A deep ALMA Band 3 survey of HDFS/MUSE3D - Survey description and initial results

Open Access

Fig. C.1.

Comparison between HST WFPC2/F814W imaging (background gray image) and the CO (2-1) maps (red contours) for the detected sources. Cutouts are 4″ wide (∼34 kpc). The contours indicate levels at $3 \times \sqrt{(} {2)}^{n} \times$ $3\times\sqrt(2)^{n}\ \times\$ RMS, where n = 0, 1, .... B15-114 is detected by HST in the South-West corner of the ALMA-114 panel, but not in CO (2-1).

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