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Push it to the limit: Local group constraints on high-redshift stellar mass functions for M* ≥ 105M⊙

  • Author(s): Graus, AS
  • Bullock, JS
  • Boylan-Kolchin, M
  • Weisz, DR
  • et al.

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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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