THE EXOPLANET MASS-RATIO FUNCTION FROM THE MOA-II SURVEY: DISCOVERY OF A BREAK AND LIKELY PEAK AT A NEPTUNE MASS
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Akihiko Fukui | Hiroshi Shibai | Ian A. Bond | Naoki Koshimoto | Masayuki Nagakane | Atsunori Yonehara | To. Saito | Takahiro Sumi | David P. Bennett | M. Donachie | M. Freeman | Y. Hirao | C. H. Ling | H. Oyokawa | A. Sharan | P. J. Tristram | Denis J. Sullivan | Yoshitaka Itow | Kimiaki Masuda | Yasushi Muraki | Nicholas J. Rattenbury | D. Bennett | H. Shibai | L. Rogers | A. Fukui | F. Abe | D. Sullivan | Y. Itow | Y. Matsubara | Y. Muraki | P. Tristram | K. Masuda | F. Abe | Aparna Bhattacharya | Leslie A. Rogers | T. Sumi | I. Bond | N. Rattenbury | K. Masuda | C. Ling | To. Saito | M. Freeman | D. Suzuki | Yutaka Matsubara | A. Yonehara | A. Bhattacharya | Y. Hirao | N. Koshimoto | Daisuke Suzuki | M. Li | Y. Asakura | A. Sharan | Y. Asakura | M. C. A. Li | K. Onishi | M. Donachie | M. Nagakane | H. Oyokawa | K. Onishi | T. Saito | H. Shibai | T. Saito
[1] C. H. Ling,et al. MICROLENSING EVENT MOA-2007-BLG-400: EXHUMING THE BURIED SIGNATURE OF A COOL, JOVIAN-MASS PLANET , 2008, 0809.2997.
[2] F. Bouchy,et al. The HARPS search for southern extra-solar planets - XXXI. The M-dwarf sample , 2011, 1111.5019.
[3] K. Ulaczyk,et al. Microlens OGLE-2005-BLG-169 Implies That Cool Neptune-like Planets Are Common , 2006 .
[4] Jack J. Lissauer,et al. KEPLER-79'S LOW DENSITY PLANETS , 2013, 1310.2642.
[5] Scott Gaudi,et al. SYNTHESIZING EXOPLANET DEMOGRAPHICS FROM RADIAL VELOCITY AND MICROLENSING SURVEYS. II. THE FREQUENCY OF PLANETS ORBITING M DWARFS , 2014, 1404.7500.
[6] Byeong-Gon Park,et al. Properties of Central Caustics in Planetary Microlensing , 2005, astro-ph/0505363.
[7] 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.
[8] X. Delfosse,et al. CFBDSIR2149-0403: a 4-7 Jupiter-mass free-floating planet in the young moving group AB Doradus ? ⋆ , 2012, 1210.0305.
[9] Bohdan Paczynski,et al. Gravitational microlensing by double stars and planetary systems , 1991 .
[10] Yossi Shvartzvald,et al. Second-generation microlensing planet surveys: a realistic simulation , 2011, 1107.5809.
[11] M. Kubiak,et al. Binary Lenses in OGLE-III EWS Database. Seasons 2006--2008 , 2004 .
[12] Jason T. Wright,et al. The California Planet Survey. II. A Saturn-Mass Planet Orbiting the M Dwarf Gl 649 , 2009, 0912.2730.
[13] B. Monard,et al. SUB-SATURN PLANET MOA-2008-BLG-310Lb: LIKELY TO BE IN THE GALACTIC BULGE , 2009, 0908.0529.
[14] S. Kane,et al. Microlensing limits on numbers and orbits of extrasolar planets from the 1998–2000 OGLE events , 2003, astro-ph/0304284.
[15] C. H. Ling,et al. MOA-2011-BLG-262Lb: A SUB-EARTH-MASS MOON ORBITING A GAS GIANT PRIMARY OR A HIGH VELOCITY PLANETARY SYSTEM IN THE GALACTIC BULGE , 2013, 1312.3951.
