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Simple Target List Of Targets Fast Xmatch with large catalogs or Simbad

Target Name (resolved by Sesame) or Position:	Target dimension:
NB: The epoch used for the query is the original epoch of the table(s)	Radius Box size

	J/A+A/713/A60	692		High radial velocity stars abundances (Alazzawi+, 2026) ReadMe+ftp 2026A&A...713A..60A Similar Catalogs Post annotation
1.	J/A+A/713/A60/stars		^(c)List of studied stars (16 rows) metaJ/A+A/713/A60/stars
2.	J/A+A/713/A60/abund		Stellar parameters and abundances for every element/ion measured (16 rows) metaJ/A+A/713/A60/abund

Simple Constraint List Of Constraints

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Column

Constraint

Explain (UCD)

(ALL)

recno

Record number assigned by the VizieR team. Should Not be used for identification. (meta.record)

(ALL)

Star

(char)

Star identifier, as used in the paper (meta.id;meta.main)

(1)

RAJ2000

"h:m:s"

⁽ⁱ⁾ Simbad right ascension (J2000) (pos.eq.ra;meta.main)

(1)

DEJ2000

"d:m:s"

⁽ⁱ⁾ Simbad declination (J2000) (pos.eq.dec;meta.main)

(1)

FileName

(char)

Name of the table with linelist of the star in subdirectory linelist (meta.id;meta.table)

(1)

SName

(char)

Simbad name (meta.id)

(1)

Simbad

(char)

ask the Simbad data-base about this object (meta.ref.url) (DATA_LINK)

(2)

Teff

Adopted effective temperature (phys.temperature.effective)

(2)

logg

[cm/s2]

Adopted surface gravity (phys.gravity)

(2)

vturb

km/s

Microturbulent velocity, xi (phys.veloc)

(2)

[Fe/H]

Derived metallicity from FeI lines (phys.abund)

ALL cols

⁽ⁱ⁾indexed column

(2)

o_O

⁽ⁿ⁾ Number of individual spectral lines used to derive the abundance of [OI] forbidden line (meta.number)

(2)

A(O)

⁽ⁿ⁾ Mean abundance log(N(O)/N(H))+12 (phys.abund)

(2)

[O/H]

⁽ⁿ⁾ Abundance relative to the Sun, A(O)-A(O)_{sun} (phys.abund)

(2)

s_O

⁽ⁿ⁾ Line-to-line scatter (standard deviation) of A(O) over the number of lines used (Note 1) (phys.atmol.number)

(2)

o_NaI

⁽ⁿ⁾ Number of individual spectral lines used to derive the abundance of NaI (meta.number)

(2)

A(NaI)

⁽ⁿ⁾ Mean abundance log(N(NaI)/N(H))+12 (phys.abund)

(2)

[NaI/H]

⁽ⁿ⁾ Abundance relative to the Sun, A(NaI)-A(NaI)_{sun} (phys.abund)

(2)

s_NaI

⁽ⁿ⁾ Line-to-line scatter (standard deviation) of A(NaI) over the number of lines used (Note 1) (phys.atmol.number)

(2)

o_MgI

Number of individual spectral lines used to derive the abundance of MgI (meta.number)

(2)

A(MgI)

Mean abundance log(N(MgI)/N(H))+12 (phys.abund)

(2)

[MgI/H]

Abundance relative to the Sun, A(MgI)-A(MgI)_{sun} (phys.abund)

(2)

s_MgI

⁽ⁿ⁾ Line-to-line scatter (standard deviation) of A(MgI) over the number of lines used (Note 1) (phys.atmol.number)

(2)

o_AlI

⁽ⁿ⁾ Number of individual spectral lines used to derive the abundance of AlI (meta.number)

ALL cols

⁽ⁿ⁾ indicates a possible blank or NULL column

⁽ⁱ⁾indexed column

(2)

A(AlI)

⁽ⁿ⁾ Mean abundance log(N(AlI)/N(H))+12 (phys.abund)

(2)

[AlI/H]

⁽ⁿ⁾ Abundance relative to the Sun, A(AlI)-A(AlI)_{sun} (phys.abund)

(2)

s_AlI

⁽ⁿ⁾ Line-to-line scatter (standard deviation) of A(AlI) over the number of lines used (Note 1) (phys.atmol.number)

(2)

o_SiI

Number of individual spectral lines used to derive the abundance of SiI (meta.number)

