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Push it to the limit: Local Group constraints on high-redshift stellar mass functions for M ⋆ ≥ 10 5 M ⊙
Abstract
We constrain the evolution of the galaxy stellar mass function from 2 2 × 105M⊙ at z = 0). The most recent studies from ZFOURGE and CANDELS also suggest flatter faint end slopes that are consistent with our results, but with a lower degree of precision. This work illustrates the strong connections between low and high-z observations when viewed through the lens of lambda cold dark matter numerical simulations.
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