Top: A68/h7 stellar population fits including nebular emission. Here the older Calzetti-based population renders the photometry longwards of 4000 Å well, but fits less the UV, and ultimately the SMC has the smallest . Bottom: full and FIR SED (red and green, respectively). Only M10 templates could produce and in particular = 4.2 for the present SED, attenuated with the SMC law. The peak and width of the dust emission distribution are well fitted here by a R09 template.
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