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Table 3

Microlensing planets with masses of less than 10 M.

Planet Mplanet (M) Mhost (M) Reference and comment
OGLE-2005-BLG-390Lb Beaulieu et al. (2006)
       
MOA-2007-BLG-192Lb Bennett et al. (2008)
       
OGLE-2013-BLG-0341Lb 1.66 ± 0.18 (solution 1) 0.11 ± 0.01 (solution 1) Gould et al. (2014)
       
2.32 ± 0.27 (solution 2) 0.15 ± 0.01 (solution 2)
       
OGLE-2016-BLG-1195Lb Bond et al. (2017), Shvartzvald et al. (2017)
       
OGLE-2016-BLG-1928L ~0.1–1.0 Mróz et al. (2020), free-floating planet
       
OGLE-2017-BLG-1434Lb 4.4 ± 0.5 0.23 ± 0.03 Udalski et al. (2018), Blackman et al. (2021)
       
KMT-2018-BLG-0029Lb Gould et al. (2020)
       
OGLE-2018-BLG-0532Lb (solution 1) (solution 1) Ryu et al. (2020)
       
(solution 2) (solution 2) Ryu et al. (2020)
       
OGLE-2018-BLG-0677Lb Herrera-Martín et al. (2020)
       
OGLE-2018-BLG-0977Lb Hwang et al. (2022)
       
KMT-2018-BLG-1025Lb (solution 1) (solution 1) Han et al. (2021a)
       
(solution 2) (solution 2)
       
KMT-2018-BLG-1988Lb This work
       
       
OGLE-2018-BLG-1185Lb Kondo et al. (2021)
       
KMT-2019-BLG-0253Lb Hwang et al. (2022)
       
KMT-2019-BLG-0842Lb 10.3 ± 5.5 0.76 ± 0.40 Jung et al. (2020b)
       
KMT-2019-BLG-0960Lb 1.4 – 3.1 0.3 – 0.6 Yee et al. (2021)
       
OGLE-2019-BLG-1053Lb Zang et al. (2021b)
       
KMT-2020-BLG-0414LAb 1.0 ± 0.3 0.3 ± 0.1 Zang et al. (2021a), planet in a binary

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