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Fig. B.2.
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Two examples of dwarf novae captured by Gaia DR3. The green points indicate the positions in the HRD of each observation while the blue square indicates the mean photometry. Top: VZ Aqr = Gaia DR3 2684755714241156736 with orbital period of 3.8h. Bottom: QW Ser = Gaia DR3 1163811724898541440 with orbital period of 1.79h.
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