J0102+1052
Four-hundred Very Metal-poor Stars Studied with LAMOST and Subaru. II. Elemental Abundances
| Teff : 5995+-120 | log g : 4.52+-0.04 | vturb : 0.30+-0.30 |
| Original Data | Converted Data Asplund et al. (2009) | |||||||
|---|---|---|---|---|---|---|---|---|
| Element | Nline | [X/H] | [X/Fe] | log-e | [X/H] | [X/Fe] | log-e | Element |
| Li I | 1 | ... | 2.00+-0.22 | 2.00+-0.22 | -1.26+-0.22 | 1.84+-0.22 | 2.00+-0.22 | Li I |
| Na I | 2 | ... | -0.57+-0.14 | 2.56+-0.14 | -3.68+-0.14 | -0.58+-0.14 | 2.56+-0.14 | Na I |
| Mg I | 2 | ... | 0.15+-0.14 | 4.64+-0.14 | -2.96+-0.14 | 0.14+-0.14 | 4.64+-0.14 | Mg I |
| Ca I | 1 | ... | -0.30+-0.19 | 2.93+-0.19 | -3.41+-0.19 | -0.31+-0.19 | 2.93+-0.19 | Ca I |
| Sc II | 1 | ... | 0.80+-0.20 | 0.84+-0.20 | -2.31+-0.20 | 0.79+-0.20 | 0.84+-0.20 | Sc II |
| Ti II | 1 | ... | 0.18+-0.20 | 2.02+-0.20 | -2.93+-0.20 | 0.17+-0.20 | 2.02+-0.20 | Ti II |
| Fe I | 14 | ... | 0.01+-0.19 | 4.40+-0.19 | -3.10+-0.19 | 0.01+-0.19 | 4.40+-0.19 | Fe I |
| Fe II | 2 | ... | 1.79+-0.27 | 6.18+-0.27 | -1.32+-0.27 | 1.79+-0.27 | 6.18+-0.27 | Fe II |
| Right Ascension : 01 02 35.03 | Declination : +10 52 45.47 | Galactic Longitude (l) : N/A | Galactic Latitude (b) : N/A |
| Date of Observation | JD | Facility | Resolution | S/N | Exposure Time | Vrad |
|---|---|---|---|---|---|---|
| N/A | N/A | SUBARUHDS | 36000 | 24.5 | N/A | -130.7 |