Structure Formation and Cosmology with high-z Clusters
Lecture4 - USP
Lecture4 - USP
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SF histories of ETGs in clusters vs field at z~1.2• General agreement <strong>with</strong> semi-analytical models (e.g. De Lucia+ 06, Menci+ 08)• Models however cannot reproduce the very tight relation in clusters (Menci+ 08)Color scatterModelsDataRedshift