Fig. C.1
Comparison of some of the Spitzer-based SED models (pink lines; Sicilia-Aguilar et al. 2011, 2013a,b) and predicted 70/160 μm fluxes with the actual Herschel/PACS observations. Filled symbols mark detections at different wavelengths. Errorbars are shown in blue for both photometry points (often smaller than the symbols) and the IRS spectra. Upper limits are marked as inverted open triangles. Marginal detections (close to 3σ or affected by nebulosity) are marked as open circles. A photospheric MARCS model is displayed as a dotted line for comparison.
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