G53-41
taken from 12 paper(s):
/P.E.Nissen et al.(2007)/
/C.J.Akerman et al.(2004)/
/J.Melendez et al.(2006)/
/P.E.Nissen et al.(2004)/
/M.Ishigaki et al.(2010)/
/J.Melendez et al.(2010)/
/D.Fabbian et al.(2009)/
/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)/

P.E.Nissen et al.,AAP, 469, 319, 2007 (A0119,ADS)
Sulphur and zinc abundances in Galactic halo stars revisited
Stellar Parameters
Teff : 5993 | log g : 4.22 | 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 |
S I | N/A | ... | 0.27 | ... | -0.81 | 0.48 | 6.31 | S I |
Fe | N/A | -1.29 | ... | ... | -1.29 | ... | 6.21 | Fe |
Zn I | N/A | ... | 0.02 | 3.33 | -1.23 | 0.06 | 3.33 | Zn I |
Observing Log
Date of Observation | JD | Facility | Resolution | S/N | Exposure Time | Vrad |
2007-06-25 | N/A | VLT | 60000 | N/A | N/A | N/A |
Galactic Longitude (l) : N/A | Galactic Latitude (b) : N/A | Declination : N/A | Right Ascension : N/A |
C.J.Akerman et al.,AAP, 414, 931, 2004 (A0123,ADS)
The evolution of the C/O ratio in metal-poor halo stars
Stellar Parameters
Teff : 5829 | log g : 4.15 | 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 |
C I | N/A | ... | ... | 7.07 | -1.36 | -0.02 | 7.07 | C I |
O I | N/A | ... | ... | 7.86 | -0.83 | 0.51 | 7.86 | O I |
Fe | N/A | -1.34 | ... | ... | -1.34 | ... | 6.16 | Fe |
Observing Log
Date of Observation | JD | Facility | Resolution | S/N | Exposure Time | Vrad |
| N/A | VLT | 60000 | 200-300 | 3600 | N/A |
Galactic Longitude (l) : N/A | Galactic Latitude (b) : N/A | Declination : N/A | Right Ascension : N/A |
J.Melendez et al.,ApJ, 642, 1082, 2006 (A0143,ADS)
PERMITTED OXYGEN ABUNDANCES AND THE TEMPERATURE SCALE OF METAL-POOR TURNOFF STARS
Stellar Parameters
Teff : 5970+-27 | log g : 4.38+-0.15 | vturb : 1.4 |
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 |
O I | N/A | ... | ... | 7.89 | -0.80 | 0.46 | 7.89 | O I |
Fe II | N/A | ... | ... | 6.24 | -1.26 | ... | 6.24 | Fe II |
Observing Log
Date of Observation | JD | Facility | Resolution | S/N | Exposure Time | Vrad |
| N/A | VLT | 60000 | 200-300 | N/A | N/A |
Galactic Longitude (l) : N/A | Galactic Latitude (b) : N/A | Declination : N/A | Right Ascension : N/A |
P.E.Nissen et al.,AAP, 415, 993, 2004 (A0160,ADS)
Sulphur and zinc abundances in Galactic stars and damped Ly alpha systems
Stellar Parameters
Teff : 5829+-70 | log g : 4.15+-0.15 | vturb : 1.3+-0.2 |
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 |
S I | N/A | -1.05 | ... | ... | -0.97 | 0.37 | 6.15 | S I |
Fe II | N/A | -1.34 | ... | ... | -1.34 | ... | 6.16 | Fe II |
Zn I | N/A | -1.29 | ... | ... | -1.28 | 0.06 | 3.28 | Zn I |
Observing Log
Date of Observation | JD | Facility | Resolution | S/N | Exposure Time | Vrad |
2001 | N/A | VLT | 60000 | 150-300 | N/A | N/A |
Galactic Longitude (l) : N/A | Galactic Latitude (b) : N/A | Declination : N/A | Right Ascension : N/A |
