HD119516
taken from 8 paper(s):
/J.Simmerer et al.(2004)/
/B.W.Carney et al.(2003)/
/M.Ishigaki et al.(2010)/
/I.U.Roederer et al.(2010)/
/M.N.Ishigaki et al.(2012)/
/M.N.Ishigaki et al.(2013)/
/L.Zhang et al.(2009)/
/I.U.Roederer et al.(2014)/
The Rise of the s-Process in the Galaxy
Stellar Parameters
Teff : 5382 | log g : 2.47 | vturb : 2.50 |
Chemical Abundances
| | Original Data | Converted Data Asplund et al. (2009) | |
Element | Nline | [X/H] | [X/Fe] | log-e | [X/H] | [X/Fe] | log-e | Element |
C | N/A | ... | -1.15 | ... | -3.08 | -0.97 | 5.35 | C |
Fe I | 7 | -2.11 | ... | ... | -2.11 | ... | 5.39 | Fe I |
Fe II | 8 | -1.85 | ... | ... | -1.85 | ... | 5.65 | Fe II |
La II | N/A | ... | ... | -0.59+-0.04 | -1.69+-0.04 | 0.42+-0.04 | -0.59+-0.04 | La II |
Eu II | N/A | ... | ... | -0.9+-0.05 | -1.42+-0.05 | 0.69+-0.05 | -0.9+-0.05 | Eu II |
Position
Right Ascension : 13 43 26.72 | Declination : +15 34 31.1 | 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 | MCDONALD | 60000 | 100 | N/A | N/A |
Spectroscopic Binaries, Velocity Jitter, and Rotation in Field Metal-poor Red Giant and Red Horizontal-Branch 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 |
Fe | N/A | -2.49 | ... | ... | -2.49 | ... | 5.01 | Fe |
Binary Parameters
Position
Right Ascension : 13 43 26.72 | Declination : +15 34 31.1 | 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 | 2445725.87455 | WYETH | N/A | N/A | N/A | -285.73+-0.68 |
N/A | 2445742.92026 | WYETH | N/A | N/A | N/A | -286.83+-0.80 |
N/A | 2445753.78800 | WYETH | N/A | N/A | N/A | -285.69+-0.69 |
N/A | 2445917.54587 | WYETH | N/A | N/A | N/A | -285.73+-0.98 |
N/A | 2446513.77786 | WYETH | N/A | N/A | N/A | -284.34+-0.65 |
N/A | 2446841.94821 | WYETH | N/A | N/A | N/A | -285.87+-0.85 |
N/A | 2447134.06273 | MMT | N/A | N/A | N/A | -285.55+-0.43 |
N/A | 2447602.84614 | WYETH | N/A | N/A | N/A | -286.50+-0.82 |
N/A | 2447695.62958 | MMT | N/A | N/A | N/A | -286.09+-0.60 |
N/A | 2448643.92104 | WYETH | N/A | N/A | N/A | -287.21+-0.98 |
N/A | 2449049.88381 | WYETH | N/A | N/A | N/A | -286.14+-0.52 |
N/A | 2450640.58243 | WYETH | N/A | N/A | N/A | -285.83+-0.72 |
Chemical Abundances of Outer Halo Stars in the Milky Way
Stellar Parameters
Teff : 5438+-75 | log g : 1.76 | vturb : 2.28 |
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 I | N/A | -1.74+-0.14 | 0.34+-0.14 | ... | -1.76+-0.14 | 0.33+-0.14 | 5.84+-0.14 | Mg I |
