The eROSITA Final Equatorial-Depth Survey (eFEDS) - A multiwavelength view of WISE mid-infrared galaxies/active galactic nuclei

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

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Fig. 12

Differences in E(B − V),, the stellar mass (M_*), the SFR, and L_IR derived from X-CIGALE in this work and those derived from the mock catalog. (a) ΔΕ(Β − V),, (b) M_*, (c) SFR, and (d) L_IR as functions of redshift. Right-hand panels: histograms of each quantity. The red dotted lines correspond to Δ = 0.

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