M.Ishigaki et al.,PASJ, 62, 143, 2010 (A0229,ADS)
Chemical Abundances of Outer Halo Stars in the Milky Way
Stellar Parameters
Teff : 5737+-68 | log g : 4.12 | vturb : 1.10 |
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 |
Na I | N/A | -1.26+-0.04 | 0.18+-0.05 | ... | -1.17+-0.04 | 0.27+-0.05 | 5.07+-0.04 | Na I |
Mg I | N/A | -1.12+-0.05 | 0.32+-0.06 | ... | -1.14+-0.05 | 0.30+-0.06 | 6.46+-0.05 | Mg I |
Si | N/A | ... | 0.39+-0.07 | ... | -1.01+-0.07 | 0.43+-0.07 | 6.50+-0.07 | Si |
Si I | 2 | -1.15+-0.10 | ... | ... | -1.11+-0.10 | 0.33+-0.10 | 6.40+-0.10 | Si I |
Si II | 1 | -0.95+-0.10 | ... | ... | -0.91+-0.10 | 0.53+-0.10 | 6.60+-0.10 | Si II |
Ca I | N/A | -1.18+-0.03 | 0.25+-0.03 | ... | -1.16+-0.03 | 0.28+-0.03 | 5.18+-0.03 | Ca I |
Ti | N/A | ... | 0.24+-0.02 | ... | -1.13+-0.02 | 0.31+-0.02 | 3.82+-0.02 | Ti |
Ti I | 6 | -1.29+-0.03 | ... | ... | -1.22+-0.03 | 0.22+-0.03 | 3.73+-0.03 | Ti I |
Ti II | 10 | -1.05+-0.03 | ... | ... | -0.98+-0.03 | 0.46+-0.03 | 3.97+-0.03 | Ti II |
Cr | N/A | ... | -0.17+-0.03 | ... | -1.58+-0.03 | -0.14+-0.03 | 4.06+-0.03 | Cr |
Cr I | 7 | -1.62+-0.02 | ... | ... | -1.59+-0.02 | -0.15+-0.02 | 4.05+-0.02 | Cr I |
Cr II | 2 | -1.34+-0.10 | ... | ... | -1.31+-0.10 | 0.13+-0.10 | 4.33+-0.10 | Cr II |
Mn I | N/A | -1.96+-0.10 | 0.10+-0.10 | ... | -2.00+-0.10 | -0.56+-0.10 | 3.43+-0.10 | Mn I |
Fe I | 56 | -1.44+-0.02 | ... | ... | -1.44+-0.02 | ... | 6.06+-0.02 | Fe I |
Fe II | 10 | -1.44+-0.03 | ... | ... | -1.44+-0.03 | ... | 6.06+-0.03 | Fe II |
Ni I | N/A | -1.50+-0.02 | -0.06+-0.03 | ... | -1.47+-0.02 | -0.03+-0.03 | 4.75+-0.02 | Ni I |
Zn I | N/A | -1.49+-0.10 | -0.06+-0.10 | ... | -1.45+-0.10 | -0.01+-0.10 | 3.11+-0.10 | Zn I |
Y II | N/A | -1.31+-0.10 | 0.13+-0.10 | ... | -1.28+-0.10 | 0.16+-0.10 | 0.93+-0.10 | Y II |
Ba II | N/A | -1.21+-0.12 | 0.23+-0.12 | ... | -1.26+-0.12 | 0.18+-0.12 | 0.92+-0.12 | 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 : |
J.Melendez et al.,AAP, 515, L3, 2010 (A0235,ADS)
Observational evidence for a broken Li Spite plateau and mass-dependent Li depletion
Stellar Parameters
Teff : 6049+-50 | log g : 4.31 |
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 | ... | ... | 2.14+-0.035 | -1.12+-0.035 | 0.12+-0.035 | 2.14+-0.035 | Li |
Fe | N/A | -1.24 | ... | ... | -1.24 | ... | 6.26 | Fe |
Observing Log
Date of Observation | JD | Facility | Resolution | S/N | Exposure Time | Vrad |
N/A | N/A | FIESNOT | 45000 | >100 | N/A | N/A |
Galactic Longitude (l) : N/A | Galactic Latitude (b) : N/A | Declination : N/A | Right Ascension : N/A |
D.Fabbian et al.,AAP, 500, 1143, 2009 (A0266,ADS)
The C/O ratio at low metallicity:constraints on early chemical evolution from observations of Galactic halo stars
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 |
C | N/A | –1.38 | ... | 7.01 | –-1.42 | -0.08 | 7.01 | C |
O | N/A | –0.88 | ... | 7.78 | –-0.91 | 0.43 | 7.78 | O |
