J1420+2305
Four-hundred Very Metal-poor Stars Studied with LAMOST and Subaru. II. Elemental Abundances
| Teff : 6442+-112 | log g : 4.10+-0.03 | vturb : 1.91+-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 |
| Na I | 2 | ... | -0.13+-0.62 | 3.60+-0.62 | -2.64+-0.62 | -0.13+-0.62 | 3.60+-0.62 | Na I |
| Mg I | 4 | ... | -0.06+-0.17 | 5.03+-0.17 | -2.57+-0.17 | -0.06+-0.17 | 5.03+-0.17 | Mg I |
| Ca I | 4 | ... | 0.65+-0.14 | 4.48+-0.14 | -1.86+-0.14 | 0.65+-0.14 | 4.48+-0.14 | Ca I |
| Sc II | 1 | ... | -0.22+-0.24 | 0.42+-0.24 | -2.73+-0.24 | -0.22+-0.24 | 0.42+-0.24 | Sc II |
| Ti II | 5 | ... | 0.20+-0.19 | 2.64+-0.19 | -2.31+-0.19 | 0.20+-0.19 | 2.64+-0.19 | Ti II |
| Cr I | 3 | ... | -0.23+-0.23 | 2.90+-0.23 | -2.74+-0.23 | -0.23+-0.23 | 2.90+-0.23 | Cr I |
| Fe I | 24 | ... | -0.00+-0.23 | 4.99+-0.23 | -2.51+-0.23 | -0.00+-0.23 | 4.99+-0.23 | Fe I |
| Fe II | 2 | ... | -0.25+-0.24 | 4.74+-0.24 | -2.76+-0.24 | -0.25+-0.24 | 4.74+-0.24 | Fe II |
| Sr II | 2 | ... | -0.42+-0.16 | -0.06+-0.16 | -2.93+-0.16 | -0.42+-0.16 | -0.06+-0.16 | Sr II |
| Ba II | 2 | ... | 0.09+-0.30 | -0.24+-0.30 | -2.42+-0.30 | 0.09+-0.30 | -0.24+-0.30 | Ba II |
| Right Ascension : 14 20 07.91 | Declination : +23 05 30.84 | 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 | 20.5 | N/A | -44.7 |
| N/A | N/A | SUBARUHDS | 36000 | 20.7 | N/A | -44.7 |