Analysis of γ-ray emission above 30 GeV from the LMC pulsar wind nebula N 157B with <i>Fermi</i>-LAT
Yunlu Gong(Yunnan University), Jun Fang(Yunnan University), Liancheng Zhou(Yunnan University), Shiting Tian(Yunnan University), Yifan Xiao(Yunnan University)
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