Photometric properties of NEWCLUSTER galaxies at z = 0.8. The x-axis shows the r-band absolute magnitude. The y-axis of the top (bottom) panel represents g − r color (g-band effective surface brightness). We also present the black arrow to show the effect of dust attenuation assuming E(B − V) = 0.1 with Calzetti attenuation curve (Calzetti et al. 2000). The color of data points indicates the mass-weighted age of galaxies. The grey contours in both panels represent local observations from SDSS (Nair & Abraham 2010).