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Fig. 30


Composite probability distribution of M1500 and M for REF and DEC+NEB(+Lyα) models at z ~ 5 and z ~ 6. The dashed black line represents the MM1500 trend found by González et al. (2011) and dotted black lines show a scatter of ±0.5 dex. The points overlaid show the median value properties for each object in the sample: black dots for “weak” nebular emitters, and white dots for “strong” nebular emitters. The overlaid contour indicates the 68% integrated probabilities on the ensemble properties measured from the centroid of the distribution. Red dots are median values of M in MUV bins.

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