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  CHIANTI - An Atomic Database For Emission Lines I. (Dere+ 1997)
Post annotation
1.J/A+AS/125/149/table3A list of observed lines and lines in the CHIANTI database between 50 and 1100 Angstroms (1768 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)
  LamObs 0.1nm Observed wavelength from literature sources (Note 1)   (em.wl)
  LamCH 0.1nm Wavelength in CHIANTI database (em.wl)
  Ion (char) Ion (spectroscopic notation) (phys.atmol.ionization)
  Level1 (char) Description of lower level of transition (phys.atmol.qn)
  Level2 (char) Description of upper level of transition (phys.atmol.qn)
  Int mW/m2/sr Predicted intensity of line in a small solar flare (Note 2)   (spect.line.intensity)
  Ref (char) Literature sources of observed wavelength (Note 3)   (meta.ref)

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usage  Display UCD1+    UCD1  

The following problems were encountered in this VizieR run:
**** -bg is an obsolete option
**** -bg is an obsolete option
**** -bg is an obsolete option
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.errorfile=/tmp/VR01642.err (2018-05-27T05:25:49)
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