Astronomy and Astrophysics – Astronomy
Scientific paper
Jan 2010
adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2010aas...21543607a&link_type=abstract
American Astronomical Society, AAS Meeting #215, #436.07; Bulletin of the American Astronomical Society, Vol. 42, p.385
Astronomy and Astrophysics
Astronomy
Scientific paper
We present the first sample of optical-selected galaxy clusters in Deep Lens Survey (DLS). A new technique for detecting clusters has been designed basing on a bayesian approach of the Matched Filter Algorithm. The method provides flexibility to determine cluster characteristics such as the redshift or richness through the maximization of a redshift-dependent filter. The sample is complete up to redshift 0.7 and we detect 780 clusters up to redshift 1.1. The algorithm has also been tested on CFHTLS Archive Research Survey data obtaining almost the same detections than they do plus additional clusters that are very probably real. In this work, we present a photometric analysis of the DLS optical cluster sample from local to high resdhift and determine their degree of evolution. Additionally, we compare and discuss the differences between the Weak Lensing and Optical Detections.
Ascaso Begoña
Dell'Antonio Ian
Khiabanian Hossein
Kubo Jisuke
Margoniner Vera
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