I work on observing galaxies at the peak of star formation (2 < z < 3) to relate galaxy properties to observable quantities. I also work to develop instruments that make new observations possible. I am currently testing new fibers that transmit photons in the infrared wavelength band to see if these fibers will be suitable for use in a fiber-fed infrared spectrograph. See my blog page for details of the research process.
This page is currently under construction.