Fig. 7.
Images of AGS25 in the H-band (1.6 μm), Ks-band (2.2 μm) and IRAC1-band (3.6 μm). The contribution of a 3″distant bright neighbor of AGS25 was subtracted to produce the IRAC image as in F20a. The red contours denote the ALMA detection at 1.1 mm at the resolution of 0
60. The magenta “x” is the ZFOURGE counterpart IDZFOURGE = 11 353.
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