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Table E.1

Required observation time in days.

(a) Nominal case

Observation Time [days]
R 20 35 50 100
S/N 1m Mirrors 5 48.6 85.7 122.5 249.1
10 194.6 342.7 490.1 996.2
15 437.8 771.0 1102.7 2241.5
20 778.3 1370.6 1960.4 3984.8

2m Mirrors 5 4.7 8.2 11.7 23.9
10 18.6 32.7 46.7 95.4
15 41.9 73.5 105.0 214.7
20 74.5 130.7 186.6 381.7

3.5 m Mirrors 5 1.0 1.7 2.4 4.9
10 3.8 6.7 9.5 19.6
15 8.6 15.1 21.5 44.2
20 15.3 26.8 38.2 78.5
(b) Optimized case

Observation Time [days]
R 20 35 50 100
S/N 1m Mirrors 5 57.7 102.5 147.1 294.7
10 230.6 410.0 588.5 1178.7
15 518.9 922.2 1324.2 2652.2
20 922.5 1639.5 2354.1 4714.9

2m Mirrors 5 4.0 7.1 10.2 20.6
10 16.0 28.5 41.0 82.3
15 36.2 64.2 92.1 185.2
20 64.4 114.2 163.8 329.2

3.5m Mirrors 5 0.6 1.0 1.4 2.9
10 2.2 3.9 5.7 11.4
15 5.0 8.9 12.7 25.7
20 8.9 15.8 22.6 45.8

Notes. Observation times necessary for LIFE to investigate an Earth-twin at 10 pc in orbit around a G2 star for the grid of R and S/N discussed in this publication. The S/N in the Table corresponds to the S/N at 11.2 µm. We consider three different aperture diameters (1m, 2m, and 3.5m) and conservatively assume a total instrument throughput of 5% (cf. Dannert et al. 2022). (a): Nominal case; (b): Optimized case.

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