Prompt and Accurate GRB Source Localization Aboard the Advanced Particle Astrophysics Telescope (APT) and its Antarctic Demonstrator (ADAPT)

Authors

Ye Htet, McKelvey School of Engineering
Marion Sudvarg, McKelvey School of Engineering
Jeremy Buhler, McKelvey School of Engineering
Roger Chamberlain, McKelvey School of Engineering
Wenlei Chen, College of Science and Engineering
James Buckley, McDonnell Center for the Space Sciences
Roger D. Chamberlain, McKelvey School of Engineering
James H. Buckley, McDonnell Center for the Space Sciences
Corrado Altomare, Istituto Nazionale di Fisica Nucleare, Sezione di Bari
Matthew Andrew, University of Hawaiʻi at Mānoa
Blake Bal, McDonnell Center for the Space Sciences
Richard G. Bose, McDonnell Center for the Space Sciences
Dana Braun, McDonnell Center for the Space Sciences
Eric Burns, Louisiana State University
Michael L. Cherry, Louisiana State University
Leonardo Di Venere, Istituto Nazionale di Fisica Nucleare, Sezione di Bari
Jeffrey Dumonthier, NASA Goddard Space Flight Center
Manel Errando, McDonnell Center for the Space Sciences
Stefan Funk, Friedrich-Alexander-Universität Erlangen-Nürnberg
Priya Ghosh, The Catholic University of America
Francesco Giordano, Politecnico di Bari
Jonah Hoffman, McDonnell Center for the Space Sciences
Zachary Hughes, McDonnell Center for the Space Sciences
Aera Jung, University of Hawaiʻi at Mānoa
Patrick L. Kelly, College of Science and Engineering
John F. Krizmanic, NASA Goddard Space Flight Center
Makiko Kuwahara, UH College of Engineering
Francesco Licciulli, Istituto Nazionale di Fisica Nucleare, Sezione di Bari
Gang Liu, SLAC National Accelerator Laboratory
Leonarda Lorusso, Politecnico di Bari
Mario Nicola Mazziotta, Istituto Nazionale di Fisica Nucleare, Sezione di Bari
John Grant Mitchell, National Aeronautics and Space Administration
John W. Mitchell, National Aeronautics and Space Administration

Document Type

Conference Proceeding

Publication Date

9-27-2024

Abstract

We characterize the performance of our computational pipeline for real-time gamma-ray burst (GRB) detection and localization aboard the Advanced Particle-astrophysics Telescope (APT) – a space-based observatory for MeV to TeV gamma-ray astronomy – and its smaller, balloon-borne prototype, the Antarctic Demonstrator for APT (ADAPT), whose scientific focus will be the detection of MeV transients. These instruments observe scintillation light from multiple Compton scattering and photoabsorption of gamma-ray photons across a series of CsI detector layers. We infer the incident angle of each photon’s first scattering to localize its source direction to a Compton ring about the vector defined by its first two interactions, then intersect rings from multiple photons to identify the GRB’s source direction. We first describe algorithmic improvements that enhance localization accuracy (measured in our previous GEANT4 model of APT) while running in under 0.5 seconds on a low-power ARMv8 processor – fast enough to permit real-time redirection of other instruments for follow-up observations. We then study our pipeline’s behavior using a model of the smaller ADAPT detector that incorporates realistic estimates of instrument noise and atmospheric background radiation. Adding SiPM-based edge detectors, which gather more light from each scintillation, greatly benefits ADAPT’s localization accuracy. We expect that ADAPT can localize normally-incident GRBs of fluence 1 MeV/cm2 and 1-second duration to within 2-3 degrees at least 68% of the time. The full APT instrument, with its larger detector area and lack of atmospheric background, should be substantially more accurate even on GRBs of fluence as low as 0.1 MeV/cm2

Publication Source (Journal or Book title)

Proceedings of Science

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