BD+51_1696
G176-53 in J.Simmerer+,ApJ, 617, 1091, 2004
taken from 9 paper(s):
/G.S.Bai et al.(2004)/
/J.Simmerer et al.(2004)/
/J.Melendez et al.(2010)/
/I.U.Roederer et al.(2010)/
/M.N.Ishigaki et al.(2012)/
/M.N.Ishigaki et al.(2013)/
/B.E.Reddy et al.(2006)/
/P.E.Nissen and W. J. Schuster(2010)/
/P. E. Nissen and W. J. Schuster(2011)/

G.S.Bai et al.,AAP, 425, 671, 2004 (A0023,ADS)
Chemical abundances of 10 metal-poor halo stars
Stellar Parameters
Teff : 5537 | log g : 4.55+-0.3 | vturb : 1.60 |
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 | ... | 0.53 | ... | -0.81 | 0.67 | 7.88 | O I |
Na I | N/A | ... | -0.61 | ... | -2.00 | -0.52 | 4.24 | Na I |
Mg I | N/A | ... | 0.18 | ... | -1.32 | 0.16 | 6.28 | Mg I |
Si I | N/A | ... | 0.35 | ... | -1.09 | 0.39 | 6.42 | Si I |
Ca I | N/A | ... | 0.29 | ... | -1.17 | 0.31 | 5.17 | Ca I |
Sc II | N/A | ... | 0.15 | ... | -1.31 | 0.17 | 1.84 | Sc II |
Ti | N/A | ... | 0.30 | ... | -1.11 | 0.37 | 3.84 | Ti |
Cr | N/A | ... | 0.04 | ... | -1.41 | 0.07 | 4.23 | Cr |
Mn I | N/A | ... | -0.20 | ... | -1.72 | -0.24 | 3.71 | Mn I |
Fe I | N/A | -1.48 | ... | ... | -1.48 | ... | 6.02 | Fe I |
Ba II | N/A | ... | 0.08 | ... | -1.45 | 0.03 | 0.73 | Ba II |
Observing Log
Date of Observation | JD | Facility | Resolution | S/N | Exposure Time | Vrad |
2001-04-21 | N/A | PFESSAO | 15000 | 170 | N/A | N/A |
Galactic Longitude (l) : N/A | Galactic Latitude (b) : N/A | Declination : N/A | Right Ascension : N/A |
J.Simmerer et al.,ApJ, 617, 1091, 2004 (A0131,ADS)
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 | ... | ... | ... | C |
Fe I | 9 | -1.34 | ... | ... | ... | ... | Fe I |
Fe II | 7 | -1.39 | ... | ... | ... | ... | Fe II |
La II | N/A | ... | ... | -0.08+-0.04 | ... | ... | La II |
Eu II | N/A | ... | ... | -0.32+-0.04 | ... | ... | Eu II |
Observing Log
Date of Observation | JD | Facility | Resolution | S/N | Exposure Time | Vrad |
| N/A | MCDONALD | 60000 | 100 | N/A | N/A |
Galactic Longitude (l) : N/A | Galactic Latitude (b) : N/A | Declination : N/A | Right Ascension : N/A |
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 : 5722+-50 | log g : 4.59 |
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 | ... | ... | 1.80+-0.035 | -1.46+-0.035 | -0.06+-0.035 | 1.80+-0.035 | Li |
Fe | N/A | -1.40 | ... | ... | -1.40 | ... | 6.10 | 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 |
I.U.Roederer et al.,ApJ, 724, 975, 2010 (A0243,ADS)
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 | ... | ... | ... | ... | Fe |
Zn I | N/A | ... | ... | 3.18 | ... | ... | Zn I |
Y II | N/A | ... | ... | 0.63 | ... | ... | Y II |
Pb I | N/A | ... | ... | <+1.05 | ... | ... | Pb I |
Observing Log
Date of Observation | JD | Facility | Resolution | S/N | Exposure Time | Vrad |
| N/A | MCDONALD | 60000 | 100 | 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 : 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 | ... | ... | ... | Mg |
Si | N/A | ... | 0.14+-0.13 | ... | ... | ... | Si |
Ca | N/A | ... | 0.10+-0.08 | ... | ... | ... | Ca |
Ti I | N/A | ... | 0.27+-0.07 | ... | ... | ... | Ti I |
Ti II | N/A | ... | 0.38+-0.08 | ... | ... | ... | Ti II |
Fe I | N/A | -1.23+-0.11 | ... | ... | ... | ... | Fe I |
