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

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Lara-López M (2013) Galaxy And Mass Assembly (GAMA): the connection between metals, specific SFR and H i gas in galaxies: the Z-SSFR relation in Monthly Notices of the Royal Astronomical Society: Letters

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Lara-López M (2013) Galaxy And Mass Assembly (GAMA): a deeper view of the mass, metallicity and SFR relationships in Monthly Notices of the Royal Astronomical Society

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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

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Liske J (2015) Galaxy And Mass Assembly (GAMA): end of survey report and data release 2 in Monthly Notices of the Royal Astronomical Society

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Loveday J (2012) Galaxy and Mass Assembly (GAMA): ugriz galaxy luminosity functions GAMA luminosity functions in Monthly Notices of the Royal Astronomical Society

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Loveday J (2015) Galaxy and Mass Assembly (GAMA): luminosity function evolution in Proceedings of the International Astronomical Union

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Mahajan S (2015) Galaxy And Mass Assembly (GAMA): the unimodal nature of the dwarf galaxy population in Monthly Notices of the Royal Astronomical Society

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McNaught-Roberts T (2014) Galaxy And Mass Assembly (GAMA): the dependence of the galaxy luminosity function on environment, redshift and colour in Monthly Notices of the Royal Astronomical Society

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Oliva-Altamirano P (2014) Galaxy And Mass Assembly (GAMA): testing galaxy formation models through the most massive galaxies in the Universe 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