-08-07T12:22:24.303780Z","title":"Schwarz, The Annals of Statistics 6, 461 (1978)","venue":null,"work_id":"c2a9f9df-ad5f-4755-a91a-b8d24cb40093","year":1978},"citing_paper":{"arxiv_id":"2505.24743","last_updated":"2025-06-11T17:49:24Z","snapshot_observed_at":"2026-08-07T12:12:18.402918Z","submitted_at":"2025-05-30T16:01:50Z","title":"What solves the Hubble tension in phenomenological dark energy models at background level?","version":2},"reference_index":65,"source":"pdf_text","source_observed_at":"2026-08-07T12:22:20.000422Z"},"links":{"citing_paper":"/paper/2505.24743"},"observation_digest":"sha256:ae7021f61cdbbb382bdd3bb2ec14b991c1b8d05999d517e236894283265537dc","observation_id":"69f276cf-2bb7-4081-a39c-31da96eb31b3","resolution":{"observed_at":"2026-08-07T12:22:24.371925Z","resolver_source":"raw_fallback","status":"verified_fuzzy"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-07T06:34:17.273281+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-07T06:34:17.273281+00:00","source":"crossref"},{"observed_at":"2026-08-07T06:34:11.927384+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":"raw_reference","pith_arxiv_id":null,"snapshot_observed_at":"2026-08-07T12:22:24.135911Z","title":null,"venue":null,"work_id":"a16eb1d6-3b91-4b24-8022-e895f883a071","year":2002},"citing_paper":{"arxiv_id":"2505.24743","last_updated":"2025-06-11T17:49:24Z","snapshot_observed_at":"2026-08-07T12:12:18.402918Z","submitted_at":"2025-05-30T16:01:50Z","title":"What solves the Hubble tension in phenomenological dark energy models at background level?","version":2},"reference_index":66,"source":"pdf_text","source_observed_at":"2026-08-07T12:22:20.114026Z"},"links":{"citing_paper":"/paper/2505.24743"},"observation_digest":"sha256:5283c42a71538f01be3d545279ef56c6f31297a80b3293f537dbd8530e3f55cc","observation_id":"f3122fbb-1ade-4f7e-ba19-7c8744fe90ad","resolution":{"observed_at":"2026-08-07T12:22:24.206622Z","resolver_source":"raw_fallback","status":"unresolved"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-07T06:34:17.273281+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-07T06:34:17.273281+00:00","source":"crossref"},{"observed_at":"2026-08-07T06:34:11.927384+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":"raw_reference","pith_arxiv_id":null,"snapshot_observed_at":"2026-08-07T12:22:24.002776Z","title":"Sahni, A","venue":null,"work_id":"e15017dd-d088-4fb8-a05b-b3f2072b8e49","year":2014},"citing_paper":{"arxiv_id":"2505.24743","last_updated":"2025-06-11T17:49:24Z","snapshot_observed_at":"2026-08-07T12:12:18.402918Z","submitted_at":"2025-05-30T16:01:50Z","title":"What solves the Hubble tension in phenomenological dark energy models at background level?","version":2},"reference_index":67,"source":"pdf_text","source_observed_at":"2026-08-07T12:22:20.233352Z"},"links":{"citing_paper":"/paper/2505.24743"},"observation_digest":"sha256:8a0185a80c9a87064285d5a01e91436cc6a916852b10b0e77b32cb0ab4835764","observation_id":"0f047df5-73af-4d99-8ac9-d0ede5ac0644","resolution":{"observed_at":"2026-08-07T12:22:24.059774Z","resolver_source":"raw_fallback","status":"verified_fuzzy"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-07T06:34:17.273281+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-07T06:34:17.273281+00:00","source":"crossref"},{"observed_at":"2026-08-07T06:34:11.927384+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":"raw_reference","pith_arxiv_id":null,"snapshot_observed_at":"2026-08-07T12:22:23.839986Z","title":null,"venue":null,"work_id":"857dad4e-7dad-4b42-bdac-3ab4e44db4f0","year":2008},"citing_paper":{"arxiv_id":"2505.24743","last_updated":"2025-06-11T17:49:24Z","snapshot_observed_at":"2026-08-07T12:12:18.402918Z","submitted_at":"2025-05-30T16:01:50Z","title":"What