Galaxy and Mass Assembly (GAMA): ugriz galaxy luminosity functions
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. At low redshift, z < 0.1, we find that blue galaxies,...[Show more]
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|Source:||Monthly Notices of the Royal Astronomical Society|
|01_Loveday_Galaxy_and_Mass_Assembly_2012.pdf||2.18 MB||Adobe PDF||Request a copy|
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