activity
20142024
most citedSOAP 2.0: A tool to estimate the photometric and radial velocity variations induced by stellar spots and plages

268 citations · 1.8k across the 34 of their papers we have counts for

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Showing 2016Show all

5 papers · 1 filter

astro-ph.EP201616 cited

On the radial velocity detection of additional planets in transiting, slowly rotating M-dwarf systems: the case of GJ 1132

Ryan Cloutier, René Doyon, Kristen Menou +3

M-dwarfs are known to commonly host high-multiplicity planetary systems. Therefore M-dwarf planetary systems with a known transiting planet are expected to contain additional small…

astro-ph.EP2016108 cited

Kepler-21b: A rocky planet around a V = 8.25 magnitude star

Mercedes Lopez-Morales, Raphaelle D. Haywood, Jeffrey L. Coughlin +36

HD 179070, aka Kepler-21, is a V = 8.25 F6IV star and the brightest exoplanet host discovered by Kepler. An early detailed analysis by Howell et al. (2012) of the first thirteen mo…

astro-ph.EP2016115 cited

Radial-Velocity Fitting Challenge. II. First results of the analysis of the data set

X. Dumusque, F. Borsa, M. Damasso +21

Radial-velocity (RV) signals induce RV variations an order of magnitude larger than the signal created by the orbit of Earth-twins, thus preventing their detection. The goal of thi…

astro-ph.EP201690 cited

A 1.9 Earth radius rocky planet and the discovery of a non-transiting planet in the Kepler-20 system

Lars A. Buchhave, Courtney D. Dressing, Xavier Dumusque +35

Kepler-20 is a solar-type star (V = 12.5) hosting a compact system of five transiting planets, all packed within the orbital distance of Mercury in our own Solar System. A transiti…

astro-ph.EP201668 cited

Radial Velocity Fitting Challenge. I. Simulating the data set including realistic stellar radial-velocity signals

X. Dumusque

Stellar signals are the main limitation for precise radial-velocity (RV) measurements. These signals arise from the photosphere of the stars. The m/s perturbation created by these…