Improved photometric redshifts with colour-constrained galaxy templates for future wide-area surveys

Abstract

Cosmology and galaxy evolution studies with LSST, \Euclid, and {\it Roman}, will require accurate redshifts for the detected galaxies. In this study, we present improved photometric redshift estimates for galaxies using a template library that populates three-color space and is constrained by \HST/CANDELS photometry. For the training sample, we use a sample of galaxies having photometric redshifts which allows us to train on a large, unbiased galaxy sample having deep, unconfused photometry at optical-to-mid infrared wavelengths. Galaxies in the training sample are assigned to cubes in three-dimensional color space, $V-H$, $I-J$, and $z-H$. We then derive the best-fit spectral energy distributions of the training sample at the fixed CANDELS median photometric redshifts to construct the new template library for each individual color cube (i.e. color-cube-based template library). We derive photometric redshifts (photo-z) of our target galaxies using our new color-cube-based template library and with photometry in only a limited set of bands, as expected for the aforementioned surveys. As a result, our method yields ${\sigma }_{NMAD}$ of 0.026 and an outlier fraction of 6\% using only photometry in the LSST and \Euclid/{\it Roman} bands. This is an improvement of $\sim$10\% on ${\sigma }_{NMAD}$ and a reduction in outlier fraction of $\sim$13\% compared to other techniques. In particular, we improve the photo-z precision by about 30\% at $2<z<3$. We also assess photo-z improvements by including $K$ or mid-infrared bands to the $ugrizYJH$ photometry. Our color-cube-based template library is a powerful tool to constrain photometric redshifts for future large surveys.

13 pages, 7 figures, 4 tables; MNRAS submitted

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