VizieR

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

VizieR

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/ApJ/931/147
  Very metal-poor stars with LAMOST & Subaru. II. (Li+, 2022)
Post annotation
img(gal)
1.J/ApJ/931/147/table2Stellar parameters of the program stars (385 rows)

 
Query by Constraints constraints help applied on Columns (Output Order: + - )
ShowSortColumn  Constraint Explain   (UCD)
  recno  Record number assigned by the VizieR team. Should Not be used for identification. (meta.record)
  ID (char) (i) Short ID of a star, Paper I (Aoki+ 2022, J/ApJ/931/146) (meta.id)
  RAJ2000 deg (i) Right Ascension in degrees (J2000) (pos.eq.ra;meta.main)
  DEJ2000 deg (i) [-7.1/60.6] Declination in degrees (J2000) (pos.eq.dec;meta.main)
  RVel km/s [-454/434] Radial velocity (observed) (phys.veloc;pos.heliocentric)
  SNR   [6.9/157] Spectral SNR around 4500 Angstrom (stat.snr)
  Teff K [4290/6731] Effective temperature derived from Subaru spectra (phys.temperature.effective)
  e_Teff K [7/584] Uncertainty on Teff (stat.error;phys.temperature.effective)
  logg [cm/s2] [0.5/4.8] Surface gravity derived from Subaru spectra (phys.gravity)
  e_logg [cm/s2] [0.01/0.7] Uncertainty on logg (stat.error)
  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
  FeH [-] [-4.4/-0.6] Metallicity derived from Subaru spectra (phys.abund.Fe)
  e_FeH [-] [0.08/0.4] Uncertainty on FeH (stat.error)
  vt km/s [0/4.1] Microturbulent velocity derived from Subaru spectra (phys.veloc)
  e_vt km/s [0.03/0.3] Uncertainty on Vt (stat.error)
  logLum [Lsun] [-0.5/3.4] Luminosity derived from the Subaru spectra (phys.luminosity;em.opt)
  e_logLum [Lsun] [0.017/0.7] Uncertainty on logLum (stat.error)
  Teff-L K [4376/6597] Effective temperature derived from LAMOST spectra (phys.temperature.effective)
  logg-L [cm/s2] [0.8/5.2] Surface gravity derived from LAMOST spectra (phys.gravity)
  FeH-L [-] [-4.2/-1.3] Metallicity derived from LAMOST spectra (phys.abund.Fe)
  Abund  Display the abundance data for this source (link to Table 3) (meta.ref.url)

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