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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/AJ/169/172	2449		Derived parameters & abundances of metal-poor stars (Mittal+, 2025) ReadMe+ftp 2025AJ....169..172M Similar Catalogs Post annotation
1.	J/AJ/169/172/table1		^(c)Effective temperatures calculated from different colors (311 rows) metaJ/AJ/169/172/table1
2.	J/AJ/169/172/table2		Derived line-by-line abundances (47921 rows) metaJ/AJ/169/172/table2
3.	J/AJ/169/172/table3		Final effective temperature and log of surface gravity values, and other final model atmosphere parameters (Teff vs log(g)) (311 rows) metaJ/AJ/169/172/table3
4.	J/AJ/169/172/table4		Derived local thermodynamic equilibrium (LTE) abundances (311 rows) metaJ/AJ/169/172/table4
			Abundances derived from O I, Na I, Mg I, Si I, K I, Fe I, and Fe II lines have been corrected for NLTE. Their LTE abundances are presented in this Table for reference, but we recommend adopting the NLTE-corrected abundances presented in Table 5.
5.	J/AJ/169/172/table5		Derived non-local thermodynamic equilibrium (NLTE) abundances (311 rows) metaJ/AJ/169/172/table5
			The number of lines listed here refers to the number of lines for which NLTE corrections were calculated using the procedure explained in Section 4.3. For O I, Na I, Mg I, Si I, K I, Fe I, and Fe II, we recommend adopting the abundances presented here.

Simple Constraint List Of Constraints

Query by Constraints constraints help

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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)

Name

(char)

⁽ⁱ⁾ Stellar identifier (meta.id;meta.main)

(1)

T(BP-RP)

[4490/7533] Effective temperature from color BP-RP (phys.temperature.effective)

(1)

e_T(BP-RP)

[64/233] Uncertainty in T (BP-RP) (stat.error)

(1)

T(BP-G)

[0/7214] Effective temperature from color BP-G (Note 1) (phys.temperature.effective)

(1)

e_T(BP-G)

[0/415] Uncertainty in T (BP-G) (Note 1) (stat.error)

(1)

T(G-RP)

[0/7489] Effective temperature from color G-RP (Note 1) (phys.temperature.effective)

(1)

e_T(G-RP)

[0/224] Uncertainty in T (G-RP) (Note 1) (stat.error)

(1)

T(BP-K)

[4463/7451] Effective temperature from color BP-K (phys.temperature.effective)

(1)

e_T(BP-K)

[49/144] Uncertainty in T (BP-K) (stat.error)

(1)

T(RP-K)

[4463/7630] Effective temperature from color RP-K (phys.temperature.effective)

ALL cols

⁽ⁱ⁾indexed column

(1)

e_T(RP-K)

[65/242] Uncertainty in T (RP-K) (stat.error)

(1)

T(G-K)

[0/7644] Effective temperature from color G-K (Note 1) (phys.temperature.effective)

(1)

e_T(G-K)

[0/99] Uncertainty in T (G-K) (Note 1) (stat.error)

(1)

SimbadName

(char)

⁽ⁿ⁾Designation understandable by the Simbad data-base (meta.id)

(1)

_RA

deg

⁽ⁱ⁾ Position from Simbad (right ascension part) (pos.eq.ra;meta.main)

(1)

_DE

deg

⁽ⁱ⁾ Position from Simbad (declination part) (pos.eq.dec;meta.main)

(2)

(char)

Species (phys.atmol.ionStage)

(2)

lambda

0.1nm

[3329.4/7775.4] Wavelength in Angstroms (em.wl)

(2)

0.1pm

[1.6/476.6] Equivalent width in milliAngstroms (spect.line.eqWidth)

(2)

loge(X)

[-]

[0.81/8.72] Log epsilon abundance of element X (phys.abund)

(2)

NLTEcorr

⁽ⁿ⁾ [-0.68/0.32] NLTE correction to log(e)(X) abundance (phys.abund;arith.diff)

