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Fig. 1.

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Multi-wavelength light curve of 1ES 0229+200 presenting long-term (2008–2024) observations of the blazar. The panels present optical Swift-UVOT observation in U, B, V filters; X-ray (0.3–10 keV) flux; and corresponding power-law photon index. Two epochs of NuSTAR observations taken in 2013 and 2021 are marked with vertical lines and noted as nu13 and nu21, respectively.

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