High Acuity Wide field K-band Imager

E668454

High Acuity Wide field K-band Imager is a near-infrared wide-field camera installed on ESO’s Very Large Telescope, designed for high-resolution astronomical imaging in the K-band.

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Label Occurrences
High Acuity Wide field K-band Imager canonical 1

Statements (45)

Predicate Object
instanceOf astronomical instrument
near-infrared camera
telescope instrument
wide-field imager
abbreviation HAWK-I NERFINISHED
commissionedBy European Southern Observatory NERFINISHED
country Chile
detectorFormat 2048 x 2048 pixels
detectorType HgCdTe infrared array
environment cryogenic
fieldOfView approximately 7.5 arcminutes by 7.5 arcminutes
hasFilter broad-band near-infrared filters
narrow-band near-infrared filters
hostTelescope VLT UT4 (Yepun) NERFINISHED
hostTelescopeAperture 8.2-metre primary mirror
installedOn Unit Telescope 4 of the Very Large Telescope NERFINISHED
locatedAt Very Large Telescope NERFINISHED
locationRegion Atacama Desert NERFINISHED
numberOfDetectors 4
observatory Paranal Observatory NERFINISHED
observingMode imaging
operatedBy European Southern Observatory NERFINISHED
organization ESO NERFINISHED
pixelScale approximately 0.1 arcseconds per pixel
purpose to provide high acuity wide-field imaging in the K-band
scienceGoal cosmological deep fields
high-resolution imaging in the near-infrared
search for distant supernovae
study of high-redshift galaxies
study of star-forming regions
study of stellar clusters
study of the Galactic Centre
wide-field surveys in the K-band
scienceUse Galactic astronomy
extragalactic astronomy
planetary nebulae studies
star formation studies
stellar astrophysics
spectralBand H-band
J-band
K-band
telescopeSite Cerro Paranal Observatory NERFINISHED
usesTechnique dithering
near-infrared imaging
wavelengthBand near-infrared

Referenced by (1)

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

HAWK-I fullName High Acuity Wide field K-band Imager