| Issue |
A&A
Volume 545, September 2012
|
|
|---|---|---|
| Article Number | A64 | |
| Number of page(s) | 18 | |
| Section | Extragalactic astronomy | |
| DOI | https://doi.org/10.1051/0004-6361/201218884 | |
| Published online | 10 September 2012 | |
Online material
 |
Fig. A.1
Voigt-profile fit of absorption lines observed at epoch II. The fit decomposition was derived from the highest S/N spectrum (obtained at epoch IV). |
| Open with DEXTER | |
 |
Fig. A.2
Voigt-profile fit of absorption lines observed at epoch I. The fit decomposition was derived from the best S/N spectrum (obtained at epoch IV). For the most poorly resolved lines, e.g., Fe iiiλ1122, we conservatively adopt upper limits, see Table 4. |
| Open with DEXTER | |
Intervening systems: identified absorption lines.
Intervening system at z = 1.6711: column densities of Al ii and Al iii.
 |
Fig. A.3
Voigt-profile fit of Al ii and Al iii – associated with an intervening system – and the host-galaxy O i, observed at epoch IV, assuming the best-fitting log N(O i,“b”) = 13.50 value. The Al iiλ1670 line at z = 1.6711 is blended with O iλ1302 at the GRB host-galaxy redshift. The O i line estimate is discussed in Sect. 3.2.3. |
| Open with DEXTER | |
© ESO, 2012
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