Table 1: Density, mass and mass perturbation ratios defining the satellite initial OD for the mergers in the SSIM.
$\epsilon$, panel * $M_{\rm ratio}$ $D_{\rm ratio}$ $M_{\rm OD}/M_{\rm BG}$ $^{\dagger}$
3/2, upper panel 0.751 0.282 1.173
3/2, middle panel $4.25\times10^{-2}$ $7.10\times10^{-2}$ $9.38\times10^{-2}$
3/2, lower panel $6.92\times10^{-2}$ 0.168 1.453
5/2, upper panel 0.889 $5.51\times10^{-2}$ 0.319
5/2, middle panel 0.439 $5.54\times10^{-2}$ 0.290
5/2, lower panel 0.178 0.454 1.133
2.9, upper panel 0.753 $9.19\times10^{-2}$ 0.416
2.9, middle panel 0.407 0.641 1.118
2.9, lower panel 0.301 $9.71\times10^{-2}$ 0.344
* Parent initial power-law seed and panel order in reference to Figs. 1-3.
$^{\dagger}$ OD perturbation compared to background region it spans, just before entering core.


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