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tokens: ACKNOWLEDGEMENTS GAMA is a joint European-Australasian project based around a spectroscopic campaign using the AngloAustralian Telescope. The GAMA input catalogue is based on the data taken from the Sloan Digital Sky Survey and the UKIRT Infrared Deep Sky Survey. Complementary imaging of the GAMA regions is being obtained by a number of independent survey programs including GALEX MIS, VST KiDS, VISTA VIKING, WISE, Herschel -ATLAS, GMRT, and ASKAP providing UV to radio coverage. The VISTA VIKING data used in this paper are based on observations made with ESO Telescopes at the La Silla Paranal Observatory under programme ID 179.A-2004. GAMA is funded by the STFC (UK), the ARC (Australia), the AAO, and the participating institutions. The GAMA website is http://www.gama-survey.org/ . This work made the extensive use of topcat Taylor ( 2005 ) and stilts Taylor ( 2006 ) software packages, which are supported by an STFC grant to the University of Bristol.