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Our analysis yields $H_0 = 68.86\\pm 0.68~\\mathrm{km\\ s^{-1} Mpc^{-1}}$ with WMAP+DESI BAO, $H_0 = 68.72\\pm 0.51~\\mathrm{km\\ s^{-1} Mpc^{-1}}$ with WMAP+ACT+DESI BAO, and $H_0 = 68.62\\pm 0.52~\\mathrm{km\\ s^{-1} Mpc^{-1}}$ with WMAP+SPT+DESI BAO. The results of non-Planck CMB+DESI BAO exhibit a $3.4\\sigma$, $3.7\\sigma$, and $3.8\\sigma$ tension"},"verification_status":{"content_addressed":true,"pith_receipt":true,"author_attested":false,"weak_author_claims":0,"strong_author_claims":0,"externally_anchored":false,"storage_verified":false,"citation_signatures":0,"replication_records":0,"graph_snapshot":true,"references_resolved":false,"formal_links_present":false},"canonical_record":{"source":{"id":"2411.14189","kind":"arxiv","version":1},"metadata":{"license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","primary_cat":"astro-ph.CO","submitted_at":"2024-11-21T14:58:40Z","cross_cats_sorted":[],"title_canon_sha256":"5129d2a19cc32fc8dbe5a50f681f53fe555de600daaf02df295e0a8cb0ec2405","abstract_canon_sha256":"0ef941f709a355f6d90b62ae829ae67d745a6bf844ae044aa494fe3c671de9a4"},"schema_version":"1.0"},"receipt":{"kind":"pith_receipt","key_id":"pith-v1-2026-05","algorithm":"ed25519","signed_at":"2026-07-05T09:38:42.969706Z","signature_b64":"JDrfYUsFI0kpGHISyziA6LF3X/cxJfWXROF/l7cLwFQnqi60mJDAeFTToGySL941fgj0aSGqyIj3sYvn14DNCA==","signed_message":"canonical_sha256_bytes","builder_version":"pith-number-builder-2026-05-17-v1","receipt_version":"0.3","canonical_sha256":"803bbaf7b346fa2e0196b26a2a14bc87751ccd5633b3b2dd658a13012134bea9","last_reissued_at":"2026-07-05T09:38:42.969252Z","signature_status":"signed_v1","first_computed_at":"2026-07-05T09:38:42.969252Z","public_key_fingerprint":"8d4b5ee74e4693bcd1df2446408b0d54"},"graph_snapshot":{"paper":{"title":"Reevaluating $H_0$ Tension with Non-Planck CMB and DESI BAO Joint Analysis","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","headline":"","cross_cats":[],"primary_cat":"astro-ph.CO","authors_text":"Qing-Guo Huang, Xue Zhang, Ye-Huang Pang","submitted_at":"2024-11-21T14:58:40Z","abstract_excerpt":"$H_0$ tension in the spatially flat $\\Lambda$CDM model is reevaluated by employing three sets of non-Planck CMB data, namely WMAP, WMAP+ACT, and WMAP+SPT, in conjunction with DESI BAO data and non-DESI BAO datasets including 6dFGS, SDSS DR7, and SDSS DR16. 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