Radio Transients: An antediluvian review

TL;DR

This review discusses the current state and future prospects of radio transient studies, emphasizing the potential for massive new transient detections with upcoming advanced radio telescopes like the Square Kilometre Array.

Contribution

It synthesizes existing knowledge of radio transient populations and projects future detection rates with next-generation arrays, highlighting the scientific opportunities ahead.

Findings

Current surveys have identified numerous radio transients with unclear origins.

Next-generation arrays could detect up to 10^5 transients annually.

The field is poised for rapid growth with new facilities.

Abstract

We are at the dawn of a new golden age for radio astronomy, with a new generation of facilities under construction and the global community focussed on the Square Kilometre Array as its goal for the next decade. These new facilities offer orders of magnitude improvements in survey speed compared to existing radio telescopes and arrays. Furthermore, the study of transient and variable radio sources, and what they can tell us about the extremes of astrophysics as well as the state of the diffuse intervening media, have been embraced as key science projects for these new facilities. In this paper we review the studies of the populations of radio transients made to date, largely based upon archival surveys. Many of these radio transients and variables have been found in the image plane, and their astrophysical origin remains unclear. We take this population and combine it with sensitivity estimates for the next generation arrays to demonstrate that in the coming decade we may find ourselves detecting 10^5 image plane radio transients per year, providing a vast and rich field of research and an almost limitless set of targets for multiwavelength follow up.