Fig. A.1.

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From top left to bottom right: mom0 maps of the most prominent PAH features (at 6.2, 7.7, 8.6, 11.3, and 12.7 μm) and the H2 0-0 S(1) 17.03 μm line. We obtained the mom0 maps after subtraction of the local continuum, from the MIRI-MRS cube re-binned to spaxel scale of 0.6″ (Sect. 3.1). Yellow contours trace the feature emission at levels of: [0.4, 0.55]×10−14 erg cm−2 s−1 (PAH 6.2); [2, 2.75]×10−14 erg cm−2 s−1 (PAH 7.7); [0.18, 0.27]×10−14 erg cm−2 s−1 (PAH 8.6); [1.5, 2]×10−14 erg cm−2 s−1 (PAH 11.3); [0.17, 0.22]×10−14 erg cm−2 s−1 (PAH 12.7); [0.19, 0.23]×10−14 erg cm−2 s−1 (H2 0-0 S(1)). Violet contours show the PAH 16.5 μm emission at [0.18, 0.225]×10−14 erg cm−2 s−1. In the top-left panel, the black arrow indicates the position angle of the jet (i.e. PAjet = 51 deg). The stars correspond to the position of the AGN. North is up, and east is to the left.
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