Table A.5
Extrasolar planets detected with transit or RV observations in wider binaries with a projected stellar separation of ), sorted by an increasing stellar separation. 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). ? ... Closer component listed in the CCDM (formerly called B) was disproved by proper motion measurements, but a new wide stellar companion was found and confirmed by common proper motion (Mugrauer et al. 2005). § ... B component is a white dwarf, see Porto de Mello & da Silva (1997).
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