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Elements & Properties
Stars With/Without Planets
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Abundances originally published in absolute A(X) notation cannot be shown when the "Original" normalization is selected since no solar normalization was specified.
Values are assigned zero for thin disk and one for thick disk.
Spectral type values are assigned a number: F = 10, G = 20, K = 30, M = 40, plus the subclass digit (1-10), plus the roman numeral value * 0.01. Example. F2V = 12.05.
Filter:
none
none
Element ratio:
H
He
Li
Be
II
B
C
N
O
F
Ne
Na
Mg
Al
II
Si
II
P
S
Cl
Ar
K
Ca
II
Sc
II
Ti
II
V
II
Cr
II
Mn
II
Fe
Co
II
Ni
II
Cu
II
Zn
II
Ga
II
Ge
As
Se
Br
Kr
Rb
Sr
II
Y
II
Zr
II
Nb
II
Mo
II
Tc
Ru
II
Rh
Pd
Ag
Cd
In
II
Sn
Sb
Te
I
Xe
Cs
Ba
II
Lu
II
Hf
II
Ta
W
II
Re
II
Os
Ir
Pt
Au
Hg
II
Tl
Pb
II
Bi
Po
At
Rn
Fr
Ra
Lr
Rf
Db
Sg
Bh
Hs
Mt
Ds
Rg
Cn
Nh
Fl
Mc
Lv
Ts
Og
La
II
Ce
II
Pr
II
Nd
II
Pm
Sm
II
Eu
II
Gd
II
Tb
II
Dy
II
Ho
II
Er
II
Tm
II
Yb
II
Ac
Th
II
Pa
U
Np
Pu
Am
Cm
Bk
Cf
Es
Fm
Md
No
Stellar property:
RA
Dec
dist
X pos
Y pos
Z pos
Teff
logg
SpecType
V mag
B mag
B-V
pmRA
pmDec
U vel
V vel
W vel
disk
smass
radius
Planet property:
period
pmass
ecc
sma
/
H
H
He
Li
Be
II
B
C
N
O
F
Ne
Na
Mg
Al
II
Si
II
P
S
Cl
Ar
K
Ca
II
Sc
II
Ti
II
V
II
Cr
II
Mn
II
Fe
Co
II
Ni
II
Cu
II
Zn
II
Ga
II
Ge
As
Se
Br
Kr
Rb
Sr
II
Y
II
Zr
II
Nb
II
Mo
II
Tc
Ru
II
Rh
Pd
Ag
Cd
In
II
Sn
Sb
Te
I
Xe
Cs
Ba
II
Lu
II
Hf
II
Ta
W
II
Re
II
Os
Ir
Pt
Au
Hg
II
Tl
Pb
II
Bi
Po
At
Rn
Fr
Ra
Lr
Rf
Db
Sg
Bh
Hs
Mt
Ds
Rg
Cn
Nh
Fl
Mc
Lv
Ts
Og
La
II
Ce
II
Pr
II
Nd
II
Pm
Sm
II
Eu
II
Gd
II
Tb
II
Dy
II
Ho
II
Er
II
Tm
II
Yb
II
Ac
Th
II
Pa
U
Np
Pu
Am
Cm
Bk
Cf
Es
Fm
Md
No
inverse
none
none
Element ratio:
H
He
Li
Be
II
B
C
N
O
F
Ne
Na
Mg
Al
II
Si
II
P
S
Cl
Ar
K
Ca
II
Sc
II
Ti
II
V
II
Cr
II
Mn
II
Fe
Co
II
Ni
II
Cu
II
Zn
II
Ga
II
Ge
As
Se
Br
Kr
Rb
Sr
II
Y
II
Zr
II
Nb
II
Mo
II
Tc
Ru
II
Rh
Pd
Ag
Cd
In
II
Sn
Sb
Te
I
Xe
Cs
Ba
II
Lu
II
Hf
II
Ta
W
II
Re
II
Os
Ir
Pt
Au
Hg
II
Tl
Pb
II
Bi
Po
At
Rn
Fr
Ra
Lr
Rf
Db
Sg
Bh
Hs
Mt
Ds
Rg
Cn
Nh
Fl
Mc
Lv
Ts
Og
La
II
Ce
II
Pr
II
Nd
II
Pm
Sm
II
Eu
II
Gd
II
Tb
II
Dy
II
Ho
II
Er
II
Tm
II
Yb
II
Ac
Th
II
Pa
U
Np
Pu
Am
