A significant fraction of galaxy formation activity is concealed from view at optical wavelengths by pbscuring dust. I will describe the nature of the population uncovered in this way, its links to more standard populations of high-redshift galaxies, and the prospects for making progress in understanding this population with ALMA and other future instruments.
Friday, 9 September 2005
11:00am
Array Operations Center Auditorium
Local Host: Chris Carilli