Fig. 13.
Spatially resolved SFR map calculated from the extinction corrected Hα emission line for each spaxel of the MUSE sub-cube. The colour-bar shows the SFR in units of M⊙ yr−1. The cross shows the location of the AGN, while the contours display the Hα flux intensity. The white background corresponds to the spaxels, which have an S/NHα < 10.
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