VizieR

JavaScript is used, and should be enabled to get full functionality.

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/683/A72	1132		Gaia RVS benchmark stars. II. (Caffau+, 2024) ReadMe+ftp 2024A&A...683A..72C Similar Catalogs Post annotation
1.	J/A+A/683/A72/rvs		Abundances of the stellar sample (43 rows) metaJ/A+A/683/A72/rvs

Simple Constraint List Of Constraints

Query by Constraints constraints help

constraints help

applied on Columns (Output Order: + - )

Show

Sort

Column

Constraint

Explain (UCD)

recno

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

Name

(char)

Name of the star as in the paper (RVSNNN) (meta.id;meta.main)

GaiaDR3

GaiaDR3 source_id (meta.id)

Star

(char)

Internal star name (meta.id)

Teff

K

Effective temperature (phys.temperature.effective)

logg

Surface gravity (phys.gravity)

micro

km/s

Microturbulence (phys.veloc.microTurb)

[Fe/H]

Metallicity (phys.abund.Z)

C1fit

⁽ⁿ⁾ [C/H]=A(C)-A(C)sun derived from fit of the Gband, with A(C)sun=8.50 (phys.abund)

s_C1fit

Uncertainty in the C abundance (stat.error;phys.abund)

C1fitFe

⁽ⁿ⁾ [CI/Fe] abundance (phys.abund)

ALL cols

⁽ⁿ⁾ indicates a possible blank or NULL column

⁽ⁱ⁾indexed column

NC1fit

[0/1] Number of C lines (meta.number)

O1fit

⁽ⁿ⁾ [O/H]=A(O)-A(O)sun derived from fit of the Gband, with A(O)sun=8.76 (phys.abund)

s_O1fit

Line-to-line scatter of O (stat.error)

O1fitFe

⁽ⁿ⁾ [OI/Fe] abundance (phys.abund)

NO1fit

[0/2] Number of OI lines (meta.number)

Na1nlte

⁽ⁿ⁾ [Na/H]=A(Na)-A(Na)sun with A(Na)sun=6.30 (phys.abund)

s_Na1nlte

Line-to-line scatter of Na (stat.error)

Na1nlteFe

⁽ⁿ⁾ [NaI/Fe] abundance (phys.abund)

NNa1nlte

[0/2] Number of NaI lines (meta.number)

corNLTENa1

NLTE correction for NaI (arith.factor)

Mg1

⁽ⁿ⁾ [Mg/H]=A(Mg)-A(Mg)sun with A(Mg)sun=7.54 (phys.abund)

s_Mg1

Line-to-line scatter of MgI (stat.error)

Mg1Fe

⁽ⁿ⁾ [MgI/Fe] abundance (phys.abund)

ALL cols

⁽ⁿ⁾ indicates a possible blank or NULL column

⁽ⁱ⁾indexed column

NMg1

[0/12] Number of MgI lines (meta.number)

Al1

⁽ⁿ⁾ [Al/H]=A(Al)-A(Al)sun with A(Al)sun=6.47 (phys.abund)

s_Al1

Line-to-line scatter of AlI (stat.error)

Al1Fe

⁽ⁿ⁾ [AlI/Fe] abundance (phys.abund)

NAl1

[0/6] Number of AlI lines (meta.number)

Si1

⁽ⁿ⁾ [Si/H]=A(Si)-A(Si)sun with A(Si)sun=7.52 (phys.abund)

s_Si1

Line-to-line scatter of SiI (stat.error)

Si1Fe

⁽ⁿ⁾ [SiI/Fe] abundance (phys.abund)

NSi1

[0/27] Number of SiI lines (meta.number)

S1nlte

⁽ⁿ⁾ [S/H]=A(S)-A(S)sun with A(S)sun=7.16 (phys.abund)

s_S1nlte

Line-to-line scatter of SI (stat.error)

S1nlteFe

⁽ⁿ⁾ [SI/Fe] abundance (phys.abund)

NS1nlte

[0/2] Number of SI lines (meta.number)

ALL cols

⁽ⁿ⁾ indicates a possible blank or NULL column

⁽ⁱ⁾indexed column

corNLTES1

NLTE correction for SI (arith.factor)

K1fit

⁽ⁿ⁾ [K/H]=A(K)-A(K)sun with A(K)sun=5.11 (phys.abund)

s_K1fit

[0/0] Line-to-line scatter of KI (stat.error)

K1fitFe

⁽ⁿ⁾ [KI/Fe] abundance (phys.abund)

NK1fit

[0/1] Number of KI lines (meta.number)

Ca1nlte

⁽ⁿ⁾ [Ca/H]=A(Ca)-A(Ca)sun with A(Ca)sun=6.33 (phys.abund)

s_Ca1nlte

Line-to-line scatter of CaI (stat.error)

Ca1nlteFe

⁽ⁿ⁾ [CaI/Fe] abundance (phys.abund)

NCa1nlte

[4/24] Number of CaI lines (meta.number)

corNLTECa1

[0.04/0.3] NLTE correction for CaI (arith.factor)

