The high-energy environment of the heavy sub-Earth GJ 367 b indicates likely complete evaporation of its atmosphere

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Fig. 1

Combined X-ray image from the first four eRASS surveys around the position of GJ 367, indicated by the circle, in the soft eROSITA X-ray band (0.2–2.3 keV). GJ 367 displays a clear excess in X-ray photons compared to the ambient background.

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