Abstract
Massive cosmological surveys such as BOSS, eBOSS and the future DESI, J-PAS, Euclid and LSST will collect data for millions to, ultimately, billions of galaxies up to redshift z = 2 and beyond, with the primary goal of understanding the nature of the dark energy that drives the present-day accelerated expansion of the universe. These galaxy samples have tremendous potential, not only with…