Fig. 7
Periodogram of the radial-velocities of HD 192310 (A)), of the residuals of the one-Keplerian model (LM1 see Table 3, B)), and of the residuals of the two-Keplerians model (LM2 see Table 3, C)). The orbital elements corresponding to the successive solutions are presented in Table 3, and compared to the published solution (Pepe et al. 2011).
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