Fig. 15.
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Number counts for galaxies without continuum detection, without a WHITE_ID. The bottom (top) panel shows the distributions for low (high) redshift galaxies with 0.3 < z < 1.5 (2.8 < z < 6) respectively. Both panels show that there is a significant popultion of galaxies detected solely on their emission line with FELINE. The solid line represents the GAMMA/DEVILS survey (Koushan et al. 2021).
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