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Table 2

Initial and final times of the intervals considered for the MCMC analysis, together with the uniform prior intervals of the parameters for the stars of our sample.

Star name t 1 t 2 i F 0 a 1,2 θ 1,2 Δλ1,2 P 1,2
(d) (d) (deg) (deg) (deg) (d)

Sun 19.8542 39.7084 70, 90 −0.03, 0.01 2 × 10-5, 0.060 0, 180 ± 13 24.0, 29.0
HD 52265 48.3125 60.2654 15, 45 −2 × 10-4, 2 × 10-4 2 × 10-7, 0.044 0, 150 ± 15 9.0, 14.0
HD 52265 60.3210 72.3890 15, 45 −2 × 10-4, 2 × 10-4 2 × 10-7, 0.044 0, 150 ± 15 9.0, 14.0
HD 181906 23.1900 28.9158 15, 40 −0.001, 0.002 2 × 10-5, 0.044 0, 120 ± 13 2.65, 2.90
HD 181906 37.9341 42.6582 15, 40 −0.001, 0.002 2 × 10-5, 0.044 0, 120 ± 13 2.65, 2.90
CoRoT-6 75.930140 82.810186 70, 90 −0.03, 0.01 2 × 10-3, 0.268 0, 180 ± 13 5.0, 9.0
KIC 7765135 88.07162 93.91567 50, 60 −0.03, 0.01 2 × 10-3, 0.268 0, 180 ± 13 1.0, 4.0
KIC 7985370 33.5126 39.07074 25, 50 −0.03, 0.01 2 × 10-3, 0.268 0, 180 ± 13 1.0, 5.0
KIC 8429280 104.49977 108.66819 65, 73 −0.02, 0.01 2 × 10-3, 0.268 0, 180 ± 13 1.0, 4.0
Kepler-30 290.99150 313.34662 60, 90 −0.03, 0.01 2 × 10-5, 0.060 0, 180 ± 13 13.0, 19.0

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