HE1300+0157
taken from 6 paper(s):
/P.S.Barklem et al.(2005)/
/A.Frebel et al.(2007)/
/J.G.Cohen et al.(2008)/
/L.Zhang et al.(2011)/
/J.G.Cohen et al.(2013)/
/A.Arentsen et al.(2019)/
The Hamburg/ESO R-process enhanced star survey (HERES). II. Spectroscopic analysis of the survey sample
Stellar Parameters
Teff : 5411 | log g : 3.38 | vturb : 1.43 |
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 | 1 | ... | 1.17+-0.29 | 5.82+-0.27 | -2.61+-0.27 | 1.13+-0.29 | 5.82+-0.27 | CH |
Mg I | 3 | ... | 0.40+-0.27 | 4.25+-0.24 | -3.35+-0.24 | 0.39+-0.27 | 4.25+-0.24 | Mg I |
Al I | 1 | ... | -0.83+-0.27 | 1.90+-0.22 | -4.55+-0.22 | -0.81+-0.27 | 1.90+-0.22 | Al I |
Ca I | 1 | ... | 0.47+-0.25 | 3.10+-0.22 | -3.24+-0.22 | 0.50+-0.25 | 3.10+-0.22 | Ca I |
Sc II | 1 | ... | 0.26+-0.29 | -0.30+-0.24 | -3.45+-0.24 | 0.29+-0.29 | -0.30+-0.24 | Sc II |
Ti | 5 | ... | 0.34+-0.28 | 1.62+-0.22 | -3.33+-0.22 | 0.41+-0.28 | 1.62+-0.22 | Ti |
Cr I | 2 | ... | -0.37+-0.25 | 1.56+-0.20 | -4.08+-0.20 | -0.34+-0.25 | 1.56+-0.20 | Cr I |
Fe | 18 | ... | 0.00+-0.22 | 3.76+-0.19 | -3.74+-0.19 | 0.00+-0.22 | 3.76+-0.19 | Fe |
Co I | 1 | ... | 0.50+-0.30 | 1.69+-0.25 | -3.30+-0.25 | 0.44+-0.30 | 1.69+-0.25 | Co I |
Ni I | 4 | ... | -0.04+-0.23 | 2.48+-0.17 | -3.74+-0.17 | 0.00+-0.23 | 2.48+-0.17 | Ni I |
Y II | 1 | ... | 0.56+-0.31 | -0.94+-0.22 | -3.15+-0.22 | 0.59+-0.31 | -0.94+-0.22 | Y II |
Position
Right Ascension : 13 02 56.24 | Declination : +01 41 52.1 | 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 | 20000 | 56 | N/A | 73.6 |
Chemical Abundance Analysis of the Extremely Metal-poor Star HE 1300+0157
Stellar Parameters
Teff : 5450+-70 | log g : 3.2+-0.3 | vturb : 1.54+-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 |
Li I | Syn | ... | ... | 1.06+-0.09 | -2.20+-0.09 | 1.58+-0.09 | 1.06+-0.09 | Li I |
CH | Syn | -2.50+-0.27 | 1.38+-0.27 | 5.89+-0.27 | -2.54+-0.27 | 1.24+-0.27 | 5.89+-0.27 | CH |
NH | Syn | <-2.66 | <1.22 | <5.12 | <-2.71 | <1.07 | <5.12 | NH |
OH | Syn | -2.12+-0.39 | 1.76+-0.39 | 6.54+-0.39 | -2.15+-0.39 | 1.63+-0.39 | 6.54+-0.39 | OH |
Na I | 2 | -3.73+-0.10 | 0.15+-0.10 | 2.44+-0.10 | -3.80+-0.10 | -0.02+-0.10 | 2.44+-0.10 | Na I |
Mg I | 6 | -3.43+-0.14 | 0.45+-0.14 | 4.10+-0.14 | -3.50+-0.14 | 0.28+-0.14 | 4.10+-0.14 | Mg I |
Al I | 1 | -4.33+-0.12 | -0.45+-0.12 | 2.04+-0.12 | -4.41+-0.12 | -0.63+-0.12 | 2.04+-0.12 | Al I |
Si I | 1 | -3.01+-0.18 | 0.87+-0.18 | 4.50+-0.18 | -3.01+-0.18 | 0.77+-0.18 | 4.50+-0.18 | Si I |
Ca I | 5 | -3.33+-0.12 | 0.55+-0.12 | 2.98+-0.12 | -3.36+-0.12 | 0.42+-0.12 | 2.98+-0.12 | Ca I |
Ca II | 4 | -3.56+-0.14 | 0.32+-0.14 | 2.75+-0.14 | -3.59+-0.14 | 0.19+-0.14 | 2.75+-0.14 | Ca II |
