F814W (in blue) and F160W (in red) imaging in CANDELS (Koekemoer et al. 2011) of six example galaxies in VUDS. The green contours show the isophote used to derive prior to the PSF and sky correction. The black ellipses are constructed from the values of r_e,b/a and θ_PA derived from GALFIT for these galaxies in each band. We refer to Figs. 4 and 11, which compare the derived sizes for the full set covered by CANDELS.