Fig. 7

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Histogram of sSFR comparing eFEDS-HECATE normal galaxies detected in eROSITA observations (solid black line) with the predictions for eFEDS detections based on SIXTE simulations (dashed red line). The black vertical dashed line shows the sSFR cut adopted to separate early-type and late-type galaxies. eFEDS observations detected almost exclusively late-type galaxies, at odds with SIXTE simulations that predicted an approximately even split within the eFEDS field.
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