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HST/WFC3 grism observations of z similar to 1 clusters
Minor mergers are thought to be responsible for the size growth of quiescent field galaxies with decreasing redshift. We test this hypothesis using the cluster environment as a laboratory. Satellite galaxies in clusters move at...
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Bulge Growth and Quenching since z = 2.5 in CANDELS/3D-HST
Exploiting the deep high-resolution imaging of all five CANDELS fields, and accurate redshift information provided by 3D-HST, we investigate the relation between structure and stellar populations for a mass-selected sample of...
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Bulge Growth and Quenching since z = 2.5 in CANDELS/3D-HST
Exploiting the deep high-resolution imaging of all five CANDELS fields, and accurate redshift information provided by 3D-HST, we investigate the relation between structure and stellar populations for a mass-selected sample of...
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