Fig. 3.
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XMM–Newton+ NuSTAR unfolded spectra of NGC 5055. The top panel shows the best-fit CUTOFFPL model. The second panel displays the SIMPL model fit. The bottom three panels show the residuals for each tested scenario with their corresponding χ2 values: CUTOFFPL (third panel), SIMPL (fourth panel), and DISKBB+DISKPBB (fifth panel).
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