Table A.4
Extrasolar planets detected with transit or RV observations in closer binaries with a projected stellar separation of , sorted by an increasing stellar separation. For the four closest systems a value for the binary semi-major axis (abin) 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). ? ... B component is a brown dwarf, see Mugrauer et al. (2006b). ? ... B component is a white dwarf, see Mugrauer & Neuhäuser (2005). § ... B component is a white dwarf, see Chauvin et al. (2007). d ... Reffert & Quirrenbach (2011) determined an astrometric mass range for the planet candidate, which is given within the brackets in the planetary mass column.
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