VizieR

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

VizieR

  
J/other/Nat/601.45
  C-19 stream members (Martin+, 2022)
ReadMe+ftp
2022Natur.601...45M
Similar Catalogs
Post annotation 		img(gal)
1.J/other/Nat/601.45/table4Spectral lines and atomic data used for the chemical abundances for the Gemini/GRACES spectra (54 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)
  lambda 0.1nm Wavelength (em.wl)
  El (char) Element (phys.atmol.element)
  xi eV Energy (phys.energy;phys.atmol.level)
  loggf [-] Oscillator strength (phys.atmol.oscStrength)
  EW1 0.1pm (n) Equivalent width for Pristine 355.1+27.9 (spect.line.eqWidth)
  n_EW1 (char) Note on EW1 (Note 1)   (meta.note)
  l_EW2 (char) Limit flag on EW2 (meta.code.error)
  EW2 0.1pm (n) Equivalent width for Pristine 354.7+30.2 (spect.line.eqWidth)
  n_EW2 (char) Note on EW2 (Note 1)   (meta.note)
  l_EW3 (char) Limit flag on EW2 (meta.code.error)
  EW3 0.1pm (n) Equivalent width for Pristine 355.2+27.7 (spect.line.eqWidth)
  n_EW3 (char) Note on EW3 (Note 1)   (meta.note)
  NLTEcorra 0.1pm (n) NLTE correction estimates from the INSPECT (http://www.inspect-stars.com) and/or MPIA database (http://nlte.mpia.de) (Note 2)   (arith.factor)
  NLTEcorrb 0.1pm (n) NLTE corrections from the private calculations of coauthor L. Mashonkina (http://www.inasan.rssi.ru/~lima/pristine). Only the NaI NLTE corrections show some star to star variations due to the differences in the line strengths (the average from the three (Note)   (arith.factor)

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