Fig. 6


Comparison between the MUSE (red) and FORS1 spectra of Rigopoulou et al. (2005; blue) for the galaxy ID#13, a strong [O ii] emitter at zMUSE = 1.2902. The strongest spectral features are indicated in black. The grey lines show the position of the sky lines. Upper panel: entire spectra; lower panel: zoom on the rest-frame 23002800 Å region, which contains strong MgII and FeII absorption features.

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