(3)

Class

(char)

Star class (Note 1) (src.class)

(3)

Teff

[4472/7451] Effective temperature (phys.temperature.effective)

ALL cols

⁽ⁿ⁾ indicates a possible blank or NULL column

⁽ⁱ⁾indexed column

(3)

e_Teff

[2/36] Uncertainty in Teff (stat.error;phys.temperature.effective)

(3)

logg

[cm/s2]

[1.08/4.82] Log of surface gravity (phys.gravity)

(3)

e_logg

[cm/s2]

[0.15/0.5] Uncertainty in logg (stat.error;phys.gravity)

(3)

E(B-V)

mag

[0.0/0.22] E(B-V) reddening (phot.color.excess)

(3)

e_E(B-V)

mag

[0.01/0.03] Uncertainty in E(B-V) (stat.error;phot.color.excess)

(3)

BC-G

mag

[-0.62/0.04] Bolometric correction in G (phot.mag.bc)

(3)

e_BC-G

mag

[0.01/0.18] Uncertainty in BC (stat.error;phot.mag.bc)

(3)

[M/H]

[-]

[-3.9/-1.0] Model metallicity adopted (phys.abund.Z;meta.modelled)

(3)

e_[M/H]

[-]

[0.3/0.3] Uncertainty in [M/H] (stat.error;phys.abund.Z;meta.modelled)

(3)

km/s

[0.8/3.5] Microturbulence velocity (phys.veloc.microTurb)

(3)

e_vt

km/s

[0.06/0.06] Uncertainty in vt (stat.error;phys.veloc.microTurb)

(4)

nFeI

[19/138] Number of FeI LTE lines used (Note 1) (meta.number)

(4)

loge(FeI)

[-]

[3.38/6.46] Log epsilon mean abundance of FeI (phys.abund;stat.mean)

ALL cols

⁽ⁿ⁾ indicates a possible blank or NULL column

⁽ⁱ⁾indexed column

(4)

[FeI/H]

[-]

[-4.12/-1.04] FeI abundance relative to H (phys.abund.Fe)

(4)

e_[FeI/H]

[-]

[0.03/0.1] Total uncertainty in [FeI/H] (stat.error;phys.abund.Fe)

(4)

nFeII

⁽ⁿ⁾ [1/13] Number of FeII LTE lines used (Note 1) (meta.number)

(4)

loge(FeII)

[-]

⁽ⁿ⁾ [3.41/6.52] Log epsilon mean abundance of FeII (phys.abund;stat.mean)

(4)

[FeII/H]

[-]

⁽ⁿ⁾ [-4.09/-0.98] FeII abundance relative to H (phys.abund.Fe)

(4)

e_[FeII/H]

[-]

⁽ⁿ⁾ [0.12/0.6] Total uncertainty in [FeII/H] (stat.error;phys.abund.Fe)

(4)

nOI

⁽ⁿ⁾ [1/4] Number of OI LTE lines used (Note 1) (meta.number)

(4)

loge(OI)

[-]

⁽ⁿ⁾ [6.55/8.72] Log epsilon mean abundance of OI (phys.abund;stat.mean)

(4)

[OI/Fe]

[-]

⁽ⁿ⁾ [0.26/2.85] OI abundance relative to FeI (phys.abund;arith.ratio)

(4)

e_[OI/Fe]

[-]

⁽ⁿ⁾ [0.09/0.31] Total uncertainty in [OI/Fe] (stat.error;phys.abund;arith.ratio)

(4)

nNaI

⁽ⁿ⁾ [1/4] Number of NaI LTE lines used (Note 1) (meta.number)

(4)

loge(NaI)

[-]

⁽ⁿ⁾ [2.42/5.33] Log epsilon mean abundance of NaI (phys.abund;stat.mean)

(4)

[NaI/Fe]

[-]

