GAMA Observing 2011
Lead Research Organisation:
University of Sussex
Department Name: Sch of Mathematical & Physical Sciences
Abstract
The main objective is to study structure on scales of 1 Megaparcsec to 1 kiloparsec. This will include galaxy clusters, groups, mergers and coarse measurements of galaxy structure (i.e., bulges and discs). It is on this scale (< 1 Mpc) at which the role of the baryons in the galaxy formation process become critical and where our understanding of structure in the Universe breaks down.
Publications
Kelvin L
(2012)
Galaxy And Mass Assembly (GAMA): Structural Investigation of Galaxies via Model Analysis GAMA: sigma
in Monthly Notices of the Royal Astronomical Society
Rowlands K
(2012)
Herschel?-ATLAS/GAMA: dusty early-type galaxies and passive spirals H-ATLAS/GAMA: dusty ETGs and passive spirals
in Monthly Notices of the Royal Astronomical Society
Bourne N
(2012)
Herschel?-ATLAS/GAMA: a census of dust in optically selected galaxies from stacking at submillimetre wavelengths H-ATLAS/GAMA: dust in optically selected galaxies
in Monthly Notices of the Royal Astronomical Society
Robotham A
(2012)
Galaxy And Mass Assembly (GAMA): in search of Milky Way Magellanic Cloud analogues GAMA: in search of MMAs
in Monthly Notices of the Royal Astronomical Society
{Driver}, S.~P. And {Hill}, D.~T. And {Kelvin}, L.~S. And {Robotham}, A.~S.~G. And {Liske}, J. And {Norberg}, P. And {Baldry}, I.~K. And {Bamford}, S.~P. And {Hopkins}, A.~M. And {Loveday}, J. And {Peacock}, J.~A. And {Andrae}, E. And {Bland-Hawthorn}, J. And {Brough}, S. And {Brown}, M.~J.~I. And {Cameron}, E. And {Ching}, J.~H.~Y. And {Colless}, M. And {Conselice}, C.~J. And {Croom}, S.~M. And {Cross}, N.~J.~G. And {de Propris}, R. And {Dye}, S. And {Drinkwater}, M.~J. And {Ellis}, S. And {Gr
(2012)
Galaxy And Mass Assembly (GAMA) DR1 (Driver+, 2011)
in VizieR Online Data Catalog
Alpaslan M
(2012)
Galaxy And Mass Assembly (GAMA): estimating galaxy group masses via caustic analysis Galaxy group masses via caustic analysis
in Monthly Notices of the Royal Astronomical Society
Driver S
(2013)
Galaxy And Mass Assembly (GAMA): the 0.013 < z < 0.1 cosmic spectral energy distribution from 0.1 m to 1 mm
in Monthly Notices of the Royal Astronomical Society
Brough S
(2013)
Galaxy And Mass Assembly: resolving the role of environment in galaxy evolution
in Monthly Notices of the Royal Astronomical Society
Robotham A
(2013)
Galaxy And Mass Assembly (GAMA): the life and times of L? galaxies
in Monthly Notices of the Royal Astronomical Society
Gunawardhana M
(2013)
Galaxy And Mass Assembly: evolution of the Ha luminosity function and star formation rate density up to z < 0.35
in Monthly Notices of the Royal Astronomical Society
Description | The Galaxy and Mass Assembly (GAMA) survey is compiling spectroscopic and multi-wavelength imaging observations for a representative and highly complete sample of galaxies in the nearby Universe. This survey is being used to understand how galaxies form and evolve, and to constrain the properties of the principal constituents of the Universe. |
Exploitation Route | SAMI followup |
Sectors | Digital/Communication/Information Technologies (including Software),Education |
URL | http://www.gama-survey.org |
Title | GAMA database |
Description | Panchromatic (X-ray - radio) on a representative sample of ~300,000 galaxies. |
Type Of Material | Database/Collection of data |
Year Produced | 2010 |
Provided To Others? | Yes |
Impact | 49 refereed publications as of October 2014 |
URL | http://www.gama-survey.org |
Description | GAMA |
Organisation | International Centre for Radio Astronomy Research (ICRAR) |
Country | Australia |
Sector | Academic/University |
PI Contribution | Member of Scientific and Strategic Advisory Council Spectroscopic flux calibration |
Collaborator Contribution | Project management |
Impact | Numerous publications |
Start Year | 2006 |
Description | Public talk |
Form Of Engagement Activity | A talk or presentation |
Part Of Official Scheme? | No |
Geographic Reach | Regional |
Primary Audience | Public/other audiences |
Results and Impact | Talk to Lewes astronomers, South Downs Astronomical Society, Vectis Astronomical Society, local schools, ... Report on most recent talk (22 Feb 2013) appeared in newsletter of Vectis Astronomical Society |
Year(s) Of Engagement Activity | Pre-2006,2006,2007,2008,2009,2010,2011,2012,2013 |
Description | School visits |
Form Of Engagement Activity | Participation in an open day or visit at my research institution |
Part Of Official Scheme? | Yes |
Geographic Reach | Local |
Primary Audience | Schools |
Results and Impact | Presentation & discussion Regular visits |
Year(s) Of Engagement Activity | 2009,2010,2011,2012,2013,2014 |
URL | http://www.sussex.ac.uk/physics/outreach/schoolslab |