Fig. 10
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Differential ∆AV extinction maps for the Orion region (30 deg × 30 deg, d < 1.5 kpc; left) in four bins of distance, as indicated in each panel. Some artefacts from the Gaia scanning law are visible in these maps, but the distance-sliced AV maps are generally complete down to AV ≳ 6 mag, with a high resolution, and correspond very well to existing 3D dust maps.
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