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The Optical/Near‐Infrared Light Curves of SN 2002ap for the First 1.5 Years after Discovery

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Predicting the Presence of Companions for Stripped-envelope Supernovae: The Case of the Broad-lined Type Ic SN 2002ap

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RELATIVISTIC SUPERNOVAE HAVE SHORTER-LIVED CENTRAL ENGINES OR MORE EXTENDED PROGENITORS: THE CASE OF SN 2012ap

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Modeling the Radio and X-ray Emission of SN 1993J and SN 2002ap

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Jets in Hydrogen-poor Superluminous Supernovae: Constraints from a Comprehensive Analysis of Radio Observations

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FUNDAMENTAL PHYSICS FROM BLACK HOLES, NEUTRON STARS AND GAMMA-RAY BURSTS

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