GAMA: towards a physical understanding of galaxy formation
astro-ph.CO
/ Authors
Simon P. Driver, Peder Norberg, Ivan K. Baldry, Steven P. Bamford, Andrew M. Hopkins, Jochen Liske, Jon Loveday, John A. Peacock, David T. Hill, Lee S. Kelvin
and 39 more authors
Aaron S. G. Robotham, Nick J. Cross, Hannah R. Parkinson, Matt Prescott, Chris J. Conselice, Loretta Dunne, Sarah Brough, Heath Jones, Rob G. Sharp, Eelco van Kampen, Seb Oliver, Isaac G. Roseboom, Joss Bland-Hawthorn, Scott M. Croom, Simon Ellis, Ewan Cameron, Shaun Cole, Carlos S. Frenk, Warrick J. Couch, Alister W. Graham, Rob Proctor, Roberto De Propris,
/ Abstract
The Galaxy And Mass Assembly (GAMA) project is the latest in a tradition of large galaxy redshift surveys, and is now underway on the 3.9m Anglo-Australian Telescope at Siding Spring Observatory. GAMA is designed to map extragalactic structures on scales of 1kpc - 1Mpc in complete detail to a redshift of z~0.2, and to trace the distribution of luminous galaxies out to z~0.5. The principal science aim is to test the standard hierarchical structure formation paradigm of Cold Dark Matter (CDM) on scales of galaxy groups, pairs, discs, bulges and bars. We will measure (1) the Dark Matter Halo Mass Function (as inferred from galaxy group velocity dispersions); (2) baryonic processes, such as star formation and galaxy formation efficiency (as derived from Galaxy Stellar Mass Functions); and (3) the evolution of galaxy merger rates (via galaxy close pairs and galaxy asymmetries). Additionally, GAMA will form the central part of a new galaxy database, which aims to contain 275,000 galaxies with multi-wavelength coverage from coordinated observations with the latest international ground- and space-based facilities: GALEX, VST, VISTA, WISE, HERSCHEL, GMRT and ASKAP. Together, these data will provide increased depth (over 2 magnitudes), doubled spatial resolution (0.7"), and significantly extended wavelength coverage (UV through Far-IR to radio) over the main SDSS spectroscopic survey for five regions, each of around 50 deg^2. This database will permit detailed investigations of the structural, chemical, and dynamical properties of all galaxy types, across all environments, and over a 5 billion year timeline.