MOA-2011-BLG-293Lb: A TEST OF PURE SURVEY MICROLENSING PLANET DETECTIONS
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A. Gal-Yam | A. Udalski | S. Kozlowski | I. A. Bond | C. H. Ling | D. Suzuki | J. Skowron | Y. Shvartzvald | E. Ofek | D. Maoz | B. Gaudi | D. Bennett | R. Poleski | D. Depoy | K. Ulaczyk | A. Gal-yam | S. Dong | L. Monard | A. Gal-Yam | R. Pogge | T. Tan | A. Fukui | A. Udalski | M. Szymański | M. Kubiak | C. Botzler | C. Henderson | S. Kaspi | P. Pietrukowicz | J. Skowron | S. Kozłowski | I. Soszyński | Ł. Wyrzykowski | W. Sweatman | D. Sullivan | Y. Itow | Y. Matsubara | Y. Muraki | P. Chote | P. Tristram | M. Bos | J. Yee | C. Han | I. Shin | Y. Shvartzvald | L. Almeida | A. Gould | T. Sumi | I. Bond | N. Rattenbury | K. Masuda | K. Furusawa | C. Ling | N. Miyake | K. Ohnishi | M. Freeman | S. Kobara | D. Suzuki | G. Christie | J. Mccormick | D. Moorhouse | T. Natusch | G. Thornley | J. Koo | C. Han | J. C. Yee | I. Manulis | V. Batista | R. Santallo | the MOA Collaboration | the OGLE Collaboration | the MicroFUN Collaboration | A. Gould | H. Ngan | K. Suzuki | E. Gorbikov | S. Kozłowski | F. Abe | S. Takino | D. McGregor | S.-Y. Park | F. Jablonski | G. Pietrzyński | J. Muñoz | C.‐U. Lee | T. Saito | W. Allen | J. Drummond | J.-Y. Choi | K. Wada | I. Finkelman | D. Higgins | G. Pietrzyński | K. Ohmori | I. Soszyński | J. A. Muñoz | David P. Bennett | Yasushi Muraki | Francisco Jablonski | C. Han | A. Gould | T. Saito | K. Masuda | Jack D. Drummond | Thiam-Guan Tan | Kantaro Ohmori | William H. Allen | D. P. Bennett | F. Jablonski
[1] OGLE-2005-BLG-071Lb, THE MOST MASSIVE M DWARF PLANETARY COMPANION? , 2008, 0804.1354.
[2] B. Gaudi,et al. Planetary Detection Efficiency of the Magnification 3000 Microlensing Event OGLE-2004-BLG-343 , 2005, astro-ph/0507079.
[3] C. H. Ling,et al. MICROLENSING EVENT MOA-2007-BLG-400: EXHUMING THE BURIED SIGNATURE OF A COOL, JOVIAN-MASS PLANET , 2008, 0809.2997.
[4] F. Bouchy,et al. The HARPS search for southern extra-solar planets - XXXI. The M-dwarf sample , 2011, 1111.5019.
[5] K. Covey,et al. CHARACTERIZING THE COOL KOIs. II. THE M DWARF KOI-254 AND ITS HOT JUPITER , 2011, 1112.0017.
[6] J. B. Marquette,et al. A frozen super-Earth orbiting a star at the bottom of the main sequence , 2010, 1009.5665.
[7] B. Monard,et al. MOA-2009-BLG-387Lb: a massive planet orbiting an M dwarf , 2011, 1102.0558.
[8] Andrew Gould,et al. Proper Motions of MACHOs , 1994 .
[9] B. Monard,et al. THE EXTREME MICROLENSING EVENT OGLE-2007-BLG-224: TERRESTRIAL PARALLAX OBSERVATION OF A THICK-DISK BROWN DWARF , 2009, 0904.0249.
[10] B. Monard,et al. SUB-SATURN PLANET MOA-2008-BLG-310Lb: LIKELY TO BE IN THE GALACTIC BULGE , 2009, 0908.0529.
[11] K. Ulaczyk,et al. A Jovian-Mass Planet in Microlensing Event OGLE-2005-BLG-071 , 2005 .
[12] C. H. Ling,et al. A NEW TYPE OF AMBIGUITY IN THE PLANET AND BINARY INTERPRETATIONS OF CENTRAL PERTURBATIONS OF HIGH-MAGNIFICATION GRAVITATIONAL MICROLENSING EVENTS , 2012, 1204.4789.
[13] K. Ulaczyk,et al. Unbound or distant planetary mass population detected by gravitational microlensing , 2011, Nature.
[14] A. Gould. Resolution of the MACHO-LMC-5 Puzzle: The Jerk-Parallax Microlens Degeneracy , 2003, astro-ph/0311548.
[15] S. Lucatello,et al. Chemical evolution of the Galactic bulge as traced by microlensed dwarf and subgiant stars IV. Two bulge populations , 2011, 1107.5606.
