Simulating Gas at High Redshift
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We discuss simulations of gas at high redshift. We briefly review the methods used and the results for quasar absorption lines. We present gas mass functions and galaxy correlation functions for 5 different cosmological models. Galaxies should be detectable at redshifts greater than 2 by SKAI, and measurements of the gas mass functions and galaxy correlation functions could be used to discriminate between different cosmological models.
9 pages, 4 figures in text, LaTex (paspconf.sty) To appear in the conference proceedings of Highly Redshifted Radio Lines
9 pages, 4 figures in text, LaTex (paspconf.sty) To appear in the conference proceedings of Highly Redshifted Radio Lines