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J/A+A/661/A103
-1
High-precision chemical abundances of Sequoia (Matsuno+, 2022)
ReadMe+ftp
2022A&A...661A.103M
Similar Catalogs
Post annotation
1.
J/A+A/661/A103/line
Line list
(3173 rows)
meta
J/A+A/661/A103/line
Simple Constraint
List Of Constraints
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Constraints
applied on Columns
(
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Column
Constraint
Explain
(
UCD
)
recno
Record number assigned by the VizieR team. Should Not be used for identification.
(
meta.record
)
(
RECORD
)
Object
(char)
Object name used in this study
(
meta.id;meta.main
)
(
ID_MAIN
)
species
(char)
Name of the species
(
phys.atmol.element
)
(
AT_SPECIES
)
lambda
0.1nm
Wavelength
(
em.wl
)
(
SPECT_WAVELENGTH_MISC
)
chi
eV
Excitation potential
(
phys.atmol.excitation
)
(
AT_ENERGY_EXCIT
)
loggf
loggf value
(
phys.atmol.oscStrength
)
(
AT_OSC_STRENGTH
)
EW
0.1pm
Equivalent width (mÅ)
(
spect.line.eqWidth
)
(
SPECT_EQ-WIDTH
)
e_EW
0.1pm
Uncertainty in equivalent width (mÅ)
(
stat.error;spect.line.eqWidth
)
(
ERROR
)
A
Abundance from this line
(
phys.abund
)
(
PHYS_ABUND_MISC
)
eAteff
Uncertainty in abundance due to effective temperature
(
stat.error
)
(
ERROR
)
eAlogg
Uncertainty in abundance due to surface gravity
(
stat.error
)
(
ERROR
)
eAvt
Uncertainty in abundance due to microturbulent velocity
(
stat.error
)
(
ERROR
)
eA[Fe/H]
Uncertainty in abundance due to metallicity
(
stat.error
)
(
ERROR
)
eAEW
(char)
Uncertainty in abundance due to equivalent widths of this star and the reference star
(
stat.error
)
(
ERROR
)
sX
Uncertainty floor
(
stat.error
)
(
ERROR
)
Weight
Weight used to obtain the best estimate for the abundance of the species
(
phys.atmol.weight;meta.modelled
)
(
WEIGHT
)
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cols
(i)
indexed column
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