OGLE-2011-BLG-0203 , the SIMBAD biblio

OGLE-2011-BLG-0203 , the SIMBAD biblio (8 results) C.D.S. - SIMBAD4 rel 1.8 - 2026.10.16CEST18:16:02

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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...820....4S 575     A     X C       14 4 9
MOA-2011-BLG-028Lb: a neptune-mass microlensing planet in the Galactic Bulge. 		SKOWRON J., UDALSKI A., POLESKI R., et al.
2016ApJ...833..145S 17       D               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 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.
2018ApJS..239...14J viz 16       D               1 1561 6 Revised exoplanet radii and habitability using Gaia data release 2. JOHNS D., MARTI C., HUFF M., et al.
2019AJ....157...72J 16       D               1 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.
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....161..293J viz 85             C       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.
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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