Table C.1
Priors imposed in the radial-velocity analyses.
| γHN-1[m s−1] | U] − ∞, + ∞[ |
| γHN-2[ms s−1] | U] − ∞, + ∞[ |
| γHIRES[m s−1] | U] − ∞, + ∞[ |
| σj, HN-1[m s−1] | U[0, + ∞ [ |
| σj, HN-2[m s−1] | U[0, + ∞[ |
| σj, HIRES[m s−1] | U[0, + ∞ [ |
| h [m s−1] | U[0, + ∞[ |
| λ [days] | U[0, 300] |
| Prot [days] | U[10, 80] |
| w | U[0.1, 5] |
| Kepler-10 b | |
| Tc[BJDTDB−2450000] |  (5034.08687, 1.8 E-04) |
| P [days] |  (0.83749070, 2.0 E-07) |
| e | 0 (fixed) |
| K [m s−1] | U[0, +∞ [ |
| Kepler-10 c | |
| Tc[BJDTDB−2450000] |  (5062.26648, 8.1 E-04) |
| P [days] |  (45.294301, 4.8 E-05) |
| e |  (0.0, 0.098) AND e < 1 |
| K [m s−1] | U[0, +∞[ |
| Kepler-10 d | |
| Tc[BJDTDB–2450000] | U[7100, 7220] |
| P [days] | U[0, +∞[ |
| e |  AND e < 1 |
| K [m s−1] | U[0, +∞[ |
Notes. γ and σj are the RV zero points and uncorrelated jitter terms (HN-1 and HN-2 refer to the old and new HARPS-N CCD, respectively); h, λ, Prot, and w are the Gaussian process hyper-parameters namely the radial-velocity semiamplitude, the exponential decay time, the rotation period, and the inverse harmonic complexity term; P and Tc are the orbital period and inferior conjunction times; e is the orbital eccentricity; and K is the RV semiamplitude. 
and U stand for normal (Gaussian) and uniform priors, respectively.
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