Table D.1
Comparison of the post-AO residuals for the LWE#1 and LWE#2 perturbations, with and without an ideal PP and PTT correction.
| LWE # | SR | rms (nm) | |
|---|---|---|---|
| 1 | Uncorrected post-AO residuals | 70 %a | 160a |
| 1 | PP+PTT ideal correction | 98 %b | 37b |
| 2 | Uncorrected post-AO residuals | 34 %c | 263c |
| 2 | PP+PTT ideal correction | 96 %d | 55d |
Notes. Residuals after the ideal PP+PTT correction give the power of the higher-order LWE petaling modes. These values are taken without atmosphere. SR values are in H band. (a) corresponds to Fig. C.1.a but without the atmosphere contribution. (b) corresponds to the OPD screen on Fig. D.1a. (c) corresponds to Fig. C.2.a but without the atmosphere contribution. (d) corresponds to the OPD screen on Fig. D.1b.
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