Cosmic Reionization on Computers: Properties of the Post-reionization IGM

Abstract

We present a comparison between several observational tests of the post-reionization intergalactic medium and the numerical simulations of reionization completed under the Cosmic Reionization On Computers (CROC) project. The CROC simulations match the gap distribution reasonably well, and also provide a good match for the distribution of peak heights, but there is a notable lack of wide peaks in the simulated spectra and the flux-probability distribution functions are poorly matched in the narrow redshift interval , with the match at other redshifts being significantly better, albeit not exact. Both discrepancies are related: simulations show more opacity than the data.