Area of research
Astronomy and Astrophysics · Instrumentation
Research interest
Research interests include Physics, Astrophysics, Stars, Astronomy, Planet, and Exoplanet.
TOI-5005 b: A super-Neptune in the savanna near the ridge
The EBLM Project– XI. Mass, radius, and effective temperature measurements for 23 M-dwarf companions to solar-type stars observed with <i>CHEOPS</i>
Expanding the frontiers of cool-dwarf asteroseismology with ESPRESSO
An unusually low-density super-Earth transiting the bright early-type M-dwarf GJ 1018 (TOI-244)
The geometric albedo of the hot Jupiter HD 189733b measured with CHEOPS
TOI-836: A super-Earth and mini-Neptune transiting a nearby K-dwarf
<i>TESS</i> spots a mini-neptune interior to a hot saturn in the TOI-2000 system
A new dynamical modeling of the WASP-47 system with CHEOPS observations
TOI-5678b: A 48-day transiting Neptune-mass planet characterized with CHEOPS and HARPS
Investigating the visible phase-curve variability of 55 Cnc e
The <i>Gaia</i>-ESO Public Spectroscopic Survey: Implementation, data products, open cluster survey, science, and legacy
The <i>Gaia</i>-ESO Public Spectroscopic Survey: Motivation, implementation, GIRAFFE data processing, analysis, and final data products
The atmosphere and architecture of WASP-189 b probed by its CHEOPS phase curve
A pair of sub-Neptunes transiting the bright K-dwarf TOI-1064 characterized with <i>CHEOPS</i>
The young HD 73583 (TOI-560) planetary system: two 10-M⊕ mini-Neptunes transiting a 500-Myr-old, bright, and active K dwarf
CHEOPS geometric albedo of the hot Jupiter HD 209458 b
Uncovering the true periods of the young sub-Neptunes orbiting TOI-2076
Investigating the architecture and internal structure of the TOI-561 system planets with CHEOPS, HARPS-N, and TESS
HD 23472: a multi-planetary system with three super-Earths and two potential super-Mercuries,
The First Near-infrared Transmission Spectrum of HIP 41378 f, A Low-mass Temperate Jovian World in a Multiplanet System
Examining the orbital decay targets KELT-9 b, KELT-16 b, and WASP-4b, and the transit-timing variations of HD 97658 b
Hot Exoplanet Atmospheres Resolved with Transit Spectroscopy (HEARTS)
The stable climate of KELT-9b
Phase curve and geometric albedo of WASP-43b measured with CHEOPS, TESS, and HST WFC3/UVIS
Connecting photometric and spectroscopic granulation signals with CHEOPS and ESPRESSO
Transit timing variations of AU Microscopii b and c
55 Cancri e’s occultation captured with CHEOPS
CHEOPS finds KELT-1b darker than expected in visible light
Analysis of Early Science observations with the CHaracterising ExOPlanets Satellite (<i>CHEOPS</i>) using<scp>pycheops</scp>
CHEOPS precision phase curve of the Super-Earth 55 Cancri e