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dc.contributor.authorGiannini, E.
dc.contributor.authorSchmidt, R. W.
dc.contributor.authorWambsganss, J.
dc.contributor.authorAlsubai, K.
dc.contributor.authorAndersen, J. M.
dc.contributor.authorAnguita, T.
dc.contributor.authorBozza, V.
dc.contributor.authorBramich, D. M.
dc.contributor.authorBrowne, P.
dc.contributor.authorCalchi Novati, S.
dc.contributor.authorDamerdji, Y.
dc.contributor.authorDiehl, C.
dc.contributor.authorDodds, P.
dc.contributor.authorDominik, M.
dc.contributor.authorElyiv, A.
dc.contributor.authorFang, X.
dc.contributor.authorFiguera Jaimes, R.
dc.contributor.authorFinet, F.
dc.contributor.authorGerner, T.
dc.contributor.authorGu, S.
dc.contributor.authorHardis, S.
dc.contributor.authorHarpsøe, K.
dc.contributor.authorHinse, T. C.
dc.contributor.authorHornstrup, A.
dc.contributor.authorHundertmark, M.
dc.contributor.authorJessen-Hansen, J.
dc.contributor.authorJørgensen, U. G.
dc.contributor.authorJuncher, D.
dc.contributor.authorKains, N.
dc.contributor.authorKerins, E.
dc.contributor.authorKorhonen, H.
dc.contributor.authorLiebig, C.
dc.contributor.authorLund, M. N.
dc.contributor.authorLundkvist, M. S.
dc.contributor.authorMaier, G.
dc.contributor.authorMancini, L.
dc.contributor.authorMasi, G.
dc.contributor.authorMathiasen, M.
dc.contributor.authorPenny, M.
dc.contributor.authorProft, S.
dc.contributor.authorRabus, M.
dc.contributor.authorRahvar, S.
dc.contributor.authorRicci, D.
dc.contributor.authorScarpetta, G.
dc.contributor.authorSahu, K.
dc.contributor.authorSchäfer, S.
dc.contributor.authorSchönebeck, F.
dc.contributor.authorSkottfelt, J.
dc.contributor.authorSnodgrass, C.
dc.contributor.authorSouthworth, J.
dc.contributor.authorSurdej, J.
dc.contributor.authorTregloan-Reed, J.
dc.contributor.authorVilela, C.
dc.contributor.authorWertz, O.
dc.contributor.authorZimmer, F.
dc.date.accessioned2017-01-23T12:30:11Z
dc.date.available2017-01-23T12:30:11Z
dc.date.issued2017-01
dc.identifier.citationGiannini , E , Schmidt , R W , Wambsganss , J , Alsubai , K , Andersen , J M , Anguita , T , Bozza , V , Bramich , D M , Browne , P , Calchi Novati , S , Damerdji , Y , Diehl , C , Dodds , P , Dominik , M , Elyiv , A , Fang , X , Figuera Jaimes , R , Finet , F , Gerner , T , Gu , S , Hardis , S , Harpsøe , K , Hinse , T C , Hornstrup , A , Hundertmark , M , Jessen-Hansen , J , Jørgensen , U G , Juncher , D , Kains , N , Kerins , E , Korhonen , H , Liebig , C , Lund , M N , Lundkvist , M S , Maier , G , Mancini , L , Masi , G , Mathiasen , M , Penny , M , Proft , S , Rabus , M , Rahvar , S , Ricci , D , Scarpetta , G , Sahu , K , Schäfer , S , Schönebeck , F , Skottfelt , J , Snodgrass , C , Southworth , J , Surdej , J , Tregloan-Reed , J , Vilela , C , Wertz , O & Zimmer , F 2017 , ' MiNDSTEp differential photometry of the gravitationally lensed quasars WFI 2033-4723 and HE 0047-1756 : microlensing and a new time delay ' , Astronomy & Astrophysics , vol. 597 , A49 . https://doi.org/10.1051/0004-6361/201527422en
dc.identifier.issn0004-6361
dc.identifier.otherPURE: 248984508
dc.identifier.otherPURE UUID: 3e8e589d-3616-4fc7-8612-fa05713fe16d
dc.identifier.otherBibCode: 2017A&A...597A..49G
dc.identifier.otherScopus: 85007348650
dc.identifier.otherWOS: 000392392900016
dc.identifier.otherORCID: /0000-0002-3202-0343/work/75996702
dc.identifier.urihttps://hdl.handle.net/10023/10157
dc.descriptionMAS. M.D. and M.H. are supported by NPRP grant NPRP-09-476-1-78 from the Qatar National Research Fund (a member of Qatar Foundation).en
dc.description.abstractAims: We present V and R photometry of the gravitationally lensed quasars WFI 2033-4723 and HE 0047-1756. The data were taken by the MiNDSTEp collaboration with the 1.54 m Danish telescope at the ESO La Silla observatory from 2008 to 2012. Methods: Differential photometry has been carried out using the image subtraction method as implemented in the HOTPAnTS package, additionally using GALFIT for quasar photometry. Results: The quasar WFI 2033-4723 showed brightness variations of order 0.5 mag in V and R during the campaign.The two lensed components of quasar HE 0047-1756 varied by 0.2-0.3 mag within five years. We provide, for the first time, an estimate of the time delay of component B with respect to A of Δt = (7.6±1.8) days for this object. We also find evidence for a secular evolution of the magnitude difference between components A and B in both filters,which we explain as due to a long-duration microlensing event. Finally we find that both quasars WFI 2033-4723 and HE 0047-1756 become bluer when brighter, which is consistent with previous studies.
dc.format.extent16
dc.language.isoeng
dc.relation.ispartofAstronomy & Astrophysicsen
dc.rights© ESO 2016. 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: https://dx.doi.org/10.1051/0004-6361/201527422en
dc.subjectGravitational lensing: microen
dc.subjectTechniques: photometricen
dc.subjectQuasars: generalen
dc.subjectQB Astronomyen
dc.subjectQC Physicsen
dc.subjectNDASen
dc.subject.lccQBen
dc.subject.lccQCen
dc.titleMiNDSTEp differential photometry of the gravitationally lensed quasars WFI 2033-4723 and HE 0047-1756 : microlensing and a new time delayen
dc.typeJournal articleen
dc.description.versionPublisher PDFen
dc.contributor.institutionUniversity of St Andrews. School of Physics and Astronomyen
dc.contributor.institutionUniversity of St Andrews. St Andrews Centre for Exoplanet Scienceen
dc.identifier.doihttps://doi.org/10.1051/0004-6361/201527422
dc.description.statusPeer revieweden
dc.identifier.urlhttp://adsabs.harvard.edu/abs/2017A%26A...597A..49Gen
dc.identifier.urlhttps://arxiv.org/abs/1610.03732en


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