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/AJ/145/107	4967		Zr, Ba, La, and Eu abundances in 19 open clusters (Jacobson+, 2013) ReadMe+ftp 2013AJ....145..107J Similar Catalogs Post annotation
1.	J/AJ/145/107/clusters		^(c)Cluster sample (table1), and their mean abundances (table8) (19 rows) metaJ/AJ/145/107/clusters
2.	J/AJ/145/107/stars		^(c)Stellar atmospheric parameters and Fe abundances (table2), individual [X/Fe] rations for Zr (table4), Ba (table5), La (table6), and Eu (table7) (50 rows) metaJ/AJ/145/107/stars
3.	J/AJ/145/107/table3		Line list (10 rows) metaJ/AJ/145/107/table3

Simple Constraint List Of Constraints

Query by Constraints constraints help

constraints help

applied on Columns (Output Order: + - )

Show

Sort

Join tables

more join

Column

Constraint

Explain (UCD)

recno

Record number assigned by the VizieR team. Should Not be used for identification. ((unassigned);meta.version;arith.diff;phys.veloc)

Cluster

(char)

⁽ⁱ⁾ Cluster name ((unassigned);meta.version;arith.diff;spect.line.veloc;arith)

Age

Gyr

Cluster age (adopted from Salaris et al., 2004A&A...414..163S) (Note 1) ((unassigned);meta.version;arith.diff;stat.filling;meta.main)

f_Age

(char)

[d] Cluster age from Villanova et al. 2007 (Note 1) ((unassigned);meta.version;arith.diff;pos.eq.dec)

Dist

kpc

Distance ((unassigned);meta.version;arith.diff;em.UV.10-50nm;arith;meta.main)

Rgc

kpc

Galactocentric distance (R_{Sun}=8.5kpc) ((unassigned);(unassigned);(unassigned);em.UV.10-50nm;(unassigned))

Ref

(char)

Reference for distances (Note 2) ((unassigned);meta.version;arith.diff;phys.veloc.dispersion;(unassigned))

N1

Number of stars ((unassigned);meta.version;arith.diff;src.var)

N2

⁽ⁿ⁾ Number of stars (from spectra obtained on Keck) ((unassigned);(unassigned);(unassigned);src.var)

Tel

(char)

Telescope (KPNO4m, Keck, or HET) (Note 3) ((unassigned);meta.version;arith.diff;spect.line.veloc;phys.mol.quadrupole.magnetic)

C

(char)

[ab] Calculation of [X/Fe] ratios (Note 4) ((unassigned);meta.version;arith.diff;pos.eq.dec)

ALL cols

⁽ⁿ⁾ indicates a possible blank or NULL column

⁽ⁱ⁾indexed column

[Fe/H]

[Sun]

Cluster mean [Fe/H] abundance ((unassigned);(unassigned);(unassigned);phys.reflectance;spect.dopplerVeloc.radio;meta.main)

s_[Fe/H]

[Sun]

1{sigma} standard deviation in [Fe/H] ((unassigned);(unassigned);(unassigned);meta.id.PI;phys.reflectance.bidirectional)

[Zr/H]

[Sun]

Cluster mean [Zr/H] abundance (time.expo;(unassigned);arith.factor;phys.polarization.stokes.Q)

s_[Zr/H]

[Sun]

1{sigma} standard deviation in [Zr/H] ((unassigned);phys.luminosity.fun;arith.factor;meta.id.PI;phys.polarization.stokes.U)

[Ba/Fe]

[Sun]

Cluster mean [Ba/Fe] abundance ((unassigned);meta.version;arith.diff;phys.polarization.stokes.Q)

s_[Ba/Fe]

[Sun]

1{sigma} standard deviation in [Ba/Fe] ((unassigned);(unassigned);(unassigned);meta.id.PI;phys.polarization.stokes.U)

[La/Fe]

[Sun]

Cluster mean [La/Fe] abundance ((unassigned);meta.version;arith.diff;phys.polarization.stokes.Q)

s_[La/Fe]

[Sun]

1{sigma} standard deviation in [La/Fe] ((unassigned);(unassigned);(unassigned);meta.id.PI;phys.polarization.stokes.U)

[Eu/Fe]

[Sun]

⁽ⁿ⁾ Cluster mean [Eu/Fe] abundance ((unassigned);meta.version;arith.diff;phys.polarization.stokes.Q)

s_[Eu/Fe]

[Sun]

⁽ⁿ⁾ 1{sigma} standard deviation in [Eu/Fe] ((unassigned);(unassigned);(unassigned);meta.id.PI;phys.polarization.stokes.U)

