The Swift Gamma-Ray Burst Mission

Bibcode
2004AIPC..727..637G
DOI
10.1063/1.1810924
Gehrels, N.
Bibliographical reference

GAMMA-RAY BURSTS: 30 YEARS OF DISCOVERY: Gamma-Ray Burst Symposium. AIP Conference Proceedings, Volume 727, pp. 637-641 (2004).

Advertised on:
9
2004
Number of authors
1
IAC number of authors
0
Citations
36
Refereed citations
34
Description
Swift is a first-of-its-kind multiwavelength transient observatory for GRB astronomy. It has the optimum capabilities for the next breakthroughs in determining the origin of GRBs and their afterglows, as well as using bursts to probe the early Universe. Swift will also perform the first sensitive hard X-ray survey of the sky. The mission is being developed by an international collaboration and consists of three instruments, the Burst Alert Telescope (BAT), the X-ray Telescope (XRT), and the Ultraviolet and Optical Telescope (UVOT). The BAT, a wide-field gamma-ray detector, will detect > 100 GRBs per year with a sensitivity >2 times that of BATSE. The sensitive narrow-field XRT and UVOT will be autonomously slewed to the burst location in 20 to 75 seconds to determine 0.3-5.0 arcsec positions and perform optical, UV, and X-ray spectrophotometry. Strong education/public outreach and follow-up programs will help to engage the public and astronomical community. The Swift launch is planned for mid 2004.
Type
Non-refereed
Gamma-ray sources
Gamma-ray bursts
Sky surveys
X-ray sources
X-ray bursts

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