G112-43
taken from 6 paper(s):
/M.Ishigaki et al.(2010)/
/M.N.Ishigaki et al.(2012)/
/M.N.Ishigaki et al.(2013)/
/L.Zhang et al.(2009)/
/P.E.Nissen and W. J. Schuster(2010)/
/P. E. Nissen and W. J. Schuster(2011)/

M.Ishigaki et al.,PASJ, 62, 143, 2010 (A0229,ADS)
Chemical Abundances of Outer Halo Stars in the Milky Way
Stellar Parameters
Teff : 5909+-52 | log g : 3.59 | vturb : 1.43 |
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 | -1.60+-0.08 | -0.09+-0.08 | ... | -1.51+-0.08 | 0.01+-0.08 | 4.73+-0.08 | Na I |
Mg I | N/A | -1.13+-0.06 | 0.39+-0.06 | ... | -1.15+-0.06 | 0.37+-0.06 | 6.45+-0.06 | Mg I |
Si | N/A | ... | 0.33+-0.08 | ... | -1.15+-0.08 | 0.37+-0.08 | 6.36+-0.08 | Si |
Si I | 1 | -1.19+-0.08 | ... | ... | -1.15+-0.08 | 0.37+-0.08 | 6.36+-0.08 | Si I |
Ca I | N/A | -1.21+-0.02 | 0.31+-0.02 | ... | -1.19+-0.02 | 0.33+-0.02 | 5.15+-0.02 | Ca I |
Ti | N/A | ... | 0.36+-0.02 | ... | -1.09+-0.02 | 0.43+-0.02 | 3.86+-0.02 | Ti |
Ti I | 7 | -1.22+-0.03 | ... | ... | -1.15+-0.03 | 0.37+-0.03 | 3.80+-0.03 | Ti I |
Ti II | 9 | -1.07+-0.03 | ... | ... | -1.00+-0.03 | 0.52+-0.03 | 3.95+-0.03 | Ti II |
Cr | N/A | ... | -0.02+-0.03 | ... | -1.51+-0.03 | 0.01+-0.03 | 4.13+-0.03 | Cr |
Cr I | 10 | -1.60+-0.04 | ... | ... | -1.57+-0.04 | -0.05+-0.04 | 4.07+-0.04 | Cr I |
Cr II | 5 | -1.39+-0.05 | ... | ... | -1.36+-0.05 | 0.16+-0.05 | 4.28+-0.05 | Cr II |
Mn I | N/A | -1.90+-0.02 | 0.03+-0.03 | ... | -1.94+-0.02 | -0.42+-0.03 | 3.49+-0.02 | Mn I |
Fe I | 67 | -1.52+-0.01 | ... | ... | -1.52+-0.01 | ... | 5.98+-0.01 | Fe I |
Fe II | 9 | -1.51+-0.02 | ... | ... | -1.51+-0.02 | ... | 5.99+-0.02 | Fe II |
Ni I | N/A | -1.49+-0.06 | 0.02+-0.07 | ... | -1.46+-0.06 | 0.06+-0.07 | 4.76+-0.06 | Ni I |
Zn I | N/A | -1.36+-0.09 | 0.15+-0.09 | ... | -1.32+-0.09 | 0.20+-0.09 | 3.24+-0.09 | Zn I |
Y II | N/A | -1.69+-0.08 | -0.17+-0.08 | ... | -1.66+-0.08 | -0.14+-0.08 | 0.55+-0.08 | Y II |
Ba II | N/A | -1.79+-0.04 | -0.28+-0.04 | ... | -1.84+-0.04 | -0.32+-0.04 | 0.34+-0.04 | Ba II |
Observing Log
Date of Observation | JD | Facility | Resolution | S/N | Exposure Time | Vrad |
2008-07-27 | N/A | SUBARUHDS | 50000 | >100 | N/A | N/A |
Galactic Longitude (l) : N/A | Galactic Latitude (b) : N/A | Declination : | Right Ascension : |
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 : 6176+-100 | log g : 4.05+-0.3 | vturb : 1.36+-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 | ... | 0.17+-0.08 | ... | -1.15+-0.08 | 0.17+-0.08 | 6.45+-0.08 | Mg |
Si | N/A | ... | 0.21+-0.13 | ... | -1.11+-0.13 | 0.21+-0.13 | 6.40+-0.13 | Si |
Ca | N/A | ... | 0.28+-0.07 | ... | -1.04+-0.07 | 0.28+-0.07 | 5.30+-0.07 | Ca |
Ti I | N/A | ... | 0.39+-0.07 | ... | -0.93+-0.07 | 0.39+-0.07 | 4.02+-0.07 | Ti I |
Ti II | N/A | ... | 0.40+-0.07 | ... | -0.92+-0.07 | 0.40+-0.07 | 4.03+-0.07 | Ti II |
