ALMA observation of an evolving magnetized corona in the radio-quiet changing-state active galactic nucleus NGC 1566

Open Access

Fig. 3.

Variation of the mm flux at 230 GHz (F_230 GHz) as a function of the 14–150 keV X-ray flux (F_{14−150 keV}). The solid red line represents the best-fit. The dashed black line represents the F_230 GHz−F_{14−150 keV} relation from Kawamuro et al. (2022).

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