CS30325-094
taken from 11 paper(s):
/R.Cayrel et al.(2004)/
/M.Spite et al.(2005)/
/W.Aoki et al.(2005)/
/M.Spite et al.(2006)/
/S.M.Andrievsky et al.(2007)/
/S.M.Andrievsky et al.(2008)/
/S.M.Andrievsky et al.(2009)/
/S.M.Andrievsky et al.(2010)/
/M.Spite et al.(2011)/
/P.Francois et al.(2007)/
/M.Spite et al.(2012)/
First stars V - Abundance patterns from C to Zn and supernova yields in the early Galaxy
Stellar Parameters
Teff : 4950 | log g : 2.0 | vturb : 1.5 |
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 |
CH | N/A | -3.32 | -0.02 | 5.20 | -3.23 | 0.07 | 5.20 | CH |
[O I] | N/A | -2.58 | 0.72 | 6.19 | -2.50 | 0.80 | 6.19 | [O I] |
Na I | 2 | -3.21 | 0.09 | 3.12 | -3.12 | 0.18 | 3.12 | Na I |
Mg I | 7 | -2.92+-0.14 | 0.38+-0.14 | 4.66+-0.14 | -2.94+-0.14 | 0.36+-0.14 | 4.66+-0.14 | Mg I |
Al I | 2 | -3.88 | -0.58 | 2.59 | -3.86 | -0.56 | 2.59 | Al I |
Si I | 1 | -2.49 | 0.81 | 5.06 | -2.45 | 0.85 | 5.06 | Si I |
K I | 1 | -2.57 | 0.73 | 2.55 | -2.48 | 0.82 | 2.55 | K I |
Ca I | 17 | -2.92+-0.11 | 0.38+-0.11 | 3.44+-0.11 | -2.90+-0.11 | 0.40+-0.11 | 3.44+-0.11 | Ca I |
Sc II | 7 | -2.97+-0.09 | 0.33+-0.09 | 0.20+-0.09 | -2.95+-0.09 | 0.35+-0.09 | 0.20+-0.09 | Sc II |
Ti I | 13 | -3.03+-0.05 | 0.27+-0.05 | 1.99+-0.05 | -2.96+-0.05 | 0.34+-0.05 | 1.99+-0.05 | Ti I |
Ti II | 29 | -3.01+-0.10 | 0.29+-0.10 | 2.01+-0.10 | -2.94+-0.10 | 0.36+-0.10 | 2.01+-0.10 | Ti II |
Cr I | 7 | -3.74+-0.09 | -0.44+-0.09 | 1.93+-0.09 | -3.71+-0.09 | -0.41+-0.09 | 1.93+-0.09 | Cr I |
Mn I | 3 | -3.85+-0.05 | -0.55+-0.05 | 1.54+-0.05 | -3.89+-0.05 | -0.59+-0.05 | 1.54+-0.05 | Mn I |
Fe I | 140 | -3.30+-0.14 | 0.00+-0.14 | 4.20+-0.14 | -3.30+-0.14 | 0.00+-0.14 | 4.20+-0.14 | Fe I |
Fe II | 8 | -3.30+-0.13 | 0.01+-0.13 | 4.20+-0.13 | -3.30+-0.13 | 0.01+-0.13 | 4.20+-0.13 | Fe II |
Co I | 3 | -3.01+-0.08 | 0.29+-0.08 | 1.91+-0.08 | -3.08+-0.08 | 0.22+-0.08 | 1.91+-0.08 | Co I |
Ni I | 3 | -3.22+-0.04 | 0.08+-0.04 | 3.03+-0.04 | -3.19+-0.04 | 0.11+-0.04 | 3.03+-0.04 | Ni I |
Zn I | 1 | -3.06 | 0.24 | 1.54 | -3.02 | 0.28 | 1.54 | Zn I |
Binary Parameters
Position
Right Ascension : 14 54 39.27 | Declination : +04 21 38.1 | 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 | 110 | 7200 | N/A |
2000-08 | N/A | VLT | 47000 | N/A | N/A | N/A |
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 : 4950 | log g : 2.0 | vturb : 1.5 |
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 |
Li I | N/A | ... | ... | <-0.25 | <-3.51 | <-0.21 | <-0.25 | Li I |
C | N/A | -3.30+-0.05 | ... | ... | -3.21+-0.05 | 0.09+-0.05 | 5.22+-0.05 | C |
N | N/A | -3.12 | ... | ... | -3.03 | 0.27 | 4.80 | N |
[O I] | N/A | -2.58 | ... | ... | -2.53 | 0.77 | 6.16 | [O I] |
Fe | N/A | -3.30 | ... | ... | -3.30 | ... | 4.20 | Fe |
Position
Right Ascension : 14 54 39.27 | Declination : +04 21 38.1 | 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 |
Spectroscopic Studies of Very Metal-poor Stars with the Subaru High Dispersion Spectrograph. III. Light Neutron-Capture Elements
Stellar Parameters
Teff : 5050 | log g : 2.1 | 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 | ... | 0.5 | 5.7 | -2.73 | 0.44 | 5.7 | CH |
