Best-fitting IR SEDs for the global ALMA Bands 9, 8, 7, and 6 continuum emission of HZ10 (77 μm, 110 μm, 158 μm, and 198 μm, respectively). The wavelength is given in the rest frame. The blue-solid line corresponds to the best-modified SED given by Eqs. (2)–(4) and using the maximum likelihood parameters (see top-left corner). The combination between new ALMA Band 9 and 7 continuum measurements (77 μm and 158 μm rest frame, respectively) allows us to probe the peak of the dust SED, and hence constrain these parameters accurately. In addition, we have included estimations of the global continuum emission flux for HZ10 from Capak et al. (2015) (orange square) and Faisst et al. (2020) (green triangles) to contrast our estimations with previous results.