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  Large Bright Quasar Survey emission lines (Forster+, 2001)
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1.J/ApJS/134/35/table1LBQS quasars excluded from emission line measurements (65 rows)
2.J/ApJS/134/35/table5Representative emission line measurements (29760 rows)
3.J/ApJS/134/35/table6Representative continuum measurements (992 rows)

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Column  Constraint Explain   (UCD)
  (ALL)recno  Record number assigned by the VizieR team. Should Not be used for identification. (meta.record)
   (ALL)LBQS (char) Designation in LBQS (Cat. J/AJ/109/1498) (;meta.main)
   (ALL)LBQS_data (char) Link to all parameters of Large Bright QSO Survey (1995AJ....109.1498H) (
   (ALL)z  Redshift (src.redshift)
  (1)Ref (char) References (Note 1)   (meta.ref)
  (1)Notes (char) Notes (Note 2)   (meta.note)
  (2)Line (char) Emission line name (
  (2)FWHM km/s Full width at half maximum of Line (spect.line.width)
  (2)E_FWHM km/s Positive error on FWHM (stat.error)
  (2)e_FWHM km/s Negative error on FWHM (stat.error)
  (2)Offset km/s Gaussian emission line model peak offset from the expected position (Note 1)   (phys.veloc;arith.diff)

ALL cols
 (i)indexed column
  (2)E_Offset km/s Positive error on Offset (stat.error)
  (2)e_Offset km/s Negative error on Offset (stat.error)
  (2)EW 0.1nm Rest frame equivalent width of line (in Å) (spect.line.eqWidth)
  (2)E_EW 0.1nm Positive error on EW (Note 2)   (stat.error)
  (2)e_EW 0.1nm Negative error on EW (Note 2)   (stat.error)
  (2)Num  Number of narrow absorption features used in modeling the emission lines (Note 3)   (meta.number)
  (3)NHGal 10+20/cm2Galactic neutral hydrogen column density (phys.columnDensity)
  (3)Sp+Index  Power law continuum slope (spect.index)
  (3)E_Sp+Index  Positive error on Sp+Index (stat.error)
  (3)e_Sp+Index  Negative error on Sp+Index (stat.error)
  (3)Wave nm Normalized rest frame wavelength (em.wl)
  (3)Flux 10-16W/m2/nmContinuum flux at Wave (in 10–14ergs/cm2/s/Å) (phot.flux.density;em.opt)
  (3)E_Flux 10-16W/m2/nmPositive error on Flux (stat.error)

ALL cols
 (i)indexed column
  (3)e_Flux 10-16W/m2/nmNegative error on Flux (stat.error)
  (3)Sp+Index2  Second power law continuum slope (spect.index)
  (3)E_Sp+Index2  Positive error on Sp+Index2 (stat.error)
  (3)e_Sp+Index2  Negative error on Sp+Index2 (stat.error)
  (3)Poly  Polynomial order required to model the blue region of the spectrum (

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