HD122563
HIP68594 in K.A.Venn+,AJ, 128, 1177, 2004
taken from 46 paper(s):
/D.L.Burris et al.(2000)/
/R.Cayrel et al.(2004)/
/S.Honda et al.(2004)/
/M.Spite et al.(2005)/
/J.A.Johnson(2002)/
/J.Westin et al.(2000)/
/J.E.Norris et al.(1997)/
/W.Aoki et al.(2005)/
/T.V.Mishenina et al.(2002)/
/T.V.Mishenina and V. V. Kovtyukh(2001)/
/B.Barbuy et al.(2003)/
/J.P.Fulbright and J. A. Johnson(2003)/
/J.J.Cowan et al.(2005)/
/S.Honda et al.(2004)/
/M.Spite et al.(2006)/
/S.M.Andrievsky et al.(2007)/
/J.A.Johnson et al.(2007)/
/W.Aoki et al.(2007)/
/S.Honda et al.(2006)/
/J.P.Fulbright(2000)/
/S.Honda et al.(2007)/
/D.K.Lai et al.(2007)/
/J.Simmerer et al.(2004)/
/C.Sneden et al.(1998)/
/M.Bergemann and T. Gehren(2008)/
/S.M.Andrievsky et al.(2008)/
/I.U.Roederer et al.(2008)/
/L.Mashonkina et al.(2008)/
/J.A.Johnson and M. Bolte(2002)/
/J.A.Johnson and M. Bolte(2001)/
/I.U.Roederer et al.(2009)/
/S.M.Andrievsky et al.(2009)/
/S.M.Andrievsky et al.(2010)/
/M.Bergemann et al.(2010)/
/I.U.Roederer et al.(2010)/
/Y.Takeda and M. Takada-Hidai(2011)/
/M.Spite et al.(2011)/
/J.K.Hollek et al.(2011)/
/C.J.Hansen et al.(2012)/
/I.U.Roederer et al.(2012)/
/M.Spite et al.(2012)/
/I.U.Roederer et al.(2014)/
/D.Prakapavicius et al.(2017)/
/C.M.Sakari et al.(2018)/
/K.A.Venn et al.(2019)/
/C.L.Kielty et al.(2021)/
NEUTRON-CAPTURE ELEMENTS IN THE EARLY GALAXY: INSIGHTS FROM A LARGE SAMPLE OF METAL-POOR GIANTS
Stellar Parameters
Teff : 4625 | log g : 1.40 | vturb : 1.70 |
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 | -2.71 | ... | ... | -2.54 | ... | 4.96 | Fe |
Sr | N/A | ... | 0.06 | 0.25 | -2.62 | -0.08 | 0.25 | Sr |
Y | N/A | ... | -0.13 | -0.60 | -2.81 | -0.27 | -0.60 | Y |
Zr | N/A | ... | 0.31 | 0.20 | -2.38 | 0.16 | 0.20 | Zr |
Ba | N/A | ... | -0.92 | -1.50 | -3.68 | -1.14 | -1.50 | Ba |
La | N/A | ... | -0.71 | -2.20 | -3.30 | -0.76 | -2.20 | La |
Nd | N/A | ... | -0.59 | -1.80 | -3.22 | -0.68 | -1.80 | Nd |
Eu | N/A | ... | -0.30 | -2.50 | -3.02 | -0.48 | -2.50 | Eu |
Dy | N/A | ... | -0.39 | -2.00 | -3.10 | -0.56 | -2.00 | Dy |
Position
Right Ascension : 14 02 31.80 | Declination : +09 41 10.0 | 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 | MAYALLKPNO | 20000 | 100-200 | N/A | N/A |
First stars V - Abundance patterns from C to Zn and supernova yields in the early Galaxy
Stellar Parameters
Teff : 4600 | log g : 1.1 | vturb : 2.0 |
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 |
CH | N/A | -3.22 | -0.41 | 5.30 | -3.13 | -0.35 | 5.30 | CH |
[O I] | N/A | -2.20 | 0.62 | 6.57 | -2.12 | 0.66 | 6.57 | [O I] |
Na I | 2 | -2.58 | 0.23 | 3.75 | -2.49 | 0.29 | 3.75 | Na I |
Mg I | 8 | -2.45+-0.12 | 0.36+-0.12 | 5.13+-0.12 | -2.47+-0.12 | 0.31+-0.12 | 5.13+-0.12 | Mg I |
Al I | 2 | -3.19 | -0.38 | 3.28 | -3.17 | -0.39 | 3.28 | Al I |
Si I | 1 | -2.35 | 0.47 | 5.20 | -2.31 | 0.47 | 5.20 | Si I |
K I | 1 | -2.30 | 0.51 | 2.82 | -2.21 | 0.57 | 2.82 | K I |
Ca I | 16 | -2.50+-0.10 | 0.31+-0.10 | 3.86+-0.10 | -2.48+-0.10 | 0.30+-0.10 | 3.86+-0.10 | Ca I |
Sc II | 7 | -2.71+-0.10 | 0.11+-0.10 | 0.46+-0.10 | -2.69+-0.10 | 0.09+-0.10 | 0.46+-0.10 | Sc II |
Ti I | 14 | -2.70+-0.10 | 0.12+-0.10 | 2.32+-0.10 | -2.63+-0.10 | 0.15+-0.10 | 2.32+-0.10 | Ti I |
Ti II | 28 | -2.64+-0.10 | 0.18+-0.10 | 2.38+-0.10 | -2.57+-0.10 | 0.21+-0.10 | 2.38+-0.10 | Ti II |
Cr I | 7 | -3.21+-0.17 | -0.40+-0.17 | 2.46+-0.17 | -3.18+-0.17 | -0.40+-0.17 | 2.46+-0.17 | Cr I |
Mn I | 3 | -3.22+-0.06 | -0.41+-0.06 | 2.17+-0.06 | -3.26+-0.06 | -0.48+-0.06 | 2.17+-0.06 | Mn I |
Fe I | 142 | -2.78+-0.17 | 0.03+-0.17 | 4.72+-0.17 | -2.78+-0.17 | 0.03+-0.17 | 4.72+-0.17 | Fe I |
Fe II | 18 | -2.85+-0.13 | -0.04+-0.13 | 4.65+-0.13 | -2.85+-0.13 | -0.04+-0.13 | 4.65+-0.13 | Fe II |
Co I | 4 | -2.53+-0.13 | 0.29+-0.13 | 2.39+-0.13 | -2.60+-0.13 | 0.18+-0.13 | 2.39+-0.13 | Co I |
Ni I | 3 | -2.78+-0.09 | 0.03+-0.09 | 3.47+-0.09 | -2.75+-0.09 | 0.03+-0.09 | 3.47+-0.09 | Ni I |
Zn I | 2 | -2.66 | 0.16 | 1.94 | -2.62 | 0.16 | 1.94 | Zn I |
Binary Parameters
Position
Right Ascension : 14 02 31.80 | Declination : +09 41 10.0 | Galactic Longitude (l) : N/A | Galactic Latitude (b) : N/A |
Observing Log
Date of Observation | JD | Facility | Resolution | S/N | Exposure Time | Vrad |
2000-07 | N/A | VLT | 47000 | 250 | N/A | N/A |
Spectroscopic Studies of Extremely Metal-Poor Stars with the Subaru High Dispersion Spectrograph. II. The r-Process Elements, Including Thorium
Stellar Parameters
Teff : 4570 | log g : 1.1 | vturb : 2.2 |
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 |
CH | N/A | ... | -0.41 | 5.38 | -3.05 | -0.29 | 5.38 | CH |
Mg I | 6 | ... | 0.54+-0.06 | 5.35+-0.06 | -2.25+-0.06 | 0.51+-0.06 | 5.35+-0.06 | Mg I |
Al I | 1 | ... | -0.4+-0.12 | 3.3+-0.12 | -3.15+-0.12 | -0.39+-0.12 | 3.3+-0.12 | Al I |
Si I | 1 | ... | 0.44+-0.12 | 5.22+-0.12 | -2.29+-0.12 | 0.47+-0.12 | 5.22+-0.12 | Si I |
Ca I | 4 | ... | 0.3+-0.1 | 3.89+-0.1 | -2.45+-0.1 | 0.31+-0.1 | 3.89+-0.1 | Ca I |
Sc II | 3 | ... | ... | 0.4+-0.07 | -2.75+-0.07 | 0.01+-0.07 | 0.4+-0.07 | Sc II |
Ti | 27 | ... | 0.2+-0.12 | 2.45+-0.12 | -2.50+-0.12 | 0.26+-0.12 | 2.45+-0.12 | Ti |
V | 4 | ... | 0.05+-0.13 | 1.28+-0.13 | -2.65+-0.13 | 0.11+-0.13 | 1.28+-0.13 | V |
Cr | 3 | ... | 0.15+-0.15 | 3.05+-0.15 | -2.59+-0.15 | 0.17+-0.15 | 3.05+-0.15 | Cr |
Mn I | 6 | ... | -0.16+-0.09 | 2.46+-0.09 | -2.97+-0.09 | -0.21+-0.09 | 2.46+-0.09 | Mn I |
Fe | 84 | -2.77+-0.19 | ... | 4.74+-0.19 | -2.76+-0.19 | ... | 4.74+-0.19 | Fe |
Co I | 3 | ... | 0.18+-0.16 | 2.33+-0.16 | -2.66+-0.16 | 0.10+-0.16 | 2.33+-0.16 | Co I |
Ni I | 2 | ... | -0.15+-0.12 | 3.33+-0.12 | -2.89+-0.12 | -0.13+-0.12 | 3.33+-0.12 | Ni I |
Cu I | 1 | ... | -0.78+-0.12 | 0.66+-0.12 | -3.53+-0.12 | -0.77+-0.12 | 0.66+-0.12 | Cu I |
Sr II | 1 | ... | -0.11+-0.12 | 0.04+-0.12 | -2.83+-0.12 | -0.07+-0.12 | 0.04+-0.12 | Sr II |
Y II | 6 | ... | -0.33+-0.12 | -0.87+-0.12 | -3.08+-0.12 | -0.32+-0.12 | -0.87+-0.12 | Y II |
Zr II | 3 | ... | -0.03+-0.11 | -0.19+-0.11 | -2.77+-0.11 | -0.01+-0.11 | -0.19+-0.11 | Zr II |
Ba II | 2 | ... | -1.21+-0.12 | -1.76+-0.12 | -3.94+-0.12 | -1.18+-0.12 | -1.76+-0.12 | Ba II |
La II | 5 | ... | -0.89+-0.12 | -2.44+-0.12 | -3.54+-0.12 | -0.78+-0.12 | -2.44+-0.12 | La II |
Nd II | 1 | ... | -0.67+-0.12 | -1.95+-0.12 | -3.37+-0.12 | -0.61+-0.12 | -1.95+-0.12 | Nd II |
Eu II | 1 | ... | -0.38+-0.12 | -2.6+-0.12 | -3.12+-0.12 | -0.36+-0.12 | -2.6+-0.12 | Eu II |
Gd II | 1 | ... | -0.63+-0.12 | -2.31+-0.12 | -3.38+-0.12 | -0.62+-0.12 | -2.31+-0.12 | Gd II |
Isotopic Ratio
Position
Right Ascension : 14 02 31.80 | Declination : +09 41 10.0 | Galactic Longitude (l) : N/A | Galactic Latitude (b) : N/A |
Observing Log
Date of Observation | JD | Facility | Resolution | S/N | Exposure Time | Vrad |
2000-07-04 | N/A | SUBARUHDS | 90000 | 374 | 1200 | -27.20+-0.33 |
2001-01-29 | N/A | SUBARUHDS | 90000 | N/A | N/A | -26.52+-0.34 |
First stars VI - Abundances of C, N, O, Li, and mixing in extremely metal-poor giants. Galactic evolution of the light elements
Stellar Parameters
Teff : 4600 | log g : 1.1 | vturb : 2.0 |
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 | ... | ... | <-0.60 | <-3.86 | <-1.04 | <-0.60 | Li I |
C | N/A | -3.29+-0.05 | ... | ... | -3.20+-0.05 | -0.38+-0.05 | 5.23+-0.05 | C |
N | N/A | -2.12 | ... | ... | -2.03 | 0.79 | 5.80 | N |
[O I] | N/A | -2.20 | ... | ... | -2.15 | 0.67 | 6.54 | [O I] |
Fe | N/A | -2.82 | ... | ... | -2.82 | ... | 4.68 | Fe |
Position
Right Ascension : 14 02 31.80 | Declination : +09 41 10.0 | 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 | VLT | 47000 | 30 | N/A | N/A |
ABUNDANCES OF 30 ELEMENTS IN 23 METAL-POOR STARS
Stellar Parameters
Teff : 4450 | log g : 0.50 | vturb : 2.30 |
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 | ... | ... | 3.70+-0.22 | -2.54+-0.22 | 0.19+-0.22 | 3.70+-0.22 | Na I |
Mg I | 5 | ... | ... | 5.52+-0.12 | -2.08+-0.12 | 0.65+-0.12 | 5.52+-0.12 | Mg I |
Al I | 1 | ... | ... | 3.61+-0.10 | -2.84+-0.10 | -0.11+-0.10 | 3.61+-0.10 | Al I |
