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    • OGLE-2005-BLG-071Lb, the Most Massive M Dwarf Planetary Companion? 

      Christie, G.W.; Gaudi, B.S.; Kubiak, M.; Szymanski, M.K.; Pietrzynski, G.; Soszynski, I.; Szewczyk, O.; Ulaczyk, K.; Wyrzykowski, L.; Fox, D.B.; Gal-Yam, A.; Han, C.; Lepine, S.; McCormick, J.; Ofek, E.; Park, B.G.; Pogge, R.W.; Abe, F.; Bennett, D.P.; Bond, I.A.; Britton, T.R.; Gilmore, A.C.; Hearnshaw, J.B.; Itow, Y.; Kamiya, K.; Kilmartin, P.M.; Korpela, A.; Masuda, K.; Matsubara, Y.; Motomura, M.; Muraki, Y.; Nakamura, S.; Ohnishi, K.; Okada, C.; Rattenbury, N.; Saito, T.; Sako, T.; Sasaki, M.; Sullivan, D.; Sumi, T.; Tristram, P.J.; Yanagisawa, T.; Yock, P.C.M.; Yoshoika, T.; Beaulieu, J.P.; Brillant, S.; Calitz, H.; Cassan, A.; Cook, K.H.; Coutures, C.; Dieters, S.; Prester, D.D.; Donatowicz, J.; Fouque, P.; Greenhill, J.; Hill, K.; Hoffman, M.; Horne, K.; Jaroszynski, M.; Dong, S.; Albrow, M.D.; Gould, A.; DePoy, D.L.; Udalski, A.; Anderson, J. (University of Canterbury. Physics and Astronomy, 2009)
      We combine all available information to constrain the nature of OGLE-2005-BLG-071Lb, the second planet discovered by microlensing and the first in a high-magnification event. These include photometric and astrometric ...