Fig. 15.
EHT2017 reconstructions of pre-2017 source models. Top: GRMHD models of M 87 from Dexter et al. (2012; left) and Mościbrodzka et al. (2016; right) described in Sect. 6.2.2. Middle: images reconstructed with SYMBA observing these images with the EHT2017 station and weather parameters, displayed on a square root scale like the other images in this paper. Bottom: reconstructed images blurred with a circular Gaussian beam with FWHM of 17.1 μas displayed on a linear scale as was done in Event Horizon Telescope Collaboration (2019b,d).
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