Extended Data Fig. 3: SED black body model fits to MATISSE aperture photometry.
From: Thermal imaging of dust hiding the black hole in NGC 1068
The figures are labelled with the aperture names defined in Fig. 2. The shaded areas show all models falling inside 1 sigma of the photometry, considering both pure amorphous olivine (magenta) and a mix of olivine and 20% amorphous carbon by weight (cyan). The plots for apertures E1 and SE are in the main article.
