Fig. 9
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Comparison of soft X-ray fluxes in the 0.2–2keV band for exoplanet host stars detected by more than one X-ray mission to fluxes detected by eRASSl. Stars detected by both eRASSl and eRASS2 are shown in red. Some individual outliers are marked by name; these objects are expected to display strong variability in X-rays.
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