Galaxy And Mass Assembly (GAMA): The 0.013 < z < 0.1 cosmic spectral energy distribution from 0.1 m to 1 mm

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dc.contributor.authorDriver, Simon
dc.contributor.authorRobotham, A. S. G.
dc.contributor.authorKelvin, L S
dc.contributor.authorAlpaslan, M
dc.contributor.authorBaldry, I. K.
dc.contributor.authorBamford, Steven P.
dc.contributor.authorBrough, Sarah
dc.contributor.authorBrown, M
dc.contributor.authorHopkins, Andrew M.
dc.contributor.authorLiske, Jochen
dc.contributor.authorColless, Matthew
dc.contributor.authorMadore, Barry
dc.contributor.authorSharp, Robert
dc.contributor.authorTuffs, Richard J
dc.contributor.authorvan Kampen, E
dc.contributor.authorAndrae, Ellen
dc.date.accessioned2015-12-13T22:41:10Z
dc.date.issued2012
dc.date.updated2016-02-24T09:32:42Z
dc.description.abstractWe use the Galaxy And Mass Assembly survey (GAMA) I data set combined with GALEX, Sloan Digital Sky Survey (SDSS) and UKIRT Infrared Deep Sky Survey (UKIDSS) imaging to construct the low-redshift (z < 0.1) galaxy luminosity functions in FUV, NUV, ugriz
dc.identifier.issn0035-8711
dc.identifier.urihttp://hdl.handle.net/1885/78393
dc.publisherBlackwell Publishing Ltd
dc.rightsAuthor/s retain copyrighten_AU
dc.sourceMonthly Notices of the Royal Astronomical Society
dc.subjectKeywords: Fundamental parameters-galaxies; Galaxies; General-galaxies; Luminosity function, mass function-cosmology; Observations-infrared; Surveys-galaxies
dc.titleGalaxy And Mass Assembly (GAMA): The 0.013 < z < 0.1 cosmic spectral energy distribution from 0.1 m to 1 mm
dc.typeJournal article
dcterms.accessRightsOpen Accessen_AU
local.bibliographicCitation.issue4
local.bibliographicCitation.lastpage3264
local.bibliographicCitation.startpage3244
local.contributor.affiliationDriver, Simon, The University of Western Australia
local.contributor.affiliationRobotham, A. S. G., University of Western Australia
local.contributor.affiliationKelvin, L S, University of Western Australia
local.contributor.affiliationAlpaslan, M, University of Western Australia
local.contributor.affiliationBaldry, I. K., Liverpool John Moores University
local.contributor.affiliationBamford, Steven P., University of Nottingham
local.contributor.affiliationBrough, Sarah, Australian Astronomical Observatory
local.contributor.affiliationBrown, M , Monash University
local.contributor.affiliationHopkins, Andrew M., Australian Astronomical Observatory
local.contributor.affiliationLiske, Jochen, European Southern Observatory
local.contributor.affiliationColless, Matthew, College of Physical and Mathematical Sciences, ANU
local.contributor.affiliationMadore, Barry, Observatories of the Carnegie Institution of Washington
local.contributor.affiliationSharp, Robert, College of Physical and Mathematical Sciences, ANU
local.contributor.affiliationTuffs, Richard J, Max Planck Institute for Nuclear Physics
local.contributor.affiliationvan Kampen, E, European Southern Observatory
local.contributor.affiliationAndrae, Ellen, Max Planck Institute for Nuclear Physics
local.contributor.authoremailu9300169@anu.edu.au
local.contributor.authoruidColless, Matthew, u9300169
local.contributor.authoruidSharp, Robert, u4954956
local.description.notesImported from ARIES
local.identifier.absfor020103 - Cosmology and Extragalactic Astronomy
local.identifier.ariespublicationf5625xPUB7050
local.identifier.citationvolume427
local.identifier.doi10.1111/j.1365-2966.2012.22036
local.identifier.scopusID2-s2.0-84875043961
local.identifier.uidSubmittedByf5625
local.type.statusPublished Version

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