Table 5: Absolute photometry and estimated physical properties for the bound and likely bound companions visible on our NACO images. The magnitudes quoted here are those derived from our relative photometry (a few companions have additional uncontaminated photometry in 2MASS). Primary spectral types are from the Hipparcos catalog, while primary masses are from Nordström et al. (2004) or Santos et al. (2005,2004). Note that Santos et al. (2005,2004) do not give uncertainties on the mass, but estimate them to be around 0.05 $M_{\odot }$. When no mass estimate was available for the primary star, we derived one using the available observational constraints and the Geneva stellar evolution code (Meynet & Maeder 2000; Eggenberger et al. 2005). Ages are from Nordström et al. (2004) or were estimated with the Geneva stellar evolution code. For the secondaries, absolute magnitudes, spectral types, and masses are based on our data and were determined as explained in Sect. 4. Projected separations were computed by combining our angular separations with the Hipparcos parallaxes.
Primary Sample Primary Primary mass Primary age Secondary Secondary Secondary Secondary Secondary Secondary mass Proj. sep.
    spec. type ($M_{\odot }$) (Gyr)   MJ MH $M_{K_{\rm s}}$ spec. type ($M_{\odot }$) (AU)

HD 142 A

 planet G1IV $1.28\pm0.05$ 2.8-5.93 HD 142 B $6.16\pm0.09$ $5.40\pm0.06$ $5.18\pm0.16$ K8.5-M1.5 $0.59\pm0.02$ $105.1\pm1.8$
HD 7895 A control K1V $0.86\pm0.05$ 0.9-4.9 HD 7895 D $8.14\pm0.07$   $7.40\pm0.07$ M2-M5 $0.24\pm0.01$ $28.7\pm0.8$
HD 16141 A planet G5IV $1.05\pm0.05$ 9.7-12.9 HD 16141 B   $7.11\pm0.18$ $6.83\pm0.13$ M1-M4 $0.31\pm0.02$ $223\pm11$
HD 24331 A control K2V $0.72\pm0.04$ 4-10 HD 24331 B $9.32\pm0.09$ $8.65\pm0.08$   M4-M6 $0.15\pm0.01$ $73.2\pm1.7$
HD 31412 Aa control F8 $1.04\pm0.06$ 3.5-8.8 HD 31412 Ab $7.25\pm0.23$ $6.37\pm0.11$ $6.18\pm0.11$ M0-M3 $0.43\pm0.02$ $7.1\pm0.3$
HD 40397 A control G0 0.86-0.02+0.05 - HD 40397 B $6.69\pm0.08$ $5.97\pm0.08$   M0-M2 $0.50\pm0.02$ $58.7\pm1.7$
HD 43834 A control G5V $0.93\pm0.05$ - HD 43834 B     $8.43\pm0.05$ M3.5-M6.5 $0.14\pm0.01$ $30.9\pm0.3$
HD 46375 A planet K1IV $0.82\pm0.05$ - HD 46375 B     $5.33\pm0.10$ K9.5-M1.5 $0.58\pm0.02$ $345\pm12$
HD 65216 A planet G5V $0.91\pm0.05$ 0.6-4.6 HD 65216 Ba     $10.02\pm0.09$ M6.5-L0 <0.1 $255.2\pm6.4$
HD 65216 Ba   M6.5-L0 <0.1 0.6-4.6 HD 65216 Bb     $10.92\pm0.09$ M7.5-L4 <0.1 $5.7\pm1.1$
HD 70923 A control G0 $1.09\pm0.05$ 4.5-8.7 HD 70923 B $8.29\pm0.17$   $7.33\pm0.12$ M2-M5 $0.24\pm0.01$ $36.9\pm1.5$
HD 78351 A control G8/K0V 0.84-0.03+0.04 - HD 78351 B   $7.15\pm0.11$ $6.85\pm0.08$ M1-M4 $0.30\pm0.01$ $70.5\pm2.6$
HD 104263 A control G5 $0.91\pm0.05$ 6-14 HD 104263 B $8.39\pm0.12$ $7.70\pm0.13$ $7.50\pm0.12$ M2.5-M4.5 $0.23\pm0.01$ $68.6\pm3.2$
HD 129642 A control K3V $0.82\pm0.05$ 5-11 HD 129642 B   $8.19\pm0.17$   M2.5-M5.5 $0.18\pm0.03$ $157.4\pm5.3$
HD 154682 A control G5V 0.99-0.04+0.06 5.0-12.1 HD 154682 B $7.85\pm0.16$ $7.41\pm0.17$ $7.10\pm0.13$ M1.5-M4.5 $0.27\pm0.02$ $45.3\pm2.3$
HD 177830 A planet K0 $1.45\pm0.15$ - HD 177830 B   $7.71\pm0.15$ $7.39\pm0.18$ M2-M5 $0.23\pm0.01$ $97.1\pm4.4$
HD 196050 A planet G3V $1.15\pm0.05$ 1.8-5.3 HD 196050 Ba     $7.02\pm0.13$ M1.5-M4.5 $0.29\pm0.02$ $501\pm22$
HD 196050 Ba   M1.5-M4.5 $0.29\pm0.02$ 1.8-5.3 HD 196050 Bb     $7.81\pm0.15$ M2.5-M5.5 $0.19\pm0.02$ $19.7\pm1.0$
HD 223913 A control G0V 1.00-0.06+0.08 - HD 223913 B     $5.59\pm0.07$ K9.5-M2.5 $0.53\pm0.01$ $314.0\pm5.1$
HD 82241 control F8V $1.15\pm0.06$ 0.2-5 CC1     $6.14\pm0.07$ M0-M3 $0.43\pm0.01$ $16.3\pm0.4$
HD 134180 control K3V $0.75\pm0.05$ 5-13 CC2     $7.85\pm0.16$ M2.5-M5.5 $0.20\pm0.01$ $505\pm28$


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