100siWe describe an updated calibration and diagnostic framework, Balrog, used to directly sample the selection and photometric biases of the Dark Energy Survey (DES) Year 3 (Y3) data set. We systematically inject onto the single-epoch images of a random 20% subset of the DES footprint an ensemble of nearly 30 million realistic galaxy models derived from DES Deep Field observations. These augmented images are analyzed in parallel with the original data to automatically inherit measurement systematics that are often too difficult to capture with generative models. The resulting object catalog is a Monte Carlo sampling of the DES transfer function and is used as a powerful diagnostic and calibration tool for a variety of DES Y3 science, parti...
102We present and characterise the galaxy shape catalogue from the first 3 years of Dark Energy Surv...
105In this work, we present the galaxy clustering measurements of the two DES lens galaxy samples: a...
99siWe present the calibration of the Dark Energy Survey Year 3 (DES Y3) weak lensing (WL) source ga...
We describe an updated calibration and diagnostic framework, Balrog, used to directly sample the sel...
We describe an updated calibration and diagnostic framework, Balrog, used to directly sample the sel...
Artículo escrito por un elevado número de autores, solo se referencian el que aparece en primer luga...
Artículo escrito por un elevado número de autores, solo se referencian el que aparece en primer luga...
We describe an updated calibration and diagnostic framework, Balrog, used to directly sample the sel...
We describe an updated calibration and diagnostic framework, Balrog, used to directly sample the sel...
International audienceWe describe an updated calibration and diagnostic framework, Balrog, used to d...
We describe an updated calibration and diagnostic framework, Balrog, used to directly sample the sel...
We describe an updated calibration and diagnostic framework, Balrog, used to directly sample the sel...
We describe an updated calibration and diagnostic framework, Balrog, used to directly sample the sel...
In this dissertation, we describe a calibration and diagnostic framework called Balrog which was use...
In this dissertation, we describe a calibration and diagnostic framework called Balrog which was use...
102We present and characterise the galaxy shape catalogue from the first 3 years of Dark Energy Surv...
105In this work, we present the galaxy clustering measurements of the two DES lens galaxy samples: a...
99siWe present the calibration of the Dark Energy Survey Year 3 (DES Y3) weak lensing (WL) source ga...
We describe an updated calibration and diagnostic framework, Balrog, used to directly sample the sel...
We describe an updated calibration and diagnostic framework, Balrog, used to directly sample the sel...
Artículo escrito por un elevado número de autores, solo se referencian el que aparece en primer luga...
Artículo escrito por un elevado número de autores, solo se referencian el que aparece en primer luga...
We describe an updated calibration and diagnostic framework, Balrog, used to directly sample the sel...
We describe an updated calibration and diagnostic framework, Balrog, used to directly sample the sel...
International audienceWe describe an updated calibration and diagnostic framework, Balrog, used to d...
We describe an updated calibration and diagnostic framework, Balrog, used to directly sample the sel...
We describe an updated calibration and diagnostic framework, Balrog, used to directly sample the sel...
We describe an updated calibration and diagnostic framework, Balrog, used to directly sample the sel...
In this dissertation, we describe a calibration and diagnostic framework called Balrog which was use...
In this dissertation, we describe a calibration and diagnostic framework called Balrog which was use...
102We present and characterise the galaxy shape catalogue from the first 3 years of Dark Energy Surv...
105In this work, we present the galaxy clustering measurements of the two DES lens galaxy samples: a...
99siWe present the calibration of the Dark Energy Survey Year 3 (DES Y3) weak lensing (WL) source ga...