Table 2
Log of the observed targets.
| Name | Observing | Mode | ΔPA | DIT | NDIT | Nexp | ϵ | τ0 | CE | Image | # frames | Exp. |
| date | (°) | (s) | (′′) | (ms) | (%) | bin | mastercube | time (s) | ||||
|
|
||||||||||||
| HIP 98470 | 2010.08.20 | ASDI-4 | 102 | 8 | 8/2 | 24+39 | 1.03 | 8.3 | 9.5 | 2 | 118 | 1888 |
| HIP 107350 | 2010.08.20 | ASDI-4 | 35 | 8 | 4 | 81 | 0.70 | 7.8 | 44.3 | 2 | 153 | 2448 |
| HIP 118008 | 2010.08.20 | ASDI | 72 | 20 | 2/11 | 5+13 | 1.05 | 7.2 | 37.8 | 1 | 144 | 2880 |
| HD 10647 | 2010.08.20 | ASDI-4 | 48 | 5 | 12/6 | 8+66 | 0.92 | 6.7 | 29.8 | 3 | 151 | 2265 |
| HIP 76829 | 2010.08.21 | ASDI-4 | 15 | 3 | 10 | 41 | 0.83 | 5.5 | 44.3 | 5 | 73 | 1095 |
| HIP 102409 | 2010.08.21 | ASDI-4 | 26 | 10 | 3 | 78 | 1.30 | 3.6 | 44.0 | 2 | 77 | 1540 |
| HIP 106231 | 2010.08.21 | ASDI-4 | 10 | 30 | 1 | 31 | 1.83 | 2.3 | 2.9 | 1 | 30 | 900 |
| HIP 114046 | 2010.08.21 | ASDI-4 | 94 | 3 | 10 | 74 | 1.26 | 3.6 | 40.2 | 4 | 135 | 1620 |
| HIP 7576 | 2010.08.21 | ASDI-4 | 31 | 30 | 1 | 68 | 1.02 | 3.1 | 45.7 | 1 | 65 | 1950 |
| HIP 14555 | 2010.08.21 | ASDI-4 | 66 | 30 | 1 | 76 | 1.16 | 3.3 | 36.8 | 1 | 74 | 2220 |
| HIP 10602 | 2010.12.18 | ASDI-4 | 41 | 4 | 8 | 70 | 0.92 | 5.1 | 42.9 | 4 | 136 | 2176 |
| HIP 18859 | 2010.12.18 | ASDI-4 | 41 | 5 | 6 | 69 | 0.85 | 5.7 | 35.5 | 2 | 201 | 2010 |
| HD 31295 | 2010.12.19 | ASDI-4 | 32 | 8 | 4 | 62 | 1.40 | 4.0 | 25.0 | 2 | 115 | 1840 |
| HD 38678 | 2010.12.19 | ASDI | 62 | 2.5 | 100 | 11 | 1.39 | 3.3 | 31.2 | 8 | 127 | 2540 |
| HIP 30314 | 2010.12.19 | ASDI-4 | 15 | 15 | 2 | 19 | 1.70 | 2.9 | 20.1 | 1 | 30 | 450 |
| Fomalhaut | 2011.10.09 | ASDI | 155 | 0.5 | 100 | 128 | 0.85 | 4.0 | 38.1 | 50 | 244 | 6100 |
Notes. ΔPA refers to the amplitude of the parallactic rotation, DIT (Detector Integration Time) to the single exposure time, NDIT (Number of Detector InTegrations) to the frame number in a single datacube, Nexp to the number of datacubes of the observing sequence, ϵ to the seeing, τ0 to the mean correlation time of the atmospheric turbulence, and CE to the coherent energy during the observations. The seeing is measured by the DIMM at 0.5 μm, hence includes high-frequency terms unseen by the AO wavefront sensor. The last two quantities are estimated by the AO system at 0.55 μm and 2.17 μm, respectively. The next three columns indicate the image binning used for constructing the science mastercube (Sect. 3.3.1), the number of frames in the mastercube, and the corresponding total exposure time on the target. For the observing mode, ASDI-4 refers to FQPM+SDI+ADI and ASDI to SDI+ADI.
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