Fig. 1
Radial velocity plotted against orbital phase of ASAS 10232. The RV data was folded with the period measured from the SuperWASP lightcurve. The RVs were determined from ESO-NTT/EMMI spectra (triangle) and Gemini/GMOS spectra (rectangular). The errors are formal 1σ uncertainties. The GMOS-RVs were shifted systematically to fit to the EMMI results.
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