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Table B.1

Equivalent widths measured for the absorption lines of the afterglow.

λ obs Feature Contaminants EW obs EW rest z
Å

4650.4 Fe ii2344.2 Fe ii2345.0 4.3 ± 0.4 2.2 ± 0.2 0.9838

4713.4 Fe ii2374.5 .... .... .... 0.9850
4720.5 .... Fe ii2381.5 8.4 ± 0.6 4.2 ± 0.3 ....
4727.2 Fe ii2382.8 .... .... .... 0.9389

5132.7 Fe ii2586.7 Mn ii2594.5 3.7 ± 0.4 1.9 ± 0.2 0.9843
5157.7 Fe ii2600.2 Mn ii2696.7, Fe ii2586.7 6.3 ± 0.5 3.2 ± 0.2 0.9836

5547.3 Mg ii2796.4 .... .... .... 0.9837
5540.8 .... .... 11.9 ± 0.4 6.0 ± 0.2 ....
5560.1 Mg ii2803.5 .... .... .... 0.9833

5660.2 Mg i2853.0 .... 4.3 ± 0.4 2.2 ± 0.2 0.9840
7806.1 Ca ii3934.8 .... 4.0 ± 0.5 2.0 ± 0.2 0.9839
7877.6 Ca ii3969.6 .... 3.3 ± 0.6 1.7 ± 0.3 0.9845

Notes.Redshift was determined for those lines with no contaminants.

(†)

Blended lines.

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