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API
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
Distance
X Position
Y Position
Z Position
Effective Temperature
log(g)
Spectral Type
Spectral Type Number
V Magnitude
B Magnitude
B-V
Proper Motion RA
Proper Motion Dec
U Velocity
V Velocity
W Velocity
Disk
Disk Number
Stellar Mass
Stellar Radius
Planet property:
Semi-Major Axis
Eccentricity
Orbital Inclination
Planet Mass
Planet Radius
Planet Letter
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
Distance
X Position
Y Position
Z Position
Effective Temperature
log(g)
Spectral Type
Spectral Type Number
V Magnitude
B Magnitude
B-V
Proper Motion RA
Proper Motion Dec
U Velocity
V Velocity
W Velocity
Disk
Disk Number
Stellar Mass
Stellar Radius
Planet property:
Semi-Major Axis
Eccentricity
Orbital Inclination
Planet Mass
Planet Radius
Planet Letter
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
Distance
X Position
Y Position
Z Position
Effective Temperature
log(g)
Spectral Type
Spectral Type Number
V Magnitude
B Magnitude
B-V
Proper Motion RA
Proper Motion Dec
U Velocity
V Velocity
W Velocity
Disk
Disk Number
Stellar Mass
Stellar Radius
Planet property:
Semi-Major Axis
Eccentricity
Orbital Inclination
Planet Mass
Planet Radius
Planet Letter
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
Distance
X Position
Y Position
Z Position
Effective Temperature
log(g)
Spectral Type
Spectral Type Number
V Magnitude
B Magnitude
B-V
Proper Motion RA
Proper Motion Dec
U Velocity
V Velocity
W Velocity
Disk
Disk Number
Stellar Mass
Stellar Radius
Planet property:
Semi-Major Axis
Eccentricity
Orbital Inclination
Planet Mass
Planet Radius
Planet Letter
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
Normalize the histogram
Solar normalization:
Grevesse & Sauval (1998)
Anders & Grevesse (1989)
Asplund et al. (2009)
Lodders et al. (2009)
Grevesse et al. (2007)
Asplund (2005)
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)
Alexeeva et al. (2023)
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)
Bergemann et al. (2017)
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. (2006; 2008)
Botelho et al. (2019)
Botelho et al. (2020)
Brady et al. (2024)
Brauner et al. (2023)
Brewer et al. (2006)
Brewer et al. (2016)
Brewer et al. (2016) - Repeat Observations 1
Brewer et al. (2018)
Brewer et al. (2018) - Repeat Observations 1
Brugamyer et al. (2011)
Bruntt et al. (2012)
Burris et al. (2000)
Cadieux et al. (2022)
Caffau et al. (2011)
Caffau et al. (2015a)
Caffau et al. (2015b)
Caffau et al. (2019)
Carlos et al. (2016)
Carlos et al. (2019)
Carretta et al. (2000)
Casali et al. (2020)
Casali et al. (2020) - Repeat Observations 1
Casamiquela et al. (2020)
Casamiquela et al. (2022)
Casamiquela et al. (2022) - Repeat Observations 1
Casamiquela et al. (2022) - Repeat Observations 2
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)
Chen et al. (2001) - Repeat Observations 1
Coelho et al. (2024)
Contursi et al. (2024)
Contursi et al. (2024) - Repeat Observations 1
Contursi et al. (2024) - Repeat Observations 2
Costa Silva et al. (2020)
Cowen et al. (2020)
Dantas et al. (2023)
da Silva et al. (2012)
da Silva et al. (2015)
da Silva et al. (2024)
de Brito Silva et al. (2024)
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)
Dencs et al. (2024)
Dimoff et al. (2024)
D'Orazi et al. (2012)
Ecuvillon et al. (2004)
Ecuvillon et al. (2006)
Edvardsson et al. (1993)
Erspamer et al. (2003)
Erspamer et al. (2003) - Repeat Observations 1
Feltzing et al. (2007)
Feltzing et al. (1998)
Fernandes de Melo et al. (2024)
Filomena et al. (2024)
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. (2010b)
Gilli et al. (2006)
Gonzalez et al. (2001)
Gonzalez et al. (2001) - Repeat Observations 1
Gonzalez et al. (2007)
Gonzalez et al. (2010a)
Gonzalez et al. (2010b)
Gonzalez et al. (2010b) - Repeat Observations 1
Gonzalez et al. (2014)
Gonzalez et al. (2015)
Gonzalez et al. (2015) - Repeat Observations 1
Gonzalez Hernandez et al. (2010)
Gonzalez Hernandez et al. (2013)
Gratton et al. (2000)
Gratton et al. (2003)
Griffith et al. (2023)
Grilo et al. (2024)
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)
Jahandar et al. (2024a)
Jahandar et al. (2024b)
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. (2022)
Korotin et al. (2021)
Lagarde et al. (2024)
Laird (1985)
Lambert et al. (2004)
Lambert et al. (1991)
Li et al. (2022)
Limberg et al. (2021)
Liu et al. (2012)
Liu et al. (2014)
Liu et al. (2018)
Liu et al. (2020)
Liu et al. (2020) - Repeat Observations 1
Lombardo et al. (2022)
Lopez-Valdivia et al. (2017)
Lopez-Valdivia et al. (2024)
Lucertini et al. (2022)
Luck & Heiter (2005)
Luck & Heiter (2005) - Repeat Observations 1
