G165-39
taken from 7 paper(s):
/J.R.Shi et al.(2007)/
/A.M.Boesgaard et al.(2005)/
/A.Stephens and A. M. Boesgaard(2002)/
/M.Ishigaki et al.(2010)/
/T.Gehren et al.(2006)/
/M.N.Ishigaki et al.(2012)/
/M.N.Ishigaki et al.(2013)/
Lithium abundances in metal-poor stars (Research Note)
Stellar Parameters
Teff : 6220 | log g : 3.96 | vturb : 1.90 |
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 | ... | ... | 2.24 | -1.02 | 0.97 | 2.24 | Li I |
Fe | N/A | -2.00 | ... | ... | -1.99 | ... | 5.51 | Fe |
Position
Observing Log
Date of Observation | JD | Facility | Resolution | S/N | Exposure Time | Vrad |
| N/A | FOCES | 40000 | 100-400 | N/A | N/A |
Lithium and Lithium Depletion in Halo Stars on Extreme Orbits
Stellar Parameters
Teff : 6118+-52 | log g : 3.53+-0.19 | vturb : 1.45+-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 | N/A | ... | ... | 2.20+-0.05 | -1.06+-0.05 | 1.09+-0.05 | 2.20+-0.05 | Li I |
Fe | N/A | -2.17+-0.04 | ... | ... | -2.15+-0.04 | ... | 5.35+-0.04 | Fe |
Position
Observing Log
Date of Observation | JD | Facility | Resolution | S/N | Exposure Time | Vrad |
| N/A | KECKHIRES | 48000 | 210 | N/A | N/A |
ABUNDANCES FROM HIGH-RESOLUTION SPECTRA OF KINEMATICALLY INTERESTING HALO STARS
Stellar Parameters
Teff : 6118+-52 | log g : 3.53+-0.19 | vturb : 1.45+-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 |
Mg I | N/A | -1.91+-0.25 | +0.27+-0.26 | ... | -1.93+-0.25 | 0.24+-0.26 | 5.67+-0.25 | Mg I |
Ca I | N/A | -1.69+-0.10 | +0.49+-0.11 | ... | -1.67+-0.10 | 0.50+-0.11 | 4.67+-0.10 | Ca I |
Ti | N/A | ... | +0.44+-0.05 | ... | -1.70+-0.05 | 0.47+-0.05 | 3.25+-0.05 | Ti |
Ti I | 7 | -1.74+-0.03 | ... | ... | -1.70+-0.03 | 0.47+-0.03 | 3.25+-0.03 | Ti I |
Ti II | 7 | -1.71+-0.05 | ... | ... | -1.67+-0.05 | 0.50+-0.05 | 3.28+-0.05 | Ti II |
Cr | N/A | ... | +0.05+-0.08 | ... | -2.10+-0.08 | 0.07+-0.08 | 3.54+-0.08 | Cr |
Cr I | 8 | -2.18+-0.08 | ... | ... | -2.15+-0.08 | 0.02+-0.08 | 3.49+-0.08 | Cr I |
Cr II | 3 | -2.02+-0.12 | ... | ... | -1.99+-0.12 | 0.18+-0.12 | 3.65+-0.12 | Cr II |
Fe | N/A | -2.18+-0.04 | ... | ... | -2.17+-0.04 | ... | 5.33+-0.04 | Fe |
Fe I | 50 | -2.17+-0.06 | ... | ... | -2.16+-0.06 | ... | 5.34+-0.06 | Fe I |
Fe II | 10 | -2.19+-0.06 | ... | ... | -2.18+-0.06 | ... | 5.32+-0.06 | Fe II |
Ni I | N/A | -2.16+-0.09 | +0.02+-0.10 | ... | -2.13+-0.09 | 0.04+-0.10 | 4.09+-0.09 | Ni I |
Y II | N/A | -2.15+-0.06 | +0.02+-0.07 | ... | -2.12+-0.06 | 0.05+-0.07 | 0.09+-0.06 | Y II |
Ba II | N/A | -2.16+-0.09 | +0.02+-0.10 | ... | -2.21+-0.09 | -0.04+-0.10 | -0.03+-0.09 | Ba II |
