A few days ago we were notified that our latest proposal to use EMIR, an IR spectrograph at 10.4m GTC, was accepted! We are going to use it to observe in the near-IR a number of Red Supergiants in the NGC 6822 and IC 10 galaxies, for which we have already obtained optical spectra with previous multi-object spectroscopic observations with OSIRIS at GTC (see our previous posts for the 2022A and 2020A periods, and on mask preparation).
