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@Article{SkowronSUHSSGPSJBBSKPSPKPUWABBBFFFILKMMMNOPRSSSTYMKFABCCDGHHJJLMNNPPYABBBCCCCCDDFGKKKMMMPRSWWWTBHHSSABBNDDDFGHHHHJKLLLMMPRRSSSSTW:2015:JoMiPl,
               author = "Skowron, J. and Shin, I-G. and Udalski, A. and Han, C. and Sumi, 
                         T. and Shvartzvald, Y. and Gould, A. and Prester, D. Dominis and 
                         Street, R. A. and Jorgensen, U. G. and Bennett, D. P. and Bozza, 
                         V. and Szymanski, M. K. and Kubiak, M. and Pietrzynski, G. and 
                         Soszynski, I. and Poleski, R. and Kozlowski, S. and Pietrukowicz, 
                         P. and Ulaczyk, K. and Wyrzykowski, L. and Abe, F. and 
                         Bhattacharya, A. and Bond, I. A. and Botzler, C. S. and Freeman, 
                         M. and Fukui, A. and Fukunaga, D. and Itow, Y. and Ling, C. H. and 
                         Koshimoto, N. and Masuda, K. and Matsubara, Y. and Muraki, Y. and 
                         Namba, S. and Ohnishi, K. and Philpott, L. C. and Rattenbury, N. 
                         and Saito, T. and Sullivan, D. J. and Suzuki, D. and Tristam, P. 
                         J. and Yock, P. C. M. and Maoz, D. and Kaspi, S. and Friedmann, M. 
                         and Almeida, Leonardo Andrade de and Batista, V. and Christie, G. 
                         and Choi, J. Y. and DePoy, D. L. and Gaudi, B. S. and Henderson, 
                         C. and Hwang, K. H. and Jablonski, Francisco Jos{\'e} and Jung, 
                         Y. K. and Lee, C. U. and McCormick, J. and Natusch, T. and Ngan, 
                         H. and Park, H. and Pogge, R. W. and Yee, J. C. and Albrow, M. D. 
                         and Bachelet, E. and Beaulieu, J. P. and Brillant, S. and 
                         Caldwell, J. A. R. and Cassan, A. and Cole, A. and Corrales, E. 
                         and Coutures, Ch. and Dieters, S. and Donatowicz, J. and 
                         Fouqu{\'e}, P. and Greenhill, J. and Kains, N. and Kane, S. R. 
                         and Kubas, D. and Marquette, J. B. and Martin, R. and Menzies, J. 
                         and Pollard, K. R. and Ranc, C. and Sahu, K. C. and Wambganss, J. 
                         and Williams, A. and Wouters, D. and Tsapras, Y. and Bramich, D. 
                         M. and Horne, K. and Hundertmark, M. and Snodgrass, C. and Steele, 
                         I. A. and Alsubai, K. A. and Browne, P. and Burgdorf, M. J. and 
                         Novati, S. Calchi and Dodds, P. and Dominik, M. and Dreizler, S. 
                         and Fang, X. S. and Gu, C. H. and Hardis and Harpsoe, K. and 
                         Hessman, F. V. and Hinse, T. C. and Hornstrup, A. and 
                         Jessen-Hansen, J. and Kerins, E. and Liebig, C. and Lund, M. and 
                         Lundkvist, M. and Mancini, L. and Mathiasen, M. and Penny, M. T. 
                         and Rahvar, S. and Ricci, D. and Scarpetta, G. and Skottfelt, J. 
                         and Southworth, J. and Surdej, J. and Tregolan-Reed, J. and Wertz, 
                         O.",
          affiliation = "{Warsaw University Observatory} and {Chungbuk National University} 
                         and {Warsaw University Observatory} and {Chungbuk National 
                         University} and {Osaka University} and {Tel-Aviv University} and 
                         {Ohio State University} and {University of Rijeka} and {Las 
                         Cumbres Observatory Global Telescope Network} and {University of 
                         Copenhagen} and {University of Notre Dame} and {Universit{\`a} 
                         degli Studi di Salerno} and {Warsaw University Observatory} and 
                         {Warsaw University Observatory} and {Warsaw University 
                         Observatory} and {Warsaw University Observatory} and {Warsaw 
                         University Observatory} and {Warsaw University Observatory} and 
                         {Warsaw University Observatory} and {Warsaw University 
                         Observatory} and {University of Cambridge} and {Nagoya University} 
                         and {University of Notre Dame} and {Massey University} and 
                         {University of Auckland} and {University of Auckland} and 
                         {National Astronomical Observatory of Japan} and {Nagoya 
                         University} and {Nagoya University} and {Massey University} and 
                         {Osaka University} and {Nagoya University} and {Nagoya University} 
                         and {Konan University} and {Osaka University} and {Nagano National 
                         College of Technology} and {University of British Columbia} and 
                         {University of Auckland} and {Tokyo Metropolitan College of 
                         Industrial Technology} and {Victoria University} and {Osaka 
                         University} and {Victoria University} and {University of Auckland} 
                         and {Tel-Aviv University} and {Tel-Aviv University} and {Tel-Aviv 
                         University} and {Instituto Nacional de Pesquisas Espaciais (INPE)} 
                         and {Ohio State University} and {Auckland Observatory} and 
                         {Chungbuk National University} and {Texas A\&M University College 
                         Station} and {Ohio State University} and {Ohio State University} 
                         and {Chungbuk National University} and {Instituto Nacional de 
                         Pesquisas Espaciais (INPE)} and {Chungbuk National University} and 
                         {Korea Astronomy and Space Science Institute} and {Centre for 
