scholarly journals CMB Polarization with BICEP2 and Keck-Array

2012 ◽  
Vol 8 (S288) ◽  
pp. 68-75
Author(s):  
Clement Pryke ◽  

AbstractBICEP2 is an evolution from the highly successful BICEP CMB polarization experiment. In turn Keck-Array is an array of BICEP2 like receivers to achieve an additional increase in sensitivity. All these experiments are located at the South Pole in Antarctica and target the CMB B-mode polarization signal which is predicted to exist in many simpler models of Inflation at angular scales of several degrees. The design and performance of BICEP2 and Keck-Array is described and some preliminary polarization maps are presented.

2020 ◽  
Vol 15 (02) ◽  
pp. T02002-T02002
Author(s):  
M.G. Aartsen ◽  
M. Ackermann ◽  
J. Adams ◽  
J.A. Aguilar ◽  
M. Ahlers ◽  
...  
Keyword(s):  

Author(s):  
Y. Abdou ◽  
K.-H. Becker ◽  
J. Berdermann ◽  
M. Bissok ◽  
C. Bohm ◽  
...  

2012 ◽  
Author(s):  
J. E. Austermann ◽  
K. A. Aird ◽  
J. A. Beall ◽  
D. Becker ◽  
A. Bender ◽  
...  

2020 ◽  
pp. 1-14 ◽  
Author(s):  
Jay A. Johnson ◽  
Tanner Kuhl ◽  
Grant Boeckmann ◽  
Chris Gibson ◽  
Joshua Jetson ◽  
...  

Abstract Over the course of the 2014/15 and 2015/16 austral summer seasons, the South Pole Ice Core project recovered a 1751 m deep ice core at the South Pole. This core provided a high-resolution record of paleoclimate conditions in East Antarctica during the Holocene and late Pleistocene. The drilling and core processing were completed using the new US Intermediate Depth Drill system, which was designed and built by the US Ice Drilling Program at the University of Wisconsin–Madison. In this paper, we present and discuss the setup, operation, and performance of the drill system.


2009 ◽  
Vol 5 (H15) ◽  
pp. 618-619
Author(s):  
Yuki D. Takahashi

AbstractBicep was a telescope designed to probe the polarization of the cosmic microwave background (CMB) for the signature of gravitational waves produced during the epoch of inflation. The instrument was developed by a team of scientists from Caltech/JPL, UC Berkeley, and UC San Diego. It was installed at the South Pole in November 2005 and the CMB observations were conducted from February to November each year with one winter-over scientist responsible for operating and maintaining the instrument. Taking advantage of the excellent atmospheric conditions at the South Pole, we mapped 2% of the sky at 100 and 150 GHz. We completed 3 years of observations from 2006 to 2008, mapping the CMB polarization anisotropy at degree angular scales with unprecedented sensitivity. In 2010, a next generation instrument, Bicep2, will be installed on the existing telescope mount for an even deeper survey.


2003 ◽  
Vol 47 (11-12) ◽  
pp. 1083-1089 ◽  
Author(s):  
Sarah Church ◽  
Peter Ade ◽  
James Bock ◽  
Melanie Bowden ◽  
John Carlstrom ◽  
...  

2018 ◽  
Vol 45 ◽  
pp. 31-38
Author(s):  
Federica La Longa ◽  
Massimo Crescimbene ◽  
Lucilla Alfonsi ◽  
Claudio Cesaroni ◽  
Vincenzo Romano
Keyword(s):  

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