Cold gas at high redshifts
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ASI Conference Series
Abstract
I will discuss the use of semi analytic models of galaxy formation for calculating the cold gas fraction in galaxies. I will apply this to compute the large scale distribution of cold gas at high redshifts and comment on observability of the signal using upgraded and upcoming radio telescopes.
Description
Only IISERM authors are available in the record.
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Citation
31st ASI Meeting, ASI Conference Series, 2013, Vol. 9, p. 85