Fe I | N/A | -1.32+-0.11 | ... | ... | -1.32+-0.11 | ... | 6.18+-0.11 | Fe I |
Fe II | N/A | -1.33+-0.12 | ... | ... | -1.33+-0.12 | ... | 6.17+-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 | -88.1+-0.5 |
Galactic Longitude (l) : N/A | Galactic Latitude (b) : N/A | Declination : | Right Ascension : |
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 : 6176 | log g : 4.05 | vturb : 1.36 |
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 | ... | -0.11+-0.12 | ... | -1.42+-0.12 | -0.11+-0.12 | 4.82+-0.12 | Na I |
Sc II | N/A | ... | 0.17+-0.07 | ... | -1.14+-0.07 | 0.17+-0.07 | 2.01+-0.07 | Sc II |
V I | N/A | ... | 0.12+-0.13 | ... | -1.19+-0.13 | 0.12+-0.13 | 2.74+-0.13 | V I |
Cr I | N/A | ... | -0.04+-0.07 | ... | -1.35+-0.07 | -0.04+-0.07 | 4.29+-0.07 | Cr I |
Cr II | N/A | ... | 0.21+-0.08 | ... | -1.10+-0.08 | 0.21+-0.08 | 4.54+-0.08 | Cr II |
Mn I | N/A | ... | -0.2+-0.08 | ... | -1.51+-0.08 | -0.20+-0.08 | 3.92+-0.08 | Mn I |
Fe I | N/A | -1.31+-0.11 | ... | ... | -1.31+-0.11 | ... | 6.19+-0.11 | Fe I |
Fe II | N/A | -1.33+-0.12 | ... | ... | -1.33+-0.12 | ... | 6.17+-0.12 | Fe II |
Co I | N/A | ... | 0.18+-0.12 | ... | -1.13+-0.12 | 0.18+-0.12 | 3.86+-0.12 | Co I |
Cu I | N/A | ... | -0.49+-0.12 | ... | -1.80+-0.12 | -0.49+-0.12 | 2.39+-0.12 | Cu I |
Zn I | N/A | ... | 0.3+-0.09 | ... | -1.01+-0.09 | 0.30+-0.09 | 3.55+-0.09 | Zn I |
Sr II | N/A | ... | 0.09+-0.2 | ... | -1.22+-0.2 | 0.09+-0.2 | 1.65+-0.2 | Sr II |
Y II | N/A | ... | -0.16+-0.08 | ... | -1.47+-0.08 | -0.16+-0.08 | 0.74+-0.08 | Y II |
Zr II | N/A | ... | 0.15+-0.1 | ... | -1.16+-0.1 | 0.15+-0.1 | 1.42+-0.1 | Zr II |
Ba II | N/A | ... | -0.21+-0.13 | ... | -1.52+-0.13 | -0.21+-0.13 | 0.66+-0.13 | Ba II |
La II | N/A | ... | 0.13+-0.11 | ... | -1.18+-0.11 | 0.13+-0.11 | -0.08+-0.11 | La II |
Eu II | N/A | ... | 0.35+-0.21 | ... | -0.96+-0.21 | 0.35+-0.21 | -0.44+-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 |
L.Zhang et al.,ApJ, 706, 1095, 2009 (A0299,ADS)
Chemical Compositions of Kinematically Selected Outer Halo Stars
Stellar Parameters
Teff : 6000+-70 | log g : 4.00+-0.10 | vturb : 1.40+-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 |
Na I | 1 | -1.34+-0.06 | -0.09 | ... | -1.25+-0.06 | -0.11 | 4.99+-0.06 | Na I |
Mg I | 1 | -0.96+-0.12 | 0.35+-0.12 | ... | -0.98+-0.12 | 0.16+-0.12 | 6.62+-0.12 | Mg I |
Si | N/A | ... | 0.26+-0.06 | ... | -1.01+-0.06 | 0.13+-0.06 | 6.50+-0.06 | Si |
Si I | 3 | -1.05+-0.06 | ... | ... | -1.01+-0.06 | 0.13+-0.06 | 6.50+-0.06 | Si I |
Si II | 1 | -1.05+-0.05 | ... | ... | -1.01+-0.05 | 0.13+-0.05 | 6.50+-0.05 | Si II |
Ca I | 23 | -1.03+-0.06 | 0.28+-0.06 | ... | -1.01+-0.06 | 0.13+-0.06 | 5.33+-0.06 | Ca I |
