The intra-hour variable quasar J1819+3845: 13-year evolution, jet polarization structure, and interstellar scattering screen properties

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Fig. 9

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A plot of the time delay of the Stokes Q and U emission with respect to the total intensity determined from the four epochs shown in Table 2. The right-hand axis shows the equivalent angular separation in microarcseconds with respect to the unpolarized emission using the relation in Eq. (4).

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