Circularized effective radius at rest-frame wavelength of 5000 Å as a function of stellar mass. Circles show the Ultra VISTA J-band sizes from our stacking analysis, corresponding roughly to a rest-frame wavelength of 5000 Å for our z ~ 1.4 sample. Squares (z ~ 1.25) and triangles (z ~ 1.75), along with their error bars, show the 16th, 50th, and 84th percentiles from van der Wel et al. (2014) for late-type galaxies as inferred using HST images of the CANDELS fields.