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Fig. C.8


Left panel: surface brightness profiles for PACS, MIPS, SPIRE, and IRAC 3.6 μm. Profiles are extracted as in Munoz-Mateos et al. (2009); those profiles are shown by solid lines, while the profiles presented here extend beyond the symbols as dashed lines. The vertical dashed lines indicate the optical radius, Ropt and 1.5 Ropt. Right panel: radial temperature trends Tdust vs. R/Ropt. For this galaxy, there are no radial bins having data with sufficient signal-to-noise to fit.

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