gptkbp:instanceOf
|
scientific research
|
gptkbp:aperture
|
26 cm
|
gptkbp:collaboratesWith
|
gptkb:Keck_Array
|
gptkbp:country
|
gptkb:United_States
|
gptkbp:endDate
|
2012
|
gptkbp:field
|
gptkb:cosmology
astrophysics
|
gptkbp:fundedBy
|
gptkb:National_Science_Foundation
|
gptkbp:goal
|
detect B-mode polarization
search for evidence of cosmic inflation
|
https://www.w3.org/2000/01/rdf-schema#label
|
BICEP2 experiment
|
gptkbp:location
|
gptkb:Amundsen–Scott_South_Pole_Station
|
gptkbp:notableAchievement
|
2014 announcement of B-mode polarization detection
results later attributed to galactic dust
|
gptkbp:operatedBy
|
gptkb:California_Institute_of_Technology
gptkb:Harvard_University
gptkb:Jet_Propulsion_Laboratory
gptkb:Stanford_University
|
gptkbp:predecessor
|
gptkb:BICEP_experiment
|
gptkbp:principalInvestigator
|
gptkb:John_Kovac
|
gptkbp:publishedIn
|
gptkb:Detection_of_B-Mode_Polarization_at_Degree_Angular_Scales_by_BICEP2_(2014)
|
gptkbp:researchInterest
|
cosmic microwave background polarization
|
gptkbp:startDate
|
2010
|
gptkbp:successor
|
gptkb:BICEP3_experiment
|
gptkbp:telescopeType
|
microwave telescope
|
gptkbp:wavelengthRange
|
150 GHz
|
gptkbp:website
|
http://bicepkeck.org/
|
gptkbp:bfsParent
|
gptkb:Cosmic_inflation
|
gptkbp:bfsLayer
|
6
|