VizieR

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

VizieR

  
J/A+A/665/A46
  High-precision abundance of the Helmi streams (Matsuno+, 2022)
ReadMe+ftp
2022A&A...665A..46M
Similar Catalogs
Post annotation 		img(gal)
1.J/A+A/665/A46/table5Linelist and line-by-line abundance (1952 rows)

Simple ConstraintList Of Constraints
 
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)
  Object (char) Object name used in this study (meta.id;meta.main)
  Species (char) Name of the species (phys.atmol.element)
  lambda 0.1nm Wavelength (em.wl)
  chi eV Excitation potential (phys.atmol.excitation)
  loggf  log gf value (phys.absorption.coeff)
  EW 0.1pm Equivalent width (in mÅ) (spect.line.eqWidth)
  e_EW 0.1pm Uncertainty in equivalent width (in mÅ) (stat.error;spect.line.eqWidth)
  A  Abundance from this line (phys.abund)
  eATeff  Uncertainty in abundance due to effective temperature (stat.error)
  eAlogg  Uncertainty in abundance due to surface gravity (stat.error)
  eAvt  Uncertainty in abundance due to microturbulent velocity (stat.error)
  eA[Fe/H]  Uncertainty in abundance due to metallicity (stat.error)
  eAEW  Uncertainty in abundance due to equivalent widths of this star and the reference star (stat.error)
  sX  Uncertainty floor (stat.error)
  Weight  Weight used to obtain the best estimate for the abundance of the species (phys.atmol.weight;meta.modelled)

ALL cols		    
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usage  Display UCD1+    UCD1  
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