HD85773
HIP48516 in K.A.Venn+,AJ, 128, 1177, 2004
taken from 9 paper(s):
/D.L.Burris et al.(2000)/
/J.Simmerer et al.(2004)/
/M.Ishigaki et al.(2010)/
/I.U.Roederer et al.(2010)/
/H.Jonsson et al.(2011)/
/M.N.Ishigaki et al.(2012)/
/M.N.Ishigaki et al.(2013)/
/L.Zhang et al.(2009)/
/M.Aoki et al.(2017)/
NEUTRON-CAPTURE ELEMENTS IN THE EARLY GALAXY: INSIGHTS FROM A LARGE SAMPLE OF METAL-POOR GIANTS
Stellar Parameters
Teff : 4450 | log g : 1.10 | vturb : 2.10 |
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 | -2.36 | ... | ... | -2.19 | ... | 5.31 | Fe |
Y | N/A | ... | -0.31 | -0.43 | -2.64 | -0.45 | -0.43 | Y |
Zr | N/A | ... | 0.07 | 0.31 | -2.27 | -0.08 | 0.31 | Zr |
Ba | N/A | ... | -0.49 | -0.72 | -2.90 | -0.71 | -0.72 | Ba |
La | N/A | ... | 0.09 | -1.05 | -2.15 | 0.04 | -1.05 | La |
Nd | N/A | ... | 0.19 | -0.67 | -2.09 | 0.10 | -0.67 | Nd |
Eu | N/A | ... | 0.24 | -1.61 | -2.13 | 0.06 | -1.61 | Eu |
Dy | N/A | ... | 0.48 | -0.78 | -1.88 | 0.31 | -0.78 | Dy |
Position
Observing Log
Date of Observation | JD | Facility | Resolution | S/N | Exposure Time | Vrad |
| N/A | MAYALLKPNO | 20000 | 100-200 | N/A | N/A |
The Rise of the s-Process in the Galaxy
Stellar Parameters
Teff : 4268 | log g : 0.87 | vturb : 2.00 |
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 | ... | -0.45 | ... | -2.89 | -0.27 | 5.54 | C |
Fe I | 13 | -2.62 | ... | ... | -2.62 | ... | 4.88 | Fe I |
Fe II | 7 | -2.39 | ... | ... | -2.39 | ... | 5.11 | Fe II |
La II | N/A | ... | ... | -1.56+-0.1 | -2.66+-0.1 | -0.04+-0.1 | -1.56+-0.1 | La II |
Eu II | N/A | ... | ... | -1.84+-0.02 | -2.36+-0.02 | 0.26+-0.02 | -1.84+-0.02 | 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 |
Chemical Abundances of Outer Halo Stars in the Milky Way
Stellar Parameters
Teff : 4146+-16 | log g : 0.01 | vturb : 2.05 |
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 | -2.93+-0.05 | -0.35+-0.06 | ... | -2.84+-0.05 | -0.25+-0.06 | 3.40+-0.05 | Na I |
Mg I | N/A | -1.79+-0.05 | 0.79+-0.05 | ... | -1.81+-0.05 | 0.78+-0.05 | 5.79+-0.05 | Mg I |
Ca I | N/A | -2.32+-0.02 | 0.26+-0.02 | ... | -2.30+-0.02 | 0.29+-0.02 | 4.04+-0.02 | Ca I |
Ti | N/A | ... | 0.18+-0.03 | ... | -2.34+-0.03 | 0.25+-0.03 | 2.61+-0.03 | Ti |
Ti I | 9 | -2.71+-0.04 | ... | ... | -2.64+-0.04 | -0.05+-0.04 | 2.31+-0.04 | Ti I |
Ti II | 6 | -2.20+-0.03 | ... | ... | -2.13+-0.03 | 0.46+-0.03 | 2.82+-0.03 | Ti II |
Cr | N/A | ... | -0.27+-0.02 | ... | -2.83+-0.02 | -0.24+-0.02 | 2.81+-0.02 | Cr |
