Thone, C. C.Kann, D. A.Johannesson, G.Selj, J. H.Jaunsen, A. O.Fynbo, J. P. U.Akerlof, C. W.Baliyan, K. S.Fruchter, A. S.Ibrahimov, MansurYuan, FangGraham, J. F.2015-12-130004-6361http://hdl.handle.net/1885/79575Aims: 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, consistingKeywords: Absorption lines; Analytical model; Broad bands; Broken power law; Central engines; Column density; Curve-of-growth; Data points; Data sets; Energy distributions; Energy injection; Galaxies:high-redshift; Gamma ray bursts; gamma rays bursts: individual: G galaxies: high-redshift; gamma rays bursts: individual: GRB 060526; ISM: abundances201010.1051/0004-6361/2008103402016-02-24