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Table A.1.

Information for the six stars observed with HARPS-N.

CWW Gaia source ID RA (J2000) Dec (J2000) Expt (s) Date-obs (y:m:d) UT (hh:mm:ss) PLX (mas) ePLX (mas) PMra (mas yr−1) ePMra (mas yr−1) PMde (mas yr−1) ePMde (mas yr−1) G (mag) GBP (mag) GRP (mag) RVGaia (km s−1)
1 4184143881214538112 19:15:26.120 −16:05:57.10 900 2016-05-24 01-37-46.061 3.163 0.049 1.709 0.085 −25.438 0.071 7.04 7.71 6.30 40.56 ± 1.89
2 4183949198935967232 19:17:23.840 −16:04:24.30 900 2016-05-24 01:56:40.485 3.237 0.049 −0.537 0.077 −26.453 0.065 7.18 7.93 6.38 38.51 ± 0.17
4 4184137077986034048 19:17:11.300 −16:03:08.20 1200 2016-05-24 02:15:32.621 3.250 0.056 −0.797 0.089 −26.997 0.077 8.02 8.66 7.31 41.33 ± 0.18
6 4087762027643173248 19:17:03.430 −17:03:13.80 1200 2016-05-24 02:38:39.041 3.291 0.068 −1.365 0.108 −26.523 0.093 8.03 8.62 7.33 41.77 ± 0.19
10 4184125807991900928 19:15:51.290 −16:17:59.10 1200 2016-05-24 03:03:21.454 3.197 0.044 −0.629 0.076 −26.895 0.071 8.12 8.73 7.42 40.80 ± 0.22
11 4183930438518525184 19:18:09.780 −16:16:22.20 1200 2016-05-24 04:44:48.073 3.368 0.042 −1.243 0.084 −27.019 0.077 8.25 8.88 7.53 41.62 ± 0.14

Notes. Observing Programme A33 DDT0. CWW is the identification in Curtis et al. (2013). Parallax, proper motions, G, GBP, GRP, and RVGaia come from Gaia DR2 (Gaia Collaboration 2018b).

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