Fig. 2.
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Evolution of NGC 1566 during 2007–2023 observations with Swift/XRT (top panel, 0.3–10 keV), Swift/BAT (bottom panel, black points, 15–150 keV), and Swift/UVOT (bottom panel, orange stars, UVW2 band [1600–2300 Å], right axis). The green, black, and red triangles indicate the Suzaku, NuSTAR, and XMM-Newton observations, respectively, used in our analysis.
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