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Fig. 13.


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Normalised physical properties of the HRS quenched galaxies as a function of /. These are the dust mass (left panel), the dust temperature (middle panel), and the FUV attenuation (right panel) normalised by the corresponding property of a reference sample built to have the same stellar mass as the quenched source. Symbols are colour-coded according to their age of quenching agetrunc.

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