International audienceWe present two galaxy shape catalogues from the Dark Energy Survey Year 1 data set, covering 1500 deg^2 with a median redshift of 0.59. The catalogues cover two main fields: Stripe 82, and an area overlapping the South Pole Telescope survey region. We describe our data analysis process and in particular our shape measurement using two independent shear measurement pipelines, metacalibration and im3shape. The metacalibration catalogue uses a Gaussian model with an innovative internal calibration scheme, and was applied to riz bands, yielding 34.8M objects. The im3shape catalogue uses a maximum-likelihood bulge/disc model calibrated using simulations, and was applied to r-band data, yielding 21.9M objects. Both catalogue...
International audienceDetermining the distribution of redshifts of galaxies observed by wide-field p...
International audienceWe use a suite of simulated images based on Year 1 of the Dark Energy Survey t...
International audienceWe present photometric redshift estimates for galaxies used in the weak lensin...
International audienceWe present two galaxy shape catalogues from the Dark Energy Survey Year 1 data...
We present two galaxy shape catalogues from the Dark Energy Survey Year 1 data set, covering 1500 de...
We present two galaxy shape catalogues from the Dark Energy Survey Year 1 data set, covering 1500 de...
International audienceWe present and characterize the galaxy shape catalogue from the first 3 yr of ...
We present and characterize the galaxy shape catalogue from the first 3 yr of Dark Energy Survey (DE...
We present two galaxy shape catalogues from the Dark Energy Survey Year 1 data set, covering 1500 de...
International audienceWe construct the largest curved-sky galaxy weak lensing mass map to date from ...
We construct the largest curved-sky galaxy weak lensing mass map to date from the DES first-year (DE...
We use a suite of simulated images based on Year 1 of the Dark Energy Survey to explore the impact o...
We present and characterize the galaxy-galaxy lensing signal measured using the first three years of...
International audienceDetermining the distribution of redshifts of galaxies observed by wide-field p...
International audienceWe use a suite of simulated images based on Year 1 of the Dark Energy Survey t...
International audienceWe present photometric redshift estimates for galaxies used in the weak lensin...
International audienceWe present two galaxy shape catalogues from the Dark Energy Survey Year 1 data...
We present two galaxy shape catalogues from the Dark Energy Survey Year 1 data set, covering 1500 de...
We present two galaxy shape catalogues from the Dark Energy Survey Year 1 data set, covering 1500 de...
International audienceWe present and characterize the galaxy shape catalogue from the first 3 yr of ...
We present and characterize the galaxy shape catalogue from the first 3 yr of Dark Energy Survey (DE...
We present two galaxy shape catalogues from the Dark Energy Survey Year 1 data set, covering 1500 de...
International audienceWe construct the largest curved-sky galaxy weak lensing mass map to date from ...
We construct the largest curved-sky galaxy weak lensing mass map to date from the DES first-year (DE...
We use a suite of simulated images based on Year 1 of the Dark Energy Survey to explore the impact o...
We present and characterize the galaxy-galaxy lensing signal measured using the first three years of...
International audienceDetermining the distribution of redshifts of galaxies observed by wide-field p...
International audienceWe use a suite of simulated images based on Year 1 of the Dark Energy Survey t...
International audienceWe present photometric redshift estimates for galaxies used in the weak lensin...