Abstract

We introduce redMaGiC, an automated algorithm for selecting Luminous Red Galaxies (LRGs). The algorithm was specifically developed to minimize photometric redshift uncertainties in photometric large-scale structure studies. redMaGiC achieves this by self-training the color-cuts necessary to produce a luminosity-thresholded LRG sample of constant comoving density. We demonstrate that redMaGiC photozs are very nearly as accurate as the best machine-learning based methods, yet they require minimal spectroscopic training, do not suffer from extrapolation biases, and are very nearly Gaussian. We apply our algorithm to Dark Energy Survey (DES) Science Verification (SV) data to produce a redMaGiC catalog sampling the redshift range z[0.2,0.8]z\in[0.2,0.8]. Our fiducial sample has a comoving space density of 103 (h1Mpc)310^{-3}\ (h^{-1} Mpc)^{-3}, and a median photoz bias (zspeczphotoz_{spec}-z_{photo}) and scatter (σz/(1+z))(\sigma_z/(1+z)) of 0.005 and 0.017 respectively. The corresponding 5σ5\sigma outlier fraction is 1.4%. We also test our algorithm with Sloan Digital Sky Survey (SDSS) Data Release 8 (DR8) and Stripe 82 data, and discuss how spectroscopic training can be used to control photoz biases at the 0.1% level

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This paper was published in UCL Discovery.

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