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Fig. 3

image

UV, optical, and NIR polarimetric measurements and results of our baseline model based on NGC 4151. Top: polarization degree P; bottom: difference between the radio position angle PA and the polarization position angle PPA (we use the convention PPA = 0 for perpendicular polarization angle and PPA = 90 for parallel polarization). Computational results from STOKES are shown by empty black circles.

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