DR1 (v1.0):
*) True stellar masses now more similar to observed stellar masses due to addition of IRX-UV data at high redshifts.  This also means that A_UV values at z>4 are more consistent with observations.
*) Less scatter in the SM--HM relationship, due to change in SFR correlation time parameter.
*) Quenched fractions now more sensible at z=0 due to the use of H-alpha derived quenced fractions instead of the Moustakas values at z=0.  This also resulted in lower star formation rates for massive halos at z>0.
*) Changes to orphan model mean that satellite fractions (and galaxy stellar mass functions) are now more consistent for simulations of different resolutions.
*) See code changelog for more specific parameter/data changes.

EDR (v0.99):
*) Initial release.