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Dark Energy Survey Year 3 Results: Point-Spread Function Modeling

M. Jarvis, G. Bernstein, A. Amon, C. Davis, P. Léget, K. Bechtol, I. Harrison, M. Gatti, A. Roodman, C. Chang, R. Chen, A. Choi, S. Desai, A. Drlica-Wagner, D. Gruen, R. Gruendl, A. Hernandez, N. MacCrann, J. Meyers, A. Navarro-Alsina, S. Pandey, A. Plazas, L. Secco, E. Sheldon, M. Troxel, S. Vorperian, K. Wei, J. Zuntz, T. Abbott, M. Aguena, S. Allam, S. Avila, S. Bhargava, S. Bridle, D. Brooks, A. Rosell, M. Kind, J. Carretero, M. Costanzi, L. da Costa, J. De Vicente, H. Diehl, P. Doel, S. Everett, B. Flaugher, P. Fosalba, J. Frieman, J. García-Bellido, E. Gaztanaga, D. Gerdes, G. Gutierrez, S. Hinton, D. Hollowood, K. Honscheid, D. James, S. Kent, K. Kuehn, N. Kuropatkin, O. Lahav, M. Maia, M. March, J. Marshall, P. Melchior, F. Menanteau, R. Miquel, R. Ogando, F. Paz-Chinchón, E. Rykoff, E. Sanchez, V. Scarpine, M. Schubnell, S. Serrano, I. Sevilla-Noarbe, M. Smith, E. Suchyta, M. Swanson, G. Tarle, T. Varga, A. Walker, W. Wester, R. Wilkinson, и D. Collaboration. (2020)cite arxiv:2011.03409Comment: 19 pages, submitted to MNRAS. See https://www.darkenergysurvey.org/des-year-3-cosmology-results-papers/ for the full DES Y3 cosmology release.

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Vicente de Haro Romo

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