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Table 2
Posterior distributions for the lens mass calculated from the Bayesian analysis.
| Percentile | 2.3th | 15.9th | 50.0th | 84.1th | 97.7th |
|---|---|---|---|---|---|
| Prior 1 | |||||
| OGLE-2012-BLG-1323 | 1.2 M⊕ | 5.0 M⊕ | 12 M⊕ | 47 M⊕ | 480 M⊕ |
| OGLE-2017-BLG-0560 | 5.7 MJup | 24 MJup | 100 MJup | 0.40 M⊙ | 0.75 M⊙ |
| OGLE-2016-BLG-1540 | 22 M⊕ | 110 M⊕ | 1.5 MJup | 47 MJup | 58 MJup |
| Prior 2 | |||||
| OGLE-2012-BLG-1323 | 3.8 M⊕ | 7.8 M⊕ | 30 M⊕ | 240 M⊕ | 990 M⊕ |
| OGLE-2017-BLG-0560 | 1.1 MJup | 13 MJup | 77 MJup | 0.35 M⊙ | 0.74 M⊙ |
| OGLE-2016-BLG-1540 | 32 M⊕ | 120 M⊕ | 2 MJup | 40 MJup | 53 MJup |
Notes. We use the Galactic model of Bennett et al. (2014) and the planetary mass function d N∕d M ∝ M−1.8 (prior 1) or d N∕dM ∝ M−1.3 (prior 2).
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