Fig. 1.

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Distributions of resolution and S/N in the 1930 spectra before the peak covering the relevant wavelength region with a clean enough signal for the S/N estimation. The bottom panel represents the redshift distribution of the 1557 objects sampled by these spectra. The dotted lines and accompanying values correspond to the medians of the three measurements. Final cuts upon S/N and resolution will be implemented based upon the results of the simulated fits.
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