[16] A. Gould. Hexadecapole Approximation in Planetary Microlensing , 2008, 0801.2578.
[17] B. Monard,et al. EXTREME MAGNIFICATION MICROLENSING EVENT OGLE-2008-BLG-279: STRONG LIMITS ON PLANETARY COMPANIONS TO THE LENS STAR , 2009, 0907.5411.
[18] Identification of the OGLE-2003-BLG-235/MOA-2003-BLG-53 Planetary Host Star* , 2006, astro-ph/0606038.
[19] Gregory Laughlin,et al. The Core Accretion Model Predicts Few Jovian-Mass Planets Orbiting Red Dwarfs , 2004, astro-ph/0407309.
[20] S. Mao,et al. Erratum: Modelling the Galactic bar using OGLE-II red clump giant stars , 2007, 0704.1614.
[21] A. Gal-Yam,et al. OGLE-2003-BLG-262: Finite-Source Effects from a Point-Mass Lens , 2003, astro-ph/0309302.
[22] A. Gould,et al. Stellar Contribution to the Galactic Bulge Microlensing Optical Depth , 2003, astro-ph/0303309.
[23] Neda Safizadeh,et al. The Use of High-Magnification Microlensing Events in Discovering Extrasolar Planets , 1997 .
[24] O. Shemmer,et al. Discovery of a planet orbiting a binary star system from gravitational microlensing , 1999, Nature.
[25] F. Thevenin,et al. The angular sizes of dwarf stars and subgiants Surface brightness relations calibrated by interferometry , 2004, astro-ph/0404180.
[26] J. Beaulieu,et al. A Complete Set of Solutions for Caustic Crossing Binary Microlensing Events , 1999, astro-ph/9903008.
[27] R. A. Street,et al. FREQUENCY OF SOLAR-LIKE SYSTEMS AND OF ICE AND GAS GIANTS BEYOND THE SNOW LINE FROM HIGH-MAGNIFICATION MICROLENSING EVENTS IN 2005–2008 , 2010, 1001.0572.
[28] D. Bennett,et al. A SECOND METHOD TO PHOTOMETRICALLY ALIGN MULTI-SITE MICROLENSING LIGHT CURVES: SOURCE COLOR IN PLANETARY EVENT MOA-2007-BLG-192 , 2009, 0910.1832.
[29] O. Pejcha,et al. EXTENDED-SOURCE EFFECT AND CHROMATICITY IN TWO-POINT-MASS MICROLENSING , 2007, 0712.2217.
[30] M. Dominik. Parameter degeneracies and (un)predictability of gravitational microlensing events , 2008, 0811.4173.
[31] M. Bessell,et al. JHKLM PHOTOMETRY: STANDARD SYSTEMS, PASSBANDS, AND INTRINSIC COLORS , 1988 .
[32] P. M. Vreeswijk,et al. Microlensing Constraints on the Frequency of Jupiter-Mass Companions: Analysis of 5 Years of PLANET Photometry , 2001, astro-ph/0104100.
[33] Andrew Gould. Theory of Pixel Lensing , 1995 .
[34] D. Fischer,et al. Extreme Solar Systems , 2008 .
[35] A. Tomaney,et al. MACHO Alert 95-30: First Real-Time Observation of Extended Source Effects in Gravitational Microlensing , 1997 .
[36] Stochastic distributions of lens and source properties for observed galactic microlensing events , 2005, astro-ph/0507540.
[37] M. Dominik,et al. Detection of Rotation in a Binary Microlens: PLANET Photometry of MACHO 97-BLG-41* , 2000 .
[38] C. H. Ling,et al. A Low-Mass Planet with a Possible Sub-Stellar-Mass Host in Microlensing Event MOA-2007-BLG-192 , 2008, 0806.0025.
[39] The distances to open clusters from main-sequence fitting. III. Improved accuracy with empirically calibrated isochrones , 2006, astro-ph/0607549.
[40] B. Monard,et al. A COLD NEPTUNE-MASS PLANET OGLE-2007-BLG-368Lb: Cold neptunes are common , 2009, 0912.1171.
[41] S Ida,et al. Toward a Deterministic Model of Planetary Formation. III. Mass Distribution of Short-Period Planets around Stars of Various Masses , 2005 .
[42] A. Udalski,et al. MOA-2011-BLG-293LB: FIRST MICROLENSING PLANET POSSIBLY IN THE HABITABLE ZONE , 2013, 1310.3706.
[43] Rapid Formation of Gas Giant Planets around M Dwarf Stars , 2006, astro-ph/0601486.
[44] Y. Watase,et al. Real-time difference imaging analysis of moa galactic bulge observations during 2000 , 2001 .
[45] Yossi Shvartzvald,et al. Second-generation microlensing planet surveys: a realistic simulation , 2011, 1107.5809.