HD122563: found in 30 paper(s).
Labels:
/D.L.Burris et al.(2000)/
/R.Cayrel et al.(2004)/
/S.Honda et al.(2004)/
/M.Spite et al.(2005)/
/J.A.Johnson(2002)/
/J.Westin et al.(2000)/
/J.E.Norris et al.(1997)/
/W.Aoki et al.(2005)/
/T.V.Mishenina et al.(2002)/
/T.V.Mishenina and V. V. Kovtyukh(2001)/
/B.Barbuy et al.(2003)/
/J.P.Fulbright and J. A. Johnson(2003)/
/J.J.Cowan et al.(2005)/
/S.Honda et al.(2004)/
/M.Spite et al.(2006)/
/S.M.Andrievsky et al.(2007)/
/J.A.Johnson et al.(2007)/
/W.Aoki et al.(2007)/
/S.Honda et al.(2006)/
/J.P.Fulbright(2000)/
/S.Honda et al.(2007)/
/D.K.Lai et al.(2007)/
/J.Simmerer et al.(2004)/
/C.Sneden et al.(1998)/
/M.Bergemann and T. Gehren(2008)/
/S.M.Andrievsky et al.(2008)/
/I.U.Roederer et al.(2008)/
/L.Mashonkina et al.(2008)/
/J.A.Johnson and M. Bolte(2002)/
/J.A.Johnson and M. Bolte(2001)/
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A0014
Title | NEUTRON-CAPTURE ELEMENTS IN THE EARLY GALAXY: INSIGHTS FROM A LARGE SAMPLE OF METAL-POOR GIANTS |
ADS | D.L.Burris et al.,ApJ, 544, 302, 2000 |
Authors | D. L. Burris, C. A. Pilachowski, T. E. Armandroff, C. Sneden, J. J. Cowan, H. Roe |
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Basic Informations
Observation Date | JD | Facility | Resolution | S/N | Exposure Time | Vrad |
N/A | N/A | MAYALLKPNO | 20000 | 100-200 | 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 | 4625 |
log g | 1.40 |
vturb | 1.70 |
Chemical Abundances
Element | Nline | [X/H] | [X/Fe] | log-e |
Fe | ... | -2.71 | ... | 4.79 |
Sr | ... | -2.65 | 0.06 | 0.25 |
Y | ... | -2.84 | -0.13 | -0.60 |
Zr | ... | -2.40 | 0.31 | 0.20 |
Ba | ... | -3.63 | -0.92 | -1.50 |
La | ... | -3.42 | -0.71 | -2.20 |
Nd | ... | -3.30 | -0.59 | -1.80 |
Eu | ... | -3.01 | -0.30 | -2.50 |
Dy | ... | -3.10 | -0.39 | -2.00 |
: Data presented in the paper
: Data converted with the solar abundance from Grevesse et al. (1996)
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 |
2000-07 | N/A | VLT | 47000 | 250 | N/A | N/A |
Galactic Longitude (l) | N/A |
Galactic Latitude (b) | N/A |
Declination | N/A |
Right Ascension | N/A |
Binarity
Photometric data
V | 6.20 |
B-V | 0.90 |
V-R | 0.81 |
J-K | 0.61 |
V-K | 2.51 |
EB-V | 0.00 |
Atmospheric data
Teff | 4600 |
log g | 1.1 |
vturb | 2.0 |
Chemical Abundances
Element | Nline | [X/H] | [X/Fe] | log-e |
CH | ... | -3.22 | -0.41 | 5.30 |
O I | ... | -2.20 | 0.62 | 6.57 |
Na I | ... | -2.58 | 0.23 | 3.75 |
Mg I | ... | -2.45+-0.12 | 0.36+-0.12 | 5.13+-0.12 |
Al I | ... | -3.19 | -0.38 | 3.28 |
Si I | ... | -2.35 | 0.47 | 5.20 |
K I | ... | -2.30 | 0.51 | 2.82 |
Ca I | ... | -2.50+-0.10 | 0.31+-0.10 | 3.86+-0.10 |
Sc II | ... | -2.71+-0.10 | 0.11+-0.10 | 0.46+-0.10 |
Ti I | ... | -2.70+-0.10 | 0.12+-0.10 | 2.32+-0.10 |
Ti II | ... | -2.64+-0.10 | 0.18+-0.10 | 2.38+-0.10 |
Cr I | ... | -3.21+-0.17 | -0.40+-0.17 | 2.46+-0.17 |
Mn I | ... | -3.22+-0.06 | -0.41+-0.06 | 2.17+-0.06 |
Fe I | ... | -2.78+-0.17 | 0.03+-0.17 | 4.72+-0.17 |
Fe II | ... | -2.85+-0.13 | -0.04+-0.13 | 4.65+-0.13 |
Co I | ... | -2.53+-0.13 | 0.29+-0.13 | 2.39+-0.13 |
Ni I | ... | -2.78+-0.09 | 0.03+-0.09 | 3.47+-0.09 |
Zn I | ... | -2.66 | 0.16 | 1.94 |
: 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 |
2000-07-04 | N/A | SUBARUHDS | 90000 | 374 | 1200 | -27.20+-0.33 |
2001-01-29 | N/A | SUBARUHDS | N/A | N/A | N/A | -26.52+-0.34 |
Galactic Longitude (l) | N/A |
Galactic Latitude (b) | N/A |
Declination | N/A |
Right Ascension | N/A |
Photometric data
V | 6.20 |
B | 7.11 |
B-V | 0.91 |
V-K | 2.47 |
H | 4.03 |
J | 4.79 |
K | 3.73 |
EB-V | 0.00 |
Atmospheric data
Teff | 4570 |
log g | 1.1 |
vturb | 2.2 |
Chemical Abundances
Element | Nline | [X/H] | [X/Fe] | log-e |
CH | ... | -3.18 | -0.41 | 5.38 |
Mg I | ... | -2.23+-0.06 | 0.54+-0.06 | 5.35+-0.06 |
Al I | ... | -3.17+-0.12 | -0.4+-0.12 | 3.3+-0.12 |
Si I | ... | -2.33+-0.12 | 0.44+-0.12 | 5.22+-0.12 |
Ca I | ... | -2.47+-0.1 | 0.3+-0.1 | 3.89+-0.1 |
Sc II | ... | -2.77+-0.07 | 0.00+-0.07 | 0.4+-0.07 |
Ti | ... | -2.57+-0.12 | 0.2+-0.12 | 2.45+-0.12 |
V | ... | -2.72+-0.13 | 0.05+-0.13 | 1.28+-0.13 |
Cr | ... | -2.62+-0.15 | 0.15+-0.15 | 3.05+-0.15 |
Mn I | ... | -2.93+-0.09 | -0.16+-0.09 | 2.46+-0.09 |
Fe | ... | -2.77+-0.19 | ... | 4.74+-0.19 |
