Discovery of an extended source of gamma-ray emission in the Southern Hemisphere
arXiv:1609.06225 · doi:10.1093/mnras/stx2779
Abstract
We report the discovery of a $3.4\degr$-wide region of high-energy emission in data from the \emph{Fermi} LAT satellite. The centroid of the emission is located in the Southern Hemisphere sky, a few degrees away from the plane of the Galaxy at the Galactic coordinates l=350.6$\degr$, b=-4.7$\degr$. It shows a hard spectrum that is compatible with a simple power-law, , in the energy range 0.7--500 GeV, with a spectral index $Γ= 1.68 \pm 0.04_{\mbox{stat}} \pm 0.1_{\mbox{sys}}$. The integrated source photon flux above 0.7 GeV is $(4.71 \pm 0.49_{\mbox{stat}}\pm 2.13_{\mbox{sys}}) \times 10^{-9}$ cm s. We discuss several hypotheses for the nature of the source, particularly that the emission comes from the shell of an unknown supernova remnant.
MNRAS published online 2017 October
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