BPS BS16080-054: found in 3 paper(s).
Labels:
/D.K.Lai et al.(2004)/
/W.Aoki et al.(2005)/
/D.K.Lai et al.(2007)/
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A0022
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Basic Informations
| Observation Date | JD | Facility | Resolution | S/N | Exposure Time | Vrad |
| 2001-07-7 | N/A | KECKII | 7000 | 150 | 450 | N/A |
Photometric data
Atmospheric data
| Teff | 4838 |
| log g | 1.83 |
| vturb | -2.75 |
Chemical Abundances
| Element | Nline | [X/H] | [X/Fe] | log-e |
| Mg I | ... | -2.06 | 0.68 | 5.52 |
| Ca I | ... | -2.42 | 0.32 | 3.94 |
| Ti II | ... | -1.87 | 0.87 | 3.15 |
| Fe I | ... | -2.74 | ... | 4.76 |
| Ba II | ... | -2.93 | -0.19 | -0.80 |
: Data presented in the paper
: Data converted with the solar abundance from Grevesse et al. (1996)
A0057
| Title | Spectroscopic Studies of Very Metal-poor Stars with the Subaru High Dispersion Spectrograph. III. Light Neutron-Capture Elements |
| ADS | W.Aoki et al.,ApJ, 632, 611, 2005 |
| Authors | W. Aoki, S. Honda, T. C. Beers, T. Kajino, H. Ando, J. E. Norris, S. G. Ryan, H. Izumiura, K. Sadakane, M. Takada-Hidai |
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Basic Informations
| Observation Date | JD | Facility | Resolution | S/N | Exposure Time | Vrad |
| 2001-07-23 | N/A | SUBARUHDS | 50000 | 89 | 20min | -120.80+-0.25 |
| Galactic Longitude (l) | N/A |
| Galactic Latitude (b) | N/A |
| Declination | +605742 |
| Right Ascension | 163918.5 |
Photometric data
| V | 12.776 |
| B | 13.550 |
| H | 10.604 |
| J | 11.082 |
| K | 10.504 |
| EB-V | 0.00 |
Atmospheric data
| Teff | 4800 |
| log g | 1.1 |
| vturb | 2.4 |
Chemical Abundances
| Element | Nline | [X/H] | [X/Fe] | log-e |
| C | ... | -2.99 | -0.1 | 4.64 |
| Mg | ... | -2.23+-0.10 | 0.66+-0.10 | 5.35+-0.10 |
| Al | ... | -3.23+-0.17 | -0.34+-0.17 | 3.26+-0.17 |
| Si | ... | -2.37+-0.12 | 0.52+-0.12 | 5.19+-0.12 |
| Ca | ... | -2.52+-0.10 | 0.37+-0.10 | 3.83+-0.10 |
| Sc | ... | -2.93+-0.23 | -0.04+-0.23 | 0.17+-0.23 |
| Ti I | ... | -2.64+-0.11 | 0.25+-0.11 | 2.30+-0.11 |
| Ti II | ... | -2.57+-0.24 | 0.32+-0.24 | 2.37+-0.24 |
| Cr | ... | -3.26+-0.11 | -0.37+-0.11 | 2.43+-0.11 |
| Mn | ... | -3.73+-0.14 | -0.84+-0.14 | 1.80+-0.14 |
| Fe I | ... | -2.89+-0.20 | ... | 4.61+-0.20 |
| Fe II | ... | -2.87+-0.18 | ... | 5.4+-0.18 |
| Co | ... | -2.70+-0.12 | 0.19+-0.12 | 2.21+-0.12 |
| Ni | ... | -3.00+-0.10 | -0.11+-0.10 | 3.25+-0.10 |
| Zn | ... | -2.59+-0.21 | 0.30+-0.21 | 2.08+-0.21 |
| Sr | ... | -2.64+-0.15 | 0.25+-0.15 | 0.28+-0.15 |
| Y | ... | -2.95+-0.24 | -0.06+-0.24 | -0.72+-0.24 |
| Zr | ... | -2.49+-0.24 | 0.40+-0.24 | 0.12+-0.24 |
| Ba | ... | -3.65+-0.23 | -0.76+-0.23 | -1.43+-0.23 |
| Nd | ... | -3.23+-0.24 | -0.34+-0.24 | -1.74+-0.24 |
| Eu | ... | -3.01+-0.24 | -0.12+-0.24 | -2.46+-0.24 |
: Data presented in the paper
: Data converted with the solar abundance from Grevesse et al. (1996)
A0128
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Basic Informations
| Observation Date | JD | Facility | Resolution | S/N | Exposure Time | Vrad |
| N/A | N/A | KECKII | 7000 | N/A | N/A | N/A |
Atmospheric data
Chemical Abundances
| Element | Nline | [X/H] | [X/Fe] | log-e |
| C | ... | -3.24+-0.26 | -0.50+-0.26 | 5.31+-0.26 |
| Fe | ... | -2.74 | ... | 4.76 |
| Sr | ... | -2.15 | 0.59 | 0.82 |
| Ba | ... | -2.93 | -0.19 | -0.80 |
: Data presented in the paper
: Data converted with the solar abundance from Grevesse et al. (1996)