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Fig. 1

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STIS and EPIC-pn light curves observed in 2014 (top panel), 2017 (central panel), and 2021 (bottom panel). Ultraviolet and X-ray light curves are binned every 10 s. The count rate is normalised for each instrument at the maximum count rate. The vertical regions indicate the high (white), low (light red), and flaring (dark red) X-ray modes.

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