Uncovering the Low Energy Emission of Fermi LAT Transients

Details Uncovering the Low Energy Emission of Fermi LAT Transients Uncovering the Low Energy Emission of Fermi LAT Transients

Jan 2012

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2012aas...21944208p&link_type=abstract

American Astronomical Society, AAS Meeting #219, #442.08

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Fermi Large Area Telescope (LAT) standard science analyses are restricted to well-reconstructed events, with energies above 100 MeV. Applying a less restrictive selection allows one to recover the high photon statistics between 30 MeV and 100 MeV in the prompt emission from Gamma-Ray Bursts (GRB) and Solar Flares (SFL), thus filling the gap between the Fermi Gamma-ray Burst Monitor (GBM) and the LAT in standard analysis mode. We present here results showing the power of this technique to extract both lightcurves and energy spectra of the transients in this energy range.

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