Table A.1
Piston noise calculated with different sets of data on VLTI telescopes in H-band.
| ATs | |||
| t0 [ms] | 2 | 4 | 8 |
|
|
|||
| E | λ/114 | λ/72 | λ/43 |
| E | λ/103 | λ/62 | λ/36 |
| G | λ/90 | λ/57 | λ/34 |
| G | λ/91 | λ/60 | λ/34 |
| M | λ/86 | λ/53 | λ/31 |
| M | λ/81 | λ/51 | λ/29 |
| B | λ/20 | λ/13 | λ/8 |
| B | λ/29 | λ/19 | λ/12 |
|
|
|||
| UTs | |||
| t0 [ms] | 1 | 2 | 4 |
|
|
|||
| G | λ/32 | λ/20 | λ/12 |
| M | λ/22 | λ/13 | λ/8 |
| M | λ/23 | λ/19 | λ/10 |
| B | λ/20 | λ/13 | λ/8 |
Notes. The noise is written with respect to the wavelength for three different integration times. The values correspond to the worst case 
. Atmospheric conditions are: Excellent (E), Good (G), Medium (M), Bad (B). The corresponding observing conditions can be found in Table 1.
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