Co I | ... | -2.59+-0.16 | 0.18+-0.16 | 2.33+-0.16 |
Ni I | ... | -2.92+-0.12 | -0.15+-0.12 | 3.33+-0.12 |
Cu I | ... | -3.55+-0.12 | -0.78+-0.12 | 0.66+-0.12 |
Sr II | ... | -2.88+-0.12 | -0.11+-0.12 | 0.04+-0.12 |
Y II | ... | -3.10+-0.12 | -0.33+-0.12 | -0.87+-0.12 |
Zr II | ... | -2.80+-0.11 | -0.03+-0.11 | -0.19+-0.11 |
Ba II | ... | -3.98+-0.12 | -1.21+-0.12 | -1.76+-0.12 |
La II | ... | -3.66+-0.12 | -0.89+-0.12 | -2.44+-0.12 |
Nd II | ... | -3.44+-0.12 | -0.67+-0.12 | -1.95+-0.12 |
Eu II | ... | -3.15+-0.12 | -0.38+-0.12 | -2.6+-0.12 |
Gd II | ... | -3.40+-0.12 | -0.63+-0.12 | -2.31+-0.12 |
: Data presented in the paper
: Data converted with the solar abundance from Grevesse et al. (1996)
Isotope ratio
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 | 4600 |
log g | 1.1 |
vturb | 2.0 |
Chemical Abundances
Element | Nline | [X/H] | [X/Fe] | log-e |
Li I | ... | <-1.76 | <1.06 | <-0.60 |
C | ... | -3.29+-0.05 | -0.47+-0.05 | 5.26+-0.05 |
N | ... | -2.12 | 0.70 | 5.85 |
O I | ... | -2.20 | 0.62 | 6.67 |
Fe | ... | -2.82 | ... | 4.68 |
: Data presented in the paper
: Data converted with the solar abundance from Grevesse et al. (1996)
A0031
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Basic Informations
Observation Date | JD | Facility | Resolution | S/N | Exposure Time | Vrad |
1997-05-12 | N/A | KECKHIRES | 45000 | 500 | 600 | N/A |
1997-06-20 | N/A | KECKHIRES | 45000 | N/A | 600 | N/A |
1998-06-09 | N/A | LICKHAMILTON | 60000 | 95 | 120 | N/A |
1997-05-12 | N/A | KECKHIRES | 45000 | 500 | 600 | N/A |
1997-06-20 | N/A | KECKHIRES | 45000 | N/A | 600 | N/A |
1998-06-09 | N/A | LICKHAMILTON | 60000 | 95 | 120 | N/A |
Galactic Longitude (l) | N/A |
Galactic Latitude (b) | N/A |
Declination | N/A |
Right Ascension | N/A |
Photometric data
V | 6.20 |
V-R | 0.805 |
V-K | 2.485 |
EB-V | 0.00 |
Atmospheric data
Teff | 4450 |
log g | 0.50 |
vturb | 2.30 |
Chemical Abundances
Element | Nline | [X/H] | [X/Fe] | log-e |
Na I | ... | -2.63+-0.22 | 0.10+-0.22 | 3.70+-0.22 |
Mg I | ... | -2.06+-0.12 | 0.67+-0.12 | 5.52+-0.12 |
Al I | ... | -2.86+-0.10 | -0.13+-0.10 | 3.61+-0.10 |
Si I | ... | -2.05+-0.20 | 0.68+-0.20 | 5.50+-0.20 |
Ca I | ... | -2.46+-0.07 | 0.27+-0.07 | 3.90+-0.07 |
Sc II | ... | -2.74+-0.10 | -0.01+-0.10 | 0.43+-0.10 |
Ti I | ... | -2.64+-0.13 | 0.09+-0.13 | 2.38+-0.13 |
Ti II | ... | -2.62+-0.08 | 0.11+-0.08 | 2.40+-0.08 |
V I | ... | -2.81+-0.02 | -0.08+-0.02 | 1.19+-0.02 |
V II | ... | -2.55+-0.05 | 0.18+-0.05 | 1.45+-0.05 |
Cr I | ... | -3.01+-0.06 | -0.28+-0.06 | 2.66+-0.06 |
Cr II | ... | -2.62+-0.06 | 0.11+-0.06 | 3.05+-0.06 |
Mn I | ... | -2.96+-0.08 | -0.23+-0.08 | 2.43+-0.08 |
Mn II | ... | -2.44+-0.15 | 0.29+-0.15 | 2.95+-0.15 |
Fe I | ... | -2.73+-0.16 | ... | 4.77+-0.16 |
Fe II | ... | -2.75+-0.11 | ... | 4.75+-0.11 |
Co I | ... | -2.40+-0.11 | 0.33+-0.11 | 2.52+-0.11 |
Ni I | ... | -2.65+-0.14 | 0.08+-0.14 | 3.60+-0.14 |
Zn I | ... | -2.60+-0.04 | 0.13+-0.04 | 2.00+-0.04 |
Y II | ... | -3.04+-0.12 | -0.31+-0.12 | -0.80+-0.12 |
Zr II | ... | -2.74+-0.12 | -0.01+-0.12 | -0.14+-0.12 |
Ba II | ... | -3.93+-0.01 | -1.20+-0.01 | -1.80+-0.01 |
La II | ... | -3.61+-0.10 | -0.88+-0.10 | -2.44+-0.10 |
Pr II | ... | <-2.26 | <0.47 | <-1.55 |
Nd II | ... | -3.37+-0.20 | -0.64+-0.20 | -1.87+-0.20 |
Eu II | ... | -3.36+-0.20 | -0.63+-0.20 | -2.85+-0.20 |
Tb II | ... | <-1.71 | <1.02 | <-1.81 |
Ho II | ... | <-1.92 | <0.81 | <-1.66 |
Er II | ... | -3.36+-0.10 | -0.63+-0.10 | -2.43+-0.10 |
Tm II | ... | <-2.33 | <0.40 | <-2.33 |
Yb II | ... | -3.86+-0.20 | -1.13+-0.20 | -2.78+-0.20 |
Hf II | ... | <-1.76 | <0.97 | <-0.88 |
Os I | ... | <-1.86 | <0.87 | <-0.41 |
: Data presented in the paper
: Data converted with the solar abundance from Grevesse et al. (1996)
A0033
Title | THE r-PROCESS-ENRICHED LOW-METALLICITY GIANT HD 115444 |
ADS | J.Westin et al.,ApJ, 530, 783, 2000 |
Authors | J. Westin, C. Sneden, B. Gustafsson, J. J. Department of Physics and Astronomy, UofOklahoma. Cowan |
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Basic Informations
Observation Date | JD | Facility | Resolution | S/N | Exposure Time | Vrad |
| N/A | MCDONALD | 60000 | 200,400,500 | N/A | N/A |
Galactic Longitude (l) | N/A |
