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. 11

Polygon containing valid stellar sources with PARSEC evolutionary tracks. The 2D histogram in the background shows a typical Gaia source population; most sources are close to the 100+ Myrs main sequence.

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