Table 3: Lines detected above 3$\sigma $ in the spectrum of GRB 011211.

$\lambda_{\rm obs}$

 $W_{\rm obs}$ (Å) ID $z_{\rm abs}$
3820.0 16.6 $\pm$ 2.1 Ly$\alpha $ $\lambda $1215 2.1423
3957.0 4.7 $\pm$ 1.1 Si  II $\lambda $1260 2.1394
  blended  with S  II $\lambda $1259  
4096.9 4.6 $\pm$ 0.7 Si  II $\lambda $1304 2.1409
  blended  with O  I $\lambda $1302  
4195.6 5.6 $\pm$ 0.8 C  II $\lambda $1334 2.1439
  blended  with C  II* $\lambda $1335  
4381.7 2.9 $\pm$ 0.6 Si  IV $\lambda $1393 2.1438
4405.9 2.0 $\pm$ 0.6 Si  IV $\lambda $1402 2.1409
4797.8 3.6 $\pm$ 0.5 Si  II $\lambda $1526 2.1426
4863.4 2.2 $\pm$ 0.4 C  IV $\lambda $1548 2.1413
4870.9 3.7 $\pm$ 0.5 C  IV $\lambda $1550 2.1410
5053.7 1.7 $\pm$ 0.5 Fe  II $\lambda $1608 2.1420
5251.7 3.5 $\pm$ 0.5 Al  II $\lambda $1670 2.1432
5828.3 1.7 $\pm$ 0.4 Al  III $\lambda $1854 2.1424
6114.2 1.3 $\pm$ 0.4    
7362.8 3.1 $\pm$ 1.0 Fe  II $\lambda $2344 2.1408
7485.5 6.5 $\pm$ 0.8 Fe  II $\lambda $2382 2.1415
8131.4 3.8 $\pm$ 1.0 Fe  II $\lambda $2586 2.1436
8171.4 3.5 $\pm$ 1.0 Fe  II $\lambda $2600 2.1426


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