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Millimagnitude photometry for transiting extrasolar planetary candidates II Transits of OGLE TR 113 B in the optical and near ir

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Figure

Fig. 1.— Portion of a SofI K s -band image including OGLE-TR-113 (K s ¼ 13:00), which is the bright star at the center
Fig. 3.— Effective temperature and distance for OGLE-TR-113b. The dashed (red ) lines show the radius-temperature constrain for main-sequence stars (errors in the optical and infrared photometry are considered)
Figure 5 shows a 12 ; 12 arcsec 2 portion of a 0.6 00 seeing image, illustrating that the candidate star is unblended
Fig. 8.— Fit to the single transit of OGLE-TR-113 in the V band. [See the electronic edition of the Journal for a color version of this figure.]
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