Kent designs and builds optical instrumentation for astronomy. The science goal of these instruments is the detection of exoplanets and exoplanet life. Astronomical instrumentation work includes: the Palomar Testbed Interfereometer, the Palomar adaptive optics system, the Keck Interferometer, and the Gemini Planet Imager (GPI). Most recently he has collaborated with Caltech on the developement of the Keck Fiber Injection Unit. He has been developing the Zernike Wavefront Sensor for precision wavefront control for high-contrast imaging.
Wavefront sensing, novel optical methods and instrumentation, exoplanet detection.
1. Ruane, G., Wang, J., Mawet, D., Jovanovic, N., Delorme, J.-R., Mennesson, B., and Wallace, J. Kent, “Efficient spectroscopy of exoplanets at small angular separations with vortex fiber nulling”, The Astrophysics Journal, Vol. 867, Issue 2, p. 143 (2018)
2. Bottom, M., Wallace, J. Kent, Bartos, R.D., Shelton, J.C., and Serabyn, E. “Speckle suppression and companion detection using coherent differential imaging”, Monthly Notices of the Royal Astronomical Society, Vol. 464, Issue 3, pp. 2937-2951 (2016)
3. Serabyn, E., Wallace, J. Kent, and Mawet, D., “Speckle-phase measurement in a tandem-vortex coronagraph”, Applied Optics, Vol. 50, Issue 28, pp. 5453-5456 (2011).