Galaxy clustering measurements out to redshift z ∼ 8 from Hubble Legacy Fields

Abstract

We present a novel approach for measuring the two-point correlation function of galaxies in narrow pencil beam surveys with varying depths. Our methodology is utilized to expand high-redshift galaxy clustering investigations up to z ∼ 8 by analysing a comprehensive sample consisting of Ng = 160 Lyman break galaxy candidates obtained through optical and near-infrared photometric data within the CANDELS GOODS data sets from the Hubble Space Telescope Legacy Fields. For bright sources with MUV < -19.8, we determine a galaxy bias of b = 9.33 ± 4.90 at z = 7.7 and a correlation length of r0 = 10.74 ± 7.06 h-1 Mpc. We obtain similar results for the XDF, with a galaxy bias measurement of b = 8.26 ±..