[16] C. H. Ling,et al. MOA-2008-BLG-379Lb: A MASSIVE PLANET FROM A HIGH MAGNIFICATION EVENT WITH A FAINT SOURCE , 2013, 1311.3424.
[17] P. Schechter,et al. DOPHOT, A CCD PHOTOMETRY PROGRAM: DESCRIPTION AND TESTS , 1993 .
[18] Zhaohuan Zhu,et al. FAST RISE OF “NEPTUNE-SIZE” PLANETS (4–8 R⊕) FROM P ∼ 10 TO ∼250 DAYS—STATISTICS OF KEPLER PLANET CANDIDATES UP TO ∼0.75 AU , 2012, 1212.4853.
[19] Scott Gaudi,et al. SYNTHESIZING EXOPLANET DEMOGRAPHICS FROM RADIAL VELOCITY AND MICROLENSING SURVEYS. I. METHODOLOGY , 2014, 1404.7495.
[20] C. H. Ling,et al. Mass measurement of a single unseen star and planetary detection efficiency for OGLE 2007-BLG-050 , 2009, 0907.3471.
[21] L. Girardi,et al. PARSEC evolutionary tracks of massive stars up to 350 M ☉ at metallicities 0.0001 ≤ Z ≤ 0.04 , 2015, 1506.01681.
[22] C. H. Ling,et al. OGLE-2012-BLG-0455/MOA-2012-BLG-206: MICROLENSING EVENT WITH AMBIGUITY IN PLANETARY INTERPRETATIONS CAUSED BY INCOMPLETE COVERAGE OF PLANETARY SIGNAL , 2014, 1403.1672.
[23] Howard Isaacson,et al. The Occurrence and Mass Distribution of Close-in Super-Earths, Neptunes, and Jupiters , 2010, Science.
[24] C. H. Ling,et al. OGLE-2012-BLG-0724LB: A SATURN-MASS PLANET AROUND AN M DWARF , 2016, 1604.05463.
[25] K. Ulaczyk,et al. CHARACTERIZING LENSES AND LENSED STARS OF HIGH-MAGNIFICATION SINGLE-LENS GRAVITATIONAL MICROLENSING EVENTS WITH LENSES PASSING OVER SOURCE STARS , 2011, 1111.4032.
[26] R. Pfeifle,et al. CONFIRMATION OF THE PLANETARY MICROLENSING SIGNAL AND STAR AND PLANET MASS DETERMINATIONS FOR EVENT OGLE-2005-BLG-169 , 2015, 1507.08661.
[27] R. Trotta. Bayes in the sky: Bayesian inference and model selection in cosmology , 2008, 0803.4089.
[28] D. Bennett. AN EFFICIENT METHOD FOR MODELING HIGH-MAGNIFICATION PLANETARY MICROLENSING EVENTS , 2009, 0911.2703.
[29] B. Monard,et al. A COLD NEPTUNE-MASS PLANET OGLE-2007-BLG-368Lb: Cold neptunes are common , 2009, 0912.1171.
[30] A. Udalski,et al. MOA-2011-BLG-293LB: FIRST MICROLENSING PLANET POSSIBLY IN THE HABITABLE ZONE , 2013, 1310.3706.
[31] Christopher W. Stubbs,et al. The macho project first-year large magellanic cloud results: The microlensing rate and the nature of the galactic dark halo , 1996 .
[32] R. Poleski,et al. The OGLE-III planet detection efficiency from six years of microlensing observations (2003–2008) , 2016, 1602.02519.
[33] Philip Yock,et al. On Planetary Companions to the MACHO 98-BLG-35 Microlens Star , 2000 .
[34] O. Szewczyk,et al. Discovery of a cool planet of 5.5 Earth masses through gravitational microlensing , 2006, Nature.
[35] C. H. Ling,et al. SPITZER OBSERVATIONS OF OGLE-2015-BLG-1212 REVEAL A NEW PATH TOWARD BREAKING STRONG MICROLENS DEGENERACIES , 2016, 1601.01699.
