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Ish: 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>

1. <i>Euclid</i> preparation

   L. Zalesky, J.R. Weaver, J. R. Weaver +112

   PreprintAstronomy and Astrophysical ResearchAstronomy and Astrophysics20260 iqtibos

   ABIABI:AkademIndex/openalex/2026.preprint.000009