G188-22
taken from 8 paper(s):
/J.R.Shi et al.(2007)/
/J.Simmerer et al.(2004)/
/I.U.Roederer et al.(2010)/
/M.N.Ishigaki et al.(2012)/
/M.N.Ishigaki et al.(2013)/
/I.U.Roederer et al.(2014)/
/P.E.Nissen and W. J. Schuster(2010)/
/P. E. Nissen and W. J. Schuster(2011)/

J.R.Shi et al.,AAP, 465, 587, 2007 (A0113,ADS)
Lithium abundances in metal-poor stars (Research Note)
Stellar Parameters
Teff : 6040 | log g : 4.37 | vturb : 1.50 |
Chemical Abundances
| | Original Data | Converted Data Asplund et al. (2009) | |
Element | Nline | [X/H] | [X/Fe] | log-e | [X/H] | [X/Fe] | log-e | Element |
Li I | N/A | ... | ... | 2.26 | -1.00 | 0.24 | 2.26 | Li I |
Fe | N/A | -1.25 | ... | ... | -1.24 | ... | 6.26 | Fe |
Observing Log
Date of Observation | JD | Facility | Resolution | S/N | Exposure Time | Vrad |
| N/A | FOCES | 40000 | 100-400 | N/A | N/A |
Galactic Longitude (l) : N/A | Galactic Latitude (b) : N/A | Declination : N/A | Right Ascension : N/A |
J.Simmerer et al.,ApJ, 617, 1091, 2004 (A0131,ADS)
The Rise of the s-Process in the Galaxy
Stellar Parameters
Teff : 5827 | log g : 4.27 | vturb : 1.20 |
Chemical Abundances
| | Original Data | Converted Data Asplund et al. (2009) | |
Element | Nline | [X/H] | [X/Fe] | log-e | [X/H] | [X/Fe] | log-e | Element |
C | N/A | ... | -0.35 | ... | -1.69 | -0.17 | 6.74 | C |
Fe I | 7 | -1.52 | ... | ... | -1.52 | ... | 5.98 | Fe I |
Fe II | 8 | -1.35 | ... | ... | -1.35 | ... | 6.15 | Fe II |
La II | N/A | ... | ... | -0.12+-0.05 | -1.22+-0.05 | 0.30+-0.05 | -0.12+-0.05 | La II |
Eu II | N/A | ... | ... | -0.6+-0.1 | -1.12+-0.1 | 0.40+-0.1 | -0.6+-0.1 | Eu II |
Observing Log
Date of Observation | JD | Facility | Resolution | S/N | Exposure Time | Vrad |
| N/A | MCDONALD | 60000 | 100 | N/A | N/A |
Galactic Longitude (l) : N/A | Galactic Latitude (b) : N/A | Declination : N/A | Right Ascension : N/A |
I.U.Roederer et al.,ApJ, 724, 975, 2010 (A0243,ADS)
THE UBIQUITY OF THE RAPID NEUTRON-CAPTURE PROCESS
Chemical Abundances
| | Original Data | Converted Data Asplund et al. (2009) | |
Element | Nline | [X/H] | [X/Fe] | log-e | [X/H] | [X/Fe] | log-e | Element |
Fe | N/A | -1.52 | ... | ... | -1.52 | ... | 5.98 | Fe |
Zn I | N/A | ... | ... | 3.24 | -1.32 | 0.20 | 3.24 | Zn I |
Y II | N/A | ... | ... | 0.94 | -1.27 | 0.25 | 0.94 | Y II |
Pb I | N/A | ... | ... | <+1.30 | <-0.74 | <0.78 | <+1.30 | Pb I |
Observing Log
Date of Observation | JD | Facility | Resolution | S/N | Exposure Time | Vrad |
| N/A | MCDONALD | 60000 | 100 | N/A | N/A |
Galactic Longitude (l) : N/A | Galactic Latitude (b) : N/A | Declination : N/A | Right Ascension : N/A |
M.N.Ishigaki et al.,ApJ, 753, 64, 2012 (A0273,ADS)
Chemical Abundances of the Milky Way Thick Disk and Stellar Halo. I. Implications of [alpha/Fe] for Star Formation Histories in Their Progenitors
Stellar Parameters
Teff : 6170+-100 | log g : 4.52+-0.3 | vturb : 1.13+-0.3 |
