UV astronomy, detector physics, and space instrumentation
NASA SmallSat mission studying diffuse O VI emission from the warm-hot circumgalactic medium of nearby galaxies using twin far-UV spectrographs.
1-meter near-UV telescope with multi-object spectrograph studying redshifted Lyman-alpha emission from circumgalactic gas.
Investigating fundamental noise properties of silicon detector arrays using single-photon detection capabilities of EMCCDs.
Developing and testing single-photon counting EMCCDs for UV astronomy applications in future space missions.
Developing delta-doped EMCCDs with high UV quantum efficiency through atomic layer deposition anti-reflection coatings.
UV-enhanced delta-doped Skipper CCDs achieving sub-electron read noise through multiple non-destructive readouts.
Specialized test facility for measuring detector quantum efficiency and noise performance in the vacuum ultraviolet regime.
Upgrading SuperLOTIS robotic telescope detector system for near-UV transient observations including GW events and GRBs.
Advanced optical metrology using interferometry, computer-generated holograms, and photogrammetry for precision space telescope alignment.
Open to discussing research opportunities in UV astronomy and detector physics.