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Fig. 1.


Postage-stamp images of GH500.30 from multiwavelength observations. From left to right and top to bottom: HST/ACS (F435+F606+F775+F850LP), HST/WFC3 (F125W+F140W+F160W), CFHT Ks, IRAC [3.6 μm], MIPS 24 μm, PACS 100 μm and 160 μm, SPIRE 250 μm, 350 μm and 500 μm, SCUBA2 850 μm, NOEMA 1.2 mm, VLA 1.4 GHz, and Chandra 0.5–8 keV. Each panel has a size of 20″ × 20″. The detailed photometry is listed in Table 1.

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