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The GAMA survey has now completed its spectroscopic campaign of over 250,000galaxies ($r<19.8$mag), and will shortly complete the assimilation of thecomplementary panchromatic imaging data from GALEX, VST, VISTA, WISE, andHerschel. In the coming years the GAMA fields will be observed by theAustralian Square Kilometer Array Pathfinder allowing a complete study of thestellar, dust, and gas mass constituents of galaxies within the low-z Universe($z<0.3$). The science directive is to study the distribution of mass, energy,and structure on kpc-Mpc scales over a 3billion year timeline. This is beingpursued both as an empirical study in its own right, as well as providing abenchmark resource against which the outputs from numerical simulations can becompared. GAMA has three particularly compelling aspects which set it apart:completeness, selection, and panchromatic coverage. The very high redshiftcompleteness ($\sim 98$\%) allows for extremely complete and robust pair andgroup catalogues; the simple selection ($r<19.8$mag) minimises the selectionbias and simplifies its management; and the panchromatic coverage, 0.2$\mu$m -1m, enables studies of the complete energy distributions for individualgalaxies, well defined sub-samples, and population assembles (either directlyor via stacking techniques). For further details and data releases see:http://www.gama-survey.org/

Galaxy And Mass Assembly (GAMA): A study of energy, mass, and structure (1kpc-1Mpc) at z < 0.3