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BICEP (Background Imaging of Cosmic Extragalactic Polarization) and the Keck Array are a series of cosmic microwave background (CMB) experiments, deployed near the South Pole. These are cryogenic telescopes with arrays of detectors sensitive to several frequencies of microwave radiation. They aim to measure the polarization of the CMB, in order to find…
Purpose and collaboration, BICEP2 & Keck Array
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array bicep2 keck bicep polarization telescope pole data bicep1 south cosmic bicep3 ghz cmb 2012 planck experiments background observing detectors
| Subject | Predicate | Object | Confidence | Src |
|---|---|---|---|---|
| BICEP and Keck Array | Alternative names | Background Imaging of Cosmic Extragalactic Polarization | 1.00 | infobox |
| BICEP and Keck Array | Coordinates | .mw-parser-output .geo-default,.mw-parser-output .geo-dms,.mw-parser-output .geo-dec{display:inline}.mw-parser-output .geo-nondefault,.mw-parser-output .geo-multi-punct,.mw-pars… | 1.00 | infobox |
| BICEP and Keck Array | Diameter | 0.25 m (9.8 in) | 1.00 | infobox |
| BICEP and Keck Array | Location | Antarctic Treaty area | 1.00 | infobox |
| BICEP and Keck Array | Wavelength | 95, 150, 220 GHz (3.2, 2.0, 1.4 mm) | 1.00 | infobox |
| BICEP and Keck Array | Website | www.cfa.harvard.edu/CMB/keckarray/ | 1.00 | infobox |
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