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Fig. 14

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Reconstruction of a simulated M87* jet observation with the EHI at 43 GHz for 60 km orbital separation. From left to right: the middle theoretical emission map in the period of 37 days (the model with 3.7 days between frames); frames of the simulated movie, each lasting 37 days, reconstructed using the snapshot imaging method. For the EHI observing at 43 GHz, this movie demonstrates the best quality, according to the NXCORR, among all reconstructions that image source dynamics. The source is varying during the simulated observation. Colours indicate brightness/pixel in mJy (square root scale). The full reconstruction is available as an online movie.

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