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Fig. 6

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Several examples illustrative of the output of the pipeline for SB1-type solutions. Each panel concerns an object whose Gaia name is given in the header. Each of the panels shows the phase diagram containing the folded RVs (data points at the centre of the ±1σ error bars) along with the fitted orbital solution. The header gives also the time span covered by the time series (ΔT). The second line gives the GRVSint$G_{{\rm{RVS}}}^{{\mathop{\rm int}} }$ magnitude of the object, the astrometric ruwe and the astrometric excess noise, whereas the third line concerns the physical parameters identifying the template used. The last line indicates the period, the eccentricity, the significance, and the statistic F2 related to the adopted solution. The objects are ordered by increasing period.

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