Chemo-dynamics of the stellar component of the Sculptor dwarf galaxy - I. Observed properties

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Table B.1

Priors used the free parameters of each population.

Parameter	Prior
m [dex/deg]	[-1,1]
ℳ₀	[-3,0]
ℳ	[-3,0]
σ_ℳ	[0,5]
𝒱 [km s⁻¹]	[90,130]
σ_𝒱 [km s⁻¹]	[0,13]
R_h [deg]	[0,2]

Notes. Range of the uniform priors used to run MCMC. Column 1 lists the parameters and Col. 2 the range for the uniform prior. For populations with a metallicity gradient ℳ₀ and m are used, while for the populations without the metallicity gradient only ℳ is needed.

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