Table B.1
Velocity time series for the iDR5 SB2 sample.
| Gaia-ESO CNAME | MJD | velocities | Remarks on CCFs | Average CCF heights | Best-mask CCF heights and widths | ||||||||||||
|---|---|---|---|---|---|---|---|---|---|---|---|---|---|---|---|---|---|
| υrad,1 | υrad,2 | mode | setup | best | Ngood | K1 | k1 | sth | k2 | sth | H1 | h1 | h2 | w1 | w2 | ||
| km s−1 | km s−1 | km s−1 | km s−1 | ||||||||||||||
| 00040663-0101512 | 56197.087034 | 28.83 ± 1.00 | −20.96 ± 5.93 | A | HR10 | 1 | 5 | 0.864 | 1.000 | 0.083 | 0.409 | 0.041 | 0.883 | 1.000 | 0.339 | 15.430 | 15.200 |
| 00040663-0101512 | 56197.107669 | 30.28 ± 1.03 | −22.99 ± 1.70 | A | HR10 | 1 | 7 | 0.791 | 1.000 | 0.207 | 0.553 | 0.099 | 0.861 | 1.000 | 0.401 | 16.110 | 18.790 |
| 00040663-0101512 | 56205.144417 | 68.48 ± 1.00 | −63.47 ± 1.00 | A | HR21 | 2 | 11 | 1.082 | 1.000 | 0.023 | 0.613 | 0.056 | 1.057 | 1.000 | 0.604 | 12.390 | 12.090 |
| 00040663-0101512 | 56205.162404 | 67.57 ± 1.00 | −64.66 ± 1.00 | A | HR21 | 2 | 8 | 1.077 | 1.000 | 0.011 | 0.606 | 0.064 | 1.061 | 1.000 | 0.590 | 13.600 | 11.910 |
| 00040663-0101512 | 56576.177839 | −37.19 ± 1.00 | 50.82 ± 1.31 | A | HR10 | 1 | 8 | 0.927 | 1.000 | 0.022 | 0.470 | 0.047 | 0.912 | 1.000 | 0.479 | 14.860 | 16.030 |
| 00041619-3659250 | 56909.271801 | 0.36 ± 1.00 | −25.50 ± 1.00 | A | HR21 | 2 | 8 | 0.895 | 1.000 | 0.016 | 0.955 | 0.085 | 0.894 | 1.000 | 0.833 | 13.060 | 11.200 |
| 00195847-5423227 | 56532.286507 | 93.78 ± 1.00 | 152.50 ± 1.00 | A | HR10 | 1 | 8 | 0.918 | 1.000 | 0.044 | 0.964 | 0.037 | 0.904 | 0.973 | 1.000 | 13.790 | 15.680 |
| 00195847-5423227 | 56532.307888 | 94.11 ± 1.00 | 151.23 ± 1.00 | A | HR10 | 1 | 8 | 0.922 | 1.000 | 0.057 | 0.986 | 0.050 | 0.929 | 0.967 | 1.000 | 14.300 | 15.990 |
Notes. The columns are the following: Gaia-ESO CNAME; MJD (day); υred,1,2 the radial velocity of the component 1 and 2 in km s−1 and its 1 – σ uncertainty; the first or second component assignation mode (A: automatic; M: manual; see Sect. 4.6); the GIRAFFE setup; the best mask ID (1: alphaCenA; 2: betaAra; 3: muLeo; 4: Sun); Ngood the number of good NACRE CCFs used for the analysis; the average CCF heights with Ki being the absolute average height (average of all measured heights over AgOOd CCFs) of the first-component’s CCF peak and k1,2 = K1,2 being the normalised average heights of each component’s peak (with the associated standard deviation around the mean); the best-mask CCF heights with H1 being the absolute height of the first-component’s CCF peak and h1,2 being the normalised height of each component’s peak; w1,2 the width of each component’s peak in km s 1. For a given system, the observations are ordered by increasing MJD and each velocity column is meant to track a given component of the system. The first component is tentatively the most luminous component of the system. We force a minimal uncertainty of I km s−1 on the velocities. Ki, ki, Hi, hi, wi are quantities obtained from the parameters of the Gaussian fit of the CCF peaks (see Sect. 3.2 and 4.6). The series for the first three objects are shown as an excerpt; the full table is available at CDS.
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