[36] K. Ulaczyk,et al. The Second Multiple-planet System Discovered by Microlensing: OGLE-2012-BLG-0026Lb, c—A Pair of Jovian Planets beyond the Snow Line , 2013 .
[37] M. R. Haas,et al. PLANET OCCURRENCE WITHIN 0.25 AU OF SOLAR-TYPE STARS FROM KEPLER , 2011, 1103.2541.
[38] 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.
[39] David P. Bennett,et al. Detection of Extrasolar Planets by Gravitational Microlensing , 2009, 0902.1761.
[40] C. H. Ling,et al. OGLE-2008-BLG-355Lb: A MASSIVE PLANET AROUND A LATE-TYPE STAR , 2014, 1403.7005.
[41] Bruce D. Clarke,et al. Identifying False Alarms in the Kepler Planet Candidate Catalog , 2016, 1602.03204.
[42] K. Ulaczyk,et al. OGLE-2012-BLG-0563Lb: A SATURN-MASS PLANET AROUND AN M DWARF WITH THE MASS CONSTRAINED BY SUBARU AO IMAGING , 2015, 1506.08850.
[43] F. Thevenin,et al. The angular sizes of dwarf stars and subgiants Surface brightness relations calibrated by interferometry , 2004, astro-ph/0404180.
[44] K. Ulaczyk,et al. MASSES AND ORBITAL CONSTRAINTS FOR THE OGLE-2006-BLG-109Lb,c JUPITER/SATURN ANALOG PLANETARY SYSTEM , 2009, 0911.2706.
[45] L. Girardi,et al. New PARSEC evolutionary tracks of massive stars at low metallicity: testing canonical stellar evolution in nearby star-forming dwarf galaxies , 2014, 1410.1745.
[46] K. Ulaczyk,et al. Discovery of a Jupiter/Saturn Analog with Gravitational Microlensing , 2008, Science.
[47] Manchester,et al. PREDICTIONS FOR MICROLENSING PLANETARY EVENTS FROM CORE ACCRETION THEORY , 2014, 1403.4936.
[48] C. H. Ling,et al. MOA 2010-BLG-477Lb: CONSTRAINING THE MASS OF A MICROLENSING PLANET FROM MICROLENSING PARALLAX, ORBITAL MOTION, AND DETECTION OF BLENDED LIGHT , 2012, 1205.6323.
[49] B. Gaudi,et al. Planetary Detection Efficiency of the Magnification 3000 Microlensing Event OGLE-2004-BLG-343 , 2005, astro-ph/0507079.
[50] C. H. Ling,et al. THE FIRST CIRCUMBINARY PLANET FOUND BY MICROLENSING: OGLE-2007-BLG-349L(AB)c , 2016, 1609.06720.
[51] K. Zebrun,et al. OGLE 2003-BLG-235/MOA 2003-BLG-53: A Planetary Microlensing Event , 2004 .
[52] D. Bennett,et al. CAN THE MASSES OF ISOLATED PLANETARY-MASS GRAVITATIONAL LENSES BE MEASURED BY TERRESTRIAL PARALLAX? , 2014, 1412.1546.
[53] J. B. Marquette,et al. ExELS: an exoplanet legacy science proposal for the ESA Euclid mission – I. Cold exoplanets , 2012, 1206.5296.
[54] K. Ulaczyk,et al. MOA-2013-BLG-220Lb: MASSIVE PLANETARY COMPANION TO GALACTIC-DISK HOST , 2014, 1403.2134.
[55] G. Marcy,et al. A PLATEAU IN THE PLANET POPULATION BELOW TWICE THE SIZE OF EARTH , 2013, 1304.0460.
[56] Stochastic distributions of lens and source properties for observed galactic microlensing events , 2005, astro-ph/0507540.
[57] Dong-Hyuk Kim,et al. A Development of Expected Loss Control Chart Using Reflected Normal Loss Function , 2016 .