Sc1

⁽ⁿ⁾ [ScI/H]=A(ScI)-A(Sc)sun with A(Sc)sun=3.10 (phys.abund)

s_Sc1

Line-to-line scatter of ScI (stat.error)

Sc1Fe

⁽ⁿ⁾ [ScI/Fe] abundance (phys.abund)

ALL cols

⁽ⁿ⁾ indicates a possible blank or NULL column

⁽ⁱ⁾indexed column

NSc1

[0/2] Number of ScI lines (meta.number)

Sc2

⁽ⁿ⁾ [ScII/H]=A(ScII)-A(Sc)sun with A(Sc)sun=3.10 (phys.abund)

s_Sc2

Line-to-line scatter of ScII (stat.error)

Sc2Fe

⁽ⁿ⁾ [ScII/Fe] abundance (phys.abund)

NSc2

[0/4] Number of ScII lines (meta.number)

Ti1

⁽ⁿ⁾ [TiI/H]=A(TiI)-A(Ti)sun with A(Ti)sun=4.90 (phys.abund)

s_Ti1

Line-to-line scatter of TiI (stat.error)

Ti1Fe

⁽ⁿ⁾ [TiI/Fe] abundance (phys.abund)

NTi1

[0/48] Number of TiI lines (meta.number)

Ti2

⁽ⁿ⁾ [TiII/H]=A(TiII)-A(Ti)sun with A(Ti)sun=4.90 (phys.abund)

s_Ti2

Line-to-line scatter of TiII (stat.error)

Ti2Fe

⁽ⁿ⁾ [TiII/Fe] abundance (phys.abund)

NTi2

[1/33] Number of TiII lines (meta.number)

ALL cols

⁽ⁿ⁾ indicates a possible blank or NULL column

⁽ⁱ⁾indexed column

V1

⁽ⁿ⁾ [VI/H]=A(VI)-A(V)sun with A(V)sun=4.00 (phys.abund)

s_V1

Line-to-line scatter of VI (stat.error)

V1Fe

⁽ⁿ⁾ [VI/Fe] abundance (phys.abund)

NV1

[0/19] Number of VI lines (meta.number)

V2

⁽ⁿ⁾ [VII/H]=A(VII)-A(Vc)sun with A(V)sun=4.00 (phys.abund)

s_V2

Line-to-line scatter of VII (stat.error)

V2Fe

⁽ⁿ⁾ [V/Fe] abundance (phys.abund)

NV2

[0/5] Number of VII lines (meta.number)

Cr1

⁽ⁿ⁾ [CrI/H]=A(CrI)-A(Cr)sun with A(Cr)sun=5.64 (phys.abund)

s_Cr1

Line-to-line scatter of CrI (stat.error)

Cr1Fe

⁽ⁿ⁾ [CrI/Fe] abundance (phys.abund)

NCr1

[1/18] Number of CrI lines (meta.number)

Cr2

⁽ⁿ⁾ [CrII/H]=A(CrII)-A(Cr)sun with A(Cr)sun=5.64 (phys.abund)

ALL cols

⁽ⁿ⁾ indicates a possible blank or NULL column

⁽ⁱ⁾indexed column

s_Cr2

Line-to-line scatter of CrII (stat.error)

Cr2Fe

⁽ⁿ⁾ [CrII/Fe] abundance (phys.abund)

NCr2

[0/4] Number of CrII lines (meta.number)

Mn1nlte3d

⁽ⁿ⁾ [MnI/H]=A(MnI)-A(Mn)sun with A(Mn)sun=5.37 (phys.abund)

s_Mn1nlte3d

Line-to-line scatter of MnI (stat.error)

Mn1nlte3dFe

⁽ⁿ⁾ [Mn/Fe] abundance (phys.abund)

NMn1nlte3d

[0/14] Number of MnI lines (meta.number)

corNLTEMn13d

(char)

NLTE correction for MnI (arith.factor)

Mn2

⁽ⁿ⁾ [MnII/H]=A(MnII)-A(Mn)sun with A(Mn)sun=5.37 (phys.abund)

s_Mn2

Line-to-line scatter of MnII (stat.error)

Mn2Fe

⁽ⁿ⁾ [MnII/Fe] abundance (phys.abund)

NMn2

[0/1] Number of MnII lines (meta.number)

Fe1

⁽ⁿ⁾ [FeI/H]=A(FeI)-A(Fe)sun with A(Fe)sun=8.52 (phys.abund)

ALL cols

⁽ⁿ⁾ indicates a possible blank or NULL column

⁽ⁱ⁾indexed column

s_Fe1

Line-to-line scatter of FeI (stat.error)

Fe1Fe

[0/0] [FeI/Fe] abundance (phys.abund)

NFe1

[9/263] Number of FeI lines (meta.number)

Fe2

⁽ⁿ⁾ FeII/H]=A(FeII)-A(Fe)sun with A(Fe)sun=8.52 (phys.abund)

s_Fe2

Line-to-line scatter of FeII (stat.error)

