The ALMA survey to Resolve exoKuiper belt Substructures (ARKS) - III. The vertical structure of debris disks

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Volume 705 (January 2026)

A&A, 705 (2026) A197

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Table 2

Summary of the fiducial parametric models for each source along with the best-fit and median values of h_HWHM and inclination (errors showing the 16th and 84th percentiles).

Source	Radial Form	Vertical Form	h_HWHM		i
			Best-fit	50th Percentile	Best-fit	50th Percentile
HD 9672	DPL	vL	0.041	${0.046}_{- 0.008}^{+ 0.008}$ $0.046_{ - 0.008}^{ + 0.008}$	80.03°	${80.18}^{\circ}_{- 0.14}^{+ 0.12}$ ${80.18^ \circ }_{ - 0.14}^{ + 0.12}$
HD 10647	DG	vDG	0.052 (91%)	${0.053}_{- 0.007}^{+ 0.006} (88 \pm 6 %)$ $0.053_{ - 0.007}^{ + 0.006}(88 \pm 6{\rm{\% }})$	78.74°	${0.225}_{- 0.002}^{+ 0.002} (12 \pm 6 %)$ $0.225_{ - 0.002}^{ + 0.002}(12 \pm 6{\rm{\% }})$
			0.226 (9%)	${80.83}^{\circ}_{- 0.18}^{+ 0.21}$ ${80.83^ \circ }_{ - 0.18}^{ + 0.21}$ (12 ± 6%)
HD 14055	DPL	vG	0.059	${0.053}_{- 0.008}^{+ 0.007}$ $0.053_{ - 0.008}^{ + 0.007}$	80.0°	${80.0}^{\circ}_{- 0.3}^{+ 0.2}$ ${80.0^ irc }_{ - 0.3}^{ + 0.2}$
HD 15115	DG	vL	0.021	${0.022}_{- 0.002}^{+ 0.002}$ $0.022_{ - 0.002}^{ + 0.002}$	86.74°	${86.79}^{\circ}_{- 0.04}^{+ 0.05}$ ${86.79^ irc }_{ - 0.04}^{ + 0.05}$
HD 32297	DPL	vL	0.0098	${0.0092}_{- 0.0012}^{+ 0.0012}$ $0.0092_{ - 0.0012}^{ + 0.0012}$	88.48°	${88.48}^{\circ}_{- 0.03}^{+ 0.04}$ ${88.48^ irc }_{ - 0.03}^{ + 0.04}$
HD 39060	DPL	vL	0.112	${0.112}_{- 0.001}^{+ 0.002}$ $0.112_{ - 0.001}^{ + 0.002}$	87.65°	${87.66}^{\circ}_{- 0.13}^{+ 0.17}$ ${87.66^ irc }_{ - 0.13}^{ + 0.17}$
HD 61005	DG	vL	0.0129	${0.0143}_{- 0.0021}^{+ 0.0020}$ $0.0143_{ - 0.0021}^{ + 0.0020}$	86.23°	${86.24}^{\circ}_{- 0.04}^{+ 0.03}$ ${86.24^ irc }_{ - 0.04}^{ + 0.03}$
HD 76582	AG	vL	0.193	${0.192}_{- 0.009}^{+ 0.009}$ $0.192_{ - 0.009}^{ + 0.009}$	72.1°	${72.6}^{\circ}_{- 0.6}^{+ 0.7}$ ${72.6^ irc }_{ - 0.6}^{ + 0.7}$
HD 109573	DG	vG	0.0065	${0.0082}_{- 0.0038}^{+ 0.0033}$ $0.0082_{ - 0.0038}^{ + 0.0033}$	76.57°	${76.62}^{\circ}_{- 0.10}^{+ 0.09}$ ${76.62^ irc }_{ - 0.10}^{ + 0.09}$
HD 131488	DG	vG	0.0048	${0.0059}_{- 0.0010}^{+ 0.0011}$ $0.0059_{ - 0.0010}^{ + 0.0011}$	84.91°	${84.87}^{\circ}_{- 0.05}^{+ 0.05}$ ${84.87^ irc }_{ - 0.05}^{ + 0.05}$
HD 131835	DG	vL	0.017	${0.022}_{- 0.006}^{+ 0.007}$ $0.022_{ - 0.006}^{ + 0.007}$	74.5°	${74.6}^{\circ}_{- 0.2}^{+ 0.2}$ ${74.6^ irc }_{ - 0.2}^{ + 0.2}$
HD 161868	DPL	vL	0.192	${0.192}_{- 0.016}^{+ 0.012}$ $0.192_{ - 0.016}^{ + 0.012}$	66.7°	${66.7}^{\circ}_{- 0.9}^{+ 0.9}$ ${66.7^ irc }_{ - 0.9}^{ + 0.9}$
HD 197481	DPL	vL	0.0026	${0.0028}_{- 0.0002}^{+ 0.0009}$ $0.0028_{ - 0.0002}^{ + 0.0009}$	88.16°	${88.13}^{\circ}_{- 0.09}^{+ 0.08}$ ${88.13^ irc }_{ - 0.09}^{ + 0.08}$

Notes. The full set of parametric modeling results, including all free parameters for the fiducial models and the AIC/BIC for each tested model, is presented in Table A.1.

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