activity
20002009
most citedProbing the distribution of dark matter in the Abell 901/902 supercluster with weak lensing

111 citations · 319 across the 8 of their papers we have counts for

collaborators

7 papers

astro-ph.CO2009★ 40 cited

Barred Galaxies in the Abell 901/2 Supercluster with STAGES

I. Marinova, S. Jogee, A. Heiderman +23

We present a study of bar and host disk evolution in a dense cluster environment, based on a sample of ~800 bright (MV <= -18) galaxies in the Abell 901/2 supercluster at z~0.165.…

astro-ph2008

Galaxy Evolution in Dense Environments: Properties of Interacting Galaxies in the A901/02 Supercluster

A. L. Heiderman, S. Jogee, D. J. Bacon +23

We present a study of galaxies in the STAGES survey of the Abell 901/902 supercluster at z~0.165, based on HST ACS F606W, COMBO-17, Spitzer 24um, XMM-Newton X-ray, and gravitationa…

astro-ph2006

A hole in the sky - The dependence of the galaxy luminosity function on the environment

S. Phleps, C. Wolf, J. A. Peacock +2

We have developed a method to calculate overdensities in multicolour surveys, and compare the local density contrast measured in galaxy samples with different redshift error distri…

astro-ph2004

Evolution of optically faint AGN from COMBO-17 and GEMS

L. Wisotzki, K. Jahnke, S. F. Sanchez +13

We have mapped the AGN luminosity function and its evolution between z=1 and z=5 down to apparent magnitudes of . Within the GEMS project we have analysed HST-ACS images of m…

astro-ph2003★ 40 cited

Constraints to the evolution of Ly-Alpha bright galaxies between z=3 and z=6

C. Maier, K. Meisenheimer, E. Thommes +6

Galaxies at high redshift with a strong Ly-Alpha emission line trace massive star formation in the absence of dust, and can therefore be regarded as a prime signature of the first…

astro-ph2001★ 111 cited

Probing the distribution of dark matter in the Abell 901/902 supercluster with weak lensing

M. E. Gray, A. N. Taylor, K. Meisenheimer +3

We present a weak shear analysis of the Abell 901/902 supercluster, composed of three rich clusters at z=0.16. Using a deep R-band image from the 0.5 x 0.5 degree MPG/ESO Wide Fiel…