A3COSMOS: The dust content of massive quiescent galaxies and its evolution with cosmic time

Open Access

Fig. D.1.

Normalised distribution of rest-frame wavelengths used to compute $L_{850}^{rest}$ $L_{850}^{\mathrm{rest}}$ for each stack in Fig. 4, weighted by the relative contribution of the individual pointing to the stacks. The vertical dashed orange and blue lines indicate $λ = \frac{hc}{k_{B} T}$ $\lambda=\frac{hc}{k_{\mathrm{B}}T}$ for a dust temperature of 21 K and 17 K, respectively.

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