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Table 3:

Geometrical parameters determined for six systems.
Transit r/R a/R b u
OGLE-TR-106 $0.1454^{\rm +0.0071}_{-0.0060}$ $13.3^{\rm +1.1}_{-2.1}$ $0.35^{\rm +0.29}_{-0.35}$ 0.6
OGLE-TR-109 $0.0771^{\rm +0.0037}_{-0.0029}$ $1.88^{\rm +0.12}_{-0.25}$ $0.17^{\rm +0.48}_{-0.16}$ 0.597*
OGLE-TR-111 $0.1284^{\rm +0.0066}_{-0.0033}$ $12.31^{\rm +0.74}_{-1.56}$ $0.31^{\rm +0.25}_{-0.31}$ 0.768*
OGLE-TR-113 $0.1451^{\rm +0.0064}_{-0.0022}$ $6.49^{\rm +0.10}_{-0.66}$ $0.11^{\rm +0.35}_{-0.09}$ 0.780*
OGLE-TR-159 $0.41^{\rm +0.03}_{-0.20}$ $4.18^{\rm +0.24}_{-0.15}$ $1.11^{\rm +0.05}_{-0.15}$ 0.6
OGLE-TR-170 $0.23^{\rm +0.19}_{-0.05}$ $2.96^{\rm +0.19}_{-0.10}$ $0.91^{\rm +0.26}_{-0.12}$ 0.6

In the columns we provide: ratio of the radii of the components r/R, ratio of the radius of the orbit of the secondary to the radius of the primary, impact parameter b, and linear limb-darkening coefficient u. For objects OGLE-TR-109, OGLE-TR-111, and OGLE-TR-113 the limb-darkening coefficient was taken from Claret (2000).


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