Revealing the dust grain size in the inner envelope of the Class I protostar Per-emb-50

C.A.G. acknowledges support from CONICYT-Becas Chile (grant 72160297). P.C, J.P and L.S acknowledge the financial support of the European Research Council (ERC; project 320620). L.T. acknowledges the financial support of the Italian Ministero dell’Istruzione, Universita e Ricerca through the grant Progetti Premiali 2012 – iALMA (CUP C52I13000140001), and by the Deutsche Forschungs-gemeinschaft (DFG, German Research Foundation) – Ref no. FOR 2634/1 TE 1024/1–1. M.T. has been supported by the DISCSIM project, grant agreement 341137 funded by the European Research Council under ERC-2013-ADG. A.M. acknowledges an ESO Fellowship.