VizieR Search Page [Back] ⋅ [Forwd] ⋅ [Print] ⋅ [Close]
  
J/MNRAS/418/1526
  Dark matter in dSph galaxies (Charbonnier+, 2011)
ReadMe+ftp
2011MNRAS.418.1526C
Similar Catalogs
Post annotation 		  
1.J/MNRAS/418/1526/cls_carCarina dSph clump luminosity (40 rows)
2.J/MNRAS/418/1526/cls_draDraco dSph clump luminosity (40 rows)
3.J/MNRAS/418/1526/cls_forFornax dSph clump luminosity (40 rows)
4.J/MNRAS/418/1526/cls_sclSculptor dSph clump luminosity (40 rows)
5.J/MNRAS/418/1526/cls_sexSextans dSph clump luminosity (40 rows)
6.J/MNRAS/418/1526/cls_umiUrsae Minor dSph clump luminosity (40 rows)

Simple ConstraintList Of Constraints
 
Query by Constraints constraints help applied on Columns (Output Order: + - )
ShowSortJoin tables
more join
Column  Constraint Explain   (UCD)
  (ALL)recno  Record number assigned by the VizieR team. Should Not be used for identification. (meta.record)
   (ALL)alpha deg Integration angle, {alpha}int (stat.fit.param)
   (ALL)J Msun+2/kpc5Integration angle dependence, J({alpha}int) (Note 1)   (stat.fit.param)
   (ALL)CL68lo Msun+2/kpc3Most-likely, 68% clump luminosity on the quantity J({alpha}int), lower limit (phys.luminosity;em.gamma)
   (ALL)CL68up Msun+2/kpc3Most-likely, 68% clump luminosity on the quantity J({alpha}int), higher limit (phys.luminosity;em.gamma)
   (ALL)CL95lo Msun+2/kpc3Most-likely, 95% clump luminosity on the quantity J({alpha}int), lower limit (phys.luminosity;em.gamma)
   (ALL)CL95up Msun+2/kpc3Most-likely, 95% clump luminosity on the quantity J({alpha}int, higher limit (phys.luminosity;em.gamma)

ALL cols		    
 (i)indexed column
Adapt form
 Display your selection only Reset to default columns
usage  Display UCD1+    UCD1  
elapse time 1