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/A+A/661/A103
  High-precision chemical abundances of Sequoia (Matsuno+, 2022)
ReadMe+ftp
2022A&A...661A.103M
Similar Catalogs
Post annotation 		img(gal)
1.J/A+A/661/A103/list(c)List of studied stars (15 rows)
2.J/A+A/661/A103/lineLine list (3173 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. ((unassigned);phys.veloc.orbital;arith.diff;phys.veloc)
   (ALL)Object (char) Object name used in this study ((unassigned);phys.veloc.orbital;arith.diff;spect.line.veloc;arith)
  (1)RAJ2000 "h:m:s" Right ascension (J2000) ((unassigned);(unassigned);(unassigned);(unassigned);arith)
  (1)DEJ2000 "d:m:s" Declination (J2000) ((unassigned);(unassigned);(unassigned);(unassigned);arith)
  (1)OName (char) Gaia EDR3 name (Gaia EDR3 NNNNNNNNNNNNNNNNNNN) ((unassigned);(unassigned);(unassigned);spect.line.veloc)
  (1)Simbad (char) ask the Simbad data-base about this object ((unassigned);(unassigned);(unassigned);pos.geocentric)
  (2)species (char) Name of the species ((unassigned);phys.veloc.orbital;arith.diff;(unassigned))
  (2)lambda 0.1nm Wavelength ((unassigned);(unassigned);(unassigned);meta.bib.author)
  (2)chi eV Excitation potential ((unassigned);phys.veloc.orbital;arith.diff;(unassigned))
  (2)loggf  loggf value ((unassigned);phys.veloc.orbital;arith.diff;(unassigned))
  (2)EW 0.1pm Equivalent width (mÅ) ((unassigned);phys.veloc.orbital;arith.diff;phys.at.moment.magnetic;meta.main)

ALL cols		    
 (i)indexed column
  (2)e_EW 0.1pm Uncertainty in equivalent width (mÅ) ((unassigned);(unassigned);(unassigned);time.age;phys.atmol.number;meta.main)
  (2)A  Abundance from this line ((unassigned);(unassigned);(unassigned);phys.polarization.stokes.Q)
  (2)eAteff  Uncertainty in abundance due to effective temperature ((unassigned);(unassigned);(unassigned);time.age;meta.main)
  (2)eAlogg  Uncertainty in abundance due to surface gravity ((unassigned);(unassigned);(unassigned);time.age;meta.main)
  (2)eAvt  Uncertainty in abundance due to microturbulent velocity ((unassigned);(unassigned);(unassigned);time.age;meta.main)
  (2)eA[Fe/H]  Uncertainty in abundance due to metallicity ((unassigned);(unassigned);(unassigned);time.age;meta.main)
  (2)eAEW (char) Uncertainty in abundance due to equivalent widths of this star and the reference star ((unassigned);phys.veloc.orbital;arith.diff;time.age;meta.main)
  (2)sX  Uncertainty floor ((unassigned);phys.veloc.orbital;arith.diff;time.age;meta.main)
  (2)Weight  Weight used to obtain the best estimate for the abundance of the species ((unassigned);(unassigned);(unassigned);(unassigned);src.orbital.inclination)

ALL cols		    
 (i)indexed column
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