Fig. 4
Top: evolution of the broad Hα line of Mrk 1018. Aperture spectra (3′′ diameter) from MUSE and three representative VIMOS IFU observations. Matching offset stellar continua model are shown. Bottom: difference spectra with respect to the minimum spectrum in October 2016. A constant stellar continuum is subtracted in each spectrum, but offset in flux to take the varying AGN continuum emission into account.
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