⁽ⁿ⁾ [-0.56/1.63] NaI abundance relative to FeI (phys.abund;arith.ratio)

ALL cols

⁽ⁿ⁾ indicates a possible blank or NULL column

⁽ⁱ⁾indexed column

(4)

e_[NaI/Fe]

[-]

⁽ⁿ⁾ [0.12/0.28] Total uncertainty in [NaI/Fe] (stat.error;phys.abund;arith.ratio)

(4)

nMgI

[1/9] Number of MgI LTE lines used (Note 1) (meta.number)

(4)

loge(MgI)

[-]

[3.81/7.18] Log epsilon mean abundance of MgI (phys.abund;stat.mean)

(4)

[MgI/Fe]

[-]

[-0.36/1.51] MgI abundance relative to FeI (phys.abund;arith.ratio)

(4)

e_[MgI/Fe]

[-]

[0.08/0.22] Total uncertainty in [MgI/Fe] (stat.error;phys.abund;arith.ratio)

(4)

nSiI

⁽ⁿ⁾ [1/4] Number of SiI LTE lines used (Note 1) (meta.number)

(4)

loge(SiI)

[-]

⁽ⁿ⁾ [3.63/6.87] Log epsilon mean abundance of SiI (phys.abund;stat.mean)

(4)

[SiI/Fe]

[-]

⁽ⁿ⁾ [-0.34/1.14] SiI abundance relative to FeI (phys.abund;arith.ratio)

(4)

e_[SiI/Fe]

[-]

⁽ⁿ⁾ [0.09/0.55] Total uncertainty in [SiI/Fe] (stat.error;phys.abund;arith.ratio)

(4)

nKI

⁽ⁿ⁾ [1/2] Number of KI LTE lines used (Note 1) (meta.number)

(4)

loge(KI)

[-]

⁽ⁿ⁾ [1.51/4.74] Log epsilon mean abundance of KI (phys.abund;stat.mean)

(4)

[KI/Fe]

[-]

⁽ⁿ⁾ [-0.08/0.88] KI abundance relative to FeI (phys.abund;arith.ratio)

(4)

e_[KI/Fe]

[-]

⁽ⁿ⁾ [0.11/0.21] Total uncertainty in [KI/Fe] (stat.error;phys.abund;arith.ratio)

ALL cols

⁽ⁿ⁾ indicates a possible blank or NULL column

⁽ⁱ⁾indexed column

(4)

nCaI

[3/14] Number of CaI LTE lines used (meta.number)

(4)

loge(CaI)

[-]

[2.45/5.58] Log epsilon mean abundance of CaI (phys.abund;stat.mean)

(4)

[CaI/Fe]

[-]

[-0.32/0.54] CaI abundance relative to FeI (phys.abund;arith.ratio)

(4)

e_[CaI/Fe]

[-]

[0.06/0.24] Total uncertainty in [CaI/Fe] (stat.error;phys.abund;arith.ratio)

(4)

nTiI

⁽ⁿ⁾ [1/19] Number of TiI LTE lines used (meta.number)

(4)

loge(TiI)

[-]

⁽ⁿ⁾ [1.21/4.21] Log epsilon mean abundance of TiI (phys.abund;stat.mean)

(4)

[TiI/Fe]

[-]

⁽ⁿ⁾ [-0.35/1.16] TiI abundance relative to FeI (phys.abund;arith.ratio)

(4)

e_[TiI/Fe]

[-]

⁽ⁿ⁾ [0.05/0.52] Total uncertainty in [TiI/Fe] (stat.error;phys.abund;arith.ratio)

(4)

nTiII

[2/34] Number of TiII LTE lines used (meta.number)

(4)

loge(TiII)

[-]

[1.31/4.4] Log epsilon mean abundance of TiII (phys.abund;stat.mean)

(4)

[TiII/Fe]

[-]

[-0.14/1.04] TiII abundance relative to FeI (phys.abund;arith.ratio)

