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Fig. 1.

Fig. 1. Refer to the following caption and surrounding text.

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Hybrid images of 3C 84 from the 2016 RadioAstron data. The core has been shifted to the map center in both images based on the values listed in Table C.2. Panel a shows the image obtained from the ground array data, whereas panel b contains data from the SRT as well. The lowest contours are at 3.7 mJy/beam for panel a and at 8.6 mJy/beam for panel b, and further contours increase by a factor of two. The image of the global array data has a total flux density of 27.8 ± 1.4 Jy, and the half-power beam width of the restoring beam is 0.35 × 0.32 mas at PA of 10.8°. The rms noise level is 0.7 mJy/beam. The super-resolved RadioAstron image has a half-power beam width of 0.13 × 0.13 mas. The rms noise level is 1.9 mJy/beam, and the total flux density is 23.0 ± 2.3 Jy.

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