A direct calibration of the IRX–β relation in Lyman-break Galaxies at z = 3–5

@article{Koprowski2018ADC,
  title={A direct calibration of the IRX–$\beta$ relation in Lyman-break Galaxies at z = 3–5},
  author={Maciej Koprowski and K. E. K. Coppin and James E. Geach and Ross J. McLure and Omar Almaini and A. W. Blain and Malcolm N. Bremer and N Bourne and Sandra C. Chapman and C. J. Conselice and James S. Dunlop and Duncan Farrah and William G. Hartley and Alexander Karim and Kirsten K. Knudsen and Michał Jerzy Michałowski and Douglas Scott and Chris Simpson and D. J. B. Smith and P van der Werf},
  journal={Monthly Notices of the Royal Astronomical Society},
  year={2018}
}
We use a sample of 4209 Lyman-break galaxies (LBGs) at z~ -3, 4, and 5 in the UKIRT Infrared Deep Sky Survey Ultra Deep Survey field to investigate the relationship between the observed slope of the stellar continuum emission in the ultraviolet, β , and the thermal dust emission, as quantified via the so-called ‘infrared excess’ (IRX≡LIR/LUV). Through a stacking analysis, we directly measure the 850-μm flux density of LBGs in our deep (0.9 mJy) James Clerk Maxwell Telescope SCUBA-2850-μm map as… 
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