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2010ApJ...708L.112D - Astrophys. J., 708, L112-L115 (2010/January-2)
The anticipated supernova associated with GRB 090618.
DADO S. and DAR A.
Abstract (from CDS):
We use the cannonball model of gamma-ray bursts (GRBs) and public data from the first day of observations of GRB 090618 to predict its X-ray and optical light curves until very late times, and, in particular, the emergence of a photometric and spectroscopic signature of an SN akin to SN1998bw in its optical afterglow with an anticipated peak brightness of magnitude ∼23.2 in the R band around 2009 July 10, if extinction in the host galaxy can be neglected.
Abstract Copyright: ∼
Journal keyword(s): gamma rays: bursts - supernovae: general
Simbad objects: 3
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