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Table B.1.

Results of the HERMES and APOGEE RV monitoring are displayed in columns 3 to 8 and 9 to 11, respectively, and are statistically combined in columns 12 to 14. Columns and σ list the mean RV and the corresponding standard deviation. The probability Prob of the star being in a binary system, from the HERMES data alone (and adopting an uncertainty of 0.07 km s−1) is listed in column 5 (in fact, Prob is the probability integral of the χ2 distribution from 0 to the observed χ2 value for N − 1 degrees of freedom) are tabulated as well. N denotes the total number of HERMES or APOGEE RV measurements for each star and Δt is the number of days between the first and the last observation. The value F2 in column 13 corresponds to the F2-statistics of the combined HERMES-APOGEE RVs, assuming a 0.4 km s−1 offset between their zero points and a minimum uncertainty on the RVs of 0.09 km s−1 (see text). Columns 15 to 18 correspond to the Gaia DR2 RV measurements, which cover the time span JD 2456863.5 to 2457531.5 (2014 July 25 to 2016 May 23), just prior to the HERMES monitoring thus. The column labelled ϵ lists the expected uncertainty on the Gaia DR2 RV (see text). The column labelled ΔRV under the heading Gaia DR2 corresponds to RVHERMES − RVDR2. ΔRV under the heading APOGEE corresponds to RVHERMES − RVAPOGEE, after applying the zero-point offset of −0.40 km s−1 to the APOGEE velocities. Values in bold face identify binary signatures. The last column summarizes the situation regarding binarity, collecting the diagnostics from HERMES, Gaia DR2, and APOGEE. When the only binary signature is an offset between Gaia DR2 and HERMES, the star is flagged as ’SB?’.

