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Fig. 3


Behavior of the measured microturbulent velocity as a function of SNR, derived with the classical method (empty circles) and the prescription by Magain (1984) (filled circles) for a giant star. Each point is the average value obtained by using 200 synthetic spectra of a given SNR, and the errorbars indicate the dispersion around the mean. Dashed lines indicate the original value of vt of the synthetic spectra. Each panel shows the results obtained by considering different thresholds for the residual errors in the EW measurement.

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