Swift: the science across the rainbow. Mission Overview and Highlights of Results

TL;DR

The Swift mission, launched in 2004, has been highly successful in detecting and observing energetic astrophysical phenomena like gamma-ray bursts and other transient events, with excellent system performance over six years.

Contribution

This paper provides a comprehensive overview of the Swift mission's operations, performance, and scientific highlights across multiple astrophysical phenomena.

Findings

High operational efficiency with 97% burst chasing mode

Diverse scientific targets including GRBs, supernovae, and active galactic nuclei

Consistent system performance over six years

Abstract

I present an overview of the Swift mission, which was launched on November 20, 2004 to discover and observe the most energetic of astrophysical phenomena, gamma-ray bursts (GRBs). After almost 6 years in space the Observatory is in excellent shape, with all systems and instruments performing nominally and in burst chasing mode for an average of 97% of the time. Swift is also a multi-purpose multi-frequency mission with the observing time evolving from mostly GRB targets, to mainly secondary science ones such as supernovae, cataclysmic variables and novae, active galactic nuclei, Galactic transients, active stars and comets. I present the most recent science highlights.