Based on the galaxies inside the ORC, it's probably at z ~ 0.55. With those distances you don't get much detail, everything is mainly slightly squashed smudges.

Based on the galaxies inside the ORC, it's probably at z ~ 0.55. With those distances you don't get much detail, everything is mainly slightly squashed smudges. The observations covers the range of 880 MHz to 1680 MHz (with some gaps to avoid RFI, see their table 2), find a spectral index between -1.9 to -0.9 with a median of -1.6. Also the image is an interferometric measurement.