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The LAT Low-Energy technique for Fermi Gamma-Ray Bursts spectral analysis
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Fermi Large Area Telescope (LAT) data analyses based on event reconstruction and classification are so far restricted to events of measured energy larger than 100 MeV. We present a new technique to recover the signal from Gamma-Ray Bursts' (GRB) prompt emission between ~30 MeV and 100 MeV, which differs from the standard LAT analysis. Filling the gap between the energy ranges where the Gamma-ray Burst Monitor (GBM) and LAT operate is important to better constrain the high-energy spectra of GRBs. The LAT Low-Energy (LLE) technique is described, first performance studies are presented, as well as preliminary spectral re-analyses of two Fermi GRBs.
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Cited by 2 Pith papers
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Lorentz Factor Evolution of an Expanding Jet Shell Observed in Gamma-ray Burst: Case study of GRB 160625B
The Lorentz factor of the GRB 160625B jet shell stays almost constant during the expansion of a single pulse, pointing to a weakly magnetized emission region.
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Gamma-ray burst prompt emission spectra at high energies
Using Fermi data for 35 GRBs, the authors report that the 10 keV to GeV prompt spectra of most bursts are well described by synchrotron emission with an electron index clustering near p=2.7.
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