Toward a population synthesis of disks and planets - II. Confronting disk models and observations at the population level

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Fig. 4

Cumulative distribution of disc lifetimes for a population with canonical parameter distribution (see text). Two exponential decays following Fedele et al. (2010) with a characteristic time of 2.3 Myr (accretion) and 3 Myr (infrared excess) and the results of Ribas et al. (2014) are shown as well.

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