Fig. 3.
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Multiwavelength light curves of 3C 120. The panels from top to bottom are the adaptive-binning Fermi-LAT γ-ray light curve, the 1 keV light curve from Swift-XRT, the ASAS-SN weekly binned light curves, the NEOWISE light curves, and the multifrequency radio light curves from RATAN-600, respectively. The three shaded gray regions correspond to the time periods of γ-ray flares, while the red dashed vertical line represents the neutrino arrival time.
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