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Work: How robustly can we constrain the low-mass end of the <i>z</i> ∼ 6−7 stellar mass function? The limits of lensing models and stellar population assumptions in the <i>Hubble Frontier Fields</i>
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Work: How robustly can we constrain the low-mass end of the <i>z</i> ∼ 6−7 stellar mass function? The limits of lensing models and stellar population assumptions in the <i>Hubble Frontier Fields</i>