EPJ Web of Conferences
Volume 11, 2011Detection and Dynamics of Transiting Exoplanets
|Number of page(s)||3|
|Section||Session 1: Detection and observation of transiting exoplanets|
|Published online||16 February 2011|
The Frequency of Hot Jupiters in the Galaxy
Research School of Astronomy and Astrophysics, The
Australian National University, Cotter Rd, Weston Creek,
The frequency of Hot Jupiters around Galactic dwarf stars is determined 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 1.1RJ and periods between 1 and 10 days, the frequency around dwarf stars is just 0.16±0.60.2%.
© Owned by the authors, published by EDP Sciences, 2011
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