Cr I | 8 | -2.92+-0.02 | ... | ... | -2.89+-0.02 | -0.30+-0.02 | 2.75+-0.02 | Cr I |
Cr II | 1 | -2.62+-0.05 | ... | ... | -2.59+-0.05 | 0.00+-0.05 | 3.05+-0.05 | Cr II |
Mn I | N/A | -3.01+-0.05 | 0.05+-0.05 | ... | -3.05+-0.05 | -0.46+-0.05 | 2.38+-0.05 | Mn I |
Fe I | 33 | -2.59+-0.01 | ... | ... | -2.59+-0.01 | ... | 4.91+-0.01 | Fe I |
Fe II | 4 | -2.55+-0.04 | ... | ... | -2.55+-0.04 | ... | 4.95+-0.04 | Fe II |
Ni I | N/A | -2.56+-0.09 | 0.02+-0.09 | ... | -2.53+-0.09 | 0.06+-0.09 | 3.69+-0.09 | Ni I |
Zn I | N/A | -2.13+-0.06 | 0.45+-0.07 | ... | -2.09+-0.06 | 0.50+-0.07 | 2.47+-0.06 | Zn I |
Y II | N/A | -3.27+-0.05 | -0.69+-0.06 | ... | -3.24+-0.05 | -0.65+-0.06 | -1.03+-0.05 | Y II |
Ba II | N/A | -3.33+-0.07 | -0.75+-0.07 | ... | -3.38+-0.07 | -0.79+-0.07 | -1.20+-0.07 | Ba II |
Position
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 |
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 | -2.62 | ... | ... | -2.62 | ... | 4.88 | Fe |
Zn I | N/A | ... | ... | 2.56 | -2.00 | 0.62 | 2.56 | Zn I |
Y II | N/A | ... | ... | -0.93 | -3.14 | -0.52 | -0.93 | Y II |
Pb I | N/A | ... | ... | <-0.15 | <-2.19 | <0.43 | <-0.15 | 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 |
Sulphur abundances in halo giants from the [SI] line at 1082 nm and the SI triplet around 1045 nm
Stellar Parameters
Teff : 4450+-100 | log g : 1.10+-0.5 | vturb : 2.10+-0.5 |
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 |
Si | N/A | ... | ... | 5.28 | -2.23 | 0.13 | 5.28 | Si |
S I | N/A | ... | ... | 5.25+-0.05 | -1.87+-0.05 | 0.49+-0.05 | 5.25+-0.05 | S I |
[S I] | N/A | ... | ... | 5.31 | -1.81 | 0.55 | 5.31 | [S I] |
Fe | N/A | -2.36+-0.09 | ... | ... | -2.36+-0.09 | ... | 5.14+-0.09 | Fe |
Position
Observing Log
Date of Observation | JD | Facility | Resolution | S/N | Exposure Time | Vrad |
2008-01-16 | N/A | VLTCRIRES | 80000 | 440-480 | 2160 | 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 : 4370+-100 | log g : 0.73+-0.3 | vturb : 2.01+-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 | ... | 0.36+-0.11 | ... | -2.07+-0.11 | 0.36+-0.11 | 5.53+-0.11 | Mg |
Ca | N/A | ... | 0.18+-0.09 | ... | -2.25+-0.09 | 0.18+-0.09 | 4.09+-0.09 | Ca |
Ti I | N/A | ... | 0.12+-0.10 | ... | -2.31+-0.10 | 0.12+-0.10 | 2.64+-0.10 | Ti I |
Ti II | N/A | ... | 0.30+-0.09 | ... | -2.13+-0.09 | 0.30+-0.09 | 2.82+-0.09 | Ti II |
Fe I | N/A | -2.43+-0.19 | ... | ... | -2.43+-0.19 | ... | 5.07+-0.19 | Fe I |
Fe II | N/A | -2.41+-0.12 | ... | ... | -2.41+-0.12 | ... | 5.09+-0.12 | 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 | 141.6+-0.3 |
