Evidence for isotropic emission in GRB991216
  The issue of the possible presence or absence of jets in GRBs is here re-examined for GRB991216. We compare and contrast our theoretically predicted afterglow luminosity in the 2-10 keV band for spherically symmetric versus jetted emission. At these wavelenghts the jetted emission can be excluded and data analysis confirms spherical symmetry. These theoretical fits are expected to be improved by the forthcoming data of the Swift mission. 
Remo Ruffini, Maria Grazia Bernardini, Carlo Luciano Bianco, Pascal   Chardonnet, Federico Fraschetti, She-Sheng Xue