Chemical Abundances
| | Original Data | Converted Data Asplund et al. (2009) | |
Element | Nline | [X/H] | [X/Fe] | log-e | [X/H] | [X/Fe] | log-e | Element |
Mg | N/A | ... | 0.28+-0.08 | ... | -0.99+-0.08 | 0.28+-0.08 | 6.61+-0.08 | Mg |
Si | N/A | ... | 0.29+-0.11 | ... | -0.98+-0.11 | 0.29+-0.11 | 6.53+-0.11 | Si |
Ca | N/A | ... | 0.26+-0.07 | ... | -1.01+-0.07 | 0.26+-0.07 | 5.33+-0.07 | Ca |
Ti I | N/A | ... | 0.35+-0.07 | ... | -0.92+-0.07 | 0.35+-0.07 | 4.03+-0.07 | Ti I |
Ti II | N/A | ... | 0.45+-0.08 | ... | -0.82+-0.08 | 0.45+-0.08 | 4.13+-0.08 | Ti II |
Fe I | N/A | -1.27+-0.10 | ... | ... | -1.27+-0.10 | ... | 6.23+-0.10 | Fe I |
Fe II | N/A | -1.28+-0.12 | ... | ... | -1.28+-0.12 | ... | 6.22+-0.12 | Fe II |
Binary Parameters
Observing Log
Date of Observation | JD | Facility | Resolution | S/N | Exposure Time | Vrad |
N/A | N/A | SUBARUHDS | 50000 | N/A | N/A | -95.7+-0.3 |
Galactic Longitude (l) : N/A | Galactic Latitude (b) : N/A | Declination : +272333.22 | Right Ascension : 214356.002 |
M.N.Ishigaki et al.,ApJ, 771, 67, 2013 (A0286,ADS)
Chemical Abundances of the Milky Way Thick Disk and Stellar Halo. II. Sodium, Iron-peak, and Neutron-capture Elements
Stellar Parameters
Teff : 6170 | log g : 4.52 | vturb : 1.13 |
Chemical Abundances
| | Original Data | Converted Data Asplund et al. (2009) | |
Element | Nline | [X/H] | [X/Fe] | log-e | [X/H] | [X/Fe] | log-e | Element |
Na I | N/A | ... | 0.02+-0.11 | ... | -1.24+-0.11 | 0.02+-0.11 | 5.00+-0.11 | Na I |
Sc II | N/A | ... | 0.23+-0.07 | ... | -1.03+-0.07 | 0.23+-0.07 | 2.12+-0.07 | Sc II |
V I | N/A | ... | 0.1+-0.13 | ... | -1.16+-0.13 | 0.10+-0.13 | 2.77+-0.13 | V I |
Cr I | N/A | ... | -0.09+-0.07 | ... | -1.35+-0.07 | -0.09+-0.07 | 4.29+-0.07 | Cr I |
Cr II | N/A | ... | 0.19+-0.07 | ... | -1.07+-0.07 | 0.19+-0.07 | 4.57+-0.07 | Cr II |
Mn I | N/A | ... | -0.27+-0.12 | ... | -1.53+-0.12 | -0.27+-0.12 | 3.90+-0.12 | Mn I |
Fe I | N/A | -1.26+-0.1 | ... | ... | -1.26+-0.1 | ... | 6.24+-0.1 | Fe I |
Fe II | N/A | -1.29+-0.12 | ... | ... | -1.29+-0.12 | ... | 6.21+-0.12 | Fe II |
Ni I | N/A | ... | -0.02+-0.08 | ... | -1.28+-0.08 | -0.02+-0.08 | 4.94+-0.08 | Ni I |
Zn I | N/A | ... | 0.11+-0.1 | ... | -1.15+-0.1 | 0.11+-0.1 | 3.41+-0.1 | Zn I |
Y II | N/A | ... | 0.26+-0.08 | ... | -1.00+-0.08 | 0.26+-0.08 | 1.21+-0.08 | Y II |
Ba II | N/A | ... | 0.32+-0.15 | ... | -0.94+-0.15 | 0.32+-0.15 | 1.24+-0.15 | Ba II |
Nd II | N/A | ... | 0.55+-0.08 | ... | -0.71+-0.08 | 0.55+-0.08 | 0.71+-0.08 | Nd II |
Eu II | N/A | ... | 0.33+-0.21 | ... | -0.93+-0.21 | 0.33+-0.21 | -0.41+-0.21 | Eu II |
Observing Log
Date of Observation | JD | Facility | Resolution | S/N | Exposure Time | Vrad |
| N/A | SUBARUHDS | 50000 | N/A | N/A | N/A |
Galactic Longitude (l) : N/A | Galactic Latitude (b) : N/A | Declination : N/A | Right Ascension : N/A |
I.U.Roederer et al.,AJ, 147, 136, 2014 (A0309,ADS)
