High resolution Cluster set
Contact Klaus Dolag (kdolag@pd.astro.it)

Parameters and Cosmological models

Parameter used
H0 Ohm0 Lam0 Sigma8 z_ini m_dm [Msol/h] f_bary [%]
0.7 0.3 0.7 0.9 60 1.3e9 13


Simulated Clusters

Clusters
References Included Physics
Name Images Haloes dm gas gas_nv csf csfc m1
g676 g676_gas
g676_gas_log_t
ID Mass M(z) M(z) M(z) M(z) M(z) M(z)
a 1.1e14 mz mz mz mz mz mz
 
 
Name Images Haloes dm gas gas_nv csf csfc m1
g914 g914_gas
g914_gas_log_t
ID Mass M(z) M(z) M(z) M(z) M(z) M(z)
a 1.3e14 mz mz mz mz mz mz
 
 
Name Images Haloes dm gas gas_nv csf csfc m1
g1542 g1542_gas
g1542_gas_log_t
ID Mass M(z) M(z) M(z) M(z) M(z) M(z)
a 1.1e14 mz mz mz mz mz mz
 
 
Name Images Haloes dm gas gas_nv csf csfc m1
g3344 g3344_gas
g3344_gas_log_t
ID Mass M(z) M(z) M(z) M(z) M(z) M(z)
a 1.1e14 mz mz mz mz mz mz
 
 
Name Images Haloes dm gas gas_nv csf csfc m1
g6212 g6212_gas
g6212_gas_log_t
ID Mass M(z) M(z) M(z) M(z) M(z) M(z)
a 1.1e14 mz mz mz mz mz mz
 
 
Name Images Haloes dm gas gas_nv csf csfc m1
g1 g1_gas
g1_gas_log_t
ID Mass M(z) M(z) M(z) M(z) M(z) M(z)
a 1.5e15 mz mz mz mz mz mz
b 4.8e14 mz mz mz mz mz mz
c 1.8e14 mz mz mz mz mz mz
d 1.6e14 mz mz mz mz mz mz
e 8.0e13 mz mz mz mz mz mz
f 5.6e13 mz mz mz mz mz mz
 
Name Images Haloes dm gas gas_nv csf csfc m1
g8 g8_gas
g8_gas_log_t
ID Mass M(z) M(z) M(z) M(z) M(z) M(z)
a 2.3e15 mz mz mz mz mz mz
b 1.3e14 mz mz mz mz mz mz
c 9.6e13 mz mz mz mz mz mz
d 9.4e13 mz mz mz mz mz mz
e 8.6e13 mz mz mz mz mz mz
f 5.8e13 mz mz mz mz mz mz
g 5.3e13 mz mz mz mz mz mz
 
Name Images Haloes dm gas gas_nv csf csfc m1
g51 g51_gas
g51_gas_log_t
ID Mass M(z) M(z) M(z) M(z) M(z) M(z)
a 1.3e15 mz mz mz mz mz mz
 
 
Name Images Haloes dm gas gas_nv csf csfc m1
g72 g72_gas
g72_gas_log_t
ID Mass M(z) M(z) M(z) M(z) M(z) M(z)
a 1.4e15 mz mz mz mz mz mz
b 2.0e14 mz mz mz mz mz mz

Note: The table is ment to acces some images and information, and also reflects the progress of the project.