Area of research
Astronomy and Astrophysics · Instrumentation
Research interest
Research interests include Physics, Astrophysics, Exoplanet, Planet, Spectrograph, and Stars.
The JWST Early Release Science Program for Direct Observations of Exoplanetary Systems. V. Do Self-consistent Atmospheric Models Represent JWST Spectra? A Showcase with VHS 1256–1257 b
Exploring the directly imaged HD 1160 system through spectroscopic characterization and high-cadence variability monitoring
The JWST Early-release Science Program for Direct Observations of Exoplanetary Systems II: A 1 to 20 μm Spectrum of the Planetary-mass Companion VHS 1256–1257 b
The JWST Early Release Science Program for Direct Observations of Exoplanetary Systems I: High-contrast Imaging of the Exoplanet HIP 65426 b from 2 to 16 μm
Direct images and spectroscopy of a giant protoplanet driving spiral arms in MWC 758
Measuring the variability of directly imaged exoplanets using vector Apodizing Phase Plates combined with ground-based differential spectrophotometry
The JWST Early Release Science Program for the Direct Imaging and Spectroscopy of Exoplanetary Systems
The HOSTS Survey for Exozodiacal Dust: Observational Results from the Complete Survey
Overview and prospects of the LBTI beyond the completed HOSTS survey
Thermal Infrared Imaging of MWC 758 with the Large Binocular Telescope: Planetary-driven Spiral Arms?
The LEECH Exoplanet Imaging Survey: Limits on Planet Occurrence Rates under Conservative Assumptions
The HOSTS Survey—Exozodiacal Dust Measurements for 30 Stars
ALES: overview and upgrades
On-sky operations with the ALES integral field spectrograph
PERSISTENT ASYMMETRIC STRUCTURE OF SAGITTARIUS A* ON EVENT HORIZON SCALES
Overview of LBTI: a multipurpose facility for high spatial resolution observations
THE LEECH EXOPLANET IMAGING SURVEY: CHARACTERIZATION OF THE COLDEST DIRECTLY IMAGED EXOPLANET, GJ 504 b, AND EVIDENCE FOR SUPERSTELLAR METALLICITY*
An 8 h characteristic time-scale in submillimetre light curves of Sagittarius A*
Constraining the sub-au-scale distribution of hydrogen and carbon monoxide gas around young stars with the Keck Interferometer