Fig. 8
Median values of accretion rate as a function of binned stellar mass. Each point is the median of 5 Ṁacc values with similar M⋆. The plotting errors were computed in the same way as in Fig. 5. The horizontal bars represent the intervals in log M⋆. The dashed line shows the two power-law relationship by Vorobyov & Basu (2009), vertically shifted by −1 dex.
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