Si I | 1 | ... | ... | 5.50+-0.20 | -2.01+-0.20 | 0.72+-0.20 | 5.50+-0.20 | Si I |
Ca I | 20 | ... | ... | 3.90+-0.07 | -2.44+-0.07 | 0.29+-0.07 | 3.90+-0.07 | Ca I |
Sc II | 10 | ... | ... | 0.43+-0.10 | -2.72+-0.10 | 0.01+-0.10 | 0.43+-0.10 | Sc II |
Ti I | 35 | ... | ... | 2.38+-0.13 | -2.57+-0.13 | 0.16+-0.13 | 2.38+-0.13 | Ti I |
Ti II | 19 | ... | ... | 2.40+-0.08 | -2.55+-0.08 | 0.18+-0.08 | 2.40+-0.08 | Ti II |
V I | 4 | ... | ... | 1.19+-0.02 | -2.74+-0.02 | -0.01+-0.02 | 1.19+-0.02 | V I |
V II | 2 | ... | ... | 1.45+-0.05 | -2.48+-0.05 | 0.25+-0.05 | 1.45+-0.05 | V II |
Cr I | 14 | ... | ... | 2.66+-0.06 | -2.98+-0.06 | -0.25+-0.06 | 2.66+-0.06 | Cr I |
Cr II | 2 | ... | ... | 3.05+-0.06 | -2.59+-0.06 | 0.14+-0.06 | 3.05+-0.06 | Cr II |
Mn I | 5 | ... | ... | 2.43+-0.08 | -3.00+-0.08 | -0.27+-0.08 | 2.43+-0.08 | Mn I |
Mn II | 1 | ... | ... | 2.95+-0.15 | -2.48+-0.15 | 0.25+-0.15 | 2.95+-0.15 | Mn II |
Fe I | 161 | ... | ... | 4.77+-0.16 | -2.73+-0.16 | ... | 4.77+-0.16 | Fe I |
Fe II | 21 | ... | ... | 4.75+-0.11 | -2.75+-0.11 | ... | 4.75+-0.11 | Fe II |
Co I | 7 | ... | ... | 2.52+-0.11 | -2.47+-0.11 | 0.26+-0.11 | 2.52+-0.11 | Co I |
Ni I | 21 | ... | ... | 3.60+-0.14 | -2.62+-0.14 | 0.11+-0.14 | 3.60+-0.14 | Ni I |
Zn I | 2 | ... | ... | 2.00+-0.04 | -2.56+-0.04 | 0.17+-0.04 | 2.00+-0.04 | Zn I |
Y II | 11 | ... | ... | -0.80+-0.12 | -3.01+-0.12 | -0.28+-0.12 | -0.80+-0.12 | Y II |
Zr II | 10 | ... | ... | -0.14+-0.12 | -2.72+-0.12 | 0.01+-0.12 | -0.14+-0.12 | Zr II |
Ba II | 4 | ... | ... | -1.80+-0.01 | -3.98+-0.01 | -1.25+-0.01 | -1.80+-0.01 | Ba II |
La II | 1 | ... | ... | -2.44+-0.10 | -3.54+-0.10 | -0.81+-0.10 | -2.44+-0.10 | La II |
Pr II | N/A | ... | ... | <-1.55 | <-2.27 | <0.46 | <-1.55 | Pr II |
Nd II | 1 | ... | ... | -1.87+-0.20 | -3.29+-0.20 | -0.56+-0.20 | -1.87+-0.20 | Nd II |
Eu II | 1 | ... | ... | -2.85+-0.20 | -3.37+-0.20 | -0.64+-0.20 | -2.85+-0.20 | Eu II |
Tb II | N/A | ... | ... | <-1.81 | <-2.13 | <0.60 | <-1.81 | Tb II |
Ho II | N/A | ... | ... | <-1.66 | <-2.13 | <0.60 | <-1.66 | Ho II |
Er II | 1 | ... | ... | -2.43+-0.10 | -3.35+-0.10 | -0.62+-0.10 | -2.43+-0.10 | Er II |
Tm II | N/A | ... | ... | <-2.33 | <-2.45 | <0.28 | <-2.33 | Tm II |
Yb II | 1 | ... | ... | -2.78+-0.20 | -3.70+-0.20 | -0.97+-0.20 | -2.78+-0.20 | Yb II |
Hf II | N/A | ... | ... | <-0.88 | <-1.59 | <1.14 | <-0.88 | Hf II |
Os I | N/A | ... | ... | <-0.41 | <-1.81 | <0.92 | <-0.41 | Os I |
Position
Right Ascension : 14 02 31.80 | Declination : +09 41 10.0 | Galactic Longitude (l) : N/A | Galactic Latitude (b) : N/A |
Observing Log
Date of Observation | JD | Facility | Resolution | S/N | Exposure Time | Vrad |
1997-05-12 | N/A | KECKHIRES | 45000 | 500 | 600 | N/A |
1997-06-20 | N/A | KECKHIRES | 45000 | N/A | 600 | N/A |
1998-06-09 | N/A | LICKHAMILTON | 60000 | 95 | 120 | N/A |
THE r-PROCESS-ENRICHED LOW-METALLICITY GIANT HD 115444
Stellar Parameters
Teff : 4500 | log g : 1.30 | vturb : 2.5 |
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 |
O I | 1 | ... | +0.61+-0.11 | +6.80+-0.11 | -1.89+-0.11 | 0.83+-0.11 | +6.80+-0.11 | O I |
Na I | 2 | ... | -0.15+-0.11 | +3.44+-0.11 | -2.80+-0.11 | -0.08+-0.11 | +3.44+-0.11 | Na I |
Mg I | 7 | ... | +0.51+-0.12 | +5.35+-0.12 | -2.25+-0.12 | 0.47+-0.12 | +5.35+-0.12 | Mg I |
Al I | 1 | ... | -0.32+-0.11 | +3.41+-0.11 | -3.04+-0.11 | -0.32+-0.11 | +3.41+-0.11 | Al I |
Si I | 1 | ... | +0.46+-0.11 | +5.27+-0.11 | -2.24+-0.11 | 0.48+-0.11 | +5.27+-0.11 | Si I |
Ca I | 13 | ... | +0.29+-0.09 | +3.91+-0.09 | -2.43+-0.09 | 0.29+-0.09 | +3.91+-0.09 | Ca I |
Sc II | 5 | ... | +0.15+-0.08 | +0.51+-0.08 | -2.64+-0.08 | 0.08+-0.08 | +0.51+-0.08 | Sc II |
Ti I | 12 | ... | +0.19+-0.07 | +2.44+-0.07 | -2.51+-0.07 | 0.21+-0.07 | +2.44+-0.07 | Ti I |
Ti II | 21 | ... | +0.28+-0.15 | +2.53+-0.15 | -2.42+-0.15 | 0.30+-0.15 | +2.53+-0.15 | Ti II |
V I | 2 | ... | +0.07+-0.11 | +1.33+-0.11 | -2.60+-0.11 | 0.12+-0.11 | +1.33+-0.11 | V I |
V II | 2 | ... | +0.14+-0.11 | +1.40+-0.11 | -2.53+-0.11 | 0.19+-0.11 | +1.40+-0.11 | V II |
Cr I | 6 | ... | -0.39+-0.15 | +2.54+-0.15 | -3.10+-0.15 | -0.38+-0.15 | +2.54+-0.15 | Cr I |
Mn I | 6 | ... | -0.26+-0.19 | +2.39+-0.19 | -3.04+-0.19 | -0.32+-0.19 | +2.39+-0.19 | Mn I |
Fe I | 158 | -2.74+-0.12 | ... | +4.78+-0.12 | -2.72+-0.12 | ... | +4.78+-0.12 | Fe I |
Fe II | 23 | -2.74+-0.10 | ... | +4.78+-0.10 | -2.72+-0.10 | ... | +4.78+-0.10 | Fe II |
Co I | 4 | ... | +0.32+-0.20 | +2.50+-0.20 | -2.49+-0.20 | 0.23+-0.20 | +2.50+-0.20 | Co I |
Ni I | 3 | ... | +0.04+-0.05 | +3.55+-0.05 | -2.67+-0.05 | 0.05+-0.05 | +3.55+-0.05 | Ni I |
Cu I | 1 | ... | -0.75+-0.11 | +0.72+-0.11 | -3.47+-0.11 | -0.75+-0.11 | +0.72+-0.11 | Cu I |
Zn I | 2 | ... | +0.20+-0.11 | +2.06+-0.11 | -2.50+-0.11 | 0.22+-0.11 | +2.06+-0.11 | Zn I |
Ge I | 1 | ... | -0.70+-0.11 | -0.03+-0.11 | -3.68+-0.11 | -0.96+-0.11 | -0.03+-0.11 | Ge I |
Sr II | 2 | ... | +0.17+-0.11 | +0.33+-0.11 | -2.54+-0.11 | 0.18+-0.11 | +0.33+-0.11 | Sr II |
Y II | 8 | ... | -0.25+-0.11 | -0.75+-0.11 | -2.96+-0.11 | -0.24+-0.11 | -0.75+-0.11 | Y II |
Zr II | 5 | ... | +0.18+-0.19 | +0.04+-0.19 | -2.54+-0.19 | 0.18+-0.19 | +0.04+-0.19 | Zr II |
Ba II | 4 | ... | -0.93+-0.13 | -1.54+-0.13 | -3.72+-0.13 | -1.00+-0.13 | -1.54+-0.13 | Ba II |
La II | 2 | ... | -0.70+-0.11 | -2.22+-0.11 | -3.32+-0.11 | -0.60+-0.11 | -2.22+-0.11 | La II |
Ce II | 1 | ... | -0.73+-0.11 | -1.92+-0.11 | -3.50+-0.11 | -0.78+-0.11 | -1.92+-0.11 | Ce II |
Nd II | 2 | ... | -0.30+-0.11 | -1.54+-0.11 | -2.96+-0.11 | -0.24+-0.11 | -1.54+-0.11 | Nd II |
Eu II | 2 | ... | -0.36+-0.11 | -2.59+-0.11 | -3.11+-0.11 | -0.39+-0.11 | -2.59+-0.11 | Eu II |
Er II | 2 | ... | -0.46+-0.11 | -2.27+-0.11 | -3.19+-0.11 | -0.47+-0.11 | -2.27+-0.11 | Er II |
Yb II | 1 | ... | -0.96+-0.11 | -2.62+-0.11 | -3.54+-0.11 | -0.82+-0.11 | -2.62+-0.11 | Yb II |
Isotopic Ratio
Position
Right Ascension : 14 02 31.80 | Declination : +09 41 10.0 | 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 | MCDONALD | 60000 | 200,400,500 | N/A | N/A |
Extremely Metal-poor Stars. IV. The Carbon-rich Objects
Stellar Parameters
Teff : 4650 | log g : 1.4 | vturb : 2.6 |
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 |
CH | N/A | ... | -0.45+-0.20 | ... | -3.00+-0.20 | -0.49+-0.20 | 5.43+-0.20 | CH |
CN | N/A | ... | +1.00 | ... | -1.46 | 1.05 | 6.37 | CN |
Mg I | 7 | ... | +0.32+-0.04 | ... | -2.38+-0.04 | 0.13+-0.04 | 5.22+-0.04 | Mg I |
Al I | 1 | ... | -0.24+-0.10 | ... | -2.90+-0.10 | -0.39+-0.10 | 3.55+-0.10 | Al I |
Ca I | 9 | ... | +0.14+-0.06 | ... | -2.52+-0.06 | -0.01+-0.06 | 3.82+-0.06 | Ca I |
Sc II | 7 | ... | +0.25+-0.11 | ... | -2.49+-0.11 | 0.02+-0.11 | 0.66+-0.11 | Sc II |
Ti I | 10 | ... | +0.12+-0.05 | ... | -2.52+-0.05 | -0.01+-0.05 | 2.43+-0.05 | Ti I |
Ti II | 32 | ... | +0.34+-0.08 | ... | -2.30+-0.08 | 0.21+-0.08 | 2.65+-0.08 | Ti II |
Cr I | 7 | ... | -0.39+-0.07 | ... | -3.04+-0.07 | -0.53+-0.07 | 2.60+-0.07 | Cr I |
Mn I | 5 | ... | -0.37+-0.05 | ... | -3.09+-0.05 | -0.58+-0.05 | 2.34+-0.05 | Mn I |
Fe I | 165 | -2.68+-0.11 | ... | ... | -2.51+-0.11 | ... | 4.99+-0.11 | Fe I |
Co I | 5 | ... | +0.33+-0.07 | ... | -2.42+-0.07 | 0.09+-0.07 | 2.57+-0.07 | Co I |
Ni I | 9 | ... | +0.21+-0.08 | ... | -2.44+-0.08 | 0.07+-0.08 | 3.78+-0.08 | Ni I |
Sr II | 2 | ... | -0.21+-0.10 | ... | -2.86+-0.10 | -0.35+-0.10 | 0.01+-0.10 | Sr II |
Y II | 1 | ... | -0.16+-0.18 | ... | -2.81+-0.18 | -0.30+-0.18 | -0.60+-0.18 | Y II |
Zr II | 1 | ... | -0.10+-0.22 | ... | -2.76+-0.22 | -0.25+-0.22 | -0.18+-0.22 | Zr II |
Ba II | 1 | ... | -0.84+-0.10 | ... | -3.57+-0.10 | -1.06+-0.10 | -1.39+-0.10 | Ba II |
La II | N/A | ... | -0.67 | ... | -3.23 | -0.72 | -2.13 | La II |
Ce II | N/A | ... | <-0.32 | ... | <-2.97 | <-0.46 | <-1.39 | Ce II |
Nd II | N/A | ... | -0.52 | ... | -3.12 | -0.61 | -1.70 | Nd II |
Sm II | N/A | ... | <-0.52 | ... | <-3.16 | <-0.65 | <-2.20 | Sm II |
Eu II | N/A | ... | -0.32 | ... | -3.01 | -0.50 | -2.49 | Eu II |
