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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