Table 1.
GC observing nights selected for Sgr A* imaging.
Date | Available | |||
---|---|---|---|---|
exposures | Nexp | ⟨σρ⟩ | ⟨σϕ⟩ | |
2021-03-30 | 13 | 13 | 4.5 × 10−2 | 33.2° |
2021-05-22 | 20 | 19 | 3.3 × 10−2 | 10.5° |
2021-05-29 | 22 | 21 | 3.5 × 10−2 | 19.3° |
2021-05-30 | 20 | 20 | 3.7 × 10−2 | 24.3° |
2021-06-24 | 32 | 29 | 3.6 × 10−2 | 20.7° |
2021-07-25 | 28 | 22 | 3.1 × 10−2 | 15.3° |
2021-07-26 | 20 | 20 | 3.6 × 10−2 | 19.6° |
2021-07-27 | 20 | 19 | 2.8 × 10−2 | 10.3° |
Notes. Each exposure amounts to a 320 s integration time. For some nights, we deselected exposures which were affected by bad weather or instrumental problems, such that the number of exposures used in the imaging, Nexp, is smaller than the total number of exposures available. The last two columns give the mean standard deviation of the closure phases and amplitudes. If a scaling factor was applied to the error bars, this is included.
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