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Fig. 6


As in Fig. 5, for the CoRoT ID 101231832 the profile fitting of an Fe I line and the Li doublet are presented. The panels a), b), c), and d) show how the errors in each stellar parameter impact the computed synthetic spectra, which were used to measure vsin (i) (panel e)) and A(Li) (panel f)), and their respective errors. For all panels, the observed spectrum is presented using a black line, whereas the synthetic spectrum, computed with the derived stellar parameters, is presented using a red line. The dashed green and blue lines represent the computed synthetic spectra with errors for a given stellar parameter.

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