Discovery of GeV gamma-ray emission from the LMC B0443-6657 with the Fermi Large Area Telescope

We report the discovery of gamma-ray detection from the Large Magellanic Cloud (LMC) B0443-6657 using the Large Area Telescope (LAT) on board the $\mathit{\text{Fermi}}\mathit{\text{Gamma-ray}}\mathit{\text{Space}}\mathit{\text{Telescope}}$. LMC B0443-6657 is a flat spectrum radio source, possibly associated with a supernova remnant in the Large Magellanic Cloud (LMC N4). Employing the LAT data of 8 years, our results show a significant excess ($>9.4\sigma$) of gamma-ray in the range of 0.2–100,GeV above the gamma-ray background. A power-law function is found to be adequate to describe the $0.2-100$ GeV $\gamma$-ray spectrum, which yields a photon flux of $3.27\pm 0.53{\mathrm{p}\mathrm{h}\mathrm{o}\mathrm{t}\mathrm{o}\mathrm{n}\mathrm{c}\mathrm{m}}^2{\mathrm{s}}^{-1}$ with a photon index of $2.35\pm 0.11$, corresponding to an isotropic gamma-ray luminosity of $5.3\times {10}^{40}{\mathrm{e}\mathrm{r}\mathrm{g}\mathrm{s}}^{-1}$. The hadronic model predicts a low X-ray and TeV flux while the leptonic model predicts an observable flux in these two energy bands. The follow-up observations of the LMC B0443-6657 in X-ray or TeV band would distinguish the radiation models of gamma-rays from this region.