International audienceWe present cosmological results from a combined analysis of galaxy clustering and weak gravitational lensing, using 1321 deg2 of griz imaging data from the first year of the Dark Energy Survey (DES Y1). We combine three two-point functions: (i) the cosmic shear correlation function of 26 million source galaxies in four redshift bins, (ii) the galaxy angular autocorrelation function of 650,000 luminous red galaxies in five redshift bins, and (iii) the galaxy-shear cross-correlation of luminous red galaxy positions and source galaxy shears. To demonstrate the robustness of these results, we use independent pairs of galaxy shape, photometric-redshift estimation and validation, and likelihood analysis pipelines. To preven...
International audienceWe present constraints on extensions of the minimal cosmological models domina...
We present cosmological constraints from the Dark Energy Survey (DES) using a combined analysis of a...
We measure the clustering of DES year 1 galaxies that are intended to be combined with weak lensing ...
International audienceWe present cosmological results from a combined analysis of galaxy clustering ...
We present cosmological results from a combined analysis of galaxy clustering and weak gravitational...
We present cosmological results from a combined analysis of galaxy clustering and weak gravitational...
We present cosmological results from a combined analysis of galaxy clustering and weak gravitational...
We present cosmological results from a combined analysis of galaxy clustering and weak gravitational...
We present cosmological results from a combined analysis of galaxy clustering and weak gravitational...
We present cosmological results from a combined analysis of galaxy clustering and weak gravitational...
We present the first cosmology results from large-scale structure using the full 5000 deg2 of imagin...
International audienceWe present the first cosmology results from large-scale structure using the fu...
We present the first cosmology results from large-scale structure using the full 5000 deg2 of imagin...
We present the first cosmology results from large-scale structure using the full 5000 deg2 of imagin...
International audienceWe present cosmological constraints from the Dark Energy Survey (DES) using a ...
International audienceWe present constraints on extensions of the minimal cosmological models domina...
We present cosmological constraints from the Dark Energy Survey (DES) using a combined analysis of a...
We measure the clustering of DES year 1 galaxies that are intended to be combined with weak lensing ...
International audienceWe present cosmological results from a combined analysis of galaxy clustering ...
We present cosmological results from a combined analysis of galaxy clustering and weak gravitational...
We present cosmological results from a combined analysis of galaxy clustering and weak gravitational...
We present cosmological results from a combined analysis of galaxy clustering and weak gravitational...
We present cosmological results from a combined analysis of galaxy clustering and weak gravitational...
We present cosmological results from a combined analysis of galaxy clustering and weak gravitational...
We present cosmological results from a combined analysis of galaxy clustering and weak gravitational...
We present the first cosmology results from large-scale structure using the full 5000 deg2 of imagin...
International audienceWe present the first cosmology results from large-scale structure using the fu...
We present the first cosmology results from large-scale structure using the full 5000 deg2 of imagin...
We present the first cosmology results from large-scale structure using the full 5000 deg2 of imagin...
International audienceWe present cosmological constraints from the Dark Energy Survey (DES) using a ...
International audienceWe present constraints on extensions of the minimal cosmological models domina...
We present cosmological constraints from the Dark Energy Survey (DES) using a combined analysis of a...
We measure the clustering of DES year 1 galaxies that are intended to be combined with weak lensing ...