J1214+0453
Four-hundred Very Metal-poor Stars Studied with LAMOST and Subaru. II. Elemental Abundances
| Teff : 6371+-153 | log g : 4.17+-0.05 | vturb : 1.29+-0.24 |
| 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 | ... | 2.15+-0.10 | 2.15+-0.10 | -1.11+-0.10 | 1.90+-0.10 | 2.15+-0.10 | Li I |
| C | ... | <1.40 | <6.82 | <-1.61 | <1.40 | <6.82 | C | |
| Na I | 2 | ... | -0.27+-0.07 | 2.96+-0.07 | -3.28+-0.07 | -0.27+-0.07 | 2.96+-0.07 | Na I |
| Mg I | 4 | ... | 0.32+-0.13 | 4.91+-0.13 | -2.69+-0.13 | 0.32+-0.13 | 4.91+-0.13 | Mg I |
| Ca I | 3 | ... | 0.26+-0.15 | 3.59+-0.15 | -2.75+-0.15 | 0.26+-0.15 | 3.59+-0.15 | Ca I |
| Sc II | 1 | ... | 0.03+-0.11 | 0.17+-0.11 | -2.98+-0.11 | 0.03+-0.11 | 0.17+-0.11 | Sc II |
| Ti II | 8 | ... | 0.31+-0.16 | 2.25+-0.16 | -2.70+-0.16 | 0.31+-0.16 | 2.25+-0.16 | Ti II |
| Cr I | 3 | ... | -0.21+-0.10 | 2.42+-0.10 | -3.22+-0.10 | -0.21+-0.10 | 2.42+-0.10 | Cr I |
| Fe I | 25 | ... | -0.00+-0.09 | 4.49+-0.09 | -3.01+-0.09 | -0.00+-0.09 | 4.49+-0.09 | Fe I |
| Fe II | 3 | ... | -0.14+-0.17 | 4.35+-0.17 | -3.15+-0.17 | -0.14+-0.17 | 4.35+-0.17 | Fe II |
| Sr II | 1 | ... | -0.30+-0.10 | -0.44+-0.10 | -3.31+-0.10 | -0.30+-0.10 | -0.44+-0.10 | Sr II |
| Right Ascension : 12 14 39.91 | Declination : +04 53 47.97 | 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 | 37.8 | N/A | 202.6 |
| N/A | N/A | SUBARUHDS | 36000 | 42.9 | N/A | 202.0 |