Simultaneous fit of the visibilities (top) and the SED (bottom) of UX Ori with a CG-disk model including an inner dust-free hole and a puffed-up inner rim. Top: comparison of the best-fit model visibilities (colored lines) to the near- and mid-infrared visibilities (data points) of UX Ori. The shadowed areas denote the telluric band gaps between the J and H and H and K band for the near-infrared (top) and the ozone feature for the mid-infrared (middle) where no data can be taken or where they are not reliable as a result of the limited transmission of the atmosphere (black line). Bottom: spectral energy distribution of UX Ori (data points) with the total flux and the single flux components of the best-fit model.