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Volumn 319, Issue 5865, 2008, Pages 927-930

Discovery of a Jupiter/Saturn analog with gravitational microlensing

(69)  Gaudi, B S a   Bennett, D P b   Udalski, A c   Gould, A a   Christie, G W d   Maoz, D e   Dong, S a   McCormick, J f   Szymanski M K c   Tristram, P J g   Nikolaev, S h   Paczynski B i   Kubiak, M c   Pietrzynski G c,j   Soszynski I c   Szewczyk, O c   Ulaczyk, K c   Wyrzykowski, L c,k   DePoy, D L a   Han, C l   more..


Author keywords

[No Author keywords available]

Indexed keywords

DETECTION METHOD; JUPITER; SATURN; SOLAR SYSTEM;

EID: 39349105578     PISSN: 00368075     EISSN: 10959203     Source Type: Journal    
DOI: 10.1126/science.1151947     Document Type: Article
Times cited : (368)

References (34)
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    • We acknowledge the following support: NSF AST-042758 (A.G, S.D, NASA NNG04GL51G (D.L.D, A.G, R.W.P, NASA/JPL 1226901 (D.L.D, B.S.G, A.G, Polish Ministerstwo Nauki i Szkolnictwa Wyższego MNiSW N20303032/4275 (OGLE, NSF AST-0708890 and NASA NNX07AL71G (D.P.B, Science Research Center, Korea Science and Engineering Foundation (C.H, Korea Astronomy and Space Science Institute (B.-G.P, Deutsche Forschungsgemeinschaft (C.S.B, Particle Physics and Astronomy Research Council (PPARC, European Union Sixth Framework Programme ANGLES (Ł.W, N.J.R, PPARC (RoboNet, Israel Science Foundation (D.M, Marsden Fund of New Zealand; Japan Ministry of Education, Culture, Sports, Science and Technology; and Japan Society for the Promotion of Science (MOA, RoboNet-1.0 is funded by the Science and Technology Facilities Council (STFC) and operates in conjunction with the eScience Telescopes for Astronomical Research project, which supports A.A. and which is jointly funded by
    • We acknowledge the following support: NSF AST-042758 (A.G., S.D.); NASA NNG04GL51G (D.L.D., A.G., R.W.P.); NASA/JPL 1226901 (D.L.D., B.S.G., A.G.); Polish Ministerstwo Nauki i Szkolnictwa Wyższego MNiSW N20303032/4275 (OGLE); NSF AST-0708890 and NASA NNX07AL71G (D.P.B.); Science Research Center, Korea Science and Engineering Foundation (C.H.); Korea Astronomy and Space Science Institute (B.-G.P.); Deutsche Forschungsgemeinschaft (C.S.B.); Particle Physics and Astronomy Research Council (PPARC), European Union Sixth Framework Programme ANGLES (Ł.W., N.J.R.); PPARC (RoboNet); Israel Science Foundation (D.M.); Marsden Fund of New Zealand; Japan Ministry of Education, Culture, Sports, Science and Technology; and Japan Society for the Promotion of Science (MOA). RoboNet-1.0 is funded by the Science and Technology Facilities Council (STFC) and operates in conjunction with the eScience Telescopes for Astronomical Research project, which supports A.A. and which is jointly funded by the Department of Trade and Industry, STFC, and the Engineering and Physical Sciences Research Council. K.H.C.'s, S.N.'s and B.M.'s work was performed under the auspices of the U.S. Department of Energy by Lawrence Livermore National Laboratory under contract DE-AC52-07NA27344. M.D. is a Royal Society University Research Fellow. We thank the MDM staff for their support. We thank D. Warren for financial support for the Mt. Canopus Observatory and M. Bode, D. Bramich, C. Mottram, S. Fraser, and C. Snodgrass for contributions to the RoboNet data.


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