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  QSO low-z Lyα absorbers (Tripp+, 1998)
Post annotation
1.J/ApJ/508/200/table5Absorption lines detected in the GHRS G140L spectrum of PG 1116+215 (31 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)
  Lambda 0.1nm Vacuum heliocentric wavelength of the line centroid (em.wl;pos.heliocentric)
  n_Lambda (char) [c] Note on Lambda (Note 1)   (meta.note)
  EW 0.1pm (n) Observed equivalent width measured as described in Tripp et al., 1996ApJS..102..239T (spect.line.eqWidth)
  e_EW 0.1pm (n) rms uncertainty on EW (stat.error;spect.line.eqWidth)
  n_EW (char) [a e] Note on EW (1) (Note 3)   (meta.note)
  EWi 0.1pm (n) For strongly blended lines, individual equivalent widths derived from profile parameters measured with VPFIT (spect.line.eqWidth)
  Line (char) Line identification (Note 2)   (;spect.line)
  n_Line (char) [abd] Note on Line (3) (Note 1)   (meta.note)
  zabs  (n) Redshift measured with VPFIT from the G140L spectrum (src.redshift)
  HV km/s (n) Heliocentric line velocity for lines due to the Galactic ISM (spect.line;pos.heliocentric)

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