                         Backyard Astrophysics} and {Auckland Observatory} and {Auckland 
                         Observatory} and {Chungbuk National University} and {Ohio State 
                         University} and {Ohio State University} and {University of 
                         Canterbury} and {Universit{\'e} de Toulouse} and {Institut 
                         d’Astrophysique de Paris} and {European Southern Observatory 
                         (ESO)} and {McDonald Observatory} and {Institut d’Astrophysique de 
                         Paris} and {University of Tasmania} and {Institut d’Astrophysique 
                         de Paris} and {Institut d’Astrophysique de Paris} and 
                         {Universit{\'e} de Toulouse} and {Technical University of Vienna} 
                         and {Universit{\'e} de Toulouse} and {University of Tasmania} and 
                         {European Southern Observatory} and {NASA Exoplanet Science 
                         Institute} and {Institut d’Astrophysique de Paris} and {Institut 
                         d’Astrophysique de Paris} and {Perth Observatory} and {South 
                         African Astronomical Observatory} and {University of Canterbury} 
                         and {Institut d’Astrophysique de Paris} and {Space Telescope 
                         Science Institute} and {Zentrum f{\"u}r Astronomie der 
                         Universit{\"a}t Heidelberg (ZAH)} and {Zentrum f{\"u}r 
                         Astronomie der Universit{\"a}t Heidelberg (ZAH)} and {Institut 
                         d’Astrophysique de Paris} and {Las Cumbres Observatory Global 
                         Telescope Network} and {Qatar Foundation} and {University of St 
                         Andrews} and {University of St Andrews} and {Max Planck Institute 
                         for Solar System Research} and {Liverpool John Moores University} 
                         and {Qatar Foundation} and {University of St Andrews} and {HE 
                         Space Operations GmbH} and {NASA Exoplanet Science Institute} and 
                         {University of St Andrews} and {University of St Andrews} and 
                         {Georg-August-Universit{"a}t} and {Chinese Academy of Sciences} 
                         and {Chinese Academy of Sciences} and {University of Copenhagen} 
                         and {University of Copenhagen} and {Georg-August-Universit{"a}t} 
                         and {Korea Astronomy and Space Science Institute} and {University 
                         of Manchester} and {Aarhus University} and {University of 
                         Manchester} and {University of St Andrews} and {Aarhus University} 
                         and {Aarhus University} and {Max Planck Institute for Astronomy} 
                         and {University of Copenhagen} and {University of Manchester} and 
                         {Sharif University of Technology} and {Institut d’Astrophysique et 
                         de G{\'e}ophysique} and {Universit{\`a} degli Studi di Salerno} 
                         and {University of Copenhagen} and {Keele University} and 
                         {Institut d’Astrophysique et de G{\'e}ophysique} and {NASA Ames 
                         Research Center} and {NASA Ames Research Center}",
                title = "OGLE-2011-BLG-0265Lb: a jovian microlensing planet orbiting an M 
                         DWARF",
              journal = "The Astrophysical Journal",
                 year = "2015",
               volume = "804",
               number = "33",
             keywords = "gravitational lensing: micro – planetary systems.",
             abstract = "We report the discovery of a Jupiter-mass planet orbiting an 
                         M-dwarf star that gave rise to the microlensing event 
                         OGLE-2011-BLG-0265. Such a system is very rare among known 
                         planetary systems and thus the discovery is important for 
                         theoretical studies of planetary formation and evolution. 
                         High-cadence temporal coverage of the planetary signal, combined 
                         with extended observations throughout the event, allows us to 
                         accurately model the observed light curve. However, the final 
                         microlensing solution remains degenerate, yielding two possible 
                         configurations of the planet and the host star. In the case of the 
                         preferred solution, the mass of the planet is M M p J = +- 0.9 0.3 
                         , and the planet is orbiting a star with a mass M M = +- 0.22 0.06 
                         M.The second possible configuration (2\σ away) consists of a 
                         planet with M M p J = +- 0.6 0.3 and host star with M M = +- 0.14 
                         0.06 M. The system is located in the Galactic disk 34 kpc toward 
                         the Galactic bulge. In both cases, with an orbit size of 1.52.0 
                         AU, the planet is a cold Jupiterlocated well beyond the snow line 
                         of the host star. Currently available data make the secure 
                         selection of the correct solution difficult, but there are 
                         prospects for lifting the degeneracy with additional follow-up 
                         observations in the future, when the lens and source star 
                         separate.",
                  doi = "10.1088/0004-637X/804/1/33",
                  url = "http://dx.doi.org/10.1088/0004-637X/804/1/33",
                 issn = "0004-637X",
             language = "en",
        urlaccessdate = "05 dez. 2020"
}


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