NAME EWS 2005-BLG-169b , the SIMBAD biblio

NAME EWS 2005-BLG-169b , the SIMBAD biblio (42 results) C.D.S. - SIMBAD4 rel 1.8 - 2026.10.17CEST10:11:41


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Title First 3 Authors
2006ApJ...644L..37G 11 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 4 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.
2007ApJ...660..781B 1 8 43 Characterization of gravitational microlensing planetary host stars. BENNETT D.P., ANDERSON J. and GAUDI B.S.
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.
2007A&A...474..293B viz 3         O           21 204 The HARPS search for southern extra-solar planets. X. A msini=11M{earth} planet around the nearby spotted M dwarf GJ 674. BONFILS X., MAYOR M., DELFOSSE X., et al.
2008A&A...483..317K 75           X         2 9 24 Limits on additional planetary companions to OGLE 2005-BLG-390L. KUBAS D., CASSAN A., DOMINIK M., et al.
2008A&A...491..587C 37           X         1 16 23 An alternative parameterisation for binary-lens caustic-crossing events. CASSAN A.
2008ApJ...689...53H 12 17 A characteristic planetary feature in double-peaked, high-magnification microlensing events. HAN C. and GAUDI B.S.
2008ApJ...689.1084K 8 2 Limits of binaries that can be characterized by gravitational microlensing. KIM D., RYU Y.-H., PARK B.-G., et al.
2009ApJ...691..452H 37           X         1 9 8 Microlensing zone of planets detectable through the channel of high-magnification events. HAN C.
2009MNRAS.396.2087H 37           X         1 10 15 A metric and optimization scheme for microlens planet searches. HORNE K., SNODGRASS C. and TSAPRAS Y.
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...505..859Z viz 37           X         1 60 114 The M dwarf planet search programme at the ESO VLT + UVES. A search for terrestrial planets in the habitable zone of M dwarfs. ZECHMEISTER M., KUERSTER M. and ENDL M.
2010ApJ...709..149S 53       D     X         2 33 29 Models of Neptune-mass exoplanets: emergent fluxes and albedos. SPIEGEL D.S., BURROWS A., IBGUI L., et al.
2010ApJ...711..731J 118           X         3 10 105 Sub-Saturn planet MOA-2008-BLG-310Lb: likely to Be in the Galactic Bulge. JANCZAK J., FUKUI A., DONG S., et al.
2010MNRAS.401.1691M 76           X         2 9 35 On the formation of hot Neptunes and super-Earths. McNEIL D.S. and NELSON R.P.
2010ApJ...719.1454M 81           X         2 1 12 The invisible majority? Evolution and detection of outer planetary systems without gas giants. MANN A.W., GAIDOS E. and GAUDI B.S.
2010ApJ...720.1073G 132       D     X         4 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.
2010MNRAS.406.1918D 15       D               2 404 29 The Hill stability of the possible moons of extrasolar planets. DONNISON J.R.
2011ApJ...728..120M 16       D               1 14 31 A Sub-Saturn mass planet, MOA-2009-BLG-319Lb. MIYAKE N., SUMI T., DONG S., et al.
2012NewAR..56...25B 53       D     X         2 30 1 The first extrasolar planet detected via gravitational microlensing. BOND I.A.
2012RAA....12..947M 16       D               1 23 52 Astrophysical applications of gravitational microlensing. MAO S.
2011PASP..123..412W viz 15       D               1 2897 398 The Exoplanet Orbit Database. WRIGHT J.T., KAKHOURI O., MARCY G.W., et al.
2013ApJ...763..141G 38           X         1 12 16 MOA-2010-BLG-523: "Failed planet" = RS CVn star. GOULD A., YEE J.C., BOND I.A., et al.
2013A&A...549A.109B viz 1 172 551 The HARPS search for southern extra-solar planets. XXXI. The M-dwarf sample. BONFILS X., DELFOSSE X., UDRY S., et al.
2013A&A...552A.119S viz 15       D               1 1487 118 Magnetic energy fluxes in sub-Alfvenic planet star and moon planet interactions. SAUR J., GRAMBUSCH T., DULING S., et al.
2013A&A...557A..42D 116           X         3 5 11 Terrestrial planets in high-mass disks without gas giants. DE ELIA G.C., GUILERA O.M. and BRUNINI A.
2014ApJ...788...73Z 15       D               1 28 24 Predictions for microlensing planetary events from core accretion theory. ZHU W., PENNY M., MAO S., et al.
2015ApJ...808..169B 76     A     X         2 4 113 Confirmation of the planetary microlensing signal and star and planet mass determinations for event OGLE-2005-BLG-169. BENNETT D.P., BHATTACHARYA A., ANDERSON J., et al.
2015ApJ...808..170B 159     A     X         4 3 117 Confirmation of the OGLE-2005-BLG-169 planet signature and its characteristics with lens-source proper motion detection. BATISTA V., BEAULIEU J.-P., BENNETT D.P., et al.
2017AJ....153..143M 16       D               1 53 15 OGLE-2016 a high-mass planet from a high-magnification pure-survey microlensing event. MROZ P., HAN C., UDALSKI A., et al.
2017AJ....154...59B 40           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.
2017MNRAS.469.2434B 40           X         1 16 24 The lowest mass ratio planetary microlens: OGLE 2016-BLG-1195Lb. BOND I.A., BENNETT D.P., SUMI T., et al.
2019AJ....157...72J 97       D       C       2 32 7 KMT-2017-BLG-0165Lb: a super-Neptune-mass planet orbiting a Sun-like host star. JUNG Y.K., GOULD A., ZANG W., et al.
2020AJ....160...17H 41           X         1 10 ~ One planet or two planets? The ultra-sensitive extreme-magnification microlensing event KMT-2019-BLG-1953. HAN C., KIM D., JUNG Y.K., et al.
2021AJ....161..279B 42           X         1 13 ~ OGLE-2017-BLG-1434Lb: confirmation of a cold super-Earth using Keck adaptive optics. BLACKMAN J.W., BEAULIEU J.-P., COLE A.A., et al.
2022A&A...662A..70H 43           X         1 16 9 KMT-2021-BLG-1077L: The fifth confirmed multiplanetary system detected by microlensing. HAN C., GOULD A., BOND I.A., et al.
2022AJ....164...75B viz 43           X         1 9 ~ MOA-2019-BLG-008Lb: A New Microlensing Detection of an Object at the Planet/Brown Dwarf Boundary. BACHELET E., TSAPRAS Y., GOULD A., et al.
2023AJ....165..103Z viz 87             C       1 45 8 Systematic KMTNet Planetary Anomaly Search. VII. Complete Sample of q < 10–4 Planets from the First 4 yr Survey. ZANG W., JUNG Y.K., YANG H., et al.
2023MNRAS.522.6055Z 44           X         1 16 1 KMT-2022-BLG-0440Lb: A new q < 10–4 microlensing planet with the central-resonant caustic degeneracy broken. ZHANG J., ZANG W., JUNG Y.K., et al.
2023A&A...675A..36H 44           X         1 20 ~ KMT-2021-BLG-1150Lb: Microlensing planet detected through a densely covered planetary-caustic signal. HAN C., JUNG Y.K., BOND I.A., et al.
2024AJ....168...24B 287       D S   X C       5 8 ~ Estimating Microlensing Parameters from Observables and Stellar Isochrones with pyLIMASS. BACHELET E., HUNDERTMARK M. and CALCHI NOVATI S.

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