Table 1: Emission-line measurements of X-ray selected QSO2s at z > 1.2.

Object
Redshift Ly $\alpha\lambda$1216a N V$\lambda $1240a C IV$\lambda $1549a He II$\lambda $1640a C III]$\lambda $1909a

CDFS-027
3.064 12.6 $\pm$ 0.7 2.5 $\pm$ 0.7 6.4 $\pm$ 0.5 2.3 $\pm$ 0.9 <2.9c
CDFS-031 1.603 -- -- 24.1 $\pm$ 1.4 13.3 $\pm$ 1.2 10.3 $\pm$ 1.3
CDFS-057 2.562 112.2 $\pm$ 1.3 8.4 $\pm$ 1.4 17.8 $\pm$ 0.8 7.6 $\pm$ 0.8 13.3 $\pm$ 0.9
CDFS-112a 2.940 58.3 $\pm$ 0.5 14.6 $\pm$ 0.8 15.2 $\pm$ 1.0 8.9 $\pm$ 0.9 4.5 $\pm$ 0.8
CDFS-153 1.536 -- -- 25.5 $\pm$ 1.4 6.2 $\pm$ 1.1 13.7 $\pm$ 1.6
CDFS-202 3.700 78.1 $\pm$ 1.0 26.8 $\pm$ 1.1 38.9 $\pm$ 1.2 19.7 $\pm$ 1.5 <12.9c
CDFS-263b 3.660 70.9 $\pm$ 0.7 4.6 $\pm$ 0.7 15.5 $\pm$ 0.8 <4.0c <7.6c
CDFS-531 1.544 -- -- 22.0 $\pm$ 1.4 17.4 $\pm$ 1.5 14.4 $\pm$ 1.5
CDFS-901 2.578 37.1 $\pm$ 0.6 6.5 $\pm$ 0.8 19.7 $\pm$ 1.0 <2.8c 3.3 $\pm$ 0.9
CXO 52b 3.288 189 $\pm$ 4 6 $\pm$ 1.2d 35 $\pm$ 2 17 $\pm$ 2 21 $\pm$ 2
a
Fluxes are in units of 10-18 erg s-1 cm-2.
b
Data taken from Stern et al. (2002).
c
3$\sigma$ upper-limit flux.
d
The error was assigned by us; see text.


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