The Optical Afterglow of GRB 020305

Details The Optical Afterglow of GRB 020305 The Optical Afterglow of GRB 020305

Sep 2004

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2004aipc..727..537g&link_type=abstract

GAMMA-RAY BURSTS: 30 YEARS OF DISCOVERY: Gamma-Ray Burst Symposium. AIP Conference Proceedings, Volume 727, pp. 537-540 (2004).

Computer Science

Gamma-Ray Sources, Gamma-Ray Bursts, Supernovae, Photography And Photometry

Scientific paper

We report ground-based and HST(+STIS) imaging of the GRB 020305 optical afterglow. The light curve and the spectral energy distribution of the afterglow might show evidence of a supernova (SN) component present ~ 15 days after the GRB, which could be explained by a nearby Ic SN. However, a SN 1998bw-like template does not yield a completely satisfactory simultaneous fit to the SED and the lightcurve. We discuss some possible reasons for this behaviour.

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