J2323+0342
Four-hundred Very Metal-poor Stars Studied with LAMOST and Subaru. II. Elemental Abundances
| Teff : 6166+-129 | log g : 4.18+-0.05 | vturb : 1.81+-0.17 |
| Original Data | Converted Data Asplund et al. (2009) | |||||||
|---|---|---|---|---|---|---|---|---|
| Element | Nline | [X/H] | [X/Fe] | log-e | [X/H] | [X/Fe] | log-e | Element |
| Na I | 2 | ... | -0.38+-0.09 | 3.53+-0.09 | -2.71+-0.09 | -0.37+-0.09 | 3.53+-0.09 | Na I |
| Mg I | 2 | ... | 0.19+-0.10 | 5.46+-0.10 | -2.14+-0.10 | 0.20+-0.10 | 5.46+-0.10 | Mg I |
| Ca I | 13 | ... | 0.51+-0.16 | 4.52+-0.16 | -1.82+-0.16 | 0.52+-0.16 | 4.52+-0.16 | Ca I |
| Sc II | 5 | ... | 0.35+-0.19 | 1.17+-0.19 | -1.98+-0.19 | 0.36+-0.19 | 1.17+-0.19 | Sc II |
| Ti II | 15 | ... | 0.62+-0.14 | 3.24+-0.14 | -1.71+-0.14 | 0.63+-0.14 | 3.24+-0.14 | Ti II |
| Cr I | 5 | ... | -0.20+-0.06 | 3.11+-0.06 | -2.53+-0.06 | -0.19+-0.06 | 3.11+-0.06 | Cr I |
| Fe I | 48 | ... | -0.01+-0.12 | 5.16+-0.12 | -2.34+-0.12 | -0.01+-0.12 | 5.16+-0.12 | Fe I |
| Fe II | 6 | ... | 0.34+-0.25 | 5.51+-0.25 | -1.99+-0.25 | 0.34+-0.25 | 5.51+-0.25 | Fe II |
| Sr II | 2 | ... | 0.02+-0.17 | 0.56+-0.17 | -2.31+-0.17 | 0.03+-0.17 | 0.56+-0.17 | Sr II |
| Ba II | 2 | ... | 0.01+-0.19 | -0.14+-0.19 | -2.32+-0.19 | 0.02+-0.19 | -0.14+-0.19 | Ba II |
| Right Ascension : 23 23 13.56 | Declination : +03 42 54.55 | 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 | 19.4 | N/A | 109.5 |