activity
20142019
most citedAn ultra-short period rocky super-Earth with a secondary eclipse and a Neptune-like companion around K2-141

137 citations · 677 across the 9 of their papers we have counts for

collaborators

9 papers

astro-ph.EP2019★ 18 cited

K2-291 b: A rocky super-Earth in a 2.2 day orbit

Molly R. Kosiarek, Sarah Blunt, Mercedes Lopez-Morales +43

K2-291 (EPIC 247418783) is a solar-type star with a radius of R_star = 0.899 0.034 R_sun and mass of M_star=0.934 0.038 M_sun. From K2 C13 data, we found one super-Eart…

astro-ph.EP2019★ 118 cited

A giant impact as the likely origin of different twins in the Kepler-107 exoplanet system

Aldo S. Bonomo, Li Zeng, Mario Damasso +49

Measures of exoplanet bulk densities indicate that small exoplanets with radius less than 3 Earth radii () range from low-density sub-Neptunes containing volatile element…

astro-ph.EP2018★ 137 cited

An ultra-short period rocky super-Earth with a secondary eclipse and a Neptune-like companion around K2-141

Luca Malavolta, Andrew W. Mayo, Tom Louden +44

Ultra-short period (USP) planets are a class of low mass planets with periods shorter than one day. Their origin is still unknown, with photo-evaporation of mini-Neptunes and in-si…

astro-ph.EP2017★ 63 cited

Precise Masses in the WASP-47 System

Andrew Vanderburg, Juliette C. Becker, Lars A. Buchhave +32

We present precise radial velocity observations of WASP-47, a star known to host a hot Jupiter, a distant Jovian companion, and, uniquely, two additional transiting planets in shor…

astro-ph.EP2017★ 57 cited

The Kepler-19 system: a thick-envelope super-Earth with two Neptune-mass companions characterized using Radial Velocities and Transit Timing Variations

Luca Malavolta, Luca Borsato, Valentina Granata +36

We report a detailed characterization of the Kepler-19 system. This star was previously known to host a transiting planet with a period of 9.29 days, a radius of 2.2 R and…

astro-ph.EP2016★ 52 cited

The Orbit and Mass of the Third Planet in the Kepler-56 System

Oderah Justin Otor, Benjamin T. Montet, John Asher Johnson +20

While the vast majority of multiple-planet systems have their orbital angular momentum axes aligned with the spin axis of their host star, Kepler-56 is an exception: its two transi…