EWS 2005-BLG-71 , the SIMBAD biblio

EWS 2005-BLG-71 , the SIMBAD biblio (48 results) C.D.S. - SIMBAD4 rel 1.7 - 2021.04.19CEST08:44:46

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Title First 3 Authors
2020AJ....159...68B 1101 T   A     X C       22 26 ~ Keck observations confirm a super-Jupiter planet orbiting M dwarf

2020AJ....160...64H 47           X         1 10 ~ KMT-2019-BLG-1339L: an M dwarf with a giant planet or a companion near the Planet/Brown dwarf boundary. HAN C., KIM D., UDALSKI A., et al.
2020AJ....160...74H 47           X         1 27 ~ OGLE-2017-BLG-0406: Spitzer microlens parallax reveals Saturn-mass planet orbiting M-dwarf host in the inner Galactic disk. HIRAO Y., BENNETT D.P., RYU Y.-H., et al.
2020AJ....160..183R 187           X         4 23 ~ OGLE-2018-BLG-0532Lb: cold Neptune with possible jovian sibling. RYU Y.-H., UDALSKI A., YEE J.C., et al.
2018AJ....155...40R 44           X         1 17 10 OGLE-2016-BLG-1190Lb: the first Spitzer bulge planet lies near the planet/brown-dwarf boundary. RYU Y.-H., YEE J.C., UDALSKI A., et al.
2018AJ....156..236Z 87             C       1 20 ~ KMT-2016-BLG-1397b: KMTNET-only discovery of a microlens giant planet. ZANG W., HWANG K.-H., KIM H.-W., et al.
2018ApJ...867..136H 44           X         1 21 ~ OGLE-2017-BLG-0039: microlensing event with light from a lens identified from mass measurement. HAN C., JUNG Y.K., UDALSKI A., et al.
2017AJ....154...59B 43           X         1 30 10 The star blended with the MOA-2008-BLG-310 source is not the exoplanet host star. BHATTACHARYA A., BENNETT D.P., ANDERSON J., et al.
2017ApJ...845..129W 17       D               1 12 4 Ground-based parallax confirmed by Spitzer: binary microlensing event MOA-2015-BLG-020. WANG T., ZHU W., MAO S., et al.
2016ApJ...821..121Y 42           X         1 10 7 Two stars two ways: confirming a microlensing binary lens solution with a spectroscopic measurement of the orbit. YEE J.C., JOHNSON J.A., SKOWRON J., et al.
2016ApJ...827L..22T 17       D               2 44 4 An opportunistic search for extraterrestrial intelligence (SETI) with the murchison widefield array. TINGAY S.J., TREMBLAY C., WALSH A., et al.
2016ApJ...830..150P 17       D               1 38 25 Is the galactic bulge devoid of planets? PENNY M.T., HENDERSON C.B. and CLANTON C.
2016ApJ...833..145S 42           X         1 64 43 The exoplanet mass-ratio function from the MOA-II survey: discovery of a break and likely peak at a Neptune mass. SUZUKI D., BENNETT D.P., SUMI T., et al.
2016MNRAS.457.1320T viz 85             C       1 8 11 The OGLE-III planet detection efficiency from six years of microlensing observations (2003-2008). TSAPRAS Y., HUNDERTMARK M., WYRZYKOWSKI L., et al.
2015ApJ...802..108S 206     A D     X         6 12 1 Constraint on additional planets in planetary systems discovered through the channel of high-magnification gravitational microlensing events. SHIN I.-G., HAN C., CHOI J.-Y., et al.
2015ApJ...809...74F 43           X         1 13 28 OGLE-2012-BLG-0563Lb: a saturn-mass planet around an M dwarf with the mass constrained by Subaru AO imaging. FUKUI A., GOULD A., SUMI T., et al.
2015ApJ...810..155Y 46           X         1 7 39 Criteria for sample selection to maximize planet sensitivity and yield from space-based microlens parallax surveys. YEE J.C., GOULD A., BEICHMAN C., et al.
2015ApJ...814L..11Y 42           X         1 5 8 Lens masses and distances from microlens parallax and flux. YEE J.C.
2014A&A...562A.108S viz 16       D               1 196 35 Search for 150 MHz radio emission from extrasolar planets in the TIFR GMRT Sky Survey. SIROTHIA S.K., LECAVELIER DES ETANGS A., GOPAL-KRISHNA, et al.
2014ApJ...782...47P 42           X         1 14 23 Super-massive planets around late-type stars–the case of OGLE-2012-BLG-0406Lb. POLESKI R., UDALSKI A., DONG S., et al.
2014ApJ...788..128K 16       D               1 20 18 OGLE-2008-BLG-355Lb: a massive planet around a late-type star. KOSHIMOTO N., UDALSKI A., SUMI T., et al.
2014MNRAS.437.4006S 166           X C       3 2 8 Degeneracies in triple gravitational microlensing. SONG Y.-Y., MAO S. and AN J.H.
