Structure Formation and Cosmology with high-z Clusters
Lecture4 - USP
Lecture4 - USP
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RDCS1252 (z = 1.24) C-M Relation <strong>with</strong> HST/ACS <strong>and</strong> VLT/ISAAC(Blakeslee et al. 03; Lidman et al. 03)HST/ACSComa at z=1.24ES0LateBlakeslee et al. 2003The scatter (0.042±0.015 mag in i-z, 0.06 in J-K) <strong>and</strong> slope of the redsequence are very similar to low-z clusters (e.g. Coma)
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