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Table 1

HERMES/Mercator and FIES/NOT radial velocities of HE 0017+0055 (without any zero-point correction).

JD Vr ± ϵ JD Vr ± ϵ
(–2 400 000) (km s-1) (–2 400 000) (km s-1)

HERMES NOT

55 053.5756 –79.423 0.008 54 314.6702 –78.622 0.007
55 053.5890 –79.431 0.005 54 338.6419 –78.944 0.007
55 053.6025 –79.382 0.009 54 373.6224 –78.691 0.009
55 087.5807 –79.899 0.011 54 396.5371 –78.583 0.007
55 087.5939 –79.823 0.006 54 406.5966 –78.505 0.012
55 087.6072 –79.851 0.006 54 480.3868 –78.183 0.012
55 098.6838 –79.597 0.008 54 793.4846 –79.098 0.018
55 098.6976 –79.590 0.006 54 820.3386 –78.830 0.017
55 098.7124 –79.738 0.007 55 059.7365 –79.922 0.008
55 159.5055 –79.417 0.006 55 149.4730 –79.647 0.010
55 159.5201 –79.429 0.006 55 207.3499 –79.391 0.015
55 159.5343 –79.463 0.014 55 415.6081 –80.439 0.009
55 418.6223 –80.099 0.008 55 439.5914 –80.778 0.010
55 423.7016 –80.118 0.003 55 503.4086 –80.330 0.023
55 497.4806 –79.992 0.007 55 738.7344 –80.148 0.008
55 938.3316 –79.977 0.008 55 776.6821 –80.675 0.008
55 956.3373 –79.944 0.003 55 821.5766 –80.870 0.009
56 109.7113 –80.056 0.005 55 944.3253 –80.429 0.011
56 140.7386 –80.201 0.006 56 139.7129 –80.857 0.010
56 311.3363 –80.588 0.007 56 241.3910 –81.420 0.018
56 481.7027 –80.278 0.007 56 545.6267 –81.474 0.011
56 511.7176 –80.560 0.007 56 652.4180 –81.951 0.015
56 557.6467 –80.868 0.006 56 686.3209 –81.538 0.015
56 634.3763 –81.416 0.007 56 840.7182 –80.866 0.028
56 849.6608 –80.395 0.017 56 888.5421 –81.261 0.013
56 904.6038 –80.550 0.016 56 917.5981 –81.398 0.014
56 947.5245 –80.919 0.014 56 987.3813 –81.885 0.009
56 994.3660 –81.219 0.013 57 257.5774 –81.396 0.010
56 996.3424 –81.103 0.012
57 052.3396 –81.528 0.005
57 052.3506 –81.422 0.013
57 056.3370 –81.287 0.018
57 056.3498 –81.274 0.017

Notes. The uncertainty quoted on the FIES RVs corresponds to the standard deviation of the correlation results from all spectral orders. For the HERMES data, the uncertainty is instead the formal error on the CCF Gaussian fit on 20 orders. A more realistic uncertainty is the long-term error describing the long-term stability of the spectrographs (see text).

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