3FGL J1924.8-1034 : A Spatially-Extended Stable Unidentified GeV Source?
arXiv:1611.05565 · doi:10.1103/PhysRevD.95.102001
Abstract
Milky Way-like galaxies are predicted to host a very large number of dark matter subhalos. Some massive and nearby subhalos could generate detectable gamma-rays, appearing as unidentified, spatially-extended and stable gamma-ray sources. We search for such sources in the third Fermi Large Area Telescope source List (3FGL) and report the identification of a new candidate, 3FGL J1924.8-1034. With the Fermi-LAT Pass 8 data, we find that 3FGL J1924.8-1034 is spatially-extended at a high confidence level of , with a best-fit extension radius of . No significant variability has been found and its gamma-ray spectrum is well fitted by the dark matter annihilation into with a mass of GeV. All these facts make 3FGL J1924.8-1034 a possible dark matter subhalo candidate. However, due to the limited angular resolution, the possibility of that the spatial extension of 3FGL J1924.8-1034 is caused by the contamination from the other un-resolved point source can not be ruled out.
10 pages including 5 figures and 1 table, accepted for publication in Phys. Rev. D
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