most citedTransit least-squares survey IV. Earth-like transiting planets expected from the PLATO mission

25 citations · 33 across the 3 of their papers we have counts for

collaborators

5 papers

astro-ph.EP202511 cited

Characterizing WASP-43b's interior structure: unveiling tidal decay and apsidal motion

Lia Marta Bernabò, Szilárd Csizmadia, Alexis M. S. Smith +8

Context. Recent developments in exoplanetary research highlight the importance of Love numbers in understanding their internal dynamics, formation, migration history and their pote…

astro-ph.EP20242 cited

CHEOPS observations confirm nodal precession in the WASP-33 system

A. M. S. Smith, Sz. Csizmadia, V. Van Grootel +86

Aims: We aim to observe the transits and occultations of WASP-33b, which orbits a rapidly-rotating Scuti pulsator, with the goal of measuring the orbital obliquity via the grav…

astro-ph.EP2023

Impact of Cosmic Rays on Atmospheric Ion Chemistry and Spectral Transmission Features of TRAPPIST-1e

Konstantin Herbst, Andreas Bartenschlager, John Lee Grenfell +10

Ongoing observing projects like the James Webb Space Telescope (JWST) and future missions offer the chance to characterize Earth-like exoplanetary atmospheres. Thereby, M-dwarfs ar…

astro-ph.EP20238 cited

The Orbit of Warm Jupiter WASP-106 b is aligned with its Star

Jan-Vincent Harre, Alexis M. S. Smith, Teruyuki Hirano +3

Understanding orbital obliquities, or the misalignment angles between a star's rotation axis and the orbital axis of its planets, is crucial for unraveling the mechanisms of planet…

astro-ph.EP202225 cited

Transit least-squares survey IV. Earth-like transiting planets expected from the PLATO mission

René Heller, Jan-Vincent Harre, Réza Samadi

In its long-duration observation phase, the PLATO satellite will observe two non-overlapping fields for a total of 4 yr. The exact duration of each pointing will be determined 2 yr…