Retrieved Lyα redshift of the candidates as compared to the miniJPAS photometric redshifts (Hernán-Caballero et al. 2021). We show spectroscopically confirmed LAEs (green filled circles) and contaminants (red empty circles), objects with extended morphology (morph_star_prob < 0.1; blue empty squares), and sources without any spectral or morphology identification (gray crosses). The dashed lines mark the confusion between Lyα and typical galactic emission lines.