covered in the spectrum. Fig. \[J021741.8-370100a\] and Fig. \[J021741.8-370100b\] show our best fit of [H]{}[i]{} lines for absorbers at $z_{\rm abs}=2.429$ and $z_{\rm abs}=2.514$ respectively.

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6.  J060008.1-504036 ($z_{\rm em}=3.130$). This quasar was discovered during the course of the Calán Tololo survey [@maza96]. No detailed analysis of this quasar has been published. A Lyman limit system at $z_{\rm LLS}=3.080$ is seen in the spectrum. We identified a DLA at $z_{\rm abs}=2.149$. The column density of the DLA is fitted using three strong components (at 24, 0, and -44 km s$^{-1}$) seen in $\ion{O}{i}$, resulting in a total column density of log $N_{{\rm H}\,{\sc \rm I}}=20.40\pm0.12$ with $b=20$ km s$^{-1}$ fixed for each component. Metal absorption lines from [O]{}[i]{} $\lambda$ 1302, [Fe]{}[ii]{} $\lambda\lambda$ 1608, 1611, [Si]{}[ii]{} $\lambda\lambda\lambda\lambda$ 1260, 1304, 1526, 1808, [C]{}[ii]{} $\lambda$ 1334, [Al]{}[ii]{} $\lambda$ 1670, and [Al]{}[iii]{} $\lambda\lambda$ 1854, 1862 at the redshift of the DLA are covered in the red part of the spectrum. Fig. \[J060008.1-504036\] shows our best fit of the neutral hydrogen column density of the DLA at $z_{\rm abs}=2.149$.

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7.  QSO B0952-0115 ($z_{\rm em}=4.426$). One damped absorber was previously reported in this quasar at $z_{\rm abs}=4.024$ [@storrie00; @prochaska07]. A Lyman limit 