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Fig. 6
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Long-term X-ray variability of the combined BC components. The average flux taken from eROSITA eRASS1:4 (blue) every six months during the years 2020–2021. The Chandra observation from year 2021 was reported in Brown et al. (2022) and year 2022 from this work during the flare (green) and non-flare (orange) time.
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