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Article . 2011 . Peer-reviewed
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The Frequency of Hot Jupiters in the Galaxy

descriptionPublicationkeyboard_double_arrow_right Article , Other literature type 01 Jan 2011Publisher:EDP SciencesJournal:EPJ Web of Conferences, volume 11, page 1,008 (eissn: 2100-014X, Copyright policy )
Authors: Penny D. Sackett; Daniel Bayliss;

doi: 10.1051/epjconf/20101101008 , 10.1051/epjconf/20111101008

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%.

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Keywords

Physics, QC1-999

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citations
This is an alternative to the "Influence" indicator, which also reflects the overall/total impact of an article in the research community at large, based on the underlying citation network (diachronically).
BIP!Citations provided by BIP!
popularity
This indicator reflects the "current" impact/attention (the "hype") of an article in the research community at large, based on the underlying citation network.
BIP!Popularity provided by BIP!
influence
This indicator reflects the overall/total impact of an article in the research community at large, based on the underlying citation network (diachronically).
BIP!Influence provided by BIP!
impulse
This indicator reflects the initial momentum of an article directly after its publication, based on the underlying citation network.
BIP!Impulse provided by BIP!
0
Average
Average
Average
Published in a Diamond OA journal