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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