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Table A.6

Inferred and derived parameters from the RV-only analysis (Sect. 4.2) for the preferred model (labeled “2p1cF”) with the inner planet in a circular orbit and the external component in an eccentric orbit.

Parameter Priors Posteriors
Planet b

Orbital period, Pb [days] 𝒢(1.8237371,0.000012)
Time of mid-transit, T0,b −2400000 [days] 𝒢(59248.377773,0.003)
RV semi-amplitude, Kb [m/s] 𝒰(0.0,100.0)
Planet mass, mb sin ib [M] (derived)
Orbit semi-major axis, ab [AU] (derived)
Relative orbital separation, ab/R (derived)
Incident flux, Finc,b [Finc,] (derived)

Planet c

Orbital period, Pc [days] ℒ𝒰(100.0,5000.0)
Time of mid-transit, T0,c − 2400000 [days] 𝒰(57200.0,62900.0)
RV semi-amplitude, Kc [m/s] 𝒰(0.0,1500.0)
Orbital eccentricity, ec 𝒰(0.0,1.0)
Arg. periastron, ωc [deg.] 𝒰(0.0,360.0)
Planet mass, mc sin ic [MJup] (derived)
Orbit semi-major axis, ac [AU] (derived)
Relative orbital separation, ac/R (derived) 810±120
Incident flux, Finc,c [Finc,⊕] (derived)

Instrument-dependent parameters

δHARPS [km s−1] 𝒰(-10,10)
δcoralie [km s−1] 𝒰(-10,10)
δpfs [km s−1] 𝒰(-10,10)
σHARPS [m/s] ℒ𝒰(0.1,2)
σCORALIE [m/s] ℒ𝒰(0.1,30)
σPFS [m/s] ℒ𝒰(0.1,5)
δFWHM,HARPS [km s−1] 𝒰(-0.5,0.5)
δFwнм,coRALIE [km s−1] 𝒰(-0.5,0.5)
σFwнм,HARPS [m/s] ℒ𝒰(0.1,300)
σғwнм,coRALiE [m/s] ℒ𝒰(0.1,300)

GP parameters

η1,fwhm [m/s] ℒ𝒰(0.01,400)
η1 [m/s] ℒ𝒰(0.01,50)
η2 [days] 𝒰(-8.0,10)
η3 [days] 𝒢(24.0,1)
η4 𝒰(0.13,7.38)

Notes:

  • 𝒢(µ, σ): Normal distribution with mean µ and width σ

  • 𝒰(a, b): Uniform distribution between a and b

  • ℒ𝒰(a, b): Log-uniform distribution between a and b

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