Galactic Latitude (b) | N/A |
Declination | N/A |
Right Ascension | N/A |
Photometric data
V | 6.18 |
B-V | 0.85 |
U-B | 0.37 |
V-K | 2.49 |
Atmospheric data
Teff | 4500 |
log g | 1.30 |
vturb | 2.5 |
Chemical Abundances
Element | Nline | [X/H] | [X/Fe] | log-e |
O I | ... | -2.13+-0.11 | +0.61+-0.11 | +6.80+-0.11 |
Na I | ... | -2.89+-0.11 | -0.15+-0.11 | +3.44+-0.11 |
Mg I | ... | -2.23+-0.12 | +0.51+-0.12 | +5.35+-0.12 |
Al I | ... | -3.06+-0.11 | -0.32+-0.11 | +3.41+-0.11 |
Si I | ... | -2.28+-0.11 | +0.46+-0.11 | +5.27+-0.11 |
Ca I | ... | -2.45+-0.09 | +0.29+-0.09 | +3.91+-0.09 |
Sc II | ... | -2.59+-0.08 | +0.15+-0.08 | +0.51+-0.08 |
Ti I | ... | -2.55+-0.07 | +0.19+-0.07 | +2.44+-0.07 |
Ti II | ... | -2.46+-0.15 | +0.28+-0.15 | +2.53+-0.15 |
V I | ... | -2.67+-0.11 | +0.07+-0.11 | +1.33+-0.11 |
V II | ... | -2.60+-0.11 | +0.14+-0.11 | +1.40+-0.11 |
Cr I | ... | -3.13+-0.15 | -0.39+-0.15 | +2.54+-0.15 |
Mn I | ... | -3.00+-0.19 | -0.26+-0.19 | +2.39+-0.19 |
Fe I | ... | -2.74+-0.12 | ... | +4.78+-0.12 |
Fe II | ... | -2.74+-0.10 | ... | +4.78+-0.10 |
Co I | ... | -2.42+-0.20 | +0.32+-0.20 | +2.50+-0.20 |
Ni I | ... | -2.70+-0.05 | +0.04+-0.05 | +3.55+-0.05 |
Cu I | ... | -3.49+-0.11 | -0.75+-0.11 | +0.72+-0.11 |
Zn I | ... | -2.54+-0.11 | +0.20+-0.11 | +2.06+-0.11 |
Ge I | ... | -3.44+-0.11 | -0.70+-0.11 | -0.03+-0.11 |
Sr II | ... | -2.57+-0.11 | +0.17+-0.11 | +0.33+-0.11 |
Y II | ... | -2.99+-0.11 | -0.25+-0.11 | -0.75+-0.11 |
Zr II | ... | -2.56+-0.19 | +0.18+-0.19 | +0.04+-0.19 |
Ba II | ... | -3.67+-0.13 | -0.93+-0.13 | -1.54+-0.13 |
La II | ... | -3.44+-0.11 | -0.70+-0.11 | -2.22+-0.11 |
Ce II | ... | -3.47+-0.11 | -0.73+-0.11 | -1.92+-0.11 |
Nd II | ... | -3.04+-0.11 | -0.30+-0.11 | -1.54+-0.11 |
Eu II | ... | -3.10+-0.11 | -0.36+-0.11 | -2.59+-0.11 |
Er II | ... | -3.20+-0.11 | -0.46+-0.11 | -2.27+-0.11 |
Yb II | ... | -3.70+-0.11 | -0.96+-0.11 | -2.62+-0.11 |
: Data presented in the paper
: Data converted with the solar abundance from Grevesse et al. (1996)
Isotope ratio
A0040
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Basic Informations
Galactic Longitude (l) | N/A |
Galactic Latitude (b) | N/A |
Declination | N/A |
Right Ascension | N/A |
Photometric data
Atmospheric data
Teff | 4650 |
log g | 1.4 |
vturb | 2.6 |
Chemical Abundances
Element | Nline | [X/H] | [X/Fe] | log-e |
CH | ... | -3.13+-0.20 | -0.45+-0.20 | 5.42+-0.20 |
CN | ... | -1.68 | +1.00 | 6.29 |
Mg I | ... | -2.36+-0.04 | +0.32+-0.04 | 5.22+-0.04 |
Al I | ... | -2.92+-0.10 | -0.24+-0.10 | 3.55+-0.10 |
Ca I | ... | -2.54+-0.06 | +0.14+-0.06 | 3.82+-0.06 |
Sc II | ... | -2.43+-0.11 | +0.25+-0.11 | 0.74+-0.11 |
Ti I | ... | -2.56+-0.05 | +0.12+-0.05 | 2.46+-0.05 |
Ti II | ... | -2.34+-0.08 | +0.34+-0.08 | 2.68+-0.08 |
Cr I | ... | -3.07+-0.07 | -0.39+-0.07 | 2.60+-0.07 |
Mn I | ... | -3.05+-0.05 | -0.37+-0.05 | 2.34+-0.05 |
Fe I | ... | -2.68+-0.11 | ... | 4.82+-0.11 |
Co I | ... | -2.35+-0.07 | +0.33+-0.07 | 2.57+-0.07 |
Ni I | ... | -2.47+-0.08 | +0.21+-0.08 | 3.78+-0.08 |
Sr II | ... | -2.89+-0.10 | -0.21+-0.10 | 0.08+-0.10 |
Y II | ... | -2.84+-0.18 | -0.16+-0.18 | -0.60+-0.18 |
Zr II | ... | -2.78+-0.22 | -0.10+-0.22 | -0.18+-0.22 |
Ba II | ... | -3.52+-0.10 | -0.84+-0.10 | -1.39+-0.10 |
La II | ... | -3.35 | -0.67 | -2.18 |
Ce II | ... | <-3.00 | <-0.32 | <-1.42 |
Nd II | ... | -3.20 | -0.52 | -1.70 |
Sm II | ... | <-3.20 | <-0.52 | <-2.19 |
Eu II | ... | -3.00 | -0.32 | -2.49 |
Dy II | ... | -3.00 | -0.32 | -1.86 |
: 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 |
2002-02-02 | N/A | SUBARUHDS | 50000 | 1500 | 15min | -25.81+-0.17 |
Galactic Longitude (l) | N/A |
Galactic Latitude (b) | N/A |
Declination | +094110 |
Right Ascension | 140231.8 |
Binarity
Photometric data
V | 6.20 |
B | 7.11 |
H | 4.03 |
J | 4.79 |
K | 3.73 |
EB-V | 0.00 |
Atmospheric data
Teff | 4600 |
log g | 1.1 |
vturb | 2.2 |
Chemical Abundances
Element | Nline | [X/H] | [X/Fe] | log-e |
CH | ... | -3.02 | -0.4 | 5.4 |
Mg I | ... | -2.09+-0.12 | 0.53+-0.12 | 5.49+-0.12 |
Al I | ... | -3.12+-0.18 | -0.5+-0.18 | 3.37+-0.18 |
Si I | ... | -2.20+-0.13 | 0.42+-0.13 | 5.36+-0.13 |
Ca I | ... | -2.44+-0.12 | 0.18+-0.12 | 3.91+-0.12 |
Sc II | ... | -2.55+-0.23 | 0.07+-0.23 | 0.55+-0.23 |
