Surface brightness profile of HD 141569A in the H band along the southern major axis (top panel) and of HD 150193A in the H band along the northern major axis (bottom panel). The 3σ upper limit on the polarized-light profile is obtained from the Q_T and U_T images. The 3σ upper limit on the scattered-light profile is obtained by assuming a conservative value for the polarization fraction of 10%. The gray area in the bottom panel denotes our measured stellar intensity profile, taking into account the 40% uncertainty from the photometric calibration. The scattered-light disk profile by Fukagawa et al. (2003) is still consistent with being an unsubtracted stellar PSF.