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arXiv · 1512.06433

Solution of newly observed transit of the exoplanet HAT-P-24b: no TTV and TDV signals

Diana Kjurkchieva·Dinko Dimitrov·Sunay Ibryamov
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Abstract

We present photometric observations of transit of the exoplanet HAT-P-24b using the Rozhen 2 m telescope. Its solution gives relative stellar radius r_{s}=0.1304 (a/R_{s}=7.669), relative planet radius r_{p}=0.01304 and orbital inclination of 90 degree. The calculated planet radius is R_{p}=1.316 R_{J} and corresponds to planet density of rho_{p}=0.37 g cm^{-3}. Our parameter values are between those of the previous two solutions. We did not find evidences of TTV and TDV signals of HAT-P-24b.

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Diana Kjurkchieva, Dinko Dimitrov, Sunay Ibryamov. 2015-12-20. Solution of newly observed transit of the exoplanet HAT-P-24b: no TTV and TDV signals. https://arxiv.org/abs/1512.06433

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