Detecting Galaxy Clusters in the DLS and CARS: a Bayesian Cluster Finder
Bego\~na Ascaso, David Wittman, Narciso Ben\'itez, the DLS, collaboration

TL;DR
This paper introduces a Bayesian matched filter algorithm for detecting galaxy clusters, demonstrating high completeness and purity in simulations and applying it successfully to real survey data, including DLS and CARS.
Contribution
The novel Bayesian cluster finder improves detection accuracy and provides estimates of cluster properties, outperforming previous methods in real survey applications.
Findings
Achieved 100% completeness and 80% purity in mock catalogs for clusters up to z<1.2
Recovered known clusters and identified new candidates in CARS data
Detected over 780 cluster candidates in DLS up to redshift 1.2
Abstract
The detection of galaxy clusters in present and future surveys enables measuring mass-to-light ratios, clustering properties or galaxy cluster abundances and therefore, constraining cosmological parameters. We present a new technique for detecting galaxy clusters, which is based on the Matched Filter Algorithm from a Bayesian point of view. The method is able to determine the position, redshift and richness of the cluster through the maximization of a filter depending on galaxy luminosity, density and photometric redshift combined with a galaxy cluster prior. We tested the algorithm through realistic mock galaxy catalogs, revealing that the detections are 100% complete and 80% pure for clusters up to z <1.2 and richer than \Lambda > 25 (Abell Richness > 0). We applied the algorithm to the CFHTLS Archive Research Survey (CARS) data, recovering similar detections as previously published…
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Taxonomy
TopicsAstronomical Observations and Instrumentation · Astronomy and Astrophysical Research
