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Fig. 9
GLM reconstruction of a simulated dusty HVC. The image is dominated by the simulated CIB anisotropies. The HVC dust emissivity corresponds to 10% (left) and 30% (right) of typical Galactic values. The black contours correspond to the HVC column density starting at 1019 cm-2 and increasing in steps of 2 × 1019 cm-2.
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