(2)

A(SiI)

Mean abundance log(N(SiI)/N(H))+12 (phys.abund)

(2)

[SiI/H]

Abundance relative to the Sun, A(SiI)-A(SiI)_{sun} (phys.abund)

(2)

s_SiI

Line-to-line scatter (standard deviation) of A(SiI) over the number of lines used (Note 1) (phys.atmol.number)

(2)

o_CaI

Number of individual spectral lines used to derive the abundance of CaI (meta.number)

(2)

A(CaI)

Mean abundance log(N(CaI)/N(H))+12 (phys.abund)

(2)

[CaI/H]

Abundance relative to the Sun, A(CaI)-A(CaI)_{sun} (phys.abund)

(2)

s_CaI

Line-to-line scatter (standard deviation) of A(CaI) over the number of lines used (Note 1) (phys.atmol.number)

(2)

o_ScII

Number of individual spectral lines used to derive the abundance of ScII (meta.number)

(2)

A(ScII)

Mean abundance log(N(ScII)/N(H))+12 (phys.abund)

ALL cols

⁽ⁿ⁾ indicates a possible blank or NULL column

⁽ⁱ⁾indexed column

(2)

[ScII/H]

Abundance relative to the Sun, A(ScII)-A(ScII)_{sun} (phys.abund)

(2)

s_ScII

Line-to-line scatter (standard deviation) of A(ScII) over the number of lines used (Note 1) (phys.atmol.number)

(2)

o_TiI

Number of individual spectral lines used to derive the abundance of TiI (meta.number)

(2)

A(TiI)

Mean abundance log(N(TiI)/N(H))+12 (phys.abund)

(2)

[TiI/H]

Abundance relative to the Sun, A(TiI)-A(TiI)_{sun} (phys.abund)

(2)

s_TiI

Line-to-line scatter (standard deviation) of A(TiI) over the number of lines used (Note 1) (phys.atmol.number)

(2)

o_TiII

Number of individual spectral lines used to derive the abundance of TiII (meta.number)

(2)

A(TiII)

Mean abundance log(N(TiII)/N(H))+12 (phys.abund)

(2)

[TiII/H]

Abundance relative to the Sun, A(TiII)-A(TiII)_{sun} (phys.abund)

(2)

s_TiII

Line-to-line scatter (standard deviation) of A(TiII) over the number of lines used (Note 1) (phys.atmol.number)

(2)

o_VI

Number of individual spectral lines used to derive the abundance of VI (meta.number)

(2)

A(VI)

Mean abundance log(N(VI)/N(H))+12 (phys.abund)

(2)

[VI/H]

Abundance relative to the Sun, A(VI)-A(VI)_{sun} (phys.abund)

ALL cols

⁽ⁿ⁾ indicates a possible blank or NULL column

⁽ⁱ⁾indexed column

(2)

s_VI

Line-to-line scatter (standard deviation) of A(VI) over the number of lines used (Note 1) (phys.atmol.number)

(2)

o_CrI

Number of individual spectral lines used to derive the abundance of CrI (meta.number)

(2)

A(CrI)

Mean abundance log(N(CrI)/N(H))+12 (phys.abund)

(2)

[CrI/H]

Abundance relative to the Sun, A(CrI)-A(CrI)_{sun} (phys.abund)

(2)

s_CrI

Line-to-line scatter (standard deviation) of A(CrI) over the number of lines used (Note 1) (phys.atmol.number)

(2)

o_CrII

Number of individual spectral lines used to derive the abundance of CrII (meta.number)

(2)

A(CrII)

Mean abundance log(N(CrII)/N(H))+12 (phys.abund)

(2)

[CrII/H]

Abundance relative to the Sun, A(CrII)-A(CrII)_{sun} (phys.abund)

(2)

s_CrII

⁽ⁿ⁾ Line-to-line scatter (standard deviation) of A(CrII) over the number of lines used (Note 1) (phys.atmol.number)

(2)

o_MnI

Number of individual spectral lines used to derive the abundance of MnI (meta.number)

(2)

A(MnI)

Mean abundance log(N(MnI)/N(H))+12 (phys.abund)

(2)

[MnI/H]

Abundance relative to the Sun, A(MnI)-A(MnI)_{sun} (phys.abund)

(2)

s_MnI

Line-to-line scatter (standard deviation) of A(MnI) over the number of lines used (Note 1) (phys.atmol.number)

