The Frequency of Hot Jupiters in the Galaxy

The Frequency of Hot Jupiters in the Galaxy

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 dw...

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Main Authors: Sackett P. D., Bayliss D. D. R.
Format: Article
Language:English
Published: EDP Sciences 2011-02-01
Series:EPJ Web of Conferences
Online Access:http://dx.doi.org/10.1051/epjconf/20101101008
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spelling doaj-369d5a0bf7c24fe18e7468ef8a57d6992021-08-02T01:13:24ZengEDP SciencesEPJ Web of Conferences2100-014X2011-02-01110100810.1051/epjconf/20101101008The Frequency of Hot Jupiters in the GalaxySackett P. D.Bayliss D. D. R.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%. http://dx.doi.org/10.1051/epjconf/20101101008
collection DOAJ
language English
format Article
sources DOAJ
author Sackett P. D.
Bayliss D. D. R.
spellingShingle Sackett P. D.
Bayliss D. D. R.
The Frequency of Hot Jupiters in the Galaxy
EPJ Web of Conferences
author_facet Sackett P. D.
Bayliss D. D. R.
author_sort Sackett P. D.
title The Frequency of Hot Jupiters in the Galaxy
title_short The Frequency of Hot Jupiters in the Galaxy
title_full The Frequency of Hot Jupiters in the Galaxy
title_fullStr The Frequency of Hot Jupiters in the Galaxy
title_full_unstemmed The Frequency of Hot Jupiters in the Galaxy
title_sort frequency of hot jupiters in the galaxy
publisher EDP Sciences
series EPJ Web of Conferences
issn 2100-014X
publishDate 2011-02-01
description 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%.
url http://dx.doi.org/10.1051/epjconf/20101101008
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