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This article has an erratum: [https://doi.org/10.1051/0004-6361/201220779e]


Table 8

Comparison between correlations of BIS and ΔV with RV for simulated data.

Star RVmax BISmax ΔVmax m BIS m ΔV ρ BIS ρ ΔV σ ρ,BIS σ ρ,ΔV

HD 166435’ 9.28e+01 1.03e+02 1.33e+02 –1.068 1.364 –0.990 0.987 9.82 9.82

Fr = 1.0% 9.98e+01 1.03e+02 1.32e+02 –0.686 0.871 –0.827 0.822 8.20 8.20
Fr = 2.0% 2.01e+02 2.10e+02 2.66e+02 –0.679 0.859 –0.820 0.812 8.17 8.08
Fr = 5.0% 5.20e+02 5.50e+02 6.94e+02 –0.655 0.811 –0.795 0.777 7.92 7.74
Fr = 10.0% 1.10e+03 1.22e+03 1.47e+03 –0.599 0.701 –0.741 0.703 7.38 7.00

vsini = 2.0 2.21e+01 1.94e+00 2.30e+00 –0.057 0.067 –0.801 0.802 7.98 7.96
vsini = 5.0 6.43e+01 3.72e+01 4.39e+01 –0.378 0.448 –0.815 0.817 8.10 8.15
vsini = 10.0 1.57e+02 2.54e+02 3.83e+02 –1.109 1.596 –0.847 0.817 8.46 8.12

Notes. When not stated, the probability of obtaining the presented ρ values from the distribution obtained by bootstrapping is lower than 1.0e-4. RV, BIS, and ΔV in units of m/s.

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