Journal
NEW ASTRONOMY REVIEWS
Volume 47, Issue 8-10, Pages 727-732Publisher
ELSEVIER SCI LTD
DOI: 10.1016/j.newar.2003.07.020
Keywords
-
Categories
Ask authors/readers for more resources
MAXIMA is a balloon-borne platform for measuring the anisotropy of the Cosmic Microwave Background (CMB). It has measured the CMB power spectrum with a 10-arcmin FWHM beam, corresponding to a detection of the power spectrum out to spherical harmonic multipole l similar to 1000. The spectrum is consistent with a flat Universe with a nearly scale-invariant initial spectrum of adiabatic density fluctuations. Moreover, the MAXIMA data are free from any notable non-Gaussian contamination and from foreground dust emission. In the same region, the WMAP experiment observes the same structure as that observed by MAXIMA, as evinced by analysis of both maps and power spectra. The next step in the evolution of the MAXIMA program is MAXIPOL, which will observe the polarization of the CMB with comparable resolution and high sensitivity over a small patch of the sky. (C) 2003 Elsevier B.V. All rights reserved.
Authors
I am an author on this paper
Click your name to claim this paper and add it to your profile.
Reviews
Recommended
No Data Available