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Simple TargetList Of TargetsFast 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/631/A43
  Late-type stars FeI & FeII NLTE line formation (Mashonkina+, 2019)
ReadMe+ftp
2019A&A...631A..43M
Similar Catalogs
Post annotation 		img(gal)
1.J/A+A/631/A43/stars(c)List of studied stars (41 rows)
2.J/A+A/631/A43/table2LTE and NLTE abundances of three halo stars (151 rows)
3.J/A+A/631/A43/table4LTE and NLTE abundances of the dSph stars (38 rows)

Simple ConstraintList Of Constraints
 
Query by Constraints constraints help applied on Columns (Output Order: + - )
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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)
  (1+3)Star (char) Star designation (meta.id;meta.main)
  (1)RAJ2000 "h:m:s" (i) Right ascension (J2000) (pos.eq.ra;meta.main)
  (1)DEJ2000 "d:m:s" (i) Declination (J2000) (pos.eq.dec;meta.main)
  (1)FileName (char) Name of the table with data for this star (meta.id;meta.table)
  (1)SimbadName (char) Designation understandable by the Simbad data-base (meta.id)
  (2)El (char) Atom (meta.id;spect.line)
  (2)Ion (char) Ion (phys.atmol.ionStage)
  (2)lambda 0.1nm Wavelength (em.wl)
  (2)Eexc eV Excitation energy (phys.atmol.excitation)
  (2)loggf  Adopted gf-value (phys.absorption.coeff)

ALL cols		    
 (i)indexed column
  (2)EW1 0.1pm (n) Equivalent width in HD 84937 (spect.line.eqWidth)
  (2)epsLTE1  (n) HD 84937 LTE abundance (log eps(H)=12) (phys.abund)
  (2)epsNLTEB1  (n) HD 84937 NLTE abundance (log eps(H)=12), B18 recipe (phys.abund)
  (2)epsNLTEY1  (n) HD 84937 NLTE abundance (log eps(H)=12), YBK18 (phys.abund)
  (2)EW2 0.1pm (n) Equivalent width in HD 140283 (spect.line.eqWidth)
  (2)epsLTE2  (n) HD 140283 LTE abundance (log eps(H)=12) (phys.abund)
  (2)epsNLTEB2  (n) HD 140283 NLTE abundance (log eps(H)=12), B18 recipe (phys.abund)
  (2)epsNLTEY2  (n) HD 140283 NLTE abundance (log eps(H)=12), YBK18 (phys.abund)
  (2)EW3 0.1pm (n) Equivalent width in HD 122563 (spect.line.eqWidth)
  (2)epsLTE3  (n) HD 122563LTE abundance (log eps(H)=12) (phys.abund)
  (2)epsNLTEB3  (n) HD 122563NLTE abundance (log eps(H)=12), B18 recipe (phys.abund)
  (2)epsNLTEY3  (n) HD 122563NLTE abundance (log eps(H)=12), YBK18 (phys.abund)
  (3)Teff K Effective temperature (phys.temperature.effective)

ALL cols		    
(n) indicates a possible blank or NULL column(i)indexed column
  (3)logg [cm/s2] Surface gravity (phys.gravity)
  (3)[Fe/H]  Metallicity (phys.abund.Fe)
  (3)xi km/s Microturbulent velocity (phys.veloc)
  (3)NFeI  Number of FeI lines (meta.number)
  (3)NFeII  Number of FeII lines (meta.number)
  (3)epsL1  Mean FeI LTE abundance (log eps(H)=12) (phys.abund)
  (3)e_epsL1  Dispersion of FeI LTE abundance (stat.error)
  (3)epsL2  Mean FeII LTE abundance (log eps(H)=12) (phys.abund)
  (3)e_epsL2  Dispersion of FeII LTE abundance (stat.error)
  (3)epsN1  Mean FeI NLTE abundance (log eps(H)=12) (phys.abund)
  (3)e_epsN1  Dispersion of FeI NLTE abundance (stat.error)
  (3)epsN2  Mean FeII NLTE abundance (log eps(H)=12) (phys.abund)
  (3)e_epsN2  Dispersion of FeII NLTE abundance (stat.error)

ALL cols		    
(n) indicates a possible blank or NULL column(i)indexed column
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