Ti I | ... | -2.51+-0.12 | 0.11+-0.12 | 2.43+-0.12 |
Ti II | ... | -2.31+-0.24 | 0.31+-0.24 | 2.63+-0.24 |
Cr I | ... | -3.04+-0.1 | -0.42+-0.1 | 2.65+-0.1 |
Mn I | ... | -3.26+-0.12 | -0.64+-0.12 | 2.27+-0.12 |
Fe I | ... | -2.62+-0.21 | ... | 4.88+-0.21 |
Fe II | ... | -2.62+-0.19 | ... | 4.88+-0.19 |
Co I | ... | -2.37+-0.11 | 0.25+-0.11 | 2.54+-0.11 |
Ni I | ... | -2.59+-0.11 | 0.03+-0.11 | 3.66+-0.11 |
Zn I | ... | -2.52+-0.21 | 0.1+-0.21 | 2.15+-0.21 |
Sr II | ... | -2.84+-0.16 | -0.22+-0.16 | 0.08+-0.16 |
Y II | ... | -3.07+-0.24 | -0.45+-0.24 | -0.84+-0.24 |
Zr II | ... | -2.75+-0.24 | -0.13+-0.24 | -0.14+-0.24 |
Ba II | ... | -3.91+-0.23 | -1.29+-0.23 | -1.69+-0.23 |
La II | ... | -3.14+-0.29 | -0.52+-0.29 | -2.37+-0.29 |
Nd II | ... | -3.42+-0.25 | -0.8+-0.25 | -1.93+-0.25 |
Eu II | ... | -3.19+-0.25 | -0.57+-0.25 | -2.64+-0.25 |
Er II | ... | -3.30+-0.25 | -0.68+-0.25 | -2.33+-0.25 |
: Data presented in the paper
: Data converted with the solar abundance from Grevesse et al. (1996)
A0070
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Basic Informations
Observation Date | JD | Facility | Resolution | S/N | Exposure Time | Vrad |
N/A | N/A | ELODIE | 42000 | >100 | N/A | N/A |
Galactic Longitude (l) | N/A |
Galactic Latitude (b) | N/A |
Declination | N/A |
Right Ascension | N/A |
Chemical Abundances
Element | Nline | [X/H] | [X/Fe] | log-e |
Fe | ... | -2.66 | ... | 4.84 |
Cu I | ... | -3.38+-0.25 | -0.72+-0.25 | 0.83+-0.25 |
Zn I | ... | -2.54+-0.19 | 0.12+-0.19 | 2.06+-0.19 |
: Data presented in the paper
: Data converted with the solar abundance from Grevesse et al. (1996)
A0071
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Basic Informations
Observation Date | JD | Facility | Resolution | S/N | Exposure Time | Vrad |
N/A | N/A | ELODIE | 42000 | >100 | N/A | N/A |
Photometric data
Atmospheric data
Teff | 4570 |
log g | 1.1 |
vturb | 1.2 |
Chemical Abundances
Element | Nline | [X/H] | [X/Fe] | log-e |
Si I | ... | -2.16 | 0.26 | 5.39 |
Ca I | ... | -2.14 | 0.28 | 4.22 |
Fe | ... | -2.42 | ... | 5.08 |
Ba II | ... | -3.53 | -1.11 | -1.40 |
: Data presented in the paper
: Data converted with the solar abundance from Grevesse et al. (1996)
A0073
Title | Oxygen Abundance in the Template Halo Giant HD 122563 |
ADS | B.Barbuy et al.,ApJ, 588, 1072, 2003 |
Authors | B. Barbuy, J. Melendez, M. Spite, F. Spite, E. Depagne, V. Hill, R. Cayrel, P. Bonifacio, A. Damineli, C. A.O. Torres |
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Basic Informations
Observation Date | JD | Facility | Resolution | S/N | Exposure Time | Vrad |
2000-05-20 | N/A | KECKNIRSPEC | 37000 | 250 | 4x120 | N/A |
2000-07-18 | N/A | VLT | 43000 | 267 | 75 | N/A |
2000-07-18 | N/A | VLT | 43000 | 305 | 75 | N/A |
2000-07-18 | N/A | VLT | 43000 | 370 | 75 | N/A |
2000-07-18 | N/A | VLT | 43000 | 390 | 75 | N/A |
2002-03-18 | N/A | FEROSESO | 37000 | 180 | 600 | N/A |
2002-03-18 | N/A | FEROSESO | 37000 | 255 | 600 | N/A |
2002-04-01 | N/A | FEROSESO | 37000 | 260 | 600 | N/A |
Galactic Longitude (l) | N/A |
Galactic Latitude (b) | N/A |
Declination | N/A |
Right Ascension | N/A |
Photometric data
V | 6.20 |
V-R | 0.805 |
J-K | 0.606 |
V-K | 2.502 |
Atmospheric data
Teff | 4600 |
log g | 1.1 |
vturb | 2.0 |
Chemical Abundances
Element | Nline | [X/H] | [X/Fe] | log-e |
O | ... | -1.87 | 0.9 | 7.00 |
Na I | ... | -2.56 | 0.21 | 3.77 |
Mg I | ... | -2.35 | +0.45 | 5.23 |
Al I | ... | -3.18 | -0.38 | 3.29 |
Si I | ... | -2.28 | +0.52 | 5.27 |
K I | ... | -2.30 | +0.50 | 2.82 |
Ca I | ... | -2.50 | +0.30 | 3.86 |
Sc II | ... | -2.70 | +0.10 | 0.47 |
Ti I | ... | -2.69 | +0.11 | 2.33 |
Ti II | ... | -2.64 | +0.16 | 2.38 |
Cr I | ... | -3.20 | -0.43 | 2.47 |
Mn I | ... | -2.94 | -0.17 | 2.45 |
Fe I | ... | -2.77 | ... | 4.73 |
Fe II | ... | -2.84 | ... | 4.66 |
Co I | ... | -2.52 | 0.25 | 2.40 |
Ni I | ... | -2.67 | 0.10 | 3.58 |
Zn I | ... | -2.63 | 0.14 | 1.97 |
: Data presented in the paper
: Data converted with the solar abundance from Grevesse et al. (1996)
A0074
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Basic Informations
Observation Date | JD | Facility | Resolution | S/N | Exposure Time | Vrad |
2001-04-05 | N/A | GECKOCFHT | 130000 | 400 | 900 | N/A |
