Characterising X-ray variability in light curves with complex sampling patterns: Application to the eROSITA south ecliptic pole survey

Open Access

Fig. 6

Comparison of the NEV_b measurements with the NIV of the light curve that it seeks to estimate, for pink-noise light curves, using Eq. (6), and the values listed in Table 1. The orange dashed line indicates the 1:1 relationship between NEV_b, and the NIV.

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