Ca I | N/A | -1.73+-0.07 | 0.35+-0.07 | ... | -1.71+-0.07 | 0.38+-0.07 | 4.63+-0.07 | Ca I |
Ti | N/A | ... | 0.21+-0.03 | ... | -1.81+-0.03 | 0.28+-0.03 | 3.14+-0.03 | Ti |
Ti I | 2 | -1.93+-0.07 | ... | ... | -1.86+-0.07 | 0.23+-0.07 | 3.09+-0.07 | Ti I |
Ti II | 6 | -1.85+-0.04 | ... | ... | -1.78+-0.04 | 0.31+-0.04 | 3.17+-0.04 | Ti II |
Cr | N/A | ... | -0.18+-0.03 | ... | -2.24+-0.03 | -0.15+-0.03 | 3.40+-0.03 | Cr |
Cr I | 3 | -2.33+-0.03 | ... | ... | -2.30+-0.03 | -0.21+-0.03 | 3.34+-0.03 | Cr I |
Cr II | 3 | -1.96+-0.08 | ... | ... | -1.93+-0.08 | 0.16+-0.08 | 3.71+-0.08 | Cr II |
Mn I | N/A | -2.57+-0.07 | 0.07+-0.07 | ... | -2.61+-0.07 | -0.52+-0.07 | 2.82+-0.07 | Mn I |
Fe I | 27 | -2.09+-0.02 | ... | ... | -2.09+-0.02 | ... | 5.41+-0.02 | Fe I |
Fe II | 6 | -2.07+-0.05 | ... | ... | -2.07+-0.05 | ... | 5.43+-0.05 | Fe II |
Ni I | N/A | -2.20+-0.07 | -0.11+-0.07 | ... | -2.17+-0.07 | -0.08+-0.07 | 4.05+-0.07 | Ni I |
Zn I | N/A | -2.18+-0.08 | -0.10+-0.08 | ... | -2.14+-0.08 | -0.05+-0.08 | 2.42+-0.08 | Zn I |
Y II | N/A | -2.26+-0.07 | -0.17+-0.07 | ... | -2.23+-0.07 | -0.14+-0.07 | -0.02+-0.07 | Y II |
Ba II | N/A | -2.01+-0.08 | 0.07+-0.08 | ... | -2.06+-0.08 | 0.03+-0.08 | 0.12+-0.08 | Ba II |
Position
Right Ascension : 13 43 26.72 | Declination : +15 34 31.1 | Galactic Longitude (l) : N/A | Galactic Latitude (b) : N/A |
Observing Log
Date of Observation | JD | Facility | Resolution | S/N | Exposure Time | Vrad |
2008-07-27 | N/A | SUBARUHDS | 50000 | >100 | N/A | N/A |
HARACTERIZING THE CHEMISTRY OF THE MILKY WAY STELLAR HALO: DETAILED CHEMICAL ANALYSIS OF A METAL-POOR STELLAR STREAM
Stellar Parameters
Teff : 5290 | log g : 1.10 | vturb : 2.25 |
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 | ... | ... | <1.14 | <-2.12 | <0.14 | <1.14 | Li I |
CH | N/A | ... | <-0.42 | <5.86 | <-2.57 | <-0.31 | <5.86 | CH |
CN | N/A | ... | <2.26 | <7.80 | <-0.03 | <2.23 | <7.80 | CN |
O I | 3 | ... | 0.61+-0.10 | 7.26+-0.10 | -1.43+-0.10 | 0.83+-0.10 | 7.26+-0.10 | O I |
Na I | 1 | ... | -0.26+-0.25 | 3.79+-0.25 | -2.45+-0.25 | -0.19+-0.25 | 3.79+-0.25 | Na I |
Mg I | 5 | ... | 0.34+-0.10 | 5.64+-0.10 | -1.96+-0.10 | 0.30+-0.10 | 5.64+-0.10 | Mg I |
Al I | 2 | ... | -0.97+-0.16 | 3.22+-0.16 | -3.23+-0.16 | -0.97+-0.16 | 3.22+-0.16 | Al I |
Si I | 1 | ... | 0.54+-0.25 | 5.81+-0.25 | -1.70+-0.25 | 0.56+-0.25 | 5.81+-0.25 | Si I |
K I | 2 | ... | 0.33+-0.15 | 3.17+-0.15 | -1.86+-0.15 | 0.40+-0.15 | 3.17+-0.15 | K I |
