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26 April 2024
 
  » arxiv » astro-ph/0012211

 Article overview



First Intrinsic Anisotropy Observations with the Cosmic Background Imager
S. Padin ; J. K. Cartwright ; B. S. Mason ; T. J. Pearson ; A. C. S. Readhead ; M. C. Shepherd ; J. Sievers ; P. S. Udomprasert ; W. L. Holzapfel ; S. T. Myers ; J. E. Carlstrom ; E. M. Leitch ; M. Joy ; L. Bronfman ; J. May ;
Date 11 Dec 2000
Journal 2001, ApJ, 549, L1-L5
Subject astro-ph
AffiliationCaltech), W. L. Holzapfel (UC Berkeley), S. T. Myers (NRAO), J. E. Carlstrom, E. M. Leitch (U. Chicago), M. Joy (NASA/Marshall), L. Bronfman, J. May (U. de Chile
AbstractWe present the first results of observations of the intrinsic anisotropy of the cosmic microwave background radiation with the Cosmic Background Imager from a site at 5080 m altitude in northern Chile. Our observations show a sharp decrease in C_l in the range l=400 - 1500. The broadband amplitudes we have measured are deltaT(band) = 58.7 (-6.3, +7.7) microK for l = 603 (-166, +180) and 29.7 (-4.2, +4.8) microK for l = 1190 (-224, +261), where these are half-power widths in l. Such a decrease in power at high l is one of the fundamental predictions of the standard cosmological model, and these are the first observations which cover a broad enough l range to show this decrease in a single experiment. The C_l we have measured enable us to place limits on the density parameter, Omega(tot) <= 0.4 or $Omega(tot) >= 0.7 (90% confidence).
Source arXiv, astro-ph/0012211
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