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Table C.1.

Radial velocity data corresponding to the spectra obtained for the present paper.

Date (KJD) RV1 (km.s−1) RV2 (km.s−1)
4054905

2639.9411 −2.474(28) 26.00(18)
2670.9044 −4.058(26) 26.47(15)
2736.8762 4.562(28) 18.46(14)
2787.6329 18.855(29) 2.62(19)
2817.8751 32.108(30) −12.81(11)
2841.5760 38.295(34) −17.03(12)
2848.6794 36.071(27) −13.26(16)
2850.5840 33.567(26) −13.05(16)
2850.6727 35.244(26) −11.20(17)
3027.9970 8.04(52) 14.68(84)
3178.8424 −1.292(28) 23.71(13)
3219.7737 −4.936(28) 25.81(11)
3444.9214 1.591(27) 21.73(16)
3446.4615 ( ⋆ ) 0.8774(34) 21.2368(34)
3450.4808 ( ⋆ ) −0.2895(34) 21.2368(34)
3454.9107 −0.991(26) 24.79(16)
3551.6723 3.716(27) 21.50(12)

4360072

2639.9215 67.012(23) ...
2670.9419 68.593(22) ...
2736.9122 68.603(22) ...
2787.6678 67.392(25) ...
2841.6178 65.674(31) ...
2848.5954 62.316(22) ...
2850.6165 64.849(23) ...
3028.8859 55.935(21) ...
3090.9026 53.876(21) ...
3182.6077 50.740(22) ...
... ... ...

Notes. Dates are mid-exposure times expressed in Kepler Julian dates (KJD), which are barycentric Julian dates BJD with an offset: KJD = BJD − 2 454 833 days. The first spectrum was taken on March 25, 2016 (KJD = 2639.9), and the last on November 15, 2020 (KJD = 4336.5). The least significant digit in brackets after the value indicates the statistical uncertainty arising from the position of the peaks in the BF. For the APO data, the dispersion of the data point with respect to the best-fit models indicate that the actual RV uncertainties are actually about 0.5 km s−1 for the giant component and 1 km s−1 for the companion. The statistical error on the BF does not include instrumental effect and atmospheric seeing. The empirical error bars were used to model our data. Dates with a ( ⋆ ) symbol correspond with data taken at OHP. The full table and the exact timestamps are provided at the CDS.

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