(4)

e_[TiII/Fe]

[-]

[0.09/0.32] Total uncertainty in [TiII/Fe] (stat.error;phys.abund;arith.ratio)

(4)

nCrI

[1/13] Number of CrI LTE lines used (meta.number)

ALL cols

⁽ⁿ⁾ indicates a possible blank or NULL column

⁽ⁱ⁾indexed column

(4)

loge(CrI)

[-]

[1.03/4.53] Log epsilon mean abundance of CrI (phys.abund;stat.mean)

(4)

[CrI/Fe]

[-]

[-0.67/0.3] CrI abundance relative to FeI (phys.abund;arith.ratio)

(4)

e_[CrI/Fe]

[-]

[0.06/0.4] Total uncertainty in [CrI/Fe] (stat.error;phys.abund;arith.ratio)

(4)

nCrII

⁽ⁿ⁾ [1/4] Number of CrII LTE lines used (meta.number)

(4)

loge(CrII)

[-]

⁽ⁿ⁾ [2.1/4.73] Log epsilon mean abundance of CrII (phys.abund;stat.mean)

(4)

[CrII/Fe]

[-]

⁽ⁿ⁾ [-0.39/0.58] CrII abundance relative to FeI (phys.abund;arith.ratio)

(4)

e_[CrII/Fe]

[-]

⁽ⁿ⁾ [0.15/0.65] Total uncertainty in [CrII/Fe] (stat.error;phys.abund;arith.ratio)

(4)

nNiI

⁽ⁿ⁾ [1/18] Number of NiI LTE lines used (meta.number)

(4)

loge(NiI)

[-]

⁽ⁿ⁾ [2.03/5.24] Log epsilon mean abundance of NiI (phys.abund;stat.mean)

(4)

[NiI/Fe]

[-]

⁽ⁿ⁾ [-0.34/0.49] NiI abundance relative to FeI (phys.abund;arith.ratio)

(4)

e_[NiI/Fe]

[-]

⁽ⁿ⁾ [0.06/0.41] Total uncertainty in [NiI/Fe] (stat.error;phys.abund;arith.ratio)

(4)

nZnI

⁽ⁿ⁾ [1/3] Number of ZnI LTE lines used (meta.number)

(4)

loge(ZnI)

[-]

⁽ⁿ⁾ [1.28/3.81] Log epsilon mean abundance of ZnI (phys.abund;stat.mean)

ALL cols

⁽ⁿ⁾ indicates a possible blank or NULL column

⁽ⁱ⁾indexed column

(4)

[ZnI/Fe]

[-]

⁽ⁿ⁾ [-0.55/1.04] ZnI abundance relative to FeI (phys.abund;arith.ratio)

(4)

e_[ZnI/Fe]

[-]

⁽ⁿ⁾ [0.1/0.54] Total uncertainty in [ZnI/Fe] (stat.error;phys.abund;arith.ratio)

(5)

nFeI-NLTE

[7/32] Number of FeI NLTE lines used (Note 1) (meta.number)

(5)

loge(FeI)-NLTE

[-]

[3.56/6.5] Log epsilon mean abundance of FeI (phys.abund;stat.mean)

(5)

[FeI/H]-NLTE

[-]

[-3.94/-1.0] FeI abundance relative to H (phys.abund.Fe)

(5)

e_[FeI/H]-NLTE

[-]

[0.06/0.18] Total uncertainty in [FeI/H]-NLTE (stat.error;phys.abund.Fe)

(5)

nFeII-NLTE

⁽ⁿ⁾ [1/13] Number of FeII NLTE lines used (Note 1) (meta.number)

(5)

loge(FeII)-NLTE

[-]

⁽ⁿ⁾ [3.42/6.5] Log epsilon mean abundance of FeII (phys.abund;stat.mean)

(5)

[FeII/H]-NLTE

[-]

⁽ⁿ⁾ [-4.08/-1.0] FeII abundance relative to H (phys.abund.Fe)

