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Swift Discovery of Gamma-Ray Bursts without Jet Break Feature in their X-Ray Afterglows

We analyze Swift gamma-ray bursts (GRBs) and X-ray afterglows for three GRBs with spectroscopic redshift determinations -- GRB 050401, XRF 050416a, and GRB 050525a. We find that the relation between spectral peak energy and isotropic energy of prompt emiss

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aAcceptedforpublicationinApJSwiftDiscoveryofGamma-rayBurstswithoutJetBreakFeatureintheirX-rayAfterglowsG.Sato1,2,R.Yamazaki3,K.Ioka4,T.Sakamoto1,5,T.Takahashi2,6,K.Nakazawa2,T.Nakamura4,K.Toma4,D.Hullinger1,7,8,M.Tashiro9,A.M.Parsons1,H.A.Krimm1,10,S.D.Barthelmy1,N.Gehrels1,D.N.Burrows11,P.T.O’Brien12,J.P.Osborne12,G.Chincarini13,14,andD.Q.Lamb15ABSTRACTWeanalyzeSwiftgamma-raybursts(GRBs)andX-rayafterglowsforthreeGRBswithspectroscopicredshiftdeterminations—GRB050401,XRF050416a,andGRB050525a.We ndthattherelationbetweenspectralpeakenergyandisotropicenergyofpromptemissions(theAmatirelation)isconsistentwiththatfortheburstsobservedinpre-Swiftera.However,we ndthattheX-rayafterglow

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