solves the Hubble tension in phenomenological dark energy models at background level?","version":2},"reference_index":68,"source":"pdf_text","source_observed_at":"2026-08-07T12:22:20.344028Z"},"links":{"citing_paper":"/paper/2505.24743"},"observation_digest":"sha256:0a8209631659c0f91dd61dcc715744594b5f9471cfd7c91be6a7dd8a8ded388f","observation_id":"7cb81790-8a16-4352-9c74-ebb56d38c3c1","resolution":{"observed_at":"2026-08-07T12:22:23.924431Z","resolver_source":"raw_fallback","status":"unresolved"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-07T06:34:17.273281+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-07T06:34:17.273281+00:00","source":"crossref"},{"observed_at":"2026-08-07T06:34:11.927384+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":"raw_reference","pith_arxiv_id":null,"snapshot_observed_at":"2026-08-07T12:22:23.679254Z","title":null,"venue":null,"work_id":"daf72cb6-932b-4974-b0b1-708b1aef350a","year":2021},"citing_paper":{"arxiv_id":"2505.24743","last_updated":"2025-06-11T17:49:24Z","snapshot_observed_at":"2026-08-07T12:12:18.402918Z","submitted_at":"2025-05-30T16:01:50Z","title":"What solves the Hubble tension in phenomenological dark energy models at background level?","version":2},"reference_index":69,"source":"pdf_text","source_observed_at":"2026-08-07T12:22:20.427407Z"},"links":{"citing_paper":"/paper/2505.24743"},"observation_digest":"sha256:7431bbcce66db1b6eb064afe607f512bb23b70c3e7e2a9d4163ebf664464e2e9","observation_id":"e3eb00e5-dc94-4466-974f-2f028c7293ec","resolution":{"observed_at":"2026-08-07T12:22:23.740518Z","resolver_source":"raw_fallback","status":"unresolved"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-07T06:34:17.273281+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-07T06:34:17.273281+00:00","source":"crossref"},{"observed_at":"2026-08-07T06:34:11.927384+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":{"arxiv_id":"1807.07323","last_updated":"2018-07-19T10:00:27Z","snapshot_observed_at":"2026-08-03T15:26:22.834750Z","submitted_at":"2018-07-19T10:00:27Z","title":"How predictions of cosmological models depend on Hubble parameter data sets","version":1},"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":"1807.07323","snapshot_observed_at":"2026-08-07T12:22:20.516212Z","title":"Sharov and V","venue":null,"work_id":null,"year":2018},"citing_paper":{"arxiv_id":"2505.24743","last_updated":"2025-06-11T17:49:24Z","snapshot_observed_at":"2026-08-07T12:12:18.402918Z","submitted_at":"2025-05-30T16:01:50Z","title":"What solves the Hubble tension in phenomenological dark energy models at background level?","version":2},"reference_index":70,"source":"pdf_text","source_observed_at":"2026-08-07T12:22:20.516212Z"},"links":{"cited_paper":"/paper/1807.07323","citing_paper":"/paper/2505.24743"},"observation_digest":"sha256:cdb79f016794e83a706e01ef19aa0be261d1118d6088b8d54d9dda47070a9c7e","observation_id":"97b7e046-1695-4fc7-bd55-97388d9f05fe","resolution":{"observed_at":"2026-08-07T12:22:20.516212Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":null,"snapshot_observed_at":"2026-08-07T12:22:20.634030Z","title":null,"venue":null,"work_id":null,"year":2020},"citing_paper":{"arxiv_id":"2505.24743","last_updated":"2025-06-11T17:49:24Z","snapshot_observed_at":"2026-08-07T12:12:18.402918Z","submitted_at":"2025-05-30T16:01:50Z","title":"What