Modeling results of the V 1094 Sco disk from ALMA observations. A Nuker profile is fitted to the continuum emission distribution of the disk in the uv-plane. The panels show: the real and imaginary part of the observed and modeled visibilities, the 1D and 2D histograms of the Nuker model free parameters, the brightness emission and cumulative distributions, the R_68% and R_95% radii, and the fit results in the image plane. The very extended emission of V1094 Sco was studied in detail in van Terwisga et al. (2018), and fitted with a more detailed function. For a comprehensive characterization of this disk we refer to that work. Nevertheless, our fit using the Nuker profile allows us to infer a characteristic radius consistent with the rest of the Lupus disk population.