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Table 3

Relative RV and bisector span (BS) measurements of HATS-2 from various instruments used for high-precision RV measurements (cf. Table 2).

BJD Relative RV σ RV BS σ BS Phase Exp. time S/N Instrument
(–2 454 000) (m s-1) (m s-1) (m s-1) (m s-1) (s)

1701.52346 − 90.37 33.00 − 63.7 79.5 0.119 1800 9.0 Coralie
1701.54622 − 238.37 36.00 117.7 83.3 0.135 1800 8.0 Coralie
1702.52760 168.63 33.00 31.3 58.6 0.860 1800 10.0 Coralie
1702.55065 169.63 33.00 − 30.8 74.2 0.877 1800 9.0 Coralie
1721.50300 204.15 71.76 120.4 93.8 0.873 2400 14.0 FEROS
1722.58300 371.99 100.77 − 146.9 640.0 0.671 2400 16.0 FEROS
1723.44500 − 330.70 73.66 − 211.0 207.2 0.307 2400 18.0 FEROS
1736.46900 164.63 38.18 149.3 86.4 0.925 2400 16.0 FEROS
1737.53800 261.69 119.02 − 130.9 287.5 0.715 1044 17.0 FEROS
1738.48600 − 47.00 58.61 − 222.1 146.9 0.415 3000 12.0 FEROS
1932.22448 − 33.63 21.80 1114.3 43.2 0.487 2400 22.7 CYCLOPS
1933.21669 − 40.53 51.20 3464.1 19.9 0.219 2400 20.7 CYCLOPS
1934.12774 75.57 65.58 − 4516.6 168.1 0.892 2400 17.6 CYCLOPS
1938.81200 − 337.82 139.13 − 436.4 449.1 0.351 2700 17.0 FEROS
1939.16016 47.07 49.44 9189.5 1723.7 0.608 2400 18.0 CYCLOPS
1990.75600 294.99 103.71 46.3 201.6 0.711 2700 15.0 FEROS
1992.82100 − 335.90 72.26 − 251.5 208.5 0.236 2700 19.0 FEROS
2035.67400 31.55 77.56 270.6 223.1 0.882 3600 22.0 FEROS

Notes. Five data points determined with FEROS are not listed here and were not used for further analysis due to high error bars caused by bad weather conditions. The Coralie RV uncertainties listed here are known to be underestimated. Updated estimates are available, but we list here the values we used in the analysis. We note that in any case a jitter is included in the analysis to account for any additional scatter to what is implied by the uncertainties, see Sect. 3.3 (cf. Table 5).

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