RANDOM CLUSTERS MOCK CATALOGUE [07/08/2003]

Same cosmological parameters as before BUT:
a) Cluster richness is increased (n*=30 with a small scatter), 
   as in Lobo et al.
b) Cut for the max. observed no. of members: 400 (otherwise clusters below 
   z=0.5 can have a too large no. of members (up to 3000)

As before, 5000 galaxies have been assigned in clusters;
now the no. of clusters is obviously smaller (49).
The field is the exactly the same as before, with 69000 galaxies.


 PARAMETERS

 H0 ......................... 65.
 Omega_M .................... 0.3
 Omega_Lambda ............... 0.7     

 Field (arcmin) ............. 60.x 60. square arcmin.
 Bright magnitude cutoff ....  17.00
 Limiting magnitude .........  24.00

 M* ......................... -22.50
 alpha ......................  -1.25

 Evolution factor ............ No
 z cutoff ...................  3.0


 BACKGROUND GALAXIES

 mcut <= Ngal <=mlim ........ 69000
 Clustering .................. No


 GALAXIES IN RANDOM CLUSTERS:

 mcut <= Ngal <=mlim ........   5000
 Cluster Centers ............. RANDOM              
 Average no. per clump <M* ...    30
 Max. observed members .......   400
 Sigma (km/s) ................   N* x 30
 Cutoff radius .................... 1.5 Mpc h^-1, i.e. 2.307692 Mpc