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dc.contributor.authorShvartzvald, Y.
dc.contributor.authorLi, Z.
dc.contributor.authorUdalski, A.
dc.contributor.authorGould, A.
dc.contributor.authorSumi, T.
dc.contributor.authorStreet, R. A.
dc.contributor.authorCalchi Novati, S.
dc.contributor.authorHundertmark, M.
dc.contributor.authorBozza, V.
dc.contributor.authorBeichman, C.
dc.contributor.authorBryden, G.
dc.contributor.authorCarey, S.
dc.contributor.authorDrummond, J.
dc.contributor.authorFausnaugh, M.
dc.contributor.authorGaudi, B. S.
dc.contributor.authorHenderson, C. B.
dc.contributor.authorTan, T. G.
dc.contributor.authorWibking, B.
dc.contributor.authorPogge, R. W.
dc.contributor.authorYee, J. C.
dc.contributor.authorZhu, W.
dc.contributor.authorTsapras, Y.
dc.contributor.authorBachelet, E.
dc.contributor.authorDominik, M.
dc.contributor.authorBramich, D. M.
dc.contributor.authorCassan, A.
dc.contributor.authorFiguera Jaimes, R.
dc.contributor.authorHorne, K.
dc.contributor.authorRanc, C.
dc.contributor.authorSchmidt, R.
dc.contributor.authorSnodgrass, C.
dc.contributor.authorWambsganss, J.
dc.contributor.authorSteele, I. A.
dc.contributor.authorMenzies, J.
dc.contributor.authorMao, S.
dc.contributor.authorPoleski, R.
dc.contributor.authorPawlak, M.
dc.contributor.authorSzymański, M. K.
dc.contributor.authorSkowron, J.
dc.contributor.authorMróz, P.
dc.contributor.authorKozłowski, S.
dc.contributor.authorWyrzykowski, Ł.
dc.contributor.authorPietrukowicz, P.
dc.contributor.authorSoszyński, I.
dc.contributor.authorUlaczyk, K.
dc.contributor.authorAbe, F.
dc.contributor.authorAsakura, Y.
dc.contributor.authorBarry, R. K.
dc.contributor.authorBennett, D. P.
dc.contributor.authorBhattacharya, A.
dc.contributor.authorBond, I. A.
dc.contributor.authorFreeman, M.
dc.contributor.authorHirao, Y.
dc.contributor.authorItow, Y.
dc.contributor.authorKoshimoto, N.
dc.contributor.authorLi, M. C. A.
dc.contributor.authorLing, C. H.
dc.contributor.authorMasuda, K.
dc.contributor.authorFukui, A.
dc.contributor.authorMatsubara, Y.
dc.contributor.authorMuraki, Y.
dc.contributor.authorNagakane, M.
dc.contributor.authorNishioka, T.
dc.contributor.authorOhnishi, K.
dc.contributor.authorOyokawa, H.
dc.contributor.authorRattenbury, N. J.
dc.contributor.authorSaito, To.
dc.contributor.authorSharan, A.
dc.contributor.authorSullivan, D. J.
dc.contributor.authorSuzuki, D.
dc.contributor.authorTristram, P. J.
dc.contributor.authorYonehara, A.
dc.contributor.authorJørgensen, U. G.
dc.contributor.authorBurgdorf, M. J.
dc.contributor.authorCiceri, S.
dc.contributor.authorD’Ago, G.
dc.contributor.authorEvans, D. F.
dc.contributor.authorHinse, T. C.
dc.contributor.authorKains, N.
dc.contributor.authorKerins, E.
dc.contributor.authorKorhonen, H.
dc.contributor.authorMancini, L.
dc.contributor.authorPopovas, A.
dc.contributor.authorRabus, M.
dc.contributor.authorRahvar, S.
dc.contributor.authorScarpetta, G.
dc.contributor.authorSkottfelt, J.
dc.contributor.authorSouthworth, J.
dc.contributor.authorPeixinho, N.
dc.contributor.authorVerma, P.
dc.contributor.authorSbarufatti, B.
dc.contributor.authorKennea, J. A.
dc.contributor.authorGehrels, N.