Mg I | 8 | ... | 0.55+-0.11 | 4.96+-0.11 | -2.64+-0.11 | 0.53+-0.11 | 4.96+-0.11 | Mg I |
Al I | 1 | ... | -0.66+-0.18 | 2.66+-0.18 | -3.79+-0.18 | -0.62+-0.18 | 2.66+-0.18 | Al I |
Si I | 2 | ... | 0.86+-0.13 | 5.25+-0.13 | -2.26+-0.13 | 0.91+-0.13 | 5.25+-0.13 | Si I |
Ca I | 9 | ... | 0.34+-0.11 | 3.52+-0.11 | -2.82+-0.11 | 0.35+-0.11 | 3.52+-0.11 | Ca I |
Sc II | 4 | ... | 0.37+-0.23 | 0.3+-0.23 | -2.85+-0.23 | 0.32+-0.23 | 0.3+-0.23 | Sc II |
Ti I | 9 | ... | 0.4+-0.12 | 2.17+-0.12 | -2.78+-0.12 | 0.39+-0.12 | 2.17+-0.12 | Ti I |
Ti II | 21 | ... | 0.44+-0.24 | 2.21+-0.24 | -2.74+-0.24 | 0.43+-0.24 | 2.21+-0.24 | Ti II |
Cr I | 5 | ... | -0.46+-0.1 | 2.06+-0.1 | -3.58+-0.1 | -0.41+-0.1 | 2.06+-0.1 | Cr I |
Mn I | 3 | ... | -1.05+-0.11 | 1.31+-0.11 | -4.12+-0.11 | -0.95+-0.11 | 1.31+-0.11 | Mn I |
Fe I | 101 | -3.17+-0.2 | ... | 4.33+-0.2 | -3.17+-0.2 | ... | 4.33+-0.2 | Fe I |
Fe II | 11 | -3.14+-0.19 | ... | 4.36+-0.19 | -3.14+-0.19 | ... | 4.36+-0.19 | Fe II |
Co I | 8 | ... | 0.52+-0.11 | 2.26+-0.11 | -2.73+-0.11 | 0.44+-0.11 | 2.26+-0.11 | Co I |
Ni I | 2 | ... | -0.11+-0.11 | 2.97+-0.11 | -3.25+-0.11 | -0.08+-0.11 | 2.97+-0.11 | Ni I |
Zn I | 1 | ... | 0.4+-0.21 | 1.9+-0.21 | -2.66+-0.21 | 0.51+-0.21 | 1.9+-0.21 | Zn I |
Sr II | 1 | ... | -2.35+-0.24 | -2.6+-0.24 | -5.47+-0.24 | -2.30+-0.24 | -2.6+-0.24 | Sr II |
Y II | N/A | ... | <0.12 | <-0.82 | <-3.03 | <0.14 | <-0.82 | Y II |
Zr II | N/A | ... | <0.13 | <-0.43 | <-3.01 | <0.16 | <-0.43 | Zr II |
Ba II | N/A | ... | <-1.76 | <-2.71 | <-4.89 | <-1.72 | <-2.71 | Ba II |
Binary Parameters
Position
Right Ascension : 14 54 39.27 | Declination : +04 21 38.1 | Galactic Longitude (l) : N/A | Galactic Latitude (b) : N/A |
Observing Log
Date of Observation | JD | Facility | Resolution | S/N | Exposure Time | Vrad |
2001-04-14 | N/A | SUBARUHDS | 50000 | 139 | 20min | -157.64+-0.25 |
First stars IX - Mixing in extremely metal-poor giants. Variation of the 12C/13C, [Na/Mg] and [Al/Mg] ratios
Stellar Parameters
Teff : 4950 | log g : 2.0 | vturb : 1.5 |
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 |
C | N/A | -3.28+-0.05 | ... | ... | -3.19+-0.05 | 0.11+-0.05 | 5.24+-0.05 | C |
N | N/A | -3.12+-0.18 | ... | ... | -3.03+-0.18 | 0.27+-0.18 | 4.80+-0.18 | N |
Fe | N/A | -3.30 | ... | ... | -3.30 | ... | 4.20 | Fe |
Isotopic Ratio
Position
Right Ascension : 14 54 39.27 | Declination : +04 21 38.1 | 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 : 4950 | log g : 2.0 | vturb : 1.5 |
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 |
Na | N/A | -3.41 | -0.11 | 2.84 | -3.40 | -0.10 | 2.84 | Na |
Fe | N/A | -3.30 | ... | ... | -3.30 | ... | 4.20 | Fe |
Position
Right Ascension : 14 54 39.27 | Declination : +04 21 38.1 | 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 |
NLTE determination of the aluminium abundance in a homogeneous sample of extremely metal-poor stars
Stellar Parameters
Teff : 4950 | log g : 2.0 | vturb : 1.5 |
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 |
Al | N/A | -3.22 | 0.08 | 3.25 | -3.20 | 0.10 | 3.25 | Al |
