Multiwavelength Study of Massive Galaxies at<i>z</i>∼2. I. Star Formation and Galaxy Growth
Multiwavelength Study of Massive Galaxies at<i>z</i>∼2. I. Star Formation and Galaxy Growth
Examining a sample of massive galaxies at 1.4<z<2.5 with K_{Vega}<22 from the Great Observatories Origins Deep Survey, we compare photometry from Spitzer at mid- and far-IR, to submillimeter, radio and rest-frame ultraviolet wavelengths, to test the agreement between different tracers of star formation rates (SFRs) and to explore the implications …