The SED fit of one galaxy (SDSS J0000+1438) in our sample. We have collected the NUV (GALEX), optical (SDSS), NIR (UKIDSS or 2MASS), and MIR (WISE) magnitudes and then performed the fitting with iSEDfit. The blue filled circles are actual photometry data used in the fitting, and the black open squares are predictions of the fitting model at the input bands. The WISE W1 and W2 bands (red open diamonds) have not been used in the fitting but only plotted as a comparison, since the PSF magnitudes will underestimate the flux of extended sources (e.g., nearby galaxies). Most of the photometry errors are tiny and thus are not visible in the plots.