J. Lewis, P. Ocvirk, Y. Dubois, D. Aubert, J. Chardin, N. Gillet, and É. Thélie. (2022)cite arxiv:2204.03949Comment: submitted to MNRAS, 1st report received: under revision Have partially addressed referee's concerns, namely that the model predicts high dust masses and redder bright galaxies than expected, by discussing this aspect around the relevant results. Work is being carried out to present a clearer parameter exploration of the dust model.