Dy II | N/A | ... | -0.32 | ... | -3.00 | -0.49 | -1.90 | Dy II |
Position
Right Ascension : 14 02 31.80 | Declination : +09 41 10.0 | Galactic Longitude (l) : N/A | Galactic Latitude (b) : N/A |
Observing Log
Spectroscopic Studies of Very Metal-poor Stars with the Subaru High Dispersion Spectrograph. III. Light Neutron-Capture Elements
Stellar Parameters
Teff : 4600 | log g : 1.1 | vturb : 2.2 |
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 |
CH | N/A | ... | -0.4 | 5.4 | -3.03 | -0.41 | 5.4 | CH |
Mg I | 8 | ... | 0.53+-0.12 | 5.49+-0.12 | -2.11+-0.12 | 0.51+-0.12 | 5.49+-0.12 | Mg I |
Al I | 1 | ... | -0.5+-0.18 | 3.37+-0.18 | -3.08+-0.18 | -0.46+-0.18 | 3.37+-0.18 | Al I |
Si I | 2 | ... | 0.42+-0.13 | 5.36+-0.13 | -2.15+-0.13 | 0.47+-0.13 | 5.36+-0.13 | Si I |
Ca I | 9 | ... | 0.18+-0.12 | 3.91+-0.12 | -2.43+-0.12 | 0.19+-0.12 | 3.91+-0.12 | Ca I |
Sc II | 5 | ... | 0.07+-0.23 | 0.55+-0.23 | -2.60+-0.23 | 0.02+-0.23 | 0.55+-0.23 | Sc II |
Ti I | 17 | ... | 0.11+-0.12 | 2.43+-0.12 | -2.52+-0.12 | 0.10+-0.12 | 2.43+-0.12 | Ti I |
Ti II | 31 | ... | 0.31+-0.24 | 2.63+-0.24 | -2.32+-0.24 | 0.30+-0.24 | 2.63+-0.24 | Ti II |
Cr I | 11 | ... | -0.42+-0.1 | 2.65+-0.1 | -2.99+-0.1 | -0.37+-0.1 | 2.65+-0.1 | Cr I |
Mn I | 10 | ... | -0.64+-0.12 | 2.27+-0.12 | -3.16+-0.12 | -0.54+-0.12 | 2.27+-0.12 | Mn I |
Fe I | 147 | -2.62+-0.21 | ... | 4.88+-0.21 | -2.62+-0.21 | ... | 4.88+-0.21 | Fe I |
Fe II | 17 | -2.62+-0.19 | ... | 4.88+-0.19 | -2.62+-0.19 | ... | 4.88+-0.19 | Fe II |
Co I | 8 | ... | 0.25+-0.11 | 2.54+-0.11 | -2.45+-0.11 | 0.17+-0.11 | 2.54+-0.11 | Co I |
Ni I | 9 | ... | 0.03+-0.11 | 3.66+-0.11 | -2.56+-0.11 | 0.06+-0.11 | 3.66+-0.11 | Ni I |
Zn I | 2 | ... | 0.1+-0.21 | 2.15+-0.21 | -2.41+-0.21 | 0.21+-0.21 | 2.15+-0.21 | Zn I |
Sr II | 2 | ... | -0.22+-0.16 | 0.08+-0.16 | -2.79+-0.16 | -0.17+-0.16 | 0.08+-0.16 | Sr II |
Y II | 6 | ... | -0.45+-0.24 | -0.84+-0.24 | -3.05+-0.24 | -0.43+-0.24 | -0.84+-0.24 | Y II |
Zr II | 4 | ... | -0.13+-0.24 | -0.14+-0.24 | -2.72+-0.24 | -0.10+-0.24 | -0.14+-0.24 | Zr II |
Ba II | 2 | ... | -1.29+-0.23 | -1.69+-0.23 | -3.87+-0.23 | -1.25+-0.23 | -1.69+-0.23 | Ba II |
La II | 1 | ... | -0.52+-0.29 | -2.37+-0.29 | -3.47+-0.29 | -0.85+-0.29 | -2.37+-0.29 | La II |
Nd II | 1 | ... | -0.8+-0.25 | -1.93+-0.25 | -3.35+-0.25 | -0.73+-0.25 | -1.93+-0.25 | Nd II |
Eu II | 3 | ... | -0.57+-0.25 | -2.64+-0.25 | -3.16+-0.25 | -0.54+-0.25 | -2.64+-0.25 | Eu II |
Er II | 1 | ... | -0.68+-0.25 | -2.33+-0.25 | -3.25+-0.25 | -0.63+-0.25 | -2.33+-0.25 | Er II |
Binary Parameters
Position
Right Ascension : 14 02 31.80 | Declination : +09 41 10.0 | Galactic Longitude (l) : N/A | Galactic Latitude (b) : N/A |
Observing Log
Date of Observation | JD | Facility | Resolution | S/N | Exposure Time | Vrad |
2002-02-02 | N/A | SUBARUHDS | 50000 | 1500 | 15min | -25.81+-0.17 |
Abundances of Cu and Zn in metal-poor stars: Clues for Galaxy evolution
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 | -2.66 | ... | ... | -2.66 | ... | 4.84 | Fe |
Cu I | N/A | ... | -0.72+-0.25 | ... | -3.36+-0.25 | -0.70+-0.25 | 0.83+-0.25 | Cu I |
Zn I | N/A | ... | 0.12+-0.19 | ... | -2.50+-0.19 | 0.16+-0.19 | 2.06+-0.19 | Zn I |
Position
Right Ascension : 14 02 31.80 | Declination : +09 41 10.0 | 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 | ELODIE | 42000 | >100 | N/A | N/A |
Analysis of neutron capture elements in metal-poor stars
Stellar Parameters
Teff : 4570 | log g : 1.1 | vturb : 1.2 |
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 |
Si I | N/A | ... | 0.26 | ... | -2.12 | 0.30 | 5.39 | Si I |
Ca I | N/A | ... | 0.28 | ... | -2.12 | 0.30 | 4.22 | Ca I |
Fe | N/A | -2.42 | ... | ... | -2.42 | ... | 5.08 | Fe |
Ba II | N/A | ... | -1.11 | ... | -3.58 | -1.16 | -1.40 | Ba II |
Position
Right Ascension : 14 02 31.80 | Declination : +09 41 10.0 | 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 | ELODIE | 42000 | >100 | N/A | N/A |
Oxygen Abundance in the Template Halo Giant HD 122563
Stellar Parameters
Teff : 4600 | log g : 1.1 | vturb : 2.0 |
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 | ... | 0.9 | ... | -1.69 | 1.08 | 7.00 | O |
Na I | 2 | -2.56 | ... | ... | -2.47 | 0.30 | 3.77 | Na I |
Mg I | 5 | -2.35 | +0.45 | ... | -2.37 | 0.40 | 5.23 | Mg I |
Al I | 2 | -3.18 | -0.38 | ... | -3.16 | -0.39 | 3.29 | Al I |
Si I | 1 | -2.28 | +0.52 | ... | -2.24 | 0.53 | 5.27 | Si I |
K I | 1 | -2.30 | +0.50 | ... | -2.21 | 0.56 | 2.82 | K I |
Ca I | 17 | -2.50 | +0.30 | ... | -2.48 | 0.29 | 3.86 | Ca I |
Sc II | 7 | -2.70 | +0.10 | ... | -2.68 | 0.09 | 0.47 | Sc II |
Ti I | 14 | -2.69 | +0.11 | ... | -2.62 | 0.15 | 2.33 | Ti I |
Ti II | 29 | -2.64 | +0.16 | ... | -2.57 | 0.20 | 2.38 | Ti II |
Cr I | 7 | -3.20 | ... | ... | -3.17 | -0.40 | 2.47 | Cr I |
Mn I | 5 | -2.94 | ... | ... | -2.98 | -0.21 | 2.45 | Mn I |
Fe I | 144 | -2.77 | ... | ... | -2.77 | ... | 4.73 | Fe I |
Fe II | 18 | -2.84 | ... | ... | -2.84 | ... | 4.66 | Fe II |
Co I | 4 | -2.52 | ... | ... | -2.59 | 0.18 | 2.40 | Co I |
Ni I | 4 | -2.67 | ... | ... | -2.64 | 0.13 | 3.58 | Ni I |
Zn I | 1 | -2.63 | ... | ... | -2.59 | 0.18 | 1.97 | Zn I |
Position
Right Ascension : 14 02 31.80 | Declination : +09 41 10.0 | Galactic Longitude (l) : N/A | Galactic Latitude (b) : N/A |
Observing Log
Date of Observation | JD | Facility | Resolution | S/N | Exposure Time | Vrad |
2000-05-20 | N/A | KECKNIRSPEC | 37000 | 250 | 4x120 | N/A |
2000-07-18 | N/A | VLT | 43000 | 267 | 75 | N/A |
2000-07-18 | N/A | VLT | 43000 | 305 | 75 | N/A |
2000-07-18 | N/A | VLT | 43000 | 370 | 75 | N/A |
2000-07-18 | N/A | VLT | 43000 | 390 | 75 | N/A |
2002-03-18 | N/A | FEROSESO | 37000 | 180 | 600 | N/A |
2002-03-18 | N/A | FEROSESO | 37000 | 255 | 600 | N/A |
2002-04-01 | N/A | FEROSESO | 37000 | 260 | 600 | N/A |
Oxygen Abundances in Metal-poor Stars
Stellar Parameters
Teff : 4650 | log g : 1.24 | vturb : 1.85 |
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 | ... | 0.74+-0.17 | 6.81+-0.18 | -1.88+-0.18 | 0.72+-0.17 | 6.81+-0.18 | O I |
Fe | N/A | -2.62 | ... | ... | -2.60 | ... | 4.90 | Fe |
Fe I | N/A | ... | ... | 4.91+-0.07 | -2.59+-0.07 | ... | 4.91+-0.07 | Fe I |
Fe II | N/A | ... | ... | 4.9+-0.04 | -2.60+-0.04 | ... | 4.9+-0.04 | Fe II |
Position
Right Ascension : 14 02 31.80 | Declination : +09 41 10.0 | Galactic Longitude (l) : N/A | Galactic Latitude (b) : N/A |
Observing Log
Date of Observation | JD | Facility | Resolution | S/N | Exposure Time | Vrad |
2001-04-05 | N/A | GECKOCFHT | 130000 | 400 | 900 | N/A |
Hubble Space Telescope Observations of Heavy Elements in Metal-Poor Galactic Halo Stars
Stellar Parameters
Teff : 4570 | log g : 1.35 | vturb : 2.90 |
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 I | N/A | -2.72 | ... | ... | -2.75 | ... | 4.75 | Fe I |
Fe II | N/A | -2.61 | ... | ... | -2.64 | ... | 4.86 | Fe II |
Ge | N/A | ... | -0.94 | -0.16 | -3.81 | -1.06 | -0.16 | Ge |
Zr | N/A | ... | +0.07 | +0.06 | -2.52 | 0.23 | +0.06 | Zr |
La | N/A | ... | -0.90 | -2.35 | -3.45 | -0.70 | -2.35 | La |
Eu | N/A | ... | -0.50 | -2.59 | -3.11 | -0.36 | -2.59 | Eu |
Os | N/A | ... | <+0.1 | <-1.2 | <-2.60 | <0.15 | <-1.2 | Os |
Ir | N/A | ... | <+0.1 | <-1.3 | <-2.68 | <0.07 | <-1.3 | Ir |
Pt | N/A | ... | <-0.3 | <-1.3 | <-2.92 | <-0.17 | <-1.3 | Pt |
Position
Right Ascension : 14 02 31.80 | Declination : +09 41 10.0 | 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 | HST | 30000 | >50 | N/A | N/A |
| N/A | KECKHIRES | 45000 | 30-200 | N/A | N/A |
Spectroscopic Studies of Extremely Metal-Poor Stars with the Subaru High Dispersion Spectrograph. I. Observational Data
Binary Parameters
Position
Right Ascension : 14 02 31.80 | Declination : +09 41 10.0 | Galactic Longitude (l) : N/A | Galactic Latitude (b) : N/A |
Observing Log
Date of Observation | JD | Facility | Resolution | S/N | Exposure Time | Vrad |
2000-07-04 | N/A | SUBARUHDS | 90000 | 374 | 1200 | -27.20+-0.33 |
2001-01-29 | N/A | SUBARUHDS | N/A | N/A | N/A | -26.52+-0.34 |
