Fig. 5

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Two bright Lyman-break galaxy candidates: their photometry, best-fit templates and uniquely high-z ℒ(z) from eazy-py, cutouts, and lightcurves. The false colour image is composed of YE, JE, and HE and the cutouts are scaled linearly such that they saturate at ±3σ. Upper limits for IE are shown by the leftmost grey bar with an arrow, while selection limits for NISP bands are shown by the grey bars.
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