Ca I | 9 | ... | 0.33+-0.10 | 4.41+-0.10 | -1.93+-0.10 | 0.33+-0.10 | 4.41+-0.10 | Ca I |
Sc II | 6 | ... | -0.09+-0.13 | 0.73+-0.13 | -2.42+-0.13 | -0.16+-0.13 | 0.73+-0.13 | Sc II |
Ti I | 16 | ... | 0.13+-0.10 | 2.84+-0.10 | -2.11+-0.10 | 0.15+-0.10 | 2.84+-0.10 | Ti I |
Ti II | 20 | ... | -0.02+-0.11 | 2.69+-0.11 | -2.26+-0.11 | 0.00+-0.11 | 2.69+-0.11 | Ti II |
V I | 1 | ... | -0.14+-0.25 | 1.58+-0.25 | -2.35+-0.25 | -0.09+-0.25 | 1.58+-0.25 | V I |
V II | 2 | ... | -0.12+-0.15 | 1.60+-0.15 | -2.33+-0.15 | -0.07+-0.15 | 1.60+-0.15 | V II |
Cr I | 10 | ... | -0.15+-0.10 | 3.24+-0.10 | -2.40+-0.10 | -0.14+-0.10 | 3.24+-0.10 | Cr I |
Cr II | 3 | ... | 0.17+-0.10 | 3.56+-0.10 | -2.08+-0.10 | 0.18+-0.10 | 3.56+-0.10 | Cr II |
Mn I | 6 | ... | -0.33+-0.17 | 2.78+-0.17 | -2.65+-0.17 | -0.39+-0.17 | 2.78+-0.17 | Mn I |
Fe I | 114 | ... | 0.00+-0.10 | 5.24+-0.10 | -2.26+-0.10 | 0.00+-0.10 | 5.24+-0.10 | Fe I |
Fe II | 10 | ... | -0.05+-0.10 | 5.19+-0.10 | -2.31+-0.10 | -0.05+-0.10 | 5.19+-0.10 | Fe II |
Co I | 3 | ... | -0.12+-0.10 | 2.52+-0.10 | -2.47+-0.10 | -0.21+-0.10 | 2.52+-0.10 | Co I |
Ni I | 6 | ... | -0.05+-0.10 | 3.92+-0.10 | -2.30+-0.10 | -0.04+-0.10 | 3.92+-0.10 | Ni I |
Zn I | 2 | ... | 0.00+-0.15 | 2.32+-0.15 | -2.24+-0.15 | 0.02+-0.15 | 2.32+-0.15 | Zn I |
Rb I | N/A | ... | <2.48 | <2.72 | <0.36 | <2.62 | <2.72 | Rb I |
Sr II | 2 | ... | 0.26+-0.15 | 0.83+-0.15 | -2.04+-0.15 | 0.22+-0.15 | 0.83+-0.15 | Sr II |
Y II | 4 | ... | -0.39+-0.10 | -0.43+-0.10 | -2.64+-0.10 | -0.38+-0.10 | -0.43+-0.10 | Y II |
Zr II | 3 | ... | -0.03+-0.10 | 0.29+-0.10 | -2.29+-0.10 | -0.03+-0.10 | 0.29+-0.10 | Zr II |
Nb II | N/A | ... | <1.08 | <0.26 | <-1.20 | <1.06 | <0.26 | Nb II |
Mo I | N/A | ... | <0.71 | <0.31 | <-1.57 | <0.69 | <0.31 | Mo I |
Tc I | N/A | ... | <3.25 | <0.97 | <0.97 | <3.23 | <0.97 | Tc I |
Ba II | 2 | ... | -0.02+-0.24 | -0.16+-0.24 | -2.34+-0.24 | -0.08+-0.24 | -0.16+-0.24 | Ba II |
La II | 4 | ... | 0.01+-0.10 | -1.08+-0.10 | -2.18+-0.10 | 0.08+-0.10 | -1.08+-0.10 | La II |
Ce II | 3 | ... | 0.21+-0.11 | -0.64+-0.11 | -2.22+-0.11 | 0.04+-0.11 | -0.64+-0.11 | Ce II |
Pr II | 3 | ... | 0.20+-0.22 | -1.23+-0.22 | -1.95+-0.22 | 0.31+-0.22 | -1.23+-0.22 | Pr II |
Nd II | 6 | ... | 0.07+-0.10 | -0.74+-0.10 | -2.16+-0.10 | 0.10+-0.10 | -0.74+-0.10 | Nd II |
Sm II | 2 | ... | 0.21+-0.15 | -1.11+-0.15 | -2.07+-0.15 | 0.19+-0.15 | -1.11+-0.15 | Sm II |
