Correlations between the Wilkinson Microwave Anisotropy Probe and MAXIMA Cosmic Microwave Background Anisotropy Maps
The Astrophysical Journal American Astronomical Society 605:2 (2004) 607-613
The angular power spectrum of NVSS radio galaxies
ArXiv astro-ph/0404085 (2004)
Abstract:
We measure the angular power spectrum of radio galaxies in the NRAO VLA Sky Survey (NVSS) using two independent methods: direct spherical harmonic analysis and maximum likelihood estimation. The results are consistent and can be understood using models for the spatial matter power spectrum and for the redshift distribution of radio galaxies at mJy flux-density levels. A good fit to the angular power spectrum can only be achieved if radio galaxies possess high bias with respect to mass fluctuations; by marginalizing over the other parameters of the model we derive a 68% confidence interval 1.53 < b_0 sigma_8 < 1.87, where b_0 is the linear bias factor for radio galaxies and sigma_8 describes the normalization of the matter power spectrum. Our models indicate that the majority of the signal in the NVSS angular power spectrum is generated at low redshifts. Individual redshifts for the NVSS sources are thus required to alleviate projection effects and probe directly the matter power spectrum on large scales.The initial conditions of the universe: how much isocurvature is allowed?
(2004)
Constraints on isocurvature models from the WMAP first-year data
PHYSICAL REVIEW D 70:10 (2004) ARTN 103520