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Table 2:

Results of the fitting procedure for the peak emission spectra.
Object Grating Line Id. Wavelength Flux FWHM FWHM
    * (Å) ** (Å)*** km s-1
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
  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
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
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
(*) 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.

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