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Fig. 2

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Measured X-ray hardness ratio HR12 of GJ 367 (red solid line, with red dotted lines indicating 1σ uncertainties) compared to the same hardness ratio for simulated X-ray spectra of different coronal temperatures (black dots and dashed line). GJ 367’s hardness ratio implies a mean coronal temperature in the 0.13–0.19 keV range, i.e. about 1.5–2.2 million K.

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