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Variability and stellar populations with deep optical IR images of the Milky Way disc: matching VVV with VLT/VIMOS data

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Figure

Fig. 1. Location of the analysed fields in Galactic coordinates.
Table 2. Census of variables detected in the VIMOS field F170.
Fig. 4. Examples of light curves of eclipsing variables with unknown period.
Table 3. Census and magnitude range of all analysed stars in fields F167 and F170.
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