VISTA Kilo-degree Infrared Galaxy survey

E668399

The VISTA Kilo-degree Infrared Galaxy survey (VIKING) is a wide-area near-infrared astronomical survey mapping large regions of the sky to study galaxy evolution, large-scale structure, and cosmology.

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Statements (47)

Predicate Object
instanceOf astronomical survey
galaxy survey
near-infrared sky survey
abbreviation VIKING
band H band
J band
Ks band
Y band
Z band
complementsSurvey KiDS
Kilo-Degree Survey
optical surveys
dataAccess ESO Science Archive
dataProduct imaging
dataReleaseType public survey
dataType photometric
enablesStudy galaxy clustering as function of redshift
galaxy luminosity functions
large-scale structure tomography
mass-to-light ratios of galaxies
photometric redshifts
stellar population synthesis in galaxies
weak gravitational lensing support
hostGalaxyType extragalactic fields
instrumentFullName VISTA InfraRed CAMera
linked to: VIRCAM
observatoryLocation Paranal Observatory
observatoryOperator European Southern Observatory
primaryScienceGoal cosmology studies
study galaxy evolution
study large-scale structure of the Universe
scienceCase constrain cosmological parameters
constrain dark energy
identify high-redshift quasars
measure galaxy clustering
study galaxy star-formation histories
study galaxy stellar masses
skyCoverage wide-area
skyCoverageUnit square degrees
surveyType multi-band imaging survey
targetPopulation Milky Way stars
galaxies
high-redshift galaxies
quasars
telescopeFullName Visible and Infrared Survey Telescope for Astronomy
linked to: VISTA telescope
usesInstrument VIRCAM
usesTelescope VISTA telescope
wavelengthRange near-infrared

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Referenced by (4)

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

VISTA supportsSurvey VISTA Kilo-degree Infrared Galaxy survey
VISTA telescope associatedSurvey VISTA Kilo-degree Infrared Galaxy Survey
linked to: VISTA Kilo-degree Infrared Galaxy survey
VIRCAM usedFor VISTA Kilo-degree Infrared Galaxy survey
VISTA Hemisphere Survey relatedSurvey VISTA Kilo-degree Infrared Galaxy survey