[58] S. Quanz,et al. Direct imaging constraints on planet populations detected by microlensing , 2012, 1203.3647.
[59] David P. Bennett,et al. Detecting Earth-Mass Planets with Gravitational Microlensing , 1996, astro-ph/9603158.
[60] K. Ulaczyk,et al. A terrestrial planet in a ~1-AU orbit around one member of a ∼15-AU binary , 2014, Science.
[61] K. Masuda,et al. MOA-cam3: a wide-field mosaic CCD camera for a gravitational microlensing survey in New Zealand , 2008 .
[62] C. H. Ling,et al. The frequency of snowline-region planets from four-years of OGLE-MOA-Wise second-generation microlensing. , 2015, Monthly notices of the Royal Astronomical Society.
[63] B. Monard,et al. EXTREME MAGNIFICATION MICROLENSING EVENT OGLE-2008-BLG-279: STRONG LIMITS ON PLANETARY COMPANIONS TO THE LENS STAR , 2009, 0907.5411.
[64] Pierre Kervella,et al. The angular sizes of dwarf stars and subgiants (Research Note) Non-linear surface brightness relations in BVRcIc from interferometry , 2008, 0809.1732.
[65] D. Charbonneau,et al. THE OCCURRENCE OF POTENTIALLY HABITABLE PLANETS ORBITING M DWARFS ESTIMATED FROM THE FULL KEPLER DATASET AND AN EMPIRICAL MEASUREMENT OF THE DETECTION SENSITIVITY , 2015, 1501.01623.
[66] Y. Watase,et al. Real-time difference imaging analysis of moa galactic bulge observations during 2000 , 2001 .
[67] OGLE-2005-BLG-071Lb, THE MOST MASSIVE M DWARF PLANETARY COMPANION? , 2008, 0804.1354.
[68] G. Marcy,et al. Prevalence of Earth-size Planets Orbiting Sun-like Stars , 2015, 1510.03902.
[69] Bohdan Paczynski,et al. Gravitational microlensing by the galactic halo , 1986 .
[70] F. Bouchy,et al. The HARPS search for southern extra-solar planets - XIII. A planetary system with 3 super-Earths (4.2, 6.9, and 9.2 M) , 2008, 0806.4587.
[71] Andrew Gould,et al. Discovering Planetary Systems through Gravitational Microlenses , 1992 .
[72] Khadeejah A. Zamudio,et al. PLANETARY CANDIDATES OBSERVED BY KEPLER. VI. PLANET SAMPLE FROM Q1–Q16 (47 MONTHS) , 2015, 1502.02038.
[73] Russel J. White,et al. A SURVEY OF STELLAR FAMILIES: MULTIPLICITY OF SOLAR-TYPE STARS , 2009, 1007.0414.
[74] M. Halpern,et al. First-Year Wilkinson Microwave Anisotropy Probe (WMAP) Observations: Parameter Estimation Methodology , 2003 .
[75] Gregory Laughlin,et al. The Core Accretion Model Predicts Few Jovian-Mass Planets Orbiting Red Dwarfs , 2004, astro-ph/0407309.
[76] B. Monard,et al. MOA-2009-BLG-387Lb: a massive planet orbiting an M dwarf , 2011, 1102.0558.
[77] Andrew Gould,et al. REDDENING AND EXTINCTION TOWARD THE GALACTIC BULGE FROM OGLE-III: THE INNER MILKY WAY'S RV ∼ 2.5 EXTINCTION CURVE , 2012, 1208.1263.
[78] S. Ida,et al. Towards a Deterministic Model of Planetary Formation I: a Desert in the Mass and Semi Major Axis Distributions of Extra Solar Planets , 2022 .
[79] M. R. Haas,et al. TERRESTRIAL PLANET OCCURRENCE RATES FOR THE KEPLER GK DWARF SAMPLE , 2015, 1506.04175.
