Dr. Nicholas Cannady is an Assistant Research Scientist at the University of Maryland, Baltimore County working at NASA GSFC as a member of the Center for Research and Exploration in Space Science and Technology (CRESST-II). His research has centered on the instrumentation to acquire, the simulation of, and the reconstruction of gamma-ray and cosmic-ray data in the MeV–TeV range. In his graduate work at Louisiana State University in the CALET collaboration, Dr. Cannady defined the separation photon primaries from charged galactic cosmic rays (GCRs), characterized the instrument response to those events, and analyzed the signals from transient and persistent astrophysical sources. He has experience with leveraging High-Performance Computer (HPC) resources for large-scale simulations, low-level data handling and processing, and getting his hands dirty with detector construction and testing in the lab.
Since coming to GSFC, Dr. Cannady has continued and expanded his work on CALET to include analysis of cosmic-ray electrons at the highest energies and ultra-heavy nuclei beyond iron. Drawing on his experience with the LSU SuperMike-II HPC cluster, he uses the NCCS ADAPT cluster at GSFC to carry out high-statistics simulations of particles interacting in the CALET calorimeter at GeV–TeV energies.
In addition to his work on CALET, Dr. Cannady has joined various teams contributing to future cosmic-ray and gamma-ray missions. He is the UMBC PI for the TIGERISS project, selected in 2022 for the NASA Astrophysics Pioneers program, for which he leads Cherenkov detector development and the Science and Mission Operations Center planning and implementation. TIGERISS will be installed on the International Space Station and measure the abundances of GCR nuclei from boron to beyond lead. Dr. Cannady is a member of the AMEGO team, contributing to the ComPair balloon-borne prototype and the proposed AMEGO-X MIDEX-class mission, leading the development of the Anti-Coincidence detectors for both. In working with the ComPair CdZnTe calorimeter subsystem team, he also works towards the reconstruction algorithms of GECCO, a proposed medium-energy gamma-ray mission using a combined coded-mask and Compton telescope imaging technique.