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Table 2

Journal of the observations of HD 17505A.

HJD − 2 450 000 Instrument Exp. time ϕ RV(Aa1) RV(Aa2) RV(Ab)
(min) (km s−1)
3327.473 ELODIE 60 0.75 –191.0 114.3 –31.3
5447.762 FIES 15 0.19 115.5 –193.3 –31.7
5577.414 FIES 13.7 0.32 90.8 –163.3 –1.15:
5812.692 FIES 11.8 0.78 –208.3 113.0 –13.6:
5814.677 FIES 9.2 0.01 –28.1 –28.1 –13.6:
5816.755 FIES 8.3 0.25 106.3 –200.4 –13.6:
6285.436 FIES 15 0.95 –128.1 43.0 9.1:
6895.965 HEROS 60 0.20 126.2 –160.5 –37.6
6897.853 HEROS 60 0.42 36.3: –88.5: –37.6
6907.940 HEROS 60 0.60 –36.1 –4.1: –37.6
6910.888 HEROS 40 0.94 –136.1 80.5 –37.6
6911.915 HEROS 60 0.06 –38.2 –38.2 –37.6
6918.869 HEROS 60 0.88 –168.5 126.3 –37.6
6925.891 HEROS 60 0.69 –127.1: 94.7 –37.6
6939.829 HEROS 60 0.32 139.1 –152.3 –37.6
6941.814 HEROS 60 0.55 –28.2 –28.2 –37.6
6943.801 HEROS 60 0.79 –171.4 136.1 –37.6
6945.770 HEROS 60 0.01 –26.4 –26.4 –37.6
6947.861 HEROS 60 0.26 144.8 –166.1 –37.6
6949.855 HEROS 20 0.49 –21.8 –21.8 –37.6
6953.787 HEROS 20 0.95 –126.8 85.6 –37.6
6955.785 HEROS 60 0.18 128.8 –142.9 –37.6

Notes. The phases (ϕ) are computed according to the ephemerides of the new orbital solution (labelled “This study” in Table 4). The typical uncertainties on the RVs are 5–15 km s−1. The colons indicate uncertainties larger than 20 km s−1. For the third component, we calculated the mean value of the RVs over each run of observations, given its long orbital period.

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