Galaxy And Mass Assembly (GAMA): A study of energy, mass, and structure
  (1kpc-1Mpc) at z < 0.3
  The GAMA survey has now completed its spectroscopic campaign of over 250,000
galaxies ($r<19.8$mag), and will shortly complete the assimilation of the
complementary panchromatic imaging data from GALEX, VST, VISTA, WISE, and
Herschel. In the coming years the GAMA fields will be observed by the
Australian Square Kilometer Array Pathfinder allowing a complete study of the
stellar, 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 being
pursued both as an empirical study in its own right, as well as providing a
benchmark resource against which the outputs from numerical simulations can be
compared. GAMA has three particularly compelling aspects which set it apart:
completeness, selection, and panchromatic coverage. The very high redshift
completeness ($\sim 98$\%) allows for extremely complete and robust pair and
group catalogues; the simple selection ($r<19.8$mag) minimises the selection
bias and simplifies its management; and the panchromatic coverage, 0.2$\mu$m -
1m, enables studies of the complete energy distributions for individual
galaxies, well defined sub-samples, and population assembles (either directly
or via stacking techniques). For further details and data releases see:
http://www.gama-survey.org/
