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Fig. C.1.
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Comparison of X-ray luminosities detected with 2RXS, eROSITA, and XMM-Newton in the ROSAT energy band after applying the respective CF shown in Table C.1. For the M10pc sample, we use the CFs from Caramazza et al. (2023). Black bars represent the sensitivity limit of 2RXS at the individual distances of the stars.
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