International audienceWe constrain cosmological parameters and galaxy-bias parameters using the combination of galaxy clustering and galaxy-galaxy lensing measurements from the Dark Energy Survey (DES) year-3 data. We describe our modeling framework and choice of scales analyzed, validating their robustness to theoretical uncertainties in small-scale clustering by analyzing simulated data. Using a linear galaxy-bias model and redMaGiC galaxy sample, we obtain 10% constraints on the matter density of the Universe. We also implement a nonlinear galaxy-bias model to probe smaller scales that includes parametrization based on hybrid perturbation theory and find that it leads to a 17% gain in cosmological constraining power. We perform robustnes...
International audienceWe study the effect of magnification in the Dark Energy Survey Year 3 analysis...
We study the effect of magnification in the Dark Energy Survey Year 3 analysis of galaxy clustering ...
International audienceWe study the effect of magnification in the Dark Energy Survey Year 3 analysis...
International audienceWe constrain cosmological parameters and galaxy-bias parameters using the comb...
We constrain cosmological parameters and galaxy-bias parameters using the combination of galaxy clus...
We constrain cosmological parameters and galaxy-bias parameters using the combination of galaxy clus...
We constrain cosmological parameters and galaxy-bias parameters using the combination of galaxy clus...
In this work, we present the galaxy clustering measurements of the two DES lens galaxy samples: a ma...
In this work, we present the galaxy clustering measurements of the two DES lens galaxy samples: a ma...
In this work, we present the galaxy clustering measurements of the two DES lens galaxy samples: a ma...
In this work, we present the galaxy clustering measurements of the two DES lens galaxy samples: a ma...
In this work, we present the galaxy clustering measurements of the two DES lens galaxy samples: a ma...
International audienceIn this work, we present the galaxy clustering measurements of the two DES len...
International audienceIn this work, we present the galaxy clustering measurements of the two DES len...
The cosmological information extracted from photometric surveys is most robust when multiple probes ...
International audienceWe study the effect of magnification in the Dark Energy Survey Year 3 analysis...
We study the effect of magnification in the Dark Energy Survey Year 3 analysis of galaxy clustering ...
International audienceWe study the effect of magnification in the Dark Energy Survey Year 3 analysis...
International audienceWe constrain cosmological parameters and galaxy-bias parameters using the comb...
We constrain cosmological parameters and galaxy-bias parameters using the combination of galaxy clus...
We constrain cosmological parameters and galaxy-bias parameters using the combination of galaxy clus...
We constrain cosmological parameters and galaxy-bias parameters using the combination of galaxy clus...
In this work, we present the galaxy clustering measurements of the two DES lens galaxy samples: a ma...
In this work, we present the galaxy clustering measurements of the two DES lens galaxy samples: a ma...
In this work, we present the galaxy clustering measurements of the two DES lens galaxy samples: a ma...
In this work, we present the galaxy clustering measurements of the two DES lens galaxy samples: a ma...
In this work, we present the galaxy clustering measurements of the two DES lens galaxy samples: a ma...
International audienceIn this work, we present the galaxy clustering measurements of the two DES len...
International audienceIn this work, we present the galaxy clustering measurements of the two DES len...
The cosmological information extracted from photometric surveys is most robust when multiple probes ...
International audienceWe study the effect of magnification in the Dark Energy Survey Year 3 analysis...
We study the effect of magnification in the Dark Energy Survey Year 3 analysis of galaxy clustering ...
International audienceWe study the effect of magnification in the Dark Energy Survey Year 3 analysis...