A SEARCH FOR STARS OF VERY LOW METAL ABUNDANCE. VI. DETAILED ABUNDANCES OF 313 METAL-POOR STARS
Stellar Parameters
Teff : 5890+-48 | log g : 3.9+-0.22 | vturb : 0.95+-0.06 |
Chemical Abundances
| | Original Data | Converted Data Asplund et al. (2009) | |
Element | Nline | [X/H] | [X/Fe] | log-e | [X/H] | [X/Fe] | log-e | Element |
Li I | 1 | ... | ... | 2.21 | -1.05 | 0.45 | 2.21 | Li I |
CH | 1 | ... | -0.10+-0.25 | 6.92 | -1.51 | -0.01+-0.25 | 6.92 | CH |
CN | 1 | ... | 0.25+-0.28 | 6.67 | -1.16 | 0.34+-0.28 | 6.67 | CN |
O I | 2 | ... | 0.43+-0.19 | 7.62 | -1.07 | 0.43+-0.19 | 7.62 | O I |
Na I | 2 | ... | -0.02+-0.22 | 4.72 | -1.52 | -0.02+-0.22 | 4.72 | Na I |
Mg I | 3 | ... | 0.36+-0.23 | 6.46 | -1.14 | 0.36+-0.23 | 6.46 | Mg I |
Al I | 1 | ... | -0.32+-0.34 | 4.63 | -1.82 | -0.32+-0.34 | 4.63 | Al I |
Si I | 3 | ... | 0.45+-0.26 | 6.46 | -1.05 | 0.45+-0.26 | 6.46 | Si I |
K I | 1 | ... | 0.35+-0.25 | 3.88 | -1.15 | 0.35+-0.25 | 3.88 | K I |
Ca I | 12 | ... | 0.42+-0.27 | 5.26 | -1.08 | 0.42+-0.27 | 5.26 | Ca I |
Sc II | 6 | ... | 0.04+-0.14 | 1.76 | -1.39 | 0.11+-0.14 | 1.76 | Sc II |
Ti I | 15 | ... | 0.22+-0.20 | 3.67 | -1.28 | 0.22+-0.20 | 3.67 | Ti I |
Ti II | 24 | ... | 0.36+-0.13 | 3.88 | -1.07 | 0.43+-0.13 | 3.88 | Ti II |
V I | 1 | ... | 0.02+-0.22 | 2.45 | -1.48 | 0.02+-0.22 | 2.45 | V I |
V II | 2 | ... | 0.15+-0.23 | 2.65 | -1.28 | 0.22+-0.23 | 2.65 | V II |
Cr I | 10 | ... | -0.13+-0.20 | 4.01 | -1.63 | -0.13+-0.20 | 4.01 | Cr I |
Cr II | 3 | ... | 0.18+-0.14 | 4.38 | -1.26 | 0.24+-0.14 | 4.38 | Cr II |
Mn I | 4 | ... | -0.44+-0.20 | 3.50 | -1.93 | -0.43+-0.20 | 3.50 | Mn I |
Fe I | 112 | -1.50+-0.21 | ... | 6.00 | -1.50+-0.21 | ... | 6.00 | Fe I |
Fe II | 11 | -1.44+-0.14 | ... | 6.06 | -1.44+-0.14 | ... | 6.06 | Fe II |
Co I | 3 | ... | -0.11+-0.26 | 3.38 | -1.61 | -0.11+-0.26 | 3.38 | Co I |
Ni I | 10 | ... | 0.07+-0.22 | 4.79 | -1.43 | 0.07+-0.22 | 4.79 | Ni I |
Cu I | 1 | ... | -0.48+-0.22 | 2.21 | -1.98 | -0.48+-0.22 | 2.21 | Cu I |
Zn I | 3 | ... | 0.16+-0.20 | 3.22 | -1.34 | 0.16+-0.20 | 3.22 | Zn I |
Rb I | 1 | ... | <1.38 | <2.40 | <0.04 | <1.54 | <2.40 | Rb I |
Sr II | 1 | ... | 0.29+-0.13 | 1.72 | -1.15 | 0.35+-0.13 | 1.72 | Sr II |
Y II | 5 | ... | -0.06+-0.15 | 0.72 | -1.49 | 0.01+-0.15 | 0.72 | Y II |
Zr II | 3 | ... | 0.45+-0.14 | 1.59 | -0.99 | 0.51+-0.14 | 1.59 | Zr II |
Nb II | 1 | ... | <1.49 | <1.51 | <0.05 | <1.55 | <1.51 | Nb II |
Mo I | 1 | ... | <0.61 | <0.99 | <-0.89 | <0.61 | <0.99 | Mo I |
Tc I | 1 | ... | ... | <1.38 | <1.38 | <2.88 | <1.38 | Tc I |
Sn I | 1 | ... | <1.54 | <2.11 | <0.04 | <1.54 | <2.11 | Sn I |
Ba II | 3 | ... | 0.29+-0.13 | 1.04 | -1.14 | 0.36+-0.13 | 1.04 | Ba II |
La II | 4 | ... | 0.12+-0.16 | -0.22 | -1.32 | 0.18+-0.16 | -0.22 | La II |
Ce II | 4 | ... | 0.13+-0.20 | 0.28 | -1.30 | 0.20+-0.20 | 0.28 | Ce II |
Nd II | 1 | ... | -0.12+-0.18 | -0.14 | -1.56 | -0.06+-0.18 | -0.14 | Nd II |
