# Superluminous supernovae at high redshift

**Authors:** Tim Abbott, Jeff Cooke, Chris Curtin, Shahab Joudaki, Antonios, Katsianis, Anton Koekemoer, Jeremy Mould, Edoardo Tescari, Syed Uddin, Lifan, Wang

arXiv: 1702.02564 · 2017-08-23

## TL;DR

This paper reviews the discovery and potential mechanisms of superluminous supernovae observed at high redshifts, including during the epoch of reionization.

## Contribution

It provides a comprehensive overview of candidate mechanisms and discovery programs for high-redshift superluminous supernovae.

## Key findings

- Superluminous supernovae are observed at redshifts during reionization.
- Multiple mechanisms are proposed to explain their luminosity.
- Discovery programs are actively identifying these distant supernovae.

## Abstract

Superluminous supernovae are beginning to be discovered at redshifts as early as the epoch of reionization. A number of candidate mechanisms is reviewed, together with the discovery programs.

## Full text

_Full body text omitted from this summary view._ Fetch the complete paper as Markdown: https://tomesphere.com/paper/1702.02564/full.md

## Figures

5 figures with captions in the complete paper: https://tomesphere.com/paper/1702.02564/full.md

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Source: https://tomesphere.com/paper/1702.02564