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Fig. 11

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Average source reconstruction performance of 2D-1D Net, Deflation Net, and CLEAN, over the test sky cubes with (upper sub-panel) a fixed test PSF cube and the noise levels σϵ ∈ {0,1,2,3,4,5,6); (lower subpanel) a fixed noise level σϵ = 3 and the 50 test PSF cubes. Regarding all of these inferences, sources in the test sky cubes have different input S/Ns. These S/Ns values can be divided into ten deciles. This figure visualizes NRMSES averaged over sources in each decile. The black whiskers indicate the standard deviations.

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