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A likely starburst galaxy (SBG), IRAS 13052-5711, which is the most distantSBG candidate discovered to date, was found by analyzing 14.4 years of datafrom the Fermi large-area telescope (Fermi-LAT). This SBG's significance levelis approximately 6.55$\sigma$ in the 0.1-500 GeV band. Its spatial position isclose to that of 4FGL J1308.9-5730, determined from the Fermi large telescopefourth-source Catalog (4FGL). Its power-law spectral index is approximately2.1, and its light curve (LC) for 14.4 years has no significant variability.These characteristics are highly similar to those of SBGs found in the past. Wecalculate the SBG's star formation rate (SFR) to be 29.38 $\rm M_{\odot}\yr^{-1}$, which is within the SFR range of SBGs found to date. Therefore, IRAS13052-5711 is considered to be a likely SBG. In addition, its 0.1-500 GeVluminosity is (3.28 $\pm$ 0.67) $\times 10^{42}\ \rm erg\ s^{-1}$, whichdeviates from the empirical relationship of the $\gamma$-ray luminosity and thetotal infrared luminosity.  We considered a hadronic model to explain the GeV spectrum of IRAS13052-5711.

Fermi-LAT detection of A new starburst galaxy candidate: IRAS 13052-5711