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Fig. 8
Residual histograms (top) and maps (bottom) for a protoplanetary disk with a warped inner disk using metrics (i) and (ii) as the metric of best fit. The histograms are displayed on a log scale to emphasise the largest residuals. Note that metrics (ii) and (iii) select the same warped inner disk parameters (see Table 2).
This figure is made of several images, please see below:
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