Fe2Fe

⁽ⁿ⁾ [FeII/Fe] abundance (phys.abund)

NFe2

[0/24] Number of FeII lines (meta.number)

Co1

⁽ⁿ⁾ [CoI/H]=A(CoI)-A(Co)sun with A(Fe)sun=4.92 (phys.abund)

s_Co1

Line-to-line scatter of CoI (stat.error)

Co1Fe

⁽ⁿ⁾ [CoI/Fe] abundance (phys.abund)

NCo1

[0/15] Number of CoI lines (meta.number)

Ni1

⁽ⁿ⁾ [NiI/H]=A(NiI)-A(Ni)sun with A(Ni)sun=6.23 (phys.abund)

s_Ni1

Line-to-line scatter of NiI (stat.error)

ALL cols

⁽ⁿ⁾ indicates a possible blank or NULL column

⁽ⁱ⁾indexed column

Ni1Fe

⁽ⁿ⁾ [NiI/Fe] abundance (phys.abund)

NNi1

[0/45] Number of NiI lines (meta.number)

Cu1

⁽ⁿ⁾ [CuI/H]=A(CuI)-A(Cu)sun with A(Cu)sun=4.21 (phys.abund)

s_Cu1

Line-to-line scatter of CuI (stat.error)

Cu1Fe

⁽ⁿ⁾ [CuI/Fe] abundance (phys.abund)

NCu1

[0/2] Number of CuI lines (meta.number)

Zn1nlte

⁽ⁿ⁾ [ZnI/H]=A(ZnI)-A(Zn)sun with A(Zn)sun=4.62 (phys.abund)

s_Zn1nlte

Line-to-line scatter of ZnI (stat.error)

Zn1nlteFe

⁽ⁿ⁾ [ZnI/Fe] abundance (phys.abund)

NZn1nlte

[0/2] Number of ZnI lines (meta.number)

corNLTEZn1

NLTE correction for ZnI (arith.factor)

Sr1

⁽ⁿ⁾ [SrI/H]=A(SrI)-A(Sr)sun with A(Sr)sun=2.92 (phys.abund)

s_Sr1

Line-to-line scatter of SrI (stat.error)

ALL cols

⁽ⁿ⁾ indicates a possible blank or NULL column

⁽ⁱ⁾indexed column

Sr1Fe

⁽ⁿ⁾ [SrI/Fe] abundance (phys.abund)

NSr1

[0/1] Number of SrI lines (meta.number)

Y2

⁽ⁿ⁾ [YII/H]=A(YII)-A(Y)sun with A(Y)sun=2.21 (phys.abund)

s_Y2

Line-to-line scatter of YII (stat.error)

Y2Fe

⁽ⁿ⁾ [YII/Fe] abundance (phys.abund)

NY2

[0/10] Number of YII lines (meta.number)

Zr1

⁽ⁿ⁾ [ZrI/H]=A(ZrI)-A(Zr)sun with A(Zr)sun=2.62 (phys.abund)

s_Zr1

Line-to-line scatter of ZrII (stat.error)

Zr1Fe

⁽ⁿ⁾ [ZrI/Fe] abundance (phys.abund)

NZr1

[0/10] Number of ZrI lines (meta.number)

Zr2

⁽ⁿ⁾ [ZrII/H]=A(ZrII)-A(Zr)sun with A(Zr)sun=2.62 (phys.abund)

s_Zr2

Line-to-line scatter of ZrII (stat.error)

Zr2Fe

⁽ⁿ⁾ [ZrII//Fe] abundance (phys.abund)

ALL cols

⁽ⁿ⁾ indicates a possible blank or NULL column

⁽ⁱ⁾indexed column

NZr2

[0/10] Number of ZrII lines (meta.number)

Ba2fit

⁽ⁿ⁾ [BaII/H]=A(BaII)-A(Ba)sun with A(Ba)sun=2.17 (phys.abund)

s_Ba2fit

Line-to-line scatter of BaII (stat.error)

Ba2fitFe

⁽ⁿ⁾ [BaII/Fe] abundance (phys.abund)

NBa2fit

[0/2] Number of BaII lines (meta.number)

Eu2fit

⁽ⁿ⁾ [EuII/H]=A(EuII)-A(Eu)sun with A(Eu)sun=0.52 (phys.abund)

s_Eu2fit

Line-to-line scatter of EuII (stat.error)

Eu2fitFe

⁽ⁿ⁾ [EuII/Fe] abundance (phys.abund)

NEu2fit

[0/3] Number of EuII lines (meta.number)

_RA

deg

⁽ⁱ⁾ Positions from Gaia DR3 (right ascension part) (pos.eq.ra;meta.main)

_DE

deg

⁽ⁱ⁾ Positions from Gaia DR3 (declination part) (pos.eq.dec;meta.main)

ALL cols

⁽ⁿ⁾ indicates a possible blank or NULL column

⁽ⁱ⁾indexed column

Adapt form	Display your selection only	Reset to default columns
	Display UCD1+ UCD1

elapse time 0