[80] C. H. Ling,et al. A SUB-SATURN MASS PLANET, MOA-2009-BLG-319Lb , 2010, 1010.1809.
[81] K. Ulaczyk,et al. DISCOVERY AND MASS MEASUREMENTS OF A COLD, 10 EARTH MASS PLANET AND ITS HOST STAR , 2011, 1106.2160.
[82] B. Scott Gaudi,et al. Microlensing Surveys for Exoplanets , 2012 .
[83] Howard Isaacson,et al. Kepler Planet-Detection Mission: Introduction and First Results , 2010, Science.
[84] 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.
[85] C. H. Ling,et al. MOA-2011-BLG-028Lb: A NEPTUNE-MASS MICROLENSING PLANET IN THE GALACTIC BULGE , 2015, 1512.03422.
[86] A. Gould,et al. Stellar Contribution to the Galactic Bulge Microlensing Optical Depth , 2003, astro-ph/0303309.
[87] 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.
[88] David P. Bennett,et al. Simulation of a Space-based Microlensing Survey for Terrestrial Extrasolar Planets , 2002 .
[89] D. Maoz,et al. A VENUS-MASS PLANET ORBITING A BROWN DWARF: A MISSING LINK BETWEEN PLANETS AND MOONS , 2015, 1507.02388.
[90] Jan Skowron,et al. TRIPLE MICROLENS OGLE-2008-BLG-092L: BINARY STELLAR SYSTEM WITH A CIRCUMPRIMARY URANUS-TYPE PLANET , 2014, 1408.6223.
[91] Howard Isaacson,et al. ALL SIX PLANETS KNOWN TO ORBIT KEPLER-11 HAVE LOW DENSITIES , 2013, 1303.0227.
[92] C. H. Ling,et al. A brown dwarf orbiting an M-dwarf: MOA 2009–BLG–411L , 2012 .
[93] C. H. Ling,et al. OGLE-2011-BLG-0265Lb: A JOVIAN MICROLENSING PLANET ORBITING AN M DWARF , 2014, 1410.8252.
[94] K. Ulaczyk,et al. Unbound or distant planetary mass population detected by gravitational microlensing , 2011, Nature.
[95] Arpita Roy,et al. Stellar activity masquerading as planets in the habitable zone of the M dwarf Gliese 581 , 2014, Science.
[96] E. L. Wright,et al. THE COLDEST BROWN DWARF (OR FREE-FLOATING PLANET)?: THE Y DWARF WISE 1828+2650 , 2013, 1301.1669.
[97] Eric B. Ford,et al. PROBABILISTIC MASS–RADIUS RELATIONSHIP FOR SUB-NEPTUNE-SIZED PLANETS , 2015, 1504.07557.
[98] A. Bhattacharya,et al. CONFIRMATION OF THE OGLE-2005-BLG-169 PLANET SIGNATURE AND ITS CHARACTERISTICS WITH LENS–SOURCE PROPER MOTION DETECTION , 2015, 1507.08914.
[99] Julien H. Girard,et al. A survey of young, nearby, and dusty stars conducted to understand the formation of wide-orbit giant planets - VLT/NaCo adaptive optics thermal and angular differential imaging , 2013 .
[100] Mauro Barbieri,et al. Improving PARSEC models for very low mass stars , 2014, 1409.0322.
[101] C. H. Ling,et al. PLANETARY AND OTHER SHORT BINARY MICROLENSING EVENTS FROM THE MOA SHORT-EVENT ANALYSIS , 2012, 1203.4560.
[102] K. Ulaczyk,et al. SPITZER PARALLAX OF OGLE-2015-BLG-0966: A COLD NEPTUNE IN THE GALACTIC DISK , 2015, 1508.07027.
[103] G. Marcy,et al. THE MASS–RADIUS RELATION FOR 65 EXOPLANETS SMALLER THAN 4 EARTH RADII , 2013, 1312.0936.
[104] C. H. Ling,et al. MOA-2010-BLG-328Lb: A SUB-NEPTUNE ORBITING VERY LATE M DWARF? , 2013, 1309.7714.