Fe II | N/A | -1.28+-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 | 63.6+-0.3 |
Galactic Longitude (l) : N/A | Galactic Latitude (b) : N/A | Declination : +505236.52 | Right Ascension : 114634.100 |
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 : 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 | ... | ... | ... | Na I |
Sc II | N/A | ... | 0.17+-0.07 | ... | ... | ... | Sc II |
V I | N/A | ... | 0.23+-0.13 | ... | ... | ... | V I |
Cr I | N/A | ... | -0.06+-0.07 | ... | ... | ... | Cr I |
Cr II | N/A | ... | 0.18+-0.09 | ... | ... | ... | Cr II |
Mn I | N/A | ... | -0.31+-0.07 | ... | ... | ... | Mn I |
Fe I | N/A | -1.23+-0.11 | ... | ... | ... | ... | Fe I |
Fe II | N/A | -1.26+-0.14 | ... | ... | ... | ... | Fe II |
Ni I | N/A | ... | -0.08+-0.09 | ... | ... | ... | Ni I |
Zn I | N/A | ... | 0.04+-0.14 | ... | ... | ... | Zn I |
Y II | N/A | ... | -0.05+-0.08 | ... | ... | ... | Y II |
Ba II | N/A | ... | 0.12+-0.16 | ... | ... | ... | Ba II |
Nd II | N/A | ... | 0.73+-0.14 | ... | ... | ... | Nd II |
Eu II | N/A | ... | 0.53+-0.11 | ... | ... | ... | 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 |
B.E.Reddy et al.,MNRAS, 367, 1329, 2006 (C0002,ADS)
Elemental abundance survey of the Galactic thick disc
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 |
O | N/A | ... | 0.99 | ... | -0.47 | 1.08 | 8.22 | O |
Na | N/A | ... | 0.18 | ... | -1.29 | 0.26 | 4.95 | Na |
Mg | N/A | ... | 0.36 | ... | -1.20 | 0.35 | 6.40 | Mg |
Si | N/A | ... | 0.34 | ... | -1.05 | 0.50 | 6.46 | Si |
Ca | N/A | ... | 0.2 | ... | -1.31 | 0.24 | 5.03 | Ca |
Sc | N/A | ... | 0.23 | ... | -1.18 | 0.37 | 1.97 | Sc |
Ti | N/A | ... | 0.1 | ... | -1.45 | 0.10 | 3.50 | Ti |
V | N/A | ... | 0.26 | ... | -1.17 | 0.38 | 2.76 | V |
Cr | N/A | ... | -0.09 | ... | -1.55 | -0.00 | 4.09 | Cr |
Mn | N/A | ... | -0.4 | ... | -1.96 | -0.41 | 3.47 | Mn |
Fe I | N/A | -1.5 | ... | ... | -1.55 | ... | 5.95 | Fe I |
Ni | N/A | ... | -0.11 | ... | -1.60 | -0.05 | 4.62 | Ni |
Cu | N/A | ... | -0.36 | ... | -1.86 | -0.31 | 2.33 | Cu |
Zn | N/A | ... | 0.08 | ... | -1.51 | 0.04 | 3.05 | Zn |
Y | N/A | ... | -0.04 | ... | -1.63 | -0.08 | 0.58 | Y |
Ba | N/A | ... | -0.05 | ... | -1.53 | 0.02 | 0.65 | Ba |
Binary Parameters
Observing Log
Date of Observation | JD | Facility | Resolution | S/N | Exposure Time | Vrad |
2004-06 | N/A | MCDONALD | 60000 | 100-200 | N/A | 64 |
Galactic Longitude (l) : N/A | Galactic Latitude (b) : N/A | Declination : N/A | Right Ascension : N/A |
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 : 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 | ... | ... | ... | Na |
Mg | N/A | ... | 0.15 | ... | ... | ... | Mg |
Si | N/A | ... | 0.15 | ... | ... | ... | Si |
Ca | N/A | ... | 0.25 | ... | ... | ... | Ca |
Ti | N/A | ... | 0.15 | ... | ... | ... | Ti |
Cr | N/A | ... | -0.01 | ... | ... | ... | Cr |
Fe | N/A | -1.34 | ... | ... | ... | ... | Fe |
Ni | N/A | ... | -0.12 | ... | ... | ... | 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 | ... | -0.35 | ... | ... | ... | Mn |
Fe | N/A | -1.34 | ... | ... | ... | ... | Fe |
Cu | N/A | ... | -0.57 | ... | ... | ... | Cu |
Zn | N/A | ... | 0.08 | ... | ... | ... | Zn |
Y | N/A | ... | -0.26 | ... | ... | ... | Y |
Ba | N/A | ... | -0.26 | ... | ... | ... | Ba |