N

Number of stars used to determined the mean abundances (Note 5) ((unassigned);(unassigned);(unassigned);src.var)

F+10

⁽ⁿ⁾Display the data from Friel et al. (2010, cat. J/AJ/139/1942) if any ((unassigned);meta.version;arith.diff;src.var)

SimbadName

(char)

Designation understandable by the Simbad data-base ((unassigned);(unassigned);(unassigned);spect.line.veloc)

ALL cols

⁽ⁿ⁾ indicates a possible blank or NULL column

⁽ⁱ⁾indexed column

_RA

deg

⁽ⁿ⁾Positions from SIMBAD database (right ascension part) ((unassigned);meta.version;arith.diff;(unassigned);arith)

_DE

deg

⁽ⁿ⁾Positions from SIMBAD database (declination part) ((unassigned);(unassigned);(unassigned);(unassigned);arith)

Star

(char)

Star name (in Cluster) ((unassigned);(unassigned);(unassigned);spect.line.veloc;arith)

Teff

K

Effective temperature ((unassigned);(unassigned);(unassigned);em.radio)

logg

Surface gravity ((unassigned);(unassigned);(unassigned);(unassigned))

vt

km/s

Microturbulent velocity ((unassigned);meta.version;arith.diff;spect.index;meta.main)

[FeI/H]

[Sun]

Metallicity from FeI lines (Note 1) ((unassigned);meta.version;arith.diff;pos.emergenceAng)

s_[FeI/H]

[Sun]

1{sigma} standard deviation in [FeI/H] (src.class.distance;em.IR.30-60um;arith.factor;meta.id.PI;phys.polarization.stokes.U)

o_[FeI/H]

Number of FeI lines ((unassigned);(unassigned);(unassigned);src.var)

[FeII/H]

[Sun]

Metallicity from FeII lines (Note 1) ((unassigned);(unassigned);(unassigned);pos.emergenceAng)

s_[FeII/H]

[Sun]

1{sigma} standard deviation in [FeII/H] ((unassigned);(unassigned);(unassigned);meta.id.PI;phys.polarization.stokes.U)

o_[FeII/H]

Number of FeII lines ((unassigned);(unassigned);(unassigned);src.var)

[Zr/Fe]1

[Sun]

Abundance from the ZrI{lambda}6127 lines (Note 7) ((unassigned);(unassigned);(unassigned);phys.polarization.stokes.Q)

ALL cols

⁽ⁿ⁾ indicates a possible blank or NULL column

⁽ⁱ⁾indexed column

[Zr/Fe]2

[Sun]

⁽ⁿ⁾ Abundance from ZrI{lambda}6134 lines (Note 7) ((unassigned);(unassigned);(unassigned);phys.polarization.stokes.Q)

[Zr/Fe]3

[Sun]

Abundance from the ZrI{lambda}6143 lines (Note 7) ((unassigned);(unassigned);(unassigned);phys.polarization.stokes.Q)

<[Zr/Fe]>

[Sun]

Mean star [Zr/Fe] abundance ((unassigned);(unassigned);(unassigned);phys.polarization.stokes.Q)

s_<[Zr/Fe]>

[Sun]

1{sigma} standard deviation in <[Zr/Fe]> ((unassigned);(unassigned);(unassigned);meta.id.PI;phys.polarization.stokes.U)

[Ba/Fe]1

[Sun]

Abundance from the BaII{lambda}5853 lines (Note 8) ((unassigned);(unassigned);(unassigned);phys.polarization.stokes.Q)

[Ba/Fe]2

[Sun]

Abundance from the BaII{lambda}6141 lines (Note 8) ((unassigned);(unassigned);(unassigned);phys.polarization.stokes.Q)

[Ba/Fe]3

[Sun]

Abundance from the BaII{lambda}6496 lines (Note 8) ((unassigned);(unassigned);(unassigned);phys.polarization.stokes.Q)

<[Ba/Fe]>

[Sun]

Mean star [Ba/Fe] abundance (Note 9) ((unassigned);(unassigned);(unassigned);phys.polarization.stokes.Q)

s_<[Ba/Fe]>

[Sun]

1{sigma} standard deviation in <[Ba/Fe]> (Note 9) ((unassigned);(unassigned);(unassigned);meta.id.PI;phys.polarization.stokes.U)

[La/Fe]1

[Sun]

⁽ⁿ⁾ Abundance from LaII{lambda}6262 lines (Note 10) ((unassigned);(unassigned);(unassigned);phys.polarization.stokes.Q)

e_[La/Fe]1

[Sun]

