Comparison of temperature profiles inside the planetary Hill sphere determined using MCRT simulations (upper row) and their differences (lower row) relative to the corresponding RHD temperature profiles. Each plot contains three color coded curves that correspond to three different model resolutions (N1, N2, and N3). Left: radial temperature profiles of the midplane in the azimuthal direction of the planet. Right: polar temperature profiles of the planetary region. The planetary mass, M_p, and the accretion parameter, A, are specified in the upper-right corner of this figure.