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K. Dawson

6 та иш

Department of Physics and Astronomy, The University of Utah, 115 South 1400 East, Salt Lake City, UT 84112, U.S.A

  1. DESI 2024 VII: cosmological constraints from the full-shape modeling of clustering measurements

    A. G. Adame, J. Aguilar, S. Ahlen +97

    МақолаCosmology and Gravitation TheoriesJournal of Cosmology and Astroparticle Physics20259 иқтибос
    ABI

  2. DESI 2024 II: sample definitions, characteristics, and two-point clustering statistics

    A. G. Adame, José Aguilar, S. Ahlen +97

    МақолаAdvanced Statistical Methods and ModelsJournal of Cosmology and Astroparticle Physics20258 иқтибос
    ABI

  3. DESI 2024 III: Baryon Acoustic Oscillations from Galaxies and Quasars

    DESI Collaboration, A. G. Adame, J. Aguilar +97

    ПрепринтGalaxies: Formation, Evolution, PhenomenaarXiv (Cornell University)20246 иқтибос
    ABI

  4. DESI 2024 V: Full-Shape Galaxy Clustering from Galaxies and Quasars

    Adame, A. G., J. Aguilar, S. Ahlen +97

    ПрепринтAstronomy and Astrophysical ResearcharXiv (Cornell University)20246 иқтибос
    ABI

  5. Optimal reconstruction of baryon acoustic oscillations for DESI 2024

    E. Paillas, Z. Ding, Xinyi Chen +71

    МақолаGalaxies: Formation, Evolution, PhenomenaJournal of Cosmology and Astroparticle Physics20253 иқтибос
    ABI

  6. Not all lensing is low: An analysis of DESI$\times$DES using the Lagrangian Effective Theory of LSS

    S. Chen, DeRose, J., Rong Zhou +39

    МақолаGalaxies: Formation, Evolution, PhenomenaarXiv (Cornell University)20240 иқтибос
    ABI