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
Loveday J
(2012)
Galaxy and Mass Assembly (GAMA): ugriz galaxy luminosity functions GAMA luminosity functions
in Monthly Notices of the Royal Astronomical Society
Kelvin L
(2014)
Galaxy And Mass Assembly (GAMA): ugrizYJHK Sersic luminosity functions and the cosmic spectral energy distribution by Hubble type
in Monthly Notices of the Royal Astronomical Society
Owers M
(2013)
GALAXY AND MASS ASSEMBLY (GAMA): WITNESSING THE ASSEMBLY OF THE CLUSTER ABELL 1882
in The Astrophysical Journal
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
Hill D
(2010)
Galaxy and Mass Assembly: FUV, NUV, ugrizYJHK Petrosian, Kron and Sérsic photometry GAMA: the photometric pipeline
in Monthly Notices of the Royal Astronomical Society
{Vazquez-Mata}, J.~A. And {Loveday}, J.
(2011)
Galaxy And Mass Assembly: Galaxy LF on host group properties
Simpson F
(2016)
Galaxy and mass assembly: Redshift space distortions from the clipped galaxy field
in Physical Review D
Brough S
(2013)
Galaxy And Mass Assembly: resolving the role of environment in galaxy evolution
in Monthly Notices of the Royal Astronomical Society
Lindsay S
(2014)
Galaxy and Mass Assembly: the evolution of bias in the radio source population to z~1.5
in Monthly Notices of the Royal Astronomical Society
{Loveday}, J.
(2011)
Galaxy luminosity function: dependence on halo mass
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 |