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Fig. 12

image

4″ × 4″ cutouts in UltraVISTA DR2 Y and J, NB118 14 and 15, and HST/ACS/F814W for two Hα emitters with significant throughput differences between filters 14 and 15. Both objects have spectroscopic redshifts from zCOSMOS (Lilly et al. 2009) and are included in Table 4. For each object, the four UltraVISTA panels are scaled to the same surface brightness in fν.

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