\begin{table}%t2 \caption{\label{tab:fit_cen}Results of the fitting procedure for the peak emission spectra.} \small%\centerline { \begin{tabular}{lllrrrr} \hline\hline Object & Grating & Line Id. & Wavelength & Flux & {\it FWHM} & {\it FWHM}\\ & & $^*$ & (\AA) & $^{**}$ & (\AA)$^{***}$ & \vel \\ \hline 4C 40.36 & V300 & Ly$\alpha$ & 3961.03 & 45.83 $\pm$ 0.23 & 28.8 & 2179.7 $\pm$ 557.3\\ & & NV & 4043.84 & 2.45 $\pm$ 0.23 & 28.8 & 2135.1 $\pm$ 545.9\\ & & CIV & 5052.75 & 6.58 $\pm$ 0.20 & 35.6 & 2112.2 $\pm$ 540.1\\ & & HeII & 5352.34 & 3.60 $\pm$ 0.20 & 35.6 & 1994.0 $\pm$ 510.0\\ & & CIII]$\lambda$1909 & 6222.77 & 3.46 $\pm$ 0.20 & 16.0 & 770.8 $\pm$ 196.9\\ \hline & V600 & Ly$\alpha$ & 3967.39 & 62.11 $\pm$ 0.85 & 27.0 & 2040.2 $\pm$ 228.3\\ & & NV & 4050.35 & 2.67 $\pm$ 0.85 & 27.0 & 1998.4 $\pm$ 223.6\\ & & CIV & 5056.13 & 9.45 $\pm$ 0.33 & 21.4 & 1268.9 $\pm$ 142.0\\ \hline 4C 48.48 & V300 & Ly$\alpha$ & 4057.26 & 46.66 $\pm$ 0.51 & 14.0 & 1034.5 $\pm$ 274.9\\ & & Ly$\alpha$ $1$ & 4058.39 & 37.47 $\pm$ 0.42 & 18.4 & 1359.2 $\pm$ 361.1\\ & & Ly$\alpha$ $2$ & 4055.83 & 11.36 $\pm$ 0.28 & 3.9 & 288.2 $\pm$ 76.6\\ & & CIV & 5170.31 & 5.16 $\pm$ 0.12 & 15.6 & 904.5 $\pm$ 240.3\\ & & CIV $1$ & 5172.25 & 4.13 $\pm$ 0.11 & 15.0 & 869.4 $\pm$ 231.0\\ & & CIV $2$ & 5165.23 & 1.00 $\pm$ 0.08 & 3.5 & 203.1 $\pm$ 54.0\\ & & HeII & 5474.06 & 4.89 $\pm$ 0.21 & 10.6 & 580.5 $\pm$ 154.2\\ & & CIII]$\lambda$1909 & 6366.45 & 4.92 $\pm$ 0.19 & 17.9 & 842.9 $\pm$ 224.0\\ \hline 4C 48.48 & V600 & Ly$\alpha$ & 4060.72 &104.29 $\pm$ 1.21 & 13.0 & 959.7 $\pm$ 43.2\\ & & Ly$\alpha$ $1$ & 4063.55 & 51.31 $\pm$ 0.99 & 16.0 &1180.4 $\pm$ 53.2\\ & & Ly$\alpha$ $2$ & 4059.41 & 52.60 $\pm$ 0.78 & 9.5 & 701.6 $\pm$ 31.6\\ & & CIV & 5172.39 & 9.30 $\pm$ 0.23 & 16.5 & 956.3 $\pm$ 43.1\\ & & CIV $1$ & 5175.85 & 6.16 $\pm$ 0.21 & 16.5 & 955.7 $\pm$ 43.1\\ & & CIV $2$ & 5168.53 & 3.17 $\pm$ 0.16 & 8.9 & 516.2 $\pm$ 23.3\\ \hline \end{tabular}} \medskip (*) $1$ indicate the broader components and $2$ the narrower one; (**)~10$^{-16}$~erg~s$^{-1}$~cm$^{-2}$~arcsec$^{-2}$; (***)~after removing the instrumental profile width. \end{table}