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arXiv · 2609.02809

17 Yr of Magnetar Bursts Observed with the Fermi Gamma-ray Burst Monitor

Matt Godwin·Özge Keskin·Mustafa Demirer·Yi-Jing Yi·Lin Lin·Oliver J. Roberts·Ersin Göğüş·Yuki Kaneko·Michael Briggs·Matthew G. Baring·Eric Burns·David M. Palmer·Boyan A. Hristov·Bagrat Mailyan·Christian Malacaria·Eva Palafox·Chryssa Kouveliotou·Alexander J. van der Horst·Peter Veres·George Younes
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Abstract

The Fermi Gamma-ray Burst Monitor (GBM) has been in operation for over 17 years, during which it has observed more than a thousand bursts from soft gamma repeaters (SGRs), also known as magnetars. Serving as a laboratory for extreme physics, magnetars are a sub-family of neutron stars characterized by extreme magnetic field strength, observed through a combination of persistent and short transient emission across the electromagnetic spectrum. We present the comprehensive GBM catalog of SGR short bursts which supersedes the 5-year catalog of Collazzi et al. 2015. The new catalog contains 1254 SGR short bursts observed over 17 years, providing the longest uninterrupted, high-sensitivity all-sky monitoring of magnetar bursts with unprecedented spectral and temporal resolution. Our catalog contains bursts from 17 unique Galactic sources, with major contributions by bursts from SGR J1935+2154 and SGR J1550-5418. We present overall characteristics of these bursts, such as the durations, spectral parameters for various photon models, fluxes, as well as their comparison with recently published catalogs of other missions and the previous GBM magnetar catalog. The machine readable catalog, as well as burst spectra and response files are made publicly available for the community.

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Matt Godwin, Özge Keskin, Mustafa Demirer, Yi-Jing Yi, Lin Lin, Oliver J. Roberts, Ersin Göğüş, Yuki Kaneko, Michael Briggs, Matthew G. Baring, Eric Burns, David M. Palmer, Boyan A. Hristov, Bagrat Mailyan, Christian Malacaria, Eva Palafox, Chryssa Kouveliotou, Alexander J. van der Horst, Peter Veres, George Younes. 2026-09-02. 17 Yr of Magnetar Bursts Observed with the Fermi Gamma-ray Burst Monitor. https://doi.org/10.3847/1538-4365%2Fae9904

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