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Pathway to the Galactic distribution of planets : combined Spitzer and ground-based microlens parallax measurements of 21 single-lens events

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dc.contributor.authorCalchi Novati, S.
dc.contributor.authorGould, A.
dc.contributor.authorUdalski, A.
dc.contributor.authorMenzies, J. W.
dc.contributor.authorBond, I. A.
dc.contributor.authorShvartzvald, Y.
dc.contributor.authorStreet, R. A.
dc.contributor.authorHundertmark, M.
dc.contributor.authorBeichman, C. A.
dc.contributor.authorYee, J. C.
dc.contributor.authorCarey, S.
dc.contributor.authorPoleski, R.
dc.contributor.authorSkowron, J.
dc.contributor.authorKozłowski, S.
dc.contributor.authorMróz, P.
dc.contributor.authorPietrukowicz, P.
dc.contributor.authorPietrzyński, G.
dc.contributor.authorSzymański, M. K.
dc.contributor.authorSoszyński, I.
dc.contributor.authorUlaczyk, K.
dc.contributor.authorWyrzykowski, Ł.
dc.contributor.authorAlbrow, M.
dc.contributor.authorBeaulieu, J. P.
dc.contributor.authorCaldwell, J. A. R.
dc.contributor.authorCassan, A.
dc.contributor.authorCoutures, C.
dc.contributor.authorDanielski, C.
dc.contributor.authorDominis Prester, D.
dc.contributor.authorDonatowicz, J.
dc.contributor.authorLončarić, K.
dc.contributor.authorMcDougall, A.
dc.contributor.authorMorales, J. C.
dc.contributor.authorRanc, C.
dc.contributor.authorZhu, W.
dc.contributor.authorAbe, F.
dc.contributor.authorBarry, R. K.
dc.contributor.authorBennett, D. P.
dc.contributor.authorBhattacharya, A.
dc.contributor.authorFukunaga, D.
dc.contributor.authorInayama, K.
dc.contributor.authorKoshimoto, N.
dc.contributor.authorNamba, S.
dc.contributor.authorSumi, T.
dc.contributor.authorSuzuki, D.
dc.contributor.authorTristram, P. J.
dc.contributor.authorWakiyama, Y.
dc.contributor.authorYonehara, A.
dc.contributor.authorMaoz, D.
dc.contributor.authorKaspi, S.
dc.contributor.authorFriedmann, M.
dc.contributor.authorBachelet, E.
dc.contributor.authorFiguera Jaimes, R.
dc.contributor.authorBramich, D. M.
dc.contributor.authorTsapras, Y.
dc.contributor.authorHorne, K.
dc.contributor.authorSnodgrass, C.
dc.contributor.authorWambsganss, J.
dc.contributor.authorSteele, I. A.
dc.contributor.authorKains, N.
dc.contributor.authorBozza, V.
dc.contributor.authorDominik, M.
dc.contributor.authorJørgensen, U. G.
dc.contributor.authorAlsubai, K. A.
dc.contributor.authorCiceri, S.
dc.contributor.authorD’Ago, G.
dc.contributor.authorHaugbølle, T.
dc.contributor.authorHessman, F. V.
dc.contributor.authorHinse, T. C.
dc.contributor.authorJuncher, D.
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.authorSchmidt, R. W.
dc.contributor.authorSkottfelt, J.
dc.contributor.authorSouthworth, J.
dc.contributor.authorStarkey, David
dc.contributor.authorSurdej, J.
dc.contributor.authorWertz, O.
dc.contributor.authorZarucki, M.
dc.contributor.authorGaudi, B. S.
dc.contributor.authorPogge, R. W.
dc.contributor.authorDePoy, D. L.
