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Fig. C.1

image

Peak line-to-continuum ratio of the a)–c) R(6) 1000–0000 line at 3 μm, d)–f) Q(6) 0110–0000 line at 14 μm, and g)–i) between 13.7 and 14.1 μm. The non-LTE models with a constant abundance and a gas-to-dust (G/D) ratio of 100, 1000 and 100 000 are shown (Fig. 6), convolved to a spectral resolving power R = λ/ Δλ between 100 and 105. Horizontal red dashed lines show the required signal-to-noise (S/N) in the continuum to detect a line at a 5σ level.

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