Eu II | 3 | ... | 0.34+-0.10 | -1.43+-0.10 | -1.95+-0.10 | 0.31+-0.10 | -1.43+-0.10 | Eu II |
Gd II | 3 | ... | 0.44+-0.10 | -0.76+-0.10 | -1.83+-0.10 | 0.43+-0.10 | -0.76+-0.10 | Gd II |
Dy II | 1 | ... | 0.45+-0.25 | -0.77+-0.25 | -1.87+-0.25 | 0.39+-0.25 | -0.77+-0.25 | Dy II |
Er II | 2 | ... | 0.34+-0.15 | -1.02+-0.15 | -1.94+-0.15 | 0.32+-0.15 | -1.02+-0.15 | Er II |
Tm II | 1 | ... | 0.22+-0.25 | -1.83+-0.25 | -1.95+-0.25 | 0.31+-0.25 | -1.83+-0.25 | Tm II |
Yb II | 1 | ... | 0.15+-0.35 | -1.21+-0.35 | -2.13+-0.35 | 0.13+-0.35 | -1.21+-0.35 | Yb II |
Hf II | 1 | ... | 0.22+-0.40 | -1.21+-0.40 | -1.92+-0.40 | 0.34+-0.40 | -1.21+-0.40 | Hf II |
Pb I | N/A | ... | <1.91 | <1.52 | <-0.52 | <1.74 | <1.52 | Pb I |
Th II | N/A | ... | <0.36 | <-1.80 | <-1.86 | <0.40 | <-1.80 | Th II |
Binary Parameters
Binarity | Negative |
Vrad | -285.9+-0.8 |
Position
Right Ascension : 13 43 26.72 | Declination : +15 34 31.1 | Galactic Longitude (l) : N/A | Galactic Latitude (b) : N/A |
Observing Log
Date of Observation | JD | Facility | Resolution | S/N | Exposure Time | Vrad |
2009-05-07-06:40 | 2454958.782 | MCDONALD | 33000 | 65 | 2700 | -285.9+-0.8 |
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 : 5605+-100 | log g : 1.94+-0.3 | vturb : 1.90+-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 | ... | 0.18+-0.08 | ... | -1.70+-0.08 | 0.18+-0.08 | 5.90+-0.08 | Mg |
Ca | N/A | ... | 0.30+-0.09 | ... | -1.58+-0.09 | 0.30+-0.09 | 4.76+-0.09 | Ca |
Ti I | N/A | ... | 0.19+-0.07 | ... | -1.69+-0.07 | 0.19+-0.07 | 3.26+-0.07 | Ti I |
Ti II | N/A | ... | 0.08+-0.09 | ... | -1.80+-0.09 | 0.08+-0.09 | 3.15+-0.09 | Ti II |
Fe I | N/A | -1.88+-0.11 | ... | ... | -1.88+-0.11 | ... | 5.62+-0.11 | Fe I |
Fe II | N/A | -1.88+-0.13 | ... | ... | -1.88+-0.13 | ... | 5.62+-0.13 | Fe II |
Binary Parameters
Position
Right Ascension : 13 43 26.72 | Declination : +15 34 31.1 | 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 | SUBARUHDS | 50000 | N/A | N/A | -288.1+-0.3 |
Chemical Abundances of the Milky Way Thick Disk and Stellar Halo. II. Sodium, Iron-peak, and Neutron-capture Elements
Stellar Parameters
Teff : 5605 | log g : 1.94 | 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 |
Sc II | N/A | ... | -0.16+-0.1 | ... | -2.05+-0.1 | -0.16+-0.1 | 1.10+-0.1 | Sc II |
V I | N/A | ... | -0.17+-0.12 | ... | -2.06+-0.12 | -0.17+-0.12 | 1.87+-0.12 | V I |
