SMSSJ010839.58-285701.5
/H.R.Jacobson et al.(2015)/ /A.F.Marino et al.(2019)/
High-Resolution Spectroscopic Study of Extremely Metal-Poor Star Candidates from the SkyMapper Survey
Teff : 4855 | log g : 1.55 | vturb : 1.90 |
Original Data | Converted Data Asplund et al. (2009) | |||||||
---|---|---|---|---|---|---|---|---|
Element | Nline | [X/H] | [X/Fe] | log-e | [X/H] | [X/Fe] | log-e | Element |
Li | 1 | ... | ... | 0.80 | -2.46 | 0.56 | 0.80 | Li |
C | 2 | -2.80 | 0.22 | 5.62 | -2.81 | 0.21 | 5.62 | C |
Na | 2 | -2.05 | 0.97 | 4.19 | -2.05 | 0.97 | 4.19 | Na |
Mg | 5 | -2.57 | 0.45 | 5.03 | -2.57 | 0.45 | 5.03 | Mg |
Al | 1 | -3.51 | -0.49 | 2.94 | -3.51 | -0.49 | 2.94 | Al |
Si | 1 | -2.53 | 0.49 | 4.98 | -2.53 | 0.49 | 4.98 | Si |
Ca | 15 | -2.60 | 0.42 | 3.74 | -2.60 | 0.42 | 3.74 | Ca |
Sc | 1 | -2.95 | 0.07 | 0.20 | -2.95 | 0.07 | 0.20 | Sc |
Ti I | 10 | -2.79 | 0.24 | 2.17 | -2.78 | 0.24 | 2.17 | Ti I |
Ti II | 29 | -2.71 | 0.31 | 2.24 | -2.71 | 0.31 | 2.24 | Ti II |
Cr I | 4 | -3.26 | -0.24 | 2.38 | -3.26 | -0.24 | 2.38 | Cr I |
Mn | 3 | -3.20 | -0.18 | 2.23 | -3.20 | -0.18 | 2.23 | Mn |
Fe I | 169 | -3.02 | 0.00 | 4.48 | -3.02 | 0.00 | 4.48 | Fe I |
Fe II | 11 | -3.02 | -0.00 | 4.48 | -3.02 | -0.00 | 4.48 | Fe II |
Co | 4 | -2.86 | 0.16 | 2.13 | -2.86 | 0.16 | 2.13 | Co |
Ni | 4 | -3.04 | -0.02 | 3.18 | -3.04 | -0.02 | 3.18 | Ni |
Zn | 2 | -2.70 | 0.32 | 1.86 | -2.70 | 0.32 | 1.86 | Zn |
Sr | 2 | -3.31 | -0.29 | -0.43 | -3.30 | -0.28 | -0.43 | Sr |
Ba | 2 | -3.27 | -0.25 | -1.08 | -3.26 | -0.24 | -1.08 | Ba |
Eu | 1 | <-2.67 | <0.35 | <-2.15 | <-2.67 | <0.35 | <-2.15 | Eu |
Vrad | 137.7 |
Right Ascension : 01 08 39.58 | Declination : -28 57 01.5 | Galactic Longitude (l) : N/A | Galactic Latitude (b) : N/A |
Date of Observation | JD | Facility | Resolution | S/N | Exposure Time | Vrad |
---|---|---|---|---|---|---|
2013-01-08 | N/A | MIKELCO | 28000 | 42-56 | 600 | 137.7 |
Keck HIRES spectroscopy of SkyMapper commissioning survey candidate extremely metal-poor stars
Teff : 4936 | log g : 1.86 | vturb : 1.68 |
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 | ... | 0.12+-0.01 | ... | -2.78+-0.01 | 0.12+-0.01 | 5.65+-0.01 | C |
Na I | 2 | ... | 0.71+-0.11 | ... | -2.19+-0.11 | 0.71+-0.11 | 4.05+-0.11 | Na I |
Mg I | 3 | ... | 0.40+-0.15 | ... | -2.50+-0.15 | 0.40+-0.15 | 5.10+-0.15 | Mg I |
Al I | 2 | ... | -0.22+-0.09 | ... | -3.12+-0.09 | -0.22+-0.09 | 3.33+-0.09 | Al I |
Si I | 2 | ... | 0.74+-0.27 | ... | -2.16+-0.27 | 0.74+-0.27 | 5.35+-0.27 | Si I |
Ca I | 1 | ... | 0.43 | ... | -2.47 | 0.43 | 3.87 | Ca I |
Ti I | 7 | ... | 0.37+-0.11 | ... | -2.53+-0.11 | 0.37+-0.11 | 2.42+-0.11 | Ti I |
Ti II | 6 | ... | 0.34+-0.08 | ... | -2.56+-0.08 | 0.34+-0.08 | 2.39+-0.08 | Ti II |
Cr I | 2 | ... | -0.20+-0.03 | ... | -3.10+-0.03 | -0.20+-0.03 | 2.54+-0.03 | Cr I |
Mn | 3 | ... | -0.59+-0.16 | ... | -3.49+-0.16 | -0.59+-0.16 | 1.94+-0.16 | Mn |
Fe I | 33 | -2.90+-0.13 | ... | ... | -2.90+-0.13 | ... | 4.60+-0.13 | Fe I |
Fe II | 1 | -2.91 | ... | ... | -2.91 | ... | 4.59 | Fe II |
Co I | 9 | ... | 0.24+-0.22 | ... | -2.66+-0.22 | 0.24+-0.22 | 2.33+-0.22 | Co I |
Zn I | 2 | ... | 0.57+-0.00 | ... | -2.33+-0.00 | 0.57+-0.00 | 2.23+-0.00 | Zn I |
Sr II | 2 | ... | 0.07+-0.01 | ... | -2.83+-0.01 | 0.07+-0.01 | 0.04+-0.01 | Sr II |
Ba II | 2 | ... | -0.41+-0.11 | ... | -3.31+-0.11 | -0.41+-0.11 | -1.13+-0.11 | Ba II |
Eu II | N/A | ... | <0.30 | ... | <-2.60 | <0.30 | <-2.08 | Eu II |
Vrad | 144.3 |
Right Ascension : 01 08 39.58 | Declination : -28 57 01.5 | 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 | KECKHIRES | 50000 | 34-35 | 300 | 144.3 |