BPS CS22952-015: found in 10 paper(s).
Labels:
/R.Cayrel et al.(2004)/
/S.Honda et al.(2004)/
/M.Spite et al.(2005)/
/A.McWilliam et al.(1995)/
/A.McWilliam et al.(1995)/
/P.S.Barklem et al.(2005)/
/S.Honda et al.(2004)/
/M.Spite et al.(2006)/
/S.M.Andrievsky et al.(2007)/
/S.M.Andrievsky et al.(2008)/
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A0016
Title | First stars V - Abundance patterns from C to Zn and supernova yields in the early Galaxy |
ADS | R.Cayrel et al.,AAP, 416, 1117, 2004 |
Authors | R. Cayrel, E. Depagne, M. Spite, V. Hill, F. Spite, P. Francois, B. Plez, T. Beers, F. Primas, J. Andersen, B. Barbuy, P. Bonifacio, P. Molaro, B. Nordstrom |
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Basic Informations
Observation Date | JD | Facility | Resolution | S/N | Exposure Time | Vrad |
2000-10 | N/A | VLT | 47000 | 150 | 10200 | N/A |
Galactic Longitude (l) | N/A |
Galactic Latitude (b) | N/A |
Declination | N/A |
Right Ascension | N/A |
Binarity
Photometric data
V | 13.28 |
B-V | 0.77 |
V-R | 0.73 |
J-K | 0.56 |
V-K | 2.34 |
EB-V | 0.01 |
Atmospheric data
Teff | 4800 |
log g | 1.3 |
vturb | 2.1 |
Chemical Abundances
Element | Nline | [X/H] | [X/Fe] | log-e |
Mg I | ... | -3.43+-0.08 | 0.00+-0.08 | 4.15+-0.08 |
Al I | ... | -3.89 | -0.46 | 2.58 |
Si I | ... | -3.10 | 0.33 | 4.45 |
K I | ... | -2.94 | 0.49 | 2.18 |
Ca I | ... | -3.29+-0.14 | 0.14+-0.14 | 3.07+-0.14 |
Sc II | ... | -3.54+-0.05 | -0.11+-0.05 | -0.37+-0.05 |
Ti I | ... | -3.33+-0.09 | 0.10+-0.09 | 1.69+-0.09 |
Ti II | ... | -3.43+-0.11 | 0.00+-0.11 | 1.59+-0.11 |
Cr I | ... | -3.89+-0.15 | -0.46+-0.15 | 1.78+-0.15 |
Mn I | ... | -3.76+-0.16 | -0.33+-0.16 | 1.63+-0.16 |
Fe I | ... | -3.45+-0.14 | -0.02+-0.14 | 4.05+-0.14 |
Fe II | ... | -3.41+-0.10 | 0.02+-0.10 | 4.09+-0.10 |
Co I | ... | -3.30+-0.10 | 0.13+-0.10 | 1.62+-0.10 |
Ni I | ... | -3.55+-0.10 | -0.12+-0.10 | 2.70+-0.10 |
Zn I | ... | -3.18 | 0.25 | 1.42 |
: Data presented in the paper
: Data converted with the solar abundance from Grevesse et al. (1996)
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 |
2000-11-11 | N/A | SUBARUHDS | 50000 | 59 | 9000 | -20.07+-0.71 |
Galactic Longitude (l) | N/A |
Galactic Latitude (b) | N/A |
Declination | N/A |
Right Ascension | N/A |
Photometric data
V | 13.27 |
B | 14.05 |
B-V | 0.78 |
V-K | 2.23 |
H | 11.02 |
J | 11.49 |
K | 10.92 |
EB-V | 0.04 |
Atmospheric data
Teff | 4850 |
log g | 1.5 |
vturb | 1.5 |
Chemical Abundances
Element | Nline | [X/H] | [X/Fe] | log-e |
CH | ... | -3.16 | -0.22 | 5.4 |
Mg I | ... | -3.13+-0.21 | -0.19+-0.21 | 4.45+-0.21 |
Al I | ... | -3.62+-0.19 | -0.68+-0.19 | 2.85+-0.19 |
Si I | ... | -2.55+-0.19 | 0.39+-0.19 | 5+-0.19 |
Ca I | ... | -2.91+-0.16 | 0.03+-0.16 | 3.45+-0.16 |
Sc II | ... | -3.30+-0.06 | -0.36+-0.06 | -0.13+-0.06 |
Ti | ... | -3.06+-0.06 | -0.12+-0.06 | 1.96+-0.06 |
V | ... | -2.97+-0.19 | -0.03+-0.19 | 1.03+-0.19 |
Mn I | ... | -3.28+-0.39 | -0.34+-0.39 | 2.11+-0.39 |
Fe | ... | -2.94+-0.26 | ... | 4.57+-0.26 |
Co I | ... | -2.88+-0.19 | 0.06+-0.19 | 2.04+-0.19 |
Ni I | ... | -3.05+-0.19 | -0.11+-0.19 | 3.2+-0.19 |
Sr II | ... | -3.65+-0.19 | -0.71+-0.19 | -0.73+-0.19 |
Ba II | ... | -4.71+-0.19 | -1.77+-0.19 | -2.49+-0.19 |
: Data presented in the paper
: Data converted with the solar abundance from Grevesse et al. (1996)
A0025
