Fig. 12
Background SED fit analysis results. Each panel shows the PDF of a given physical parameter (top left: energy fraction absorbed by the ISM as estimated from stellar-dominated, OPT, or dust-dominated photometry, IR; top middle left: total effective V-band optical depth seen by stars in birth clouds; top middle right: warm dust temperature in birth clouds; top right: stellar mass; bottom left: star-formation rate; bottom middle-left: specific star-formation rate; bottom middle right: dust luminosity; bottom right: dust mass). The red inverted triangles indicate the 16th, 50th, and 84th percentiles.
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