HAWK-I

E176897

HAWK-I is a high-sensitivity near-infrared wide-field imaging camera used for astronomical observations on the European Southern Observatory’s Very Large Telescope.

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Label Occurrences
HAWK-I canonical 1

Statements (48)

Predicate Object
instanceOf astronomical instrument
near-infrared camera
wide-field imager
bandCoverage H band
J band
K band
Y band
country Chile
detectorType infrared detector array
fieldOfView wide field
fullName High Acuity Wide field K-band Imager
hostFacility Very Large Telescope
surface form: Very Large Telescope array
locatedAt Paranal Observatory
mountedOn Very Large Telescope
observatorySite Paranal Observatory
surface form: Cerro Paranal
observingMode imaging
operatedBy European Southern Observatory
operationalStatus in operation
organization European Southern Observatory
partOf VLT instrumentation suite
primaryUse astronomical imaging
deep sky surveys
extragalactic astronomy
galaxy evolution studies
high-redshift galaxy observations
star formation studies
stellar cluster observations
scienceCapability faint object detection
high spatial resolution imaging
wide-field near-infrared imaging
scienceGoal study of galaxy formation and evolution
study of stellar populations
study of the early universe
sensitivity high sensitivity
spectralRegion infrared
telescopeType 8.2-metre class telescope instrument
telescopeUnit Very Large Telescope
surface form: VLT Unit Telescope 4
telescopeUnitName Yepun
usedFor cosmological surveys
imaging of nearby galaxies
mapping of the Milky Way structure
observations of distant galaxies
observations of galaxy clusters
observations of star-forming regions
searches for high-redshift objects
studies of brown dwarfs
studies of variable stars
wavelengthRange near-infrared

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