BPS BS16929-005: found in 6 paper(s).
Labels:
/S.Honda et al.(2004)/
/D.K.Lai et al.(2004)/
/S.Honda et al.(2004)/
/W.Aoki et al.(2007)/
/D.K.Lai et al.(2007)/
/D.K.Lai et al.(2008)/
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A0017
| Title | Spectroscopic Studies of Extremely Metal-Poor Stars with the Subaru High Dispersion Spectrograph. II. The r-Process Elements, Including Thorium |
| ADS | S.Honda et al.,ApJ, 607, 474, 2004 |
| Authors | S. Honda, W. Aoki, T. Kajino, H. Ando, T. C. Beers, H. Izumiura, K. Sadakane, M. Takada-Hidai |
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Basic Informations
| Observation Date | JD | Facility | Resolution | S/N | Exposure Time | Vrad |
|---|
| 2001-01-30 | N/A | SUBARUHDS | 50000 | 56 | 5400 | -51.29+-0.43 |
| Galactic Longitude (l) | N/A |
| Galactic Latitude (b) | N/A |
| Declination | N/A |
| Right Ascension | N/A |
Photometric data
| V | 13.61 |
| B | 14.23 |
| B-V | 0.62 |
| V-K | 1.91 |
| H | 11.75 |
| J | 12.17 |
| K | 11.67 |
| EB-V | 0.01 |
Atmospheric data
| Teff | 5270 |
| log g | 2.7 |
| vturb | 1.3 |
Chemical Abundances
| Element | Nline | [X/H] | [X/Fe] | log-e |
|---|
| CH | ... | -2.17 | 0.92 | 6.39 |
| Mg I | ... | -2.71+-0.32 | 0.38+-0.32 | 4.87+-0.32 |
| Al I | ... | -3.94+-0.16 | -0.85+-0.16 | 2.53+-0.16 |
| Si I | ... | -2.71+-0.16 | 0.38+-0.16 | 4.84+-0.16 |
| Ca I | ... | -2.63+-0.17 | 0.46+-0.17 | 3.73+-0.17 |
| Sc II | ... | -3.62+-0.16 | -0.53+-0.16 | -0.45+-0.16 |
| Ti | ... | -2.67+-0.12 | 0.42+-0.12 | 2.35+-0.12 |
| Mn I | ... | -3.83+-0.16 | -0.74+-0.16 | 1.56+-0.16 |
| Fe | ... | -3.09+-0.15 | ... | 4.52+-0.15 |
| Co I | ... | -2.73+-0.06 | 0.36+-0.06 | 2.19+-0.06 |
| Ni I | ... | -3.18+-0.16 | -0.09+-0.16 | 3.07+-0.16 |
| Sr II | ... | -2.81+-0.16 | 0.28+-0.16 | 0.11+-0.16 |
| Y II | ... | -2.93+-0.16 | 0.16+-0.16 | -0.7+-0.16 |
| Ba II | ... | -3.68+-0.16 | -0.59+-0.16 | -1.46+-0.16 |
: Data presented in the paper
: Data converted with the solar abundance from Grevesse et al. (1996)
Isotope ratio
A0022
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Basic Informations
| Observation Date | JD | Facility | Resolution | S/N | Exposure Time | Vrad |
|---|
| 2003-04-23 | N/A | KECKII | 7000 | 150 | 900 | N/A |
Binarity
Photometric data
Atmospheric data
| Teff | 5212 |
| log g | 2.78 |
| vturb | -3.25 |
Chemical Abundances
| Element | Nline | [X/H] | [X/Fe] | log-e |
|---|
| Mg I | ... | -2.64 | 0.63 | 4.94 |
| Ti II | ... | -2.74 | 0.53 | 2.28 |
| Fe I | ... | -3.27 | ... | 4.23 |
| Ba II | ... | -3.47 | -0.20 | -1.34 |
: Data presented in the paper
: Data converted with the solar abundance from Grevesse et al. (1996)
A0085
| Title | Spectroscopic Studies of Extremely Metal-Poor Stars with the Subaru High Dispersion Spectrograph. I. Observational Data |
| ADS | S.Honda et al.,ApJS, 152, 113, 2004 |
| Authors | S. Honda, W. Aoki, H. Ando, H. Izumiura, T. Kajino, E. Kambe, S. Kawanomoto, K. Noguchi, K. Okita, K. Sadakane, B. Sato, M. Takada-Hidai, Y. Takeda, E. Watanabe, T. C. Beers, J. E. Norris, S. G. Ryan |
Get more information of this paper.
