GroundBIRD: an experiment for CMB polarization measurements at a large angular scale from the ground

Author(s):  
Osamu Tajima ◽  
Jhoon Choi ◽  
Masashi Hazumi ◽  
Hikaru Ishitsuka ◽  
Masanori Kawai ◽  
...  
2003 ◽  
Vol 47 (11-12) ◽  
pp. 953-966 ◽  
Author(s):  
J.E. Carlstrom ◽  
J. Kovac ◽  
E.M. Leitch ◽  
C. Pryke

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

2014 ◽  
Vol 176 (5-6) ◽  
pp. 691-697 ◽  
Author(s):  
S. Oguri ◽  
◽  
J. Choi ◽  
M. Hazumi ◽  
M. Kawai ◽  
...  

2021 ◽  
Vol 922 (2) ◽  
pp. 212
Author(s):  
Kathleen Harrington ◽  
Rahul Datta ◽  
Keisuke Osumi ◽  
Aamir Ali ◽  
John W. Appel ◽  
...  

Abstract The Cosmology Large Angular Scale Surveyor (CLASS) is a four-telescope array observing the largest angular scales (2≲ ℓ ≲ 200) of the cosmic microwave background (CMB) polarization. These scales encode information about reionization and inflation during the early universe. The instrument stability necessary to observe these angular scales from the ground is achieved through the use of a variable-delay polarization modulator as the first optical element in each of the CLASS telescopes. Here, we develop a demodulation scheme used to extract the polarization timestreams from the CLASS data and apply this method to selected data from the first 2 yr of observations by the 40 GHz CLASS telescope. These timestreams are used to measure the 1/f noise and temperature-to-polarization (T → P) leakage present in the CLASS data. We find a median knee frequency for the pair-differenced demodulated linear polarization of 15.12 mHz and a T → P leakage of <3.8 × 10−4 (95% confidence) across the focal plane. We examine the sources of 1/f noise present in the data and find the component of 1/f due to atmospheric precipitable water vapor (PWV) has an amplitude of 203 ± 12 μ K RJ s for 1 mm of PWV when evaluated at 10 mHz; accounting for ∼17% of the 1/f noise in the central pixels of the focal plane. The low levels of T → P leakage and 1/f noise achieved through the use of a front-end polarization modulator are requirements for observing of the largest angular scales of the CMB polarization by the CLASS telescopes.


Author(s):  
Shunsuke Honda ◽  
Jihoon Choi ◽  
Ricardo T. Génova-Santos ◽  
Makoto Hattori ◽  
Masashi Hazumi ◽  
...  

2012 ◽  
Author(s):  
J. W. Henning ◽  
P. Ade ◽  
K. A. Aird ◽  
J. E. Austermann ◽  
J. A. Beall ◽  
...  

2004 ◽  
Author(s):  
Ettore Carretti ◽  
Stefano Cortiglioni ◽  
Claudio Macculi ◽  
Carla Sbarra ◽  
Giulio Ventura ◽  
...  

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