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A new $\gamma$-ray source with a significance level of approximately5$\sigma$ was reported in the region of SNR G272.2-3.2, analysing theapproximately 12.4 years of observation data from the Fermi Large AreaTelescope (Fermi-LAT). Its $\gamma$-ray spatial distribution did not showextended feature, and it had a soft spectrum with the spectral index of2.56$\pm$0.01 of a power-law model. No significant variability of its lightcurve (LC) with 10 time bins was identified, and its spatial positions in theX-ray and GeV bands overlapped. We suggest that the new $\gamma$-ray source isa likely counterpart of SNR G272.2-3.2. Analysing its spectrum, we discussedthe likely origins of the $\gamma$-ray emission.

Fermi-LAT detection of GeV $\gamma$-ray emission from Type Ia supernova remnant G272.2-3.2