Constraining differential rotation in γ Doradus stars from the properties of inertial dips

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Table G.1.

Results of three different implementations of the MCMC.

	α_rot	Γ(h)	Ω_env/2π	Π₀(s)

Input	0.98	10	2.16	4175
Case 1	$0 . 974_{- 0.001}^{0.001}$ $0.974^{0.001}_{-0.001}$	$12 . 96_{- 0.12}^{0.12}$ $12.96^{0.12}_{-0.12}$	$2 . 167_{- 0.29}^{0.13}$ $2.167^{0.13}_{-0.29}$	$4232_{- 2}^{2}$ $4232^{2}_{-2}$
Case 2	$0 . 981_{- 0.003}^{0.003}$ $0.981^{0.003}_{-0.003}$	$12 . 50_{- 1.13}^{1.13}$ $12.50^{1.13}_{-1.13}$	$2 . 166_{- 0.001}^{0.001}$ $2.166^{0.001}_{-0.001}$	$4260_{- 17}^{10}$ $4260^{10}_{-17}$
Case 3	$0 . 981_{- 0.004}^{0.004}$ $0.981^{0.004}_{-0.004}$	$10 . 66_{- 1.49}^{1.80}$ $10.66^{1.80}_{-1.49}$	$2 . 168_{- 0.011}^{0.008}$ $2.168^{0.008}_{-0.011}$	$4235_{- 37}^{28}$ $4235^{28}_{-37}$

Notes. The values of the retrieved parameters along with their uncertainties are shown, as well as the listed input parameters on the first row. Uncertainties are given in term of the 16th and 84th percentiles around the 50th percentile of the samples in the marginalized distributions.

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