DoAr 33: a good candidate for revealing dust growth and settling in protoplanetary disks

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Table A.1

Starting points of the Markov chains for both disk scenarios.

Parameter	I	II	III	IV	V

L_⋆ [L_⊙]	1.0	1.2	1.4	1.5	1.2
R_in [AU]	0.1	0.1	0.2	1.0	0.3
R_out [AU]	200	300	400	350	300
M_dust [10^-5 M_⊙]	5	10	50	25	50
α	1.55	2.00	2.5	2.7	2.0
β	1.05	1.10	1.20	1.15	1.05
h₁₀₀ [AU]	8.00	10.0	15.0	10.0	7.0
	10.0	12.0	8.0	10.0	14.0
ϵ ⁽¹⁾	0.1	0.01	0.001	0.005	0.001
a_max [μm] ⁽²⁾	1000	512	1000	1000	800
i [°]	60	45	30	60	50

Notes. (1) For the well-mixed model, H_ratio and ϵ are fixed to 1 (see Sect. 2.2.2). (2) For the settled disk model (see Sect. 2.2.1), a_max represents the maximum grain size for the large grain population.

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