Kevin COOKE
(Rochester Institute of Technology)
I present preliminary results of the investigation regarding the effect of local galaxy density on the star formation characteristics of ULIRGs and Most-Massive Group Galaxies between 2 < z < 3. Our sample is chosen to be >10^10 M_solar, with detections in at least one Herschel band. I will discuss the use of SED3FIT to fit this sample, and the resulting estimates for SFR, stellar mass, and AGN contribution to the far-infrared.