SMSSJ135625.09-161538.7
High-Resolution Spectroscopic Study of Extremely Metal-Poor Star Candidates from the SkyMapper Survey
| Teff : 4765 | log g : 1.50 | vturb : 2.00 |
| Original Data | Converted Data Asplund et al. (2009) | |||||||
|---|---|---|---|---|---|---|---|---|
| Element | Nline | [X/H] | [X/Fe] | log-e | [X/H] | [X/Fe] | log-e | Element |
| C | 2 | -2.58 | 0.18 | 5.85 | -2.58 | 0.18 | 5.85 | C |
| Na | 1 | -2.49 | 0.27 | 3.75 | -2.49 | 0.27 | 3.75 | Na |
| Mg | 5 | -2.35 | 0.41 | 5.25 | -2.35 | 0.41 | 5.25 | Mg |
| Al | 1 | -4.05 | -1.29 | 2.40 | -4.05 | -1.29 | 2.40 | Al |
| Si | 1 | -2.16 | 0.60 | 5.35 | -2.16 | 0.60 | 5.35 | Si |
| Ca | 9 | -2.40 | 0.36 | 3.94 | -2.40 | 0.36 | 3.94 | Ca |
| Sc | 1 | -3.17 | -0.41 | -0.02 | -3.17 | -0.41 | -0.02 | Sc |
| Ti I | 9 | -2.65 | 0.11 | 2.30 | -2.65 | 0.11 | 2.30 | Ti I |
| Ti II | 33 | -2.45 | 0.31 | 2.50 | -2.45 | 0.31 | 2.50 | Ti II |
| Cr I | 7 | -3.08 | -0.32 | 2.56 | -3.08 | -0.32 | 2.56 | Cr I |
| Mn | 2 | -3.01 | -0.25 | 2.42 | -3.01 | -0.25 | 2.42 | Mn |
| Fe I | 124 | -2.76 | 0.00 | 4.74 | -2.76 | 0.00 | 4.74 | Fe I |
| Fe II | 9 | -2.75 | 0.01 | 4.75 | -2.75 | 0.01 | 4.75 | Fe II |
| Co | 3 | -3.06 | -0.31 | 1.93 | -3.06 | -0.30 | 1.93 | Co |
| Ni | 1 | -2.67 | 0.09 | 3.55 | -2.67 | 0.09 | 3.55 | Ni |
| Zn | 1 | -2.35 | 0.41 | 2.21 | -2.35 | 0.41 | 2.21 | Zn |
| Sr | 2 | -3.42 | -0.66 | -0.55 | -3.42 | -0.66 | -0.55 | Sr |
| Ba | 2 | -2.91 | -0.15 | -0.72 | -2.90 | -0.14 | -0.72 | Ba |
| Eu | 1 | <-2.42 | <0.34 | <-1.90 | <-2.42 | <0.34 | <-1.90 | Eu |
| Vrad | 294.0 |
| Right Ascension : 13 56 25.09 | Declination : -16 15 38.7 | Galactic Longitude (l) : N/A | Galactic Latitude (b) : N/A |
| Date of Observation | JD | Facility | Resolution | S/N | Exposure Time | Vrad |
|---|---|---|---|---|---|---|
| 2012-05-12 | N/A | MIKELCO | 35000 | 25-41 | 2600 | 294.0 |