Abstract
This chapter describes the assumed specifications and sensitivities for HI galaxy surveys with SKA1 and SKA2. It addresses the expected galaxy number densities based on available simulations as well as the clustering bias over the underlying dark matter. It is shown that a SKA1 HI galaxy survey should be able to find around galaxies over 5,000 deg (up to ), while SKA2 should find galaxies over 30,000 deg (up to ). The numbers presented here have been used throughout the cosmology chapters for forecasting.
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