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Table A.2

Prior distributions for the HD 40307 system.

Orbital parameters Prior distribution

Orbital period, P [days] J(1.0,104)
RV amplitude, K [m s-1] U(0.0,200)
Eccentricity, e B(0.867,3.03)
Argument of periastron, ω [deg] U(0,360)
Mean longitude at epoch, L0 [deg] U(0,360)
Systemic velocity, V0 [km s-1] U(28.996,33.668)
Velocity drift (long-term activity effect)

Scaling constant, α [m s-1/dex] U(0,100)
Linear [10-4 dex yr-1] N(373.8,8.6)
Quadratic [10-4 dex yr-2] N(46.3,4.6)
Cubic [10-4 dex yr-3] N(−17.3,1.0)
Noise model

Additional noise at = –5, σJ | -5.0 [m s-1] U(0,50)
Slope, αJ [m s-1/dex] U(0,50)

Notes. Priors are identical for all signals in the model. The epoch is BJD = 2 454 521.6791. The argument of periastron ω is unconstrained for these nearly-circular orbits. U(xmin;xmax): uniform distribution between xmin and xmax. J(xmin;xmax): Jeffreys (log-flat) distribution between xmin and xmax. N(μ;σ): normal distribution with mean μ and standard deviation σ. B(a,b): beta distribution.

(⋆)

See Sect. 4.3.

(‡)

The additional (stellar) noise for measurement i is .

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