Galactic Longitude (l) | N/A |
Galactic Latitude (b) | N/A |
Declination | N/A |
Right Ascension | N/A |
Photometric data
V | 6.18 |
B-V | 0.85 |
V-R | 0.82 |
V-K | 2.49 |
Atmospheric data
Teff | 4650 |
log g | 1.24 |
vturb | 1.85 |
Chemical Abundances
Element | Nline | [X/H] | [X/Fe] | log-e |
O I | ... | -1.88+-0.17 | 0.74+-0.17 | 6.81+-0.18 |
Fe | ... | -2.62 | ... | 4.88 |
Fe I | ... | -2.59+-0.07 | ... | 4.91+-0.07 |
Fe II | ... | -2.60+-0.04 | ... | 4.9+-0.04 |
: Data presented in the paper
: Data converted with the solar abundance from Grevesse et al. (1996)
A0076
Title | Hubble Space Telescope Observations of Heavy Elements in Metal-Poor Galactic Halo Stars |
ADS | J.J.Cowan et al.,ApJ, 627, 238, 2005 |
Authors | J. J. Cowan, C. Sneden, T. C. Beers, J. E. Lawler, J. Simmerer, J. W. Truran, F. Primas, J. Collier, S. Burles |
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Basic Informations
Observation Date | JD | Facility | Resolution | S/N | Exposure Time | Vrad |
N/A | N/A | HST | 30000 | >50 | N/A | N/A |
N/A | N/A | KECKHIRES | 45000 | 30-200 | N/A | |
Galactic Longitude (l) | N/A |
Galactic Latitude (b) | N/A |
Declination | N/A |
Right Ascension | N/A |
Photometric data
Atmospheric data
Teff | 4570 |
log g | 1.35 |
vturb | 2.90 |
Chemical Abundances
Element | Nline | [X/H] | [X/Fe] | log-e |
Fe I | ... | -2.72 | ... | 4.78 |
Fe II | ... | -2.61 | ... | 4.89 |
Ge | ... | -3.66 | -0.94 | -0.16 |
Zr | ... | -2.65 | +0.07 | +0.06 |
La | ... | -3.62 | -0.90 | -2.35 |
Eu | ... | -3.22 | -0.50 | -2.59 |
Os | ... | <-2.62 | <+0.1 | <-1.2 |
Ir | ... | <-2.62 | <+0.1 | <-1.3 |
Pt | ... | <-3.02 | <-0.3 | <-1.3 |
: 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 |
2000-07-04 | N/A | SUBARUHDS | 90000 | 374 | 1200 | -27.20+-0.33 |
2001-01-29 | N/A | SUBARUHDS | N/A | N/A | N/A | -26.52+-0.34 |
Galactic Longitude (l) | N/A |
Galactic Latitude (b) | N/A |
Declination | N/A |
Right Ascension | N/A |
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 | 4600 |
log g | 1.1 |
vturb | 2.0 |
Chemical Abundances
Element | Nline | [X/H] | [X/Fe] | log-e |
C | ... | -3.21+-0.05 | -0.39+-0.05 | 5.34+-0.05 |
N | ... | -2.12+-0.15 | 0.70+-0.15 | 5.85+-0.15 |
Fe | ... | -2.82 | ... | 4.68 |
: Data presented in the paper
: Data converted with the solar abundance from Grevesse et al. (1996)
Isotope ratio
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 | 4600 |
log g | 1.1 |
vturb | 2.0 |
Chemical Abundances
Element | Nline | [X/H] | [X/Fe] | log-e |
Na | ... | -3.05 | -0.23 | 3.20 |
Fe | ... | -2.82 | ... | 4.68 |
: Data presented in the paper
: Data converted with the solar abundance from Grevesse et al. (1996)
A0114
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Basic Informations
Observation Date | JD | Facility | Resolution | S/N | Exposure Time | Vrad |
2003-08-31 | N/A | RCKPNO | N/A | 267 | 600 | N/A |
Galactic Longitude (l) | N/A |
Galactic Latitude (b) | N/A |
Declination | N/A |
Right Ascension | N/A |
Photometric data
V | 6.196 |
B-V | 0.912 |
U-B | 0.340 |
V-R | 0.580 |
V-K | 2.473 |
EB-V | 0.02 |
Atmospheric data
Teff | 4615 |
log g | 1.27 |
vturb | 2.10 |
Chemical Abundances
Element | Nline | [X/H] | [X/Fe] | log-e |
C | ... | -3.42+-0.29 | -0.95+-0.29 | 5.14+-0.25 |
N | ... | -1.47+-0.25 | +1.00+-0.25 | 6.58+-0.25 |
Fe | ... | -2.47+-0.21 | ... | 5.03+-0.21 |
: Data presented in the paper
: Data converted with the solar abundance from Grevesse et al. (1996)
A0117
Title | Spectroscopic Studies of Extremely Metal-poor Stars with the Subaru High-Dispersion Spectrograph. IV. The alpha-Element–Enhanced Metal-poor Star BS 16934-002 |
ADS | W.Aoki et al.,ApJ, 660, 747, 2007 |
Authors | W. Aoki, S. Honda, T. C. Beers, M. Takada-Hidai, N. Iwamoto, N. Tominaga, H. Umeda, K. Nomoto, J. E. Norris, S. G. Ryan |
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Basic Informations
Observation Date | JD | Facility | Resolution | S/N | Exposure Time | Vrad |
2005-06-19 | 2453541 | SUBARUHDS | 60000 | 300 | 240 | -26.0+-0.2 |
Galactic Longitude (l) | N/A |
Galactic Latitude (b) | N/A |
Declination | N/A |
Right Ascension | N/A |
Atmospheric data
Teff | 4600 |
log g | 1.1 |
vturb | 2.2 |
Chemical Abundances
