2006/07/03 by M. Schirmer, Mischa Schirmer, Thomas Erben +5
Physics and Astronomy · #Adaptive optics and wavefront sensing #Astronomy and Astrophysical Research #Galaxies: Formation, Evolution, Phenomena #astro-ph
paper · pdf · doi:10.1051/0004-6361:20065955
published as Astron.Astrophys. 462 (2007) 875 · 25 pages, 18 figures, submitted to A&A; for a better print version, see http://www.astro.uni-bonn.de/~mischa/astroph_0607022.pdf
arxiv created 2006/07/03 · openalex publication_date 2006/11/13 · arxiv updated 2009/12/01 · openalex created_date 2025/10/10 · openalex updated_date 2026/07/31
Aims.The aim of the present work is the construction of a mass-selected galaxy cluster sample based on weak gravitational lensing methods. This sample will be subject to spectroscopic follow-up observations.