**Table 2:** Simulations: initial values.
N	Q	$M_{\rm disk}$	${\it z}$	$M_{\rm DM}$	$R_{\rm DM}$	$\alpha ~ r_{\rm m}$	${v_m}\over{{(\alpha G M_{\rm disk})}^{1/2}}$	halo
c1	0.5	1	2	0.64	0.64	1.9	0.67
c2	0.5	0.33	2	0.64	1.94	1.	1.08
c3	0.5	0.1	2	0.64	6.4	0.9	1.68
c4	1.5	0.33	2	0.64	1.94	1.	1.08
c5	1.5	0.1	2	0.64	6.4	0.9	1.68
c6	0.5	0.33	1	0.67	2.0	1.05	1.05
c7	0.5	0.1	1	0.67	6.7	1.	1.6
i1	1.5	0.33		0.64	1.94	1	1.08	cosm
i2	1.5	0.1		0.64	6.4	0.9	1.68	cosm
i3	1.5	0.33		0.64	1.94	1	1.08	cosm/frozen disk
i4	1.5	0.33		0.95	2.87	0.85	1.5	NFW
i5	1.5	0.1		0.95	9.5	1.27	1.25	NFW

Column 1: simulation number and simulation type (c: cosmological simulations, i: isolated simulations); Col. 2: Q initial value of the disk; Col. 3: mass of the disk in $5.9\times 10^{10}~ M_{\odot}$ ; Col. 4: initial redshift (for the cosmological cases); Col. 5: initial DM mass inside the disk radius; Col. 6: initial halo-to-disk mass ratio inside the disk radius; Cols. 7 and 8: Efstathiou et al. (1982) parameters, where: $\alpha={r_0}^{-1}$ , $v_{\rm m}$ is the maximum rotational velocity, and $r_{\rm m}$ the corresponding radius; Col. 9: type of halo used (for the isolated cases).

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