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Fig. 13

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Upper: mass-period diagram for all objects with (minimum) masses between 9 and 90 MJup that orbit solar-type stars with a period shorter than 1  ×  104 days. Lower: eccentricity-period diagram for the same sample of objects. In both panels the objects reported in this paper are shown as red squares. The other coloured symbols represent companions for which the true mass is known either by astrometry (blue circles) or because they transit their host star (green circles). The rest of the objects are candidates detected by RV surveys (white circles), and the plotted mass should be interpreted as a lower limit. Owing to the wide range of objects represented, the error bars for some of them are smaller than the symbol used in the plot.

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