We study the fraction of tidal interactions and mergers with well identified observability timescales (fTIM) in group, cluster, and accompanying field galaxies and its dependence on redshift (z), cluster velocity dispersion (sigma) and environment analyzing HST-ACS images and catalogs from the ESO Distant Cluster Survey (EDisCS). Our sample consists of 11 clusters, 7 groups, and accompanying field galaxies at 0:4 equal or less z equal or less 0:8. We derive fTIM using both a visual classification of galaxy morphologies and an automated method, the G-M20 method. We calibrate this method using the visual classifications that were performed on a subset of our sample. We find marginal evidence for a trend between fTIM and z, in that higher z va...
Context. We present a spectrophotometric analysis of the galaxy population in the area of the merg...
We examine the effects of an impending cluster merger on galaxies in the large-scale structure (LSS)...
Combining resolved optical spectroscopy with panoramic HST imaging, we study the dynamical propertie...
International audienceWe study the fraction of tidal interactions and mergers (TIMs) with well-ident...
We study the morphological content of a large sample of high-redshift clusters to determine its depe...
We compile a sample of spectroscopically and photometrically selected cluster galaxies from four hig...
We describe Hubble Space Telescope (HST) imaging of 10 of the 20 ESO Distant Cluster Survey (EDisCS)...
We study the morphological content of a large sample of high-redshift clusters to determine its depe...
We explore the possible effect of cluster environments on the structure and star formation histories...
At redshifts of z ≲ 1.3, early-type galaxies (ETGs) and passive galaxies are mainly found in dense e...
Minor mergers are thought to be responsible for the size growth of quiescent field galaxies with dec...
© 2018 The Author(s). We present an analysis of the kinematics of a sample of 14 galaxy clusters via...
Combining resolved optical spectroscopy with panoramic HST imaging, we study the dynamical propertie...
I present a study of the merger rate of galaxies in various cluster environments. Mergers are thoug...
Context. We present a spectrophotometric analysis of the galaxy population in the area of the merg...
We examine the effects of an impending cluster merger on galaxies in the large-scale structure (LSS)...
Combining resolved optical spectroscopy with panoramic HST imaging, we study the dynamical propertie...
International audienceWe study the fraction of tidal interactions and mergers (TIMs) with well-ident...
We study the morphological content of a large sample of high-redshift clusters to determine its depe...
We compile a sample of spectroscopically and photometrically selected cluster galaxies from four hig...
We describe Hubble Space Telescope (HST) imaging of 10 of the 20 ESO Distant Cluster Survey (EDisCS)...
We study the morphological content of a large sample of high-redshift clusters to determine its depe...
We explore the possible effect of cluster environments on the structure and star formation histories...
At redshifts of z ≲ 1.3, early-type galaxies (ETGs) and passive galaxies are mainly found in dense e...
Minor mergers are thought to be responsible for the size growth of quiescent field galaxies with dec...
© 2018 The Author(s). We present an analysis of the kinematics of a sample of 14 galaxy clusters via...
Combining resolved optical spectroscopy with panoramic HST imaging, we study the dynamical propertie...
I present a study of the merger rate of galaxies in various cluster environments. Mergers are thoug...
Context. We present a spectrophotometric analysis of the galaxy population in the area of the merg...
We examine the effects of an impending cluster merger on galaxies in the large-scale structure (LSS)...
Combining resolved optical spectroscopy with panoramic HST imaging, we study the dynamical propertie...