Further results of DL07 SED fitting including artificial ALMA band 6 photometry. Color coding is based on the number of available photometric bands (see Fig. 17). Left: exposure time estimate (without overheads) for ALMA band 6 observations of Herschel-detected galaxies. The t_exp estimate for individual sources (upper bigger panel, dots) are shown and summed up to compute the cumulative t_exp needed to observe all sources above a given value of M_dust (solid histograms). Dotted histograms represent the number distribution of sources. Right: distribution of ALMA band 6 expected fluxes, as a function of dust mass, for galaxies detected by Herschel in the GOODS-S field. The horizontal dashed lines correspond to 0.38 and 0.18 [mJy] flux limits (dark and light gray, respectively). The right side and bottom panel show the projected 1D distributions. The hatched dark and light gray histograms only include sources above the flux limits indicated.