K. Bechtol, I. Sevilla-Noarbe, A. Drlica-Wagner, B. Yanny, R. A. Gruendl, E. Sheldon, E. S. Rykoff, J. De Vicente, M. Adamów, Dhayaa Anbajagane, M. R. Becker, G. M. Bernstein, A. Carnero Rosell, J. Gschwend, Miranda Gorsuch, W G Hartley, Mike Jarvis, T. Jeltema, R. Kron, T. Andrew Manning, J. O’Donnell, A Pieres, M. Rodríguez-Monroy, D. Sanchez Cid, M. Tabbutt, C. Y. Tan, L. Toribio San Cipriano, D. L. Tucker, N. Weaverdyck, M. Yamamoto, T. M. C. Abbott, M. Aguena, A. Alarcón, S. Allam, A. Amon, F. Andrade-Oliveira, S. Avila, P. H. Bernardinelli, E. Bertin, J. Blazek, D. Brooks, D. L. Burke, J. Carretero, F. J. Castander, R. Cawthon, C. Chang, A. Choi, C. Conselice, M. Costanzi, M. Crocce, L. N. da Costa, T. M. Davis, S. Desai, H. T. Diehl, S. Dodelson, P. Doel, C. Doux, A. Ferté, B. Flaugher, P. Fosalba, J. Frieman, J. García-Bellido, M. Gatti, E. Gaztanaga, G. Giannini, D. Gruen, G. Gutierrez, K. Herner, S. R. Hinton, D. L. Hollowood, K. Honscheid, D. Huterer, N. Jeffrey, E. Krause, K. Kuehn, O. Lahav, S. Lee, C. Lidman, M. Lima, H. Lin, J. L. Marshall, J. Mena-Fernández, R. Miquel, J. J. Mohr, J. Muir, J. Myles, R. L. C. Ogando, A. Palmese, A. A. Plazas Malagón, A. Porredon, J. Prat, M. Raveri, A. K. Romer, A. Roodman, S. Samuroff, E. Sanchez, V. Scarpine, M. Smith, M. Soares-Santos, E. Suchyta
Abstract We describe the photometric dataset assembled from the full 6 yr of observations by the Dark Energy Survey (DES) in support of static-sky cosmology analyses. DES Y6 Gold is a curated dataset derived from DES Data Release 2 (DR2) that incorporates improved measurement, photometric calibration, object classification and value-added information. Y6 Gold comprises nearly 5000 deg 2 of grizY imaging in the south Galactic cap and includes 669 million objects with a depth of i AB ∼ 23.4 mag at a signal-to-noise ratio ∼ 10 for extended objects and a top-of-the-atmosphere photometric uniformity <2 mmag. Y6 Gold augments DES DR2 with simultaneous fits to multiepoch photometry for more robust galaxy shapes, colors, and photometric redshift estimates. Y6 Gold features improved morphological star–galaxy classification with an efficiency of 98.6% and a contamination of 0.8% for galaxies with 17.5 < i AB < 22.5. Additionally, it includes per-object quality information, and accompanying maps of the footprint coverage, masked regions, imaging depth, survey conditions, and astrophysical foregrounds that are used for cosmology analyses. After quality selections, benchmark samples contain 448 million galaxies and 120 million stars. This publication is complemented by data access and documentation.