The Star Formation Rate Function for Redshift z~4-7 Galaxies: Evidence for a Uniform Build-Up of Star-Forming Galaxies During the First 3 Gyr of Cosmic Time
Renske Smit (1), Rychard J. Bouwens (1), Marijn Franx (1), Garth D., Illingworth (2), Ivo Labb\'e (1), Pacal A. Oesch (2), Pieter G. van Dokkum, (3) ((1) Leiden Observatory, Leiden University, (2) UCO/Lick Observatory,, University of California, Santa Cruz

TL;DR
This study derives star formation rate functions for galaxies at redshifts 4 to 7, revealing a consistent, linear growth in galaxy build-up over the first 3 billion years of cosmic history, validated by dust correction methods.
Contribution
It introduces a new method to derive SFR functions from UV LFs and dust corrections, showing a uniform galaxy build-up during early cosmic times.
Findings
SFR functions are well-described by Schechter relations.
The characteristic SFR shows a linear increase from z~8 to z~2.
No significant evolution in the low-end slope of SFR functions.
Abstract
We combine recent estimates of dust extinction at z~4-7 with UV luminosity function (LF) determinations to derive star formation rate (SFR) functions at z~4, 5, 6 and 7. SFR functions provide a more physical description of galaxy build-up at high redshift and allow for direct comparisons to SFRs at lower redshifts determined by a variety of techniques. Our SFR functions are derived from well-established z~4-7 UV LFs, UV-continuum slope trends with redshift and luminosity, and IRX-beta relations. They are well-described by Schechter relations. We extend the comparison baseline for SFR functions to z~2 by considering recent determinations of the H{\alpha} and mid-IR luminosity functions. The low-end slopes of the SFR functions are flatter than for the UV LFs, \Delta\alpha\sim+0.13, and show no clear evolution with cosmic time (z~0-7). In addition, we find that the characteristic value…
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