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

Open Access

Table 3

Best-fitting parameters describing the intrinsic scatter of the NIV, as a function of N_seg and NIV_∞, if the segments are adjoined.

Parameter	Value
m	0.1782 ± 0.0027
k	0.0824 ± 0.0063

Notes. They relate to Eq. (14). These parameter values can be used alongside those listed in Table 2 to determine the intrinsic scatter, when combing Eqs. (10) and (14).

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