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Gamma-Ray Burst Detection with Poisson-FOCuS and Other Trigger Algorithms

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Gamma-Ray Burst Detection with Poisson-FOCuS and Other Trigger Algorithms. / Dilillo, Giuseppe; Ward, Kes; Eckley, Idris A. et al.
In: The Astrophysical Journal, Vol. 962, No. 2, 137, 14.02.2024.

Research output: Contribution to Journal/MagazineJournal articlepeer-review

Harvard

Dilillo, G, Ward, K, Eckley, IA, Fearnhead, P, Crupi, R, Evangelista, Y, Vacchi, A & Fiore, F 2024, 'Gamma-Ray Burst Detection with Poisson-FOCuS and Other Trigger Algorithms', The Astrophysical Journal, vol. 962, no. 2, 137. https://doi.org/10.3847/1538-4357/ad15ff

APA

Dilillo, G., Ward, K., Eckley, I. A., Fearnhead, P., Crupi, R., Evangelista, Y., Vacchi, A., & Fiore, F. (2024). Gamma-Ray Burst Detection with Poisson-FOCuS and Other Trigger Algorithms. The Astrophysical Journal, 962(2), Article 137. https://doi.org/10.3847/1538-4357/ad15ff

Vancouver

Dilillo G, Ward K, Eckley IA, Fearnhead P, Crupi R, Evangelista Y et al. Gamma-Ray Burst Detection with Poisson-FOCuS and Other Trigger Algorithms. The Astrophysical Journal. 2024 Feb 14;962(2):137. doi: 10.3847/1538-4357/ad15ff

Author

Dilillo, Giuseppe ; Ward, Kes ; Eckley, Idris A. et al. / Gamma-Ray Burst Detection with Poisson-FOCuS and Other Trigger Algorithms. In: The Astrophysical Journal. 2024 ; Vol. 962, No. 2.

Bibtex

@article{13394149ca5f4451afe422034c6954c0,
title = "Gamma-Ray Burst Detection with Poisson-FOCuS and Other Trigger Algorithms",
abstract = "We describe how a novel online change-point detection algorithm, called Poisson-FOCuS, can be used to optimally detect gamma-ray bursts within the computational constraints imposed by miniaturized satellites such as the upcoming HERMES-Pathfinder constellation. Poisson-FOCuS enables testing for gamma-ray burst onset at all intervals in a count time series, across all timescales and offsets, in real time and at a fraction of the computational cost of conventional strategies. We validate an implementation with automatic background assessment through exponential smoothing, using archival data from Fermi-GBM. Through simulations of lightcurves modeled after real short and long gamma-ray bursts, we demonstrate that the same implementation has higher detection power than algorithms designed to emulate the logic of Fermi-GBM and Compton-BATSE, reaching the performance of a brute-force benchmark with oracle information on the true background rate, when not hindered by automatic background assessment. Finally, using simulated data with different lengths and means, we show that Poisson-FOCuS can analyze data twice as fast as a similarly implemented benchmark emulator for the historic Fermi-GBM on-board trigger algorithms.",
keywords = "Transient detection, Algorithms, Artificial satellites, Astrostatistics techniques, Gamma-ray bursts",
author = "Giuseppe Dilillo and Kes Ward and Eckley, {Idris A.} and Paul Fearnhead and Riccardo Crupi and Yuri Evangelista and Andrea Vacchi and Fabrizio Fiore",
year = "2024",
month = feb,
day = "14",
doi = "10.3847/1538-4357/ad15ff",
language = "English",
volume = "962",
journal = "The Astrophysical Journal",
issn = "0004-637X",
publisher = "Institute of Physics Publishing",
number = "2",

}

RIS

TY - JOUR

T1 - Gamma-Ray Burst Detection with Poisson-FOCuS and Other Trigger Algorithms

AU - Dilillo, Giuseppe

AU - Ward, Kes

AU - Eckley, Idris A.

AU - Fearnhead, Paul

AU - Crupi, Riccardo

AU - Evangelista, Yuri

AU - Vacchi, Andrea

AU - Fiore, Fabrizio

PY - 2024/2/14

Y1 - 2024/2/14

N2 - We describe how a novel online change-point detection algorithm, called Poisson-FOCuS, can be used to optimally detect gamma-ray bursts within the computational constraints imposed by miniaturized satellites such as the upcoming HERMES-Pathfinder constellation. Poisson-FOCuS enables testing for gamma-ray burst onset at all intervals in a count time series, across all timescales and offsets, in real time and at a fraction of the computational cost of conventional strategies. We validate an implementation with automatic background assessment through exponential smoothing, using archival data from Fermi-GBM. Through simulations of lightcurves modeled after real short and long gamma-ray bursts, we demonstrate that the same implementation has higher detection power than algorithms designed to emulate the logic of Fermi-GBM and Compton-BATSE, reaching the performance of a brute-force benchmark with oracle information on the true background rate, when not hindered by automatic background assessment. Finally, using simulated data with different lengths and means, we show that Poisson-FOCuS can analyze data twice as fast as a similarly implemented benchmark emulator for the historic Fermi-GBM on-board trigger algorithms.

AB - We describe how a novel online change-point detection algorithm, called Poisson-FOCuS, can be used to optimally detect gamma-ray bursts within the computational constraints imposed by miniaturized satellites such as the upcoming HERMES-Pathfinder constellation. Poisson-FOCuS enables testing for gamma-ray burst onset at all intervals in a count time series, across all timescales and offsets, in real time and at a fraction of the computational cost of conventional strategies. We validate an implementation with automatic background assessment through exponential smoothing, using archival data from Fermi-GBM. Through simulations of lightcurves modeled after real short and long gamma-ray bursts, we demonstrate that the same implementation has higher detection power than algorithms designed to emulate the logic of Fermi-GBM and Compton-BATSE, reaching the performance of a brute-force benchmark with oracle information on the true background rate, when not hindered by automatic background assessment. Finally, using simulated data with different lengths and means, we show that Poisson-FOCuS can analyze data twice as fast as a similarly implemented benchmark emulator for the historic Fermi-GBM on-board trigger algorithms.

KW - Transient detection

KW - Algorithms

KW - Artificial satellites

KW - Astrostatistics techniques

KW - Gamma-ray bursts

U2 - 10.3847/1538-4357/ad15ff

DO - 10.3847/1538-4357/ad15ff

M3 - Journal article

VL - 962

JO - The Astrophysical Journal

JF - The Astrophysical Journal

SN - 0004-637X

IS - 2

M1 - 137

ER -