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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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