activity
20162024
most citedSix transiting planets and a chain of Laplace resonances in TOI-178

195 citations · 2.5k across the 69 of their papers we have counts for

collaborators
Showing 2020Show all

9 papers · 1 filter

astro-ph.EP2020★ 65 cited

WASP-186 and WASP-187: two hot Jupiters discovered by SuperWASP and SOPHIE with additional observations by TESS

N. Schanche, G. Hébrard, A. Collier Cameron +15

We present the discovery of two new hot Jupiters identified from the WASP survey, WASP-186b and WASP-187b (TOI-1494.01 and TOI-1493.01). Their planetary nature was established from…

astro-ph.EP2020★ 46 cited

K2-111: an old system with two planets in near-resonance

A. Mortier, M. R. Zapatero Osorio, L. Malavolta +64

This paper reports on the detailed characterisation of the K2-111 planetary system with K2, WASP, and ASAS-SN photometry as well as high-resolution spectroscopic data from HARPS-N…

astro-ph.EP2020★ 109 cited

The hot dayside and asymmetric transit of WASP-189b seen by CHEOPS

M. Lendl, Sz. Csizmadia, A. Deline +102

The CHEOPS space mission dedicated to exoplanet follow-up was launched in December 2019, equipped with the capacity to perform photometric measurements at the 20 ppm level. As CHEO…

astro-ph.EP2020★ 60 cited

An unusually low density ultra-short period super-Earth and three mini-Neptunes around the old star TOI-561

G. Lacedelli, L. Malavolta, L. Borsato +38

Based on HARPS-N radial velocities (RVs) and TESS photometry, we present a full characterisation of the planetary system orbiting the late G dwarf TOI-561. After the identification…

astro-ph.SR2020★ 122 cited

Three Years of HARPS-N High-Resolution Spectroscopy and Precise Radial Velocity Data for the Sun

X. Dumusque, M. Cretignier, D. Sosnowska +35

The solar telescope connected to HARPS-N has been observing the Sun since the summer of 2015. Such high-cadence, long-baseline data set is crucial for understanding spurious radial…

astro-ph.SR2020★ 44 cited

The dust never settles: collisional production of gas and dust in evolved planetary systems

Andrew Swan, Jay Farihi, Thomas G. Wilson +1

Multi-epoch infrared photometry from Spitzer is used to monitor circumstellar discs at white dwarfs, which are consistent with disrupted minor planets whose debris is accreted and…

astro-ph.EP2020★ 45 cited

TOI-1235 b: a keystone super-Earth for testing radius valley emergence models around early M dwarfs

Ryan Cloutier, Joseph E. Rodriguez, Jonathan Irwin +85

Small planets on close-in orbits tend to exhibit envelope mass fractions of either effectively zero or up to a few percent depending on their size and orbital period. Models of the…

astro-ph.EP2020★ 99 cited

TESS Hunt for Young and Maturing Exoplanets (THYME) III: a two-planet system in the 400 Myr Ursa Major Group

Andrew W. Mann, Marshall C. Johnson, Andrew Vanderburg +51

Exoplanets can evolve significantly between birth and maturity, as their atmospheres, orbits, and structures are shaped by their environment. Young planets (1 Gyr) offer an oppo…

astro-ph.IM2020★ 46 cited

IGAPS: the merged IPHAS and UVEX optical surveys of theNorthern Galactic Plane

M. Monguió, R. Greimel, J. E. Drew +47

The INT Galactic Plane Survey (IGAPS) is the merger of the optical photometric surveys, IPHAS and UVEX, based on data from the Isaac Newton Telescope (INT) obtained between 2003 an…