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Table 3:

QSOs without detected DLAs and/or sub-DLAs.

QSO
$z_{\rm em}$ $z_{\rm min}$ $z_{\rm max}$ Note*
PSS0014+3032 4.470 2.866 4.415  
SDSS0210-0018 4.700 3.177 4.643 4, 5
PSS0248+1802 4.430 3.118 4.376 2
PSS0452+0355 4.395 3.115 4.341  
PSS0852+5045 4.216 2.939 4.164  
PSS0926+3055 4.198 2.951 4.146  
SDSS0941+5947 4.820 3.322 4.762 4, 5
PSS1140+6205 4.509 3.113 4.454 4, 5
SDSS1310-0055 4.152 2.830 4.101 4, 5
PSS1339+5154 4.080 2.783 4.029 5
PSS1401+4111 4.026 2.866 3.976 4, 5
PSS1403+4126 3.862 2.866 3.813 4, 5
PSS1418+4449 4.323 2.974 4.270 4, 5
PSS1430+2828 4.306 2.811 4.253 2
PSS1458+6813 4.291 2.990 4.238  
GB1508+5714 4.304 3.217 4.251 2
PSS1543+3417 4.407 3.071 4.353 5
PSS1615+1803 4.010 2.783 3.960  
PSS1721+3256 4.040 2.802 3.990 1, 2
PSS2154+0335 4.359 3.400 4.305 1, 2, 3
PSS2244+1005 4.040 2.810 3.990  

* Quasars from this survey were previously used for $\Omega_{\rm DLA, H_I}$ estimations by: (1) Péroux et al. (2001); (2) Péroux et al. (2003); (3) Péroux et al. (2005); (4) Prochaska et al. (2005); Prochaska & Wolfe (2009).

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