The GRB/SN Connection: An Improved Spectral Flux Distribution for the Supernova Candidate Associated with GRB 970228

Details The GRB/SN Connection: An Improved Spectral Flux Distribution for the Supernova Candidate Associated with GRB 970228 The GRB/SN Connection: An Improved Spectral Flux Distribution for the Supernova Candidate Associated with GRB 970228

1999-11-15

arxiv.org/abs/astro-ph/9911282v1

Astronomy and Astrophysics

Astrophysics

To appear in Proc. of the 10th Annual October Astrophysics Conference in Maryland: Cosmic Explosions, 4 pages, LaTeX

Scientific paper

10.1063/1.1291722

We better determine the spectral flux distribution of the supernova candidate
associated with GRB 970228 by modeling the spectral flux distribution of the
host galaxy of this burst, fitting this model to measurements of the host
galaxy, and using the fitted model to better subtract out the contribution of
the host galaxy to measurements of the afterglow of this burst.

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