Fe | N/A | -1.29 | ... | ... | -1.34 | ... | 6.16 | Fe |
Observing Log
Date of Observation | JD | Facility | Resolution | S/N | Exposure Time | Vrad |
2001 | N/A | VLT | 60000 | N/A | N/A | N/A |
Galactic Longitude (l) : N/A | Galactic Latitude (b) : N/A | Declination : N/A | Right Ascension : N/A |
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 : 6070+-100 | log g : 4.56+-0.3 | vturb : 0.77+-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 | ... | 0.16+-0.13 | ... | -0.98+-0.13 | 0.16+-0.13 | 6.62+-0.13 | Mg |
Si | N/A | ... | 0.13+-0.14 | ... | -1.01+-0.14 | 0.13+-0.14 | 6.50+-0.14 | Si |
Ca | N/A | ... | 0.21+-0.07 | ... | -0.93+-0.07 | 0.21+-0.07 | 5.41+-0.07 | Ca |
Ti I | N/A | ... | 0.27+-0.07 | ... | -0.87+-0.07 | 0.27+-0.07 | 4.08+-0.07 | Ti I |
Ti II | N/A | ... | 0.32+-0.08 | ... | -0.82+-0.08 | 0.32+-0.08 | 4.13+-0.08 | Ti II |
Fe I | N/A | -1.14+-0.12 | ... | ... | -1.14+-0.12 | ... | 6.36+-0.12 | Fe I |
Fe II | N/A | -1.15+-0.11 | ... | ... | -1.15+-0.11 | ... | 6.35+-0.11 | 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 | 84.8+-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 : 6070 | log g : 4.56 | vturb : 0.77 |
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 | ... | 0.1+-0.1 | ... | -1.04+-0.1 | 0.10+-0.1 | 5.20+-0.1 | Na I |
Sc II | N/A | ... | 0.1+-0.07 | ... | -1.04+-0.07 | 0.10+-0.07 | 2.11+-0.07 | Sc II |
V I | N/A | ... | 0.02+-0.14 | ... | -1.12+-0.14 | 0.02+-0.14 | 2.81+-0.14 | V I |
Cr I | N/A | ... | -0.09+-0.07 | ... | -1.23+-0.07 | -0.09+-0.07 | 4.41+-0.07 | Cr I |
Cr II | N/A | ... | 0.17+-0.09 | ... | -0.97+-0.09 | 0.17+-0.09 | 4.67+-0.09 | Cr II |
Mn I | N/A | ... | -0.32+-0.08 | ... | -1.46+-0.08 | -0.32+-0.08 | 3.97+-0.08 | Mn I |
Fe I | N/A | -1.14+-0.12 | ... | ... | -1.14+-0.12 | ... | 6.36+-0.12 | Fe I |
Fe II | N/A | -1.15+-0.11 | ... | ... | -1.15+-0.11 | ... | 6.35+-0.11 | Fe II |
Ni I | N/A | ... | -0.14+-0.09 | ... | -1.28+-0.09 | -0.14+-0.09 | 4.94+-0.09 | Ni I |
Cu I | N/A | ... | -0.75+-0.12 | ... | -1.89+-0.12 | -0.75+-0.12 | 2.30+-0.12 | Cu I |
Zn I | N/A | ... | 0.04+-0.12 | ... | -1.10+-0.12 | 0.04+-0.12 | 3.46+-0.12 | Zn I |
Y II | N/A | ... | 0.1+-0.09 | ... | -1.04+-0.09 | 0.10+-0.09 | 1.17+-0.09 | Y II |
Ba II | N/A | ... | 0.54+-0.15 | ... | -0.60+-0.15 | 0.54+-0.15 | 1.58+-0.15 | Ba II |
La II | N/A | ... | 0.57+-0.12 | ... | -0.57+-0.12 | 0.57+-0.12 | 0.53+-0.12 | La II |
Nd II | N/A | ... | 0.61+-0.12 | ... | -0.53+-0.12 | 0.61+-0.12 | 0.89+-0.12 | Nd II |
Eu II | N/A | ... | 0.49+-0.07 | ... | -0.65+-0.07 | 0.49+-0.07 | -0.13+-0.07 | 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 : 5840+-80 | log g : 4.51+-0.24 | vturb : 1.10+-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 | -0.97+-0.08 | 0.25+-0.08 | ... | -0.88+-0.08 | 0.17+-0.08 | 5.36+-0.08 | Na I |
Mg I | 1 | -1.00+-0.08 | 0.22+-0.08 | ... | -1.02+-0.08 | 0.03+-0.08 | 6.58+-0.08 | Mg I |
