SMSSJ202659.41-031149.2
taken from 1 paper(s):
/A.F.Marino et al.(2019)/

Keck HIRES spectroscopy of SkyMapper commissioning survey candidate extremely metal-poor stars
Stellar Parameters
| Teff : 4918 | log g : 1.80 | vturb : 1.74 |
Chemical Abundances
| | 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 | ... | -0.06+-0.03 | ... | -3.00+-0.03 | -0.06+-0.03 | 5.43+-0.03 | C |
| Na I | 2 | ... | 0.44+-0.03 | ... | -2.50+-0.03 | 0.44+-0.03 | 3.74+-0.03 | Na I |
| Mg I | 2 | ... | 0.42+-0.12 | ... | -2.52+-0.12 | 0.42+-0.12 | 5.08+-0.12 | Mg I |
| Al I | 2 | ... | -0.54+-0.23 | ... | -3.48+-0.23 | -0.54+-0.23 | 2.97+-0.23 | Al I |
| Si I | 2 | ... | 0.75+-0.32 | ... | -2.19+-0.32 | 0.75+-0.32 | 5.32+-0.32 | Si I |
| Ca I | 2 | ... | 0.39+-0.01 | ... | -2.55+-0.01 | 0.39+-0.01 | 3.79+-0.01 | Ca I |
| Sc II | 1 | ... | 0.41 | ... | -2.53 | 0.41 | 0.62 | Sc II |
| Ti I | 2 | ... | 0.39+-0.16 | ... | -2.55+-0.16 | 0.39+-0.16 | 2.40+-0.16 | Ti I |
| Ti II | 7 | ... | 0.43+-0.17 | ... | -2.51+-0.17 | 0.43+-0.17 | 2.44+-0.17 | Ti II |
| Cr I | 3 | ... | -0.12+-0.15 | ... | -3.06+-0.15 | -0.12+-0.15 | 2.58+-0.15 | Cr I |
| Mn | 3 | ... | -0.84+-0.03 | ... | -3.78+-0.03 | -0.84+-0.03 | 1.65+-0.03 | Mn |
| Fe I | 30 | -2.94+-0.14 | ... | ... | -2.94+-0.14 | ... | 4.56+-0.14 | Fe I |
| Fe II | 2 | -2.84+-0.17 | ... | ... | -2.84+-0.17 | ... | 4.66+-0.17 | Fe II |
| Co I | 8 | ... | 0.32+-0.23 | ... | -2.62+-0.23 | 0.32+-0.23 | 2.37+-0.23 | Co I |
| Sr II | 2 | ... | -1.94+-0.06 | ... | -4.88+-0.06 | -1.94+-0.06 | -2.01+-0.06 | Sr II |
| Ba II | 1 | ... | -1.69+-0.00 | ... | -4.63+-0.00 | -1.69+-0.00 | -2.45+-0.00 | Ba II |
| Eu II | N/A | ... | <0.10 | ... | <-2.84 | <0.10 | <-2.32 | Eu II |
Binary Parameters
Position
| Right Ascension : | Declination : | Galactic Longitude (l) : | Galactic Latitude (b) : |
Observing Log
| Date of Observation | JD | Facility | Resolution | S/N | Exposure Time | Vrad |
| N/A | N/A | KECKHIRES | 50000 | 28-29 | 600 | -199.1 |