MOA 2003-BLG-53b , the SIMBAD biblio

MOA 2003-BLG-53b , the SIMBAD biblio (26 results) C.D.S. - SIMBAD4 rel 1.8 - 2026.10.14CEST10:24:11

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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
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.
2007LAstr.121...17C 7 0 Des planetes extra-solaires revelees par effet de microlentille gravitationnelle. CASSAN A.
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 40         O X         1 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...491..587C 16 23 An alternative parameterisation for binary-lens caustic-crossing events. CASSAN A.
2009AJ....137..329J 37           X         1 9 9 Construction of coupled period-mass functions in extrasolar planets through a nonparametric approach. JIANG I.-G., YEH L.-C., CHANG Y.-C., et al.
2009ApJ...695..970D 43           X         1 13 164 OGLE-2005-BLG-071Lb, the most massive M dwarf planetary companion? DONG S., GOULD A., UDALSKI A., et al.
2010ApJ...716.1408B 39           X         1 19 52 An efficient method for modeling high-magnification planetary microlensing events. BENNETT D.P.
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.
2010MNRAS.406.1918D 15       D               1 404 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.
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.
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.
2013ApJ...768..126G 38           X         1 12 8 OGLE-2011-BLG-0417: a radial velocity testbed for microlensing. GOULD A., SHIN I.-G., HAN C., et al.
2014ApJ...782...47P 77           X         2 14 23 Super-massive planets around late-type stars–the case of OGLE-2012-BLG-0406Lb. POLESKI R., UDALSKI A., DONG S., et al.
2014MNRAS.439..604S 39           X         1 15 29 MOA-2011-BLG-322Lb: a `second generation survey' microlensing planet. SHVARTZVALD Y., MAOZ D., KASPI S., et al.
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.
2017AJ....153..143M 175       D     X C       4 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....3K 41           X         1 7 24 MOA-2016-BLG-227Lb: a massive planet characterized by combining light-curve analysis and Keck AO imaging. KOSHIMOTO N., SHVARTZVALD Y., BENNETT D.P., et al.
2022MNRAS.515.5927S 17       D               1 37 1 Earth through the looking glass: how frequently are we detected by other civilizations through photometric microlensing? SUPHAPOLTHAWORN S., AWIPHAN S., CHATCHADANORASET T., et al.
2023AJ....165..206B 44           X         1 3 ~ Confirmation of Color-dependent Centroid Shift Measured After 1.8 Years with HST. BHATTACHARYA A., BENNETT D.P., BEAULIEU J.P., 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....167..145R 63       D     X         2 14 ~ Precise Mass Measurement of OGLE-2013-BLG-0132/MOA-2013-BLG-148: A Saturn-mass Planet Orbiting an M Dwarf. REKTSINI N.E., BATISTA V., RANC C., et al.

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