First stars IX - Mixing in extremely metal-poor giants. Variation of the 12C/13C, [Na/Mg] and [Al/Mg] ratios
Stellar Parameters
Teff : 4600 | log g : 1.1 | vturb : 2.0 |
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 | -3.21+-0.05 | ... | ... | -3.12+-0.05 | -0.30+-0.05 | 5.31+-0.05 | C |
N | N/A | -2.12+-0.15 | ... | ... | -2.03+-0.15 | 0.79+-0.15 | 5.80+-0.15 | N |
Fe | N/A | -2.82 | ... | ... | -2.82 | ... | 4.68 | Fe |
Isotopic Ratio
Position
Right Ascension : 14 02 31.80 | Declination : +09 41 10.0 | 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 | VLT | 47000 | 130 | N/A | N/A |
NLTE determination of the sodium abundance in a homogeneous sample of extremely metal-poor stars
Stellar Parameters
Teff : 4600 | log g : 1.1 | vturb : 2.0 |
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 | -3.05 | -0.23 | 3.20 | -3.04 | -0.22 | 3.20 | Na |
Fe | N/A | -2.82 | ... | ... | -2.82 | ... | 4.68 | Fe |
Position
Right Ascension : 14 02 31.80 | Declination : +09 41 10.0 | 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 | VLT | 43000 | 200 | N/A | N/A |
A Search for Nitrogen-enhanced Metal-poor Stars
Stellar Parameters
Teff : 4615 | log g : 1.27 | 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 |
C | N/A | ... | -0.95+-0.29 | 5.14+-0.25 | -3.29+-0.25 | -0.84+-0.29 | 5.14+-0.25 | C |
N | N/A | ... | +1.00+-0.25 | 6.58+-0.25 | -1.25+-0.25 | 1.20+-0.25 | 6.58+-0.25 | N |
Fe | N/A | -2.47+-0.21 | ... | ... | -2.45+-0.21 | ... | 5.05+-0.21 | Fe |
Position
Right Ascension : 14 02 31.80 | Declination : +09 41 10.0 | Galactic Longitude (l) : N/A | Galactic Latitude (b) : N/A |
Observing Log
Date of Observation | JD | Facility | Resolution | S/N | Exposure Time | Vrad |
2003-08-31 | N/A | RCKPNO | N/A | 267 | 600 | N/A |
Spectroscopic Studies of Extremely Metal-poor Stars with the Subaru High-Dispersion Spectrograph. IV. The alpha-Element Enhanced Metal-poor Star BS 16934-002
Stellar Parameters
Teff : 4600 | log g : 1.1 | vturb : 2.2 |
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 |
CH | N/A | ... | -0.35+-0.17 | 5.45+-0.17 | -2.98+-0.17 | -0.34+-0.17 | 5.45+-0.17 | CH |
CN | N/A | ... | +0.61+-0.29 | 5.80+-0.29 | -2.03+-0.29 | 0.61+-0.29 | 5.80+-0.29 | CN |
O I | 2 | ... | +0.74+-0.19 | 6.81+-0.19 | -1.88+-0.19 | 0.76+-0.19 | 6.81+-0.19 | O I |
Na I | 2 | ... | -0.19+-0.13 | 3.39+-0.13 | -2.85+-0.13 | -0.21+-0.13 | 3.39+-0.13 | Na I |
Mg I | 6 | ... | +0.49+-0.11 | 5.44+-0.11 | -2.16+-0.11 | 0.48+-0.11 | 5.44+-0.11 | Mg I |
Al I | 1 | ... | -0.40+-0.18 | 3.38+-0.18 | -3.07+-0.18 | -0.43+-0.18 | 3.38+-0.18 | Al I |
Si I | 4 | ... | +0.41+-0.16 | 5.34+-0.16 | -2.17+-0.16 | 0.47+-0.16 | 5.34+-0.16 | Si I |
Ca I | 20 | ... | +0.20+-0.11 | 3.93+-0.11 | -2.41+-0.11 | 0.23+-0.11 | 3.93+-0.11 | Ca I |
Sc II | 14 | ... | +0.11+-0.23 | 0.57+-0.23 | -2.58+-0.23 | 0.06+-0.23 | 0.57+-0.23 | Sc II |
Ti I | 27 | ... | +0.11+-0.12 | 2.42+-0.12 | -2.53+-0.12 | 0.11+-0.12 | 2.42+-0.12 | Ti I |
Ti II | 41 | ... | +0.27+-0.24 | 2.58+-0.24 | -2.37+-0.24 | 0.27+-0.24 | 2.58+-0.24 | Ti II |
Cr I | 13 | ... | -0.38+-0.10 | 2.57+-0.10 | -3.07+-0.10 | -0.43+-0.10 | 2.57+-0.10 | Cr I |
Mn I | 8 | ... | -0.57+-0.13 | 2.23+-0.13 | -3.20+-0.13 | -0.56+-0.13 | 2.23+-0.13 | Mn I |
Fe I | 214 | -2.59+-0.20 | ... | 4.86+-0.20 | -2.64+-0.20 | ... | 4.86+-0.20 | Fe I |
Fe II | 20 | -2.58+-0.19 | ... | 4.87+-0.19 | -2.63+-0.19 | ... | 4.87+-0.19 | Fe II |
Co I | 7 | ... | +0.15+-0.11 | 2.48+-0.11 | -2.51+-0.11 | 0.13+-0.11 | 2.48+-0.11 | Co I |
Ni I | 15 | ... | +0.02+-0.11 | 3.66+-0.11 | -2.56+-0.11 | 0.08+-0.11 | 3.66+-0.11 | Ni I |
Zn I | 2 | ... | +0.06+-0.21 | 2.08+-0.21 | -2.48+-0.21 | 0.16+-0.21 | 2.08+-0.21 | Zn I |
Sr II | 2 | ... | -0.30+-0.15 | 0.08+-0.15 | -2.79+-0.15 | -0.15+-0.15 | 0.08+-0.15 | Sr II |
Ba II | 2 | ... | -1.28+-0.23 | -1.69+-0.23 | -3.87+-0.23 | -1.23+-0.23 | -1.69+-0.23 | Ba II |
Position
Right Ascension : 14 02 31.80 | Declination : +09 41 10.0 | Galactic Longitude (l) : N/A | Galactic Latitude (b) : N/A |
Observing Log
Date of Observation | JD | Facility | Resolution | S/N | Exposure Time | Vrad |
2005-06-19 | 2453541 | SUBARUHDS | 60000 | 300 | 240 | -26.0+-0.2 |
Neutron-Capture Elements in the Very Metal Poor Star HD 122563
Stellar Parameters
Teff : 4570+-100 | log g : 1.1+-0.3 | vturb : 2.2+-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 |
Fe | N/A | -2.77+-0.19 | ... | ... | -2.82+-0.19 | ... | 4.68+-0.19 | Fe |
Cu | 3 | ... | -1.15+-0.29 | 0.98+-0.29 | -3.21+-0.29 | -0.39+-0.29 | 0.98+-0.29 | Cu |
Zn | 4 | ... | +0.18+-0.16 | 2.01+-0.16 | -2.55+-0.16 | 0.27+-0.16 | 2.01+-0.16 | Zn |
Sr | 3 | ... | -0.26+-0.08 | -0.11+-0.08 | -2.98+-0.08 | -0.16+-0.08 | -0.11+-0.08 | Sr |
Y | 15 | ... | -0.37+-0.09 | -0.93+-0.09 | -3.14+-0.09 | -0.32+-0.09 | -0.93+-0.09 | Y |
Zr | 17 | ... | -0.10+-0.16 | -0.28+-0.16 | -2.86+-0.16 | -0.04+-0.16 | -0.28+-0.16 | Zr |
Nb | 2 | ... | -0.13+-0.17 | -1.48+-0.17 | -2.94+-0.17 | -0.12+-0.17 | -1.48+-0.17 | Nb |
Mo | 1 | ... | -0.02+-0.17 | -0.87+-0.17 | -2.75+-0.17 | 0.07+-0.17 | -0.87+-0.17 | Mo |
Ru | 2 | ... | +0.07+-0.17 | -0.86+-0.17 | -2.61+-0.17 | 0.21+-0.17 | -0.86+-0.17 | Ru |
Rh | 1 | ... | <+0.45 | <-1.20 | <-2.11 | <0.71 | <-1.20 | Rh |
Pd | 2 | ... | -0.28+-0.17 | -1.36+-0.17 | -2.93+-0.17 | -0.11+-0.17 | -1.36+-0.17 | Pd |
Ag | 1 | ... | -0.05+-0.17 | -1.88+-0.17 | -3.08+-0.17 | -0.26+-0.17 | -1.88+-0.17 | Ag |
Ba | 4 | ... | -1.02+-0.12 | -1.62+-0.12 | -3.80+-0.12 | -0.98+-0.12 | -1.62+-0.12 | Ba |
La | 5 | ... | -1.02+-0.10 | -2.66+-0.10 | -3.76+-0.10 | -0.94+-0.10 | -2.66+-0.10 | La |
Ce | 6 | ... | -0.64+-0.18 | -1.83+-0.18 | -3.41+-0.18 | -0.59+-0.18 | -1.83+-0.18 | Ce |
Pr | 1 | ... | -0.09+-0.17 | -2.15+-0.17 | -2.87+-0.17 | -0.05+-0.17 | -2.15+-0.17 | Pr |
Nd | 4 | ... | -0.69+-0.10 | -2.01+-0.10 | -3.43+-0.10 | -0.61+-0.10 | -2.01+-0.10 | Nd |
Sm | 2 | ... | -0.40+-0.17 | -2.16+-0.17 | -3.12+-0.17 | -0.30+-0.17 | -2.16+-0.17 | Sm |
Eu | 1 | ... | -0.52+-0.17 | -2.77+-0.17 | -3.29+-0.17 | -0.47+-0.17 | -2.77+-0.17 | Eu |
Gd | 2 | ... | -0.76+-0.17 | -2.44+-0.17 | -3.51+-0.17 | -0.69+-0.17 | -2.44+-0.17 | Gd |
Dy | 2 | ... | -0.99+-0.17 | -2.62+-0.17 | -3.72+-0.17 | -0.90+-0.17 | -2.62+-0.17 | Dy |
Ho | 1 | ... | <+0.26 | <-2.00 | <-2.47 | <0.35 | <-2.00 | Ho |
Er | 2 | ... | -0.82+-0.17 | -2.66+-0.17 | -3.58+-0.17 | -0.76+-0.17 | -2.66+-0.17 | Er |
Tm | 1 | ... | <-0.23 | <-3.00 | <-3.12 | <-0.30 | <-3.00 | Tm |
Yb | 2 | ... | -1.09+-0.17 | -2.78+-0.17 | -3.70+-0.17 | -0.88+-0.17 | -2.78+-0.17 | Yb |
Ir | 2 | ... | <-0.21 | <-1.60 | <-2.98 | <-0.16 | <-1.60 | Ir |
Th | 1 | ... | <-0.34 | <-3.05 | <-3.11 | <-0.29 | <-3.05 | Th |
Position
Right Ascension : 14 02 31.80 | Declination : +09 41 10.0 | Galactic Longitude (l) : N/A | Galactic Latitude (b) : N/A |
Observing Log
Date of Observation | JD | Facility | Resolution | S/N | Exposure Time | Vrad |
2004-04-30 | N/A | SUBARUHDS | 90000 | 140-1340 | 5400 | N/A |
ABUNDANCES AND KINEMATICS OF FIELD HALO AND DISK STARS. I. OBSERVATIONAL DATA AND ABUNDANCE ANALYSIS
Stellar Parameters
Teff : 4425 | log g : 0.6 | 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 | ... | 0.1 | ... | -2.60 | 0.17 | 3.64 | Na I |
Mg I | N/A | ... | 0.63 | ... | -2.18 | 0.59 | 5.42 | Mg I |
Si I | N/A | ... | 0.42 | ... | -2.33 | 0.44 | 5.18 | Si I |
Ca I | N/A | ... | 0.33 | ... | -2.44 | 0.33 | 3.90 | Ca I |
Ti | N/A | ... | 0.22 | ... | -2.53 | 0.24 | 2.42 | Ti |
V I | N/A | ... | -0.04 | ... | -2.76 | 0.01 | 1.17 | V I |
Cr I | N/A | ... | -0.25 | ... | -3.01 | -0.24 | 2.63 | Cr I |
Fe | N/A | -2.79 | ... | ... | -2.77 | ... | 4.73 | Fe |
Ni I | N/A | ... | 0.12 | ... | -2.64 | 0.13 | 3.58 | Ni I |
Y II | N/A | ... | -0.44 | ... | -3.20 | -0.43 | -0.99 | Y II |
Zr II | N/A | ... | -0.08 | ... | -2.85 | -0.08 | -0.27 | Zr II |
Ba II | N/A | ... | -1.04 | ... | -3.88 | -1.11 | -1.70 | Ba II |
Position
Right Ascension : 14 02 31.80 | Declination : +09 41 10.0 | Galactic Longitude (l) : N/A | Galactic Latitude (b) : N/A |
Observing Log
