activity
20172020
most citedAn Ultra-Hot Neptune in the Neptune desert

85 citations · 245 across the 7 of their papers we have counts for

collaborators

10 papers

astro-ph.EP202085 cited

An Ultra-Hot Neptune in the Neptune desert

James S. Jenkins, Matías R. Díaz, Nicolás T. Kurtovic +81

About one out of 200 Sun-like stars has a planet with an orbital period shorter than one day: an ultra-short-period planet (Sanchis-ojeda et al. 2014; Winn et al. 2018). All of the…

astro-ph.EP202041 cited

A multiple planet system of super-Earths orbiting the brightest red dwarf star GJ887

S. V. Jeffers, S. Dreizler, J. R. Barnes +29

The nearest exoplanets to the Sun are our best possibilities for detailed characterization. We report the discovery of a compact multi-planet system of super-Earths orbiting the ne…

astro-ph.EP202035 cited

Search for Nearby Earth Analogs. II. detection of five new planets, eight planet candidates, and confirmation of three planets around nine nearby M dwarfs

Fabo Feng, R. Paul Butler, Stephen A. Shectman +9

Zechmeister et al. (2009) surveyed 38 nearby M dwarfs from March 2000 to March 2007 with VLT2 and the UVES spectrometer. This data has recently been reanalyzed (Butler et al. 2019)…

astro-ph.EP201930 cited

TOI-132 b: A short-period planet in the Neptune desert transiting a G-type star

Matías R. Díaz, James S. Jenkins, Davide Gandolfi +45

The Neptune desert is a feature seen in the radius-mass-period plane, whereby a notable dearth of short period, Neptune-like planets is found. Here we report the {\it TESS} discove…

astro-ph.EP201927 cited

GJ357: A low-mass planetary system uncovered by precision radial-velocities and dynamical simulations

James S. Jenkins, Francisco J. Pozuelos, Mikko Tuomi +5

We report the detection of a new planetary system orbiting the nearby M2.5V star GJ357, using precision radial-velocities from three separate echelle spectrographs, HARPS, HiRES, a…

astro-ph.EP2019

Frequency of planets orbiting M dwarfs in the Solar neighbourhood

M. Tuomi, H. R. A. Jones, R. P. Butler +14

The most abundant stars in the Galaxy, M dwarfs, are very commonly hosts to diverse systems of low-mass planets. Their abundancy implies that the general occurrence rate of planets…