Chromatically modeling the parsec-scale dusty structure in the center of NGC 1068

Open Access

Fig. C.4.

V² of the polychromatic model. The colors represent the PA on sky of the telescope pair used for that point. The color scheme is continuous and cyclical about π, due to the fact that a V² measurement at PA =x and x + π are equivalent. The line is the best polychromatic model by maximum likelihood evaluated at different PA in $\frac{π}{6}$ $\frac{\pi}{6}$ intervals.

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