The first planetary microlensing event with two microlensed source stars
We present the analysis of microlensing event MOA-2010-BLG-117, and show that the light curve can only be explained by the gravitational lensing of a binary source star by a star with a Jupiter mass ratio planet. It was necessary to modify standard microlensing modeling methods to find the correct l...
Gespeichert in:
| Hauptverfasser: | , |
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| Dokumenttyp: | Article (Journal) Kapitel/Artikel |
| Sprache: | Englisch |
| Veröffentlicht: |
22 Mar 2018
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| Ausgabe: | Version V3 |
| In: |
Arxiv
Year: 2017, Pages: 1-17 |
| DOI: | 10.48550/arXiv.1707.09667 |
| Online-Zugang: | Resolving-System, kostenfrei, Volltext: https://doi.org/10.48550/arXiv.1707.09667 Verlag, kostenfrei, Volltext: http://arxiv.org/abs/1707.09667 
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| Verfasserangaben: | D.P. Bennett, A. Udalski, C. Han, I.A. Bond, J.-P. Beaulieu, J. Skowron, B.S. Gaudi, N. Koshimoto and F. Abe, Y. Asakura, R.K. Barry, A. Bhattacharya, M. Donachie, P. Evans, A. Fukui, Y. Hirao, Y. Itow, M.C.A. Li, C.H. Ling, K. Masuda, Y. Matsubara, Y. Muraki, M. Nagakane, K. Ohnishi, H. Oyokawa, C. Ranc, N.J. Rattenbury, M.K. Rosenthal, To. Saito, A. Sharan, D.J. Sullivan, T. Sumi, D. Suzuki, P.J. Tristram, A. Yonehara (The MOA Collaboration); M.K. Szymánski, R. Poleski, I. Soszynski, K. Ulaczyk, L. Wyrzykowski (The OGLE Collaboration); R. DePoy, A. Gould, R. W. Pogge,.C. Yee (The μ FUN Collaboration); M.D. Albrow, E. Bachelet, V. Batista, R. Bowens-Rubin, S. Brillant, J.A.R. Caldwell, A. Cole, C. Coutures, S. Dieters, D. Dominis Prester, J. Donatowicz, P. Fouqúe, K. Horne, M. Hundertmark, N. Kains, S.R. Kane, J.-B. Marquette, J. Menzies, K.R. Pollard, C. Ranc, K.C. Sahu, J. Wambsganss, A. Williams, and M. Zub (The PLANET Collaboration) |
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