Binary Parameters
Position
Observing Log
Date of Observation | JD | Facility | Resolution | S/N | Exposure Time | Vrad |
| 2450595.267 | KECKHIRES | 48000 | 210 | 300 | -170.6+-0.7 |
Chemical Abundances of Outer Halo Stars in the Milky Way
Stellar Parameters
Teff : 6162+-68 | log g : 3.62 | vturb : 1.57 |
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 | -2.41+-0.06 | -0.21+-0.06 | ... | -2.32+-0.06 | -0.12+-0.06 | 3.92+-0.06 | Na I |
Mg I | N/A | -1.75+-0.07 | 0.45+-0.07 | ... | -1.77+-0.07 | 0.43+-0.07 | 5.83+-0.07 | Mg I |
Ca I | N/A | -1.74+-0.02 | 0.46+-0.02 | ... | -1.72+-0.02 | 0.48+-0.02 | 4.62+-0.02 | Ca I |
Ti | N/A | ... | 0.46+-0.02 | ... | -1.67+-0.02 | 0.53+-0.02 | 3.28+-0.02 | Ti |
Ti I | 5 | -1.77+-0.03 | ... | ... | -1.70+-0.03 | 0.50+-0.03 | 3.25+-0.03 | Ti I |
Ti II | 9 | -1.67+-0.04 | ... | ... | -1.60+-0.04 | 0.60+-0.04 | 3.35+-0.04 | Ti II |
Cr | N/A | ... | -0.03+-0.04 | ... | -2.20+-0.04 | 0.00+-0.04 | 3.44+-0.04 | Cr |
Cr I | 2 | -2.38+-0.05 | ... | ... | -2.35+-0.05 | -0.15+-0.05 | 3.29+-0.05 | Cr I |
Cr II | 2 | -2.08+-0.05 | ... | ... | -2.05+-0.05 | 0.15+-0.05 | 3.59+-0.05 | Cr II |
Mn I | N/A | -2.69+-0.05 | 0.05+-0.05 | ... | -2.73+-0.05 | -0.53+-0.05 | 2.70+-0.05 | Mn I |
Fe I | 39 | -2.20+-0.01 | ... | ... | -2.20+-0.01 | ... | 5.30+-0.01 | Fe I |
Fe II | 10 | -2.19+-0.02 | ... | ... | -2.19+-0.02 | ... | 5.31+-0.02 | Fe II |
Ni I | N/A | -2.28+-0.05 | -0.08+-0.05 | ... | -2.25+-0.05 | -0.05+-0.05 | 3.97+-0.05 | Ni I |
Zn I | N/A | -2.23+-0.07 | -0.03+-0.07 | ... | -2.19+-0.07 | 0.01+-0.07 | 2.37+-0.07 | Zn I |
Y II | N/A | -2.14+-0.06 | 0.06+-0.06 | ... | -2.11+-0.06 | 0.09+-0.06 | 0.10+-0.06 | Y II |
Ba II | N/A | -2.37+-0.04 | -0.18+-0.04 | ... | -2.42+-0.04 | -0.22+-0.04 | -0.24+-0.04 | Ba II |
Position
Observing Log
Date of Observation | JD | Facility | Resolution | S/N | Exposure Time | Vrad |
2008-07-27 | N/A | SUBARUHDS | 50000 | 375 | 1200 | -170.3+-0.3 |
Na, Mg and Al abundances as a population discriminant for nearby metal-poor stars
Stellar Parameters
Teff : 6220 | log g : 3.96+-0.30 | vturb : 1.9 |
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 | 2 | ... | 0.04 | ... | -1.87 | 0.12 | 4.37 | Na I |
Mg I | 4 | ... | 0.09 | ... | -1.93 | 0.06 | 5.67 | Mg I |
Al I | 1 | ... | -0.92 | ... | -2.90 | -0.91 | 3.55 | Al I |
Fe | N/A | -2.00 | ... | ... | -1.99 | ... | 5.51 | Fe |
Position
Observing Log
Date of Observation | JD | Facility | Resolution | S/N | Exposure Time | Vrad |
| N/A | FOCES | 40000 | 200 | 1800 | N/A |
