Gamma-ray flares from the jet of the blazar CTA 102 in 2016–2018

Open Access

Fig. 14.

Quasi-simultaneous γ-ray versus optical (R-band) fluxes in log–log space. The data was taken from the six-year observation period in γ-rays (MJD 56200–58400). The best-fit solution of the flux–flux relation shows $F_{IC} \propto F_{sync}^{0.87 \pm 0.04}$ $F_{\mathrm{IC}} \propto F_{\mathrm{sync}}^{0.87 \pm 0.04}$ (plotted in black and red).

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