Cm
Bk
Cf
Es
Fm
Md
No
Stellar property:
RA
Dec
dist
X pos
Y pos
Z pos
Teff
logg
SpecType
V mag
B mag
B-V
pmRA
pmDec
U vel
V vel
W vel
disk
smass
radius
Planet property:
period
pmass
ecc
sma
/
H
H
He
Li
Be
II
B
C
N
O
F
Ne
Na
Mg
Al
II
Si
II
P
S
Cl
Ar
K
Ca
II
Sc
II
Ti
II
V
II
Cr
II
Mn
II
Fe
Co
II
Ni
II
Cu
II
Zn
II
Ga
II
Ge
As
Se
Br
Kr
Rb
Sr
II
Y
II
Zr
II
Nb
II
Mo
II
Tc
Ru
II
Rh
Pd
Ag
Cd
In
II
Sn
Sb
Te
I
Xe
Cs
Ba
II
Lu
II
Hf
II
Ta
W
II
Re
II
Os
Ir
Pt
Au
Hg
II
Tl
Pb
II
Bi
Po
At
Rn
Fr
Ra
Lr
Rf
Db
Sg
Bh
Hs
Mt
Ds
Rg
Cn
Nh
Fl
Mc
Lv
Ts
Og
La
II
Ce
II
Pr
II
Nd
II
Pm
Sm
II
Eu
II
Gd
II
Tb
II
Dy
II
Ho
II
Er
II
Tm
II
Yb
II
Ac
Th
II
Pa
U
Np
Pu
Am
Cm
Bk
Cf
Es
Fm
Md
No
inverse
none
none
Element ratio:
H
He
Li
Be
II
B
C
N
O
F
Ne
Na
Mg
Al
II
Si
II
P
S
Cl
Ar
K
Ca
II
Sc
II
Ti
II
V
II
Cr
II
Mn
II
Fe
Co
II
Ni
II
Cu
II
Zn
II
Ga
II
Ge
As
Se
Br
Kr
Rb
Sr
II
Y
II
Zr
II
Nb
II
Mo
II
Tc
Ru
II
Rh
Pd
Ag
Cd
In
II
Sn
Sb
Te
I
Xe
Cs
Ba
II
Lu
II
Hf
II
Ta
W
II
Re
II
Os
Ir
Pt
Au
Hg
II
Tl
Pb
II
Bi
Po
At
Rn
Fr
Ra
Lr
Rf
Db
Sg
Bh
Hs
Mt
Ds
Rg
Cn
Nh
Fl
Mc
Lv
Ts
Og
La
II
Ce
II
Pr
II
Nd
II
Pm
Sm
II
Eu
II
Gd
II
Tb
II
Dy
II
Ho
II
Er
II
Tm
II
Yb
II
Ac
Th
II
Pa
U
Np
Pu
Am
Cm
Bk
Cf
Es
Fm
Md
No
Stellar property:
RA
Dec
dist
X pos
Y pos
Z pos
Teff
logg
SpecType
V mag
B mag
B-V
pmRA
pmDec
U vel
V vel
W vel
disk
smass
radius
Planet property:
period
pmass
ecc
sma
/
H
H
He
Li
Be
II
B
C
N
O
F
Ne
Na
Mg
Al
II
Si
II
P
S
Cl
Ar
K
Ca
II
Sc
II
Ti
II
V
II
Cr
II
Mn
II
Fe
Co
II
Ni
II
Cu
II
Zn
II
Ga
II
Ge
As
Se
Br
Kr
Rb
Sr
II
Y
II
Zr
II
Nb
II
Mo
II
Tc
Ru
II
Rh
Pd
Ag
Cd
In
II
Sn
Sb
Te
I
Xe
Cs
Ba
II
Lu
II
Hf
II
Ta
W
II
Re
II
Os
Ir
Pt
Au
Hg
II
Tl
Pb
II
Bi
Po
At
Rn
Fr
Ra
Lr
Rf
Db
Sg
Bh
Hs
Mt
Ds
Rg
Cn
Nh
Fl
Mc
Lv
Ts
Og
La
II
Ce
II
Pr
II
Nd
II
Pm
Sm
II
Eu
II
Gd
II
Tb
II
Dy
II
Ho
II
Er
II
Tm
II
Yb
II
Ac
Th
II
Pa
U
Np
Pu
Am
Cm
Bk
Cf
Es
Fm
Md
No
inverse
X-axis:
Fe
Element ratio:
H
He
Li
Be
II
B
C
N
O
F
Ne
Na
Mg
Al
II
Si
II
P
S
Cl
Ar
K
Ca
II
Sc
II
Ti
II
V
II
Cr
II
Mn
II
Fe
Co
II
Ni
II
Cu
II
Zn
II
Ga
II
Ge
As
Se
Br
Kr
Rb
Sr
II
Y
II
Zr
II
Nb
II
Mo
II
Tc
Ru
II
Rh
Pd
Ag
Cd
In
II
Sn
Sb
Te
I
Xe
Cs
Ba
II
Lu
II
Hf
II
Ta
W
II
Re
II
Os
Ir
Pt
Au
Hg
II
Tl
Pb
II
Bi
Po
At
Rn
Fr
Ra
Lr
Rf
Db
Sg
Bh
Hs
Mt
Ds
Rg
Cn
Nh
Fl
Mc
Lv