solves the Hubble tension in phenomenological dark energy models at background level?","version":2},"reference_index":71,"source":"pdf_text","source_observed_at":"2026-08-07T12:22:20.634030Z"},"links":{"citing_paper":"/paper/2505.24743"},"observation_digest":"sha256:dc1bf7b7f116abeab01e3fa6e7accd766f835fd9ba2d808fbf9b9fba5edf3afa","observation_id":"258d3013-9740-4d86-ac0d-b19d39452016","resolution":{"observed_at":"2026-08-07T12:22:20.634030Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":"raw_reference","pith_arxiv_id":null,"snapshot_observed_at":"2026-08-07T12:22:23.485033Z","title":"pandas-dev/pandas: Pandas,","venue":null,"work_id":"102692b6-9e8a-4fb3-8504-dbea53724916","year":2020},"citing_paper":{"arxiv_id":"2505.24743","last_updated":"2025-06-11T17:49:24Z","snapshot_observed_at":"2026-08-07T12:12:18.402918Z","submitted_at":"2025-05-30T16:01:50Z","title":"What solves the Hubble tension in phenomenological dark energy models at background level?","version":2},"reference_index":72,"source":"pdf_text","source_observed_at":"2026-08-07T12:22:20.777923Z"},"links":{"citing_paper":"/paper/2505.24743"},"observation_digest":"sha256:100273888adbc0e2874c7fd84014077edddc1df66dbec3a3d51d6998b46ef298","observation_id":"70e549cc-49f3-441a-a130-12d265941cd3","resolution":{"observed_at":"2026-08-07T12:22:23.556842Z","resolver_source":"raw_fallback","status":"verified_fuzzy"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-07T06:34:17.273281+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-07T06:34:17.273281+00:00","source":"crossref"},{"observed_at":"2026-08-07T06:34:11.927384+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":"raw_reference","pith_arxiv_id":null,"snapshot_observed_at":"2026-08-07T12:22:23.269528Z","title":"Virtanen et al., Nature Methods 17, 261 (2020)","venue":null,"work_id":"9a1882df-8313-4eac-b920-eb30815d826a","year":2020},"citing_paper":{"arxiv_id":"2505.24743","last_updated":"2025-06-11T17:49:24Z","snapshot_observed_at":"2026-08-07T12:12:18.402918Z","submitted_at":"2025-05-30T16:01:50Z","title":"What solves the Hubble tension in phenomenological dark energy models at background level?","version":2},"reference_index":73,"source":"pdf_text","source_observed_at":"2026-08-07T12:22:20.909920Z"},"links":{"citing_paper":"/paper/2505.24743"},"observation_digest":"sha256:9ed042267640f05b75646a0a793894836d17e8c57e895daa00ce703287ee9224","observation_id":"207581f1-6ad4-4687-8cc9-955c6077e8c9","resolution":{"observed_at":"2026-08-07T12:22:23.366645Z","resolver_source":"raw_fallback","status":"verified_fuzzy"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-07T06:34:17.273281+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-07T06:34:17.273281+00:00","source":"crossref"},{"observed_at":"2026-08-07T06:34:11.927384+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":null,"snapshot_observed_at":"2026-08-07T12:22:21.024444Z","title":"Foreman-Mackey, D","venue":null,"work_id":null,"year":2013},"citing_paper":{"arxiv_id":"2505.24743","last_updated":"2025-06-11T17:49:24Z","snapshot_observed_at":"2026-08-07T12:12:18.402918Z","submitted_at":"2025-05-30T16:01:50Z","title":"What solves the Hubble tension in phenomenological dark energy models at background