Weak lensing survey of galaxy clusters in the CFHTLS Deep ^*

Laboratoire d'Astrophysique de Toulouse-Tarbes, Observatoire Midi-Pyrénées, UMR5572 CNRS & Université Paul Sabatier, 14 Avenue Edouard Belin, 31400 Toulouse, France e-mail: gavazzi@physics.ucsb.edu

Received: 23 May 2006
Accepted: 30 October 2006

Abstract

Aims. We present a weak lensing search of galaxy clusters in the 4 deg² of the CFHT Legacy Survey Deep. This work aims at building a mass-selected sample of clusters with well controlled selection effects. This present survey is a preliminary step toward a full implementation in the forthcoming 170 deg² of the CFHTLS Wide survey.

Methods. We use the deep i' band images observed under subarcsecond seeing conditions to perform weak lensing mass reconstructions and to identify high convergence peaks. Thanks to the availability of deep  exposures, sources are selected from their photometric redshifts in the weak lensing analysis. We also use lensing tomography to derive an estimate of the lens redshift. After considering the raw statistics of peaks we check whether they can be associated to a clear optical counterpart or to published X-ray selected clusters.

Results. Among the 14 peaks found above a signal-to-noise detection threshold , nine are secure detections with estimated redshift and a velocity dispersion . This low mass range is accessible thanks to the high density of background sources. Considering the intersection between the shear-selected clusters and XMM-LSS X-ray clusters in the D1 field, we observe that the ICM gas in these low-mass clusters ( keV) is not hotter than the temperature inferred from shear, this trend being different for published massive clusters. A more extended weak lensing survey, with higher statistics of mass structures will be a promising way to bypass several of the problems related to standard detection methods based on the complex physics of baryons.