Chao-Ling HUNG
(IfA, Hawaii)
I will present a morphological analysis of 2084 Herschel-selected galaxies at 0.2<z<1.5. I will discuss what is the frequency of disk-like galaxies and interacting systems as a function of galaxy's infrared luminosity, stellar mass, and the location on the SFR-Mass relation (or "galaxy main sequence").