Open Access

Table 1.

Microlensing events with four or more bodies.

Event Anomaly type Reference
OGLE-2006-BLG-109 3L1S (multiple planets) Gaudi et al. (2008), Bennett et al. (2010)
OGLE-2012-BLG-0026 3L1S (multiple planets) Han et al. (2013), Beaulieu et al. (2016)
OGLE-2018-BLG-1011 3L1S (multiple planets) Han et al. (2019)
OGLE-2019-BLG-0468 3L1S (multiple planets) Han et al. (2022f)
KMT-2021-BLG-1077 3L1S (multiple planets) Han et al. (2022a)
KMT-2021-BLG-0240 3L1S (multiple planets) Han et al. (2022d)

OGLE-2006-BLG-284 3L1S (binary+planet) Bennett et al. (2020)
OGLE-2007-BLG-349 3L1S (binary+planet) Bennett et al. (2016)
OGLE-2008-BLG-092 3L1S (binary+planet) Poleski et al. (2014)
OGLE-2016-BLG-0613 3L1S (binary+planet) Han et al. (2017)
OGLE-2018-BLG-1700 3L1S (binary+planet) Han et al. (2020)
KMT-2020-BLG-0414 3L1S (binary+planet) Zang et al. (2021)

KMT-2019-BLG-1715 3L2S (binary+planet) Han et al. (2021c)

MOA-2010-BLG-117 2L2S Bennett et al. (2018)
KMT-2018-BLG-1743 2L2S Han et al. (2021a)
OGLE-2016-BLG-1003 2L2S Jung et al. (2017)
KMT-2019-BLG-0797 2L2S Han et al. (2021b)
KMT-2021-BLG-1898 2L2S Han et al. (2022b)

Notes. In the case of KMT-2019-BLG-1715, the lens is composed of three masses and the source is a binary.

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