Chun-Hao To

TL;DR: The Dark Energy Survey (DES) photometric data set Y3 GOLD as discussed by the authors contains nearly 5000 deg2 of grizY imaging in the south Galactic cap including nearly 390 million objects, with depth reaching a signal-to-noise ratio ∼10 for extended objects up to i AB ∼ 23.0, and top-of-the-atmosphere photometric uniformity 98% and purity >99% for galaxies with 19 < i AB < 22.5.

TL;DR: In this paper, a joint analysis of the counts and weak lensing signal of redMaPPer clusters selected from the DES Year 1 dataset was performed using the same shear and source photometric redshifts estimates as were used in the DES combined probes analysis.

TL;DR: Amon et al. as mentioned in this paper present cosmic shear measurements and cosmological constraints from over 100 million source galaxies in the DES Year 3 data, and compare their measurement with constraints from two other contemporary weak-lensing experiments: the Kilo-Degree Survey (KiDS) and Hyper-Suprime Camera Subaru Strategic Program (HSC).

TL;DR: In this article, the authors present the Dark Energy Survey Year 3 cosmic shear measurements and cosmological constraints based on an analysis of over 100 million source galaxies, with the data spanning 4143 deg$^2$ on the sky, divided into four redshift bins, with a signal-to-noise of 40.4 dB.

TL;DR: The Dark Energy Survey (DES) photometric data set Y3 Gold as discussed by the authors contains nearly 5000 square degrees of grizY imaging in the south Galactic cap, including nearly 390 million objects, with depth reaching S/N ~ 10 for extended objects up to 23.5.