Natascha Greisel, Stella Seitz, Niv Drory, Ralf Bender, Roberto Saglia, Jan Snigula
We describe the construction of a template set of spectral energy distributions (SEDs) for the estimation of photometric redshifts of luminous red galaxies (LRGs) with a Bayesian template fitting method. By examining the color properties of several publicly available SED sets within a redshift range of 00.15) of 0.12%. We show that templates that optimally describe the brightest galaxies (-24.5View original: http://arxiv.org/abs/1303.3005
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