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Table C.1.

Stellar parameters for directly imaged systems with SPHERE.

Name Spec type M*M L*L Age Dist
(Myr) (pc)
HD 1466 F8 1.1 1.6 45 42.9 ± 0.4 a
HD 3003 A0 2.1 18.2 45 45.5 ± 0.4 b
HD 15115 F2 1.3 3.9 45 48.2 ± 1 a
HD 30447 F3 1.3 3.9 42 80.3 ± 1.6 a
HD 35114 F6 1.2 2.3 42 47.4 ± 0.5 a
ζ Lep A2 1.9 21.6 300 ± 180 21.6 ± 0.1 b
HD 43989 F9 1.1 1.6 45 51.2 ± 0.8 a
HD 61005 G8 0.9 0.7 50 36.7 ± 0.4 a
HD 71155 A0 2.4 40.5 260 ± 75 37.5 ± 0.3 b
HD 75416 B8 3 106.5 11 ± 3 95 ± 1.4 b
HD 84075 G2 1.1 1.4 50 62.9 ± 0.9 a
HD 95086 A8 1.6 8 16 ± 5 83.8 ± 1.9 a
β Leo A3 1.9 14.5 50 11 ± 0.1 b
HD 106906 F5 2.7 c 6.8 16±5 102.8 ± 2.5 a
HD 107301 B9 2.4 42.6 16 ± 5 93.9 ± 3 b
HR 4796 A0 2.3 26.8 10 ± 3 72.8 ± 1.7 b
ρ Vir A0 1.9 15.9 100 ± 80 36.3 ± 0.3 b
HD 122705 A2 1.8 12.3 17 ± 5 112.7 ± 9.3 b
HD 131835 A2 1.9 15.8 17 ± 5 145.6 ± 8.5 a
HD 133803 A9 1.6 6.2 17 ± 5 111.8 ± 3.3 a
β Cir A3 2 18.5 400 ± 140 30.6 ± 0.2 b
HD 140840 B9 2.3 37.4 17 ± 5 165 ± 10.4 a
HD 141378 A5 1.9 17 380 ± 190 55.6 ± 2.1 a
π Ara A5 1 13.7 600 ± 220 44.6 ± 0.5 b
HD 174429 G9 1 1.6 24 ± 5 51.5 ± 2.6 b
HD 178253 A2 2.2 31 380 ± 90 38.4 ± 0.4 b
η Tel A0 2.2 21.3 24 ± 5 48.2 ± 0.5 b
HD 181327 F6 1.3 3 24 ± 5 48.6 ± 1.1 a
HD 188228 A0 2.3 26.6 50 32.2 ± 0.2 b
ρ Aql A2 2.1 21.6 350 ± 150 46 ± 0.5 b
HD 202917 G7 0.9 0.8 45 47.6 ± 0.5 a
HD 206893 F5 1.3 3 250 40.7 ± 0.4 a
HR 8799 A5 1.5 8 42 40.4 ± 1 a
HD 219482 F6 1 2.3 400 20.5 ± 0.1 b
HD 220825 A0 2.1 22.9 149 47.1 ± 0.6 b

Notes. For each star we show spectral type, mass (in solar mass units), luminosity (in solar luminosity units), age and distance.

Gaia parallaxes (Lindegren et al. 2016);

Hipparcos parallaxes (van Leeuwen 2007);

Mass of the star from Bonavita et al. (2016).

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