activity
20042009
most citedSpectroscopy of clusters in the ESO distant cluster survey (EDisCS).II. Redshifts, velocity dispersions, and substructure for clusters in the last 15 fields

84 citations · 85 across the 2 of their papers we have counts for

collaborators

6 papers

astro-ph.CO20091 cited

The ESO Distant Cluster Sample: galaxy evolution and environment out to z=1

Bianca M. Poggianti, Alfonso Aragon-Salamanca, Steven Bamford +25

The ESO Distant Cluster Survey (EDisCS, P.I. Simon D.M. White, LP 166.A-0162) is an ESO large programme aimed at studying clusters and cluster galaxies at z=0.4-1. How different is…

astro-ph200884 cited

Spectroscopy of clusters in the ESO distant cluster survey (EDisCS).II. Redshifts, velocity dispersions, and substructure for clusters in the last 15 fields

Bo Milvang-Jensen, Stefan Noll, Claire Halliday +17

AIMS. We present spectroscopic observations of galaxies in 15 survey fields as part of the ESO Distant Cluster Survey (EDisCS). We determine the redshifts and velocity dispersions…

astro-ph2005

EDisCS -- the ESO Distant Cluster Survey -- Sample Definition and Optical Photometry

S. D. M. White, D. I. Clowe, L. Simard +23

We present the ESO Distant Cluster Survey (EDisCS) a survey of 20 fields containing distant galaxy clusters with redshifts ranging from 0.4 to almost 1.0. Candidate clusters were c…

astro-ph2004

Spectroscopy of clusters in the ESO Distant Cluster Survey (EDisCS)

C. Halliday, B. Milvang-Jensen, S. Poirier +12

We present spectroscopic observations of galaxies in 4 clusters at z = 0.7-0.8 and in one cluster at z~0.5 obtained with the FORS2 spectrograph on the VLT as part of the ESO Distan…

astro-ph2004

The build-up of the red-sequence in galaxy clusters since z~0.8

G. De Lucia, B. M. Poggianti, A. Aragon-Salamanca +10

We study the rest-frame (U-V) color-magnitude relation in 4 clusters at redshifts 0.7-0.8, drawn from the ESO Distant Cluster Survey. We confirm that red-sequence galaxies in these…

astro-ph2004

Observing the build-up of the colour-magnitude relation at redshift ~0.8

G. De Lucia, B. M. Poggianti, A. Aragon-Salamanca +11

We analyse the rest-frame (U-V) colour-magnitude relation for 2 clusters at redshift 0.7 and 0.8, drawn from the ESO Distant Cluster Survey. By comparing with the population of red…