... Carina[*]
Based on observations collected with the UVES and FLAMES spectrographs at the VLT/UT2 Kueyen telescope (Paranal Observatory, ESO, Chile, Programme 72.C-0191).
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...[*]
Table 8 is only available in electronic form at http://www.edpsciences.org
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... scenarios[*]
We subsequently confirmed the orbit with the HARPS spectrometer in January 2005 while the present paper was being reviewed.
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... transits[*]
A given transit signal will be easier to detect if the data points are distributed among a larger number of different transits than if they are grouped in a low number of transits. The reason is that if the number of transits is low, systematic drifts in other parts of the lightcurve will produce some noise in the periodogram used to detect the signal, and result in a higher effective detection threshold.
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Copyright ESO 2005