Basic Informations
| Observation Date | JD | Facility | Resolution | S/N | Exposure Time | Vrad |
|---|
| 2001-01-30 | N/A | SUBARUHDS | 50000 | 56 | 5400 | -51.29+-0.43 |
| Galactic Longitude (l) | N/A |
| Galactic Latitude (b) | N/A |
| Declination | 335106 |
| Right Ascension | 130329.4 |
Binarity
Photometric data
A0122
| Title | Carbon-enhanced Metal-poor Stars. I. Chemical Compositions of 26 Stars |
| ADS | W.Aoki et al.,ApJ, 655, 492, 2007 |
| Authors | W. Aoki, T. Beers, N. Christlieb, J. E. Norris, S. G. Ryan, S. Tsangarides |
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Basic Informations
| Observation Date | JD | Facility | Resolution | S/N | Exposure Time | Vrad |
|---|
| 2003-05-25 | N/A | SUBARUHDS | 50000 | N/A | 600 | -50.4+-0.13 |
| Galactic Longitude (l) | N/A |
| Galactic Latitude (b) | N/A |
| Declination | +335106 |
| Right Ascension | 130329.4 |
Binarity
Photometric data
| V | 13.610 |
| B | 14.228 |
| H | 11.750 |
| J | 12.170 |
| K | 11.670 |
| EB-V | 0.01 |
Atmospheric data
| Teff | 5250 |
| log g | 2.8 |
| vturb | 2.3 |
Chemical Abundances
| Element | Nline | [X/H] | [X/Fe] | log-e |
|---|
| C | ... | -2.09+-0.16 | 1.08+-0.16 | 6.3+-0.16 |
| CN | ... | <-0.78+-0.07 | <2.39+-0.07 | <7.0+-0.07 |
| Na I | ... | -3.23+-0.17 | -0.06+-0.17 | 2.94+-0.17 |
| Mg I | ... | -2.68+-0.10 | 0.49+-0.10 | 4.85+-0.10 |
| Ca I | ... | -3.04+-0.09 | 0.13+-0.09 | 3.27+-0.09 |
| Ti II | ... | -2.73+-0.14 | 0.44+-0.14 | 2.17+-0.14 |
| Cr I | ... | -3.51+-0.09 | -0.34+-0.09 | 2.14+-0.09 |
| Fe I | ... | -3.17+-0.14 | ... | 4.28+-0.14 |
| Fe II | ... | -3.18+-0.13 | ... | 4.27+-0.13 |
| Ba II | ... | -3.65+-0.12 | -0.48+-0.12 | -1.48+-0.12 |
: 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 | ... | -2.22+-0.22 | 1.05+-0.22 | 6.33+-0.22 |
| Fe | ... | -3.27 | ... | 4.23 |
| Sr | ... | -2.75 | 0.52 | 0.22 |
| Ba | ... | -3.47 | -0.20 | -1.34 |
: 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 |
|---|
| 2003-06-06 | N/A | KECKHIRES | N/A | 108 | 1800 | -51.7+-0.2 |
| 2004-04-08 | N/A | KECKHIRES | N/A | 137 | 7200 | -51.3+-0.2 |
| 2004-04-09 | N/A | KECKHIRES | N/A | 117 | 2700 | -52.5+-0.5 |
| Galactic Longitude (l) | N/A |
| Galactic Latitude (b) | N/A |
| Declination | N/A |
| Right Ascension | N/A |
Photometric data
Atmospheric data
| Teff | 5245+-100 |
| log g | 2.70+-0.2 |
| vturb | 1.6+-0.2 |
Chemical Abundances
| Element | Nline | [X/H] | [X/Fe] | log-e |
|---|
| C | ... | -2.37+-0.23 | 0.97+-0.23 | 6.18+-0.23 |
| N | ... | -3.02+-0.32 | 0.32+-0.32 | 4.95+-0.32 |
| Na | ... | -3.35+-0.12 | -0.01+-0.12 | 2.98+-0.12 |
| Mg | ... | -2.89+-0.10 | 0.45+-0.10 | 4.69+-0.10 |
| Al | ... | -4.00+-0.06 | -0.66+-0.06 | 2.47+-0.06 |
| Ca | ... | -3.01+-0.04 | 0.33+-0.04 | 3.35+-0.04 |
| Sc II | ... | -3.37+-0.16 | -0.03+-0.16 | -0.20+-0.16 |
| Ti I | ... | -2.89+-0.06 | 0.45+-0.06 | 2.13+-0.06 |
| Ti II | ... | -2.84+-0.06 | 0.50+-0.06 | 2.18+-0.06 |
| V II | ... | -3.33+-0.17 | 0.01+-0.17 | 0.67+-0.17 |
| Cr I | ... | -3.84+-0.06 | -0.50+-0.06 | 1.83+-0.06 |
| Mn I | ... | -4.14+-0.10 | -0.80+-0.10 | 1.25+-0.10 |
| Fe I | ... | -3.34+-0.03 | ... | 4.16+-0.03 |
| Fe II | ... | -3.39+-0.11 | ... | 4.11+-0.11 |
| Co | ... | -2.96+-0.06 | 0.38+-0.06 | 1.96+-0.06 |
| Ni | ... | -3.26+-0.07 | 0.08+-0.07 | 2.99+-0.07 |
| Sr II | ... | -2.97+-0.08 | 0.37+-0.08 | 0.00+-0.08 |
| Y II | ... | -3.12+-0.07 | 0.22+-0.07 | -0.88+-0.07 |
| Zr II | ... | -2.81+-0.10 | 0.53+-0.10 | -0.21+-0.10 |
| Ba II | ... | -3.62+-0.10 | -0.28+-0.10 | -1.49+-0.10 |
| Eu II | ... | <-3.31 | <0.03 | <-2.80 |
: Data presented in the paper
: Data converted with the solar abundance from Grevesse et al. (1996)