Relation between our catalog’s Hα flux and the detection magnitude (stack of F444W and F210M). The solid, black line represents a Bayesian linear fit, while the shadowed area represents the intrinsic 1σ dispersion around the mean relation. Grey, filled circles are the sources with completeness below 65%, while red circles correspond to galaxies with higher completeness. As can be seen, our catalog of Hα emitters is starting to become incomplete at ∼3 × 10⁻¹⁸ erg s⁻¹ cm⁻², where we are likely missing emitters that are not included in our parent catalog or are not extracted due to our requirements on photo-zs.