Simulating Gas at High Redshift

Authors

N Katz, University of Massachusetts - AmherstFollow
L Hernquist
DH Weinberg

Publication Date

1998

Journal or Book Title

Highly Redshifted Radio Lines

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 maWe 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.ss functions and galaxy correlation functions could be used to discriminate between different cosmological models.

Comments

This is the pre-published version harvested from ArXiv. The published version is located at http://www.aspbooks.org/a/volumes/article_details/?paper_id=16598

Pages

1

Volume

156

Recommended Citation

Katz, N; Hernquist, L; and Weinberg, DH, "Simulating Gas at High Redshift" (1998). Highly Redshifted Radio Lines. 982.
Retrieved from https://scholarworks.umass.edu/astro_faculty_pubs/982