Parameters and Cosmological models

Parameter used
				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		ID	Mass	M(z)	M(z)	M(z)	M(z)	M(z)	M(z)
		a	1.1e14
Name	Images	Haloes		dm	gas	gas_nv	csf	csfc	m1
g914		ID	Mass	M(z)	M(z)	M(z)	M(z)	M(z)	M(z)
		a	1.3e14
Name	Images	Haloes		dm	gas	gas_nv	csf	csfc	m1
g1542		ID	Mass	M(z)	M(z)	M(z)	M(z)	M(z)	M(z)
		a	1.1e14
Name	Images	Haloes		dm	gas	gas_nv	csf	csfc	m1
g3344		ID	Mass	M(z)	M(z)	M(z)	M(z)	M(z)	M(z)
		a	1.1e14
Name	Images	Haloes		dm	gas	gas_nv	csf	csfc	m1
g6212		ID	Mass	M(z)	M(z)	M(z)	M(z)	M(z)	M(z)
		a	1.1e14
Name	Images	Haloes		dm	gas	gas_nv	csf	csfc	m1
g1		ID	Mass	M(z)	M(z)	M(z)	M(z)	M(z)	M(z)
		a	1.5e15
		b	4.8e14
		c	1.8e14
		d	1.6e14
		e	8.0e13
		f	5.6e13
Name	Images	Haloes		dm	gas	gas_nv	csf	csfc	m1
g8		ID	Mass	M(z)	M(z)	M(z)	M(z)	M(z)	M(z)
		a	2.3e15
		b	1.3e14
		c	9.6e13
		d	9.4e13
		e	8.6e13
		f	5.8e13
		g	5.3e13
Name	Images	Haloes		dm	gas	gas_nv	csf	csfc	m1
g51		ID	Mass	M(z)	M(z)	M(z)	M(z)	M(z)	M(z)
		a	1.3e15
Name	Images	Haloes		dm	gas	gas_nv	csf	csfc	m1
g72		ID	Mass	M(z)	M(z)	M(z)	M(z)	M(z)	M(z)
		a	1.4e15
		b	2.0e14

• The M(z) images appears indicates, that the simulation is finished, all data are transfered to the data server leonardo and post processing was performed up to mergertree reconstruction.