File:Observing—and Imaging—Active Galactic Nuclei with the Event Horizon Telescope Fig3.png

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Summary

Description	English: Figure 3. BSSpM reconstruction of a disk-jet model of M87 at 1.3 mm. (a) The original model [45]. (b) The model convolved with a 10 μas Gaussian. (c) The BSSpM reconstruction of the image from simulated data [44]. The fringe spacing of the longest baseline is approximately 25 μas. (d) The BSSpM reconstruction convolved with a 10 μas Gaussian. BSSpM successfully recovers features of the model at a superresolution of 40% of the fringe spacing.
Date	1 July 2016
Source	http://www.mdpi.com/2075-4434/4/4/54
Author	Vincent L. Fish, Kazunori Akiyama, Katherine L. Bouman, Andrew A. Chael, Michael D. Johnson, Sheperd S. Doeleman, Lindy Blackburn, John F. C. Wardle, William T. Freeman, the Event Horizon Telescope Collaboration.
Permission (Reusing this file)	Unless otherwise stated, articles published on the MDPI websites are labeled as “Open Access” and licensed by the respective authors in accordance with the Creative Commons Attribution (CC-BY) license.

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