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Fig. 11.

image

Redshift distribution of galaxies selected to have a positive excess in the J0660 filter associated to line emission. Top, middle, and bottom panels: results employing different magnitude thresholds, Δm >  0.2, Δm >  0.4, and Δm >  0.4, plus the 3σ significance level with respect to the J-PLUS typical uncertainties. The blue histograms show galaxies selected using the 3FM of Vilella-Rojo et al. (2015), whereas the red dashed histograms show galaxies selected using the true magnitude excess associated with a line emission.

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