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Fig. 4

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Cumulative distributions functions generated by the Kaplan-Meier estimator. Top: cumulative distribution of the dust mass, normalized by the fraction of detected sources in each star-forming regions. Bottom: cumulative distribution of the dust-to-stellar mass ratio. The bottom distributions include disks not detected in millimeter emission. Those are scattered over the distribution of Mdust /M (see Sect. 4.2.3). We indicate 1σ confidence intervals.

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