Composite NIRCam image of the Bar showing the NIRSpec mosaic footprint (white boundary). The composite image is composed of F335M (AIB emission) in red, F470N-F480M (H₂ emission) in green, and F187N (Paschen α emission) in blue (Habart et al. 2024). Bright stars θ¹ Ori C and θ² Ori A are indicated with black circles in the left panel. In the right panel the five black boxes indicate the apertures used to extract our five template spectra. The dot-dashed line indicates the cut perpendicular to the Bar (position angle, PA, of 155.79°), while the dashed line indicates the position of the ionisation front in the NIRSpec FOV (PA=46.2l°). The protoplanetary disks 203–504 and 203–506 are indicated with black circles.