Structure Formation and Cosmology with high-z Clusters
Lecture4 - USP
Lecture4 - USP
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Distribution of baryons <strong>and</strong> DM in a distant cluster (z=1.24)RDCS1252Hot GasHot gas <strong>with</strong>Ch<strong>and</strong>raK-b<strong>and</strong> lightStellar mass<strong>with</strong> VLT/ISAACDM MassWeak Lensing<strong>with</strong> HST/ACSLombardi et al. 05" Weak lensing feasible <strong>with</strong> HST: good news for mass calibration of distant clusters