Abstract

We analyze a representative sample of dusty star-forming galaxies in the Extended Groth Strip (EGS) with deep infrared HST imaging to assess the recent claim of morphological transformation with redshift. We support the claim that disks are the dominant morphology, with bulges being developed along the way, in a similar way to other optically-selected massive star-forming galaxies in the field. We will also briefly summarize the mapping efforts conducted with the TolTEC camera in Large Millimeter Telescope (LMT) to uncover samples of tens of thousands of dusty galaxies in these fields that will tie the dust and star formation properties of the luminous infrared galaxy population (>10 Msun/yr) at z<10.