Evolution Of Cosmic Star Formation In The Scuba-2 Cosmology Legacy Survey

This dataset consists of tabulated data from the figures included in the referenced publication. The following datasets are included: Stacked SFR obscuration (IRX=IR/UV) of UVJ-selected star-forming galaxies: Weighted mean IRX as a function of Muv & stellar mass (Figure 12): MUV_irx1.dat Weighted mean IRX as a function of beta, over all masses and redshifts: beta_irx.dat Weighted mean IRX as a function of beta, binned by stellar mass (Figure 13): beta_irx_mstar.dat Weighted mean IRX as a function of beta, binned by redshift (Figure 14): beta_irx_z.dat Cosmic SFR density as a function of redshift for massive galaxies log(Ms/Msol)>10 (Figure 15): All mass-selected galaxies: sfrd_massive.dat UV-luminous galaxies Muv<M*; log(Ms/Msol)>10: sfrd_hiLUV.dat IR-luminous galaxies detected at 450µm: sfrd_IRdet.dat Cosmic SFR density as a function of redshift corrected to all stellar masses (Figure 16): All mass-selected galaxies: sfrd_uvlfcorr.dat UV-luminous galaxies Muv<M*; log(Ms/Msol)>10: sfrd_hiLUV_uvlfcorr.dat Full details of the binning and stacking methodology are explained in the paper.