Table 1: Table of observed and calculated properties of select systems.

We list the properties of the observed white dwarf systems hosting dusty debris disks, along with our computed sublimation radii within those systems for various planetary materials and rigid-body Roche limits for typical endmember planetesimal densities. The observed locations of the disks are in alignment with the calculated sublimation radii (inner disk edge) and Roche radii (outer disk edge).

System	Observed Properties				Disk Inner Edge/Sublimation Radius ($R_{\odot }$)				Rigid Roche Limit ($R_{\odot }$)
	Teff (K)	Mass ($M_{\odot }$)	Cooling Ages (MYR)	Modeled Disk range ($R_{\odot }$)	Forsterite	Fayalite	Iron	Enstatite	$\frac{{\rho }_{object}}{2000}$ = kg/m3	$\frac{{\rho }_{object}}{3500}$ = kg/m3
G29–38	11357a	0.62	450	0.15 – 0.28b,c,d,e	0.11 – 0.13	0.16 – 0.19	0.15 – 0.18	0.30 – 0.35	0.92 – 0.99	0.77 – 0.82
WD 2115-560	9674f	0.59b	640	0.17 – 0.32b	0.08	0.11	0.11	0.21	0.98	0.81
GD 362	9740g	0.71l		0.08 – 0.50b	0.072	0.11	0.10	0.20	1.00	0.83
GD 56	151510b	0.62b	200	0.21 – 0.58b	0.18 – 0.19	0.27 – 0.29	0.26 – 0.27	0.51 – 0.54	0.90 – 0.93	0.75 – 0.77
PG 1541+651	11,278h	0.60h	440	0.13 – 0.36i	0.10	0.16	0.15	0.29	1.01	0.84
LSPM J0207+3331	6120j	0.69j	3000	0.047 – 0.21, ~0.94	0.030	0.044	0.041	0.081	0.99	0.82
PG 0010+280	24206h	0.52h	17	Inner:0.13 – 0.65k Outer:0.52 – 1.3k	0.66	0.98	0.93	1.8	0.93	0.77

^[a]Refs: Kepler & Nelan, 1993

^[b] von Hippel et al. 2007

^[c]Zuckerman & Becklin, 1997

^[d] Jura, 2003

^[e] Reach et al. 2005

^[f] Koester et al. 2005

^[g] Gianninas et al. 2004

^[h] Gianninas et al. 2011

^[i] Kilic et al. 2012

^[j] Debes et al. 2019

^[k] Xu et al. 2015

^[l] Kilic et al. 2008