Most likely model from the theoretical formalism (based on the Bayes factor, row 5) of Table 1. In the left panel, we show the dirty image of the joined ACA+ALMA observations. The second panel is the likelihood-weighted model reconstruction from the nested sampling routine. The third panel shows the model corrected for the incomplete uv-coverage of the observations. On the right, we show the residuals by subtracting the model from the observed visibilities. The black contours are drawn at [−4.5, −3.5, −2.5, −1.5, 1.5, 2.5, 3.5]-σ based on the noise in the residual map. The third panel also includes the 0σ level. The contours in the second panel are drawn at [−6.5, −4.5, −2.5, 2.5, 3.5]-σ. The model shows a clear resemblance to the data.