Central 36×36 region of NGC 7319, which includes the AGN and the northern radio lobe and hotspot N2. First row, from left to right: [Ne II]12.81 μm, [Ne III]15.56 μm, [Ne V]14.32 μm, and [Ne VI]7.65 μm MIRI MRS line maps. The dashed circles on the [Ne II] map are the AGN and N2 extraction apertures. Second row, from left to right: [Ar II]6.99 μm, [Fe II]5.34 μm, H₂ S(5) 6.91 μm, and [Mg V]5.61 μm MIRI MRS line maps. The contours on the second panel represent the 1.4 GHz emission, as in Fig. 1. Third row: first two panels are the same as the top-row panels of Fig 1. The third panel is the JWST/NIRCam F090W (λ_p=0.90 μm) image after dividing by a Gaussian (FWHM = 142) smoothed version of itself to highlight finer details. The fourth panel is the H₂ S(2) 12.28 μm emission line. The dotted and dashed black lines trace the jet axis (N2 hotspot–AGN axis) and disk dust lanes, respectively. The red hatched circles represent the PSF FWHM, ∼026–060 depending on the wavelength, estimated from the unresolved AGN continuum.