Simulating the high-redshift universe in the sub-mm

Abstract

I present various simulations of an on-going large sub-mm survey, SHADES, showing how constraints can be put on galaxy formation models and cosmology from this survey.

4 pages, 1 figure, to appear in Proceeding of the ''Multi-wavelength Cosmology'', Conference held in Mykonos, Greece, June 2003

References in corpus (3)

• The Canada-UK Deep Submillimeter Survey VI: The 3-Hour Field
• The coincidence and angular clustering of Chandra and SCUBA sources
• Damped Lyman alpha systems and disk galaxies: number density, column density distribution and gas density