VizieR

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VizieR

  
J/MNRAS/418/1526
  Dark matter in dSph galaxies (Charbonnier+, 2011)
Post annotation
  
1.J/MNRAS/418/1526/cls_sclSculptor dSph clump luminosity (40 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)
  alpha deg Integration angle, αint (stat.fit.param)
  J Msun+2/kpc5Integration angle dependence, J(αint) (Note 1)   (stat.fit.param)
  CL68lo Msun+2/kpc3Most-likely, 68% clump luminosity on the quantity J(αint), lower limit (phys.luminosity;em.gamma)
  CL68up Msun+2/kpc3Most-likely, 68% clump luminosity on the quantity J(αint), higher limit (phys.luminosity;em.gamma)
  CL95lo Msun+2/kpc3Most-likely, 95% clump luminosity on the quantity J(αint), lower limit (phys.luminosity;em.gamma)
  CL95up Msun+2/kpc3Most-likely, 95% clump luminosity on the quantity J(αint, higher limit (phys.luminosity;em.gamma)

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