(a) L(Lyα) as a function of M_*. Our sample is indicated by the same markers, and the filled and open gray diamonds represent the less luminous samples of LAEs at z > 4.5 and z ≤ 4.5 from I24, respectively. The dashed line is the best-fit linear function to the z > 4.5 subsample. (b) Comparing the stellar masses derived from the SED fitting with the inclusion (M_*) and exclusion (M_*,-F410M) of F410M; the horizontal axis represents the sum of two colors, F200W − F277W and F410M − F277W.