Element | Nline | [X/H] | [X/Fe] | log-e |
CH | ... | -2.94+-0.17 | -0.35+-0.17 | 5.45+-0.17 |
CN | ... | -1.98+-0.29 | +0.61+-0.29 | 5.80+-0.29 |
O I | ... | -1.85+-0.19 | +0.74+-0.19 | 6.81+-0.19 |
Na I | ... | -2.78+-0.13 | -0.19+-0.13 | 3.39+-0.13 |
Mg I | ... | -2.10+-0.11 | +0.49+-0.11 | 5.44+-0.11 |
Al I | ... | -2.99+-0.18 | -0.40+-0.18 | 3.38+-0.18 |
Si I | ... | -2.18+-0.16 | +0.41+-0.16 | 5.34+-0.16 |
Ca I | ... | -2.39+-0.11 | +0.20+-0.11 | 3.93+-0.11 |
Sc II | ... | -2.48+-0.23 | +0.11+-0.23 | 0.57+-0.23 |
Ti I | ... | -2.48+-0.12 | +0.11+-0.12 | 2.42+-0.12 |
Ti II | ... | -2.32+-0.24 | +0.27+-0.24 | 2.58+-0.24 |
Cr I | ... | -2.97+-0.10 | -0.38+-0.10 | 2.57+-0.10 |
Mn I | ... | -3.16+-0.13 | -0.57+-0.13 | 2.23+-0.13 |
Fe I | ... | -2.59+-0.20 | ... | 4.86+-0.20 |
Fe II | ... | -2.58+-0.19 | ... | 4.87+-0.19 |
Co I | ... | -2.44+-0.11 | +0.15+-0.11 | 2.48+-0.11 |
Ni I | ... | -2.57+-0.11 | +0.02+-0.11 | 3.66+-0.11 |
Zn I | ... | -2.53+-0.21 | +0.06+-0.21 | 2.08+-0.21 |
Sr II | ... | -2.89+-0.15 | -0.30+-0.15 | 0.08+-0.15 |
Ba II | ... | -3.87+-0.23 | -1.28+-0.23 | -1.69+-0.23 |
: Data presented in the paper
: Data converted with the solar abundance from Grevesse et al. (1996)
A0121
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Basic Informations
Observation Date | JD | Facility | Resolution | S/N | Exposure Time | Vrad |
2004-04-30 | N/A | SUBARUHDS | 90000 | 140-1340 | 5400 | N/A |
Galactic Longitude (l) | N/A |
Galactic Latitude (b) | N/A |
Declination | N/A |
Right Ascension | N/A |
Atmospheric data
Teff | 4570+-100 |
log g | 1.1+-0.3 |
vturb | 2.2+-0.5 |
Chemical Abundances
Element | Nline | [X/H] | [X/Fe] | log-e |
Fe | ... | -2.77+-0.19 | ... | 4.73+-0.19 |
Cu | ... | -3.92+-0.29 | -1.15+-0.29 | 0.98+-0.29 |
Zn | ... | -2.59+-0.16 | +0.18+-0.16 | 2.01+-0.16 |
Sr | ... | -3.03+-0.08 | -0.26+-0.08 | -0.11+-0.08 |
Y | ... | -3.14+-0.09 | -0.37+-0.09 | -0.93+-0.09 |
Zr | ... | -2.87+-0.16 | -0.10+-0.16 | -0.28+-0.16 |
Nb | ... | -2.90+-0.17 | -0.13+-0.17 | -1.48+-0.17 |
Mo | ... | -2.79+-0.17 | -0.02+-0.17 | -0.87+-0.17 |
Ru | ... | -2.70+-0.17 | +0.07+-0.17 | -0.86+-0.17 |
Rh | ... | <-2.32 | <+0.45 | <-1.20 |
Pd | ... | -3.05+-0.17 | -0.28+-0.17 | -1.36+-0.17 |
Ag | ... | -2.82+-0.17 | -0.05+-0.17 | -1.88+-0.17 |
Ba | ... | -3.79+-0.12 | -1.02+-0.12 | -1.62+-0.12 |
La | ... | -3.79+-0.10 | -1.02+-0.10 | -2.66+-0.10 |
Ce | ... | -3.41+-0.18 | -0.64+-0.18 | -1.83+-0.18 |
Pr | ... | -2.86+-0.17 | -0.09+-0.17 | -2.15+-0.17 |
Nd | ... | -3.46+-0.10 | -0.69+-0.10 | -2.01+-0.10 |
Sm | ... | -3.17+-0.17 | -0.40+-0.17 | -2.16+-0.17 |
Eu | ... | -3.29+-0.17 | -0.52+-0.17 | -2.77+-0.17 |
Gd | ... | -3.53+-0.17 | -0.76+-0.17 | -2.44+-0.17 |
Dy | ... | -3.76+-0.17 | -0.99+-0.17 | -2.62+-0.17 |
Ho | ... | <-2.51 | <+0.26 | <-2.00 |
Er | ... | -3.59+-0.17 | -0.82+-0.17 | -2.66+-0.17 |
Tm | ... | <-3.00 | <-0.23 | <-3.00 |
Yb | ... | -3.86+-0.17 | -1.09+-0.17 | -2.78+-0.17 |
Ir | ... | <-2.98 | <-0.21 | <-1.60 |
Th | ... | <-3.11 | <-0.34 | <-3.05 |
: Data presented in the paper
: Data converted with the solar abundance from Grevesse et al. (1996)
A0126
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Basic Informations
Observation Date | JD | Facility | Resolution | S/N | Exposure Time | Vrad |
1998067-8 | N/A | LICKHAMILTON | N/A | 95 | 120 | |
Photometric data
Atmospheric data
Teff | 4425 |
log g | 0.6 |
vturb | 2.05 |
Chemical Abundances
Element | Nline | [X/H] | [X/Fe] | log-e |
Na I | ... | -2.69 | 0.1 | 3.64 |
Mg I | ... | -2.16 | 0.63 | 5.42 |
Si I | ... | -2.37 | 0.42 | 5.18 |
Ca I | ... | -2.46 | 0.33 | 3.90 |
Ti | ... | -2.57 | 0.22 | 2.45 |
V I | ... | -2.83 | -0.04 | 1.17 |
Cr I | ... | -3.04 | -0.25 | 2.63 |
Fe | ... | -2.79 | ... | 4.71 |
Ni I | ... | -2.67 | 0.12 | 3.58 |
Y II | ... | -3.23 | -0.44 | -0.99 |
Zr II | ... | -2.87 | -0.08 | -0.27 |
Ba II | ... | -3.83 | -1.04 | -1.70 |
: Data presented in the paper
: Data converted with the solar abundance from Grevesse et al. (1996)
A0127
Title | Neutron-Capture Elements in the Very Metal-poor Star HD 88609: Another Star with Excesses of Light Neutron-Capture Elements |
ADS | S.Honda et al.,ApJ, 666, 1189, 2007 |
Authors | S. Honda, W. Aoki, Y. Ishimaru, S. Wanajo |
