X-rays: individual: GRB 050820A GRB 050904 GRB 060418 GRB 070125 GRB 080319B

The Collimation and Energetics of the Brightest Swift Gamma-ray Bursts

Long-duration gamma-ray bursts (GRBs) are widely believed to be highly collimated explosions (bipolar conical outflows with half- opening angle þeta≈ 1°-10°). As a result of this beaming factor, the true energy release from a GRB is usually several …