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  The simultaneous optical-to-X-ray SED of AGNs (Grupe+, 2010)
Post annotation
1.J/ApJS/187/64/table5Properties of the Spectral Energy Distribution (91 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)
  Seq  Running number (;meta.main)
  Name (char) Object identification (
  Segment (char) Segment number(s) (;obs)
  alphaX  X-ray slope in the 0.2-2.0keV energy range (spect.index)
  e_alphaX  Uncertainty on AlphaX (stat.error)
  alphaUV  Optical/UV slope corrected for Galactic reddening (spect.index)
  e_alphaUV  Uncertainty on AlphaUV (stat.error)
  alphaOX  UV-to-X-ray spectra slope αox, as defined by Tananbaum et al. (1979ApJ...234L...9T) (spect.index)
  alphaUVc  (n) Optical/UV slope corrected for Galactic and intrinsic reddening (spect.index)
  e_alphaUVc  (n) Uncertainty on AlphaUVc (stat.error)

ALL cols
(n) indicates a possible blank or NULL column(i)indexed column
  alphaOXc  (n) UV-to-X-ray spectra slope αox, corrected for Galactic & intrinsic reddening (spect.index)
  logLx [W] Rest-frame 0.2-2.0keV X-ray luminosity (phys.luminosity;em.X-ray)
  logLbbb [W] Luminosity in the BBB (big-blue-bump) emission (Note 1)   (phys.luminosity;em.opt.B)
  L/LEdd  L/LEdd ratio (phys.luminosity;arith.ratio)
  logLbbb2 [W] Luminosity using the broken power-law model as shown in Figure 1 (phys.luminosity;em.opt.B)
  log5100 [W] Luminosity at 5100Å (phys.luminosity)
  logLbbbc [W] (n) logLbbb corrected for intrinsic reddening (phys.luminosity;em.opt.B)
  L/LEddc  (n) L/LEdd corrected for intrinsic reddening (phys.luminosity;arith.ratio)
  log5100c [W] (n) log5100 corrected for intrinsic reddening (phys.luminosity)

ALL cols
(n) indicates a possible blank or NULL column(i)indexed column
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