Chemical Abundances of the Milky Way Thick Disk and Stellar Halo. II. Sodium, Iron-peak, and Neutron-capture Elements
Stellar Parameters
Teff : 4370 | log g : 0.73 | vturb : 2.01 |
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 |
V I | N/A | ... | -0.19+-0.14 | ... | -2.60+-0.14 | -0.19+-0.14 | 1.33+-0.14 | V I |
Cr I | N/A | ... | -0.2+-0.07 | ... | -2.61+-0.07 | -0.20+-0.07 | 3.03+-0.07 | Cr I |
Cr II | N/A | ... | 0.21+-0.12 | ... | -2.20+-0.12 | 0.21+-0.12 | 3.44+-0.12 | Cr II |
Mn I | N/A | ... | -0.17+-0.12 | ... | -2.58+-0.12 | -0.17+-0.12 | 2.85+-0.12 | Mn I |
Fe I | N/A | -2.41+-0.19 | ... | ... | -2.41+-0.19 | ... | 5.09+-0.19 | Fe I |
Fe II | N/A | -2.44+-0.12 | ... | ... | -2.44+-0.12 | ... | 5.06+-0.12 | Fe II |
Ni I | N/A | ... | -0.02+-0.1 | ... | -2.43+-0.1 | -0.02+-0.1 | 3.79+-0.1 | Ni I |
Cu I | N/A | ... | -0.75+-0.12 | ... | -3.16+-0.12 | -0.75+-0.12 | 1.03+-0.12 | Cu I |
Zn I | N/A | ... | 0.51+-0.2 | ... | -1.90+-0.2 | 0.51+-0.2 | 2.66+-0.2 | Zn I |
Y II | N/A | ... | -0.57+-0.1 | ... | -2.98+-0.1 | -0.57+-0.1 | -0.77+-0.1 | Y II |
Zr II | N/A | ... | -0.22+-0.12 | ... | -2.63+-0.12 | -0.22+-0.12 | -0.05+-0.12 | Zr II |
Ba II | N/A | ... | -0.52+-0.2 | ... | -2.93+-0.2 | -0.52+-0.2 | -0.75+-0.2 | Ba II |
Nd II | N/A | ... | -0.24+-0.12 | ... | -2.65+-0.12 | -0.24+-0.12 | -1.23+-0.12 | Nd II |
Sm II | N/A | ... | -0.18+-0.22 | ... | -2.59+-0.22 | -0.18+-0.22 | -1.63+-0.22 | Sm II |
Eu II | N/A | ... | -0.03+-0.08 | ... | -2.44+-0.08 | -0.03+-0.08 | -1.92+-0.08 | 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 |
Chemical Compositions of Kinematically Selected Outer Halo Stars
Stellar Parameters
Teff : 4205+-50 | log g : 0.32+-0.20 | vturb : 1.60+-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 | -3.29+-0.08 | -0.71+-0.08 | ... | -3.20+-0.08 | -0.79+-0.08 | 3.04+-0.08 | Na I |
Mg I | 3 | -2.29+-0.09 | 0.29+-0.09 | ... | -2.31+-0.09 | 0.10+-0.09 | 5.29+-0.09 | Mg I |
Ca I | 17 | -2.34+-0.07 | 0.24+-0.07 | ... | -2.32+-0.07 | 0.09+-0.07 | 4.02+-0.07 | Ca I |
Sc II | 4 | -2.60+-0.06 | -0.02+-0.06 | ... | -2.66+-0.06 | -0.25+-0.06 | 0.49+-0.06 | Sc II |
Ti | N/A | ... | 0.28+-0.07 | ... | -2.26+-0.07 | 0.15+-0.07 | 2.69+-0.07 | Ti |
Ti I | 21 | -2.30+-0.07 | ... | ... | -2.26+-0.07 | 0.15+-0.07 | 2.69+-0.07 | Ti I |
Ti II | 7 | -2.25+-0.08 | ... | ... | -2.21+-0.08 | 0.20+-0.08 | 2.74+-0.08 | Ti II |
Cr | N/A | ... | -0.27+-0.07 | ... | -2.82+-0.07 | -0.41+-0.07 | 2.82+-0.07 | Cr |
