We derive the stellar mass fraction in the galaxy cluster RXC J2248.7-4431 observed with the Dark Energy Survey (DES) during the Science Verification period. We compare the stellar mass results from DES (five filters) with those from the Hubble Space Telescope Cluster Lensing And Supernova Survey (CLASH; 17 filters). When the cluster spectroscopic redshift is assumed, we show that stellar masses from DES can be estimated within 25 per cent of CLASH values. We compute the stellar mass contribution coming from red and blue galaxies, and study the relation between stellar mass and the underlying dark matter using weak lensing studies with DES and CLASH. An analysis of the radial profiles of the DES total and stellar mass yields a stellar-to-to...
We present a detailed investigation of the cluster stellar mass-to-light (M∗/L) ratio and cumulative...
Splashback refers to the process of matter that is accreting onto a dark matter halo reaching its fi...
In the formation of galaxy groups and clusters, the dark matter haloes containing satellite galaxies...
International audienceWe derive the stellar mass fraction in the galaxy cluster RXC J2248.7-4431 obs...
Galaxy clusters are massive dark matter halos, with masses as high as a few times 10^15 M⊙, each hos...
The masses of galaxy clusters are dominated by dark matter, and a robust determination of their mass...
We study the effect of diffuse intracluster light on the critical surface mass density estimated fro...
We measure the weak lensing masses and galaxy distributions of four massive galaxy clusters observed...
We introduce a galaxy cluster mass observable, μ⋆, based on the stellar masses of cluster members, a...
This work observationally addresses the relative distribution of total and optically luminous matter...
Weak lensing source galaxy catalogues used in estimating the masses of galaxy clusters can be heavil...
We present cosmological constraints from the Dark Energy Survey (DES) using a combined analysis of a...
We present forecasts on the capability of future wide-area high-sensitivity X-ray surveys of galaxy ...
International audienceMeasurements of the galaxy stellar mass function are crucial to understand the...
We use weak-lensing shear measurements to determine the mean mass of optically selected galaxy clust...
We present a detailed investigation of the cluster stellar mass-to-light (M∗/L) ratio and cumulative...
Splashback refers to the process of matter that is accreting onto a dark matter halo reaching its fi...
In the formation of galaxy groups and clusters, the dark matter haloes containing satellite galaxies...
International audienceWe derive the stellar mass fraction in the galaxy cluster RXC J2248.7-4431 obs...
Galaxy clusters are massive dark matter halos, with masses as high as a few times 10^15 M⊙, each hos...
The masses of galaxy clusters are dominated by dark matter, and a robust determination of their mass...
We study the effect of diffuse intracluster light on the critical surface mass density estimated fro...
We measure the weak lensing masses and galaxy distributions of four massive galaxy clusters observed...
We introduce a galaxy cluster mass observable, μ⋆, based on the stellar masses of cluster members, a...
This work observationally addresses the relative distribution of total and optically luminous matter...
Weak lensing source galaxy catalogues used in estimating the masses of galaxy clusters can be heavil...
We present cosmological constraints from the Dark Energy Survey (DES) using a combined analysis of a...
We present forecasts on the capability of future wide-area high-sensitivity X-ray surveys of galaxy ...
International audienceMeasurements of the galaxy stellar mass function are crucial to understand the...
We use weak-lensing shear measurements to determine the mean mass of optically selected galaxy clust...
We present a detailed investigation of the cluster stellar mass-to-light (M∗/L) ratio and cumulative...
Splashback refers to the process of matter that is accreting onto a dark matter halo reaching its fi...
In the formation of galaxy groups and clusters, the dark matter haloes containing satellite galaxies...