[105] C. H. Ling,et al. MOA-2010-BLG-523: “FAILED PLANET” = RS CVn STAR , 2012, 1210.6045.
[106] Neda Safizadeh,et al. The Use of High-Magnification Microlensing Events in Discovering Extrasolar Planets , 1997 .
[107] D. Bennett,et al. A New Nonplanetary Interpretation of the Microlensing Event OGLE-2013-BLG-0723 , 2016, 1604.06533.
[108] Andrew Gould,et al. Extending the MACHO Search to approximately 10 6 M sub sun , 1992 .
[109] C. H. Ling,et al. MOA-2011-BLG-322Lb: a ‘second generation survey’ microlensing planet , 2013, 1310.0008.
[110] Andrew Cumming,et al. The Keck Planet Search: Detectability and the Minimum Mass and Orbital Period Distribution of Extrasolar Planets , 2008, 0803.3357.
[111] C. H. Ling,et al. MOA-2010-BLG-353Lb: A Possible Saturn Revealed , 2015, 1510.01393.
[112] C. H. Ling,et al. MOA-2010-BLG-311: A planetary candidate below the threshold of reliable detection , 2012, 1210.6041.
[113] A. Gal-Yam,et al. MOA-2011-BLG-293Lb: A TEST OF PURE SURVEY MICROLENSING PLANET DETECTIONS , 2012, 1201.1002.
[114] B. Scott Gaudi,et al. Distinguishing Between Binary-Source and Planetary Microlensing Perturbations , 1998 .
[115] C. G. Tinney,et al. Catalog of nearby exoplanets , 2006 .
[116] B. Scott Gaudi,et al. Characterization of Gravitational Microlensing Planetary Host Stars , 2007 .
[117] D. Lin,et al. Toward a Deterministic Model of Planetary Formation. I. A Desert in the Mass and Semimajor Axis Distributions of Extrasolar Planets , 2004 .
[118] C. Snodgrass,et al. The abundance of Galactic planets from OGLE-III 2002 microlensing data , 2004, astro-ph/0403387.
[119] Identification of the OGLE-2003-BLG-235/MOA-2003-BLG-53 Planetary Host Star* , 2006, astro-ph/0606038.
[120] Daniel Foreman-Mackey,et al. emcee: The MCMC Hammer , 2012, 1202.3665.
[121] K. Ulaczyk,et al. One or more bound planets per Milky Way star from microlensing observations , 2012, Nature.
[122] Scott J. Kenyon,et al. Planet Formation around Stars of Various Masses: The Snow Line and the Frequency of Giant Planets , 2007, 0710.1065.
[123] B. Monard,et al. THE EXTREME MICROLENSING EVENT OGLE-2007-BLG-224: TERRESTRIAL PARALLAX OBSERVATION OF A THICK-DISK BROWN DWARF , 2009, 0904.0249.
[124] John Asher Johnson,et al. THE TRENDS HIGH-CONTRAST IMAGING SURVEY. IV. THE OCCURRENCE RATE OF GIANT PLANETS AROUND M DWARFS , 2013, 1307.5849.
[125] M. J. Lehner,et al. First Observation of Parallax in a Gravitational Microlensing Event , 1995, astro-ph/9506114.
[126] K. Ulaczyk,et al. SPITZER AS A MICROLENS PARALLAX SATELLITE: MASS MEASUREMENT FOR THE OGLE-2014-BLG-0124L PLANET AND ITS HOST STAR , 2014, 1410.4219.
[127] Kaspar von Braun,et al. STELLAR DIAMETERS AND TEMPERATURES. IV. PREDICTING STELLAR ANGULAR DIAMETERS , 2013, 1311.4901.
[128] D. Hogg,et al. EXOPLANET POPULATION INFERENCE AND THE ABUNDANCE OF EARTH ANALOGS FROM NOISY, INCOMPLETE CATALOGS , 2014, 1406.3020.