The radio identification of submillimeter galaxies is revolutionizing our understanding of this enigmatic population. The combination of radio/submm photometric redshifts, spectroscopy of the optically brighter sources, and modeling of the population are leading us slowly towards the goal of a redshift distribution for SCUBA galaxies.
Friday, 10 May 2002
11:00am
Array Operations Center Auditorium
Local Host: Chris Carilli