Title | First stars VI – Abundances of C, N, O, Li, and mixing in extremely metal-poor giants. Galactic evolution of the light elements |
ADS | M.Spite et al.,AAP, 430, 655, 2005 |
Authors | M. Spite, R. Cayrel, B. Plez, V. Hill, F. Spite, E. Depagne, P. Francois, P. Bonifacio, B. Barbuy, T. Beers, J. Andersen, P. Molaro, B. Nordstrom, F. Primas |
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Basic Informations
Observation Date | JD | Facility | Resolution | S/N | Exposure Time | Vrad |
N/A | N/A | VLT | 47000 | 30 | N/A | N/A |
Galactic Longitude (l) | N/A |
Galactic Latitude (b) | N/A |
Declination | N/A |
Right Ascension | N/A |
Photometric data
Atmospheric data
Teff | 4800 |
log g | 1.3 |
vturb | 2.1 |
Chemical Abundances
Element | Nline | [X/H] | [X/Fe] | log-e |
Li I | ... | <-1.56 | <1.87 | <-0.40 |
C | ... | -4.02+-0.08 | -0.59+-0.08 | 4.53+-0.08 |
N | ... | -2.12 | 1.31 | 5.85 |
Fe | ... | -3.43 | ... | 4.07 |
: Data presented in the paper
: Data converted with the solar abundance from Grevesse et al. (1996)
A0038
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Basic Informations
Observation Date | JD | Facility | Resolution | S/N | Exposure Time | Vrad |
N/A | N/A | FRUTTI | 22000 | N/A | N/A | N/A |
Photometric data
V | 13.26 |
B-V | 0.767 |
V-R | 0.505 |
A0039
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Basic Informations
Observation Date | JD | Facility | Resolution | S/N | Exposure Time | Vrad |
| N/A | FRUTTI | 22000 | N/A | N/A | N/A |
Galactic Longitude (l) | N/A |
Galactic Latitude (b) | N/A |
Declination | N/A |
Right Ascension | N/A |
Photometric data
V | 13.26 |
B-V | 0.767 |
V-R | 0.505 |
Atmospheric data
Teff | 4720 |
log g | 0.90+-0.27 |
vturb | 2.55+-0.08 |
Chemical Abundances
Element | Nline | [X/H] | [X/Fe] | log-e |
C | ... | -3.48 | -0.10 | 5.07 |
Na | ... | -3.56 | -0.18 | 2.77 |
Mg | ... | -3.71 | -0.33 | 3.87 |
Ca | ... | -3.04 | 0.34 | 3.32 |
Fe I | ... | -3.38 | ... | 4.12 |
Fe II | ... | -3.42 | ... | 4.08 |
Ni | ... | -3.37 | 0.01 | 2.88 |
Sr | ... | -4.32 | -0.94 | -1.35 |
Ba | ... | -4.83 | -1.45 | -2.70 |
: Data presented in the paper
: Data converted with the solar abundance from Grevesse et al. (1996)
A0052
Title | The Hamburg/ESO R-process enhanced star survey (HERES). II. Spectroscopic analysis of the survey sample |
ADS | P.S.Barklem et al.,AAP, 439, 129, 2005 |
Authors | P. S. Barklem, N. Christlieb, T. C. Beers, V. Hill, M. S. Bessell, J. Holmberg, B. Marsteller, S. Rossi, F. -J. Zickgraf, D. Reimers |
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Basic Informations
Observation Date | JD | Facility | Resolution | S/N | Exposure Time | Vrad |
N/A | N/A | VLT | 20000 | 72 | N/A | -18.5 |
Photometric data
Atmospheric data
Teff | 4820 |
log g | 1.51 |
vturb | 2.15 |
Chemical Abundances
Element | Nline | [X/H] | [X/Fe] | log-e |
CH | ... | -4.23+-0.28 | -0.67+-0.30 | 4.32+-0.28 |
Mg I | ... | -3.35+-0.23 | 0.06+-0.23 | 4.23+-0.19 |
Al I | ... | -3.76+-0.24 | -0.36+-0.26 | 2.71+-0.24 |
Ca I | ... | -3.31+-0.20 | 0.10+-0.25 | 3.05+-0.20 |
Sc II | ... | -3.43+-0.24 | -0.02+-0.24 | -0.25+-0.22 |
Ti | ... | -3.41+-0.23 | 0.00+-0.23 | 1.61+-0.21 |
Cr I | ... | -3.99+-0.20 | -0.59+-0.22 | 1.68+-0.20 |
Mn I | ... | -4.13+-0.23 | -0.72+-0.23 | 1.26+-0.21 |
Fe | ... | -3.41+-0.18 | 0.00+-0.22 | 4.09+-0.18 |