Date of Observation | JD | Facility | Resolution | S/N | Exposure Time | Vrad |
1998067-8 | N/A | LICKHAMILTON | 50000 | 95 | 120 | N/A |
Neutron-Capture Elements in the Very Metal-poor Star HD 88609: Another Star with Excesses of Light Neutron-Capture Elements
Stellar Parameters
Teff : 4570+-100 | log g : 1.1+-0.3 | vturb : 2.2+-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 |
Fe | N/A | -2.77+-0.19 | ... | ... | -2.82+-0.19 | ... | 4.68+-0.19 | Fe |
Cu | 3 | ... | -0.46+-0.14 | 0.98+-0.14 | -3.21+-0.14 | -0.39+-0.14 | 0.98+-0.14 | Cu |
Zn | 4 | ... | +0.18+-0.15 | 2.01+-0.15 | -2.55+-0.15 | 0.27+-0.15 | 2.01+-0.15 | Zn |
Sr | 3 | ... | -0.27+-0.14 | -0.12+-0.14 | -2.99+-0.14 | -0.17+-0.14 | -0.12+-0.14 | Sr |
Y | 15 | ... | -0.37+-0.09 | -0.93+-0.09 | -3.14+-0.09 | -0.32+-0.09 | -0.93+-0.09 | Y |
Zr | 17 | ... | -0.10+-0.16 | -0.28+-0.16 | -2.86+-0.16 | -0.04+-0.16 | -0.28+-0.16 | Zr |
Nb | 2 | ... | -0.13+-0.14 | -1.48+-0.14 | -2.94+-0.14 | -0.12+-0.14 | -1.48+-0.14 | Nb |
Mo | 1 | ... | -0.02+-0.14 | -0.87+-0.14 | -2.75+-0.14 | 0.07+-0.14 | -0.87+-0.14 | Mo |
Ru | 2 | ... | 0.07+-0.14 | -0.86+-0.14 | -2.61+-0.14 | 0.21+-0.14 | -0.86+-0.14 | Ru |
Rh | 1 | ... | <+0.45 | <-1.20 | <-2.11 | <0.71 | <-1.20 | Rh |
Pd | 1 | ... | -0.23+-0.14 | -1.31+-0.14 | -2.88+-0.14 | -0.06+-0.14 | -1.31+-0.14 | Pd |
Ag | 1 | ... | -0.05+-0.14 | -1.88+-0.14 | -3.08+-0.14 | -0.26+-0.14 | -1.88+-0.14 | Ag |
Ba | 4 | ... | -1.05+-0.12 | -1.65+-0.12 | -3.83+-0.12 | -1.01+-0.12 | -1.65+-0.12 | Ba |
La | 5 | ... | -0.96+-0.16 | -2.60+-0.16 | -3.70+-0.16 | -0.88+-0.16 | -2.60+-0.16 | La |
Ce | 5 | ... | -0.72+-0.17 | -1.91+-0.17 | -3.49+-0.17 | -0.67+-0.17 | -1.91+-0.17 | Ce |
Pr | 2 | ... | -0.09+-0.14 | -2.15+-0.14 | -2.87+-0.14 | -0.05+-0.14 | -2.15+-0.14 | Pr |
Nd | 4 | ... | -0.69+-0.16 | -2.01+-0.16 | -3.43+-0.16 | -0.61+-0.16 | -2.01+-0.16 | Nd |
Sm | 2 | ... | -0.40+-0.14 | -2.16+-0.14 | -3.12+-0.14 | -0.30+-0.14 | -2.16+-0.14 | Sm |
Eu | 1 | ... | -0.52+-0.14 | -2.77+-0.14 | -3.29+-0.14 | -0.47+-0.14 | -2.77+-0.14 | Eu |
Gd | 2 | ... | -0.76+-0.14 | -2.44+-0.14 | -3.51+-0.14 | -0.69+-0.14 | -2.44+-0.14 | Gd |
Dy | 2 | ... | -0.99+-0.14 | -2.62+-0.14 | -3.72+-0.14 | -0.90+-0.14 | -2.62+-0.14 | Dy |
Ho | 1 | ... | <+0.26 | <-2.00 | <-2.47 | <0.35 | <-2.00 | Ho |
Er | 2 | ... | -0.82+-0.14 | -2.66+-0.14 | -3.58+-0.14 | -0.76+-0.14 | -2.66+-0.14 | Er |
Tm | 1 | ... | <-0.23 | <-3.00 | <-3.12 | <-0.30 | <-3.00 | Tm |
Yb | 2 | ... | -1.09+-0.14 | -2.78+-0.14 | -3.70+-0.14 | -0.88+-0.14 | -2.78+-0.14 | Yb |
Ir | 2 | ... | <-0.21 | <-1.60 | <-2.98 | <-0.16 | <-1.60 | Ir |
Th | 1 | ... | <-0.34 | <-3.05 | <-3.11 | <-0.29 | <-3.05 | Th |
Position
Right Ascension : 14 02 31.80 | Declination : +09 41 10.0 | Galactic Longitude (l) : N/A | Galactic Latitude (b) : N/A |
Observing Log
Date of Observation | JD | Facility | Resolution | S/N | Exposure Time | Vrad |
2004-04-20 | N/A | SUBARUHDS | 90000 | 120,240 | 3600 | |
2005-10-19 | N/A | SUBARUHDS | 90000 | 150,330 | 9000 | -37.69+-0.3 |
Carbon and Strontium Abundances of Metal-poor 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 | ... | -0.40+-0.19 | ... | -2.81+-0.19 | -0.44+-0.19 | 5.62+-0.19 | C |
Fe | N/A | -2.54 | ... | ... | -2.37 | ... | 5.13 | Fe |
Sr | N/A | ... | -0.06 | ... | -2.57 | -0.20 | 0.30 | Sr |
Ba | N/A | ... | -1.01 | ... | -3.60 | -1.23 | -1.42 | Ba |
Position
Right Ascension : 14 02 31.80 | Declination : +09 41 10.0 | 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 | KECKII | 7000 | N/A | N/A | N/A |
The Rise of the s-Process in the Galaxy
Stellar Parameters
Teff : 4572 | log g : 1.36 | vturb : 2.90 |
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 | ... | -0.6 | ... | -3.14 | -0.42 | 5.29 | C |
Fe I | 8 | -2.72 | ... | ... | -2.72 | ... | 4.78 | Fe I |
Fe II | 7 | -2.61 | ... | ... | -2.61 | ... | 4.89 | Fe II |
La II | N/A | ... | ... | -2.35+-0.1 | -3.45+-0.1 | -0.73+-0.1 | -2.35+-0.1 | La II |
Eu II | N/A | ... | ... | -2.59+-0.04 | -3.11+-0.04 | -0.39+-0.04 | -2.59+-0.04 | Eu II |
Position
Right Ascension : 14 02 31.80 | Declination : +09 41 10.0 | 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 | MCDONALD | 60000 | 100 | N/A | N/A |
Hubble Space Telescope Observations of Neutron-Capture Elements in Very Metal Poor Stars
Stellar Parameters
Teff : 4625 | log g : 1.40 | vturb : 2.0 |
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 | -2.71 | ... | ... | -2.71 | ... | 4.79 | Fe |
Ge I | N/A | ... | -0.80 | -0.10 | -3.75 | -1.04 | -0.10 | Ge I |
Zr II | N/A | ... | +0.35 | +0.22 | -2.36 | 0.35 | +0.22 | Zr II |
Os I | N/A | ... | <-0.05 | <-1.30 | <-2.70 | <0.01 | <-1.30 | Os I |
Pt I | N/A | ... | <-0.30 | <-1.20 | <-2.82 | <-0.11 | <-1.20 | Pt I |
Pb I | N/A | ... | <-0.15 | -0.80 | -2.84 | <-0.13 | -0.80 | Pb I |
Position
Right Ascension : 14 02 31.80 | Declination : +09 41 10.0 | 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 | 32000 | 50-70 | N/A | N/A |
NLTE abundances of Mn in a sample of metal-poor stars
Stellar Parameters
Teff : 4600+-100 | log g : 1.50+-0.20 | vturb : 1.9+-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 |
Mg | N/A | ... | 0.45 | ... | -2.08 | 0.43 | 5.52 | Mg |
Mn | 7 | ... | -0.59+-0.1 | ... | -3.14+-0.1 | -0.63+-0.1 | 2.29+-0.1 | Mn |
Fe | N/A | -2.51+-0.05 | ... | ... | -2.51+-0.05 | ... | 4.99+-0.05 | Fe |
Position
Right Ascension : 14 02 31.80 | Declination : +09 41 10.0 | Galactic Longitude (l) : N/A | Galactic Latitude (b) : N/A |
Observing Log
NLTE determination of the aluminium abundance in a homogeneous sample of extremely metal-poor stars
Stellar Parameters
Teff : 4600 | log g : 1.1 | vturb : 2.0 |
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 |
Al | N/A | -2.92 | -0.10 | 3.55 | -2.90 | -0.08 | 3.55 | Al |
Fe | N/A | -2.82 | ... | ... | -2.82 | ... | 4.68 | Fe |
Position
Right Ascension : 14 02 31.80 | Declination : +09 41 10.0 | 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 | VLT | 47000 | 120 | N/A | N/A |
Europium, Samarium, and Neodymium Isotopic Fractions in Metal-Poor Stars
Stellar Parameters
Teff : 4430+-100 | log g : 0.55+-0.3 | vturb : 2.4+-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 |
Fe I | N/A | -2.83+-0.15 | ... | ... | -2.81+-0.15 | ... | 4.69+-0.15 | Fe I |
Fe II | N/A | -2.79 | ... | ... | -2.77 | ... | 4.73 | Fe II |
Binary Parameters
Binarity | Negative |
Vrad | -26.0+-0.3 |
Position
Right Ascension : 14 02 31.80 | Declination : +09 41 10.0 | Galactic Longitude (l) : N/A | Galactic Latitude (b) : N/A |
Observing Log
Date of Observation | JD | Facility | Resolution | S/N | Exposure Time | Vrad |
2006-06-12 | N/A | MCDONALD | 120000 | 430-1000 | 30min | -26.0+-0.3 |
Non-LTE line formation for heavy elements in four very metal-poor stars
Stellar Parameters
Teff : 4600 | log g : 1.50+-0.2 | vturb : 1.9 |
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 | -2.51+-0.04 | ... | ... | -2.42+-0.04 | 0.11+-0.04 | 3.82+-0.04 | Na |
Mg | N/A | -2.39+-0.10 | ... | ... | -2.41+-0.10 | 0.12+-0.10 | 5.19+-0.10 | Mg |
Al | N/A | -3.13 | ... | ... | -3.11 | -0.58 | 3.34 | Al |
K | N/A | -2.25+-0.02 | ... | ... | -2.16+-0.02 | 0.37+-0.02 | 2.87+-0.02 | K |
Ca I | N/A | -2.52+-0.10 | ... | ... | -2.50+-0.10 | 0.03+-0.10 | 3.84+-0.10 | Ca I |
Fe | N/A | -2.53+-0.02 | ... | ... | -2.53+-0.02 | ... | 4.97+-0.02 | Fe |
Sr | N/A | -2.85 | ... | ... | -2.75 | -0.22 | 0.12 | Sr |
Ba | N/A | -3.57 | ... | ... | -3.62 | -1.09 | -1.44 | Ba |
Eu | N/A | -3.16 | ... | ... | -3.17 | -0.64 | -2.65 | Eu |
Position
Right Ascension : 14 02 31.80 | Declination : +09 41 10.0 | Galactic Longitude (l) : N/A | Galactic Latitude (b) : N/A |
Observing Log
Date of Observation | JD | Facility | Resolution | S/N | Exposure Time | Vrad |
2002-02-02 | N/A | SUBARUHDS | 90000 | >200 | N/A | N/A |
| N/A | VLT | 80000 | >200 | N/A | N/A |
The r-Process in the Early Galaxy
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 | -2.75 | ... | ... | -2.58 | ... | 4.92 | Fe |
