activity
20032023
most citedInternal kinematics of spiral galaxies in distant clusters Part I

45 citations · 157 across the 14 of their papers we have counts for

collaborators

14 papers

astro-ph.GA2023★ 3 cited

Exploring the stellar populations of backsplash galaxies

Ignacio Ferreras, Asmus Böhm, Keiichi Umetsu +2

Backsplash galaxies are those that traverse and overshoot cluster cores as they fall into these structures. They are affected by environment, and should stand out in contrast to th…

astro-ph.GA2015★ 8 cited

Linking the Structural Properties of Galaxies and their Star Formation Histories with STAGES

Carlos Hoyos, Alfonso Aragón-Salamanca, Meghan E. Gray +5

We study the links between star formation history and structure for a large mass-selected galaxy sample at 0.05 < z_phot < 0.30. The galaxies inhabit a very broad range of environm…

astro-ph.CO2013★ 21 cited

Tully-Fisher analysis of the multiple cluster system Abell 901/902

Benjamin Bösch, Asmus Böhm, Christian Wolf +7

We derive rotation curves from optical emission lines of 182 disk galaxies (96 in the cluster and 86 in the field) in the region of Abell 901/902 located at . We focus…

astro-ph.CO2012★ 37 cited

Ram pressure and dusty red galaxies - key factors in the evolution of the multiple cluster system Abell 901/902

Benjamin Bösch, Asmus Böhm, Christian Wolf +6

We present spectroscopic observations of 182 disk galaxies (96 in the cluster and 86 in the field environment) in the region of the Abell 901/902 multiple cluster system, which is…

astro-ph.CO2011★ 15 cited

Spatial matter density mapping of the STAGES Abell A901/2 supercluster field with 3D lensing

P. Simon, C. Heymans, T. Schrabback +13

We present weak lensing data from the HST/STAGES survey to study the three-dimensional spatial distribution of matter and galaxies in the Abell 901/902 supercluster complex. Our me…

astro-ph.CO2010★ 26 cited

The hierarchical build-up of the Tully-Fisher relation

Chiara Tonini, Claudia Maraston, Bodo Ziegler +4

We use the semi-analytic model GalICS to predict the Tully-Fisher relation in the B, I and for the first time, in the K band, and its evolution with redshift, up to z~1. We refined…