@inproceedings{e97701005ce24e838cf5c00064dbb726,
title = "The frequency of Hot Jupiters in the Galaxy",
abstract = "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%.",
author = "Bayliss, {D. D.R.} and Sackett, {P. D.}",
note = "Publisher Copyright: {\textcopyright} 2011 Owned by the authors, published by EDP Sciences.; 2010 International Conference on Transiting Planets: Detection and Dynamics ; Conference date: 23-08-2010 Through 27-08-2010",
year = "2011",
month = feb,
day = "16",
doi = "10.1051/epjconf/20101101008",
language = "English",
series = "EPJ Web of Conferences",
publisher = "EDP Sciences",
editor = "R. Diaz and C. Moutou and F. Bouchy",
booktitle = "Detection and Dynamics of Transiting Exoplanets",
address = "France",
}