TY - GEN
T1 - Machine Learning Aboard the ADAPT Gamma-Ray Telescope
AU - Htet, Ye
AU - Sudvarg, Marion
AU - Butzel, Andrew
AU - Buhler, Jeremy D.
AU - Chamberlain, Roger D.
AU - Buckley, James H.
N1 - Publisher Copyright:
© 2024 IEEE.
PY - 2024
Y1 - 2024
N2 - The Advanced Particle-astrophysics Telescope (APT) is an orbital mission concept designed to contribute to multi-messenger observations of transient phenomena in deep space. APT will be uniquely able to detect and accurately localize short-duration gamma-ray bursts (GRBs) in the sky in real time. Current detection and analysis systems require resource-intensive ground-based computations; in contrast, APT will perform on-board analysis of GRBs, demanding analytical tools that deliver accurate results under severe size, weight, and power constraints.In this work, we describe a neural network approach in our computation pipeline for GRB localization, demonstrating the capabilities of two neural networks: one to discard signals from background radiation, and one to estimate the uncertainty of GRB source direction constraints associated with individual gamma-ray photons. We validate the accuracy and computational efficiency of our networks using a physical simulation of GRB detection in the Antarctic Demonstrator for APT (ADAPT), a high-altitude balloon-borne prototype for APT.
AB - The Advanced Particle-astrophysics Telescope (APT) is an orbital mission concept designed to contribute to multi-messenger observations of transient phenomena in deep space. APT will be uniquely able to detect and accurately localize short-duration gamma-ray bursts (GRBs) in the sky in real time. Current detection and analysis systems require resource-intensive ground-based computations; in contrast, APT will perform on-board analysis of GRBs, demanding analytical tools that deliver accurate results under severe size, weight, and power constraints.In this work, we describe a neural network approach in our computation pipeline for GRB localization, demonstrating the capabilities of two neural networks: one to discard signals from background radiation, and one to estimate the uncertainty of GRB source direction constraints associated with individual gamma-ray photons. We validate the accuracy and computational efficiency of our networks using a physical simulation of GRB detection in the Antarctic Demonstrator for APT (ADAPT), a high-altitude balloon-borne prototype for APT.
KW - machine learning
KW - multi-messenger astrophysics
KW - neural networks
UR - http://www.scopus.com/inward/record.url?scp=85217162546&partnerID=8YFLogxK
U2 - 10.1109/SCW63240.2024.00008
DO - 10.1109/SCW63240.2024.00008
M3 - Conference contribution
AN - SCOPUS:85217162546
T3 - Proceedings of SC 2024-W: Workshops of the International Conference for High Performance Computing, Networking, Storage and Analysis
SP - 4
EP - 10
BT - Proceedings of SC 2024-W
PB - Institute of Electrical and Electronics Engineers Inc.
T2 - 2024 Workshops of the International Conference for High Performance Computing, Networking, Storage and Analysis, SC Workshops 2024
Y2 - 17 November 2024 through 22 November 2024
ER -