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Resolving the ISM at the Peak of Cosmic Star Formation with ALMA:The Distribution of CO and Dust Continuum in z ˜ 2 5 Submillimeter Galaxies

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Figure

Table 1Description of the ALMA Cycle 2 Band 3 observations and native beam properties
Figure 1. Analysis of the CO(3-2) data: Thefor ALESS49.1, ALESS57.1, ALESS67.1 and ALESS122.1, respectively
Figure 2. CO(3-2) velocity averaged contours overlaid on optical/near-IR cutouts from the availableare achieved through natural weighting
Table 2CO(3-2) line properties and estimated quantities.
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