Laerte Sodre
Brasil – Universidade de São Paulo
A photometric estimator of galaxy cluster masses
Abstract: We model the cumulative galaxy number profile of SDSS clusters of galaxies with a Sérsic profile plus a two-halo term, using photometric redshifts to ascribe cluster membership. The fitted parameters allow us to obtain the splashback radii of the clusters. Using masses obtained by weak lensing for calibration, we show that we are able to estimate cluster masses from the splashback radii with a dispersion of 0.12 dex. The results are robust with
respect to the magnitude limit adopted for the analysis and show that we are able to estimate cluster masses with good accuracy by using photometric information only.