Fig. 4.
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Fits to the variations in the PA of the radio jet at 43 GHz and 86 GHz based on the expected jet precession in the disk model by Dey et al. (2018). The red and black lines correspond to the model predictions at 43 GHz and 86 GHz, respectively. The innermost PA value from RadioAstron is marked with black diamond, and VLBA-BU-BLAZAR data points are marked with red circles.
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