Sr II | N/A | ... | ... | -0.24+-0.30 | -3.11+-0.30 | -0.53+-0.30 | -0.24+-0.30 | Sr II |
Y II | N/A | ... | ... | -0.80+-0.10 | -3.01+-0.10 | -0.43+-0.10 | -0.80+-0.10 | Y II |
Zr II | N/A | ... | ... | -0.14+-0.08 | -2.72+-0.08 | -0.14+-0.08 | -0.14+-0.08 | Zr II |
Pd I | N/A | ... | ... | <-0.60 | <-2.17 | <0.41 | <-0.60 | Pd I |
Ba II | N/A | ... | ... | -1.80+-0.11 | -3.98+-0.11 | -1.40+-0.11 | -1.80+-0.11 | Ba II |
Position
Right Ascension : 14 02 31.80 | Declination : +09 41 10.0 | Galactic Longitude (l) : N/A | Galactic Latitude (b) : N/A |
Observing Log
Date of Observation | JD | Facility | Resolution | S/N | Exposure Time | Vrad |
1997-05-12 | N/A | KECKHIRES | 45000 | 500 | 600 | N/A |
1997-06-20 | N/A | KECKHIRES | 45000 | | 600 | N/A |
1998-06-09 | N/A | LICKHAMILTON | 60000 | 95 | 120 | N/A |
Th Ages for Metal-poor Stars
Stellar Parameters
Teff : 4450 | log g : 0.50 | vturb : 2.30 |
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 I | 161 | -2.75+-0.15 | ... | ... | -2.58+-0.15 | ... | 4.92+-0.15 | Fe I |
Fe II | 21 | -2.77+-0.08 | ... | ... | -2.60+-0.08 | ... | 4.90+-0.08 | Fe II |
Ba II | 4 | ... | -1.17+-0.11 | ... | -3.97+-0.11 | -1.39+-0.11 | -1.79+-0.11 | Ba II |
La II | 1 | ... | -0.90+-0.11 | ... | -3.53+-0.11 | -0.95+-0.11 | -2.43+-0.11 | La II |
Pr II | N/A | ... | <0.50 | ... | <-2.26 | <0.32 | <-1.54 | Pr II |
Nd II | 1 | ... | -0.61+-0.20 | ... | -3.28+-0.20 | -0.70+-0.20 | -1.86+-0.20 | Nd II |
Eu II | 1 | ... | -0.60+-0.21 | ... | -3.36+-0.21 | -0.78+-0.21 | -2.84+-0.21 | Eu II |
Tb II | N/A | ... | <0.62 | ... | <-2.12 | <0.46 | <-1.80 | Tb II |
Ho II | N/A | ... | <0.60 | ... | <-2.12 | <0.46 | <-1.65 | Ho II |
Er II | 1 | ... | -0.60+-0.10 | ... | -3.34+-0.10 | -0.76+-0.10 | -2.42+-0.10 | Er II |
Tm II | N/A | ... | <0.30 | ... | <-2.44 | <0.14 | <-2.32 | Tm II |
Yb II | 1 | ... | -1.10+-0.20 | ... | -3.82+-0.20 | -1.24+-0.20 | -2.90+-0.20 | Yb II |
Hf II | N/A | ... | <1.00 | ... | <-1.73 | <0.85 | <-1.02 | Hf II |
Os I | N/A | ... | <0.90 | ... | <-1.80 | <0.78 | <-0.40 | Os I |
Th II | N/A | ... | <-0.30 | ... | <-3.03 | <-0.45 | <-2.97 | Th II |
Isotopic Ratio
Position
Right Ascension : 14 02 31.80 | Declination : +09 41 10.0 | Galactic Longitude (l) : N/A | Galactic Latitude (b) : N/A |
Observing Log
Date of Observation | JD | Facility | Resolution | S/N | Exposure Time | Vrad |
1997-05-12 | N/A | KECKHIRES | 45000 | 500 | 600 | N/A |
1997-06-20 | N/A | KECKHIRES | 45000 | | 600 | N/A |
1998-06-09 | N/A | LICKHAMILTON | 60000 | 95 | 120 | N/A |
The End of Nucleosynthesis: Production of Lead and Thorium in the Early Galaxy
Stellar Parameters
Teff : 4570 | log g : 1.35 | vturb : 2.90 |
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 | -2.72 | ... | ... | -2.72 | ... | 4.78 | Fe |
La II | N/A | ... | ... | -2.40+-0.13 | -3.50+-0.13 | -0.78+-0.13 | -2.40+-0.13 | La II |
Eu II | N/A | ... | ... | -2.75+-0.11 | -3.27+-0.11 | -0.55+-0.11 | -2.75+-0.11 | Eu II |
Er II | N/A | ... | ... | -2.30+-0.21 | -3.22+-0.21 | -0.50+-0.21 | -2.30+-0.21 | Er II |
Hf II | N/A | ... | ... | <-1.89 | <-2.60 | <0.12 | <-1.89 | Hf II |
Ir I | N/A | ... | ... | <1.16 | <-0.22 | <2.50 | <1.16 | Ir I |
Pb I | N/A | ... | ... | <-0.42 | <-2.46 | <0.26 | <-0.42 | Pb I |
Th II | N/A | ... | ... | <-2.43 | <-2.49 | <0.23 | <-2.43 | Th II |
Isotopic Ratio
Position
Right Ascension : 14 02 31.80 | Declination : +09 41 10.0 | 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 | HST | 30000 | 50 | N/A | N/A |
| N/A | KECKHIRES | 45000 | 30-200 | N/A | N/A |
Evolution of the barium abundance in the early Galaxy from a NLTE analysis of the Ba lines in a homogeneous sample of EMP stars
Stellar Parameters
Teff : 4600 | log g : 1.1 | vturb : 2.0 |
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 | -2.82 | ... | ... | -2.82 | ... | 4.68 | Fe |
Ba | 3 | ... | ... | -1.59 | -3.77 | -0.95 | -1.59 | Ba |
Position
Right Ascension : 14 02 31.80 | Declination : +09 41 10.0 | 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 | VLT | 45000 | 130 | N/A | N/A |
Non-LTE abundances of Mg and K in extremely metal-poor stars and the evolution of [O/Mg], [Na/Mg], [Al/Mg], and [K/Mg] in the Milky Way
Stellar Parameters
Teff : 4600 | log g : 1.1 | vturb : 2.0 |
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 | ... | ... | 5.29 | -2.31 | 0.51 | 5.29 | Mg |
K | N/A | ... | ... | 2.78 | -2.25 | 0.57 | 2.78 | K |
Fe | N/A | -2.82 | ... | ... | -2.82 | ... | 4.68 | Fe |
Position
Right Ascension : 14 02 31.80 | Declination : +09 41 10.0 | 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 | VLT | 45000 | 120 | N/A | N/A |
NLTE analysis of Co i /Co ii lines in spectra of cool stars with new laboratory hyperfine splitting constants
Stellar Parameters
Teff : 4600+-120 | log g : 1.50+-0.20 | vturb : 1.9 |
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 | -2.51 | ... | ... | -2.51 | ... | 4.99 | Fe |
Co | 3 | ... | -0.07+-0.06 | ... | -2.58+-0.06 | -0.07+-0.06 | 2.41+-0.06 | Co |
Position
Right Ascension : 14 02 31.80 | Declination : +09 41 10.0 | 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 | VLT | N/A | N/A | 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 | -2.77 | ... | ... | -2.77 | ... | 4.73 | Fe |
Zn I | N/A | ... | ... | 1.97 | -2.59 | 0.18 | 1.97 | Zn I |
Y II | N/A | ... | ... | -0.92 | -3.13 | -0.36 | -0.92 | Y II |
Pb I | N/A | ... | ... | <-0.42 | <-2.46 | <0.31 | <-0.42 | Pb I |
Position
Right Ascension : 14 02 31.80 | Declination : +09 41 10.0 | 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 | MCDONALD | 60000 | 100 | N/A | N/A |
Exploring the [S/Fe] Behavior of Metal-Poor Stars with the Si 1.046 um Lines
Stellar Parameters
Teff : 4572 | log g : 1.36 | vturb : 2.90 |
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 | ... | ... | 5.29 | -1.83 | 0.78 | 5.29 | S I |
Fe | N/A | -2.61 | ... | ... | -2.61 | ... | 4.89 | Fe |
Position
Right Ascension : 14 02 31.80 | Declination : +09 41 10.0 | Galactic Longitude (l) : N/A | Galactic Latitude (b) : N/A |
Observing Log
Date of Observation | JD | Facility | Resolution | S/N | Exposure Time | Vrad |
2009-07-29 | N/A | SUBARUIRCS | 20000 | 100-200 | N/A | N/A |
First stars. XIV. Sulfur abundances in extremely metal-poor stars
Stellar Parameters
Teff : 4600 | log g : 1.1 | vturb : 2.0 |
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 | 2 | ... | ... | 4.87+-0.10 | -2.25+-0.10 | 0.57+-0.10 | 4.87+-0.10 | S I |
Fe | N/A | -2.82 | ... | ... | -2.82 | ... | 4.68 | Fe |
Position
Right Ascension : 14 02 31.80 | Declination : +09 41 10.0 | 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 | VLT | 43000 | 180 | N/A | N/A |
The Chemical Abundances of Stars in the Halo (CASH) Project. II. A Sample of 14 Extremely Metal-poor Stars
Stellar Parameters
Teff : 4450 | log g : 0.50 | vturb : 2.30 |
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 | ... | ... | <0.87+-0.15 | <-2.39+-0.15 | <0.57+-0.15 | <0.87+-0.15 | Li I |
C | N/A | ... | -0.22+-0.20 | 5.25+-0.20 | -3.18+-0.20 | -0.22+-0.20 | 5.25+-0.20 | C |
Mg I | 4 | ... | 0.41+-0.13 | 5.05+-0.13 | -2.55+-0.13 | 0.41+-0.13 | 5.05+-0.13 | Mg I |
Ca I | 20 | ... | 0.36+-0.11 | 3.74+-0.11 | -2.60+-0.11 | 0.36+-0.11 | 3.74+-0.11 | Ca I |
Sc II | 11 | ... | 0.07+-0.29 | 0.26+-0.29 | -2.89+-0.29 | 0.07+-0.29 | 0.26+-0.29 | Sc II |
Ti I | 20 | ... | 0.13+-0.11 | 2.12+-0.11 | -2.83+-0.11 | 0.13+-0.11 | 2.12+-0.11 | Ti I |
Ti II | 43 | ... | 0.25+-0.15 | 2.24+-0.15 | -2.71+-0.15 | 0.25+-0.15 | 2.24+-0.15 | Ti II |
Cr I | 15 | ... | -0.23+-0.14 | 2.45+-0.14 | -3.19+-0.14 | -0.23+-0.14 | 2.45+-0.14 | Cr I |
Cr II | 2 | ... | 0.25+-0.21 | 2.75+-0.21 | -2.89+-0.21 | 0.07+-0.21 | 2.75+-0.21 | Cr II |
Mn I | 4 | ... | -0.47+-0.18 | 2.00+-0.18 | -3.43+-0.18 | -0.47+-0.18 | 2.00+-0.18 | Mn I |
Fe | N/A | -2.96 | ... | ... | -2.96 | ... | 4.54 | Fe |
Co I | 1 | ... | 0.17+-0.00 | 2.2+-0.00 | -2.79+-0.00 | 0.17+-0.00 | 2.2+-0.00 | Co I |
Ni I | 7 | ... | 0.17+-0.14 | 3.43+-0.14 | -2.79+-0.14 | 0.17+-0.14 | 3.43+-0.14 | Ni I |
