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Table 1
5σ Teff, MP detection limits at 1 and 5 Gyr obtained for ϵ Ind Ab from NaCo L′ observations, at a separation of 1.5′′ and 3′′ from the central star, using RSM contrast curves derived at a TPR of 50 and 90%.
| Model, assumed age | Teff [K] at 1.5′′ | MP [MJ ] at 1.5′′ | Teff [K] at 3′′ | MP [MJ] at 3′′ |
|---|---|---|---|---|
| (TPR 50%, 90%) | (TPR 50%, 90%) | (TPR 50%, 90%) | (TPR 50%, 90%) | |
| AMES-Cond 2000, 1 Gyr | 199, 216 | 1.7, 1.9 | 189, 193 | 1.5, 1.6 |
| Morley et al. (2012, 2014), 1 Gyr | 247, 264 | 2.6, 3 | 234, 240 | 2.3, 2.4 |
| AMES-Cond 2000, 5 Gyr | 198, 220 | 4.4, 5.3 | 186, 190 | 4, 4.1 |
| Morley et al. (2012, 2014), 5 Gyr | 247, 264 | 6.4, 7.3 | 234, 240 | 5.9, 6.1 |
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