Fig. 9.
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Multi-filter light curves derived from 2018 up to 2022 for ESO 511-G030 using Swift-XRT and -UVOT. Until the end of 2021 (MJD < 59580), after which a moderate increase of ultraviolet emission can be observed, the optical-UV curves could be highly affected by the host emission. We noticed that to quantify the actual amplitude of the optical-UV emission, an estimate of the contribution of the host galaxy is required (see Sect. 6).
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