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Fig. 11


Upper panel: detection probability as a function of period, calculated as described in the text, consideting only the first four (full line) or two (dotted line) nights. Lower panel: probability, as a function of period, that an EHB binary would show a significant RV variation only in the fourth night of our observations, as found for the star #7700.

This figure is made of several images, please see below:

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