Table A.10

Normalized power P and cv values inferred from the bp-corrected GLS (P_bp, cv_bp) and oc-corrected GLS (P_oc, cv_oc) for HD 192310. They are evaluated at the stellar rotation period (P_rot) and at the at the orbital periods (P_orb) of the hosted exoplanets found by Pepe et al. (2011). The first two rows show P inferred from the ∆RV^* signals, while in the last row P are computed after removing the Keplerian signal of P_orb,1 = 75 days from the ∆RV^* signals. Both the two planets would be visible in the GLS after applying the bp method and the iterative removal of planetary signals, as P_bp are always above the respective cv_bp values.