Fig. 18.
Total stellar XUV (< 100 nm) emission integrated between 1 and 1000 Myr (upper-left) and between 1000 and 5000 Myr (upper-right) and XUV fluence (time integrated XUV flux) in the habitable zone between 1 and 1000 Myr (lower-left) and between 1000 and 5000 Myr (lower-right) as functions of stellar mass for the slow, medium, and fast rotator cases. The background circles show the values for each star in our model distribution.
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