Radial location of the peak of the emission of the various molecular tracers, compared to radial profiles of SPHERE scattered light and ALMA band 7 continuum intensity. Top panel: radial profiles of the ALMA band 7 continuum intensity (blue line, Isella et al. 2019) and SPHERE J-band polarized intensity (pink line, Keppler et al. 2018). The gray shadow shows the radius of the coronagraph in the J-band observations (Keppler et al. 2018). Bottom panel: radial position of the peak of the emission and its related uncertainty, for each detected line. The background color-bar refers to the radial profile of the ALMA band 7 continuum intensity. The two vertical dashed white lines indicate the planets position (Wang et al. 2021).