Ts
Og
La
II
Ce
II
Pr
II
Nd
II
Pm
Sm
II
Eu
II
Gd
II
Tb
II
Dy
II
Ho
II
Er
II
Tm
II
Yb
II
Ac
Th
II
Pa
U
Np
Pu
Am
Cm
Bk
Cf
Es
Fm
Md
No
Stellar property:
RA
Dec
dist
X pos
Y pos
Z pos
Teff
logg
SpecType
V mag
B mag
B-V
pmRA
pmDec
U vel
V vel
W vel
disk
smass
radius
Planet property:
period
pmass
ecc
sma
/
H
H
He
Li
Be
II
B
C
N
O
F
Ne
Na
Mg
Al
II
Si
II
P
S
Cl
Ar
K
Ca
II
Sc
II
Ti
II
V
II
Cr
II
Mn
II
Fe
Co
II
Ni
II
Cu
II
Zn
II
Ga
II
Ge
As
Se
Br
Kr
Rb
Sr
II
Y
II
Zr
II
Nb
II
Mo
II
Tc
Ru
II
Rh
Pd
Ag
Cd
In
II
Sn
Sb
Te
I
Xe
Cs
Ba
II
Lu
II
Hf
II
Ta
W
II
Re
II
Os
Ir
Pt
Au
Hg
II
Tl
Pb
II
Bi
Po
At
Rn
Fr
Ra
Lr
Rf
Db
Sg
Bh
Hs
Mt
Ds
Rg
Cn
Nh
Fl
Mc
Lv
Ts
Og
La
II
Ce
II
Pr
II
Nd
II
Pm
Sm
II
Eu
II
Gd
II
Tb
II
Dy
II
Ho
II
Er
II
Tm
II
Yb
II
Ac
Th
II
Pa
U
Np
Pu
Am
Cm
Bk
Cf
Es
Fm
Md
No
log
inverse
Y-axis:
Si
Element ratio:
H
He
Li
Be
II
B
C
N
O
F
Ne
Na
Mg
Al
II
Si
II
P
S
Cl
Ar
K
Ca
II
Sc
II
Ti
II
V
II
Cr
II
Mn
II
Fe
Co
II
Ni
II
Cu
II
Zn
II
Ga
II
Ge
As
Se
Br
Kr
Rb
Sr
II
Y
II
Zr
II
Nb
II
Mo
II
Tc
Ru
II
Rh
Pd
Ag
Cd
In
II
Sn
Sb
Te
I
Xe
Cs
Ba
II
Lu
II
Hf
II
Ta
W
II
Re
II
Os
Ir
Pt
Au
Hg
II
Tl
Pb
II
Bi
Po
At
Rn
Fr
Ra
Lr
Rf
Db
Sg
Bh
Hs
Mt
Ds
Rg
Cn
Nh
Fl
Mc
Lv
Ts
Og
La
II
Ce
II
Pr
II
Nd
II
Pm
Sm
II
Eu
II
Gd
II
Tb
II
Dy
II
Ho
II
Er
II
Tm
II
Yb
II
Ac
Th
II
Pa
U
Np
Pu
Am
Cm
Bk
Cf
Es
Fm
Md
No
Stellar property:
RA
Dec
dist
X pos
Y pos
Z pos
Teff
logg
SpecType
V mag
B mag
B-V
pmRA
pmDec
U vel
V vel
W vel
disk
smass
radius
Planet property:
period
pmass
ecc
sma
/
H
H
He
Li
Be
II
B
C
N
O
F
Ne
Na
Mg
Al
II
Si
II
P
S
Cl
Ar
K
Ca
II
Sc
II
Ti
II
V
II
Cr
II
Mn
II
Fe
Co
II
Ni
II
Cu
II
Zn
II
Ga
II
Ge
As
Se
Br
Kr
Rb
Sr
II
Y
II
Zr
II
Nb
II
Mo
II
Tc
Ru
II
Rh
Pd
Ag
Cd
In
II
Sn
Sb
Te
I
Xe
Cs
Ba
II
Lu
II
Hf
II
Ta
W
II
Re
II
Os
Ir
Pt
Au
Hg
II
Tl
Pb
II
Bi
Po
At
Rn
Fr
Ra
Lr
Rf
Db
Sg
Bh
Hs
Mt
Ds
Rg
Cn
Nh
Fl
Mc
Lv
Ts
Og
La
II
Ce
II
Pr
II
Nd
II
Pm
Sm
II
Eu
II
Gd
II
Tb
II
Dy
II
Ho
II
Er
II
Tm
II
Yb
II
Ac
Th
II
Pa
U
Np
Pu
Am
Cm
Bk
Cf
Es
Fm
Md
No
log
inverse
Z-axis (color):
none
none
Element ratio:
H
He
Li
Be
II
B
C
N
O
F
Ne
Na
Mg
Al
II
Si
II
P
S
Cl
Ar
K
Ca
II
Sc
II
Ti
II
V
II
Cr
II
Mn
II
Fe
Co
II
Ni
II
Cu
II
Zn
II
Ga
II
Ge
As
Se
Br
Kr
Rb
Sr
II
Y
II
Zr
II
Nb
II
Mo
II
Tc
Ru
II
Rh
Pd
Ag
Cd
In
II
