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Work: GRB Radiative Efficiencies Derived from the<i>Swift</i>Data: GRBs versus XRFs, Long versus Short

  1. THE AFTERGLOWS OF<i>SWIFT</i>-ERA GAMMA-RAY BURSTS. I. COMPARING PRE-<i>SWIFT</i>AND<i>SWIFT</i>-ERA LONG/SOFT (TYPE II) GRB OPTICAL AFTERGLOWS

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  2. Multicolour modelling of SN 2013dx associated with GRB 130702A★

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  3. The central engine of GRB 130831A and the energy breakdown of a relativistic explosion

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  4. GRB 051008: a long, spectrally hard dust-obscured GRB in a Lyman-break galaxy at z ≈ 2.8★

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