Fig. C.3

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Correlations between RFUV/NUV and the NUV and FUV excesses (left and right respectively). The colour and shape of the markers represent the stellar variability and chemistry type as in Fig. 4. Grey markers are those without correction from dust attenuation. The dotted lines link the markers for the same sources before and after the dust attenuation correction. The dashed lines represents linear fits to the points.
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