Fig. 6.
β-slope vs. FUV-magnitudes of our sample. Gray circles indicate the individual measurements for the galaxies with most reliable photometry, and gray crosses for the remaining ones. Blue circles are biweight means in bins of 0.7 mag size. The straight blue line is the linear fit to the biweight mean values. The colored crosses are values from Bouwens et al. (2014) and Castellano et al. (2012) at different redshifts.
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