We present and characterize the galaxy-galaxy lensing signal measured using the first three years of data from the Dark Energy Survey (DES Y3) covering 4132 deg2. These galaxy-galaxy measurements are used in the DES Y3 3 ?? 2 pt cosmological analysis, which combines weak lensing and galaxy clustering information. We use two lens samples: a magnitude-limited sample and the redMaGiC sample, which span the redshift range-0.2???1 with 10.7 and 2.6 M galaxies, respectively. For the source catalog, we use the METACALIBRATION shape sample, consisting of -100 M galaxies separated into four tomographic bins. Our galaxy-galaxy lensing estimator is the mean tangential shear, for which we obtain a total SNR of-148 for MagLim (-120 for redMaGiC), and-67...
Using the first three years of data from the Dark Energy Survey (DES), we use ratios of small-scale ...
In this work, we present the galaxy clustering measurements of the two DES lens galaxy samples: a ma...
International audienceUsing the first three years of data from the Dark Energy Survey (DES), we use ...
We present and characterize the galaxy-galaxy lensing signal measured using the first three years of...
We present and characterize the galaxy-galaxy lensing signal measured using the first three years of...
We present and characterize the galaxy-galaxy lensing signal measured using the first three years of...
We present and characterize the galaxy-galaxy lensing signal measured using the first three years of...
We present and characterize the galaxy-galaxy lensing signal measured using the first three years of...
International audienceWe present galaxy-galaxy lensing measurements from 1321 sq. deg. of the Dark E...
International audienceWe present galaxy-galaxy lensing measurements from 1321 sq. deg. of the Dark E...
We present galaxy-galaxy lensing measurements from 1321 sq. deg. of the Dark Energy Survey (DES) Yea...
Using the first three years of data from the Dark Energy Survey (DES), we use ratios of small-scale ...
Using the first three years of data from the Dark Energy Survey (DES), we use ratios of small-scale ...
Using the first three years of data from the Dark Energy Survey (DES), we use ratios of small-scale ...
Using the first three years of data from the Dark Energy Survey (DES), we use ratios of small-scale ...
Using the first three years of data from the Dark Energy Survey (DES), we use ratios of small-scale ...
In this work, we present the galaxy clustering measurements of the two DES lens galaxy samples: a ma...
International audienceUsing the first three years of data from the Dark Energy Survey (DES), we use ...
We present and characterize the galaxy-galaxy lensing signal measured using the first three years of...
We present and characterize the galaxy-galaxy lensing signal measured using the first three years of...
We present and characterize the galaxy-galaxy lensing signal measured using the first three years of...
We present and characterize the galaxy-galaxy lensing signal measured using the first three years of...
We present and characterize the galaxy-galaxy lensing signal measured using the first three years of...
International audienceWe present galaxy-galaxy lensing measurements from 1321 sq. deg. of the Dark E...
International audienceWe present galaxy-galaxy lensing measurements from 1321 sq. deg. of the Dark E...
We present galaxy-galaxy lensing measurements from 1321 sq. deg. of the Dark Energy Survey (DES) Yea...
Using the first three years of data from the Dark Energy Survey (DES), we use ratios of small-scale ...
Using the first three years of data from the Dark Energy Survey (DES), we use ratios of small-scale ...
Using the first three years of data from the Dark Energy Survey (DES), we use ratios of small-scale ...
Using the first three years of data from the Dark Energy Survey (DES), we use ratios of small-scale ...
Using the first three years of data from the Dark Energy Survey (DES), we use ratios of small-scale ...
In this work, we present the galaxy clustering measurements of the two DES lens galaxy samples: a ma...
International audienceUsing the first three years of data from the Dark Energy Survey (DES), we use ...