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Basic Informations
Observation Date | JD | Facility | Resolution | S/N | Exposure Time | Vrad |
2004-04-20 | N/A | SUBARUHDS | 90000 | 120,240 | 3600 | |
2005-10-19 | N/A | SUBARUHDS | 90000 | 150,330 | 9000 | -37.69+-0.3 |
Galactic Longitude (l) | N/A |
Galactic Latitude (b) | N/A |
Declination | N/A |
Right Ascension | N/A |
Atmospheric data
Teff | 4570+-100 |
log g | 1.1+-0.3 |
vturb | 2.2+-0.5 |
Chemical Abundances
Element | Nline | [X/H] | [X/Fe] | log-e |
Fe | ... | -2.77+-0.19 | ... | 4.73+-0.19 |
Cu | ... | -3.23+-0.14 | -0.46+-0.14 | 0.98+-0.14 |
Zn | ... | -2.59+-0.15 | +0.18+-0.15 | 2.01+-0.15 |
Sr | ... | -3.04+-0.14 | -0.27+-0.14 | -0.12+-0.14 |
Y | ... | -3.14+-0.09 | -0.37+-0.09 | -0.93+-0.09 |
Zr | ... | -2.87+-0.16 | -0.10+-0.16 | -0.28+-0.16 |
Nb | ... | -2.90+-0.14 | -0.13+-0.14 | -1.48+-0.14 |
Mo | ... | -2.79+-0.14 | -0.02+-0.14 | -0.87+-0.14 |
Ru | ... | -2.70+-0.14 | 0.07+-0.14 | -0.86+-0.14 |
Rh | ... | <-2.32 | <+0.45 | <-1.20 |
Pd | ... | -3.00+-0.14 | -0.23+-0.14 | -1.31+-0.14 |
Ag | ... | -2.82+-0.14 | -0.05+-0.14 | -1.88+-0.14 |
Ba | ... | -3.82+-0.12 | -1.05+-0.12 | -1.65+-0.12 |
La | ... | -3.73+-0.16 | -0.96+-0.16 | -2.60+-0.16 |
Ce | ... | -3.49+-0.17 | -0.72+-0.17 | -1.91+-0.17 |
Pr | ... | -2.86+-0.14 | -0.09+-0.14 | -2.15+-0.14 |
Nd | ... | -3.46+-0.16 | -0.69+-0.16 | -2.01+-0.16 |
Sm | ... | -3.17+-0.14 | -0.40+-0.14 | -2.16+-0.14 |
Eu | ... | -3.29+-0.14 | -0.52+-0.14 | -2.77+-0.14 |
Gd | ... | -3.53+-0.14 | -0.76+-0.14 | -2.44+-0.14 |
Dy | ... | -3.76+-0.14 | -0.99+-0.14 | -2.62+-0.14 |
Ho | ... | <-2.51 | <+0.26 | <-2.00 |
Er | ... | -3.59+-0.14 | -0.82+-0.14 | -2.66+-0.14 |
Tm | ... | <-3.00 | <-0.23 | <-3.00 |
Yb | ... | -3.86+-0.14 | -1.09+-0.14 | -2.78+-0.14 |
Ir | ... | <-2.98 | <-0.21 | <-1.60 |
Th | ... | <-3.11 | <-0.34 | <-3.05 |
: 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 | ... | -2.94+-0.19 | -0.40+-0.19 | 5.61+-0.19 |
Fe | ... | -2.54 | ... | 4.96 |
Sr | ... | -2.60 | -0.06 | 0.37 |
Ba | ... | -3.55 | -1.01 | -1.42 |
: Data presented in the paper
: Data converted with the solar abundance from Grevesse et al. (1996)
A0131
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Basic Informations
Observation Date | JD | Facility | Resolution | S/N | Exposure Time | Vrad |
N/A | N/A | MCDONALD | 60000 | 100 | N/A | N/A |
Atmospheric data
Teff | 4572 |
log g | 1.36 |
vturb | 2.90 |
Chemical Abundances
Element | Nline | [X/H] | [X/Fe] | log-e |
C | ... | -3.32 | -0.6 | 5.23 |
Fe I | ... | -2.72 | ... | 4.78 |
Fe II | ... | -2.61 | ... | 4.89 |
La II | ... | -3.52+-0.1 | -0.80+-0.1 | -2.35+-0.1 |
Eu II | ... | -3.10+-0.04 | -0.38+-0.04 | -2.59+-0.04 |
: Data presented in the paper
: Data converted with the solar abundance from Grevesse et al. (1996)
A0132
Title | Hubble Space Telescope Observations of Neutron-Capture Elements in Very Metal Poor Stars |
ADS | C.Sneden et al.,ApJ, 496, 235, 1998 |
Authors | C. Sneden, J. J. Cowan, D. L. Burris, J. W. Truran |
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Basic Informations
Observation Date | JD | Facility | Resolution | S/N | Exposure Time | Vrad |
| N/A | N/A | 32000 | 50-70 | N/A | N/A |
Galactic Longitude (l) | N/A |
Galactic Latitude (b) | N/A |
Declination | N/A |
Right Ascension | N/A |
Atmospheric data
Teff | 4625 |
log g | 1.40 |
vturb | 2.0 |
Chemical Abundances
Element | Nline | [X/H] | [X/Fe] | log-e |
Ge I | ... | -3.51 | -0.80 | -0.10 |
Zr II | ... | -2.38 | +0.35 | +0.22 |
Os I | ... | <-2.75 | <-0.05 | <-1.30 |
Pt I | ... | <-3.00 | <-0.30 | <-1.20 |
Pb I | ... | -2.75 | <-0.15 | -0.80 |
: Data presented in the paper
: Data converted with the solar abundance from Grevesse et al. (1996)
A0170
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Basic Informations
Galactic Longitude (l) | N/A |
Galactic Latitude (b) | N/A |
Declination | N/A |
Right Ascension | N/A |
Atmospheric data
Teff | 4600+-100 |
log g | 1.50+-0.20 |
vturb | 1.9+-0.2 |
Chemical Abundances
Element | Nline | [X/H] | [X/Fe] | log-e |
Mg | ... | -2.06 | 0.45 | 5.52 |
Mn | ... | -3.10+-0.1 | -0.59+-0.1 | 2.29+-0.1 |
Fe | ... | -2.51+-0.05 | ... | 4.99+-0.05 |
: 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 | 4600 |
