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Related papers: MOA-2011-BLG-293Lb: First Microlensing Planet poss…

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We have detected a 12 M$_{\rm Jup}$ planet orbiting in or near the habitable zone of a main-sequence A star via the pulsational phase shifts induced by orbital motion. The planet has an orbital period of $840\pm20$ d and an eccentricity of…

Solar and Stellar Astrophysics · Physics 2016-08-17 Simon J. Murphy , Timothy R. Bedding , Hiromoto Shibahashi

We present the discovery of a Neptune-mass planet OGLE-2007-BLG-368Lb with a planet-star mass ratio of q=[9.5 +/- 2.1] x 10^{-5} via gravitational microlensing. The planetary deviation was detected in real-time thanks to the high cadence of…

Earth and Planetary Astrophysics · Physics 2012-08-27 T. Sumi , D. P. Bennett , I. A. Bond , A. Udalski , V. Batista , M. Dominik , P. Fouqué , D. Kubas , A. Gould , B. Macintosh , K. Cook , S. Dong , L. Skuljan , A. Cassan , The MOA Collaboration , : , F. Abe , C. S. Botzler , A. Fukui , K. Furusawa , J. B. Hearnshaw , Y. Itow , K. Kamiya , P. M. Kilmartin , A. Korpela , W. Lin , C. H. Ling , K. Masuda , Y. Matsubara , N. Miyake , Y. Muraki , M. Nagaya , T. Nagayama , K. Ohnishi , T. Okumura , Y. C. Perrott , N. Rattenbury , To. Saito , T. Sako , D. J. Sullivan , W. L. Sweatman , P. , P. C. M. Yock , The PLANET Collaboration , : , J. P. Beaulieu , A. Cole , Ch. Coutures , M. F. Duran , J. Greenhill , F. Jablonski , U. Marboeuf , E. Martioli , E. Pedretti , O. Pejcha , P. Rojo , M. D. Albrow , S. Brillant , M. Bode , D. M. Bramich , M. J. Burgdorf , J. A. R. Caldwell , H. Calitz , E. Corrales , S. Dieters , D. Dominis Prester , J. Donatowicz , K. Hill , M. Hoffman , K. Horne , U. G. J , N. Kains , S. Kane , J. B. Marquette , R. Martin , P. Meintjes , J. Menzies , K. R. Pollard , K. C. Sahu , C. Snodgrass , I. Steele , R. Street , Y. Tsapras , J. Wambsganss , A. Williams , M. Zub , The OGLE Collaboration , : , M. K. Szyma , M. Kubiak , G. Pietrzy , I. Soszy , O. Szewczyk , K. Ulaczyk , The microFUN Collaboration , : , W. Allen , G. W. Christie , D. L. DePoy , B. S. Gaudi , C. Han , J. Janczak , C. -U. Lee , J. McCormick , F. Mallia , B. Monard , T. Natusch , B. -G. Park , R. W. Pogge , R. Santallo

We present the analysis of OGLE-2016-BLG-0613, for which the lensing light curve appears to be that of a typical binary-lens event with two caustic spikes but with a discontinuous feature on the trough between the spikes. We find that the…

The core accretion theory of planetary formation does not predict that super-Jupiters will form beyond the snow line of a low mass stars. We present a discovery of 3.9 +- 1.2 M_Jup mass planet orbiting the 0.59 +- 0.17 M_Sun star using the…

We search for microlensing planets with signals exhibiting no caustic-crossing features, considering the possibility that such signals may be missed due to their weak and featureless nature. For this purpose, we reexamine the lensing events…

High-cadence observations of the Galactic bulge by the microlensing surveys led to the discovery of a handful of extremely short-timescale microlensing events that can be attributed to free-floating or wide-orbit planets. Here, we report…

Current microlensing surveys are sensitive to free-floating planets down to Earth-mass objects. All published microlensing events attributed to unbound planets were identified based on their short timescale (below two days), but lacked an…

