Table A.4
Approximate predictions for the asymptotic upper limits in detector thermal background and detector dark current perturbation to stay in the fundamental noise dominated case.
| np = xns | x= 1 | x = 5 |
|---|---|---|
| Thermal background temperature (K) | 15.1 | 13.4 |
| Detector dark current (e−1 s−1 px−1) | 4.6 • 10−3 | 7.5 • 10−5 |
Notes. 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 correspond to the limits in Fig. A.3.
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