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Galaxy and Mass Assembly (GAMA): ugriz galaxy luminosity functions

2011; Oxford University Press; Volume: 420; Issue: 2 Linguagem: Inglês

10.1111/j.1365-2966.2011.20111.x

1365-2966

J. Loveday, P. Norberg, I. K. Baldry, Simon P. Driver, Andrew Hopkins, J. A. Peacock, S. P. Bamford, J. Liske, Joss Bland‐Hawthorn, Sarah Brough, M. J. I. Brown, Ewan Cameron, Christopher J. Conselice, S. M. Croom, Carlos S. Frenk, M. L. P. Gunawardhana, David T. Hill, D. H. Jones, L. S. Kelvin, Konrad Kuijken, R. C. Nichol, H. R. Parkinson, S. Phillipps, Kevin A. Pimbblet, C. C. Popescu, M. Prescott, A. S. G. Robotham, R. Sharp, William J. Sutherland, Edward N. Taylor, D. Thomas, R. J. Tuffs, E. van Kampen, D. Wijesinghe,

Gamma-ray bursts and supernovae

Galaxy and Mass Assembly (GAMA) is a project to study galaxy formation and evolution, combining imaging data from ultraviolet to radio with spectroscopic data from the AAOmega spectrograph on the Anglo-Australian Telescope. Using data from Phase 1 of GAMA, taken over three observing seasons, and correcting for various minor sources of incompleteness, we calculate galaxy luminosity functions (LFs) and their evolution in the ugriz passbands.