All Tables

Table 1: Number of stars, light curves and age of the open clusters used in the present analysis.
Table 2: Correlation coefficients (r), number of stars used to define the upper envelope (N), parameters of the linear, exponential and power law weighted fits to the data upper envelope of $A_{\max}-P$ and $A_{\max}-R_{\rm 0}$ relations and reduced chi-squares ( $\chi ^2_{\rm\nu }$ ).
Table 3: Correlation coefficients (r), number of stars used to define the upper envelope (N), parameters of the linear, exponential and power law weighted fits to the upper data envelope of the $L_{\rm X}$ / $L_{\rm bol}$ -P and $L_{\rm X}$ / $L_{\rm bol}$ - $R_{\rm0}$ relations and reduced chi-squares ( $\chi ^2_{\rm\nu }$ ).
Table 4: Coefficients of correlation (r), number of stars used in the fit (N), parameters (a and b) of the linear, exponential and power law weighted fits to the lower envelope of the $L_{\rm X}$ / $L_{\rm bol}$ - $A_{{\rm max}}$ distribution in the fast rotation regime ( $P \ge 1.1$ d) and reduced chi-squares ( $\chi ^2_{\rm\nu }$ ).