Image Details
Caption: Fig. 1.
Relative corrections of cluster radio halos to the thermal SZ angular power spectrum evaluated at ﹩\nu =30﹩ GHz and for ﹩f_{\mathrm{RH}\,}=1/ 3﹩ (solid line). Contribution of clusters in different redshift ranges are also shown.
© 2004. The American Astronomical Society. All rights reserved. Printed in U.S.A.