Sn
Sb
Te
I
Xe
Cs
Ba
II
Lu
II
Hf
II
Ta
W
II
Re
II
Os
Ir
Pt
Au
Hg
II
Tl
Pb
II
Bi
Po
At
Rn
Fr
Ra
Lr
Rf
Db
Sg
Bh
Hs
Mt
Ds
Rg
Cn
Nh
Fl
Mc
Lv
Ts
Og
La
II
Ce
II
Pr
II
Nd
II
Pm
Sm
II
Eu
II
Gd
II
Tb
II
Dy
II
Ho
II
Er
II
Tm
II
Yb
II
Ac
Th
II
Pa
U
Np
Pu
Am
Cm
Bk
Cf
Es
Fm
Md
No
Stellar property:
RA
Dec
dist
X pos
Y pos
Z pos
Teff
logg
SpecType
V mag
B mag
B-V
pmRA
pmDec
U vel
V vel
W vel
disk
smass
radius
Planet property:
period
pmass
ecc
sma
/
H
H
He
Li
Be
II
B
C
N
O
F
Ne
Na
Mg
Al
II
Si
II
P
S
Cl
Ar
K
Ca
II
Sc
II
Ti
II
V
II
Cr
II
Mn
II
Fe
Co
II
Ni
II
Cu
II
Zn
II
Ga
II
Ge
As
Se
Br
Kr
Rb
Sr
II
Y
II
Zr
II
Nb
II
Mo
II
Tc
Ru
II
Rh
Pd
Ag
Cd
In
II
Sn
Sb
Te
I
Xe
Cs
Ba
II
Lu
II
Hf
II
Ta
W
II
Re
II
Os
Ir
Pt
Au
Hg
II
Tl
Pb
II
Bi
Po
At
Rn
Fr
Ra
Lr
Rf
Db
Sg
Bh
Hs
Mt
Ds
Rg
Cn
Nh
Fl
Mc
Lv
Ts
Og
La
II
Ce
II
Pr
II
Nd
II
Pm
Sm
II
Eu
II
Gd
II
Tb
II
Dy
II
Ho
II
Er
II
Tm
II
Yb
II
Ac
Th
II
Pa
U
Np
Pu
Am
Cm
Bk
Cf
Es
Fm
Md
No
log
inverse
Solar normalization:
Lodders et al. (2009)
Asplund et al. (2009)
Grevesse et al. (2007)
Asplund et al. (2005)
Grevesse & Sauval (1998)
Anders & Grevesse (1989)
Absolute
Original
If element ratio is in multiple catalogs:
Use the median
Use the mean
Exclude
Allow only
catalogs:
Abia et al. (2020)
Adamczak et al. (2013)
Adamow et al. (2014)
Adibekyan et al. (2012)
Adibekyan et al. (2015)
Adibekyan et al. (2016)
Allen et al. (2006)
Allen et al. (2011)
Allende Prieto et al. (2004)
Amarsi et al. (2019)
Baratella et al. (2021)
Battistini et al. (2015)
Battistini et al. (2016)
Baumann et al. (2010)
Bedell et al. (2017)
Bedell et al. (2018)
Behmard et al. (2023)
Bensby et al. (2005)
Bensby et al. (2014)
Bensby et al. (2018)
Bergemann et al. (2010)
Bertran de Lis et al. (2015)
Biazzo et al. (2012)
Biazzo et al. (2022)
Bodaghee et al. (2003)
Boesgaard et al. (2011)
Boesgaard et al. (2022)
Bond et al. 2008)] (2008)
Botelho et al. (2019)
Botelho et al. (2020)
Brauner et al. (2023)
Brewer et al. (2006)
Brewer et al. (2016)
Brewer et al. (2018)
Brugamyer et al. (2011)
Bruntt et al. (2012)
Burris et al. (2000)
Cadieux et al. (2022)
Caffau et al. (2011)
Caffau et al. (2015z)
Caffau et al. (2019)
Carlos et al. (2016)
Carlos et al. (2019)
