Fig. 5
Spatially resolved properties of the ASASSN-15lh host. In the top row, reconstructed images of total intensity in the MUSE spectral range (4650 Å to 9300 Å) in the left panel, and the central component of Hα emission in the right panel. The bottom row shows the stellar velocity field (left panel) and velocity dispersion σ(right panel). Each of these images is 6.′′2 by 6.′′2, which corresponds to 23 kpc by 23 kpc at the redshift of ASASSN-15lh. North is up and east is to the left.
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