Table 1.
Li abundances for the microlensed bulge dwarfs.
| Name | Nr | A(Li) | A(Li)l | A(Li)h | ΔNLTE | Flag |
|---|---|---|---|---|---|---|
| ⋮ | ⋮ | ⋮ | ⋮ | ⋮ | ⋮ | ⋮ |
| MOA-2010-BLG-167S | 910167 | 1.27 | 1.22 | 1.31 | 0.08 | 0 |
| ⋮ | ⋮ | ⋮ | ⋮ | ⋮ | ⋮ | ⋮ |
Notes. For each star we give the NLTE corrected A(Li) abundance and the low and high values determined by changing the effective temperatures by their uncertainties. The Li NLTE corrections that were added are also given. The last column is a flag where the value “0” means that it is a value from a well-fitted line. A value of “1” means that the Li abundance is an upper limit. All other parameters are given in Bensby et al. (2017) in which the two identifiers (Name and Nr) are given in the same way for easy cross-matching. This table is only available in electronic form at the CDS.
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