log g | 1.1 |
vturb | 2.0 |
Chemical Abundances
Element | Nline | [X/H] | [X/Fe] | log-e |
Al | ... | -2.92 | -0.10 | 3.55 |
Fe | ... | -2.82 | ... | 4.68 |
: Data presented in the paper
: Data converted with the solar abundance from Grevesse et al. (1996)
A0177
Title | Europium, Samarium, and Neodymium Isotopic Fractions in Metal-Poor Stars |
ADS | I.U.Roederer et al.,ApJ, 675, 723, 2008 |
Authors | I. U. Roederer, J. E. Lawler, C. Sneden, J. J. Cowan, J. S. Sobeck, C. A. Pilachowski |
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Basic Informations
Observation Date | JD | Facility | Resolution | S/N | Exposure Time | Vrad |
2006-06-12 | N/A | MCDONALD | 120000 | 430-1000 | 30min | -26.0+-0.3 |
Galactic Longitude (l) | N/A |
Galactic Latitude (b) | N/A |
Declination | N/A |
Right Ascension | N/A |
Binarity
Binarity | Negative |
Vrad | -26.0+-0.3 |
Atmospheric data
Teff | 4430+-100 |
log g | 0.55+-0.3 |
vturb | 2.4+-0.3 |
Chemical Abundances
Element | Nline | [X/H] | [X/Fe] | log-e |
Fe I | ... | -2.83+-0.15 | ... | 4.67+-0.15 |
Fe II | ... | -2.79 | ... | 4.71 |
: Data presented in the paper
: Data converted with the solar abundance from Grevesse et al. (1996)
A0179
Title | Non-LTE line formation for heavy elements in four very metal-poor stars |
ADS | L.Mashonkina et al.,ApJ, 679, 1549, 2008 |
Authors | L. Mashonkina, G. Zhao, T. Gehren, W. Aoki, M. Bergemann, K. Noguchi, J. R. Shi, M. Takada-Hidai, H. W. Zhang |
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Basic Informations
Observation Date | JD | Facility | Resolution | S/N | Exposure Time | Vrad |
2002-02-02 | N/A | SUBARUHDS | 90000 | >200 | N/A | N/A |
| N/A | VLT | 80000 | >200 | N/A | N/A |
Galactic Longitude (l) | N/A |
Galactic Latitude (b) | N/A |
Declination | N/A |
Right Ascension | N/A |
Atmospheric data
Teff | 4600 |
log g | 1.50+-0.2 |
vturb | 1.9 |
Chemical Abundances
Element | Nline | [X/H] | [X/Fe] | log-e |
Na | ... | -2.51+-0.04 | 0.02+-0.04 | 3.82+-0.04 |
Mg | ... | -2.39+-0.10 | 0.14+-0.10 | 5.19+-0.10 |
Al | ... | -3.13 | -0.60 | 3.34 |
K | ... | -2.25+-0.02 | 0.28+-0.02 | 2.87+-0.02 |
Ca I | ... | -2.52+-0.10 | 0.01+-0.10 | 3.84+-0.10 |
Fe | ... | -2.53+-0.02 | ... | 4.97+-0.02 |
Sr | ... | -2.85 | -0.32 | 0.12 |
Ba | ... | -3.57 | -1.04 | -1.44 |
Eu | ... | -3.16 | -0.63 | -2.65 |
: Data presented in the paper
: Data converted with the solar abundance from Grevesse et al. (1996)
A0185
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Basic Informations
Observation Date | JD | Facility | Resolution | S/N | Exposure Time | Vrad |
1997-05-12 | N/A | KECKHIRES | 45000 | 500 | 600 | N/A |
1997-06-20 | N/A | KECKHIRES | 45000 | N/A | 600 | N/A |
1998-06-09 | N/A | LICKHAMILTON | 60000 | 95 | 120 | N/A |
Chemical Abundances
Element | Nline | [X/H] | [X/Fe] | log-e |
Fe | ... | -2.75 | ... | 4.75 |
Sr II | ... | -3.21+-0.30 | -0.46+-0.30 | -0.24+-0.30 |
Y II | ... | -3.04+-0.10 | -0.29+-0.10 | -0.80+-0.10 |
Zr II | ... | -2.74+-0.08 | 0.01+-0.08 | -0.14+-0.08 |
Pd I | ... | <-2.29 | <0.46 | <-0.60 |
Ba II | ... | -3.93+-0.11 | -1.18+-0.11 | -1.80+-0.11 |
: Data presented in the paper
: Data converted with the solar abundance from Grevesse et al. (1996)
A0186
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Atmospheric data
Teff | 4450 |
log g | 0.50 |
vturb | 2.30 |
Chemical Abundances
Element | Nline | [X/H] | [X/Fe] | log-e |
Fe I | ... | -2.75+-0.15 | ... | 4.75+-0.15 |
Fe II | ... | -2.77+-0.08 | ... | 4.73+-0.08 |
Ba II | ... | -3.92+-0.11 | -1.17+-0.11 | -1.79+-0.11 |
La II | ... | -3.65+-0.11 | -0.90+-0.11 | -2.48+-0.11 |
Pr II | ... | <-2.25 | <0.50 | <-1.54 |
Nd II | ... | -3.36+-0.20 | -0.61+-0.20 | -1.86+-0.20 |
Eu II | ... | -3.35+-0.21 | -0.60+-0.21 | -2.84+-0.21 |
Tb II | ... | <-2.13 | <0.62 | <-2.23 |
Ho II | ... | <-2.15 | <0.60 | <-1.89 |
Er II | ... | -3.35+-0.10 | -0.60+-0.10 | -2.42+-0.10 |
Tm II | ... | <-2.45 | <0.30 | <-2.45 |
Yb II | ... | -3.85+-0.20 | -1.10+-0.20 | -2.77+-0.20 |
Hf II | ... | <-1.75 | <1.00 | <-0.87 |
Os I | ... | <-1.85 | <0.90 | <-0.40 |
Th II | ... | <-3.05 | <-0.30 | <-3.05 |
: Data presented in the paper
: Data converted with the solar abundance from Grevesse et al. (1996)
Isotope ratio