ASPCS
 
Back to Volume
Paper: Simulating Gas at High Redshift
Volume: 156, Highly Redshifted Radio Lines
Page: 1
Authors: Katz, N.; Hernquist, L.; Weinberg, D. H.
Abstract: 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.
Back to Volume