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Fig. 2

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Spatial distribution of our selection for 12 disk streams in heliocentric Galactic coordinates. Colors have the same meaning as in Fig. 1. Because of sensitivity, the elongations of these disk streams are lower limits to their true elongation. The dashed rectangle indicates the search volume of approximately 2503 pc3 within which we aim to identify the local disk stream population. Many of the progenitor streams identified extend far beyond the initial search box.

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