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MOA-2010-BLG-328Lb : a sub-Neptune orbiting very Late M dwarf?
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dc.contributor.author | Furusawa, K. | |
dc.contributor.author | Udalski, A. | |
dc.contributor.author | Sumi, T. | |
dc.contributor.author | Bennett, D. P. | |
dc.contributor.author | Bond, I. A. | |
dc.contributor.author | Gould, A. | |
dc.contributor.author | Jørgensen, U. G. | |
dc.contributor.author | Snodgrass, C. | |
dc.contributor.author | Dominis Prester, D. | |
dc.contributor.author | Albrow, M. D. | |
dc.contributor.author | Abe, F. | |
dc.contributor.author | Botzler, C. S. | |
dc.contributor.author | Chote, P. | |
dc.contributor.author | Freeman, M. | |
dc.contributor.author | Fukui, A. | |
dc.contributor.author | Harris, P. | |
dc.contributor.author | Itow, Y. | |
dc.contributor.author | Ling, C. H. | |
dc.contributor.author | Masuda, K. | |
dc.contributor.author | Matsubara, Y. | |
dc.contributor.author | Miyake, N. | |
dc.contributor.author | Muraki, Y. | |
dc.contributor.author | Ohnishi, K. | |
dc.contributor.author | Rattenbury, N. J. | |
dc.contributor.author | Saito, To. | |
dc.contributor.author | Sullivan, D. J. | |
dc.contributor.author | Suzuki, D. | |
dc.contributor.author | Sweatman, W. L. | |
dc.contributor.author | Tristram, P. J. | |
dc.contributor.author | Wada, K. | |
dc.contributor.author | Yock, P. C. M. | |
dc.contributor.author | Szymański, M. K. | |
dc.contributor.author | Soszyński, I. | |
dc.contributor.author | Kubiak, M. | |
dc.contributor.author | Poleski, R. | |
dc.contributor.author | Ulaczyk, K. | |
dc.contributor.author | Pietrzyński, G. | |
dc.contributor.author | Wyrzykowski, Ł. | |
dc.contributor.author | Choi, J.-Y. | |
dc.contributor.author | Christie, G. W. | |
dc.contributor.author | DePoy, D. L. | |
dc.contributor.author | Dong, Subo | |
dc.contributor.author | Drummond, J. | |
dc.contributor.author | Gaudi, B. S. | |
dc.contributor.author | Han, C. | |
dc.contributor.author | Hung, L.-W. | |
dc.contributor.author | Hwang, K.-H. | |
dc.contributor.author | Lee, C.-U. | |
dc.contributor.author | McCormick, J. | |
dc.contributor.author | Moorhouse, D. | |
dc.contributor.author | Natusch, T. | |
dc.contributor.author | Nola, M. | |
dc.contributor.author | Ofek, E. | |
dc.contributor.author | Pogge, R. W. | |
dc.contributor.author | Shin, I.-G. | |
dc.contributor.author | Skowron, J. | |
dc.contributor.author | Thornley, G. | |
dc.contributor.author | Yee, J. C. | |
dc.contributor.author | Alsubai, K. A. | |
dc.contributor.author | Bozza, V. | |
dc.contributor.author | Browne, P. | |
dc.contributor.author | Burgdorf, M. J. | |
dc.contributor.author | Calchi Novati, S. | |
dc.contributor.author | Dodds, P. | |
dc.contributor.author | Dominik, M. | |
dc.contributor.author | Finet, F. | |
dc.contributor.author | Gerner, T. | |
dc.contributor.author | Hardis, S. | |
dc.contributor.author | Harpsøe, K. | |
dc.contributor.author | Hinse, T. C. | |
dc.contributor.author | Hundertmark, M. | |
dc.contributor.author | Kains, Noé | |
dc.contributor.author | Kerins, E. | |
dc.contributor.author | Liebig, C. | |
dc.contributor.author | Mancini, L. | |
dc.contributor.author | Mathiasen, M. | |
