Open Access
Table A.1
Predicted planet yield around Sun-like stars for the different planet populations, median exozodiacal dust levels z, interferometric baseline length optimization schemes, and mirror diameters D.
Population | ![]() |
baseline optimization | D (m) | Ndet | Ndet,opt HZ | Ndet,con HZ | Ndet,EEC |
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1.0 | ![]() |
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opt HZ | 2.0 | ![]() |
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hab2min | 3 | 3.5 | ![]() |
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1.0 | ![]() |
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con HZ | 2.0 | ![]() |
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3.5 | ![]() |
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1.0 | ![]() |
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opt HZ | 2.0 | ![]() |
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hab2max | 3 | 3.5 | ![]() |
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1.0 | ![]() |
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con HZ | 2.0 | ![]() |
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3.5 | ![]() |
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1.0 | ![]() |
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opt HZ | 2.0 | ![]() |
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hab2min | 12 | 3.5 | ![]() |
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1.0 | ![]() |
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con HZ | 2.0 | ![]() |
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3.5 | ![]() |
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1.0 | ![]() |
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opt HZ | 2.0 | ![]() |
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hab2max | 12 | 3.5 | ![]() |
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1.0 | ![]() |
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con HZ | 2.0 | ![]() |
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3.5 | ![]() |
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