Luck et al. (2006)
Luck et al. (2007)
Luck (2015)
Luck (2015) - Repeat Observations 1
Luck (2017)
Luck (2017) - Repeat Observations 1
Luck (2018)
Lyubimkov et al. (2012)
Lyubimkov et al. (2015)
Lyubimkov et al. (2019)
Maas et al. (2016)
Maas et al. (2017)
Mass et al. (2019)
Mass et al. (2019) - Repeat Observations 1
Maas & Pilachowski (2021)
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)
Martos et al. (2023) - Repeat Observations 1
Mashonkina et al. (2007)
Mashonkina & Romanovskaya (2022)
Melendez et al. (2004)
Melo et al. (2024)
Merle et al. (2016)
Mikolaitis et al. (2019)
Mikolaitis et al. (2019) - Repeat Observations 1
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. (2015) - Repeat Observations 1
Mishenina et al. (2016)
Mishenina et al. (2016) - Repeat Observations 1
Mishenina et al. (2017)
Mishenina et al. (2019a)
Mishenina et al. (2019b)
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)
Moya et al. (2022) - Repeat Observations 1
Mucciarelli et al. (2022)
Nagar et al. (2019)
Nandakumar et al. (2022)
Nandakumar et al. (2023a; 2023b)
Nandakumar et al. (2024a; 2024b)
Nelson et al. (2024)
Nelson et al. (2024) - Repeat Observations 1
Neves et al. (2009)
Niemczura et al. (2015)
Niemczura et al. (2017)
Nissen & Schuster (2010)
Nissen & Schuster (2010) - Repeat Observations 1
Nissen & Schuster (2011)
Nissen & Schuster (2011) - Repeat Observations 1
Nissen et al. (2013)
Nissen et al. (2014)
Nissen et al. (2015)
Nissen et al. (2016)
Nissen et al. (2017)
Nissen et al. (2020)
Nissen et al. (2024)
Nissen & Schuster (1997)
Notsu et al. (2016)
Ou et al. (2020)
Ou et al. (2020) - Repeat Observations 1
Ou et al. (2020) - Repeat Observations 2
Pagano (2014)
Pavlenko et al. (2019)
Pereira et al. (2011)
Peterson et al. (2013)
Petigura et al. (2011)
Petigura et al. (2011) - Repeat Observations 1
Pilachowski & Pace (2015)
Plotnikova et al. (2024)
Plotnikova et al. (2024) - Repeat Observations 1
Polanski et al. (2022)
Pozhath and Lambert (2024)
Ramirez et al. (2007)
Ramirez et al. (2009)
Ramirez et al. (2012a)
Ramirez et al. (2012b)
Ramirez et al. (2013)
Ramirez et al. (2014a)
Ramirez et al. (2014b)
Ramaya et al. (2019)
Recio Blanco et al. (2012)
Reddy et al. (2003)
Reddy et al. (2006)
Reggiani et al. (2017)
Reggiani et al. (2019)
Rice & Brewer (2020)
Rice & Brewer (2020) - Repeat Observations 1
Rice & Brewer (2020) - Repeat Observations 2
Roederer et al. (2014a)
Roederer et al. (2014b)
Roederer & Barklem (2018)
Roederer et al. (2020)
Roederer et al. (2021)
Roederer et al. (2022)
Roriz et al. (2021a; 2021b)
Roriz et al. (2024)
Ryde et al. (2020)
Sadakane et al. (2002)
Santos-Peral et al. (2023)
Santos et al. (2015)
Santos et al. (2015) - Repeat Observations 1
Schmidt et al. (2009)
Schuler et al. (2011)
Schuler et al. (2015)
Shan et al. (2021)
Shejeelammal et al. (2020)
Shejeelammal et al. (2024)
Sheminova et al. (2024)
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)
Soto et al. (2018) - Repeat Observations 1
Soto et al. (2018) - Repeat Observations 2
Soto et al. (2018) - Repeat Observations 3
Souto et al. (2020)
Souto et al. (2022)
Spina et al. (2016b)
Spina et al. (2018)
Spina et al. (2021)
Spina et al. (2021) - Repeat Observations 1
Spite et al. (2022)
Spite et al. (2024)
Stonkute et al. (2012)
Stonkute et al. (2013)
Stonkute et al. (2020)
Strassmeier et al. (2023)
Suarez-Andres et al. (2017)
Sun et al. (2024)
Tabernero et al. (2024)
Takeda et al. (2005c)
Takeda et al. (2005d)
Takeda et al. (2005f)
Takeda et al. (2007d)
Takeda et al. (2007f)
Takeda et al. (2010)
Takeda et al. (2014)
Takeda et al. (2015)
Takeda et al. (2017)
Takeda et al. (2019)
Takeda et al. (2019b)
Takeda et al. (2020a)
Takeda & Honda (2020)
Takeda (2021)
Takeda (2022a)
Takeda (2022b)
Tautvaisiene et al. (2020)
Tautvaisiene et al. (2021)
Tautvaisiene et al. (2022)
Teske et al. (2014)
Thevenin (1998)
Thevenin (1998) - Repeat Observations 1
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)
Valenti & Fischer (2005) - Repeat Observations 1
Vernekar et al. (2024)
Vitali et al. (2024)
Wang et al. (2011)
Woolf et al. (2005)
Woolf et al. (2006)
Woolf et al. (2009)
Woolf et al. (2020)
Woolf et al. (2020) - Repeat Observations 1
Woolf et al. (1995)
Woolf et al. (1999)
Wu et al. (2015)
Xu et al. (2022)
Yan et al. (2015)
Yan et al. (2016)
Yan et al. (2016) - Repeat Observations 1
Yang et al. (2024)
Zenoviene et al. (2014)
Zenoviene et al. (2015)
Zepeda et al. (2022)
Zhang & Zhao (2006)
Zhang et al. (2016ab)
Zhao et al. (2002)
Exclude
Allow only
stars by
any
SIMBAD
name.
Selected
352
stars.
Clear selection
Show gridlines
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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