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Fig. 1.


Distribution of the integrated flux density and bolometric L/M of all ATLASGAL sources (in blue filled contours, the darker region corresponds to higher density) (Urquhart et al. 2018) and the target sources observed with SABOCA (gray pluses and dots) at different distance ranges. The histograms on the right side and in the top panel show the 1D distributions of integrated flux density and L/M of all ATLASGAL sources (blue) and all target sources (gray), respectively.

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