scholarly journals The Sunyaev‐Zel'dovich Effect in CMB‐calibrated Theories Applied to the Cosmic Background Imager Anisotropy Power atl> 2000

2005 ◽  
Vol 626 (1) ◽  
pp. 12-30 ◽  
Author(s):  
J. R. Bond ◽  
C. R. Contaldi ◽  
U.‐L. Pen ◽  
D. Pogosyan ◽  
S. Prunet ◽  
...  
Keyword(s):  
Cosmic Background ◽  
Sunyaev Zel'dovich Effect ◽  
Cosmic Background Imager

scholarly journals The Anisotropy of the Microwave Background tol= 3500: Deep Field Observations with the Cosmic Background Imager

2003 ◽  
Vol 591 (2) ◽  
pp. 540-555 ◽  
Author(s):  
B. S. Mason ◽  
T. J. Pearson ◽  
A. C. S. Readhead ◽  
M. C. Shepherd ◽  
J. Sievers ◽  
...  
Keyword(s):  
Field Observations ◽  
Microwave Background ◽  
Cosmic Background ◽  
Cosmic Background Imager

scholarly journals Observations of Galactic star-forming regions with the Cosmic Background Imager at 31 GHz

2015 ◽  
Vol 453 (2) ◽  
pp. 2082-2093 ◽  
Author(s):  
C. Demetroullas ◽  
C. Dickinson ◽  
D. Stamadianos ◽  
S. E. Harper ◽  
K. Cleary ◽  
...  
Keyword(s):  
Star Forming ◽  
Star Forming Regions ◽  
Cosmic Background ◽  
Cosmic Background Imager

Ionization History of the Cosmic Plasma in the Light of the Recent Cosmic Background Imager and FuturePlanckData

2003 ◽  
Vol 586 (2) ◽  
pp. 709-717 ◽  
Author(s):  
A. G. Doroshkevich ◽  
I. P. Naselsky ◽  
P. D. Naselsky ◽  
I. D. Novikov
Keyword(s):  
Cosmic Plasma ◽  
Cosmic Background ◽  
History Of ◽  
Cosmic Background Imager

scholarly journals The Cosmic Background Imager

2002 ◽  
Vol 114 (791) ◽  
pp. 83-97 ◽  
Author(s):  
S. Padin ◽  
M. C. Shepherd ◽  
J. K. Cartwright ◽  
R. G. Keeney ◽  
B. S. Mason ◽  
...  
Keyword(s):  
Cosmic Background ◽  
Cosmic Background Imager

Extended Mosaic Observations with the Cosmic Background Imager

2004 ◽  
Vol 609 (2) ◽  
pp. 498-512 ◽  
Author(s):  
A. C. S. Readhead ◽  
B. S. Mason ◽  
C. R. Contaldi ◽  
T. J. Pearson ◽  
J. R. Bond ◽  
...  
Keyword(s):  
Cosmic Background ◽  
Cosmic Background Imager

First Intrinsic Anisotropy Observations with the Cosmic Background Imager

2001 ◽  
Vol 549 (1) ◽  
pp. L1-L5 ◽  
Author(s):  
S. Padin ◽  
J. K. Cartwright ◽  
B. S. Mason ◽  
T. J. Pearson ◽  
A. C. S. Readhead ◽  
...  
Keyword(s):  
Cosmic Background ◽  
Intrinsic Anisotropy ◽  
Cosmic Background Imager

scholarly journals Implications of the Cosmic Background Imager Polarization Data

2007 ◽  
Vol 660 (2) ◽  
pp. 976-987 ◽  
Author(s):  
J. L. Sievers ◽  
C. Achermann ◽  
J. R. Bond ◽  
L. Bronfman ◽  
R. Bustos ◽  
...  
Keyword(s):  
Polarization Data ◽  
Cosmic Background ◽  
Cosmic Background Imager

scholarly journals The Cosmic Background Imager

2005 ◽  
Vol 201 ◽  
pp. 23-32
Author(s):  
T. J. Pearson ◽  
B. S. Mason ◽  
S. Padin ◽  
A. C. S. Readhead ◽  
M. C. Shepherd ◽  
...  
Keyword(s):  
Background Radiation ◽  
Clusters Of Galaxies ◽  
Microwave Background ◽  
Owens Valley ◽  
Radio Observatory ◽  
San Pedro ◽  
Cosmic Background ◽  
Microwave Background Radiation ◽  
Cmb Fluctuations ◽  
Cosmic Background Imager

The Cosmic Background Imager (CBI) is an instrument designed to make images of the cosmic microwave background radiation and to measure its statistical properties on angular scales from about 3 arc minutes to one degree (spherical harmonic scales from l ˜ 4250 down to l ˜ 400). The CBI is a 13-element interferometer mounted on a 6 meter platform operating in ten 1-GHz frequency bands from 26 GHz to 36 GHz. The instantaneous field of view of the instrument is 45 arcmin (FWHM) and its resolution ranges from 3 to 10 arcmin; larger fields can be imaged by mosaicing. At this frequency and resolution, the primary foreground is due to discrete extragalactic sources, which are monitored at the Owens Valley Radio Observatory and subtracted from the CBI visibility measurements.The instrument has been making observations since late 1999 of both primordial CMB fluctuations and the Sunyaev-Zeldovich effect in clusters of galaxies from its site at an altitude of 5080 meters near San Pedro de Atacama, in northern Chile. Observations will continue until August 2001 or later. We present preliminary results from the first few months of observations.

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