dc.contributor.author | Penny, M. T. | |
dc.contributor.author | Proft, S. | |
dc.contributor.author | Rahvar, S. | |
dc.contributor.author | Ricci, D. | |
dc.contributor.author | Scarpetta, G. | |
dc.contributor.author | Schäfer, S. | |
dc.contributor.author | Schönebeck, F. | |
dc.contributor.author | Southworth, J. | |
dc.contributor.author | Surdej, J. | |
dc.contributor.author | Wambsganss, J. | |
dc.contributor.author | Street, R. A. | |
dc.contributor.author | Bramich, D. M. | |
dc.contributor.author | Steele, I. A. | |
dc.contributor.author | Tsapras, Y. | |
dc.contributor.author | Horne, K. | |
dc.contributor.author | Donatowicz, J. | |
dc.contributor.author | Sahu, K. C. | |
dc.contributor.author | Bachelet, E. | |
dc.contributor.author | Batista, V. | |
dc.contributor.author | Beatty, T. G. | |
dc.contributor.author | Beaulieu, J.-P. | |
dc.contributor.author | Bennett, C. S. | |
dc.contributor.author | Black, C. | |
dc.contributor.author | Bowens-Rubin, R. | |
dc.contributor.author | Brillant, S. | |
dc.contributor.author | Caldwell, J. A. R. | |
dc.contributor.author | Cassan, A. | |
dc.contributor.author | Cole, A. A. | |
dc.contributor.author | Corrales, E. | |
dc.contributor.author | Coutures, C. | |
dc.contributor.author | Dieters, S. | |
dc.contributor.author | Fouqué, P. | |
dc.contributor.author | Greenhill, J. | |
dc.contributor.author | Henderson, C. B. | |
dc.contributor.author | Kubas, D. | |
dc.contributor.author | Marquette, J.-B. | |
dc.contributor.author | Martin, R. | |
dc.contributor.author | Menzies, J. W. | |
dc.contributor.author | Shappee, B. | |
dc.contributor.author | Williams, A. | |
dc.contributor.author | Wouters, D. | |
dc.contributor.author | van Saders, J. | |
dc.contributor.author | Zellem, R. | |
dc.contributor.author | Zub, M. | |
dc.date.accessioned | 2014-09-23T15:31:01Z | |
dc.date.available | 2014-09-23T15:31:01Z | |
dc.date.issued | 2013-12-20 | |
dc.identifier.citation | Furusawa , K , Udalski , A , Sumi , T , Bennett , D P , Bond , I A , Gould , A , Jørgensen , U G , Snodgrass , C , Dominis Prester , D , Albrow , M D , Abe , F , Botzler , C S , Chote , P , Freeman , M , Fukui , A , Harris , P , Itow , Y , Ling , C H , Masuda , K , Matsubara , Y , Miyake , N , Muraki , Y , Ohnishi , K , Rattenbury , N J , Saito , T , Sullivan , D J , Suzuki , D , Sweatman , W L , Tristram , P J , Wada , K , Yock , P C M , Szymański , M K , Soszyński , I , Kubiak , M , Poleski , R , Ulaczyk , K , Pietrzyński , G , Wyrzykowski , Ł , Choi , J-Y , Christie , G W , DePoy , D L , Dong , S , Drummond , J , Gaudi , B S , Han , C , Hung , L-W , Hwang , K-H , Lee , C-U , McCormick , J , Moorhouse , D , Natusch , T , Nola , M , Ofek , E , Pogge , R W , Shin , I-G , Skowron , J , Thornley , G , Yee , J C , Alsubai , K A , Bozza , V , Browne , P , Burgdorf , M J , Calchi Novati , S , Dodds , P , Dominik , M , Finet , F , Gerner , T , Hardis , S , Harpsøe , K , Hinse , T C , Hundertmark , M , Kains , N , Kerins , E , Liebig , C , Mancini , L , Mathiasen , M , Penny , M T , Proft , S , Rahvar , S , Ricci , D , Scarpetta , G , Schäfer , S , Schönebeck , F , Southworth , J , Surdej , J , Wambsganss , J , Street , R A , Bramich , D M , Steele , I A , Tsapras , Y , Horne , K , Donatowicz , J , Sahu , K C , Bachelet , E , Batista , V , Beatty , T G , Beaulieu , J-P , Bennett , C S , Black , C , Bowens-Rubin , R , Brillant , S , Caldwell , J A R , Cassan , A , Cole , A A , Corrales , E , Coutures , C , Dieters , S , Fouqué , P , Greenhill , J , Henderson , C B , Kubas , D , Marquette , J-B , Martin , R , Menzies , J W , Shappee , B , Williams , A , Wouters , D , van Saders , J , Zellem , R & Zub , M 2013 , ' MOA-2010-BLG-328Lb : a sub-Neptune orbiting very Late M dwarf? ' , Astrophysical Journal , vol. 779 , no. 2 , 91 . https://doi.org/10.1088/0004-637X/779/2/91 | en |
dc.identifier.issn | 0004-637X | |
dc.identifier.other | PURE: 149343104 | |
dc.identifier.other | PURE UUID: cc03b4f4-aa4b-437e-8d8f-3fd649bce0f7 | |
dc.identifier.other | BibCode: 2013ApJ...779...91F | |
dc.identifier.other | Scopus: 84890062483 | |
dc.identifier.other | ORCID: /0000-0002-3202-0343/work/75996725 | |
dc.identifier.uri | https://hdl.handle.net/10023/5488 | |
dc.description | K.A., D.M.B., M.D., K.H., M.H., C.L., C.S., R.A.S., and Y.T. are thankful to Qatar National Research Fund (QNRF), a member of the Qatar Foundation, for support by grant NPRP 09-476-1-078. K.H. is supported by a Royal Society Leverhulme Trust Senior Research Fellowship. | en |
dc.description.abstract | We analyze the planetary microlensing event MOA-2010-BLG-328. The best fit yields host and planetary masses of M h = 0.11 ± 0.01 M ☉ and M p = 9.2 ± 2.2 M ⊕, corresponding to a very late M dwarf and sub-Neptune-mass planet, respectively. The system lies at D L = 0.81 ± 0.10 kpc with projected separation r ⊥ = 0.92 ± 0.16 AU. Because of the host's a priori unlikely close distance, as well as the unusual nature of the system, we consider the possibility that the microlens parallax signal, which determines the host mass and distance, is actually due to xallarap (source orbital motion) that is being misinterpreted as parallax. We show a result that favors the parallax solution, even given its close host distance. We show that future high-resolution astrometric measurements could decisively resolve the remaining ambiguity of these solutions. | |
dc.format.extent | 12 | |
dc.language.iso | eng | |
dc.relation.ispartof | Astrophysical Journal | en |
dc.rights | Copyright 2013. The American Astronomical Society. All rights reserved. | en |
dc.subject | Gravitational lensing: micro | en |
dc.subject | Planetary systems | en |
dc.subject | QB Astronomy | en |
dc.subject | QC Physics | en |
dc.subject.lcc | QB | en |
dc.subject.lcc | QC | en |
dc.title | MOA-2010-BLG-328Lb : a sub-Neptune orbiting very Late M dwarf? | en |
dc.type | Journal article | en |
dc.contributor.sponsor | Science & Technology Facilities Council | en |
dc.contributor.sponsor | Science & Technology Facilities Council | en |
dc.description.version | Publisher PDF | en |
dc.contributor.institution | University of St Andrews. School of Physics and Astronomy | en |
dc.identifier.doi | https://doi.org/10.1088/0004-637X/779/2/91 | |
dc.description.status | Peer reviewed | en |
dc.identifier.grantnumber | ST/K001515/1 | en |
dc.identifier.grantnumber | ST/J001651/1 | en |
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