Zn I | 1 | ... | 0.24+-0.15 | 1.84+-0.15 | -2.72+-0.15 | 0.24+-0.15 | 1.84+-0.15 | Zn I |
Sr II | 2 | ... | 0.08+-0.15 | -0.01+-0.15 | -2.88+-0.15 | 0.08+-0.15 | -0.01+-0.15 | Sr II |
Y II | 1 | ... | -0.37+-0.15 | -1.12+-0.15 | -3.33+-0.15 | -0.37+-0.15 | -1.12+-0.15 | Y II |
Zr II | ... | <-0.50+-0.15 | <-0.88+-0.15 | <-3.46+-0.15 | <-0.50+-0.15 | <-0.88+-0.15 | Zr II |
Ba II | 3 | ... | -1.04+-0.15 | -1.82+-0.15 | -4.00+-0.15 | -1.04+-0.15 | -1.82+-0.15 | Ba II |
La II | ... | <1.51+-0.15 | <-0.35+-0.15 | <-1.45+-0.15 | <1.51+-0.15 | <-0.35+-0.15 | La II |
Eu II | ... | <0.73+-0.15 | <-1.71+-0.15 | <-2.23+-0.15 | <0.73+-0.15 | <-1.71+-0.15 | Eu II |
Position
Right Ascension : 14 02 31.80 | Declination : +09 41 10.0 | Galactic Longitude (l) : N/A | Galactic Latitude (b) : N/A |
Observing Log
Date of Observation | JD | Facility | Resolution | S/N | Exposure Time | Vrad |
2009-03-01 | N/A | HRSHET | 15000 | 300 | 30 | -25.4 |
2009-07-26 | N/A | MIKELCO | 35000 | 35 | 5 | -25.7 |
Silver and palladium help unveil the nature of a second r-process
Stellar Parameters
Teff : 4560+-100 | log g : 0.90+-0.25 | vturb : 1.8+-0.15 |
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 | -2.81+-0.15 | ... | ... | -2.81+-0.15 | ... | 4.69+-0.15 | Fe |
Sr | N/A | ... | 0.04+-0.13 | ... | -2.77+-0.13 | 0.04+-0.13 | 0.10+-0.13 | Sr |
Y | N/A | ... | -0.10+-0.16 | ... | -2.91+-0.16 | -0.10+-0.16 | -0.70+-0.16 | Y |
Zr | N/A | ... | 0.07+-0.18 | ... | -2.74+-0.18 | 0.07+-0.18 | -0.16+-0.18 | Zr |
Pd | N/A | ... | 0.12+-0.20 | ... | -2.69+-0.20 | 0.12+-0.20 | -1.12+-0.20 | Pd |
Ag | N/A | ... | 0.10+-0.25 | ... | -2.97+-0.25 | -0.16+-0.25 | -1.77+-0.25 | Ag |
Ba | N/A | ... | -0.85+-0.14 | ... | -3.66+-0.14 | -0.85+-0.14 | -1.48+-0.14 | Ba |
Eu | N/A | ... | -0.51+-0.16 | ... | -3.32+-0.16 | -0.51+-0.16 | -2.80+-0.16 | Eu |
Position
Right Ascension : 14 02 31.80 | Declination : +09 41 10.0 | 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 | VLT | 40000 | >100 | N/A | N/A |
NEW HUBBLE SPACE TELESCOPE OBSERVATIONS OF HEAVY ELEMENTS IN FOUR METAL-POOR STARS
Stellar Parameters
Teff : 4450 | log g : 1.37 | 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 |
Fe I | 211 | -3.06+-0.10 | +0.00+-0.16 | +4.44+-0.16 | -3.06+-0.10 | +0.00+-0.16 | +4.44+-0.16 | Fe I |
Fe II | 20 | -2.61+-0.12 | +0.00+-0.20 | +4.89+-0.20 | -2.61+-0.12 | +0.00+-0.20 | +4.89+-0.20 | Fe II |
Cu I | 1 | ... | -1.03+-0.22 | +0.10+-0.22 | -4.09+-0.22 | -1.03+-0.22 | +0.10+-0.22 | Cu I |
Zn I | 4 | ... | +0.49+-0.21 | +1.99+-0.21 | -2.57+-0.21 | 0.49+-0.21 | +1.99+-0.21 | Zn I |
Ge I | 3 | ... | -1.47+-0.21 | -0.88+-0.21 | -4.53+-0.21 | -1.47+-0.21 | -0.88+-0.21 | Ge I |
Rb I | 1 | ... | <+1.74 | <+1.20 | <-1.16 | <1.90 | <+1.20 | Rb I |
Sr II | 3 | ... | -0.28+-0.19 | -0.02+-0.19 | -2.89+-0.19 | 0.17+-0.19 | -0.02+-0.19 | Sr II |
Y II | 10 | ... | -0.55+-0.21 | -0.95+-0.21 | -3.16+-0.21 | -0.10+-0.21 | -0.95+-0.21 | Y II |
Zr II | 26 | ... | -0.13+-0.22 | -0.16+-0.22 | -2.74+-0.22 | 0.32+-0.22 | -0.16+-0.22 | Zr II |
Nb II | 3 | ... | -0.37+-0.22 | -1.52+-0.22 | -2.98+-0.22 | 0.08+-0.22 | -1.52+-0.22 | Nb II |
Mo I | 1 | ... | -0.04+-0.31 | -1.22+-0.31 | -3.10+-0.31 | -0.04+-0.31 | -1.22+-0.31 | Mo I |
Mo II | 1 | ... | <+0.08 | <-0.65 | <-2.53 | <0.53 | <-0.65 | Mo II |
Ru I | 3 | ... | +0.27+-0.27 | -1.04+-0.27 | -2.79+-0.27 | 0.27+-0.27 | -1.04+-0.27 | Ru I |
Rh I | 1 | ... | +0.27+-0.31 | -1.73+-0.31 | -2.64+-0.31 | 0.42+-0.31 | -1.73+-0.31 | Rh I |
Pd I | 1 | ... | -0.37+-0.32 | -1.78+-0.32 | -3.35+-0.32 | -0.29+-0.32 | -1.78+-0.32 | Pd I |
Ag I | 2 | ... | <+0.23 | <-1.63 | <-2.83 | <0.23 | <-1.63 | Ag I |
Cd I | 1 | ... | <-1.50 | <-2.85 | <-4.56 | <-1.50 | <-2.85 | Cd I |
Sn I | 1 | ... | <+1.37 | <+0.38 | <-1.69 | <1.37 | <+0.38 | Sn I |
Ba II | 2 | ... | -1.35+-0.22 | -1.78+-0.22 | -3.96+-0.22 | -0.90+-0.22 | -1.78+-0.22 | Ba II |
La II | 3 | ... | -0.97+-0.24 | -2.48+-0.24 | -3.58+-0.24 | -0.52+-0.24 | -2.48+-0.24 | La II |
Ce II | 6 | ... | -0.91+-0.18 | -1.94+-0.18 | -3.52+-0.18 | -0.46+-0.18 | -1.94+-0.18 | Ce II |
Pr II | 1 | ... | <-0.26 | <-2.15 | <-2.87 | <0.19 | <-2.15 | Pr II |
Nd II | 3 | ... | -0.87+-0.19 | -2.06+-0.19 | -3.48+-0.19 | -0.42+-0.19 | -2.06+-0.19 | Nd II |
Sm II | 3 | ... | -0.66+-0.20 | -2.31+-0.20 | -3.27+-0.20 | -0.21+-0.20 | -2.31+-0.20 | Sm II |
Eu II | 3 | ... | -0.68+-0.19 | -2.77+-0.19 | -3.29+-0.19 | -0.23+-0.19 | -2.77+-0.19 | Eu II |
Gd II | 1 | ... | -0.76+-0.24 | -2.30+-0.24 | -3.37+-0.24 | -0.31+-0.24 | -2.30+-0.24 | Gd II |
Dy II | 1 | ... | -0.88+-0.24 | -2.39+-0.24 | -3.49+-0.24 | -0.43+-0.24 | -2.39+-0.24 | Dy II |
Ho II | 1 | ... | <-0.30 | <-2.43 | <-2.90 | <0.16 | <-2.43 | Ho II |
Yb II | 1 | ... | -1.00+-0.24 | -2.69+-0.24 | -3.61+-0.24 | -0.55+-0.24 | -2.69+-0.24 | Yb II |
Lu II | 1 | ... | -0.38+-0.33 | -2.89+-0.33 | -2.98+-0.33 | 0.08+-0.33 | -2.89+-0.33 | Lu II |
Hf II | 1 | ... | -0.71+-0.41 | -2.47+-0.41 | -3.18+-0.41 | -0.12+-0.41 | -2.47+-0.41 | Hf II |
Os I | 1 | ... | <+0.41 | <-1.25 | <-2.65 | <0.41 | <-1.25 | Os I |
Ir I | 3 | ... | <+0.33 | <-1.35 | <-2.73 | <0.33 | <-1.35 | Ir I |
Pt I | 2 | ... | <-0.71 | <-2.15 | <-3.77 | <-0.71 | <-2.15 | Pt I |
Pb I | 3 | ... | <-0.43 | <-1.45 | <-3.49 | <-0.43 | <-1.45 | Pb I |
Position
Right Ascension : 14 02 31.80 | Declination : +09 41 10.0 | Galactic Longitude (l) : N/A | Galactic Latitude (b) : N/A |
Observing Log
Date of Observation | JD | Facility | Resolution | S/N | Exposure Time | Vrad |
1999-07-29 | N/A | HST | 30000 | 60-400 | 10400 | N/A |
2011-07-24 | N/A | HST | 30000 | 60-400 | 9900 | N/A |
2011-08-06 | N/A | HST | 30000 | 60-400 | 9900 | N/A |
2009-02-19 | N/A | MIKELCO | 41000 | 220-640 | 30 | N/A |
1999-04-21 | N/A | KECKHIRES | 45000 | 160-540 | 600 | N/A |
NLTE determination of the calcium abundance and 3D corrections in extremely metal-poor stars
Stellar Parameters
Teff : 4600 | log g : 1.1 | vturb : 2.0 |
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 |
Ca | N/A | -2.39 | 0.42 | ... | -2.37 | 0.45 | 3.97 | Ca |
Fe | N/A | -2.82 | ... | ... | -2.82 | ... | 4.68 | Fe |
Position
Right Ascension : 14 02 31.80 | Declination : +09 41 10.0 | 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 | VLT | 45000 | 150 | N/A | N/A |
A SEARCH FOR STARS OF VERY LOW METAL ABUNDANCE. VI. DETAILED ABUNDANCES OF 313 METAL-POOR STARS
Stellar Parameters
Teff : 4500+-34 | log g : 0.55+-0.15 | vturb : 1.95+-0.06 |
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 | 1 | ... | ... | <-0.15 | <-3.41 | <-0.44 | <-0.15 | Li I |
CH | 1 | ... | -0.45+-0.25 | 5.06 | -3.37 | -0.40+-0.25 | 5.06 | CH |
NH | 1 | ... | 0.60+-0.36 | 5.51 | -2.32 | 0.65+-0.36 | 5.51 | NH |
O I | 3 | ... | <0.63 | <6.35 | <-2.34 | <0.63 | <6.35 | O I |
Mg I | 6 | ... | 0.51+-0.17 | 5.14 | -2.46 | 0.51+-0.17 | 5.14 | Mg I |
Al I | 1 | ... | -0.44+-0.26 | 3.04 | -3.41 | -0.44+-0.26 | 3.04 | Al I |
Si I | 1 | ... | 0.62+-0.23 | 5.16 | -2.35 | 0.62+-0.23 | 5.16 | Si I |
K I | 1 | ... | 0.30+-0.18 | 2.36 | -2.67 | 0.30+-0.18 | 2.36 | K I |
Ca I | 11 | ... | 0.35+-0.17 | 3.73 | -2.61 | 0.36+-0.17 | 3.73 | Ca I |
Sc II | 6 | ... | -0.07+-0.14 | 0.15 | -3.00 | -0.03+-0.14 | 0.15 | Sc II |
Ti I | 19 | ... | 0.06+-0.14 | 2.04 | -2.91 | 0.06+-0.14 | 2.04 | Ti I |
Ti II | 27 | ... | 0.19+-0.15 | 2.21 | -2.74 | 0.23+-0.15 | 2.21 | Ti II |
V I | 1 | ... | -0.17+-0.17 | 0.79 | -3.14 | -0.17+-0.17 | 0.79 | V I |
V II | 2 | ... | 0.04+-0.23 | 1.04 | -2.89 | 0.08+-0.23 | 1.04 | V II |
Cr I | 11 | ... | -0.31+-0.14 | 2.37 | -3.27 | -0.30+-0.14 | 2.37 | Cr I |
Cr II | 3 | ... | 0.08+-0.16 | 2.79 | -2.85 | 0.12+-0.16 | 2.79 | Cr II |
Mn I | 4 | ... | -0.38+-0.14 | 2.09 | -3.34 | -0.37+-0.14 | 2.09 | Mn I |
Fe I | 108 | -2.97+-0.15 | ... | 4.53 | -2.97+-0.15 | ... | 4.53 | Fe I |
Fe II | 12 | -2.93+-0.15 | ... | 4.57 | -2.93+-0.15 | ... | 4.57 | Fe II |
Co I | 3 | ... | -0.17+-0.24 | 1.85 | -3.14 | -0.17+-0.24 | 1.85 | Co I |
Ni I | 11 | ... | 0.16+-0.18 | 3.41 | -2.81 | 0.16+-0.18 | 3.41 | Ni I |