Cr I | 12 | -2.85+-0.07 | ... | ... | -2.82+-0.07 | -0.41+-0.07 | 2.82+-0.07 | Cr I |
Cr II | 4 | -2.40+-0.10 | ... | ... | -2.37+-0.10 | 0.04+-0.10 | 3.27+-0.10 | Cr II |
Mn I | 2 | -3.02+-0.06 | -0.44+-0.06 | ... | -3.06+-0.06 | -0.65+-0.06 | 2.37+-0.06 | Mn I |
Fe | N/A | -2.58+-0.05 | ... | ... | -2.41+-0.05 | ... | 5.09+-0.05 | Fe |
Fe I | 60 | -2.58+-0.05 | ... | ... | -2.41+-0.05 | ... | 5.09+-0.05 | Fe I |
Fe II | 9 | -2.58+-0.05 | ... | ... | -2.41+-0.05 | ... | 5.09+-0.05 | Fe II |
Ni I | 15 | -2.58+-0.08 | 0.00+-0.08 | ... | -2.55+-0.08 | -0.14+-0.08 | 3.67+-0.08 | Ni I |
Zn I | 3 | -2.14+-0.05 | 0.44+-0.05 | ... | -2.10+-0.05 | 0.31+-0.05 | 2.46+-0.05 | Zn I |
Y II | 1 | -3.15+-0.05 | -0.57+-0.05 | ... | -3.12+-0.05 | -0.71+-0.05 | -0.91+-0.05 | Y II |
Ba II | 4 | -3.27+-0.06 | -0.69+-0.06 | ... | -3.32+-0.06 | -0.91+-0.06 | -1.14+-0.06 | Ba II |
Binary Parameters
Position
Observing Log
Date of Observation | JD | Facility | Resolution | S/N | Exposure Time | Vrad |
2003-02 | N/A | SUBARUHDS | 50000 | N/A | 1200 | 148.2 |
Diversity of Abundance Patterns of Light Neutron-capture Elements in Very-metal-poor Stars
Stellar Parameters
Teff : 4268 | log g : 0.87 | vturb : 1.98 |
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 | -2.62 | ... | ... | -2.62 | ... | 4.88 | Fe |
Sr II | 2 | ... | -0.25+-0.20 | 0.00+-0.20 | -2.87+-0.20 | -0.25+-0.20 | 0.00+-0.20 | Sr II |
Y II | 3 | ... | -0.55+-0.28 | -0.96+-0.28 | -3.17+-0.28 | -0.55+-0.28 | -0.96+-0.28 | Y II |
Zr II | 4 | ... | -0.19+-0.19 | -0.23+-0.19 | -2.81+-0.19 | -0.19+-0.19 | -0.23+-0.19 | Zr II |
Mo I | 1 | ... | -0.23+-0.26 | -0.97+-0.26 | -2.85+-0.26 | -0.23+-0.26 | -0.97+-0.26 | Mo I |
Ru I | 2 | ... | -0.14+-0.28 | -1.01+-0.28 | -2.76+-0.28 | -0.14+-0.28 | -1.01+-0.28 | Ru I |
Pd I | 1 | ... | -0.25+-0.22 | -1.30+-0.22 | -2.87+-0.22 | -0.25+-0.22 | -1.30+-0.22 | Pd I |
Ba II | 4 | ... | -0.33+-0.18 | -0.77+-0.18 | -2.95+-0.18 | -0.33+-0.18 | -0.77+-0.18 | Ba II |
La II | 3 | ... | -0.23+-0.18 | -1.75+-0.18 | -2.85+-0.18 | -0.23+-0.18 | -1.75+-0.18 | La II |
Ce II | 4 | ... | -0.36+-0.19 | -1.40+-0.19 | -2.98+-0.19 | -0.36+-0.19 | -1.40+-0.19 | Ce II |
Nd II | 5 | ... | -0.07+-0.19 | -1.27+-0.19 | -2.69+-0.19 | -0.07+-0.19 | -1.27+-0.19 | Nd II |
Eu II | 3 | ... | 0.02+-0.20 | -2.08+-0.20 | -2.60+-0.20 | 0.02+-0.20 | -2.08+-0.20 | Eu II |
Binary Parameters
Position
Observing Log
Date of Observation | JD | Facility | Resolution | S/N | Exposure Time | Vrad |
2007-02-08 | N/A | SUBARUHDS | 90000 | 220 | 10800 | 147.7+-0.8 |