  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 SFR* from the
Schechter fit to SFR function exhibits consistent, and substantial, linear
growth as a function of redshift from ~5 M_sun/yr at z~8, 650 Myr after the Big
Bang, to ~100 M_sun/yr at z~2, ~2.5 Gyr later. Recent results at z~10, close to
the onset of galaxy formation, are consistent with this trend. The uniformity
of this evolution is even greater than seen in the UV LF over the redshift
range z~2-8, providing validation for our dust corrections. These results
provide strong evidence that galaxies build up uniformly over the first 3 Gyr
of cosmic time.
