Dr. Nicholas Cannady is a Research Astrophysicist at NASA GSFC. 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 taken on leadership of the CALET US team, and is the US member of the CALET International Executive Committee. He 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 a member of 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 also the GSFC institutional PI of the pGRAMS mission, which is a balloon-borne prototype for the GRAMS detector concept. GRAMS uses a LAr Time Projection Chamber in conjunction with a time-of-flight detector to address science goals pertaining to both MeV gamma-ray astronomy and cosmic-ray anti-particle detection.
Dr. Cannady also participates in a number of efforts towards future gamma-ray and cosmic-ray missions, including ComPair (a prototype for the AMEGO family of MeV gamma-ray observatories) and GALE (a balloon-borne MeV gamma-ray telescope utilizing a coded aperture for fine spatial resolution).