Sc II | 9 | -1.07+-0.05 | 0.24+-0.05 | ... | -1.13+-0.05 | 0.01+-0.05 | 2.02+-0.05 | Sc II |
Ti | N/A | ... | 0.40+-0.05 | ... | -0.87+-0.05 | 0.27+-0.05 | 4.08+-0.05 | Ti |
Ti I | 27 | -0.91+-0.05 | ... | ... | -0.87+-0.05 | 0.27+-0.05 | 4.08+-0.05 | Ti I |
Ti II | 2 | -0.86+-0.07 | ... | ... | -0.82+-0.07 | 0.32+-0.07 | 4.13+-0.07 | Ti II |
Cr | N/A | ... | -0.11 | ... | -1.39 | -0.25 | 4.25 | Cr |
Cr I | 13 | -1.37+-0.05 | ... | ... | -1.34+-0.05 | -0.20+-0.05 | 4.30+-0.05 | Cr I |
Cr II | 2 | -1.20+-0.04 | ... | ... | -1.17+-0.04 | -0.03+-0.04 | 4.47+-0.04 | Cr II |
Mn I | 2 | -1.58+-0.03 | -0.3 | ... | -1.62+-0.03 | -0.48 | 3.81+-0.03 | Mn I |
Fe | N/A | -1.31+-0.05 | ... | ... | -1.14+-0.05 | ... | 6.36+-0.05 | Fe |
Fe I | 95 | -1.31+-0.05 | ... | ... | -1.14+-0.05 | ... | 6.36+-0.05 | Fe I |
Fe II | 13 | -1.31+-0.06 | ... | ... | -1.14+-0.06 | ... | 6.36+-0.06 | Fe II |
Ni I | 14 | -1.29+-0.05 | 0.02+-0.05 | ... | -1.26+-0.05 | -0.12+-0.05 | 4.96+-0.05 | Ni I |
Zn I | 3 | -1.12+-0.04 | 0.19+-0.04 | ... | -1.08+-0.04 | 0.06+-0.04 | 3.48+-0.04 | Zn I |
Y II | 2 | -1.4+-0.05 | -0.14 | ... | -1.37+-0.05 | -0.23 | 0.84+-0.05 | Y II |
Ba II | 3 | -1.61+-0.06 | -0.36 | ... | -1.66+-0.06 | -0.52 | 0.52+-0.06 | Ba II |
Binary Parameters
Observing Log
Date of Observation | JD | Facility | Resolution | S/N | Exposure Time | Vrad |
2003-02 | N/A | SUBARUHDS | 50000 | N/A | 900 | -83.8 |
Galactic Longitude (l) : N/A | Galactic Latitude (b) : N/A | Declination : -000400.9 | Right Ascension : 074343.97 |
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 : 6074 | log g : 4.03 | vturb : 1.3 |
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 |
Na | N/A | ... | -0.11 | ... | -1.27 | -0.02 | 4.97 | Na |
Mg | N/A | ... | 0.21 | ... | -1.06 | 0.19 | 6.54 | Mg |
Si | N/A | ... | 0.15 | ... | -1.06 | 0.19 | 6.45 | Si |
Ca | N/A | ... | 0.29 | ... | -0.94 | 0.31 | 5.40 | Ca |
Ti | N/A | ... | 0.29 | ... | -0.89 | 0.36 | 4.06 | Ti |
Cr | N/A | ... | 0.00 | ... | -1.22 | 0.03 | 4.42 | Cr |
Fe | N/A | -1.25 | ... | ... | -1.25 | ... | 6.25 | Fe |
Ni | N/A | ... | -0.02 | ... | -1.24 | 0.01 | 4.98 | Ni |
Observing Log
Date of Observation | JD | Facility | Resolution | S/N | Exposure Time | Vrad |
2002-02-17-0213 | N/A | VLT | 55000 | 340 | N/A | -83.7 |
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 | ... | -0.19 | ... | -1.48 | -0.23 | 3.95 | Mn |
Fe | N/A | -1.25 | ... | ... | -1.25 | ... | 6.25 | Fe |
Cu | N/A | ... | -0.52 | ... | -1.75 | -0.50 | 2.44 | Cu |
Zn | N/A | ... | 0.3 | ... | -0.91 | 0.34 | 3.65 | Zn |
Y | N/A | ... | -0.14 | ... | -1.36 | -0.11 | 0.85 | Y |
Ba | N/A | ... | -0.27 | ... | -1.57 | -0.32 | 0.61 | Ba |
Observing Log
Date of Observation | JD | Facility | Resolution | S/N | Exposure Time | Vrad |
2002-02-17-0213 | N/A | VLT | 55000 | 340 | N/A | -83.7 |