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 2300−2800 Å region, which contains strong MgII and FeII absorption features.
Current usage metrics show cumulative count of Article Views (full-text article views including HTML views, PDF and ePub downloads, according to the available data) and Abstracts Views on Vision4Press platform.
Data correspond to usage on the plateform after 2015. The current usage metrics is available 48-96 hours after online publication and is updated daily on week days.
Initial download of the metrics may take a while.