activity
20192021
most citedCHEOPS observations of the HD 108236 planetary system: A fifth planet, improved ephemerides, and planetary radii

82 citations · 258 across the 6 of their papers we have counts for

collaborators

8 papers

astro-ph.EP202127 cited

A HARPS-N mass for the elusive Kepler-37d: a case study in disentangling stellar activity and planetary signals

V. M. Rajpaul, L. A. Buchhave, G. Lacedelli +22

To date, only 18 exoplanets with radial velocity (RV) semi-amplitudes m/s have had their masses directly constrained. The biggest obstacle to RV detection of such exoplanets i…

astro-ph.EP20211 cited

Exploiting timing capabilities of the CHEOPS mission with warm-Jupiter planets

Borsato L, Piotto G, Gandolfi D +75

We present 17 transit light curves of seven known warm-Jupiters observed with the CHaracterising ExOPlanet Satellite (CHEOPS). The light curves have been collected as part of the C…

astro-ph.EP202130 cited

A PSF-based Approach to TESS High quality data Of Stellar clusters (PATHOS) -- IV. Candidate exoplanets around stars in open clusters: frequency and age-planetary radius distribution

D. Nardiello, M. Deleuil, G. Mantovan +7

The knowledge of the ages of stars hosting exoplanets allows us to obtain an overview on the evolution of exoplanets and understand the mechanisms affecting their life. The measure…

astro-ph.EP2021

Detecting General Relativistic Orbital Precession in Transiting Hot Jupiters

G. Antoniciello, L. Borsato, G. Lacedelli +3

Both classical and relativistic weak-field and slow-motion perturbations to planetary orbits can be treated as perturbative corrections to the Keplerian model. In particular, tidal…

astro-ph.EP202182 cited

CHEOPS observations of the HD 108236 planetary system: A fifth planet, improved ephemerides, and planetary radii

A. Bonfanti, L. Delrez, M. J. Hooton +106

The detection of a super-Earth and three mini-Neptunes transiting the bright ( = 9.2 mag) star HD 108236 (also known as TOI-1233) was recently reported on the basis of TESS and…

astro-ph.EP2020

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…