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. Croom & 23 others L. 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

Research output: Contribution to journalArticle

64 Citations (Scopus)

Fingerprint Dive into the research topics of 'Galaxy And Mass Assembly (GAMA): The 0.013 < z < 0.1 cosmic spectral energy distribution from 0.1 μm to 1 mm'. Together they form a unique fingerprint.

Physics & Astronomy

Physics

General

Aerospace Sciences

Chemistry and Materials

Earth & Environmental Sciences