The Swift Gamma-Ray Burst Mission
Swift was launched at 17:16 GMT
on 20th November 2004
Status of Swift
Swift is part of NASA's medium explorer program, with the hardware
being developed by an international team from the United States, the United
Kingdom and Italy, with additional scientific involvement by France, Japan,
Germany, Denmark, Spain, and South Africa. It is the first multi-wavelength
observatory dedicated to the study of gamma-ray burst science. The main aims of the Swift mission are to:
- determine the origin of gamma-ray bursts
- classify gamma-ray bursts and search for new types
- determine how the blast-wave evolves and interacts with the surroundings
- use gamma-ray bursts to study the early Universe
- perform the first sensitive hard X-ray survey of the sky
How Swift operates
- Burst Alert Telescope triggers on GRB and calculates position to within 4-arc-min.
- Spacecraft autonomously slews to GRB position in 20-70 seconds.
- X-ray Telescope determines position to within ~5-arc-sec.
- UV/Optical Telescope images field and transmits finding chart to ground.
As described in the Instruments on-board Swift section, the Burst Alert Telescope is the instrument which detects elevated gamma-ray emission. The BAT has a large field of view, allowing it to detect elevated gamma-ray emission from a large portion of the sky at any one time.
After this initial detection, Swift slews rapidly and autonomously, re-pointing itself to bring the detected burst into the field of view of the sensitive narrow field instruments (XRT and UVOT), which then observe the afterglow. Swift will provide spectra and multi-wavelength light-curves for the duration of the afterglow and, where possible, distance determinations. This will enable the most comprehensive study of GRBs and their host galaxies to date.
Naming Convention
New sources discovered by Swift will be designated SWIFT JHHMM.m +/-
DDMM or SWIFT JHHMMSS.s +/- DDMMSS
Follow the links below to learn more about Swift and gamma-ray bursts themselves or read the NASA Swift fact-sheet.
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UK Swift Science Data Centre
Last updated 2010 March 15
Web page maintained by Kim Page ()
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