We analyze the planetary microlensing event MOA-2010-BLG-328. The best fit yields host and planetary masses of Mh = 0.11+/-0.01 M_{sun} and Mp = 9.2+/-2.2M_Earth, corresponding to a very late M dwarf and sub-Neptune-mass planet,…

Earth and Planetary Astrophysics · Physics 2015-06-17 K. Furusawa , A. Udalski , T. Sumi , D. P. Bennett , I. A. Bond , A. Gould , U. G. Jorgensen , C. Snodgrass , D. Dominis Prester , M. D. Albrow , F. Abe , C. S. Botzler , P. Chote , M. Freeman , A. Fukui , P. Harris , Y. Itow , C. H. Ling , K. Masuda , Y. Matsubara , N. Miyake , Y. Muraki , K. Ohnishi , N. J. Rattenbury , To. Saito , D. J. Sullivan , D. Suzuki , W. L. Sweatman , P. J. Tristram , K. Wada , P. C. M. Yock , M. K. Szymanski , I. Soszynski , M. Kubiak , R. Poleski , K. Ulaczyk , G. Pietrzynski , L. Wyrzykowski , J. Y. Choi , G. W. Christie , D. L. DePoy , S. Dong , J. Drummond , B. S. Gaudi , C. Han , L. -W. Hung , Y. -K. Jung , C. -U. Lee , J. McCormick , D. Moorhouse , T. Natusch , M. Nola , E. Ofek , B. G. Park , H. Park , R. W. Pogge , I. -G. Shin , J. Skowron , G. Thornley , J. C. Yee , K. A. Alsubai , V. Bozza , P. Browne , M. J. Burgdorf , S. Calchi Novati , P. Dodds , M. Dominik , F. Finet , T. Gerner , S. Hardis , K. Harpsoe , T. C. Hinse , M. Hundertmark , N. Kains , E. Kerins , C. Liebig , L. Mancini , M. Mathiasen , M. T. Penny , S. Proft , S. Rahvar , D. Ricci , G. Scarpetta , S. Schafer , F. Schonebeck , J. Southworth , J. Surdej , J. Wambsganss , R. A. Street , D. M. Bramich , I. A. Steele , Y. Tsapras , K. Horne , J. Donatowicz , K. C. Sahu , E. Bachelet , V. Batista , T. G. Beatty , J. -P. Beaulieu , C. S. Bennett , C. Black , R. Bowens-Rubin , S. Brillant , J. A. R. Caldwell , A. Cassan , A. A. Cole , E. Corrales , C. Coutures , S. Dieters , P. Fouque , J. Greenhill , C. B. Henderson , D. Kubas , J. -B. Marquette , R. Martin , J. W. Menzies , B. Shappee , A. Williams , D. Wouters , J. van Saders , R. Zellem , M. Zub

We observed the microlensing event MOA-2007-BLG-192 at high angular resolution in JHKs with the NACO adaptive optics system on the VLT while the object was still amplified by a factor 1.23 and then at baseline 18 months later. We analyzed…

We analyze the MOA-2020-BLG-208 gravitational microlensing event and present the discovery and characterization of a new planet, MOA-2020-BLG-208Lb, with an estimated sub-Saturn mass. With a mass ratio $q = 3.17^{+0.28}_{-0.26} \times…

We report the discovery of a giant planet in the KMT-2016-BLG-1397 microlensing event, which was found by The Korea Microlensing Telescope Network (KMTNet) alone. The time scale of this event is t_E = 40.0 +- 0.5 days and the mass ratio…

High-magnification gravitational microlensing events provide an important channel of detecting planetary systems with multiple giants located at their birth places. In order to investigate the potential existence of additional planets, we…

Earth and Planetary Astrophysics · Physics 2015-06-23 I. -G. Shin , C. Han , J. -Y. Choi , K. -H. Hwang , Y. K. Jung , H. Park

We present the result of microlensing event MOA-2016-BLG-290, which received observations from the two-wheel Kepler (K2), Spitzer, as well as ground-based observatories. A joint analysis of data from K2 and the ground leads to two…

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