Comparison between the azimuthally averaged ALMA Band 7, 6, 3, and VLA Ka band surface brightness radial profiles (purple solid line and shaded region, including the calibration uncertainty) with the posterior distribution of our fit (black dashed line and shaded region, for the median and the area between the 16^th and 84^th percentiles). Results from the high (low) resolution fit are displayed for ALMA (VLA) data. An excellent agreement between models and observations can be seen.