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Rezaie, M. Schubnell, M. S. Wang, M. Vargas-Maga\\~na, M. Walther, M. White, N.A. Roe, N. Deiosso, N. Findlay, N. G. Kara\\c{c}ayl{\\i}, N. M. Nguyen, N. Padmanabhan, N. Palanque-Delabrouille, N. Weaverdyck, O. Alves, P. Doel, P. Fagrelius, P. Martini, P. McDonald, P. Zarrouk, R. Blum, R. Calderon, R. Canning, R. Cereskaite, R. Gsponer, R. H. Wechsler, R. Kehoe, R. Miquel, R. Neveux, R. Ruggeri, R. Sharples, R. Vaisakh, R. Zhao, R. Zhou, S. Ahlen, S. Alam, S. Avila, S. Bailey, S. BenZvi, S. Brieden, S. Chabanier, S. Chen, S. Cole, S. Eftekharzadeh, S. E. Koposov, S. Ferraro, S. Gontcho A Gontcho, S. Juneau, S. Kent, S. Moore, S. Nadathur, S. Penmetsa, S. Ramirez-Solano, S. Trusov, S. Yuan, T. Claybaugh, T. M. Davis, T. S. Li, T. Tan, T.-W. Lan, U. Andrade, V. Gonzalez-Perez, V. Ir\\v{s}i\\v{c}, V. Ruhlmann-Kleider, W. J. Percival, X. Chen, Y. Lai, Y. Yu, Z. Ding","cross_cats":[],"headline":"The first-year full-shape analysis of galaxy clustering constrains the matter density to 0.296 and the Hubble constant to 68.63 km/s/Mpc.","license":"http://creativecommons.org/licenses/by-nc-nd/4.0/","primary_cat":"astro-ph.CO","submitted_at":"2024-11-18T20:03:34Z","title":"DESI 2024 V: Full-Shape Galaxy Clustering from Galaxies and Quasars"},"references":{"count":195,"internal_anchors":67,"resolved_work":195,"sample":[{"cited_arxiv_id":"2411.12022","doi":"","is_internal_anchor":true,"ref_index":1,"title":"DESI 2024 VII: Cosmological Constraints from the Full-Shape Modeling of Clustering Measurements","work_id":"ff3623b2-379a-4d24-80dd-3266aa77a5ff","year":2024},{"cited_arxiv_id":"","doi":"","is_internal_anchor":false,"ref_index":2,"title":"J. Huchra, M. Davis, D. Latham and J. Tonry,A survey of galaxy redshifts. IV - The data, ApJS52(1983) 89","work_id":"94ebe16f-9914-4837-bcb1-ad0f2bd12a5a","year":1983},{"cited_arxiv_id":"","doi":"","is_internal_anchor":false,"ref_index":3,"title":"M. Davis, G. Efstathiou, C.S. Frenk and S.D.M. White,The evolution of large-scale structure in a universe dominated by cold dark matter, ApJ292(1985) 371","work_id":"34824f2d-da1a-4785-9cc3-5efd92f30d28","year":1985},{"cited_arxiv_id":"","doi":"","is_internal_anchor":false,"ref_index":4,"title":"G. Efstathiou, W.J. Sutherland and S.J. Maddox,The cosmological constant and cold dark matter, Nature348(1990) 705","work_id":"16fde72d-b96b-4bfd-9014-64860362f325","year":1990},{"cited_arxiv_id":"astro-ph/0106498","doi":"","is_internal_anchor":true,"ref_index":5,"title":"The 2dF Galaxy Redshift Survey: Spectra and redshifts","work_id":"343d2b46-5e4c-4847-b4b5-53e79ee2574e","year":2001}],"snapshot_sha256":"cf3a20037002de67666e24534bcdb7679bb06546349def7113a4ebd748f9aa5f"},"source":{"id":"2411.12021","kind":"arxiv","version":5},"verdict":{"created_at":"2026-05-17T05:54:43.897098Z","id":"f6d9fc9e-cf45-4ddf-864d-32fccd04fce6","model_set":{"reader":"grok-4.3"},"one_line_summary":"DESI DR1 full-shape galaxy clustering constrains Omega_m = 0.296 ± 0.010, H0 = 68.63 ± 0.79 km/s/Mpc, and sigma_8 = 0.841 ± 0.034, consistent with LambdaCDM and Planck.","pipeline_version":"pith-pipeline@v0.9.0","pith_extraction_headline":"The first-year full-shape analysis of galaxy clustering constrains the matter density to 0.296 and the Hubble constant to 68.63 km/s/Mpc.","strongest_claim":"Using a Big Bang Nucleosynthesis Gaussian prior on the baryon density parameter, and a Gaussian prior on the spectral index, we constrain the matter density is Ω_m=0.296±0.010 and the Hubble constant H_0=(68.63 ± 0.79)[km s^{-1}Mpc^{-1}]. 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