Fig. 5
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Left: λmax map for NGC-3244, obtained by fitting Serkowski laws to each 5 × 5 pix2 bin and filtering the results of those fits using the criteria defined in Section 4. Center: λmax map inference performed by INLA on the λmax map on the left. Right: b_HIGH pointing image of NGC-3244 (MW field star regions were masked during the data reduction process). All images are presented at the same spatial scale.
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