Galaxy And Mass Assembly (GAMA): The 0.013 < z < 0.1 cosmic spectral energy distribution from 0.1 μm to 1 mm

S. P. Driver*, A. S G Robotham, L. Kelvin, M. Alpaslan, I. K. Baldry, S. P. Bamford, S. Brough, M. Brown, A. M. Hopkins, J. Liske, J. Loveday, P. Norberg, J. A. Peacock, E. Andrae, J. Bland-Hawthorn, N. Bourne, E. Cameron, M. Colless, C. J. Conselice, S. M. CroomL. Dunne, C. S. Frenk, Alister W. Graham, M. Gunawardhana, D. T. Hill, D. H. Jones, K. Kuijken, B. Madore, R. C. Nichol, H. R. Parkinson, K. A. Pimbblet, S. Phillipps, C. C. Popescu, M. Prescott, M. Seibert, R. G. Sharp, W. J. Sutherland, E. N. Taylor, D. Thomas, R. J. Tuffs, E. van Kampen, D. Wijesinghe, S. Wilkins

*Corresponding author for this work

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