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 : 6449+-100 | log g : 4.07+-0.3 | vturb : 1.29+-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 | ... | 0.21+-0.07 | ... | -1.76+-0.07 | 0.21+-0.07 | 5.84+-0.07 | Mg |
Ca | N/A | ... | 0.44+-0.07 | ... | -1.53+-0.07 | 0.44+-0.07 | 4.81+-0.07 | Ca |
Ti I | N/A | ... | 0.51+-0.07 | ... | -1.46+-0.07 | 0.51+-0.07 | 3.49+-0.07 | Ti I |
Ti II | N/A | ... | 0.48+-0.08 | ... | -1.49+-0.08 | 0.48+-0.08 | 3.46+-0.08 | Ti II |
Fe I | N/A | -1.97+-0.09 | ... | ... | -1.97+-0.09 | ... | 5.53+-0.09 | Fe I |
Fe II | N/A | -1.98+-0.11 | ... | ... | -1.98+-0.11 | ... | 5.52+-0.11 | Fe II |
Binary Parameters
Position
Observing Log
Date of Observation | JD | Facility | Resolution | S/N | Exposure Time | Vrad |
N/A | N/A | SUBARUHDS | 50000 | N/A | N/A | -169.6+-0.6 |
Chemical Abundances of the Milky Way Thick Disk and Stellar Halo. II. Sodium, Iron-peak, and Neutron-capture Elements
Stellar Parameters
Teff : 6449 | log g : 4.07 | vturb : 1.29 |
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 | ... | -0.01+-0.09 | ... | -1.99+-0.09 | -0.01+-0.09 | 4.25+-0.09 | Na I |
Sc II | N/A | ... | 0.21+-0.08 | ... | -1.77+-0.08 | 0.21+-0.08 | 1.38+-0.08 | Sc II |
Cr I | N/A | ... | -0.04+-0.08 | ... | -2.02+-0.08 | -0.04+-0.08 | 3.62+-0.08 | Cr I |
Cr II | N/A | ... | 0.13+-0.1 | ... | -1.85+-0.1 | 0.13+-0.1 | 3.79+-0.1 | Cr II |
Mn I | N/A | ... | -0.38+-0.07 | ... | -2.36+-0.07 | -0.38+-0.07 | 3.07+-0.07 | Mn I |
Fe I | N/A | -1.98+-0.09 | ... | ... | -1.98+-0.09 | ... | 5.52+-0.09 | Fe I |
Fe II | N/A | -1.98+-0.11 | ... | ... | -1.98+-0.11 | ... | 5.52+-0.11 | Fe II |
Co I | N/A | ... | 0.09+-0.1 | ... | -1.89+-0.1 | 0.09+-0.1 | 3.10+-0.1 | Co I |
Ni I | N/A | ... | -0.09+-0.09 | ... | -2.07+-0.09 | -0.09+-0.09 | 4.15+-0.09 | Ni I |
Cu I | N/A | ... | -4.91 | ... | -6.89 | -4.91 | -2.70 | Cu I |
Zn I | N/A | ... | 0.1+-0.08 | ... | -1.88+-0.08 | 0.10+-0.08 | 2.68+-0.08 | Zn I |
Sr II | N/A | ... | 0.31+-0.21 | ... | -1.67+-0.21 | 0.31+-0.21 | 1.20+-0.21 | Sr II |
Y II | N/A | ... | 0.06+-0.09 | ... | -1.92+-0.09 | 0.06+-0.09 | 0.29+-0.09 | Y II |
Ba II | N/A | ... | -0.01+-0.11 | ... | -1.99+-0.11 | -0.01+-0.11 | 0.19+-0.11 | Ba II |
Nd II | N/A | ... | 0.53+-0.1 | ... | -1.45+-0.1 | 0.53+-0.1 | -0.03+-0.1 | Nd II |
Eu II | N/A | ... | 0.48+-0.21 | ... | -1.50+-0.21 | 0.48+-0.21 | -0.98+-0.21 | Eu II |
Position
Observing Log
Date of Observation | JD | Facility | Resolution | S/N | Exposure Time | Vrad |
| N/A | SUBARUHDS | 50000 | N/A | N/A | N/A |