HERMES APOGEE Gaia DR2 HER
HER & APO
&APO & DR2

Star class F2 Prob N Δt SB N ΔRV σ F2 SB ϵ ΔRV SB SB
(km/s) (d) (km/s) (km/s) (km/s) (km/s) (km/s) (km/s)
O1 AP 5.56 ± 2.33 41 1.0 7 1390 SB 8.23 1 -2.67 2.36 45 SB 1.86 ± 1.39 1.04 3.70 SB SBe
O2 AP −16.30 ± 0.11 1.2 0.8762 8 1083 −16.26 ± 0.06 3 -0.04 0.10 0.77 −15.62 ± 0.47 0.78 -0.68
O3 AR −29.27 ± 3.39 53 1.0 7 1392 SB −22.13 1 -7.14 4.03 66 SB −30.39 ± 2.40 0.87 1.12 SBa SBc
O4 AR −150.89 ± 0.23 2.6 0.9953 3 708 −151.01 ± 0.03 3 0.12 0.16 2.2 - - - -
O5 AP 5.84 ± 0.14 2.1 0.9807 7 1082 6.23 ± 0.16 5 -0.39 0.24 6.9 SB 6.15 ± 0.23 0.42 -0.31 SB
O6 AP −30.86 ± 0.12 1.4 0.9162 7 1391 −30.78 1 -0.08 0.12 1.3 −30.06 ± 0.47 1.41 -0.80
O7 AP 2.00 ± 0.07 -0.6 0.2840 6 1390 1.98 ± 0.07 2 0.02 0.06 -0.92 3.18± 1.00 1.37 -1.18
O8 AP −46.47 ± 0.10 0.7 0.7537 9 1392 −46.75 ± 0.11 3 0.28 0.16 3.5 SB −47.73 ± 0.58 1.11 1.26 SB
O9 AP −69.82 ± 0.12 1.3 0.9073 8 1128 −69.77 ± 0.06 4 -0.05 0.10 0.92 −69.45 ± 0.27 0.64 -0.37
O10 AP 6.99 ± 0.09 0.2 0.5624 7 1393 6.96± 0.25 8 0.03 0.19 5.3 SB 7.55 ± 0.84 0.81 -0.56 SB
O11 AP −5.98 ± 0.07 -0.6 0.2677 7 1392 −5.93 ± 0.07 3 -0.05 0.07 -0.82 −5.41 ± 0.29 0.50 -0.57
O12 AP 29.21 ± 0.12 1.3 0.9021 7 1391 29.09 ± 0.10 5 0.12 0.13 2.1 29.97 ± 0.40 0.99 -0.76
O13 AP −41.42 ± 0.09 0.2 0.5625 6 1389 −41.01 ± 0.08 3 -0.41 0.22 5.2 SB −41.19 ± 0.52 0.80 -0.23 SB
Y1 YAR −5.78 ± 0.10 0.6 0.7089 13 1080 −5.75 1 -0.03 0.09 0.49 −4.80 ± 0.41 0.94 -0.98
Y2 YAR 6.30 ± 0.20 4.0 1.0 7 1382 SB 6.11 ± 0.15 3 0.19 0.20 4.9 SB 7.02 ± 0.63 1.00 -0.72 SB
Y3 YAR −83.48 ± 0.13 2.0 0.9795 10 2208 −83.78 ± 0.05 3 0.30 0.18 4.5 SB −82.95 ± 0.49 0.82 -0.53 SB
Y4 YAR −70.62 ± 3.30 30 1.0 3 648 SB −75.73 1 4.31 3.71 41 SB −70.54 ± 1.48 0.82 -0.08 SBc
Y5 YAR −86.11 ± 0.10 0.7 0.7430 8 1382 −86.10 ± 0.05 5 -0.01 0.08 -0.17 −85.98 ± 0.60 1.12 -0.13
Y6 YAR −24.07 ± 4.52 71 1.0 8 1386 SB −18.41 ± 0.20 2 -5.66 4.65 83 SB −19.71± 1.84 0.61 -4.36 SB SBb,c
Y7 YAR −39.23 ± 2.16 41 1.0 8 1382 SB −39.16 1 -0.07 2.02 43 SB −36.65± 1.51 2.39 -2.58 SBb
Y8 YAR −44.36 ± 1.22 24 1.0 7 1387 SB −39.98 1 -4.38 1.92 38 SB −43.58 ± 0.75 0.58 -0.78 SBd
Y9 YAR −33.45 ± 3.19 55 1.0 8 1381 SB −37.98 ± 0.10 5 4.43 3.34 76 SB −31.94 ± 0.93 0.55 -1.51 SB SBb,c
Y10 YAR −56.97 ± 0.12 1.6 0.9454 10 2213 −56.94 1 -0.03 0.12 1.5 −56.59 ± 0.25 0.62 -0.38
Y11 YAR −26.73 ± 0.08 -0.3 0.3809 11 2208 −26.75 1 0.02 0.08 -0.44 −25.95 ± 0.70 1.18 -0.78
Y12 YAR −46.81 ± 0.81 25 1.0 13 1842 SB −46.80± 1.08 8 -0.01 0.90 35 SB −45.74 ± 0.38 0.70 -1.07 SB b
Y13 YAR −62.15 ± 0.09 -0.1 0.4566 14 1488 −62.30 ± 0.06 3 0.15 0.10 0.79 −61.73 ± 0.15 0.37 -0.42
Y14 AR −45.46 ± 0.08 -1.6 0.0063 2 309 −44.97 ± 0.11 5 -0.49 0.26 5.6 SB −44.90 ± 0.41 1.22 -0.56 SB
Y15 AR −54.79 ± 0.21 4.1 1.0 7 1604 SB −55.68 1 0.89 0.37 9.2 SB −55.57 ± 0.57 1.52 0.78 SB
Y16 YAR −15.15 ± 0.03 -2.0 0.0223 5 1603 −15.25 ± 0.00 2 0.10 0.05 -1.3 −14.63 ± 0.27 0.83 -0.52
Y17 AR −67.70 ± 0.08 0.1 0.5427 4 1603 −67.71 ± 0.06 2 0.01 0.07 -0.43 −66.45 ± 0.57 0.80 -1.25
Y18 YAR 2.17 ± 0.15 2.1 0.9812 6 1604 2.18 ± 0.03 2 -0.01 0.13 1.7 3.55 ± 0.77 0.77 -1.38
Y19 AR −41.10 ± 0.06 -0.9 0.1893 6 1604 −41.03 1 -0.07 0.06 -0.90 −40.28 ± 0.45 0.82 -0.82
Y20 AR −30.63 ± 0.15 2.0 0.9768 6 1603 −30.87 1 0.24 0.16 2.8 −31.05 ± 0.65 0.66 0.42
Y21 AR −30.71 ± 0.07 -0.4 0.3427 7 1602 −30.89 ± 0.12 5 0.18 0.13 2.4 −29.91 ± 0.75 1.40 -0.80
Y22 AR 75.64 ± 0.05 -1.2 0.1128 6 1604 75.89 ± 0.08 3 -0.25 0.14 2.3 76.37 ± 0.46 0.47 -0.73
Y23 AR −121.84 ± 0.07 -0.4 0.3349 5 1605 −122.02 1 0.18 0.10 0.57 −121.06 ± 0.40 0.47 -0.78
Y24 AR −51.08 ± 0.07 -0.3 0.3895 5 1603 −51.31 ± 0.04 2 0.23 0.13 1.8 −49.72 ± 0.40 1.01 -1.36
Y25 AR −49.41 ± 0.52 13 1.0 9 1604 SB −43.35 1 -6.06 1.98 44 SB −43.23± 1.32 1.37 -6.18 SB SBd
Y26 AR −87.78 ± 3.94 59 1.0 7 1604 SB −84.22 ± 0.25 3 -3.56 3.65 70 SB −93.54 ± 0.55 0.67 5.76 SB SBd
Y27 AR −3.60 ± 0.09 0.3 0.6345 6 1602 −3.65 ± 0.04 3 0.05 0.08 -0.13 −2.15±0.94 1.94 -1.45
Y28 YAR 9.06 ± 1.03 20 1.0 6 1606 SB 11.15 ± 0.14 3 -2.09 1.32 31 SB 9.40 ± 0.52 0.85 -0.34 SB

Notes.

a

The Gaia eDR3 RUWE (’reduced unit-weight error’) parameter is 4.01 for this star, further indicative of its binary nature.

b

Spectroscopic orbit available from HERMES data (see Appendix B.1).

c

Spectroscopic orbit available from Gaia DR3 (see Appendix B.1).

d

First-degree RV trend in Gaia DR3

e

Second-degree RV trend in Gaia DR3

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