How Swift is Redefining Time Domain Astronomy
Abstract
NASA's Swift satellite has completed ten years of amazing discoveries in time domain astronomy. Its primary mission is to chase gamma-ray bursts (GRBs), but due to its scheduling flexibility it has subsequently become a prime discovery machine for new types of behavior. The list of major discoveries in GRBs and other transients includes the long-lived X-ray afterglows and flares from GRBs, the first accurate localization of short GRBs, the discovery of GRBs at high redshift (z>8), supernova shock break-out from SN Ib, a jetted tidal disruption event, an ultra-long class of GRBs, high energy emission from flare stars, novae and supernovae with unusual characteristics, magnetars with glitches in their spin periods, and a short GRB with evidence of an accompanying kilonova. Swift has developed a dynamic synergism with ground based observatories. In a few years gravitational wave observatories will come on-line and provide exciting new transient sources for Swift to study.
Cite
@article{arxiv.1502.03064,
title = {How Swift is Redefining Time Domain Astronomy},
author = {Neil Gehrels and John K. Cannizzo},
journal= {arXiv preprint arXiv:1502.03064},
year = {2015}
}
Comments
14 pages, 14 figures, accepted into the Journal of High Energy Astrophysics for the dedicated issue: "Swift: Ten Years of Discovery" (revised version with additional text & references)