D. Watson

4 ta ish

Dark Cosmology Centre, Niels Bohr Institute, University of Copenhagen, Juliane Maries Vej 30, DK-2100 København Ø, Denmark

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

   Д. А. Канн, S. Klose, Bing Zhang +73

   MaqolaGamma-ray bursts and supernovaeThe Astrophysical Journal20106 iqtibos

   ABIABI:AkademIndex/openalex/2010.article.000002

2. A log <i>N</i>_{H <scp>i</scp>}= 22.6 Damped Lyα Absorber in a Dark Gamma‐Ray Burst: The Environment of GRB 050401

   D. Watson, J. P. U. Fynbo, C. Ledoux +33

   MaqolaGamma-ray bursts and supernovaeThe Astrophysical Journal20064 iqtibos

   ABIABI:AkademIndex/openalex/2026.other.006208

3. The nature of the X-ray flash of August 24 2005

   J. Sollerman, J. P. U. Fynbo, J. Gorosabel +23

   MaqolaGamma-ray bursts and supernovaeAstronomy and Astrophysics20071 iqtibos

   ABIABI:AkademIndex/openalex/2026.other.006260

4. The nature of the X-ray flash of August 24 2005 Photometric evidence for an on-axis z = 0.83 burst with continuous energy injection and an associated supernova?

   J. Sollerman, J. P. U. Fynbo, J. Gorosabel +23

   MaqolaGamma-ray bursts and supernovaeFigshare20071 iqtibos

   ABIABI:AkademIndex/openalex/2026.other.006651