level?","version":2},"reference_index":74,"source":"pdf_text","source_observed_at":"2026-08-07T12:22:21.024444Z"},"links":{"citing_paper":"/paper/2505.24743"},"observation_digest":"sha256:8d09a8a89ff6871b7b85f64b065b9a2cb66660c0ee5e742def9bf3aee4e49e35","observation_id":"c29ce3fd-215e-43fa-b800-8c40653e1d03","resolution":{"observed_at":"2026-08-07T12:22:21.024444Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":"raw_reference","pith_arxiv_id":null,"snapshot_observed_at":"2026-08-07T12:22:23.049697Z","title":"lmfit/lmfit-py: 1.2.2,","venue":null,"work_id":"6c57ef12-443c-40e6-bf01-677f226a3a40","year":2023},"citing_paper":{"arxiv_id":"2505.24743","last_updated":"2025-06-11T17:49:24Z","snapshot_observed_at":"2026-08-07T12:12:18.402918Z","submitted_at":"2025-05-30T16:01:50Z","title":"What solves the Hubble tension in phenomenological dark energy models at background level?","version":2},"reference_index":75,"source":"pdf_text","source_observed_at":"2026-08-07T12:22:21.140245Z"},"links":{"citing_paper":"/paper/2505.24743"},"observation_digest":"sha256:b9e11100e30ee5da7b48d1354c09dee235c0edabe5719ea54cb81040d059f8ba","observation_id":"39257727-e522-47f6-a335-456b5e81d010","resolution":{"observed_at":"2026-08-07T12:22:23.141981Z","resolver_source":"raw_fallback","status":"verified_fuzzy"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-07T06:34:17.273281+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-07T06:34:17.273281+00:00","source":"crossref"},{"observed_at":"2026-08-07T06:34:11.927384+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":"raw_reference","pith_arxiv_id":null,"snapshot_observed_at":"2026-08-07T12:22:22.869803Z","title":"Abril-Pla et al., PeerJ Computer Science 9, e1516 (2023)","venue":null,"work_id":"421e43b5-8023-42c1-8b5f-4e7972737cc7","year":2023},"citing_paper":{"arxiv_id":"2505.24743","last_updated":"2025-06-11T17:49:24Z","snapshot_observed_at":"2026-08-07T12:12:18.402918Z","submitted_at":"2025-05-30T16:01:50Z","title":"What solves the Hubble tension in phenomenological dark energy models at background level?","version":2},"reference_index":76,"source":"pdf_text","source_observed_at":"2026-08-07T12:22:21.252327Z"},"links":{"citing_paper":"/paper/2505.24743"},"observation_digest":"sha256:49a93b3f78296504072397c4cbd1a9dd73cdb64966f2c3120ac1827e6d8a5b4f","observation_id":"7b4f80b3-d8f7-4c58-b4e1-38ef1723f415","resolution":{"observed_at":"2026-08-07T12:22:22.956864Z","resolver_source":"raw_fallback","status":"verified_fuzzy"},"standing_notice":{"events":[],"observation":"No event found in the named queried sources as of 2026-08-07T06:34:17.273281+00:00.","reason":null,"source_receipts":[{"observed_at":"2026-08-07T06:34:17.273281+00:00","source":"crossref"},{"observed_at":"2026-08-07T06:34:11.927384+00:00","source":"retraction_watch"}],"state":"measured"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":null,"snapshot_observed_at":"2026-08-07T12:22:21.393535Z","title":null,"venue":null,"work_id":null,"year":2021},"citing_paper":{"arxiv_id":"2505.24743","last_updated":"2025-06-11T17:49:24Z","snapshot_observed_at":"2026-08-07T12:12:18.402918Z","submitted_at":"2025-05-30T16:01:50Z","title":"What solves the Hubble tension in phenomenological dark energy models at background level?","version":2},"reference_index":77,"source":"pdf_text","source_observed_at":"2026-08-07T12:22:21.393535Z"},"links":{"citing_paper":"/paper/2505.24743"},"observation_digest":"sha256:1d91f4c504d4b9c01f8ccb2ef53f33afe52486f33a6a8ccd54d87bef7d37852d","observation_id":"3ab34140-77ae-48d7-a98a-9a1c58eb276f","resolution":{"observed_at":"2026-08-07T12:22:21.393535Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":null,"snapshot_observed_at":"2026-08-07T12:22:21.557120Z","title":"Foreman-Mackey, The