Spectra extracted from the MIR continuum peaks of the two protostars. Several absorption features associated with ice and dust are seen in both sources and emission lines coming from the disk and central protostars, although some contamination with outflows and winds is also possible. Top-left: zoom-in on the two hydrogen recombination lines detected in emission towards protostars. Bottom-right: spectra revealing molecular gas emission and corresponding slab models of CO (green) and H₂O (orange).