Area of research
Astronomy and Astrophysics · Instrumentation
Research interest
Research interests include Physics, Exoplanet, Astronomy, Stars, Astrophysics, and Large Binocular Telescope.
Technical description and performance of the phase II version of the Keck Planet Imager and Characterizer
Paths to robust exoplanet science yield margin for the Habitable Worlds Observatory
HWO yield sensitivities in the NIR and NUV
Nancy Grace Roman Space Telescope coronagraph instrument overview and status
Large Interferometer For Exoplanets (LIFE)
Phase II of the Keck Planet Imager and characterizer: system-level laboratory characterization and preliminary on-sky commissioning
The need for a multi-purpose, optical–NIR space facility after HST and JWST
The HOSTS Survey for Exozodiacal Dust: Observational Results from the Complete Survey
The HOSTS Survey—Exozodiacal Dust Measurements for 30 Stars
The Habitable Exoplanet Observatory (HabEx) Mission Concept Study Interim Report
The path towards high-contrast imaging with the VLTI: the Hi-5 project
The Habitable Exoplanet Observatory
A near-infrared interferometric survey of debris-disc stars. VI. Extending the exozodiacal light survey with CHARA/JouFLU
A HIGH-PRECISION NEAR-INFRARED SURVEY FOR RADIAL VELOCITY VARIABLE LOW-MASS STARS USING CSHELL AND A METHANE GAS CELL
Overview of LBTI: a multipurpose facility for high spatial resolution observations
Nulling Data Reduction and On-Sky Performance of the Large Binocular Telescope Interferometer
FIRST-LIGHT LBT NULLING INTERFEROMETRIC OBSERVATIONS: WARM EXOZODIACAL DUST RESOLVED WITHIN A FEW AU OF η Crv
EXO-zodi modeling for the large binocular telescope interferometer
Apollo (University of Cambridge) 2015cited by 32position: middle
CONSTRAINING THE EXOZODIACAL LUMINOSITY FUNCTION OF MAIN-SEQUENCE STARS: COMPLETE RESULTS FROM THE KECK NULLER MID-INFRARED SURVEYS
Operation and performance of the mid-infrared camera, NOMIC, on the Large Binocular Telescope
L'-band AGPM vector vortex coronagraph's first light on LBTI/LMIRCam
Review of small-angle coronagraphic techniques in the wake of ground-based second-generation adaptive optics systems