Extended Data Fig. 2: ALMA images of 1.4 mm continuum emission.
From: Warm gas in the vicinity of a supermassive black hole 13 billion years ago
From left to right, the observed clean images and the dirty images after subtraction of the best-fit one- and two-component models are shown. The spatial resolution of the images is 0.050″×0.039″. Dashed and solid contours are plotted every -1σ from -5σ and every 1σ from 5σ, respectively. The effective radii of the best-fit model are shown by the magenta lines.
