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Potential contribution from gamma-ray sources to the Galactic diffuse gammarays observed above 100 TeV (sub-PeV energy range) by the Tibet AS{\gamma}experiment is an important key to interpreting recent multi-messengerobservations. This paper reveals a surprising fact: none of the 23 TibetAS{\gamma} diffuse gamma-ray events above 398TeV within the Galacticlatitudinal range of |b| < 10 deg. come from the 43 sub-PeV gamma-ray sourcesreported in the 1LHAASO catalog, which proves that these sources are not theorigins of the Tibet AS{\gamma} diffuse gamma-ray events. No positional overlapbetween the Tibet AS{\gamma} diffuse gamma-ray events and the sub-PeV LHAASOsources currently supports the diffusive nature of the Tibet AS{\gamma} diffusegamma-ray events, although their potential origin in the gamma-ray sources yetunresolved in the sub-PeV energy range cannot be ruled out.

On the source contribution to the Galactic diffuse gamma rays above 398 TeV detected by the Tibet AS{\gamma} experiment