activity
19982004
most citedGaBoDS: The Garching-Bonn Deep Survey -- I. Anatomy of galaxy clusters in the background of NGC 300

59 citations · 104 across the 6 of their papers we have counts for

collaborators

16 papers

astro-ph2004

The galaxy-dark matter bias in the Garching-Bonn Deep Survey

Patrick Simon, Peter Schneider, Thomas Erben +3

We measured the bias and correlation factor of galaxies with respect to the dark matter using the aperture statistics including the aperture mass from weak gravitational lensing. T…

astro-ph200444 cited

GaBoDS: The Garching-Bonn Deep Survey -- II. Confirmation of EIS cluster candidates by weak gravitational lensing

Mischa Schirmer, Thomas Erben, Peter Schneider +2

We report the first confirmation of colour-selected galaxy cluster candidates by means of weak gravitational lensing. Significant lensing signals were identified in the course of t…

astro-ph20031 cited

Cosmic Shear from STIS pure parallels: III. Analysis of Cycle 9 pure parallels

J. -M. Miralles, T. Erben, H. Haemmerle +4

Following the detection of a cosmic shear signal at the 30'' scale using archival parallel data from the STIS CCD camera onboard HST in Haemmerle et al. (2002), we analyzed a large…

astro-ph200359 cited

GaBoDS: The Garching-Bonn Deep Survey -- I. Anatomy of galaxy clusters in the background of NGC 300

Mischa Schirmer, Thomas Erben, Peter Schneider +4

The Garching-Bonn Deep Survey (GaBoDS) is a virtual 12 square degree cosmic shear and cluster lensing survey, conducted with the [email protected] MPG/ESO telescope at La Silla. It consists…

astro-ph2003

Galaxy-galaxy lensing results from COMBO-17

Martina Kleinheinrich, Peter Schneider, Thomas Erben +4

We use galaxy-galaxy lensing to study the statistical properties of the dark matter halos of galaxies. Our data is taken from the COMBO-17 survey which has imaged 1 square degree i…

astro-ph2002

Weak lensing study of Abell 2029

Brice Menard, Thomas Erben, Yannick Mellier

Abell 2029 is one of the most studied clusters due to its proximity (z=0.07), its strong X-ray brightness and its giant cD galaxy which is one of the biggest stellar aggregates we…