Cr I | N/A | ... | -0.2+-0.07 | ... | -2.09+-0.07 | -0.20+-0.07 | 3.55+-0.07 | Cr I |
Cr II | N/A | ... | 0.05+-0.1 | ... | -1.84+-0.1 | 0.05+-0.1 | 3.80+-0.1 | Cr II |
Mn I | N/A | ... | -0.43+-0.1 | ... | -2.32+-0.1 | -0.43+-0.1 | 3.11+-0.1 | Mn I |
Fe I | N/A | -1.89+-0.11 | ... | ... | -1.89+-0.11 | ... | 5.61+-0.11 | Fe I |
Fe II | N/A | -1.92+-0.13 | ... | ... | -1.92+-0.13 | ... | 5.58+-0.13 | Fe II |
Co I | N/A | ... | -0.11+-0.11 | ... | -2.00+-0.11 | -0.11+-0.11 | 2.99+-0.11 | Co I |
Cu I | N/A | ... | -0.83 | ... | -2.72 | -0.83 | 1.47 | Cu I |
Y II | N/A | ... | -0.27+-0.12 | ... | -2.16+-0.12 | -0.27+-0.12 | 0.05+-0.12 | Y II |
Ba II | N/A | ... | -0.1+-0.14 | ... | -1.99+-0.14 | -0.10+-0.14 | 0.19+-0.14 | Ba II |
La II | N/A | ... | 0.15+-0.12 | ... | -1.74+-0.12 | 0.15+-0.12 | -0.64+-0.12 | La II |
Nd II | N/A | ... | 0.19+-0.12 | ... | -1.70+-0.12 | 0.19+-0.12 | -0.28+-0.12 | Nd II |
Sm II | N/A | ... | 0.36+-0.1 | ... | -1.53+-0.1 | 0.36+-0.1 | -0.57+-0.1 | Sm II |
Eu II | N/A | ... | 0.41+-0.07 | ... | -1.48+-0.07 | 0.41+-0.07 | -0.96+-0.07 | Eu II |
Position
Right Ascension : 13 43 26.72 | Declination : +15 34 31.1 | 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 | SUBARUHDS | 50000 | N/A | N/A | N/A |
Chemical Compositions of Kinematically Selected Outer Halo Stars
Stellar Parameters
Teff : 5550+-50 | log g : 2.20+-0.20 | vturb : 2.00+-0.3 |
Chemical Abundances
| | Original Data | Converted Data Asplund et al. (2009) | |
Element | Nline | [X/H] | [X/Fe] | log-e | [X/H] | [X/Fe] | log-e | Element |
Na I | 2 | -1.66+-0.07 | 0.16+-0.07 | ... | -1.57+-0.07 | 0.08+-0.07 | 4.67+-0.07 | Na I |
Mg I | 3 | -1.66+-0.09 | 0.16+-0.09 | ... | -1.68+-0.09 | -0.03+-0.09 | 5.92+-0.09 | Mg I |
Ca I | 19 | -1.60+-0.07 | 0.22+-0.07 | ... | -1.58+-0.07 | 0.07+-0.07 | 4.76+-0.07 | Ca I |
Sc II | 8 | -1.74+-0.07 | 0.08+-0.07 | ... | -1.80+-0.07 | -0.15+-0.07 | 1.35+-0.07 | Sc II |
Ti | N/A | ... | 0.31+-0.10 | ... | -1.47+-0.10 | 0.18+-0.10 | 3.48+-0.10 | Ti |
Ti I | 20 | -1.51+-0.10 | ... | ... | -1.47+-0.10 | 0.18+-0.10 | 3.48+-0.10 | Ti I |
Ti II | 8 | -1.55+-0.08 | ... | ... | -1.51+-0.08 | 0.14+-0.08 | 3.44+-0.08 | Ti II |
Cr | N/A | ... | -0.15+-0.08 | ... | -1.94+-0.08 | -0.29+-0.08 | 3.70+-0.08 | Cr |
Cr I | 12 | -1.97+-0.08 | ... | ... | -1.94+-0.08 | -0.29+-0.08 | 3.70+-0.08 | Cr I |
Cr II | 5 | -1.74+-0.08 | ... | ... | -1.71+-0.08 | -0.06+-0.08 | 3.93+-0.08 | Cr II |
