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The supermassive black hole coincident with the luminous transient ASASSN 15lh

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Academic year: 2020

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Fig. 1. HST WFC3 image in the F606W filter in the main panel. The image spans approximately 60 00 by 60 00 , which is 220 kpc by 220 kpc at the redshift z = 0.232 of ASASSN-15lh and corresponds to the field of view of our MUSE integral field spectroscopy (
Fig. 2. Zoom in on the HST WFC3/F606W image to highlight the ASASSN-15lh host galaxy morphology (left panel, logarithmic  scal-ing) and the transient (right panel, linear scalscal-ing)
Fig. 4. Empirical model of transient plus stellar emission fit to the X-shooter and MUSE spectra for measuring the stellar kinematics in the wavelength range of the strong Ca ii H+K doublet, Hδ, Hγ, and the G band
Fig. 6. Physical model of transient plus multiple stellar populations fitted to the nuclear spectra (radius of 0
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