Swift BAT

E1027634

Swift BAT is a highly sensitive gamma-ray telescope aboard NASA’s Swift satellite, designed to detect and locate cosmic gamma-ray bursts.

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Statements (44)

Predicate Object
instanceOf coded-aperture mask telescope
gamma-ray telescope
space telescope instrument
acronym BAT NERFINISHED
alertsDistributedVia Gamma-ray Coordinates Network NERFINISHED
dataProduct gamma-ray burst light curves
gamma-ray burst spectra
hard X-ray source catalogs
designedBy NASA Goddard Space Flight Center and collaborators NERFINISHED
energyRange 15–150 keV
fieldOfView approximately one-sixth of the sky
fieldOfViewType wide field of view
fullName Burst Alert Telescope NERFINISHED
hasDetectorArea about 5200 square centimeters
hasDetectorMaterial CdZnTe
hasDetectorType cadmium zinc telluride detector
hasMaskType random-pattern coded mask
launchDate 2004-11-20
launchSite Cape Canaveral Air Force Station NERFINISHED
launchVehicle Delta II 7320-10C NERFINISHED
missionRole detection of gamma-ray bursts
localization of gamma-ray bursts
observes gamma rays
gamma-ray bursts
onboardSpacecraft Swift Gamma-Ray Burst Explorer NERFINISHED
operator NASA
partOf Swift satellite
performs all-sky hard X-ray survey
primaryFunction onboard burst localization
rapid burst detection
provides burst positions to ground in near real time
providesLocalizationAccuracy arcminute scale positions for gamma-ray bursts
scientificObjective study of prompt emission of gamma-ray bursts
survey of hard X-ray and soft gamma-ray sky
sensitivity high sensitivity to transient gamma-ray events
spacecraftFrame low Earth orbit via Swift satellite
supportsScience multiwavelength follow-up of gamma-ray bursts
studies of X-ray binaries in hard X-rays
studies of active galactic nuclei in hard X-rays
triggers Swift UVOT follow-up observations
Swift XRT follow-up observations
uses coded-aperture mask imaging
wavelengthBand hard X-ray
soft gamma-ray

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