Instrumentation
Exoplanet Transmission Spectroscopy:
I build and use instruments to characterize the atmospheres of exoplanets using transit spectroscopy. I'm currently working on a new type of spectrograph:
I am the lead scientist and optical engineer for the Exoplanet Transmission Spectroscopy Imager (ETSI). It is unlike any other spectrographs in that it uses a thin-film optical coated multiband filter with 15 bandpasses simultaneously imaged on two detectors and novel data processing techniques.
In prep: the theory behind how the ETSI instrument will make precision spectrophotometric measurements & characterization of the atmosphere of a hot-saturn (retrieval in image above)
Direct Imaging of Exoplanets:
Prior to my current exoplanet/exomoon PhD research, I spent the first decade of my career as an optical engineer. I have led the optical design of nearly half a dozen astronomical instruments, including major instruments on 8-10 meter class telescopes. I primarily design and build specialized exoplanet instrumentation. Recently, I have worked on several of the integral field spectrographs (IFSs) for exoplanet high-contrast imaging and spectroscopy:
I am currently part of the Gemini Planet Imager (GPI) Consortium. I am the optical designer for the upgrades of the IFS:
 GPI 2.0: Characterizing Self-Luminous Exoplanets Through Low-Resolution Infrared Spectroscopy
GPI 2.0: performance of upgrades to the Gemini Planet Imager CAL and IFS
I was lead optical engineer and part of the science team for the Subaru/SCExAO/CHARIS IFS:
I also helped design a high contrast IFS (HCIFS) testbed for the Nancy Grace Roman Space Telescope:
Photo Credit: Robert de Rosa and Christian Marois
Past Research:
Instrument Pipelines and Simulators:
Direct Imaging of Exoplanets
(AO & Coronagraphy):