G166-37
taken from 8 paper(s):
/R.Smiljanic et al.(2009)/
/A.M.Boesgaard et al.(2005)/
/A.Stephens and A. M. Boesgaard(2002)/
/M.Ishigaki et al.(2010)/
/M.N.Ishigaki et al.(2012)/
/M.N.Ishigaki et al.(2013)/
/L.Zhang et al.(2009)/
/K.A.Venn et al.(2004)/
Beryllium abundances and star formation in the halo and in the thick disk
Stellar Parameters
Teff : 5300 | log g : 4.69 | vturb : 0.6 |
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 | N/A | ... | ... | 1.28 | -1.98 | -0.78 | 1.28 | Li |
Fe | N/A | -1.2 | ... | ... | -1.20 | ... | 6.30 | Fe |
Position
Right Ascension : 14 34 51.11 | Declination : +25 10 03.6 | Galactic Longitude (l) : N/A | Galactic Latitude (b) : N/A |
Observing Log
Lithium and Lithium Depletion in Halo Stars on Extreme Orbits
Stellar Parameters
Teff : 5350+-86 | log g : 4.71+-0.36 | vturb : 0.00+-0.50 |
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 | ... | ... | 1.20+-0.07 | -2.06+-0.07 | -0.69+-0.07 | 1.20+-0.07 | Li I |
Fe | N/A | -1.39+-0.10 | ... | ... | -1.37+-0.10 | ... | 6.13+-0.10 | Fe |
Position
Right Ascension : 14 34 51.11 | Declination : +25 10 03.6 | Galactic Longitude (l) : N/A | Galactic Latitude (b) : N/A |
Observing Log
Date of Observation | JD | Facility | Resolution | S/N | Exposure Time | Vrad |
| N/A | KECKHIRES | 48000 | 110 | N/A | N/A |
ABUNDANCES FROM HIGH-RESOLUTION SPECTRA OF KINEMATICALLY INTERESTING HALO STARS
Stellar Parameters
Teff : 5350+-86 | log g : 4.71+-0.36 | vturb : 0.00+-0.50 |
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 |
Na I | N/A | -1.75+-0.10 | -0.35+-0.13 | ... | -1.66+-0.10 | -0.27+-0.13 | 4.58+-0.10 | Na I |
Mg I | N/A | -1.19+-0.05 | +0.21+-0.10 | ... | -1.21+-0.05 | 0.18+-0.10 | 6.39+-0.05 | Mg I |
Si | N/A | ... | +0.16+-0.10 | ... | -1.20+-0.10 | 0.19+-0.10 | 6.31+-0.10 | Si |
Si I | 3 | -1.24+-0.06 | ... | ... | -1.20+-0.06 | 0.19+-0.06 | 6.31+-0.06 | Si I |
Ca I | N/A | -1.20+-0.10 | +0.21+-0.13 | ... | -1.18+-0.10 | 0.21+-0.13 | 5.16+-0.10 | Ca I |
Ti | N/A | ... | +0.22+-0.11 | ... | -1.14+-0.11 | 0.25+-0.11 | 3.81+-0.11 | Ti |
Ti I | 19 | -1.21+-0.09 | ... | ... | -1.17+-0.09 | 0.22+-0.09 | 3.78+-0.09 | Ti I |
Ti II | 7 | -1.10+-0.14 | ... | ... | -1.06+-0.14 | 0.33+-0.14 | 3.89+-0.14 | Ti II |
Cr | N/A | ... | +0.04+-0.10 | ... | -1.33+-0.10 | 0.06+-0.10 | 4.31+-0.10 | Cr |
Cr I | 13 | -1.45+-0.09 | ... | ... | -1.42+-0.09 | -0.03+-0.09 | 4.22+-0.09 | Cr I |
Cr II | 3 | -1.28+-0.09 | ... | ... | -1.25+-0.09 | 0.14+-0.09 | 4.39+-0.09 | Cr II |
Fe | N/A | -1.40+-0.08 | ... | ... | -1.39+-0.08 | ... | 6.11+-0.08 | Fe |
Fe I | 67 | -1.38+-0.09 | ... | ... | -1.37+-0.09 | ... | 6.13+-0.09 | Fe I |
Fe II | 12 | -1.46+-0.16 | ... | ... | -1.45+-0.16 | ... | 6.05+-0.16 | Fe II |
