Oxford University Press (OUP), Monthly Notices of the Royal Astronomical Society, 3(436), p. 2435-2453
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We use galaxies from the Herschel-ATLAS (H-ATLAS) survey, and a suite of ancillary simulations based on an isothermal dust model, to study our ability to determine the effective dust temperature, luminosity and emissivity index of 250 mu m selected galaxies in the local Universe (z