\begin{table}%t3 \caption{\label{tab:rat}Line ratios for the total emission and the perturbed and quiescent components with it was possible to decouple them.} \small%\centerline { \begin{tabular}{rrlllllll} \hline\hline Object & Dataset & Ly$\alpha$/HeII & Ly$\alpha$/CIV & Ly$\alpha$/NV & NV/HeII & CIV/HeII & CIV/CIII] & CIII]/HeII \\ \hline 4C 40.36 & V300 & 12.73 $\pm$ 0.23 & 6.97 $\pm$ 0.07 & 18.71 $\pm$ 0.48 & 0.68 $\pm$ 0.03 & 1.83 $\pm$ 0.05 & 1.90 $\pm$ 0.05 & 0.96 $\pm$ 0.03 \\ & V600 & & 6.57 $\pm$ 0.13 & 23.26 $\pm$ 1.45 & & & & \\ \hline & V01$^*$& 14.7 & 8.4 & 39.2 & 0.37 & 1.8 & 1.8 & 1.0 \\ & H05$^{**}$ & 11.6 & 7.1 & 19.3 & 0.6 & 1.6 & 2.2 & 0.7 \\ \hline 4C48.48 & V300 & 9.57 $\pm$ 0.13 & 9.04 $\pm$ 0.12 & $>$17.9 & $<$0.38 & 1.06 $\pm$ 0.03 & 1.05 $\pm$ 0.03 & 1.01 $\pm$ 0.03 \\ \multicolumn{2}{r}{Broader} & & 9.07 $\pm$ 0.15 & & & & & \\ \multicolumn{2}{r}{Narrower} & & 11.36 $\pm$ 0.75 & & & & & \\ 4C48.48 & V600 & & 11.21 $\pm$ 0.21 & $>$65.2 & & & & \\ \multicolumn{2}{r}{Broader} & & 8.33 $\pm$ 0.24 & & & & & \\ \multicolumn{2}{r}{Narrower} & & 16.59 $\pm$ 0.88 & & & & & \\ \hline & V01$^*$& 13.2 & 12.6 & 48.3 & 0.27 & 1.0 & 1.7 & 0.6 \\ & H07$^{**}$ & 11.3 & 8.2 & 12.6 & 0.9 & 1.4 & 2.6 & 0.5 \\ \hline \end{tabular}} \medskip $^{*}$ Vernet et~al. (2001); $^{**}$ Humphrey (\cite{hump07}). \end{table}