Table A.3
Approximate predictions for the maximum allowed perturbation rms to stay in the fundamental noise dominated case.
σfund = xσinst OPD error rms (nm) | x = 1 Relative | x = 5 amplitude error rms (in %) |
---|---|---|
0.75 | 0 | … |
0.50 | 0.02 | … |
0.16 | 0.08 | 0 |
0.10 | 0.13 | 0.02 |
0.05 | 0.24 | 0.05 |
0.01 | 0.62 | 0.12 |
0 | 0.67 | 0.14 |
Notes. rms perturbations values are given relative to the reference wavelength of 10 µm. Presented values are for an observation of an Earth-twin at 10 pc with LIFE configured in the baseline scenario in the λb = 4.1 µm wavelength bin, i.e., the given values follow the contours in Fig. A.2. The asymptotic upper limits are indicated by the bold text.
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