\begin{table}%t2
\caption{\label{tab:rms}The correlation of the  {rms} fluctuation of the continuum intensity with our resulting correlations. Generally, the correlations are higher for parameters of the lower forming line (index~1) indicating a larger seeing influence.}
%\centering
\par
\begin{tabular}{lr|lr}
\hline\hline
$\left\langle {\rm rms},\left\langle I,r_{1}\right\rangle\right\rangle$ & $-0.54$ & $\left\langle {\rm rms},\left\langle I,v_{2}\right\rangle\right\rangle$ & $-0.02$ \\
$\left\langle {\rm rms},\left\langle r_{1},r_{2}\right\rangle\right\rangle$ & 0.02 & $\left\langle {\rm rms},\left\langle r_{1},v_{2}\right\rangle\right\rangle$ & 0.05 \\
$\left\langle {\rm rms},\left\langle I,r_{2}\right\rangle\right\rangle$ & $-0.22$ & $\left\langle {\rm rms},\left\langle r_{2},v_{2}\right\rangle\right\rangle$ & $-0.21$ \\
$\left\langle {\rm rms},\left\langle v_{1},v_{2}\right\rangle\right\rangle$ & $-0.27$ & & \\
\hline
\end{tabular}
\end{table}