The eROSITA Final Equatorial-Depth Survey (eFEDS) - The Stellar Counterparts of eROSITA sources identified by machine learning and Bayesian algorithms

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

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Fig. 5

Distribution of the Bayes factor B^p as a function of the activity F_X/F_G and the color BP-RP for the eFEDS counterparts. The ranges of the spectral types are indicated at the bottom of the figure.

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