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Fig. A.1.

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XMM-Newton Optical Monitor (OM) UVW1 light curve of IRAS 13224-3809 during the 2016 campaign. The source shows a stable UV emission with a peak-to-peak variability amplitude of only ∼0.17 mag (< 2%) over the entire observation period. The average magnitude is mUVW1 = 15.36 with a standard deviation of 0.03 mag.
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