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  The Auriga-California molecular cloud (Broekhoven-Fiene+, 2014)
Post annotation
1.J/ApJ/786/37/sedSED modelling results in Class II (table 7) and Class III table 8) sources (108 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)
  Class (char) II for Class II sources (table 7) and III for Class III sources (table 8) (src.class)
  ID   [2/166] YSO ID number (
  Fitted (char) [K7-A0] Fitted stellar spectrum to the SED (src.spType)
  Av mag Extinction value fitted to the optical data (phys.absorption;em.opt)
  L* Lsun Luminosity of the fitted stellar component (phys.luminosity)
  lambda-TO um Last wavelength before an excess >80% is measured (Note 1)   (em.wl.effective)
  alpha-ex  (n) Slope of SED across wavelengths longward of lambda-TO (Note 2)   (spect.index)
  Ld/L*  Ratio of disk luminosity to luminosity of fitted stellar component (phys.luminosity;arith.ratio)

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