Fig. 2.
Integrated central MUSE aperture spectra within a diameter of 3′′ for HE 0227–0913 and HE 0351+0240. The total spectrum (black lines) is decomposed into a point-like QSO and extended host-galaxy contribution using the nonparametric QSO-host galaxy decomposition algorithm implemented in QDeblend3D (Husemann et al. 2013, 2014).
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