Galaxy and mass assembly (GAMA): the GAMA galaxy group catalogue (G(3)Cv1)

Aaron S. G. Robotham, Peder Norberg, Simon P. Driver, Ivan K. Baldry, Steven P. Bamford, Andrew M. Hopkins, Jochen Liske, Jon Loveday, A. Merson, John A. Peacock, Sarah Brough, Ewan Cameron, Christopher J. Conselice, Scott M. Croom, Carlos S. Frenk, M. L. P. Gunawardhana, David T. Hill, David Heath Jones, Lee S. Kelvin, Konrad KuijkenRobert C. Nichol, Hannah R. Parkinson, Kevin A. Pimbblet, Steven Phillipps, Cristina C. Popescu, Matthew Prescott, Robert G. Sharp, Will J. Sutherland, Edward N. Taylor, Daniel Thomas, Richard J. Tuffs, Eelco Van Kampen, D. B. Wijesinghe

Research output: Contribution to journalArticlepeer-review


Using the complete Galaxy and Mass Assembly I (GAMA-I) survey covering ∼142 deg2 to rAB= 19.4, of which ∼47 deg2 is to rAB= 19.8, we create the GAMA-I galaxy group catalogue (G3Cv1), generated using a friends-of-friends (FoF) based grouping algorithm. Our algorithm has been tested extensively on one family of mock GAMA lightcones, constructed from Λ cold dark matter N-body simulations populated with semi-analytic galaxies. Recovered group properties are robust to the effects of interlopers and are median unbiased in the most important respects. G3Cv1 contains 14 388 galaxy groups (with multiplicity ≥2), including 44 186 galaxies out of a possible 110 192 galaxies, implying ∼40 per cent of all galaxies are assigned to a group. The similarities of the mock group catalogues and G3Cv1 are multiple: global characteristics are in general well recovered. However, we do find a noticeable deficit in the number of high multiplicity groups in GAMA compared to the mocks. Additionally, despite exceptionally good local spatial completeness, G3Cv1 contains significantly fewer compact groups with five or more members, this effect becoming most evident for high multiplicity systems. These two differences are most likely due to limitations in the physics included of the current GAMA lightcone mock. Further studies using a variety of galaxy formation models are required to confirm their exact origin. The G3Cv1 catalogue will be made publicly available as and when the relevant GAMA redshifts are made available at
Original languageEnglish
Pages (from-to)2640-2668
JournalMonthly Notices of the Royal Astronomical Society
Issue number4
Early online date1 Oct 2011
Publication statusPublished - 2011


  • galaxies: groups: general
  • galaxies: haloes
  • dark matter
  • large-scale structure of Universe


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