Data
Please contact me for data from any of my publications. Selected results are listed below.
Herschel-ATLAS/GAMA: a census of dust in optically selected galaxies from stacking at submillimetre wavelengths (Bourne et al. 2012)
| Stacked sub-millimetre fluxes, luminosities, and derived dust masses and temperatures for GAMA galaxies: | ADS link | |
| as a function of stellar mass, optical colour and redshift | FITS table | README |
| as a function of r-band absolute magnitude, optical colour and redshift | FITS table | README |
Figure 15b, MNRAS 421, 3027
Figure 16, MNRAS 421, 3027
Evolution of cosmic star formation in the SCUBA-2 Cosmology Legacy Survey (Bourne et al. 2017)
IRX(β,M) and IRX(Muv,M)
| Average obscuration IR/UV of UVJ-selected star-forming galaxies: | ADS link |
| weighted mean IRX as a function of Muv & stellar mass (Figure 12) | ascii table |
| IRX-β relation for UVJ-selected star-forming galaxies: | |
| weighted means over all masses and redshifts | ascii table |
| binned by stellar mass (Figure 13) | ascii table |
| binned by redshift (Figure 14) | ascii table |
SFRD(z)
| Cosmic SFR density as a function of redshift for massive galaxies log(Ms/Msol)>10 (Figure 15): | ADS link |
| all mass-selected galaxies | ascii table |
| UV-luminous galaxies Muv<M*; log(Ms/Msol)>10 | ascii table |
| IR-luminous galaxies detected at 450µm | ascii table | Cosmic SFR density as a function of redshift corrected to all stellar masses (Figure 16): |
| all mass-selected galaxies | ascii table |
| UV-luminous galaxies Muv<M* | ascii table |
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