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

Open Access

Table 1

Best-fitting parameters of $\log (\bar{σ_{b}})$ $\log \left( {\overline {{\sigma _{\rm{b}}}} } \right)$ as a function of log(NIV) using Eq. (6).

Parameter	Value
m_y	−0.1034 ± 0.0047
M_y	−0.1850 ± 0.0021
k_y	−1.410 ± 0.0011
m_a	−0.0296 ± 0.0019
M_a	0.0363 ± 0.0025
k_a	0.0698 ± 0.0055
m_b	−0.1137 ± 0.0066
M_b	0.1474 ± 0.0088
k_b	0.796 ± 0.019
m_c	−0.1036 ± 0.0061
M_c	0.1580 ± 0.0083
k_c	−0.078 ± 0.018

Current usage metrics show cumulative count of Article Views (full-text article views including HTML views, PDF and ePub downloads, according to the available data) and Abstracts Views on Vision4Press platform.

Data correspond to usage on the plateform after 2015. The current usage metrics is available 48-96 hours after online publication and is updated daily on week days.

Initial download of the metrics may take a while.