2017MNRAS.465..672M

We present the results of a new study of the K-band galaxy luminosity function (KLF) at redshifts z <= 3.75, based on a nested combination of the UltraVISTA, Cosmic Assembly Near-infrared Deep Legacy Extragalactic Survey and HUDF surveys. The large dynamic range in luminosity spanned by this new data set (3-4 dex over the full redshift range) is sufficient to clearly demonstrate for the first time that the faint-end slope of the KLF at z >= 0.25 is relatively steep (-1.3 <= α <= -1.5 for a single Schechter function), in good agreement with recent theoretical and phenomenological models. Moreover, based on our new data set, we find that a double Schechter function provides a significantly improved description of the KLF at z <= 2. At redshifts z >= 0.25, the evolution of the KLF is remarkably smooth, with little or no evolution evident at faint (M_K >= -20.5) or bright magnitudes (M_K <= -24.5). Instead, the KLF is seen to evolve rapidly at intermediate magnitudes, with the number density of galaxies at M_K ≃-23 dropping by a factor of ≃5 over the redshift interval 0.25 <= z <= 3.75. Motivated by this, we explore a simple description of the evolving KLF based on a double Schechter function with fixed faint-end slopes (α₁ = -0.5, α₂ = -1.5) and a shared characteristic magnitude (M_K^*^). According to this parametrization, the normalization of the component which dominates the faint end of the KLF remains approximately constant, with φ^*^₂ decreasing by only a factor of ≃2 between z ≃0 and 3.25. In contrast, the component which dominates the bright end of the KLF at low redshifts evolves dramatically, becoming essentially negligible by z ≃3. Finally, we note that within this parametrization, the observed evolution of M_K^*^ between z ≃0 and 3.25 is entirely consistent with M_K^*^ corresponding to a constant stellar mass of M_* ≃5 x 10¹⁰ M_☉ at all redshifts.