Sc II | 12 | -3.42+-0.15 | 0.46+-0.15 | -0.37+-0.15 | -3.52+-0.15 | 0.26+-0.15 | -0.37+-0.15 | Sc II |
Ti I | 4 | -3.24+-0.14 | 0.64+-0.14 | 1.66+-0.14 | -3.29+-0.14 | 0.49+-0.14 | 1.66+-0.14 | Ti I |
Ti II | 40 | -3.13+-0.16 | 0.75+-0.16 | 1.77+-0.16 | -3.18+-0.16 | 0.60+-0.16 | 1.77+-0.16 | Ti II |
V I | 4379 | <-2.85 | <1.03 | <1.15 | <-2.78 | <1.00 | <1.15 | V I |
Cr I | 5 | -4.13+-0.15 | -0.25+-0.15 | 1.51+-0.15 | -4.13+-0.15 | -0.35+-0.15 | 1.51+-0.15 | Cr I |
Cr II | 2 | -3.99+-0.13 | -0.11+-0.13 | 1.65+-0.13 | -3.99+-0.13 | -0.21+-0.13 | 1.65+-0.13 | Cr II |
Mn I | 1 | -4.34+-0.13 | -0.46+-0.13 | 1.05+-0.13 | -4.38+-0.13 | -0.60+-0.13 | 1.05+-0.13 | Mn I |
Mn II | 1 | -4.50+-0.13 | -0.62+-0.13 | 0.89+-0.13 | -4.54+-0.13 | -0.76+-0.13 | 0.89+-0.13 | Mn II |
Fe I | 101 | -3.73+-0.16 | 0.15+-0.16 | 3.72+-0.16 | -3.78+-0.16 | 0.15+-0.16 | 3.72+-0.16 | Fe I |
Fe II | 7 | -3.88+-0.14 | 0.00+-0.14 | 3.57+-0.14 | -3.93+-0.14 | 0.00+-0.14 | 3.57+-0.14 | Fe II |
Co I | 16 | -3.12+-0.15 | 0.76+-0.15 | 1.80+-0.15 | -3.19+-0.15 | 0.59+-0.15 | 1.80+-0.15 | Co I |
Ni I | 25 | -3.62+-0.20 | 0.26+-0.20 | 2.61+-0.20 | -3.61+-0.20 | 0.17+-0.20 | 2.61+-0.20 | Ni I |
Zn I | 4810 | <-2.97 | <0.91 | <1.63 | <-2.93 | <0.85 | <1.63 | Zn I |
Sr II | 4077 | <-5.56 | <-1.68 | <-2.64 | <-5.51 | <-1.73 | <-2.64 | Sr II |
Y II | 4884 | <-3.14 | <0.74 | <-0.93 | <-3.14 | <0.64 | <-0.93 | Y II |
Zr II | 4497 | <-2.66 | <1.22 | <-0.07 | <-2.65 | <1.13 | <-0.07 | Zr II |
Ba II | 4554 | <-4.73 | <-0.85 | <-2.56 | <-4.74 | <-0.96 | <-2.56 | Ba II |
Eu II | 4129 | <-2.32 | <1.56 | <-1.80 | <-2.32 | <1.46 | <-1.80 | Eu II |
Pb I | 4057 | <-1.10 | <2.78 | <0.90 | <-1.14 | <2.64 | <0.90 | Pb I |
Position
Right Ascension : 13 02 56.24 | Declination : +01 41 52.1 | Galactic Longitude (l) : N/A | Galactic Latitude (b) : N/A |
Observing Log
Date of Observation | JD | Facility | Resolution | S/N | Exposure Time | Vrad |
2004-05-30-0737 | N/A | SUBARUHDS | 60000 | 70-170 | 30min | 75.3 |
2004-06-01-0539 | N/A | SUBARUHDS | 60000 | 70-170 | 270min | 74.6 |
2005-03-02-1208 | N/A | SUBARUHDS | 60000 | 35-70 | 180min | 74.6 |
New Extremely Metal-Poor Stars in the Galactic Halo
Stellar Parameters
Teff : 5632 | log g : 3.37 | vturb : 1.3 |
Chemical Abundances
| | Original Data | Converted Data Asplund et al. (2009) | |
Element | Nline | [X/H] | [X/Fe] | log-e | [X/H] | [X/Fe] | log-e | Element |
CH | 1 | ... | 1.23 | 6.43 | -2.00 | 1.44 | 6.43 | CH |
NH | 1 | ... | <0.71 | <5.25 | <-2.58 | <0.86 | <5.25 | NH |
OH | 2 | ... | 1.69+-0.18 | 7.13+-0.18 | -1.56+-0.18 | 1.88+-0.18 | 7.13+-0.18 | OH |
Na I | 2 | ... | -0.49+-0.07 | 2.44+-0.07 | -3.80+-0.07 | -0.36+-0.07 | 2.44+-0.07 | Na I |
