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%
It has been suggested that the occurrence rate of hot Jupiters (HJs) in open clusters might reach se...
International audienceContext. The discovery of about 700 extrasolar planets, so far, has lead to th...
The properties of a planetary system may be influenced by properties of the host star, such as its b...
The frequency of Hot Jupiters around Galactic dwarf stars is determined from the ...
Abstract. The frequency of Hot Jupiters around Galactic dwarf stars is deter-mined from the results ...
We derive the frequencies of hot Jupiters (HJs) with 3--5 day periods and very hot Jupiters (VHJs) w...
We determine the fraction of F, G, and K dwarfs in the solar neighborhood hosting hot Jupiters as me...
We present the results of the SuperLupus Survey for transiting hot Jupiter planets, which monitored ...
We discuss our high-precision radial velocity results of a sample of 90 M dwarfs observed with the H...
Context. Hot Jupiters form an enigmatic class of object whose formation pathways are not yet clear. ...
The WFCAM Transit Survey (WTS) is a near-infrared transit survey running on the United Kingdom Infra...
The Pan-Planets survey observed an area of 42 sq deg. in the galactic disk for about 165 h. The main...
We present the results of a deep, wide-field search for transiting hot Jupiter (HJ) planets in the g...
The Pan-Planets survey observed an area of 42 sq deg. in the galactic disk for about 165 h. The main...
I investigate the observational biases inherent in exoplanet transit surveys and explain the methodo...
It has been suggested that the occurrence rate of hot Jupiters (HJs) in open clusters might reach se...
International audienceContext. The discovery of about 700 extrasolar planets, so far, has lead to th...
The properties of a planetary system may be influenced by properties of the host star, such as its b...
The frequency of Hot Jupiters around Galactic dwarf stars is determined from the ...
Abstract. The frequency of Hot Jupiters around Galactic dwarf stars is deter-mined from the results ...
We derive the frequencies of hot Jupiters (HJs) with 3--5 day periods and very hot Jupiters (VHJs) w...
We determine the fraction of F, G, and K dwarfs in the solar neighborhood hosting hot Jupiters as me...
We present the results of the SuperLupus Survey for transiting hot Jupiter planets, which monitored ...
We discuss our high-precision radial velocity results of a sample of 90 M dwarfs observed with the H...
Context. Hot Jupiters form an enigmatic class of object whose formation pathways are not yet clear. ...
The WFCAM Transit Survey (WTS) is a near-infrared transit survey running on the United Kingdom Infra...
The Pan-Planets survey observed an area of 42 sq deg. in the galactic disk for about 165 h. The main...
We present the results of a deep, wide-field search for transiting hot Jupiter (HJ) planets in the g...
The Pan-Planets survey observed an area of 42 sq deg. in the galactic disk for about 165 h. The main...
I investigate the observational biases inherent in exoplanet transit surveys and explain the methodo...
It has been suggested that the occurrence rate of hot Jupiters (HJs) in open clusters might reach se...
International audienceContext. The discovery of about 700 extrasolar planets, so far, has lead to th...
The properties of a planetary system may be influenced by properties of the host star, such as its b...
DOI
Add to ORKG