Fig. B.1.
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Channel maps of the quasar host–MQN01-QC system extracted from the continuum-subtracted ALMA band 3 datacube. Each panel was obtained by averaging channels in the datacube within 100 km s−1-wide windows, as reported at the top of each panel. The original datacube used for the kinematical modeling has a channel width of 25 km s−1. The maps are color-coded based on the signal-to-noise ratio. The gray contours show −2 × S/N (dotted), and 2n × S/N (solid) isophotes, where n ≥ 1 is an integer number. The green contours show the best-fit rotating disk model as obtained with 3DBAROLO.
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