0.0$ km s$^{-0}$. Several metal absorption lines from [Fe]{}[ii]{} $\lambda\lambda\lambda\lambda\lambda$ 0000, 0000, 0000, 0000, 0000, [Si]{}[ii]{} $\lambda\lambda\lambda\lambda$ 0000, 0000, 0000, 0000 [C]{}[ii]{} $\lambda$ 0000, [Al]{}[ii]{} $\lambda$ 0000, [Al]{}[iii]{} $\lambda\lambda$ 0000, 0000, and [Si]{}[iv]{} $\lambda\lambda$ 0000, 0000 associated with the DLA are covered in the red part of the spectrum. Fig. \[B0000-0000\] shows our best fit 