The authors wish to thank J.-L. Puget for many suggestions and fruitful discussions. They wish to thank the referee, M. Birkinshaw, for his helpful comments that much improved the paper. The authors thank J.F. Navarro, C. Frenk and S.D. White for kindly providing us a FORTRAN routine, computing the concentrations and the critical densities of the dark matter profiles, and J.R. Bond for providing the CMB map used in the analysis. The power spectra of the primary fluctuations were performed using the CMBFAST code (M. Zaldarriaga & U. Seljak). In addition, we thank F. Bernardeau, F.-X. Désert, Y. Mellier and J. Silk for helpful discussions and A. Jones for his careful reading of the paper.
© European Southern Observatory (ESO) 1998
Online publication: May 15, 1998