Journal of Open Source Software 1, 24 (2016)","venue":null,"work_id":null,"year":2016},"citing_paper":{"arxiv_id":"2505.24743","last_updated":"2025-06-11T17:49:24Z","snapshot_observed_at":"2026-08-07T12:12:18.402918Z","submitted_at":"2025-05-30T16:01:50Z","title":"What solves the Hubble tension in phenomenological dark energy models at background level?","version":2},"reference_index":78,"source":"pdf_text","source_observed_at":"2026-08-07T12:22:21.557120Z"},"links":{"citing_paper":"/paper/2505.24743"},"observation_digest":"sha256:36a5967bd13563966be2d38f52f529c9583593e2f27d3a2139c40cb0b0bcd9af","observation_id":"28987390-a6fa-4189-a452-c202b3bd179c","resolution":{"observed_at":"2026-08-07T12:22:21.557120Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":null,"snapshot_observed_at":"2026-08-07T12:22:21.685178Z","title":null,"venue":null,"work_id":null,"year":2021},"citing_paper":{"arxiv_id":"2505.24743","last_updated":"2025-06-11T17:49:24Z","snapshot_observed_at":"2026-08-07T12:12:18.402918Z","submitted_at":"2025-05-30T16:01:50Z","title":"What solves the Hubble tension in phenomenological dark energy models at background level?","version":2},"reference_index":79,"source":"pdf_text","source_observed_at":"2026-08-07T12:22:21.685178Z"},"links":{"citing_paper":"/paper/2505.24743"},"observation_digest":"sha256:997a3839e3ecd3c2b0e77f60c42191570ca3c1fb3d1df416297a5b5f91e60312","observation_id":"b02f8820-2edb-45f2-8f60-b14de36a679f","resolution":{"observed_at":"2026-08-07T12:22:21.685178Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}},{"citation":{"cited_paper":null,"cited_work":{"arxiv_id":null,"doi":null,"metadata_source":null,"pith_arxiv_id":null,"snapshot_observed_at":"2026-08-07T12:22:21.787388Z","title":null,"venue":null,"work_id":null,"year":2007},"citing_paper":{"arxiv_id":"2505.24743","last_updated":"2025-06-11T17:49:24Z","snapshot_observed_at":"2026-08-07T12:12:18.402918Z","submitted_at":"2025-05-30T16:01:50Z","title":"What solves the Hubble tension in phenomenological dark energy models at background level?","version":2},"reference_index":80,"source":"pdf_text","source_observed_at":"2026-08-07T12:22:21.787388Z"},"links":{"citing_paper":"/paper/2505.24743"},"observation_digest":"sha256:5ba27e7deae782a829502d1f2cc52fbb9edf2a2033f7d9bfa00525fa80bbf34f","observation_id":"4fac0795-f344-4b0b-9398-57df02cf551a","resolution":{"observed_at":"2026-08-07T12:22:21.787388Z","resolver_source":null,"status":"unresolved"},"standing_notice":{"events":[],"reason":"canonical_work_link_unavailable","source_receipts":[],"state":"unavailable"}}],"paper":{"arxiv_id":"2505.24743","last_updated":"2025-06-11T17:49:24Z","latest_version":2,"primary_category":"astro-ph.CO","snapshot_observed_at":"2026-08-07T12:12:18.402918Z","submitted_at":"2025-05-30T16:01:50Z","title":"What solves the Hubble tension in phenomenological dark energy models at background level?"},"reference_resolution":{"displayed":80,"state_counts":{"malformed_identifier":0,"metadata_mismatch":0,"parse_uncertain":0,"unresolved":37,"verified_exact":2,"verified_fuzzy":41},"total_outbound_references":80},"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":"2026-08-07T06:34:17.273281+00:00","source":"crossref"},{"observed_at":"2026-08-07T06:34:11.927384+00:00","source":"retraction_watch"}],"thesis":"As of 7 August 2026, this Paper Citation Record lists 80 of 80 outbound references and 1 inbound Pith citation observation for arXiv:2505.24743."}