Unravelling sub-stellar magnetospheres | Astronomy & Astrophysics (A&A)

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Table C.1

List of the priors adopted for each parameter in our model.

Parameter	Value
cos i	𝒰(0, 1)
β(º)	𝒰(0, 90)
ϕ₀	𝒰(0, 1)
α (º)	𝒰(0, 90)
∆α (º)	𝒰(0, 10)
θ_B(º)	𝒰(0, θ_max)
ϕ_B (º)	𝒰(0, 360)
F_B (mJy)	𝒰(1, 10)

Notes. Each value is drawn from a uniform distribution 𝒰, with the proceeding numbers indicating the lower and upper limit. Throughout the paper, the subscript ‘B’ is interchanged for the AFL number (in our case, 1 or 2).

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