MOA 2010-BLG-117 , the SIMBAD biblio

MOA 2010-BLG-117 , the SIMBAD biblio (18 results) C.D.S. - SIMBAD4 rel 1.8 - 2026.10.16CEST05:01:57

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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
2016ApJ...833..145S 135       D     X         4 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.
2018AJ....155..141B 523           X C       12 7 9 The first planetary microlensing event with two microlensed source stars. BENNETT D.P., UDALSKI A., HAN C., et al.
2018AJ....155..263S 80           X         2 16 8 A likely detection of a two-planet system in a low-magnification microlensing event. SUZUKI D., BENNETT D.P., UDALSKI A., et al.
2018AJ....156..113B 40           X         1 21 9 A planetary microlensing event with an unusually red source star: MOA-2011-BLG-291. BENNETT D.P., UDALSKI A., BOND I.A., et al.
2019AJ....157..232R 41           X         1 22 1 OGLE-2015-BLG-1670Lb: a cold Neptune beyond the snow line in the provisional WFIRST microlensing survey Field. RANC C., BENNETT D.P., HIRAO Y., et al.
2020ApJ...890...23L viz 16       D               1 4936 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.
2021A&A...649A..91H 125     A D     X         4 26 ~ KMT-2019-BLG-0797: Binary-lensing event occurring on a binary stellar system. HAN C., LEE C.-U., RYU Y.-H., et al.
2021A&A...652A.145H 84           X         2 15 ~ KMT-2018-BLG-1743: planetary microlensing event occurring on two source stars. HAN C., ALBROW M.D., CHUNG S.-J., et al.
2022A&A...658A..93H 43           X         1 31 10 OGLE-2019-BLG-0468Lb,c: Two microlensing giant planets around a G-type star. HAN C., UDALSKI A., LEE C.-U., et al.
2022NatAs...6..121C 17       D               1 115 8 Microlensing mass measurement from images of rotating gravitational arcs. CASSAN A., RANC C., ABSIL O., et al.
2022A&A...663A.145H 153     A     X         4 16 7 KMT-2021-BLG-1898: Planetary microlensing event involved with binary source stars. HAN C., GOULD A., KIM D., et al.
2022A&A...664A.114H 85           X         2 19 7 KMT-2021-BLG-0240: Microlensing event with a deformed planetary signal. HAN C., KIM D., YANG H., et al.
2023A&A...670A.172H 17       D               1 23 1 OGLE-2018-BLG-0584 and KMT-2018-BLG-2119: Two microlensing events with two lens masses and two source stars. HAN C., UDALSKI A., JUNG Y.K., et al.
2023A&A...678A.101H 44           X         1 21 ~ KMT-2021-BLG-1547Lb: Giant microlensing planet detected through a signal deformed due to source binarity. HAN C., ZANG W., JUNG Y.K., et al.
2024AJ....168...15B 179           X         4 23 ~ Keck and Hubble Observations Show that MOA-2008-BLG-379Lb is a Super-Jupiter Orbiting an M Dwarf. BENNETT D.P., BHATTACHARYA A., BEAULIEU J.-P., et al.
2024A&A...692A.221H 18       D               1 31 ~ KMT-2021-BLG-0284, KMT-2022-BLG-2480, and KMT-2024-BLG-0412: Three microlensing events involving two lens masses and two source stars. HAN C., UDALSKI A., BOND I.A., et al.
2025A&A...700A.181H 47           X         1 23 ~ KMT-2024-BLG-0404L: A triple microlensing system consisting of a star, a brown dwarf, and a planet. HAN C., UDALSKI A., LEE C.-U., et al.
2025PASP..137j4501H 47           X         1 34 ~ Three Binary-source Binary-lens Microlensing Events from the 2024 Microlensing Campaign. HAN C., LEE C.-U., UDALSKI A., et al.

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