Ni I | N/A | -1.56+-0.07 | -0.16+-0.11 | ... | -1.53+-0.07 | -0.14+-0.11 | 4.69+-0.07 | Ni I |
Y II | N/A | -1.28+-0.05 | +0.12+-0.09 | ... | -1.25+-0.05 | 0.14+-0.09 | 0.96+-0.05 | Y II |
Ba II | N/A | -1.26+-0.08 | +0.14+-0.11 | ... | -1.31+-0.08 | 0.08+-0.11 | 0.87+-0.08 | Ba II |
Binary Parameters
Position
Right Ascension : 14 34 51.11 | Declination : +25 10 03.6 | Galactic Longitude (l) : N/A | Galactic Latitude (b) : N/A |
Observing Log
Date of Observation | JD | Facility | Resolution | S/N | Exposure Time | Vrad |
| 2450820.657 | KECKHIRES | 48000 | 110 | 1600 | 368.4+-0.7 |
Chemical Abundances of Outer Halo Stars in the Milky Way
Stellar Parameters
Teff : 5355+-90 | log g : 4.95 | vturb : 0.05 |
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 | -1.68+-0.09 | -0.37+-0.09 | ... | -1.59+-0.09 | -0.28+-0.09 | 4.65+-0.09 | Na I |
Mg I | N/A | -0.91+-0.08 | 0.40+-0.09 | ... | -0.93+-0.08 | 0.38+-0.09 | 6.67+-0.08 | Mg I |
Si | N/A | ... | 0.20+-0.09 | ... | -1.07+-0.09 | 0.24+-0.09 | 6.44+-0.09 | Si |
Si I | 1 | -1.11+-0.08 | ... | ... | -1.07+-0.08 | 0.24+-0.08 | 6.44+-0.08 | Si I |
Ca I | N/A | -1.12+-0.03 | 0.19+-0.03 | ... | -1.10+-0.03 | 0.21+-0.03 | 5.24+-0.03 | Ca I |
Ti | N/A | ... | 0.28+-0.03 | ... | -0.96+-0.03 | 0.35+-0.03 | 3.99+-0.03 | Ti |
Ti I | 11 | -1.10+-0.03 | ... | ... | -1.03+-0.03 | 0.28+-0.03 | 3.92+-0.03 | Ti I |
Ti II | 4 | -0.89+-0.05 | ... | ... | -0.82+-0.05 | 0.49+-0.05 | 4.13+-0.05 | Ti II |
Cr | N/A | ... | -0.08+-0.03 | ... | -1.36+-0.03 | -0.05+-0.03 | 4.28+-0.03 | Cr |
Cr I | 8 | -1.41+-0.03 | ... | ... | -1.38+-0.03 | -0.07+-0.03 | 4.26+-0.03 | Cr I |
Cr II | 1 | -1.30+-0.08 | ... | ... | -1.27+-0.08 | 0.04+-0.08 | 4.37+-0.08 | Cr II |
Mn I | N/A | -1.81+-0.02 | 0.03+-0.03 | ... | -1.85+-0.02 | -0.54+-0.03 | 3.58+-0.02 | Mn I |
Fe I | 39 | -1.31+-0.02 | ... | ... | -1.31+-0.02 | ... | 6.19+-0.02 | Fe I |
Fe II | 5 | -1.31+-0.04 | ... | ... | -1.31+-0.04 | ... | 6.19+-0.04 | Fe II |
Ni I | N/A | -1.35+-0.09 | -0.04+-0.09 | ... | -1.32+-0.09 | -0.01+-0.09 | 4.90+-0.09 | Ni I |
Zn I | N/A | -1.45+-0.09 | -0.14+-0.09 | ... | -1.41+-0.09 | -0.10+-0.09 | 3.15+-0.09 | Zn I |
Y II | N/A | -1.23+-0.09 | 0.08+-0.09 | ... | -1.20+-0.09 | 0.11+-0.09 | 1.01+-0.09 | Y II |
Ba II | N/A | -1.25+-0.09 | 0.06+-0.09 | ... | -1.30+-0.09 | 0.01+-0.09 | 0.88+-0.09 | Ba II |
Position
Right Ascension : 14 34 51.11 | Declination : +25 10 03.6 | Galactic Longitude (l) : N/A | Galactic Latitude (b) : N/A |
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 |
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 : 5433+-100 | log g : 5.00+-0.3 | vturb : 0.05+-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+-0.14 | ... | -1.02+-0.14 | 0.17+-0.14 | 6.58+-0.14 | Mg |
