MOA 2011-BLG-291 , the SIMBAD biblio

MOA 2011-BLG-291 , the SIMBAD biblio (6 results) C.D.S. - SIMBAD4 rel 1.8 - 2026.10.15CEST16:37:09


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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....156..113B 787 T   A     X C       18 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.
2019MNRAS.488.3308L 41           X         1 5 2 OGLE-2017-BLG-1186: first application of asteroseismology and Gaussian processes to microlensing. LI S.-S., ZANG W., UDALSKI A., 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.
2021AJ....162...17K viz 17       D               1 54 ~ KMT-2019-BLG-0371 and the limits of Bayesian analysis. KIM Y.H., CHUNG S.-J., YEE J.C., 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.

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