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Fig. 2

image

Full PACS + SPIRE spectra for IRAS 23133+6050 (top, blue) and S 106 (bottom, red, multiplied by 0.01 for clarity). In addition we include the IRAS photometric points for each source (triangles), and for IRAS 23133+6050 also the WISE photometry (Wright et al. 2010) as squares and the SCUBA observations of Thompson et al. (2006) as diamonds. A modified blackbody fit for each spectrum is shown as a dashed line.

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