Si | N/A | ... | 0.23+-0.07 | ... | -0.95+-0.07 | 0.10+-0.07 | 6.56+-0.07 | Si |
Si I | 2 | -0.99+-0.07 | ... | ... | -0.95+-0.07 | 0.10+-0.07 | 6.56+-0.07 | Si I |
Si II | 1 | -0.89+-0.04 | ... | ... | -0.85+-0.04 | 0.20+-0.04 | 6.66+-0.04 | Si II |
Ca I | 22 | -1.02+-0.06 | 0.20+-0.06 | ... | -1.00+-0.06 | 0.05+-0.06 | 5.34+-0.06 | Ca I |
Sc II | 8 | -1.04+-0.07 | 0.18+-0.07 | ... | -1.10+-0.07 | -0.05+-0.07 | 2.05+-0.07 | Sc II |
Ti | N/A | ... | 0.26+-0.08 | ... | -0.92+-0.08 | 0.13+-0.08 | 4.03+-0.08 | Ti |
Ti I | 29 | -0.96+-0.08 | ... | ... | -0.92+-0.08 | 0.13+-0.08 | 4.03+-0.08 | Ti I |
Ti II | 11 | -0.80+-0.08 | ... | ... | -0.76+-0.08 | 0.29+-0.08 | 4.19+-0.08 | Ti II |
Cr | N/A | ... | -0.13+-0.06 | ... | -1.32+-0.06 | -0.27+-0.06 | 4.32+-0.06 | Cr |
Cr I | 14 | -1.35+-0.06 | ... | ... | -1.32+-0.06 | -0.27+-0.06 | 4.32+-0.06 | Cr I |
Cr II | 5 | -1.03+-0.09 | ... | ... | -1.00+-0.09 | 0.05+-0.09 | 4.64+-0.09 | Cr II |
Mn I | 2 | -1.62+-0.03 | -0.41+-0.03 | ... | -1.66+-0.03 | -0.61+-0.03 | 3.77+-0.03 | Mn I |
Fe | N/A | -1.22+-0.05 | ... | ... | -1.05+-0.05 | ... | 6.45+-0.05 | Fe |
Fe I | 93 | -1.22+-0.05 | ... | ... | -1.05+-0.05 | ... | 6.45+-0.05 | Fe I |
Fe II | 12 | -1.22+-0.06 | ... | ... | -1.05+-0.06 | ... | 6.45+-0.06 | Fe II |
Ni I | 17 | -1.29+-0.07 | -0.07+-0.07 | ... | -1.26+-0.07 | -0.21+-0.07 | 4.96+-0.07 | Ni I |
Zn I | 3 | -1.28+-0.05 | -0.06+-0.05 | ... | -1.24+-0.05 | -0.19+-0.05 | 3.32+-0.05 | Zn I |
Y II | 2 | -1.12+-0.05 | 0.10+-0.05 | ... | -1.09+-0.05 | -0.04+-0.05 | 1.12+-0.05 | Y II |
Ba II | 3 | -0.95+-0.06 | 0.27+-0.06 | ... | -1.00+-0.06 | 0.05+-0.06 | 1.18+-0.06 | Ba II |
Binary Parameters
Observing Log
Date of Observation | JD | Facility | Resolution | S/N | Exposure Time | Vrad |
| N/A | SUBARUHDS | 50000 | N/A | 1800 | 88.2 |
Galactic Longitude (l) : N/A | Galactic Latitude (b) : N/A | Declination : +012400.1 | Right Ascension : 102724.25 |
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 : 5859 | log g : 4.27 | 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 | ... | 0.23 | ... | -0.88 | 0.32 | 5.36 | Na |
Mg | N/A | ... | 0.24 | ... | -0.98 | 0.22 | 6.62 | Mg |
Si | N/A | ... | 0.24 | ... | -0.92 | 0.28 | 6.59 | Si |
Ca | N/A | ... | 0.31 | ... | -0.87 | 0.33 | 5.47 | Ca |
Ti | N/A | ... | 0.14 | ... | -0.99 | 0.21 | 3.96 | Ti |
Cr | N/A | ... | -0.03 | ... | -1.20 | 0.00 | 4.44 | Cr |
Fe | N/A | -1.20 | ... | ... | -1.20 | ... | 6.30 | Fe |
Ni | N/A | ... | -0.09 | ... | -1.26 | -0.06 | 4.96 | Ni |
Observing Log
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 | ... | -0.38 | ... | -1.62 | -0.42 | 3.81 | Mn |
Fe | N/A | -1.2 | ... | ... | -1.20 | ... | 6.30 | Fe |
Zn | N/A | ... | 0.03 | ... | -1.13 | 0.07 | 3.43 | Zn |
Y | N/A | ... | 0.05 | ... | -1.12 | 0.08 | 1.09 | Y |
Ba | N/A | ... | 0.24 | ... | -1.01 | 0.19 | 1.17 | Ba |