Fe | N/A | -3.30 | ... | ... | -3.30 | ... | 4.20 | Fe |
Position
Right Ascension : 14 54 39.27 | Declination : +04 21 38.1 | 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 |
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 : 4950 | log g : 2.0 | vturb : 1.5 |
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 | -3.30 | ... | ... | -3.30 | ... | 4.20 | Fe |
Ba | N/A | ... | ... | <-3.05 | <-5.23 | <-1.93 | <-3.05 | Ba |
Position
Right Ascension : 14 54 39.27 | Declination : +04 21 38.1 | 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 : 4950 | log g : 2.0 | vturb : 1.5 |
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 |
Mg | N/A | ... | ... | 4.81 | -2.79 | 0.51 | 4.81 | Mg |
K | N/A | ... | ... | 2.65 | -2.38 | 0.92 | 2.65 | K |
Fe | N/A | -3.30 | ... | ... | -3.30 | ... | 4.20 | Fe |
Position
Right Ascension : 14 54 39.27 | Declination : +04 21 38.1 | 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 |
First stars. XIV. Sulfur abundances in extremely metal-poor stars
Stellar Parameters
Teff : 4950 | log g : 2.0 | vturb : 1.5 |
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 |
S I | 2 | ... | ... | 4.64+-0.18 | -2.48+-0.18 | 0.82+-0.18 | 4.64+-0.18 | S I |
Fe | N/A | -3.30 | ... | ... | -3.30 | ... | 4.20 | Fe |
Position
Right Ascension : 14 54 39.27 | Declination : +04 21 38.1 | 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 |
First stars. VIII. Enrichment of the neutron-capture elements in the early Galaxy
Stellar Parameters
Teff : 4950 | log g : 2.0 | vturb : 1.5 |
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 | -3.30 | ... | ... | -3.30 | ... | 4.20 | Fe |
Sr | 2 | ... | -2.24 | ... | -5.49 | -2.19 | -2.62 | Sr |
Y | N/A | ... | <-1.54 | ... | <-4.81 | <-1.51 | <-2.60 | Y |
Zr | N/A | ... | <-1.54 | ... | <-4.82 | <-1.52 | <-2.24 | Zr |
Ba | 2 | ... | -1.88 | ... | -5.23 | -1.93 | -3.05 | Ba |
La | N/A | ... | <-0.27 | ... | <-3.50 | <-0.20 | <-2.40 | La |
Ce | 1 | ... | +0.42 | ... | -2.88 | 0.42 | -1.30 | Ce |
Pr | 1 | ... | <+0.64 | ... | <-2.67 | <0.63 | <-1.95 | Pr |
Nd | 1 | ... | 0.00 | ... | -3.22 | 0.08 | -1.80 | Nd |
Sm | N/A | ... | <0.49 | ... | <-2.76 | <0.54 | <-1.80 | Sm |
Eu | N/A | ... | <-0.11 | ... | <-3.42 | <-0.12 | <-2.90 | Eu |
Gd | N/A | ... | <+0.18 | ... | <-3.07 | <0.23 | <-2.00 | Gd |
Dy | N/A | ... | <-0.34 | ... | <-3.60 | <-0.30 | <-2.50 | Dy |
Ho | N/A | ... | <+0.34 | ... | <-3.17 | <0.13 | <-2.70 | Ho |
Er | N/A | ... | <+0.07 | ... | <-3.22 | <0.08 | <-2.30 | Er |
Position
Right Ascension : 14 54 39.27 | Declination : +04 21 38.1 | 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 | >50 | N/A | N/A |
NLTE determination of the calcium abundance and 3D corrections in extremely metal-poor stars
Stellar Parameters
Teff : 4950 | log g : 2.0 | vturb : 1.5 |
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 |
Ca | N/A | -2.75 | 0.55 | ... | -2.73 | 0.57 | 3.61 | Ca |
Fe | N/A | -3.30 | ... | ... | -3.30 | ... | 4.20 | Fe |
Position
Right Ascension : 14 54 39.27 | Declination : +04 21 38.1 | 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 |