Fig. A.1.
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IXPE, NuSTAR and XMM-Newton light curves of the three observing campaigns of MCG-05-23-16 are shown. Except for the third IXPE observation, where we only had DU1 and DU3 available for the analysis, data counts from DU1, DU2 and DU3 on board of IXPE and from FPMA/A and FPMA/B on board of NuSTAR have been summed. The full energy bands of the three satellites have been used and we adopted a 3 ks time binning.
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