G176-53
taken from 7 paper(s):
/J.Simmerer et al.(2004)/
/I.U.Roederer et al.(2010)/
/M.N.Ishigaki et al.(2012)/
/M.N.Ishigaki et al.(2013)/
/H.L.Yan et al.(2016)/
/P.E.Nissen and W. J. Schuster(2010)/
/P. E. Nissen and W. J. Schuster(2011)/
The Rise of the s-Process in the Galaxy
Stellar Parameters
Teff : 5593 | log g : 4.50 | 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 | ... | -0.05 | ... | -1.21 | 0.13 | 7.22 | C |
Fe I | 9 | -1.34 | ... | ... | -1.34 | ... | 6.16 | Fe I |
Fe II | 7 | -1.39 | ... | ... | -1.39 | ... | 6.11 | Fe II |
La II | N/A | ... | ... | -0.08+-0.04 | -1.18+-0.04 | 0.16+-0.04 | -0.08+-0.04 | La II |
Eu II | N/A | ... | ... | -0.32+-0.04 | -0.84+-0.04 | 0.50+-0.04 | -0.32+-0.04 | Eu II |
Position
Observing Log
Date of Observation | JD | Facility | Resolution | S/N | Exposure Time | Vrad |
| N/A | MCDONALD | 60000 | 100 | N/A | N/A |
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 | -1.34 | ... | ... | -1.34 | ... | 6.16 | Fe |
Zn I | N/A | ... | ... | 3.18 | -1.38 | -0.04 | 3.18 | Zn I |
Y II | N/A | ... | ... | 0.63 | -1.58 | -0.24 | 0.63 | Y II |
Pb I | N/A | ... | ... | <+1.05 | <-0.99 | <0.35 | <+1.05 | Pb I |
Position
Observing Log
Date of Observation | JD | Facility | Resolution | S/N | Exposure Time | Vrad |
| N/A | MCDONALD | 60000 | 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 : 5753+-100 | log g : 5.00+-0.3 | vturb : 0.17+-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 | ... | 0.12+-0.09 | ... | -1.11+-0.09 | 0.12+-0.09 | 6.49+-0.09 | Mg |
Si | N/A | ... | 0.14+-0.13 | ... | -1.09+-0.13 | 0.14+-0.13 | 6.42+-0.13 | Si |
Ca | N/A | ... | 0.10+-0.08 | ... | -1.13+-0.08 | 0.10+-0.08 | 5.21+-0.08 | Ca |
Ti I | N/A | ... | 0.27+-0.07 | ... | -0.96+-0.07 | 0.27+-0.07 | 3.99+-0.07 | Ti I |
Ti II | N/A | ... | 0.38+-0.08 | ... | -0.85+-0.08 | 0.38+-0.08 | 4.10+-0.08 | Ti II |
Fe I | N/A | -1.23+-0.11 | ... | ... | -1.23+-0.11 | ... | 6.27+-0.11 | Fe I |
Fe II | N/A | -1.28+-0.11 | ... | ... | -1.28+-0.11 | ... | 6.22+-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 | 63.6+-0.3 |
Chemical Abundances of the Milky Way Thick Disk and Stellar Halo. II. Sodium, Iron-peak, and Neutron-capture Elements
Stellar Parameters
Teff : 5753 | log g : 5 | vturb : 0.17 |
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 | ... | -0.3+-0.12 | ... | -1.53+-0.12 | -0.30+-0.12 | 4.71+-0.12 | Na I |
Sc II | N/A | ... | 0.17+-0.07 | ... | -1.06+-0.07 | 0.17+-0.07 | 2.09+-0.07 | Sc II |
V I | N/A | ... | 0.23+-0.13 | ... | -1.00+-0.13 | 0.23+-0.13 | 2.93+-0.13 | V I |
Cr I | N/A | ... | -0.06+-0.07 | ... | -1.29+-0.07 | -0.06+-0.07 | 4.35+-0.07 | Cr I |
Cr II | N/A | ... | 0.18+-0.09 | ... | -1.05+-0.09 | 0.18+-0.09 | 4.59+-0.09 | Cr II |
