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J/ApJ/934/110
  Abundance analysis of 4 HES metal-poor stars (Shejeelammal+, 2022)
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2022ApJ...934..110S
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1.J/ApJ/934/110/stars(c)Basic information (Table 1) and derived atmospheric parameters and radial velocity (Table 2) of the program stars (9 rows)
2.J/ApJ/934/110/table9Equivalent widths of Fe lines used for deriving atmospheric parameters (52 rows)
3.J/ApJ/934/110/table10Equivalent widths of lines used for deriving elemental abundances (172 rows)
4.J/ApJ/934/110/table11Lines used to derive the elemental abundance from spectral synthesis (31 rows)

Simple ConstraintList 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)
  (1)Name (char) Star name (meta.id;meta.main)
  (1)RAJ2000 "h:m:s" (n)(i) Hour of right ascension (J2000) (pos.eq.ra;meta.main)
  (1)DEJ2000 "d:m:s" (n)(i) Degree of declination (J2000) (pos.eq.dec;meta.main)
  (1)Bmag mag (n) [11.8/15.9] B magnitude (phot.mag;em.opt.B)
  (1)Vmag mag (n) [10.9/14.3] V magnitude (phot.mag;em.opt.V)
  (1)Jmag mag (n) [8.9/11.9] J-band magnitude (phot.mag;em.IR.J)
  (1)Hmag mag (n) [8.4/11.3] H-band magnitude (phot.mag;em.IR.H)
  (1)Kmag mag (n) [8.1/11.1] K band magnitude (phot.mag;em.IR.K)
  (1)SN4200A  (n) [8/16] S/N at 4200Å (stat.snr)
  (1)SN5500A  (n) [29/56] S/N at 5500Å (stat.snr)

ALL cols		    
(n) indicates a possible blank or NULL column(i)indexed column
  (1)SN7700A  (n) [49/90] S/N at 7700Å (stat.snr)
  (1)Ab1 (char) Equivalent widths of Fe lines used for deriving atmospheric parameters (link to Table 9) (meta.ref.url)
  (1)Ab2 (char) Equivalent widths of lines used for deriving elemental abundances (link to Table 10) (meta.ref.url)
  (1)Ab3 (char) Lines used to derive the elemental abundance from spectral synthesis (link to Table 11) (meta.ref.url)
  (1)Teff K (n) [4240/5380] Effective temperature (phys.temperature.effective)
  (1)logg [cm/s2] (n) [0.5/3] Log of surface gravity (phys.gravity)
  (1)Vt km/s (n) [0.69/3.5] Microturbulent velocity (phys.veloc)
  (1)[FeI/H] Sun [-3.5/-0.7] Log of FeI/H abundance (phys.abund)
  (1)e_[FeI/H] Sun (n) [0.06/0.2] [FeI/H] uncertainty (stat.error;phys.abund)
  (1)[FeII/H] Sun (n) [-2.9/-0.7] Log of FeII/H abundance (phys.abund)
  (1)e_[FeII/H] Sun (n) [0.01/0.2] [FeII/H] uncertainty (stat.error;phys.abund)
  (1)RV km/s (n) [49/180] Radial velocity (phys.veloc;pos.heliocentric)
  (1)e_RV km/s (n) [0.02/2.2] RV uncertainty (stat.error)

ALL cols		    
(n) indicates a possible blank or NULL column(i)indexed column
  (1)RVGaia  (n) [52.4/178] Gaia DR2 radial velocity (phys.veloc;pos.heliocentric)
  (1)e_RVGaia  (n) [0.3/1.5] RVGaia uncertainty (stat.error)
  (1)RVrave  (n) [72/178] RAVE DR4 radial velocity (phys.veloc;pos.heliocentric)
  (1)e_RVrave  (n) [1.5/2.2] RVrave uncertainty (stat.error)
  (1)Ref   [1/4] Reference (Note 1)   (meta.ref;pos.frame)
  (1)Simbad (char) ask the Simbad data-base about this object (meta.ref.url)
  (2+3+4)lambda 0.1nm [4132.9/6430.9] Wavelength, Angstroms (em.wl)
  (2+3+4)El (char) Element (phys.atmol.element)
  (2+3+4)Elow eV [0.087/4.6] Energy, lower level (phys.energy;phys.atmol.level)
  (2+3+4)loggf [-] [-4.95/-0.02] Log, statistical weight*oscillator strength (stat.weight;phys.atmol.oscStrength)
  (2+3)EW-HE0457 0.1pm (n) [55/145.6] Equivalent width of line, HE0457-1805 (spect.line.eqWidth)
  (2+3+4)Ab-HE0457 [-] (n) [5.3/5.7] Derived absolute abundance for line, HE 0457-1805 (phys.abund)
  (2+3)EW-HE0920 0.1pm (n) [27.4/92] Equivalent width of line, HE0920-0506 (spect.line.eqWidth)

ALL cols		    
(n) indicates a possible blank or NULL column(i)indexed column
  (2+3+4)Ab-HE0920 [-] (n) [6.6/6.9] Derived absolute abundance for line, HE 0920-0506 (phys.abund)
  (2+3)EW-HE1241 0.1pm (n) [20.5/151] Equivalent width of line, HE1241-0337 (spect.line.eqWidth)
  (2+3+4)Ab-HE1241 [-] (n) [4.8/5.3] Derived absolute abundance for line, HE 1241-0337 (phys.abund)
  (2+3)EW-HE1327 0.1pm (n) [20/83.4] Equivalent width of line, HE1327-2116 (spect.line.eqWidth)
  (2+3+4)Ab-HE1327 [-] (n) [4.5/4.8] Derived absolute abundance for line, HE 1327-2116 (phys.abund)

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