Carretta et al. (2000)
Casamiquela et al. (2020)
Casamiquela et al. (2022)
Castro et al. (1997)
Castro et al. (1999)
Charbonnel et al. (2020)
Chavero et al. (2019)
Chavez & Lambert (2009)
Chen et al. (2000)
Chen et al. (2001)
Costa Silva et al. (2020)
Cowen et al. (2020)
D'Orazi et al. (2012)
da Silva et al. (2012)
da Silva et al. (2015)
Dantas et al. (2023)
de Castro et al. (2016)
Delgado Mena et al. (2010)
Delgado Mena et al. (2014)
Delgado Mena et al. (2015)
Delgado Mena et al. (2017)
Delgado Mena et al. (2021)
delPeloso et al. (2005)
Ecuvillon et al. (2004)
Ecuvillon et al. (2006)
Edvardsson et al. (1993)
Erspamer et al. (2003)
Feltzing et al. (1998)
Feltzing et al. (2007)
Fishlock et al. (2017)
Forsberg et al. (2019)
Forsberg et al. (2022)
Francois (1986)
Francois (1988)
Fuhrmann (1998)
Fulbright (2000)
Galeev et al. (2004)
Gebran et al. (2010)
Gebruers et al. (2021)
Gehren et al. (2004)
Gehren et al. (2006)
Gent et al. (2022)
Ghezzi et al. (2010z)
Gilli et al. (2006)
Gonzalez et al. (2001)
Gonzalez et al. (2007)
Gonzalez et al. (2010z)
Gonzalez et al. (2014)
Gonzalez et al. (2015)
Gonzalez Hernandez et al. (2010)
Gonzalez Hernandez et al. (2013)
Gratton et al. (2000)
Gratton et al. (2003)
Griffith et al. (2023)
Guerco et al. (2019)
Gustafsson et al. (1999)
Hansen et al. (2020)
Hawkins et al. (2020)
Hojjatpanah et al. (2019)
Huang et al. (2005)
Ishigaki et al. (2012)
Ishigaki et al. (2013)
Ishikawa et al. (2020)
Ishikawa et al. (2022)
Israelian et al. (2004)
Israelian et al. (2009)
Ivanyuk et al. (2017)
Jacobson et al. (2014)
Jofre et al. (2015)
Jofre et al. (2018)
Jonsell et al. (2005)
Jonsson et al. (2016)
Jorissen et al. (2019)
Kang et al. (2011)
Karinkuzhi & Goswami (2014)
Karinkuzhi & Goswami (2015)
Karinkuzhi et al. (2018)
Karinkuzhi et al. (2021)
Karinkuzhi et al. (2023)
Koch & Edvardsson (2002)
Kolecki & Wang (2022)
Kong et al. (2018)
Korotin et al. (2021)
Korotin et al. (2022)
Lagarde et al. (2024)
Laird (1985)
Lambert et al. (1991)
Lambert et al. (2004)
Li et al. (2022)
Limberg et al. (2021)
Liu et al. (2012)
Liu et al. (2014)
Liu et al. (2018)
Liu et al. (2020)
Lombardo et al. (2022)
Lopez-Valdivia et al. (2017)
