Keck Array

GPTKB entity

Statements (56)
Predicate Object
gptkbp:instance_of gptkb:astronomy
gptkbp:collaboration gptkb:Mc_Gill_University
gptkb:Harvard_University
gptkb:Princeton_University
gptkb:Stanford_University
gptkb:University_of_British_Columbia
gptkb:University_of_California
gptkb:University_of_Chicago
gptkb:University_of_Toronto
gptkb:University_of_Minnesota
gptkb:NASA
gptkbp:components gptkb:Control
gptkb:astronomy
gptkb:scanner
receiver
signal processing unit
gptkbp:data_type radio astronomy data
gptkbp:design multiple aperture synthesis
gptkbp:field_of_study gptkb:cosmology
gptkbp:funding gptkb:National_Science_Foundation
gptkb:Department_of_Energy
gptkb:NASA
https://www.w3.org/2000/01/rdf-schema#label Keck Array
gptkbp:lighting gptkb:2013
gptkbp:location Mauna Kea, Hawaii
gptkbp:notable_achievements influenced future telescope designs
contributed to public understanding of science
developed new observational techniques
engaged in outreach activities
advanced technology in radio astronomy
collaborated on international projects
contributed to astrophysical research
contributed to understanding of inflation
enhanced precision of cosmological measurements
enhanced understanding of early universe
explored large scale structure of the universe
fostered collaboration among institutions
inspired new generations of astronomers
investigated dark energy
mapped cosmic microwave background
measured B-mode polarization
provided data for cosmological models
provided insights into cosmic evolution
published numerous research papers
studied gravitational waves
supported graduate research projects
gptkbp:notable_galaxies gptkb:10
gptkbp:notable_project gptkb:BICEP2
gptkbp:operated_by gptkb:California_Institute_of_Technology
gptkbp:sensitivity high sensitivity to faint signals
gptkbp:type gptkb:Interpol
gptkbp:used_for observing cosmic microwave background radiation
gptkbp:bfsParent gptkb:BICEP/_Keck_Collaboration
gptkb:BICEP2
gptkb:BICEP3
gptkbp:bfsLayer 7