Si | N/A | ... | 0.13+-0.20 | ... | -1.06+-0.20 | 0.13+-0.20 | 6.45+-0.20 | Si |
Ca | N/A | ... | 0.15+-0.06 | ... | -1.04+-0.06 | 0.15+-0.06 | 5.30+-0.06 | Ca |
Ti I | N/A | ... | 0.25+-0.09 | ... | -0.94+-0.09 | 0.25+-0.09 | 4.01+-0.09 | Ti I |
Ti II | N/A | ... | 0.47+-0.32 | ... | -0.72+-0.32 | 0.47+-0.32 | 4.23+-0.32 | Ti II |
Fe I | N/A | -1.19+-0.20 | ... | ... | -1.19+-0.20 | ... | 6.31+-0.20 | Fe I |
Fe II | N/A | -1.30+-0.15 | ... | ... | -1.30+-0.15 | ... | 6.20+-0.15 | Fe II |
Binary Parameters
Position
Right Ascension : 14 34 51.11 | Declination : +25 10 03.6 | Galactic Longitude (l) : N/A | Galactic Latitude (b) : N/A |
Observing Log
Date of Observation | JD | Facility | Resolution | S/N | Exposure Time | Vrad |
N/A | N/A | SUBARUHDS | 50000 | N/A | N/A | 367.3+-0.3 |
Chemical Abundances of the Milky Way Thick Disk and Stellar Halo. II. Sodium, Iron-peak, and Neutron-capture Elements
Stellar Parameters
Teff : 5433 | log g : 5 | vturb : 0.05 |
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 | ... | -0.39+-0.13 | ... | -1.57+-0.13 | -0.39+-0.13 | 4.67+-0.13 | Na I |
Sc II | N/A | ... | 0.15+-0.1 | ... | -1.03+-0.1 | 0.15+-0.1 | 2.12+-0.1 | Sc II |
V I | N/A | ... | 0.14+-0.21 | ... | -1.04+-0.21 | 0.14+-0.21 | 2.89+-0.21 | V I |
Cr I | N/A | ... | -0.08+-0.08 | ... | -1.26+-0.08 | -0.08+-0.08 | 4.38+-0.08 | Cr I |
Cr II | N/A | ... | 0.2+-0.1 | ... | -0.98+-0.1 | 0.20+-0.1 | 4.66+-0.1 | Cr II |
Mn I | N/A | ... | -0.29+-0.09 | ... | -1.47+-0.09 | -0.29+-0.09 | 3.96+-0.09 | Mn I |
Fe I | N/A | -1.18+-0.21 | ... | ... | -1.18+-0.21 | ... | 6.32+-0.21 | Fe I |
Fe II | N/A | -1.3+-0.15 | ... | ... | -1.30+-0.15 | ... | 6.20+-0.15 | Fe II |
Ni I | N/A | ... | -0.22+-0.16 | ... | -1.40+-0.16 | -0.22+-0.16 | 4.82+-0.16 | Ni I |
Cu I | N/A | ... | -0.37+-0.12 | ... | -1.55+-0.12 | -0.37+-0.12 | 2.64+-0.12 | Cu I |
Zn I | N/A | ... | -0.1+-0.21 | ... | -1.28+-0.21 | -0.10+-0.21 | 3.28+-0.21 | Zn I |
Y II | N/A | ... | 0.02+-0.12 | ... | -1.16+-0.12 | 0.02+-0.12 | 1.05+-0.12 | Y II |
Ba II | N/A | ... | 0.13+-0.15 | ... | -1.05+-0.15 | 0.13+-0.15 | 1.13+-0.15 | Ba II |
Nd II | N/A | ... | 0.46+-0.18 | ... | -0.72+-0.18 | 0.46+-0.18 | 0.70+-0.18 | Nd II |
Eu II | N/A | ... | 0.86+-0.14 | ... | -0.32+-0.14 | 0.86+-0.14 | 0.20+-0.14 | Eu II |
Position
Right Ascension : 14 34 51.11 | Declination : +25 10 03.6 | Galactic Longitude (l) : N/A | Galactic Latitude (b) : N/A |
Observing Log
Date of Observation | JD | Facility | Resolution | S/N | Exposure Time | Vrad |
| N/A | SUBARUHDS | 50000 | N/A | N/A | N/A |
Chemical Compositions of Kinematically Selected Outer Halo Stars
Stellar Parameters
Teff : 5335+-100 | log g : 4.98+-0.30 | vturb : 0.00+-0.1 |
