Overview of the different spatial components of the HH 48 NE system using a composition of observations. The JWST/NIRSpec disk continuum at 4 µm is shown in red, the jet is shown in blue using HST/ACS observations of the [O I] line at 0.6 µm (Stapelfeldt et al. 2014), and the vertically extended disk wind is shown in green using the H₂ 0–0 S(9) transition. The region used to extract a disk-integrated spectrum is shown by the dashed rectangle. The continuum in this region is shown on a logarithmic scale in Fig. 4. The direction toward HH 48 SW is marked with a white arrow.