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Fig. B.2

image

Radial velocity variability amplitude versus photometric variability amplitude of periodic variables in NGC 3766 having VLT/GIRAFFE spectra taken in this program. The RV variability amplitude QRV is computed using the 9010% inter-percentile range. Indicator symbols and colors have the same meanings as in Fig. 2. Stars showing an RV variability amplitude larger than 7 km s-1 are labeled with their star IDs next to the indicators.

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