The submm proprieties of extremely red objects

A basic but crucial step toward our understanding of the evolution of the Universe and the objects within it is a complete accounting of the systems which produce the far-infrared background light. Once identified, the relationship between these populations and their role in the formation of galaxies must be determined. In this paper we focus on two equally interesting high-redshift populations: the submillimeter (submm) bright galaxies and the Extremely Red Objects (EROs)