(5)

e_[FeII/H]-NLTE

[-]

⁽ⁿ⁾ [0.13/0.6] Total uncertainty in [FeII/H]-NLTE (stat.error;phys.abund.Fe)

(5)

nOI-NLTE

⁽ⁿ⁾ [1/4] Number of OI NLTE lines used (Note 1) (meta.number)

(5)

loge(OI)-NLTE

[-]

⁽ⁿ⁾ [6.55/8.72] Log epsilon mean abundance of OI (phys.abund;stat.mean)

(5)

[OI/Fe]-NLTE

[-]

⁽ⁿ⁾ [0.1/2.85] OI abundance relative to FeI (phys.abund;arith.ratio)

ALL cols

⁽ⁿ⁾ indicates a possible blank or NULL column

⁽ⁱ⁾indexed column

(5)

e_[OI/Fe]-NLTE

[-]

⁽ⁿ⁾ [0.13/0.33] Total uncertainty in [OI/Fe]-NLTE (stat.error;phys.abund;arith.ratio)

(5)

nNaI-NLTE

⁽ⁿ⁾ [1/4] Number of NaI NLTE lines used (Note 1) (meta.number)

(5)

loge(NaI)-NLTE

[-]

⁽ⁿ⁾ [2.38/5.22] Log epsilon mean abundance of NaI (phys.abund;stat.mean)

(5)

[NaI/Fe]-NLTE

[-]

⁽ⁿ⁾ [-0.63/1.53] NaI abundance relative to FeI (phys.abund;arith.ratio)

(5)

e_[NaI/Fe]-NLTE

[-]

⁽ⁿ⁾ [0.16/0.31] Total uncertainty in [NaI/Fe]-NLTE (stat.error;phys.abund;arith.ratio)

(5)

nMgI-NLTE

[1/9] Number of MgI NLTE lines used (Note 1) (meta.number)

(5)

loge(MgI)-NLTE

[-]

[4.02/7.18] Log epsilon mean abundance of MgI (phys.abund;stat.mean)

(5)

[MgI/Fe]-NLTE

[-]

[-0.36/1.58] MgI abundance relative to FeI (phys.abund;arith.ratio)

(5)

e_[MgI/Fe]-NLTE

[-]

[0.1/0.26] Total uncertainty in [MgI/Fe]-NLTE (stat.error;phys.abund;arith.ratio)

(5)

nSiI-NLTE

⁽ⁿ⁾ [1/4] Number of SiI NLTE lines used (Note 1) (meta.number)

(5)

loge(SiI)-NLTE

[-]

⁽ⁿ⁾ [3.63/6.86] Log epsilon mean abundance of SiI (phys.abund;stat.mean)

(5)

[SiI/Fe]-NLTE

[-]

⁽ⁿ⁾ [-0.29/1.14] SiI abundance relative to FeI (phys.abund;arith.ratio)

(5)

e_[SiI/Fe]-NLTE

[-]

⁽ⁿ⁾ [0.13/0.56] Total uncertainty in [SiI/Fe]-NLTE (stat.error;phys.abund;arith.ratio)

ALL cols

⁽ⁿ⁾ indicates a possible blank or NULL column

⁽ⁱ⁾indexed column

(5)

nKI-NLTE

⁽ⁿ⁾ [1/2] Number of KI NLTE lines used (Note 1) (meta.number)

(5)

loge(KI)-NLTE

[-]

⁽ⁿ⁾ [1.43/4.21] Log epsilon mean abundance of KI (phys.abund;stat.mean)

(5)

[KI/Fe]-NLTE

(char) [-]

KI abundance relative to FeI (phys.abund;arith.ratio)

(5)

e_[KI/Fe]-NLTE

[-]

⁽ⁿ⁾ [0.17/0.26] Total uncertainty in [KI/Fe]-NLTE (stat.error;phys.abund;arith.ratio)

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