Transient astronomy will take another leap forward with the wide-field samples from LSST and WFIRST. It is imperative that we plan for ultraviolet capabilities to maximize our understanding of these explosions, their use as cosmological probes, and for comparisons with high redshift supernovae in the early universe.
The full text of this article is only available in PDF format:
Creative Commons Attribution 4.0 International License (CC-BY 4.0)
