Fig. 4.
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Optical polarization of 3C 371 during the 2018–2020 period compared to the jet optical flux. From top to bottom: R-band optical light curve (dereddened and host-galaxy-subtracted flux densities), observed polarization degree, intrinsic polarization degree, corrected EVPA behavior. Different colors and symbols are used to distinguish the contributing datasets, as specified in Table 2.
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