Co I | ... | -3.19+-0.22 | 0.22+-0.24 | 1.73+-0.22 |
Ni I | ... | -3.44+-0.23 | -0.03+-0.23 | 2.82+-0.22 |
Sr | ... | -4.25+-0.27 | -0.84+-0.27 | -1.28+-0.27 |
Ba II | ... | -4.71+-0.23 | -1.30+-0.24 | -2.58+-0.23 |
: 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 |
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Basic Informations
Observation Date | JD | Facility | Resolution | S/N | Exposure Time | Vrad |
2000-11-11 | N/A | SUBARUHDS | 50000 | 59 | 9000 | -20.07+-0.71 |
Galactic Longitude (l) | N/A |
Galactic Latitude (b) | N/A |
Declination | -054756 |
Right Ascension | 233728.6 |
Binarity
Photometric data
A0091
Title | First stars IX - Mixing in extremely metal-poor giants. Variation of the 12C/13C, [Na/Mg] and [Al/Mg] ratios |
ADS | M.Spite et al.,AAP, 455, 291, 2006 |
Authors | M. Spite, R. Cayrel, V. Hill, F. Spite, P. Francois, B. Plez, P. Bonifacio, P. Molaro, E. Depagne, J. Andersen, B. Barbuy, T. C. Beers, B. Nordstrom, F. Primas |
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Basic Informations
Observation Date | JD | Facility | Resolution | S/N | Exposure Time | Vrad |
| N/A | VLT | 47000 | 130 | N/A | N/A |
Galactic Longitude (l) | N/A |
Galactic Latitude (b) | N/A |
Declination | N/A |
Right Ascension | N/A |
Photometric data
Atmospheric data
Teff | 4800 |
log g | 1.3 |
vturb | 2.1 |
Chemical Abundances
Element | Nline | [X/H] | [X/Fe] | log-e |
C | ... | -4.02+-0.08 | -0.59+-0.08 | 4.53+-0.08 |
N | ... | -2.12+-0.10 | 1.31+-0.10 | 5.85+-0.10 |
Fe | ... | -3.43 | ... | 4.07 |
: Data presented in the paper
: Data converted with the solar abundance from Grevesse et al. (1996)
A0110
Title | NLTE determination of the sodium abundance in a homogeneous sample of extremely metal-poor stars |
ADS | S.M.Andrievsky et al.,AAP, 464, 1081, 2007 |
Authors | S. M. Andrievsky, M. Spite, S. A. Korotin, F. Spite, P. Bonifacio, R. Cayrel, V. Hill, P. Francois |
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Basic Informations
Observation Date | JD | Facility | Resolution | S/N | Exposure Time | Vrad |
| N/A | VLT | 43000 | 200 | N/A | N/A |
Galactic Longitude (l) | N/A |
Galactic Latitude (b) | N/A |
Declination | N/A |
Right Ascension | N/A |
Photometric data
Atmospheric data
Teff | 4800 |
log g | 1.3 |
vturb | 2.1 |
Chemical Abundances
Element | Nline | [X/H] | [X/Fe] | log-e |
Na | ... | -2.92 | +0.51 | 3.33 |
Fe | ... | -3.43 | ... | 4.07 |
: Data presented in the paper
: Data converted with the solar abundance from Grevesse et al. (1996)
A0176
Title | NLTE determination of the aluminium abundance in a homogeneous sample of extremely metal-poor stars |
ADS | S.M.Andrievsky et al.,AAP, 481, 481, 2008 |
Authors | S. M. Andrievsky, M. Spite, S. A. Korotin, F. Spite, P. Bonifacio, R. Cayrel, V. Hill, P. François |
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Basic Informations
Observation Date | JD | Facility | Resolution | S/N | Exposure Time | Vrad |
| N/A | VLT | 47000 | 120 | N/A | N/A |
Galactic Longitude (l) | N/A |
Galactic Latitude (b) | N/A |
Declination | N/A |
Right Ascension | N/A |
Atmospheric data
Teff | 4800 |
log g | 1.3 |
vturb | 2.1 |
Chemical Abundances
Element | Nline | [X/H] | [X/Fe] | log-e |
Al | ... | -3.42 | 0.01 | 3.05 |
Fe | ... | -3.43 | ... | 4.07 |
: Data presented in the paper
: Data converted with the solar abundance from Grevesse et al. (1996)