Mn I | 2 | -2.23+-0.04 | -0.41+-0.04 | ... | -2.27+-0.04 | -0.62+-0.04 | 3.16+-0.04 | Mn I |
Fe | N/A | -1.82+-0.05 | ... | ... | -1.65+-0.05 | ... | 5.85+-0.05 | Fe |
Fe I | 82 | -1.82+-0.05 | ... | ... | -1.65+-0.05 | ... | 5.85+-0.05 | Fe I |
Fe II | 10 | -1.82+-0.07 | ... | ... | -1.65+-0.07 | ... | 5.85+-0.07 | Fe II |
Ni I | 6 | -1.89+-0.10 | -0.07+-0.10 | ... | -1.86+-0.10 | -0.21+-0.10 | 4.36+-0.10 | Ni I |
Zn I | 3 | -1.96+-0.07 | -0.06+-0.07 | ... | -1.92+-0.07 | -0.27+-0.07 | 2.64+-0.07 | Zn I |
Y II | 2 | -1.96+-0.05 | -0.14+-0.05 | ... | -1.93+-0.05 | -0.28+-0.05 | 0.28+-0.05 | Y II |
Ba II | 3 | -1.71+-0.06 | 0.11+-0.06 | ... | -1.76+-0.06 | -0.11+-0.06 | 0.42+-0.06 | Ba II |
Binary Parameters
Position
Right Ascension : 13 43 26.72 | Declination : +15 34 31.1 | Galactic Longitude (l) : N/A | Galactic Latitude (b) : N/A |
Observing Log
Date of Observation | JD | Facility | Resolution | S/N | Exposure Time | Vrad |
2003-02 | N/A | SUBARUHDS | 50000 | N/A | 600 | -284.5 |
A SEARCH FOR STARS OF VERY LOW METAL ABUNDANCE. VI. DETAILED ABUNDANCES OF 313 METAL-POOR STARS
Stellar Parameters
Teff : 5660+-40 | log g : 1.9+-0.29 | vturb : 1.9+-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 | ... | ... | <1.05 | <-2.21 | <-0.27 | <1.05 | Li I |
CH | 1 | ... | -0.42+-0.25 | 6.08 | -2.35 | -0.41+-0.25 | 6.08 | CH |
CN | 1 | ... | <1.80 | <7.70 | <-0.13 | <1.81 | <7.70 | CN |
O I | 3 | ... | -0.18+-0.17 | 6.57 | -2.12 | -0.18+-0.17 | 6.57 | O I |
Na I | 1 | ... | -0.45+-0.24 | 3.85 | -2.39 | -0.45+-0.24 | 3.85 | Na I |
Mg I | 5 | ... | 0.18+-0.17 | 5.84 | -1.76 | 0.18+-0.17 | 5.84 | Mg I |
Al I | 1 | ... | -0.77+-0.26 | 3.74 | -2.71 | -0.77+-0.26 | 3.74 | Al I |
Si I | 2 | ... | 0.43+-0.25 | 6.00 | -1.51 | 0.43+-0.25 | 6.00 | Si I |
K I | 2 | ... | -0.03+-0.20 | 3.06 | -1.97 | -0.03+-0.20 | 3.06 | K I |
Ca I | 10 | ... | 0.28+-0.19 | 4.68 | -1.66 | 0.28+-0.19 | 4.68 | Ca I |
Sc II | 5 | ... | -0.06+-0.14 | 1.16 | -1.99 | -0.05+-0.14 | 1.16 | Sc II |
Ti I | 16 | ... | 0.17+-0.17 | 3.18 | -1.77 | 0.17+-0.17 | 3.18 | Ti I |
Ti II | 19 | ... | 0.16+-0.15 | 3.18 | -1.77 | 0.17+-0.15 | 3.18 | Ti II |
V I | 1 | ... | -0.08+-0.19 | 1.91 | -2.02 | -0.08+-0.19 | 1.91 | V I |
V II | 2 | ... | 0.07+-0.23 | 2.06 | -1.87 | 0.07+-0.23 | 2.06 | V II |
Cr I | 9 | ... | -0.16+-0.16 | 3.54 | -2.10 | -0.16+-0.16 | 3.54 | Cr I |
Cr II | 3 | ... | 0.16+-0.15 | 3.87 | -1.77 | 0.17+-0.15 | 3.87 | Cr II |