Mg I | 3 | ... | 0.32+-0.10 | 4.47+-0.10 | -3.13+-0.10 | 0.31+-0.10 | 4.47+-0.10 | Mg I |
Al I | 1 | ... | -0.24 | 2.83 | -3.62 | -0.18 | 2.83 | Al I |
Si I | 1 | ... | 0.49 | 4.64 | -2.87 | 0.57 | 4.64 | Si I |
Ca I | 2 | ... | 0.26+-0.13 | 3.23+-0.13 | -3.11+-0.13 | 0.33+-0.13 | 3.23+-0.13 | Ca I |
Ca II | 1 | ... | 0.10 | 3.07 | -3.27 | 0.17 | 3.07 | Ca II |
Sc II | 1 | ... | 0.17 | -0.12 | -3.27 | 0.17 | -0.12 | Sc II |
Ti II | 8 | ... | 0.12+-0.06 | 1.72+-0.06 | -3.23+-0.06 | 0.21+-0.06 | 1.72+-0.06 | Ti II |
Cr I | 4 | ... | -0.53+-0.07 | 1.74+-0.07 | -3.90+-0.07 | -0.46+-0.07 | 1.74+-0.07 | Cr I |
Mn I | 2 | ... | -0.86+-0.02 | 1.13+-0.02 | -4.30+-0.02 | -0.86+-0.02 | 1.13+-0.02 | Mn I |
Mn II | 2 | ... | -0.66+-0.16 | 1.33+-0.16 | -4.10+-0.16 | -0.66+-0.16 | 1.33+-0.16 | Mn II |
Fe I | 36 | -3.39+-0.19 | ... | 4.06+-0.19 | -3.44+-0.19 | ... | 4.06+-0.19 | Fe I |
Fe II | 6 | -3.55+-0.11 | -0.16+-0.11 | 3.90+-0.11 | -3.60+-0.11 | -0.16+-0.11 | 3.90+-0.11 | Fe II |
Co I | 3 | ... | 0.39+-0.08 | 1.92+-0.08 | -3.07+-0.08 | 0.37+-0.08 | 1.92+-0.08 | Co I |
Ni I | 2 | ... | -0.02+-0.06 | 2.83+-0.06 | -3.39+-0.06 | 0.05+-0.06 | 2.83+-0.06 | Ni I |
Cu I | 2 | ... | -0.68+-0.02 | 0.13+-0.02 | -4.06+-0.02 | -0.62+-0.02 | 0.13+-0.02 | Cu I |
Sr II | 1 | ... | -1.55 | -2.05 | -4.92 | -1.48 | -2.05 | Sr II |
Ba II | 2 | ... | <-0.63+-0.20 | <-1.89+-0.20 | <-4.07+-0.20 | <-0.63+-0.20 | <-1.89+-0.20 | Ba II |
Position
Right Ascension : 13 02 56.24 | Declination : +01 41 52.1 | Galactic Longitude (l) : N/A | Galactic Latitude (b) : N/A |
Observing Log
Date of Observation | JD | Facility | Resolution | S/N | Exposure Time | Vrad |
| 2452830.50 | | | | | +73.6+-2.0 |
| 2453157.74 | | | | | +74.6+-0.6 |
| 2453432.01 | | | | | +74.6+-0.6 |
| 2453843.87 | KECKHIRES | 35000 | >110 | 3600 | +73.4+-0.1 |
The Hamburg/ESO R-process Enhanced Star survey (HERES). VI. The Galactic chemical evolution of silicon
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 | -2.70 | 1.06 | 5.82 | -2.61 | 1.15 | 5.82 | C |
Fe | N/A | -3.76 | ... | ... | -3.76 | ... | 3.74 | Fe |
Position
Right Ascension : 13 02 56.24 | Declination : +01 41 52.1 | 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 | 20000 | N/A | N/A | N/A |
Normal and Outlying Populations of the Milky Way Stellar Halo at [Fe/H] <-2
Stellar Parameters
Teff : 5550+-100 | log g : 3.3+-0.25 | vturb : 1.3+-0.2 |
Chemical Abundances
| | Original Data | Converted Data Asplund et al. (2009) | |
Element | Nline | [X/H] | [X/Fe] | log-e | [X/H] | [X/Fe] | log-e | Element |
CH | N/A | ... | 1.13 | ... | -2.20 | 1.34 | 6.23 | CH |
NH | 1 | ... | <0.61 | ... | <-2.78 | <0.76 | <5.05 | NH |
O I | 2 | ... | 1.49+-0.18 | ... | -1.76+-0.18 | 1.78+-0.18 | 6.93+-0.18 | O I |
