EWS 2005-BLG-71 , the SIMBAD biblio

EWS 2005-BLG-71 , the SIMBAD biblio (58 results) C.D.S. - SIMBAD4 rel 1.8 - 2024.04.19CEST04:52:07

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Bibcode/DOI Score in Title|Abstract|
Keywords 		in a table in teXt, Caption, ... Nb occurence Nb objects in ref Citations
(from ADS) 		Title First 3 Authors
2005ApJ...628L.109U 23 3 213 A Jovian-mass planet in microlensing event OGLE-2005-BLG-071. UDALSKI A., JAROSZYNSKI M., PACZYNSKI B., et al.
2006ApJ...642..842D 5 11 110 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 17 8 275 Microlens OGLE-2005-BLG-169 implies that cool Neptune-like planets are common. GOULD A., UDALSKI A., AN D., et al.
2006ApJ...647L.171B 6 8 104 Identification of the OGLE-2003-BLG-235/MOA-2003-BLG-53 planetary host star. BENNETT D.P., ANDERSON J., BOND I.A., et al.
2007A&A...466..157S viz 34 0 Spectroscopic and light curve characterization of bulge microlensing events. SOTO M., MINNITI D. and REJKUBA M.
2007ApJ...660..823M 110 111 Formation of earth-like planets during and after giant planet migration. MANDELL A.M., RAYMOND S.N. and SIGURDSSON S.
2007AcA....57..281S 16 16 Binary lenses in OGLE III EWS database. Season 2005. SKOWRON J., JAROSZYNSKI M., UDALSKI A., et al.
2008ApJ...681.1593G 19 2 79 Hexadecapole approximation in planetary microlensing. GOULD A.
2008ApJ...687.1339K 237 103 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.
2009ApJ...690.1772P 191           X C F     3 16 80 Extended-source effect and chromaticity in two-point-mass microlensing. PEJCHA O.R. and HEYROVSKY D.
2009ApJ...694..107B 38           X         1 11 11 Analytical solutions for radiative transfer: implications for giant planet formation by disk instability. BOSS A.P.
2009ApJ...695..970D 195           X C F     3 13 164 OGLE-2005-BLG-071Lb, the most massive M dwarf planetary companion? DONG S., GOULD A., UDALSKI 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.
2009A&A...508..467B 38           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.
2010ApJ...710.1800G 39           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 192       S   X         4 19 52 An efficient method for modeling high-magnification planetary microlensing events. BENNETT D.P.
2010ApJ...717..435H 38           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 30 287 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.
2010AcA....60..197J 38           X         1 63 12 Binary lenses in OGLE-III EWS database. Seasons 2006-2008. JAROSZYNSKI M., SKOWRON J., UDALSKI A., et al.
2011MNRAS.412..607P 78           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 77           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.
2012NewAR..56...25B 116           X         3 30 1 The first extrasolar planet detected via gravitational microlensing. BOND I.A.
2012ApJ...755..102Y 50           X         1 7 161 MOA-2011-BLG-293Lb: a test of pure survey microlensing planet detections. YEE J.C., SHVARTZVALD Y., GAL-YAM A., et al.
2013A&A...552A.119S viz 16       D               1 1487 118 Magnetic energy fluxes in sub-Alfvenic planet star and moon planet interactions. SAUR J., GRAMBUSCH T., DULING S., et al.
2013ApJ...768..126G 78           X         2 12 8 OGLE-2011-BLG-0417: a radial velocity testbed for microlensing. GOULD A., SHIN I.-G., HAN C., et al.
2014MNRAS.437.4006S 159           X C       3 2 8 Degeneracies in triple gravitational microlensing. SONG Y.-Y., MAO S. and AN J.H.
2014ApJ...782...47P 39           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.
2014A&A...562A.108S viz 16       D               1 196 44 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...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.
2015ApJ...802..108S 199     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 41           X         1 13 35 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 42           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 40           X         1 5 8 Lens masses and distances from microlens parallax and flux. YEE J.C.
2016ApJ...821..121Y 40           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.
2016MNRAS.457.1320T viz 81             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.
2016ApJ...827L..22T 16       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 16       D               1 38 33 Is the galactic bulge devoid of planets? PENNY M.T., HENDERSON C.B. and CLANTON C.
2016ApJ...833..145S 42           X         1 64 176 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.
2017AJ....154...59B 41           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 16       D               1 12 8 Ground-based parallax confirmed by Spitzer: binary microlensing event MOA-2015-BLG-020. WANG T., ZHU W., MAO S., et al.
2018AJ....155...40R 42           X         1 17 21 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 82             C       1 20 5 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 41           X         1 21 4 OGLE-2017-BLG-0039: microlensing event with light from a lens identified from mass measurement. HAN C., JUNG Y.K., UDALSKI A., et al.
2020AJ....159...68B 1005 T   A     X C       22 26 ~ Keck observations confirm a super-Jupiter planet orbiting M dwarf

OGLE-2005-BLG-071L. 		BENNETT D.P., BHATTACHARYA A., BEAULIEU J.-P., et al.
2020ApJ...890...23L viz 17       D               1 4935 35 Current population statistics do not favor photoevaporation over core-powered mass loss as the dominant cause of the exoplanet radius gap. LOYD R.O.P., SHKOLNIK E.L., SCHNEIDER A.C., et al.
2020AJ....160...64H 43           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 viz 43           X         1 29 ~ 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 170           X         4 23 ~ OGLE-2018-BLG-0532Lb: cold Neptune with possible jovian sibling. RYU Y.-H., UDALSKI A., YEE J.C., et al.
2021AJ....161..293J viz 45           X         1 27 27 OGLE-2018-BLG-0567Lb and OGLE-2018-BLG-0962Lb: two microlensing planets through the planetary-caustic channel. JUNG Y.K., HAN C., UDALSKI A., et al.
2021A&A...649A..90H viz 87             C       1 22 ~ KMT-2018-BLG-1025Lb: microlensing super-Earth planet orbiting a low-mass star. HAN C., UDALSKI A., LEE C.-U., et al.
2021AJ....162...60B 87           X         2 9 ~ MOA-2007-BLG-400 a super-Jupiter-mass planet orbiting a Galactic bulge K-dwarf revealed by Keck adaptive optics imaging. BHATTACHARYA A., BENNETT D.P., BEAULIEU J.P., et al.
2021AJ....162..180Y 46           X         1 16 39 OGLE-2019-BLG-0960 lb: the smallest microlensing planet. YEE J.C., ZANG W., UDALSKI A., et al.
2022NatAs...6..121C 18       D               1 115 8 Microlensing mass measurement from images of rotating gravitational arcs. CASSAN A., RANC C., ABSIL O., et al.
2022A&A...664A..13G 45           X         1 21 18 Systematic KMTNet planetary anomaly search. V. Complete sample of 2018 prime-field. GOULD A., HAN C., ZANG W., et al.
2023AJ....165..206B 75     A     X         2 3 ~ Confirmation of Color-dependent Centroid Shift Measured After 1.8 Years with HST. BHATTACHARYA A., BENNETT D.P., BEAULIEU J.P., et al.
2023AJ....165..226J 47           X         1 26 4 Systematic KMTNet Planetary Anomaly Search. VIII. Complete Sample of 2019 Subprime Field Planets. JUNG Y.K., ZANG W., WANG H., et al.
2023AJ....166..145G 47           X         1 18 ~ OGLE-2016-BLG-1195 AO: Lens, Companion to Lens or Source, or None of the Above? GOULD A., SHVARTZVALD Y., ZHANG J., et al.

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