Table 1
Parameters of the theoretical emission maps used.
| Source | Time interval (h) | Movie duration (months) | ν (GHz) | Total flux (Jy) | FoV (μas) |
|---|---|---|---|---|---|
| 230 | 0.84–1.31 | 190.9 | |||
| M87* | 89 (10 tG) | 10 (800 tG) | 560 | 0.47–0.84 | 190.9 |
| 5000 | 0.10–0.18 | 190.9 | |||
| 43 | 0.60–0.82 | 763.7 | |||
| NGC 1052 | 89 | 10 | 43 | 7.0–7.6 | 9.6 × 103 |
| 230 | 0.93–1.04 | 190.9 | |||
| M87* | 8.9 (1 tG) | 2.5 (200 tG) | 560 | 0.48–0.56 | 190.9 |
| 5000 | 0.10–0.12 | 190.9 | |||
| 43 | 0.69–0.72 | 763.7 | |||
| NGC 1052 | 8.9 | 2.5 | 43 | 7.39–7.46 | 9.6 × 103 |
Notes. Duration of movies was calculated as time intervals between frames multiplied by the number of frames in sets. For uυ-coverage calculation, the same time intervals between frames in movies were used as for M87* since the black hole mass was not properly scaled for NGC 1052 models when changing the angular size of the source.
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