Mn I | 4 | ... | -0.36+-0.16 | 3.13 | -2.30 | -0.36+-0.16 | 3.13 | Mn I |
Fe I | 86 | -1.94+-0.17 | ... | 5.56 | -1.94+-0.17 | ... | 5.56 | Fe I |
Fe II | 10 | -1.93+-0.15 | ... | 5.57 | -1.93+-0.15 | ... | 5.57 | Fe II |
Co I | 3 | ... | -0.20+-0.20 | 2.85 | -2.14 | -0.20+-0.20 | 2.85 | Co I |
Ni I | 6 | ... | -0.03+-0.20 | 4.24 | -1.98 | -0.04+-0.20 | 4.24 | Ni I |
Zn I | 3 | ... | -0.04+-0.17 | 2.58 | -1.98 | -0.04+-0.17 | 2.58 | Zn I |
Rb I | 1 | ... | <2.10 | <2.68 | <0.32 | <2.26 | <2.68 | Rb I |
Sr II | 2 | ... | 0.53+-0.23 | 1.46 | -1.41 | 0.53+-0.23 | 1.46 | Sr II |
Y II | 4 | ... | -0.36+-0.16 | -0.09 | -2.30 | -0.36+-0.16 | -0.09 | Y II |
Zr II | 3 | ... | 0.10+-0.15 | 0.75 | -1.83 | 0.11+-0.15 | 0.75 | Zr II |
Nb II | 1 | ... | <1.00 | <0.53 | <-0.93 | <1.01 | <0.53 | Nb II |
Mo I | 1 | ... | <0.54 | <0.48 | <-1.40 | <0.54 | <0.48 | Mo I |
Tc I | 1 | ... | ... | <1.13 | <1.13 | <3.07 | <1.13 | Tc I |
Sn I | 1 | ... | <1.81 | <1.94 | <-0.13 | <1.81 | <1.94 | Sn I |
Ba II | 2 | ... | 0.17+-0.16 | 0.42 | -1.76 | 0.18+-0.16 | 0.42 | Ba II |
La II | 4 | ... | 0.24+-0.15 | -0.60 | -1.70 | 0.24+-0.15 | -0.60 | La II |
Ce II | 4 | ... | 0.18+-0.17 | -0.17 | -1.75 | 0.19+-0.17 | -0.17 | Ce II |
Pr II | 2 | ... | 0.41+-0.19 | -0.80 | -1.52 | 0.42+-0.19 | -0.80 | Pr II |
Nd II | 5 | ... | 0.29+-0.17 | -0.23 | -1.65 | 0.29+-0.17 | -0.23 | Nd II |
Sm II | 2 | ... | 0.28+-0.16 | -0.69 | -1.65 | 0.29+-0.16 | -0.69 | Sm II |
Eu II | 3 | ... | 0.45+-0.16 | -0.97 | -1.49 | 0.45+-0.16 | -0.97 | Eu II |
Gd II | 3 | ... | 0.58+-0.19 | -0.28 | -1.35 | 0.59+-0.19 | -0.28 | Gd II |
Dy II | 2 | ... | 0.61+-0.16 | -0.22 | -1.32 | 0.62+-0.16 | -0.22 | Dy II |
Er II | 2 | ... | 0.52+-0.18 | -0.49 | -1.41 | 0.53+-0.18 | -0.49 | Er II |
Tm II | 1 | ... | 0.45+-0.25 | -1.38 | -1.50 | 0.44+-0.25 | -1.38 | Tm II |
Yb II | 1 | ... | 0.35+-0.25 | -0.66 | -1.58 | 0.36+-0.25 | -0.66 | Yb II |
Hf II | 1 | ... | <0.48 | <-0.60 | <-1.31 | <0.63 | <-0.60 | Hf II |
Pb I | 1 | ... | <1.49 | <1.59 | <-0.45 | <1.49 | <1.59 | Pb I |
Th II | 1 | ... | <0.67 | <-1.20 | <-1.26 | <0.68 | <-1.20 | Th II |
Binary Parameters
Binarity | Negative |
Vrad | -285.9 |
Position
Right Ascension : 13 43 26.72 | Declination : +15 34 31.1 | Galactic Longitude (l) : N/A | Galactic Latitude (b) : N/A |
Observing Log
Date of Observation | JD | Facility | Resolution | S/N | Exposure Time | Vrad |
2009-05-07-06:40 | 2454958.782 | MCDONALD | 33000 | 65-175 | 2700 | -285.9 |