What is it about?
A comprehensive, up-to-date review of the observational and physical properties of gamma-ray burst supernovae.
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Why is it important?
It is the most up-to-date review of GRB-SNe, and discusses and presents key facts of their general properties, as well as describing in details the key outliers in the general GRB-SN population. Many of their key physical processes as determined via observations are thoroughly reviewed.
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This page is a summary of: The Observer’s Guide to the Gamma-Ray Burst Supernova Connection, Advances in Astronomy, January 2017, Hindawi Publishing Corporation,
DOI: 10.1155/2017/8929054.
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