. Several metal absorption lines from [O]{}[i]{} $\lambda$ 0000, [Fe]{}[ii]{} $\lambda\lambda\lambda\lambda\lambda\lambda$ 0000, 0000, 0000, 0000, 0000, 0000, [Si]{}[ii]{} $\lambda\lambda\lambda\lambda\lambda$ 0000, 0000, 0000, 0000, 0000, [C]{}[ii]{} $\lambda$ 0000, [Al]{}[ii]{} $\lambda$ 0000, [Mg]{}[ii]{} $\lambda\lambda$ 0000, 0000, [Al]{}[iii]{} $\lambda\lambda$ 0000, 0000, [Si]{}[iv]{} $\lambda\lambda$ 0000, 0000, and [C]{}[iv]{} $\lambda\lambda$ 0000, 0000 associated with sub-DLA are covered in the red part of the spectrum. Fig. \[J000000.0-000000\] shows our best fit 