| J/A+A/512/A41/table5 | Abundances of microlensed stars in the Bulge (Bensby+, 2010) Abundances and uncertainties for each star (13 rows) | Name==MACHO-1999-BLG-022S |
| Column | Value | Explain (UCD) | |
| 5recno | 5 | Record number assigned by the VizieR team. Should Not be used for identification. (meta.record) | |
| Name | MACHO-1999-BLG-022S | Star name (meta.id;meta.main) | |
| [Fe/H] | -0.49 | [Sun] | Normalised abundance (phys.abund) |
| e_[Fe/H] | 0.14 | [Sun] | Error in abundance ratio (stat.error;phys.abund.Fe) |
| [O/Fe] | [Sun] | Normalised abundance (not NLTE corrected) (phys.abund) | |
| e_[O/Fe] | [Sun] | Error in abundance ratio (phys.abund) | |
| [Na/Fe] | 0.01 | [Sun] | Normalised abundance (phys.abund) |
| e_[Na/Fe] | 0.07 | [Sun] | Error in abundance ratio (phys.abund) |
| [Mg/Fe] | 0.35 | [Sun] | Normalised abundance (phys.abund) |
| e_[Mg/Fe] | 0.13 | [Sun] | Error in abundance ratio (phys.abund) |
| [Al/Fe] | 0.31 | [Sun] | Normalised abundance (phys.abund) |
| e_[Al/Fe] | 0.10 | [Sun] | Error in abundance ratio (phys.abund) |
| [Si/Fe] | 0.25 | [Sun] | Normalised abundance (phys.abund) |
| e_[Si/Fe] | 0.13 | [Sun] | Error in abundance ratio (phys.abund) |
| [Ca/Fe] | 0.18 | [Sun] | Normalised abundance (phys.abund) |
| e_[Ca/Fe] | 0.13 | [Sun] | Error in abundance ratio (phys.abund) |
| [Ti/Fe] | 0.25 | [Sun] | Normalised abundance (phys.abund) |
| e_[Ti/Fe] | 0.24 | [Sun] | Error in abundance ratio (phys.abund) |
| [Cr/Fe] | -0.03 | [Sun] | Normalised abundance (phys.abund) |
| e_[Cr/Fe] | 0.14 | [Sun] | Error in abundance ratio (phys.abund) |
| [Ni/Fe] | 0.00 | [Sun] | Normalised abundance (phys.abund) |
| e_[Ni/Fe] | 0.10 | [Sun] | Error in abundance ratio (phys.abund) |
| [Zn/Fe] | [Sun] | Normalised abundance (phys.abund) | |
| e_[Zn/Fe] | 0.19 | [Sun] | Error in abundance ratio (phys.abund) |
| [Y/Fe] | 0.01 | [Sun] | Normalised abundance (phys.abund) |
| e_[Y/Fe] | 0.31 | [Sun] | Error in abundance ratio (phys.abund) |
| [Ba/Fe] | 0.15 | [Sun] | Normalised abundance (phys.abund) |
| e_[Ba/Fe] | 0.12 | [Sun] | Error in abundance ratio (phys.abund) |
| e_[O/H] | [Sun] | Error in abundance ratio (stat.error;phys.abund) | |
| e_[Na/H] | 0.14 | [Sun] | Error in abundance ratio (stat.error;phys.abund) |
| e_[Mg/H] | 0.23 | [Sun] | Error in abundance ratio (stat.error;phys.abund) |
| e_[Al/H] | 0.06 | [Sun] | Error in abundance ratio (stat.error;phys.abund) |
| e_[Si/H] | 0.06 | [Sun] | Error in abundance ratio (stat.error;phys.abund) |
| e_[Ca/H] | 0.25 | [Sun] | Error in abundance ratio (stat.error;phys.abund) |
| e_[Ti/H] | 0.16 | [Sun] | Error in abundance ratio (stat.error;phys.abund) |
| e_[Cr/H] | 0.11 | [Sun] | Error in abundance ratio (stat.error;phys.abund) |
| e_[Ni/H] | 0.08 | [Sun] | Error in abundance ratio (stat.error;phys.abund) |
| e_[Zn/H] | 0.10 | [Sun] | Error in abundance ratio (stat.error;phys.abund) |
| e_[Y/H] | 0.22 | [Sun] | Error in abundance ratio (stat.error;phys.abund) |
| e_[Ba/H] | 0.15 | [Sun] | Error in abundance ratio (stat.error;phys.abund) |
| n(Fe) | 97 | Number of Fe lines used (meta.number) | |
| n(O) | Number of O lines used (meta.number) | ||
| n(Na) | 3 | Number of Na lines used (meta.number) | |
| n(Mg) | 1 | Number of Mg lines used (meta.number) | |
| n(Al) | 2 | Number of Al lines used (meta.number) | |
| n(Si) | 7 | Number of Si lines used (meta.number) | |
| n(Ca) | 16 | Number of Ca lines used (meta.number) | |
| n(Ti) | 14 | Number of Ti lines used (meta.number) | |
| n(Cr) | 2 | Number of Cr lines used (meta.number) | |
| n(Ni) | 21 | Number of Ni lines used (meta.number) | |
| n(Zn) | Number of Zn lines used (meta.number) | ||
| n(Y) | 2 | Number of Y lines used (meta.number) | |
| n(Ba) | 3 | Number of Ba lines used (meta.number) | |