Table 3: Orbital solutions corresponding to the RVs of the N  IV $\lambda $4058 emission line within different data sets. The quoted errors correspond to 1$\sigma $ uncertainties. Symbols have the canonical meaning. The last three correspond, respectively, to the mass function, the standard deviation of the fit and the number of data points involved.
    HRS only   HRS+MRS+LRS   All + published

P [d]		   208.3 $\pm$ 0.2   207.9 $\pm$ 0.1   207.85 $\pm$ 0.02
V0 [km s-1]   -30.6 $\pm$ 0.7   -34.2 $\pm$ 0.7   -34.6 $\pm$ 0.5
K [km s-1]   33 $\pm$ 2   42 $\pm$ 2   44 $\pm$ 2
e   0.35 $\pm$ 0.03   0.48 $\pm$ 0.02   0.50 $\pm$ 0.02
$\omega$ [degrees]   227 $\pm$ 4   216 $\pm$ 3   215 $\pm$ 3
$T_{\rm Periast}$ [d]$^{\ast}$   1598 $\pm$ 3   1597 $\pm$ 2   1598 $\pm$ 1
$T_{\rm RV max}$ [d]$^{\ast}$   1654 $\pm$ 3   1655 $\pm$ 2   1654 $\pm$ 1
$a~\sin i$ [$R_\odot$]   125 $\pm$ 8   151 $\pm$ 9   156 $\pm$ 8
$F(\mathcal{M})$ $[M_\odot]$   0.6 $\pm$ 0.1   1.1 $\pm$ 0.2   1.2 $\pm$ 0.2
$\sigma $ [km s-1]   2.5       3.7       4.7    
n   50       70       124    

$\ast$: Heliocentric Julian Date 2 450 000+.

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