BAT

E1027633

BAT is a high-energy astrophysics instrument designed to rapidly detect and locate gamma-ray bursts in space.

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Statements (46)

Predicate Object
instanceOf coded-aperture mask telescope
gamma-ray detector
space telescope instrument
abbreviation CZT
acronymFor Burst Alert Telescope NERFINISHED
alertSystem rapid GRB alert dissemination to ground
dataProducts light curves
source catalogs
spectra
detectionMethod coded mask imaging
scintillation detection
detectorArrayArea_cm2 5200
detectorMaterial cadmium zinc telluride
energyRangeLowerBound_keV 15
energyRangeUpperBound_keV 150
fieldOfView approximately one-sixth of the sky
fieldOfViewType wide field of view
fullName Burst Alert Telescope NERFINISHED
launchDate 2004-11-20
launchedWith Swift spacecraft NERFINISHED
launchVehicle Delta II rocket NERFINISHED
localizationAccuracy_arcmin 1–4
missionType high-energy astrophysics
numberOfDetectors 32768
observes gamma-ray bursts
hard X-ray sources
soft gamma-ray sources
onboardProcessing automatic burst localization
real-time burst detection algorithms
operator NASA
partOf Neil Gehrels Swift Observatory NERFINISHED
primaryScienceGoal detection of gamma-ray bursts
localization of gamma-ray bursts
provides burst sky positions
burst trigger times
hard X-ray survey data
scientificContribution constraints on GRB rates and luminosity functions
discovery of many new hard X-ray sources
study of GRB prompt emission
spaceAgency NASA
spacecraftBus Swift observatory bus
supports multiwavelength follow-up observations
surveyCapability all-sky hard X-ray survey
timeResolution milliseconds
triggers Swift UV/Optical Telescope repointing
Swift X-Ray Telescope repointing

Referenced by (1)

Full triples — surface form annotated when it differs from this entity's canonical label.