https://doi.org/10.1051/epjconf/20101101008
The Frequency of Hot Jupiters in the Galaxy
Research School of Astronomy and Astrophysics, The
Australian National University, Cotter Rd, Weston Creek,
ACT 2611,
Australia
[daniel@mso.anu.edu.au]
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
