Photometry and spectroscopy of GRB 060526: A detailed study of the afterglow and host galaxy of a z = 3.2 gamma-ray burst
Aims: With this paper we want to investigate the highly variable afterglow light curve and environment of gamma-ray burst (GRB) 060526 at z = 3.221. Methods: We present one of the largest photometric datasets ever obtained for a GRB afterglow, consisting
|Collections||ANU Research Publications|
|Source:||Astronomy and Astrophysics|
|01_Thone_Photometry_and_spectroscopy_of_2010.pdf||1.35 MB||Adobe PDF||Request a copy|
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