⁽ⁿ⁾ Uncertainty in [La/Fe]1 (Note 11) ((unassigned);(unassigned);(unassigned);time.age;phys.polarization.stokes.U)

[La/Fe]2

[Sun]

⁽ⁿ⁾ Abundance from LaII{lambda}6390 lines (Note 10) ((unassigned);(unassigned);(unassigned);phys.polarization.stokes.Q)

e_[La/Fe]2

[Sun]

⁽ⁿ⁾ Uncertainty in [La/Fe]2 (Note 11) ((unassigned);(unassigned);(unassigned);time.age;phys.polarization.stokes.U)

ALL cols

⁽ⁿ⁾ indicates a possible blank or NULL column

⁽ⁱ⁾indexed column

<[La/Fe]>

[Sun]

⁽ⁿ⁾ Mean star [La/Fe] abundance ((unassigned);(unassigned);(unassigned);phys.polarization.stokes.Q)

s_<[La/Fe]>

[Sun]

⁽ⁿ⁾ 1{sigma} standard deviation in <[La/Fe]> ((unassigned);(unassigned);(unassigned);meta.id.PI;phys.polarization.stokes.U)

[Eu/Fe]1

[Sun]

⁽ⁿ⁾ Abundance from EuII{lambda}6437 lines (Note 12) ((unassigned);(unassigned);(unassigned);phys.polarization.stokes.Q)

e_[Eu/Fe]1

[Sun]

⁽ⁿ⁾ Uncertainty in [Eu/Fe]1 (Note 13) ((unassigned);(unassigned);(unassigned);time.age;phys.polarization.stokes.U)

[Eu/Fe]2

[Sun]

⁽ⁿ⁾ Abundance from EuII{lambda}6645 lines (Note 12) ((unassigned);(unassigned);(unassigned);phys.polarization.stokes.Q)

e_[Eu/Fe]2

[Sun]

⁽ⁿ⁾ Uncertainty in [Eu/Fe]2 (Note 13) ((unassigned);(unassigned);(unassigned);time.age;phys.polarization.stokes.U)

<[Eu/Fe]>

[Sun]

⁽ⁿ⁾ Mean star [Eu/Fe] abundance ((unassigned);(unassigned);(unassigned);phys.polarization.stokes.Q)

s_<[Eu/Fe]>

[Sun]

⁽ⁿ⁾ 1{sigma} standard deviation in <[Eu/Fe]> ((unassigned);(unassigned);(unassigned);meta.id.PI;phys.polarization.stokes.U)

OCat

⁽ⁿ⁾Cross-match with Yong et al. (2012, cat. J/AJ/144/95), Jacobson et al. (2009, cat. J/AJ/137/4753), and Friel et al. (2010, cat. J/AJ/139/1942) within 1.5" ((unassigned);(unassigned);(unassigned);pos.geocentric)

El

(char)

Element/Ion (Zr I, Ba II, La II, or Eu II) ((unassigned);(unassigned);(unassigned);phys.veloc.orbital)

lambda

0.1nm

Wavelength (Å) ((unassigned);(unassigned);(unassigned);meta.bib.author)

EP

eV

Excitation potential ((unassigned);(unassigned);(unassigned);(unassigned))

loggf

[-]

Log of the oscillator strength ((unassigned);(unassigned);(unassigned);(unassigned))

ALL cols

⁽ⁿ⁾ indicates a possible blank or NULL column

⁽ⁱ⁾indexed column

f_loggf

(char)

[e] Origin of loggf (Note 2) ((unassigned);(unassigned);(unassigned);pos.eq.dec)

Abund1

[-]

Element Solar abundance (log{epsilon}(Fe)) (Note 3) ((unassigned);(unassigned);(unassigned);phys.polarization.stokes.Q)

Abund2

[-]

Element Solar abundance (log{epsilon}(Fe)) (Note 4) ((unassigned);(unassigned);(unassigned);phys.polarization.stokes.Q)

Abund3

[-]

Element Arcturus abundance (log{epsilon}(X)) (Note 5) ((unassigned);(unassigned);(unassigned);phys.polarization.stokes.Q)

f_Abund3

(char)

[f] This abundance is forced to match that for the EuII 6645 feature; details in Section 3.2.4 ((unassigned);(unassigned);(unassigned);pos.eq.dec)

[X/Fe]

[Sun]

Arcturus [X/Fe] ratio (Note 6) ((unassigned);(unassigned);(unassigned);phys.polarization.stokes.Q)

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 3