Cu I | 1 | ... | <-0.94 | <0.28 | <-3.91 | <-0.94 | <0.28 | Cu I |
Zn I | 2 | ... | 0.29+-0.14 | 1.88 | -2.68 | 0.29+-0.14 | 1.88 | Zn I |
Rb I | 1 | ... | <1.78 | <1.33 | <-1.03 | <1.94 | <1.33 | Rb I |
Sr II | 2 | ... | -0.19+-0.18 | -0.25 | -3.12 | -0.15+-0.18 | -0.25 | Sr II |
Y II | 5 | ... | -0.62+-0.15 | -1.34 | -3.55 | -0.58+-0.15 | -1.34 | Y II |
Zr II | 3 | ... | -0.20+-0.15 | -0.55 | -3.13 | -0.16+-0.15 | -0.55 | Zr II |
Nb II | 1 | ... | <0.95 | <-0.52 | <-1.98 | <0.99 | <-0.52 | Nb II |
Tc I | 1 | ... | ... | <-0.54 | <-0.54 | <2.43 | <-0.54 | Tc I |
Sn I | 1 | ... | <1.31 | <0.41 | <-1.66 | <1.31 | <0.41 | Sn I |
Ba II | 3 | ... | -1.17+-0.15 | -1.92 | -4.10 | -1.13+-0.15 | -1.92 | Ba II |
La II | 2 | ... | -1.03+-0.22 | -2.86 | -3.96 | -0.99+-0.22 | -2.86 | La II |
Ce II | 1 | ... | -0.93+-0.29 | -2.28 | -3.86 | -0.89+-0.29 | -2.28 | Ce II |
Pr II | 1 | ... | <0.00 | <-2.21 | <-2.93 | <0.04 | <-2.21 | Pr II |
Nd II | 1 | ... | -1.02+-0.24 | -2.53 | -3.95 | -0.98+-0.24 | -2.53 | Nd II |
Sm II | 2 | ... | <-0.53 | <-2.50 | <-3.46 | <-0.49 | <-2.50 | Sm II |
Eu II | 2 | ... | -0.84+-0.21 | -3.25 | -3.77 | -0.80+-0.21 | -3.25 | Eu II |
Gd II | 2 | ... | <0.08 | <-1.78 | <-2.85 | <0.12 | <-1.78 | Gd II |
Tb II | 3 | ... | <0.00 | <-2.63 | <-2.95 | <0.02 | <-2.63 | Tb II |
Dy II | 1 | ... | <-0.70 | <-2.53 | <-3.63 | <-0.66 | <-2.53 | Dy II |
Er II | 2 | ... | <-0.57 | <-2.58 | <-3.50 | <-0.53 | <-2.58 | Er II |
Tm II | 2 | ... | <0.14 | <-2.69 | <-2.81 | <0.16 | <-2.69 | Tm II |
Yb II | 1 | ... | -1.37+-0.42 | -3.38 | -4.30 | -1.33+-0.42 | -3.38 | Yb II |
Hf II | 2 | ... | <0.36 | <-1.72 | <-2.43 | <0.54 | <-1.72 | Hf II |
Ir I | 1 | ... | <0.43 | <-1.16 | <-2.54 | <0.43 | <-1.16 | Ir I |
Pb I | 1 | ... | <0.97 | <0.04 | <-2.00 | <0.97 | <0.04 | Pb I |
Th II | 2 | ... | <0.31 | <-2.56 | <-2.62 | <0.35 | <-2.56 | Th II |
Binary Parameters
Binarity | Negative |
Vrad | -26.1 |
Position
Right Ascension : 14 02 31.80 | Declination : +09 41 10.0 | Galactic Longitude (l) : N/A | Galactic Latitude (b) : N/A |
Observing Log
Date of Observation | JD | Facility | Resolution | S/N | Exposure Time | Vrad |
2008-05-26-06:53 | 2454612.791 | HRSHET | 30000 | 85-540 | 120 | -26.1 |
2009-02-18-12:40 | 2454881.031 | MCDONALD | 33000 | 85-540 | 60 | -26.5 |
2009-02-19-09:53 | 2454881.915 | MIKELCO | 41000 | 145-505 | 26 | -25.7 |
Three-dimensional hydrodynamical CO5BOLD model atmospheres of red giant stars. V. Oxygen abundance in the metal-poor giant HD 122563 from OH UV lines
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 |
OH | N/A | ... | 0.25+-0.16 | 6.41+-0.16 | -2.28+-0.16 | 0.32+-0.16 | 6.41+-0.16 | OH |
Fe | N/A | -2.60 | ... | ... | -2.60 | ... | 4.90 | Fe |
Position
Right Ascension : 14 02 31.80 | Declination : +09 41 10.0 | 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 | VLT | 60000 | 55-195 | N/A | N/A |
The R-Process Alliance: First Release from the Northern Search for r-process-enhanced Metal-poor Stars in the Galactic Halo
Stellar Parameters
Teff : 4374 | log g : 0.46 | vturb : 2.06 |
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 | 5 | ... | 0.48+-0.02 | ... | -2.48+-0.02 | 0.48+-0.02 | 5.12+-0.02 | Mg |
K | 1 | ... | 0.34+-0.10 | ... | -2.62+-0.10 | 0.34+-0.10 | 2.41+-0.10 | K |
Ca | 20 | ... | 0.30+-0.01 | ... | -2.66+-0.01 | 0.30+-0.01 | 3.68+-0.01 | Ca |
Sc | 9 | ... | 0.14+-0.02 | ... | -2.82+-0.02 | 0.14+-0.02 | 0.33+-0.02 | Sc |
Ti I | 20 | ... | 0.15 | ... | -2.81 | 0.15 | 2.14 | Ti I |
Ti II | 32 | ... | 0.21+-0.01 | ... | -2.75+-0.01 | 0.21+-0.01 | 2.20+-0.01 | Ti II |
V | 2 | ... | -0.17+-0.01 | ... | -3.13+-0.01 | -0.17+-0.01 | 0.80+-0.01 | V |
Cr | 2 | ... | 0.13+-0.06 | ... | -2.83+-0.06 | 0.13+-0.06 | 2.81+-0.06 | Cr |
Mn | 3 | ... | -0.36+-0.01 | ... | -3.32+-0.01 | -0.36+-0.01 | 2.11+-0.01 | Mn |
Fe | N/A | -2.96 | ... | ... | -2.96 | ... | 4.54 | Fe |
Co | 2 | ... | 0.33+-0.06 | ... | -2.63+-0.06 | 0.33+-0.06 | 2.36+-0.06 | Co |
Ni | 13 | ... | 0.08+-0.01 | ... | -2.88+-0.01 | 0.08+-0.01 | 3.34+-0.01 | Ni |
Zn | 2 | ... | 0.15+-0.05 | ... | -2.81+-0.05 | 0.15+-0.05 | 1.75+-0.05 | Zn |
Sr | 1 | ... | -0.13+-0.10 | ... | -3.09+-0.10 | -0.13+-0.10 | -0.22+-0.10 | Sr |
Y | 4 | ... | -0.36+-0.03 | ... | -3.32+-0.03 | -0.36+-0.03 | -1.11+-0.03 | Y |
Ba | 3 | ... | -0.92+-0.03 | ... | -3.88+-0.03 | -0.92+-0.03 | -1.70+-0.03 | Ba |
Eu | 2 | ... | -0.32+-0.05 | ... | -3.28+-0.05 | -0.32+-0.05 | -2.76+-0.05 | Eu |
Binary Parameters
Position
Right Ascension : 14 02 31.92 | Declination : +09 41 09.6 | Galactic Longitude (l) : N/A | Galactic Latitude (b) : N/A |
Observing Log
Date of Observation | JD | Facility | Resolution | S/N | Exposure Time | Vrad |
2016-02-17 | N/A | APO | 31500 | 200-500 | 600 | -23.3+-0.5 |
The Pristine survey – IX. CFHT ESPaDOnS spectroscopic analysis of 115 bright metal-poor candidate stars
Stellar Parameters
Teff : 4625+-50 | log g : 1.6+-0.1 | vturb : 2.0 |
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 | 2 | ... | 0.21+-0.11 | ... | -2.55+-0.11 | 0.21+-0.11 | 3.69+-0.11 | Na |
Mg | 3 | ... | 0.18+-0.09 | ... | -2.58+-0.09 | 0.18+-0.09 | 5.02+-0.09 | Mg |
Ca | 8 | ... | 0.32+-0.14 | ... | -2.44+-0.14 | 0.32+-0.14 | 3.90+-0.14 | Ca |
Sc | 2 | ... | 0.19+-0.11 | ... | -2.57+-0.11 | 0.19+-0.11 | 0.58+-0.11 | Sc |
Ti I | 9 | ... | 0.07+-0.05 | ... | -2.69+-0.05 | 0.07+-0.05 | 2.26+-0.05 | Ti I |
Ti II | 9 | ... | 0.46+-0.08 | ... | -2.30+-0.08 | 0.46+-0.08 | 2.65+-0.08 | Ti II |
Cr | 3 | ... | -0.39+-0.08 | ... | -3.15+-0.08 | -0.39+-0.08 | 2.49+-0.08 | Cr |
Fe | N/A | -2.76+-0.01 | ... | ... | -2.76+-0.01 | ... | 4.74+-0.01 | Fe |
Fe I | 98 | ... | ... | 4.73+-0.15 | -2.77+-0.15 | ... | 4.73+-0.15 | Fe I |
Fe II | 5 | ... | ... | 4.86+-0.16 | -2.64+-0.16 | ... | 4.86+-0.16 | Fe II |
Ni | 5 | ... | +0.05+-0.10 | ... | -2.71+-0.10 | 0.05+-0.10 | 3.51+-0.10 | Ni |
Y | 2 | ... | -0.15+-0.11 | ... | -2.91+-0.11 | -0.15+-0.11 | -0.70+-0.11 | Y |
Ba | 3 | ... | -0.77+-0.08 | ... | -3.53+-0.08 | -0.77+-0.08 | -1.35+-0.08 | Ba |
Position
Right Ascension : 14 02 31.84 | Declination : +09 41 09.94 | 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 | ESPADONSCFHT | 68000 | N/A | N/A | N/A |
The Pristine survey - XII. Gemini-GRACES chemo-dynamical study of newly discovered extremely metal-poor stars in the Galaxy
Stellar Parameters
Teff : 4749+-89 | log g : 1.12+-0.11 |
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 | ... | ... | <-0.18 | <-3.44 | <-0.56 | <-0.18 | Li |
Na I | 2 | ... | 0.43+-0.11 | ... | -2.45+-0.11 | 0.43+-0.11 | 3.79+-0.11 | Na I |
Mg I | 4 | ... | 0.62+-0.09 | ... | -2.26+-0.09 | 0.62+-0.09 | 5.34+-0.09 | Mg I |
Ca I | 14 | ... | 0.31+-0.08 | ... | -2.57+-0.08 | 0.31+-0.08 | 3.77+-0.08 | Ca I |
Ti I | 1 | ... | 0.15+-0.16 | ... | -2.73+-0.16 | 0.15+-0.16 | 2.22+-0.16 | Ti I |
Ti II | 10 | ... | 0.33+-0.07 | ... | -2.55+-0.07 | 0.33+-0.07 | 2.40+-0.07 | Ti II |
Cr I | 8 | ... | -0.08+-0.12 | ... | -2.96+-0.12 | -0.08+-0.12 | 2.68+-0.12 | Cr I |
Mn I | N/A | ... | <-0.25 | ... | <-3.13 | <-0.25 | <2.30 | Mn I |
Fe | 63 | -2.88+-0.07 | ... | ... | -2.88+-0.07 | ... | 4.62+-0.07 | Fe |
Fe I | 54 | -2.89+-0.10 | ... | ... | -2.89+-0.10 | ... | 4.61+-0.10 | Fe I |
Fe II | 9 | -2.87+-0.09 | ... | ... | -2.87+-0.09 | ... | 4.63+-0.09 | Fe II |
Ni I | 1 | ... | 0.00+-0.13 | ... | -2.88+-0.13 | 0.00+-0.13 | 3.34+-0.13 | Ni I |
Cu I | N/A | ... | <-0.60 | ... | <-3.48 | <-0.60 | <0.71 | Cu I |
Zn I | 1 | ... | 0.30+-0.13 | ... | -2.58+-0.13 | 0.30+-0.13 | 1.98+-0.13 | Zn I |
Y II | 4 | ... | -0.15+-0.15 | ... | -3.03+-0.15 | -0.15+-0.15 | -0.82+-0.15 | Y II |
Ba II | 2 | ... | -0.95+-0.15 | ... | -3.83+-0.15 | -0.95+-0.15 | -1.65+-0.15 | Ba II |
La II | N/A | ... | <0.45 | ... | <-2.43 | <0.45 | <-1.33 | La II |
Nd II | N/A | ... | <0.05 | ... | <-2.83 | <0.05 | <-1.41 | Nd II |
Eu II | N/A | ... | <0.60 | ... | <-2.28 | <0.60 | <-1.76 | Eu II |
Position
Right Ascension : | Declination : | Galactic Longitude (l) : N/A | Galactic Latitude (b) : N/A |
Observing Log