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dc.contributor.authorNegrello, M.
dc.contributor.authorHopwood, R.
dc.contributor.authorDye, S.
dc.contributor.authorda Cunha, E.
dc.contributor.authorSerjeant, S.
dc.contributor.authorFritz, J.
dc.contributor.authorRowlands, K.
dc.contributor.authorFleuren, S.
dc.contributor.authorBussmann, R. S.
dc.contributor.authorCooray, A.
dc.contributor.authorDannerbauer, H.
dc.contributor.authorGonzalez-Nuevo, J.
dc.contributor.authorLapi, A.
dc.contributor.authorOmont, A.
dc.contributor.authorAmber, S.
dc.contributor.authorAuld, R.
dc.contributor.authorBaes, M.
dc.contributor.authorButtiglione, S.
dc.contributor.authorCava, A.
dc.contributor.authorDanese, L.
dc.contributor.authorDariush, A.
dc.contributor.authorDe Zotti, G.
dc.contributor.authorDunne, L.
dc.contributor.authorEales, S.
dc.contributor.authorIbar, E.
dc.contributor.authorIvison, R. J.
dc.contributor.authorKim, S.
dc.contributor.authorLeeuw, L.
dc.contributor.authorMaddox, S.
dc.contributor.authorMichalowski, M. J.
dc.contributor.authorMassardi, M.
dc.contributor.authorPascale, E.
dc.contributor.authorPohlen, M.
dc.contributor.authorRigby, E.
dc.contributor.authorSmith, D. J. B.
dc.contributor.authorSutherland, W.
dc.contributor.authorTemi, P.
dc.contributor.authorWardlow, J.
dc.date.accessioned2014-09-09T09:01:07Z
dc.date.available2014-09-09T09:01:07Z
dc.date.issued2014-05-21
dc.identifier.citationNegrello , M , Hopwood , R , Dye , S , da Cunha , E , Serjeant , S , Fritz , J , Rowlands , K , Fleuren , S , Bussmann , R S , Cooray , A , Dannerbauer , H , Gonzalez-Nuevo , J , Lapi , A , Omont , A , Amber , S , Auld , R , Baes , M , Buttiglione , S , Cava , A , Danese , L , Dariush , A , De Zotti , G , Dunne , L , Eales , S , Ibar , E , Ivison , R J , Kim , S , Leeuw , L , Maddox , S , Michalowski , M J , Massardi , M , Pascale , E , Pohlen , M , Rigby , E , Smith , D J B , Sutherland , W , Temi , P & Wardlow , J 2014 , ' Herschel-ATLAS : deep HST/WFC3 imaging of strongly lensed submillimetre galaxies ' , Monthly Notices of the Royal Astronomical Society , vol. 440 , no. 3 , pp. 1999-2012 . https://doi.org/10.1093/mnras/stu413en
dc.identifier.issn0035-8711
dc.identifier.otherPURE: 135026832
dc.identifier.otherPURE UUID: 123afc61-7754-4363-9a59-daadea609ff5
dc.identifier.otherWOS: 000334744000009
dc.identifier.otherScopus: 84898792324
dc.identifier.otherWOS: 000334744000009
dc.identifier.urihttp://hdl.handle.net/10023/5381
dc.descriptionThis work is supported by STFC (grants PP/D002400/1 and ST/G002533/1)en
dc.description.abstractWe report on deep near-infrared observations obtained with the Wide Field Camera-3 (WFC3) onboard the Hubble Space Telescope (HST) of the first five confirmed gravitational lensing events discovered by the Herschel Astrophysical Terahertz Large Area Survey (H-ATLAS). We succeed in disentangling the background galaxy from the lens to gain separate photometry of the two components. The HST data allow us to significantly improve on previous constraints of the mass in stars of the lensed galaxy and to perform accurate lens modelling of these systems, as described in the accompanying paper by Dye et al. We fit the spectral energy distributions of the background sources from near-IR to millimetre wavelengths and use the magnification factors estimated by Dye et al. to derive the intrinsic properties of the lensed galaxies. We find these galaxies to have star-formations rates (SFR) ∼ 400–2000 M⊙ yr−1, with ∼(6–25) × 1010 M⊙ of their baryonic mass already turned into stars. At these rates of star formation, all remaining molecular gas will be exhausted in less than ∼100 Myr, reaching a final mass in stars of a few 1011 M⊙. These galaxies are thus proto-ellipticals caught during their major episode of star formation, and observed at the peak epoch (z ∼ 1.5–3) of the cosmic star formation history of the Universe.
dc.format.extent14
dc.language.isoeng
dc.relation.ispartofMonthly Notices of the Royal Astronomical Societyen
dc.rights© 2014 The Authors Published by Oxford University Press on behalf of the Royal Astronomical Societyen
dc.subjectGravitational lensing: strongen
dc.subjectGalaxies: elliptical and lenticular, cDen
dc.subjectGalaxies: evolutionen
dc.subjectGalaxies: formationen
dc.subjectInfrared: galaxiesen
dc.subjectSubmillimetre: galaxiesen
dc.subjectScience demonstration phaseen
dc.subjectExtragalactic surveyen
dc.subjectLuminosity functionsen
dc.subjectInfrared-emissionen
dc.subjectHigh-redshiften
dc.subjectSimple-modelen
dc.subjectBlack-holesen
dc.subjectDusten
dc.subjectEvolutionen
dc.subjectStellaren
dc.subjectQB Astronomyen
dc.subjectQC Physicsen
dc.subject.lccQBen
dc.subject.lccQCen
dc.titleHerschel-ATLAS : deep HST/WFC3 imaging of strongly lensed submillimetre galaxiesen
dc.typeJournal articleen
dc.description.versionPublisher PDFen
dc.contributor.institutionUniversity of St Andrews.School of Physics and Astronomyen
dc.identifier.doihttps://doi.org/10.1093/mnras/stu413
dc.description.statusPeer revieweden


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