The Frequency of Hot Jupiters in the Galaxy
EPJ Web of Conferences(2011)
摘要
The frequency of Hot Jupiters around Galactic dwarf stars is determ ined from the results of the SuperLupus transit survey and realistic Monte Carlo simulations of the survey efficiency. We find that for Hot Jupiters with mean radii of 1.1R(J) and periods between 1 and 10 days, the frequency around dwarf stars is just 0.16 +/-(0.6)(0.2)%.
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关键词
monte carlo simulation
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