Fig. C.1.
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Same as Fig. 7 but with the apparent silicate strength as calculated by Eq. 6 (red), which shows no trend. The 12.7/11.3 PAH EW ratio is also shown (blue) against HCN-vib on the right-hand axis of each plot and shows a very weak trend. A comparison with Fig. 7 shows the value in accounting for the star-forming contribution to properly recover properties of the obscured nucleus.
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