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 | -1.58+-0.05 | -0.22+-0.05 | ... | -1.49+-0.05 | -0.30+-0.05 | 4.75+-0.05 | Na I |
Mg I | 2 | -1.11+-0.07 | 0.25+-0.07 | ... | -1.13+-0.07 | 0.06+-0.07 | 6.47+-0.07 | Mg I |
Si | N/A | ... | 0.18+-0.07 | ... | -1.14+-0.07 | 0.05+-0.07 | 6.37+-0.07 | Si |
Si I | 2 | -1.18+-0.07 | ... | ... | -1.14+-0.07 | 0.05+-0.07 | 6.37+-0.07 | Si I |
Ca I | 20 | -1.21+-0.05 | 0.15+-0.05 | ... | -1.19+-0.05 | -0.00+-0.05 | 5.15+-0.05 | Ca I |
Sc II | 8 | -1.02+-0.06 | 0.34+-0.06 | ... | -1.08+-0.06 | 0.11+-0.06 | 2.07+-0.06 | Sc II |
Ti | N/A | ... | 0.17+-0.06 | ... | -1.15+-0.06 | 0.04+-0.06 | 3.80+-0.06 | Ti |
Ti I | 26 | -1.05+-0.05 | ... | ... | -1.01+-0.05 | 0.18+-0.05 | 3.94+-0.05 | Ti I |
Ti II | 10 | -0.93+-0.08 | ... | ... | -0.89+-0.08 | 0.30+-0.08 | 4.06+-0.08 | Ti II |
Cr | N/A | ... | -0.06+-0.06 | ... | -1.39+-0.06 | -0.20+-0.06 | 4.25+-0.06 | Cr |
Cr I | 15 | -1.42+-0.06 | ... | ... | -1.39+-0.06 | -0.20+-0.06 | 4.25+-0.06 | Cr I |
Cr II | 2 | -1.21+-0.04 | ... | ... | -1.18+-0.04 | 0.01+-0.04 | 4.46+-0.04 | Cr II |
Mn I | 1 | -1.84+-0.06 | -0.48+-0.07 | ... | -1.88+-0.06 | -0.69+-0.07 | 3.55+-0.06 | Mn I |
Fe | N/A | -1.36+-0.08 | ... | ... | -1.19+-0.08 | ... | 6.31+-0.08 | Fe |
Fe I | 86 | -1.36+-0.08 | ... | ... | -1.19+-0.08 | ... | 6.31+-0.08 | Fe I |
Fe II | 12 | -1.36+-0.07 | ... | ... | -1.19+-0.07 | ... | 6.31+-0.07 | Fe II |
Ni I | 18 | -1.43+-0.03 | -0.07+-0.03 | ... | -1.40+-0.03 | -0.21+-0.03 | 4.82+-0.03 | Ni I |
Zn I | 2 | -1.62+-0.04 | -0.26+-0.05 | ... | -1.58+-0.04 | -0.39+-0.05 | 2.98+-0.04 | Zn I |
Y II | 2 | -1.27+-0.06 | 0.09+-0.06 | ... | -1.24+-0.06 | -0.05+-0.06 | 0.97+-0.06 | Y II |
Ba II | 4 | -1.19+-0.10 | 0.16+-0.10 | ... | -1.24+-0.10 | -0.05+-0.10 | 0.94+-0.10 | Ba II |
Binary Parameters
Position
Right Ascension : 14 34 51.11 | Declination : +25 10 03.6 | Galactic Longitude (l) : N/A | Galactic Latitude (b) : N/A |
Observing Log
Date of Observation | JD | Facility | Resolution | S/N | Exposure Time | Vrad |
2003-02 | N/A | SUBARUHDS | 50000 | N/A | 5400 | 369.4 |
Stellar Chemical Signatures and Hierarchical Galaxy Formation
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 | ... | -0.46 | ... | -1.77 | -0.37 | 4.47 | Na |
Mg | N/A | ... | 0.1 | ... | -1.32 | 0.08 | 6.28 | Mg |
Ca | N/A | ... | 0.12 | ... | -1.26 | 0.14 | 5.08 | Ca |
Ti | N/A | ... | 0.25 | ... | -1.08 | 0.32 | 3.87 | Ti |
Fe | N/A | -1.4 | ... | ... | -1.40 | ... | 6.10 | Fe |
Ni | N/A | ... | -0.12 | ... | -1.49 | -0.09 | 4.73 | Ni |
Y | N/A | ... | 0.1 | ... | -1.27 | 0.13 | 0.94 | Y |
Ba | N/A | ... | 0.07 | ... | -1.38 | 0.02 | 0.80 | Ba |
Position
Right Ascension : 14 34 51.11 | Declination : +25 10 03.6 | Galactic Longitude (l) : N/A | Galactic Latitude (b) : N/A |
Observing Log