dc.date.accessioned2016-11-17T12:30:17Z
dc.date.available2016-11-17T12:30:17Z
dc.date.issued2016-11-10
dc.identifier247651003
dc.identifier4b4b2ff8-2a9c-4c80-b60e-45e881947ed6
dc.identifier84994524532
dc.identifier000400474400003
dc.identifier.citationShvartzvald , Y , Li , Z , Udalski , A , Gould , A , Sumi , T , Street , R A , Calchi Novati , S , Hundertmark , M , Bozza , V , Beichman , C , Bryden , G , Carey , S , Drummond , J , Fausnaugh , M , Gaudi , B S , Henderson , C B , Tan , T G , Wibking , B , Pogge , R W , Yee , J C , Zhu , W , Tsapras , Y , Bachelet , E , Dominik , M , Bramich , D M , Cassan , A , Figuera Jaimes , R , Horne , K , Ranc , C , Schmidt , R , Snodgrass , C , Wambsganss , J , Steele , I A , Menzies , J , Mao , S , Poleski , R , Pawlak , M , Szymański , M K , Skowron , J , Mróz , P , Kozłowski , S , Wyrzykowski , Ł , Pietrukowicz , P , Soszyński , I , Ulaczyk , K , Abe , F , Asakura , Y , Barry , R K , Bennett , D P , Bhattacharya , A , Bond , I A , Freeman , M , Hirao , Y , Itow , Y , Koshimoto , N , Li , M C A , Ling , C H , Masuda , K , Fukui , A , Matsubara , Y , Muraki , Y , Nagakane , M , Nishioka , T , Ohnishi , K , Oyokawa , H , Rattenbury , N J , Saito , T , Sharan , A , Sullivan , D J , Suzuki , D , Tristram , P J , Yonehara , A , Jørgensen , U G , Burgdorf , M J , Ciceri , S , D’Ago , G , Evans , D F , Hinse , T C , Kains , N , Kerins , E , Korhonen , H , Mancini , L , Popovas , A , Rabus , M , Rahvar , S , Scarpetta , G , Skottfelt , J , Southworth , J , Peixinho , N , Verma , P , Sbarufatti , B , Kennea , J A & Gehrels , N 2016 , ' The first simultaneous microlensing observations by two space telescopes : Spitzer and Swift reveal a brown dwarf in event OGLE-2015-BLG-1319 ' , Astrophysical Journal , vol. 831 , no. 2 , 183 . https://doi.org/10.3847/0004-637X/831/2/183en
dc.identifier.issn0004-637X
dc.identifier.otherBibCode: 2016ApJ...831..183S
dc.identifier.otherORCID: /0000-0002-3202-0343/work/75996790
dc.identifier.urihttps://hdl.handle.net/10023/9834
dc.description.abstractSimultaneous observations of microlensing events from multiple locations allow for the breaking of degeneracies between the physical properties of the lensing system, specifically by exploring different regions ofthe lens plane and by directly measuring the “microlens parallax.” We report the discovery of a 30–65M J brown dwarf orbiting a K dwarf in the microlensing event OGLE-2015-BLG-1319. The system is located at a distance of ∼5 kpc toward the Galactic Bulge. The event was observed by several ground-based groups as well as by Spitzer and Swift, allowing a measurement of the physical properties. However, the event is still subject to an eight-fold degeneracy, in particular the well-known close-wide degeneracy, and thus the projected separation between the two lens components is either ∼0.25 au or ∼45 au. This is the first microlensing event observed by Swift, with the UVOT camera. We study the region of microlensing parameter space to which Swift is sensitive,finding that though Swift could not measure the microlens parallax with respect to ground-based observations for this event, it can be important for other events. Specifically, it is important for detecting nearby brown dwarfs and free-floating planets in high magnification events.
dc.format.extent1161587
dc.language.isoeng
dc.relation.ispartofAstrophysical Journalen
dc.subjectBinaries: generalen
dc.subjectBrown dwarfsen
dc.subjectGalaxy: bulgeen
dc.subjectGravitational lensing: microen
dc.subjectQB Astronomyen
dc.subjectQC Physicsen
dc.subjectNDASen
dc.subject.lccQBen
dc.subject.lccQCen
dc.titleThe first simultaneous microlensing observations by two space telescopes : Spitzer and Swift reveal a brown dwarf in event OGLE-2015-BLG-1319en
dc.typeJournal articleen
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.doi10.3847/0004-637X/831/2/183
dc.description.statusPeer revieweden
dc.identifier.urlhttp://adsabs.harvard.edu/abs/2016ApJ...831..183Sen


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