2013A&A...552A.119S viz 16       D               1 1488 42 Magnetic energy fluxes in sub-Alfvenic planet star and moon planet interactions. SAUR J., GRAMBUSCH T., DULING S., et al.
2013ApJ...768..126G 80           X         2 12 8 OGLE-2011-BLG-0417: a radial velocity testbed for microlensing. GOULD A., SHIN I.-G., HAN C., et al.
2012ApJ...755..102Y 45           X         1 7 83 MOA-2011-BLG-293Lb: a test of pure survey microlensing planet detections. YEE J.C., SHVARTZVALD Y., GAL-YAM A., et al.
2012NewAR..56...25B 119           X         3 30 1 The first extrasolar planet detected via gravitational microlensing. BOND I.A.
2011MNRAS.412..607P 80           X         2 10 28 Detectability of orbital motion in stellar binary and planetary microlenses. PENNY M.T., MAO S. and KERINS E.
2011MNRAS.413.1244H 79           X         2 10 1 OGLE-2009-BLG-023/MOA-2009-BLG-028: characterization of a binary microlensing event based on survey data. HWANG K.-H., HAN C., UDALSKI A., et al.
2010AcA....60..197J 39           X         1 63 12 Binary lenses in OGLE-III EWS database. Seasons 2006-2008. JAROSZYNSKI M., SKOWRON J., UDALSKI A., et al.
2010ApJ...710.1800G 40           X         1 7 24 A second method to photometrically align multi-site microlensing light curves: source color in planetary event MOA-2007-BLG-192. GOULD A., DONG S., BENNETT D.P., et al.
2010ApJ...716.1408B 196       S   X         4 19 52 An efficient method for modeling high-magnification planetary microlensing events. BENNETT D.P.
2010ApJ...717..435H 39           X         1 13 4 Determining the physical lens parameters of the binary gravitational microlensing event MOA-2009-BLG-016. HWANG K.-H., HAN C., BOND I.A., et al.
2010ApJ...720.1073G 42           X         1 30 211 Frequency of solar-like systems and of ice and gas giants beyond the snow line from high-magnification microlensing events in 2005-2008. GOULD A., DONG S., GAUDI B.S., et al.
2009A&A...508..467B 39           X         1 17 17 Mass measurement of a single unseen star and planetary detection efficiency. for OGLE 2007-BLG-050. BATISTA V., DONG S., GOULD A., et al.
2009AN....330....4T 4 7 59 RoboNet-II: Follow-up observations of microlensing events with a robotic network of telescopes. TSAPRAS Y., STREET R., HORNE K., et al.
2009ApJ...690.1772P 194           X C F     3 16 49 Extended-source effect and chromaticity in two-point-mass microlensing. PEJCHA O.R. and HEYROVSKY D.
2009ApJ...694..107B 39           X         1 11 11 Analytical solutions for radiative transfer: implications for giant planet formation by disk instability. BOSS A.P.
2009ApJ...695..970D 196           X C F     3 13 88 OGLE-2005-BLG-071Lb, the most massive M dwarf planetary companion? DONG S., GOULD A., UDALSKI A., et al.
2008ApJ...681.1593G 11 2 47 Hexadecapole approximation in planetary microlensing. GOULD A.
2008ApJ...687.1339K 237 77 Extrasolar giant planets and X-ray activity. KASHYAP V.L., DRAKE J.J. and SAAR S.H.
2008ApJ...689...53H 12 17 A characteristic planetary feature in double-peaked, high-magnification microlensing events. HAN C. and GAUDI B.S.
2007A&A...466..157S viz 34 0 Spectroscopic and light curve characterization of bulge microlensing events. SOTO M., MINNITI D. and REJKUBA M.
2007AcA....57..281S 16 16 Binary lenses in OGLE III EWS database. Season 2005. SKOWRON J., JAROSZYNSKI M., UDALSKI A., et al.
2007ApJ...660..823M 110 82 Formation of earth-like planets during and after giant planet migration. MANDELL A.M., RAYMOND S.N. and SIGURDSSON S.
2006ApJ...642..842D 3 11 84 Planetary detection efficiency of the magnification 3000 microlensing event OGLE-2004-BLG-343. DONG S., DEPOY D.L., GAUDI B.S., et al.
2006ApJ...644L..37G 13 8 212 Microlens OGLE-2005-BLG-169 implies that cool Neptune-like planets are common. GOULD A., UDALSKI A., AN D., et al.
2006ApJ...647L.171B 3 8 56 Identification of the OGLE-2003-BLG-235/MOA-2003-BLG-53 planetary host star. BENNETT D.P., ANDERSON J., BOND I.A., et al.
2005ApJ...628L.109U 28 3 168 A Jovian-mass planet in microlensing event OGLE-2005-BLG-071. UDALSKI A., JAROSZYNSKI M., PACZYNSKI B., et al.

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