论文标题
黑暗能源调查3年结果:弱透镜形状目录
Dark Energy Survey Year 3 Results: Weak Lensing Shape Catalogue
论文作者
论文摘要
我们介绍并描述了来自黑暗能源调查(DES)观测的前三年的星系形状目录,在〜4143度$^2 $的有效区域的南部天空中。我们描述了我们的数据分析过程以及我们的自我校准剪切测量管道元素校准,该过程在DES 1年级分析中在几个方面使用的管道建立和改进。 DES 3年级弱透明形状目录由100,204,026个星系组成,以$ riz $ bands测量,导致加权源数密度为$ n _ {\ rm eff} = 5.59 $ gal/arcmin $ ^{2} $ ^{2} $,并相应的形状噪声$σ_e= 0.261 $ = 0.261 $。我们在目录上执行了一系列内部无效测试,包括有关与点传播功能(PSF)建模,虚假目录B模式信号,目录污染和星系属性相关的系统学测试。
We present and characterise the galaxy shape catalogue from the first 3 years of Dark Energy Survey (DES) observations, over an effective area of ~4143 deg$^2$ of the southern sky. We describe our data analysis process and our self-calibrating shear measurement pipeline METACALIBRATION, which builds and improves upon the pipeline used in the DES Year 1 analysis in several aspects. The DES Year 3 weak-lensing shape catalogue consists of 100,204,026 galaxies, measured in the $riz$ bands, resulting in a weighted source number density of $n_{\rm eff} = 5.59$ gal/arcmin$ ^{2}$ and corresponding shape noise $σ_e = 0.261$. We perform a battery of internal null tests on the catalogue, including tests on systematics related to the point-spread function (PSF) modelling, spurious catalogue B-mode signals, catalogue contamination, and galaxy properties.