Lucertini et al. (2022)
Luck (2015)
Luck (2017)
Luck (2018)
Luck & Heiter (2005)
Luck et al. (2006)
Luck et al. (2007)
Lyubimkov et al. (2012)
Lyubimkov et al. (2015)
Lyubimkov et al. (2019)
Maas & Pilachowski (2021)
Maas et al. (2016)
Maas et al. (2017)
Maas et al. (2022)
Mack et al. (2016)
Mahdi et al. (2016)
Maldonado et al. (2013)
Maldonado et al. (2015)
Maldonado et al. (2016)
Maldonado et al. (2018)
Maldonado et al. (2020)
Mallik et al. (2003)
Mann et al. (2013)
Martos et al. (2023)
Mashonkina & Romanovskaya (2022)
Mashonkina et al. (2007)
Mass et al. (2019)
Melendez et al. (2004)
Merle et al. (2016)
Mikolaitis et al. (2019)
Mishenina et al. (2003)
Mishenina et al. (2004)
Mishenina et al. (2008)
Mishenina et al. (2011)
Mishenina et al. (2012)
Mishenina et al. (2013)
Mishenina et al. (2015)
Mishenina et al. (2016)
Mishenina et al. (2017)
Mishenina et al. (2019z)
Mishenina et al. (2021)
Mishenina et al. (2022)
Montes et al. (2018)
Morel & Micela (2004)
Morel et al. (2021)
Mortier et al. (2013)
Moya et al. (2022)
Mucciarelli et al. (2022)
Nagar et al. (2019)
Nandakumar et al. (2022)
Nandakumar et al. 2023b)] (2023z)
Neves et al. (2009)
Niemczura et al. (2017)
Nissen & Schuster (1997)
Nissen & Schuster (2010)
Nissen & Schuster (2011)
Nissen et al. (2013)
Nissen et al. (2014)
Nissen et al. (2015)
Nissen et al. (2016)
Nissen et al. (2017)
Nissen et al. (2020)
Notsu et al. (2016)
Ou et al. (2020)
Pagano (2014)
Pavlenko et al. (2019)
Pereira et al. (2011)
Peterson et al. (2013)
Petigura et al. (2011)
Pilachowski & Pace (2015)
Polanski et al. (2022)
Ramaya et al. (2019)
Ramirez et al. (2007)
Ramirez et al. (2009)
Ramirez et al. (2012z)
Ramirez et al. (2013)
Ramirez et al. (2014z)
Recio Blanco et al. (2012)
Reddy et al. (2003)
Reddy et al. (2006)
Reggiani et al. (2017)
Reggiani et al. (2019)
Rice & Brewer (2020)
Roederer & Barklem (2018)
Roederer et al. (2014z)
Roederer et al. (2020)
Roederer et al. (2021)
Roederer et al. (2022)
Roriz et al. (2021)
Ryde et al. (2020)
Sadakane et al. (2002)
Santos et al. (2015)
Santos-Peral et al. (2023)
Schmidt et al. (2009)
Schuler et al. (2011)
Schuler et al. (2015)
Shan et al. (2021)
Shejeelammal et al. (2020)
