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Five new transit epochs of the exoplanet ogle tr 111b

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Academic year: 2020

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Figure

Figure 1. Portion of 0.  5 × 0.  5 images of the night 2008 May 3 observed with FORS2 at VLT
Figure 2.Light curve of OGLE-TR-111 (top) and two comparison stars (middle) of the 2008 May 3 night observed with FORS2 at VLT
Figure 3. 3000 results of 10,000 Monte Carlo iterations (using JTKEBOP with the data of the night 2008 May 12) which show the correlation between the parameters fitted from the light curves: k, r p + r s , T c , i, and the linear coefficient u 1X of a quad
Figure 5. Light curves of all transits of OGLE-TR-111b. The solid lines show our best model fits produced by JKTEBOP
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