Upper panel: the nuclear SED of the dust continuum emission in NGC 1068 derived using NIR and MIR continuum and spectroscopy data (blue squares) from Alonso-Herrero et al. (2011), and the ALMA data points in Bands 7 and 9 (red stars). The SED was derived in apertures centered at the AGN that range from (~14 pc) for NIR data to (~35 pc) for MIR and Band-7 ALMA data. The best CLUMPY model fit to the observations (curve) and the 1σ uncertainty range of the fit (gray shaded region) are superposed onto the data points. Lower panel: a close-up view of the dust continuum emission in Band 9. Levels and markers are as in Fig. 1. The ()-aperture used to extract the flux at the position of the AGN is plotted as an ellipse.