Fig. 5.
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Number fractions of galaxies in our OFG sample that are identified as LBGs (blue shaded region), H-dropouts (red shaded region), and the remaining OFGs (orange filled region) that are missed by the first two selection techniques. The OFGs undetected by the LBGs and H-dropouts criteria represent approximately 75% at stellar masses between log(M⋆/M⊙) = 9.5 − 10.5.
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