dc.date.accessioned2015-06-08T11:10:06Z
dc.date.available2015-06-08T11:10:06Z
dc.date.issued2015-05-01
dc.identifier.citationCalchi Novati , S , Gould , A , Udalski , A , Menzies , J W , Bond , I A , Shvartzvald , Y , Street , R A , Hundertmark , M , Beichman , C A , Yee , J C , Carey , S , Poleski , R , Skowron , J , Kozłowski , S , Mróz , P , Pietrukowicz , P , Pietrzyński , G , Szymański , M K , Soszyński , I , Ulaczyk , K , Wyrzykowski , Ł , Albrow , M , Beaulieu , J P , Caldwell , J A R , Cassan , A , Coutures , C , Danielski , C , Dominis Prester , D , Donatowicz , J , Lončarić , K , McDougall , A , Morales , J C , Ranc , C , Zhu , W , Abe , F , Barry , R K , Bennett , D P , Bhattacharya , A , Fukunaga , D , Inayama , K , Koshimoto , N , Namba , S , Sumi , T , Suzuki , D , Tristram , P J , Wakiyama , Y , Yonehara , A , Maoz , D , Kaspi , S , Friedmann , M , Bachelet , E , Figuera Jaimes , R , Bramich , D M , Tsapras , Y , Horne , K , Snodgrass , C , Wambsganss , J , Steele , I A , Kains , N , Bozza , V , Dominik , M , Jørgensen , U G , Alsubai , K A , Ciceri , S , D’Ago , G , Haugbølle , T , Hessman , F V , Hinse , T C , Juncher , D , Korhonen , H , Mancini , L , Popovas , A , Rabus , M , Rahvar , S , Scarpetta , G , Schmidt , R W , Skottfelt , J , Southworth , J , Starkey , D , Surdej , J , Wertz , O , Zarucki , M , Gaudi , B S , Pogge , R W & DePoy , D L 2015 , ' Pathway to the Galactic distribution of planets : combined Spitzer and ground-based microlens parallax measurements of 21 single-lens events ' , Astrophysical Journal , vol. 804 , no. 1 . https://doi.org/10.1088/0004-637X/804/1/20en
dc.identifier.issn0004-637X
dc.identifier.otherPURE: 192933669
dc.identifier.otherPURE UUID: fda2df11-9e39-4dab-88a0-b63110f3bcad
dc.identifier.otherBibCode: 2015ApJ...804...20C
dc.identifier.otherScopus: 84946160882
dc.identifier.otherWOS: 000354189500020
dc.identifier.otherORCID: /0000-0002-3202-0343/work/75996699
dc.identifier.urihttps://hdl.handle.net/10023/6778
dc.description.abstractWe present microlens parallax measurements for 21 (apparently) isolated lenses observed toward the Galactic bulge that were imaged simultaneously from Earth and Spitzer, which was ~1 AU west of Earth in projection. We combine these measurements with a kinematic model of the Galaxy to derive distance estimates for each lens, with error bars that are small compared to the Sun's galactocentric distance. The ensemble therefore yields a well-defined cumulative distribution of lens distances. In principle, it is possible to compare this distribution against a set of planets detected in the same experiment in order to measure the Galactic distribution of planets. Since these Spitzer observations yielded only one planet, this is not yet possible in practice. However, it will become possible as larger samples are accumulated.
dc.language.isoeng
dc.relation.ispartofAstrophysical Journalen
dc.rights© 2015. The American Astronomical Society. All rights reserved.en
dc.subjectGravitational lensing: microen
dc.subjectPlanetary systemsen
dc.subjectPlanets and satellites: dynamical evolution and stabilityen
dc.subjectQB Astronomyen
dc.subjectQC Physicsen
dc.subject3rd-DASen
dc.subject.lccQBen
dc.subject.lccQCen
dc.titlePathway to the Galactic distribution of planets : combined Spitzer and ground-based microlens parallax measurements of 21 single-lens eventsen
dc.typeJournal articleen
dc.contributor.sponsorThe Royal Societyen
dc.contributor.sponsorScience & Technology Facilities Councilen
dc.contributor.sponsorScience & Technology Facilities Councilen
dc.contributor.sponsorScience & Technology Facilities Councilen
dc.description.versionPostprinten
dc.contributor.institutionUniversity of St Andrews. School of Physics and Astronomyen
dc.identifier.doihttps://doi.org/10.1088/0004-637X/804/1/20
dc.description.statusPeer revieweden
dc.identifier.urlhttp://adsabs.harvard.edu/abs/2015ApJ...804...20Cen
dc.identifier.grantnumberUF100010 / UF130581en
dc.identifier.grantnumberST/J001651/1en
dc.identifier.grantnumberST/M001296/1en
dc.identifier.grantnumberST/K001515/1en


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