Comparison of the FOV between Mrk 1044’s observations with HST WFC3/UVIS image in the F547M filter (left), VLT MUSE WFM (center), and VLT MUSE NFM-AO (right). The two images from MUSE are white-light images which were created by integration over the wavelength axis. Both WFC3/UVIS and MUSE WFM have a FOV that covers the host galaxy beyond its effective radius of its disk r_e = 7.14 ± 0.04 kpc (Wang et al. 2014), whereas MUSE NFM-AO only captures the innermost 3.1 × 3.2 kpc.