\emph{Fermi}-LAT Detection of the Young SuperNova Remnant Tycho
Aug, 2011Citations per year
Abstract: (arXiv)
After almost three years of data taking in sky survey mode, the \emph{Fermi}-LAT has detected γ-ray emission toward the Tycho's Supernova Remnant (SNR). The Tycho SNR is among the youngest remnants in the Galaxy, originating from a Type Ia Supernova in AD 1572. The γ-ray integral flux from 400 MeV up to 100 GeV has been measured to be (3.5±1.1stat±0.7syst)×10−9 cm−2s−1 with a photon index of 2.3±0.2stat±0.1syst.References(23)
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