ALL cols

⁽ⁿ⁾ indicates a possible blank or NULL column

⁽ⁱ⁾indexed column

(2)

o_FeII

Number of individual spectral lines used to derive the abundance of FeII (meta.number)

(2)

A(FeII)

Mean abundance log(N(FeII)/N(H))+12 (phys.abund)

(2)

[FeII/H]

Abundance relative to the Sun, A(FeII)-A(FeII)_{sun} (phys.abund)

(2)

s_FeII

Line-to-line scatter (standard deviation) of A(FeII) over the number of lines used (Note 1) (phys.atmol.number)

(2)

o_CoI

Number of individual spectral lines used to derive the abundance of CoI (meta.number)

(2)

A(CoI)

Mean abundance log(N(CoI)/N(H))+12 (phys.abund)

(2)

[CoI/H]

Abundance relative to the Sun, A(CoI)-A(CoI)_{sun} (phys.abund)

(2)

CoI

Line-to-line scatter (standard deviation) of A(CoI) over the number of lines used (Note 1) (phys.atmol.number)

(2)

o_NiI

Number of individual spectral lines used to derive the abundance of NiI (meta.number)

(2)

A(NiI)

Mean abundance log(N(NiI)/N(H))+12 (phys.abund)

(2)

[NiI/H]

Abundance relative to the Sun, A(NiI)-A(NiI)_{sun} (phys.abund)

(2)

s_NiI

Line-to-line scatter (standard deviation) of A(NiI) over the number of lines used (Note 1) (phys.atmol.number)

(2)

o_CuI

⁽ⁿ⁾ Number of individual spectral lines used to derive the abundance of CuI (meta.number)

ALL cols

⁽ⁿ⁾ indicates a possible blank or NULL column

⁽ⁱ⁾indexed column

(2)

A(CuI)

⁽ⁿ⁾ Mean abundance log(N(CuI)/N(H))+12 (phys.abund)

(2)

[CuI/H]

⁽ⁿ⁾ Abundance relative to the Sun, A(CuI)-A(CuI)_{sun} (phys.abund)

(2)

s_CuI

⁽ⁿ⁾ Line-to-line scatter (standard deviation) of A(CuI) over the number of lines used (Note 1) (phys.atmol.number)

(2)

o_ZnI

Number of individual spectral lines used to derive the abundance of ZnI (meta.number)

(2)

A(ZnI)

Mean abundance log(N(ZnI)/N(H))+12 (phys.abund)

(2)

[ZnI/H]

Abundance relative to the Sun, A(ZnI)-A(ZnI)_{sun} (phys.abund)

(2)

s_ZnI

⁽ⁿ⁾ Line-to-line scatter (standard deviation) of A(ZnI) over the number of lines used (Note 1) (phys.atmol.number)

(2)

o_YII

Number of individual spectral lines used to derive the abundance of YII (meta.number)

(2)

A(YII)

Mean abundance log(N(YII)/N(H))+12 (phys.abund)

(2)

[YII/H]

Abundance relative to the Sun, A(YII)-A(YII)_{sun} (phys.abund)

(2)

s_YII

Line-to-line scatter (standard deviation) of A(YII) over the number of lines used (Note 1) (phys.atmol.number)

(2)

o_ZrII

Number of individual spectral lines used to derive the abundance of ZrII (meta.number)

(2)

A(ZrII)

Mean abundance log(N(ZrII)/N(H))+12 (phys.abund)

ALL cols

⁽ⁿ⁾ indicates a possible blank or NULL column

⁽ⁱ⁾indexed column

(2)

[ZrII/H]

Abundance relative to the Sun, A(ZrII)-A(ZrII)_{sun} (phys.abund)

(2)

s_ZrII

⁽ⁿ⁾ Line-to-line scatter (standard deviation) of A(ZrII) over the number of lines used (Note 1) (phys.atmol.number)

(2)

o_MoI

⁽ⁿ⁾ Number of individual spectral lines used to derive the abundance of MoI (meta.number)

(2)

A(MoI)

⁽ⁿ⁾ Mean abundance log(N(MoI)/N(H))+12 (phys.abund)

(2)

[MoI/H]

⁽ⁿ⁾ Abundance relative to the Sun, A(MoI)-A(MoI)_{sun} (phys.abund)

