6M.Amenomori,Z.Cao.L.K.Ding,Z.Y.Feng,K.Hibino,N.Hotta,Q.Huang,A.X.Huo,H.Y.Jia,G.Z.Jiang,S.Q.Jiao,F.Kajino,K.Kasahara,Labaciren,D.M.Mei,L.Meng,X.R.Meng,Mimaeiren,K.Mizutani,J.Mu,H.Nanjo,M.Nishizawa,Nusang,A.Oguro,M.Ohnishi,I.Ohta,J.R.Ren,To.saito,M.Sakata,Z.Z.Shi,M.Shibata,T.shirai,H.sugimoto,X.X.Sun,A.Tai,K.Taira,Y.H.Tan,N.Tateyama,S.Torii,H.Wang,C.Z.Wen,Y.Yamamoto,X.Y.Yao,G.C.Yu,P.Yuan,T.Yuda,J.G.Zeng,C.S.Zhang,H.M.Zhang,L.Zhang,Zhasang,Zhaxlclren,W.D.Zhou.Search for Steady Emission of 10—TeV Gamma Rays from the Crab Nebula,Cygnus X—3,and Hercules X—1 Using the Tibet Air Shower Array[J].西藏大学学报(社会科学版),1993,8(4):71-75.
