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Physical properties and radius variations in the HAT P 5 planetary system from simultaneous four colour photometry

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Figure

Table 3. Times of minimum light of HAT-P-5 and their residuals versus theephemeris derived in this work.
Table 4. Parameters of the JKTEBOP fits to the light curves of HAT-P-5. The final parameters are the weighted means of theresults for the six data sets
Figure 3. As for Fig. 2 but for the z and R light curves of HAT-P-5 presentedby Bakos et al
Table 5. Fractional planetary radius values (rb = Rba ) foundfrom the available data with the linear LD coefficient eitherfitted or fixed, when the other photometric parameters are fixedat their known/final values.
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