Galaxy And Mass Assembly (GAMA): The 0.013 < z < 0.1 cosmic spectral energy distribution from 0.1 m to 1 mm
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Driver, Simon
Robotham, A. S. G.
Kelvin, L S
Alpaslan, M
Baldry, I. K.
Bamford, Steven P.
Brough, Sarah
Brown, M
Hopkins, Andrew M.
Liske, Jochen
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Blackwell Publishing Ltd
Abstract
We use the Galaxy And Mass Assembly survey (GAMA) I data set combined with GALEX, Sloan Digital Sky Survey (SDSS) and UKIRT Infrared Deep Sky Survey (UKIDSS) imaging to construct the low-redshift (z < 0.1) galaxy luminosity functions in FUV, NUV, ugriz
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Monthly Notices of the Royal Astronomical Society
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Open Access
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