Fermi-GBM Discovery of GRB 221009A: An Extraordinarily Bright GRB from Onset to Afterglow

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2303.14172.pdf (1.56 MB)

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https://arxiv.org/abs/2303.14172

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https://doi.org/10.48550/arXiv.2303.14172
 http://hdl.handle.net/11603/27628

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UMBC Physics Department
UMBC Center for Space Sciences and Technology (CSST) / Center for Research and Exploration in Space Sciences & Technology II (CRSST II)
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https://orcid.org/0000-0002-6548-5622

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2023-03-24

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journal articles
preprints
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"This work was written as part of one of the author's official duties as an Employee of the United States Government and is therefore a work of the United States Government. In accordance with 17 U.S.C. 105, no copyright protection is available for such works under U.S. Law. "
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Abstract

We report the discovery of GRB 221009A, the highest flux gamma-ray burst ever observed by the Fermi Gamma-ray Burst Monitor (Fermi-GBM). This GRB has continuous prompt emission lasting more than 600 seconds, afterglow visible in the Fermi-GBM energy range (8 keV–40 MeV), and total energetics higher than any other burst in the Fermi-GBM sample. By using a variety of new and existing analysis techniques we probe the spectral and temporal evolution of GRB 221009A. We find no emission prior to the Fermi-GBM trigger time (tₒ; 2022 October 9 at 13:16:59.99 UTC), indicating that this is the time of prompt emission onset. The triggering pulse exhibits distinct spectral and temporal properties suggestive of shock-breakout with significant emission up to ∼15 MeV. We characterize the onset of external shock at tₒ+600 s and find evidence of a plateau region in the early-afterglow phase which transitions to a slope consistent with Swift-XRT afterglow measurements. We place the total energetics of GRB 221009A in context with the rest of the Fermi-GBM sample and find that this GRB has the highest total isotropic-equivalent energy (Eγ,iso = 1.0 × 10⁵⁵ erg) and second highest isotropic-equivalent luminosity (Lγ,iso = 9.9×10⁵³ erg/s) based on redshift of z = 0.151. These extreme energetics are what allowed Fermi-GBM to observe the continuously emitting central engine from the beginning of the prompt emission phase through the onset of early afterglow.