Mn I | N/A | ... | -0.31+-0.07 | ... | -1.54+-0.07 | -0.31+-0.07 | 3.89+-0.07 | Mn I |
Fe I | N/A | -1.23+-0.11 | ... | ... | -1.23+-0.11 | ... | 6.27+-0.11 | Fe I |
Fe II | N/A | -1.26+-0.14 | ... | ... | -1.26+-0.14 | ... | 6.24+-0.14 | Fe II |
Ni I | N/A | ... | -0.08+-0.09 | ... | -1.31+-0.09 | -0.08+-0.09 | 4.91+-0.09 | Ni I |
Zn I | N/A | ... | 0.04+-0.14 | ... | -1.19+-0.14 | 0.04+-0.14 | 3.37+-0.14 | Zn I |
Y II | N/A | ... | -0.05+-0.08 | ... | -1.28+-0.08 | -0.05+-0.08 | 0.93+-0.08 | Y II |
Ba II | N/A | ... | 0.12+-0.16 | ... | -1.11+-0.16 | 0.12+-0.16 | 1.07+-0.16 | Ba II |
Nd II | N/A | ... | 0.73+-0.14 | ... | -0.50+-0.14 | 0.73+-0.14 | 0.92+-0.14 | Nd II |
Eu II | N/A | ... | 0.53+-0.11 | ... | -0.70+-0.11 | 0.53+-0.11 | -0.18+-0.11 | 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 |
Non-LTE analysis of copper abundances for the two distinct halo populations in the solar neighborhood
Stellar Parameters
Teff : 5523 | log g : 4.48 | vturb : 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 |
Fe | N/A | -1.34 | ... | ... | -1.34 | ... | 6.16 | Fe |
Cu | N/A | ... | -0.66+-0.00 | ... | -1.98+-0.00 | -0.64+-0.00 | 2.21+-0.00 | Cu |
Position
Observing Log
Date of Observation | JD | Facility | Resolution | S/N | Exposure Time | Vrad |
| N/A | FIESNOT | 40000 | 140-200 | N/A | N/A |
Two distinct halo populations in the solar neighborhood. Evidence from stellar abundance ratios and kinematics
Stellar Parameters
Teff : 5523 | log g : 4.48 | vturb : 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 | N/A | ... | -0.36 | ... | -1.61 | -0.27 | 4.63 | Na |
Mg | N/A | ... | 0.15 | ... | -1.21 | 0.13 | 6.39 | Mg |
Si | N/A | ... | 0.15 | ... | -1.15 | 0.19 | 6.36 | Si |
Ca | N/A | ... | 0.25 | ... | -1.07 | 0.27 | 5.27 | Ca |
Ti | N/A | ... | 0.15 | ... | -1.12 | 0.22 | 3.83 | Ti |
Cr | N/A | ... | -0.01 | ... | -1.32 | 0.02 | 4.32 | Cr |
Fe | N/A | -1.34 | ... | ... | -1.34 | ... | 6.16 | Fe |
Ni | N/A | ... | -0.12 | ... | -1.43 | -0.09 | 4.79 | Ni |
Position
Observing Log
Date of Observation | JD | Facility | Resolution | S/N | Exposure Time | Vrad |
2008-05-17-2224 | N/A | FIESNOT | 40000 | 170 | N/A | 64.9 |
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 | ... | -0.35 | ... | -1.73 | -0.39 | 3.70 | Mn |
Fe | N/A | -1.34 | ... | ... | -1.34 | ... | 6.16 | Fe |
Cu | N/A | ... | -0.57 | ... | -1.89 | -0.55 | 2.30 | Cu |
Zn | N/A | ... | 0.08 | ... | -1.22 | 0.12 | 3.34 | Zn |
Y | N/A | ... | -0.26 | ... | -1.57 | -0.23 | 0.64 | Y |
Ba | N/A | ... | -0.26 | ... | -1.65 | -0.31 | 0.53 | Ba |
Position
Observing Log
Date of Observation | JD | Facility | Resolution | S/N | Exposure Time | Vrad |
2008-05-17-2224 | N/A | FIESNOT | 40000 | 170 | N/A | 64.9 |