The effect of ionizing background fluctuations on the spatial correlations of high redshift Ly-emitting galaxies
arXiv:2208.04203 · doi:10.1093/mnras/stac2268
Abstract
We investigate the possible influence of fluctuations in the metagalactic photoionizing ultra-violet background (UVBG) on the clustering of Ly-emitting galaxies through the modulation of the ionization level of the gas surrounding the systems. At redshifts , even when assuming the reionization of the intergalactic medium has completed, the fluctuations are sufficiently large that they may non-negligibly enhance, and possibly even dominate, the angular correlation function on scales up to a few hundred arcsecs. Whilst a comparison with observations at is statistically consistent with no influence of UVBG fluctuations, allowing for the fluctuations opens up the range of acceptable models to include those with relatively low bias factors for the Ly-emitting galaxies. In this case, the evolution in the bias factor of Ly-emitters over the approximate redshift range corresponds to a nearly constant halo mass for Ly-emitting galaxies of .
arXiv comment11 pages, 8 figures; accepted for publication in MNRAS
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