paper

Dark Energy Survey Year 3 Results: Cosmological Constraints from Galaxy Clustering and Weak Lensing

arXiv:2105.13549 · doi:10.1103/PhysRevD.105.023520

Abstract

We present the first cosmology results from large-scale structure in the Dark Energy Survey (DES) spanning 5000 deg. We perform an analysis combining three two-point correlation functions (32pt): (i) cosmic shear using 100 million source galaxies, (ii) galaxy clustering, and (iii) the cross-correlation of source galaxy shear with lens galaxy positions. The analysis was designed to mitigate confirmation or observer bias; we describe specific changes made to the lens galaxy sample following unblinding of the results. We model the data within the flat CDM and CDM cosmological models. We find consistent cosmological results between the three two-point correlation functions; their combination yields clustering amplitude and matter density in CDM, mean with 68% confidence limits; , , and dark energy equation-of-state parameter in CDM. This combination of DES data is consistent with the prediction of the model favored by the Planck 2018 cosmic microwave background (CMB) primary anisotropy data, which is quantified with a probability-to-exceed to . When combining DES 32pt data with available baryon acoustic oscillation, redshift-space distortion, and type Ia supernovae data, we find . Combining all of these data sets with Planck CMB lensing yields joint parameter constraints of , , , and in CDM; , , , and in CDM. (abridged)

See https://www.darkenergysurvey.org/des-year-3-cosmology-results-papers/ for the full DES Y3 3x2pt cosmology release. Matches version accepted in PRD