Article ID | Journal | Published Year | Pages | File Type |
---|---|---|---|---|
8175760 | Nuclear Instruments and Methods in Physics Research Section A: Accelerators, Spectrometers, Detectors and Associated Equipment | 2014 | 4 Pages |
Abstract
The Fermi Large Area Telescope (LAT) has been exploring the high-energy γ-ray sky since its launch on June 11, 2008. After 5 years of essentially flawless operations, the LAT collected more than 800 million γ rays from 20 MeV to more than 300 GeV. With its uniform coverage of the sky, the LAT allowed the first high statistics observations of γ-ray sources of known classes as well as the discovery of new emitters. The LAT also allowed a detailed study of the diffuse γ-ray emission, which constitutes roughly 90% of the LAT photons, and constrains cosmic-ray production and propagation in our own Galaxy. In this talk I will review the status and the performance of the LAT and describe some of the most important scientific results.
Keywords
Related Topics
Physical Sciences and Engineering
Physics and Astronomy
Instrumentation
Authors
Carmelo Sgrò, on behalf of the Fermi LAT collaboration on behalf of the Fermi LAT collaboration,