The Swift satellite lives up to its name, revealing cosmic explosions as they happen

TL;DR

The Swift satellite has significantly advanced our understanding of Gamma-ray Bursts by providing rapid, detailed observations of these powerful cosmic explosions across the electromagnetic spectrum, revealing new insights into their origins and host galaxies.

Contribution

This paper summarizes key discoveries made by the Swift satellite, highlighting its role in improving real-time detection and understanding of Gamma-ray Bursts.

Findings

Swift enables rapid detection of Gamma-ray Bursts.

New insights into the origins of Gamma-ray Bursts.

Identification of host galaxies for Gamma-ray Bursts.

Abstract

Gamma-ray Bursts are the most powerful objects in the Universe. Discovered in the 1960's as brief flashes of gamma-radiation, we now know they emit across the entire electromagnetic spectrum, are located in distant galaxies and comprise two distinct populations, one of which may originate in the deaths of massive stars. The launch of the Swift satellite in 2004 has brought a flurry of new discoveries, advancing our understanding of these sources and the galaxies that host them. We highlight a number of important results from the Swift era thus far.