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Fig. 9.

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Log average dust mass recovered as a function of the (log) stellar mass in each redshift bin. The circles represent detections (above 3σ), and the 3σ upper limits are represented by down-pointing arrows. We overplot the z = 1 and z = 6 dust mass-stellar mass relation from Popping et al. (2017) and the z ∼ 1 and z ∼ 5 relations from Lagos et al. (2019) (SHARK model), Triani et al. (2020), and Vijayan et al. (2019). We show the average dust mass directly predicted by the SHARK model and the dust mass computed from the predicted band 6 flux following Eq. (1).

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