Eu II | 2 | ... | 0.12+-0.14 | -0.80 | -1.32 | 0.18+-0.14 | -0.80 | Eu II |
Gd II | 1 | ... | <0.53 | <0.16 | <-0.91 | <0.59 | <0.16 | Gd II |
Tb II | 4 | ... | <0.95 | <-0.19 | <-0.51 | <0.99 | <-0.19 | Tb II |
Dy II | 1 | ... | <0.26 | <-0.08 | <-1.18 | <0.32 | <-0.08 | Dy II |
Er II | 1 | ... | <0.91 | <0.39 | <-0.53 | <0.97 | <0.39 | Er II |
Tm II | 1 | ... | <1.66 | <0.32 | <0.20 | <1.70 | <0.32 | Tm II |
Hf II | 2 | ... | <1.00 | <0.41 | <-0.30 | <1.20 | <0.41 | Hf II |
Pb I | 1 | ... | <1.29 | <1.83 | <-0.21 | <1.29 | <1.83 | Pb I |
Binary Parameters
Binarity | Negative |
Vrad | -94.4 |
Observing Log
Date of Observation | JD | Facility | Resolution | S/N | Exposure Time | Vrad |
2008-08-13-09:38 | 2454691.906 | MCDONALD | 33000 | 60-170 | 5400 | -94.3 |
2008-09-05-06:51 | 2454714.79 | MCDONALD | 33000 | 60-170 | 3600 | -94.6 |
Galactic Longitude (l) : N/A | Galactic Latitude (b) : N/A | Declination : N/A | Right Ascension : N/A |
P.E.Nissen et al.,AAP, 511, L10, 2010 (C0012,ADS)
Two distinct halo populations in the solar neighborhood. Evidence from stellar abundance ratios and kinematics
Stellar Parameters
Teff : 5974 | log g : 4.18 | vturb : 1.5 |
Chemical Abundances
| | Original Data | Converted Data Asplund et al. (2009) | |
Element | Nline | [X/H] | [X/Fe] | log-e | [X/H] | [X/Fe] | log-e | Element |
Na | N/A | ... | -0.04 | ... | -1.27 | 0.05 | 4.97 | Na |
Mg | N/A | ... | 0.39 | ... | -0.95 | 0.37 | 6.65 | Mg |
Si | N/A | ... | 0.37 | ... | -0.91 | 0.41 | 6.60 | Si |
Ca | N/A | ... | 0.37 | ... | -0.93 | 0.39 | 5.41 | Ca |
Ti | N/A | ... | 0.28 | ... | -0.97 | 0.35 | 3.98 | Ti |
Cr | N/A | ... | -0.04 | ... | -1.33 | -0.01 | 4.31 | Cr |
Fe | N/A | -1.32 | ... | ... | -1.32 | ... | 6.18 | Fe |
Ni | N/A | ... | -0.01 | ... | -1.30 | 0.02 | 4.92 | Ni |
Observing Log
Date of Observation | JD | Facility | Resolution | S/N | Exposure Time | Vrad |
2003-08-09-0608 | N/A | VLT | 55000 | 450 | N/A | -93.9 |
Galactic Longitude (l) : N/A | Galactic Latitude (b) : N/A | Declination : N/A | Right Ascension : N/A |
P. E. Nissen et al.,AAP, 530, A15, 2011 (C0013,ADS)
Two distinct halo populations in the solar neighborhood II. Evidence from stellar abundances of Mn, Cu, Zn, Y, and Ba
Stellar Parameters
Chemical Abundances
| | Original Data | Converted Data Asplund et al. (2009) | |
Element | Nline | [X/H] | [X/Fe] | log-e | [X/H] | [X/Fe] | log-e | Element |
Mn | N/A | ... | -0.34 | ... | -1.70 | -0.38 | 3.73 | Mn |
Fe | N/A | -1.32 | ... | ... | -1.32 | ... | 6.18 | Fe |
Cu | N/A | ... | -0.41 | ... | -1.71 | -0.39 | 2.48 | Cu |
Zn | N/A | ... | 0.15 | ... | -1.13 | 0.19 | 3.43 | Zn |
Y | N/A | ... | 0.15 | ... | -1.14 | 0.18 | 1.07 | Y |
Ba | N/A | ... | 0.03 | ... | -1.34 | -0.02 | 0.84 | Ba |
Observing Log
Date of Observation | JD | Facility | Resolution | S/N | Exposure Time | Vrad |
2003-08-09-0608 | N/A | VLT | 55000 | 450 | N/A | -93.9 |