Fig. 7
Differential flux F13b of a planet predicted by the evolutionary model BT-Settl (Allard et al. 2012) as a function of mass for all targets and three separations (rows). The stars are sorted by age, <100 Myr (left column) and ≥100 Myr (right column). The top right part of the right panels shows the curve for HIP 114046, which is a very old star (8 Gyr, Table 1).
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