Fig. 9
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Compatibility limits for the three stars studied, HD 10700 (top), HD 102365 (middle), and HD 304636 (bottom). The maximum semi-major RV amplitude of the samples is plotted for each of the RV calculation methods model, and telluric correction set; HZ limits as presented in Table 5 and orbital properties of announced planed described in Sect. 2 are shown.
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