Fig. E.1

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Population diagrams for SiO for the three stars, IRAS 15194–5115 (left), IRAS 15082–4808 (centre), and IRAS 07454–7112 (right). The solid line (red) is the best-fit linear model to the data (black). Rotation temperatures, Trot, and source-averaged column densities, Ntot, are listed in the legends. Circle and square points denote lines observed with ALMA and APEX, respectively. Hollow circles denote lines for which data combination (see Sect. 3.3) was performed.
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