308 citations · 3.6k across the 90 of their papers we have counts for
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Galaxy stellar mass functions of different morphological types in clusters, and their evolution between z=0.8 and z=0
Benedetta Vulcani, Bianca M. Poggianti, Alfonso Aragón-Salamanca +11
We present the galaxy stellar mass function (MF) and its evolution in clusters from z~0.8 to the current epoch, based on the WIde-field Nearby Galaxy-cluster Survey (WINGS) (0.04<z…
Star Formation in the XMMU J2235.3-2557 Galaxy Cluster at z=1.39
Amanda E. Bauer, Ruth Grutzbauch, Inger Jorgensen +2
We present the first results of a narrow-band photometric study of the massive galaxy cluster XMMU J2235.3-2557 at z=1.39. We obtained deep narrow-band imaging with NIRI on Gem…
How does galaxy environment matter? The relationship between galaxy environments, colour and stellar mass at 0.4 < z < 1 in the Palomar/DEEP2 survey
Ruth Grützbauch, Christopher J. Conselice, Jesús Varela +4
We present a study characterizing the environments of galaxies in the redshift range of 0.4 < z < 1 based on data from the POWIR near infrared imaging and DEEP2 spectroscopic redsh…
The evolution of the density of galaxy clusters and groups: denser environments at higher redshifts
Bianca M. Poggianti, Gabriella De Lucia, Jesus Varela +5
We show that, observationally, the projected local density distribution in high-z clusters is shifted towards higher values compared to clusters at lower redshift. To search for th…