activity
19952009
most citedA direct empirical proof of the existence of dark matter

2.4k citations · 5k across the 17 of their papers we have counts for

collaborators
Showing 2004 · astro-phShow all

6 papers · 2 filters

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-ph200463 cited

Weak lensing study of dark matter filaments and application to the binary cluster A 222 and A 223

J. P. Dietrich, P. Schneider, D. Clowe +2

We present a weak lensing analysis of the double cluster system Abell 222 and Abell 223. The lensing reconstruction shows evidence for a possible dark matter filament connecting bo…

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…

astro-ph2004

Weak lensing evidence for a filament between A222/A223

J. P. Dietrich, D. Clowe, P. Schneider +2

We present a weak lensing analysis and comparison to optical and X-ray maps of the close pair of massive clusters A222/223. Indications for a filamentary connection between the clu…

astro-ph2004

Effects of asphericity and substructure on the determination of cluster mass with weak gravitational lensing

D. Clowe, G. De Lucia, L. King

Weak gravitational lensing can be used to directly measure the mass along a line-of-sight without any dependence on the dynamical state of the mass, and thus can be used to measure…