Fig. 1.
Effective area versus depth for different NIR surveys available in the H-band (∼5σ), both in blank fields (UltraVISTA, CANDELS, HUDF and XDF) and lensing clusters (CLASH and Hubble Frontier Fields). The appropriate correction was applied to CLASH and Hubble Frontier Fields to account for lensing effects on the effective area beyond the limiting magnitude, assuming z ∼ 7 for the source plane.
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