Shetye et al. (2018)
Shetye et al. (2020)
Shetye et al. (2021)
Shi et al. (2004)
Shi et al. (2012)
Shi et al. (2018)
Sikora et al. (2019)
Sitnova et al. (2015)
Sitnova et al. (2018)
Sitnova et al. (2022)
Sneden et al. (2021)
Sneden et al. (2023)
Solakci et al. (2014)
Soto et al. (2018)
Souto et al. (2020)
Souto et al. (2022)
Spina et al. (2016z)
Spina et al. (2018)
Spina et al. (2021)
Stonkute et al. (2012)
Stonkute et al. (2013)
Stonkute et al. (2020)
Strassmeier et al. (2023)
Suarez-Andres et al. (2017)
Takeda (2021)
Takeda (2022z)
Takeda & Honda (2020)
Takeda et al. (2005z)
Takeda et al. (2007z)
Takeda et al. (2010)
Takeda et al. (2014)
Takeda et al. (2015)
Takeda et al. (2017)
Takeda et al. (2019)
Takeda et al. (2019z)
Takeda et al. (2020z)
Tautvaisiene et al. (2020)
Tautvaisiene et al. (2021)
Tautvaisiene et al. (2022)
Teske et al. (2014)
Thevenin (1998)
Thoren et al. (2004)
Tomkin et al. (1995)
Trevisan et al. (2011)
Trevisan et al. (2014)
Tucci Maia et al. (2016)
Unterborn et al. (2015)
Valenti & Fischer (2005)
Wang et al. (2011)
Woolf et al. (1995)
Woolf et al. (1999)
Woolf et al. (2005)
Woolf et al. (2006)
Woolf et al. (2009)
Woolf et al. (2020)
Wu et al. (2015)
Xu et al. (2022)
Yan et al. (2015)
Yan et al. (2016)
Zenoviene et al. (2014)
Zenoviene et al. (2015)
Zepeda et al. (2022)
Zhang & Zhao (2006)
Zhang et al. (2016z)
Zhao et al. (2002)
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stars by
HIP ID
HD ID
or full name:
Selected
352
stars.
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Stellar Data Table
Use stars plotted in the graph above
Use stars from a list of
HIP
HD
identifiers:
H
He
Li
Be
II
B
C
N
O
F
Ne
Na
Mg
Al
II
Si
II
P
S
Cl
Ar
K
Ca
II
Sc
II
Ti
II
V
II
Cr
II
Mn
II
Fe
Co
II
Ni
II
Cu
II
Zn
II
Ga
II
Ge
As
Se
Br
Kr
Rb
Sr
II
Y
II
Zr
II
Nb
II
Mo
II
Tc
Ru
II
Rh
Pd
Ag
Cd
In
II
Sn
Sb
Te
I
Xe
Cs
Ba
II
Lu
II
Hf
II
Ta
W
II
Re
II
Os
Ir
Pt
Au
Hg
II
Tl
Pb
II
Bi
Po
At
Rn
Fr
Ra
Lr
Rf
Db
Sg
Bh
Hs
Mt
Ds
Rg
Cn
Nh
Fl
Mc
Lv
Ts
Og
La
II
Ce
II
Pr
II
Nd
II
Pm
Sm
II
Eu
II
Gd
II
Tb
II
Dy
II
Ho
II
Er
II
Tm
II
Yb
II
Ac
Th
II
Pa
U
Np
Pu
Am
Cm
Bk
Cf
Es
Fm
Md
No
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