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dc.contributor.authorDavies, L. J. M.
dc.contributor.authorDriver, S. P.
dc.contributor.authorRobotham, A. S. G.
dc.contributor.authorGrootes, M. W.
dc.contributor.authorPopescu, C. C.
dc.contributor.authorTuffs, R. J.
dc.contributor.authorHopkins, A.
dc.contributor.authorAlpaslan, M.
dc.contributor.authorAndrews, S. K.
dc.contributor.authorBland-Hawthorn, J.
dc.contributor.authorBremer, M. N.
dc.contributor.authorBrough, S.
dc.contributor.authorBrown, M. J. I.
dc.contributor.authorCluver, M. E.
dc.contributor.authorCroom, S.
dc.contributor.authorda Cunha, E.
dc.contributor.authorDunne, L.
dc.contributor.authorLara-López, M. A.
dc.contributor.authorLiske, J.
dc.contributor.authorLoveday, J.
dc.contributor.authorMoffett, A. J.
dc.contributor.authorOwers, M.
dc.contributor.authorPhillipps, S.
dc.contributor.authorSansom, A. E.
dc.contributor.authorTaylor, E. N.
dc.contributor.authorMichalowski, M. J.
dc.contributor.authorIbar, E.
dc.contributor.authorSmith, M.
dc.contributor.authorBourne, N.
dc.identifier.citationDavies , L J M , Driver , S P , Robotham , A S G , Grootes , M W , Popescu , C C , Tuffs , R J , Hopkins , A , Alpaslan , M , Andrews , S K , Bland-Hawthorn , J , Bremer , M N , Brough , S , Brown , M J I , Cluver , M E , Croom , S , da Cunha , E , Dunne , L , Lara-López , M A , Liske , J , Loveday , J , Moffett , A J , Owers , M , Phillipps , S , Sansom , A E , Taylor , E N , Michalowski , M J , Ibar , E , Smith , M & Bourne , N 2016 , ' GAMA/H-ATLAS: a meta-analysis of SFR indicators – comprehensive measures of the SFR– M * relation and cosmic star formation history at z < 0.4 ' , Monthly Notices of the Royal Astronomical Society , vol. 461 , no. 1 , pp. 458-485 .
dc.identifier.otherPURE: 246756250
dc.identifier.otherPURE UUID: 40d862ae-3d26-4f40-90be-c104b2a4b160
dc.identifier.otherRIS: urn:D70500D875D38D330E1460BE0A942FA7
dc.identifier.otherScopus: 84988825976
dc.identifier.otherWOS: 000383272500037
dc.description.abstractWe present a meta-analysis of star formation rate (SFR) indicators in the Galaxy And Mass Assembly (GAMA) survey, producing 12 different SFR metrics and determining the SFR–M* relation for each. We compare and contrast published methods to extract the SFR from each indicator, using a well-defined local sample of morphologically selected spiral galaxies, which excludes sources which potentially have large recent changes to their SFR. The different methods are found to yield SFR–M* relations with inconsistent slopes and normalizations, suggesting differences between calibration methods. The recovered SFR–M* relations also have a large range in scatter which, as SFRs of the targets may be considered constant over the different time-scales, suggests differences in the accuracy by which methods correct for attenuation in individual targets. We then recalibrate all SFR indicators to provide new, robust and consistent luminosity-to-SFR calibrations, finding that the most consistent slopes and normalizations of the SFR–M* relations are obtained when recalibrated using the radiation transfer method of Popescu et al. These new calibrations can be used to directly compare SFRs across different observations, epochs and galaxy populations. We then apply our calibrations to the GAMA II equatorial data set and explore the evolution of star formation in the local Universe. We determine the evolution of the normalization to the SFR–M* relation from 0 < z < 0.35 – finding consistent trends with previous estimates at 0.3 < z < 1.2. We then provide the definitive z < 0.35 cosmic star formation history, SFR–M* relation and its evolution over the last 3 billion years.
dc.relation.ispartofMonthly Notices of the Royal Astronomical Societyen
dc.rights© 2016 The Authors Published by Oxford University Press on behalf of the Royal Astronomical Society. This work is made available online in accordance with the publisher’s policies. This is the final published version of the work, which was originally published at:
dc.subjectGalaxies: evolutionen
dc.subjectGalaxies: star formationen
dc.subjectQB Astronomyen
dc.subjectQC Physicsen
dc.titleGAMA/H-ATLAS: a meta-analysis of SFR indicators – comprehensive measures of the SFR–M* relation and cosmic star formation history at z < 0.4en
dc.typeJournal articleen
dc.description.versionPublisher PDFen
dc.contributor.institutionUniversity of St Andrews.School of Physics and Astronomyen
dc.description.statusPeer revieweden

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