VizieR

CfA VizieR . ADAC VizieR . Cambridge (UK) VizieR . IUCAA VizieR . INASAN VizieR .

VizieR

Simple TargetList Of TargetsFast Xmatch with large catalogs or Simbad
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NB: The epoch used for the query is the original epoch of the table(s)Radius Box size

  
J/ApJ/931/147
  Very metal-poor stars with LAMOST & Subaru. II. (Li+, 2022)
Post annotation
img(gal)
1.J/ApJ/931/147/table2(c)Stellar parameters of the program stars (385 rows)
2.J/ApJ/931/147/table3Abundances and abundance error estimations of the program stars (8470 rows)

 
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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)ID (char) (i) Short ID of a star, Paper I (Aoki+ 2022, J/ApJ/931/146) (meta.id)
  (1)RAJ2000 deg (i) Right Ascension in degrees (J2000) (pos.eq.ra;meta.main)
  (1)DEJ2000 deg (i) [-7.1/60.6] Declination in degrees (J2000) (pos.eq.dec;meta.main)
  (1)RVel km/s [-454/434] Radial velocity (observed) (phys.veloc;pos.heliocentric)
  (1)SNR   [6.9/157] Spectral SNR around 4500 Angstrom (stat.snr)
  (1)Teff K [4290/6731] Effective temperature derived from Subaru spectra (phys.temperature.effective)
  (1)e_Teff K [7/584] Uncertainty on Teff (stat.error;phys.temperature.effective)
  (1)logg [cm/s2] [0.5/4.8] Surface gravity derived from Subaru spectra (phys.gravity)
  (1)e_logg [cm/s2] [0.01/0.7] Uncertainty on logg (stat.error)
  (1)f_logg  (n) [0/1] Flag on logg (Note 1)   (meta.code)

ALL cols
    
(n) indicates a possible blank or NULL column(i)indexed column
  (1)FeH [-] [-4.4/-0.6] Metallicity derived from Subaru spectra (phys.abund.Fe)
  (1)e_FeH [-] [0.08/0.4] Uncertainty on FeH (stat.error)
  (1)vt km/s [0/4.1] Microturbulent velocity derived from Subaru spectra (phys.veloc)
  (1)e_vt km/s [0.03/0.3] Uncertainty on Vt (stat.error)
  (1)logLum [Lsun] [-0.5/3.4] Luminosity derived from the Subaru spectra (phys.luminosity;em.opt)
  (1)e_logLum [Lsun] [0.017/0.7] Uncertainty on logLum (stat.error)
  (1)Teff-L K [4376/6597] Effective temperature derived from LAMOST spectra (phys.temperature.effective)
  (1)logg-L [cm/s2] [0.8/5.2] Surface gravity derived from LAMOST spectra (phys.gravity)
  (1)FeH-L [-] [-4.2/-1.3] Metallicity derived from LAMOST spectra (phys.abund.Fe)
  (1)Abund (char) Display the abundance data for this source (link to Table 3) (meta.ref.url)
  (2)Ion (char) Species of atom (phys.atmol.ionStage)
  (2)l_logeps (char) Limit flag for logeps (meta.code.error)
  (2)logeps [-] (n) [-2.9/8.42] Log number abundance of Ion (meta.id;meta.main)

ALL cols
    
(n) indicates a possible blank or NULL column(i)indexed column
  (2)l_XFe (char) Limit flag for XFe (meta.code.error)
  (2)XFe [-] (n) [-2.2/4.6] Abundance ratio of [X/Fe] (phys.abund)
  (2)sigTeff  (n) [-0.31/0.5] Abundance error associated with Teff uncertainty (stat.error)
  (2)siglogg  (n) [-0.26/0.26] Abundance error associated with logg uncertainty (stat.error)
  (2)sigFeH  (n) [-0.15/0.11] Abundance error associated with [Fe/H] uncertainty (stat.error)
  (2)sigvt  (n) [-0.22/0.14] Abundance error associated with microturbulent velocity uncertainty (stat.error)
  (2)sigN  (n) [0/0.8] Abundance error associated with measurement uncertainty (stat.error)
  (2)sigTot  (n) [0.01/0.8] Total abundance error (stat.error)
  (2)Nl   [0/163] Number of adopted lines (meta.number)

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