The eROSITA Final Equatorial-Depth Survey (eFEDS) - The first archetypal quasar in the feedback phase discovered by eROSITA

The Early Data Release of eROSITA and Mikhail Pavlinsky ART-XC on the SRG mission

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Fig. A.1

Best-fit SED from X-ray to FIR of eFEDS J091157.4+014327 obtained using X-CIGALE. The black points are all the photometric data, and the solid grey line represents the best-fit SED. The inset shows the SED at 0.1–500 μm where the contributions from the stellar, nebular, AGN, and SF components to the total SED are shown as labelled.

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