POLARBEAR
Diameter | 2.5 m (8 ft 2 in) |
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Angular resolution | 3.5 arcminute ![]() |
Website | bolo |
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POLARBEAR (POLARization of the Background Radiation)[1] is a cosmic microwave background polarization experiment located in the Atacama Desert of northern Chile in the Antofagasta Region. The POLARBEAR experiment is mounted on the Huan Tran Telescope (HTT) at the James Ax Observatory in the Chajnantor Science Reserve. The HTT is located near the Atacama Cosmology Telescope on the slopes of Cerro Toco at an altitude of nearly 5,200 m (17,100 ft).[2][3]
POLARBEAR was developed by an international collaboration which includes
History
The instrument was first installed at the Combined Array for Research in Millimeter-wave Astronomy site near Westgard Pass in California (USA) for an engineering run in 2010. It was then moved to its final destination in the Atacama Desert in September 2011. POLARBEAR saw first light on January 10, 2012, and began its first observing season in April 2012.[4]
In October 2014, POLARBEAR published a measurement of
POLARBEAR's published measurements focused on a small but clean patch of the sky where galactic foregrounds should be subdominant to gravitational lensing B-modes. The POLARBEAR team was able to report that the measured B-mode polarization was of cosmic origin at a 97.2% confidence level by focusing their observing time on this small patch where they are highly sensitive to arcminute anisotropies. However, this observing strategy is insensitive to the larger degree-scale inflationary B-modes that BICEP2 and Keck Array have searched for. [6]
See also
- Atacama Cosmology Telescope
- BICEP and Keck Array
- Brian Keating
- LiteBIRD
- Llano de Chajnantor Observatory
- Simons Observatory
References
- S2CID 118546886.
- )
- .
- ^ "First Light in Chile!". University of California Berkeley Department of Physics. Retrieved March 5, 2012.
- S2CID 118598825.
- ^ "POLARBEAR project offers clues about origin of universe's cosmic growth spurt". Christian Science Monitor. October 21, 2014.