(2)

s_MoI

⁽ⁿ⁾ Line-to-line scatter (standard deviation) of A(MoI) over the number of lines used (Note 1) (phys.atmol.number)

(2)

o_BaII

Number of individual spectral lines used to derive the abundance of BaII (meta.number)

(2)

A(BaII)

Mean abundance log(N(BaII)/N(H))+12 (phys.abund)

(2)

[BaII/H]

Abundance relative to the Sun, A(BaII)-A(BaII)_{sun} (phys.abund)

(2)

s_BaII

⁽ⁿ⁾ Line-to-line scatter (standard deviation) of A(BaII) over the number of lines used (Note 1) (phys.atmol.number)

(2)

o_LaII

Number of individual spectral lines used to derive the abundance of LaII (meta.number)

(2)

A(LaII)

Mean abundance log(N(LaII)/N(H))+12 (phys.abund)

(2)

[LaII/H]

Abundance relative to the Sun, A(LaII)-A(LaII)_{sun} (phys.abund)

ALL cols

⁽ⁿ⁾ indicates a possible blank or NULL column

⁽ⁱ⁾indexed column

(2)

s_LaII

Line-to-line scatter (standard deviation) of A(LaII) over the number of lines used (Note 1) (phys.atmol.number)

(2)

o_CeII

Number of individual spectral lines used to derive the abundance of CeII (meta.number)

(2)

A(CeII)

Mean abundance log(N(CeII)/N(H))+12 (phys.abund)

(2)

[CeII/H]

Abundance relative to the Sun, A(CeII)-A(CeII)_{sun} (phys.abund)

(2)

s_CeII

⁽ⁿ⁾ Line-to-line scatter (standard deviation) of A(CeII) over the number of lines used (Note 1) (phys.atmol.number)

(2)

o_PrII

⁽ⁿ⁾ Number of individual spectral lines used to derive the abundance of PrII (meta.number)

(2)

A(PrII)

⁽ⁿ⁾ Mean abundance log(N(PrII)/N(H))+12 (phys.abund)

(2)

[PrII/H]

⁽ⁿ⁾ Abundance relative to the Sun, A(PrII)-A(PrII)_{sun} (phys.abund)

(2)

s_PrII

⁽ⁿ⁾ Line-to-line scatter (standard deviation) of A(PrII) over the number of lines used (Note 1) (phys.atmol.number)

(2)

o_NdII

Number of individual spectral lines used to derive the abundance of NdII (meta.number)

(2)

A(NdII)

Mean abundance log(N(NdII)/N(H))+12 (phys.abund)

(2)

[NdII/H]

Abundance relative to the Sun, A(NdII)-A(NdII)_{sun} (phys.abund)

(2)

s_NdII

Line-to-line scatter (standard deviation) of A(NdII) over the number of lines used (Note 1) (phys.atmol.number)

ALL cols

⁽ⁿ⁾ indicates a possible blank or NULL column

⁽ⁱ⁾indexed column

(2)

o_SmII

Number of individual spectral lines used to derive the abundance of SmII (meta.number)

(2)

A(SmII)

Mean abundance log(N(SmII)/N(H))+12 (phys.abund)

(2)

[SmII/H]

Abundance relative to the Sun, A(SmII)-A(SmII)_{sun} (phys.abund)

(2)

s_SmII

⁽ⁿ⁾ Line-to-line scatter (standard deviation) of A(SmII) over the number of lines used (Note 1) (phys.atmol.number)

(2)

o_EuII

Number of individual spectral lines used to derive the abundance of EuII (meta.number)

(2)

A(EuII)

Mean abundance log(N(EuII)/N(H))+12 (phys.abund)

(2)

[EuII/H]

⁽ⁿ⁾ Abundance relative to the Sun, A(EuII)-A(EuII)_{sun} (phys.abund)

(2)

s_EuII

⁽ⁿ⁾ Line-to-line scatter (standard deviation) of A(EuII) over the number of lines used (Note 1) (phys.atmol.number)

ALL cols

⁽ⁿ⁾ indicates a possible blank or NULL column

⁽ⁱ⁾indexed column

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If the access to catalogues with VizieR was helpful for your research work,the following acknowledgment would be appreciated: This research has made use of the VizieR catalogue access tool, CDS, Strasbourg, France (DOI: 10.26093/cds/vizier). The original description of the VizieR service was published in A&AS 143, 23