# Cluster Number Counts for no-evolution of the X-ray luminosity function, 
# from Rosati et al.  Annu.Rev.Astron.Astrohys. 2002, 40, 539 (Fig.7).
#Col 1 - Flux S in (0.5-2.0 keV) band
#Col 2 - Number of clusters per deg^2 at flux>S
#
  9.99999996E-12  0.00125596754
  6.30957352E-12  0.00292663602
  3.98107155E-12  0.00640544761
  2.51188632E-12  0.0133626685
  1.58489313E-12  0.0268354099
  9.99999996E-13  0.0522356331
  6.30957309E-13  0.0990179405
  3.98107139E-13  0.18338941
  2.51188637E-13  0.332626462
  1.58489311E-13  0.591761768
  9.99999915E-14  1.03385556
  6.30957282E-14  1.77463114
  3.98107145E-14  2.99076033
  2.5118862E-14  4.93987989
  1.584893E-14  7.98845148
  9.99999898E-15  12.6505318
  6.30957256E-15  19.6380596
  3.98107137E-15  29.8870926
  2.51188616E-15  44.7268181
  1.58489298E-15  65.9893265
  9.99999898E-16  96.1079102
  6.30957278E-16  138.451157
  3.981071E-16  197.119751
  2.511886E-16  277.585327
  1.58489288E-16  386.079041
  9.99999818E-17  529.481445