J0728+3112
Four-hundred Very Metal-poor Stars Studied with LAMOST and Subaru. II. Elemental Abundances
| Teff : 6390+-117 | log g : 4.34+-0.03 | vturb : 1.44+-0.21 |
| 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 | ... | 2.46+-0.15 | 2.46+-0.15 | -0.80+-0.15 | 1.18+-0.15 | 2.46+-0.15 | Li I |
| C | ... | <0.80 | <7.25 | <-1.18 | <0.80 | <7.25 | C | |
| Na I | 2 | ... | -0.25+-0.11 | 4.01+-0.11 | -2.23+-0.11 | -0.25+-0.11 | 4.01+-0.11 | Na I |
| Mg I | 2 | ... | 0.26+-0.11 | 5.88+-0.11 | -1.72+-0.11 | 0.26+-0.11 | 5.88+-0.11 | Mg I |
| Ca I | 17 | ... | 0.28+-0.12 | 4.64+-0.12 | -1.70+-0.12 | 0.28+-0.12 | 4.64+-0.12 | Ca I |
| Sc II | 2 | ... | 0.41+-0.30 | 1.58+-0.30 | -1.57+-0.30 | 0.41+-0.30 | 1.58+-0.30 | Sc II |
| Ti II | 13 | ... | 0.43+-0.16 | 3.40+-0.16 | -1.55+-0.16 | 0.43+-0.16 | 3.40+-0.16 | Ti II |
| Cr I | 5 | ... | -0.25+-0.08 | 3.41+-0.08 | -2.23+-0.08 | -0.25+-0.08 | 3.41+-0.08 | Cr I |
| Fe I | 71 | ... | 0.00+-0.15 | 5.52+-0.15 | -1.98+-0.15 | 0.00+-0.15 | 5.52+-0.15 | Fe I |
| Fe II | 6 | ... | -0.13+-0.15 | 5.39+-0.15 | -2.11+-0.15 | -0.13+-0.15 | 5.39+-0.15 | Fe II |
| Ni I | 1 | ... | -0.10+-0.15 | 4.14+-0.15 | -2.08+-0.15 | -0.10+-0.15 | 4.14+-0.15 | Ni I |
| Sr II | 2 | ... | 0.49+-0.15 | 1.38+-0.15 | -1.49+-0.15 | 0.49+-0.15 | 1.38+-0.15 | Sr II |
| Ba II | 2 | ... | -0.32+-0.11 | -0.12+-0.11 | -2.30+-0.11 | -0.32+-0.11 | -0.12+-0.11 | Ba II |
| Right Ascension : 07 28 56.17 | Declination : +31 12 27.53 | 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 | 19.5 | N/A | 157.7 |