posted on 2012-10-24, 09:05authored byDe Ugarte Postigo A, A. J. Castro-Tirado, J. Gorosabel, S. Guzyi, M. Jelínek, G. Jóhannesson, G. Björnsson, E. H. Gudmundsson, M. Bremer, S. Pak, N. Tanvir, J. M. C. Cerón, S. Klose, D. Pérez-Ramírez, J. Aceituno, N. Cardiel, U. Thiele, A. C. Bagatín, S. Covino, D. Malesani, G. Ghisellini, M. Stefanon, T. Fathkullin, V. Sokolov, A. A. Henden, S. Huferath, L. Wisotzki, Y. Kurata, F. Mannucci, L. Hunt, P. Ruiz-Lapuente, L. A. Antonelli, Di Paola A, V. Testa, C. Bartolini, A. Guarnieri, A. Piccioni, A. Boattini, G. Pizzichini, N. Masetti, E. Palazzi, Del Principe M, D. Fugazza, T. Konstantinova, E. Pian, P. J. Tristram
GRB 021004 is one of the best sampled gamma-ray bursts (GRB) to date, although the nature of its light curve is still being debated. Here we present 107 new optical, near-infrared (NIR) and millimetre observations, ranging from 2 h to more than a year after the burst. Fitting the multiband data to a model based on multiple energy injections suggests that at least 7 refreshed shocks took place during the evolution of the afterglow, implying a total energy release (collimated within an angle of 1$\fdg$8) of ~ $8 \times 10^{51}$ erg. Analysis of the late photometry reveals that the GRB 021004 host is a low extinction ( $A_{\rm V}\sim0.1$) starburst galaxy with $M_{B}\simeq-22.0$.
History
Citation
Astronomy & Astrophysics, 2005, 443 (3), pp. 841-849
Version
VoR (Version of Record)
Published in
Astronomy & Astrophysics
Publisher
EDP Sciences for European Southern Observatory (ESO)