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gptkbp:instanceOf
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cosmic microwave background experiment
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gptkbp:country
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gptkb:United_States
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gptkbp:fieldOfStudy
|
gptkb:cosmology
astrophysics
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|
gptkbp:firstLight
|
2011
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gptkbp:fundedBy
|
gptkb:W._M._Keck_Foundation
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gptkbp:goal
|
measure polarization of the cosmic microwave background
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|
https://www.w3.org/2000/01/rdf-schema#label
|
Keck Array
|
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gptkbp:location
|
gptkb:South_Pole
|
|
gptkbp:namedAfter
|
gptkb:W._M._Keck_Foundation
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gptkbp:numberOfSatellites
|
5
|
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gptkbp:operatedBy
|
gptkb:California_Institute_of_Technology
gptkb:Harvard_University
gptkb:National_Institute_of_Standards_and_Technology
gptkb:Princeton_University
gptkb:Stanford_University
gptkb:University_of_California,_Berkeley
gptkb:University_of_Chicago
gptkb:University_of_Minnesota
|
|
gptkbp:predecessor
|
gptkb:BICEP_experiment
|
|
gptkbp:relatedTo
|
gptkb:SPTpol
gptkb:BICEP2
|
|
gptkbp:sensorType
|
transition-edge sensor bolometers
|
|
gptkbp:successor
|
gptkb:BICEP3
|
|
gptkbp:telescopeType
|
microwave telescope
|
|
gptkbp:wavelengthRange
|
95 GHz
150 GHz
220 GHz
|
|
gptkbp:bfsParent
|
gptkb:BICEP2
|
|
gptkbp:bfsLayer
|
6
|