Table A.6

Extrasolar planets detected with transit or RV observations in stellar systems with more than two components, sorted by the increasing projected separation of the host star and the nearest stellar component (). For the closest systems a value for the binary semi-major axis (a_bin) is known from multi-epoch observations (listed in brackets in the column). If RV and transit measurements are available the true mass of the exoplanet candidate is given in the table. ?  ... New system compared to the latest published overview by Mugrauer & Neuhäuser (2009).

Note	Host-star	NPl	N⋆	MPlsini [MJup]	aPl[AU]		Reference
?	HD 126614 A	1	3	0.38	2.35	36.2	Howard et al. (2010); Ginski et al. (2012)
	HD 19994 A	1	3	1.68	1.42	51.5	Mayor et al. (2004); Raghavan et al. (2006)
							Roell et al. (2011)
?	GJ 667 C	2	3	0.018      and      0.014	0.05      and      0.12	227.0	Anglada-Escudé et al. (2012)
	HD 65216 A	1	3	1.21	1.37	256.3	Mayor et al. (2004); Mugrauer et al. (2007b)
?	HD 132563 B	1	3	1.49	2.62	365.2	Desidera et al. (2011)
	HD 196050 A	1	3	3.00	2.50	511.2	Jones et al. (2002); Mugrauer et al. (2005)
							Eggenberger et al. (2007)
	HD 178911 B	1	3	6.29	0.32	794.3	Zucker et al. (2002); Eggenberger et al. (2003)
	16 Cyg B	1	3	1.68	1.68	859.7	Cochran et al. (1997); Raghavan et al. (2006)
?	30 Ari B	1	3	9.88	0.995	1517	Guenther et al. (2009)
	HD 40979 A	1	3	3.32	0.81	6395	Fischer et al. (2003b); Eggenberger et al. (2003)
							Mugrauer et al. (2007a)