Bar fraction as a function of apparent F150W magnitude (top panel) and effective radius (bottom panel) for a population of massive (10 < log M_*/M_⊙ < 11) galaxies at z < 1. The blue solid line indicates the observed fraction, while the black dashed line shows the best fit (see text for details). The red solid line and shaded region show the corrected fractions and associated uncertainties after applying the weights.