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dc.contributor.authorKettlety, Ten_US
dc.contributor.authorHesling, Jen_US
dc.contributor.authorPhillipps, Sen_US
dc.contributor.authorBremer, MNen_US
dc.contributor.authorCluver, MEen_US
dc.contributor.authorTaylor, ENen_US
dc.contributor.authorBland-Hawthorn, Jen_US
dc.contributor.authorBrough, Sen_US
dc.contributor.authorDe Propris, Ren_US
dc.contributor.authorDriver, SPen_US
dc.contributor.authorHolwerda, BWen_US
dc.contributor.authorKelvin, LSen_US
dc.contributor.authorSutherland, Wen_US
dc.contributor.authorWright, AHen_US
dc.date.accessioned2017-12-14T15:17:18Z
dc.date.available2017-09-11en_US
dc.date.issued2018en_US
dc.date.submitted2017-12-07T10:31:18.854Z
dc.identifier.issn0035-8711en_US
dc.identifier.urihttp://qmro.qmul.ac.uk/xmlui/handle/123456789/30363
dc.format.extent776 - 783en_US
dc.relation.ispartofMONTHLY NOTICES OF THE ROYAL ASTRONOMICAL SOCIETYen_US
dc.subjectgalaxies: evolutionen_US
dc.subjectgalaxies: fundamental parametersen_US
dc.subjectgalaxies: photometryen_US
dc.subjectgalaxies: stellar contenten_US
dc.subjectinfrared: galaxiesen_US
dc.titleGalaxy and mass assembly (GAMA): the consistency of GAMA and <i>WISE</i> derived mass-to-light ratiosen_US
dc.typeArticle
dc.rights.holder© 2017 The Authors Published by Oxford University Press on behalf of the Royal Astronomical Society
dc.identifier.doi10.1093/mnras/stx2379en_US
pubs.author-urlhttps://www.webofscience.com/api/gateway?GWVersion=2&SrcApp=PARTNER_APP&SrcAuth=LinksAMR&KeyUT=WOS:000415653600061&DestLinkType=FullRecord&DestApp=ALL_WOS&UsrCustomerID=612ae0d773dcbdba3046f6df545e9f6aen_US
pubs.issue1en_US
pubs.notesNo embargoen_US
pubs.publication-statusPublisheden_US
pubs.volume473en_US


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