Na I | 2 | ... | -0.26+-0.07 | ... | -3.67+-0.07 | -0.13+-0.07 | 2.57+-0.07 | Na I |
Mg I | 3 | ... | 0.34+-0.1 | ... | -3.21+-0.1 | 0.33+-0.1 | 4.39+-0.1 | Mg I |
Al I | 1 | ... | -0.22 | ... | -3.69 | -0.15 | 2.76 | Al I |
Si I | 1 | ... | 0.48 | ... | -2.97 | 0.57 | 4.54 | Si I |
Ca I | 2 | ... | 0.27+-0.13 | ... | -3.20+-0.13 | 0.34+-0.13 | 3.14+-0.13 | Ca I |
Ca II | 1 | ... | 0.14 | ... | -3.33 | 0.21 | 3.01 | Ca II |
Sc II | 1 | ... | 0.19 | ... | -3.35 | 0.19 | -0.20 | Sc II |
Ti II | 8 | ... | 0.15+-0.06 | ... | -3.30+-0.06 | 0.24+-0.06 | 1.65+-0.06 | Ti II |
Cr I | 4 | ... | -0.52+-0.07 | ... | -3.98+-0.07 | -0.44+-0.07 | 1.66+-0.07 | Cr I |
Mn I | 2 | ... | -0.86+-0.02 | ... | -4.39+-0.02 | -0.85+-0.02 | 1.04+-0.02 | Mn I |
Mn II | 2 | ... | -0.63+-0.16 | ... | -4.16+-0.16 | -0.62+-0.16 | 1.27+-0.16 | Mn II |
Fe I | N/A | -3.49+-0.14 | ... | ... | -3.54+-0.14 | ... | 3.96+-0.14 | Fe I |
Fe II | 6 | -3.61+-0.11 | -0.12+-0.11 | ... | -3.66+-0.11 | -0.12+-0.11 | 3.84+-0.11 | Fe II |
Co I | 3 | ... | 0.39+-0.08 | ... | -3.17+-0.08 | 0.37+-0.08 | 1.82+-0.08 | Co I |
Ni I | 2 | ... | -0.03+-0.06 | ... | -3.49+-0.06 | 0.05+-0.06 | 2.73+-0.06 | Ni I |
Cu I | 2 | ... | -0.69+-0.02 | ... | -4.16+-0.02 | -0.62+-0.02 | 0.03+-0.02 | Cu I |
Sr II | 1 | ... | -1.53 | ... | -4.99 | -1.45 | -2.12 | Sr II |
Ba II | 1 | ... | <-0.74 | ... | <-4.28 | <-0.74 | <-2.10 | Ba II |
Binary Parameters
Position
Right Ascension : 13 02 56.24 | Declination : +01 41 52.1 | Galactic Longitude (l) : N/A | Galactic Latitude (b) : N/A |
Observing Log
Date of Observation | JD | Facility | Resolution | S/N | Exposure Time | Vrad |
2006-04 | N/A | KECKHIRES | 36000 | >150 | 3600 | 73.4 |
Binarity among CEMP-no stars: an indication of multiple formation pathways?
Stellar Parameters
Chemical Abundances
| | Original Data | Converted Data Asplund et al. (2009) | |
Element | Nline | [X/H] | [X/Fe] | log-e | [X/H] | [X/Fe] | log-e | Element |
C | N/A | ... | 1.31 | 5.99 | -2.44 | 1.31 | 5.99 | C |
Fe | N/A | -3.75 | ... | ... | -3.75 | ... | 3.75 | Fe |
Ba | N/A | ... | <-0.85 | ... | <-4.60 | <-0.85 | <-2.42 | Ba |
Binary Parameters
Binarity | Negative |
Vrad | 74.40+-0.70 |
Position
Right Ascension : 13 02 56.2 | Declination : +01 41 52 | Galactic Longitude (l) : N/A | Galactic Latitude (b) : N/A |
Observing Log
Date of Observation | JD | Facility | Resolution | S/N | Exposure Time | Vrad |
2013-08-15-171648 | 2456520.22 | GECKOCFHT | 68000 | N/A | N/A | 75.4+-1.06 |
2014-01-18-040447 | 2456675.67 | GECKOCFHT | 68000 | N/A | N/A | 72.89+-1.2 |
2014-02-12-004311 | 2456700.53 | GECKOCFHT | 68000 | N/A | N/A | 74.6+-0.44 |
2014-04-12-184311 | 2456760.28 | GECKOCFHT | 68000 | N/A | N/A | 74.67+-0.72 |