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Fig. 11


Histograms showing the redshift distribution of the 831 emission line selected galaxies from the first year of MUSE-Wide observations. Redshifts with confidence values 3, 2, and 1 are shown in dark grey, grey, and light grey, respectively. Left panel: redshift distribution for the rest-frame optical emission line selected galaxies. Horizontal bars indicate the redshift range of the MUSE wavelength coverage for the strongest emission lines of star-forming galaxies. The bin size is Δz = 0.1. Right panel: redshift distribution for the 238 high-z galaxies. The bin size is Δz = 0.2.

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