BPS BS16084-160: found in 4 paper(s).
Labels:
/D.K.Lai et al.(2004)/
/W.Aoki et al.(2005)/
/D.K.Lai et al.(2007)/
/D.K.Lai et al.(2008)/
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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 |
Binarity
Photometric data
Atmospheric data
| Teff | 4762 |
| log g | 1.66 |
| vturb | -3.00 |
Chemical Abundances
| Element | Nline | [X/H] | [X/Fe] | log-e |
|---|
| Mg I | ... | -2.59 | 0.34 | 4.99 |
| Ca I | ... | -2.82 | 0.11 | 3.54 |
| Ti II | ... | -2.65 | 0.28 | 2.37 |
| Fe I | ... | -2.93 | ... | 4.57 |
| Ba II | ... | -4.64 | -1.71 | -2.51 |
: 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 | 102 | 40min | -118.71+-0.24 |
| Galactic Longitude (l) | N/A |
| Galactic Latitude (b) | N/A |
| Declination | +543703 |
| Right Ascension | 162850.7 |
Binarity
Photometric data
| V | 13.144 |
| B | 14.002 |
| H | 10.849 |
| J | 11.358 |
| K | 10.740 |
| EB-V | 0.00 |
Atmospheric data
| Teff | 4650 |
| log g | 1.1 |
| vturb | 2.2 |
Chemical Abundances
| Element | Nline | [X/H] | [X/Fe] | log-e |
|---|
| CH | ... | -3.00 | 0.1 | 5.2 |
| Mg I | ... | -2.78+-0.13 | 0.32+-0.13 | 4.8+-0.13 |
| Al I | ... | -3.46+-0.19 | -0.36+-0.19 | 3.03+-0.19 |
| Si I | ... | -2.47+-0.15 | 0.63+-0.15 | 5.09+-0.15 |
| Ca I | ... | -2.88+-0.13 | 0.22+-0.13 | 3.47+-0.13 |
| Ti I | ... | -3.14+-0.14 | -0.04+-0.14 | 1.8+-0.14 |
| Ti II | ... | -3.02+-0.25 | 0.08+-0.25 | 1.92+-0.25 |
| Cr I | ... | -3.62+-0.12 | -0.52+-0.12 | 2.07+-0.12 |
| Mn I | ... | -4.10+-0.13 | -1+-0.13 | 1.43+-0.13 |
| Fe I | ... | -3.1+-0.21 | ... | 4.4+-0.21 |
| Fe II | ... | -3.1+-0.2 | ... | 4.4+-0.2 |
| Co I | ... | -2.90+-0.12 | 0.2+-0.12 | 2.01+-0.12 |
| Ni I | ... | -3.18+-0.13 | -0.08+-0.13 | 3.07+-0.13 |
| Zn I | ... | <-2.88 | <0.22 | <1.79 |
| Sr II | ... | -5.44+-0.25 | -2.34+-0.25 | -2.52+-0.25 |
| Y II | ... | <-3.43 | <-0.33 | <-1.20 |
| Zr II | ... | <-3.42 | <-0.32 | <-0.81 |
| Ba II | ... | -5.45+-0.22 | -2.35+-0.22 | -3.23+-0.22 |
: 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 | ... | -3.08+-0.26 | -0.15+-0.26 | 5.47+-0.26 |
| Fe | ... | -2.93 | ... | 4.57 |
| Sr | ... | -4.90 | -1.97 | -1.93 |
| Ba | ... | <-4.64 | <-1.71 | <-2.51 |
: Data presented in the paper
: Data converted with the solar abundance from Grevesse et al. (1996)
A0181
| Title | Detailed Abundances for 28 Metal-poor Stars: Stellar Relics in the Milky Way |
| ADS | D.K.Lai et al.,ApJ, 681, 1524, 2008 |
| Authors | D. K. Lai, M. Bolte, J. A. Johnson, S. Lucatello |
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Basic Informations
| Observation Date | JD | Facility | Resolution | S/N | Exposure Time | Vrad |
|---|
| 2001-08-25 | N/A | KECKHIRES | N/A | 103 | 7200 | -123.2+-0.2 |
| 2004-04-09 | N/A | KECKHIRES | N/A | 140 | 1800 | -141.5+-0.2 |
| 2005-05-29 | N/A | KECKHIRES | N/A | 111 | 5400 | -126.6+-0.2 |
| Galactic Longitude (l) | N/A |
| Galactic Latitude (b) | N/A |
| Declination | N/A |
| Right Ascension | N/A |
Binarity
Photometric data
Atmospheric data
| Teff | 4728+-100 |
| log g | 1.26+-0.2 |
| vturb | 2.1+-0.2 |
Chemical Abundances
| Element | Nline | [X/H] | [X/Fe] | log-e |
|---|
| C | ... | -3.32+-0.22 | -0.12+-0.22 | 5.23+-0.22 |
| N | ... | -2.42+-0.30 | 0.78+-0.30 | 5.55+-0.30 |
| OH | ... | -2.93+-0.31 | 0.27+-0.31 | 5.94+-0.31 |
| Na | ... | -3.42+-0.10 | -0.22+-0.10 | 2.91+-0.10 |
| Mg | ... | -2.99+-0.05 | 0.21+-0.05 | 4.59+-0.05 |
| Al | ... | -4.17+-0.05 | -0.97+-0.05 | 2.30+-0.05 |
| Si | ... | -2.58+-0.15 | 0.62+-0.15 | 4.97+-0.15 |
| Ca | ... | -3.02+-0.05 | 0.18+-0.05 | 3.34+-0.05 |
| Sc II | ... | -3.11+-0.06 | 0.09+-0.06 | 0.06+-0.06 |
| Ti I | ... | -3.22+-0.07 | -0.02+-0.07 | 1.80+-0.07 |
| Ti II | ... | -3.11+-0.06 | 0.09+-0.06 | 1.91+-0.06 |
| V II | ... | -3.34+-0.07 | -0.14+-0.07 | 0.66+-0.07 |
| Cr I | ... | -3.62+-0.06 | -0.42+-0.06 | 2.05+-0.06 |
| Mn I | ... | -3.75+-0.09 | -0.55+-0.09 | 1.64+-0.09 |
| Mn II | ... | -3.64+-0.07 | -0.44+-0.07 | 1.75+-0.07 |
| Fe I | ... | -3.20+-0.09 | ... | 4.30+-0.09 |
| Fe II | ... | -3.26+-0.08 | ... | 4.24+-0.08 |
| Co | ... | -3.11+-0.08 | 0.09+-0.08 | 1.81+-0.08 |
| Ni | ... | -3.33+-0.07 | -0.13+-0.07 | 2.92+-0.07 |
| Cu | ... | -4.84+-0.10 | -1.64+-0.10 | -0.63+-0.10 |
| Sr II | ... | -5.30+-0.18 | -2.10+-0.18 | -2.33+-0.18 |
| Ba II | ... | -5.19+-0.10 | -1.99+-0.10 | -3.06+-0.10 |
| Eu II | ... | <-3.45 | <-0.25 | <-2.94 |
: Data presented in the paper
: Data converted with the solar abundance from Grevesse et al. (1996)