Extended Data Fig. 7: Comparison of reconstructed images at four wavelengths from four algorithms.
From: Thermal imaging of dust hiding the black hole in NGC 1068
From left to right: the MIRA image reconstruction, the IRBis image reconstruction, the overfitted point source model (convolved with the beam), and Gaussian model for four selected wavelengths. The plot uses a 0.6 power colour scaling for visual purposes. Each method reveals similar structures and morphology.
