My early enthusiasm for astronomy was fueled by a passion for telescopes and optics.  At both Caltech and MIT, the development of astronomical instrumentation has been an ongoing focus of my research. 

   During my graduate years, I participated in the construction of the "Large Format Camera" for the 200 inch Hale Telescope at Palomar Observatory.  LFC covers the 200 inch prime focus with an array of eight 2048 x 4096 pixel CCDs, creating a 24 arcminute field of view. 

   Since arriving at MIT, I have become interested in infrared spectroscopy as a tool for studying intergalactic matter in the early universe.  I am currently working with a team at MIT, the University of Michigan, and the University of Rochester to develop FIRE, a new spectrometer for the 6.5 meter Magellan telescopes.  FIRE will operate in the 1-2.5 micron wavelength range, offering both the sensitivity and wavelength resolution required for the study of distant galaxies and quasars. 

   For more information on any of these facilities or instruments, please follow the links below.

• The LFC (Large Format Camera)
• FIRE
• Palomar Observatory
• The Magellan Telescopes
• Keck Observatory